Climate change and Palaeoclimatology
‘Hard’ Snowball Earth softens
May 2010
The original hypothesis of Neoproterozoic global glacial conditions, proposed by Joe Kirschvink (California Institute of Technology) and Paul Hoffman (emeritus at Harvard) in the 1990s was that conditions became so severe that the Earth was encased in glacial- and sea ice from pole to pole. As EPN has charted since 2000, that 'hard' Snowball variant has become increasingly less favoured by most geoscientists (Kerr, R.A. 2010. Snowball Earth has melted back to a profound wintry mix. Science, v. 327, p. 1186). However, evidence supporting low latitude glaciations continues to emerge (, F.A. and 9 others 2010. Calibrating the Cryogenian. . Science, v. 327, p. 1241-1243). In the latest, diamictites of the so-called 'Sturtian' glaciation in north-western Canada are interbedded with volcanic rocks that give a very precise age of 716.5 Ma. That age happens to coincide with outpouring of the regionally massive Franklin flood basalts whose palaeomagnetism gives equatorial latitudes, the first recorded for the Sturtian glaciation: the later Marinoan glaciation (˜635 Ma) provides most low-latitude evidence for Snowball conditions. The paper by Francis Macdonald and co-workers also gives detailed carbon isotope data for a continuous sedimentary record from >811 to 583 Ma.
A potential spanner in the works for the entire Snowball Earth hypothesis is the discovery of a strange anomaly concerning palaeomagnetic pole positions during latest Neoproterozoic times (Abrajevitch, A. & van der Voo, R. 2010. Incompatible Ediacaran paleomagnetic directions suggest an equatorial geomagnetic dipole hypothesis. Earth and Planetary Science Letters, v. 293, p. 164-170). Paleomagnetism from glaciogenic rocks is the lynchpin for the notion of Snowball Earth, some occurrences recording tropical latitudes. Alexandra Abrajevitch (Kochi University, Japan) and Rob van der Voo (University of Michigan) report palaeomagnetic results for igneous rocks between 600 and 550 Ma in what are now North America and Scandinavia. The data show original inclinations of the magnetic field that are both steep and shallow, indicating high and low latitudes respectively. Plotting inclination against radiometric age for what were separate continental masses in the Ediacaran Period reveals repeated rapid changes from high to low palaeolatitudes that simply cannot be accounted for by continental drift: plate tectonic rates would have to have been unaccountably fast (˜45 cm yr-1). To account for the abrupt shifts the authors turn not to true polar wander - due to changes in the geometry of the geomagnetic dipole - but to rapid flips in the orientation of the dipole between a coaxial and an equatorial alignment, perhaps due to dramatic changes of circulation within the liquid outer core. Familiar geomagnetic reversals normally shift the magnetic poles between roughly the geographic pole positions. Yet there are data showing that for brief periods the reversing poles do pass through equatorial latitudes but at very low magnetic field strength. In the cases from the Ediacaran the geomagnetic poles dwelt at tropical latitudes for long periods and maintained a strong field. Were such strange behaviour demonstrated earlier in the Neoproterozoic, during the Cryogenian period of supposed Snowball events, that would undermine the whole basis for the hypothesis. It seems inevitable that geophysicists will scurry to check the earlier palaeomagnetic data, analysing more igneous rocks on all continents at the narrowest possible time intervals.
A challenge to sea-level calibration
March 2010
As well as revealing the Milankovich pacemaker for past climate change, studies of oxygen isotopes from deep-water of benthic foraminifera in marine sediment cores also give a guide to the height of former sea levels. That approach is based on several assumptions, of which two are central. One is that the isolation of deep-water organisms from temperature variations at the sea surface, which control the take up of 18O by near surface plankton: well supported by the measured constancy of cold deep ocean water. The other is that oxygen is rapidly and homogeneously mixed throughout the ocean water column. The reason why good mixing is critical stems from the very purpose of measuring benthic oxygen isotopes, itself based on a sound assumption. Ice masses on land lock up a proportion of evaporated ocean water. Evaporation favours the lighter 16O isotope in water molecules over the heavier, so that atmospheric water vapour has a lower 18O/16O ratio than seawater. When snow falls and turns into glacial ice that build up ice caps, surface water of the oceans becomes depleted in 16O so that its 18O/16O ratio (standardised as the δ18O value) increases. That makes oceanic δ18O values, measured from benthic foram shells, an indirect or proxy measure of both the amount of ice locked up on land and changing sea levels: the principal quantification of past global climate change whose record goes back to the oldest preserved ocean floor (Lower Jurassic, ~205 Ma). Modern humans eventually left Africa to colonise the rest of the world sometime before 60 Ma ago, the first reliable age of evidence for colonisation outside Africa. Africa is surrounded by sea, except for the narrow strip of land into Palestine that ends up in a desert dead end to further migrations. So, it seems likely that the exodus was across the outlet of the Red Sea that would have become narrower and shallower as sea level fell when the Earth moved into the last glacial epoch after 117 thousand years ago, when sea-level was as high as it is today.
The assumption of rapid, efficient mixing of the oceans has not been thoroughly tested. In fact it is estimated that any complete turnover takes around a thousand years, so there is likely to be a significant time lag in the sea-floor record. New, independent evidence also suggests that the calibration of benthic δ18O needs revision (Dorale, J.A. et al. 2010. Sea-level highstand 81,000 years ago in Mallorca. Science, v. 327, p. 860-863). It comes from caves on the Mediterranean island of Mallorca that connect directly with the sea. Stalactites and stalagmites (collectively called speleothem) have formed in the caves, their growth being affected by flooding and drying as sea level rose and fell during the last 130 ka. At each flooding level encrustations formed around the speleothem to produce bulbous growths at different heights in the caves, which are clearly forming today at mean sea level. The researchers from the US, Mallorca, Italy and Romania dated the bulbs using the U/Th method appropriate for speleothems, and found three stages of formation: at 121, 116 and 80-82 ka. The two older encrustations are at ~2.6 m above modern sea level, bang on the oxygen isotope calibration for the end of the last interglacial. However, those formed between 80-82 ka ago – a period of warming during the overall trend to colder conditions as ice sheets grew – are about a metre above modern sea level: very different from the estimate of 10-20 m below¬ based on the benthic δ18O calibration.
It is too early to tell in what quandary palaeo-oceanographers will be placed by this large discrepancy. There are four main possibilities for the aberrant results. First, the Mediterranean might have stood higher that global sea level for some reason, but that seems highly unlikely as the connection through the Straits of Gibraltar is deep enough to have maintained flow even at the last glacial maximum when global sea level was around 120 m below the present. Second is that the means of calibration using raised coral reefs on tectonically rising coastlines of New Guinea and Barbados is seriously out for part of the last glacial period. Thirdly, somehow the Mallorcan crust was depressed during the last glacial period. The island is rising at about 0.2 mm yr-1, which would give an uplift of 16 m since 81 ka, but that conflicts with the good match with the last highest sea level at 121 and 116 ka. Finally, the authors suggest that at 81 ka the volume of the world’s ice caps was much the same as today, despite the higher-than-present δ18O values in contemporary sea-floor sediments.
Climate-CO2 links since the Miocene
January 2010
The November 2009 issue of EPN (Boron isotopes and climate change) described how the 11B/10B ratios of planktonic forams correlate with the pH of seawater, and thus with the amount of dissolved CO2 that increases acidity. In fact the more easily analysed ratio between the boron and calcium contents of forams does the same, and for the last 800 ka correlates with the measured CO2 content of bubbles in Antarctic ice, which itself correlates very well with temperatures and sea levels (Tripati, A.K. et al. 2009. Coupling of CO2 and ice sheet stability over major climate transitions of the last 20 million years. Science, v. 326, p. 1394-1397). Extending this approach back to 20 Ma shows that in the Middle Miocene (~10 Ma) when glacial cover began to expand atmospheric CO2 fell from levels similar to those of the present day (387 ppm) to approximately those of the pre-industrial Holocene (~250 ppm). In the earlier Miocene from 14 to 20 Ma global mean surface temperatures were 3-6º C higher and sea level stood 40 m higher than at present. As well as this grim reminder of a possible future, the data support the general notion of a coupling between atmospheric CO2 and global climate.
Was the Archaean blazing hot or balmy?
January 2010
Silica-rich sediments, notably cherts have been used to estimate ocean temperatures in the far off Archaean Eon. This is possible because SiO2 and water exchange oxygen atoms as the silica mud is forming, and in doing so its two main stable isotopes (18O and 16O) are preferentially treated depending on water temperature. The cooler it is the more 18O ends up in silica. Early Archaean cherts commonly show lower δ18O values than silica-rich ocean sediments forming now, so much lower that the temperature of Palaeoarchaean seas has been judged to have been between 55 to 85º C. Discomfortingly hot for bathers, and not very plausible considering that without a CO2-rich atmosphere Archaean oceans would have been frozen solid because the Sun emitted much less energy than it does now. However, such estimates have to assume that the oxygen isotopic composition of seawater at 3.5 Ga was the same as now, when in fact it is known that environmental δ18O probably changes over long time periods. A way of avoiding an untestable assumption is to measure the isotopic composition of hydrogen (1H and 2H or D) in chert as well as that of oxygen. The cooler water is, the lower δD values are in silica that is precipitated from it. Ordinary quartz contains no hydrogen except in unstable fluid inclusions, but the way chert forms as colloidal precipitates of opal-like material locks hydrogen in the form of OH- ions into its silica (Hren, M.T. et al. 2009. Oxygen and hydrogen isotope evidence for a temperate climate 3.42 billion years ago. Nature, v. 462, p. 205-208). Combining the two measures for 3.42 Ga cherts from the famous Barberton Mountain Land Archaean complex results in a sea-surface temperature estimate of no more than 40ºC.
Boron isotopes and climate change
November 2009
Boron has two stable isotopes, 10B and 11B. Like all isotopes of the same element, when boron is shifted from one host to another some fractionation between its isotopes is likely. In the case of boron being taken-up by planktonic foraminifera, their shells' 11B/10B ratios correlate with the pH of seawater. Since the pH of the oceans is dominated by the effects of dissolved CO2, itself in equilibrium with the gas's atmospheric concentration, boron isotope ratios in foram shells are a proxy for the greenhouse effect produced by carbon dioxide. This finding dates back to 1992, but has only recently been used. It is especially revealing for the period around the Eocene-Oligocene boundary (see Lead-in to icehouse conditions in July 2009 issue of EPN) when other evidence indicates that global cooling eventually allowed glaciers to grow on Antarctica and possibly at northern high latitudes (Pearson, P.N. et al. 2009. Atmospheric carbon dioxide through the Eocene-Oligocene climate transition. Nature, v. 461, p. 1110-1113). The boron data indicate a downward shift in atmospheric CO2 from around 1100 to 750 ppm by volume from 34.2-33.5 Ma, the lower value just preceding δ18O data for a rapid increase in polar glaciers. Oddly, δ11B then rises to levels suggesting a return to CO2 levels of >1000 ppm by volume at a time of constant high δ18O that show the survival of ice caps; perhaps a result of increased albedo forcing.
Impact cause for Younger Dryas panned again
November 2009
In 2007 two dozen scientists presented evidence to suggest that onset of the Younger Dryas, extinction of many North American mammal species and the sudden end of the Clovis culture at 12.9 ka followed upper atmosphere explosions of cometary material (see Whizz-bang view of Younger Dryas and Impact cause for Younger Dryas draws flak in EPN of July 2007 and May 2008). The Clovis culture of North America, signified by superbly crafted stone spear points, occupied a narrow time range between 13.3 and 12.8 ka, i.e. up to the start of the Younger Dryas interstadial. Some Clovis occupation sites are buried by organic-rich soils. Remarkably, the original proposers of a catastrophic event (Firestone, R.B. and 25 others 2007. Evidence for an extraterrestrial impact 12,900 years ago that contributed to the megafaunal extinctions and the Younger Dryas cooling. Proceedings of the National Academy of Sciences of the United States of America, v. 104, 16016-16021) claimed that the veneers contain magnetic microspherules, magnetic grains, iridium and nickel, charcoal, soot and polycyclic hydrocarbons, carbon spherules, fullerenes that trap helium with extraterrestrial isotopic proportions, glass-like carbon, and nanodiamonds. Missing from what looks like a supportive package are shocked minerals, which are the only materials formed uniquely by impact events.
Experts on extraterrestrial influences considered the team to be 'over-enthusiastic'. In response Firestone and co-workers made replicate samples available for independent confirmation or refutation of their claims. This offer seems not to have been followed-up, but another large team recollected the black soil veneers from two of the same sites and 5 others of similar age (Surovell, T.A. and 8 others 2009. An independent evaluation of the Younger Dryas extraterrestrial impact hypothesis. Proceedings of the National Academy of Sciences of the United States of America, v. 106, p. 18155-18158). They focussed on the claim for magnetic spherules, using the same techniques as Firestone et al. (2007), yet failed to find anomalous peaks at the time of the Clovis demise and opening of the Younger Dryas massive global cooling. Their conclusion was, ' In short, we find no support for the extraterrestrial impact hypothesis as proposed by Firestone et al.'. However, Surovell et al. did find magnetic spherules before, during and after the interstadial event. In fact, magnetic spherules are quite common in many sedimentary settings and have a history of controversy. In the late 1980s Robert S. Foote, an oil explorationist claimed that many oilfields were associated with geomagnetic anomalies with distinctive short wavelength 'signatures'. He became widely regarded as a crank. But he persisted and discovered the first tangible evidence for lifeforms that thrive at high temperatures in deep oil wells - shiny, tiny magnetic spherules made of magnetite (Fe3O4). Magnetotactic bacteria living in highly reducing conditions produce them to form magnetosome chains. Magnetosomes are also present in the brains of far-migrating birds, with connections to their remarkable feats of navigation.
Just when you think it's going to turn out alright...
November 2009
The millennium of Younger Dryas global cooling from 12.8 to 11.5 ka ago caught forager-hunters on the hop as they followed herds in the wake of the general glacial retreat after 18 ka. The shut-down of the Gulf Stream when high-latitude North Atlantic surface waters freshened may have occurred in a decade or so. The end of the YD marked the start of more modern conditions in the Holocene Epoch, when northward recolonisation resumed in earnest. Climate records, such as the δ18O proxy for air temperature in the Greenland ice cores, suggest long-term but 'noisy' climatic constancy. That is, until one spreads out the Holocene records. At around 8200 years ago is a 200-year downward 'blip' in temperature to well below the Holocene average and then recovery. The perturbation also shows up in a Newfoundland mire (Daley, T.J. et al. 2009. Terrestrial climate signal of the "8200 yr B.P. cold event" in the Labrador Sea region. Geology, v. 37, p. 831-834) as a pronounced change in δ18O from moss cellulose. The event has been ascribed to slow-down in thermohaline circulation following a further freshening of North Atlantic surface water by drainage of a remaining ice-dammed lake (Lake Agassiz) on the Canadian Shield. By 8.2 Ka the northward spread of flora and fauna from refugia around the Mediterranean Sea was well underway, and included the arrival in southern Europe of Neolithic farming practices: the start of an agricultural revolution that was to reshape the entire sociocultural ethos of the 'Old World', from which today's globalisation emerged. So it is interesting to learn that the 'cold blip' also left a signature at 41° N in northern Greece (Pross, J. et al. 2009. Massive perturbation in terrestrial ecosystems of the Eastern Mediterranean region associated with the 8.2 kyr B.P. climatic event. Geology, v. 37, p. 887-890). This study uses pollens collected from a lake-bed sediment core. The climatic event involved a rapid drop by 30 % in tree pollen abundances, matched by a 10% increase in pollen from shrubs, such as Artemisia (wormwood) normally associated with steppes further north. The end of the event involves a more sedate recolonisation by trees. From the pollen can be estimated the actual fall in winter temperature, which amounts to a devastating (for agriculture) decrease that was greater on average than 4° C. Interestingly, the German-French-Greek-Australian team ascribe some influence on the cooling to a spread of the Siberian High, a winter build-up of cold air on the steppes to the north of the Carpathians. The magnitude and extent of the Siberian High depends to a large extent on the albedo of the steppes in winter, which depends on snow cover and its persistence. This is a major influence today across much of Western Europe, as cold Siberian air spills from the continental anticyclone. At 8.2 ka it may have forced katabatic winds through Carpathian passes to cause winters that may have devastated the early farmers of northern Greece.
The Mother of all climate models and deglaciation hiccups
September 2009
In his latest book, The Vanishing Face of Gaia: A Final Warning (Allen Lane, London, 2009, ISBN 978186141850), James Lovelock more or less gives up on the ability of humanity in general, and science and engineering in particular, to fend off looming climatic catastrophe. He reserves his sharpest criticism for what he calls ‘American science’; a fundamentally reductionist approach that is fed into prediction of the future. For Lovelock, the assumption ‘that all we need to know about the climate can come from modelling the physics and chemistry of the air in ever more powerful computers’ has been a disastrous mistake. He is obviously not one for humble retrospection, as his early Gaia writings had at their centre a sort of reductio ad absurdum of that now prevailing genre in Earth system science. Daisyworld, reduced a planet’s life forms to white and black daisies, whose interplay with climatic change was governed by a formula known as a difference equation in the manner of Lotka and Volterra’s work on predator-prey interrelationships. The simplest difference equation is xnext = rx(1-x). Solving such non-linear relationships for minute increments in x led to the unmasking of chaos theory, the first instance being Edward Lorentz’s discovery that the simplest models of climatic turbulence go wonky if you tinker with them: the ‘Butterfly Effect’.
When his Gaia hypothesis drew together all manner of people from New Ageists mathematicians working on complex systems James Lovelock was exposed to friendly criticism and education about non-linearity and chaos. Clearly that revolutionised his world-view, which is fine, albeit a cause of some glumness for him. Far sadder is that he is probably right in criticising climate modelling - now that it has a stranglehold on the entire climate debate and indeed on the ears of the ‘Great and the Good’. A measure of where modelling has led is a simulation of what happened as the Northern Hemisphere emerged from the last glacial maximum, between 22 and 10 ka (Liu, Z. and 13 others 2009. Transient simulation of last deglaciation with a new mechanism for Bølling-Allerød warming. Science, v. 325, p. 310-314). These ~10 millennia saw a return to a see-saw climate that lasted from 60 to 30 Ma as the Earth cooled towards the last glacial epoch, dominated by cooling-warming cycles with a similar pattern of slow cooling-sudden descent into frigidity-thousand year cold spells-sudden warming known as Dansgaard-Oeschger cycles.
The Chinese-US team developed and ran the first synchronously coupled atmosphere-ocean general circulation model to investigate a hiccup in warming of the sea surface one northern ice caps began to melt decisively. It is said to be ‘one of the most epic numerical modelling efforts of the climate community to date’ (Timmermann, A. & Menviel, L. 2009. What drives climate flip-flops? Science, v. 325, p. 273-274). Epic, well yes: one of the world’s largest operational supercomputer (Jaguar at the Oak Ridge National Laboratory, USA) was wrangling for 18 months. Lots of known empirical data for the period were fed in: insolation determined by astronomic effects; changes in greenhouse gases from ice cores; shifts in coastlines and ice-sheet volumes. Tinkering with the model involved varying freshwater influx to high-latitude North Atlantic seawater. The result was crude simulation of what actually happened to sea-surface temperatures at several locations around the North Atlantic, giving some insights into why changes occurred. But climate scientists have long suggested mechanisms for the Dansgaard-Oeschger cycles, Bølling-Allerød warming, and the final frigid paroxysm of the Younger Dryas in much the same framework, the only difference being they didn’t produce numerical models that mimicked reality.
It seems that another 2 to 3 million hours of time on Jaguar are needed to bring the project through to the present. The enormous funding needed to get this kind of number crunching done can only have been on the back of claims that it will help predict future anthropogenic climate shifts. Based on real data, it still didn’t get things right – millennium-long cooling and warmings are not trivial events. There are conflicting kinds of data for changes in the parameters since the start of the Industrial Revolution preceded by 10 ka of relatively stable Holocene conditions. The best that climate forecasting for the next 100 years has been able to do, also using pretty large amounts of CPU time, is a range of straight lines showing increases in global mean surface temperature. Yes, hindsight is wonderful...
Lead-in to icehouse conditions
July 2009
At 33.5 Ma, around the time of the Eocene-Oligocene boundary, Earth’s climate took a sudden shift towards cooler conditions, coinciding with the onset of glaciation in the Northern Hemisphere and growth of Antarctic ice cover. Studies of a variety of proxies, including the density of pores or stomata on plant leaves, suggests that the transition resulted from a halving of atmospheric CO2 content from more than 1000 ppm in the Early Eocene to ~560 ppm in the Oligocene. So, even at twice the pre-industrial level greenhouse warming was compatible with high-latitude frigidity. Ocean-floor sediments from a site close to the Arctic Circle in the Norwegian-Greenland Sea yield pollen and spore records that chart vegetation change from 50 to 30 Ma (Eldrett, J.S et al. 2009. Increased seasonality through the Eocene to Oligocene transition in high northern latitudes. Nature, v. 459, p. 969-973. The proxy data suggest that in the period preceding the decisive global climate change conditions became increasingly seasonal, with greater differences between winter and summer temperatures. This was largely due to increasingly cold winters, a more constant summer temperature suggesting that any land ice on Greenland was of the valley type rather than an all-covering ice sheet.
On the edge of chaos in the Younger Dryas
May 2009
Around 13 thousand years ago, the world was warming rapidly and the great northern ice sheets in retreat. Plants, animals and humans in Europe were able to and did migrate northwards. Sea level still being low, there was nothing to stop decolonisation of Britain by crossing the huge fluviatile plain of Doggerland where the southern North Sea now stands.(see Return to ‘Doggerland’ in September 2008 issue of EPN). At 12.9 ka there came the shock of a rapid temperature fall at the start of the Younger Dryas episode, when ice sheets began to re-establish themselves in the upland areas of Britain and Scandinavia. What happened to those intrepid migrants we may never know, but what they would have faced had they chosen to remain in the game-teeming NW Europe of that episode has become clearer with detailed investigations in sediments at the bottom of a Norwegian lake supplied by melt water from glaciers (Bakke, J. et al. 2009. Rapid oceanic and atmospheric changes during the Younger Dryas cold period. Nature Geoscience, v. 2, p. 202-205).
The research by Norwegian and German scientists used two interesting proxies for glacial advance and retreat: the amount of sedimentary titanium and the density of the sediment, both of which would have varied with the rate of glacial erosion. The data were calibrated to time by 96 14C dates, and the sampling frequency (every 0.06 mm for Ti and 5 mm for density through a 1.4m core that represents 1700 years) was sufficient potentially to resolve events to a few days and 6 months respectively. Allowing for background ‘noise’ effects, certainly monthly and annual changes should show up, and indeed they do. The pattern is one of rapidly changing conditions between warm and frigid, which the authors interpret as a result of repeated ‘boom and bust’. At 12.18 ka, further cooling occurred and the late Younger Dryas is the more chaotic part of the record. The hypothesis is that the fluctuations reflect growth and shrinkage of sea ice in the North Atlantic, matched by growth and melting of glaciers. Brief warming during periods of prevailing westerly winds melted glaciers, but fed vast amounts of fresh water to the North Atlantic that in turn encouraged surface waters to freeze. Sea-ice formation and the build-up of a polar high pressure area drove weather systems conducive to westerlies southwards, when glaciers grew. Something suddenly stopped this chaotic behaviour and high latitudes rapidly emerged from frigidity at 11.7 ka: the Holocene had begun and, soon, so would humanity in an equally chaotic manner.
Climate at the Eocene-Oligocene (E-O) boundary
May 2009
Oxygen isotopes from benthic foraminifera in deep-sea sediment cores show an abrupt increase in d18O at around 34 Ma, which spanned a mere 300 ka. This is taken to indicate withdrawal of ocean water to polar ice caps on land that diamictites from high southern latitudes link to the beginning of glaciation of Antarctic. Then as now, the south polar region was thermally isolated, probably as a result of its having become surrounded by seaways and development of the Antarctic Circumpolar Current from the Palaeocene onwards as a result of the final break-up of Gondwana when it became separated from Australia and South America. Other factors at the E-O boundary seem to have been decreasing atmospheric CO2 and low solar heating as a result of the Milankovich effect. Cooling due to such factors was disrupted and delayed by the spectacular global warming at the Palaeocene-Eocene boundary (55.8 Ma) as a result of massive methane release to the atmosphere. Detailed proxy records from both high- and low-latitude sea-floor sediment cores now resolve fine detail of the shifts in sea-surface temperature (SST) at the E-O boundary (Liu, Z. et al. 2009. Global cooling during the Eocene-Oligocene climate transition. Science, v. 323, p. 1187-1190). The most profound shift in SST took place at high latitudes (in both Northern and Southern Hemispheres) with a drop of around 5 to 9°C between 34 to 33.5 Ma. This was followed by slight rise to about 3ºC below pre-E-O conditions. Surprisingly, data from low latitudes ‘flat-lined’ at around 28°C across the transition, suggesting steady evaporation of seawater, more of which would have precipitated as snow at high latitudes. The ‘hothouse’ conditions of the Cretaceous and early Cenozoic saw estimated high-latitude sea-surface temperatures rise from about 7°C to 12°C by the Early Eocene. The protracted global cooling that followed reached about 7°C by about 42 Ma, which stabilised until 40 Ma when SST fell to about 4°C just before the E-O boundary (see http://www.learner.org/courses/envsci/visual/visual.php?shortname=cenozoic).
The sudden start of Antarctic glaciation at 34 Ma looks increasing like an example of a chaos-like ‘flip’ in global climatic conditions brought on by a blend of factors that collectively reached a threshold, which once crossed permitted no escape, at least not over the last 30 Ma or so (Kump, L.R. 2009. Tipping pointedly colder. Science, v. 323, p. 1175-1176). That is a point that should not be lost at a time when anthropogenic global warming continues unabated, despite so much hype by the G20 leaders at their London meeting in early April 2009. Climatic ‘flips’ can go either way.
See also: Documenting the Palaeogene transition from ‘hothouse’ to ‘icehouse’ in EPN for August 2005, and Magmatic link to the Palaeocene-Eocene warming in EPN for July 2007
Rainfall-magnetic field link during the Holocene
March 2009
One of the fuelling factors in the debate about short-term climate change during the Holocene is the suggestion that variations in cosmic-ray bombardment might affect climate through these extra-solar particles’ possibly nucleating low-altitude clouds. It is a complicated idea, because changes in the Sun’s activity – the solar wind – modulate the cosmic ray flux, and short-term changes in solar irradiance at the Earth’s surface have also been suggested as a climate driver. To further obscure matters, any changes in the geomagnetic field would also affect cosmic-ray flux, yet geomagnetism is in turn a measurable proxy for cosmic ray intensities on Earth (Knudsen, M.F. & Riisager, P. 2009. Is there a link between Earth’s magnetic field and low latitude precipitation? Geology, v. 37, p. 71-74). The two Danish scientists have compiled the Holocene record of the geomagnetic dipole moment: effectively a measure of the strength of the magnetic field. In the paper they compare that record with δ18O changes in stalactites from China and the Oman, which are a proxy for changing low-latitude precipitation – in part the signal of the Indian Ocean monsoons. A correlation did emerge from the study, supporting the cosmic ray-climate theory. This further complicates the Earth’s climate system and therefore the models used by climatologists.
Mantle rock and carbon dioxide sequestration
January 2009
The peridotite mantle sequence of ophiolites often shows signs of having been altered by processes that form calcite and magnesite (CaCO3 and MgCO3) veins. It is a mundane feature and few geologists have paid it any heed, other than to note the veining. Such theories as there are generally suggest that the veining took place at the time of obduction of the ophiolitic masses onto continental margins, which was generally accompanied by some metamorphism. Nonetheless, the veins must have taken up carbon dioxide from some reservoir, either hydrothermal fluids derived from seawater or groundwater, but ultimately from the atmosphere: there are no primary carbonates in ophiolites. Dating the veins was deemed impossible, but someone had a go at veins in the Oman ophiolite using the 14C method (Keleman, P.B. & Matter, J. 2008. In situ carbonation of peridotite for CO2 storage. Proceedings of The National Academy of Sciences of the USA, v. 105, p. 17295-17300), discovering a great surprise; the veins are very much younger than the Eocene age of ophiolite emplacement. Their ages span 1.6 to 43 ka, about the same as the period over which a surface tufa deposit formed. Calcite and magnesite form by the breakdown of olivine and clinopyroxene in the presence of slightly acid water in which CO2 is dissolved, their young ages suggesting the veins formed during weathering by rainwater, the tufa deposits probably forming through related processes. Keleman and Matter estimated the volume of veins in peridotites exposed in new road cuttings at about 1%. The 15 m thick weathering horizon in the exposed Oman peridotite therefore corresponds to about 1012 kg of CO2, which accumulated at an average rate of around 4 x107 kg of CO2 per year. If this could be increased by 100 thousand times, the Oman peridotite could sequester about 10% of anthropogenic emissions. Is that possible?
Higher temperatures could speed up the carbonation reactions. The reactions are exothermic and sustaining a temperature around 185ºC is feasible by stimulating the reactions through shallow drilling and pumping carbon dioxide and water into shattered rock. Interestingly, the reactions might be capable of limited geothermal power generation. The potential absorption by such a plant in the Oman ophiolite could be up to 1 billion tonnes of CO2, and there are many other ophiolites rich in olivine. But that is not the end of the story: other olivine breakdown reactions involving water generate hydrogen, as discovered by Australian hydrogeologist Gordon Stanger. While conducting his PhD field work in Oman as part of the Open University Oman Ophiolite Project, Stanger discovered natural springs from which hydrogen gas was bubbling (Stanger, G. 1986. The hydrogeology of the Oman mountains. Unpublished PhD thesis, The Open University, Milton Keynes, UK).
East African evidence for Late Pleistocene climate change
November 2008
The most interesting times in human prehistory were those when African beings set off from their home continent for new habitats. The earliest seems to have been the migration of Homo ergaster some 1.8 Ma ago, and the most riveting, of course, was that of modern humans who set out to colonise the entire habitable planet sometime around 80 to 60 ka ago. It is pretty certain that the population movements were driven by environmental changes that provided a driving pressure to seek survivable conditions beyond Africa, such as episodes of drying in East Africa, and passable exits from the continent, such as sea-level falls to produce land bridges like that of the Straits of Bab el Mandab. One of the glaring gaps in knowledge about those circumstances is evidence for climate change from Africa itself. The problem has been that many of the Great Lakes did not fill until the last 12 ka or so, so provide no sediment cores and proxy climate records for the crucial period in human history. Lake Tanganyika is an exception, being so enormously deep that it survived much of the last glacial episode when Africa was probably a lot drier than now. Cores of Lake Tanganyika sediment reach back at least to 60 ka (more might be had if coring was done using drilling rather than piston coring) and a surprising record has emerged from that time (Tierney, J.E. et al. 2008. Northern Hemisphere controls on tropical southeast African climate during the last 60,000 years. Science, v. 322, p. 252-255).
Deuterium and organic geochemical data from the cores are proxies for water temperature and precipitation in the lake’s catchment, and show fluctuations that clearly match the familiar patterns of climate change from Greenland ice cores, and the intensity of the Asian monsoon recorded in Chinese cave deposits. This match shows clearly that the East African climate followed closely the orbitally-induced changes in solar input at high northern latitudes. But the cause of the linkage is not clear. One candidate is the varying position of the Intertropical Convergence Zone (ITCZ). Yet it seems that known shifts in the ITCZ are not linked to East African fluctuations. So the connection with the Asian monsoon hints at controls by the changes in Indian Ocean sea-surface temperature. The ‘teleconnection’ is characterised by very abrupt shifts from humidity to aridity, and profound aridity around 57, 47.5 and 38 ka. These may have resulted in extreme ecological shifts in the southern East African Rift System, resulting in considerable stresses on human groups. Sadly, data from the most probable first period of migration out of Africa by modern humans (70-80 ka) have not been reached by the piston coring method – maybe they will eventually be accessed by rotary drilling. However, the close linkage with the Greenland record does suggest that cool/arid conditions occurred in the modern human heartland around 70 and 74 ka, when sea level was beginning to fall to 80 m below that at present.
Younger Dryas and the Bat Cave
November 2008
It seems that bats have a remarkable loyalty to their chosen cave, whatever the weather. Thick guano deposits coat the floors of most caves that are now popular with bats. While the deposits are bioturbated by a narrow range of unwholesome insects, sufficient stratigraphy remains intact for more intrepid scientists to chance their hand at proxy records of climate in the caves’ vicinity; but data are, unsurprisingly, rather scanty. Arid conditions enhance preservation of such cave-floor deposits, and Bat Cave in the Grand Canyon of Arizona has attracted attention (Wurtster, C.M. et al. 2008. Stable carbon and hydrogen isotopes from bat guano in the Grand Canyon, USA, reveal Younger Dryas and 8.2 ka events. Geology, v. 36, p. 683-688). The team from Scotland, Canada, the USA and New Zealand show that both the Younger Dryas and a lesser global cold spell at 8.2 ka are discernible in the guano core from Bat Cave, but the signals arise from a rather circuitous cause. Bat guano is largely made up of the chitinous remains of the insects eaten by the bats, and it is the isotopic variation in the insects’ diet that the chitin preserves. That in turn stems from local vegetation, in some cases pollen or nectar consumed by the bugs, or even the blood of mammals or birds taken by bloodsucking insects – itself several metabolic steps from the local vegetation. These complexities may account for the rather ‘noisy’ guano data, yet it seems likely that other caves will be probed in arid areas where speleothem (from stalactites) has not developed continually through the caves’ lifetimes.
Testing hypotheses for the onset of Northern Hemisphere glaciation
September 2008
Whereas Antarctica began to develop significant ice caps in the early Oligocene (maybe in late Eocene times) those of the Northern Hemisphere, principally on Greenland, did not arise until about 3 Ma ago. There are several hypotheses for that onset of the Great Ice Age: closure of the Panama seaway and increased poleward heat transport in the North Atlantic; perhaps related development of the El Niño cycle in the East Pacific; uplift of the Himalaya and Rocky Mountains changing atmospheric circulation; lowered atmospheric CO2, and a combination of all four that allowed the Milankovich astronomical forcing to get a grip on Earth’s climate ‘machine’. Testing the hypotheses is somewhat more difficult than find empirical support for them; i.e. coincidences in timing. Climate scientists from Bristol, Cambridge and Leeds universities in the UK have attempted such a test, using a complex climate model involving coupled atmosphere-ocean circulation and ice-sheet models (Lunt, D.J. et al. 2008. Late Pliocene Greenland glaciation controlled by a decline in atmospheric CO2 levels. Nature, v. 454, p. 1102-1105). Only a decrease in the greenhouse effect could have transformed climate over Greenland sufficiently to equip it with a large ice sheet, the other three main hypotheses falling a long way short, although each could have led to small ice volumes. Significantly, the study failed to find support for any of the terrestrial processes having been capable of ‘priming’ orbital and rotational forcing to such an extent that they triggered glaciation. Despite the claims by the authors, as computing power goes up and the resolution of feasible climate modelling comes down it is quite likely that within a few years there will be another view ‘supported’ by models.
Climate shock of the Younger Dryas
September 2008
Between 12,900-11,500 years before the present, high northern latitudes returned to almost full glacial conditions, after about 6000 years of warming since the last glacial maximum. Just prior to the Younger Dryas cooling event, conditions had warmed sufficiently that European people had migrated northwards, some to occupy what are now the British Isles. Temperate grasslands teeming with game were the probable attraction, and still-low sea levels permitted crossing of what became the North Sea. Although it is possible that some people remained in Britain through the thousand-year mini glaciation, conditions would have been at the extremes of winter cold and year-long windiness, judging from the Greenland ice-core records of air temperature and dust. Those records have shown for some time that the transition from warmth to frigidity was rapid, but not how rapid. The cold spell had much in common with sudden, millennial-scale coolings repeated several times during the run-up to the last glacial maximum. Each such event has been linked with interruptions in the shallow and deep circulation of North Atlantic ocean waters, a likely trigger having been reduction in the salinity of surface waters as a result of floods of fresh water, either through collapses of ice caps and melting of icebergs or, in the case of the Younger Dryas, release of massive amounts of fresh water from glacially-blocked lakes in North America. One result would have been failure of cold surface water to sink at high latitudes, thereby shutting down the suction effect that drags warm water northwards to raise temperatures, especially in NW Europe.
There are concerns that unsuspected climate shifts that stem from the Earth System rather than astronomical influences – the Milankovich effect – may characterise the period of global warming caused by human activities. Increased precipitation at high northern latitudes or melting of ice on Greenland could result in falling ocean salinity and slowing or shutdown of the North Atlantic heat conveyor. Two sets of data published in August 2008 highlight potential climate shifts that may arise with virtually no warning. Both rely on the potentially high resolution of cores through ice caps and stagnant lakes that are annually layered, which has hitherto not been fully exploited by climate scientists. European and North American researchers have focussed on the upper part of the latest core through the Greenland ice cap, using two or three samples from each annual layer (Steffensen, J.P. and 19 others 2008. High-resolution Greenland ice core data show abrupt climate change happens in few years. Science, v. 321, p. 680-684). Deuterium and oxygen isotopes during the onset of the Younger Dryas show a marked cooling at the source of moisture precipitated as snow within 1 to 3 years, which the authors ascribe to the Intertropical Convergence Zone migrating northwards through a major change in atmospheric circulation. Temperature over the Greenland ice cap also changed, but over about 50 years [note however, that the sharp warming of the Bolling episode took less than a decade].
The second study uses annually varved lake sediments that accumulated in an isolated lake in central Germany that filled a circular depression formed by explosive volcanism (Brauer, A. et al. 2008. An abrupt wind shift in western Europe at the onset of the Younger Dryas cold period. Nature Geoscience, v. 1, 520-523). The seasonal sediment layers change in thickness, colour and mineralogy as warmth gave way to the frigidity of the Younger Dryas. One of the proxies, the iron content of the sediments deposited under anoxic conditions during winters fell significantly within a year at 12679 BP, along with a 4-5 fold increase in the rate of sediment deposition. Together with shifts in the lake biota, these features suggest to the authors that within a year wind strength increased greatly, probably due to a greater incidence of storm-force westerlies brought on by a change in the position of the jet stream. Today, westerly winds add to warming in northern Europe, around 12.7 ka they added to cooling, which can only be explained by global cooling or a southward excursion of sea ice in the North Atlantic.
Neither abrupt climate shift can be produced by validation of today’s climate models using actual data from the time just before they took place. It follows therefore that similar shifts in the near future could make themselves felt with no warning.
Opinion has drifted back and forth regarding the global effects of the Younger Dryas, evidence for its effects in the Southern Hemisphere being scanty. The best place to look for direct evidence would be in mid-latitude glaciers, especially where they are abundant in South America and New Zealand. A study of the largest of these, the Southern Patagonian Icefield (Ackert, R.P et al. 2008. Patagonian glacier response during the late glacial-Holocene transition. Science, v. 321, p. 392-395) indicates that the ice there advanced around the time of the YD. However, its dating indicates that the advance lay outside the 1300 year span of the cold period in the Northern Hemisphere. It was more likely due to a local response to increased precipitation from air moving from the east.
See also: Flückiger, J. 2008. Did you say “fast”? Science, v. 321, p. 650-651.
A 0.8 Ma history of changing greenhouse gases
July 2008
Polar ice cores have presented us with the most exquisite records of how high-latitude climate has changed in the recent past from indirect clues presented by variations in stable isotopes of oxygen and deuterium (temperature change), dust and sulfate content (aridity and volcanicity respectively) in layers of ice. That proxy record extends back to 800 ka in the Dome C core from Antarctica, showing in great detail the course of the last nine glacial-interglacial cycles, both the astronomical effect of a changeover from a 40 ka pacing to one of around 100 ka and many intricacies on a millennial time scale. The most tangible archive of information resides in the air bubbles trapped by the original snow that eventually turned into ice. That reveals how the intricate pacing of climate change has been almost perfectly tracked by the global carbon cycle as shown by changes in the concentrations of carbon dioxide and methane. This was first demonstrated by cores through the Greenland ice cap, which penetrate just the last glacial episode and the warmth before and after.
After several years of painstaking bubble analyses at many collaborating labs, the full 800 ka greenhouse-gas records from Antarctica have now appeared (Luthi, D. and 10 others 2008. High resolution carbon dioxide concentration record 650,000-800,000 years before present. Nature, v. 453, p. 379-382. Lulergue, L. and 9 others 2008. Orbital and millennial-scale features of atmospheric CH4 over the past 800,000 years. Nature, v. 453, p. 383-386). These long records demonstrate the close connection between climate and greenhouse gases that must be maintained by complex (and not fully understood) feedback mechanisms. Different Earth processes affect the two principal gases, methane probably being controlled by effects of varying temperature and rainfall on peat-rich swamps in the tropics, whereas carbon dioxide’s main driver is capture and release of carbon by the oceans. The central feature remains that of astronomical forces, with perhaps some sign of a signal from the 413 ka component of orbital eccentricity from a shift in the range of temperatures and greenhouse gases in 100 ka cycles around 450 ka ago, and a broad change in methane concentrations. Yet, despite being a pole away from high northern latitudes where comparison of the Greenland ice record with North Atlantic sea-floor sediment data revealed a northern cause for dramatic short term shifts, much the same millennial cycles characterise the whole Antarctic record. It could be that these rapid changes are proxies for the course of northern climate vagaries – there are about 75 of them in the methane Antarctic record. So stunning are the new data that they are sure to spur attempts to go back even further by more drilling in Antarctica, probably in the eastern ice cap where current air temperature and snow fall are extremely low and a greater length of time may be preserved in a smaller thickness of ice. That is because the faster snow and ice accumulate the more rapidly flow removes the record: the reason why the thick Greenland ice, although capable of yielding time resolution of as little as individual years, cannot retain records much beyond 200 ka.
See also: Brook, E. 2008. Windows on the greenhouse. Nature, v. 453, p. 291-292.
The yellowing of the Sahara
July 2008
As Earth emerged steadily from the last glacial maximum, around 14.8 ka when temperatures were close to those of the Holocene yet sea level still had a way to rise before reaching its current level, the Sahara became a land of wetlands, lakes and grassland. Many caves within its modern arid confines contain superb artwork depicting its fauna and the forager-hunters that preyed on it. Around the time of the earliest Pharaonic civilisation on the Nile floodplain (~3000 BCE) the humid episode ended, forcing inhabitants of the Sahara either to the Nile valley of the Mediterranean coast. Having spanned the millennium-long climatic upheaval of the Younger Dryas and the relative stability and warmth of the early Holocene, why it ended is something of a mystery. A small, amazingly beautiful lake in northern Chad seems to hold the key, as it has existed and gathered sediment for at least 6 thousand years (Kröpelin, S and 14 others 2008. Climate-driven ecosystem succession in the Sahara: the past 6000 years. Science, v. 320, p. 765-768), Lake Yoa is one of several permanent lakes fed by ancient groundwater from the vast Nubian Sandstone aquifer, yet receives negligible rainfall. The uppermost lake sediments are laminated in an annual fashion so that each layer and its contents of aquatic organisms, pollen and dust can be precisely dated.
Between 4200 and 3900 years ago the lake changed from a freshwater habitat to a salt lake when evaporation overcame recharge by rain. However, the environment as a whole did not change suddenly, but progressively. The sudden change in salinity resulted from Lake Yoa losing any outflow, which previously had removed salts accumulated by evaporation of the inflowing groundwater. The lake would then no longer have had any use for humans and their livestock, but conditions did not drive people out of the Sahara suddenly.
Impact cause for Younger Dryas draws flak
May 2008
Almost a year ago two dozen scientists presented evidence to suggest that onset of the Younger Dryas at 12.9 ka followed upper atmosphere explosions of cometary material (Firestone, R.B. and 25 others 2007. Evidence for an extraterrestrial impact 12,900 years ago that contributed to the megafaunal extinctions and the Younger Dryas cooling. Proceedings of the National Academy of Sciences of the United States of America, v. 104, 16016-16021; see Whizz-bang view of Younger Dryas in EPN July 2007). Evidence cited included: excess iridium; tiny spherules; fullerenes containing extraterrestrial helium; nanodiamonds and evidence for huge wildfires. Not quite the Full Monty, as neither crater nor shocked mineral grains were claimed, hence the teams’ opting for a cometary airburst. In North America such signs were said to overly the last known occurrences of Clovis tools at 7 archaeological sites (see Clovis First hypothesis dumped above). It was pretty clear that the suggestion for a hitherto unnoticed event with a widespread signature – 26 sites either side of the Atlantic were cited – was going to be challenged, and so it has (see Kerr, R.A. Experts find no evidence for a mammoth-killer impact. Science, v. 319, p. 1331-1332), perhaps not unconnected with the blaze of publicity surrounding the paper’s appearance, including several TV documentaries.
Well, say experts, sooty layers do suggest large-scale fires, but forest fires occur every year, especially when humans are around. Fullerenes or ‘buckyballs’ equally can form terrestrially, except those containing ET helium. The last is regarded by many critics as ‘inventive’; they have never been isolated since such combinations were first reported in 2001 (see Extinctions by impacts: smoking artillery in EPN March 2002). The accepted methodology for detection of tiny diamonds seems to have been ignored, and that claimed to have found them misused. The iridium ‘spike’ – crucial in identifying the global nature of the K-T event – by itself is not enough for claims of impacts. Astonishingly, the authors cited such a Younger Dryas iridium spike in a Greenland ice core, yet the originator of those data says his paper does not report abnormal iridium at 12.9 ka or anywhere during the YD. Microspherules rain down all the time with interplanetary dust, and do not constitute sound evidence either.
So, what on Earth is going on? A collaboration between 26 authors, who willingly supply other workers with materials for checking surely cannot be conspiring at a hoax. Impact experts are hinting at ‘over-enthusiasm’ by a team outside the ‘impact community’. It all sounds oddly similar to the furore that in 1980 greeted first suggestions by the Alvarezes for the K-T impact…
Neoproterozoic climate modelling supports a ‘slushball’ Earth
January 2008
Following its first discovery, evidence for low-latitude glacial action at several times during the Neoproterozoic has fuelled one of the most publicised controversies in the geosciences. Was the Earth totally frozen over during these episodes, or was ice confined only to parts of the surface? Whatever, the last part of the Precambrian witnessed huge fluctuations of many kinds, and after the cold epochs the first large animals made a sudden appearance. The most dramatic geochemical ups and downs in Earth history took place, in the form of sudden extreme shifts in the relative proportions of the stable isotopes of carbon in seawater, as recorded by marine carbonate rocks. These fluctuations correlate closely with the evidence for low-latitude glaciations: large negative excursions of d13C with glacial epochs, and positive values developing between them. The first can be interpreted as the result of massive declines in photosynthetic fixation of organic carbon. The second suggests repeated recoveries of such biological productivity, which favours the extraction of 12C from seawater and an increase in the relative proportion of the heavier isotope as organic carbon becomes buried in seafloor sediments.
Since organic carbon is ultimately extracted photosynthetically from carbon dioxide in the atmosphere, a link between climate and living processes (and those that bury dead organisms) can be the basis for models attempting to explain the extraordinary events of Neoproterozoic times. If large amounts of organic carbon are buried or remain suspended in the oceans, the drawdown of atmospheric CO2 reduces the greenhouse effect and leads to cooling. Conceivably, the effect could be to so reduce global mean surface temperature that freezing conditions grip even the lowest latitudes. Once glacial and sea ice becomes established, its high reflectivity reduces the amount of incoming solar radiation that is absorbed to warm the Earth. The two processes combined would tend to lock frigid conditions in place until such time as gradual release of volcanic CO2 increased the atmospheric greenhouse effect. That is the theoretical essence of the Snowball Earth hypothesis in which complete ice cover sterilised surface biology for long periods. However, it leaves out two important factors: as water cools it is able to dissolve more gases from the atmosphere; organic carbon in ocean water can be transformed to dissolved CO2 if it is oxidised, thereby reducing the amount of carbon being buried. Modelling the carbon-climate link in the Neoproterozoic requires that both factors are accounted for (Peltier et al. 2007. Snowball Earth prevention by dissolved organic carbon remineralization. Nature, v. 450, p. 813-818).
The model devised by Richard Peltier and colleagues from the University of Toronto also incorporates the distribution of land at the time. Results from it show a looping behaviour, with recovery from frigidity as increases in dissolved oxygen convert organic carbon to dissolved carbon dioxide, whose increasing concentration in turn leads to more escape of the gas to the atmosphere. The model also suggests how glacial and sea ice might have developed during such a cycle, and with the late Precambrian configuration of drifting continents it allows for low-latitude continental glaciation, but not for all-enveloping sea ice. The implication is indeed glacial events vastly greater than those of the late Palaeozoic and during the present Ice Age, but less effect on marine photosynthesis than from Snowball conditions – a ‘Slushball’ Peltier et al. explain why the cyclical processes suggested by the model stopped before the start of the Phanerozoic, from carbon-isotope evidence for a massive oxidation of suspended marine organic carbon around 550 Ma. Thereafter, abundant oxygen and large animals ensured most dead organic carbon was oxidised in the oceans.
Unsurprisingly, one of the authors of the Snowball hypothesis finds flaws in the geochemical argument for its impossibility (Kaufman, A.J. 2007. Slush find. Nature, v. 450, p. 807-808). Not only was oxygen likely to have been at far lower atmospheric concentrations than it became in the Phanerozoic, the glacial epochs provide evidence that its concentration in seawater was very low. The marine diamictites associated with each contain both ironstones and iron-oxide cements. For them to have formed demands high concentrations of dissolved iron in sea water, in the form of reduced Fe2+ ions; incompatible with widespread oxidizing conditions that would favour Fe3+ whose compounds are insoluble.
Some good news about carbon burial
January 2008
The second largest ‘sink’ for atmospheric CO2, after silicate weathering and formation of carbonate sediments, is the burial of organic carbon. Derived from photosynthesis of carbon dioxide in the air or dissolved in water, organic carbon descends from the photic zone of the oceans or is carried from the land by rivers. In the second case it is often believed that more than 70% of the carbon load of rivers is oxidised back to CO2 before having a chance of being buried in marine sediments. To estimate the proportion that does contribute to carbon sequestration is a complicated matter, involving measurement of the carbon budgeting for an entire river basin and its offshore sediments. This has been done by a team of French geochemists for the huge Ganges-Brahmaputra system that drains the northern Indian subcontinent and much of the Himalaya (Galy, V. et al. 2007. Efficient carbon burial in the Bengal fan sustained by the Himalayan erosional system. Nature, v. 450, p. 407-410). This system carries a stupendous load of sediment, especially during the monsoon season. At 1 to 2 billion t of sediment deposited from suspension in the Bay of Bengal each year, this is the largest single flux of sediment from land to the ocean floor. Even more is delivered as bed load (rolling and bouncing sand particles) to build up the Ganges-Brahmaputra delta of Bangladesh and West Bengal, India. The authors found that recently produced organic carbon is about 4 to 5 times more abundant in the suspended sediment load than is reworked fossil carbon derived by erosion of ancient sedimentary rocks, which itself is predominant in the bed load. Fossil carbon makes no difference to the modern carbon cycle, provided it does not get oxidised, which is less likely than for recent organic carbon in a form that can be metabolised.
By comparing the recent organic carbon load suspended in the rivers’ flow with that in the fine sediments of the Bengal Fan, Galy et al. have been able to show that most of that carbon is conserved without oxidation. As a result, the Bengal Fan accounts annually for about 15% of global carbon burial. There are two reasons for this remarkable efficiency: the low oxygen availability in deep waters of the Bay of Bengal; the very high sediment load from erosion of the Himalaya that buries carbon before oxidation is possible. Orogenic belts in humid areas are therefore key factors in exerting negative feedback on climate, whereas drainages of flat areas, such as the Amazon and especially its main tributary the Rio Negro, encourage oxidation in their lower reaches and offshore and are less important.
Cyclicity of Neoproterozoic glacial epochs
September 2007
The concept of ‘snowball’ conditions on Earth in the late Precambrian is that climate reached a state that drove it into semi-permanent frigidity, so encasing the globe in ice. The idea has been challenged by several lines of evidence since its first proposal in the late 1990s. Few authorities doubt that the Neoproterozoic was punctuated by several periods of extreme cold whose effects extended to tropical latitudes, but many reckon that climate never reached runaway ‘snowball’ conditions. It now seems that the glacial episodes had something in common with those of the Pleistocene, and exhibited cyclicity (Rieu, R. et al. 2007. Climatic cycles during a Neoproterozoic ‘snowball’ glacial epoch. Geology, v. 35, p. 299-302). The evidence comes from one of the youngest sequences of glacial and non-glacial sediments in the Neoproterozoic: the Fiq Formation in Oman. It is in the form of mineral and geochemical indices of alteration, based on the climate dependence of chemical weathering in the source area for sediments.
Both the chemical and mineralogical indices show considerable variation in the Fiq Formation, peaks and troughs in both data sets correlating well. There appear to have been three glacial-interglacial cycles. Troughs in the indices coincide with diamictites that contain dropstones and are usually interpreted as having been deposited partly from floating ice shelves. Peaks are found in mudstone and sandstone sequences that contain no evidence for glacial conditions. Unfortunately, the lack of precise dating rules out useful knowledge of cycle duration. An extremely crude estimate based on assumed deposition rates and the 200-500 m thickness of each cycle suggests far longer periods (1 to 5 Ma) than in the present glacial epoch.
The Fiq Formation is by no means the only Neoproterozoic sequence containing repeated diamictites. For instance, the 900 m thick Port Askaig Formation from the Dalradian of Scotland and Ireland contains around 30 diamictite horizons separated by non-glaciogenic siltstones and sandstones. Were those alternations to be shown to involve similar variations in indices of alteration, a similar crude estimate of cycle duration would be of the order of hundreds of ka; i.e. comparable with Pleistocene cycles.
See also: Lorentz, N.J. & Corsetti, F.A. 2007. Another test for snowball Earth. Geology, v. 35, p. 383-384
An early Greenland ice cap
May 2007
Around 34 Ma the oxygen isotopes in deep-water forams from ocean-floor cores show a jump towards more ‘heavy’ 18O. Together with the sudden appearance of coarse debris in oceanic sediments around Antarctica, the early Oligocene isotopic shift has been taken to represent the first sizeable build-up of land ice since the Carboniferous-Permian glacial epoch over 200 Ma earlier. It is also a marker for the later decline in overall surface temperature, culminating at 2.5 Ma with the onset of cyclical glaciation of high northern latitudes. This has to be revised after discovery of older ice-rafted debris in ocean-floor sediments in the North Atlantic between Greenland and Norway (Eldrett, J.S. et al. 2007. Continental ice in Greenland during the Eocene and Oligocene. Nature, v. 446, p. 176-179). The debris occurs in layers dated between 30 to 38 Ma. Direct evidence for cooling that supported ice-cap formation in both polar areas from the end of the Eocene is not matched by indirect evidence for the contemporary state of the global ‘greenhouse’. Proxy data suggest that the CO2 content of the atmosphere was around 7 times higher than in recent, pre-industrial times, falling dramatically in the middle Oligocene (~30 Ma) to about twice those in the Holocene, then slowly declining through the Neogene.
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Climate change and the penguin
March 2007
The Adélie penguin nests on rocky outcrops in coastal Antarctica. Because the climate is extremely dry, their nesting sites are rich in mummified remains. It would not occur to everyone to date penguin mummies (Emslie, S.D. et al . 2007. A 45,000 yr record of Adélie penguins and climate change in the Ross Sea, Antarctica. Geology, v. 35, p. 61-64), but since the Adélie, like all penguins, is oddly choosy it is a useful thing to try. Not only do Adélies demand dry sites, but they have to be within easy reach of open water during the nesting season. Abandoned sites are a proxy for those demands as they existed in the past. Emslie and colleagues were able to show that from 45 to 27 ka conditions for Adélies prevailed in the Ross Sea area, but penguins abandoned it until 8 ka, when they returned. Conditions did not suit them throughout the Holocene, however, and most modern colonies were established only in the last two millennia.
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Clear signs of a north-south climatic linkage
January 2007
The climate records obtained from cores through the ice cap of Greenland reveal so much because they enable very fine time-resolution. That is because it snows a lot in Greenland and the ice accumulation rate is high. The down-side is that Greenland 's glaciers move quickly and little more than the last glacial period (since 140 ka) is preserved. Antarctica is a great deal bigger than Greenland , and less water vapour reaches the accumulation zone of its ice cap. As a result, the record from Antarctic ice goes back much further, to 800 ka (see Yet further back in the Antarctic ice and Calibrating the deepest ice core, December 2005 and November 2006 issues of EPN). For most of the Antarctic cores the slow ice accumulation gives coarser time-resolution than available from Greenland . For the astronomically modulated long-term fluctuations in climate, that doesn't matter a great deal, but it poses a problem for understanding more rapid climate change that is bound up with the Earth system itself. Variations with periods of the order of a thousand years and less are products of atmospheric and oceanic circulation, in which climatologists expect different behaviour in the two hemispheres. An example is the thermohaline circulation of the North Atlantic, linked with the Gulf Stream . A widely held view is that the millennial variations in climate, which are such strong features in the record of the last glacial period, relate to periodic shutting down and restarting of the circulation, connected with changes in the salinity of the North Atlantic at high latitudes as ice sheets wax and wane. By delivering heat northwards, the North Atlantic thermohaline circulation may reduce available oceanic heat in the Southern Hemisphere: Greenland and Antarctica records should reveal whether or not there is a short-term ‘see-saw' effect on climate of the two hemispheres. The different time-resolutions have prevented that hypothesis from being confirmed or refuted. November 2006 saw publication of a much more detailed Antarctic record from closer to the Southern Ocean, in which 2500 m of ice represents 150 ka (EPICA Community Members 2006. One-to-one coupling of glacial climate variability in Greenland and Antarctica. Nature, v. 444, p. 195-198).
To splice the Greenland and Antarctic records together the EPICA team used the atmospheric methane record preserved in air bubble from both, calibrated to time using annual layering back to 41 ka and flow modelling for earlier periods. Indeed, there is evidence for the predicted ‘see-saw' between the hemispheres. As Greenland entered a cold stadial so Antarctica experienced a warming, and vice versa. That does not necessarily confirm a mechanism controlled by the North Atlantic thermohaline circulation: on a global scale its effect on heat transport is a lot less than processes involving atmospheric circulation. So there is a clear coupling, but also a need for a viable explanation. Interestingly, the enormous plunge back to almost full-glacial conditions in the Northern Hemisphere of the Younger Dryas (around 12 to 13 ka) still does not show up in the Antarctic record, even at a resolution of around 15 years for the new core.
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Calibrating the deepest ice core
November 2006
Although the ice that forms the upper parts of the Greenland and Antarctic ice sheets is annually layered, before about 70 ka the layering disappears because of plastic deformation. Earlier ages have to be estimated from models of the deformation, and a second check is to match the data records from ice cores against those from sea floor sediments. Different processes contribute to those records: for instance, the marine record of oxygen isotopes in benthonic forams tracks the changing volume of ice locked on land, while the same record from ice cores depends on the air temperature above the ice cap. The correlation does seem to work, however. But not, it seems, for the very deepest ice recovered from beneath Antarctica (see Yet further back in the Antarctic ice in the December 2005 issue of EPN) which extends to around 800 ka.
French scientists involved in the EPICA Dome C ice-core project have cunningly discovered a means of checking on the otherwise problematic deep Antarctic ice (Raisbeck, G.M. et al. 2006. 10Be evidence for the Matuyama-Brunhes geomagnetic reversal in the EPICA Dome C ice core. Nature, v. 444, p. 82-84). The core penetrated to an estimated time that should include the most recent magnetic reversal, dated very precisely to 778±2 ka. Although the exact details of how the magnetic field behaved during this reversal are unclear, it is known that when polarity flips the intensity of the field becomes very small. While the field is stable it is sufficiently strong to deflect charged particles, both in the solar wind and in cosmic rays, so that less pass through the atmosphere. Cosmic rays are so energetic that they can induce isotopic transformations, one product being 10Be. So if the magnetic field decreased so the proportion of 10Be in the atmosphere would go up. Raisbeck and colleagues have examined the EPICA core's 10Be record in great detail. In a 10 m thick section from a depth of almost 3.2 km the isotope rises to a peak, which they interpret as the signature of the reversal. If correct, this gives a `golden spike' against which the depth-to-age conversion can be refined.
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Balmy shores of the Precambrian
November 2006
Before the appearance of fossil organisms that could give clues to past climates the only sources of information are in the form of proxies. One of the best examples might seem to be the oxygen isotope composition of carbonate rocks that relate to sea-surface temperature. In fact it isn't useful for the Precambrian because estimates of SST depend on being able to identify the shells of planktonic animals and use their δ18O as a proxy. That is a pity, because limestones are common throughout the geological record and various aspects of their geochemistry have been used extensively as proxies for other crucial information, such as the relationship between their strontium isotope composition and the pace of continental weathering. Nonetheless, information about the mean temperature of all ocean water would be very useful. But a further problem is that many Precambrian limestones have been subject to alteration and perhaps changes in their oxygen isotope composition.
Another palaeothermometer also relies on the temperature-dependent fractionation of oxygen isotopes between seawater and silica that has precipitated from it to form cherts. In that case, the δ18O of chert decreases with temperature. The trouble is that silica is notoriously prone to being remobilised and reprecipitated as pH changes in the fluids within sedimentary rocks. Some Precambrian cherts gave such low δ18O that seawater temperature would have been tens of degrees higher than they were during the Phanerozoic. Such extraordinary results raise the suspicion of oxygen isotopes having been altered by warmer fluids passing through cherty sequences. Now the chert method has been given a boost by geochemists at the French National History Museum (Robert, F. & Chaussidon, M. 2006. A paleaotemperature curve for the Precambrian ocean based on silicon isotopes in cherts. Nature, v. 443, p. 969-972).
François Robert and Marc Chaussidon analysed the silicon isotopes in cherts for which oxygen isotope data are available. Since the two isotopic systems would both change, yet would behave differently during hydrothermal or metamorphic alteration, if the results correlate well both should be undisturbed. Except in samples that show the lowest δ18O values (i.e. highest temperatures) there is a good correlation. The finding validates many of the O-isotope seawater temperatures, but Si isotopes fractionate during precipitation too, again in relation to temperature. So Robert and Chaussidon take Precambrian ocean temperature data to a new level with estimates based on two methods. Their results are fascinating: as well as confirming a decline from around 70°C 3400 Ma ago to between 10 to 40°C in the Phanerozoic, the δ30Si data show sharp downward `spikes' at about 2500 Ma and 1800 Ma. From 1500 to 600 Ma ocean temperature seems steady at around 20°C, so there is no sign of continually cold oceans through the period of `Snowball Earth' events—the number of samples cannot yet resolve the individual events, but the `Cryogenian' is an obvious target for more work. The data are also important as they hint at all kinds of possible biological outcomes for such global warmth, and explanations are definitely needed. Does the record suggest greater geothermal heating, or was it an outcome of the greenhouse effect? Will more details correlate with periods of changing burial of organic carbon? Whatever, the Precambrian has become a stranger world to contemplate.
See also: de la Rocha, C.L. 2006. In hot water. Nature, v. 443, p. 920-921.
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Another blow for `Snowball Earth'
October 2006
The so-called Cryogenian Period of the Neoproterozoic rests on evidence for coincident glaciation at all latitudes. It has been supposed to include at least two, maybe three and perhaps more frigid `snowball' events, each with a pattern of lower diamictites and an upper carbonate cap rock. The most widely supposed glacial epochs are the Sturtian at 712 Ma, the Marinoan at 635 Ma and the Gaskiers at 580 Ma, but Precambrian sedimentary sequences are notoriously difficult to tie down in time. Only if dateable igneous events bracket evidence for glaciation is an age truly valid. Yet the global 3-fold division depends largely on correlation of stratigraphic and carbon-isotope sequences with the odd few that are dated in an absolute time-frame. The developing field of rhenium-osmium (Re-Os) radiometric dating offers a more universal check, since it provides a means of dating highly reduced black shales, that are abundant in the Neoproterozoic. The first reported results come as a blow to the `Snowball Earth' community (Kendall, B. et al. 2006. Re-Os geochronology of postglacial black shales in Australia: constraints on the timing of the `Sturtian' glaciation. Geology, v. 34, p. 729-732).
Bruce Kendall and colleagues from the Universities of Alberta, Canada and Durham, UK have constrained some of the principal occurrences of the Sturtian event in Australia to between 643 and 657 Ma, by dating the shales which envelop the diamictites and cap carbonates. They are younger than even the widest range previously suggested for the Sturtian: either the glaciation was grossly diachronous, or this is yet another glaciation of `Sturtian' type. The best that can be concluded is that the `Cryogenian' was cold but glaciation shifted from place to place – a `slushball' model?
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Pliocene climate and a lesson for the near future?
August 2006
While most geoscientists use the products of processes that operate today to judge environments of the past, climatologists do the reverse: the past is the key to the present. While the climate record of the last 2.5 Ma is a key to understanding and perhaps even predicting rapid climate shifts during glacial-interglacial periods uncontaminated by human influences, such is the extent to which greenhouse emissions have affected the current climate that we have little idea what the outcomes may be. The possibility of greenhouse warming has become higher than in any previous interglacial epoch. To get even an inkling of what that might set in motion requires looking back to warmer times than the Late Pliocene and Pleistocene, at around 3 to 5 Ma. In the Early Pliocene it is very likely that CO 2 in the atmosphere was no more than nowadays. Because the Earth's geography was little different from the way it is now and the Milankovich forcing was the same too, modelling Early Pliocene climate might seem to result in similar patterns, but it doesn't (Fedorov, A.V. et al. 2006. The Pliocene paradox (mechanisms for a permanent El Niño). Science , v. 312 , p. 1485-1489). Sea level was some 25 metres higher than it is at present and mean global temperature was an extra 3 ° C, and sea-surface temperatures (from the oxygen isotopes in planktonic foraminifera) were high as well. Despite much the same forcing factors as today, the Pliocene lacked large high-latitude ice caps in Arctic regions. Milankovich-related fluctuations were damped down compared with those of the Pleistocene. Both modelling and geological evidence from the Early Pliocene suggests that Earth's climate was dominated by a perpetual El Niño in the tropical oceans, because of an inability of cold water to upwell periodically along the western tropical margins of Africa and South America . Quite probably such conditions had persisted for the previous 50 Ma, despite gradual overall cooling.
Fedorov and colleagues point to very different Early Pliocene climates in several regions: Mild winters in central and north-eastern North America; droughts in Indonesia and torrential rains in western North and South America . Overall, it was a much more humid world, and since water vapour is a powerful greenhouse gas warmth and humidity were sustained despite no higher CO 2 levels than now. At about 3 Ma, ocean surface waters began to cool, with signs that the alternations associated with El Niño and La Niña in the eastern Pacific began. An explanation for this is the gradual build up of very cold water deep in the ocean as a result of winds from continents cooling ocean surface water at high latitudes and causing it to sink. Without periodic upwellings, warm surface waters and cold deep waters could not mix, so inevitably the interface became shallower. At some critical depth, this thermocline could break surface, transforming both climate patterns and those of ocean currents, eventually to end up as the present tropical climate cyclicity which is connected with other climate features of the Great Ice Age.
Fedorov et al speculate that only a small descent of the ocean thermocline – a matter of a few tens of metres – could re-establish Pliocene conditions. That might occur because of continued anthropogenic warming, and the `flip' might be as quick as a few decades to centuries.
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The Younger Dryas and the Flood
June 2006
Between about 12.9 and 11.5 ka the progress of warming from the frigidity of the Last Glacial Maximum was rudely interrupted. For over a thousand years conditions returned to those of a mini ice age, with continental glaciers re-advancing on a large scale, an increase in aridity and a reversal of colonisation of high northern latitudes by both plants and humans. Pollen records become dominated by those of a diminutive alpine plant, the mountain avens (Dryas octopetala) from which the cold snap gets its name – the Younger Dryas. The pace at which cooling took place was dramatic, and glacial conditions swept in within a decade at most. The most likely scenario is failure of North Atlantic Deep Water to form, thereby shutting down the thermohaline circulation that draws the warming Gulf Stream into the Arctic Ocean off the northern cape of Norway. The reason for that was a massive and sudden freshening of surface water at high latitudes in the North Atlantic, but where the influx of fresh water came from is a puzzle. Wallace Broeker of the Lamont-Doherty Earth Observatory in New York State resurrected an earlier idea that a vast lake of meltwater in the region of the Great Lakes of North America burst down the St Lawrence Seaway, instead of quietly escaping to the Gulf of Mexico along the Missouri-Mississippi system. Broeker has recently reviewed this hypothesis (Broeker, W.S. 2006. Was the Younger Dryas triggered by a flood? Science, v. 312, p. 1146-1148).
Oxygen isotope records from sediments in the Gulf of Mexico had been recording massive influx there of water depleted in 18O; a sure sign that the Mississippi was carrying much of the water produced by melting of the Laurentian ice sheet. That signature stops abruptly at the outset of the Younger Dryas. The meltwater must have found another outlet, but so far its oxygen isotope signature has not been conclusively discovered. As well as the St Lawrence escape route there are three other possibilities: north-westwards along the MacKenzie River valley; beneath the great ice sheet and through Hudson Bay; and by massive break-up of the ice sheet to launch an `armada' of icebergs that quickly melted to freshen northern Atlantic waters. One of the clearest signs that vast proglacial lakes suddenly emptied is that they carve immense channels resembling canyons, in which there is abundant evidence for extreme scouring. Examples are the `channelled scablands' of the state of Washington, and the Minnesota River valley. The volume escaping at the start of the Younger Dryas would have been so immense that such overflow channels would be dominant features of northern North America's terrain; but there are few that fit the bill, and those that do exist are poorly constrained by radiocarbon dating. The lack of accurate dates for sediments and channels associated with the demise of the Laurentian ice sheet is the main obstacle, and surely evidence for exactly how the sudden plunge into glacial conditions was triggered will emerge sooner rather than later. One thing seems certain, the Younger Dryas was a freak event. The new ice core from Antarctica (see Yet further back in the Antarctic ice in the December 2005 issue of EPN) penetrates the previous six glacial maxima and shows no sign of a similar event at their terminations.
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Sedimentary evolution of the Arctic Ocean: a start is made
For the Northern Hemisphere, especially around the North Atlantic, what happens in the Arctic exerts a strong influence over climate. On the one hand, ice-cover increases the proportion of solar energy that is reflected back to space, giving a cooling effect. On the other, cooling and increasing salinity of high-latitude water at the ocean surface results in its sinking to draw in warmer waters from further south, to extend warming further north. The two are linked intricately, for sea-ice formation adds to surface waters' salinity. How and when the delicate balances arose remained poorly known while thick sea ice prevented ships penetrating to the highest possible latitudes in the Arctic Ocean, because the key to climate evolution depends on access to long core through ocean-floor sediments. Ironically, the decrease in Arctic ice cover with global warming has created greater access by icebreakers and drilling vessels. A consortium of countries around the Arctic funded a major effort to resolve the gap in knowledge through such a marine drilling programme in 2004. Results from the polar expedition have just begun to emerge (Moran, K and 36 other 2006. The Cenozoic palaeoenvironment of the Arctic Ocean. Nature, v. 441, p. 601-605). The cores were taken almost at the North geographic pole on the Lomonosov Ridge, a sliver of continental crust separated from its connection with the northern Russian continental shelf when North Atlantic sea-floor spreading nosed into the Arctic about 57 Ma ago.
The core is from sediments deposited on the Lomonosov ridge since it became detached from Russia, and is over 400 m long. Analyses are not yet complete, and the report by the IODP Arctic Coring Expedition covers the simplest parameters to determine: sediment bulk density and lithology, and micro-organisms. Nonetheless, these preliminary results provide a major surprise. Previously it was believed that frigid conditions in northern polar regions became established long after the Antarctic developed an ice cap 43 Ma ago, which matches the Cenozoic fall in atmospheric CO2 and other evidence for lower mean global temperatures. The first glaciation in the Arctic was thought to be at 2-3 Ma, when pebbles dropped by icebergs first appear in the cores from the North Atlantic floor. In the Arctic Ocean core, such pebbles appear at much the same time as those around the Antarctic. They become widespread by 14 Ma. At the time of the Palaeocene-Eocene global warming, in response to massive methane emissions at 55 Ma, the Arctic waters were as warm as 18°C. The record is one of transition from a greenhouse world to an ice house. Surprisingly, considering the later influence of thermohaline processes that draw in warm water from lower latitudes, the earliest period is marked by fresh or at most slightly brackish waters. That was probably a result of isolation from the Atlantic and an excess of precipitation over evaporation. The early sediments record abundant carbon, then at around 14 Ma, the percentage of buried organic carbon drops dramatically to mark the start of increasing frigidity, when icebergs dropped significantly more debris in the Arctic Ocean.
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Yet further back in the Antarctic ice
December 2005
The groundbreaking Vostok ice core from Antarctica is the deepest ever to have been drilled. It recorded 440 ka of climate and atmospheric history, but unfortunately the very depth of the ice beneath the drilling station made that the limit in time terms. Thick ice begins to deform and flow, and the lowest parts of the Vostok core were clearly scrambled by that. The European Project for Ice Coring in Antarctica (EPICA) focussed its effort on a region of the East Antarctic ice sheet (Dome Concordia) whose location may always have ensured low accumulation of snow. Hopefully that would ensure that ice thickness was not so much as to result in complex flow at depth and that a fuller record would be preserved. The idea paid off, and the Dome C core penetrates back as far as 740 ka, giving an additional 3 glacial-interglacial cycles during the early part of the 100 ka periodicity; but falling just short of the first of those major cycles that are reflected in the marine oxygen-isotope record.
Results are now starting to emerge from Dome C (Siegenthaler, U and 10 others 2005. Stable carbon cycle-climate relationship during the Late Pleistocene. Science, v. 310, p. 1313-1317. Spahni, R. and 10 others 2005. Atmospheric methane and nitrous oxide of the Late Pleistocene from Antarctic ice cores. Science, v. 310, p. 1317-1321). The results are high-quality, and reveal some new features. The first three cycles conform to the 100 ka signal of the very weak variation in orbital eccentricity, as expected, but show lower amplitude shifts in CO2 and methane in air trapped in bubbles than do the later four cycles. The two `greenhouse' gases vary in concert, and their earlier low levels match with less extreme shifts in temperature as shown by the changes in deuterium content of the ice itself. This is probably due to the transition from the previous dominance by the 40 ka pace of changing axial tilt. Nitrous oxide values, although patchy down the core, seem to have fluctuated but at much the same amplitude throughout the last 720 00 ka. Dome C has yet to be `bottomed out' so there is a chance that the record may yet reach the 40-100 ka boundary around 900 ka ago. What is striking – and should ring alarm bells – from the results so far is that in each of the previous 7 interglacials atmospheric neither CO2 nor methane levels came close to those of the last century. Whatever its eventual effects, anthropogenic addition to the `greenhouse effect' is an incontrovertible fact.
See also: Brook, E.J. 2005. Tiny bubbles tell all. Science, v. 210, p. 1285-7
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Climate and the end-Permian extinction
October 2005
A time in Earth history (~251 Ma) when life was all but snuffed out and from which the creatures most familiar to us eventually emerged is understandably revisited quite often. Causes ranging from impacts (no convincing evidence as yet), through flood-basalt emissions, catastrophic methane release, low atmospheric oxygen to ocean anoxia have all been proposed. Hesitantly, opinion is converging on a climatic crisis of some kind, and indeed the coincidence of both terrestrial and marine faunal and flora extinctions points to climate being the global transmitter of some cause or a coincidence of causes. After the waning of Southern Hemisphere glaciations, the late Permian was warm, even at high latitudes. Until recently, attempts at modelling the end-Permian climate have not been entirely convincing because of limitations in the models themselves. Jeffrey Kiehl and Christine Shields of the US National Center for Atmospheric Research in Colorado have assembled a model that couples land, atmosphere, oceans, sea-ice and palaeogeography for the period (Kiehl, J.T. & Shields, C.A. 2005. Climate simulation of the latest Permian: Implications for mass extinction. Geology, v. 33, p. 757-760).
The critical test for the model is running it with parameters for the near-present, and it performs well. Several lines of evidence point to a much higher CO2 level in the Permian atmosphere, so this is the main input parameter. The outcome is a world with a mean surface temperature that is 8° C higher than now. Unlike today, there was no geographic hindrance to poleward heat transport, so the high mean temperature is reflected in the summer warmth and humidity of Permian high-latitude land. The sub–tropics on the other hand were scorching (around an average summer minimum of 51° C, 15° C higher than now); a clear contributor to minimising life there. Sea-surface temperatures at high latitudes are higher in the model outcomes, this warmth extending to depths of 3 km. Surprisingly, low-latitude sea temperature emerges as much the same as now. The model also suggests that seawater was saltier than now, and that results in greater uniformity of density with depth and location: a hindrance to bottomward circulation and mixing. There would probably have been no thermohaline circulation worth speaking of. The model helps confirm the likelihood of an oxygen-free lower ocean and little transfer of nutrients. The oceans too would have been inhospitable. A shutdown of biological productivity and therefore carbon burial would have accelerated warming. So, pushing the biosphere into a mass extinction would have been inevitable. The last straw may have been the additional stress of increasing acidity from sulphur dioxide emissions from the Siberian flood basalts.
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Milankovich forcing and Early Jurassic methane
October 2005
Periods of environmental crisis less severe than those leading to mass extinction appear throughout the fossil record. As well as minor extinction peaks they are often signified by departures of carbon-isotope records from long-lasting norms. Such a crisis appears in the d 13C record of the Early Jurassic, and is beautifully preserved in about 15 m of black shales on the North Yorkshire coast of England. Geoscientists from the Open University, UK and the University of Cologne, Germany have produced an extremely high-resolution time series of carbon-isotope data from the section (Kemp, D.B. et al. 2005. Astronomical pacing of methane release in the Early Jurassic period. Nature, v. 437, p. 396-399). The quality is sufficiently good to analyse the time series using Fourier analysis that yields the frequencies that contribute to the observed wave-like patterns in the data. Of course, the time in a stratigraphic time series is measured in metres, unless it is possible to calibrate the section by precise radiometric dating. The Yorkshire Jurassic contains only fossils and no dateable horizons, but the fine stratigraphic division based on ammonites is also widespread and calibration is possible from dates obtained elsewhere. The overwhelmingly dominant frequency in the carbon-isotope curve is 1.23 cycles m-1, which represents 21 ka after the calibration of depth to time. That is the signal of precession of the equinoxes, part of the astronomical forcing bound up in Miliutin Milankovich's theory of astronomical forcing of climate.
Astronomical pacing turns up throughout the stratigraphic column, wherever sediments are suitable for time-series analysis (steady, unbroken sedimentation), so a precessional signal is no great surprise. The important feature is the profundity of the d 13C excursions; a total of –7‰, largely accomplished by three abrupt shifts of –2 to –3‰. The first two coincide with bursts in extinctions. The most likely phenomenon to have produced these shifts is massive release of methane by destabilization of submarine gas hydrates. Emissions seem to have been blurting out on a regular basis as the Earth's rotational axis precessed like a gyroscope. So, the complete time period was one in which gas hydrate was unstable, probably due to overall warming. Yet something else must have triggered vast releases three times. The Lower Jurassic extinctions link in time with massive magmatism in Southern Africa and Antarctic (the Karoo-Ferrar large igneous province). Perhaps especially large volcanic events there set the stage for large precessional methane releases. An alternative view is that volcanic emissions of CO2 gradually produced enough widespread warming for the astronomical trigger to cause breakdown of gas hydrate simultaneously over very wide areas of the ocean floor. Other explanations have been suggested for the Lower Jurassic warming and carbon-isotope excursions, such as wildfires, impacts and connections with petroleum maturation and migration. The clear cyclicity rules them out.
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Documenting the Palaeogene transition from `hothouse' to `icehouse'
August 2005
It is well-established that the first large ice sheets that presaged descent into the oscillating climate of the Neogene formed about 34 Ma ago (the Eocene-Oligocene boundary) on Antarctica. Some 21 Ma before, at the Palaeocene-Eocene boundary, global temperatures had leaped following what many believe was a massive blurt of methane previously held in cold storage in ocean-floor sediments as gas hydrate. A monstrous `greenhouse' climatic system must sometime in the interim have reverted to the cooling trend begun at the outset of the Cenozoic. Defining that transformation relies on assembling and interpreting newly available, high-resolution records of climatic proxies through the Eocene and Early Oligocene (Tripati, A. et al. 2005. Eocene bipolar glaciation associated with global carbon cycle changes. Nature, v. 436, p. 341-346). Hitherto, the Eocene part of the ocean-floor sedimentary column had been poorly sampled, so that only broad trends showed.
As you might expect, the change was not a simple transition. At about 42 Ma the record of the Pacific Ocean calcite compensation depth (CCD – the depth at which carbonate remains are dissolved in the deep oceans) shows a remarkable perturbation long before the CCD dipped decisively from about 3.5 km to around 5 km at the start of the Oligocene. A close look at the oxygen isotope record of that age in a highly detailed marine sediment core shows an increase in d 18O that corresponds to either some 6° of cooling or a 120 m fall in sea-level due to build-up somewhere of ice on land. Coinciding with this perturbation are shifts in the carbon-isotope record in carbonates. The authors suggest that the mid-Eocene cooling and continental glaciation that produced falling sea level triggered the weathering of shallow-water carbonates, which together with river transport increased the oceans' alkalinity. That would have increased deep-water carbonate formation enormously and accelerated the effective `burial' of carbon from the atmosphere.
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Tracking ocean circulation during the last glacial period
May 2005
The use of various ocean-floor sediment proxies for climate change, such as the ups and downs of heavy 18O that chart waxing and waning continental ice cover, has progressively revealed the complexity of shifts during glacial and interglacial periods. Yet more emerged from finer-resolution time-series contained with Greenland and Antarctic ice cores. The diversity of information that proxy for many different, climate-related processes has in the last decade enabled palaeoclimatologists to begin piecing together possible causative mechanisms, beyond the initial discovery of an astronomical signal in early oxygen-isotope records. One of enormous significance is the possibility that sudden millennial-scale cooling and warming link to changes in ocean circulation, especially that performed by the Gulf Stream driven by thermohaline processes at high northern latitudes. Shutting down that poleward transfer of heat, probably because freshwater made high-latitude surface water less dense, has been implicated in sudden cooling or "stadials", and its restart linked to warming or "or interstadials". The last such sudden climate event, the Younger Dryas between about 12 and 11 thousand years ago, is widely believed to have resulted from a collapse of the Gulf Stream. That has raised fears that current anthropogenic warming might achieve the same thing, thereby plunging Western Europe into a counterintuitive frigid period through loss of its maritime warming.
Ocean circulation has lacked a proxy that might help resolve such worrying scenarios, but it seems that one has arrived, because of improvements in mass spectrometry (Piotrowski, A.M. et al. 2005. Temporal relationships of carbon cycling and ocean circulation at glacial boundaries. Science, v. 307, p. 1933-1938). Different bodies of ocean-surface water have subtly different chemical compositions, due to the varied geochemistry of surrounding landmasses. Weathering of exposed rocks results in some elements entering solution in river water, and that mixes with surface water in the nearby ocean. Among the most useful elements are those with an isotope to which radioactive decay of unstable isotopes of another element contributes. A good example is 87Sr that is formed when 87Rb decays. Where continents expose large expanses of very ancient rocks they contribute more 87Sr to seawater than do continents veneered with younger rocks. Strontium isotopes have been used successfully for charting very-long term changes in the overall erosion of continental crust, in relation to climate shifts, but being related to calcium are taken up quickly by carbonate secreting organisms, such as foraminifera, at many different levels in the ocean as it circulates. So they are not very useful for short-term studies. A more useful isotopic system involving an daughter of slow radioactive decay is that of neodymium, because it does not get taken up in this way. It does however enter the manganese minerals that slowly precipitate on the deep ocean floor. Moreover, its isotopic composition varies greatly in different ocean-water masses. Piotrowski et al. used neodymium isotopes from deep ocean cores to see if changes in this circulation proxy coincided with known climate proxies. For interstadial, warming events there is a match, so a Gulf-stream control over millennial-scale climate shifts is indeed supported. But for the start and end of the full glacial period control by ocean circulation did not happen. Instead, changes in the neodymium record lag behind the climate proxies, suggesting climatic control of circulation, which then "kicked in" to boost changes that were well underway.
See also: Kerr, R.A. 2005. Ocean flow amplified, not triggered, climate change. Science, v. 307, p. 1854.
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Snowball Earth gets a boost
May 2005
Since Paul Hoffman and others launched their hypothesis of successive Earth-enveloping glaciations during the Neoproterozoic Eon, that notion of "Snowball" conditions has received many severe knocks, charted by numerous items in EPN. Geochemists and geologists from the Universities of Vienna and Witwatersrand realised that a good test of the hypothesis would be to concentrate on a rather obvious property of an ice-bound planet (Bodiselitsch, B. et al. 2005. Estimating duration and intensity of Neoproterozoic Snowball glaciations from Ir anomalies. Science, v. 308. P. 239-242). Whatever falls on an ice sheet, whether it is cosmic dust from outside the Earth or ash from volcanoes, becomes trapped in the annual layers of ice. When the ice melts, that accumulated content is transferred to the oceans very quickly. With weathering in suspended animation during the glacial epoch, transport of many elements would have slowed to very low levels. So, marine sediments deposited immediately after the diamictites that are allegedly glaciogenic ought to contain anomalously high levels of several elements. The most important of these would be those which show very different abundance patterns in meteorites form those in terrestrial rocks.
Bodiselitsch et al. hit what seems to be "paydirt" in carbonates above a prominent diamictite in central Africa. Their samples are impeccable, being from diamond-drill cores produced during evaluation of sediment-hosted mineralization in the famous Neoproterozoic Copper Belt of Zambia and Congo. The core contains a prominent iridium anomaly at the very base of the carbonates, with a "signature" relative to other anomalous elements that points to a cosmic origin. Normally such an anomaly would be ascribed to a meteorite impact, but in this case the coincidence would be too good to be true. Instead, the authors use the magnitude of the anomaly to estimate how long cosmic dust had to accumulate to build up such a high level if it was released by rapid deglaciation. Deep-ocean sediments from the last 80 Ma are a guide to the long-term accumulation rate of cosmic material. If that rate is applied to the cap-carbonate anomaly, it gives a total time for accumulation in the hypothesised global ice cover of around 12 Ma. Presumably this would have been from ice immediately overlying the area being studied. An ice age that long defies any idea of more "normal", astronomically forced glaciation, which would be expected to have cyclically formed and receded many times, thereby releasing the dust particles much more gradually. Any anomalies would be expected in the diamictites themselves, yet there are none. Although sample spacing is rather patchy through the entire succession, they are most dense around the anomaly itself. Moreover, another suspected glaciogenic "package" higher in the sequence shows exactly the same iridium "spike".
Arguing against such support for the "Snowball Earth" hypothesis will be difficult, but other sequences require similar tests, most importantly those of Namibia, where Hoffman and colleagues developed their ideas, and the much more extensive deposits of Australia. This diamictite sequence is reckoned to represent both postulated deep-freeze events of the Neoproterozoic, around 710 Ma (Sturtian) and 635 Ma (Marinoan). There is one nagging problem. Data from one area are likely to record ice-retained cosmic dust only from ice in its immediate vicinity, and therefore do not represent the entire planet. Much of the controversy is between supporters of a whole-Earth ice cover, and those who favour patchy glaciation (the "Slushball" model). Unfortunately, Neoproterozoic stratigraphic correlation and radiometric age calibration is not sufficiently good to detect the same intervals elsewhere and look for anomalies there. In fact, the stratigraphy is generally correlated from place to place by matching the diamictites themselves. There is plenty of evidence that they may all coincide in time.
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Making sense of glacial-interglacial cycles?
April 2005
The competing periodicities of the three astronomical "drivers" of climate – orbital eccentricity (~100 ka), axial obliquity (~40 ka) and axial precession (~20 ka) – lie behind several models for the climate changes of the last 0.7 Ma. Taking in the theories that sway towards the influence of variables in the Earth system itself, around 30 models have some currency at present. Since climate forecasters have to take account of which factors drive climate in the absence of human emissions, as well as piece together their own particular models, it is easy to see how critics of global warming get a wide hearing: compared with creationists, they have it easy! Is there any way of resolving what is quite bluntly a theoretical mess? It is a mess simply because the available data are so complex, and in the case of both main sources, ocean-floor sediments and ice cores, not only are their devils in the detail, but there are whopping contradictions, such as the mismatches in timing between the Greenland and Antarctic ice cores. Add all the other sources, such as stalactites, tree rings etcetera, together with caveats like the difficulty in time calibration using 14C dating, and the volume of diverse records become bewildering.
It is tempting that a reversion to a statistical approach, that includes more bells and whistles than hitherto (see Evolutionary rhythms below), can resolve matters. Peter Huybers and Carl Wunch, of Woods Hole Oceanographic Institution and MIT, have tried that for pacing of the last 0.7 Ma of climate cycles (Huybers, P. * Wunsche, C. 2005. Obliquity pacing of the late Pleistocene glacial terminations. Nature, v. 434, p. 491-494). Generally accepted "wisdom" holds that the last 7 glacial-interglacial cycles are paced by ~100 ka eccentricity forcing, even though it has the weakest effect on solar heating, by a very long way. But there are smidgens of evidence for some interaction between that and the much stronger influence of changes in the Earth's axial tilt or obliquity. Huybers and Wunsch go for the Popperian rigor of first defining a null hypothesis, that obliquity has no effect, and then designing a test. It isn't easy to decide how the contrary hypothesis that it does can be evaluated though. The clearest features in all climate records are the ends of glacial epochs or termination: they are sudden, sharp and generally look the same. Most other features have some kind of pattern, but little consistent comparability. Using the most advanced statistical techniques, which employ many iterations to test for stability in statistical models, they can show that the null hypothesis fails. The positive result is that the time between terminations that are repeatedly modelled falls into two envelopes, around 120 and 80 ka, which simple arithmetic shows are divisible by 40 ka.
But how can axial obliquity only have an effect every two of three of its cycles, while a single cycle does not appear in the time-series; is it nature skipping beats somehow. One means that the authors suggest is that the underlying pace of eccentricity can effect the temperature at the base of ice sheets, depending on their thickness. If they are thin, then the heating is insufficient to trigger ice-sheet collapse because the base is very cold, whereas if ice is thick the effects of thermal conductivity and heat flow makes the ice base warmer and more subject to perturbation beyond its failure limit. It was at this point that I gave up, but wish the authors good luck in promoting their possibly unifying hypothesis for what finishes off glacial epochs…..
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Warming may have triggered Northern Hemisphere glaciation
February 2005
While I write this issue of EPN it is supposed to be early spring outside, and that is clearly what the ducks reckon as well – they are beginning to, er um, frolic. But there has been two weeks of snow and frost. Britain and the rest of Europe owe the frigid snap to cold air spilling westwards from northern Asia; the influence of the Siberian winter high-pressure area. Although somewhat lost in the recent kerfuffles about whether or not global warming is a fact or a misreading of data, the inevitable build up of mid-continental cold dense air in winter might have interesting consequences, should climate warm. Normally, areas far from the oceans remain dry as well as getting very cold through radiative heat loss in winter. When spring comes, such snow as there is soon disappears and the extremes of cold are replaced by surprisingly high summer temperatures, as anyone who has visited Siberia or Northern Canada will know. Should moist air find its way into such areas during winter, vastly more snow would fall. Its melting would take longer, and more solar radiation would be reflected back to space in spring. Such an albedo feedback could induce generalised cooling. Now evidence has emerged that the earliest known growth of land ice in North America was linked to warming of the ocean from which winds blew over it (Haug G.H. et al. 2005. North Pacific seasonality and the glaciation of North America 2.7 million years ago. Nature, v. 433, p. 821-825). In fact it is axiomatic that growth of continental ice sheets requires a supply of moisture and snow that exceeds the rate of summer melting and ablation, as well as cold winters.
Most theorising about the onset of Northern Hemisphere glaciation has centred on changes in North Atlantic circulation due to closures of the straits where the Isthmus of Panama now links North and South America, and the start of southward deep-water circulation from the latitude of Iceland. In fact both are known to have preceded the last Ice Age by a good 2 Ma. The actual start around 2.7 Ma coincided with an increase in obliquity of the Earth's orbit that would have led to periods with cold northern summers. Without abundant mid-continent snowfall, that in itself would not have set ice sheets forming in earnest. The multinational team of oceanographers studied sea-floor sediment cores from the sub-Arctic Pacific. To their surprise, sea-surface temperatures provided by evidence from planktonic organisms show evidence at 2.7 Ma for on the one hand cooling of the sea surface (from foraminifer oxygen isotopes) yet considerable warming on the other (from organic chemicals secreted by coccolithophores). Resolving this paradox requires a careful assessment of the ecological behaviour of the two groups of organisms. The authors' explanation involves the onset of density stratification in the North Pacific, so that the surface warmed quickly in summer, retaining warmth during autumn, and warmed slowly in spring from its minimum temperature. Both result from the high thermal inertia of water. The productivity of silica-secreting diatoms plummeted to a fifth of its earlier levels at 2.7 Ma as well, explained by ocean stratification reducing the supply of nutrients from deep water upwellings. Intuitively, a warm sea upwind of the North American continental interior should have generated high snowfall in late autumn and winter. Haug and colleagues modelled the contrasting effects of an ocean with water overturn and mixing with one that tends to become stratified, to simulate snowfall over the North American Arctic. From a situation in the Pliocene with snowfall over Greenland and the Arctic islands, the scenario shifts to heavy snow over the whole Arctic in the earliest Pleistocene. It seems that the trigger for the Great Ice Age was a hemisphere away from the "usual culprit", the North Atlantic, although its vagaries, once glacial cycles were underway, probably controlled the details thereafter.
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And was there a mighty wind?
January 2005
Readers will be familiar with the to-ing and fro-ing that surrounds the idea of Neoproterozoic Snowball Earth episodes from earlier issues of EPN. The leading proponent and sturdy defender of the hypothesis, Paul Hoffman of Harvard University, re-enters the fray as co-author of a paper that builds on the idea that following global glaciation the climate became not only very warm but also violent (Allen, P.A. & Hoffman, P.F. 2005. Extreme winds and waves in the aftermath of a Neoproterozoic glaciation. Nature, v. 433, p. 123-127). They document evidence from "cap carbonates" in northern Canada and Spitzbergen that succeed diamictites of "Marinoan" (~635 Ma) age, in the form of large-scale sedimentary structures. Many of these are submarine ripples with amplitudes up to 40 cm, and forms that suggest they were produced by sea-bed motion due to surface waves, down to 200-400 m, far deeper than modern storm-wave base. Central to their argument is hydrodynamic modelling of wind speeds that might have produced such large ripples, and their specific shapes – steep sided. Being based on experiment and observation of modern sea-bed processes, the theory seems quite rigorous. It retrodicts wave periods that are somewhat longer than those commonly seen in modern ocean storms. From that they derive sustained wind speeds that exceed 70 km per hour across open oceans, extraordinary by modern ocean wind standards.
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Torrid times in the Cretaceous Arctic
December 2004
Despite its latitude (above the Arctic Circle) the sedimentary depocentre of northern Alaska is becoming famous for its Cretaceous terrestrial flora and fauna. Plant remains indicate luxuriant vegetation cover, and high excitement greeted the discovery of 8 species of dinosaurs (4 herbivores and 4 theropod predators (Fiorillo, A.R. 2004. The dinosaurs of Arctic Alaska. Scientific American, v. 291(6), p. 60-67). How dinosaurs were able to survive the darkness of the Arctic winter is a bit of a mystery, unless the migrated as do modern caribou – Fiorillo cites evidence for small juveniles that would have been unlikely to have migrated far, because compared with adults they were much smaller than young caribou. There would have been sufficient winter biomass for survival during the Cretaceous, but seeing and being active as cold-blooded reptiles pose problems. At least one of the species had unusually large eyes, so one of the conditions for dinosaur's remaining year-round seems established. New data regarding climatic conditions in the far north have turned up after an most unusual and intrepid programme of drilling through a drifting island of pack ice over the Arctic Ocean's Alpha Ridge, not far short of the geographic North Pole. An extraordinary feature of the programme is that it took place between 1963-74, the core having only been examined in detail in the last year (Jenkyns, H.C. et al. 2004. High temperatures in the Late Cretaceous Arctic Ocean. Nature, v. 432, p. 888-892). The Late Cretaceous part of the cores is black mud rich in terrestrial vegetation remains and marine diatoms, and totally lacking in evidence for dropstones and other debris from floating ice shelves. Unfortunately, the Arctic sediments lack carbonate-shelled plankton remains, so the now standard method of sea-surface temperature measurement is not possible. However, Jenkyns et al. were able to use a method based on the fatty acids that survive in plankton membranes, results from which match oxygen-isotope palaeo-temperature measurements in Cretaceous cores from lower latitudes. Astonishingly, even at polar latitudes, the Cretaceous Arctic Ocean seems to have been as warm as 15 degrees C. Climate modelling based on lower latitude data and estimates of CO2 concentration in the Late Cretaceous atmosphere falls around 10 degrees short of these levels. The conventional modelling requires 3 to 6 times more "greenhouse" warming than generally accepted, to account for Arctic sea temperatures in which we could swim in moderate comfort. Possibly the modelling is awry. One of the most important features of Late Cretaceous palaeogeography was a major seaway across North America that connected the Arctic with tropical latitudes. It existed because global sea level was far higher than now, probably due to the oceans' volume having been substantially reduced by huge magmatic outpourings on the floor of the West Pacific basin (the Ontong-Java Plateau), earlier in Cretaceous times, together with higher rates of sea-floor spreading. The seaway would have been shallow, and thereby easily warmed. Had poleward currents been possible in it, their flow would have acted very like the modern Gulf Stream to warm high latitudes. Despite palaeoclimatologists reliance on models of heat circulation, it needs to be remembered that they are based on grossly simplified geographic features. If they get it very wrong indeed for the well-studied Cretaceous, that casts doubts on climate modelling's predictive powers for the course of current climate evolution.
See also: Poulsen, C.J. 2004. A balmy Arctic. Nature, v. 432, p. 814-815
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Update on the "Snowball"
November 2004
Two recent papers add weight to the "against" view expressed in For and against "Snowball Earth in EPN of October 2004" One gives age of 709 ± 5 Ma for tuff immediately beneath a supposed Sturtian diamictite from the western USA (Fanning, C.M & Link, P.K. 2004. U-Pb SHRIMP ages of Neoproterozoic (Sturtian) glaciogenic Pocatello Formation, southeastern Idaho. Geology, v. 32, p.881-884), which does not tally with the radiometric age (685 Ma) of similar rocks not far away. The other (Calver, C.R. et al. 2004. U-Pb zircon age constraints on late Neoproterozoic glaciation in Tasmania. Geology, v. 32, p.893-896), gives a 575 ± 3 Ma age for sills intruding a "Marinoan" diamictite in Tasmana, and 582 ± 4 Ma for a rhyodacite immediately beneath it. This suggests that these antipodean glaciogenic rocks are correlative with those in Newfoundland and Norway , that are supposedly representatives of the Varangerian glacial epoch. Yet the authors are pains to state that the Marinoan and the Varangerian are one and the same. Read these papers if you are still confused!
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How often did it rain?
September 2004
Geoscientists have become used to masses of climate data, often with better than 50 years resolution, from cores through ice sheets and sea-floor sediments. But all of it is from some kind of proxy; oxygen isotopes for air temperature and land-ice volume, methane for humidity, dust for windiness, and so forth. One aspect of both climate and the British obsession with weather is raininess, for which there is scant evidence. How many rainy days occur in a British summer is interesting, but for studies of past climate evidence for the onset or disappearance of seasonality, and the annual intensity and duration of rainfall would be invaluable, if it could be had. A piece of ingenious research shows that it is possible (Kano, A. et al. 2004. High-resolution records of rainfall events from clay bands in tufa. Geology, v. 32, p. 793-796). Akihiro Kano and Japanese colleagues studied the well-known layering of tufa – carbonate veneers laid down in freshwater that has high dissolved bicarbonate and calcium ions. In "hard-water" areas tufa can be deposited very quickly, at rates above a few millimetres per year, and it tends to be preserved, being quite tough. So tufas have the potential for preserving annual records of various fluctuations. Kano and colleagues saw that colour laminations represented clays deposited in the tufa when the water was turbid after prolonged rainfall. To record the variations they simply measured fluorescent X-rays emitted by silicon when slices of tufa were examined in an electron microprobe – silicon is present in clays and silt, but not in carbonate minerals. Because they used tufa deposited in recent times (1988-2002) they were able to correlate variations in clay content with detailed weather records from the site, thereby calibrating their method. The match was very good and followed rainfall closely at the level of a few days. Of 112 high rainfall days in the abnormally wet year of 1993, 100 showed up in the clay record. So, tufas are potentially more revealing than even the annual growth rings in wood, and some tufa deposits preserve long records.
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Details of the last interglacial climate
September 2004
Worries about how anthropogenic warming will affect the course of the Holocene interglacial in which we live might be tempered or exacerbated by knowing what went on during the previous, Eemian interglacial that ended about 120 ka ago. Data from cores through the Greenland and Antarctic ice sheets have been both ambiguous and plagued by resolution that does not show enough detail, but a core from a new position in Greenland seems to resolve both problems (North Greenland Ice Core Project members 2004. High-resolution record of Northern Hemisphere climate extending into the last interglacial period. Nature, v. 431, p. 147-151). Uniquely, the NGRIP ice still preserves the annual snow layering as far back as 123 ka. This is because the site shows little sign of the deformation at deep levels that characterised previous Greenland cores. That is probably because the site lies above a zone of high heat flow through the underlying crust, so that the base of the ice has melted. Melting helps prevent internal deformation, but that in itself is a surprise because the site was chosen because it is colder and drier at the surface than other sites. The drilling objective was to penetrate older ice than the Eemian to give a fuller record than from earlier cores, yet anticipated poor time resolution. The presence of resolvable annual records from depth was both a surprise and a bonus, although the melting had removed ice from the earliest part of the last interglacial. Despite that, preliminary oxygen-isotope results from the NGRIP core suggest that the Eemian had a remarkably stable climate and one that was warmer than that of the Holocene by about 5ºC; maybe it is an analogue for climate evolution during a future, artificially warmed world. That possibility stems from the observation that around 115 ka, North Atlantic climate suddenly warmed Thereafter, interglacial conditions did not suddenly change to glacial, as happened several times during the course of the last glacial epoch, but took around five millennia after the sudden warming. The authors make no claims that their preliminary data help resolve current fears of warming collapsing to glacial conditions in a matter of years to decades. That grim scenario has been widely trumpeted both by the media and some climate scientists. There is more to the Eemian than the period after 123 ka, and who knows what the eventual annual resolution will show up? The data presented in the paper are from a coarse sampling of 55 cm that represents about 40 year intervals.
See also: Kuffey, K.M. 2004. Into an ice age. Nature, v. 431, p. 133-134
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For and against "Snowball Earth"
September 2004
Reputedly glaciogenic sediments in the Neoproterozoic are reckoned to represent at least three separate cold episodes, the Sturtian (~720 Ma), Marinoan (~600 Ma) and Varangerian (~580 Ma). Sadly, the diamictites that characterise these episodes are not easily dated. Only two have well-defined radiometric ages, the Gubrah Member in the Oman (713 Ma), said to be Sturtian, and the Gaskiers Formation of Newfoundland (580 Ma), a possible example of the Varangerian that is better exposed in northern Norway. The truly whopping Sturtian and Marinoan diamictites of Australia are fitted to a global stratigraphy on the basis of carbon isotope variations, as are those of Namibia on which Paul Hoffman and colleagues stake their claims to "Snowball Earth" events. Another Hoffman, native to Namibia, and geochemists at MIT, have finally given a believable age to one of the Namibian diamictites (Hoffman, K.-H. et al 2004. U-Pb zircon dates from the Neoproterozoic Ghaub Formation, Namibia: constraints on Marinoan glaciation. Geology, v. 32, p. 817-820). Their zircons come from a thin volcanic ash within isolated Neoproterozoic diamictites in central Namibia, and yield an age of 636±1 Ma. Correlating the studied diamictites with the Namibian sequences elsewhere in the country relies on the presence of a supposed cap carbonate rather than lateral continuity. The authors link them with the younger of the two Namibian diamictites, the Ghaub Formation, rather than the Chuos Formation that lies at depth, despite the fact that both well-studied units are sometimes overlain by carbonate sediments. The conclusion is that the Ghaub is Marinoan, previously thought to be somewhere between 600 and 660 Ma. Interestingly, the new occurrence of diamictites is divided vertically by two thick sequences of volcanic lavas, neither of which have been dated by the authors.
One of the leading experts on what actually constitutes incontrovertible evidence for glacial sedimentation is Nicholas Eyles of the University of Toronto. He has become increasingly disenchanted with notions of Snowball conditions, on the basis of ambiguity in the very evidence said to signify them; diamictites with drop stones. He and Nicole Januszczac have assembled a monumental paper that counsels caution, and perhaps more (Eyles, N. & Januszczac, N. 2004. "Zipper-rift": a tectonic model for Neoproterozoic glaciations during breakup of Rodinia after 750 Ma. Earth-Science Reviews, v. 65, p. 1-73). Part of their argument rests on the very lack of robust ages for Neoproterozoic diamictites that prevents believable correlations from continent to continent. It is the globally synchronous nature assumed for these glaciations that gave rise to the "Snowball Earth" notion. The palaeomagnetic latitudes are often used to support this, but they are error prone both palaeogeographically and geochronologically. Accepting evidence for glaciation at low latitudes is no guarantee of support for even cold extremes, let alone an icebound world. Solar heating in the Neoproterozoic was lower than now, and so, therefore, would be the elevations at which glaciers might form at different latitudes. But the main problem is reconciling the features of many supposed glaciogenic diamictites with modern ideas of what truly constitutes evidence for glacial transport and deposition. Few of the units on which the "Snowball Earth" hypothesis is based stand up to modern scrutiny. Most of the diamictite packages occur in tectonically controlled basins, that were subject to episodic rifting. Each can be considered to form the base of a "tectonostratigraphic" cycle, and many show abundant evidence of having formed as mass flows from a shelf into the basin. They include olistostromes with huge rafts of carbonates likely to represent failure of carbonate platforms and huge submarine landslides, similar to those being discovered off many large islands today. The 750 to 580 Ma period was one of the most dramatic episodes of continental break-up in Earth's history as the Rodinia supercontinent was disassembled. Continental uplift, resulting either from mantle plume activity or rebound of rift shoulders, could have resulted in large areas rising above the ice limit, even at low latitudes in those cooler times. Those diamictites that are undoubtedly glaciogenic could easily have formed haphazardly in time. The carbon isotope record of immense shifts in δ13C during the Neoproterozoic, linked by some to repeated collapses and resurrections of life, might just as easily have occurred through efficient organic burial in active extensional basins and repeated major volcanism from plumes. Only evidence of timing will tell, and three good dates for "Snowball Earth" events are simply not enough.
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Influence of continental weathering on climate boosted
February 2004
Since the resurrection of Chamberlin's idea that the rate of chemical weathering of continental crust helps regulate atmospheric CO2 by Maureen Raymo, the hypothesis has not yet been supported by convincing geochemical evidence. There is such a lag between changes in ocean chemistry and evidence for global climate change, that correlations are flimsy. The need is for a proxy for weathering of the land surface that resides in seawater for a geologically very short period. Such an element is osmium (Os), which passes from river water through the oceans to sea-floor sediments in about 25 thousand years, so changes in its abundance in sediments ought to match the pace of any climatic shifts. In principle, there are two main sources for elements in seawater, from sea-floor hydrothermal alteration of oceanic crust, and from continental weathering. The first can be considered to be more or less constant, except on time scales of tens of million years. Continental weathering is a response to climate change, and keeps pace with it. Researchers at the UK Open University and the University of Köln in Germany analysed samples for osmium and carbon isotopes through a sequence of Jurassic mudstones on the NE coast of England (Cohen, A.S. et al. 2004. Osmium isotope evidence for the regulation of atmospheric CO2 by continental weathering. Geology, v. 32, p. 157-160). The carbon isotopes show a sudden drop in δ13C within a very hydrocarbon-rich unit famous for it contribution of jet (oil-rich lignite) to Victorian funereal jewellery. This negative excursion is recognisable world-wide at around 180 Ma. The most likely explanation is a monstrous blurt of methane from destabilised gas hydrate on the Jurassic sea floor (see Methane hydrate – more evidence for the ‘greenhouse' time bomb, August 2000 issue of EPN). The Jet Rock of the Whitby coast therefore preserves a nice example of sudden climatic change, and by the end of its deposition carbon isotopes returned to Jurassic background values. Methane, a powerful "greenhouse" gas, is rapidly oxidised to CO2 in the atmosphere, so reducing its initial warming effect, but climate would have been hotter for some time afterwards until the excess CO2 was drawn down somehow. Interestingly, the Jet Rock also shows a sudden leap in the abundance of 187Os, reflected in the 187Os/186Os ratio of the samples, and an upward step in the value of the 87Sr/86Sr ratio – one of the fastest rises known. The latter is generally assigned to an increase in continental weathering, since continental crust contains more radiogenic 87Sr than does oceanic crust. The implication of the osmium-isotopic shift is odd; it requires an increase in the rate of continental weathering by 4 to 8 times that in the preceding period. That is a vast change, even if it only lasted for a short period, but it tallies with what is known about the temperature dependence of the dissolved loads of rivers in more recent times. If the osmium isotope excursion truly reflects massive continental weathering, then it is possible to calculate the drawdown of the excess CO2 in the atmosphere from a commensurate flux of calcium and magnesium ions from the continents, that would eventually form marine carbonates. The authors estimate a mere 37-123 ka to get rid of it. Yet continent-derived radiogenic 87Sr remained high for much longer, and the authors' arguments become tricky. One interesting aside is that, unlike today, more groundwater found its way to the oceans than surface run-off during the Jurassic, perhaps 6 times more. It is easy to look on weathering as what happens at the interface between rocks and the weather; the land surface. Not so. A great deal of chemistry that releases soluble ions goes on in the subsurface, above and below the water table. It is by no means as simple as reactions between carbonic acid in rainwater and silicate minerals. Weathering is the product of hydrogen ions' (whatever their source) effects on silicates. Bacteria are extremely important actors in modifying pH below the surface, for example the sulphate-sulphide reducers, and the oxidative dissolution of sulphides produces sulphuric acid. Even more interesting for the chemistry of groundwater is the curious role of iron hydroxide. Under oxidising conditions it adsorbs many elements from solution, including platinum-group elements, such as osmium. Should conditions become reducing, dissolution of goethite skins on sedimentary grains releases the accumulated elements. A warming trend almost inevitably results in increased precipitation, and rising water tables. It also should boost biological productivity on land and an increase in the amount of buried organic matter, which create reducing conditions in groundwater.
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Collapse of the continental margin and methane release
January 2004
The vast reserves of peculiar methane-water ice deposits (gas hydrate or clathrate) in sea-floor sediments are the most likely source of methane releases that could generate sudden warming events, such as that at the end of the Palaeocene, and left traces in polar ice cores during the last few glacial-interglacial episodes. Methane probably leaks from the sea floor all the time, but is soon oxidised to the lesser "greenhouse" gas CO2 in the atmosphere, so muting its potential effects to a low background level. For methane to have a sizeable effect on global warming, lots of it has to blurt out suddenly. Possibly the only mechanism that can trigger such explosive releases are failures of sea-floor sediments, either by those beneath a steep surface slope collapsing under gravity, or as a result of seismicity. Geoscientists from University College London and the British Geological Survey have tried to correlate known peaks in atmospheric methane from the recent past (shown by ice cores) with episodes of mass flow on the seabed (Maslin, M. et al. 2004. Linking continental-slope failures and climate change: Testing the clathrate gun hypothesis. Geology, v. 32, p. 53-56). They found that the periods of greatest disturbance of continental-slope sediments over the last 45 ka took place at the tail-end of the last glaciation, between 13 and 15 ka and 8 to 11 ka. Each correlates with methane highs in the Greenlandic ice cores and with bouts of rapidly rising sea level (the Bølling-Ållerød and Preboreal warming periods). So they conclude that there is support for a "clathrate gun" model for sudden warming associated with glacial to interglacial transitions. However, seafloor collapses also correlate with Heinrich events (ice-sheet surges that launched iceberg "armadas" to low latitudes) that punctuated glacial times. These marked brief periods, repeating every 1000 years or so, which mark cooling when sea-levels were low. None are associated with upsurges in atmospheric methane., although the following interstadial warmings are. This lack of correlation rules out a "clathrate gun" influence on millennial-scale climate fluctuations during glaciations.
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Super-eruptions and climate
January 2004
The biggest known, young volcanic crater is that of Toba on Sumatra, which is a caldera complex measuring 30 x 100 km. Around 74 ka Toba emitted an eruption that dwarfed any in more recent times, and spread a dust cloud around the world – it is present in ice cores from Greenland, and has been linked with a cooling step during the onset of the last glaciation. It happened around the time that fully modern humans had begun to spread across Asia after migrating from NE Africa – an Acheulean hand-axe has been found in the Toba Tuff – and may have deeply affected those pioneering bands. There are older ash levels that can also be attributed to Toba eruptions, one found 2500 km away in the sediments of the South China Sea (Lee, M-Y. et al. 2004. First Toba supereruption revival. Geology, v. 32, p. 61-64) and at other sites up to 3000 km from Toba. This gives an age around 800 ka. Lee and colleagues from Academica Sinica (Taiwan), the National Taiwan University and the University of Rhode Island estimate that almost 1000 km3 of ash was expelled by the eruption. Unlike the 74 ka ash, this layer falls in the transition from a glaciation to an interglacial period; instead of a possible cooling influence through dust blocking solar heating, there is a warming trend. Although not quite as big as the 74 ka eruption of Toba, that of 800 ka is still vastly bigger than any other explosive volcanism during the Pleistocene. So, it suggests that super-eruptions are not significant climate triggers after all.
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High- and low-latitude climate changes almost match
October 2003
Ten years ago the records of climate proxies from the Greenland ice sheet set new benchmarks for understanding how climate has varied over the last 100 thousand years – annual ice layers allowed division of that data to as fine as decades. Variations in the ice cores helped explain many of the variations found in more blurred data from sea-floor sediment cores in the Northern Hemisphere. Variations could be correlated with changes in the formation of North Atlantic deep water at high latitudes and the destabilisation of North American and Scandinavian glaciers. The whole hemisphere behaved in concert, through long-distance connections in climatic processes, but high-latitude processes seemed to dominate. Development of 234U/230Th dating extended high precision to carbonates that have been precipitated from groundwater to form stalagmites or speleothem. The latest results from speleothem, collected on the Indian Ocean island of Socotra, cover 14 thousand years between 56 and 42 ka, and resolve down to only 8 year intervals (Burns, S.J. et al. 2003. Indian Ocean climate and an absolute chronology over Dansgaard/Oeschger events 9 to 13. Science, v. 301, p. 1365-1367). They show variations in rainfall on the island, though the δ18O proxy, and thus changes in the strength of the Indian Ocean monsoon. In terms of shape, the stalagmite record closely resembles δ18O changes in the Greenland ice cores, although the two have opposite senses, because the Greenland proxy is for air temperature above the ice cap. During the frigid Heinrich events that saw massive southward waves of icebergs, rainfall over Socotra was low. It became higher as high-latitude conditions warmed in Dansgaard-Oeschger events. The fine speleothem resolution shows a dramatic change-over that took only 25 years or so. The explanation is that warmer conditions increased equatorial evaporation from the oceans. But water vapour is the dominant "greenhouse" gas, and a wetter atmosphere would become warmer. So the question of whether low- or high latitudes drove the changes is still an open one. If North Atlantic events were the driver, then the tropical processes would greatly amplify their effects. One big problem emerges from the joint research by US, Swiss and Yemeni scientists. The highly reliable U/Th dating gives ages for each event that are about 3000 years older than those interpreted from the ice cores. The authors are convinced that the ice-core ages need revision, yet there are discrepancies with the event-ages from other similarly dated speleothems. Commenting on the paper, Frank Sirocko of Johannes Gutenberg University of Mainz in Germany (Sirocko, F. 2003. What drove past teleconnections. Science, v. 301, p. 1336-1337) makes the point that maybe the quality and age of ice core records lie behind the widely accepted view that high-latitude process drive climate. He presents an excellent global image of modern sea-surface temperatures that show the main oceanic shifts of energy – the leakage of cold circum-Antarctic waters northwards, the westward movement of equatorial warm waters to which the El Niño – Southern Oscillation (ENSO) is due, and the unique movement of warm water to Arctic regions in the North Atlantic that is connected to deep water formation. To that he adds the major effect of continental winter snow cover in central Eurasia, that affects albedo and the size of the winter high-pressure zone there. Is there a teleconnection between that and events in the North Atlantic? Nobody knows, because there are no data to compare, yet. Another uncharted but likely linkage is between the ENSO and processes in the circum-Antarctic current. Using currently accepted dating of ice cores, records from those in the Antarctic show air temperature changes that precede those from Greenland by several thousand years. In that respect, the Socotra record possibly has a link with the South Polar climate. Until the issue of dating is sorted out, it will always be difficult to make concrete statements about global climate change.
Interestingly, in the same issue of Science, sea-floor data (between 9 and 16 ka) from the Cariaco Basin off Venezuela, at about the same latitude as Socotra, mimic the Greenland records to within 30 to 90 years (Lea, D.W. et al, 2003. Synchroneity of tropical and high-latitude Atlantic temperatures over the last glacial termination. Science, v. 301, p. 1361-1364).
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"Greenhouse" controls challenged
October 2003
There's data gathering and there's theorising. In palaeoclimate studies the two come into conflict. Theory suggests that CO2 is likely to be the principal driver for climatic ups and downs, probably on all time scales. Atmospheric CO2 estimates from the past are based on proxies of different kind, and the various models that they support do not tally vary well. Worst of all they do not fit climate records through the Phanerozoic at all well, except in the crudest possible way. Only the long-lived Carboniferous to Permian "icehouse" and Tertiary cooling tally, and then only in Berner's GeocarbIII model. One of the best records of major climate shifts, aside from continental tillites, are marine sediments that contain ice-rafted debris, in particular the palaeolatitudes to which they extend. They record four major cooling episodes: Late Ordovician; Devonian to Late Permian; Late Jurassic to Mid Cretaceous; and those since about 35 Ma ago. The oxygen isotope record from Phanerozoic fossils, partly correlated with ocean temperatures also suggest 4 global coolings in the last 545 Ma. Either the CO2 modelling needs more detail, or the whole issue of the "greenhouse" effect is under question. That is the conclusion of a study by Nir Shaviv of the Hebrew University of Jerusalem, and Ján Veiser of the Ruhr University and The University of Ottawa (Shaviv, N.J. & Veiser, J. 2003. Celestial driver of Phanerozoic climate? GSA Today, Huly 2003, p. 4-10). Veiser has been analysing the chemistry of carbonates, especially their oxygen isotopes, for his 30 year career, and has amassed more data than any other geochemist on carbonate-related issues. The two have worked together because their interests fit together extremely well. Shaviv has reconstructed the variation of cosmic ray flux from studies of the exposure of iron meteorites to them, blended with analysis of how the Solar System moves through the spiral arms of our galaxy. Cosmic rays are known to affect the Earth's cloudiness and therefore albedo. Greater cosmic ray flux should increase the amount of solar energy reflected away by the Earth, thereby causing global cooling. The degree of fit between the cosmic ray flux and palaeoclimatic records is so good that up to 2/3 of climate variation may be connected with the Earth's celestial position. That is, as it passes through the star-rich spiral arms cosmic rays intensities go up. This happens every 140 Ma or so, which fits very well with the 4 icehouse periods during the Phanerozoic. They even suggest that the climate-CO2 relationship may be the opposite of that generally agreed; climate might drive carbon dioxide levels. A secondary role for "greenhouse" gases wreaks havoc on attempts at modelling climate change feared to result from increasing anthropogenic releases. Shaviv and Veiser's work comes at a particularly awkward time for climate modellers, who have just initiated a programme for running huge simulations by corralling the combined computing power of millions of home PC users, similar to the approach pioneered by the SETI Institute (Allen, M.R. Possible or probable. Nature, v. 425, p. 242). Perhaps the view of Phillip Stott, that climate modelling is a complete waste of time (Stott, P. 2003. You can't control the climate. New Scientist, 20 September 2003, p. 25) might sink in as a result of the possible link between cosmic ray flux and climates of the past. Stott believes that acting on the output of such models might perhaps even be dangerous, since we clearly do not understand short-term climate change well enough.
Precambrian CO2 levels
October 2003
Whether or not fluctuations in the "greenhouse" effect drive climate change, the fact remains that CO2, methane and water vapour all act to retain solar heat in the Earth system. Were it nor for their presence in the atmosphere, the Earth would be about 33 degrees colder than it is. It would be covered by ice. Theoretical modelling of how stars evolve suggests that the Sun had progressive less energy output going back in Earth's history. Only gaseous heat retention could have prevented a sterile, frigid planet. Yet periods of cooling sufficient to hold large amounts of water in surface ice have occurred only a few times, 4 in the Phanerozoic, a flurry of so-called "Snowball" epochs in the Neoproterozoic and the earliest known glaciation around 2200 Ma ago. The earliest coincided with the first evidence for free oxygen in the atmosphere, and may have been caused by that. Methane, a more powerful "greenhouse" gas than water or carbon dioxide and abundantly produced by anaerobic decay, is easily oxidised. In later time, it has been ephemeral in the atmosphere, unless continuously released, for instance by destabilisation of gas hydrate in sea-floor sediments. Warming by CO2 has undoubtedly kept total frigidity at bay since then. The problem is charting just how much was in the air, because most estimates have been based on studies of palaeosols that give odd and very imprecise results for the early Palaeozoic (see Shaviv and Veiser, 2003; previous item).
Photosynthetic organisms derived their carbon from CO2, either in the air or dissolved in water through equilibration with the atmosphere. The extraction favours lighter 12C, so biological activity results in their products being depleted in the heavier 13C by about 25 parts per thousand (‰) relative to carbon in air and water. If organic carbon becomes buried, the remaining carbon in the surface environment gets richer in 13C, and that signature becomes fixed in contemporaneous carbonates, both organic and inorganic. It is therefore possible to use the two carbon-isotope signatures to estimate the reservoir of CO2; its proportion in contemporary air. However, the degree of fractionation depends on the specific carbon metabolism of different organisms, yet most organic carbon in sediments is a mixed product of widely differing life styles. That severely blurs estimates of atmospheric carbon dioxide content. What is needed are data from a single source with known metabolism. Acritarchs are fossil remains of single-celled marine eukaryotes that were, and still are, marine photosynthesisers. They are made of degraded hydrocarbons. Advanced ion-microprobe resolution is now sufficient to produce carbon-isotope measurements of individual fossils (about 200 micrometres across). Sediments from northern China, roughly 1400 Ma old, contain abundant little-altered acritarchs and carbon isotope data from them give good estimates of atmospheric CO2 levels, that are independent of other methods (Kauffman, A.J. & Xiao, S. 2003. High CO2 levels in the Proterozoic atmosphere estimated from analyses of individual microfossils. Nature, v. 425, p. 279-282). The estimates suggest between 10 to 200 times higher contents than today, but just about sufficient to keep the Earth above the limit of glacial temperatures when solar luminosity was about 88% of the present. Acritarchs are present throughout the Neoproterozoic, and it should prove possible to examine the critical periods of "Snowball" conditions using this method.
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Iron isotopes and ocean evolution
August 2003
The main driver for biological activity in the oceans far from land is the availability of iron, and this helps control the burial of organic carbon and hence aspects of global climate. At low Fe concentrations, as they have been since the oxygenation of the surface environment from 2 billion years ago, iron is cycled in the marine environment in a matter of a few hundred years. So, ocean water responds very quickly, in geological terms, to changes in the source of any dissolved iron. There are two main sources, discharge of hydrothermal fluids from the oceanic lithosphere and delivery of river water and dust derived from the continents. Of the last, riverine sources probably end up in near-shore sediments and only dust contributes significantly to deep ocean water. The slowly growing nodules and crusts, composed mainly of iron and manganese compounds, on the ocean floor can chart variations in the relative proportions of these sources, because their growth produces zonation. Measurements of δ56Fe in various materials show that the two sources are different in isotopic composition (Beard, B.L. et al. 2003. Iron isotope constrains on Fe cycling and mass balance in oxygenated Earth oceans. Geology, v. 31, p. 629-632). While continent derived materials exude iron that is essentially the same as that in terrestrial volcanic rocks (δ56Fe ~0.0‰), ocean-floor hydrothermal activity is significantly depleted in 56Fe (‰56Fe ~ -0.38‰). From 6 Ma to 1.7 Ma iron-manganese crusts record iron with a dominant hydrothermal origin, but during the glaciation-dominated period since 1.7 Ma the contribution of continent-derived dusts becomes overwhelming – cooling forces drying on a global scale. Because hydrothermal contributions probably stay much the same over very long periods, because of the sluggishness of plate tectonics, iron isotopes in deep marine sediments, such as Fe-Mn crusts, may be important tracers for glacial events in the distant past, such as the glaciations during the Neoproterozoic and Palaeozoic. Interestingly, the largest iron-rich deposits on the planet, the BIFs that peaked during Archaean and Palaeoproterozoic times, record far larger excursions in iron isotopes than any other. The very low δ56Fe values of some BIFs (down to – 2.4‰) probably signify the dominance of sea-floor sources, although a non-oxidising atmosphere would have mobilised dissolved iron from the continents too, which explains the range in BIFs up to +1.0‰.
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The gas-hydrate "gun"
July 2003
As fears of anthropogenic climate warming have risen, so more geoscientists have looked in detail at the stratigraphic record for signs of past warming, and funds have become more targeted towards palaeoclimatology. One of the most important discoveries was that the end of the Palaeocene, about 55 Ma ago, was a time of sudden global warming during the overall cooling that has characterised the Cenozoic. The first sign that something strange had happened then came from using the oxygen isotope geothermometer on plankton tests from marine drill core that passed through the boundary. There seemed to have been a 7º C jump in surface seawater temperature. An explanation for the thermal spike arose after carbon isotopes revealed a coincident spike in the lighter 12C. Periods of low primary biological production can impose such anomalies, because photosynthesis selectively binds light carbon in carbohydrate. However, some of that light carbon ends up buried in sea-floor sediments, so another explanation for a negative excursion in δ13C is that organic carbon has somehow been released from sedimentary storage to the atmosphere. So, either there was a sterile ocean or a massive release of organic carbon at the Palaeocene/Eocene boundary. Some kind of erosion to achieve the second possibility could not have led to such a speedy shift in carbon isotopes. The accepted explanation, suggested in 1995, stemmed from organic carbon that had been metabolised by methanogen bacteria in anaerobic sea-floor sediments to form methane. Given low enough sea-bottom temperatures and sufficient pressure, methane can crystallise with water to form an icy substance, known as gas-hydrate or clathrate, in sea-floor sediments. Being an unstable compound, gas hydrate can break down rapidly if seafloor temperature rises or sea-level falls. And, of course, the methane can rush to the surface as bubbles. Being 4 times more efficient than carbon dioxide at trapping thermal radiation emitted by the Earth's surface, methane releases are excellent explanations for sudden warmings in the stratigraphic record. And there is a great deal of methane locked as gas hydrate beneath the sea floor, about 2 teratonnes (2 x 1012 t). Quirin Schiermeier reviews the basic concept (Scheiermeier, Q. 2003. Nature, v. 423, p. 681-682), but poses the question of how methane-induced warming is reversed. Methane is quickly oxidised to CO2 in the atmosphere, so lessening its warming effect. So a "spike" that lasts thousands of years has to be fed by continual releases. Since warming drives gas hydrate breakdown, something must intervene to stop the releases before the warming becomes a "runaway greenhouse". One view, and probably the correct one, is that warmth and more CO2 drives up biological activity so that the increased atmospheric carbon is "pumped" down by living processes, back to sedimentary burial. If sufficient nutrients are available, there is no way of stopping this negative feedback until a balance is restored. Schiermeier reports that new ocean drilling plans to test the hypothesis that the Palaeocene/Eocene warming accelerated continental erosion, which was able to wash the crucial nutrients phosphorus and iron into the oceans. Experiments have shown that increased iron in ocean-surface water far from land – now pretty sterile because it is iron-deficient – sparks up photosynthetic plankton. That is one possible way of artificially drawing down anthropogenic CO2. The problem is, if such a process was involved in cooling the Eocene Earth, it took about 100 thousand years.
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Red Sea record links to northern hemisphere climate
July 2003
In his forthcoming book, Out of Eden: the Peopling of the World (Constable and Robinson, July 2003), Stephen Oppenheimer offers the novel suggestion that fully modern humans left Africa by island hopping on log rafts across the Straits of Bab el Mandab, which connects the Red Sea to the Indian Ocean. The rationale to his suggestion is that sea-level falls during major glaciations would have partially exposed the shelf that lies beneath the Straits, presenting a route to SW Arabia across only 18 km of island-dotted sea. As today, it would have been impossible to trek across the deserts of the Middle East after a northward African migration along the Nile, without chains of wells. His thesis then sees humans migrating along coasts eventually to reach east Asia at about 70 ka. Precisely when the Straits of Bab el Mandab became shallow enough would have been determined by global climatic conditions, for only glacial maxima result in sufficient sea-level falls for such island hopping to be possible.
The shallowing of the shelf across the southern outlet of the Red Sea would have had a profound impact on seawater circulation. Already having restricted connection to the world's oceans, Red Sea water has elevated 18O levels, because evaporation from it favours loss of lighter 16O. With more restricted circulation, evaporation would have driven this up further. Geoscientists from the Universities of Southampton, Tuebingen and Göttingen, and the Geological Survey of Israel have analysed the variation in oxygen isotopes of foraminifera from a Red Sea core to quantify ups and downs in sea level in more detail than possible from open-ocean cores, which have uncertainties of about ±30m) (Siddall, M. and 6 others 2003. Sea-level fluctuations during the last glacial cycle. Nature, v. 423, p. 853-858). The method that they used models the effects on Red Sea oxygen isotopes of evaporation and changed circulation to estimate how the depth of the Straits of Bab el Mandab changed. They claim a precision of ±12m. Through the period from 70 to 20 ka, leading up to the last glacial maximum, their sea-level record tallies nicely with climate records from both Antarctic and Greenland ice cores, including shifts linked to the short-lived Heinrich and Dansgaard-Oeschger cycles. During the last glacial maximum(18-20 ka), sea-level fell by almost 120 m, so that the Straits of Bab el Mandab were on average only 15 m deep. The first human Exodus out of Africa to populate Eurasia would have been between 120 to 130 ka, as suggested by Oppenheimer, when sea level probably fell a little further. However, at about 65 ka, sea level dropped to about 100 m below modern levels, perhaps presenting another window of opportunity.
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Broecker reviews climate triggers
July 2003
Wallace Broecker, of the Lamont-Doherty Earth Observatory at Columbia University, was the first to quantify in 1975 the 19th century prediction of Svante Arrhenius that increasing atmospheric carbon dioxide would drive up global temperatures. Broecker's early work lies at the centre of concern about global warming, and his subsequent contributions are enmeshed with the entire study of past climate change. A review by him of current ideas on palaeoclimates of the recent past is therefore compulsory reading, for all geoscientists (Broecker, W.S. 2003. Does the trigger for abrupt climate change reside in the ocean or in the atmosphere? Science, v. 300, p. 1519-1522. As well as the astronomically connected cyclicity that is apparent in all kinds of climate record through the Pleistocene, those records are punctuated by sudden, short-lived phenomena, whose magnitudes and pace are sufficiently dramatic to focus attention on processes that are probably entirely terrestrial. Foremost among these during the last glacial interglacial cycle are the astonishing coolings of Heinrich's iceberg armada events and the possibly catastrophic (in a human as well as an ecological sense) Younger Dryas, which reversed warming from the last Glacial Maximum, and the equally sudden warmings associated with Dansgaard-Oeschger events. Broecker's review focuses on the two mechanisms that have been suggested to underlie these overturns. One links such changes to shifts in whole-ocean water circulation, especially the ons and offs of deep-water circulation beneath the North Atlantic, the other to perturbations of the way in which atmosphere and ocean interact in the tropics.
An entirely plausible scenario for climate-driving changes in North Atlantic water circulation is flushes of freshwater from the surrounding continents, so that formation of sea ice leaves residual water that is not saline or dense enough to sink and drag in water from lower latitudes. The problem is that the complete thermohaline cycle, which impacts on global atmospheric circulation, has a period longer than the changes that might be induced by its perturbation in the North Atlantic. Tropical atmosphere-ocean dynamics are the largest elements in global climate, in terms of the energy and mass that are shifted, so they are a natural candidate for a driving mechanism. Tropical climate shifts abruptly today in well-known ways, most important being the El Niño-La Niña cycle. There is no ponderous underlying dynamic that would damp down connections between cause and global effect, and prevent sudden climate change. Yet, some kind of "flywheel" is essential to keep long-term cyclicity going and lock sudden changes into century to millennium-long climate "states", which should rapidly decay if effect rebounded on cause, as it does in the case of El Niño-La Niña. Broecker covers all the critical evidence that has borne on both hypotheses up to now. His conclusion is interesting. Both hypotheses are very much model led, and in need of as much empirical support as can be had. Yet, and here is the nub, the crucial data are those bearing on correlating times of events that are recognised all over the place. Time resolution is of the greatest importance, since climate transitions are fast; faster in fact than we can presently resolve before historical times. It is entirely likely that suitable resolution of times past may be absolutely impossible. Both hypotheses have a lot of empirical and theoretical support. So, what is the problem of combining them in a cunning way? Partly, that may be because reductionism (controlling a few variables and looking for developments in another simple set) still plagues science. That is odd in climatology, where all motions and energy changes palpably relate to one another, with no control of a rational kind. Reductionism demands ever more staggering computing power and speed, to "keep all the eggs in the air". There is always the feeling, as Jimmy "Shnozzle" Durante observed in his musical monologue, The Man Who Found The Lost Chord, that if you find a hitherto overlooked connection, then everything goes well; if you can remember it! Broecker suggests that the missing connection must "transmit" from deep ocean water to tropical atmosphere.
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No glacial refugia in the Amazon Basin?
May 2003
Tropical rainforest in Africa and South America is the most diverse biome on the planet, both as regards plants and animals. One view of how such luxuriance arose is that the forests have blanketed the humid tropics for as long as 50 or 60 million years, and the fact that they encompass a huge variety of environments created by different levels in the dominant and diverse vegetation. Thousands of niches and the interactions between organisms that exploit them during lengthy stasis inevitably drives rapid evolution towards all kinds of specialisation. The other view is that rainforests are by no means static over millions of years, but climate shifts have caused them to retreat and advance, perhaps hundreds of times during the Cenozoic. Amazonia in particular shows surprising variation in diversity, some patches being far more biologically rich than others, and having regionally distinct assemblages of plants and animals. This theory suggests that climatic stress, probably drying associated with globally cool episodes, resulted in rainforest shrinking to "refugia". In them, populations of plants and animals shrank, thereby reducing the gene pool and giving greater chance for evolution by natural selection; different in different refuge areas.
Tropical soils are continually reworked and their highly oxidising nature destroys organic remains. So no record of its development exists in rainforest. However, wind and rivers transport spores, pollen and other biomarkers to seafloor sediments, where a complete record of fluctuations in biomass and diversity becomes preserved. A test of the popular refugia hypothesis is therefore to analyse organic matter in continuous cores taken from offshore sediment. Known fluctuations in global climate, from the oxygen isotope record should be matched by changes in the record of terrestrial biomarkers carried to the sea. Cores from the deep-sea sediment fan off the mouth of the Amazon potentially provide such a test (Kastner, T.P. & Goñi, M.A. 2003. Constancy in the vegetation of the Amazon Basin during the late Pleistocene: Evidence from the organic matter composition of Amazon deep sea fan sediments. Geology, v. 31, p. 291-294). Kastner and Goñi, from the University of South Carolina, examined phenols and organic acids in the cores, which can discriminate between grassy plants and trees that would have dominated savannah and rainforest, whose relative cover of the Amazon basin should have changed, according to the refugia hypothesis, as climate shifted from globally cool-dry to warm-humid.. Although their record only spans the last glacial cycle since 70 ka, they detected no significant change in the proportion of grasses and trees in the Amazon catchment. Moreover, the biomarkers remained similar to those carried by the Amazon today, right through the last glacial maximum, when drying of the tropics would have been most likely to have driven a shrinkage of rainforest area. It seems unlikely that forest refugia developed during one of the most extreme climate shifts in the last 55 Ma. Global climate fluctuations were considerably less before 1 million years ago, when the current round of 100 ka cycles began. So there is little reason to doubt that the Amazon rainforest has had a more or less constant area for much of the Cenozoic. The same cannot be said for those in Africa and SE Asia, partly because there are no useful data from offshore sediments, but also because those regions have experienced changing topography due to major tectonic activity, whereas eastern South America has remained stable. To conclude, as the authors do, that the data signify no great fluctuation in rainfall is not so certain.
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Antarctic melting and northern hemisphere deglaciation
April 2003
There is a large body of opinion, supported by plenty of circumstantial evidence, that the end of the last glacial maximum around 20 ka was controlled by processes that operated in the North Atlantic and its seaboard. A favoured mechanism is the re-establishment of thermohaline circulation involving North Atlantic deep water that dragged surface water northwards from the tropics, to set up the Gulf Stream. Temporary shut-down of thermohaline flux, probably by massive release of freshwater to the North Atlantic from melting of ice sheets, is widely understood to have triggered the sudden reversal to frigid conditions in the Younger Dryas around 11.5 ka. The largest warming pulse in the northern hemisphere, between 14.6 to 14.0 ka, is recorded by a sudden increase in δ18O of ice in the Greenland cores, and is known as the Bølling-Allerød warm interval. Around that time, sea level rose by 20 m in a few hundred years, and that involved production of fresh glacial meltwater at a rate equivalent to the continual flow of five rivers the size of the Amazon. Such rapid sea-level rise drowned coastlines and in some areas killed coral reefs. On such drowned reef in the Caribbean gave a date of 14.2 ka, which since 1989 has been the only indicator of precise timing for the massive influx of meltwater to the oceans. The date is within the Bølling-Allerød, hence the link between warming and events around the North Atlantic. That central hypothesis is now under threat, following the dating of drowned coral reefs on the Sunda Shelf at 14.7 ka, and a re-evaluation of the Caribbean data. (Weaver, A.J. et al. 2003. Meltwater pulse 1A from Antarctica as a trigger of the Bølling-Allerød warm interval. Science, v. 299, p. 1709-1713).
Using the revised ages and climate modelling, Andrew Weaver and colleagues from the Universities of Victoria and Toronto, Canada and Oregon State University see the massive ice-melting as the precursor to the Bølling-Allerød warm interval and deglaciation of lands around the North Atlantic. A more plausible source of freshwater influx is a major melting event in Antarctica, so warming in the south may well have driven that of the northern hemisphere.
See also: Kerr, R.A. 2003. Who pushed whom out of the last ice age. Science, v. 299, p. 1645.
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When did southern Tibet get so high?
March 2003
For about a decade it has been suggested that the Tibetan Plateau, which rises to more than 5000 metres, has a profound effect on climate. This may be partly due to the way such a high and enormous area deflects regional wind patterns, but largely to its profound interconnection with the South Asian monsoon. When such a circulation barrier arose is critical to understanding how it relates to climate evolution in the latter part of the Cenozoic. There are various suggestions, based on aspects of its structural and magmatic evolution. Theory suggests that the southern part came into being in Eocene times, possibly because a segment of the lithosphere beneath broke off to subside into the mantle – there are volcanic rocks whose chemistry does suggest such a mechanism. About 8 Ma ago the southern Plateau began to spread laterally, producing a series of N-S extensional basins, which suggests that by then sufficient gravitational potential had accumulated to make the thickened crust unstable. About that time various signatures arose in foraminifera of the Indian Ocean and sediments derived by erosion, which suggest that the monsoon increased in intensity.
When the Plateau attained sufficient elevation above sea level to start spreading sideways and affect atmospheric circulation largely rests on these theoretical judgements. For the ideas to firm up needs some means of estimating topographic elevation, which is not easy to do. One way is to use plant remains that can give clues, either because the species involved are sensitive to elevation today, or the morphology of their leaves shows signs of physiological adaptation to elevation. The first is ruled out in old sediments, simply because the species present are now extinct.. Plants metabolism is dependent on diffusion of water and CO2 into their leaves during photosynthesis, and features, such as stomata density, give clues to the conditions for such diffusion. Luckily, sediments from southern Tibet do contain well-preserved plants, and a multinational group led by Bob Spicer of the British Open University have attempted to assess palaeo-elevation for the time at which they were deposited (Spicer, R.A. and 7 others 2003. Constant elevation of southern Tibet over the last 15 million years. Nature, v. 421, p. 622-624). Their method relies on linking leaf morphology to a property of the atmosphere, known as moist static energy (MSE), through estimates of atmospheric enthalpy from the leaves. That is not the end of the estimation, because MSE needs to be related to elevation and the only way is to use climatic modelling for the past. Whatever, Spicer and colleagues reckon that 15 Ma ago their sampling site was more or less at the same elevation as today, around 4.5 km above sea level. If true, they have established that the south part of the Plateau was already in existence during the Middle Miocene. Being so convoluted, despite its apparent precision, the leaf analysis method does need independent confirmation. There is a much easier and arguably more reliable method, based on the change in the size of bubbles formed by gas escaping from lavas, according to atmospheric pressure (see Cunning means of estimating uplift in November 2002 issue of Earth Pages News). There are lavas in southern Tibet that date from Cretaceous times, including some about a million years younger than the plant remains.
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Precambrian warmth and methane
March 2003
Methane is a more efficient "greenhouse" gas than CO2, but it soon oxidises in the presence of oxygen. During the Phanerozoic there have been several massive releases of methane, probably from gas hydrates in deep-ocean sediments, which produced warming spikes that decayed away quickly in geological terms. Before there was much, if any, oxygen in the atmosphere, methane could linger and add to the retention of heat by carbon dioxide and water in the atmosphere. One of the longest running disputes in environmental geochemistry concerns when oxygen levels became significant in the Precambrian, and what they were compared with later times. Whether the Earth was warm or cold has a bearing on this. Cosmological theory suggest that stars similar to the Sun progressively grow more energetic with time. Without some kind of greenhouse effect, the Earth would have been condemned to frigidity from its outset. Even today, with a more radiant Sun, only atmospheric retention of solar heat keeps overall temperature from being well below freezing. The further back in time, the greater the "greenhouse" effect would have to have been to stave off complete ice cover and a runaway "icehouse". Methane almost certainly played a part in this once methane generating organisms evolved, up to about 2200 Ma, when there are signs (continental redbeds and soils rich in iron oxides) that atmospheric oxygen was appreciable. However, warmth prevailed for about 1.5 billion years thereafter, until the plunges into frigid conditions of the so-called "Snowball Earth" period from about 700 to 550 Ma. Somehow, the greenhouse effect lingered.
Alexander Pavlov of the University of Colorado, and colleagues from Pennsylvania State University have addressed the implications of this continued warmth in terms of maximum oxygen levels needed to avoid complete oxidation of methane releases (Pavlov, A.A. et al. 2003. Methane-rich Proterozoic atmosphere? Geology, v. 31, p. 87-90). Today, more than 90% of all methane production beneath the ocean floor is consumed by bacteria, depending on the amount of dissolved oxygen and sulphate ions (for aerobic and anaerobic methanotrophs). There is plenty of evidence that deep Precambrian ocean water was anoxic, so a great deal more methane would have emerged from them. That it was also poor in sulphate ions is shown by their low levels in solid solution with carbonates and Proterozoic sulphur isotopes in marine sediments. The authors argue that this signifies low atmospheric oxygen levels, around 5 to 18 percent of modern concentrations. The scene may have been set for an excess of methane production over its oxidation, thereby keeping the "greenhouse" warming above the levels when glaciation would have been widespread.. If so, something completely upset this balancing act in the Neoproterozoic, to drive down temperatures several times – the "Snowball Earth" events. The trigger may have been a boost in oxygen production and retention in the atmosphere.
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El Niño in the Eocene
March 2003
The oceanographic-climatic phenomenon in the equatorial Pacific, known as the El Niño-Southern Oscillation (ENSO), now seems to be major force in driving climate shifts far afield, such as the current drought in the Horn of Africa. Its cyclicity relieves the suffering brought by El Niño events, yet the processes may well be highly unstable. Some believe that it is only a matter of time before ENSO reverts to a permanent El Niño condition, with disastrous consequences. Such a stabilisation in the past may have resulted in warming at high latitudes that permitted lush vegetation in near-polar regions, during the Cretaceous and the Eocene. The Eocene was much warmer than now, as a result of a massive release of methane from seafloor sediments around 55 Ma. So it makes sense to look at its climate record to check for a permanent El Niño. Matthew Huber and Rodrigo Caballero of the University of Copenhagen have compared climate records from annually layered lake sediments from the Eocene of Germany and Wyoming in the western USA with climate models to test the hypothesis (Huber, M. & Caballero, R. 2003. Eocene El Niño: Evidence for robust tropical dynamics in the "hothouse". Science, v. 299, p. 877-881). The climate data from the lake sediments (thickness variations in annual layers) show clear signs of a roughly 5-year cycle of climate change, attributed to an Eocene ENSO. This tallies nicely with simulations for the Eocene continent-ocean set-up. Although the authors claim that their findings refute the hypothesis that global warming tends to shut down ENSO, which is a comforting thought, Eocene ocean and air circulation was not the same as now by any means. There have been interglacial periods during the Pliocene to present climate system in which temperatures exceeded those of the Holocene. Surely, annually layered sediments from those times will provide a better test.
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Freezing the Antarctic
February 2003
Records of seawater oxygen isotopes and its Ca/Mg ratio shows that a substantial permanent ice sheet first formed in Antarctica in the Oligocene Epoch, about 34 Ma ago. The favoured explanation, until this month, was that the South polar continent became thermally isolated from the rest of the planet when circumpolar currents were able to flow around it, once South America and Australia had separated from Antarctica and opened the "gateways" of the Drake and Tasmanian Passages. But what if atmospheric CO2 played a role? A drop in the "greenhouse" effect and global cooling could have driven polar temperatures low enough for ice formation without an oceanographic influence. Once established, the albedo effect of a large ice sheet would seal Antarctica into permanent freeze-up. Factoring all the likely components in a general circulation model leads to a surprise (DeConto, R.M. & Pollard, D. 2003. Rapid Cenozoic glaciation of Antarctica by declining atmospheric CO2, Nature, v. 421, p. 245-249). The opening of the Drake and Tasmanian Passages was not accompanied by a sufficient depth of water to support massive current reorganisation until several million years after the ice cap left its clear imprint on the marine record. DeConto and Pollard's model shows that even with closed Passages an ice cap would have formed, if CO2 levels had fallen below three times those that prevailed in the Holocene, before industrial emissions began. Global cooling had begun somewhat earlier than Antarctic freeze-up, following the high around the Palaeocene/Eocene boundary (~55 Ma), falling to a plateau about 40 Ma ago. Undoubtedly CO2 concentrations had fallen globally for this to have happened. Of course, there is no Oligocene ice, from which glaciologists might extract trapped bubbles and samples of ancient air with which to refute or confirm the model. However, a decrease in carbon dioxide would also cause the acidity of rainfall to decrease as well as the amount of rainfall globally, and that might show up in changed weathering processes, especially in the tropics of the time.
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How patterned ground forms
February 2003
Visiting flat areas of permanently frozen ground brings you face to face with truly bizarre patterns at the ground surface. Some are perfect hexagons of stones around finer soils, others doughnut-like circles and then a perplexing range of other features that look for all the world as though they were built by humans. Undoubtedly, they result from the forces at work when the top soil layer freezes and thaws annually, together with soil creep down extremely shallow slopes, repeated over millennia. However, exactly how the patterned ground develops has eluded geomorphologists for more than a century. Rejecting the reductionist approach that any landform's evolution can be deduced from basic principles of physics seems to be the key (Kessler, M.A. & Werner, B.T. 2003. Self-organization of sorted patterned ground. Science, v. 299, p. 380-383). Kessler and Werner of the University of California modelled the two likely processes of ice lensing that sorts stones and finer soil, and the transport of individual stones along the lines of accumulated stones as freezing fines expand, building in elements of spatial and time scales plus other parameters such as surface slope. Their model is self-organising, and proceeds to mimic many of the intricacies of patterned ground, even the most labyrinthine. It might seem a little heavy handed to crunch numbers to help explain what are really quite minor features. But having demonstrated the power of non-linear modelling here, the authors open up a novel approach to landscape evolution of every scale and antiquity.
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Hair trigger for gas hydrates
January 2003
The curious mix of water ice and methane, known as gas hydrate or clathrate, which is stable at ocean depths greater than 300 m, is one of the largest potential components of the active carbon cycle (~1013t). Its methane content stems from bacterial breakdown of organic matter buried in anaerobic sea-floor sediments. As well as being pressure sensitive, gas hydrate also has a narrow stability "window" as regards temperature. Geothermal heat therefore limits the depth of gas-hydrate accumulations to a few tens to hundreds of metres below the seabed. Its vast methane content is clearly something on which energy transnationals have an eye. However, methane is almost four times more powerful as a "greenhouse gas" than CO2emissions. Carbon-isotope studies from sedimentary rocks show signs that several times in the distant past methane was released catastrophically to the atmosphere, the timing coinciding with signs of rapid global warming. The last major event of this kind was around 55 Ma ago, when the end of the Palaeocene Epoch witnessed an 8°C global temperature rise in a matter of a few thousand years (Thomas, D. et al. 2002. Warming the fuel for the fire: Evidence for the thermal dissociation of methane hydrate during the Paleocene-Eocene thermal maximum. Geology, v. 30, p.1067-1070). The warming "spike" eases because methane is quickly oxidised to water and CO2in the atmosphere, but that still allows abnormally warm conditions to linger.
Sonar surveys of the seabed, including that of the North Sea, reveal pits and funnels that probably mark sites of past methane releases from destabilised gas hydrates. In theory, two general processes lead to their instability: falling global sea level that reduces the pressure on gas hydrates formed at shallow water depths; a rise in the temperature of ocean-bottom water. The second could produce more widespread methane release than the first. Refining these crude prognoses needs detail about the structure of gas-hydrate zones beneath the seabed. Conventional seismic surveys conducted at the sea surface show the clathrate-rich zones just beneath the sea floor, but no detail. Towing sources and receivers just above the seabed reveals intricate structures (Wood, W.T. et al. 2002. Decreased stability of methane hydrates in marine sediments owing to phase-boundary roughness. Nature, v. 420, p. 656-660). Wood and co-workers from the US Naval Research Laboratory, the University of Victoria and the Pacific Geoscience Centre in British Columbia, Canada surveyed the Pacific floor off Vancouver Island. Their most striking observation is of many vertical, chimney-like structures that puncture the gas-hydrate zone in the upper sediment layer. They reckon that these structures are where methane and warm fluids find their way to the seabed; they are probably the expression in cross section of the surface pitting formed by past degassing. They also may supply gas to the zone where it becomes locked in metastable water ice. The sheer number of the "chimneys" indicates that the surface area of gas-hydrate stability is many times larger than previously supposed, as a result of their "roughening" effect. Since the base of the gas-hydrate stability zone is most prone to the effect of warming of sea-bottom water, which shifts the geotherm slightly, an increase in its surface area, together with its closer approach to the seabed around the "chimneys", could further increase its sensitivity to small changes. Up to now, many specialists have suggested that major methane releases resulted from sudden collapses of sea-floor sediments in tectonically unstable areas, such as the Storegga Slide off western Norway. They may instead have been due to more widespread instability resulting from environmental change. Since the largest pressure decreases due to sea-level falls accompanied glacial epochs, some clues to whether the "chimney" effect has had an influence may come from a fresh look at methane contents of trapped air bubbles in Antarctic and Greenlandic ice cores. The extent to which methane releases might effect climate depends on how much is oxidised to CO2in sea water, before it can enter the atmosphere to enhance the "greenhouse" effect. Little is know about such processes.
See also: Pecher, I.A. 2002. Gas hydrates on the brink. Nature, v. 420, p, 622-623.
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Snowball Earth hypothesis challenged, again
December 2002
Palaeomagnetic
data from localities famed for their Neoproterozoic glaciogenic rocks point persuasively
to several epochs between 750 and 550 Ma when widespread continental glaciation
took place at low latitudes. It is this
evidence, along with theoretical consideration of drastic changes in the Earth's
albedo that would result from tropical land ice, that encouraged the idea of pole
to pole ice cover. Only a build-up of
volcanogenic CO2 in the atmosphere could prevent such a "Snowball Earth"
lasting indefinitely, and even with such relief it would have endured for millions
of years. Much of the geological evidence
cited by those who support and promote this neo-catastrophic idea comes from excellent,
but geographically quite limited occurrences of tillites or glaciomarine sediments,
such as those of Namibia. Some occurrences
have never been seriously analysed, except as examples that superficially support
the hypothesis. One such sequence is that
of Arabia, easily accessed in northern Oman and described by a British-Swiss team
(Leather, J. et al. 2002. Neoproterozoic snowball Earth under scrutiny:
Evidence from the Fiq glaciation of Oman. Geology, v. 30, p. 891-894).
Isotopic studies of carbonates from glaciogenic sediments (see Meltdown
for Snowball Earth? in Earth Pages News for January 2002) seriously
undermined several arguments by "Snowball Earth" supporters, but are open to various
interpretations. Hard geological evidence
is less easy to rationalize. A growing number of Neoproterozoic
glaciogenic sequences, such as the Port Askaig Tillite of the Scottish Dalradian
Supergroup and others from the Congo and Kalahari cratons, and Laurentia, show
dropstone-rich diamictites interbedded with sediments that show little if any
sign of a glacial influence (Condon, D.J. et al. 2002. Neoproterozoic glacial-rainout intervals: Observations and implications.
Geology, v. 30, p. 35-38).
Such evidence can be explained by climatic change and a fully functioning
hydrological cycle. The report on the Omani example by Leather
and colleagues highlights splendid examples of sediments that mark cycles of glacial
advance and retreat, reminiscent of those of the Pleistocene glacial epoch and
more or less the same as in many Neoproterozoic occurrences. It can only be a matter of time before Australian
geologists enter the fray decisively, for glaciogenic sediments comprise up to
30% of the many-kilometres thick Umberatana Group in the Neoproterozoic of the
Flinders Range in South Australia, and there are several other stratigraphically
distinct diamictite sequences.
It seems likely that the "Snowball Earth" hypothesis is waning; an embarrassment
for those geologists who have promoted it so assiduously over the last several
years. However, the enigma of low-latitude
glaciation on a vast scale is likely to remain, unless, that is, all the diamictites
can be shown to have non-glacial origins, which is not as unlikely as it might
seem. The Fiq sequence of Oman, like the Dalradian
example in Scotland, formed in an actively extending basin. Repeated seismicity on rift-bounding faults
could have launched debris flows to deposit diamictites (a purely descriptive
term for sediments containing a wide variety of clast sizes). The most spectacular diamictite in the Dalradian
Supergroup, and perhaps anywhere, is the Great Breccia of the Garvellachs.
Recent work suggests strongly that it is not glaciogenic, but the product
of such a debris flow (Arnaud, E. & Eyles, C.H. 2002.
Catastrophic mass failure of a Neoproterozoic glacially influenced continental
margin, the Great Breccia, Port Askaig Formation, Scotland. Sedimentary
Geology, v. 151, p. 313-333).
The supposedly clinching evidence for diamictites' origin from iceberg
armadas is the way in which some clasts ("dropstones") puncture underlying stratification. All that is required is a means of puncturing,
and sediment compaction around large, resistant clasts in a water saturated matrix
is quite capable of doing that. Even the long-held belief that glaciation is uniquely signified
by polished and striated surfaces beneath diamictites containing similarly scratched
clasts is coming into question. Sites
of large impacts, such as the Ries crater in Germany, include exactly similar
features caused by ejecta blasted from the crater, cited by Vern Oberbeck, formerly
of NASA, in a little-cited paper that proposed an impact origin for diamictites
(Oberbeck, V.R. et al. 1993. Impacts, tillites
and the breakup of Gondwanaland. Journal
of Geology, v. 101, p. 1-19).
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Post-apocalypse weathering in the Early Triassic
December 2002
Environmental crises do not come bigger than that at the end of the Permian, when marine ecosystems
virtually collapsed, and similar extinctions of terrestrial flora and fauna are
becoming clear. Whereas the Siberian Traps may indeed have
been a triggering mechanism, there are carbon-isotope indicators that vast amounts
of methane entered the atmosphere shortly afterwards, rapidly being oxidised to
CO2. The density of respiratory
openings (stomata) in fossil leaves from the lowest Triassic is unusually low,
indicating an abundance of CO2 in the atmosphere and probably enhanced
"greenhouse" conditions. Hot and humid
conditions encourage weathering of the continental surface, and there are many
Early Triassic palaeosols, some which mimic those in the tropics being found at
unusually high palaeolatitudes. Such soils harbour crucial evidence for surface
conditions, and the high-latitude ones present a surprise (Sheldon, N.D. &
Retallack, G.J. 2002. Low oxygen levels
in earliest Triassic soils. Geology,
v. 30, p. 919-922). Unlike tropical laterites, which are rich in
kaolinite, high-latitude soils are dominated by illitic clays that signify incomplete
breakdown of silicates. The surprise comes
in the form of an unusual mineral, berthierine; a green, serpentine-like mineral
that is easily confused with chlorites in hand specimen. It can form by reaction between clays and ferric
oxy-hydroxides, but only under highly reducing conditions. Because most soils since about 2000 Ma ago
have formed in contact with an increasingly oxygen-rich atmosphere, achieving
suitably reducing conditions demands input of a reductant to the soil "atmosphere".
The most likely candidate is methane, whose oxidation would consume oxygen. However, methane's residence time in the air is around 10 years,
because it is quickly oxidised to CO2, so methane release following
the P-Tr boundary event seems as if it was sufficiently prolonged to influence
considerably longer term soil formation.
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Africa's first ice core record
November 2002
Melting of low-latitude glaciers in Africa is so rapid that, unless they are
cored soon, their content of long-term climate data may soon be gone forever.
So the first detailed isotopic record from Africa's highest glacier on Kilimanjaro
is cause for some relief. Intrepid glaciologist Lonnie Thompson welded a large
team together for this important task (Thompson, L. 2002. Kilimanjaro ice core
records: evidence of Holocene climate change in tropical Africa. Science,
v. 298, p. 589-593). The annually layered ice goes back only about 12
ka, but nonetheless gives a precious account of climate change at the heart
of the continent, far more detailed than sparse lake-bed cores from various
places.
The core confirms a broad pattern of warm, wet conditions from 11 to 4 ka,
before the long-term cooling and drying of historical times. These reflect
likely weakening of monsoonal conditions in the late Holocene. However, assigning
precise ages to depth in the cores is not as easy as in those from high-latitude
ice sheets, because of a lack of good layering (presumably) and dateable carbon.
At about 5200 years ago, the record shows an abrupt fall in δ18O,
a sign of drying and cooling that took place over perhaps a matter of decades.
This correlates with disruption of early civilisations in India, Egypt and the
Middle East, and probably stemmed from cooling in the North Atlantic. However,
an equally rapid deterioration occurred around 6300 years bp, although not so
extreme, to presage a millennium of arid conditions at the heart of Africa.
Important as these data are, the team's estimates of current retreat rates of
the Kilimanjaro glaciers are alarming. Quite probably, the white cap of Africa's
highest mountain will have disappeared within the next 20 years.
Lonnie Thompson is obviously both keyed- and clued up about extracting climatic
data from ice at high elevations. So much so, that Science has printed
a lengthy account of his exploits, mainly on low-latitude glaciers (Krajick,
K. 2002. Ice man: Lonnie Thompson scales the peaks for science. Science,
v. 298, p. 518-522
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Reviews of climate and the hydrological cycle
October 2002
Earth Pages News has commented several times on developments in the
connection between ocean currents and climate, over the last 3 years. The subject
has many aspects, and these have been bundled and brought up to date in one
of a series of review articles on the relationship between climate and the hydrological
cycle in Nature's occasional Insight series (Rahmstorf, S. 2002. Ocean
circulation and climate during the last 120,000 years. Nature, v. 419,
p. 207-214). Stefan Rahmsdorf covers the evidence to date that implicates changes
in deep circulation in rapid and dramatic climate shifts, such as changed air
temperatures over the Greenland ice cap and iceberg armadas in the North Atlantic.
Another review outlines the longer-term perspective of links between atmosphere,
oceans, ice sheets, solid-Earth processes and astronomical forcing in shifts
of climate and sea level over the last 3 Ma. Central to this linked system
is the transfer of tens of millions of cubic kilometres of water from tropics
to poles, and from ice sheets to sea levels (Lambeck, K. et al. 2002.
Links between climate and sea levels for the past three million years. Nature,
v. 419, p. 199-206).
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Alaskan source proposed for end-Palaeocene warming
October 2002
Between 58 and 52 Ma, around the Palaeocene-Eocene boundary, Earth's climate
bucked the long-term cooling trend during the Cenozoic, by warming considerably.
Since the warming lasted for so long, it seems likely to have been caused by
an enhanced atmospheric "greenhouse" gases rather than by either astronomical
or oceanic causes. Carbon isotope data around the P-E boundary can be interpreted
in terms of massive releases of biogenic methane, perhaps from gas hydrates
on the sea floor. However, such releases are likely to have been sudden, and
a more continual release of "greenhouse" gases fits the record better; but that
begs the questions where and how? Catastrophic methane release has been invoked
for the dramatic rise in deep-ocean and high-latitude temperatures within 10
thousand years exactly at the P-E boundary.
Lengthy climatic warming can stem from increased volcanism and sea-floor spreading,
but there is scanty evidence for either during this period. Another possibility
is production of gases as a result of tectonic activity, either by involvement
of carbonate sediments in metamorphism, which releases CO2, or "stewing"
organic matter in thick sedimentary sequences. Candidates for the last are
the thick accretionary prisms at Pacific destructive margins, an especially
appropriate example being that of the Gulf of Alaska which grew rapidly during
this period (Hudson, T.I. & Magoon, I.B. 2002. Tectonic controls on greenhouse
gas flux to the Paleogene atmosphere from the Gulf of Alaska accretionary prism.
Geology, v. 30, p. 547-550). Oceanic and continental margin sediments
scraped off descending oceanic lithosphere contain buried organic matter. Increased
heat flow, perhaps associated with rising magmas, can cause organic debris to
break down to hydrocarbons. Over-maturation results in the formation of methane,
potentially in vast volumes, that can leak continually to the atmosphere. Methane
rapidly oxidizes to CO2, decreasing the warming effect, but able
to linger for considerable periods. Hudson and Magoo calculate such enormous
releases, that even disputes over the amount of accreted sediment in the Gulf
of Alaska do little to rule out its being a major source for climatically implicated
gases. This first suggestion of a role for accretionary prisms in climate change
may spur studies of such processes elsewhere, in an attempt to remove much of
the load from the BLAG hypothesis that involves metamorphic release of CO2
in a difficult to verify process of lithospheric flatus.
See also: Clift, P. & Bice, K. 2002. Baked Alaska. Science,
v. 419, p.129-130
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Long-range forecast: a prolonged interglacial
July 2002
Provided the Milankovich theory of astronomical influences on insolation is indeed behind the pacing of glacial-interglacial episodes of the near past, it should be easier to forecast future change in overall climate than that of weather. It turns out that the fluctuation of Earth's orbital eccentricity (behind the roughly 100 ka periodicity of climate change for the past 1 Ma) is entering an historic low, due to the 400 ka period of one of its two cycles. Modelling future insolation at high northern latitudes results in a damping of its fluctuations over the next 100 ka (Berger, A. and Loutre, M.F. 2002. An exceptionally long interglacial ahead? Science, v. 297, p. 1287-1288). Left to climates own devices, the small changes in insolation may prolong the Holocene interglacial for as much as another 50 ka, instead of being now on the cusp of a descent into more frigid conditions. Until recently, many climatologists looked to the last, Eemian interglacial as the model for the current one, and that lasted only 10 ka.
Of course, climate is no longer at the whim of astronomical forces and the Earth's own circulation of energy, principally by the flow of energy in North Atlantic water, driven by deep water formed by sea-ice around Iceland. Atmospheric CO2 stands about 30% higher than during previous interglacials, because of anthropogenic emissions. Berger and Loutre factor in the "greenhouse" influence of the additional CO2, to find an ominous possibility that the Greenland ice sheet might well melt, with the climate entering an irreversible warming. The climate, however, is not a model, and there is really no inkling of what surprises are in store from counter-intuitive behaviour of the many forces at work in it, under conditions that have no analogue during the whole of human evolutionary history.
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Analogue of Archaean carbon cycle in Black Sea reefs
July 2002
The Archaean world almost certainly had an atmosphere and oceans that were more or less free of oxygen. Under such conditions the fate of dead organisms in the ocean, perhaps the remains of photosynthesizing cyanobacteria, would have been bacterial fermentation and the production of massive amounts of methane. Along with volcanic emissions of carbon dioxide, methane in the atmosphere would have helped warm the planet at a time when the Sun emitted considerably less energy than it does now. Methane is more strongly depleted in 13C than any organic or inorganic carbon compound. So large falls in the d13C composition of organic carbon in Archaean rocks, around 2700 Ma have been taken by some palaeobiologists to signify methane metabolism. Most methane-consuming bacteria today produce oxygen as a biproduct, so the negative excursions might indicate an early build up of more than a trace of oxygen in the Archaean atmosphere. Discovery of bacterial communities on the floor of the Black Sea, which consume methane without oxygen production (Michaelis, W. and 16 others 2002. Microbial reefs in the Black Sea fuelled by anaerobic oxidation of methane. Science, v. 297, p. 1013-1015), suggest strongly that there may be little reason to suppose that Archaean conditions did involve free oxygen.
Off the coast of Crimea there are numerous sea-bed methane seeps in shallow water. Surprisingly they are well-colonized by primitive bacteria, which produce thick mats held together by carbonate precipitates in completely anoxic conditions. Laboratory cultures of the communities reveal that the consist of archaea and bacteria that respectively consume methane and reduce sulphate ions to sulphide. The net result is that methane is oxidized by sulphate to produce calcium and magnesium carbonates, and lots of hydrogen sulphide (methane donates electrons for sulphate reduction, thereby becoming a source of carbon for cell metabolism). Since much of the methane's carbon ends up in stable carbonate – perhaps ten times more than in organic matter, such a process in the Archaean would have helped stabilize the "greenhouse effect" then.
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Prolonged Cretaceous hothouse
March 2002
Hothouse conditions were forced by massive emission of CO2
during the mid-Cretaceous superplume event that created huge submarine basalt
plateaux and began the development of many island chains that litter the floor
of the central Pacific. It was at this time that dinosaur-infested forests cloaked
high latitudes, almost to both poles. Terrestrial evidence suggests that conditions
cooled somewhat in the later Cretaceous, and sequence stratigraphy indicates
cyclic sea-level fluctuations, ascribed by some to the development of Antarctic
ice sheets. Resolving later Cretaceous global mean temperatures, and the ice-sheet
question relies on oxygen isotopes from sea-floor sediments. These are now available
with sufficient precision and resolution to show that hothouse conditions lasted
a great deal longer than suspected (Huber, B.T. et al. 2002. Deep-sea paleotemperature
record of extreme warmth during the Cretaceous. Geology, v. 30,
p. 123-126).
The Pacific superplume's maximum activity was over a period
of 15 Ma from 125 to 110 Ma (Barremian and Aptian), although it lasted until
the early Campanian (80 Ma). Contrary to the supposed magnitude of CO2 release
by volcanism, heating reached a maximum from 94 to 80 Ma. Even at high southern
latitudes, deep-ocean water remained at 14 to 19°C for these 14 Ma. Until
the end of the Cretaceous it rarely fell below 10°C. The data rule out any
circulation of cold, dense brines into the deep ocean basins from the formation
of boreal sea ice, and consequently any influence by polar ice sheets. Sea level
reached its highest during this period, almost certainly because the volume
of the ocean basins shrank, being floored by young, warm, low-density crust
formed by the superplume. Mid to late-Cretaceous flooding of the continental
margins created uniquely favourable conditions for an explosive development
of carbonate-secreting organisms of many kinds. Despite the burial of vast carbonate
platforms, as well as thick boreal coal seams, these limestone "factories"
seem incapable of having kept pace with greenhouse warming. Was CO2 the only
means then of global warming?
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Review of thermohaline circulation
February 2002
The central factor in abrupt climatic shifts
during the last glacial period was change in thermohaline circulation (THC),
particularly in the Atlantic Ocean. Two
general processes underpin THC: differences in solar heating from low to high
latitudes drive polewards flow of surface water; formation beneath sea-ice of
dense brine that sinks to form an equatorwards flow of North Atlantic Deep Water
(NADW). Freshwater influx at high latitudes
suppresses the formation of NADW, which, together with enhanced low-latitude
evaporation, slows polewards surface flow.. Currently, the thermal influence and NADW formation
dominates heat transport northwards in the North Atlantic, by carrying about
a petaWatt at mid latitudes. THC is
of little consequence in the North Pacific, partly because its fresher surface
water hinders dense-brine formation, and partly because any deep water formed
beneath sea ice in the Arctic cannot flow through the very shallow Bering Straits.
Clearly THC is a sensitive mechanism, inseparable
from other factors in climate forcing. Having such a vast influence on heat transport, if it changes there
are likely to be dramatic outcomes for climate, particularly along the eastern
flank of the North Atlantic where much of the transported heat arrives. Sea-ice formation around Iceland is decreasing, so a review article on
THC and rapid climate change is essential reading (Clark, P.U. et
al. 2002. The role of thermohaline
circulation in abrupt climate change. Nature, v. 415, p. 863-869). It is now
known that the last glacial period was punctuated by short-period (~ 1-2 ka)
warming-cooling episodes, known as Dansgaard-Oeschger events, one aspect of
which was the launching of "armadas" of icebergs to latitudes as far south as
Portugal (known as Heinrich events), which left their mark as occasional gravel
layers in the otherwise muddy sediments on the deep Atlantic floor. These episodes involved temperature changes
over the Greenland icecap of as much as 15°C. They began with warming
on this scale within a matter of decades followed by slow cooling to minimal
temperatures, before the next turn-over. The
deep cooling seems to have accompanied slowing and shut-down of THC. Current global warming is likely to do three things: increasing low-latitude evaporation, increasing freshwater influx to
high-latitude Atlantic surface water and a decrease in sea-ice formation at
the site of NADW formation. Because
all three drive down polewards heat flux, anthropogenic warming may well result
in contrary climate shift in Western Europe and Scandinavia – freeze rather
than thaw. If it happens, chances are that it will be
upon us with little warning.
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Meltdown for Snowball Earth?
January 2002
Following on from their linking carbon-isotope
excursions associated with Neoproterozoic diamictite-cap carbonate sequences
to methane release (see Methane and Snowball
Earth in Earth Pages, December
2001), Martin Kennedy, Nicholas Christie-Blick and Anthony Prave turned to the
δ13C
values in the diamictites for which a glaciogenic interpretation forms the main
plank of the Snowball Earth hypothesis (Kennedy, M.J. . 2001. Carbon isotope
composition of Neoproterozoic glacial carbonates as a test of paleoceanographic
models for snowball Earth phenomena. Geology, v. 29, p. 1135-1138). Complete
ice cover of the oceans would chemically isolate ocean water from the atmosphere,
and would effectively shut down the organic sinks for atmospheric carbon dioxide. While they operate, the exclusion of 13C relative to lighter
carbon by organisms drives up δ13C in sea water, to be preserved in
carbonate sediments. The Snowball Earth
model predicts negative δ13C, approaching the -5‰ of the mantle, in carbonates deposited during
all-enveloping glacial epochs. However,
few researchers have made the measurements needed to test that part of the hypothesis.
Kennedy and co-workers show from three such
diamictite sequences that the carbonate precipitated as cement in them has consistently
positive δ13C. Although that does not disprove
the existence of glaciation at tropical latitudes, it is not consistent with
the dreadful scenario of totally ice-bound oceans devoid of life. Nor, for that matter, is there any evidence from strontium isotope variations
in carbonate cap rocks for the massive continental weathering that the Snowball
Earth devotees propose as a means of escape from the eventual hot-house that
build up of volcanic CO2 emissions to release Earth from the mothers
of all cold snaps would create. Expect
interesting news in later Earth Pages
of how the greatest Earth science debate of the 21st century develops.
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Strontium load of Himalayan rivers
November 2001
One process connected to long-term climate change is the way that weakly acid
rainwater (containing dissolved CO2) weathers silicates in continental
rocks, one product being carbonate in soils. The process should draw CO2
from the atmosphere, thereby reducing its "greenhouse" effect. The idea is
by no means new, but received a boost in the mid 1990's from Maureen Raymo's
suggestion that fluctuations in the strontium-isotope composition of the oceans
through geological time should be a proxy for changes in the rate of continental
weathering. The 87Sr/86Sr of marine carbonates does show
clear correlation with long-term climate shifts during the Phanerozoic..
Continental weathering should increase as topographic relief becomes greater
through mountain building episodes. The Himalaya's rise through the late-Tertiary
has been suggested as a major influence over climatic deterioration, partly
by its effect on the Asian monsoon and partly as a huge site for the sequestration
of atmospheric CO2 by chemical weathering. Himalayan rivers have
enormous flows and equally large sediment and dissolved element loads. In particular
they carry far more strontium than other rivers, and it has a highly radiogenic
content of 87Sr. There are three means of attaining these levels:
from average continental crust which has a higher 87Sr/86Sr
ratio than oceanic crust (the other main source of seawater strontium); from
strontium rich limestones that acquired their isotopic signatures from the ocean
when they were deposited; or from sources with unusually high 87Sr/86Sr
ratios. The Himalaya are well known for carbonate sediments, and for granites
formed by melting of deeper, older continental material that gives them very
high proportions of radiogenic strontium. Recent work now shows that a significant
contribution of highly radiogenic strontium to Himalayan rivers is hydrothermal
activity (Evans, M.J. et al. 2001. Hydrothermal source of radiogenic
strontium to Himalayan rivers. Geology, v. 29, p. 803-806).
Hot springs feeding a major tributary of the Ganges contribute up to 30% of
its strontium load, and incidentally a great deal of CO2. Both result
from hydrothermal alteration of deeper rocks, and are unrelated to weathering
if the water involved emanates from the deep crust. It seems that these waters
are recycled rainwater, so this is a case of a high-temperature chemical weathering.
Whatever, it further complicates the original notion of linkage between mountain
building and climate.
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Methane and Snowball Earth
The well-publicized "Snowball Earth " model for Neoproterozoic glaciogenic
rocks that occur at tropical palaeolatitudes has to involve an escape mechanism
from global frigidity. Without some means of warming, the high albedo of widespread
ice would have locked the Earth into perpetual glaciation, which of course did
not happen.
The main proponents of the model, Paul Hoffman and Dan Schragg of Harvard University
suggested a gradual build up of volcanogenic CO2 during "Snowball"
conditions, when a dry atmosphere would have retained the "greenhouse" gas instead
of its being sequestered to the oceans and carbonate rocks by acid rain and
continental weathering. Gradually, atmospheric temperatures would have risen
due to trapping of outgoing, long-wave radiation by CO2. This simple
aspect of the model leads to scenarios where warming overruns once ice sheets
disappeared, to give extremely high-temperature conditions. Using carbon-isotope
data from marine carbonates is a means of supporting or refuting this escape
mechanism, and also of detecting the influences of other components of the carbon
cycle. Carbonates take up carbon dissolved in seawater without fractionating
its different isotopes, and provide measures of the degree to which organic
processes did contributed to fractionation. Cell processes preferentially take
up 12C, and if large masses of undecayed organic matter ends up in
seafloor sediments, the proportion of "heavier" 13C (indicated by
the standardized ratio of the two main isotopes δ13C) increases in seawater and the atmosphere. Carbon
of mantle origin, that emerges as volcanic CO2, has a constant δ13C of about -5‰. So these two processes contribute to
an isotopic balance, which for most of the Mesozoic and Cenozoic Eras established
a δ13C of between 0 and +4 ‰ in sea water and limestones.
This is interpreted as a sign that the recent carbon cycle achieved a balance
between volcanic additions and organic carbon burial weighted towards trapping
of undecayed carbohydrate in sea-floor sediments. Explanations for broad climate
changes since 250 Ma therefore rely more on other mechanisms than on the carbon
cycle
The most comprehensive study of Neoproterozoic carbon (Walter, M.R. et al.
2000. Dating the 840-544 Ma Neoproterozoic interval by isotopes of strontium,
carbon and sulfur in seawater, and some interpretative models. Precambrian
Research, v. 100, p. 371-433) does indeed show dramatic see-sawing
of δ13C through supposed "Snowball"
events, from highly positive values (<+10‰) before glaciogenic sedimentation
to highly negative (>-10‰) in the immediate aftermath. However, few data
were available from within glaciogenic sediments, and resolution is insufficient
to detect tell-tale trends. The key approach needs detailed carbon isotopes
through a single event, and such data appeared recently for the famous Neoproterozoic
glaciogenic-cap carbonate sequence of Namibia (Kennedy, M.J. et al. 2001.
Are Proterozoic cap carbonates and isotopic excursions a record of gas hydrate
destabilization following Earth's coldest intervals. Geology, v. 29,
p. 443-446)
Kennedy et al. measure δ13C
in carbonate cements in the glaciogenic diamictites, in overlying cap carbonates
and in cement to later clastic rocks. Interestingly, there is little sign of
a gradual decrease in 13C through the glaciogenic rocks. Constant
oceanic carbon composition would be expected if no volcanic CO2 entered
seawater during frigid, dry conditions, and living processes were minimal.
In the cap carbonates δ13C plummets from +3% to -4%. One simple explanation
would be massive "rain-out" of volcanic CO2 (δ13C of -5%) that had built up in the
air during the "Snowball" episode.
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Climate and heavy breathing
June 2001
The kingdom of the eukaryotes rests on a very simple environmental economy. Plants are producers of carbohydrate through photosynthesis, thereby generating excess oxygen from the photo- and molecular chemistry involved. Animal consumers use up oxygen in their metabolism and return carbon dioxide, the ultimate source of carbohydrate, to the air. A simple view is that animals contribute to global warming, whereas plants help cool the world. Perhaps because of that "common sense" view, most environmental scientists take a very different line, linking it with volcanic exhalation of CO2, "capture of carbon through rock weathering and the burial of dead organic matter in the global carbon cycle. Greg Retallack of the University of Oregon is about to publish a reappraisal of the animal versus plant part of the C-cycle (in press, Journal of Geology) that is based on observed imbalances between the two opposed kinds of respiration. Specialists in the C-cycle hold that there is a an overall balance, taking all components into account, whose inevitable result is the build up of oxygen in the atmosphere of an inhabited world. Yet oxygen is extremely reactive and should quickly combine in mineral oxides and hydroxides – after all, the iron in an untended car reverts to its oxide ore in the space of a few decades at most.
Partly following James Lovelock's Gaia hypothesis, Retallack focuses on the major fluctuations in atmospheric chemistry evidenced in the geochemical record, the most immediate being the see-saw fluctuation of modern levels of CO2 in the atmosphere – a 2% annual variation controlled by the waxing and waning of vegetation in the northern hemisphere (where plant cover is greatest) according to season. One of the largest shifts in atmospheric CO2 concentration followed the evolution of land plants from about 450 Ma ago. To thrive, they had to develop hard cellular material (lignin) that formed stems and trunks, which animals of the Palaeozoic were unable to oxidise efficiently. Both living biomass and burial of undigested lignin drew down CO2 and boosted oxygen levels. Animal evolution eventually exploited this "free lunch" through the humble termite and reptilian and then mammalian megafauns. Retallack believes that heavy breathing that resulted from lignin digestion reversed the declining CO2 trend for the 200 Ma following the Carboniferous to Permian glacial epoch in Gondwana. Though displaying some ups and downs, the Mesozoic saw a "greenhouse" world. Removal of the mighty and extremely abundant herbivorous dinosaurs by the K-T mass extinction provided and opportunity for plant diversification. Many Mesozoic plants evolved armour against browsing dinosaurs, exemplified by the surviving Andean "monkey puzzle" tree Araucaria. Their demise removed the need, and the plant Kingdom's evolutionary response was the appearance of grasses. Reatallack points out that grass itself is not as good as lignin-rich plants in holding CO2, but grasslands encourage the development of thick carbon-rich soils that hold more than the soils of the forest floor. It is this development that Retallack believes lay at the base of the decline in average global temperature through the Cainozoic, to culminate in the present Ice Age. Unsurprisingly, proponents of the complexity and diversity of the C-cycle, particularly in the oceans, are disinclined to have truck with the hypothesis.
Source: Pearce, F. The Kingdoms of Gaia. New Scientist, 16 June 2001, p. 30-33.
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Carbonates and biofilms
June 2001
Above the low level that is essential for their role in molecular "information" transfer, calcium ions pose a fatal threat to cell processes. That is simply because excess calcium combines with carbonate ions to form minute calcium carbonate crystals within the cell when the solubility product of calcite is exceeded. The solubility product is the concentration of calcium ions multiplied by that of carbonate ions, so that increase in one or the other can lead to supersaturation of calcium carbonate and imminent precipitation. Because CO2 is an essential need for photosynthesis and a product of animal metabolism, this risk is always present. In the most common photosynthesising bacteria, the cyanobacteria that have been around for at least 3.6 billion years, the drawing in of CO2 in the form of carbonate (CO32-) or bicarbonate (HCO3-) ions in water can result in supersaturation immediately around the cell. When it occurs, the "blue-green" bacterial biofilms induce precipitation of calcium carbonate. That is why such micro-organisms can act as reef builders, as they did to great effect during the early Precambrian (stromatolites), and also from Cambrian to Cretaceous times.
Calcite mineralization by biofilms is, however, a complicated process. It is connected with highly reactive substances that cyanobacteria exude outside their cell walls. Depending on their degree of ordering and the supply of calcium ions, these substances control the manner in which calcium carbonate precipitates. The detailed biochemistry and the form of calcite biofilms obtained by study of modern cyanobacteria in different watery environments has allowed Gernot Arp and co-workers at the University of Göttingen to evaluate varying calcium and CO2 concentrations in ocean water since 540 Ma, and suggest differences in Precambrian oceans (Arp, G. et al. 2001. Photosynthesis-induced biofilm calcification and calcium concentrations in Phanerozoic oceans. Science, v. 292, p. 1701-1704).
Their studies suggest that up to the Cretaceous, the Phanerozoic oceans must have had higher calcium contents than they do today. Microbial reefs formed in that period preserve details of the "blue-green's" cell structure, suggesting that calcite was nucleated directly by the extracellular substances. Vast burial of the calcite shells of planktonic metazoan organisms to form the Chalk deposits of Cretaceous age reduced very high levels to give the calcium-depleted oceans that prevailed during the Cainozoic. Microbial carbonates of these younger ages show no structure. The stromatolites that are so characteristic of Precambrian limestones are stuctureless too, although they show evidence of progressive build-up from myriads of thin layers. Irrespective of the Precambrian oceans' calcium content, this lack of structure can be explained by more dissolved CO2 that resulted from its higher concentration in the atmosphere. About 700-750 Ma ago, stromatolites that contain calcified cyanobacterial cells appear, and that may signify the massive drawdown of CO2 from the atmosphere that is implicated in creating icehouse conditions on a global scale during the late Proterozoic Aeon.
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Phanerozoic CO2 levels
May 2001
Because climate depends partly on the retention of solar heat by carbon dioxide in the atmosphere, a record of past CO2 fluctuations is important in linking evidence for shifting climate and environments to models. Conversely, models that seek to mimic climates of the past depend heavily on the assumption that the "greenhouse" effect and the carbon cycle underpin global temperature and precipitation. Current theorists consider that shifts in CO2 content of the atmosphere reflect a balance between its release through volcanism (itself a reflection of the rate of plate tectonics) and its removal by weathering of silicate minerals and burial of dead biomass.
The GEOCARB III model predicts rising atmospheric CO2 following the ice-house condition of the late-Precambrian, when rapid sea-floor spreading broke up and began to reassemble supercontinents during the Lower Palaeozoic. In the early Cambrian CO2 levels come out at 25 times the modern amount. Colonization of the land by plants through the Upper Palaeozoic, and the burial of a proportion of the increased amount of carbon fixed by them, allows the model to predict a massive fall in CO2. That tallies very well with the long period of glaciation in southern Pangaea during the Carboniferous and Permian. GEOCARB III suggests a recovery in levels through the Mesozoic, punctuated by extraordinary releases from plume activity, such as that implicated in the formation of ocean plateaux beneath the Pacific about 120 Ma ago.
From GEOCARB modelling stem predictions of the overall forcing of global temperatures. However, only the last 100 Ma can be assessed as regards temperatures, by using accurate proxies provided by oxygen isotopes and the Ca:Mg ratio of marine carbonates. Two of the leading climatic theorists, Thomas Crowley and Robert Berner of Texas A&M and Yale universities usefully summarise the range of other proxies that help validate their kind of modelling (Crowley, T.J. and Berner, R.A. 2001. CO2 and climate change. Science, v. 292, p. 870-872). These include estimates from fossil soils, carbon isotopes in sediments, the pores in plant leaves (see Plant respiration and climate) and how much boron is taken up in the shells of fossil animals. There are considerable discrepancies with modelling, albeit encompassed by the high uncertainties in the calculations. Crowley and Berner acknowledge the complexity of other factors that affect the global redistribution of heat, such as continental configurations in terms of area, geographic position, their effects on ocean circulation and even on the pace of the carbon cycle. They see the need to expand climate models, taking other factors on board, in an attempt to quantify the discrepancies.
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Methane and escape from Snowball Earth
May 2001
Palaeomagnetic pole positions determined from areas characterized by thick glacigenic deposits around 750 Ma old leave little doubt that large volumes of ice covered the Earth to tropical latitudes. Such evidence suggests an ice-bound world from which escape would have been very difficult because much of the Sun's energy would have been reflected back to space. Extreme and prolonged frigidity, from which Earth's climate did escape is seen by a growing number of palaeobiologists as the most profound influence over later evolution and diversification of life. The first fossil metazoans appear in the record shortly after a "Snowball Earth" event at 650 Ma, and the Cambrian explosion of animals with hard parts followed close on the heels of the last. Carbon isotope studies from marine carbonates suggest that each global glaciation witnessed massive extinctions of single-celled organisms, and surviving life was presented with a virtual tabula rasa of niches to fill. Such survivors, possessing characters that had ensured their survival – at which we can only guess – exploited them to the full. It is reasonable to speculate that without such climatic upheavals life would not be as it is now, and that our eventual appearance depended on them.
That Earth's climate broke out of runaway ice-house conditions is obvious, the question being how was that possible. Volcanic emissions of carbon dioxide, which neither the Neoproterozoic biosphere nor silicate weathering were able to draw down into ocean water and sediments, would have accumulated in the atmosphere, to create "greenhouse" conditions. That simple scenario, envisaging a spectacular shift from frigid to hot conditions, has its problems. In order for climate to stabilize, without rushing into runaway heating along the path followed by Venus, demands implausibly high rates of silicate weathering to draw down CO2 in the period following the end of each "Snowball" event, and strontium isotopes that record the rate of continental weathering shwo no sign of anything so dramatic. It also poses the question of how global ice cover could remain while CO2 slowly built up. The key seems to lie in carbonates that everywhere cap the glacigenic deposits of this age. The cap carbonates record rapid falls in the 13C proportion of the carbon in carbonate. 13C shows a rise in the glacial epochs that signifies massive burial of dead organic matter (enriched in lighter 12C), probably through mass extinction. In a review of the geochemical basis for changes in oceanic carbon isotopes, and high-resolution data from cap carbonates, scientists from the University of California and the Lamont-Doherty Earth Observatory, suggest that the isotopic excursions could reflect massive release of methane from gas-hydrate layers in sediments that were frigid during the Snowball event (Kennedy, M.J. et al. 2001. Are Proterozoic cap carbonates and isotopic excursions a record of gas hydrate destabilization following Earth's coldest intervals? Geology, v. 29, p. 443-446). Backing up this hypothesis are examples of structures in cap carbonates that are identical to those formed in modern sediments affected by break down of gas hydrates and release of methane from the sea floor.
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Plant respiration and climate
May 2001
Leaf surfaces are pockmarked by pores (stomata), through which cell metabolism draws in the carbon dioxide involved in photosynthesis and transpires its products, including oxygen. When CO2 levels are low, more pores are needed, and vice versa. Surprisingly, museum specimens of leaves collected since the start of the Industrial Revolution do show a decrease in the density of such pores that matches the documented rise in atmospheric CO2 levels. Were it possible to find fossils of the same plant species, pore density would be an excellent proxy for the "greenhouse" effect. That is not possible, because of evolution. However, plants related to the Ginkgo have a pedigree that goes back about 300 Ma. Morphologically, the four genera of Ginkgo-like leaves are very similar, so using them potentially gives an independent record of the "greenhouse" effect.
Gregory Retallack of the University of Oregon has measured the stomatal index of sufficient Ginkgo and related leaves to assess CO2 levels in a broad-brush sense for the period since the early Permian (Retallack, G.J. 2001. A 300-million-year record of atmospheric carbon dioxide from fossil plant cuticles. Nature, v. 411, p, 287-290). His results tally broadly with oxygen-isotope and other proxies for palaeotemperature variations, and to some extent with CO2 modelling (see Phanerozoic CO2 levels). However, the stomatal record shows changes up to 10 Ma in advance of shifts in temperature. That might be due to coarse resolution in Retallack's data, but could signify other forces at work other than the "greenhouse" effect. The most significant advance provided by leaf studies is that they help account for mismatches between evidence for cooling and predictions of high CO2 by modelling, for the Jurassic and Cretaceous, that have been a thorn in the side of the modellers. Given fossil leaves more closely spaced in time, and using other plant groups, Retallack's method potentially could revolutionize climate analyses and extend them back as far as 400 Ma ago.
See also: Kürschner, W.M. 2001. Leaf sensor for CO2 in deep time. Nature, v. 411, p. 247-248.
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April 2001
The most favoured means whereby the weak fluctuation in solar radiation due to the Milankovich-Croll Effect become amplified to affect climate's ups and downs is the switching on and off of thermohaline circulation in the North Atlantic Ocean. The key to such ocean circulation is formation today of dense, cold brine through sea-ice formation around Iceland. To set circulation in motion, however, depends on these brines being able to move southwards, which they do now in a sea-floor channel between Shetland and the Faeroe Islands. When the North Atlantic began to open, this route was blocked by a ridge between Greenland and Shetland, buoyed up by residual warmth in the lithosphere from volcanic activity at the Iceland plume.
It is important to assess when the Shetland-Faeroe "gateway" formed, so that the effects of thermohaline circulation on pre-glacial climate can be assessed. Petroleum exploration using high-resolution seismic reflection profiles and drilling has resolved this particular issue. Geologists and geophysicists from Exxon and Cardiff University have found signs that sediment drift dragged by such a deep flow began in the early Oligocene (about 35 Ma ago) (Davies, R. et al. 2001. Early Oligocene initiation of North Atlantic Deep Water formation. Nature, v. 410, p. 917-920). The evidence takes the form of multiple, moat-like erosion surfaces down to the base of sediment fill between the Faeroes and Shetland, shown superbly by the seismic data. Drilling shows that these signs of deep-water flow stop abruptly in Early Oligocene sediments.
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Astrology and ice
April 2001
The early Oligocene marked the onset of serious ice cover on Antarctica, and it shows as a dramatic increase in 18O values in the ocean-floor record of benthic forms – lighter 16O had been trapped in land ice. That may or may not be a coincidence with the finding about the start of North Atlantic thermohaline flow in the previous item. A lesser, but still dramatic increase marks the Oligocene-Miocene boundary, suggesting further growth of the Antarctic ice sheet, which is not so readily matched empirically. Detailed study of the isotopic "blip" at this time by a team from the Universities of California, Cambridge and South Florida (Zachos, J.C. et al. 2001. Climate response to orbital forcing across the Oligocene-Miocene boundary. Science, V. 292, p. 274–278) suggests that it related to a remarkable coincidence in the astronomical record of solar heating.
Round 23 Ma ago, the orbital eccentricity dropped almost to zero – Earth's orbit would have been circular – at the same time as its axial tilt became very stable, the one reinforcing the climatic effect of the other. The isotopic "blip" coincides exactly with the coincidence. The detailed record also shows very clearly that minor fluctuations in climate at that time were in step with the 400 and 100 ka periods in the eccentricity variations, and with those of 41 ka that relate to changes in axial tilt. If nothing else, these results confirm that it is unnecessary to turn to extraterrestrial influences over climate other than those which are predictable from Milankovich's theory.
Additional source: Kerr, R.A. 2001. An orbital confluence leaves its mark. Science, v. 292, p. 191.
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Start of Pleistocene environmental change in tropical Africa
April 2001
Pollen records from an ODP core drilled off the Congo estuary provide a record of the fluctuation in the monsoon of western tropical Africa (Dupont, L.M. et al. 2001. Mid-Pleistocene environmental change in tropical Africa began as early as 1.05 Ma. Geology, v. 29, p. 1195-198). Before 1.05 Ma there is little sign of a glacial-interglacial pulse in the fluctuation of vegetation in the Congo Basin. Thereafter, ups and downs in pollen from various vegetation groups correlate well with the benthic foram oxygen-isotope time series. However there are a few surprises.
Conventional wisdom is that Africa experienced drying during glacial epochs, rain forest expanding during interglacials. In the Congo basin, grasses and savannah trees increased during interglacials while mountain trees fell in their influence, up to 600 ka. This suggests the opposite trend of warm, dry interglacials and cool, humid conditions during glacial periods, similar to the record for tropical South America. In the later Pleistocene, the fluctuation switched to that indicated by fluctuating lake levels throughout the continent. The pollen variations are backed up by variations in dinoflagellate cysts, which show that discharge from the Congo dropped during interglacials. The other surprise is that the onset of astronomically paced environmental change in west Africa predated the change to a 100 ka domination of global climate, and the increase in amplitude of changes in land-ice volume at 900 ka by a hundred thousand years. Dupont et al. suggest that the changes in albedo in tropical West Africa in response to vegetation changes could have had an influence on global climate when the fluctuations began.
As well as being interesting in terms of climate change, the new data throw doubt on the hypothesized link between climate in Africa and pulses of migration of early human species, such as H. ergaster and H. erectus. There were fluctuations in humidity in the earlier Pleistocene, but they show no link to global climate change. So, it seems unwise simply to look to the Milankovich forcing as a pacemaker in early human affairs.
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A Late-Jurassic methane "gun"
April 2001
Massive releases of methane from gas hydrate layers beneath the ocean floor, and its subsequent oxidation to carbon dioxide have been implicated in major climatic and oceanographic changes in the mid-Jurassic, Cretaceous and Palaeocene. They can be detected by drops in the 13C content of marine carbonates, caused by the "light" carbon trapped in biogenic methane. All those known also correlate with evidence for climatic warming.
The Swiss Jura mountains are a repository of great thicknesses of Jurassic carbonates, whose ammonite faunas allow fine stratigraphic division. Between 157 and 156 Ma (late Middle Oxfordian) there is a major negative excursion in 13C whose duration was as short as 180 ka (Padden, M. et al. 2001. Evidence for Late Jurassic release of methane from gas hydrate. Geology, v. 29, p. 223–226). The Swiss-French geochemists who discovered the anomaly believe that the release may have linked to opening of the ocean gateway that connected currents between Tethys and the easter Pacific oceans through what is now the Atlantic.
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Mantle overturn and oxygenation of the atmosphere
March 2001
The presence of abundant oxygen in Earth's atmosphere defies Le Chatelier's Principle – it should react rapidly with the rest of the environment through oxidation. That it does not is sufficient evidence for an alien observer to conclude that our planet is dominated by photosynthetic life at its surface and the burial of carbohydrate by geological processes. So, Le Chatelier is not defied on the long term, because the CO2 + H2O = carbohydrate + oxygen equilibrium does not reach a balance because of continual removal of organic material from the right-hand side! That Mars has no atmospheric oxygen bears witness to its lifelessness in that respect, as concluded decades back by James Lovelock.
Before 2.5 Ga ago, in the Archaean, atmospheric oxygen was a trace gas. Preservation of detrital grains of sulphides and uranium oxides in Archaean clastic sequences, that would have broken down in an oxidizing environment, is the main evidence for that. The other side of the coin is that oxygen-producing photosynthesizers – the cyanobacteria – were abundant throughout the Archaean, leaving their trace as common stromatolitic carbonates and signs of the crucial enzyme rubisco in kerogens and the carbon-isotope record.
If cyanobacteria generated oxygen, then why did it not build up in the atmosphere throughout the Archaean, instead of from about 2.2 Ga ago? The most likely explanation is that Archaean magmatism released vast amounts of Fe-II or ferrous iron to sea water, which then reacted with available oxygen to form the ferric oxide of banded iron formations (BIFs), with the biproduct of hydrogen gas that further drove Archaean environmental chemistry into a reducing condition. Seawater circulating through Archaean ocean crust would also have enriched basalts in ferric iron by the same oxidizing reaction. Such a chemical model still leaves unexplained the shift to an oxygenated atmosphere after the Archaean.
Norman Sleep of Stanford University, reviews an article by Kump et al. in Geochemistry, Geophysics, Geosystems (2001) that deals with this dilemma (Sleep, N.H. 2001. Oxygenating the atmosphere. Nature, v. 410, p. 317-319). Kump and his co-workers suggest that, rather than relating to a change in palaeoecology, the shift arose from subduction of dense ferric oxide-rich lithosphere to settle at the core-mantle boundary. By the end of the Archaean oxidized material filled the lower mantle. Heating reduced its density so that it became buoyant. If that deep oxidized layer rose to displace more primitive, reducing mantle, later magmatism would have released less Fe-II, thereby allowing biologically generated oxygen to build up. The converse effect would have been to bring down levels of reducing atmospheric gases, such as hydrogen, methane and carbon monoxide, to trace levels.
Except to its primitive producer – cyanobacteria – oxygen would have been anathema to the dominant anaerobic Bacteria and Archaea that constituted Archaean life. An end-Archaean mantle overturn, implicated by the tectonic pandemonium from 2.7 Ga, could well have triggered accelerated extinction and evolution that encouraged the rise of the eukaryote cell that requires oxygen for its basic metabolism. Nonetheless, such an upheaval would have been directly connected with earlier living processes. That is something which will delight followers of the Gaia hypothesis.
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Siberian role in climate change? January 2001
Climate researchers at MIT in Cambridge, Massachusetts have analysed Northern Hemisphere climate data from 1972 to 1999, in the search for correlations that might help improve long–term weather forecasting. The most striking match to emerge is that of winter climate with the extent of autumn snow cover in Siberia. Snow reflects back to space a far greater proportion of incoming solar energy than any other kind of surface, with the exception of salt. More snow results in less warming in the area. Although Siberia is at the heart of the Asian continent, and therefore pretty dry, it has cold winters, so that when snow falls it covers large areas and tends to remain. It is the focus for an enormous mid–continent high–pressure area in winter, appropriately named the Siberian High, which is one of three systems that dominate northern climate.
High–pressure areas do two things: air spills from them into surrounding areas; they isolate the area beneath them from warming, moist winds blowing from the oceans. In winter the second creates cooling so intense that temperatures can steadily drop to –50°C or below , further building pressure because of the increase in air density. Siberia sheds cold air westwards into Europe and over the North Pole into North America. The MIT study bears out the obvious prediction based on this tendency. However, it may also add the Siberian High to the range of large–scale terrestrial processes – shifts in air pressure over oceans, such as the El–Niño of the tropical Pacific and the North Atlantic Oscillation, and thermohaline controls over Atlantic surface currents – that make ice–age climate patterns so complex.
Cooling of northern Europe and the Canadian Shield does not have to be very extreme to lower the topographic elevation at which snow remains permanently, the glaciation limit – at present that level is only a couple of hundred metres above the tops of Britain's highest mountains. Should permanent snow cover return to the highest areas around the North Atlantic, that would amplify the present effect of Siberian autumnal snow and expand the high–pressure area. That is a positive feedback driving climate towards increased frigidity, and larger winter highs would hold back maritime warming influences.
Computer modelling of the air–flow patterns over Asia shows that the primary influence is the Himalaya and Tibetan Plateau. In particular, they dry out air passing over them during the South Asian Monsoon, and hinder its influence further into central Asia. The two huge massifs seem to have risen rapidly and recently, beginning about 8 million years ago, despite the fact that India collided with Asia about 50 million years ago. Together with other roughly E–W high mountain ranges in central Asia, they also channel Siberian cold air to spill westwards and eastwards, and over the pole. Behaviour of the Siberian High almost certainly dates from the uplift of the Himalaya and Tibetan Plateau.
Adding another controlling factor to long–term northern climate has an intrinsic potential in refining academic studies of Pleistocene climate. However, there is an immediacy to the observations. For snow to cause cooling by reflecting away solar heat it does not have to be thick; a few centimetres will suffice. The critical factor is the area covered by it. Siberia is so cold in autumn and winter that it will snow there, provided moist air can enter. Should more get in then more snow will cover a greater area, to feed the positive feedback to cooling. Perversely, the more the climate warms globally, the more moisture evaporates from tropical and mid–latitude oceans to move polewards and towards continental interiors
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Mismatches from north to south proven January 2001
Whether or not climate changes, especially those of shorter duration than the full glacial–interglacial cycle, occur at the same time everywhere is something that vexes all climatologists. It encapsulates all the problems of causation: orbital forcing, thermohaline circulation, shifts in the Polar Front and Intertropical Convergence Zone, etcetera. The problem mainly stems from uncertainties in the correlation of time series that show proxies for climate change. This is particularly bad for ocean–floor sediment cores, which depend upon radiometric dates for calibration from depth to time sequences and an assumption of constant rates of sedimentation between dated samples. Imprecision often means that correlations are not believable, except at a very general level. Many analyses end up by correlating the patterns shown by the proxies, which defeats the object of assessing the degree of global synchronicity of climate changes.
Cores taken through ice sheets offer a way out, for annual layers of ice are there to be counted, but only in the upper parts. For deeper parts, converting depth to time relies on models of how ice compacts and how it thins by glacial flow. Another seeming advantage of ice-core records is that a great deal more ice accumulates than does ocean–floor sediment over a particular time. That means that the resolution of ice core records can be finer – potentially at the level of decades compared with hundreds of years for sediment cores. A seeming key to correlation between ice cores lies in the way that ice traps air. Being rapidly mixed, the atmosphere should have the same composition everywhere. This is particularly so for methane, partly because it soon becomes oxidised to carbon dioxide, and partly because its level is highly variable from emissions by rotting vegetation and unstable gas hydrate on the shallow ocean floor. Thomas Blunier and Edward Brook of Princeton University and the University of Berne used the methane records of Greenland and Antarctic ice to correlate the other proxies therein over the last 90 thousand years (Blunier, T. and Brook, E.J. 2001. Timing of millennial–scale climate change in Antarctica and Greenland during the last glacial period. Science, v. 291, p. 109–112). They show a consistent mismatch between rapid warmings of the air over the two polar ice sheets, where Antarctic changes precede those over Greenland by 1500 to 3000 years. Interestingly, when frigidity gave way to comparative warmth in a matter of a few decades over Greenland, the Antarctic was shifting from warm to cool conditions.
Commenting on the paper in Science's Compass, Nicholas Shackleton of Cambridge University shows yet more emerging oddities (Shackleton, N. 2001. Climate change across the hemispheres. Science, v. 291, p. 58–59). In the North Atlantic Ocean, surface water temperatures apparently changed according to Greenland's pace, while those for deep water match that of the Antarctic. To add to the complexity of climate change through the last glacial period – until a few years ago it was all supposed to link to the astronomical forcing of solar heating at high northern latitudes – the oxygen isotope changes in the same deep water of the North Atlantic match those of ice volume around the north pole.
Whereas Blunier and Brook have proved that air–temperature changes above ice sheets at high northern and southern latitudes are not synchronous, this still leaves problems in correlating between ice and sediment cores, and between the oceanic record at the many sites world–wide, especially those at low latitudes. With a growing number of hypotheses for climate changes of the order of a few thousand years – driven by changes associated with northern ice sheets, Antarctica and the tropics – onlookers await with interest the development of a means of precise correlation among all the time series.
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Role for tropical weather in last glacial epoch
December 2000
The Cariaco Basin off Venezuela lies in an area that is sensitive to climate change and has been for at least the last 90 thousand years. As the trade winds change with the seasonal migration of the Intertropical Convergence Zone (ITCZ), cold, nutrient-rich waters well up along the coast of northern Venezuela. Biological productivity waxes and wanes on an annual rhythm, as too do sediments transported into the basin by the great rivers of this part of South America – shifts of the ITCZ also impose annual wet and dry seasons over land. This cyclicity seems to have functioned since at least 90 ka ago, and drill cores from the Cariaco trench are dateable at the annual level because of the colour banding of seasonal sediments (Peterson, L.C. et al, 2000. Rapid changes in the hydrological cycle of the tropical Atlantic during the last glacial. Science, v. 290, p. 1947-1951).
Matching the varying thicknesses of colour bands beneath the Cariaco Basin to the high-latitude climate record preserved in Greenlandic ice-cores shows a remarkable correlation. Warming (interstadials) over Greenland correspond to periods of increased rainfall and ocean bio-productivity (the layers are thicker) off Venezuela. Peterson and his co-workers believe that this could signify periods of greater transport of water vapour from the Atlantic to the Pacific. That would increase the salinity of the Atlantic. Working through to high latitudes, saltier surface water would more easily become dense cold brine once sea ice had been frozen from it. That would enhance the thermohaline deep circulation of the North Atlantic, so that warm, tropical waters might be dragged further to the north during interstadials, in the manner of today's Gulf Stream. It is hard to see how just melting ice sheets during interstadials could do that; in fact that would encourage a further reduction of deep circulation. So, a tropical connection seems plausible. However, interstadials stopped extremely rapidly, repeatedly plunging high latitudes into full glacial, or stadial conditions. That may well have been an outcome of all the fresh water from melting glaciers acting to dilute surface waters' saltiness, and thereby shutting down thermohaline processes.
The annual precision of sediment cores from the Cariaco Basin carries a bonus, by helping better to calibrate 14C dating. Radiocarbon dates have long been known not to correspond predictably to calendar years. For instance, dates from around 11 ka ago, the time of the last major glacial advance (the Younger Dryas) show a mismatch of about a thousand years between dates based on counting tree rings and annual ice layers (exact calendar years), and those provided by 14C dating of carbon-rich samples. The reason for this is partly fluctuations in the production of 14C by bombardment of nitrogen atoms in the stratosphere by cosmic radiation and the solar wind. The Cariaco Basin layering extends calendar dating at least 5 000 years further back, into the period when deglaciation accelerated as the Earth's climate emerged from the last glacial maximum (Hughen, K.A. et al., 2000. Synchronous radiocarbon and climate shifts during the last glaciation. Science, v. 290, p. 1951-1954). That helps to evaluate shifting rates of 14C production over this part of the core (maybe related to varying solar output because they match shifts in 10Be, also produced by upper atmosphere processes), and to add meaning to radiocarbon dates from it. However, not all the shifts in 14C can be due to solar fluctuations, and it is clear that the largest, during the Younger Dryas event, stemmed from increased carbon preservation on the ocean floor, that removes all isotopes of such carbon from the atmosphere and upper ocean. This supports the notion that the Younger Dryas, and perhaps all the stadial-interstadial events of the last 90 ka stem from changes in ocean processes.
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No escape from global warming?
November 2000
Palaeoclimatology is well-funded because it is believed to shed light on the likely consequences of anthropogenic warming caused by CO2 emissions, and perhaps even technical solutions that allow us to continue burning fossil fuels. There is no doubt that throwing money at the range of associated phenomena and data has produced many astonishing findings and connections for the last 2.5 Ma. There is now sufficient high-quality data to reviewing them in their proper context; that of the climatic aspect of the "human condition". That is the task that yet another multinational group of scientists set themselves at an International Biosphere-Geosphere Programme (IBGP) workshop at the Royal Swedish Academy of Science in November 1999 (Falkowski, P. and 16 others 2000. The global carbon cycle: a test of our knowledge of earth as a system. Science, 290, 291-296).
The workshop used two generalized outcomes of many years of work on Antarctic ice cores: the variation over more than 400 ka of CO2 in trapped air bubbles with temperature shifts; the frequencies and amplitudes of changes in atmospheric CO2. They compare these with human effects over the last 200 years. A great deal of discussion and qualification surrounds the workshop's conclusions, but they are stark and simple. Anthropogenic change falls way outside that induced by natural processes (whatever they are), and its period bears no relationship to those involved in short- to long term processes. Despite the seeming attraction of technical fixes, such as boosting ocean productivity and the deep-water carbon sink (above), and intervention in terrestrial plant processes to increase CO2 sequestration from the atmosphere, both face the likelihood of weakening natural feedbacks due to the massive change that has taken place. Indeed, the consequences of strategies of these kinds aimed at mitigating climate change cannot be known in advance. This grim conclusion stems from the fact that no matter how well we get to know the climate system of the past, it is no longer what it was. Even a complete halt to all anthropogenic emissions now cannot reverse the trend in the short to medium term.
The group suggests Earth's entry into a new Epoch (the Anthropocene) of uncertainty, but brimming with growing knowledge. To them, this seeming paradox must not be "used as an excuse to postpone prudent policy decisions based on the best information available at the time". They also highlight the disciplinary compartmentalization of research that hinders a "proper" understanding of the Earth system. I suppose what they are getting at is the continuing ethos of Descartes' 400-year old reductionism in science, yet surely their call for a "systems approach " is merely dressing up reductionist empiricism in a more complicated guise; hurling yet more intricate maths at the problem. That is indeed the goal of climate modelling and has been for well over a decade. Perhaps the solution lies not in descriptive retrospection by scientists and in "policy ", but with society as a whole that now begins to confront the mismatch between several thousand years of divided human activity with the rest of the world.
Daniel Sigman and Edward Boyle, of Princeton University and MIT, USA, usefully review the whole issue of varying CO2 through the 420 ka Antarctic ice-core record, together with its environmental buffering (Sigman, D.M. and Boyle, E.A. 2000. Glacial/interglacial variations in atmospheric carbon dioxide. Nature, 407, 859-869). Their article helps see the views of Falkowski et al. from a broad and detailed context, and links to News from the South (above), because Sigman and Boyle conclude that while the pacing of climate change tracks the combined effects of orbital processes on solar energy input at high northern latitudes the "greenhouse" effect changes because of biological and physical processes in the Southern Ocean that surrounds Antarctica.
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The nudge of noise
November 2000
The emergence of a signal in the climate shifts through the last ice age and the Holocene with a roughly 1 000 to 1 500 year period (see Earth Pages Archive, A new regular pulse in recent climate, September 2000) finds no link with processes linked to Earth's orbital behaviour. It must be generated within the Earth system itself. That being said, there is a lot of debate over what precisely is involved. It's safe to say that debate will continue.
However, another factor might well be involved; one that is as much to do with statistics as with phenomena with sufficient power to flip climate patterns. Random noise is everywhere in nature. If strong enough at a critical time, such stochastic noise might resonate with an otherwise weak, periodic phenomenon to give it sufficient push that it shows up in a climate change. Let's say that there is some weak pulsation that bears on climate – not really known with certainty, but having a 1 500 year period. If resonance with noise was involved, we might expect to see 1 500, 3 000, 4 500 year periods in the climate record (1-, 2- and 3-cycle shifts), with the first more common than the last two – that is how the statistics should work. The fact that short-term climate pulses (the stadial-interstadial events) cluster around 1 000 to 1 500 years might indicate that random noise is implicated. However, only the last 120 000 years of climate data have sufficient precision for such statistical analyses, so it might be fortuitous.
The same nudge of randon climatic noise has also been called on to explain the jump from a roughly 41 000 year cyclicity to the present one of 100 000 years about 700 000 years ago. The first correlates with the period of changes in the Earth's axial tilt, and the second with changes in the eccentricity of its elliptical orbit. The effect of orbital variations on the energy received from the Sun is so very small that it cannot have much of an effect on climate by itself, but changes related to axial tilt are ten times bigger. The change in behaviour seven ice ages ago is therefore hard to explain, without the nudge of noise.
Source: Kerr, R.A. 2000. Does a climate clock get a noisy boost. Science, v. 290, p. 697-698.
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Plankton and the end of the Palaeocene-Eocene global warming
November 2000
Various geochemical signals show that the Palaeocene-Eocene boundary (at 55 Ma) was a time of global warming superimposed on the general Cainozoic cooling from the 'hothouse' of the Cretaceous Period. Some also point to an enhanced 'greenhouse' effect driven by massive methane release from gas hydrates on the sea floor. Methane, a 'greenhouse' gas in its own right, oxidizes to CO2 in the atmosphere, transferring its carbon that eventually ends up in the shells of marine organisms. It is the carbon-isotope blip at the P-E boundary that points to methane as a source of the warming. Not only does it appear in the marine C-isotope record from foraminifera shells in cores, but also in the teeth of terrestrial mammals, which means that the carbon reservoirs of both atmosphere and seawater were globally changed. Using the magnitude of that signal allowed palaeoclimatologists to estimate the amount of methane released – about 1 500 billion tonnes. On a millennial scale, that is comparable to a rate of warming similar to that currently induced by human activities.
The P-E boundary marks the most dramatic biological changes since the mass extinction 10 million years before at the Cretaceous-Tertiary boundary. But its underlying control is sufficiently close to what is happening to climate now to form both an object lesson and a means of modelling what may happen if current emissions continue. One of the important aspects needing scrutiny is how such warming events come to an end. British and American oceanographers have taken a look at the P-E record in ocean sediment cores, and believe they have come up with an answer, at least in part (Bains, S., 2000. Termination of global warmth at the Palaeocene/Eocene boundary through productivity feedback. Nature, v. 407 14 September 2000, p. 171-174).
Most such studies focus on oxygen- and carbon-isotope records in the carbonate of foraminifera shells, revealing ups and downs in seawater temperature and volume of land ice, and of biological productivity and releases of 'greenhouse' gases. Unfortunately, neither isotopic record properly resolves the alternative contributions to variation. Santo Bains and colleagues add another parameter that helps resolve the influence of biological productivity in the oceans. Marine organisms, especially plankton, either precipitate barium sulphate (barite) in tiny crystals within their cells or induce its precipitation once they die and decay. Because barite is not prone to much change by later events on the sea floor, counting its crystals in marine cores is a reliable proxy for the varying abundance of plankton through time.
One strong possibility during major warming events is that ocean circulation becomes sluggish, perhaps stopping altogether. That slows the re-supply of nutrients to sunlit upper layers, and works to reduce photosynthetic life in the oceans. The barite record produced by Bains et al. shows the opposite for the P-E events. For about 40 000 years after the P-E event biogenic barite rose to more than twice its normal abundance. The ocean biosphere responded to the methane blurt by blooming. Why it did so is not yet clear, but such a spurt in drawing CO2 into living and dead and buried tissue would work to reverse the warming event. The barite peak coincides exactly with the oxygen- and carbon-isotope records' features that signify temperature and the influence of isotopically light carbon from methane released by gas-hydrate breakdown. It might seem as if life did regulate climate in a geologically rapid manner following the P-E event, to the delight of Gaians. However, the control over biological productivity is ultimately nutrients, and life has little influence over their supply to the oceans. Among the possibilities for an essential nutrient bonanza, and increased circulation of the oceans is definitely ruled out during major warmings, are hugely increased rainfall to wash terrestrial sediments and dissolved matter into the oceans, and increased volcanism that would supply fine ash to the distant ocean surface.
Converging on an explanation for the end of a period of global warming is far from showing how this might be achieved for a warming induced by human activities. That might well prove eventually to be a life-or-death necessity for our species, bearing in mind that the P-E warming was a fatal crisis for many land mammals of the time.
See also: Schmitz, B., 2000. Plankton cooled a greenhouse. Nature, v. 407 14 September 2000, p. 143-144.
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A new regular pulse in recent climate
November 2000
Gerard Bond of the Lamont-Doherty Earth Observatory at Columbia University, Palisades, New York has taken his analysis of high-frequency climatic shifts in the last glaciation into the Holocene record. Previously, Bond had tried to make sense of the sharp fluctuations of the order of a few thousand years that are seen as gravel layers in the uppermost levels of sea-floor cores and in the oxygen isotope records of cores through the Greenlandic and Antarctic ice sheets. The first signs of short ups and downs in climate were the coarse layers first found by Hartmut Heinrich in the glacial part of the sea-floor record. Heinrich ascribed them to periodic releases of iceberg armadas as the ice sheets of the last glaciation became unstable. Bond's latest work also focuses on Heinrich events, but he has used specific lithologies as markers rather than merely grain-size variations. In particular, hematite-stained quartzo-feldspathic materials seem likely to have come from altered rocks in east Greenland and Svalbard, far distant from the drill sites whose cores he has examined. The proportion of reddish grains varies systematically in the cores, some layers coinciding with Heinrich events, but there are many more. The layers appear roughly every 1500 years. This periodicity coincides with cycles of dust blown from the Sahara to form layers in cores from the west African coast, so whatever the pulses represent, they are global signals.
Interestingly, the cycles show little sign of change in the period after the melt back that signified the beginning of the Holocene interglacial. Behind the long-term climatic shifts in glacials and interglacials, that coincide with the 100, 41, 23 and 19 thousand year fluctuations in solar warming of the northern hemisphere, some other process must be put-putting in the background. The 1500 year cycles may stem from processes that shift heat in the oceans and atmosphere. A likely candidate is the production of deep currents by sea-ice formation in the northern North Atlantic. However, detailed calculations of tides suggest a similar pacing that might change the mixing of surface and deep water in the ocean conveyor system.
Whatever the driving force, this periodicity strikes a chord with emerging details of Holocene climate changes from lake-sediments studies and the historic record. One such recent cooling pulse that might have delivered icebergs to mid-latitudes in the North Atlantic was the Little Ice Age that peaked in the 17th century that saw prolonged stresses on the population of Europe, and major political changes that resulted from such events as the Peasants' Revolt and repeated famines.
Source: Pearce, F. 2000. Feel the pulse. New Scientist, 2 September 2000, p. 30-33.
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News from the South
November 2000
Increasingly, evidence of many kinds points to a dominant influence on climatic ups and down through the last 2.5 Ma by processes in the northern hemisphere. Empirically, at least, the global-climate time series seems to show patterns that closely resemble Milankovic's predictions of varying insolation at high northern latitudes. For millennial-scale fluctuations, such as Heinrich events and the Dansgaard-Oeschger cycles in ocean and ice-sheet cores respectively, the focus is on changes in deep-water formation in the North Atlantic. The South cannot be set aside, however, and there are two important issues that crop up in October's publications. One is the extent to which climatic events in the southern hemisphere tracked those in the North, and the other is the role of the southern oceans in the global carbon cycle that underpins the climate-related fluctuations in atmospheric CO2 concentrations.
Both the Greenlandic and Antarctic ice cores show synchronicity of CO2 trapped in air bubbles with the records of local air temperature and global land-ice volume, going back over 400 ka in Antarctica. With more or less constant additions from volcanism, the ups and downs of the primary "greenhouse" gas have to be mediated by removal of carbon in one form or another from the ocean-atmosphere system through the agency of biological processes. Just what process, where it is most active and the controls underlying it form a topic of continual discussion and research. One possibility is variation in the biological productivity of the open oceans, coupled with removal of carbon from the ocean-atmosphere interface.
In terms of size and potential, the Southern Ocean is overwhelmingly the most likely candidate for a control. It is today the largest repository of unused nutrients in surface waters (by comparison with its potential for supporting phytoplankton it is a "wet" desert), but also a major source of deep-water formation that could sequester carbon from the surface environment. The late John Martin suggested that the main control over ocean productivity is soluble iron, currently at low concentrations far from land. The first realistic experiment to verify this involved "seeding" a small area of the equatorial Pacific with iron sulphate in 1995. Sure enough, that provoked a short-lived bloom of microscopic marine plants and local changes in dissolved CO2, but a boost in productivity at low latitudes is unlikely to lead to carbon removal from the surface part of the C-cycle.
Eighteen months ago, a multinational team of 35 ocean scientists conducted a similar experiment off Antarctica at 60°S (Boyd, P.W. et al. 2000. A mesoscale phytoplankton bloom in the polar Southern Ocean stimulated by iron fertilization. Nature, 407, 695-702. See also: Chisholm, S.W. 2000. Stirring times in the Southern Ocean. Nature, 407, 685-687). Once again bio-productivity soared by three times, and an input of 9 t of ferrous sulphate into about 50 km2 of ocean triggered an estimated 600 to 3000 t of extra algal carbon production. The "bloom" lasted for at least 6 weeks, being transformed into a swirling ribbon 150 km long. But it did not seem to be absorbed into deep water, merely mixing at the surface. In principle, iron dissolved from dust blown far from land during cold, dry episodes might have drawn down CO2 levels, but it is still uncertain. Yet the dust records trapped in ice cores do show a pronounced negative correlation with both CO2 and climate proxies.
Millennial-scale climate shifts are best known from the area around the North Atlantic. The most recent of these, and the most dramatic, was a sudden reversal from the warming trend out of the last glacial maximum around 13 ka ago, which lasted around 1800 years. This is recorded in many ways everywhere around the North Atlantic, and takes the name Younger Dryas (YD) from the associated increase in sediment cores of pollen of the cold-resistant mountain avens (Dryas octopetala). For some years there have been reports of a YD signal in climate records from the southern hemisphere, and some suggesting it was not felt there at all, the most detailed counter-evidence being the lack of the YD signal in Antarctic ice cores (ascribed by some to climatic inertia of the ice-bound continent).
The YD interrupted warming and wetting in the lead-up to the Holocene interglacial, so its signal ought to be easy to verify or rule out, simply because no later glacial advances have obliterated suitable investigation sites and many lakes at high altitudes and latitudes formed about that time. The problem for southern-hemisphere work has been a lack of precise dates. Southern Chile proves to be an excellent place to check, because lakes there go back further and contain evidence for many glacial advances and retreats (Bennett, K.D. et al. 2000. The last glacial-Holocene transition in Southern Chile. Science, 290, 325-328). Moreover, the sediment cores provide sufficient high-precision dates to construct a believably detailed time scale. Bennett and co-workers show that during the YD Chilean glaciers were retreating rather than advancing. That seems to knock the idea of "teleconnections" spanning both hemispheres for this particularly dramatic event, although its signal extends to the north Pacific. Like the mountain avens, however, disputing palaeoclimatologists are a hardy lot. It could be that the site of Bennett and colleagues work was far from a boundary between pollen-shedding species that was sensitive to climate change, despite the excellence of their record (see also Rodbell, D.T. 2000. The Younger Dryas: cold, cold everywhere? Science, 290, 285-286).
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Ups and downs of the "greenhouse" effect
November 2000
Several gases have the property of absorbing radiation in the wavelength range emitted by the Earth because of its surface temperature, including methane as well as carbon dioxide, the usual culprit. By doing so, they delay the escape of thermal energy through the atmosphere to outer space and give the Earth a higher surface temperature than it would have if they were not present. Because methane oxidizes to CO2 more rapidly than the latter gas's recycling time, a record of atmospheric carbon dioxide is the best guide to fluctuations in the "greenhouse" effect through the past glacial-interglacial cycles. Bubbles in cores through the ice sheets of Greenland and Antarctica trapped air at the time when snow converted to ice within a few decades after it fell in polar regions.
The publication of data of all kinds from the ice-core drilled beneath the Vostok camp in Antarctica (see Earth Pages archive – Milankovic forcing flawed? July 2000) opened up 420 000 years worth of atmospheric composition shifts. Daniel Sigman and Edward Boyle, of Princeton University and MIT, Massachusetts, review all the bio-geochemical factors that might have contributed to the CO2 time series for the last 4 major climate cycles (Sigman, D. M. & Boyle, E.A. 2000. Glacial/interglacial variations in atmospheric carbon dioxide. Nature, v. 407, p. 859-869).
While work continues to fully grasp this climate forcing function, Sigman and Boyle argue convincingly that the overwhelmingly dominant influence on it is the combined biological and physical carbon "pump" of the ocean around Antarctica.
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Milankovic forcing flawed?
Milutin Milankovic built on James Croll's notion that perturbation of Earth's astronomical behaviour is likely to cause variations in solar heating that might lie behind repeated glacial epochs. One of the most fertile discoveries in Earth science since World War 2 is that the periodicities that Milankovic calculated do seem to dominate the time-record of climate change over the last 2.5 million years, when 50 glacial-interglacial cycles forced changes in the oxygen isotope content of fossils from deep-ocean cores. These data record the variations in long-term storage of water in continental ice sheets, and are a near-incontrovertible 'proxy' for both varying extents of glaciation and sea levels Much the same kinds of signals also appear to turn up in time series of other kinds from sediments of a much wider range of ages. Milankovic theory now has as much popular support as Alfred Wegener's idea of drifting continents. But problematic aspects refuse to go away. Not the least of these is the conversion of depth to time in oceanic sediments from which the longest and most detailed records have emerged. An analysis of the frequencies involved in past climate change rests or falls on the accurate conversion of depths in sediment cores to time. In oceanic sediments this is by no means an easy job, because of a lack of material that can be dated precisely.
The first attempt to unscramble the complex variation in ocean cores used a few calibration points in climate time series onshore, whose shapes seemed to match those of ocean records. The most crucial of these was that for the rise in sea level at the end of the ice age before last (called Termination II) recorded in coral reefs in the Caribbean. The most widely used date for Termination II in the Caribbean is 127+6 thousand years (ka). It was from using this date as a global time correlation that the Milankovic signals of 100, 41, 23 and 19 ka periodicities popped out of the mathematical analysis. One surprise was that the match with the prediction of varying solar heating referred to the Northern rather than the Southern Hemisphere, or the planet as a whole. A great deal of later work hangs on that, and much of it has simply assumed the Northern-Hemisphere pacemaker, such as the widely used SPECMAP time scale.
Daniel Karner and Richard Muller of the University of California in Berkeley summarise the most contrary pieces of evidence for the timing of climatic change in a recent issue of Science (Karner, D.B. and Muller, R.A., 2000. A causality problem for Milankovitch. Science, 288, p.2143-2144). Using a different dating approach the Caribbean timing of Termination II comes out at 132 ka, while for a series of coral reefs in Papua New Guinea it appears as early as 142 ka.
Detailed climate changes recorded in stalactitic material from a cave in Nevada (Devils Hole) also show an 'early' Termination II. All these ages are as precise or better than the accepted 127ka date for Termination II, so Karner and Muller see a big problem. Whereas the end of the last glaciation (Termination I) is pretty well tied down to about 12 ka, and corresponds to increased solar heating in the Northern Hemisphere from the Milankovic predictions, Termination II bucks that by 5 to 10 thousand years. A theory that is only 50% believable needs a serious seeing to!
For the last four terminations, the most varied and informative data come from cores through the Antarctic ice sheet. Though that too has its problems regarding calibration of depth to time, a recent evaluation of the climate variations over the last 420 ka (Petit, J.R. et al., 2000. Climate and atmospheric history of the past 420,000 years from the Vostok ice core, Antarctica. Nature, 399, p. 429-436) shows significant differences between the last four terminations. Karner and Muller suggest that each glacial-interglacial cycle may have different controls, and encourage a new look at the wealth of data, unbiased by earlier ideas centring on pacing by a single, astronomical pacemaker and accepting that climate controls are multidimensional.
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Another nail in the coffin for fossil fuels
The 30- or more year long debate about anthropogenic climate change resulting from the 'greenhouse' effect of carbon dioxide releases by fossil-fuel burning has grown sharper in recent years. Some specialists have cast doubt on climatologists' ability to unravel human effects on the undoubted rise in mean surface temperature over the last 150 years from underlying fluctuations that stem from natural processes. Considering the number of forcing factors, both large and small and with different periodicities, such doubts are valid, even though they may well be overemphasised in order to support continued and rising use of petroleum and coal.
The climate record for the last millennium is known to have been one of considerable change, involving a mediaeval warm period during its first half and the so-called 'Little Ice Age' from around 1600 to the mid 19th century. Even within the recent warming trend there have been climatic ups and downs in the northern hemisphere, such as the mid-20th century warm period and several documented examples of cooling associated with major volcanism than punched aerosols into the stratosphere.
Thomas Crowley of Texas A&M University (Crowley, T.J., 2000. Causes of climate change over the past 1000 years. Science, v. 289, p 270-277) has attempted to isolate the known natural forcing functions and model their individual effects on mean surface temperatures in the northern hemisphere, to isolate meaningful signs of human effects from the various records temperature changes. Even charting the changes is no simple task, as most records are local to regional, rather than valid for the whole hemisphere. The most comprehensive climate data model uses proxy indicators from ice cores, tree-ring studies and coral time series, scaled to instrumental temperature records for the century from 1860-1965.
Uncertainty increases backwards with time, to around + 0.3°C in year 1000 AD. This is somewhat greater than the fluctuations recorded in the temperature reconstructions, that Crowley and others have derived by a complex statistical method that fits a smoothed trend to the temperature fluctuations modelled from proxy data.
The approach used in Crowley's analysis is to identify each likely, natural factor that influences energy balance in the northern hemisphere, and then to model the trends that they produced, and should continue to be producing. There are two factors that are significant in millennial to shorter timescales: influences of volcanic aerosols, as timed by ash layers in ice-sheet cores; and variations in solar output based on 10Be and 14C variations in ice cores and tree rings (solar radiation generates both at the top of the atmosphere). Possible anthropogenic forcing factors are numerous, including industrial aerosols and emitted gases other than the usual suspect, carbon dioxide. The end product is a temperature time series which removes the effects of all known forcing factors, except those connected with 'greenhouse' gases, from the northern-hemisphere temperature model. Until the early 19th century, this hovers close to zero variation, and then starts an upward rise to a value of about 0.75°C by now.
Crowley's modelling adds significantly to the case for a detectable economic influence on climatic warming, by showing that known natural forcings cannot account for the rising trend since the start of the Industrial Revolution. It does not prove the case, and leaves several features in recent climatic change unexplained, notably the cooling in the late 19th century. Also, this approach does not exhaust all possibilities involved in climate shifts, such as linked fluctuations in energy movement by ocean-atmosphere circulation that work to make some regions experience cooling while others warm. Such processes might respond to variations in solar-energy input by a kind of complex resonance, which remains to be looked at. See also: 20 percent more oil in the ground.
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Methane hydrate – more evidence for the 'greenhouse' time bomb
Where ocean water is more than 400 metres deep and bottom temperatures fall below 1 to 2°C methane and water can freeze to form crystals of methane hydrate. These efficiently absorb more methane in a gas-solid solution, known as a clathrate. Being lighter than seawater, methane clathrates do not carpet the ocean floor, but occupy pore spaces in sediments. Under the anaerobic conditions of marine sediments, bacteria break down buried organic matter to release methane. Build up of the gas in clathrates forms distinct reflecting horizons seen on many seismic sections of marine basins. Estimates suggest that methane clathrates contain around the same amount of buried carbon as all fossil fuels lumped together. Since methane is a powerful 'greenhouse' gas when released into the atmosphere, breakdown of the clathrates is a potential mechanism for global warming.
In 1995, evidence began to emerge that 55 million years ago, at the Palaeocene-Eocene boundary, a pulse of global warming probably stemmed from catastrophic release of methane from ocean-floor clathrates. The signs lay in the proportions of 12C to 13C in organic matter within marine sediments of that age. Since organisms selectively take up the light isotope of carbon, when organic matter becomes buried, seawater becomes enriched in 13C. Buried carbon, both in organic molecules and in marine carbonates, takes on the isotopic signature of seawater at the time. This means that the ups and downs of carbon burial leave an imprint in the carbon-isotope record of marine sediments. When warming of deep-ocean water or a pressure release caused by a lowering of sea-level releases biogenic methane from clathrates, its high 12C content quickly appears in the carbon in seawater as a whole, by oxidation to CO2 and solution. This reduces the proportion of heavy to light carbon in both buried organic matter and marine carbonates, forming a downward 'spike' in the carbon-isotope record. Other processes can produce the same effect, such as increased release of volcanic CO2, which is also isotopically light, or a collapse of the marine biosphere. So 12C 'spikes' need to be matched with other evidence.
Co-workers from Britain and Denmark have just reported in detail on just such an excursion that took place about 183 Ma ago, during a period of massive burial of carbon in the Jurassic Period (Hesselbo, S.P. et al., 2000. Massive dissociation of gas hydrate during a Jurassic ocean anoxic event. Nature, v. 406, p. 392-395). The Early Toarcian was a period where circulation in the deep ocean stopped, to give anoxic conditions, ideal for burial of dead organisms. While that lasted, important hydrocarbon-rich source rocks for petroleum reserves were laid down, and the carbon isotopes in sea water became unusually 'heavy'. Several stratigraphic sections show evidence for a 12C 'spike' in the middle of this period of general 13C enrichment of the oceans. Hesselbo and co-workers isotopically analysed Toarcian mudstones exposed on the Yorkshire coast in England, which contain both marine matter and fragments of wood formed in terrestrial ecosystems. Both show 12C enrichment, and that means that the entire carbon cycle at the time was somehow perturbed. With no sign of massive extinction, the signature pointed either to a methane release or to hugely increased volcanism.
Although there was strong volcanic activity on Earth during the Toarcian, it came nowhere near being able to generate the anomaly. Also the 'spike' occupies at most a period of a few tens of thousand years. Only catastrophic release of methane from clathrates, equivalent to 20% of those estimated to be present today, is able to account for the anomaly. Why it happened is nor certain; it may have been a result of either increased temperature of deep-ocean water by general global warming, to which it added, or perhaps too great a release of methane by decay in organic-rich sediments to be taken in by clathrates. Another trigger, for which evidence is lacking at present, is through a comet impact in an ocean basin.
Methane hydrate layers in the oceans pose an ever-present threat today, because of their extreme sensitivity to temperature and pressure. Some scientists believe that small releases may lie behind inexplicable disappearances of ships due to the drop in bulk density of seawater frothed by bubbles. Also many areas of shallow seas are pockmarked by vents marking methane release when sea level stood lower during glacial epochs, and at least one methane spike in ice-core records can be correlated with a massive submarine landslide off western Norway.
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Silica as a control over atmospheric CO2 levels
Today the oceans far from land are the equivalent of deserts, having very low biological productivity. This is not due to a lack of the main nutrients, potassium, nitrogen and phosphorus, or to too little sunlight for photosynthesis. For some time, marine specialists have suggested that the culprit is too little soluble iron – a micronutrient at the core of pigments and the enzyme RuBisCO, on which photosynthesis and the fundamental Calvin cycle depend. The halving of atmospheric CO2 levels during glacial maxima is widely believed to reflect more efficient ocean bioproductivity and thus burial of dead organic matter. The idea that general dryness and windiness during glacial epochs delivered soluble iron to the remote ocean surface is one means of explaining this. However, it took CO2 8000 years to rise to pre-industrial levels after the last dusty period when ice sheets reacehd their maximum extent, whereas iron lingers in seawater for only a few tens of years at most. Dust carries far more silica than soluble iron, and SiO2 resides for 15000 years or so. This encourages the blooming of silica secreting diatoms in competition with calcium-carbonate secreting plankton.
Carbonate production by cells actually generates CO2, so less carbonate secreters relative to those producing silica shells means that tendency is offset by a greater contribution to buried carbon from dead silica secreters
Source: Tréguer, P and Pndaven, P., 2000. Silica control of carbon dioxide. Nature, v. 406, p. 358-359)
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