Subducted slab being torn apart

The Mediterranean area is possibly the most tectonically complicated area there is.  It’s a plexus of microplates, all shuffling and jostling like guilty schoolboys accused of sticking gum under their desks.  That is a result of the misfit between the continental masses carried on the Eurasian and African plates, which was never resolved by the collision between the two that threw up the Alpine chain.  Complex as it is, the region is small enough, close enough to research institutes and pleasant enough to work in for there to have been a great deal of effort to understand its active plate tectonics.

The latest method to be applied is the analysis of seismic waves’ arrivals at seismometers in the manner of body scanning – seismic tomography.  Combining these new 3-D data of deep motions in the mantle with a review of surface geology, M.J.R. Wortel and W. Spakman of the Vening Mensz Research School of Geodynamics at the University of Utrecht build a remarkable picture of what seems to be going on (Wortel, M.J.R. and Spakman, W. 2000.  Subduction and slab detachment in the Mediterranean-Carpathian region.  Science, v. 290, p. 1910-1917).  One of their remarkable conclusions is a suggestion that subducted slabs are becoming detached, thereby changing the configuration of slab-pull forces in the region.  They sketch out how that might happen, by the formation of small ‘nicks’ in the short subducting slabs that focus slab-pull force along the reduced length of intact slab.  Thus focused, the pull more rapidly helps propagate the “nick” into a fully-fledged tear, which will migrate over the remaining length of the subduction zone.

Mechanically, that is interesting enough, but should it happen at a shallow depth influx of asthenosphere would generate magma on a small scale, and perhaps induce hydrothermal activity and unusual sequences of metamorphism in the overlying crust.  Isostatic responses might change depositional process at the surface too.  Wortel and Spakman suggest that there is geological evidence throughout the region for this process having operated in the past, with consequences such as these, as well as going on today.

Role for tropical weather in last glacial epoch

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.

Slime to the rescue

In waters that are anaerobic, metabolism of dead organic matter requires a means of accepting electrons transferred away from the necessary oxidation, other than that which involves oxygen as an electron acceptor.  Some heterotrophic bacteria achieve this by the simple chemical trick of reducing sulphate ions (SO42-) to sulphide ions (S2-).  This form of heterotrophy does not oxidise carbohydrate back to carbon dioxide plus water, but produces methane.  In the context of economic geology, it is the generation of sulphide ions that is more interesting, for any dissolved metal ions will swiftly combine with sulphide to form highly insoluble sulphides – the general form taken by many ore minerals.  This is the process observed to occur around deep-ocean hydrothermal vents, where biogenic sulphide ions cause metals dissolved in the hot water to precipitate and form the dark clouds from which such vents get their name – “black smokers”.  Many metal deposits are now known to have formed in such an environment, notably the volcanogenic massive sulphide or VMS ores.

However, there are many sulphide ores that have no obvious relationship to hydrothermal vents, such as sediment hosted deposits like the massive lead and zinc sulphide deposits of the Mississippi type.  Moreover, most sulphate-reducing bacteria are intolerant of oxygen whereas sediment-hosted deposits often bear isotopic witness to the presence of oxygen.  But, deposits of that kind often show intricate fine banding, suggesting slow deposition of fine-grained sulphides.  Some light is thrown on the problem by a daring piece of research involving sampling from flooded caves in a flooded Pb-Zn mine in Wisconsin (Labrenz, M.  et al. 2000.  Formation of sphalerite (ZnS) deposits in natural biofilms of sulfate-reducing bacteria.  Science, v. 290, p. 1744-1747).  SCUBA divers recovered scum formed by bacterial filaments or biofilm, and analyses showed the clear association of the bacterial cells with nanometre-scale spheres of zinc sulphide.  The species of sulphate-reducing bacteria involved is not exactly oxygen-loving, but will tolerate moderate levels dissolved in water.  Here clearly is a means for the formation of low-temperature massive Pb-Zn sulphide deposits.

The astonishing feature of the results of Lanbrenz and co-workers is that the zinc sulphide forms from water with very low levels of the metal (less than one part per million).  The bacteria, or at least their metabolic products, scavenge the metal, and quite probably dangerous cadmium, extremely efficiently.  Chances are that similar bacteria could also pick out lead and arsenic.  That opens up a new means of  bio-remediation – clean-up of both mine waste and contaminated drinking water.

The activity of sulphate reducers leaves its signature on the sulphur isotopes of ancient sediments, revealing periods when the burgeoned, as in Phanerozoic black-shale strata.  They were most active in this respect before about 2 billion years ago, when atmospheric oxygen levels were so low as to diminish oxidation by that highly active gas.  It seems that sulphate reducers also promote the precipitation of dolomite – (Ca,Mg)CO3 – over that of calcite in sea water.  This tallies with the common association of dolomitization of calcite in many sedimentary sulphide deposits, and also with the predominance of dolomites over limestones in the early Precambrian. [see also:  Vasconcelos, C. and McKenzie, J.A. 2000.  Sulphate reducers – dominant players in a low-oxygen world.  Science, v.  290, p. 1711-1712].

More evidence for water on early Mars?

The Mars Orbiter Camera aboard the Mars Global Surveyor spacecraft is one of those little irritations that irks Earth-oriented remote sensers.  It captures pictures with resolutions as fine (1.5 m) as those from “spies in the sky” of a decade back, and the best commercially available imaging systems in orbit around our home world (they cost between US$16 to 44 per km2).  Nor surprisingly, geologists interpreting features of the Martian surface are having a heyday (there is no damned cloud or atmospheric haze either, and it’s the dry season all the time!)

Nearly every report focuses on water, either that supposed to have flowed after recent (most unlikely) melting of ice in the upper veneer of Martian “soil” (see Earth Pages xx  2000, and the episode of catastrophic melting early in Mars’ history  that cut huge valleys.  The latest shows abundant topographic features that speak plainly of layer-cake sediments (Malin, M.C. and Edgett, K.S.  2000.  Sedimentary rocks of early Mars.  Science, v. 290, p. 1927-1937).  Even unconformities and exhumed channel-like features show up, and some of the deposits partly fill ancient impact craters.  While aeolian and volcanic processes, and those associated with impact ejecta might all form sediments – we can be certain that all these processes have operated on Mars – to conclude that some of the sediments might be waterlain is not so easily assumed.  Thankfully, Malin and Edgett are cautious, for there is no definitive sign that the Martian sediments are waterlain – but some might have been.

Having just returned from a technical meeting with people working for humanitarian relief agencies, and heard of their needs for remote-sensing data that should show up habitations clearly enough to estimate numbers of people affected by disasters, I did not read this paper with any great relish.  NASA’s determination to convince itself that indeed water lies waiting to be tapped on the “Red Planet” by the first staffed mission there sits uneasily with the fact that the best part of a billion people on Earth have neither enough nor much with a safely drinkable quality.  It’s a pity that there isn’t an “Earth Orbiter Camera” that would serve their needs rather than those of a few earnest astronauts and some ambitious bureaucrats.

Early life survived lunar cataclysm

The last real “geology” on the Moon was the formation of the maria and their filling with basaltic magma.  Both resulted from the unimaginable energies released by a storm of impacts on the lunar surface, from which the Earth cannot conceivably have escaped.  This “late, heavy bombardment” occurred between 4.15 and 3.8 billion years ago, and overlapped the ages of Earth’s oldest rocks in West Greenland and Northern Canada (The Akilia supracrustals and the Akasta Gneiss respectively, dated around 4 billion years).  Such was the energy involved in each of the maria-forming impacts – and the Earth would have had more and bigger impacts at that time – that it seems likely that any surface water on our planet would have boiled away.  That poses the issue of whether life emerged several times, only to be literally blown away and having to start over.  Two sets of new data help answer this awful question.

Though they have been sitting in Houston for a generation, the Apollo lunar samples still provide useful information.  In the early 1990s precise dating of glass spherules in lunar soil samples found evidence for 12 impacts, but they clustered around 3.9 billion years.  It was this find that supported the cataclysm  proposed on stratigraphic grounds from photo interpretation of the maria.  When planets form, they undoubtedly do so by accreting debris from the vicinity of their orbits.  However, their growing gravitational attraction intuitively suggests that the big chunks are swept up early in planet formation.  On those grounds it can be predicted that additions tail off in mass and impact energy over time.  So there should be a spread of ages from about 4.5 billion years onwards of a dwindling number of big events.  The lunar glasses buck that trend severely, as do the ages of the voluminous maria lavas, for there are few ages between 4.5 and 4.0 billion years.  One objection has been that later events obliterate signs of earlier ones.  Another centred on how a clutch of whopping impactors might survive in Earth’s orbit without having been swept up early on, or how a maria-forming storm of many such bodies might have appeared in the Earth-Moon vicinity almost simultaneously from elsewhere in the Solar System.

The monster events are mainly on the Moon’s near-side, which is where the Apollo samples come from.  Consequently, the objection to the “late, heavy bombardment” seems valid – the data could be biased.  Meteorites found on the Earth, which have geochemistries signifying a lunar origin, potentially offer a check, because they could have formed by late impacts anywhere on the lunar surface, including the unanalysed far-side.  Barbara Cohen, Timothy Swindle and David Kring of the University of Arizon, Tucson, report ages of glasses from four such meteorites (Cohen, B.A. et al., 2000.  Support for the lunar cataclysm hypothesis from lunar meteorite impact melt ages.  Science, v. 290, p. 1754-1755).  All the glasses show evidence of having originated from the ancient, anorthositic lunar highlands, which dominate the far-side.  The results show seven distinct events, and none are older than 3.9 billion years.  Although the work began as a way of perhaps disproving the cataclysm, it turns out to support it even more strongly.  It still poses the question of how and where the bulky culprits appeared.  One possibility lies in the idea that the outermost giant planets, Uranus and Neptune entered their present orbits far later than expected.  Harold Levinson (in press, Icarus) of the Southwest Research Institute of Boulder , Colorado, has suggested that the two planets’ materials accreted between Jupiter and Saturn, but eventually became orbitally unstable, and zoomed off into the outer limits.  The gravitational perturbations by such a theorized event would have been immense, sufficient to set the asteroid belt and the much more distant source of comets juddering.  [See also:  Kerr, R.A.  2000.  Beating up on a young Earth, and possibly life.  Science, v. 290, p. 1677].

Whatever the debate about the “late, heavy bombardment’s” possible tight time span, at the time the Moon did experience awesome delivery of impact energy, and so must have the Earth.  Hence the deep interest in its effect on living processes.  The Akilia sedimentary rocks of West Greenland formed at least 3.85 billion years ago.  Carbon isotopes trapped in minerals that are resistant to metamorphic effects show beyond any reasonable doubt that living things, probably primitive bacteria, dwelt in the waters that laid down the Akilia sediments.  If the cataclysmic bombardment still going on at that time had been continually thwarting lifes puny efforts at survival, then the Akilia rocks should contain a lot of elements concentrated in asteroidal material.  They should be rich in iridium, the ubiquitous signalling element of the Chicxulub impact that terminated the Mesozoic.  Curiously, they are not unusual in that respect.  In a paper soon to be published in the Journal of Geophysics Research (Planets), Ariel Anbar and Gail Arnold of the University of Rochester in New York will report a distinct lack of success in finding iridium spike in the Akilia sedimentary rocks (Source:  Hecht, J.  2000.  It’s a bug’s life.  New Scientist,1 December 200 issue, p. 11). 

Other searches for iridium spikes in early Archaean rocks have also proved fruitless, although impact-generated glass spherules have been found in the sediments of the Barberton greenstones of Swaziland.  That rules out a continuous bombardment by giant impactors.  Quite possibly big impacts came only every 10 to 100 Ma.  Also, the discovery of primitive bacteria living today in cracks in hot, deep rocks as well as around ocean-floor hydrothermal vents, suggests a high chance that such hyper-thermophilic life might well have survived anything the Solar System might have flung at it.  Molecular phylogenies of bacteria seem to point strongly to all life having arisen ultimately from heat-loving ancestors.  Quite possibly, the “late, heavy bombardment” shaped the molecular basis for all later biological evolution.  Certainly, many bio-molecules in all modern cells are but a short chemical step away from the heat-shock proteins possessed by modern hyper-thermophiles.

Delusions of adequacy?

Earth science competes for space in both the prestigious scientific journals, Nature and Science, and the popular science press with the rest of the sciences.  2000 AD was the year of the genome (human and watercress), nanobots, AIDS in Africa, the quark-gluon plasma of the Big Bang, killer proteins and stem cells.  In Nature’s review of the year (2000 in context.  Nature, v. 408, 21/28 December 2000 issue, p. 894-904), only water on Mars and global warming figured as aspects of Earth science with “big-push-forward” status.  No doubt Science will conclude much the same, in the manner of the Time-Newsweek topic tracking.

The 2000 AD issues of Earth Pages have shown that, even in the pages of the “Big Two”, Earth scientists  from many branches have had that wider impact that heads everyone’s wish list, but one that continues to dwindle in proportion to other headlining subject areas.

A publication in Nature or Science is today a waving Papuan head-dress, not just a feather in a researcher’s cap.  An item in News and Views or Perspectives, provoked by their publication, is the nearest Earth scientists ever come to a Nobel Prize, for the eponymous pyrotechnician eschewed the breadth of our discipline.  Well, perhaps not the ultimate “gong”, but definitely an accolade that did not stem from incestuous back slapping.

My personal Hogmanay thought, in the run-up to the odd “cup of kindness”, is a bit depressing.  If a department that inwardly congratulates itself – probably about now in its end of year festivities – on the quality and quantity of its research neither features in News and Views, nor in the popular-science press, does it really have any status?  It seems no longer enough to pursue “scholarship” for its own, self-defined sake, as if it ever was.  Without more effort to raise awareness, in the widest sense, of Earth science’s relevance, much of it risks being sidelined.  Whose interest do we serve now, and how should we foster wider impact beyond the Disneyesque view of the K-T boundary and that of the damp anorak seen dimly in the mist?

Comments welcomed!  Maybe Earth Pages should open a discussion on “branding” in the New Year.

Petals unfolding on ASTER

The 15-channel imaging system aboard the first of NASA’s Earth Observing System constellation of satellites (Terra) began to demonstrate its potential in November.  The 9 month delay between Terra’s launch in December 1999 and the appearance of its first scientific data irked many potential users, already chewing carpets because of the 18 month delay in the launch.  However, wrangling between ASTER’s designers at ERSDAC, the Japanese space agency, and NASA was resolved by November 17th.  If you are interested, the data can be accessed at the new EOS Data Gateway (edcimswww.cr.usgs.gov/imswelcome/).  Some 70 000 scenes are already “in the can”, but slow processing means that only a trickle of calibrated (Level 1b) data adds to the archive daily, so that cover is very patchy at present.  Nonetheless, quality of cloud-free scenes is excellent, and the new potential, especially for geological challenges, is dramatic.  It is worth noting that the data are in a somewhat difficult format, and can be had either on tape (tar format) or by ftp downloads (file format 125 Mb per scene).  The EOS Data Gateway does plan for release eventually on CDs..

More molecular evidence for Cro-Magnon migration into Europe

For two weeks in December both adults and infants in Britain have been plagued by nightmares figuring the superb prosthetic and dramatic reconstruction of a Neanderthal family in Channel 4’s Neanderthals.  As London University human geneticist, Steve Jones, has observed, “If you met an unwashed Cro Magnon dressed in a business suit on the Underground, you would probably change seats.  If you met a similarly garbed Neanderthal, you would undoubtedly change trains”.  Of course, the big issue is not that Neanderthals were muscled hulks with gigantic noses, beetling brows and little in the way of chins, but who were the interlopers that drove them to oblivion?  Apart from the fact that Neanderthals portrayed Cro Magnons as being pretty cool, with a trendy line in face paint, there is little doubt that their only advantage over the chinless ones was one of lifestyle.  Being migrants from Africa via the Middle East, Cro Magnons had to have been nomadic hunter gatherers.  Neanderthals had survived at least two full ice ages in Europe, and subsisted from fixed ranges around their homes.  Game husbandry in a severe climate meant two things: small Neanderthal bands supported by large ranges, and little communication with neighbouring bands.  Entry of nomadic hunters into ranges inevitably depleted resources for the territorial first occupants, without the two groups even coming into direct conflict.  Nomads can move to fresh hunting grounds, thereby avoiding starvation.

Recent molecular studies of modern mens’ Y chromosomes (see also Eve never met Adam, October-November 2000 Earth Pages) confirms archaeological evidence that the sad drama of Neanderthal decline and eventual extinction began with the entry of fully modern humans about 40 000 years ago (Semino, O. et al., 2000.  The genetic legacy of Paleolithic Homo sapiens sapiens in extant Europeans: a Y chromosome perspective.  Science, v. 290, p. 1155-1159).  Eighty percent of modern European mens’ Y chromosomes stem from two ancient haplotypes.  The divergence can be calculated to have occurred around 40 ka from one now vanished, apart from its trace in molecular relatedness.  That trace itself is related to another, older one, found in modern Siberian and native peoples of the Americas.  It looks as if migrants from Africa remained fixed for a long time in the near East, then to move west and east as the climate cooled.  It was the carriers of the now dominant European male Y chromosome that interacted ecologically with the Neanderthals, to the extent that the latter died out.

The molecular statistics suggests that these early “Aurignacian” people – named after their stone-tool culture recovered from archaeological sites – dominated northern Europe.  Deepening glacial climate forced them into refuges in the Ukraine and Iberia during the last glacial maximum around 24 to 16 ka ago.  At this climatic low point, a further migration into southern Europe emerges from the genetic analyses; that of a population which probably brought in the more advanced “Gravettian” culture.  They too survived in a refuge, but in the Balkans.  The fact that the Aurignacian genetic trace is so dominant among European men today probably signifies that its population moved rapidly out of its refuge areas, growing numbers re-stocking much of the continent left empty by the demise of the Neanderthals.

Considering the explosive influence of an entirely different culture on the history of Europe during the last 10 thousand years – that of agriculture – it comes as a great surprise that genetic evidence of its likely source is restricted to at most 20 % of modern Europeans.  Four new mutations can be dated to have appeared around 9 000 years ago, at the beginning of the Neolithic explosion from which all modern economies date.  They almost certainly arose in the “fertile crescent” of the Middle East where farming first shows in the record around that time.

In the same way that Channel 4’s Neanderthals came to be made, the evidence needs imagination to enliven it.  One thing does seem likely; the earliest modern Europeans probably learned their farming, and possibly much else besides, from a trickle of new immigrants, once climate had finally improved to a near-modern state.  More intriguing is to wonder why the earliest Cro Magnons were moved to walk into an increasingly frigid Europe in the first place.  Were they pariahs in what became the “fertile crescent”?  Did they get sick of oppressive “Big Men” who ruled the roost there?  Incidentally, that seems to have spurred much of the historical movement of peoples in Africa.  Or, did drying at low-latitudes, which accompanied more northerly cooling, mean that worsening conditions in the Middle East demanded urgent migration in any direction that presented itself?  Perhaps we shall see a drama relating this story, and the sudden explosion of art at the depth of an ice age.  An expression of relief and celebration of good luck?

See also:  Gibbons, A.  2000.  Europeans trace ancestry to Paleolithic people.  Science, v.  290, p. 1080-181

Discovery of huge primate buttock print

The search for the Sasquatch is a story that runs and runs.  Generally it has been stoked up by dubious evidence, such as plaster casts of gigantic footprints and a film of a rather portly and somewhat camp being striding through the woods of Washington State.  Scorn poured on “Bigfoot” research by zoologists and anthropologists may have to be retracted after the latest revelation (Kleiner, K.  2000.  Bigfoot’s buttocks.  New Scientist, 23/30 December 200 issue, p. 8).

The Bigfoot Field Researchers Organization set out in September to lure a Sasquatch with a mixture of pheromones (whose, I wonder!), supposed cries of wandering, pedally challenged anthropoids, and…. apples.  The trap was laid in a muddy clearing in the Gifford Pinchot National Forest of southern Washington state.  The following day, researchers found an impression interpreted as that made by forearm, hip, thigh heel and a gigantic, hairy bottom, as if some naked… thing… had sat down to munch the bait.

Now this is exactly what I would have needed to sustain my early belief in Santa Claus; something going beyond the drained sherry glass and crumbs of cake on the hearthstone.  Using comparative anatomy, the prints suggest a being more than 2.5 metres tall, in keeping with the well-known size 24 feet.  Personally, I get the whiff of smoked fish, because the heel print bore markings remarkably like those of human fingerprints.  As they say, the jury is still out….., probably having a stiff drink.

Earth’s core

New Scientist’s excellent Inside Science pull-out series now includes one on the Earth’s core (Bowler, S. 2000.  Journey to the Centre of the Earth.  Inside Science #134,  New Scientist 14 October 2000).  This covers the origin and evolution of the core, how geologists can assess its composition and structure, and the link between motions in the core and the fluctuations in the Earth’s magnetic field.  Like all the Inside Science pull-outs, Sue Bowler’s treatment is at a level easily followed by non-Earth scientists but nonetheless informative and up to date.

Fish ears at the Eocene-Oligocene boundary

About 33.7 Ma ago, at the Eocene-Oligocene boundary marine invertebrates suffered their largest downturn in the Cainozoic.  Marine-core oxygen isotope records suggested that this coincided with a major cooling, when East and West Antarctica both possessed ice sheets.  Deep ocean water temperatures, recorded by the oxygen isotopes of benthonic forams, fell by 3-4°C, yet surface waters at low latitudes appear to show little detectable change in the isotopics of planktonic forams.  Data from cores become less well resolved in time, the older the sediments are, for a variety of reasons.  Tying down a climatic cause for the E/O extinction demands much better precision.

From an astonishing piece of ingenuity and technical skill, we are closer to an answer.  Lida Ivany and colleagues, from the Universities of Michigan and Syracuse, USA, collected the tiny ear bones or otoliths of fossil fish from a boundary section on the Gulf of Mexico.  Because these grow with the fish and contain growth layers, potentially they can give resolution to the level of a single season.  The trick is to get samples on a layer by layer basis and then analyse the tiny masses so extracted for oxygen isotopes.  That is what the team managed to do (Ivany, L.C. et al.  2000.  Cooler winters as a possible cause of mass extinctions at the Eocene/Oligocene boundary.  Nature,  407, 887-890).  Comparing the fine detail from Eocene and Oligocene fish ears shows that the local climate was much more seasonal in the early-Oligocene.  While summer temperatures stayed at much the same level as in the immediately preceding Eocene, early-Oligocene winters were much colder.  That would account for the inability of marine core data to detect any significant global cooling, and seasonal contrasts could have knocked out marine invertebrates evolved to more equable conditions.

News and Views in the same issue of Nature includes a fascinating look at these novel data in the context of wider knowledge of what was happening at the E/O boundary (Elderfield, H.  2000.  A world in transition…  Nature,  407, 851-852

Primordial slime

A timeless phrase from the film One-eyed Jacks is Marlon Brando’s, “You ain’t nothin’ but a ball o’ spit”, to the oppressive and corrupt lawman played by Slim Pickens.  Some molecular biologists would come close to agreeing, though not in anyway to mock that fine actor.  In Lyn Margulis’ theory of endosymbiotic origin for the Eucarya, of which we are a multicellular one, a candidate for the organism that played host to several others that went on to become eucaryan organelles is a slimy beast.  It is Thermoplasma acidophilum, a member of one of the three fundamental domains of living things, the Archaea.  Thermoplasma has no proper cell wall, contains DNA with proteins like those which bind nucleic acid in eucaryan cells, and it thrives in burning coal heaps.  It is pretty much slime that needs both highly acid and very hot conditions to metabolise, and both result from the spontaneous oxidation of sulphides in coal exposed to air.  Its very sliminess makes it worth considering as the original envelope for the baggage of the first Eucarya, so that they could get in.  It is also an anaerobic fermenter – a methanogen – on whose waste products aerobic Bacteria might live while protecting the host from oxygen that would be highly toxic to it and perhaps supplying it with useful chemical products.  Very roughly, that is how Margulis explained mitochondria, the organelles that are common to all eucaryan life.  For a symbiosis to become a cellular unit from which all animals, plants etc descended demands an exchange of genetic material between all the participants, so that they become incapable of independent reproduction.

A few months after gongs were beaten to announce the completion of the human genome sequencing, Andreas Ruepp and colleagues from Germany and the USA laid out the genome of the loathsome Thermoplasma (Ruepp, A. and 9 others  2000.  The genome sequence of the thermoacidophilic scavenger Thermoplasma acidiphilumNature, 407, 508-513).  Thermoplasma, being an “extremophile” is also a candidate for having evolved in the hot environment of sea-floor, hydrothermal vents.  It comes equipped with so-called heat-shock proteins, that eucaryan cells have turned to a multiplicity of other uses in their later, cooler, oxygen-loving evolution.  The astonishing feature of its genome is that it is either a molecular thief or prone to being burgled.  Many of its genes are identical to those in the sequences of other bacteria species whose habitats overlap with that of Thermoplasma.  As well as offering little hindrance to large molecules entering it, the archaean seems not to generate enzymes that in many other cells detect and destroy alien DNA.  The fact that Thermoplasma shows less affinities with eucaryan genetics than with that of Bacteria, suggests that it probably was not our ultimate ancestor.  But that is hardly surprising, since such an organism would have had to share an environment with aerobic ancestors of organelles, one very different from the high temperatures and low pH of Thermoplasma and its fellows.  To me, the new information serves to show strongly that an endosymbiotic origin of the Eucarya was indeed possible, given this mixture of larcenous and tolerant metabolism.

See also: Cowan, D.  2000.  Use your neighbour’s genes. Nature, 407, 466-467

Eve never met Adam

A bit of molecular biology never did Earth scientists any harm, and new research on connectedness in DNA between people now living in different parts of the world sheds new light on the origin of fully modern humans.

All humans are, at most, one tenth of a percent different in their genetic make up; we are ten times more closely related than are chimps from different bands in the forests of West Africa.  This low variance almost certainly results from the origin of fully modern humans in very recent times.  The well-known comparison between DNA in mitochondria (mtDNA) of people across the world points to a divergence in our “bush” of descent about 140 000 years ago.  Because mtDNA passes through the female line, this aspect of modern human origins has been said to stem from a mitochondrial “Eve” living in Africa at the time.  This does not mean that only one fully-modern woman was alive at the time, but that lines of descent from others died out subsequently.

The other side of the evolutionary coin is descent worked out through the male line.  Molecular biologists have focussed on DNA in Y-chromosomes that only men possess and pass on to their sons.  A team at Stanford University in California used cell material from over a thousand men from 24 widely separated regions to investigate relatedness and divergence with the highest precision yet.  Their results point to a time of divergence between 50 and 70 000 years ago; half that for female inheritance.  While the mismatch certainly knocks creationism and its literal reading of the Old Testament still further out of the park, how the mismatch arose is hard to fathom.  One possibility is that a mutation affecting Y-chromosome DNA only imparted such an advantage to the males who carried it that their descendants survived, while those not so favoured had their lines snuffed out.  Alternatively, it may simply have been that some important technological discovery, or maybe even a cultural change, such as art that seems to first appear in Africa around 70 000 years ago, gave a very small family group the potential for only their descendants to survive through 3 to 4 000 generations.  Whatever, the “bottleneck” through which all our genes passed at the time was in Africa.

Source:  Cohen, P.  2000, Eve came first.  New Scientist, 4 November 2000, p. 16.

The undead

The notion of bringing to life ancient organisms carries overtones of Jurassic Park, and more scientifically those of contamination by modern organisms.  But has it been done?   Russell Vreeland and colleagues from West Chester University, USA, claim to have cultured bacteria preserved in fluid inclusions from a Permian salt deposit (Vreeland, R.H. et al.  2000.  Isolation of a 250 million-year-old halotolerant bacterium from a primary salt crystal.  Nature, 407, 897-900).  The stringent conditions of sampling suggest that indeed this is an old bug, as does the fact that it seems to be a salt-tolerant bacterium.  However, it is hard to believe that living organic material can survive without apparent damage for so long.

In the accompanying News and Views pages, John Parkes, of the University of Bristol, UK, discusses the ramifications, and that surrounding claimed revival of bee-dwelling bacteria from Miocene amber.  Some are worrying. Bacterial spores might survive indefinitely, to be released on an ill prepared world that has lost any shred of resistance to pathogens.  Others bring a spark to some dormant ideas, particularly that of life spreading galactically by meteorite transportation.

Chinese crust in miraculous escape

Ultra-high pressure (UHP) metamorphic rocks from the Yankou region in China have been down a subduction zone to more than 200 km and then rebounded to the surface.  Kai Ye, Bolin Cong and Danian Ye of the Chinese Academy of Science in Beijing have worked on barometric indicators from eclogites and garnet peridotites to reach this conclusion (Ye, K. et al. 2000.  The possible subduction of continental material to depths greater than 200 km.  Nature, 407, 734-736).  It is no surprise to learn that basaltic and peridotitic materials have been down a subduction zone, because that is what oceanic lithosphere does continually, though how they return to the surface as intact slabs is problematic.

What is surprising is that such highly compressed rocks are associated with similarly UHP materials that are chemically normal materials of the continental crust.  The Yankou rocks now hold the record for deep diving.   Sialic subduction is not easy because of its reluctance to reach densities that exceed that of the mantle.  That being said, there are growing suspicions that continental materials may contribute to the composition of alkaline magmas formed deep beneath hot spots.  If sial does not reach 200 km depth, its density always lies above that of the mantle, and it must be buoyant.  Taken deeper, however, the situation reverses because of phase changes that compress silica and feldspar, so that at 300 km depth they become much denser than mantle, and must continue sinking to become potential contributors to later mantle melting.

In this case it seems as if the slab of Chinese sial was dragged from the lower crust by its attachment to enough basic and ultrabasic rocks that the whole lot broke the buoyancy barrier by their density change at high pressures.  Getting back to the surface poses the big problem, the authors proposing that they were rafted by rocks beneath them.  Somehow, a large mass of UHP basic-ultrabasic material must have become detached from sialic materials before the combined slab passed the 300 km boundary and became doomed to long-term mantle residence.  That would give them and any eclogites remaining attached to them sufficient buoyancy to bob up once again.

Ups and downs of the “greenhouse” effect

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.

News from the South

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).

No escape from global warming?

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.

The nudge of noise

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.

Heads or tails?

The basalt floods draped over some great continental plateaux and considerable areas of the ocean floor, ocean islands far from plate boundaries and the volcanic provinces sitting at the ends of various oceanic island chains are with little doubt the product of plume-like masses rising from great depth in the mantle.  What is not so well agreed is just what bit of a plume underwent partial melting to make the magma, the depth at which that took place and the prevailing temperature.  There is some support for plumes that rise from a mantle transition zone about 700 km down, where there is an abrupt increase in temperature.  Such plumes form a hot head when they impact the lithosphere, and that should be the source for magma.  Plumes that rise from the core mantle boundary, should in theory have heads that are cooler than their tails, and which grow hugely by being stalled at the 700 km discontinuity.  The two combined might form little plumes that rise from a big head at 700 km that spreads laterally.  Nicholas Arndt gives a neat summary of these unseen ramifications in a recent issue of Nature (Arndt, N.  2000.  Hot heads and cold tails. Nature, 407, 458-461).

Arndt was moved to make his comments by evidence from Namibian flood basalts from the 128-138 Ma old Paraná-Etendeka large igneous province (Thompson, R.N. and Gibson, S.A. 2000.  Transient high temperatures in mantle plume heads inferred from magnesian olivines in Phanerozoic picrites. Nature, 407, 502-506).  Thompson and Gibson found highly magnesian olivine crystals, among more normal ones, in basaltic dykes that cut the Etendeka basalts.  The more Mg-rich an olivine is the more primitive (the more like the composition of the mantle) the magma from which it crystallized.  They calculate that these anomalous olivines equilibrated with a magma with 24% MgO (compared with the <10% of most basalts) – probably a komatiite.  But they are in much more evolved basalts, so they suggest that a primitive magma at the hot head of a plume that hit the lithosphere itself underwent fractional crystallization to produce plain basalt.  They draw from that the conclusion that the plume head was 300-400°C hotter than the surrounding mantle – as expected in the first plume model above.  Arndt is sceptical, partly because there are so many unknowns about the source region and partly because there are many other possible explanations.  He suggests more similar work and other kinds of geochemical research on large igneous provinces in general.  To that might be added looking for some of the possible mechanical consequences of hot or cool plume heads.

Cashing in on T. rex

In the United States’ legal system I believe there is a statute of limitations.  It doesn’t apply to the Cretaceous Period.  More precisely, the most complete and fierce-looking specimen of a Tyrannosaurus rex skeleton has been the subject of legal wrangles from the moment she – a female named Sue after Sue Hendrickson of the Black Hills Institute of Geological Research (BHIGR), South Dakota who found her – was excavated.  The legal saga is the subject of a new book by a lawyer, Steve Fiffer (Tyrannosaurus Sue, Freeman, New York, ISBN 0-7167-4017-6).  The trouble started when the owner of the land on which Sue was discovered in 1990 was paid a paltry US$5000 for the privilege of seeing the awful fossil removed.  The rancher’s subsequent claim on her was matched by another from the Cheyenne River Sioux, because the owner had placed his land in trust with the US Department of the Interior, and that conveys certain advantages to Native Americans….  The plot indeed thickened.  The FBI and the local sheriff pounced on the hapless saurischian in 1992, and the National Guard supervised her impoundment, pending due process of law.  Five years of hearings and criminal proceedings later –  a raft of 148 felonies and 6 misdemeanours fell on the owners of BHIGR and one was jailed for 18 months – Sue became probably the oddest lot at Sotheby’s auction rooms.  To add further insult, the auction price of US$8.36 million was partly raised by Disney and McDonald’s, and the landowner made US$7.6 million after commission.  Sue now entertains in Chicago’s Field Museum of Natural History.

Source: Pojeta, J., 2000.  Fossils, G-men, money and museums.  Science, v. 289 8 September 2000, p. 1695-1696.

Molecular ‘fossils’ and the emergence of photosynthesis

The most familiar photosynthesis is that associated with green plants, members of the Eucarya, in which organelles known as chloroplasts play a crucial role.  Lyn Margulis’ theory of endosymbiotic incorporation of various bacteria in the origin of the eukaryote cell, sees cyanobacteria as the most likely progenitors of chloroplasts in plants.  Aspects of the genetic material in chloroplasts are sufficiently similar to that of blue-green bacteria to make this a robust view.  Tracking down when that melding of bacterial ancestors took place is a difficult task, both for molecular biologists and palaeontologists, partly because the record of cell material similar to that of cyanobacteria goes cold about 2.5 billion years ago.

Stromatolites, which today grow through the action of cyanobacteria excluding calcium from their cells in hypersaline environments, go back into the Archaean 3.46 billion years ago, but there is no guarantee that stromatolite forms were always confined to oxygenic photosynthesisers.  However, the manner in which photosynthesis by blue-greens fractionates carbon isotopes possibly gives a signal in the d13C record of ancient hydrocarbons.  Sadly, the overlaps between carbon-isotope fractionation oxygenic photosynthesisers, chemoautotrophs and anoxygenic photoautotrophs are too broad for this kind of study to give a definitive answer.  Nonetheless, some researchers have claimed an Archaean origin for the cyanobacteria using this approach.

The advance of molecular biology, which compares gene sequences among living organisms to seek degrees of relatedness (phylogenies), steadily moves towards widely accepted molecular “clocks” that might resolve the timing of emergent life processes.  A joint US-Japan team of molecular biologists have compared the photosynthetic genes of two modern photoautotrophs – green sulphur and green nonsulphur bacteria, neither of which are oxygen producing – with those of other photosynthetic bacteria (Xiong, J. et al., 2000.  Molecular evidence for the early evolution of photosynthesis.  Science, v.  289 8 September 2000, p. 1724-1730).  Their results firmly place oxygenic photosynthesis, as in cyanobacteria, as descendent from earlier anoxygenic photoautotrophy, purple bacteria likely being the first to emerge by developing pigments capable of using solar energy to fuel proton pumping across cell walls.  Jin Xiong and co. do not derive any timing for this phylogeny, but palaeobiologists are suggesting from their evidence that the six major photosynthetic bacterial lineages were around in the mid-Archaean (2.8 to 3.0 billion years ago) and maybe earlier.  This comes nowhere close to the greater antiquity of stromatolites, but tagging purple bacteria as the first photosynthetic organisms, albeit not producing oxygen, gives a helping hand.  Organic molecules originating in them are sufficiently distinct to already have shown up in kerogen from ancient shales, and such precursors to petroleum are present in Archaean sediments.

The interest in the emergence of photosynthesis is understandable, because of the huge increase in opportunities that it presented, by comparison with chemoautotrophic metabolism that seems likely to have been the first life strategy.  The latter depends on chemical tricks with reduced materials, such as S, Fe2+ and methane delivered by sea-floor hydrothermal vents.  Assuming appropriate rates for Archaean magmatism, that could sustain about 1012 moles of carbon fixing in cells per year.  The anoxygenic photosynthetic pathway would have multiplied that by ten times.  However, it is oxygenic photosynthesis that exploded life’s potential for interaction with the inorganic world, and that stemmed from the chemical-physical process at the root of what blue-greens did.  The essence of oxygenic photosynthesis is that the pigments (like chlorophyll in plants) involved in transforming photon energies into electron flows, which are essential in the reduction of CO2 and water to carbohydrates, actually break the very strong bond between hydrogen and oxygen in water; that is why it releases free oxygen as a by-product.  That feat involves a combination of the processes used by green sulphur and purple bacteria, which in itself implies the later emergence of cyanobacteria as confirmed by Xiong et al’s work.  By using water molecules in this way, however, oxygenic photosynthesis opened up the whole near-surface of the hydrosphere, increasing potential bioproductivity by a further two or three orders of magnitude at least.  It can be said that such a development truly brought life onto the front stage from hiding in obscure nooks and crannies.  But we still have little precise idea of when that happened.

See also:  Des Marais, D., 2000.  When did photosynthesis emerge on Earth? Science, v.  289 8 September 2000, p. 1703-1705.

Rhenium fever drives miners into the volcano

Satellites demand durable components, and for some applications the metal rhenium is irreplaceable.  But it is hard to smelt, as well as being rare.  Its current price of US$1.45 per gram reflects its conventional extraction from gases emitted by roasting molybdenum ore, a by-product of copper mining.  At around one sixth the value of gold and with work beginning in earnest on the US-Russian International Space Station, a sizeable chunk of rhenium promises a quick profit.  For geologists in the economic black hole that was the Soviet Union, rhenium has become a magnet and they are developing possibly the most extraordinary mining venture ever attempted.

Volcanologists of the Russian Institute of Experimental Mineralogy discovered, in 1992, that fumaroles of the volcano Kudriavy in the Kuril Archepelago exhale and precipitate pure rhenium sulphide – the hitherto unknown mineral rheniite.  The vents’ build-ups contain at least ten tonnes of rhenium, and fumarole gases replenish it at a rate of several grammes each day.  As well as mining the vents, even condensing rheniite is an economically attractive proposition.  Even now, scientists of the Moscow-based Institute of Mineralogy, Geochemistry and Crustal Chemistry are building a wooden pyramid to cap one of the vents.  This will funnel fumarole gases into a chemical trap for rhenium, that uses zeolites as an ion extractor.  Future plans, sensibly, focus on concrete or ceramic caps to tap all the fumaroles in Kudriavy’s crater. 

Source:  Jones, N., 2000.  Outrageous fortune.  New Scientist, 26 August 2000, p 24-26

Unravelling Neoproterozoic environments

The latest Precambrian or Neoproterozoic, from1000 to 544 Ma ago, and especially from 700 Ma to the start of the Cambrian, is the most important episode in the history of biological evolution.  That is the episode during which remains of large, soft-bodied animals (the Ediacaran fauna) first appear and at whose end animals able to secrete hard parts burst onto the scene.  It marks the preparation for the beginning of life as we know it best; the Cambrian Explosion.  This period is remarkable also by its huge climatic upheavals that twice turned Earth into a planetary snowball, when ice masses extended to tropical latitudes.  As if these unprecedented and never repeated big freezes were not sufficient to focus geologists’ undivided attention on the late-Neoproterozoic, seawater became for a time so depleted in oxygen that soluble ferrous iron entered shelf areas to precipitate out as banded iron formations, which had vanished around 2.2 Ga when oxygen first entered the oceans in any amounts.  Neoproterozoic world events opened with all continental lithosphere known to be around at the time consolidated in the mother of all continents, literally called Rodinia from the Russian for motherland.  Rodinia broke up with the as yet unexplained break out of Laurentia from close to its heart.  A massive round of sea-floor spreading saw tiles from the Rodinian mosaic reassembled as the core of the Gondwana supercontinent beginning around 650 Ma ago.  Gondwana played a massive role in subsequent tectonics until it too broke up in the Mesozoic.  These were interesting times, relative to which the Phanerozoic seems somewhat tame, except for its tangible record of life’s ups and downs.

But there is a problem; with magmatic activity sparsely distributed in Neoproterozoic space and time, and a lack of rapidly changing biomarkers, division of events through time and, more important, correlating events from place to place has proved difficult, except in a barely useful and often mistaken way.  Geological accounts of the late-Precambrian have been permissive and provocative, to say the least.  That seems likely to change rapidly.  Frustration centred on the time problem set against the undoubted drama of events had spurred the development other means of stratigraphic division and correlation.

The geologically instantaneous mixing of isotopes affected by global processes forms the basis for identifying large events that fractionate them in stratigraphic sections everywhere.  That has been the biggest contribution of the oxygen-isotope data in seafloor sediment cores for the Neogene, in which fluctuating volumes of land ice shifted the proportion of 16O to 18O in ocean water, so that features in d18O records become means of fine-tuned correlation world-wide for climate shifts.  Carbon isotopes play a similar role in charting changes in global bio-productivity and burial of dead matter and carbonate hard parts.  Strontium serves to detect changing balances between supply of dissolved material from oceanic magmatism and from erosion of 87Sr-enriched continental crust.  Sulphur isotopes also help chart supply and demand among organic and inorganic processes.  Such chemo-stratigraphic methods were recognised as a lifeline for resolving Precambrian evolution in the late 1980s.  A decade on, painstaking work  has begun to bear fruit, as covered by a Special Issue of the 100th volume of Precambrian Research (v. 100(1), 2000).  Andrew Knoll of the Botanical Museum, Harvard, USA summarises progress (Knoll, A.H., 2000.  Learning to tell Neoproterozoic time.  Precambrian Research, v. 100, p. 3-20), but details of the chemo-stratigraphic approach and what the prominent isotopic markers might mean appear in a paper of monographic proportions from a team at the Department of Earth and Planetary Sciences, Macquarie University, Australia (Walter, M.R. et al., 2000.  Dating the 840-544 Ma Neoproterozoic interval by isotopes of strontium, carbon and sulphur in seawater, and some interpretative models.  Precambrian Research, v. 100, p. 371-433)

Chemostratigraphy seems to resolve the question of how many late-Precambrian icehouse conditions of global significance.  Though some have speculated on as many as 5 or 6 from occurrences of glacigenic rocks, only two match with isotopic signals, one (Sturtian) around 700 Ma and one around 600 Ma (Marinoan).  Both have associated negative d13C excursions in carbonates to the level of mantle carbon, which suggest that life was reduced to a minimum by ‘Snowball Earth’ conditions.  Associated shifts in the proportion of isotopically heavy sulphur are different.  Sturtian glaciation matches with an increase in d34S, a likely product of ocean anoxia, the involvement of light 32S in bacterial reduction of sulphate to sulphide ions, and the burial of iron sulphide at sources of ferrous iron around sea-floor hydrothermal systems.  The anoxia was sufficiently extreme for Fe2+ to dissolve and mix throughout the ocean water column, so that precipitation as ferric oxy-hydroxides burgeoned in shelf seas to form BIFs a little younger than the glacigenic rocks.  Marinoan glaciation, though equally catastrophic for bioproductivity,  did not fully deplete the oceans of oxygen.  Massive peaks of d13C prior to glaciations suggest that intense precipitation of carbonates in the limestones so common in the run-up to frigidity, plus burial of abundant dead organic matter in the case of the Marinoan, dramatically drew down CO2 from the atmosphere.  Life’s recovery after the Sturtian, together with organic burial, boosted oxygen levels, as too following the 600 Ma Marinoan.  Possibly the delivery of huge amounts of glacially ground rock flour added nutrients that helped fuel this biological pump, and an increase in 87Sr/86Sr after the Marinoan could reflect such fertilization.  There is much more in the paper that will fuel advances in ideas of the co-linkage of glaciation and biological evolution – essentially adaptive radiation by the few eukaryotes that survived anoxia and other stresses – and the evidence for large increases in oxygen production that are prerequisites for the origin of large, oxygen-demanding animals in the Ediacaran fauna.  What came as complete surprise to me, a non-specialist, was clear evidence from several well-studied sections for the largest negative d13C excursion in geological history only 2 Ma before the Cambrian Explosion, which took less than a million years to develop..  Other isotopic trends seem to indicate a brief but highly intense global warming that snuffed the Ediacaran animals from the fossil record.  The unique depletion in heavy carbon points strongly to the seabed belching teratonnes of methane in unstable gas hydrate, a product of double selection of 12C by photosynthesizing plankton and methanogen bacteria metabolizing dead planktonic matter within ocean-floor sediments.

Isotopically, the late-Neoproterozoic was chaotic.  Carbon in particular records ups and downs with amplitudes and frequencies that dwarf those of the far-better recorded Phanerozoic, even in later glacial epochs and mass extinctions.  It was two evolutionary developments that probably damped down excursions in carbon isotopes in later times: the stirring of deep-ocean muds by burrowing animals to promote more rapid oxidation of buried organic matter; the increased efficiency of CO2 drawdown by organisms that secreted carbonate hard parts.  Perhaps Precambrian events were not so dramatic after all, equally disturbing events being smudged in the Phanerozoic by the rapid adaptive radiation following the Cambrian Explosion.

My prediction is that this issue of Precambrian Research will become the starting post for a major shift of research into Neoproterozoic and earlier Precambrian sedimentary piles, after two decades of getting things straight in the Mesozoic and Cainozoic.  I feel confident in that, because the stories of Snowball Earth and near extinction of all oxygen demanding life around 700, 600 and now 545 Ma are ones that will, as the Sun might say, run and run.

Plankton and the end of the Palaeocene-Eocene global warming

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.

A new regular pulse in recent climate

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.

End-Permian devastation of land plants

The mass extinction that marks the boundary between the Palaeozoic and Mesozoic Eras snuffed out more than 90% of marine animal species and about 70% of terrestrial vertebrates.  The most complete record of the Permian-Triassic boundary is in marine sediments atop an obducted ophiolite in Japan (Isozaki, Y., 1997.  Permo-Triassic boundary superanoxia and stratified superocean: records from lost deep sea.  Science, v. 276, p. 235-238).  These record a 20 million-year period when deep ocean water was lacking in oxygen, and the anoxia reached extreme conditions for about 4 million years across the boundary.  All the palaeontological signs are that shallow marine faunas dwindled slowly in the 10 million years before the P-T event.  Carbon isotopes from hydrocarbon-rich boundary strata in Canada suggest that over a period of  only 1000 years the oceans were almost devoid of life.  The open oceans had become dead from top to bottom; a scenario graphically expressed by Ken Hsu as a “Strangelove” ocean.  Whatever the pace of preceding extinctions the boundary event was a catastrophe, and the Japanese and Canadian sections suggest that maybe a half-million years passed before surviving organisms began to recover and diverge.

The much-studied K-T boundary’s association with abundant evidence for an associated giant impact, prompted geologists to look for a similar story for the near end of Earth’s life 190 million years earlier.  Supporting evidence has yet to emerge, although the boundary includes the period when huge volumes of continental flood basalts poured over what is now Siberia.

Terrestrial records are far less easy to divide into fine time divisions, partly because they record both deposition and erosion, and partly because fossils are less well-preserved than in marine sediments.  Continental sediments spanning the P-T boundary are particularly frustrating, because of the wide extent of arid to semi-arid conditions then.  The Karoo Basin of South Africa does record wonderfully the fate of vertebrates (only 6 out of 44 genera survived the  boundary event), but less so that of plants.  Abrupt changes in plant-life are equally as important as those of animals, simply because they are at the base of the terrestrial food chain.  One way of addressing vegetation shifts of the most general kind is to look for evidence of how river systems changed their patterns of deposition, and this is what a team from the University of Washington (Seattle) and the South African Museum have done in the Karoo Basin (Ward et al., 2000.  Altered river morphology in South Africa related to the Permian-Triassic extinction.  Science, v. 289 8 September 2000, p. 1740-1743).

Peter Ward, David Montgomery and Roger Smith examined sedimentary structures produced by river channels in the sandstone members of the Karoo sedimentary pile.  Permian rivers seem to have flowed in distinct, meandering channels, whereas those of Triassic age laid down sands that show consistent evidence for intricately braided  channel systems.  The shift from one to the other type falls right at the P-T boundary.  Meanders of large river channels typify land surfaces with abundant vegetation that binds alluvium.  Where vegetation cover is sparse, there is little to constrain river flow and alluvial erosion, and wide braided river courses develop.  The authors conclusion is that vegetation suffered a catastrophic die off at the P-T boundary, leaving formerly lush plains as sandy wastes.  Such a loss of plants that would previously have contributed to balancing the atmosphere’s CO2 levels and the proportions of light and heavy carbon isotopes in the global environment would have helped produce the “Strangelove” signal in the ocean sediments.  The land was seared, and evidence from similar sediments in Australia and Antarctica suggests a global loss of plant life.  Incidentally, the boundary in many places shows a leap in the abundance of fungal spores, so the Mesozoic began with decay on a grand scale.

See also: Kerr, R.A., 2000.  Biggest extinction his land and sea.  Science, v. 289 8 September 2000, p. 1666-1667.

Carbon isotopes of individual microfossils

Organisms at the base of the food chain, autotrophs that synthesise biological compounds directly from carbon dioxide, water and other fundamental materials in their environment, favour incorporating the lighter of the two common isotopes of carbon, 12C, as opposed to 13C.  Consequently, one of the prime signatures of life in the carbon found in rock is a depletion in 13C, usually expressed as d13C with a negative value.  It is this signature that has allowed the origin of life to be pushed back almost to the age of the oldest rocks on Earth (around 3.9 billion years ago) from carbon isotope studies of carbonaceous compounds (kerogen) in ancient sediments.

Different organisms alive today, particularly among the ecologically diverse bacteria, use different biochemical reactions in synthesising living material.  Each of these have different effects on d13C.  Potentially these differences could be used to identify roughly the kinds of bacteria that lived in the distant past.  Up to now, however, isotopic studies of organic carbon have only been possible for bulk extracts from rock.  That enables some bold conclusions, such as the current suggestion that oxygen-producing blue-green bacteria were around 3.5 billion years ago, but whole-rock results are ambiguous because of mixing of carbon originating from different metabolic pathways. 

Being able to analyse carbon isotopes from individual fossil cells is a major breakthrough, and a team of palaeobiologists from the universities of California and Regensburg, Germany has done just that (House, C.H. et al., 2000.  Carbon isotope composition of individual Precambrian microfossils.  Geology, v. 28, p. 707-710).  They used an ion microprobe that allowed the discovery of biological carbon encapsulated in resistant materials from 3.8 billion-year old metamorphosed iron formations from West Greenland.  That involved probably mixed carbon of biological origin.  In the new work, the isotopic analyses are from individual bacterial cells preserved in 850 and 2100 Ma banded iron formations, and suspected to be blue-green bacteria.  The results clearly distinguish one metabolic pathway – the Calvin cycle used by blue-greens – from other possibilities.

Tangible bacterial fossils go back, albeit rarely, to more than 3 billion years ago.  It is the older life forms that are most intriguing, because by 2100 Ma ago the Earth’s atmosphere had become oxygen bearing, thereby allowing the rise of the Eucarya from which we stem.  Older material might give clues to the more primitive Bacteria and Archaea that were the exclusive rulers of the biosphere before about 2200 Ma, and controllers of the Earth’s atmospheric composition and thereby its climate, which remains a mystery.

Timing the uplift of the Tibetan Plateau

The rise of the huge Tibetan Plateau, with an average elevation of 5 km, presented a major barrier to atmospheric circulation, perhaps one of the largest that has ever existed.  With its latitude close to the down flow of the tropical Hadley cells, it has had an effect on the Asian monsoon in particular, strengthening its effects.  Many climatologists believe that Tibet has played a major role in global climatic change towards the end of the Cainozoic.  So, timing the uplift is critical in assessing the modelled effects in relation to detailed climate records of the Neogene.  This is by no means easy, for the late-Tertiary sediments are terrestrial in origin.

A team of Australian and Chinese geologists focussed on the sedimentary record in the Tarim Basin, north of the Kunlun mountains that form the northern flank of the Tibetan Plateau (Zheng, H.  et al., 2000.  Pliocene uplift of the northern Tibetan Plateau.  Geology, v. 28, p. 715-718).  Sediments there change from redbeds deposited in gently sloping flood plains to coarse debris laid down by flash floods at a rising mountain front; exactly the relationship that records the beginning of uplift in northern Tibet.  Dating this is no easy matter, however.  The technique that the team used is magnetostratigraphy, based on highly sensitive measurements of the polarity of 2500 samples of weakly magnetized sediments.

The change in facies spans a period when the Earth’s magnetic field was reversed – the Gilbert reversed chron – which occurred between 4.5 to 3.5 Ma ago.  The maximum age for the beginning of Tibetan uplift in the north is therefore 4.5 Ma, in the Pliocene.  This contrasts with the accepted age of Oligocene – Miocene for uplift of the Himalaya and southern Tibet, and with models that postulate climatic change that followed it.  Whereas the Tarim Basin today is arid, the sediments indicate that until the Pliocene abundant water flowed at the surface, to deposit great thicknesses of fine alluvium.

Danger of CO2 release in Cameroon

On 21 August 1986 a huge cloud of carbon dioxide gas was released from Lake Nyos located at 300 metres in the Highlands of Yaounde District of Cameroon. Because carbon dioxide is more dense than air it hugged the ground and flowed down valleys. The cloud travelled as far as 15 miles (25 km) from the lake. It was moving fast enough (as much as 80 kph) to flatten vegetation. 1,700 local people died by suffocation, probably unaware of their plight.   Two years earlier 37 people died similarly in a gas release from nearby Lake Monoun

Lake Nyos is in the Oku volcanic field, and is one of several maars produced by one-off explosive events in the recent past.  Isotopic analyses of gas remaining dissolved in the lake show that the CO2 is of volcanic origin.  The lakes are fed by springs on their beds, which is where the CO2 enters.  Being extremely deep (about 200 metres) and with no surface inlet the lake water is strongly stratified, so that CO2-rich water builds up at the bottom.  The gas release must have involved an overturn of the stratification, so that dissolved gas came out of solution as pressure decreased.  What triggered the overturn is hard to establish, but one possibility is that during August (both catastrophes occurred in that month) cold weather cools surface waters so that they sink.  Other possibilities are storms, landslides or earthquakes, but there are no records of any of these preceding either event; they came completely unannounced.

Since 1986, gas levels have built up, and now stand at twice their concentration following the disaster, so danger threatens the local people and their livestock once again.  An international team, headed by George Kling a geologist at Michigan University, USA, has devised a means of venting the gas harmlessly.  This involves sinking 15 centimetre diameter polyethylene pipes to the lake bed.  Once pumping starts, gas bubbles forming as pressure releases will drag the water upwards, as a self-sustaining siphon, similar to the air-lift dredges used in marine archaeology.  Four such pipes would rid the lake of its lethal gas content in two years, and even one would reduce the hazard considerably.

Sources:  Observer, 20 August 2000, University of Michigan (http://www,biology.lsa.umich.edu/~gwk/research/nyos.html)

Inglorious mudstones

Because they succumb to erosion easily, mudrocks do not outcrop well, except on the coast or in arid lands.  Often they show little if any stratification that field workers can distinguish from the partings imparted by compaction and dewatering, which make shales from them.  Yet they are repositories of a great deal of information (see Earth Pages archives – Methane hydrate – more evidence for the ‘greenhouse’ time bomb).  In hand specimen their two main components, silt-sized quartz grains (<62 microns) and clay minerals (>4 microns) only become distinguishable by chewing!  They are irresolvable using optical microscopes, and detailed work needs scanning electron microscopy.

Silt to clay proportions in mudrocks are variable. The first is generally taken as an indicator of suspended debris from land masses and its proximity to where the mud accumulated.  The more clay, the further muds were from exposed continents, or so sedimentologists used to assume.   That approach has taken a hard knock from some recent detailed work on Devonian mudrocks (Schieber, J. et al., 2000.  Diagenetic origin of quartz silt in mudstones and implications for silica cycling.  Nature, v.  406 31 August 2000, p 981-985).

Jurgen Schrieber of the University of Texas (Arlington), Dave Krinsley of the University of Oregon and Lee Riciputi of the Oak Ridge National Laboratory in Tennessee used scanning electron microscopy, cathodoluminescence and ion-probe techniques to discriminate between detrital quartz grains and those formed by precipitation of silica from pore water in the original muds.  Those grains that do not luminesce probably formed by silica solution and reprecipitation, and the Devonian mudrocks contain mainly non-luminescent quartz grains.  Oxygen isotope ratios from individual grains confirm this in situ origin.  The researchers had no reason to suspect that their Devonian samples would give such results, and assumptions based on silt to clay ratios from any mudrock are now in doubt.

Worse still, silt in ocean-floor muds, cores of which form the linchpin for Pleistocene climate studies, has been a rough and ready way of estimating wind speeds as climate shifted from glacial to interglacial conditions.  These silts could be precipitates too, and the variations in their proportions may stem from changes in the delivery of dissolved silica from land to the oceans.

See also:  Kemp, A.  2000.   Probing the memory of mud.  Nature, v. 406 31 August 2000, p 951-953

Atmosphere linked to Earth’s rotation

One of the annoying features of the Earth as a planet is that it engages in a kind of Saint Vitus’ dance.  The best known of its wandering are those involving variations in the eccentricity of its orbit, and the tilt and precession of its axis of rotation.  These follow from the gravitational influences of massive planets elsewhere in the Solar System, and are implicated in the modulation of climatic change through the last 2.5 Ma.  Rather less well-known, and even more aggravating are far more rapid, but geometrically quite small deviations from good behaviour.  One of these is the habit of the spin axis to wander around the geographic poles within a circle roughly 3 to 6 metres across.  It does this every 14 months.  It takes a certain degree of dedication to chart such a tiny planetary tic.  Chandler Wobble is the single claim to fame of its eponymous discoverer.  Seth Carlo Chandler Jr, an American businessman and amateur astronomer, discovered the quirk in 1891 by observing stars with a degree of single-mindedness that might have put a lesser mortal on the couch.  He set out to verify the famous Swiss mathematician Leonhard Euler’s prediction that the Earth ought to wobble every year, and he did.

So minuscule is Chandler Wobble, that keeping it going is something of a vexing problem, for a single jostle’s effect ought to fade away in a few years.  There are innumerable ways of nudging the Earth, and deciding which is sufficiently regular and just right to maintain the wobble is no easy task.  Following in the great tradition of Seth Chandler, Richard Gross of the Jet Propulsion Laboratory compared Wobbling between 1985 and 1996 with the continual but inconstant motions of atmosphere and oceans, as simulated by super-computer modelling of climate.  The forces of winds and currents are simply insufficient to induce the Wobble, but variations in atmospheric and deep-water pressure, together with their positional shifts are, in the manner of Goldilocks and the little bear’s porridge, just about right.  Because changes in water depth are wind-driven (as for instance with the wandering hump in the Pacific’s surface, linked with El Niño), ‘weather’ is the ultimate driving force for Chandler Wobble.

Why devote time to this picayune curiosity?  The answer is to chart more accurately the position of distant spacecraft; not easy when the measuring platform is behaving like a Womble.

Source:  Richard A. Kerr, 2000.  Atmosphere drives earth’s tipsiness.  Science, v. 289, p. 710.

The guts of a sea-floor spreading system

What goes on beneath constructive plate margins, and ocean ridges has, up to now, been largely a matter of conjecture, blended with the geology of ophiolite complexes obducted onto continents.  Ophiolites are perhaps not such a good model, since the low buoyancy of the basalt capped lithosphere that they represent prevented them from subduction, and stems from unusual conditions.  The bulk of oceanic lithosphere is destined for resorption into the mantle, and it forms at common or garden ridge systems.

One way of modelling magmatism at ridges is through geochemical analysis of mid-ocean ridge basalts matched with topographic and structural detail of the ridge itself, but this is a blurred approach.  It shows that part of the process must involve ponding of magma in chambers at shallow levels beneath the ridges.  The other aspect is the form taken by the mantle that must rise to undergo adiabatic partial melting.  For fast-spreading ridges, such as the East Pacific Rise, there are two such models: constraint of rising mantle in two-dimensional sheets descending from beneath the ridge itself; three-dimensional plumes of mantle from which magma migrates laterally to ridge segments.  Amplifying geochemical-structural models needs a better idea of the actual processes and the geometries that they take.  A means of getting this information is to use a technique well-honed by petroleum exploration; 3-D seismic reflection profiling.

A consortium of geophysicists from the universities of California and Cambridge used this costly method, involving 200 profiles, to look at 400 km2 of the East Pacific Rise at 9°N (Kent, G.M. and 10 others, 2000.  Evidence from three-dimensional seismic reflectivity images for enhanced melt supply beneath mid-ocean-ridge discontinuities.  Nature, v. 406, p. 614-618).  Melts have about half the seismic velocity of solid rock, and so boundaries between melt and solid show up with better contrast on seismic records than do boundaries in piles of sedimentary rocks.  The surprising result is that instead of vertically extensive magma chambers, expected from either hypothesis, melt occurs in a narrow, continuous sill-like body beneath the ridge.  This connects to a plunging tongue that is probably the path taken by magma from the zone of partial melting in the mantle.  The sill itself occurs at a fixed depth below that predicted from ophiolite studies for the level at which vertical sheeted dykes form the lower part of the petrologically defined crust.  This suggests that the magma simply cannot rise en masse to inject along extensional fissures as the lower crust fails, the sheeted dyke layer acting like a seal in the flow of petroleum in sedimentary basins.  Instead, it seems more likely that magma ekes out as rising rivulets that follow the base of the dyke layer until the reach dilatations at the ridge.

Although results from this study are inconclusive as regards the two models for rising mantle, the detail that it reveals augurs well for further 3-D surveys of ocean magmatism that will complement seismic tomography of the deep mantle.

Flood basalt events and mass extinctions

Searching for sudden events that might explain the disappearance of sizeable proportions of fossil taxa is a growing cottage industry among geologists.  Until 1980, with Alvarez’ discovery of geochemical evidence for a comet or asteroid impact at the Cretaceous-Tertiary boundary, such tumbles in life’s diversity and volume were merely palaeontological markers which geologists chose to divide the stratigraphic column of the Phanerozoic into Periods and Stages.  Mass extinctions now take on a much greater importance through the hunt to explain them.  The popular vision of herds of dinosaurs writhing in the inferno following the Chixculub bolide strike at the K-T boundary dwarfs to a large degree the equally certain knowledge that at the same time vast basalt floods in what is now north-western India may have had an equally doleful outcome.

Super-large volcanic events, akin to the Deccan Traps, are a great deal simpler to spot than the subtle signs of impacts in the rock record.  Improved precision in dating such basalt piles shows that three of the “Big Five” mass extinctions occurred within the 1 to 2 million-year life spans of flood-basalt paroxysms: the Deccan Traps at the K-T; The Parana Basalts at the Triassic-Jurassic; and the Siberian Traps at the Permian-Triassic boundaries.  A similar correlation exists for the lesser Palaeocene-Eocene boundary event at 55 Ma, which implicates the North Atlantic large igneous province responsible for flood basalts in north-west Scotland and Greenland.

The scales have tilted further towards a terrestrial cause for mass death with the recent discovery that the Karoo and Ferrar flood-basalt provinces of South Africa and Antarctica formed at a time (183.6+ 1 Ma) that brackets a lesser extinction event in the early Jurassic Period.  Jósef Pálfy of the Hungarian Natural History Museum and Paul Smith of the University of British Columbia (Pálfy, J.  and Smith, P.L., 2000. Synchrony between Early Jurassic extinction, oceanic anoxic event, and the Karoo-Ferrar flood basalt volcanism. Geology; v. 28, p. 747–750) use U-Pb dating of thin volcanic ash layers in the Jurassic sedimentary pile of North America to calibrate the ages of individual ammonite Zones of the Pliensbachian and Toarcian Stages of the Jurassic.  At that time, about 25 % of organisms at the family level became extinct globally over a period of about 4 million years – the Pliensbachian-Toarcian event was not abrupt.  The record in the British Jurassic for extinction of marine animal species shows a marked change at around 183 Ma, within the time span of the Karoo-Ferrar eruptions.

This correlation ties in well with the Toarcian ocean-anoxia event, recorded in the British and Swedish Jurassic (see Earth Pages archives – Methane hydrate – more evidence for the ‘greenhouse’ time bomb) which seems to have coincided with a huge gush of methane into the atmosphere, released by methane hydrate layers in ocean-floor sediments.  Methane, a greenhouse gas in its own right, oxidizes to carbon dioxide.  What may have happened is that the Karoo-Ferrar volcanism injected massive amounts of CO2, leading to global warming.  This, transmitted to deep ocean water, could have triggered breakdown of methane hydrate to give a massive positive feedback to global climate.  The heat itself might have driven species and families to extinction, or changed ocean circulation to induce stagnation and anoxia.

Important as Pálfy and Smith’s findings are, they by no means resolve the complexities of interwoven terrestrial events.  The 90 million-year old Cenomanian-Turonian ocean-anoxia and extinction event had an associated methane burst, but no flood basalts.  That at the Palaeocene-Eocene boundary has no associated anoxia.  The largest basalt flood known, beneath the Pacific to form the Ontong-Java Plateau about 120 Ma ago, induced methane release and anoxia, but has no associated extinction peak

Despite well-funded attempts to link mass extinctions, other than the K-T event, to impacts, there is little tangible sign of such a connection using precise radiometric dating.  Still, the focus of high-profile stratigraphic research is on boundaries rather than what lies between them.

Putting numbers on ecological effects

In the same issue of Geology a team of American palaeoecologists (Droser, M.L.. Bottjer, D.J., Sheehan, P.M. and McGhee, G.R., 2000. Decoupling of taxonomic and ecologic severity of Phanerozoic marine mass extinctions. Geology; v. 28, p. 675–678) assess the degree to which ecologies change after mass extinctions.  They focus on the Late Ordovician and Late Devonian events (two of the “Big Five”).  Although both involved similar levels of loss of taxonomic diversity (about 22% decline in marine families), marine ecosystems underwent no significant change after the Ordovician event.  Following that towards the end of the Devonian, however, marine ecology changed drastically.  One example is reefs colonized by tabulate corals.  The early corals were devastated by both extinctions, losing about 75% of taxa.  Coral-rich reefs continued after the Ordovician, but virtually disappear from marine ecosystems after the Devonian, until much later in geological time.  The most likely explanation for this is that Palaeozoic reefs formed mainly from organisms known as stromatoporoids, which gave the 3-D structure required for tabulate corals.  Stromatoporoids lost 50% of their diversity after the Devonian event, and did not recover as reef-formers.  The main implication of this study is that the effects of extinctions do not simply depend on the quantity of taxa that are snuffed out, but on specific components of the ecosystems involved.