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Australia: The Land Where Time Began |
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Severe Selenium depletion in the Oceans of the Phanerozoic as a
Factor in 3 Global Mass Extinction Events
The key trace element that is required by all animal and most plant life
is selenium (Se) and deficiencies of Se in the food chain lead to
pathologies or death. In this study Long et
al., show that, based
on new geochemical analyses of trace elements in marine pyrite from the
Phanerozoic that sustained periods of severe Se depletion in the oceans
of the past correlate closely with 3 major mass extinction events, at
the end of the Ordovician,
Devonian and
Triassic
periods. Periods of Se depletion >1.5-2 orders of magnitude lower than
abundance in the oceans of the present, being within the range where it
could cause severe pathological damage in extant organisms that are
Se-reliant. Long et
al., suggest that
selenium may have been one of several factors in these complex
extinction events. It is considered likely that recovery from the
depletion/extinction events is part of a natural marine cycle, though
rapid rises of global oxygen that result from sudden major increases in
marine productivity and biomass of plants following each extinction
event may also have played a crucial role.
The formation and sustainability of life many trace elements (TEs)
require many essential trace elements (Mertz, 1957; Klasing, 1998;
Eisler, 2000). In this study Long et
al. used as a new
dataset of TE abundances in oceans of the past (Large
et al., 2014; Large
et al., 2015a) in
order to discuss whether 3 of the 5 mass extinction events that occurred
in the Phanerozoic could have been influenced by extreme low abundances
of selenium, a trace element.
Such TE have been measured by the use of new laser ablation-inductively
coupled plasma mass spectrometry (LA-ICPMS) techniques with accuracy
down to single ppb in pyrite from marine black shales. Essential TEs in
the ocean fell below critical thresholds during 3 mass extinction events
at the end of the Ordovician, Devonian and Triassic, as has been
revealed by this dataset of
TE throughout the past 3 Gyr (billion years), initially based on some
pyrite analyses from 1885 (Large et
al., 2014), and now
updated to include more than 2,200 analyses for the Late
Neoproterozoic-Phanerozoic (Large et
al., 2015a). The
mechanisms for these extinction events are debated, though global
climate change that was associated with widespread anoxia and changes of
eustatic sea level (Ordovician, Devonian) as well as the Central
Atlantic Magmatic Province (CAMP) eruptions (Triassic) were involved. In
this paper Long et al.
present evidence that is based on known environmental and tolerance
levels of selenium in a range of extant organisms from phytoplankton to
vertebrates to propose the way in which distinct periods of Se depletion
in the oceans of the past offer a potential new causal factor in these
mass extinction events.
Selenium, weathering and oceans
Selenium is a metalloid that occurs naturally, which is unique in that
it may be toxic at high concentrations, though it is an essential
micronutrient in most organisms, including bacteria, archaea, fish and
shellfish, and has a concentration window for sustaining life in the
oceans of the world, as is discussed further below. In the crust of the
Earth the content of selenium averages 0.05 ppm, with the highest levels
being found in shales (up to 675 ppm), coals (up to 20 ppm) and volcanic
tuffs (up to 9.2 ppm), compared with igneous rocks that range from 0.01
to <2 ppm (Plant et
al., 2005). It has
also been reported that organic-bearing chalks from the Cretaceous
contain up to 70 ppm Se (Kulp & Pratt, 2004).
There are multiple oxidation states of Se -2, 0, +4, and +6.
1.
under oxic conditions Selenate (Se6+) is the predominate
inorganic species;
2.
Under suboxic conditions selenite (Se4+) is predominant, but
3.
Under anoxic to euxinic conditions selenide (Se2-)
organo-selenium complexes and elemental Se0 are most stable.
Selenite and selenate are highly soluble, though selenite is readily
absorbed onto iron oxides and organic matter, especially in environments
where the pH is low, which leads to its retention in the soil profile
under favourable conditions (Neal et
al., 1987).
Consequently, selenite is less bioavailable than selenate (Fordyce,
2007). Oxidation of Se4+ to Se6+ enhances the
mobility of Se and persistence in natural waters.
Disseminated pyrite in sedimentary and volcanic rocks where the Se
substitutes for sulphur (S) in the structure of pyrite is the principal
source of weathering of the crust. From <0.5 to 5209 ppm Selenium with
an arithmetic mean of 145 ppm is contained in sedimentary pyrite (Large
et al., 2015a). The
release of selenium as both selenate and selenite species results from
oxidative weathering of pyrite. The selenate species remains highly
soluble under neutral to alkaline conditions, where it can readily be
transported by river systems to the ocean (Cutter, 1989). Continental
weathering releases little soluble Se as selenide under reduced
conditions, and elemental Se (Seo) and organo-selenium
complexes are relatively insoluble (Kulp & Pratt, 2004). A major
increase in the soluble Se to the ocean therefore results from
significant increases in atmospheric oxygen, accompanied by active
erosion. The degree of oxidation and pH controls the ratio of selenate
to selenite of the selenium that is released, which in turn controls the
solubility of Se in surface runoff, and consequently the amount of Se
that is released to the oceans, if other factors remain constant. It is
indicated by studies of dissolved TE supply from rivers to the ocean (Kharkar
et al., 1968) that Se
has a narrow range of concentration, similar to Ag, Co, Rb and Cs, and
in contrast to Mo, Cr, Sb which exhibit extremely large variations from
river to river. It was also shown by this study that most of the stream
load of Se was dissolved, and only 10% adsorbed to the particles, and
when it made contact with the seawater it was desorbed. There are 3
species that are present in the marine environment, selenite, selenate
and a form of organic selenides (Cutter & Bruland, 1984). Decomposition
of selenite-silicate compounds provides the selenite in the hard tissue
of phytoplankton in the tropical and subtropical parts of the Pacific
Ocean (Nakaguchi et
al., 2008). Surface
waters down to about 200 m are dominated by organic selenides
(seleno-amino acids in complex peptides), below which selenite and
selenate are the major dissolved species (Cutter & Cutter, 1995). In the
upper layers of the ocean the low concentrations of dissolved oxidised
Se results from biochemical reduction of oxidised species into labile
organic particles during assimilation by marine organisms, which sink,
die and dissolve, and consequently regenerating the dissolved selenate
and selenite species at lower levels in the ocean, which is typical of a
nutrient profile. The oxidised Se species are reduced to Seo
or Se- in the deep ocean, and are incorporated into
pyrite (Mitchell et
al., 2012). A small
fraction of the selenium that is organically fixed eventually deposits
in muds on the seafloor (Herring, 1991). It was shown (Ryser
et al., 2005) that
selenium in black shale is present as products of anaerobic microbial
respiration that result from the microbial reduction of Se oxyanions,
which includes Se-substitutes for sulphur in pyrite, di-selenide carbon
compounds and dzharkenite (FeSe2: an isometric polymorph of
ferroselite). It was indicated by experimental studies (Diener
et al., 2012) that Se2-
is taken up (98%) by pyrite to produce a FeSSe compound with a pyrite
structure that is distorted slightly Ferroselite. (FeSe2)
has also been produced by reacting nanoparticles of pyrite and greigite
with selenite and selenate solutions (Charlet
et al., 2012). It was
indicated by the LA-ICPMS imaging of pyrite in black shales of various
metamorphic grades that pyrite is enriched considerably in Se compared
with the clay-rich and organic-rich matrices. The analytical data of
Long et
al. indicate that in
selenium in pyrite is enriched, 5.8 times on average, over the selenium
content in the black shale matrix (which commonly contains microscopic
pyrite grains). This compares with Mo which is enriched only 2.5 times
relative to the matrix.
Se depletion and mass extinctions
Throughout the Phanerozoic the overall trend for levels of Se that were
observed showed that selenium dropped dramatically relative to modern
levels in the oceans below critical thresholds during 3 mass extinction
events at the end of the Ordovician, Devonian and Triassic. These 3 key
biotic crises are analysed further and discussed in detail below.
End-Ordovician extinction event
Commencing about 455 Ma, the end-Ordovician extinction was a complex
event that ended with 2 pulses, 445 Ma and 443 Ma, which were preceded
by glaciations of the South Pole (Harper et
al., 2013). Long
et al. suggest it is
possible that dramatic changes in sea level coupled with cooling of the
tropical ocean played a role in the extinctions (Finnegan
et al., 2012), while
it was suggested by others that euxinia and a sudden drop in oxygen
caused the first pulse, and transgression of anoxic water onto
continental shelves drove the second pulse (Hammerlund
et al., 2012). A
massive drop in Se levels in pyrite is shown by the Se curve from a peak
at 523 Ma of 548 ppm Se (geometric mean) or 365 ppt for seawater Se by
use of the concentration factor that was outlined above, to lows of
about 2 ppm (Se in pyrite) equivalent to about 1 ppt (seawater Se) by
455 Ma, which equates to approximately <1% of the current levels in the
oceans of the present, well within the Se deficient zone based on known
tolerance levels for many extant marine organisms as discussed above.
Levels of Se then rise steeply into the Silurian.
Following 2 prolonged pulses of Se depletion the 2 end-Ordovician
extinction events occurred. It has been documented that the first of the
major extinctions occurred in the latter half of the second phase of Se
depletion (~457-449 Ma), with select families of brachiopods (Foliomeria
and Probosciambon faunas, early virgianid faunas which declined from
about 450-448 Ma (Sutcliffe et al.,
2001). In the oceans extreme Se deficiency fluctuated for about 13 Myr
before the first major pulse of extinction took effect, and the second,
most severe pulse at the end of the Hirnantian only 2 Myr later (Harper
et al., 2013). At the end of
Se phase the extended phase of severe marine Se depletion would have
made it difficult for complex organisms that had selenoproteomes to
survive, and could therefore affected much of the food chain, and the
first species to go extinct would have been specie that were more
dependent on selenium. Throughout the Ordovician, and peaking earlier
than the Katian (Servais et al.,
2010), the great Ordovician biodiversification event took place
throughout the Ordovician and was apparently not affected by the Se
depletion events at the close of the period.
Middle-Late extinction events
There were 2 pairs of pulses of extinction events that comprised the
Middle-Late Devonian extinctions. Beginning with:
1)
Taghanic and Frasne Crises (House, 2002; McGhee et
al., 2013; McGhee, 2014),
which were followed by 2 events near the Frasnian-Famennian boundary
(Kellwasser event; Gereke and Schindler, 2012) and
2)
at the end of the Devonian (Hangenberg event; Sallan & Coates, 2010).
3)
The Mid-Givetian Taghanic event (~385 Ma), is ranked as the 7th
most severe biotic crisis in the Phanerozoic, in which 71 families of
marine invertebrates went extinct (McGhee et
al., 2013).
4)
The Frasnian-Famennian Kellwasser event dated to 373-374 Ma, involved
widespread loss of marine species (13-40% loss at family level, 50-60%
of all genera, 72-80% loss of all marine species lost; McGhee, 2014).
The Hangenberg events (~359 Ma) in which there were further extinctions
with about 50% of all vertebrate diversity lost (Sallan & Coates, 2010).
The Kellwasser event has been characterised by the spread of oceanic
anoxia (Riquier et al.,
2006), though it may have been restricted to epicontinental shelf seas
and not necessarily as widespread as has previously been thought to be
(George et al., 2014).
A trend is shown of sequential deficiency at staggered periods between
400 and 350 Ma, by analyses of the bioessential abundance of TE (such as
Co, Cu, Ni, Mn, Zn Mo and Cd) through the Devonian. The sequence of
deficiency is:
·
Emsian Co,
·
Givetian Mn, Cu, Ni, Zn,
·
Famennian Mo and Se,
·
Famennian-Tournasian Cd.
According to Long et al. the
sequential deficiency is most likely to be redox potential and residence
times of the respective TE. Under oxidised conditions Co and Mn are
least soluble with short residence times, whereas the most soluble with
longer residence times are Se, Mo and Cd (Large et
al., 2015a). Cu, Ni and Zn
have intermediate residence times. As global anoxia increased through
the Middle to Late Devonian, therefore, the TE was drawn down
sequentially. The peak Mo, Se and Cd deficiencies in seawater over the
Famennian to Tournasian period could have affected the marine organisms
that are not affected by the sequential deficiencies of Co, Cu, Ni or Zn
in the Emsian to Givetian. The Cd, Ni and Zn cycling in the oceans is
tied intimately to biogenic cycles (Armour et
al., 1985), and Cu is
associated with micronutrient cycles and a deep water scavenging process
(Daniellson et al., 1985). Co
and Cd can both substitute for Zn in diatoms in waters that are Zn
depleted so it has been suggested that substitutions by other trace
metals or metalloenzymes under certain TE impoverished conditions could
be a common strategy for phytoplankton survival (Price & Morel, 1990).
Based on the data of Long et al.
at certain critical times this strategy may not have been possible,
which shows overlapping periods of peak depletion for many elements.
A sudden drop at the end of the Emsian, about 393 Ma, is another
observation that arose from the Devonian Se chart. According to Long et
al. this corresponds with
another series of minor extinction events that occurred in the marine
realm, during which many vertebrate groups (most families of
osteostracans, galeaspids, heterostracans, and several placoderm
families), went extinct (Long, 1993; Janvier, 1996) and these were
followed by 2 pulses of extinction in which guilds of invertebrates went
extinct in the early and end Eifelian (lower & upper Kacak events;
McGhee et al., 2013).
Just following the Frasnian-Famennian event the longest period of Se
deficiency occurred at about 367 Ma. Fish began breathing air at this
time leading up to 370 Ma (Clack, 2007; Clement & Long, 2010) and
tetrapods, which were the first vertebrates that were equipped to leave
the water and venture out on land, also appeared (Clack, 2014). A factor
in the attempts by tetrapods to leave the water and move out onto land
was possibly related to the collapse of the food chain that resulted
from the biotic crises at this time, though it wasn’t until the Early
Carboniferous that the complete tetrapod terrestriality was effectively
achieved (Long & Gordon, 2004).
SeO32- and SeO42- were
likely to have been drawn down as they are relatively soluble under an
oxygenated atmosphere as insoluble HSe- species over the long
span of the Frasnian-Famennian anoxia. Large inputs of oxygen from the
rapid increase in terrestrial biomass over the Middle-Late Devonian
could have reversed this pattern (Algeo et
al., 2001; Gibling & Davies,
2012). The evolution of plant secondary growth led to an increase in
heights of about 2 m in the Middle Devonian to large trees up to 20 m by
the Late Famennian (Algeo et al.,
2001). Large plant cover increased by from about 10% to 30% at this time
and spread from the lowlands and eventually included upland
habitats (Gibling & Davies, 2010). The significant increase in global
biomass was helped by both these factors between the Mid-Late Devonian,
and therefore, a large source of new atmospheric oxygen. It was also
noted by Long et al. that
massive exhalation of seafloor from mid-ocean ridges and continental
margins that was occurring as part of the Variscan orogeny from 356 to
345 Ma accounts for further increase of nutrients into the oceans and
thereby bringing about an increase in marine photosynthesis and
therefore more oxygen (Tornos, 2006).
End-Triassic extinction event
At the end of the Triassic about 201 Ma extinctions include many major
losses in marine as well as terrestrial habitats and are ranked as the
second most severe biodiversity crisis in the Phanerozoic. About 20% of
families and up to 50% of genera went extinct in the marine realm,
including the iconic conodonts (Onoue et
al., 2012). Included among
terrestrial vertebrate extinctions are large archosaurs, with the
exception of the dinosaurs, which paved the way for occupation of niches
by radiation of Dinosaurs in the Jurassic.
The Central Atlantic Magmatic Province underwent massive volcanic
eruptions that caused a rapid rise in atmospheric CO2 and
methane, and led to acidification and localised anoxia that drove marine
extinctions, Based on the recognition of shocked quartz impacts of
asteroids at this time have been invoked by some authors (Bice et
al., 1992), though this has
been dismissed as having extinction events that were localised (Onoue et
al., 2012). A strong warming
effect on land that resulted from greenhouse gases has been suggested by
data from long chain n-alkanes that were preserved in fossil plants (Ruhl
et al., 2011).
It is implied by the data of Long et
al. that extremely low Se
levels in the ocean between 202 and 190 Ma that were close to the levels
at the end of the Ordovician and Late Devonian as pyrite Se levels are
about 2 orders of magnitude lower than pyrite in the modern ocean, and
therefore a similar extinction could have been operating as during these
earlier mass extinction events. At 202-190 Ma extremely low levels of Cd
are lower than at any other time in the Phanerozoic.
The end Triassic, as mentioned above, was a time of in increasing CO2
levels (Royer, 2006) and high fire regimes that were widespread (Belcher
et al., 2010). It is shown by
one model that O2 levels were rising from about 10% PAL at
205 Ma about 17% Ma PAL by 190 Ma (Falkowski et
al., 2005), whereas O2
levels are shown by another dropping from high levels at the end of the
Triassic (23% PAL; about 220 Ma) to a peak low at about 180 Ma of 14%
PAL, which was followed by a gradual rise (Berner, 2009). The rapid
decline in marine Se levels at this time is clear, and might therefore
been a more significant factor than in marine extinctions, in spite of
conflicting estimates of O2 levels at this time. It has been
proposed that gaseous exchange of Se from phytoplankton to the
atmosphere was a way in which the biogenic cycle of Se in the ocean can
influence directly terrestrial Se levels (Armouroux et
al., 2001), so could have
affected the terrestrial food chain.
Discussion
It has not yet been determined what caused the Se and other TE
depletions in the ocean, though theoretically it is explainable (Large
et al., 2014, 2015,a,b).
Increased biogenic productivity in the ocean is driven by increased
nutrients and, as a consequence, there is more burial of organic matter
which fuels increased oxygen production further as a positive feedback
loop (Large et al., 2015a).
Se levels increased in the oceans as this regime continued. Subsequently
lower amounts of TEs was transported to the oceans as lower atmospheric
oxygen or larger areas of the land was covered by higher sea levels, and
this resulted in less erosion resulting from less terrestrial oxidation.
Rapid drawdown of Se and certain other TEs was caused by this and this
led to levels falling below critical thresholds that were necessary for
sustaining most marine life. The periods of minimum marine Se may have
lasted for up to 10 Myr before rebound, based on the TE data. As a
result of lower productivity of the oceans during Se minima, there would
have been a dramatic slowdown of TE drawdown; nutrient supply that was
related to continental erosion would, however, be on-going. The result
of this was a gradual buildup of TEs to the ocean, which activated a
rebound of marine life, and a consequent positive feedback of increased
atmospheric oxygen. The upturn in recovery of oxygen and Se and recovery
from extinction conditions may have, therefore, been a part of the
ocean-atmosphere cycles.
Alternatively, jumps in global oxygen from sudden major increases in
plant biomass may have broken the Se depletion cycles. The primary
invasion of land plants in the Silurian was widespread (Gibling &
Davies, 2010). There was a massive increase in the size of land plants
in the Late Devonian from predominantly mid-sized forms to (about 2-3 m)
in the Middle Devonian, to an abundance of forms of tree size up to 20 m
by the end Devonian, and plants occupied much larger areas of the land
(Algeo et al., 2001). Major
increases in global CO2 that was associated with high
floristic turnover also characterised the end Triassic (Belcher et
al., 2010). In each of the 3
extinction scenarios it was possible, therefore, that the increase in
atmospheric oxygen that was supplied by increasing biomass could have
been the significant factor in breaking the anoxia-Se cycle and
restoring balance to the marine TE cycle.
According to Long et al. the
new data also fit well with the current explanation for the end Permian
mass extinction event that was caused by massive volcanic eruptions, in
which major marine extinctions are not related to anomalous TE levels
(Knoll et al., 2007). Prior
to the K-Pg Boundary extinctions at 66 Ma, there are also several Se
depletion events. Long et al.
found no evidence in the fossil record to suggest that these depletions
had any major effect on marine ecosystems at the time, though they noted
that the combination of low Sea levels with low oxygen (Falkowski et
al., 2005) was only attained
during the other 3 prior major extinction events that have been
discussed in this paper. At about 93 Ma the global extinction of
ichthyosaurs (Bardet, 1992) could potentially reflect the beginning of
changes to the food chain that was caused by such effects or might
simply be an artefact of poor sampling.
Conclusions
It is suggested by Long et al.
that depletion of essential TEs (Se in particular) to levels that were
potentially lethal was shown to be correlated highly, and a likely
contributing factor, at least 3 mass extinction events in the marine
realm, in association with a range of other environmental factors such
as global oxygen and carbon dioxide levels that are
increasing/decreasing, euxinia and major eustatic sea level changes in
the oceans. Oxidative erosion was increased by increased atmospheric
oxidation, which released more Se, Mo, Ni, and other TEs into the
oceans. Increased biogenic productivity, and consequently more burial of
organic matter, which further fuelled increased production of oxygen as
a possible feedback loop, was driven by increased nutrients in the
ocean. Se levels increased in the ocean as this regime continued. Rapid
drawdown of Se and certain other TEs resulted from increased global
anoxia in the oceans. Less erosion due to less terrestrial oxidation
resulted from lower atmospheric oxygen or higher sea level coverage of
land area, therefore lower amounts of TEs flowed back into the oceans,
which led to levels falling below critical thresholds that were
necessary for a high percentage of marine life. Sudden changes in oxygen
levels broke the cycle, possibly as a result of rapid recovery by
increased biomass of plants on land responding to high CO2
concentrations, or by invading more land area, as was the case at each
of the 3 mass extinction events.
The new data also fit well with the current explanation for the mass
extinction event at the end Permian, when major marine extinctions are
not seen to have been related to anomalous TE levels. Long et
al. do not have Se data
across the Cretaceous-Palaeogene boundary, so cannot make any comment in
the paper.
The hypothesis of Long et al.
is based on a 3.5 Gyr history of trace element abundance in the oceans,
though it now needs further refinement from additional data, not only
from temporal gaps in their database being filled from pyrite samples,
but also on minimal Se and other TE requirements across a wider range of
living organisms in order to develop the test models of ecosystem
collapse under times of severe TE depletion in the oceans.
Long, J. A., et al. (2016). "Severe selenium depletion in the
Phanerozoic oceans as a factor in three global mass extinction events."
Gondwana Research 36:
209-218.
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