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Coextinction
of a species is the loss of one species upon the extinction of another.
The term was originally used in the context of the extinction of.. |
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Biodiversity
or biological diversity is the diversity of life. There are a number of
definitions and measures of biodiversity. Biodiversity is a neologism
and a... |
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In
paleontology, a Lazarus taxon is a taxon that disappears from one or
more periods of the fossil record, only to appear again later. The term
refers to... |
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An
endangered species is a population of organisms which is either (a) so
few in number or (b) threatened by changing environmental or predation
parameters that... |
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An
extinction event occurs when a large number of species die out in a
relatively short period of time. Based on the fossil record, the
background... |
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Human
extinction would be the extinction of the human species, Homo sapiens,
whether on Earth or from the entire universe. Attitudes to human... |
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An extinction event (also extinction-level event, ELE)
occurs when a large number of species die out in a relatively short
period of time. Based on the fossil record, the background rate of
extinctions on Earth is about two to five taxonomic families of marine
invertebrates and vertebrates every million years.
Since
life began on Earth, a number of major mass extinctions have greatly
exceeded the background extinction rate present at other times. Though
there were undoubtedly mass extinctions in the Archean and Proterozoic,
it is only during the Phanerozoic Eon that the emergence of bones and
shells in the evolutionary tree has provided a sufficient fossil record
from which to make a systematic study of extinction patterns. The
number of major mass extinctions attributed to this most recent 540
million years varies from source to source, with some authorities
arguing for as few as 5 or more than 20. These differences stem
primarily from the threshold chosen for describing an extinction event
as "major", and what set of data one chooses to believe is the best
measure of past diversity.
Extinction events The
classical "Big Five" mass extinctions identified by Raup and Sepkoski
(1982) are widely agreed upon as some of the most significant: End
Ordovician, Late Devonian, End Permian, End Triassic, and End
Cretaceous.
These and a selection of other extinction events are highlighted below:
- 488
million years ago — a series of mass extinctions at the
Cambrian-Ordovician transition (the Cambrian-Ordovician extinction
events) eliminated many brachiopods and conodonts and severely reduced
the number of trilobite species.
- 444 million years ago — at the
Ordovician-Silurian transition two Ordovician-Silurian extinction
events occurred, probably as the result of a period of glaciation.
Marine habitats changed drastically as sea levels decreased, causing
the first die-off, and then another occurred between 500 thousand to a
million years later when sea levels rose rapidly. It has been suggested
that a gamma ray burst may have triggered this extinction.
- 360 million years ago — near the
Devonian-Carboniferous transition (the Late Devonian extinction) a
prolonged series of extinctions led to the elimination of about 70% of
all species. This was not a sudden event, with the period of decline
lasting perhaps as long as 20 million years. However, there is evidence
for a series of extinction pulses within this period.
- 251 million years ago — at the
Permian-Triassic transition (the Permian-Triassic extinction event)
about 95% of all marine species went extinct. This catastrophe was
Earth's worst mass extinction, killing 53% of marine families, 84% of
marine genera, and an estimated 70% of land species (including plants,
insects, and vertebrate animals.)
- 200 million years ago — at the
Triassic-Jurassic transition (the Triassic-Jurassic extinction event)
about 20% of all marine families as well as most non-dinosaurian
archosaurs, most therapsids, and the last of the large amphibians were
eliminated.
- 65 million years ago — at the
Cretaceous-Paleogene transition (the Cretaceous-Tertiary extinction
event) about 50% of all species became extinct (including all non-avian
dinosaurs). This extinction is widely believed to have resulted from an
asteroid or comet impact event.
- Present day — the Holocene
extinction event. A 1998 survey by the American Museum of Natural
History found that 70% of biologists view the present era as part of a
mass extinction event ,the fastest to have ever occurred. Some, such as
E. O. Wilson of Harvard University, predict that man's destruction of
the biosphere could cause the extinction of one-half of all species in
the next 100 years. Research and conservation efforts, such as the
IUCN's annual "Red List" of threatened species, all point to an ongoing
period of enhanced extinction, though some offer much lower rates and
hence longer time scales before the onset of catastrophic damage. The
extinction of many megafauna near the end of the most recent ice age is
also sometimes considered a part of the Holocene extinction event.
Causes for mass extinction
With
the exception of the Cretaceous-Tertiary mass extinction, which is
widely attributed to an impact event, and modern day extinctions
associated with the proliferation of human civilization, it is not well
known what has caused other mass extinctions. Some of the hypotheses
are discussed below.
- Impact
events - The impact of a sufficiently large asteroid or comet could
create Megatsunamis, global forest fires, and simulate nuclear winter
from the dust it puts in the atmosphere. Taken together, it is not
surprising that these and other related effects might be sufficiently
severe as to disrupt the global ecosystem and cause extinctions. Only
for the End Cretaceous extinctions is there strong evidence of such an
impact. Circumstantial evidence of such events is also given for the
End Permian, End Ordovician, End Jurassic and End Eocene extinctions.
- Climate change - Rapid transitions
in climate may be capable of stressing the environment to the point of
extinction. However, it is worth observing the recent cycles of ice
ages are only believed to have had very mild impacts on biodiversity.
Extinctions suggested to have this cause include: End Ordovician, End
Permian, Late Devonian, and others.
- Volcanism - The formation of large
igneous provinces, which can involve the outflow of millions of cubic
kilometers of lava in a short duration, are suggested to poison the
atmosphere and oceans in a way that may cause extinctions. This cause
has been proposed for the End Cretaceous, End Permian, End Triassic,
and End Jurassic extinctions.
- Gamma ray burst - A nearby gamma
ray burst (less than 6000 light years distance) could sufficiently
irradiate the surface of the Earth to kill organisms living there and
destroy the ozone layer in the process. From statistical arguments,
approximately 1 gamma ray burst would be expected to occur in close
proximity to Earth in the last 540 million years. This has been
suggested as an explanation for the End Ordovician extinction event.
- Plate tectonics - It has been
suggested that the opening and closing of seaways and land bridges may
play a role in extinction events as previously isolated populations are
brought into contact and new dynamics are established in the ecosystem.
This is most frequently discussed in relation to the End Permian mass
extinction.
Other
hypotheses, such as the spread of a new disease or simple
out-competition following an especially successful biological
innovation are also considered; however, it is often thought that the
major mass extinctions in Earth's history are too sudden and too
extensive to have resulted solely from biological events.
Postulated extinction cycles
It
has been suggested by several sources that biodiversity and/or
extinction events may be influenced by cyclic processes. The best-known
of these claims is the 26 to 30 million year viral cycle in extinctions
proposed by Raup and Sepkoski (1986). More recently, Rohde and Muller
(2005) have suggested that biodiversity fluctuates primarily on 62 ± 3
million cycles.
It is difficult to
evaluate the validity of these claims except through reduction to
statistical arguments regarding how plausible or implausible it is for
the observed data to exhibit a particular pattern, as the causes of
most extinction events are still too uncertain to attribute to them any
specific cause let alone a recurring one. Much early work in this area
also suffered from poor knowledge of the geological time scale (errors
> 10 million years at times), though the time scale now available
(uncertainties all < 4 million years) should be adequate for
studying these processes.
While the
statistics alone have been judged as sufficiently compelling to warrant
publication, it is important to consider processes that might be
responsible for a cyclic pattern of extinctions and future work may
focus on trying to find evidence of such processes.
One
theory, for which no real evidence exists, suggests that the extinction
cycle could be caused by the orbit of a hypothetical companion star
dubbed Nemesis that periodically disturbs the Oort cloud, sending
storms of large asteroids and comets towards the Solar System. Another
similar theory suggests that the Solar System's oscillations through
the plane of the galaxy results in periods of comet showers. Other
theories suggest geological instabilities that might allow heat to
periodically build up deep in the Earth, which is then released through
mantle plumes, periods of major volcanism and active plate tectonics.
If
any of these theories are correct, then it is worth noting that both
Raup and Sepkoski and Rohde & Muller predict another naturally
caused mass extinction event within the next 10 million years. |
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