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05-22-2003, 07:26 AM | #1 |
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Extinctions: Volcanic Trapps, Meteorits, or other?
there have been several hypothesis to explain the big extinctions, among which the most famous (not the biggest) is the one occuring between Cretaceous and Tertiary (K/T).
I have heard for hypothesis: -variation of sea level (don't remember the name of who propose this) -apparition of new volcanic hot spot -> Volcanic Trapps expansion (Vincent Courtillot) for K/T extinction, Deccan Trapps -Big impact of space object (Luis Alvarez). For K/T extinction, Chicxulub crater. Has become the most popular explanation for K/T extinction. I have read recently an interview of Vincent Courtillot stating that the conflicting propositions are progressively reaching an agreement: he agrees that for K/T extinction, Chicxulub impact was probably an important factor, and he says that Alvarez agree that it is probably the only extinction when an impact had influence. Does some of you have informations on the latest state of theart about this subject? And on explanation of other mass extinctions? |
05-22-2003, 08:09 AM | #2 |
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The K/T is the only one of the 5 mass extinctions conclusively tied to an impact event. I wrote a mini-review on the Permian-Triassic extinction for my web site that discusses hypotheses relating to that extinction. It has some crappy grammer and could be better organized, but there is some good info there too:
click here Patrick |
05-22-2003, 08:44 AM | #3 |
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IIRC, there is a current theory that the Deccan Traps were caused by the Chixtulub impact. Allowing for continental drift, India was on the opposite side of the planet from Chixtulub at the time: impact shock waves would have converged on that point.
Presumably, if the same thing happened in the Permian (Siberian Traps), the impact site would have been in the deep ocean opposite Pangaea and would likely have been subducted by now, unless it's still in the Pacific. |
05-22-2003, 09:24 AM | #4 | |
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Quote:
Patrick |
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05-22-2003, 09:41 AM | #5 | |
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I have read (not in a scientific paper, but in a review of Courtillot's book "Evolutionary Catastrophes: the Science of Mass Extinction" that: "In fact, the famous KT iridium-signature has recently been identified in Deccan interflow sediments."
http://www.sfsite.com/05a/ec80.htm Has it been confirmed? if yes, is it consistent with Quote:
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05-22-2003, 08:33 PM | #6 |
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Patrick, perhaps I could trouble you to help here?
I saw a PBS show recently that discussed the Permian extinction. Briefly, it attributed a 1-2 degree rise in temperature to the global warming effect of the meteor impact. It then discussed Siberian lava traps, and a release of another gas (can't remember which one) that further raised the temperature 1-2 degrees. The combined effect of both events created the Permian extinction. The show estimated that it took 10 million years, from beginning to end. Apologies if I don't have the the explanation 100% correct - feel free to fix it up. Here's my question - with an extinction event caused by a meteor impact of this kind, I can't see how life would live past the first five years afterwards, much less for 5 or 10 million years. After the dust particles obscured the sun for a year or two, I would imagine that the foundation food sources would all be gone. It seems that if plants and plant-like life (algae, plankton, etc.) are the foundation of life, then any even that threatens them would send a deadly shock wave up the food chain immediately. Are there any explanations for the Permian extinction that address my question? Thank you. |
05-23-2003, 12:57 AM | #7 | |
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Which meteor for the Permian extinction?
Patrick told that Quote:
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05-23-2003, 07:14 AM | #8 | |||
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Quote:
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Becker et al (2001) argued for an impact event based on the isotopic ratios of nobles gasses trapped in fullerene molecules (which are something like cages) from two P-Tr boundary sections: one in Meishan, China, and one in Sasayama, Japan (one in Bükk mountains in Northern Hungary was tested, but not ET signature was detected). Purportedly the isotopic ratios of helium and argon are consistent with the impact of a chondritic meteorite, but not likely to be derived from a terrestrial source. This phenomena has also been associated with the K-T. However, the existence of an noble gas ET signature at both the Chinese and Japanese P-Tr sections was immediately questioned (Farley et al, 2001). In the Chinese section, no fullerence ET signature could be detected, despite testing more samples and from more levels than Becker et al, and Isozaki pointed out that the Beckers Japanese section was actually well below the P-Tr boundary. So, all in all, I think the evidence for an impact is pretty scant. But to answer your question -- how could any animals survive if the sun was obscured for 1-2 years? The answer is that if the sun were totally obscured for 1-2 years, they couldn't. However, some animals would easily be able to survive as long as there was some sunlight. I dont how long dust can remain in the atmosphere, but I dont think it possible that enough dust could remain in the atmosphere for 1-2 years to totally obscure the sun. I imagine a few dozen very dark days and alot of gray days after that. Plus, keep in mind that primary productivity almost did shut down across the P-Tr, judging from the remarkable P-Tr stratigraphic 'dead zone'! Refs Becker, Luann, Robert J. Poreda, Andrew G. Hunt, Theodore E. Bunch, and Michael Rampino (2001) Impact event at the Permian-Triassic boundary: evidence from extraterrestrial noble gases in fullerenes. Science, vol. 291, p. 1530-1533. Farley, K. A., Mukhopadhyay, S., Isozaki, Y., Becker, L., Poreda, R. J. (2001). An Extraterrestrial Impact at the Permian-Triassic Boundary?. Science 293: 2343a-2343. Patrick |
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05-23-2003, 07:20 AM | #9 | |
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Sauron,
Regarding volcanism, warming, and methane release at the P-Tr, this is from the little mini-review I linked to above. Quote:
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05-23-2003, 07:39 AM | #10 | |
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Regarding animals, anything that is a scavenger would do quite well in the days or years following such an event, when other animals are dying off in large numbers and leaving their corpses lying around! I imagine fungi (really just another kind of scavenger) would also do quite well with lots of dead vegetation lying around. In other words, what is devastating to one species might be a very, very good thing for another. I was recently working on a paper reviewing some of the recent molecular phylogenies of angiosperms (flowering plants) and two interesting results are coming out of such studies: first, that several major groups of plants are older than previously suspected, and second, that the major radiations of these groups began shortly after the KT extinction. I expect to see more papers in the future dealing with this. |
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