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      Baby, it's cold outside: Climate model simulations of the effects of the asteroid impact at the end of the Cretaceous : CHICXULUB IMPACT COOLING

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      Geophysical Research Letters
      Wiley-Blackwell

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          The Chicxulub asteroid impact and mass extinction at the Cretaceous-Paleogene boundary.

          The Cretaceous-Paleogene boundary approximately 65.5 million years ago marks one of the three largest mass extinctions in the past 500 million years. The extinction event coincided with a large asteroid impact at Chicxulub, Mexico, and occurred within the time of Deccan flood basalt volcanism in India. Here, we synthesize records of the global stratigraphy across this boundary to assess the proposed causes of the mass extinction. Notably, a single ejecta-rich deposit compositionally linked to the Chicxulub impact is globally distributed at the Cretaceous-Paleogene boundary. The temporal match between the ejecta layer and the onset of the extinctions and the agreement of ecological patterns in the fossil record with modeled environmental perturbations (for example, darkness and cooling) lead us to conclude that the Chicxulub impact triggered the mass extinction.
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            Warm tropical sea surface temperatures in the Late Cretaceous and Eocene epochs.

            Climate models with increased levels of carbon dioxide predict that global warming causes heating in the tropics, but investigations of ancient climates based on palaeodata have generally indicated cool tropical temperatures during supposed greenhouse episodes. For example, in the Late Cretaceous and Eocene epochs there is abundant geological evidence for warm, mostly ice-free poles, but tropical sea surface temperatures are generally estimated to be only 15-23 degrees C, based on oxygen isotope palaeothermometry of surface-dwelling planktonic foraminifer shells. Here we question the validity of most such data on the grounds of poor preservation and diagenetic alteration. We present new data from exceptionally well preserved foraminifer shells extracted from impermeable clay-rich sediments, which indicate that for the intervals studied, tropical sea surface temperatures were at least 28-32 degrees C. These warm temperatures are more in line with our understanding of the geographical distributions of temperature-sensitive fossil organisms and the results of climate models with increased CO2 levels.
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              Solar Models: Current Epoch and Time Dependences, Neutrinos, and Helioseismological Properties

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                Author and article information

                Journal
                Geophysical Research Letters
                Geophys. Res. Lett.
                Wiley-Blackwell
                00948276
                January 16 2017
                January 16 2017
                : 44
                : 1
                : 419-427
                Article
                10.1002/2016GL072241
                187df5de-7aab-4bba-af10-047dcd936b10
                © 2017

                http://doi.wiley.com/10.1002/tdm_license_1

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