2016
DOI: 10.1038/srep28427
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Global climate change driven by soot at the K-Pg boundary as the cause of the mass extinction

Abstract: The mass extinction of life 66 million years ago at the Cretaceous/Paleogene boundary, marked by the extinctions of dinosaurs and shallow marine organisms, is important because it led to the macroevolution of mammals and appearance of humans. The current hypothesis for the extinction is that an asteroid impact in present-day Mexico formed condensed aerosols in the stratosphere, which caused the cessation of photosynthesis and global near-freezing conditions. Here, we show that the stratospheric aerosols did no… Show more

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Cited by 81 publications
(145 citation statements)
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References 71 publications
(100 reference statements)
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“…Soot was apparently lost by oxidation in aerobic deep-water sites in the 66 million years since emplacement. There is debate about whether these particles originated from global wildfires, or from the impact itself (Belcher et al, 2003(Belcher et al, , 2004(Belcher et al, , 2005Belcher, 2009;Harvey et al, 2008;Robertson et al, 2013a;Pierazzo and Artemieva, 2012;Premović, 2012;Morgan et al, 2013;Kaiho et al, 2016). Robertson et al (2013a), Pierazzo and Artemieva (2012), Premović (2012) and Morgan et al (2013) argue that it is implausible that there was enough carbon at the impact site to produce the amount of soot observed by Wolbach et al (1988).…”
Section: Soot From the Chicxulub Impactmentioning
confidence: 99%
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“…Soot was apparently lost by oxidation in aerobic deep-water sites in the 66 million years since emplacement. There is debate about whether these particles originated from global wildfires, or from the impact itself (Belcher et al, 2003(Belcher et al, , 2004(Belcher et al, , 2005Belcher, 2009;Harvey et al, 2008;Robertson et al, 2013a;Pierazzo and Artemieva, 2012;Premović, 2012;Morgan et al, 2013;Kaiho et al, 2016). Robertson et al (2013a), Pierazzo and Artemieva (2012), Premović (2012) and Morgan et al (2013) argue that it is implausible that there was enough carbon at the impact site to produce the amount of soot observed by Wolbach et al (1988).…”
Section: Soot From the Chicxulub Impactmentioning
confidence: 99%
“…We use these most likely values in Table 1. Kaiho et al (2016) argue that the soot came from burning hydrocarbons in the crater and that the total mass emitted was either 5 × 10 2 , 15 × 10 2 , or 26 × 10 2 Tg. If we reduce these values by the authors' factor of 2.6 to represent the stratospheric emissions, they are 0.4, 1.0, and 1.7 % of the globally distributed elemental carbon reported by Wolbach et al (1990b).…”
Section: Soot From the Chicxulub Impactmentioning
confidence: 99%
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