¹Burbine, T.H.,²Greenwood, R.C.
Space Science Reviews 216, 59 Link to Article [DOI: 10.1007/s11214-020-00671-0]
¹Department of Astronomy, Mount Holyoke College, South Hadley, MA 01075, United States
²Planetary and Space Sciences, School of Physical Sciences, The Open University, Walton Hall, Milton Keynes, MK7 6AA, United Kingdom

We currently do not have a copyright agreement with this publisher and cannot display the abstract here

¹Kleine, T.,¹Budde, G.,¹Burkhardt, C.,²Kruijer, T.S.,¹Worsham, E.A.,³Morbidelli, A.,
⁴Nimmo, F.
Space Science Reviews 216, 55 Link to Article [DOI: 10.1007/s11214-020-00675-w]
¹Institut für Planetologie, University of Münster, Wilhelm-Klemm-Str. 10, Münster, 48149, Germany
²Lawrence Livermore National Laboratory, Nuclear and Chemical Sciences Division, 7000 East Avenue, Livermore, CA 94550, United States
³Observatoire de la Cote d’Azur, CS 34229, Nice Cedex 4, 06304, France
⁴Department of Earth and Planetary Sciences, University of California Santa Cruz, 1156 High Street, Santa Cruz, CA 95064, United States

We currently do not have a copyright agreement with this publisher and cannot display the abstract here

¹Żbik, M.S.
Advances in Space research (in Press) Link to Article [DOI: 10.1016/j.asr.2020.04.017]
¹Faculty of Geology, University of Warsaw, ul. Żwirki i Wigury 93, Warsaw, 02-089, Poland

We currently do not have a copyright agreement with this publisher and cannot display the abstract here

^1,2Sharygin, V.V.
Minerals, 10, 437 Link to Article [DOI: 10.3390/min10050437]
¹V.S. Sobolev Institute of Geology and Mineralogy, Siberian Branch of the RAS, 3 Acad. Koptyuga pr., Novosibirsk, 630090, Russian Federation
²ExtraTerra Consortium, Institute of Physics and Technology, Ural Federal University, 19 Mira str., Ekaterinburg, 620002, Russian Federation

We currently do not have a copyright agreement with this publisher and cannot display the abstract here

^1,2Alfio Alessandro Chiarenza,³Alexander Farnsworth,²Philip D. Mannion,³Daniel J. Lunt,³Paul J. Valdes,¹Joanna V. Morgan,¹Peter A. Allison
Proceedings of the National Academy of Sciences of the United States of America 117, 17084-17093 Link to Article [DOI: https://doi.org/10.1073/pnas.2006087117]
¹Department of Earth Science and Engineering, Imperial College London, South Kensington, SW7 2AZ London, United Kingdom;
²Department of Earth Sciences, University College London, WC1E 6BT London, United Kingdom;
³School of Geographical Sciences, University of Bristol, BS8 1TH Bristol, United Kingdom

The Cretaceous/Paleogene mass extinction, 66 Ma, included the demise of non-avian dinosaurs. Intense debate has focused on the relative roles of Deccan volcanism and the Chicxulub asteroid impact as kill mechanisms for this event. Here, we combine fossil-occurrence data with paleoclimate and habitat suitability models to evaluate dinosaur habitability in the wake of various asteroid impact and Deccan volcanism scenarios. Asteroid impact models generate a prolonged cold winter that suppresses potential global dinosaur habitats. Conversely, long-term forcing from Deccan volcanism (carbon dioxide [CO₂]-induced warming) leads to increased habitat suitability. Short-term (aerosol cooling) volcanism still allows equatorial habitability. These results support the asteroid impact as the main driver of the non-avian dinosaur extinction. By contrast, induced warming from volcanism mitigated the most extreme effects of asteroid impact, potentially reducing the extinction severity.