ANALYSES OF SHOCKED QUARTZ AT THE GLOBAL K-P BOUNDARY INDICATE AN ORIGIN FROM A SINGLE, HIGH-ANGLE, OBLIQUE IMPACT AT CHICXULUB

dc.contributor.authorMorgan J.
dc.contributor.authorLana C.
dc.contributor.authorColes B.
dc.contributor.authorKearsley A.
dc.contributor.authorBelcher C.
dc.contributor.authorMontanari S.
dc.contributor.authorDíaz-Martínez E.
dc.contributor.authorBarbosa A.
dc.contributor.authorNeumann V.
dc.date.accessioned2024-09-28T07:10:22Z
dc.date.available2024-09-28T07:10:22Z
dc.date.issued2006
dc.description.abstractThe precise cause and timing of the Cretaceous-Paleocene (K-P) mass extinction 65 Ma ago remains a matter of debate. Many advocate that the extinction was caused by a meteorite impact at Chicxulub, Mexico, and a number of potential kill-mechanisms have been proposed for this. Although we now have good constraints on the size of this impact and chemistry of the target rocks, estimates of its environmental consequences are hindered by a lack of knowledge about the obliquity of this impact. An oblique impact is likely to have been far more catastrophic than a sub-vertical one, because greater volumes of volatiles would have been released into the atmosphere. The principal purpose of this study was to characterize shocked quartz within distal K-P ejecta, to investigate whether the quartz distribution carried a signature of the direction and angle of impact. Our analyses show that the total number, maximum and average size of shocked quartz grains all decrease gradually with paleodistance from Chicxulub. We do not find particularly high abundances in Pacific sites relative to Atlantic and European sites, as has been previously reported, and the size-distribution around Chicxulub is relatively symmetric. Ejecta samples at any one site display features that are indicative of a wide range of shock pressures, but the mean degree of shock increases with paleodistance. These shock- and size-distributions are both consistent with the K-P layer having been formed by a single impact at Chicxulub. One site in the South Atlantic contains quartz indicating an anomalously high average shock degree, that may be indicative of an oblique impact with an uprange direction to the southeast ± 45°. The apparent continuous coverage of proximal ejecta in this quadrant of the crater, however, suggests a relatively high impact angle of > 45°. We conclude that some of the more extreme predictions of the environmental consequences of a low-angle impact at Chicxulub are probably not applicable. © 2006 Elsevier B.V. All rights reserved.
dc.identifierhttps://www.elibrary.ru/item.asp?id=14425787
dc.identifier.citationEarth and Planetary Science Letters, 2006, 251, 3-4, 264-279
dc.identifier.doi10.1016/j.epsl.2006.09.009
dc.identifier.issn0012-821X
dc.identifier.urihttps://repository.geologyscience.ru/handle/123456789/45400
dc.subjectCHICXULUB
dc.subjectIMPACT CRATERING
dc.subjectJOIDES RESOLUTION
dc.subjectK-P BOUNDARY
dc.subjectLEG 130 SITE 803D
dc.subjectLEG 198 SITE 1209
dc.subjectLEG 207 SITE 1258A
dc.subjectLEG 208 SITE 1262
dc.subjectLEG LL44 SITE GPC3
dc.subjectOBLIQUITY OF IMPACT
dc.subjectOCEAN DRILLING PROGRAM
dc.subjectSHOCKED QUARTZ
dc.subject.ageМезозой::Меловая
dc.subject.ageКайнозой::Палеоген::Эоцен
dc.subject.ageКайнозой::Палеоген::Палеоцен
dc.subject.ageMesozoic::Cretaceous
dc.subject.ageCenozoic::Paleogene::Eocene
dc.subject.ageCenozoic::Paleogene::Paleocene
dc.titleANALYSES OF SHOCKED QUARTZ AT THE GLOBAL K-P BOUNDARY INDICATE AN ORIGIN FROM A SINGLE, HIGH-ANGLE, OBLIQUE IMPACT AT CHICXULUB
dc.typeСтатья

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