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Mineralogy of Cretaceous/Tertiary boundary clays in the Chicxulub structure in northern YucatanThe Cretaceous/Tertiary (K/T) boundary clay layer is thought to be derived from ejecta material from meteorite impact, based on the anomalous concentrations of noble metals in the layer. Because of recent findings of a half-meter thick ejecta deposit at the K/T boundary in Haiti, efforts have focused on locating a large impact feature in the Caribbean and the Gulf of Mexico. One of the leading candidates for the site of a large impact is the Chicxulub structure located on the northern Yucatan Peninsula in Mexico. The Chicxulub structure is a subsurface zone of upper Cretaceous igneous rocks, carbonates, and breccias. The structure has been interpreted to be a 200 km diameter; however, there is some question to the size of the structure or to the fact that it even is an impact feature. Little is known about the mineralogy of this structure; the objective of this study was to determine the clay mineralogy of core samples from within the Chicxulub structure.
Document ID
19920001035
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Ming, D. W.
(Lunar and Planetary Inst. Houston, TX., United States)
Sharpton, Virgil L.
(NASA Lyndon B. Johnson Space Center Houston, TX, United States)
Schuraytz, B. C.
(Lunar and Planetary Inst. Houston, TX., United States)
Date Acquired
September 6, 2013
Publication Date
January 1, 1991
Publication Information
Publication: Program and Abstracts for Clay Minerals Society 28th Annual Meeting
Subject Category
Astrophysics
Accession Number
92N10253
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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