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Chicxulub multiring impact basin - Size and other characteristics derived from gravity analysisThe buried Chicxulub impact structure in Mexico, which is linked to the Cretaceous-Tertiary (K-T) boundary layer, may be significantly larger than previously suspected. Reprocessed gravity data over Northern Yucatan reveal three major rings and parts of a fourth ring, spaced similarly to those observed at multiring impact basins on other planets. The outer ring, probably corresponding to the basin's topographic rim, is almost 300 kilometers in diameter, indicating that Chicxulub may be one of the largest impact structures produced in the inner solar system since the period of early bombardment ended nearly 4 billion years ago.
Document ID
19940035514
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Sharpton, Virgil L.
(Lunar and Planetary Inst. Houston, TX, United States)
Burke, Kevin
(Houston Univ. TX, United States)
Camargo-Zanoguera, Antonio
(Petroleos Mexicanos-PEMEX Gerencia Divisional de Programacion y Evaluacion, Mexico City, Mexico)
Hall, Stuart A.
(Houston Univ. TX, United States)
Lee, D. S.
(Lunar and Planetary Inst. Houston, TX, United States)
Marin, Luis E.
(NASA Headquarters Washington, DC United States)
Suarez-Reynoso, Gerardo
(Univ. Nacional Autonoma de Mexico Mexico City, United States)
Quezada-Muneton, Juan M.
(Petroleos Mexicanos-PEMEX Gerencia Divisional de Programacion y Evaluacion, Mexico City, Mexico)
Spudis, Paul D.
(Lunar and Planetary Inst. Houston, TX, United States)
Urrutia-Fucugauchi, Jaime
(Univ. Nacional Autonoma de Mexico Mexico City, United States)
Date Acquired
August 16, 2013
Publication Date
September 17, 1993
Publication Information
Publication: Science
Volume: 261
Issue: 5128
ISSN: 0036-8075
Subject Category
Geophysics
Accession Number
94A12169
Funding Number(s)
CONTRACT_GRANT: NASW-4574
Distribution Limits
Public
Copyright
Other

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