Cited by 164

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Chicxulub Multiring Impact Basin: Size and Other Characteristics Derived from Gravity Analysis

Sharpton, Virgil L., Burke, Kevin, Camargo-Zanoguera, Antonio, Hall, Stuart A., Lee, D. Scott, Marín, Luis E., Suáarez-Reynoso, Gerardo, Quezada-Muñeton, Juan Manuel, Spudis, Paul D., Urrutia-Fucugauchi, Jaime·1993·Science

Abstract

The 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.

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Crossref · 10.1126/science.261.5128.1564

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Research works printed but not linked: 25

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Metadata

Authors
Sharpton, V. L., Burke, K., Camargo-Zanoguera, A., Hall, S. A., Lee, D. S., Marín, L. E., Suáarez-Reynoso, G., Quezada-Muñeton, J. M., Spudis, P. D., & Urrutia-Fucugauchi, J.
Affiliations
  • Lunar and Planetary Institute, 3600 Bay Area Boulevard, Houston, TX 77058
  • Department of Geosciences, University of Houston, Houston, TX 77004
  • Gerencia Divisional de Programacion y Evaluación, Petr6leos Mexicanos, Marina Nacional 329, Mexico City, Mexico 01131
  • Instituto de Geofisica, Universidad Nacional Autonoma de M6xico, Mexico City, Mexico 04510
Venue
Science
Published
1993-09-17
Volume
261
Issue
5128
Pages
1564-1567
ISSN
  • 0036-8075
  • 1095-9203
Cited by
164
References
0
Language
en

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