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Mapping Chicxulub crater structure with gravity and seismic reflection data
Abstract
Aside from its significance in establishing the impact-mass extinction paradigm, the Chicxulub crater will probably come to exemplify the structure of large complex craters. Much of Chicxulub’s structure may be ‘mapped’ by tying its gravity expression to seismic-reflection profiles revealing an ∼180 km diameter for the now-buried crater. The distribution of karst topography aids in outlining the peripheral crater structure as also revealed by the horizontal gradient of the gravity anomaly. The fracturing inferred to control groundwater flow is apparently related to subsidence of the crater fill. Modelling the crater’s gravity expression based on a schematic structural model reveals that the crater fill is also responsible for the majority of the negative anomaly. The crater’s melt sheet and central structural uplift are the other significant contributors to its gravity expression. The Chicxulub impact released ∼1.2 × 10 31 ergs based on the observed collapsed disruption cavity of ∼86 km diameter reconstructed to an apparent disruption cavity ( D ad ) of ∼94 km diameter (equivalent to the excavation cavity) and an apparent transient cavity ( D at ) of ∼80 km diameter. This impact energy, together with the observed ∼2 × 10 11 g global Ir fluence in the Cretaceous-Tertiary (K-T) fireball layer indicates that the impactor was a comet estimated as massing ∼1.8 × 10 18 g of ∼16.5 km diameter assuming a 0.6 gcm −3 density. Dust-induced darkness and cold, wind, giant waves, thermal pulses from the impact fireball and re-entering ejecta, acid rain, ozone-layer depletion, cooling from stratospheric aerosols, H 2 O greenhouse, CO 2 greenhouse, poisons and mutagens, and oscillatory climate have been proposed as deleterious environmental effects of the Chicxulub impact with durations ranging from a few minutes to a million years. This succession of effects defines a temperature curve that is characteristic of large impacts. Although some patterns may be recognized in the K-T extinctions, and the survivorship rules changed across the boundary, relating specific environmental effects to species’ extinctions is not yet possible. Geochemical records across the boundary support the occurrence a prompt thermal pulse, acid rain and a ∼5000 year-long greenhouse. The period of extinctions seems to extend into the earliest Tertiary.
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“Based on the central high gravity and magnetic anomalies, Hildebrand et al. (1998) included a structural uplift zone with a diameter of 40-50 km in their forward modelling of the potential field data.”
From Observations and interpretations at Vredefort, Sudbury, and Chicxulub: Towards an empirical model of terrestrial impact basin formation (2008) · cites this paper as Hildebrand et al. 1998
In the citing paper
“The final crater diameter at Chicxulub has generally been quoted as ~180 km, primarily on the basis of the outer edge of the gravity low (Hildebrand et al. 1998), and between 180 and 200 km on the basis of faults in the target rock observed on marine seismic reflection data (e.g., Fig. 11; Morgan et al. 1997).”
From Observations and interpretations at Vredefort, Sudbury, and Chicxulub: Towards an empirical model of terrestrial impact basin formation (2008) · cites this paper as Hildebrand et al. 1998
In the citing paper
“In keeping with these observations, it is more likely that the density changes corresponding to this discrete megabreccia zone in the Hildebrand et al. (1998) model are either due to lateral and depth variations in the degree of fracturing and disruption of the basement rocks of the structural uplift, and/or to a change in mineralogy.”
From Observations and interpretations at Vredefort, Sudbury, and Chicxulub: Towards an empirical model of terrestrial impact basin formation (2008) · cites this paper as Hildebrand et al. 1998
In the citing paper
“Given the relative paucity of measured densities and density contrasts at Chicxulub, the model by Hildebrand et al. (1998) may be too complex in detail.”
From Observations and interpretations at Vredefort, Sudbury, and Chicxulub: Towards an empirical model of terrestrial impact basin formation (2008) · cites this paper as Hildebrand et al. 1998
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GRIEVE, R. A. F., REIMOLD, W. U., MORGAN, J., RILLER, U., & PILKINGTON, M. (2008) · Meteoritics & Planetary Science · doi:10.1111/j.1945-5100.2008.tb01086.x · Cited by 90
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Metadata
- Authors
- Hildebrand, A. R., Pilkington, M., Ortiz-Aleman, C., Chavez, R. E., Urrutia-Fucugauchi, J., Connors, M., Graniel-Castro, E., Camara-Zi, A., Halpenny, J. F., & Niehaus, D.
- Affiliations
- Geological Survey of Canada 615 Booth Street, Ottawa, Ontario, Canada K1A 0E9
- Instituto de Geofisica, UNAM, Ciudad Universitaria Codigo 04510, México, D. F., México
- Athabasca University 1, University Drive, Athabasca, Alberta, Canada T9S 3A3
- Facultad de Ingeniería, Universidad Autónoma de Yucatán Apdo. Postal No. 150, Cordemex 97111, Mérida, Yucatán, México
- Geomatics Canada 615 Booth Street, Ottawa, Ontario, Canada K1A 0E9
- PCI Enterprises 50 West Wilmot Street, Richmond Hill, Ontario, Canada, L4B 1M5
- Venue
- Geological Society, London, Special Publications
- Publisher
- Geological Society of London
- Published
- 1998-01
- Volume
- 140
- Issue
- 1
- Pages
- 155-176
- ISSN
- 0305-8719
- 2041-4927
- Cited by
- 64
- References
- 0
- Language
- en
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