2004
DOI: 10.1111/j.1945-5100.2004.tb01130.x
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Stratigraphic and sedimentological observations from seismic data across the Chicxulub impact basin

Abstract: Abstract-Seismic data across the offshore half of the Chicxulub impact crater reveal a 145 kmdiameter post-impact basin to be a thickening of Tertiary sediment, which thickens by ~0.7 sec from the basin margin to the basin center. The basin existed long after the impact and was gradually infilled to its current flat surface. A suite of seismic horizons within the impact basin have been picked on four reflection lines across the crater. They reveal that the western and northwestern parts of the impact basin wer… Show more

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Cited by 38 publications
(40 citation statements)
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“…Morgan and Warner (1999) argue that the head scarp of this terrace zone is analogous to the crater rim in peak-ring craters ( Figure F1), and rings outside the head scarp (Figure F3) suggest that Chicxulub is a multi-ring basin (Morgan et al, 1997;Gulick et al, 2008). The acquired seismic data show that the water was deeper and the Mesozoic sediments thicker in the northeast quadrant of the crater than in the other quadrants (Bell et al, 2004;Gulick et al, 2008) and that lateral variation in the target at the impact site might explain the current crater asymmetry (Collins et al, 2008). Velocities and densities of the rocks that form the peak ring are low (Morgan et al, 2000;Vermeesch and Morgan, 2008;Barton et al, 2010), and a high-resolution velocity model obtained using full-waveform inversion ( Figure F4) shows that the uppermost peak ring is formed from about 100-150 m of rocks with low P-wave velocity (3000-3200 m/s) (Morgan et al, 2011).…”
Section: Introductionmentioning
confidence: 86%
“…Morgan and Warner (1999) argue that the head scarp of this terrace zone is analogous to the crater rim in peak-ring craters ( Figure F1), and rings outside the head scarp (Figure F3) suggest that Chicxulub is a multi-ring basin (Morgan et al, 1997;Gulick et al, 2008). The acquired seismic data show that the water was deeper and the Mesozoic sediments thicker in the northeast quadrant of the crater than in the other quadrants (Bell et al, 2004;Gulick et al, 2008) and that lateral variation in the target at the impact site might explain the current crater asymmetry (Collins et al, 2008). Velocities and densities of the rocks that form the peak ring are low (Morgan et al, 2000;Vermeesch and Morgan, 2008;Barton et al, 2010), and a high-resolution velocity model obtained using full-waveform inversion ( Figure F4) shows that the uppermost peak ring is formed from about 100-150 m of rocks with low P-wave velocity (3000-3200 m/s) (Morgan et al, 2011).…”
Section: Introductionmentioning
confidence: 86%
“…At Chicxulub crater, several small-throw faults restricted to the Cenozoic post-impact succession are observed and are mainly concentrated above the "inner ring" and peak ring (Fig. 3b) and the crater rim (e.g., Bell et al 2004). In detail, the internal post-impact depositional patterns reveal discrete fluxes in relative post-impact vertical movements, with sedimentation initially diminishing the impact-generated relief and subsequent differential compaction creating additional relief that is also filled (black triangles, Figs.…”
Section: Faultingmentioning
confidence: 99%
“…Continued deposition subsequently created a substantial overburden. For the Chicxulub crater, Bell et al (2004) postulated a spatially progressive infilling. In particular, the western and northwestern parts of the Chicxulub post-impact Cenozoic basin were filled ∼25 million years after the impact, whereas during a major marine regression a shelf progradation took place in the east ∼45 million years after the impact (in Early Miocene).…”
Section: Post-impact Infillingmentioning
confidence: 99%
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