UNAM scientific drilling program of Chicxulub impact structure - Evidence for a 300 kilometer crater diameter

被引:76
作者
UrrutiaFucugauchi, J
Marin, L
TrejoGarcia, A
机构
[1] Institute de Geofisica, Univ. Nacional Autonoma de Mexico, Mexico
[2] Instituto de Geofisica, Univ. Nacional Autonoma de Mexico
关键词
D O I
10.1029/96GL01566
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
As part of the UNAM drilling program at the Chicxulub structure, two 700 m deep continuously cored boreholes were completed between April and July, 1995. The Peto UNAM-6 and Tekax UNAM-7 drilling sites are similar to 150 km and 125 km, respectively, SSE of Chicxulub Puerto, near the crater's center. Core samples from both sites show a sequence of post-crater carbonates on top of a thick impact breccia pile covering the disturbed Mesozoic platform rocks. At UNAM-7, two;impact breccia units were encountered: (1) an upper breccia, mean magnetic susceptibility is high (similar to 55 x 10(-6) SI units), indicating a large component of silicate basement has been incorporated into this breccia, and (2) an evaporite-rich, low susceptibility impact breccia similar in character to the evaporite-rich breccias observed at the PEMEX drill sites further out. The upper breccia was encountered at similar to 226 m below the surface and is similar to 125 m thick; the lower breccia is immediately subjacent and is >240 m thick. This two-breccia sequence is typical of the suevite-Bunte breccia sequence found within other well preserved impact craters. The suevitic upper unit is not present at UNAM-6. Instead, a >240 m thick evaporite-rich breccia unit, similar to the lower breccia at UNAM-7, was encountered at a depth of similar to 280 m. The absence of an upper breccia equivalent at UNAM-6 suggests some portion of the breccia sequence has been removed by erosion. This is consistent with interpretations that place the high-standing crater rim at 130-150 km from the center. Consequently, the stratigraphic observations and magnetic susceptibility records on the upper and lower breccias (depth and thickness) support a similar to 300 km diameter crater model.
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页码:1565 / 1568
页数:4
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