Size and morphology of the Chicxulub impact crater

被引:227
作者
Morgan, J
Warner, M
Brittan, J
Buffler, R
Camargo, A
Christeson, G
Denton, P
Hildebrand, A
Hobbs, R
Macintyre, H
Mackenzie, G
Maguire, P
Marin, L
Nakamura, Y
Pilkington, M
Sharpton, V
Snyder, D
Suarez, G
Trejo, A
机构
[1] UNIV LONDON IMPERIAL COLL SCI TECHNOL & MED,DEPT GEOL,LONDON SW7 2BP,ENGLAND
[2] UNIV TEXAS,INST GEOPHYS,AUSTIN,TX 78759
[3] PETR MEXICANOS,VILLAHERMOSA 86030,MEXICO
[4] UNIV LEICESTER,LEICESTER LE1 7RH,LEICS,ENGLAND
[5] GEOL SURVEY CANADA,OTTAWA,ON K1A 0Y3,CANADA
[6] UNIV CAMBRIDGE,BULLARD LABS,BIRPS,CAMBRIDGE CB3 0EZ,ENGLAND
[7] UNIV NACL AUTONOMA MEXICO,MEXICO CITY 04510,DF,MEXICO
[8] LUNAR & PLANETARY INST,HOUSTON,TX 77058
关键词
D O I
10.1038/37291
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
The Chicxulub impact in Mexico has been linked to the mass extinction of species at the end of the Cretaceous period. From seismic data collected across the offshore portion of the Impact crater, the diameter of the transient cavity is determined to be about 100 km. This parameter is critical for constraining impact-related effects on the Cretaceous environment, with previous estimates of the cavity diameter spanning an order of magnitude in impact energy. The offshore seismic data indicate that the Chicxulub crater has a multi-ring basin morphology, similar to large Impact structures observed on other planets, such as Venus.
引用
收藏
页码:472 / 476
页数:5
相关论文
共 32 条
  • [1] Alexopoulos J.S, 1994, Large Meteorite Impacts and Planetary Evolution, P29, DOI DOI 10.1130/SPE293-P29
  • [2] MULTIRINGED IMPACT CRATERS ON VENUS - AN OVERVIEW FROM ARECIBO AND VENERA IMAGES AND INITIAL MAGELLAN DATA
    ALEXOPOULOS, JS
    MCKINNON, WB
    [J]. ICARUS, 1992, 100 (02) : 347 - 363
  • [3] EXTRATERRESTRIAL CAUSE FOR THE CRETACEOUS-TERTIARY EXTINCTION - EXPERIMENTAL RESULTS AND THEORETICAL INTERPRETATION
    ALVAREZ, LW
    ALVAREZ, W
    ASARO, F
    MICHEL, HV
    [J]. SCIENCE, 1980, 208 (4448) : 1095 - 1108
  • [4] Camargo-Zanoguera A., 1994, B ASOCIACION MEXICAN, V34, P1
  • [5] CROFT SK, 1980, P 11 LUN PLAN SCI C, P2347
  • [6] DHONDT S, 1994, GEOLOGY, V22, P983, DOI 10.1130/0091-7613(1994)022<0983:SWAAEA>2.3.CO
  • [7] 2
  • [8] A MODEL OF THE CHICXULUB IMPACT STRUCTURE (YUCATAN, MEXICO) BASED ON ITS GRAVITY AND MAGNETIC SIGNATURES
    ESPINDOLA, JM
    MENA, M
    DELAFUENTE, M
    CAMPOSENRIQUEZ, JO
    [J]. PHYSICS OF THE EARTH AND PLANETARY INTERIORS, 1995, 92 (3-4) : 271 - 278
  • [9] SIZE AND STRUCTURE OF THE CHICXULUB CRATER REVEALED BY HORIZONTAL GRAVITY GRADIENTS AND CENOTES
    HILDEBRAND, AR
    PILKINGTON, M
    CONNORS, M
    ORTIZALEMAN, C
    CHAVEZ, RE
    [J]. NATURE, 1995, 376 (6539) : 415 - 417
  • [10] HILDEBRAND AR, 1991, GEOLOGY, V19, P867, DOI 10.1130/0091-7613(1991)019<0867:CCAPCT>2.3.CO