Expedition 364 Chicxulub: Chicxulub Peak Ring Formation
Expedition 364 Chicxulub: Chicxulub Peak Ring Formation
批准号:
NE/P011195/1
负责人:
Gareth Collins
金额:
$3.21万
依托单位:
依托单位国家:
英国
项目类别:
Research Grant
财政年份:
2017
资助国家:
英国
项目状态:
已结题
起止时间:
2017 至 --
中文摘要
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英文摘要
The Chicxulub impact crater, Mexico, is unique. It is the only known terrestrial impact structure that has been directly linked to a mass extinction event, and the only terrestrial impact with a global ejecta layer. Of the three largest impact structures on Earth, Chicxulub is the best preserved. Chicxulub is also the only known terrestrial impact structure with an intact, unequivocal topographic "peak ring". Chicxulub's role in the K-Pg mass extinction and its exceptional state of preservation make it an important natural laboratory for the study of both large impact crater formation on Earth and other planets, and the effects of large impacts on the Earth's environment and ecology. Our understanding of the impact process is far from complete and, despite over 30 years of intense debate, we are still striving to answer the question as to why this impact was so catastrophic.Expedition 364 is the first drill hole into an intact topographic peak ring, and the first to penetrate the offshore portion of the Chicxulub crater. Peak rings are a ring of hills that protrude through the crater floor within large impact basins on the terrestrial planets, and there is no consensual agreement on either their formational mechanism or the nature of the rocks that form them. Geophysical data indicate that the peak ring at Chicxulub is formed from rocks that have a low velocity and density, and one explanation for this is that they are highly fractured and porous. Immediately after impact the peak ring was submerged under water, and located adjacent to a thick pool of hot melt rocks. Hence, we would expect intense hydrothermal activity within the peak ring. This activity may have provided a niche for exotic life forms, in a similar way that hydrothermal vent systems do in the oceans. Drilling the peak ring will determine the origin, lithology, and physical state of the rocks that form it, allow us to distinguish between competing models of peak-ring formation, as well as document the hydrothermal systems and any associated microbiology. Immediately after impact the ocean is, locally, likely to have been sterile. We will use core through the post-impact sediments to examine the recolonization of the ocean, including: what biota came back first (benthic, dinoflagellates, specialists vs generalists), and how long did it take to return to normal conditions? The proposed drilling directly contributes to IODP goals in the: Deep Biosphere and the Subseafloor Ocean and Environmental Change, Processes and Effects, in particular the environmental and biological perturbations caused by Chicxulub.
期刊论文(10)
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Author Correction: Rock fluidization during peak-ring formation of large impact structures.
作者更正:大型冲击结构峰环形成过程中的岩石流化。
DOI:
10.1038/s41586-018-0748-0
发表时间:
2018
期刊:
Nature
影响因子:
64.8
作者:
[Riller U]
通讯作者:
Riller U
DOI:
10.1073/pnas.1909479116
发表时间:
2019-09-24
期刊:
PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA
影响因子:
11.1
作者:
[Gulick, Sean P. S., Bralowe, Timothy J., Wittmann, Axel]
通讯作者:
Wittmann, Axel
DOI:
10.1016/j.gca.2020.04.031
发表时间:
2020-07
期刊:
Geochimica et Cosmochimica Acta
影响因子:
5
作者:
[N. Timms;C. Kirkland;A. Cavosie;A. Rae;W. Rickard;N. Evans;T. Erickson;A. Wittmann;L. Ferrière;G. Collins;S. Gulick]
通讯作者:
N. Timms;C. Kirkland;A. Cavosie;A. Rae;W. Rickard;N. Evans;T. Erickson;A. Wittmann;L. Ferrière;G. Collins;S. Gulick
DOI:
10.1007/s00410-019-1565-7
发表时间:
2019-05
期刊:
Contributions to Mineralogy and Petrology
影响因子:
3.5
作者:
[N. Timms;M. Pearce;T. Erickson;A. Cavosie;A. Rae;J. Wheeler;A. Wittmann;L. Ferrière;M. Poelchau;N. Tomioka;G. Collins;S. Gulick;C. Rasmussen;J. Morgan]
通讯作者:
N. Timms;M. Pearce;T. Erickson;A. Cavosie;A. Rae;J. Wheeler;A. Wittmann;L. Ferrière;M. Poelchau;N. Tomioka;G. Collins;S. Gulick;C. Rasmussen;J. Morgan
Peering inside the peak ring of the Chicxulub Impact Crater-its nature and formation mechanism
窥探希克苏鲁伯陨石坑峰环内部——其性质和形成机制
DOI:
10.1111/gto.12261
发表时间:
2019
期刊:
Geology Today
影响因子:
--
作者:
[Urrutia-Fucugauchi J]
通讯作者:
Urrutia-Fucugauchi J
共 10 条
Planetary Origins and Evolution at Imperial (2019-2022)
-
批准号:ST/S000615/1
-
项目类别:Research Grant
-
资助金额:$110.87万
-
财政年份:2019
-
负责人:Gareth Collins
-
依托单位:
Planetary Origins and Evolution at Imperial (2016-2019)
-
批准号:ST/N000803/1
-
项目类别:Research Grant
-
资助金额:$112.03万
-
财政年份:2016
-
负责人:Gareth Collins
-
依托单位:
Bridging funds for consolidated grant ST/J001260/1 (Solar System Origin & Evolution at Imperial)
-
批准号:ST/M007642/1
-
项目类别:Research Grant
-
资助金额:$10.7万
-
财政年份:2015
-
负责人:Gareth Collins
-
依托单位:
Solar System Origin & Evolution at Imperial
-
批准号:ST/J001260/1
-
项目类别:Research Grant
-
资助金额:$175.12万
-
财政年份:2012
-
负责人:Gareth Collins
-
依托单位:
3D Numerical Modelling of Impact Cratering in the Solar System
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批准号:ST/G002452/1
-
项目类别:Research Grant
-
资助金额:$22.72万
-
财政年份:2009
-
负责人:Gareth Collins
-
依托单位:
3D Numerical Modelling of Large, Rapid, Violent Geologic Processes
-
批准号:NE/E013589/1
-
项目类别:Fellowship
-
资助金额:$54.81万
-
财政年份:2007
-
负责人:Gareth Collins
-
依托单位:
国内基金
海外基金
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批准号:31970086
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项目类别:面上项目
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资助金额:58.0万元
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负责人:秦加阳
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资助金额:20.0万元
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负责人:周春香
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批准号:41772050
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资助金额:73.0万元
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负责人:肖龙
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依托单位: