Probing the hydrothermal system of the Chicxulub impact crater

The Chicxulub impact event generated a long-duration hydrothermal system suitable for microbial life. The ~180-km-diameter Chicxulub peak-ring crater and ~240-km multiring basin, produced by the impact that terminated the Cretaceous, is the largest remaining intact impact basin on Earth. Internation...

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Veröffentlicht in:Science advances 2020-05, Vol.6 (22), p.eaaz3053-eaaz3053
Hauptverfasser: Kring, David A., Tikoo, Sonia M., Schmieder, Martin, Riller, Ulrich, Rebolledo-Vieyra, Mario, Simpson, Sarah L., Osinski, Gordon R., Gattacceca, Jérôme, Wittmann, Axel, Verhagen, Christina M., Cockell, Charles S., Coolen, Marco J. L., Longstaffe, Fred J., Gulick, Sean P. S., Morgan, Joanna V., Bralower, Timothy J., Chenot, Elise, Christeson, Gail L., Claeys, Philippe, Ferrière, Ludovic, Gebhardt, Catalina, Goto, Kazuhisa, Green, Sophie L., Jones, Heather, Lofi, Johanna, Lowery, Christopher M., Ocampo-Torres, Rubén, Perez-Cruz, Ligia, Pickersgill, Annemarie E., Poelchau, Michael H., Rae, Auriol S. P., Rasmussen, Cornelia, Sato, Honami, Smit, Jan, Tomioka, Naotaka, Urrutia-Fucugauchi, Jaime, Whalen, Michael T., Xiao, Long, Yamaguchi, Kosei E.
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container_end_page eaaz3053
container_issue 22
container_start_page eaaz3053
container_title Science advances
container_volume 6
creator Kring, David A.
Tikoo, Sonia M.
Schmieder, Martin
Riller, Ulrich
Rebolledo-Vieyra, Mario
Simpson, Sarah L.
Osinski, Gordon R.
Gattacceca, Jérôme
Wittmann, Axel
Verhagen, Christina M.
Cockell, Charles S.
Coolen, Marco J. L.
Longstaffe, Fred J.
Gulick, Sean P. S.
Morgan, Joanna V.
Bralower, Timothy J.
Chenot, Elise
Christeson, Gail L.
Claeys, Philippe
Ferrière, Ludovic
Gebhardt, Catalina
Goto, Kazuhisa
Green, Sophie L.
Jones, Heather
Lofi, Johanna
Lowery, Christopher M.
Ocampo-Torres, Rubén
Perez-Cruz, Ligia
Pickersgill, Annemarie E.
Poelchau, Michael H.
Rae, Auriol S. P.
Rasmussen, Cornelia
Sato, Honami
Smit, Jan
Tomioka, Naotaka
Urrutia-Fucugauchi, Jaime
Whalen, Michael T.
Xiao, Long
Yamaguchi, Kosei E.
description The Chicxulub impact event generated a long-duration hydrothermal system suitable for microbial life. The ~180-km-diameter Chicxulub peak-ring crater and ~240-km multiring basin, produced by the impact that terminated the Cretaceous, is the largest remaining intact impact basin on Earth. International Ocean Discovery Program (IODP) and International Continental Scientific Drilling Program (ICDP) Expedition 364 drilled to a depth of 1335 m below the sea floor into the peak ring, providing a unique opportunity to study the thermal and chemical modification of Earth’s crust caused by the impact. The recovered core shows the crater hosted a spatially extensive hydrothermal system that chemically and mineralogically modified ~1.4 × 10 5 km 3 of Earth’s crust, a volume more than nine times that of the Yellowstone Caldera system. Initially, high temperatures of 300° to 400°C and an independent geomagnetic polarity clock indicate the hydrothermal system was long lived, in excess of 10 6 years.
doi_str_mv 10.1126/sciadv.aaz3053
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International Ocean Discovery Program (IODP) and International Continental Scientific Drilling Program (ICDP) Expedition 364 drilled to a depth of 1335 m below the sea floor into the peak ring, providing a unique opportunity to study the thermal and chemical modification of Earth’s crust caused by the impact. The recovered core shows the crater hosted a spatially extensive hydrothermal system that chemically and mineralogically modified ~1.4 × 10 5 km 3 of Earth’s crust, a volume more than nine times that of the Yellowstone Caldera system. 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International Ocean Discovery Program (IODP) and International Continental Scientific Drilling Program (ICDP) Expedition 364 drilled to a depth of 1335 m below the sea floor into the peak ring, providing a unique opportunity to study the thermal and chemical modification of Earth’s crust caused by the impact. The recovered core shows the crater hosted a spatially extensive hydrothermal system that chemically and mineralogically modified ~1.4 × 10 5 km 3 of Earth’s crust, a volume more than nine times that of the Yellowstone Caldera system. 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L. ; Longstaffe, Fred J. ; Gulick, Sean P. S. ; Morgan, Joanna V. ; Bralower, Timothy J. ; Chenot, Elise ; Christeson, Gail L. ; Claeys, Philippe ; Ferrière, Ludovic ; Gebhardt, Catalina ; Goto, Kazuhisa ; Green, Sophie L. ; Jones, Heather ; Lofi, Johanna ; Lowery, Christopher M. ; Ocampo-Torres, Rubén ; Perez-Cruz, Ligia ; Pickersgill, Annemarie E. ; Poelchau, Michael H. ; Rae, Auriol S. 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P.</creatorcontrib><creatorcontrib>Rasmussen, Cornelia</creatorcontrib><creatorcontrib>Sato, Honami</creatorcontrib><creatorcontrib>Smit, Jan</creatorcontrib><creatorcontrib>Tomioka, Naotaka</creatorcontrib><creatorcontrib>Urrutia-Fucugauchi, Jaime</creatorcontrib><creatorcontrib>Whalen, Michael T.</creatorcontrib><creatorcontrib>Xiao, Long</creatorcontrib><creatorcontrib>Yamaguchi, Kosei E.</creatorcontrib><collection>CrossRef</collection><collection>MEDLINE - Academic</collection><collection>Hyper Article en Ligne (HAL)</collection><collection>Hyper Article en Ligne (HAL) (Open Access)</collection><collection>PubMed Central (Full Participant titles)</collection><jtitle>Science advances</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Kring, David A.</au><au>Tikoo, Sonia M.</au><au>Schmieder, Martin</au><au>Riller, Ulrich</au><au>Rebolledo-Vieyra, Mario</au><au>Simpson, Sarah L.</au><au>Osinski, Gordon R.</au><au>Gattacceca, Jérôme</au><au>Wittmann, Axel</au><au>Verhagen, Christina M.</au><au>Cockell, Charles S.</au><au>Coolen, Marco J. L.</au><au>Longstaffe, Fred J.</au><au>Gulick, Sean P. S.</au><au>Morgan, Joanna V.</au><au>Bralower, Timothy J.</au><au>Chenot, Elise</au><au>Christeson, Gail L.</au><au>Claeys, Philippe</au><au>Ferrière, Ludovic</au><au>Gebhardt, Catalina</au><au>Goto, Kazuhisa</au><au>Green, Sophie L.</au><au>Jones, Heather</au><au>Lofi, Johanna</au><au>Lowery, Christopher M.</au><au>Ocampo-Torres, Rubén</au><au>Perez-Cruz, Ligia</au><au>Pickersgill, Annemarie E.</au><au>Poelchau, Michael H.</au><au>Rae, Auriol S. P.</au><au>Rasmussen, Cornelia</au><au>Sato, Honami</au><au>Smit, Jan</au><au>Tomioka, Naotaka</au><au>Urrutia-Fucugauchi, Jaime</au><au>Whalen, Michael T.</au><au>Xiao, Long</au><au>Yamaguchi, Kosei E.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Probing the hydrothermal system of the Chicxulub impact crater</atitle><jtitle>Science advances</jtitle><date>2020-05-29</date><risdate>2020</risdate><volume>6</volume><issue>22</issue><spage>eaaz3053</spage><epage>eaaz3053</epage><pages>eaaz3053-eaaz3053</pages><issn>2375-2548</issn><eissn>2375-2548</eissn><abstract>The Chicxulub impact event generated a long-duration hydrothermal system suitable for microbial life. The ~180-km-diameter Chicxulub peak-ring crater and ~240-km multiring basin, produced by the impact that terminated the Cretaceous, is the largest remaining intact impact basin on Earth. International Ocean Discovery Program (IODP) and International Continental Scientific Drilling Program (ICDP) Expedition 364 drilled to a depth of 1335 m below the sea floor into the peak ring, providing a unique opportunity to study the thermal and chemical modification of Earth’s crust caused by the impact. The recovered core shows the crater hosted a spatially extensive hydrothermal system that chemically and mineralogically modified ~1.4 × 10 5 km 3 of Earth’s crust, a volume more than nine times that of the Yellowstone Caldera system. Initially, high temperatures of 300° to 400°C and an independent geomagnetic polarity clock indicate the hydrothermal system was long lived, in excess of 10 6 years.</abstract><pub>American Association for the Advancement of Science (AAAS)</pub><pmid>32523986</pmid><doi>10.1126/sciadv.aaz3053</doi><orcidid>https://orcid.org/0000-0002-4749-4429</orcidid><orcidid>https://orcid.org/0000-0002-6844-7023</orcidid><orcidid>https://orcid.org/0000-0002-5271-8554</orcidid><orcidid>https://orcid.org/0000-0003-0556-7471</orcidid><orcidid>https://orcid.org/0000-0002-0602-595X</orcidid><orcidid>https://orcid.org/0000-0002-9082-6230</orcidid><orcidid>https://orcid.org/0000-0002-3227-0676</orcidid><orcidid>https://orcid.org/0000-0002-0101-4397</orcidid><orcidid>https://orcid.org/0000-0003-3420-4135</orcidid><orcidid>https://orcid.org/0000-0001-7572-0801</orcidid><orcidid>https://orcid.org/0000-0002-3503-859X</orcidid><orcidid>https://orcid.org/0000-0002-1002-6453</orcidid><orcidid>https://orcid.org/0000-0002-1639-7140</orcidid><orcidid>https://orcid.org/0000-0002-6070-4865</orcidid><orcidid>https://orcid.org/0000-0002-1458-5148</orcidid><orcidid>https://orcid.org/0000-0001-5452-2849</orcidid><orcidid>https://orcid.org/0000-0002-7468-0454</orcidid><orcidid>https://orcid.org/0000-0002-4377-7018</orcidid><orcidid>https://orcid.org/0000-0003-2590-5239</orcidid><orcidid>https://orcid.org/0000-0001-8728-6918</orcidid><orcidid>https://orcid.org/0000-0002-7304-2821</orcidid><orcidid>https://orcid.org/0000-0002-1832-5925</orcidid><orcidid>https://orcid.org/0000-0002-3440-6282</orcidid><orcidid>https://orcid.org/0000-0001-9524-8284</orcidid><orcidid>https://orcid.org/0000-0003-3628-890X</orcidid><orcidid>https://orcid.org/0000-0003-4740-9068</orcidid><orcidid>https://orcid.org/0000-0001-5725-9513</orcidid><orcidid>https://orcid.org/0000-0002-0417-920X</orcidid><orcidid>https://orcid.org/0000-0002-4585-7687</orcidid><orcidid>https://orcid.org/0000-0002-3832-2959</orcidid><orcidid>https://orcid.org/0000-0003-4103-4808</orcidid><orcidid>https://orcid.org/0000-0001-6256-5945</orcidid><orcidid>https://orcid.org/0000-0002-3803-6792</orcidid><orcidid>https://orcid.org/0000-0003-2933-9473</orcidid><orcidid>https://orcid.org/0000-0003-3107-8954</orcidid><oa>free_for_read</oa></addata></record>
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subjects Earth Sciences
Geology
Planetary Science
Planetology
SciAdv r-articles
Sciences of the Universe
title Probing the hydrothermal system of the Chicxulub impact crater
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