Bedrock Geochemistry and Alteration History of the Clay‐Bearing Glen Torridon Region of Gale Crater, Mars
Glen Torridon is a topographic trough located on the slope of Aeolis Mons, Gale crater, Mars. It corresponds to what was previously referred to as the “clay‐bearing unit,” due to the relatively strong spectral signatures of clay minerals (mainly ferric smectites) detected from orbit. Starting in Jan...
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creator | Dehouck, Erwin Cousin, Agnès Mangold, Nicolas Frydenvang, Jens Gasnault, Olivier Forni, Olivier Rapin, William Gasda, Patrick J. Caravaca, Gwénaël David, Gaël Bedford, Candice C. Lasue, Jérémie Meslin, Pierre‐Yves Rammelkamp, Kristin Desjardins, Marine Le Mouélic, Stéphane Thorpe, Michael T. Fox, Valerie K. Bennett, Kristen A. Bryk, Alexander B. Lanza, Nina L. Maurice, Sylvestre Wiens, Roger C. |
description | Glen Torridon is a topographic trough located on the slope of Aeolis Mons, Gale crater, Mars. It corresponds to what was previously referred to as the “clay‐bearing unit,” due to the relatively strong spectral signatures of clay minerals (mainly ferric smectites) detected from orbit. Starting in January 2019, the Curiosity rover explored Glen Torridon for more than 700 sols (Martian days). The objectives of this campaign included acquiring a detailed understanding of the geologic context in which the clay minerals were formed, and determining the intensity of aqueous alteration experienced by the sediments. Here, we present the major‐element geochemistry of the bedrock as analyzed by the ChemCam instrument. Our results reveal that the two main types of bedrock exposures identified in the lower part of Glen Torridon are associated with distinct chemical compositions (K‐rich and Mg‐rich), for which we are able to propose mineralogical interpretations. Moreover, the topmost stratigraphic member exposed in the region displays a stronger diagenetic overprint, especially at two locations close to the unconformable contact with the overlying Stimson formation, where the bedrock composition significantly deviates from the rest of Glen Torridon. Overall, the values of the Chemical Index of Alteration determined with ChemCam are elevated by Martian standards, suggesting the formation of clay minerals through open‐system weathering. However, there is no indication that the alteration was stronger than in some terrains previously visited by Curiosity, which in turn implies that the enhanced orbital signatures are mostly controlled by non‐compositional factors.
Plain Language Summary
In early 2019, the Curiosity rover embarked on a multi‐year exploration of the Glen Torridon region, a topographic trough on the flank of Aeolis Mons, the sedimentary mound inside Gale crater, Mars. Orbital instruments have detected clay minerals over Glen Torridon, making it a primary target for Curiosity, because clay minerals are indicators of past interactions with water, and provide a medium favorable to the preservation of organic compounds. Understanding the context of formation of the clay minerals, and determining how much the sediments have been altered by water were among the objectives of the Glen Torridon campaign. Based on the chemical compositions measured by the ChemCam instrument, we show that the amount of water that interacted with the sediments was high enough to take a |
doi_str_mv | 10.1029/2021JE007103 |
format | Article |
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Plain Language Summary
In early 2019, the Curiosity rover embarked on a multi‐year exploration of the Glen Torridon region, a topographic trough on the flank of Aeolis Mons, the sedimentary mound inside Gale crater, Mars. Orbital instruments have detected clay minerals over Glen Torridon, making it a primary target for Curiosity, because clay minerals are indicators of past interactions with water, and provide a medium favorable to the preservation of organic compounds. Understanding the context of formation of the clay minerals, and determining how much the sediments have been altered by water were among the objectives of the Glen Torridon campaign. Based on the chemical compositions measured by the ChemCam instrument, we show that the amount of water that interacted with the sediments was high enough to take away part of the most soluble elements. Nonetheless, similar levels of alteration have been observed in other parts of Gale, which implies that the signal observed from orbit is not controlled solely by the abundance of clay minerals in the rocks. Finally, in the highest part of Glen Torridon, we analyzed an area of light‐toned rocks with distinct chemical compositions, which likely result from further modification by groundwater long after the main phase of alteration.
Key Points
The Curiosity rover explored Glen Torridon, a section of Aeolis Mons previously referred to as the “clay‐bearing unit” of Gale crater
Bedrock compositions measured by ChemCam show variations correlated with changes in outcrop expression and with diagenetic overprint
The relatively strong clay mineral signatures detected from orbit over Glen Torridon are not caused by a greater intensity of alteration</description><identifier>ISSN: 2169-9097</identifier><identifier>EISSN: 2169-9100</identifier><identifier>DOI: 10.1029/2021JE007103</identifier><language>eng</language><publisher>Washington: Blackwell Publishing Ltd</publisher><subject>aqueous alteration ; Bedrock ; Chemical composition ; Clay minerals ; Context ; Curiosity (Mars rover) ; Earth Sciences ; Gale crater ; Geochemistry ; Groundwater ; Mars ; Mars craters ; Mars rovers ; Mars surface ; Mars surface sediments ; Minerals ; Moisture content ; Organic compounds ; Planetology ; Rocks ; Sciences of the Universe ; Sediments ; Smectites ; Spectral signatures ; Stratigraphy ; Topography ; Water content ; Weathering</subject><ispartof>Journal of geophysical research. Planets, 2022-12, Vol.127 (12), p.n/a</ispartof><rights>2022. The Authors.</rights><rights>2022. This article is published under http://creativecommons.org/licenses/by-nc-nd/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a4029-25841be117d81bebe1ee78b96795158a934ab8b2ec525ad9ab76d017732682ed3</citedby><cites>FETCH-LOGICAL-a4029-25841be117d81bebe1ee78b96795158a934ab8b2ec525ad9ab76d017732682ed3</cites><orcidid>0000-0002-2719-1586 ; 0000-0003-4808-0823 ; 0000-0003-4660-8006 ; 0000-0001-9294-1227 ; 0000-0002-6979-9012 ; 0000-0002-0783-1064 ; 0000-0001-5260-1367 ; 0000-0001-8105-7129 ; 0000-0002-2013-7456 ; 0000-0002-3409-7344 ; 0000-0003-0895-1153 ; 0000-0001-6772-9689 ; 0000-0003-4445-7996 ; 0000-0002-1368-4494 ; 0000-0002-0022-0631 ; 0000-0001-9082-4457 ; 0000-0002-0972-1192 ; 0000-0001-7823-7794 ; 0000-0002-0703-3951 ; 0000-0002-4138-0471 ; 0000-0002-1235-9016</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://onlinelibrary.wiley.com/doi/pdf/10.1029%2F2021JE007103$$EPDF$$P50$$Gwiley$$Hfree_for_read</linktopdf><linktohtml>$$Uhttps://onlinelibrary.wiley.com/doi/full/10.1029%2F2021JE007103$$EHTML$$P50$$Gwiley$$Hfree_for_read</linktohtml><link.rule.ids>230,314,776,780,881,1411,1427,27901,27902,45550,45551,46384,46808</link.rule.ids><backlink>$$Uhttps://hal.science/hal-03812638$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Dehouck, Erwin</creatorcontrib><creatorcontrib>Cousin, Agnès</creatorcontrib><creatorcontrib>Mangold, Nicolas</creatorcontrib><creatorcontrib>Frydenvang, Jens</creatorcontrib><creatorcontrib>Gasnault, Olivier</creatorcontrib><creatorcontrib>Forni, Olivier</creatorcontrib><creatorcontrib>Rapin, William</creatorcontrib><creatorcontrib>Gasda, Patrick J.</creatorcontrib><creatorcontrib>Caravaca, Gwénaël</creatorcontrib><creatorcontrib>David, Gaël</creatorcontrib><creatorcontrib>Bedford, Candice C.</creatorcontrib><creatorcontrib>Lasue, Jérémie</creatorcontrib><creatorcontrib>Meslin, Pierre‐Yves</creatorcontrib><creatorcontrib>Rammelkamp, Kristin</creatorcontrib><creatorcontrib>Desjardins, Marine</creatorcontrib><creatorcontrib>Le Mouélic, Stéphane</creatorcontrib><creatorcontrib>Thorpe, Michael T.</creatorcontrib><creatorcontrib>Fox, Valerie K.</creatorcontrib><creatorcontrib>Bennett, Kristen A.</creatorcontrib><creatorcontrib>Bryk, Alexander B.</creatorcontrib><creatorcontrib>Lanza, Nina L.</creatorcontrib><creatorcontrib>Maurice, Sylvestre</creatorcontrib><creatorcontrib>Wiens, Roger C.</creatorcontrib><title>Bedrock Geochemistry and Alteration History of the Clay‐Bearing Glen Torridon Region of Gale Crater, Mars</title><title>Journal of geophysical research. Planets</title><description>Glen Torridon is a topographic trough located on the slope of Aeolis Mons, Gale crater, Mars. It corresponds to what was previously referred to as the “clay‐bearing unit,” due to the relatively strong spectral signatures of clay minerals (mainly ferric smectites) detected from orbit. Starting in January 2019, the Curiosity rover explored Glen Torridon for more than 700 sols (Martian days). The objectives of this campaign included acquiring a detailed understanding of the geologic context in which the clay minerals were formed, and determining the intensity of aqueous alteration experienced by the sediments. Here, we present the major‐element geochemistry of the bedrock as analyzed by the ChemCam instrument. Our results reveal that the two main types of bedrock exposures identified in the lower part of Glen Torridon are associated with distinct chemical compositions (K‐rich and Mg‐rich), for which we are able to propose mineralogical interpretations. Moreover, the topmost stratigraphic member exposed in the region displays a stronger diagenetic overprint, especially at two locations close to the unconformable contact with the overlying Stimson formation, where the bedrock composition significantly deviates from the rest of Glen Torridon. Overall, the values of the Chemical Index of Alteration determined with ChemCam are elevated by Martian standards, suggesting the formation of clay minerals through open‐system weathering. However, there is no indication that the alteration was stronger than in some terrains previously visited by Curiosity, which in turn implies that the enhanced orbital signatures are mostly controlled by non‐compositional factors.
Plain Language Summary
In early 2019, the Curiosity rover embarked on a multi‐year exploration of the Glen Torridon region, a topographic trough on the flank of Aeolis Mons, the sedimentary mound inside Gale crater, Mars. Orbital instruments have detected clay minerals over Glen Torridon, making it a primary target for Curiosity, because clay minerals are indicators of past interactions with water, and provide a medium favorable to the preservation of organic compounds. Understanding the context of formation of the clay minerals, and determining how much the sediments have been altered by water were among the objectives of the Glen Torridon campaign. Based on the chemical compositions measured by the ChemCam instrument, we show that the amount of water that interacted with the sediments was high enough to take away part of the most soluble elements. Nonetheless, similar levels of alteration have been observed in other parts of Gale, which implies that the signal observed from orbit is not controlled solely by the abundance of clay minerals in the rocks. Finally, in the highest part of Glen Torridon, we analyzed an area of light‐toned rocks with distinct chemical compositions, which likely result from further modification by groundwater long after the main phase of alteration.
Key Points
The Curiosity rover explored Glen Torridon, a section of Aeolis Mons previously referred to as the “clay‐bearing unit” of Gale crater
Bedrock compositions measured by ChemCam show variations correlated with changes in outcrop expression and with diagenetic overprint
The relatively strong clay mineral signatures detected from orbit over Glen Torridon are not caused by a greater intensity of alteration</description><subject>aqueous alteration</subject><subject>Bedrock</subject><subject>Chemical composition</subject><subject>Clay minerals</subject><subject>Context</subject><subject>Curiosity (Mars rover)</subject><subject>Earth Sciences</subject><subject>Gale crater</subject><subject>Geochemistry</subject><subject>Groundwater</subject><subject>Mars</subject><subject>Mars craters</subject><subject>Mars rovers</subject><subject>Mars surface</subject><subject>Mars surface sediments</subject><subject>Minerals</subject><subject>Moisture content</subject><subject>Organic compounds</subject><subject>Planetology</subject><subject>Rocks</subject><subject>Sciences of the Universe</subject><subject>Sediments</subject><subject>Smectites</subject><subject>Spectral signatures</subject><subject>Stratigraphy</subject><subject>Topography</subject><subject>Water content</subject><subject>Weathering</subject><issn>2169-9097</issn><issn>2169-9100</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><sourceid>24P</sourceid><recordid>eNp90EFPwjAUB_DFaCJBb36AJp5MmPa1bG2PQHBIMCYEz023PWAwVuyGhpsfwc_oJ7EENZ7s5b388-tL-4LgCugtUKbuGGUwHlIqgPKToMUgVqECSk9_eqrEeXBZ1yvqj_QR8Faw7mPubLYmCdpsiZuibtyemConvbJBZ5rCVmTkU-tjOyfNEsmgNPvP948-GldUC5KUWJGZda7IvZ3i4nDF08SU3voR6Drk0bj6Ijibm7LGy-_aDp7vh7PBKJw8JQ-D3iQ0Xf-RkEWyCykCiFz66jtEIVMVCxVBJI3iXZPKlGEWscjkyqQizikIwVksGea8Hdwc5y5Nqbeu2Bi319YUetSb6ENGuQQWc_kK3l4f7dbZlx3WjV7Znav88zQTMRUKFOVedY4qc7auHc5_xwLVh-3rv9v3nB_5W1Hi_l-rx8l0yEByxb8ASn-EWQ</recordid><startdate>202212</startdate><enddate>202212</enddate><creator>Dehouck, Erwin</creator><creator>Cousin, Agnès</creator><creator>Mangold, Nicolas</creator><creator>Frydenvang, Jens</creator><creator>Gasnault, Olivier</creator><creator>Forni, Olivier</creator><creator>Rapin, William</creator><creator>Gasda, Patrick J.</creator><creator>Caravaca, Gwénaël</creator><creator>David, Gaël</creator><creator>Bedford, Candice C.</creator><creator>Lasue, Jérémie</creator><creator>Meslin, Pierre‐Yves</creator><creator>Rammelkamp, Kristin</creator><creator>Desjardins, Marine</creator><creator>Le Mouélic, Stéphane</creator><creator>Thorpe, Michael T.</creator><creator>Fox, Valerie K.</creator><creator>Bennett, Kristen A.</creator><creator>Bryk, Alexander B.</creator><creator>Lanza, Nina L.</creator><creator>Maurice, Sylvestre</creator><creator>Wiens, Roger C.</creator><general>Blackwell Publishing Ltd</general><general>Wiley-Blackwell</general><scope>24P</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope><scope>1XC</scope><scope>VOOES</scope><orcidid>https://orcid.org/0000-0002-2719-1586</orcidid><orcidid>https://orcid.org/0000-0003-4808-0823</orcidid><orcidid>https://orcid.org/0000-0003-4660-8006</orcidid><orcidid>https://orcid.org/0000-0001-9294-1227</orcidid><orcidid>https://orcid.org/0000-0002-6979-9012</orcidid><orcidid>https://orcid.org/0000-0002-0783-1064</orcidid><orcidid>https://orcid.org/0000-0001-5260-1367</orcidid><orcidid>https://orcid.org/0000-0001-8105-7129</orcidid><orcidid>https://orcid.org/0000-0002-2013-7456</orcidid><orcidid>https://orcid.org/0000-0002-3409-7344</orcidid><orcidid>https://orcid.org/0000-0003-0895-1153</orcidid><orcidid>https://orcid.org/0000-0001-6772-9689</orcidid><orcidid>https://orcid.org/0000-0003-4445-7996</orcidid><orcidid>https://orcid.org/0000-0002-1368-4494</orcidid><orcidid>https://orcid.org/0000-0002-0022-0631</orcidid><orcidid>https://orcid.org/0000-0001-9082-4457</orcidid><orcidid>https://orcid.org/0000-0002-0972-1192</orcidid><orcidid>https://orcid.org/0000-0001-7823-7794</orcidid><orcidid>https://orcid.org/0000-0002-0703-3951</orcidid><orcidid>https://orcid.org/0000-0002-4138-0471</orcidid><orcidid>https://orcid.org/0000-0002-1235-9016</orcidid></search><sort><creationdate>202212</creationdate><title>Bedrock Geochemistry and Alteration History of the Clay‐Bearing Glen Torridon Region of Gale Crater, Mars</title><author>Dehouck, Erwin ; Cousin, Agnès ; Mangold, Nicolas ; Frydenvang, Jens ; Gasnault, Olivier ; Forni, Olivier ; Rapin, William ; Gasda, Patrick J. ; Caravaca, Gwénaël ; David, Gaël ; Bedford, Candice C. ; Lasue, Jérémie ; Meslin, Pierre‐Yves ; Rammelkamp, Kristin ; Desjardins, Marine ; Le Mouélic, Stéphane ; Thorpe, Michael T. ; Fox, Valerie K. ; Bennett, Kristen A. ; Bryk, Alexander B. ; Lanza, Nina L. ; Maurice, Sylvestre ; Wiens, Roger C.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a4029-25841be117d81bebe1ee78b96795158a934ab8b2ec525ad9ab76d017732682ed3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>aqueous alteration</topic><topic>Bedrock</topic><topic>Chemical composition</topic><topic>Clay minerals</topic><topic>Context</topic><topic>Curiosity (Mars rover)</topic><topic>Earth Sciences</topic><topic>Gale crater</topic><topic>Geochemistry</topic><topic>Groundwater</topic><topic>Mars</topic><topic>Mars craters</topic><topic>Mars rovers</topic><topic>Mars surface</topic><topic>Mars surface sediments</topic><topic>Minerals</topic><topic>Moisture content</topic><topic>Organic compounds</topic><topic>Planetology</topic><topic>Rocks</topic><topic>Sciences of the Universe</topic><topic>Sediments</topic><topic>Smectites</topic><topic>Spectral signatures</topic><topic>Stratigraphy</topic><topic>Topography</topic><topic>Water content</topic><topic>Weathering</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Dehouck, Erwin</creatorcontrib><creatorcontrib>Cousin, Agnès</creatorcontrib><creatorcontrib>Mangold, Nicolas</creatorcontrib><creatorcontrib>Frydenvang, Jens</creatorcontrib><creatorcontrib>Gasnault, Olivier</creatorcontrib><creatorcontrib>Forni, Olivier</creatorcontrib><creatorcontrib>Rapin, William</creatorcontrib><creatorcontrib>Gasda, Patrick J.</creatorcontrib><creatorcontrib>Caravaca, Gwénaël</creatorcontrib><creatorcontrib>David, Gaël</creatorcontrib><creatorcontrib>Bedford, Candice C.</creatorcontrib><creatorcontrib>Lasue, Jérémie</creatorcontrib><creatorcontrib>Meslin, Pierre‐Yves</creatorcontrib><creatorcontrib>Rammelkamp, Kristin</creatorcontrib><creatorcontrib>Desjardins, Marine</creatorcontrib><creatorcontrib>Le Mouélic, Stéphane</creatorcontrib><creatorcontrib>Thorpe, Michael T.</creatorcontrib><creatorcontrib>Fox, Valerie K.</creatorcontrib><creatorcontrib>Bennett, Kristen A.</creatorcontrib><creatorcontrib>Bryk, Alexander B.</creatorcontrib><creatorcontrib>Lanza, Nina L.</creatorcontrib><creatorcontrib>Maurice, Sylvestre</creatorcontrib><creatorcontrib>Wiens, Roger C.</creatorcontrib><collection>Wiley Online Library Open Access</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Hyper Article en Ligne (HAL)</collection><collection>Hyper Article en Ligne (HAL) (Open Access)</collection><jtitle>Journal of geophysical research. Planets</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Dehouck, Erwin</au><au>Cousin, Agnès</au><au>Mangold, Nicolas</au><au>Frydenvang, Jens</au><au>Gasnault, Olivier</au><au>Forni, Olivier</au><au>Rapin, William</au><au>Gasda, Patrick J.</au><au>Caravaca, Gwénaël</au><au>David, Gaël</au><au>Bedford, Candice C.</au><au>Lasue, Jérémie</au><au>Meslin, Pierre‐Yves</au><au>Rammelkamp, Kristin</au><au>Desjardins, Marine</au><au>Le Mouélic, Stéphane</au><au>Thorpe, Michael T.</au><au>Fox, Valerie K.</au><au>Bennett, Kristen A.</au><au>Bryk, Alexander B.</au><au>Lanza, Nina L.</au><au>Maurice, Sylvestre</au><au>Wiens, Roger C.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Bedrock Geochemistry and Alteration History of the Clay‐Bearing Glen Torridon Region of Gale Crater, Mars</atitle><jtitle>Journal of geophysical research. Planets</jtitle><date>2022-12</date><risdate>2022</risdate><volume>127</volume><issue>12</issue><epage>n/a</epage><issn>2169-9097</issn><eissn>2169-9100</eissn><abstract>Glen Torridon is a topographic trough located on the slope of Aeolis Mons, Gale crater, Mars. It corresponds to what was previously referred to as the “clay‐bearing unit,” due to the relatively strong spectral signatures of clay minerals (mainly ferric smectites) detected from orbit. Starting in January 2019, the Curiosity rover explored Glen Torridon for more than 700 sols (Martian days). The objectives of this campaign included acquiring a detailed understanding of the geologic context in which the clay minerals were formed, and determining the intensity of aqueous alteration experienced by the sediments. Here, we present the major‐element geochemistry of the bedrock as analyzed by the ChemCam instrument. Our results reveal that the two main types of bedrock exposures identified in the lower part of Glen Torridon are associated with distinct chemical compositions (K‐rich and Mg‐rich), for which we are able to propose mineralogical interpretations. Moreover, the topmost stratigraphic member exposed in the region displays a stronger diagenetic overprint, especially at two locations close to the unconformable contact with the overlying Stimson formation, where the bedrock composition significantly deviates from the rest of Glen Torridon. Overall, the values of the Chemical Index of Alteration determined with ChemCam are elevated by Martian standards, suggesting the formation of clay minerals through open‐system weathering. However, there is no indication that the alteration was stronger than in some terrains previously visited by Curiosity, which in turn implies that the enhanced orbital signatures are mostly controlled by non‐compositional factors.
Plain Language Summary
In early 2019, the Curiosity rover embarked on a multi‐year exploration of the Glen Torridon region, a topographic trough on the flank of Aeolis Mons, the sedimentary mound inside Gale crater, Mars. Orbital instruments have detected clay minerals over Glen Torridon, making it a primary target for Curiosity, because clay minerals are indicators of past interactions with water, and provide a medium favorable to the preservation of organic compounds. Understanding the context of formation of the clay minerals, and determining how much the sediments have been altered by water were among the objectives of the Glen Torridon campaign. Based on the chemical compositions measured by the ChemCam instrument, we show that the amount of water that interacted with the sediments was high enough to take away part of the most soluble elements. Nonetheless, similar levels of alteration have been observed in other parts of Gale, which implies that the signal observed from orbit is not controlled solely by the abundance of clay minerals in the rocks. Finally, in the highest part of Glen Torridon, we analyzed an area of light‐toned rocks with distinct chemical compositions, which likely result from further modification by groundwater long after the main phase of alteration.
Key Points
The Curiosity rover explored Glen Torridon, a section of Aeolis Mons previously referred to as the “clay‐bearing unit” of Gale crater
Bedrock compositions measured by ChemCam show variations correlated with changes in outcrop expression and with diagenetic overprint
The relatively strong clay mineral signatures detected from orbit over Glen Torridon are not caused by a greater intensity of alteration</abstract><cop>Washington</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1029/2021JE007103</doi><tpages>29</tpages><orcidid>https://orcid.org/0000-0002-2719-1586</orcidid><orcidid>https://orcid.org/0000-0003-4808-0823</orcidid><orcidid>https://orcid.org/0000-0003-4660-8006</orcidid><orcidid>https://orcid.org/0000-0001-9294-1227</orcidid><orcidid>https://orcid.org/0000-0002-6979-9012</orcidid><orcidid>https://orcid.org/0000-0002-0783-1064</orcidid><orcidid>https://orcid.org/0000-0001-5260-1367</orcidid><orcidid>https://orcid.org/0000-0001-8105-7129</orcidid><orcidid>https://orcid.org/0000-0002-2013-7456</orcidid><orcidid>https://orcid.org/0000-0002-3409-7344</orcidid><orcidid>https://orcid.org/0000-0003-0895-1153</orcidid><orcidid>https://orcid.org/0000-0001-6772-9689</orcidid><orcidid>https://orcid.org/0000-0003-4445-7996</orcidid><orcidid>https://orcid.org/0000-0002-1368-4494</orcidid><orcidid>https://orcid.org/0000-0002-0022-0631</orcidid><orcidid>https://orcid.org/0000-0001-9082-4457</orcidid><orcidid>https://orcid.org/0000-0002-0972-1192</orcidid><orcidid>https://orcid.org/0000-0001-7823-7794</orcidid><orcidid>https://orcid.org/0000-0002-0703-3951</orcidid><orcidid>https://orcid.org/0000-0002-4138-0471</orcidid><orcidid>https://orcid.org/0000-0002-1235-9016</orcidid><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 2169-9097 |
ispartof | Journal of geophysical research. Planets, 2022-12, Vol.127 (12), p.n/a |
issn | 2169-9097 2169-9100 |
language | eng |
recordid | cdi_hal_primary_oai_HAL_hal_03812638v1 |
source | Wiley Free Content; Wiley Online Library Journals Frontfile Complete; Alma/SFX Local Collection |
subjects | aqueous alteration Bedrock Chemical composition Clay minerals Context Curiosity (Mars rover) Earth Sciences Gale crater Geochemistry Groundwater Mars Mars craters Mars rovers Mars surface Mars surface sediments Minerals Moisture content Organic compounds Planetology Rocks Sciences of the Universe Sediments Smectites Spectral signatures Stratigraphy Topography Water content Weathering |
title | Bedrock Geochemistry and Alteration History of the Clay‐Bearing Glen Torridon Region of Gale Crater, Mars |
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