Early diagenesis at and below Vera Rubin ridge, Gale crater, Mars

Abstract Data returned by NASA’s Mars Science Laboratory Curiosity rover showed evidence for abundant secondary materials, including Fe‐oxides, phyllosilicates, and an amorphous component on and below Vera Rubin ridge in the Murray formation. We used equilibrium thermochemical modeling to test the h...

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Published in:Meteoritics & Planetary Science
Main Authors: Turner, S. M. R., Schwenzer, S. P., Bridges, J. C., Rampe, E. B., Bedford, C. C., Achilles, C. N., McAdam, A. C., Mangold, N., Hicks, L. J., Parnell, J., Fraeman, A. A., Reed, M. H.
Other Authors: UK Space Agency
Format: Article in Journal/Newspaper
Language:English
Published: Wiley 2021
Subjects:
Online Access:http://dx.doi.org/10.1111/maps.13748
https://onlinelibrary.wiley.com/doi/pdf/10.1111/maps.13748
https://onlinelibrary.wiley.com/doi/full-xml/10.1111/maps.13748
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spelling crwiley:10.1111/maps.13748 2024-06-23T07:57:27+00:00 Early diagenesis at and below Vera Rubin ridge, Gale crater, Mars Turner, S. M. R. Schwenzer, S. P. Bridges, J. C. Rampe, E. B. Bedford, C. C. Achilles, C. N. McAdam, A. C. Mangold, N. Hicks, L. J. Parnell, J. Fraeman, A. A. Reed, M. H. UK Space Agency 2021 http://dx.doi.org/10.1111/maps.13748 https://onlinelibrary.wiley.com/doi/pdf/10.1111/maps.13748 https://onlinelibrary.wiley.com/doi/full-xml/10.1111/maps.13748 en eng Wiley http://onlinelibrary.wiley.com/termsAndConditions#vor Meteoritics & Planetary Science volume 56, issue 10, page 1905-1932 ISSN 1086-9379 1945-5100 journal-article 2021 crwiley https://doi.org/10.1111/maps.13748 2024-06-11T04:46:08Z Abstract Data returned by NASA’s Mars Science Laboratory Curiosity rover showed evidence for abundant secondary materials, including Fe‐oxides, phyllosilicates, and an amorphous component on and below Vera Rubin ridge in the Murray formation. We used equilibrium thermochemical modeling to test the hypothesis that altered sediments were deposited as detrital igneous grains and subsequently underwent diagenesis. Chemical compositions of the Murray formations’ altered components were calculated using data returned by the chemistry and mineralogy X‐ray diffraction instrument and the alpha particle X‐ray spectrometer on board Curiosity. Reaction of these alteration compositions with a CO 2 ‐poor and oxidizing dilute aqueous solution was modeled at 25–100 °C, with 10–50% Fe 3+ /Fe tot of the host rock. The modeled alteration assemblages included abundant phyllosilicates and Fe‐oxides at water‐to‐rock ratios >100. Modeled alteration abundances were directly comparable to observed abundances of hematite and clay minerals at a water‐to‐rock ratio of 10,000, for system temperatures of 50–100 °C with fluid pH ranging from 7.9 to 9.3. Modeling results suggest that the hematite–clay mineral assemblage is primarily the result of enhanced groundwater flow compared to the Sheepbed mudstone observed at Yellowknife Bay, and underwent further, localized alteration to produce the mineralogy observed by Curiosity. Article in Journal/Newspaper Yellowknife Wiley Online Library Rubin ENVELOPE(65.493,65.493,-73.438,-73.438) Yellowknife Yellowknife Bay ENVELOPE(-114.336,-114.336,62.367,62.367) Meteoritics & Planetary Science 56 10 1905 1932
institution Open Polar
collection Wiley Online Library
op_collection_id crwiley
language English
description Abstract Data returned by NASA’s Mars Science Laboratory Curiosity rover showed evidence for abundant secondary materials, including Fe‐oxides, phyllosilicates, and an amorphous component on and below Vera Rubin ridge in the Murray formation. We used equilibrium thermochemical modeling to test the hypothesis that altered sediments were deposited as detrital igneous grains and subsequently underwent diagenesis. Chemical compositions of the Murray formations’ altered components were calculated using data returned by the chemistry and mineralogy X‐ray diffraction instrument and the alpha particle X‐ray spectrometer on board Curiosity. Reaction of these alteration compositions with a CO 2 ‐poor and oxidizing dilute aqueous solution was modeled at 25–100 °C, with 10–50% Fe 3+ /Fe tot of the host rock. The modeled alteration assemblages included abundant phyllosilicates and Fe‐oxides at water‐to‐rock ratios >100. Modeled alteration abundances were directly comparable to observed abundances of hematite and clay minerals at a water‐to‐rock ratio of 10,000, for system temperatures of 50–100 °C with fluid pH ranging from 7.9 to 9.3. Modeling results suggest that the hematite–clay mineral assemblage is primarily the result of enhanced groundwater flow compared to the Sheepbed mudstone observed at Yellowknife Bay, and underwent further, localized alteration to produce the mineralogy observed by Curiosity.
author2 UK Space Agency
format Article in Journal/Newspaper
author Turner, S. M. R.
Schwenzer, S. P.
Bridges, J. C.
Rampe, E. B.
Bedford, C. C.
Achilles, C. N.
McAdam, A. C.
Mangold, N.
Hicks, L. J.
Parnell, J.
Fraeman, A. A.
Reed, M. H.
spellingShingle Turner, S. M. R.
Schwenzer, S. P.
Bridges, J. C.
Rampe, E. B.
Bedford, C. C.
Achilles, C. N.
McAdam, A. C.
Mangold, N.
Hicks, L. J.
Parnell, J.
Fraeman, A. A.
Reed, M. H.
Early diagenesis at and below Vera Rubin ridge, Gale crater, Mars
author_facet Turner, S. M. R.
Schwenzer, S. P.
Bridges, J. C.
Rampe, E. B.
Bedford, C. C.
Achilles, C. N.
McAdam, A. C.
Mangold, N.
Hicks, L. J.
Parnell, J.
Fraeman, A. A.
Reed, M. H.
author_sort Turner, S. M. R.
title Early diagenesis at and below Vera Rubin ridge, Gale crater, Mars
title_short Early diagenesis at and below Vera Rubin ridge, Gale crater, Mars
title_full Early diagenesis at and below Vera Rubin ridge, Gale crater, Mars
title_fullStr Early diagenesis at and below Vera Rubin ridge, Gale crater, Mars
title_full_unstemmed Early diagenesis at and below Vera Rubin ridge, Gale crater, Mars
title_sort early diagenesis at and below vera rubin ridge, gale crater, mars
publisher Wiley
publishDate 2021
url http://dx.doi.org/10.1111/maps.13748
https://onlinelibrary.wiley.com/doi/pdf/10.1111/maps.13748
https://onlinelibrary.wiley.com/doi/full-xml/10.1111/maps.13748
long_lat ENVELOPE(65.493,65.493,-73.438,-73.438)
ENVELOPE(-114.336,-114.336,62.367,62.367)
geographic Rubin
Yellowknife
Yellowknife Bay
geographic_facet Rubin
Yellowknife
Yellowknife Bay
genre Yellowknife
genre_facet Yellowknife
op_source Meteoritics & Planetary Science
volume 56, issue 10, page 1905-1932
ISSN 1086-9379 1945-5100
op_rights http://onlinelibrary.wiley.com/termsAndConditions#vor
op_doi https://doi.org/10.1111/maps.13748
container_title Meteoritics & Planetary Science
container_volume 56
container_issue 10
container_start_page 1905
op_container_end_page 1932
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