Architecture of Fluvial and Deltaic Deposits Exposed Along the Eastern Edge of the Western Fan of Jezero Crater, Mars.
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| Title: | Architecture of Fluvial and Deltaic Deposits Exposed Along the Eastern Edge of the Western Fan of Jezero Crater, Mars. |
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| Authors: | Mangold, N.1 (AUTHOR) nicolas.mangold@univ-nantes.fr, Caravaca, G.2 (AUTHOR), Gupta, S.3 (AUTHOR), Williams, R. M. E.4 (AUTHOR), Dromart, G.5 (AUTHOR), Gasnault, O.2 (AUTHOR), Le Mouélic, S.1 (AUTHOR), Paar, G.6 (AUTHOR), Bell, J.7 (AUTHOR), Beyssac, O.8 (AUTHOR), Carlot, N.1 (AUTHOR), Cousin, A.2 (AUTHOR), Dehouck, E.5 (AUTHOR), Horgan, B.9 (AUTHOR), Kah, L. C.10 (AUTHOR), Lasue, J.2 (AUTHOR), Maurice, S.2 (AUTHOR), Núñez, J. I.11 (AUTHOR), Shuster, D.12 (AUTHOR), Stack, K. M.13 (AUTHOR) |
| Source: | Journal of Geophysical Research. Planets. Mar2024, Vol. 129 Issue 3, p1-19. 19p. |
| Subject Terms: | *Lake sediments, Alluvium, Mars (Planet), Submarine fans, Boulders, Sandstone, Lunar craters |
| Abstract: | Early observations from the Perseverance rover suggested a deltaic origin for the western fan of Jezero crater only from images of the Kodiak butte. Here, we use images from the SuperCam Remote Micro‐Imager and the Mastcam‐Z camera to analyze the western fan front along the rover traverse, and further assess its depositional origin. Outcrops in the middle to lower half of the hillslopes comprise planar and inclined beds of sandstone that are interpreted as foresets of deltaic deposits. Foresets are locally structured in ∼20–25 m thick, ∼80–100 m long, antiformal structures interpreted as deltaic mouth bars. Above these foresets, interbedded sandstones and boulder conglomerates are interpreted as fluvial topset beds. One well‐preserved lens of boulder conglomerate displays rounded clasts within well‐sorted sediment deposited in overall fining upward beds. We interpret these deposits as resulting from lateral accretion within fluvial channels. Estimations of peak discharge rates give a range between ∼100 and ∼500 m3 s−1. By contrast, boulder conglomerates exposed in the uppermost part of hillslopes are poorly sorted and truncate the underlying beds. The presence of these boulder deposits suggests that intense sediment‐laden flood episodes occurred after the deltaic foreset and topset beds were deposited, although the origin, timing, and relationship of these boulder deposits to the ancient lake that once filled Jezero crater remains undetermined. Overall, these observations confirm the deltaic nature of the fan front, and suggest a highly variable fluvial input. Plain Language Summary: Early observations from the Perseverance rover of the Kodiak butte suggested a deltaic origin for the western fan of Jezero crater. Here, we use images from the SuperCam Remote Micro‐Imager and the Mastcam‐Z camera to analyze the western fan front along the rover traverse, and further assess its origin. We observe strata in the lower part of the fan front that we interpret as deltaic deposits formed below water in a lake. The strata of the upper part of the fan front contain sediments interpreted as fluvial deposits formed under various fluvial regimes, with some of them being deposited by the rivers that also fed the Jezero paleolake. Overall, these observations confirm the deltaic nature of the fan front, and suggest a highly variable fluvial input. Key Points: New observations from the Perseverance rover of the western fan front confirm a deltaic originDeltaic foresets in the lower fan front are organized as antiformal structures interpreted as delta mouth barsSandstones and conglomerates in the upper part of the fan front suggest a highly variable fluvial input [ABSTRACT FROM AUTHOR] |
| Copyright of Journal of Geophysical Research. Planets is the property of Wiley-Blackwell and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.) | |
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| Header | DbId: 8gh DbLabel: GreenFILE An: 176244983 AccessLevel: 6 PubType: Academic Journal PubTypeId: academicJournal PreciseRelevancyScore: 0 |
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| Items | – Name: Title Label: Title Group: Ti Data: Architecture of Fluvial and Deltaic Deposits Exposed Along the Eastern Edge of the Western Fan of Jezero Crater, Mars. – Name: Author Label: Authors Group: Au Data: <searchLink fieldCode="AR" term="%22Mangold%2C+N%2E%22">Mangold, N.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<i> nicolas.mangold@univ-nantes.fr</i><br /><searchLink fieldCode="AR" term="%22Caravaca%2C+G%2E%22">Caravaca, G.</searchLink><relatesTo>2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Gupta%2C+S%2E%22">Gupta, S.</searchLink><relatesTo>3</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Williams%2C+R%2E+M%2E+E%2E%22">Williams, R. M. E.</searchLink><relatesTo>4</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Dromart%2C+G%2E%22">Dromart, G.</searchLink><relatesTo>5</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Gasnault%2C+O%2E%22">Gasnault, O.</searchLink><relatesTo>2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Le+Mouélic%2C+S%2E%22">Le Mouélic, S.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Paar%2C+G%2E%22">Paar, G.</searchLink><relatesTo>6</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Bell%2C+J%2E%22">Bell, J.</searchLink><relatesTo>7</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Beyssac%2C+O%2E%22">Beyssac, O.</searchLink><relatesTo>8</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Carlot%2C+N%2E%22">Carlot, N.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Cousin%2C+A%2E%22">Cousin, A.</searchLink><relatesTo>2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Dehouck%2C+E%2E%22">Dehouck, E.</searchLink><relatesTo>5</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Horgan%2C+B%2E%22">Horgan, B.</searchLink><relatesTo>9</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Kah%2C+L%2E+C%2E%22">Kah, L. C.</searchLink><relatesTo>10</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Lasue%2C+J%2E%22">Lasue, J.</searchLink><relatesTo>2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Maurice%2C+S%2E%22">Maurice, S.</searchLink><relatesTo>2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Núñez%2C+J%2E+I%2E%22">Núñez, J. I.</searchLink><relatesTo>11</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Shuster%2C+D%2E%22">Shuster, D.</searchLink><relatesTo>12</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Stack%2C+K%2E+M%2E%22">Stack, K. M.</searchLink><relatesTo>13</relatesTo> (AUTHOR) – Name: TitleSource Label: Source Group: Src Data: <searchLink fieldCode="JN" term="%22Journal+of+Geophysical+Research%2E+Planets%22">Journal of Geophysical Research. Planets</searchLink>. Mar2024, Vol. 129 Issue 3, p1-19. 19p. – Name: Subject Label: Subject Terms Group: Su Data: *<searchLink fieldCode="DE" term="%22Lake+sediments%22">Lake sediments</searchLink><br /><searchLink fieldCode="DE" term="%22Alluvium%22">Alluvium</searchLink><br /><searchLink fieldCode="DE" term="%22Mars+%28Planet%29%22">Mars (Planet)</searchLink><br /><searchLink fieldCode="DE" term="%22Submarine+fans%22">Submarine fans</searchLink><br /><searchLink fieldCode="DE" term="%22Boulders%22">Boulders</searchLink><br /><searchLink fieldCode="DE" term="%22Sandstone%22">Sandstone</searchLink><br /><searchLink fieldCode="DE" term="%22Lunar+craters%22">Lunar craters</searchLink> – Name: Abstract Label: Abstract Group: Ab Data: Early observations from the Perseverance rover suggested a deltaic origin for the western fan of Jezero crater only from images of the Kodiak butte. Here, we use images from the SuperCam Remote Micro‐Imager and the Mastcam‐Z camera to analyze the western fan front along the rover traverse, and further assess its depositional origin. Outcrops in the middle to lower half of the hillslopes comprise planar and inclined beds of sandstone that are interpreted as foresets of deltaic deposits. Foresets are locally structured in ∼20–25 m thick, ∼80–100 m long, antiformal structures interpreted as deltaic mouth bars. Above these foresets, interbedded sandstones and boulder conglomerates are interpreted as fluvial topset beds. One well‐preserved lens of boulder conglomerate displays rounded clasts within well‐sorted sediment deposited in overall fining upward beds. We interpret these deposits as resulting from lateral accretion within fluvial channels. Estimations of peak discharge rates give a range between ∼100 and ∼500 m3 s−1. By contrast, boulder conglomerates exposed in the uppermost part of hillslopes are poorly sorted and truncate the underlying beds. The presence of these boulder deposits suggests that intense sediment‐laden flood episodes occurred after the deltaic foreset and topset beds were deposited, although the origin, timing, and relationship of these boulder deposits to the ancient lake that once filled Jezero crater remains undetermined. Overall, these observations confirm the deltaic nature of the fan front, and suggest a highly variable fluvial input. Plain Language Summary: Early observations from the Perseverance rover of the Kodiak butte suggested a deltaic origin for the western fan of Jezero crater. Here, we use images from the SuperCam Remote Micro‐Imager and the Mastcam‐Z camera to analyze the western fan front along the rover traverse, and further assess its origin. We observe strata in the lower part of the fan front that we interpret as deltaic deposits formed below water in a lake. The strata of the upper part of the fan front contain sediments interpreted as fluvial deposits formed under various fluvial regimes, with some of them being deposited by the rivers that also fed the Jezero paleolake. Overall, these observations confirm the deltaic nature of the fan front, and suggest a highly variable fluvial input. Key Points: New observations from the Perseverance rover of the western fan front confirm a deltaic originDeltaic foresets in the lower fan front are organized as antiformal structures interpreted as delta mouth barsSandstones and conglomerates in the upper part of the fan front suggest a highly variable fluvial input [ABSTRACT FROM AUTHOR] – Name: AbstractSuppliedCopyright Label: Group: Ab Data: <i>Copyright of Journal of Geophysical Research. Planets is the property of Wiley-Blackwell and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.) |
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| RecordInfo | BibRecord: BibEntity: Identifiers: – Type: doi Value: 10.1029/2023JE008204 Languages: – Code: eng Text: English PhysicalDescription: Pagination: PageCount: 19 StartPage: 1 Subjects: – SubjectFull: Lake sediments Type: general – SubjectFull: Alluvium Type: general – SubjectFull: Mars (Planet) Type: general – SubjectFull: Submarine fans Type: general – SubjectFull: Boulders Type: general – SubjectFull: Sandstone Type: general – SubjectFull: Lunar craters Type: general Titles: – TitleFull: Architecture of Fluvial and Deltaic Deposits Exposed Along the Eastern Edge of the Western Fan of Jezero Crater, Mars. Type: main BibRelationships: HasContributorRelationships: – PersonEntity: Name: NameFull: Mangold, N. – PersonEntity: Name: NameFull: Caravaca, G. – PersonEntity: Name: NameFull: Gupta, S. – PersonEntity: Name: NameFull: Williams, R. M. E. – PersonEntity: Name: NameFull: Dromart, G. – PersonEntity: Name: NameFull: Gasnault, O. – PersonEntity: Name: NameFull: Le Mouélic, S. – PersonEntity: Name: NameFull: Paar, G. – PersonEntity: Name: NameFull: Bell, J. – PersonEntity: Name: NameFull: Beyssac, O. – PersonEntity: Name: NameFull: Carlot, N. – PersonEntity: Name: NameFull: Cousin, A. – PersonEntity: Name: NameFull: Dehouck, E. – PersonEntity: Name: NameFull: Horgan, B. – PersonEntity: Name: NameFull: Kah, L. C. – PersonEntity: Name: NameFull: Lasue, J. – PersonEntity: Name: NameFull: Maurice, S. – PersonEntity: Name: NameFull: Núñez, J. I. – PersonEntity: Name: NameFull: Shuster, D. – PersonEntity: Name: NameFull: Stack, K. M. IsPartOfRelationships: – BibEntity: Dates: – D: 01 M: 03 Text: Mar2024 Type: published Y: 2024 Identifiers: – Type: issn-print Value: 21699097 Numbering: – Type: volume Value: 129 – Type: issue Value: 3 Titles: – TitleFull: Journal of Geophysical Research. Planets Type: main |
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