Sequence of infilling events in Gale Crater, Mars: Results from morphology, stratigraphy, and mineralogy
International audience Gale Crater is filled by sedimentary deposits including a mound of layered deposits, Aeolis Mons. Using orbital data, we mapped the crater infillings and measured their geometry to determine their origin. The sediment of Aeolis Mons is interpreted to be primarily air fall mate...
Published in: | Journal of Geophysical Research: Planets |
---|---|
Main Authors: | , , , , , |
Other Authors: | , , , , , , , , , , |
Format: | Article in Journal/Newspaper |
Language: | English |
Published: |
HAL CCSD
2013
|
Subjects: | |
Online Access: | https://hal.science/hal-02359919 https://hal.science/hal-02359919/document https://hal.science/hal-02359919/file/Le%20Deit_etal_JGR%202013_Sequence%20of%20infilling%20events%20in%20Gale%20Crater%20Mars%20Results%20from%20morphology%20stratigraphy%20and%20mineralogy.pdf https://doi.org/10.1002/2012JE004322 |
id |
ftccsdartic:oai:HAL:hal-02359919v1 |
---|---|
record_format |
openpolar |
spelling |
ftccsdartic:oai:HAL:hal-02359919v1 2024-01-21T10:09:37+01:00 Sequence of infilling events in Gale Crater, Mars: Results from morphology, stratigraphy, and mineralogy Le Deit, L. Hauber, E. Fueten, F. Pondrelli, M Rossi, A., P Jaumann, R. DLR Institut für Planetenforschung Deutsches Zentrum für Luft- und Raumfahrt Berlin (DLR) Laboratoire de Planétologie et Géodynamique UMR 6112 (LPG) Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST) Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS) Deutsches Zentrum für Luft- und Raumfahrt (DLR) Department of Earth Sciences St. Catharines Brock University Canada Jacobs University = Constructor University Bremen DLR Institute of Planetary Research German Aerospace Center (DLR) 2013 https://hal.science/hal-02359919 https://hal.science/hal-02359919/document https://hal.science/hal-02359919/file/Le%20Deit_etal_JGR%202013_Sequence%20of%20infilling%20events%20in%20Gale%20Crater%20Mars%20Results%20from%20morphology%20stratigraphy%20and%20mineralogy.pdf https://doi.org/10.1002/2012JE004322 en eng HAL CCSD Wiley-Blackwell info:eu-repo/semantics/altIdentifier/doi/10.1002/2012JE004322 hal-02359919 https://hal.science/hal-02359919 https://hal.science/hal-02359919/document https://hal.science/hal-02359919/file/Le%20Deit_etal_JGR%202013_Sequence%20of%20infilling%20events%20in%20Gale%20Crater%20Mars%20Results%20from%20morphology%20stratigraphy%20and%20mineralogy.pdf doi:10.1002/2012JE004322 info:eu-repo/semantics/OpenAccess ISSN: 2169-9097 EISSN: 2169-9100 Journal of Geophysical Research. Planets https://hal.science/hal-02359919 Journal of Geophysical Research. Planets, 2013, 118, ⟨10.1002/2012JE004322⟩ [SDU.STU.PL]Sciences of the Universe [physics]/Earth Sciences/Planetology info:eu-repo/semantics/article Journal articles 2013 ftccsdartic https://doi.org/10.1002/2012JE004322 2023-12-24T00:04:30Z International audience Gale Crater is filled by sedimentary deposits including a mound of layered deposits, Aeolis Mons. Using orbital data, we mapped the crater infillings and measured their geometry to determine their origin. The sediment of Aeolis Mons is interpreted to be primarily air fall material such as dust, volcanic ash, fine-grained impact products, and possibly snow deposited by settling from the atmosphere, as well as wind-blown sands cemented in the crater center. Unconformity surfaces between the geological units are evidence for depositional hiatuses. Crater floor material deposited around Aeolis Mons and on the crater wall is interpreted to be alluvial and colluvial deposits. Morphologic evidence suggests that a shallow lake existed after the formation of the lowermost part of Aeolis Mons (the Small yardangs unit and the mass-wasting deposits). A suite of several features including patterned ground and possible rock glaciers are suggestive of periglacial processes with a permafrost environment after the first hundreds of thousands of years following its formation, dated to~3.61 Ga, in the Late Noachian/Early Hesperian. Episodic melting of snow in the crater could have caused the formation of sulfates and clays in Aeolis Mons, the formation of rock glaciers and the incision of deep canyons and valleys along its flanks as well as on the crater wall and rim, and the formation of a lake in the deepest portions of Gale. Article in Journal/Newspaper permafrost Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe) Journal of Geophysical Research: Planets 118 12 2439 2473 |
institution |
Open Polar |
collection |
Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe) |
op_collection_id |
ftccsdartic |
language |
English |
topic |
[SDU.STU.PL]Sciences of the Universe [physics]/Earth Sciences/Planetology |
spellingShingle |
[SDU.STU.PL]Sciences of the Universe [physics]/Earth Sciences/Planetology Le Deit, L. Hauber, E. Fueten, F. Pondrelli, M Rossi, A., P Jaumann, R. Sequence of infilling events in Gale Crater, Mars: Results from morphology, stratigraphy, and mineralogy |
topic_facet |
[SDU.STU.PL]Sciences of the Universe [physics]/Earth Sciences/Planetology |
description |
International audience Gale Crater is filled by sedimentary deposits including a mound of layered deposits, Aeolis Mons. Using orbital data, we mapped the crater infillings and measured their geometry to determine their origin. The sediment of Aeolis Mons is interpreted to be primarily air fall material such as dust, volcanic ash, fine-grained impact products, and possibly snow deposited by settling from the atmosphere, as well as wind-blown sands cemented in the crater center. Unconformity surfaces between the geological units are evidence for depositional hiatuses. Crater floor material deposited around Aeolis Mons and on the crater wall is interpreted to be alluvial and colluvial deposits. Morphologic evidence suggests that a shallow lake existed after the formation of the lowermost part of Aeolis Mons (the Small yardangs unit and the mass-wasting deposits). A suite of several features including patterned ground and possible rock glaciers are suggestive of periglacial processes with a permafrost environment after the first hundreds of thousands of years following its formation, dated to~3.61 Ga, in the Late Noachian/Early Hesperian. Episodic melting of snow in the crater could have caused the formation of sulfates and clays in Aeolis Mons, the formation of rock glaciers and the incision of deep canyons and valleys along its flanks as well as on the crater wall and rim, and the formation of a lake in the deepest portions of Gale. |
author2 |
DLR Institut für Planetenforschung Deutsches Zentrum für Luft- und Raumfahrt Berlin (DLR) Laboratoire de Planétologie et Géodynamique UMR 6112 (LPG) Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST) Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS) Deutsches Zentrum für Luft- und Raumfahrt (DLR) Department of Earth Sciences St. Catharines Brock University Canada Jacobs University = Constructor University Bremen DLR Institute of Planetary Research German Aerospace Center (DLR) |
format |
Article in Journal/Newspaper |
author |
Le Deit, L. Hauber, E. Fueten, F. Pondrelli, M Rossi, A., P Jaumann, R. |
author_facet |
Le Deit, L. Hauber, E. Fueten, F. Pondrelli, M Rossi, A., P Jaumann, R. |
author_sort |
Le Deit, L. |
title |
Sequence of infilling events in Gale Crater, Mars: Results from morphology, stratigraphy, and mineralogy |
title_short |
Sequence of infilling events in Gale Crater, Mars: Results from morphology, stratigraphy, and mineralogy |
title_full |
Sequence of infilling events in Gale Crater, Mars: Results from morphology, stratigraphy, and mineralogy |
title_fullStr |
Sequence of infilling events in Gale Crater, Mars: Results from morphology, stratigraphy, and mineralogy |
title_full_unstemmed |
Sequence of infilling events in Gale Crater, Mars: Results from morphology, stratigraphy, and mineralogy |
title_sort |
sequence of infilling events in gale crater, mars: results from morphology, stratigraphy, and mineralogy |
publisher |
HAL CCSD |
publishDate |
2013 |
url |
https://hal.science/hal-02359919 https://hal.science/hal-02359919/document https://hal.science/hal-02359919/file/Le%20Deit_etal_JGR%202013_Sequence%20of%20infilling%20events%20in%20Gale%20Crater%20Mars%20Results%20from%20morphology%20stratigraphy%20and%20mineralogy.pdf https://doi.org/10.1002/2012JE004322 |
genre |
permafrost |
genre_facet |
permafrost |
op_source |
ISSN: 2169-9097 EISSN: 2169-9100 Journal of Geophysical Research. Planets https://hal.science/hal-02359919 Journal of Geophysical Research. Planets, 2013, 118, ⟨10.1002/2012JE004322⟩ |
op_relation |
info:eu-repo/semantics/altIdentifier/doi/10.1002/2012JE004322 hal-02359919 https://hal.science/hal-02359919 https://hal.science/hal-02359919/document https://hal.science/hal-02359919/file/Le%20Deit_etal_JGR%202013_Sequence%20of%20infilling%20events%20in%20Gale%20Crater%20Mars%20Results%20from%20morphology%20stratigraphy%20and%20mineralogy.pdf doi:10.1002/2012JE004322 |
op_rights |
info:eu-repo/semantics/OpenAccess |
op_doi |
https://doi.org/10.1002/2012JE004322 |
container_title |
Journal of Geophysical Research: Planets |
container_volume |
118 |
container_issue |
12 |
container_start_page |
2439 |
op_container_end_page |
2473 |
_version_ |
1788700712925921280 |