Nature and origin of sulfate deposits in equatorial and polar regions of Mars. Morphological and mineralogical comparison of Aram Chaos and the North Polar Cap.
Important sulfate deposits have been discovered in various equatorial regions of Mars : the canyons of Valles Marineris, chaotic terrains, and Meridiani plains. In order to explain the chemical composition of these deposits and the formation of such a large volume of sediments displaying the same co...
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ftccsdartic:oai:HAL:tel-00762257v1 2023-05-15T14:04:01+02:00 Nature and origin of sulfate deposits in equatorial and polar regions of Mars. Morphological and mineralogical comparison of Aram Chaos and the North Polar Cap. Nature et origine des dépôts de sulfates dans les régions équatoriales et polaires de Mars. Comparaison morphologique et minéralogique entre Aram Chaos et la calotte polaire Nord. Massé, Marion 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) Université de Nantes Olivier Bourgeois 2010-12-02 https://tel.archives-ouvertes.fr/tel-00762257 https://tel.archives-ouvertes.fr/tel-00762257/document https://tel.archives-ouvertes.fr/tel-00762257/file/these_Masse.pdf fr fre HAL CCSD tel-00762257 https://tel.archives-ouvertes.fr/tel-00762257 https://tel.archives-ouvertes.fr/tel-00762257/document https://tel.archives-ouvertes.fr/tel-00762257/file/these_Masse.pdf info:eu-repo/semantics/OpenAccess https://tel.archives-ouvertes.fr/tel-00762257 Planétologie. Université de Nantes, 2010. Français weathering chaotic terrains polar cap hyperspectral-imaging geomorphology Mars composition altération terrains chaotiques calotte polaire spectro-imagerie géomorphologie [SDU.STU.PL]Sciences of the Universe [physics]/Earth Sciences/Planetology info:eu-repo/semantics/doctoralThesis Theses 2010 ftccsdartic 2021-10-24T15:41:30Z Important sulfate deposits have been discovered in various equatorial regions of Mars : the canyons of Valles Marineris, chaotic terrains, and Meridiani plains. In order to explain the chemical composition of these deposits and the formation of such a large volume of sediments displaying the same composition and various and extensive terrains, one of the latest hypotheses suggests a glacial origin. The aim of this thesis is to evaluate the consistency of this hypothesis by an integrated morphological and mineralogical study of sulfates found on the North Polar Cap and on equatorial chaotic terrains (Aram Chaos). The analysis of the North Polar Cap reveals that all the superficial sediments contain gypsum. These sulfate-bearing particles have been released directly from the ice cap by sublimation. Winds are then responsible for the reworking of these sediments and their accumulation in the circumpolar dune field. The analysis of Aram Chaos sulfate deposits reveals some bright, layered outcrops, similar to those observed in Valles Marineris and in Meridiani Planum they contain a mixture of monohydrated sulfates, ferric oxides and hydrated minerals. These deposits could also originate from glacial processes because climate models and morphological analyses show that, during periods of high obliquity, ice accumulations can have formed in the lower latitudes. Moreover, the observation of terrestrial analogs in Antarctica demonstrates that sulfates can form in ice by post-depositional processes. These processes could reproduce the chemical composition of the Martian equatorial deposits if ice and some volcanic materials were accumulated at the same time. D'importants dépôts de sulfates ont été découverts dans certaines régions équatoriales de Mars : les canyons de Valles Marineris, les terrains chaotiques, et les plaines de Meridiani. Afin d'expliquer la chimie de ces dépôts, ainsi que la formation d'un tel volume de sédiments de même composition, sur des surfaces aussi larges et variées, l'une des hypothèses les ... Doctoral or Postdoctoral Thesis Antarc* Antarctica Ice cap Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe) Valles ENVELOPE(-58.783,-58.783,-62.167,-62.167) |
institution |
Open Polar |
collection |
Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe) |
op_collection_id |
ftccsdartic |
language |
French |
topic |
weathering chaotic terrains polar cap hyperspectral-imaging geomorphology Mars composition altération terrains chaotiques calotte polaire spectro-imagerie géomorphologie [SDU.STU.PL]Sciences of the Universe [physics]/Earth Sciences/Planetology |
spellingShingle |
weathering chaotic terrains polar cap hyperspectral-imaging geomorphology Mars composition altération terrains chaotiques calotte polaire spectro-imagerie géomorphologie [SDU.STU.PL]Sciences of the Universe [physics]/Earth Sciences/Planetology Massé, Marion Nature and origin of sulfate deposits in equatorial and polar regions of Mars. Morphological and mineralogical comparison of Aram Chaos and the North Polar Cap. |
topic_facet |
weathering chaotic terrains polar cap hyperspectral-imaging geomorphology Mars composition altération terrains chaotiques calotte polaire spectro-imagerie géomorphologie [SDU.STU.PL]Sciences of the Universe [physics]/Earth Sciences/Planetology |
description |
Important sulfate deposits have been discovered in various equatorial regions of Mars : the canyons of Valles Marineris, chaotic terrains, and Meridiani plains. In order to explain the chemical composition of these deposits and the formation of such a large volume of sediments displaying the same composition and various and extensive terrains, one of the latest hypotheses suggests a glacial origin. The aim of this thesis is to evaluate the consistency of this hypothesis by an integrated morphological and mineralogical study of sulfates found on the North Polar Cap and on equatorial chaotic terrains (Aram Chaos). The analysis of the North Polar Cap reveals that all the superficial sediments contain gypsum. These sulfate-bearing particles have been released directly from the ice cap by sublimation. Winds are then responsible for the reworking of these sediments and their accumulation in the circumpolar dune field. The analysis of Aram Chaos sulfate deposits reveals some bright, layered outcrops, similar to those observed in Valles Marineris and in Meridiani Planum they contain a mixture of monohydrated sulfates, ferric oxides and hydrated minerals. These deposits could also originate from glacial processes because climate models and morphological analyses show that, during periods of high obliquity, ice accumulations can have formed in the lower latitudes. Moreover, the observation of terrestrial analogs in Antarctica demonstrates that sulfates can form in ice by post-depositional processes. These processes could reproduce the chemical composition of the Martian equatorial deposits if ice and some volcanic materials were accumulated at the same time. D'importants dépôts de sulfates ont été découverts dans certaines régions équatoriales de Mars : les canyons de Valles Marineris, les terrains chaotiques, et les plaines de Meridiani. Afin d'expliquer la chimie de ces dépôts, ainsi que la formation d'un tel volume de sédiments de même composition, sur des surfaces aussi larges et variées, l'une des hypothèses les ... |
author2 |
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) Université de Nantes Olivier Bourgeois |
format |
Doctoral or Postdoctoral Thesis |
author |
Massé, Marion |
author_facet |
Massé, Marion |
author_sort |
Massé, Marion |
title |
Nature and origin of sulfate deposits in equatorial and polar regions of Mars. Morphological and mineralogical comparison of Aram Chaos and the North Polar Cap. |
title_short |
Nature and origin of sulfate deposits in equatorial and polar regions of Mars. Morphological and mineralogical comparison of Aram Chaos and the North Polar Cap. |
title_full |
Nature and origin of sulfate deposits in equatorial and polar regions of Mars. Morphological and mineralogical comparison of Aram Chaos and the North Polar Cap. |
title_fullStr |
Nature and origin of sulfate deposits in equatorial and polar regions of Mars. Morphological and mineralogical comparison of Aram Chaos and the North Polar Cap. |
title_full_unstemmed |
Nature and origin of sulfate deposits in equatorial and polar regions of Mars. Morphological and mineralogical comparison of Aram Chaos and the North Polar Cap. |
title_sort |
nature and origin of sulfate deposits in equatorial and polar regions of mars. morphological and mineralogical comparison of aram chaos and the north polar cap. |
publisher |
HAL CCSD |
publishDate |
2010 |
url |
https://tel.archives-ouvertes.fr/tel-00762257 https://tel.archives-ouvertes.fr/tel-00762257/document https://tel.archives-ouvertes.fr/tel-00762257/file/these_Masse.pdf |
long_lat |
ENVELOPE(-58.783,-58.783,-62.167,-62.167) |
geographic |
Valles |
geographic_facet |
Valles |
genre |
Antarc* Antarctica Ice cap |
genre_facet |
Antarc* Antarctica Ice cap |
op_source |
https://tel.archives-ouvertes.fr/tel-00762257 Planétologie. Université de Nantes, 2010. Français |
op_relation |
tel-00762257 https://tel.archives-ouvertes.fr/tel-00762257 https://tel.archives-ouvertes.fr/tel-00762257/document https://tel.archives-ouvertes.fr/tel-00762257/file/these_Masse.pdf |
op_rights |
info:eu-repo/semantics/OpenAccess |
_version_ |
1766274958960361472 |