Methane Clathrates in the Solar System
International audience We review the reservoirs of methane clathrates that may exist in the different bodies of the Solar System. Methane was formed in the interstellar medium prior to having been embedded in the protosolar nebula gas phase. This molecule was subsequently trapped in clathrates that...
Published in: | Astrobiology |
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Main Authors: | , , , , , , , , , , |
Other Authors: | , , , , , , , , , , , , , , , , , , |
Format: | Article in Journal/Newspaper |
Language: | English |
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HAL CCSD
2015
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Online Access: | https://hal.science/hal-01153201 https://doi.org/10.1089/ast.2014.1189 |
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Institut national des sciences de l'Univers: HAL-INSU |
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English |
topic |
[SDU]Sciences of the Universe [physics] |
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[SDU]Sciences of the Universe [physics] Mousis, O. Chassefière, E. Holm, N.G. Bouquet, Alain Waite, J.H. Geppert, W. D. Picaud, S. Aikawa, Yuri Ali-Dib, M. Charlou, J.-L. Rousselot, Philippe Methane Clathrates in the Solar System |
topic_facet |
[SDU]Sciences of the Universe [physics] |
description |
International audience We review the reservoirs of methane clathrates that may exist in the different bodies of the Solar System. Methane was formed in the interstellar medium prior to having been embedded in the protosolar nebula gas phase. This molecule was subsequently trapped in clathrates that formed from crystalline water ice during the cooling of the disk and incorporated in this form into the building blocks of comets, icy bodies, and giant planets. Methane clathrates may play an important role in the evolution of planetary atmospheres. On Earth, the production of methane in clathrates is essentially biological, and these compounds are mostly found in permafrost regions or in the sediments of continental shelves. On Mars, methane would more likely derive from hydrothermal reactions with olivine-rich material. If they do exist, martian methane clathrates would be stable only at depth in the cryosphere and sporadically release some methane into the atmosphere via mechanisms that remain to be determined. In the case of Titan, most of its methane probably originates from the protosolar nebula, where it would have been trapped in the clathrates agglomerated by the satellite's building blocks. Methane clathrates are still believed to play an important role in the present state of Titan. Their presence is invoked in the satellite's subsurface as a means of replenishing its atmosphere with methane via outgassing episodes. The internal oceans of Enceladus and Europa also provide appropriate thermodynamic conditions that allow formation of methane clathrates. In turn, these clathrates might influence the composition of these liquid reservoirs. Finally, comets and Kuiper Belt Objects might have formed from the agglomeration of clathrates and pure ices in the nebula. The methane observed in comets would then result from the destabilization of clathrate layers in the nuclei concurrent with their approach to perihelion. Thermodynamic equilibrium calculations show that methane-rich clathrate layers may exist on Pluto ... |
author2 |
Laboratoire d'Astrophysique de Marseille (LAM) Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS) Univers, Transport, Interfaces, Nanostructures, Atmosphère et environnement, Molécules (UMR 6213) (UTINAM) Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Franche-Comté (UFC) Université Bourgogne Franche-Comté COMUE (UBFC)-Université Bourgogne Franche-Comté COMUE (UBFC) Géosciences Paris Sud (GEOPS) Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS) Department of Geological Sciences Stockholm Stockholm University Space Science and Engineering Division San Antonio Southwest Research Institute San Antonio (SwRI) The University of Texas at San Antonio (UTSA) Department of Physics Stockholm Stockholm University Astrobiology Centre Department of Earth and Planetary Sciences Kobe Kobe University Géosciences Marines (GM) Institut Français de Recherche pour l'Exploitation de la Mer (IFREMER) ANR-11-IDEX-0001,Amidex,INITIATIVE D'EXCELLENCE AIX MARSEILLE UNIVERSITE(2011) |
format |
Article in Journal/Newspaper |
author |
Mousis, O. Chassefière, E. Holm, N.G. Bouquet, Alain Waite, J.H. Geppert, W. D. Picaud, S. Aikawa, Yuri Ali-Dib, M. Charlou, J.-L. Rousselot, Philippe |
author_facet |
Mousis, O. Chassefière, E. Holm, N.G. Bouquet, Alain Waite, J.H. Geppert, W. D. Picaud, S. Aikawa, Yuri Ali-Dib, M. Charlou, J.-L. Rousselot, Philippe |
author_sort |
Mousis, O. |
title |
Methane Clathrates in the Solar System |
title_short |
Methane Clathrates in the Solar System |
title_full |
Methane Clathrates in the Solar System |
title_fullStr |
Methane Clathrates in the Solar System |
title_full_unstemmed |
Methane Clathrates in the Solar System |
title_sort |
methane clathrates in the solar system |
publisher |
HAL CCSD |
publishDate |
2015 |
url |
https://hal.science/hal-01153201 https://doi.org/10.1089/ast.2014.1189 |
genre |
Ice permafrost |
genre_facet |
Ice permafrost |
op_source |
ISSN: 1531-1074 Astrobiology https://hal.science/hal-01153201 Astrobiology, 2015, 15 (4), pp.308-326 (IF 2,512). ⟨10.1089/ast.2014.1189⟩ |
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info:eu-repo/semantics/altIdentifier/arxiv/1510.07693 info:eu-repo/semantics/altIdentifier/doi/10.1089/ast.2014.1189 hal-01153201 https://hal.science/hal-01153201 ARXIV: 1510.07693 doi:10.1089/ast.2014.1189 |
op_doi |
https://doi.org/10.1089/ast.2014.1189 |
container_title |
Astrobiology |
container_volume |
15 |
container_issue |
4 |
container_start_page |
308 |
op_container_end_page |
326 |
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1797584524153978880 |
spelling |
ftinsu:oai:HAL:hal-01153201v1 2024-04-28T08:23:54+00:00 Methane Clathrates in the Solar System Mousis, O. Chassefière, E. Holm, N.G. Bouquet, Alain Waite, J.H. Geppert, W. D. Picaud, S. Aikawa, Yuri Ali-Dib, M. Charlou, J.-L. Rousselot, Philippe Laboratoire d'Astrophysique de Marseille (LAM) Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS) Univers, Transport, Interfaces, Nanostructures, Atmosphère et environnement, Molécules (UMR 6213) (UTINAM) Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Franche-Comté (UFC) Université Bourgogne Franche-Comté COMUE (UBFC)-Université Bourgogne Franche-Comté COMUE (UBFC) Géosciences Paris Sud (GEOPS) Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS) Department of Geological Sciences Stockholm Stockholm University Space Science and Engineering Division San Antonio Southwest Research Institute San Antonio (SwRI) The University of Texas at San Antonio (UTSA) Department of Physics Stockholm Stockholm University Astrobiology Centre Department of Earth and Planetary Sciences Kobe Kobe University Géosciences Marines (GM) Institut Français de Recherche pour l'Exploitation de la Mer (IFREMER) ANR-11-IDEX-0001,Amidex,INITIATIVE D'EXCELLENCE AIX MARSEILLE UNIVERSITE(2011) 2015 https://hal.science/hal-01153201 https://doi.org/10.1089/ast.2014.1189 en eng HAL CCSD Mary Ann Liebert info:eu-repo/semantics/altIdentifier/arxiv/1510.07693 info:eu-repo/semantics/altIdentifier/doi/10.1089/ast.2014.1189 hal-01153201 https://hal.science/hal-01153201 ARXIV: 1510.07693 doi:10.1089/ast.2014.1189 ISSN: 1531-1074 Astrobiology https://hal.science/hal-01153201 Astrobiology, 2015, 15 (4), pp.308-326 (IF 2,512). ⟨10.1089/ast.2014.1189⟩ [SDU]Sciences of the Universe [physics] info:eu-repo/semantics/article Journal articles 2015 ftinsu https://doi.org/10.1089/ast.2014.1189 2024-04-05T00:50:19Z International audience We review the reservoirs of methane clathrates that may exist in the different bodies of the Solar System. Methane was formed in the interstellar medium prior to having been embedded in the protosolar nebula gas phase. This molecule was subsequently trapped in clathrates that formed from crystalline water ice during the cooling of the disk and incorporated in this form into the building blocks of comets, icy bodies, and giant planets. Methane clathrates may play an important role in the evolution of planetary atmospheres. On Earth, the production of methane in clathrates is essentially biological, and these compounds are mostly found in permafrost regions or in the sediments of continental shelves. On Mars, methane would more likely derive from hydrothermal reactions with olivine-rich material. If they do exist, martian methane clathrates would be stable only at depth in the cryosphere and sporadically release some methane into the atmosphere via mechanisms that remain to be determined. In the case of Titan, most of its methane probably originates from the protosolar nebula, where it would have been trapped in the clathrates agglomerated by the satellite's building blocks. Methane clathrates are still believed to play an important role in the present state of Titan. Their presence is invoked in the satellite's subsurface as a means of replenishing its atmosphere with methane via outgassing episodes. The internal oceans of Enceladus and Europa also provide appropriate thermodynamic conditions that allow formation of methane clathrates. In turn, these clathrates might influence the composition of these liquid reservoirs. Finally, comets and Kuiper Belt Objects might have formed from the agglomeration of clathrates and pure ices in the nebula. The methane observed in comets would then result from the destabilization of clathrate layers in the nuclei concurrent with their approach to perihelion. Thermodynamic equilibrium calculations show that methane-rich clathrate layers may exist on Pluto ... Article in Journal/Newspaper Ice permafrost Institut national des sciences de l'Univers: HAL-INSU Astrobiology 15 4 308 326 |