Degassing of volatiles in the geological history of Mars

I obtain an estimate of the total mass of degassed volatiles on Mars and the distribution of degassing in time. The amount of volatiles degassed in all the history of Mars is of the order of 3.73x1020 kg, i.e. 16 000 times the current Martian atmosphere. The bulk of the degassing occurred in Early,...

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Main Author: Héctor Javier Durand-Manterola
Format: Article
Language:English
Published: Universidad Nacional Autónoma de México, Instituto de Geofísica 2003-06-01
Series:Geofísica Internacional
Subjects:
Online Access:http://www.geofisica.unam.mx/unid_apoyo/editorial/publicaciones/investigacion/geofisica_internacional/anteriores/2003/01/durand.pdf
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author Héctor Javier Durand-Manterola
author_facet Héctor Javier Durand-Manterola
author_sort Héctor Javier Durand-Manterola
collection DOAJ
description I obtain an estimate of the total mass of degassed volatiles on Mars and the distribution of degassing in time. The amount of volatiles degassed in all the history of Mars is of the order of 3.73x1020 kg, i.e. 16 000 times the current Martian atmosphere. The bulk of the degassing occurred in Early, Middle, and Late Noachian, and in Early Hesperian. Degassing was monotonically decreasing in the last five epochs, from Early Hesperian to Late Amazonian. The amount of liquid water at the surface in the past was very little or none, thus the existence of life is doubtful.
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spelling doaj.art-789a3a5c84e74306b51f26b1c67ed23f2023-09-02T13:30:14ZengUniversidad Nacional Autónoma de México, Instituto de GeofísicaGeofísica Internacional0016-71692003-06-01421157162Degassing of volatiles in the geological history of MarsHéctor Javier Durand-ManterolaI obtain an estimate of the total mass of degassed volatiles on Mars and the distribution of degassing in time. The amount of volatiles degassed in all the history of Mars is of the order of 3.73x1020 kg, i.e. 16 000 times the current Martian atmosphere. The bulk of the degassing occurred in Early, Middle, and Late Noachian, and in Early Hesperian. Degassing was monotonically decreasing in the last five epochs, from Early Hesperian to Late Amazonian. The amount of liquid water at the surface in the past was very little or none, thus the existence of life is doubtful.http://www.geofisica.unam.mx/unid_apoyo/editorial/publicaciones/investigacion/geofisica_internacional/anteriores/2003/01/durand.pdfMars atmospheredegassingvolcanism
spellingShingle Héctor Javier Durand-Manterola
Degassing of volatiles in the geological history of Mars
Geofísica Internacional
Mars atmosphere
degassing
volcanism
title Degassing of volatiles in the geological history of Mars
title_full Degassing of volatiles in the geological history of Mars
title_fullStr Degassing of volatiles in the geological history of Mars
title_full_unstemmed Degassing of volatiles in the geological history of Mars
title_short Degassing of volatiles in the geological history of Mars
title_sort degassing of volatiles in the geological history of mars
topic Mars atmosphere
degassing
volcanism
url http://www.geofisica.unam.mx/unid_apoyo/editorial/publicaciones/investigacion/geofisica_internacional/anteriores/2003/01/durand.pdf
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