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Stormy water on Mars: The distribution and saturation of atmospheric water during the dusty season
Author(s) -
Anna Fedorova,
Franck Montmessin,
Oleg Korablev,
Mikhail Luginin,
Аlexander Trokhimovskiy,
Denis Belyaev,
N. Ignatiev,
Franck Lefèvre,
Juan Alday,
P. G. J. Irwin,
Kevin Olsen,
JeanLoup Bertaux,
Ehouarn Millour,
Anni Määttänen,
Alexey Shakun,
Аlexey Grigoriev,
Andrey Patrakeev,
Svyatoslav Korsa,
Nikita Kokonkov,
Lucio Baggio,
F. Forget,
Colin Wilson
Publication year - 2020
Publication title -
science
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 12.556
H-Index - 1186
eISSN - 1095-9203
pISSN - 0036-8075
DOI - 10.1126/science.aay9522
Subject(s) - mars exploration program , environmental science , saturation (graph theory) , atmospheric sciences , astrobiology , geology , physics , mathematics , combinatorics
Water reaches Mars' upper atmosphere Mars once hosted abundant water on its surface but subsequently lost most of it to space. Small amounts of water vapor are still present in the atmosphere, which can escape if they reach sufficiently high altitudes. Fedorovaet al. used data from the ExoMars Trace Gas Orbiter spacecraft to determine the distribution of water in Mars' atmosphere and investigate how it varies over seasons. Water vapor is sometimes heavily saturated, and its distribution is affected by the planet's large dust storms. Water can efficiently reach the upper atmosphere when Mars is in the warmest part of its orbit, and this behavior may have controlled the overall rate at which Mars lost its water.Science , this issue p.297

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