Stormy water on Mars: The distribution and saturation of atmospheric water during the dusty season
The loss of water from Mars to space is thought to result from the transport of water to the upper atmosphere, where it is dissociated to hydrogen and escapes the planet. Recent observations have suggested large, rapid seasonal intrusions of water into the upper atmosphere, boosting the hydrogen abu...
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| Veröffentlicht in: | Science (American Association for the Advancement of Science) 2020-01, Vol.367 (6475), p.297-300 |
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| creator | Fedorova, Anna A Montmessin, Franck Korablev, Oleg Luginin, Mikhail Trokhimovskiy, Alexander Belyaev, Denis A Ignatiev, Nikolay I Lefèvre, Franck Alday, Juan Irwin, Patrick G J Olsen, Kevin S Bertaux, Jean-Loup Millour, Ehouarn Määttänen, Anni Shakun, Alexey Grigoriev, Alexey V Patrakeev, Andrey Korsa, Svyatoslav Kokonkov, Nikita Baggio, Lucio Forget, Francois Wilson, Colin F |
| description | The loss of water from Mars to space is thought to result from the transport of water to the upper atmosphere, where it is dissociated to hydrogen and escapes the planet. Recent observations have suggested large, rapid seasonal intrusions of water into the upper atmosphere, boosting the hydrogen abundance. We use the Atmospheric Chemistry Suite on the ExoMars Trace Gas Orbiter to characterize the water distribution by altitude. Water profiles during the 2018-2019 southern spring and summer stormy seasons show that high-altitude water is preferentially supplied close to perihelion, and supersaturation occurs even when clouds are present. This implies that the potential for water to escape from Mars is higher than previously thought. |
| doi_str_mv | 10.1126/science.aay9522 |
| format | Article |
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Recent observations have suggested large, rapid seasonal intrusions of water into the upper atmosphere, boosting the hydrogen abundance. We use the Atmospheric Chemistry Suite on the ExoMars Trace Gas Orbiter to characterize the water distribution by altitude. Water profiles during the 2018-2019 southern spring and summer stormy seasons show that high-altitude water is preferentially supplied close to perihelion, and supersaturation occurs even when clouds are present. 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Recent observations have suggested large, rapid seasonal intrusions of water into the upper atmosphere, boosting the hydrogen abundance. We use the Atmospheric Chemistry Suite on the ExoMars Trace Gas Orbiter to characterize the water distribution by altitude. Water profiles during the 2018-2019 southern spring and summer stormy seasons show that high-altitude water is preferentially supplied close to perihelion, and supersaturation occurs even when clouds are present. 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| fulltext | fulltext |
| identifier | ISSN: 0036-8075 |
| ispartof | Science (American Association for the Advancement of Science), 2020-01, Vol.367 (6475), p.297-300 |
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| language | eng |
| recordid | cdi_hal_primary_oai_HAL_insu_02440376v1 |
| source | American Association for the Advancement of Science |
| subjects | Altitude Atmosphere Atmospheric chemistry Atmospheric water Dust storms High altitude High-altitude environments Mars Mars atmosphere Mars dust Mars surface Organic chemistry Perihelions Sciences of the Universe Spacecraft Storms Supersaturation Trace gases Upper atmosphere Water Water distribution Water engineering Water vapor |
| title | Stormy water on Mars: The distribution and saturation of atmospheric water during the dusty season |
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