Volatiles and Refractories in Surface-Bounded Exospheres in the Inner Solar System.
Exosphere
Ions
Magnetosphere
Mercury
Moon
Neutrals
Refractories
Solar wind
Volatiles
Journal
Space science reviews
ISSN: 0038-6308
Titre abrégé: Space Sci Rev
Pays: Netherlands
ID NLM: 100971458
Informations de publication
Date de publication:
2021
2021
Historique:
received:
22
12
2020
accepted:
21
05
2021
entrez:
1
11
2021
pubmed:
2
11
2021
medline:
2
11
2021
Statut:
ppublish
Résumé
Volatiles and refractories represent the two end-members in the volatility range of species in any surface-bounded exosphere. Volatiles include elements that do not interact strongly with the surface, such as neon (detected on the Moon) and helium (detected both on the Moon and at Mercury), but also argon, a noble gas (detected on the Moon) that surprisingly adsorbs at the cold lunar nighttime surface. Refractories include species such as calcium, magnesium, iron, and aluminum, all of which have very strong bonds with the lunar surface and thus need energetic processes to be ejected into the exosphere. Here we focus on the properties of species that have been detected in the exospheres of inner Solar System bodies, specifically the Moon and Mercury, and how they provide important information to understand source and loss processes of these exospheres, as well as their dependence on variations in external drivers.
Identifiants
pubmed: 34720217
doi: 10.1007/s11214-021-00833-8
pii: 833
pmc: PMC8550778
doi:
Types de publication
Journal Article
Review
Langues
eng
Pagination
61Informations de copyright
© The Author(s) 2021.
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