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Volatiles and Refractories in Surface-Bounded Exospheres in the Inner Solar System
Journal article   Open access   Peer reviewed

Volatiles and Refractories in Surface-Bounded Exospheres in the Inner Solar System

Cesare Grava, Rosemary M. Killen, Mehdi Benna, Alexey A. Berezhnoy, Jasper S. Halekas, François Leblanc, Masaki N. Nishino, Christina Plainaki, Jim M. Raines, Menelaos Sarantos, …
Space science reviews, Vol.217(5), pp.61-61
08/01/2021
DOI: 10.1007/s11214-021-00833-8
PMCID: PMC8550778
PMID: 34720217
url
https://doi.org/10.1007/s11214-021-00833-8View
Published (Version of record) Open Access

Abstract

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.
Exobiology Space Sciences (General)

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