1. Volatiles and Refractories in Surface-Bounded Exospheres in the Inner Solar System
- Author
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Alexey A. Berezhnoy, Rosemary M. Killen, Jasper Halekas, B. D. Teolis, Cesare Grava, Masaki N. Nishino, Jim M. Raines, Mehdi Benna, Christina Plainaki, Audrey Vorburger, François Leblanc, Ronald J. Vervack, Menelaos Sarantos, Orenthal J. Tucker, Southwest Research Institute [San Antonio] (SwRI), NASA Goddard Space Flight Center (GSFC), University of Maryland [Baltimore], Sternberg Astronomical Institute [Moscow], Lomonosov Moscow State University (MSU), Institute of Physics [Kazan] (IoP), Kazan Federal University (KFU), Department of Physics and Astronomy [Iowa City], University of Iowa [Iowa City], HELIOS - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency [Sagamihara] (JAXA), Italian Space Agency, Department of Climate and Space Sciences and Engineering (CLaSP), University of Michigan [Ann Arbor], University of Michigan System-University of Michigan System, Johns Hopkins University Applied Physics Laboratory [Laurel, MD] (APL), Physikalisches Institut [Bern], Universität Bern [Bern], and Open Access funding provided by Universität Bern. Grava was supported by LRO, funded by NASA through contract NNG05EC87C. Berezhnoy was supported by RFBR grant No. 18-03-00726. Halekas was supported by SSERVI and NASA grant 80NSSC20K0311. Raines was supported by the NASA Discovery Data Analysis Program, grants NNX15AL01G and 80NSSC19K0204. Vervack was supported by NASA grant 80NSSC18K0857 (subcontract to JH-APL).
- Subjects
Volatiles ,Solar System ,Materials science ,010504 meteorology & atmospheric sciences ,Solar wind ,chemistry.chemical_element ,01 natural sciences ,Article ,Astrobiology ,Physics::Geophysics ,Neon ,Neutrals ,0103 physical sciences ,Physics::Atomic and Molecular Clusters ,Moon ,010303 astronomy & astrophysics ,Helium ,0105 earth and related environmental sciences ,Ions ,Argon ,[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] ,Refractories ,Noble gas ,Astronomy and Astrophysics ,Mercury ,Planetary science ,chemistry ,13. Climate action ,Space and Planetary Science ,Magnetosphere ,Physics::Space Physics ,Astrophysics::Earth and Planetary Astrophysics ,Exosphere - 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.
- Published
- 2021
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