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

被引：15

作者：

Grava, Cesare ^{[1
]}

Killen, Rosemary M. ^{[2
]}

Benna, Mehdi ^{[2
,3
]}

Berezhnoy, Alexey A. ^{[4
,5
]}

Halekas, Jasper S. ^{[6
]}

Leblanc, Francois ^{[7
]}

Nishino, Masaki N. ^{[8
]}

Plainaki, Christina ^{[9
]}

Raines, Jim M. ^{[10
]}

Sarantos, Menelaos ^{[2
]}

Teolis, Benjamin D. ^{[1
]}

Tucker, Orenthal J. ^{[2
]}

Vervack, Ronald J. ^{[11
]}

Vorburger, Audrey ^{[12
]}

机构：

[1] Southwest Res Inst, San Antonio, TX USA

[2] NASA, Goddard Space Flight Ctr, Greenbelt, MD USA

[3] Univ Maryland Baltimore Cty, Baltimore, MD 21228 USA

[4] Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow, Russia

[5] Kazan Fed Univ, Inst Phys, Kazan, Russia

[6] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA

[7] Sorbonne Univ, UVSQ, CNRS, LATMOS,IPSL, Paris, France

[8] Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Sagamihara, Kanagawa, Japan

[9] Italian Space Agcy, Rome, Italy

[10] Univ Michigan, Dept Climate & Space Sci & Engn, Ann Arbor, MI 48109 USA

[11] Johns Hopkins Appl Phys Lab, Laurel, MD USA

[12] Univ Bern, Phys Inst, Bern, Switzerland

来源：

SPACE SCIENCE REVIEWS | 2021年 / 217卷 / 05期

关键词：

Moon; Mercury; Exosphere; Refractories; Volatiles; Solar wind; Magnetosphere; Neutrals; Ions; MERCURYS DAYSIDE MAGNETOSPHERE; SUNLIT LUNAR EXOSPHERE; MESSENGER OBSERVATIONS; SPATIAL-DISTRIBUTION; WATER-VAPOR; SEASONAL-VARIATIONS; MOLECULAR-HYDROGEN; SPACE ENVIRONMENT; METEOROID STREAM; UPPER LIMIT;

D O I：

10.1007/s11214-021-00833-8

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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.

引用

页数：47

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