Water Group Exospheres and Surface Interactions on the Moon, Mercury, and Ceres.
Title: | Water Group Exospheres and Surface Interactions on the Moon, Mercury, and Ceres. |
---|---|
Authors: | Schörghofer, Norbert, Benna, Mehdi, Berezhnoy, Alexey A., Greenhagen, Benjamin, Jones, Brant M., Li, Shuai, Orlando, Thomas M., Prem, Parvathy, Tucker, Orenthal J., Wöhler, Christian |
Source: | Space Science Reviews; Sep2021, Vol. 217 Issue 6, p1-35, 35p |
Subject Terms: | SURFACE interactions, CERES (Dwarf planet), METEOROIDS, SOLAR system, MERCURY (Planet), LUNAR exploration, LUNAR surface, ELECTRON traps |
Abstract: | Water ice, abundant in the outer solar system, is volatile in the inner solar system. On the largest airless bodies of the inner solar system (Mercury, the Moon, Ceres), water can be an exospheric species but also occurs in its condensed form. Mercury hosts water ice deposits in permanently shadowed regions near its poles that act as cold traps. Water ice is also present on the Moon, where these polar deposits are of great interest in the context of future lunar exploration. The lunar surface releases either OH or H |
Copyright of Space Science Reviews is the property of Springer Nature and its content may not be copied or emailed to multiple sites or posted to a listserv without the copyright holder's express written permission. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.) | |
Database: | Complementary Index |
Full text is not displayed to guests. | Login for full access. |
Be the first to leave a comment!