Vorburger, Audrey;
Pfleger, Martin;
Lindkvist, Jesper;
Holmström, Mats;
Lammer, Helmut;
Lichtenegger, Herbert I. M.;
Galli, André;
Rubin, Martin;
Wurz, Peter
Three‐Dimensional Modeling of Callisto's Surface Sputtered Exosphere Environment
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Media type:
E-Article
Title:
Three‐Dimensional Modeling of Callisto's Surface Sputtered Exosphere Environment
Contributor:
Vorburger, Audrey;
Pfleger, Martin;
Lindkvist, Jesper;
Holmström, Mats;
Lammer, Helmut;
Lichtenegger, Herbert I. M.;
Galli, André;
Rubin, Martin;
Wurz, Peter
imprint:
American Geophysical Union (AGU), 2019
Published in:Journal of Geophysical Research: Space Physics
Language:
English
DOI:
10.1029/2019ja026610
ISSN:
2169-9380;
2169-9402
Origination:
Footnote:
Description:
<jats:title>Abstract</jats:title><jats:p>We study the release of various elements from Callisto's surface into its exosphere by plasma sputtering. The cold Jovian plasma is simulated with a 3‐D plasma‐planetary interaction hybrid model, which produces 2‐D surface precipitation maps for magnetospheric H<jats:sup>+</jats:sup>, O<jats:sup>+</jats:sup>, O<jats:sup>++</jats:sup>, and S<jats:sup>++</jats:sup>. For the hot Jovian plasma, we assume isotropic precipitation onto the complete spherical surface. Two scenarios are investigated: one where no ionospheric shielding takes place and accordingly full plasma penetration is implemented (<jats:italic>no‐ionosphere</jats:italic> scenario) and one where an ionosphere lets virtually none of the cold plasma but all of the hot plasma reach Callisto's surface (<jats:italic>ionosphere</jats:italic> scenario). In the 3‐D exosphere model, neutral particles are sputtered from the surface and followed on their individual trajectories. The 3‐D density profiles show that whereas in the no‐ionosphere scenario the ram direction is favored, the ionosphere scenario produces almost uniform density profiles. In addition, the density profiles in the ionosphere scenario are reduced by a factor of ∼2.5 with respect to the no‐ionosphere scenario. We find that the Neutral Gas and Ion Mass Spectrometer, which is part of the Particle Environment Package on board the JUpiter ICy moons Explorer mission, will be able to detect the different sputter populations from Callisto's icy surface and the major sputter populations from Callisto's nonicy surface. The chemical composition of Callisto's exosphere can be directly linked to the chemical composition of its surface and will offer us information not only on Callisto's formation scenario but also on the building blocks of the Jupiter system.</jats:p>