Europa’s ice-related atmosphere: The sputter contribution

Vorburger, Audrey Helena; Wurz, Peter (2018). Europa’s ice-related atmosphere: The sputter contribution. Icarus, 311, pp. 135-145. Elsevier 10.1016/j.icarus.2018.03.022

Text 1-s2.0-S0019103517305377-main.pdf - Published Version Restricted to registered users only Available under License Publisher holds Copyright. Download (830kB)

Europa, Jupiter’s innermost icy satellite, is embedded well within Jupiter’s magnetospheric plasma, an intense flux of ions and electrons that approximately corotate with Jupiter. The plasma can be thought of as consisting of two populations: The cold, thermal plasma containing charged particles with energies ranging from 1 eV to 1 keV, and the hot, energetic plasma containing charged particles with energies ranging from 10 keV to 10 0 MeV. When the charged particles interact with Europa’s surface, they not only chemically and physically alter the icy surface, but also liberate material from the surface through a process called sputtering, which in turn forms a tenuous atmosphere.
In this paper we calculate the sputter contribution to the atmosphere by modeling the formation of Europa’s ice-sputtered atmosphere ab initio. We consider the species H, H 2, O, OH, H 2 O, O 2 , HO 2 , H 2 O 2 , and O 3 , all of which are related to the water–ice surface. Whereas the ice sputter yields of H2O, H2, and O2 have been well established, the ice sputter yields (and the resulting density profiles) of H, O, OH, HO 2 and O 3 are small and largely unknown. As model input we use available plasma ion and electron energy spectra as well as available water-ice sputter yields. Based on first principles, i.e., without applying any scaling to observed data, we calculate atmospheric densities ab initio.
Our results match available observational data and previously published modeling efforts well. Europa’s exosphere is dominated by thermally accommodated O 2 close to the surface (below a few 100 km), and the much lighter H 2 molecules at higher altitudes. The water-ice related species that stick to the surface (freeze out) are liberated by cold and hot plasma sputtering in about equal amounts. In addition, in the case of H 2 , O 2 , and H
2 O 2, electrons contribute almost as significantly to the sputter yield as ions do.

Interest & Impact

Downloads

4 since deposited on 03 May 2018
0 in the past 12 months

Citations

5 Citations in Web of Science ®
6 Citations in Scopus

Search

in Google Scholar™

Services

Actions (login required)

Edit item

Actions (login required)

Edit item