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Callisto’s atmosphere: First evidence for H2, and the implications this has for Europa’s and Ganymede’s atmosphere

Authors :
Shane Carberry Mogan
Orenthal J. Tucker
Robert E. Johnson
Lorenz Roth
Juan Alday
Audrey Vorburger
Peter Wurz
Andre Galli
H. Todd Smith
Apurva V. Oza
Lucas Liuzzo
Andrew R. Poppe
Publication Year :
2023
Publisher :
Copernicus GmbH, 2023.

Abstract

We explore the parameter space for the contribution to Callisto's H corona observed by the Hubble Space Telescope from sublimated H2O and radiolytically produced H2 using the Direct Simulation Monte Carlo (DSMC) method. The spatial morphology of this corona produced via photo- and magnetospheric electron impact-induced dissociation is described by tracking the motion of and simulating collisions between the hot H atoms and thermal molecules including a near-surface O2 component. Our results presented indicate that sublimated H2O produced from the surface ice, whether assumed to be intimately mixed with or distinctly segregated from the dark non-ice or ice-poor regolith, cannot explain the observed structure of the H corona. On the other hand, a global H2 component can reproduce the observation, and is also capable of producing the enhanced electron densities observed at high altitudes by Galileo's plasma-wave instrument, providing the first evidence of H2 in Callisto's atmosphere. Finally, we discuss the implications of these results, in particular how they compare to Europa and Ganymede.

Details

Database :
OpenAIRE
Accession number :
edsair.doi...........f2ae7b1fc13a9b8be7d1f51ba1aa096f
Full Text :
https://doi.org/10.5194/egusphere-egu23-8541