A sublimated water atmosphere on Ganymede detected from Hubble Space Telescope observations
Lorenz Roth, Nickolay Ivchenko, G. Randall Gladstone, Joachim Saur,, Denis Grodent, Bertrand Bonfond, Philippa M. Molyneux, Kurt D. Retherford

TL;DR
Hubble Space Telescope observations reveal that Ganymede's atmosphere contains sublimated water vapor, with its abundance and distribution influenced by surface temperature and sublimation processes, indicating a significant water component beyond previously detected oxygen.
Contribution
This study provides the first high-sensitivity detection of water vapor in Ganymede's atmosphere, demonstrating sublimation as a key source and revealing spatial variations in atmospheric composition.
Findings
H$_2$O is more abundant than O$_2$ near the sub-solar point.
Water vapor is concentrated above the warmer trailing hemisphere.
Estimated H$_2$O column density is approximately 10$^{15}$ molecules per cm$^2$.
Abstract
Ganymede's atmosphere is produced by charged particle sputtering and sublimation of its icy surface. Previous far-ultraviolet observations of the O{\small I\,}1356-{\AA} and O{\small I\,}1304-{\AA} oxygen emissions were used to infer sputtered molecular oxygen (O) as an atmospheric constituent, but an expected sublimated water (HO) component remained undetected. Here we present an analysis of high-sensitivity spectra and spectral images acquired by the Hubble Space Telescope revealing HO in Ganymede's atmosphere. The relative intensity of the oxygen emissions requires contributions from dissociative excitation of water vapor, indicating that HO is more abundant than O around the sub-solar point. Away from the sub-solar region, the emissions are consistent with a pure O atmosphere. Eclipse observations constrain atomic oxygen to be at least two orders of magnitude…
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