Ground-based spectroscopy of Ganymede’s surface has revealed the surprising presence of dense-phase molecular oxygen (O2) via weak absorptions at visible wavelengths. To date, the state and stability of this O2 […]
Ganymede
Evidence For A Sublimated Water Atmosphere On Ganymede From Hubble Space Telescope Observations
Ganymede’s atmosphere is produced by charged particle sputtering and sublimation of its icy surface. Previous far-ultraviolet observations of the OI1356-A and OI1304-A oxygen emissions were used to derive sputtered molecular […]
Jupiter's Moons Could Be Warming Each Other
Jupiter’s moons are hot. Well, hotter than they should be, for being so far from the Sun. In a process called tidal heating, gravitational tugs from Jupiter’s moons and the […]
Powering the Galilean Satellites with Moon-Moon Tides
There is compelling evidence for subsurface water oceans among the three outer Galilean satellites, and evidence for an internal magma ocean in the innermost moon, Io. Tidal forces from Jupiter […]
On the Orbital Variability of Ganymede's Atmosphere
Ganymede’s atmosphere is produced by radiative interactions with its surface, sourced by the Sun and the Jovian plasma. The sputtered and thermally desorbed molecules are tracked in our Exospheric Global […]
NASA To Discuss Hubble Observations of Ganymede
NASA will host a teleconference at 11 a.m. EDT on Thursday, March 12, to discuss Hubble Space Telescope’s observations of Ganymede, Jupiter’s largest moon. These results will help scientists in […]
