Results 101 to 110 of about 3,808 (204)
Crater Morphometry on Callisto
Impact crater formation is affected by the physical properties of planetary crusts, allowing comparison of crater dimensions to serve as a proxy for comparing the crustal properties of different planetary bodies.
V. J. Bray, P. M. Schenk
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Viability of the Early JUICE Flyby Trajectories to Confirm Ocean Existence at Ganymede
Ganymede is the largest moon in our solar system, and unique in producing its own magnetic field, as well as possibly possessing a subsurface ocean. The data analysis from the Galileo spacecraft provided two models for the internal field—a dipole and ...
Shivangi Sharan +4 more
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Absorption Coefficients of Condensed O2: Application to Ganymede
Two absorption features in the visible reflectance spectra of the icy Galilean satellites are associated with dense phase molecular oxygen (O _2 ). These were identified from ground-based and Hubble Space Telescope data on Ganymede, Europa, and Callisto.
Wendy M. Calvin
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On the identification of hyperhydrated sodium chloride hydrates, stable at icy moon conditions. [PDF]
Journaux B +14 more
europepmc +1 more source
Salty ice and the dilemma of ocean exoplanet habitability. [PDF]
Journaux B.
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In situ and remote observations of the ultraviolet footprint of the moon Callisto by the Juno spacecraft. [PDF]
Rabia J +25 more
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Thermodynamic Constraints on the Citric Acid Cycle and Related Reactions in Ocean World Interiors. [PDF]
Işık S +4 more
europepmc +1 more source
Titan's strong tidal dissipation precludes a subsurface ocean. [PDF]
Petricca F +15 more
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Unraveling the complex inventory of biorelevant organics in the plumes of icy moons. [PDF]
Kaiser RI.
europepmc +1 more source

