On the identification of hyperhydrated sodium chloride hydrates, stable at icy moon conditions. [PDF]
Significance The finding of sodium chloride hydrate phases allows an update to the phase diagram of the canonical H2O–NaCl binary system in over 150 y.
Journaux B +14 more
europepmc +4 more sources
New Signatures of Bio-Molecular Complexity in the Hypervelocity Impact Ejecta of Icy Moon Analogues [PDF]
Impact delivery of prebiotic compounds to the early Earth from an impacting comet is considered to be one of the possible ways by which prebiotic molecules arrived on the Earth.
Surendra V. Singh +11 more
doaj +3 more sources
Saturn's Icy Moon Rhea: a Prediction for Bulk Chemical Composition and Physical Structure at the Time of the Cassini Spacecraft First Flyby [PDF]
I report a model for the formation of Saturn's family of mid-sized icy moons to coincide with the first flypast of Rhea by the Cassini Orbiter spacecraft on 26 November 2005.
Andrew J. R. Prentice +18 more
core +4 more sources
Growth, physiology, and metabolism of Halomonas meridiana in aqueous ammonium sulfate with implications for icy moon astrobiology [PDF]
The discovery of extraterrestrial reservoirs of liquid water has motivated missions to icy moons Europa and Titan. Tentative evidence of ammonium sulfate ((NH4)2SO4) has been detected on the surface of Europa, and (NH4)2SO4 could be a prominent ...
Cassie M. Hopton +2 more
doaj +3 more sources
Icy Moon Penetrator Organic Analyzer Post-Impact Component Analysis
Europa is an established high-priority astrobiology target where identifying chemical signatures of life is one of NASA’s highest-priority goals. Remote sensing techniques are powerful tools for extraterrestrial exploration, but in situ data through ...
Chinmayee Govinda Raj +8 more
doaj +2 more sources
Nonsynchronous rotation of icy moon ice shells: The thermal wind perspective. [PDF]
The ice shells of icy satellites have been hypothesized to undergo nonsynchronous rotation (NSR) under the influence of tidal torques and/or ocean currents.
Kang W.
europepmc +2 more sources
Several bodies in the outer solar system are believed to host liquid water oceans underneath their icy surfaces. Knowledge of the hydrosphere properties is essential for understanding and assessing their habitability.
Flavio Petricca +5 more
doaj +2 more sources
A Passive Probe for Subsurface Oceans and Liquid Water in Jupiter's Icy Moons [PDF]
We describe an interferometric reflectometer method for passive detection of subsurface oceans and liquid water in Jovian icy moons using Jupiter's decametric radio emission (DAM).
Heggy, Essam +5 more
core +2 more sources
Understanding tidal dissipation in gaseous giant planets from their core to their surface [PDF]
Tidal dissipation in planetary interiors is one of the key physical mechanisms that drive the evolution of star-planet and planet-moon systems. Tidal dissipation in planets is intrinsically related to their internal structure.
Guenel M., Mathis S., Remus F.
doaj +3 more sources
DNA Polymerization in Icy Moon Abyssal Pressure Conditions
Evidence of stable liquid water oceans beneath the ice crust of moons within the Solar System is of great interest for astrobiology. In particular, subglacial oceans may present hydrothermal processes in their abysses, similarly to terrestrial ...
Lorenzo Carré +5 more
semanticscholar +5 more sources

