ENCELADUS GEODETIC FRAMEWORK [PDF]
The small (approximately 500 km in diameter) satellite Enceladus is moving near the equatorial plane and deep in the gravity field of its parent planet Saturn.
J. Oberst +7 more
doaj +4 more sources
A Review on Hypothesized Metabolic Pathways on Europa and Enceladus: Space-Flight Detection Considerations [PDF]
Enceladus and Europa, icy moons of Saturn and Jupiter, respectively, are believed to be habitable with liquid water oceans and therefore are of interest for future life detection missions and mission concepts. With the limited data from missions to these
Jessica M. Weber +5 more
doaj +2 more sources
On the charge of nanograins in cold environments and Enceladus dust [PDF]
In very-low energy plasmas, the size of nanograins is comparable to the distance (the so-called Landau length) at which the interaction energy of two electrons equals their thermal energy.
N. Meyer‐Vernet
openalex +4 more sources
Using Tidally‐Driven Elastic Strains to Infer Regional Variations in Crustal Thickness at Enceladus [PDF]
Constraining the spatial variability of the thickness of the ice shell of Enceladus (i.e., the crust) is central to our understanding of the internal dynamics and evolution of this small Saturnian moon.
Alexander Berne +3 more
doaj +2 more sources
The Carbonate Geochemistry of Enceladus' Ocean
The plume composition at Enceladus contains clues about conditions and processes in the interior. We present new geochemical interpretations of Cassini mass spectrometry data from the plume gas and salt‐rich ice grains.
Christopher Glein, J Hunter Waite, Jr
exaly +2 more sources
Biological methane production under putative Enceladus-like conditions
Many methanogenic archaea use H2 and CO2 to produce methane. Here, Taubner et al. show that Methanothermococcus okinawensis produces methane under conditions extrapolated for Saturn’s icy moon, Enceladus, and estimate that serpentinization may produce ...
Ruth-Sophie Taubner +2 more
exaly +2 more sources
Enceladus's internal ocean and ice shell constrained from Cassini gravity, shape, and libration data
The intense plume activity at the South Pole of Enceladus together with the recent detection of libration hints at an internal water ocean underneath the outer ice shell.
Ondřej P Čadek +2 more
exaly +2 more sources
Variations in plume activity reveal the dynamics of water-filled faults on Enceladus [PDF]
After discovering a jet activity near the south pole of Saturn’s moon Enceladus, the Cassini mission demonstrated the existence of a subsurface water ocean with a unique sampling opportunity through flybys.
Ondřej Souček +4 more
doaj +2 more sources
A multi-lander New Frontiers mission concept study for Enceladus: SILENUS
Enceladus, with its subsurface ocean, is amongst the top priority targets in the search for life beyond Earth. Following on discoveries from the Cassini mission that Enceladus possesses a global subsurface ocean containing salt and organic compounds ...
Erica Nathan +11 more
doaj +1 more source
The ETNA mission concept: Assessing the habitability of an active ocean world
Enceladus is an icy world with potentially habitable conditions, as suggested by the coincident presence of a subsurface ocean, an active energy source due to water-rock interactions, and the basic chemical ingredients necessary for terrestrial life ...
Ariel N. Deutsch +16 more
doaj +1 more source

