Results 31 to 40 of about 7,875 (212)
A LIBRATION MODEL FOR ENCELADUS BASED ON GEODETIC CONTROL POINT NETWORK ANALYSIS [PDF]
A new global control point network was derived for Enceladus, based on Cassini and Voyager-2 image data. Cassini images were taken from 2005 to 2014, for Voyager we have only one flyby in the middle of 1981.
I. E. Nadezhdina +3 more
doaj +1 more source
The Role of Ejecta in the Small Crater Populations on the Mid-Sized Saturnian Satellites
We find evidence that crater ejecta play an important role in the small crater populations on the Saturnian satellites, and more broadly, on cratered surfaces throughout the Solar System. We measure crater populations in Cassini images of Enceladus, Rhea,
Alvarellos +61 more
core +1 more source
Possibility for albedo estimation of exomoons: Why should we care about M dwarfs? [PDF]
Occultation light curves of exomoons may give information on their albedo and hence indicate the presence of ice cover on the surface. Icy moons might have subsurface oceans thus these may potentially be habitable.
Dobos, Vera +3 more
core +2 more sources
Enceladus, one of Saturn’s moons, is considered one of the most promising places in the solar system to find life. The Cassini mission discovered organic-rich water plumes from Enceladus’s subsurface ocean, prompting new lander mission planning.
M. F. L. Meersman +2 more
doaj +1 more source
Returning Samples From Enceladus for Life Detection
Evidence suggests that Saturn's icy moon Enceladus has a subsurface ocean that sources plumes of water vapor and ice vented to space from its south pole.
Marc Neveu +11 more
doaj +1 more source
THEO Concept Mission: Testing the Habitability of Enceladus's Ocean
Saturn's moon Enceladus offers a unique opportunity in the search for life and habitable environments beyond Earth, a key theme of the National Research Council's 2013-2022 Decadal Survey. A plume of water vapor and ice spews from Enceladus's south polar
Budney, Charles J. +19 more
core +1 more source
A primordial origin for the atmospheric methane of Saturn's moon Titan [PDF]
The origin of Titan's atmospheric methane is a key issue for understanding the origin of the Saturnian satellite system. It has been proposed that serpentinization reactions in Titan's interior could lead to the formation of the observed methane ...
Alibert +41 more
core +4 more sources
Local Time Asymmetry in Energetic Electron Distribution Within Saturn's Inner Magnetosphere
Abstract Electrons of several hundred keV in Saturn's ring current are important seed components of the radiation belt. In this study, we have statistically analyzed the spatial distribution of energetic electrons on the equatorial plane of the inner magnetosphere based on the Cassini in situ observations.
Yimeng Li +5 more
wiley +1 more source
Using Tidally‐Driven Elastic Strains to Infer Regional Variations in Crustal Thickness at Enceladus
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 +1 more source
In 1980, telescopes revealed that one of Saturn’s rings is centered at the orbit of Enceladus, a medium-sized Saturnian moon. It was the first hint that Enceladus is a world like no other.
openaire +1 more source

