Results 31 to 40 of about 554 (200)
Formation of Water-rich Giant Planet Satellites at Decretion Disk Ice Lines
The volatile budgets of giant planet satellites are critical to unraveling the origin of their building blocks within the circumplanetary disks that hosted them.
Teng Ee Yap, David J. Stevenson
doaj +1 more source
Exploring Enceladus's Interior Structure Using Electromagnetic Induction
Abstract Electromagnetic (EM) sounding can constrain the electrical structure of Enceladus and, in turn, the salinity of its ocean and the porosity, fluid content, and thermal state of its hydrothermally active core. Here, we assess the feasibility of EM sounding at Enceladus using both global (orbiter) and local (lander) EM induction transfer ...
Alexander Grayver, Joachim Saur
wiley +1 more source
Four, and possibly as many as six, new satellites of Saturn have been found as a result of data from the Voyager 2 encounter with the planet in August 1981. The discoveries bring the number of Saturnian satellites to between 21 and 23. The two ‘possible’ satellites were seen in only one observation each, so their orbits are not yet confirmed.The ...
openaire +1 more source
The PHESAT95 catalogue of observations of the mutual events of the Saturnian satellites [PDF]
In 1994-1996 the Sun and the Earth passed through the equatorial plane of Saturn and therefore through the orbital planes of its main satellites. During this period, phenomena involving seven of these satellites were observed. Light curves of eclipses by Saturn and of mutual eclipses and occultations were recorded by the observers of the international ...
Thuillot, W. +29 more
openaire +3 more sources
The Potential for Organic Synthesis in the Ocean of Enceladus
The Cassini spacecraft detected a soup of organics in the plume of Saturn’s moon Enceladus. Those compounds could provide building blocks for the potential emergence or sustenance of microbial life in Enceladus’ subsurface ocean. However, the sources and
Can Liu +8 more
doaj +1 more source
Shallow Impact Craters Suggest Titan Stores Methane in an Insulating Clathrate Crust
Abstract Multiple lines of evidence suggest that a methane‐clathrate crustal layer exists in Titan. However, we have not directly confirmed the existence or thickness of this hypothesized layer, a potentially important methane reservoir. Here, we model impact crater formation and subsequent viscoelastic evolution in Titan's ice shell with methane ...
L. R. Schurmeier +7 more
wiley +1 more source
A JWST Study of CO2 on the Satellites of Saturn
Solid state CO _2 has been detected throughout the outer solar system, even at temperatures where crystalline CO _2 is unstable, requiring that the CO _2 be trapped in a separate host material. The Saturnian satellites provide an ideal laboratory for the
Michael E. Brown +4 more
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Abstract Saturn's magnetosphere is continuously supplied with neutrals from the Enceladus plume and the icy rings, which undergo ionization and charge‐exchange to form a complex water‐group plasma environment. While the Cassini Plasma Spectrometer (CAPS) instrument has provided extensive compositional information, detailed separation of individual ...
Thomas K. Kim +13 more
wiley +1 more source
Enough Sulfur and Iron for Potential Life Make Enceladus’s Ocean Fully Habitable
The Cassini spacecraft revealed life-forming elements like CHNOP and diverse organic compounds from Enceladus’s ocean. However, the availability of minor but bio-essential nutrients such as iron and sulfur remains unknown.
Weiming Xu +7 more
doaj +1 more source
Modeling Ganymede's Surface Charging in Preparation for the JUICE Mission
Abstract The European Space Agency's (ESA) JUICE mission (JUpiter ICy moons Explorer) is en route to the Jovian system to characterize Ganymede's subsurface ocean. Determining the ocean's conductivity and depth requires precise measurements of its induced magnetic field at the position of JUICE.
Betty Pei‐Chun Tsai +10 more
wiley +1 more source

