Results 61 to 70 of about 130,149 (150)
Water masers in the Saturnian system
Context. The presence of water has long been seen as a key condition for life in planetary environments. The Cassini spacecraft discovered water vapour in the Saturnian system by detecting absorption of UV emission from a background star.
I. M. Avruch +13 more
core +1 more source
Voyager 1 and 2 Atlas of Six Saturnian Satellites [PDF]
Maps, compiled with data gathered primarily by Voyager 1 and 2 spacecraft, are presented which show the diversity among six of the Saturnian moons. Mimas and Enceladus are mapped in detail. Prelimary maps are given for the other four satellites. Diameter,
Batson, R. M.
core
Feeling the Pressure: Effects of Formation Pressure on the Physical Properties of Titan Haze Analogs
The Cassini–Huygens mission detected large negative ions in Titan’s ionosphere at pressures as low as 10 ^−6 Torr. These ions ultimately polymerize to form Titan’s complex organic haze particles, which are observed throughout the atmosphere and ...
Adis Husić +5 more
doaj +1 more source
Investigating Tidal Stripping of a Preexisting Moon as the Origin of Saturn’s Young Icy Rings
The origin of Saturn’s rings has been debated for decades. Measurements from Voyager and Cassini have suggested that the rings could be as young as ∼100 Myr and composed of nearly pure ice. Several scenarios have been proposed to explain these properties.
Yifei Jiao +3 more
doaj +1 more source
Micrometeoroid infall onto Saturn's rings constrains their age to no more than a few hundred million years. [PDF]
Kempf S +5 more
europepmc +1 more source
Observations of Titan’s Stratosphere during Northern Summer: Temperatures, CH3CN and CH3D Abundances
Titan’s atmospheric composition and dynamical state have previously been studied over numerous epochs by both ground- and space-based facilities. However, stratospheric measurements remain sparse during Titan’s northern summer and fall.
Alexander E. Thelen +13 more
doaj +1 more source
Titan is unique among the icy satellites in that it has a thick atmosphere, stable surficial bodies of liquid, and a precipitation system that promotes interactions between the two.
Anna E. Engle +11 more
doaj +1 more source
Origin and Evolution of Enceladus's Tidal Dissipation. [PDF]
Nimmo F, Neveu M, Howett C.
europepmc +1 more source
Exploring the Interior Structure and Mode of Tidal Heating in Enceladus
Enceladus is among the most intriguing bodies in the solar system due to its astrobiological potential. Determining the extent and duration of habitability (i.e., sustained habitability ) requires characterizing the interior properties and the level and ...
Amirhossein Bagheri +6 more
doaj +1 more source
Spectroscopic Detection of Biosignatures in Natural Ice Samples as a Proxy for Icy Moons. [PDF]
Calapez F +6 more
europepmc +1 more source

