Results 81 to 90 of about 7,875 (212)
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 +1 more source
Ocean stratification impedes particulate transport to the plumes of Enceladus
Water-vapour plumes erupting from Enceladus’ south pole provide a window into the properties of its subsurface ocean, a prime target in the search for life. However, the extent to which plume material represents conditions at Enceladus’ depths is unclear,
Flynn Ames +3 more
doaj +1 more source
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 +14 more
doaj +1 more source
Mapping spiral waves and other radial features in Saturn's rings
We have analyzed the highest-quality images to be obtained by Cassini of Saturn's main rings after the Saturn Orbit Insertion (SOI) and before the Ring Grazing Orbits (RGO) and Grand Finale (GF).
Harris, Brent E., Tiscareno, Matthew S.
core +1 more source
Evidence of an Extended Alfvén Wing System at Enceladus: Cassini's Multi‐Instrument Observations
Abstract We report in situ evidence for Enceladus' Alfvén wing system and its coupling with Saturn's ionosphere, based on multi‐instrument observations from the Cassini spacecraft. Analysis of 36 events, including 13 from non‐flyby paths, confirms the existence of a Main Alfvén Wing (MAW) current system generated at Enceladus, and associated Reflected ...
L. Z. Hadid +28 more
wiley +1 more source
Differentiating Plumes and Local Torus Segments of Enceladus
Abstract Enceladus's south polar plumes and their surrounding torus segments (local plasma regions formed by plume material diffusion) are key to understanding its magnetospheric interaction; however, clear observational criteria to distinguish them remain lacking.
Shangchun Teng +6 more
wiley +1 more source
Towards Determining Biosignature Retention in Icy World Plumes
With the discovery of the persistent jets of water being ejected to space from Enceladus, an understanding of the effect of the space environment on potential organisms and biosignatures in them is necessary for planning life detection missions.
Kathryn Bywaters +3 more
doaj +1 more source
Seismic wave propagation in icy ocean worlds
Seismology was developed on Earth and shaped our model of the Earth's interior over the 20th century. With the exception of the Philae lander, all in situ extraterrestrial seismological effort to date was limited to other terrestrial planets. All have in
Kedar, Sharon +6 more
core +1 more source
Effects of immersed moonlets in the ring arc particles of Saturn
Ring arcs are the result of particles in corotation resonances with nearby satellites. Arcs are present in Saturn and Neptune systems, in Saturn they are also associated with small satellites immersed on them.
Madeira, Gustavo +1 more
core +2 more sources
Analysis of Ion Cyclotron Waves during Cassini’s Flybys of Enceladus
Ion cyclotron waves (ICWs) are ubiquitous phenomena within Saturn’s magnetosphere, particularly in the vicinity of Enceladus. This study focuses on the Cassini spacecraft’s flyby data of Enceladus to investigate the spatial distribution and properties of
Shangchun Teng +3 more
doaj +1 more source

