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Enceladus' Water Vapor Plume
TLDR
The Cassini spacecraft flew close to Saturn's small moon Enceladus three times in 2005 and observed stellar occultations on two flybys and confirmed the existence, composition, and regionally confined nature of a water vapor plume in the south polar region of Ence Gladus.
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The Cassini Ultraviolet Imaging Spectrograph Investigation
The Cassini Ultraviolet Imaging Spectrograph (UVIS) is part of the remote sensing payload of the Cassini orbiter spacecraft. UVIS has two spectrographic channels that provide images and spectra…
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Self‐gravity wakes in Saturn's A ring measured by stellar occultations from Cassini
An azimuthal brightness asymmetry in Saturn's A ring is caused by ephemeral agglomerations that continually form under the mutual gravity of the ring particles only to be torn apart by Keplerian…
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Sulfur Dioxide: Episodic Injection Shows Evidence for Active Venus Volcanism
  • L. Esposito
  • Environmental Science, Geology
    Science
  • 9 March 1984
TLDR
Pioneer Venus ultraviolet spectra from the first 5 years of operation show a decline in sulfur dioxide abundance at the cloud tops and in the amount of submicron haze above the clouds, implying the episodic injection of sulfur dioxide possibly caused by episodic volcanism.
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Self-gravity wakes and radial structure of Saturn's B ring
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Particulate matter in the Venus atmosphere
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Monte Carlo simulations of the water vapor plumes on Enceladus
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The structure of Saturn's rings: Implications from the Voyager stellar occultation
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Saturn's rings - Properties and processes
In the present consideration of the structural and particle properties of Saturn's rings, emphasis is given to spacecraft observations and an attempt is made to relate observed properties to favored…
Saturn from Cassini-Huygens
This book comprehensively reviews our current knowledge of Saturn featuring the latest results obtained by the Cassini-Huygens mission.
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