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  5. Saturn System
 

Saturn System

Date Issued
2019
Author(s)
FILACCHIONE, GIANRICO  
•
CIARNIELLO, Mauro  
DOI
10.1016/B978-0-12-409548-9.11924-4
Abstract
As the second most massive gaseous planet of our Solar System, Saturn is of scarce interest for geologists. Conversely, its giant moon Titan, the eight mid-sized icy satellites and the numerous minor moons offer a wide choice of sizes, morphologies, structures, composition, and processes of interest. The Cassini mission has revealed cryovolcanic activity on the south region of Enceladus, the highly porous, sponge-like moon Hyperion and the equatorial mountain ridge on the surface of Iapetus, the moon divided into very dark and very bright hemispheres. Moreover, the planet is encircled by the largest planetary ring system known.
Coverage
Encyclopedia of Geology
Start page
123
Uri
http://hdl.handle.net/20.500.12386/30480
Url
https://www.sciencedirect.com/science/article/pii/B9780124095489119244?via%3Dihub
Ads BibCode
2019rmes.bookE...1F
Rights
restricted
File(s)
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Name

Filacchione_Ciarniello_Reference_Module_Saturn_2019.pdf

Description
[Administrators only]
Size

2.98 MB

Format

Adobe PDF

Checksum (MD5)

a74f333a9109658bd7d2f94b75f35c5c

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