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- W4239713145 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." @default.
- W4239713145 created "2022-05-12" @default.
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- W4239713145 date "2021-01-01" @default.
- W4239713145 modified "2023-09-27" @default.
- W4239713145 title "Saturn System" @default.
- W4239713145 cites W2022283492 @default.
- W4239713145 cites W2147015115 @default.
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- W4239713145 doi "https://doi.org/10.1016/b978-0-12-409548-9.11924-4" @default.
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