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ACCRETION OF SATURN’S INNER MID-SIZED MOONS FROM A MASSIVE PRIMORDIAL ICE RING
Saturn’s rings are rock-poor, containing 90 to 95% ice by mass. As a group, Saturn’s moons interior to and including Tethys are also about 90% ice. Tethys itself contains < 6% rock by mass, in contrast to its similar-mass outer neighbor Dione, which contains > 40% rock. Here we simulate the ev...
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| Veröffentlicht in: | Astrophys J |
|---|---|
| Hauptverfasser: | , |
| Format: | Artigo |
| Sprache: | Inglês |
| Veröffentlicht: |
2017
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| Schlagworte: | |
| Online Zugang: | https://ncbi.nlm.nih.gov/pmc/articles/PMC6476552/ https://ncbi.nlm.nih.gov/pubmed/31019332 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.3847/1538-4357/836/1/109 |
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