| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 8144190 | Planetary and Space Science | 2012 | 8 Pages |
Abstract
⺠This paper reports a suite of Titan interior models for comparison with Cassini gravity data. ⺠Titan's observed moment of inertia is strongly indicative of a large, low-density core. ⺠The core must consist of either hydrous silicates, or a mixture of ice + anhydrous silicates. ⺠Either of these possibilities requires that Titan's core is comparatively cool, 500-800 K.
Keywords
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geophysics
Authors
A.D. Fortes,