The long-wavelength topography of Titan has an amplitude larger than that expected from tidal and rotational distortions at its current distance from Saturn. This topography is associated with small gravity anomalies, indicating a high degree of compensation. Both observations can be explained if Ti
The long wavelength topography of Beethoven and Tolstoj basins, Mercury
✍ Scribed by André, Sarah L.; Watters, Thomas R.; Robinson, Mark S.
- Book ID
- 119666564
- Publisher
- American Geophysical Union
- Year
- 2005
- Tongue
- English
- Weight
- 239 KB
- Volume
- 32
- Category
- Article
- ISSN
- 1944-8007
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