Composition, structure and evolution of Uranian and Neptunian satellites
Large uncertainties in the current estimated densities of all of these satellites prevent detailed modeling or predictions. Nevertheless, current evidence suggests that at least Titania and Oberon might have anomalously high densities of 2-39 cm(-3), possibly requiring almost ice-free hydrated silicates or formation in a CO-rich environment, implying presence of CO-clathrate and a small ice/rock ratio. Trition and the four largest satellites of Uranus are massive enough to have undergone significant accretional heating and early differentiation; NH3-H2O volcanism; partial outgassing of CO, N2, Ch4; formation of dark surficial deposits of carbon-rich material obtained by UV irradiation of outgassed material; and, at least in the cases of Ariel and Triton, a possibility of weak ongoing icy volcanic activity. Triton may be the largest captured body in the solar system, with an unusual history and composition, including the possibility of substantial liquid or solid nitrogen obtained from either primordial NH3 photolysis or clathrate decomposition.
- Research Organization:
- California Inst. of Tech., Pasadena (USA)
- OSTI ID:
- 5971243
- Report Number(s):
- N-85-11944
- Resource Relation:
- Other Information: In JPL Uranus and Neptune, 405-423p (N--85-11927 02-91)
- Country of Publication:
- United States
- Language:
- English
Similar Records
Comparative global albedo and color maps of the Uranian satellites
FREE TRANSLATIONAL OSCILLATIONS OF ICY BODIES WITH A SUBSURFACE OCEAN USING A VARIATIONAL APPROACH