Io: Thermal models and chemical evolution
- 31 July 1981
- journal article
- Published by Elsevier BV in Icarus
- Vol. 47 (1), 36-45
- https://doi.org/10.1016/0019-1035(81)90089-0
Abstract
No abstract availableKeywords
This publication has 14 references indexed in Scilit:
- Kinetic inhibition of CO and N2 reduction in circumplanetary nebulae - Implications for satellite compositionThe Astrophysical Journal, 1981
- Mass-injection rate from Io into the Io plasma torusIcarus, 1980
- Stability of sulfur slopes on IoIcarus, 1980
- Evolution of Io's volatile inventoryIcarus, 1980
- Volcanic resurfacing rates and implications for volatiles on IoNature, 1979
- Significance of absorption features in Io's IR reflectance spectrumNature, 1979
- Origin of the jovian ring and the galilean satellitesNature, 1979
- The formation of saturn's satellites and rings, as influenced by saturn's contraction historyIcarus, 1976
- The Temperature Gradient in the Solar NebulaScience, 1974
- Petrogenesis of Lunar Basalts and the Internal Constitution and Origin of the MoonScience, 1970