Add to ORKGAbstracts presented at a session, Satellites of Saturn, at the 12th Lunar and Planetary Science Conference, 17 March 1981.Compiled by the Lunar and Planetary Institute.Evolution of the Saturnian Satellites: The Role of Impact / E.M. Shoemaker and R.F. Wolfe--Variations in Crater Densities on Mimas, Dione, and Rhea / J.B. Plescia and J.M. Boyce--Crater Populations on Mimas, Dione and Rhea / R.G. Strom--Enceladus: Evolution and Possible Relationship to Saturn's E-Ring / R.J. Terrile and A.F. Cook--Bulk Properties of the Saturnian Satellites: Implications for Evolution / L.A. Soderblom and T.V. Johnson
The Moon is an archive of impact cratering in the Solar System throughout the past 4.5 billion years...
The dynamical features of the irregular satellites of the giant planets argue against an in-situ for...
The Program Committee for the Twentieth Lunar and Planetary Science Conference has chosen these cont...
Abstract Saturn is the first giant planet to be visited by an orbiting spacecraft that can transmit ...
Topics addressed include: chemical abundances; asteroidal belt evolution; sources of meteors and met...
Topics addressed include: chemical abundances; asteroidal belt evolution; sources of meteors and met...
A review is provided of current concepts concerning the formation of the Saturn system and the subse...
The sizes of the Saturnian icy satellites range from ~ 1;500 km in diameter (Rhea) to ~20km (Calypso...
The Program Committee for the Tenth Lunar and Planetary Science Conference has chosen these contribu...
A number of important cosmogonic questions concerning the Saturn system can be addressed with a Satu...
The Program Committee for the Eighteenth Lunar and Planetary Science Conference has chosen these con...
Maps, compiled with data gathered primarily by Voyager 1 and 2 spacecraft, are presented which show ...
Context. The small (≤135 km mean radius) satellites of Saturn are closely related to its rings and t...
The Program Committee for the Eleventh Lunar and Planetary Science Conference has chosen these contr...
The Program Committee for the Seventeenth Lunar and Planetary Science Conference has chosen these co...
The Moon is an archive of impact cratering in the Solar System throughout the past 4.5 billion years...
The dynamical features of the irregular satellites of the giant planets argue against an in-situ for...
The Program Committee for the Twentieth Lunar and Planetary Science Conference has chosen these cont...
Abstract Saturn is the first giant planet to be visited by an orbiting spacecraft that can transmit ...
Topics addressed include: chemical abundances; asteroidal belt evolution; sources of meteors and met...
Topics addressed include: chemical abundances; asteroidal belt evolution; sources of meteors and met...
A review is provided of current concepts concerning the formation of the Saturn system and the subse...
The sizes of the Saturnian icy satellites range from ~ 1;500 km in diameter (Rhea) to ~20km (Calypso...
The Program Committee for the Tenth Lunar and Planetary Science Conference has chosen these contribu...
A number of important cosmogonic questions concerning the Saturn system can be addressed with a Satu...
The Program Committee for the Eighteenth Lunar and Planetary Science Conference has chosen these con...
Maps, compiled with data gathered primarily by Voyager 1 and 2 spacecraft, are presented which show ...
Context. The small (≤135 km mean radius) satellites of Saturn are closely related to its rings and t...
The Program Committee for the Eleventh Lunar and Planetary Science Conference has chosen these contr...
The Program Committee for the Seventeenth Lunar and Planetary Science Conference has chosen these co...
The Moon is an archive of impact cratering in the Solar System throughout the past 4.5 billion years...
The dynamical features of the irregular satellites of the giant planets argue against an in-situ for...
The Program Committee for the Twentieth Lunar and Planetary Science Conference has chosen these cont...