Satellite Mass Determination in the Uranian System

Details Satellite Mass Determination in the Uranian System Satellite Mass Determination in the Uranian System

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.242..109v&link_type=abstract

The Solid Bodies of the Outer Solar System, Proceedings of a conference held at Vulcano, Italy, 9-13 September, 1985. Compiled

Computer Science

1

Scientific paper

The main characteristics of Uranian satellite orbital motion are given. Various sets of orbital elements are presented together with the available observational data. The Laplacian resonance between Miranda, Ariel and Umbriel is described on both the theoretical and observational aspects. Information on how the satellite masses can be derived from this resonance and pericenter and node motions is given. All these aspects are presented mainly with the aim of clarifying the knowledge of the satellite masses.

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