Other
Scientific paper
Mar 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979icar...37..575d&link_type=abstract
Icarus, vol. 37, Mar. 1979, p. 575-586.
Other
28
Asteroids, Geodesy, Moments Of Inertia, Natural Satellites, Planetary Structure, Density Distribution, Galilean Satellites, Theoretical Studies, Models, Deformation, Ceres, Pallas, Vesta, Satellites, Asteroids, Jupiter, Saturn, Io, Europa, Ganymede, Callisto, Titan, Diona, Mimas, Tethys, Surface, Orbits, Evolution, Rotation, Density, Gravitational Moments, Shapes, Mantle, Water, Ice, Hydrostatics, Equilibrium
Scientific paper
The shapes and gravitational moments of tidally and rotationally distorted satellites with nonuniform internal density distributions are calculated. Spacecraft determinations of the radii and the gravitational moments of some satellites of Jupiter and Saturn, particularly Io, Ganymede and Titan, or the shapes of some others, particularly Mimas and Tethys, could provide unambiguous evidence of either internal differentiation or orbital evolution. The shapes of rotationally distorted asteroids are discussed briefly.
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