Surface properties and photometry of the Uranian satellites

Astronomy and Astrophysics – Astronomy

Scientific paper

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Astronomical Photometry, Satellite Surfaces, Spaceborne Astronomy, Surface Properties, Uranus (Planet), Astronomical Spectroscopy, Natural Satellites, Voyager Project, Uranus, Satellites, Surface, Physical Properties, Photometry, Spectra, Spacecraft Observations, Voyager 2 Mission, Pps Instrument, Imagery, Parameters, Miranda, Ariel, Umbriel, Titania, Oberon, Albedo, Color, Optical Properties, Phases, Comparisons, Radiative Transfer, Models, Regolith, Compaction, Roughness, Photographs, Brightness, Icy Bodi

Scientific paper

Voyager photographic images and photopolarimetric experiment observations have been used to obtain the spectral geometric and Bond albedos, phase integrals, color-dependent phase coefficients, and integrated solar phase-curve parameters of the five Uranian satellites Miranda, Ariel, Umbriel, Titania, and Oberon. While the results obtained confirm those of Nelson et al. (1987) and Veverka et al. (1987) that these five largest Uranian satellites constitute a unique class of low-albedo and spectrally flat objects, attention is presently given to important differences among the five moons' surface physical properties.

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