Near-Infrared Spectral Reflectivity of Puck

Details Near-Infrared Spectral Reflectivity of Puck Near-Infrared Spectral Reflectivity of Puck

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997hst..prop.7183s&link_type=abstract

HST Proposal ID #7183

Computer Science

Hst Proposal Id #7183

Scientific paper

Voyager provided no information on the spectral reflectivities of the small, dark, inner satellites that it discovered around Uranus and Neptune. These objects are too faint and too close to their respective planets to be well measured from the ground. Observations should be made when Puck is near maximum elongation and with Uranus just outside the field of view. Multispectral filter photometry of Puck, the brightest of the small dark Uranus satellites, will be done in filters identical to those used on Neptune's Proteus. Puck has an albedo of 0.07, similar to that of Proteus, suggesting common origin. Intercomparisons will be made among the dark bodies of the outer solar system and the small, dark satellites of Mars.

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