Visible Phase Curves and Internal Heat Flow for Uranus

Details Visible Phase Curves and Internal Heat Flow for Uranus Visible Phase Curves and Internal Heat Flow for Uranus

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agufm.p11b1281w&link_type=abstract

American Geophysical Union, Fall Meeting 2008, abstract #P11B-1281

Physics

0343 Planetary Atmospheres (5210, 5405, 5704), 5704 Atmospheres (0343, 1060), 5724 Interiors (8147), 6293 Uranus

Scientific paper

Images of Uranus acquired by Voyager 1 during the 1980s were re-analyzed using improved calibrations. These images provide disk-averaged reflectivities in six bands, at phase angles from 28 to 100 degrees. These, along with measurements made by the Voyager 2 spacecraft during 1986, are being used to constrain an atmospheric model of Uranus to generate a new bolometric Bond albedo for the planet in the 1980s epoch. Improved phase curves, atmospheric models, albedos, and a recomputed heat flow will be presented.

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