A Photometric Study of Uranus
β Scribed by Paul Slavenas
- Publisher
- John Wiley and Sons
- Year
- 1928
- Tongue
- English
- Weight
- 128 KB
- Volume
- 233
- Category
- Article
- ISSN
- 0004-6337
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
We have supplemented Voyager imaging data from Enceladus (limited to phase angles of \(13^{\circ}-43^{\circ}\) ) with recent Earth-based CCD observations to obtain an improved determination of the Bond albedo, to construct an albedo map of the satellite, and to constrain parameters in Hapke's (1986,
The ring model of Irvine (1966, J. Geophys. Res. 71, 2931-2937) is used to explain the longitudinal brightness variation of the Ξ΅ ring of Uranus observed by Voyager 2 and with the Hubble Space Telescope, while basic ring properties are based on occultation data. The observations span a factor of 600