Photometry of Saturn's satellites: The opposition effect of Iapetus at maximum light and the variability of Titan
- 30 November 1974
- Vol. 23 (3) , 355-362
- https://doi.org/10.1016/0019-1035(74)90053-0
Abstract
No abstract availableKeywords
This publication has 13 references indexed in Scilit:
- Six-color photometry of lapetus, Titan, Rhea, Dione and TethysIcarus, 1974
- Determination of radii of satellites and asteroids from radiometry and photometryIcarus, 1973
- Saturn's rings—A surveyIcarus, 1973
- UBV photometry of IapetusIcarus, 1973
- Radii, Albedos, and 20-MICRON Brightness Temperatures of Iapetus and RHEAThe Astrophysical Journal, 1972
- A dynamical model for the radial structure of Saturn's rings. IIIcarus, 1971
- An explanation of the light curve of IapetusIcarus, 1970
- Optical properties of Saturn's rings. II. Two-color phase curves of the 2 bright rings.The Astronomical Journal, 1965
- The Color-Magnitude Diagram of the Hyades Cluster.The Astrophysical Journal, 1962
- The Effects of Collisions on Saturn's RingsMonthly Notices of the Royal Astronomical Society, 1947