A refined “standard” thermal model for asteroids based on observations of 1 Ceres and 2 Pallas
- 1 November 1986
- Vol. 68 (2) , 239-251
- https://doi.org/10.1016/0019-1035(86)90021-7
Abstract
No abstract availableKeywords
This publication has 16 references indexed in Scilit:
- Ellipsoidal geometry in asteroid thermal models: The standard radiometric modelIcarus, 1985
- Submillimeter observations of the asteroid 10 hygieaIcarus, 1985
- Absolute calibration of photometry at 1 through 5 micronsThe Astronomical Journal, 1985
- 2 Pallas: 1982 and 3 lightcurves and a new pole solutionIcarus, 1984
- A reevaluation of the 20-micron magnitude systemThe Astronomical Journal, 1984
- Worldwide photometry and lightcurve observations of 1 Ceres during the 1975–1976 apparitionIcarus, 1983
- Calibration of the radiometric asteroid scale using occultation diametersIcarus, 1982
- Radiometric diameters for an additional 22 asteroidsThe Astrophysical Journal, 1976
- Rotation and photometric characteristics of PallasIcarus, 1976
- Recalibration of the photometric/radiometric niethod of determining asteroid sizesThe Astronomical Journal, 1974