have been observed at 870 ΞΌm (345 GHz) using the MPIfR 19-Channel Bolometer of the Heinrich-Hertz Submillimeter Telescope. Only Ceres displayed a lightcurve with an amplitude (βΌ50%, peak to peak) that was significantly greater than the uncertainty in the observations. When thermal fluxes and brightn
β¦ LIBER β¦
J, H, K photometry of 433 Eros and other asteroids
β Scribed by Clark R. Chapman; David Morrison
- Book ID
- 107765256
- Publisher
- Elsevier Science
- Year
- 1976
- Tongue
- English
- Weight
- 315 KB
- Volume
- 28
- Category
- Article
- ISSN
- 0019-1035
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