Computer Science
Scientific paper
Dec 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979icar...40..364d&link_type=abstract
Icarus, vol. 40, Dec. 1979, p. 364-374. NASA-supported research.
Computer Science
37
Albedo, Asteroids, Light Curve, Polarization Characteristics, Spectral Reflectance, Color, Polarimetry, Spectral Energy Distribution, Vesta Asteroid, Ceres Asteroid, Juno Asteroid, Vesta Asteroid, Hebe Asteroid, Asteroids, Metis Asteroid, Eunomia Asteroid, Psyche Asteroid, Fortuna Asteroid, Themis Asteroid, Phocaea Asteroid, Amphitrite Asteroid, Laetitia Asteroid, Nysa Asteroid, Pales Asteroid, Niobe Asteroid, Sylvia Asteroid, Surfaces, Eukrate Asteroid, Dembowska Asteroid, Eros Asteroid, Harvard Asteroid,
Scientific paper
Asteroids in general display only small or negligible variations in spectrum or albedo during a rotational cycle. Color variations with rotation are described in the literature but are usually comparable to the noise in the measurements. Twenty-four asteroids have been systematically monitored for such color changes. Only 3 Juno, 4 Vesta, 6 Hebe, 71 Niobe, 349 Dembowska, and 944 Hidalgo display color variations larger than 0.03 mag. In each of these cases the asteroid appears redder near maximum brightness. Of seven asteroids monitored polarimetrically, only 4 Vesta shows a convincing variation, attributed to an albedo change with rotation. The lightcurve can be explained by albedo differences alone; Vesta apparently has a nearly spheroidal shape. Notwithstanding the above results, the degree of uniformity of most asteroid surfaces is remarkable. If asteroids exist with large discrete domains of ferrosilicate, metallic, and/or carbonaceous material together on their surfaces, they have not yet been identified.
Degewij Johan
Tedesco Edward F.
Zellner Ben
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