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8. Microwave Brightnesses of 1 Ceres and 4 Vesta

Published online by Cambridge University Press:  12 April 2016

E. K. Conklin ,
B. L. Ulich ,
J. R. Dickel  and
D. T. Ther

Abstract

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The brightnesses of Ceres and Vesta were observed at 3 mm wavelength. For Ceres, pure rock cannot reproduce the observed values, and a dust layer is required, much similar to lunar material. For Vesta, its different thermal characteristics appear to require a more compacted layer of material on its surface.

Type
Part IV. Physical Nature of Asteroids
Information
International Astronomical Union Colloquium , Volume 39: Comets, Asteroids, Meteorites: Interrelations, Evolution and Origins , December 1977 , pp. 257 - 261
Copyright
Copyright © A.H. Delsemme 1977

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