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Spatially Varying Optical Properties of the Zodiacal Dust

Published online by Cambridge University Press:  14 August 2015

S. S. Hong  and
S. M. Kwon
S. S. Hong
Affiliation:
Department of Astronomy, Seoul National University, Korea
S. M. Kwon
Affiliation:
Space Astronomy Laboratory, University of Florida, U.S.A.

Abstract

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Analyses of both the zodiacal light in the visible and the zodiacal emission in the infrared have provided us with ample evidence to claim that the interplanetary dust particles are mixtures or coagulations of more than one constituents and their mixing ratios vary with the distance from the sun.

Type
Joint Discussions
Information
Highlights of Astronomy , Volume 8: Highlights of Astronomy. As presented at the XXth General Assembly of the IAU, 1988 , 1989 , pp. 267 - 272
Copyright
Copyright © Kluwer 1989

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