An Analysis of IRAS Solar System Dust Bands

作者: S. F. Dermott , P. D. Nicholson , J. A. Burns , J. R. Houck

DOI: 10.1007/978-94-009-5464-9_77

关键词: Eccentricity (behavior)Orbital elementsInfrared astronomyAsteroid beltAstrophysicsSolar SystemPhysicsBrightnessElliptic orbitInterplanetary dust cloudAstronomy

摘要: Measurements of longitudinal variations in the brightness and latitude solar system dust bands recently discovered by IRAS will determine orbital elements particles involved may discriminate between cometary asteroidal models origin these bands. The expected for with common small eccentricity inclination are calculated as functions semimajor axis.

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