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 elements 、 Infrared astronomy 、 Asteroid belt 、 Astrophysics 、 Solar System 、 Physics 、 Brightness 、 Elliptic orbit 、 Interplanetary dust cloud 、 Astronomy
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.