Modeling the dust bands: Structure in zodiacal clouds

Details Modeling the dust bands: Structure in zodiacal clouds Modeling the dust bands: Structure in zodiacal clouds

Apr 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998exdu.work..269g&link_type=abstract

Exozodiacal Dust Workshop, p. 269

Astronomy and Astrophysics

Astronomy

Zodiacal Dust, Mathematical Models, Solar System, Asteroid Belts, Size Distribution, Frequency Distribution, Infrared Astronomy Satellite

Scientific paper

The solar system dust bands discovered by IRAS are toroidal distributions of dust particles with common proper inclinations. The manner in which dust band profiles change around the sky should allow the determination of the origin of the bands, their radial extent and the size-frequency distribution of the material. The equilibrium model of the dust bands associating the dust bands with the major Hirayama families, suggests Eos as the parent of the 10 degree pair. Comparisons of IRAS observations with two Eos dust band models are presented.

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