Origin of the solar system dust bands discovered by IRAS

Details Origin of the solar system dust bands discovered by IRAS Origin of the solar system dust bands discovered by IRAS

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984natur.312..505d&link_type=abstract

Nature (ISSN 0028-0836), vol. 312, Dec. 6, 1984, p. 505-509. NASA-NSF-supported research.

Astronomy and Astrophysics

Astronomy

82

Brightness Distribution, Galactic Evolution, Infrared Astronomy Satellite, Interplanetary Dust, Solar System, Zodiacal Light, Asteroids, Astronomical Models, Comets, Eccentric Orbits, Orbital Elements, Particle Size Distribution, Spaceborne Astronomy

Scientific paper

It is shown that distinctive longitudinal variations in thermal flux and mean latitude can be used to determine the typical orbits of the grains comprising the Solar System bands. In particular, how the bands should vary if they are debris associated with the three principal asteroid families is predicted. Based on these ideas, IRAS observations may allow discrimination between asteroidal and cometary origins of the dust bands and, perhaps, of the entire zodiacal cloud.

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