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Collisions Among Interplanetary Dust Grains

Published online by Cambridge University Press:  14 August 2015

L.B. Le Sergeant  and
P.L. Lamy
L.B. Le Sergeant
Affiliation:
Laboratoire d'Astronomie Spatiale, Marseille, France
P.L. Lamy
Affiliation:
Laboratoire d'Astronomie Spatiale, Marseille, France

Abstract

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Assuming that the zodiacal cloud is composed of two populations, the effect of collisions among the largest grains is investigated. It is found that the population of fragments is unable to explain the observed flux of submicron grains.

Type
III: The Interplanetary Dust Complex 1. Sources, Evolution, and Dynamics
Information
Symposium - International Astronomical Union , Volume 90: Solid Particles in the Solar System , 1980 , pp. 289 - 292
Copyright
Copyright © Reidel 1980 

References

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