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Analysis of Interplanetary Dust Collections

Published online by Cambridge University Press:  14 August 2015

D. E. Brownlee ,
L. Pilachowski ,
E. Olszewski  and
P. W. Hodge
D. E. Brownlee
Affiliation:
Department of Astronomy, University of Washington, 98195
L. Pilachowski
Affiliation:
Department of Astronomy, University of Washington, 98195
E. Olszewski
Affiliation:
Department of Astronomy, University of Washington, 98195
P. W. Hodge
Affiliation:
Department of Astronomy, University of Washington, 98195

Abstract

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Interplanetary dust particles collected in the form of micrometeorites in the stratosphere and meteor ablation spherules in deep sea sediments are possibly a relatively unbiased sample of the micrometeoroid complex near 1 AU. Detailed laboratory analysis of the particles has provided information on physical properties which may be useful in modeling a variety of aspects of interplanetary dust.

Type
IV: The Interplanetary Dust Complex 2. Physical Properties
Information
Symposium - International Astronomical Union , Volume 90: Solid Particles in the Solar System , 1980 , pp. 333 - 342
Copyright
Copyright © Reidel 1980 

References

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