Aug 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992stin...9318554b&link_type=abstract
In its Exobiology in Solar Research Exploration p 145-158 (SEE N93-18545 06-51)
Biology
Carbonaceous Materials, Chemical Composition, Chemical Evolution, Cosmic Dust, Exobiology, Interplanetary Dust, Interstellar Matter, Planetary Composition, Planetary Nebulae, Galaxies, Interstellar Chemistry, Solar System
Scientific paper
Dust is a ubiquitous component of our galaxy and the solar system. The collection and analysis of extraterrestrial dust particles is important to exobiology because it provides information about the sources of biogenically significant elements and compounds that accumulated in distant regions of the solar nebula and that were later accreted on the planets. The topics discussed include the following: general properties of interplanetary dust; the carbonaceous component of interplanetary dust particles; and the presence of an interstellar component.
Brownlee Donald E.
Sandford Scott A.
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