Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979ap%26ss..65..275w&link_type=abstract
(Workshop on Thermodynamics and Kinetics of Dust Formation in the Space Medium, Houston, Tex., Sept. 6-8, 1978.) Astrophysics an
Astronomy and Astrophysics
Astrophysics
22
Carbonaceous Chondrites, Cosmology, Meteoritic Composition, Planetary Nebulae, Solar System, Stellar Evolution, Electron Microscopy, Grains, Inclusions, Meteoritic Microstructures, Planetary Evolution, Pyroxenes, Supernova Remnants
Scientific paper
The paper applies the supernova-trigger hypothesis for solar system formation to explain properties of the Allende meteorite. This carbonaceous chondrite meteorite is an assemblage of Ca-Al-rich inclusions (CAI's) alkali-rich spinel aggregates, and olivine chondrules in a fine-grained black matrix. Isotopic, chemical, and textural properties show that these components formed as independent cosmic grains. It appears that in the environment where these materials formed, condensation moved in the direction of increasing olivine and decreasing refractory element and (0-16) content. These properties are accounted for in a model in which a supernova remnant (SNR) in the snowplow phase pushes into a dark interstellar cloud, and condensation of CAI's begins in the SNR shell when it has been diluted with about 2500 times its mass of matter from the cloud. The retardation of the SNR by the cloud propels condensed grains ahead toward the cloud under their own momentum, and continuing dilution by the cloud can explain the fractionation patterns and depletion of refractory elements in successive condensates.
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