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Updated: Jul 11, 2026

Simulation of the Planetary Interior Differentiation Processes in the Laboratory
06:04

Simulation of the Planetary Interior Differentiation Processes in the Laboratory

Published on: November 15, 2013

炭酸性隕石の原始核組成の成分である

R N Clayton, L Grossman, T K Mayeda

    Science (New York, N.Y.)
    |November 2, 1973
    PubMed
    まとめ

    隕石の酸素同位体は,純粋な16O成分を示し,重い枯渇を示しています. これは,太陽系前の恒星間塵が,太陽系より前の恒星間塵の源である可能性を示唆しています.

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