月の岩12013からの粉の化学組成と,ジャワのテクタイトと岩石の比較

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Updated: Jul 12, 2026

Scattering And Absorption of Light in Planetary Regoliths
11:34

Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

D L Showalter, H Wakita, R H Smith

    Science (New York, N.Y.)
    |January 14, 1972
    PubMed
    まとめ

    インストゥルメンタルニュートロン活性化分析により,アポロ12013号の岩石断片と粉は,類似の主要な元素の豊富さにもかかわらず,Java tektiteガラスと化学的に似ていないことが明らかになりました. ソーダストは,正確な元素組成分析のために汚染補正を必要とします.

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