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Updated: Dec 26, 2025

Measurement of the Potential Rates of Dissimilatory Nitrate Reduction to Ammonium Based on 14NH4+/15NH4+ Analyses via Sequential Conversion to N2O
08:05

Measurement of the Potential Rates of Dissimilatory Nitrate Reduction to Ammonium Based on 14NH4+/15NH4+ Analyses via Sequential Conversion to N2O

Published on: October 7, 2020

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アムニウム 塩 は,彗星 の 核 や 恐らく 幾つ か の 小惑星 に ある 窒素 の 貯蔵 庫 です

Olivier Poch1, Istiqomah Istiqomah2, Eric Quirico2

  • 1Université Grenoble Alpes, Centre National de la Recherche Scientifique (CNRS), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), 38000 Grenoble, France. olivier.poch@univ-grenoble-alpes.fr.

Science (New York, N.Y.)
|March 14, 2020
PubMed
まとめ

67P/Churyumov-Gerasimenko彗星には,窒素と炭素の比率の不一致を解決するアンモニア塩の形で重要な窒素が含まれています. これらの塩は,彗星と小惑星を組成的に結びつける主要な窒素貯蔵庫です.

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