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木星のHCNと染色体の形成

J P Ferris1, Y Ishikawa

  • 1Department of Chemistry, Rensselaer Polytechnic Institute, Troy, New York 12180-3590, USA.

Nature
|April 23, 1987
PubMed
まとめ

アンモニアとアセチレン混合物の光分解は,木星の還元大気中の水素シアン化物 (HCN) と染色体の形成を説明することができます. この光化学的プロセスは,大気化学の大きなパズルの潜在的な解決策を提供します.

キーワード:
NASAの規律 エクゾバイオロジー非NASAのセンターです.

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