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Updated: Apr 9, 2026

Laboratory Simulation of an IronII-rich Precambrian Marine Upwelling System to Explore the Growth of Photosynthetic Bacteria
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初期の太陽星雲における酸素同位体異常の起源として,COの自己遮蔽

J R Lyons1, E D Young

  • 1Institute of Geophysics and Planetary Physics, University of California, Los Angeles, California 90095, USA. jrl@ess.ucla.edu

Nature
|May 20, 2005
PubMed
まとめ

隕石の酸素同位体異常 (カルシウム・アルミニウムに富んだ含有物) は,渦巻原惑星円盤におけるCO光解離によって説明される. このプロセスは,強烈な紫外線放射によって駆動され,酸素同位体を分断し,水 (H2O) の組成に影響を与えます.

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