在原始泰坦上,高温冲击形成N2和有机物

C P McKay1, T W Scattergood, J B Pollack

  • 1Solar System Exploration Branch, NASA Ames Research Center, Moffett Field, California 94035, USA.

Nature
|April 7, 1988
PubMed
概括

在行星形成过程中的冲击可能在泰坦早期的大气中将氨 (NH3) 转化为 (N2). 激光冲击实验表明,这个过程有效地产生N2和其他分子,支持泰坦大气演化的理论.

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