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Formación de HCN y cromóforos en Júpiter

J P Ferris1, Y Ishikawa

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

Nature
|April 23, 1987
PubMed
Resumen

La fotólisis de mezclas de amoníaco y acetileno puede explicar la formación de cianuro de hidrógeno (HCN) y cromóforos en la atmósfera reductora de Júpiter. Este proceso fotoquímico ofrece una solución potencial a un gran rompecabezas de la química atmosférica.

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La disciplina de la NASA es la exobiología.No perteneciente al Centro de la NASA.

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