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The origin of life as a planetary phenomenon.
Sasselov, Dimitar D; Grotzinger, John P; Sutherland, John D.
Afiliação
  • Sasselov DD; Department of Astronomy, Harvard University, 60 Garden St., Cambridge, MA 02138, USA.
  • Grotzinger JP; Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA.
  • Sutherland JD; MRC Laboratory of Molecular Biology, Francis Crick Ave., Cambridge CB2 0QH, UK.
Sci Adv ; 6(6): eaax3419, 2020 02.
Article em En | MEDLINE | ID: mdl-32076638
ABSTRACT
We advocate an integrative approach between laboratory experiments in prebiotic chemistry and geologic, geochemical, and astrophysical observations to help assemble a robust chemical pathway to life that can be reproduced in the laboratory. The cyanosulfidic chemistry scenario described here was developed by such an integrative iterative process. We discuss how it maps onto evolving planetary surface environments on early Earth and Mars and the value of comparative planetary evolution. The results indicate that Mars can offer direct evidence for geochemical conditions similar to prebiotic Earth, whose early record has been erased. The Jezero crater is now the chosen landing site for NASA's Mars 2020 rover, making this an extraordinary opportunity for a breakthrough in understanding life's origins.

Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2020 Tipo de documento: Article

Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2020 Tipo de documento: Article