The origin of life as a planetary phenomenon
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.
Additional Information
© 2020 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. No claim to original U.S. Government Works. Distributed under a Creative Commons Attribution NonCommercial License 4.0 (CC BY-NC). Received for publication March 14, 2019. Accepted for publication November 22, 2019. Published 5 February 2020. We thank our colleagues A. Knoll, D. Catling, E. Boyd, J. Szostak, J. Hurowitz, and S. Ranjan for reading the manuscript and providing numerous helpful comments and suggestions, which improved our paper. Our reviewers J. Kasting and N. Tosca made excellent suggestions for which we are very thankful. Funding: We thank the Simons Foundation for funding (D.D.S.: grant no. 290360; J.D.S.: grant no. 290362; J.P.G.: grant no. 477125). D.D.S. acknowledges the Harvard Origins of Life Initiative. Author contributions: All three authors participated in coming up with the original idea for the paper, in writing portions of the main text, and in editing the entire paper for accuracy and clarity. The authors declare that they have no competing interests. Data and materials availability: All data needed to evaluate the conclusions in the paper are present in the paper and/or the materials cited here. Additional data related to this paper may be requested from the authors.Attached Files
Published - eaax3419.full.pdf
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Additional details
- PMCID
- PMC7002131
- Eprint ID
- 101170
- Resolver ID
- CaltechAUTHORS:20200206-125057632
- Simons Foundation
- 290360
- Simons Foundation
- 290362
- Simons Foundation
- 477125
- Harvard Origins of Life Initiative
- Created
-
2020-02-06Created from EPrint's datestamp field
- Updated
-
2022-02-16Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences (GPS)