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Published Online: 5 January 2021

Elements for the Origin of Life on Land: A Deep-Time Perspective from the Pilbara Craton of Western Australia

Publication: Astrobiology
Volume 21, Issue Number 1

Abstract

For decades, deep sea hydrothermal vents have been a preferred setting for the Origin of Life, but “The Water Problem” as relates to polymerization of organic molecules, together with a propensity to dilute critical prebiotic elements as well as a number of other crucial factors, suggests that a terrestrial hot spring field with the capacity for wetdry cycling and element concentration may represent a more likely candidate. Here, we investigate a 3.5 billion-year-old, anoxic hot spring setting from the Pilbara Craton (Australia) and show that its hydrothermal veins and compositionally varied pools and springs concentrated all of the essential elements required for prebiotic chemistry (including B, Zn, Mn, and K, in addition to C, H, N, O, P, and S). Temporal variability (seasonal to decadal), together with the known propensity of hot springs for wetdry cycling and information exchange, would lead to innovation pools with peaks of fitness for developing molecules. An inference from the chemical complexity of the Pilbara analogue is that life could perhaps get started quickly on planets with volcanoes, silicate rocks, an exposed land surface, and water, ingredients that should form the backbone in the search for life in the Universe.

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Associate Editor: David Deamer

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Published In

cover image Astrobiology
Astrobiology
Volume 21Issue Number 1January 2021
Pages: 39 - 59
PubMed: 33404294

History

Published online: 5 January 2021
Published in print: January 2021
Accepted: 3 March 2020
Received: 22 May 2019

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Martin J. Van Kranendonk [email protected]
Australian Centre for Astrobiology, School of Biological Earth and Environmental Sciences, University of New South Wales Sydney, Kensington, Australia.
Pheasant Memorial Laboratory, Institute for Planetary Materials, Okayama University, Misasa, Japan.
Raphael Baumgartner
Australian Centre for Astrobiology, School of Biological Earth and Environmental Sciences, University of New South Wales Sydney, Kensington, Australia.
Tara Djokic
Australian Centre for Astrobiology, School of Biological Earth and Environmental Sciences, University of New South Wales Sydney, Kensington, Australia.
Tsutomu Ota
Pheasant Memorial Laboratory, Institute for Planetary Materials, Okayama University, Misasa, Japan.
Luke Steller
Australian Centre for Astrobiology, School of Biological Earth and Environmental Sciences, University of New South Wales Sydney, Kensington, Australia.
Ulf Garbe
Australian Nuclear Science and Technology Organisation, Kirrawee, Australia.
Eizo Nakamura
Pheasant Memorial Laboratory, Institute for Planetary Materials, Okayama University, Misasa, Japan.

Notes

Address correspondence to: Martin J. Van Kranendonk, Australian Centre for Astrobiology, School of Biological Earth and Environmental Sciences, University of New South Wales Sydney, Kensington 2052, Australia [email protected]

Author Disclosure Statement

No competing financial interests exist.

Funding Information

M.V.K., T.D., and R.B. acknowledge support from UNSW, the Sloan Foundation of the Carnegie Institution of Washington, the ARC Centre of Excellence for Core to Crust Fluid Systems (CCFS), and funds from ARC Discovery Project 180103204. E.N. and T.O. are supported by MEXT, Japan. This is CCFS Publication number 1486.

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