High Carbonate Alkalinity Lakes on Mars and their Potential Role in an Origin of Life Beyond Earth
Abstract
The exploration of Mars has revealed that its ancient surface hosted lakes with a dazzling array of chemical and physical conditions and processes. The potential habitability of surface waters has driven studies aimed at understanding whether or not Mars once hosted life. High levels of atmospheric carbon dioxide are probable on early Mars, which means that lakes derived from weathering fluids could have contained substantial carbonate alkalinity. Recent studies show that lakes with high carbonate alkalinity are able to concentrate the phosphate and cyanide that are critical for molecular synthesis in the origin of life. While evidence for carbonate-rich Martian lakes remains limited, NASA's Perseverance rover may reveal clues about the past existence of such waters in Jezero Crater.
Additional Information
© 2023 Mineralogical Society of America. JA Hurowitz, DC Catling, and WW Fischer gratefully acknowledge funding from the Simons Collaboration on the Origin of Life (SCOL), award numbers 572786, 511570, and 554187, respectively. DC Catling also acknowledges funding from NASA grant 80NSSC21K0149. We gratefully acknowledge insightful reviews by Eva Stüeken and an anonymous reviewer.Additional details
Identifiers
- Eprint ID
- 122550
- Resolver ID
- CaltechAUTHORS:20230726-216909500.10
Funding
- Simons Foundation
- 572786
- Simons Foundation
- 511570
- Simons Foundation
- 554187
- NASA
- 80NSSC21K0149
Dates
- Created
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2023-08-14Created from EPrint's datestamp field
- Updated
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2023-08-14Created from EPrint's last_modified field