The formation of carbonates on Mars have been suggested based on evidence of the presence of liquid water and atmospheric carbon dioxide in the planet's early stages.[1] Moreover, due to their utility in registering changes in environmental conditions such as pH, temperature, fluid composition,[2] carbonates have been considered as a primary target for planetary scientists' research.[1] However, since their first detection in 2008,[3] the large deposits of carbonates that were one expected on Mars have not been found,[4] leading to multiple potential explanations that can explain why carbonates did not form massively on the planet.
^ abNiles, Paul B.; Catling, David C.; Berger, Gilles; Chassefière, Eric; Ehlmann, Bethany L.; Michalski, Joseph R.; Morris, Richard; Ruff, Steven W.; Sutter, Brad (January 2013). "Geochemistry of Carbonates on Mars: Implications for Climate History and Nature of Aqueous Environments". Space Science Reviews. 174 (1–4): 301–328. doi:10.1007/s11214-012-9940-y. ISSN 0038-6308.
^Bridges, John C.; Hicks, Leon J.; Treiman, Allan H. (2019-01-01), Filiberto, Justin; Schwenzer, Susanne P. (eds.), "Chapter 5 - Carbonates on Mars", Volatiles in the Martian Crust, Elsevier, pp. 89–118, doi:10.1016/b978-0-12-804191-8.00005-2, ISBN 978-0-12-804191-8, retrieved 2024-04-30
^Ehlmann, Bethany L.; Mustard, John F.; Murchie, Scott L.; Poulet, Francois; Bishop, Janice L.; Brown, Adrian J.; Calvin, Wendy M.; Clark, Roger N.; Marais, David J. Des; Milliken, Ralph E.; Roach, Leah H.; Roush, Ted L.; Swayze, Gregg A.; Wray, James J. (19 December 2008). "Orbital Identification of Carbonate-Bearing Rocks on Mars". Science. 322 (5909): 1828–1832. Bibcode:2008Sci...322.1828E. doi:10.1126/science.1164759. PMID 19095939. S2CID 1190585.
^Fairén, Alberto G.; Fernández-Remolar, David; Dohm, James M.; Baker, Victor R.; Amils, Ricardo (September 2004). "Inhibition of carbonate synthesis in acidic oceans on early Mars". Nature. 431 (7007): 423–426. doi:10.1038/nature02911. ISSN 1476-4687.
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