Venus-like massive CO2 atmospheres can form through primary outgassing, secondary volcanic degassing, or crustal carbonate remobilization, making them equifinal rather than diagnostic of a temperate past.
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Equifinality of Venus-like CO$_2$ Atmospheres
Venus-like massive CO2 atmospheres can form through primary outgassing, secondary volcanic degassing, or crustal carbonate remobilization, making them equifinal rather than diagnostic of a temperate past.