A team of researchers suggest that liquid carbon dioxide (CO2) could have formed minerals on Mars, in addition to water.
Observations of minerals on the Martian surface suggest the presence of liquid water, but the researchers propose that liquid CO2 could have played a role.
They explain that carbon sequestration processes, which liquefy CO2 on Earth and bury it underground, could have caused liquid CO2 to form and alter mineral composition on Mars.
Further testing under more realistic Martian conditions is needed to confirm these findings.