Abstract
Organic matter in the Martian sediments may provide a key to understanding the prebiotic chemistry and habitability of early Mars. The Curiosity rover has measured highly variable and (13)C-depleted carbon isotopic values in early Martian organic matter whose origin is uncertain. One hypothesis suggests the deposition of simple organic molecules generated from (13)C-depleted CO derived from CO(2) photochemical reduction in the atmosphere. Here, we present a coupled photochemistry-climate evolution model incorporating carbon isotope fractionation processes induced by CO(2) photolysis, carbon escape, and volcanic outgassing in an early Martian atmosphere of 0.5-2 bar, composed mainly of CO(2), CO, and H(2) to track the evolution of the carbon isotopic composition of C-bearing species. The calculated carbon isotopic ratio in formaldehyde (H(2)CO) can be highly depleted in (13)C due to CO(2)-photolysis-induced fractionation and is variable with changes in atmospheric CO/CO(2) ratio, surface pressure, albedo, and H(2) outgassing rate. Conversely, CO(2) becomes enriched in (13)C, as estimated from the carbonates preserved in ALH84001 meteorite. Complex organic matter formed by the polymerization of such H(2)CO could explain the strong depletion in (13)C observed in the Martian organic matter. Mixing with other sources of organic matter would account for its unique variable carbon isotopic values.