Climate Cycling on Early Mars Caused by the Carbonate-Silicate Cycle

TL;DR

This paper proposes a geophysical model explaining climate cycles on early Mars driven by the carbonate-silicate cycle, involving glaciation and deglaciation periods influenced by CO2 and H2 outgassing.

Contribution

It introduces a novel climate cycling model for early Mars that accounts for extended glaciation and warming periods, integrating the effects of CO2 and H2 outgassing.

Findings

Climate cycles with up to 10 million years of warm periods.

CO2 alone cannot deglaciate early Mars in the model.

H2 outgassing enhances greenhouse effect and climate variability.

Abstract

For decades, scientists have tried to explain the evidence for fluvial activity on early Mars, but a consensus has yet to emerge regarding the mechanism for producing it. One hypothesis suggests early Mars was warmed by a thick greenhouse atmosphere. Another suggests that early Mars was generally cold but was warmed occasionally by impacts or by episodes of enhanced volcanism. These latter hypotheses struggle to produce the amounts of rainfall needed to form the martian valleys, but are consistent with inferred low rates of weathering compared to Earth. Here, we provide a geophysical mechanism that could have induced cycles of glaciation and deglaciation on early Mars. Our model produces dramatic climate cycles with extended periods of glaciation punctuated by warm periods lasting up to 10 Myr, much longer than those generated in other episodic warming models. The cycles occur because stellar insolation was low, and because CO2 outgassing is not able to keep pace with CO2 consumption by silicate weathering followed by deposition of carbonates. While CO2 by itself is not able to deglaciate early Mars in our model, we assume that the greenhouse effect is enhanced by substantial amounts of H2 outgassed from Mars' reduced crust and mantle. Our hypothesis can be tested by future Mars exploration that better establishes the time scale for valley formation.