Warming Early Mars with Climate Cycling: The Effect of CO2-H2 Collision-induced Absorption
arXiv:2004.09076 · doi:10.1016/j.icarus.2020.113770
Abstract
Explaining the evidence for surface liquid water on early Mars has been a challenge for climate modelers, as the sun was ~30% less luminous during the late-Noachian. We propose that the additional greenhouse forcing of CO2-H2 collision-induced absorption is capable of bringing the surface temperature above freezing and can put early Mars into a limit-cycling regime. Limit cycles occur when insolation is low and CO2 outgassing rates are unable to balance with the rapid drawdown of CO2 during warm weathering periods. Planets in this regime will alternate between global glaciation and transient warm climate phases. This mechanism is capable of explaining the geomorphological evidence for transient warm periods in the martian record. Previous work has shown that collision-induced absorption of CO2-H2 was capable of deglaciating early Mars, but only with high H2 outgassing rates (greater than ~600 Tmol/yr) and at high surface pressures (between 3 to 4 bars). We used new theoretically derived collision-induced absorption coefficients for CO2-H2 to reevaluate the climate limit cycling hypothesis for early Mars. Using the new and stronger absorption coefficients in our 1-dimensional radiative convective model as well as our energy balance model, we find that limit cycling can occur with an H2 outgassing rate as low as ~300 Tmol/yr at surface pressures below 3 bars. Our results agree more closely with paleoparameters for early martian surface pressure and hydrogen abundance.
Publication date July 15 2020
References in corpus (7)
- Global modelling of the early Martian climate under a denser CO2 atmosphere: Water cycle and ice evolution
- The faint young Sun problem
- Warming early Mars with CO2 and H2
- A warmer and wetter solution for early Mars and the challenges with transient warming
- Testing the Early Mars H2-CO2 Greenhouse Hypothesis with a 1-D Photochemical Model
- Climate Cycling on Early Mars Caused by the Carbonate-Silicate Cycle
- Mars Obliquity History Constrained by Elliptic Crater Orientations
Cited by in corpus (6)
- Thermodynamic and Energetic Limits on Continental Silicate Weathering Strongly Impact the Climate and Habitability of Wet, Rocky Worlds
- Can Volcanism Build Hydrogen-Rich Early Atmospheres?
- Did Mars possess a dense atmosphere during the first ~400 million years?
- An Energy Balance Model for Rapidly and Synchronously Rotating Terrestrial Planets
- The influence of surface condensation on the evolution of warm and cold rocky planets orbiting Sun-like stars
- 3-D Global modelling of the early martian climate under a dense CO2+H2 atmosphere and for a wide range of surface water inventories