P065-0002
Rainfall, snowfall, and fluvial activity on early Mars
Abstract:
We present results from our recent and ongoing works in which we implement a 3D Global Climate Model (GCM) to answer the questions: What is the nature of rainfall in a canonical “warm and wet” climate (global mean annual temperature, GMAT, ~273 K)? Is the distribution of VNs/lakes more consistent with the model-predicted distribution of fluvial activity in a “warm and wet” or “cold and icy” climate? And, finally, if rainfall was responsible for VN/lake formation, not snowmelt, what climate characteristics (e.g. GMAT), are required for widespread rainfall to occur in all areas where VNs/lakes are distributed?
We assume present-day topography [e.g. 1] and a relevant Noachian surface water inventory of ~34 m GEL [e.g. 2] and show that:
- In a canonical “warm and wet” climate (GMAT ~273 K), rainfall is negligible and precipitation and fluvial activity would be dominated by snowfall and melting [e.g. 3].
- The distribution of VNs/lakes is more consistent with the distribution of model-predicted fluvial activity in a “cold and icy” climate than in a “warm and wet” climate.
- GMAT >285 K is required for widespread rainfall to occur [e.g. 4].
In summary, we have shown that either (1) snow accumulation and melting was responsible for VN/lake formation or (2) GMAT was >285 K and widespread rainfall was responsible for VN/lake formation.
[1] Smith et al. (1999), Science 284, p1495.
[2] Carr and Head (2015), GRL 42, 2014GL062464.
[3] Palumbo and Head (2018), GRL 45, 2018GL079767.
[4] Palumbo and Head, In review at Icarus Note.