P065-0001
The Noachian Climate of Mars: Overview of Critical Mars System Science Questions
Abstract:
1) Planetary Origin: Location and growth rates; volatile budget; earliest bombardment history?
2) Crustal Formation & Evolution: Nature of magma ocean, its aftermath; primary/secondary crust formation; associated outgassing history?
3) Geodynamic Evolution & Petrogenetic History: Core formation, ensuing mantle convection patterns; magnetic field; redox state(s), petrogenetic evolution; timing, role of basins.
4) Primary & Secondary Atmospheres: Nature of each, transition, inheritance?
What was the nature and evolution of the Noachian climate?
1) Nature of Ancient Atmosphere & Climate: What were Noachian “ambient conditions”: ‘warm and wet’ or ‘cold and icy’? How did volatile species/quantities change with time; volcanic outgassing, relationship to evolving atmospheric pressure; nature/scale/duration of ambient climate perturbations; losses and influence on Mean Annual Temperature?
2) Candidate Climate Perturbations: Identify perturbations to the ambient atmosphere? Role of seasonal, spin axis/orbital variations, impacts, greenhouse gas input, hydrolysis, clouds, solar variability?
3) Water Cycle: Initial water inventory, changes with time; vertically integrated hydrological cycle; oceans? How was water partitioned (sources, sinks, D/H, loss to space)?
4) Sulfur Cycle: Total S budget, partitioning with time; nature of volcanic S exsolution with evolving atmospheric pressure; S cycle (sources, sinks, evolution); origin of Valles Marineris Interior Layered Deposits?
5) Mineralogy/Geomorphology Evolution & Implications: Causes of phyllosilicate/sulfate diversity of occurrences? Origin of salts/carbonates/silica-rich deposits? Relation to LN-H climate and weathering processes, rates. How are crater degradation and valley network/closed-basin/open-basin lake origin linked to LN-H mineralogy, climate?
6) Formation/Evolution of Life: Evolving paradigms include an ambient ‘cold and icy’ climate with warming perturbations: What strategies/proxies are needed to explore potential biotic environments on extremely cold surfaces above a warmer, wetter, geochemically active ‘Mars underground’?