| Abstrakt: |
Near the Noachian‐Hesperian boundary (∼3.6 billion years ago), most of Mars' near‐surface water inventory was likely frozen in large southern ice sheets and Mars' CO2 atmosphere had eroded enough that it began to periodically collapse. Here, I report model results showing that thermal blanketing of a southern H2O ice sheet by a CO2 ice cap formed during atmospheric collapse would produce melt equivalent to ∼0.2–2.0 × Mars' present‐day global near‐surface H2O inventory. I then model downstream flow, demonstrating the likely development of an ice‐covered fluviolacustrine system with 1,000s‐of‐kilometer‐long rivers, an overtopped Mediterranean‐Sea‐sized lake in Argyre Basin, and substantial water delivery into Margaritifer Terra and potentially Chryse Planitia. This study shows that a steady‐state hydrologic cycle driven by pole‐to‐equator melt and equator‐to‐pole sublimation and atmospheric transport lasting 105–107 year could occur multiple times throughout a ∼108‐year window during which atmospheric pressure was low enough to collapse yet CO2 and H2O inventories and geothermal heat output were high enough to produce substantial meltwater. The nature of this proposed hydrologic cycle is consistent with estimates of the timing, duration, and intermittency of Noachian‐Hesperian fluvial activity. Thus, meltwater release triggered by atmospheric collapse potentially played an important role in the intense pulse of Noachian‐Hesperian fluvial activity: directly so for the Argyre‐Margaritifer‐Chryse system and perhaps indirectly for other catchments. Finally, this study demonstrates that large amounts of water can mobilize in a cold climate, driven by the same atmospheric collapse process occurring on Mars today, without invoking late‐stage warming processes. Plain Language Summary: Approximately 3.6 billion years ago, most of Mars' water was likely frozen in large southern ice sheets and Mars' atmosphere had thinned to the point that it began to collapse, periodically forming a massive south polar CO2 ice cap. I model the thermal blanketing effect of the CO2 ice cap overlying the water ice sheets, demonstrating that it leads to massive meltwater liberation. I also model downstream meltwater, showing that it flowed through 1,000‐km‐long, ice‐covered rivers, filling and then overtopping an ice‐covered lake in Argyre Basin with approximately the volume of the Mediterranean Sea, eventually emptying 8,000 km away into the northern plains. This is the first model that produces enough water to overtop Argyre, consistent with decades‐old geologic observations. Basal melting events likely occurred multiple times, 0.1‐to‐10 million years at a time, during a one‐hundred‐million‐year era about 3.6 billion years ago. Water sublimed downstream likely returned to the south polar cap, perpetuating a pole‐to‐equator hydrologic cycle that may have played an important role in Mars' enigmatic pulse of late‐stage intense fluvial activity. Finally, this study demonstrates that large amounts of water can mobilize in a cold climate without invoking the fraught paradigm of late‐stage climatic warming. Key Points: Collapsing Mars' atmosphere onto an ice sheet ∼3.6 billion years ago can melt and liberate about half of Mars' water inventoryMeltwater feeds an ice‐covered fluviolacustrine system with 1,000s‐km‐long rivers and a breached Mediterranean‐Sea‐sized Argyre Basin lakeThis hydrologic process was likely important for Mars' intense Noachian‐Hesperian fluvial period and does not require late‐stage warming [ABSTRACT FROM AUTHOR] |
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