Grad Students Find Missing Link in Early Martian Water Cycle
- Researchers Mohammad Afzal Shadab and Eric Hiatt, pursuing their graduate studies at The University of Texas at Austin, have created a model to examine how water moved through early Mars’ surface down to underground aquifers.
- Their computer model simulates how water took between 50 and 200 years to seep from Mars’ surface down to an aquifer about a mile underground.
- The findings suggest much of Mars’ ancient water was trapped underground and less was available to replenish surface lakes, lakes, or the atmosphere through evaporation.
- Their model suggests that the underground water may have formed a reservoir at least 300 feet deep, and Hiatt noted that the water infiltrating the Martian crust was not escaping into space.
- This research revises Mars’ early hydrology picture, implying limited surface water stability and supporting future missions focused on subsurface water and astrobiology.
12 Articles
12 Articles
Missing link in early Martian water cycle discovered
Astronomers have filled a large gap in knowledge about Mars' water cycle. Their research on water percolating from surface to aquifer could change the picture of what early Mars was like, suggesting that less of the planet's water may have been available to become rain and refill lakes and oceans.
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