Titan Subsurface Reservoirs Artist Concept
Scientists modeled how methane rainfall runoff would interact with the porous, icy crust of Saturn moon Titan and found that a subsurface methane aquifer might have its composition changed over time due to the formation of materials called clathrates.
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Details
NASA ID
PIA18417
Date Created
September 3, 2014
Center
JPL
Media Type
image
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