NASA would like your attention long enough to explain a thing or two about how—
Icy aquifers on Saturn's moon Titan transform methane rainfall: go.nasa.gov/1t1BLOr @CassiniSaturn http://t.co/wmXCP9LG75—
(@NASA) September 04, 2014
—absolutely cool the Cassini-Huygens mission really is.
The NASA and European Space Agency Cassini mission has revealed hundreds of lakes and seas spread across the north polar region of Saturn’s moon Titan. These lakes are filled not with water but with hydrocarbons, a form of organic compound that is also found naturally on Earth and includes methane. The vast majority of liquid in Titan’s lakes is thought to be replenished by rainfall from clouds in the moon’s atmosphere. But how liquids move and cycle through Titan’s crust and atmosphere is still relatively unknown.
A recent study led by Olivier Mousis, a Cassini research associate at the University of Franche-Comté, France, examined how Titan’s methane rainfall would interact with icy materials within underground reservoirs. They found that the formation of materials called clathrates changes the chemical composition of the rainfall runoff that charges these hydrocarbon “aquifers.” This process leads to the formation of reservoirs of propane and ethane that may feed into some rivers and lakes.
And it doesn’t stop there.