PIA18417: Titan's Subsurface Reservoirs (Artist's Concept)
 Target Name:  Titan
 Is a satellite of:  Saturn
 Mission:  Cassini-Huygens
 Spacecraft:  Cassini Orbiter
 Product Size:  1800 x 1019 pixels (w x h)
 Produced By:  European Space Agency (ESA)
 Full-Res TIFF:  PIA18417.tif (5.505 MB)
 Full-Res JPEG:  PIA18417.jpg (230.1 kB)

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Figure 1
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This artist's rendering shows a cross-section of the surface and subsurface of Saturn's moon Titan, with a possible model for the structure of underground liquid reservoirs there.

Hundreds of lakes and seas are spread across the surface of Saturn's moon Titan -- its northern polar region in particular. These lakes are filled with hydrocarbons, a form of organic compound that is also found naturally on Earth and includes methane.

While most of the liquid in the lakes is thought to be replenished by rainfall from clouds in Titan's atmosphere, the cycling of liquid between the subsurface, surface and atmosphere is still not well understood.

Scientists have modeled how a subsurface reservoir of liquid hydrocarbons, also called an "alkanofer," once filled with methane rainfall runoff, would diffuse through Titan's porous, icy crust. They found that this diffusion could cause a new reservoir -- formed from clathrates -- to form where the bottom of the original underground reservoir meets layers of non-porous ice.

Clathrates are compounds that form a crystal structure with small cages that trap other substances like methane and ethane. Titan's subsurface clathrate reservoirs would interact with and the methane-rich liquid within the original underground hydrocarbon lake, slowly changing its composition. Eventually, subsurface alkanofers that come into contact with the clathrate layer would mainly be composed of either propane or ethane, depending on the type of clathrate that had formed.

Importantly, this process would continue up to Titan's surface. Lakes fed by these propane or ethane subsurface reservoirs would show the same kind of composition, whereas those fed by rainfall would be different and contain methane, nitrogen, and trace amounts of argon and carbon monoxide. In other words, the composition of the lake could indicate what is happening deep underground.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colo.

For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov and http://www.nasa.gov/cassini.

Image Credit:
ESA/ATG medialab

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