Titan’s Misty Mountains May Have “Roots As Nobody Sees”

A model of the layers of Titan  (Credit: A. Tavani)

Existing model of the layers of Titan (Credit: A. Tavani)

It’s been thought for some time that Saturn’s largest moon Titan has a complex internal structure consisting of multiple layers of ice and liquid water. At one point it was even suggested that there are water ice “cryovolcanoes” on Titan, where watery slush oozes to the surface and freezes solid in the moon’s 270-degree-below temperatures, in very much the same way that liquid rock does on Earth. Now, thanks to recent gravitational observations by Cassini (and who else?) some researchers think that Titan’s icy shell may be much thicker in places than once thought, making the existence of ice volcanoes and Earthlike plate tectonics much less likely.

An analysis of gravity and topography data from the Saturnian moon Titan obtained by NASA’s Cassini spacecraft suggests there could be something unexpected about the moon’s outer ice shell. The findings, published on Aug. 28 in the journal Nature, suggest that Titan’s ice shell could be rigid, and that relatively small topographic features on the surface could be associated with large ice “roots” extending into the underlying ocean.

The study was led by planetary scientists Douglas Hemingway and Francis Nimmo at the University of California, Santa Cruz, who used data from Cassini. The researchers were surprised to find a counterintuitive relationship between gravity and topography.

“Normally, if you fly over a mountain, you expect to see an increase in gravity due to the extra mass of the mountain,” said Nimmo, a Cassini participating scientist. “On Titan, when you fly over a mountain, the gravity gets lower. That’s a very odd observation.”

Wide-angle view of Titan's surface taken by the Huygens lander on Jan. 14, 2005 (ESA/NASA/JPL/University of Arizona)

Wide-angle view of Titan’s surface taken by the Huygens lander on Jan. 14, 2005 (ESA/NASA/JPL/University of Arizona)

One potential explanation is that each bump in the topography on the surface of Titan is offset by a deeper “root” that is big enough to overwhelm the gravitational effect of the bump on the surface. The root could act like an iceberg extending below the ice shell into the ocean underneath it. In this model, Cassini would detect less gravity wherever there is a big chunk of ice rather than water because ice is less dense than water.

“It’s like a big beach ball under the ice sheet pushing up on it, and the only way to keep it submerged is if the ice sheet is strong,” said Hemingway, the paper’s lead author and a Cassini team associate. “If large roots under the ice shell are the explanation, this means that Titan’s ice shell must have a very thick rigid layer.”

If these findings are correct, a thick rigid ice shell makes it very difficult to have ice volcanoes, which some scientists have proposed to explain other features seen on the surface. They also suggest that convection or plate tectonics are not recycling Titan’s ice shell, as they do with Earth’s geologically active crust.

Source: NASA/JPL

“What has roots as nobody sees,
Is taller than trees,
Up, up it goes,
And yet never grows?”

– One of Gollum’s riddles, The Hobbit*

*This is especially fitting considering these findings, as the IAU has approved the naming of features on Titan after people and places in Tolkien’s Middle Earth. Yes, there are actually Misty Mountains on Titan!


About Jason Major

Jason is a Rhode Island-based graphic designer, photographer, nature lover, space exploration fanatic, and coffee addict. In no particular order.

Posted on September 5, 2013, in Saturn's Moons and tagged , , , , , , , , , , , . Bookmark the permalink. 1 Comment.

  1. How interesting – and thanks for sharing the terrific graphic.


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