NASA / JPL / Space Science Institute
NASA’s Cassini spacecraft chronicled the change of seasons as it captured clouds concentrated near the equator of Saturn’s largest moon, Titan, on Oct. 18, 2010.
updated 4/11/2011 3:47:00 PM ET 2011-04-11T19:47:00

Just a few months after scientists presented tantalizing evidence of ice volcanoes reshaping the surface of Titan, the largest moon of Saturn, a new study is throwing some cold water on the prospect.

In the new study, a team of scientists say Titan's identifiable surface features were likely created by weather or other external forces — meteorite strikes, wind and rain — rather than volcanic activity. This suggests that the huge moon's interior may be cool and dormant, incapable of causing active ice volcanoes, also known as cryovolcanoes.

"It would be fantastic to find strong evidence that clearly shows Titan has an internal heat source that causes ice volcanoes and lava flows to form," study lead author Jeff Moore of NASA's Ames Research Center in Moffett Field, Calif., said in a statement released April 7. "But  we find that the evidence presented to date is unconvincing, and recent studies of Titan's interior conducted by geophysicists and gravity experts also weaken the possibility of volcanoes there."

Ice volcanoes on Titan?
Last December, researchers studying observations from NASA's Cassini spacecraft announced that they had found solid evidence of ice volcanoes on Titan.  

The scientists pointed to a region near a Titan landform called Sotra Facula, which appeared to have three large conical features with material flowing outward from them, as well as several deep pits. These signs all pointed to recently active ice volcanoes, the researchers said at the time.

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Icy cryovolcanoes are known to exist on the Saturn moon Enceladus, and some researchers think they may be common on the frigid satellites of the outer solar system. While the new study — which looked at more Cassini observations — doesn't comment directly on the Sotra Facula analysis, it concludes that the weight of the evidence points to no ice volcanoes on Titan.

No exotic explanations are needed to account for Titan's observable landforms, according to the new study. Rather, researchers said, Titan's surface looks a lot like that of the Jupiter moon Callisto — which almost certainly lacks cryovolcanoes because of its cool interior.

"Every feature we have seen on Titan can be explained by wind, rain and meteorite impacts, rather than from internal heating," Moore said.

The researchers report their results in the April 2011 edition of the journal Icarus.

Further study needed
Titan is the only moon known to have a dense atmosphere, which is composed primarily of nitrogen. It's a frigid, fascinating place with a methane-based weather system: Methane rain falls, pooling in liquid-methane lakes.

Titan's dense atmosphere makes its surface difficult to study with visible-light cameras, but Cassini's infrared instruments and radar signals can peer through the haze. So the probe will continue scrutinizing Titan, helping researchers better understand just what processes are shaping the surface of the huge moon.

For now, the jury may be out.

"Titan is a fascinating world," said study co-author Robert Pappalardo, a research scientist at NASA's Jet Propulsion Laboratory in Pasadena, Calif. "Its uniqueness comes from its atmosphere and organic lakes, but in this study, we find no strong evidence for icy volcanism on Titan."

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