Advertisement

If you have an ACS member number, please enter it here so we can link this account to your membership. (optional)

ACS values your privacy. By submitting your information, you are gaining access to C&EN and subscribing to our weekly newsletter. We use the information you provide to make your reading experience better, and we will never sell your data to third party members.

ENJOY UNLIMITED ACCES TO C&EN

Physical Chemistry

Methane Lakes On Titan

Cassini spacecraft finds long-predicted bodies of liquid

by Elizabeth K. Wilson
January 8, 2007 | A version of this story appeared in Volume 85, Issue 2

[+]Enlarge
Credit: NASA/JPL/USGS
In this false-color radar image, lakes dot the surface of Saturn's moon Titan. The lakes likely are filled with liquid methane.
Credit: NASA/JPL/USGS
In this false-color radar image, lakes dot the surface of Saturn's moon Titan. The lakes likely are filled with liquid methane.

It's official: The northern hemisphere of Saturn's giant moon Titan is dotted with liquid hydrocarbon lakes. The finding vindicates a long-standing prediction that Titan, shrouded in dense nitrogen and methane clouds, should also have reservoirs of liquid—likely methane—on its surface.

Images showing the lakes, taken by NASA's Cassini spacecraft as it scanned the northern area of Titan with its cloud-piercing radar, were initially released last July. Now, after detailed scrutiny, scientists are confident that they're seeing about 75 lakes, some enclosed by craterlike rims and some intersected with riverlike channels (Nature 2007, 445, 61).

"They have so many characteristics expected of lakes," says Ellen R. Stofan, a planetary scientist at Proxemy Research in Laytonsville, Md., who is on the Cassini radar team.

The discovery also adds weight to the idea that cold, dense methane on Titan participates in a cycle of evaporation and precipitation as does water here on Earth. "This is the first body we have found in the solar system besides Earth that has an active hydrologic cycle—only in Titan's case, the fluid is methane, not water," Stofan says.

Cassini, which has been orbiting Saturn since June 2004, provided the first detailed view of Titan's surface, but no lakes or oceans were seen initially. A small lander piggybacking on Cassini, the Huygens probe, touched down on Titan's surface two years ago, snapping pictures that showed an eroded, dry landscape with drainage channels that indicate liquid had once flowed there. Scientists began to wonder if Titan's methane source lay underground.

According to Cassini scientists, some of the depressions are formed by volcanism and some lakes may be fed by surface drainage and rainfall, whereas others, without river channels, may be fed by a subsurface methane table.

Cassini is scheduled to fly by Titan 22 more times. "But to really understand the chemistry of these lakes, we will need a follow-up lander mission to directly measure their composition," Stofan tells C&EN.

Advertisement

Article:

This article has been sent to the following recipient:

0 /1 FREE ARTICLES LEFT THIS MONTH Remaining
Chemistry matters. Join us to get the news you need.