Titan yields surprises

The Cassini spacecraft reveals strange cloud formations on Saturn's moon Titan.
By | Published: December 13, 2006
A full-disk Titan view reveals secrets about the new mountainous discoveries and how they tie into Titan’s past. Researchers believe the large, bright circular feature above center is the scar of an ancient impact basin. The prominent, long, dark feature above the impact scar may have resulted from tectonic activity caused by energy released by this impact – the same process that created the newly discovered mountains. This scenario begins to provide researchers with a potential global story for the geographical history of Titan, something that is just now emerging from the moon’s cloudy past.
NASA/JPL/University of Arizona
December 13, 2006
On Tuesday, scientists at the American Geophysical Union meeting in San Francisco announced significant new findings from Saturn’s moon Titan. The surprises include the moon’s largest known mountain range, which is coated with multiple layers of organic material; odd clouds that may be created like orographic clouds (those that form due to mountains) on Earth; and glimpses of a tectonic system on the moon that may explain how all these processes tie together in Titan’s history.

“We see a massive mountain range that kind of reminds me of the Sierra Nevada Mountains in the western United States,” says Bob Brown, team leader of the Cassini Visual and Infrared Mapping Spectrometer (VIMS). Brown presented his results along with Dennis L. Matson, Cassini’s project scientist, and Rosaly Lopes, Cassini radar team member.

Strange clouds are visible in this pair of images made during the October 25 Titan flyby. Cassini scientists emphasize the importance of combining high-resolution radar images with those taken by the Visible and Infrared Mapping Spectrometer (VIMS). This pair of images was made at a distance of 9,300 miles (15,000 km) from Titan and shows two views of the area riddled by mountain ranges. Note the bright band of clouds near the bottom of the right-hand image. These clouds probably resulted when methane in Titan’s atmosphere cooled and condensed into fog over the mountains, similar to the process that forms orographic clouds on Earth.
NASA/JPL/University of Arizona
The new results came from a flyby October 25, 2006, designed to yield the highest-resolution images yet taken of the enigmatic moon by Cassini. During this procedure, which allowed correlation of the VIMS data with radar data (to give the scientists more power to interpret features they saw), Brown, Lopes, and colleagues created images that resolve features on Titan as small as 1,300 feet (400 meters).

“You have to remember that Titan is the most earthlike place in the solar system,” says Lopes, “except it’s in a deep freeze.” If Titan were Earth, the newly discovered mountains would lie south of the equator, somewhere in New Zealand. They stretch 93 miles (150 kilometers) long, are about 19 miles (30 km) wide, and probably stand about nearly a mile (1.5 km) high. The mountains are surprising, in part, because Titan’s surface is clearly an active one that is relatively young, with active erosion and other processes going on. What could have created such a mammoth chain of mountains?

Processes that could have formed the mountains puzzled astronomers. So too did the nature of the mountains themselves. “These mountains are probably as hard as rock,” says Larry Soderblom, a Cassini team member at the U.S. Geological Survey, “made of icy materials, and are coated with different layers of organics.” Soderblom emphasizes the strange nature of what Cassini scientists know about the composition of the mountains. “There seem to be layers and layers of various coats of organic ‘paint’ on top of each other on these mountaintops,” he says, “almost like a painter laying the background on a canvas.”

A massive mountain range lying just south of Titan’s equator runs northwest-southeast through this newly released image from the Cassini spacecraft. The range, called by scientists “Titan’s Sierra,” extends 93 miles (150 km) long by 19 mi (30 km) wide. Cryogenic lava, a soup of ammonia and water, welling up from below as Titan’s crust was pulled apart tectonically probably created it. The image was created on October 25, 2006, during a flyby that returned Casssini’s highest-yet resolution views of the saturnian moon. The picture reveals features as small as 1,300 feet (400 meters) across.
NASA/JPL/University of Arizona
To heighten the mystery, Cassini scientists identified a series of dune-like features in and around the mountain range, and puzzle over what these dunes are made of. Although they do not yet know how all the puzzle pieces fit together, Brown and Lopes feel tectonic and volcanic processes are involved. An image shot October 9 reveals a circular feature they feel is an ancient impact scar, and a long, dark linear feature nearby, presumably a tectonic feature created from the impact’s energy. The scenario goes like this: Titan gets whacked by a large body, which punches through the moon’s crust. The impact creates the scar, and the dark tectonic feature and others formed as cryogenic lava flows upward. This is not lava anything like molten basalt on Earth, mind you — it’s “warm” only because it’s warmer than the frozen material around it, and it probably consists of a sludge containing ammonia, water, and possibly some methanol. The mountains form as a tectonic response to the impact, and dunes form too as material is pushed up and blows around. What are the dunes made of? The researchers don’t yet know. The dunes are colored like organic materials ought to be, but they might consist of ice coated by complex organic molecules, like chains of hydrocarbons.

Strangely, Brown and Lopes also found that weird clouds seem to form near the mountains, and “It’s difficult to explain,” says Brown, “how they do it.” After analyzing several scenarios, however, Brown feels the clouds form when methane is pushed over ridges, cools, and condenses. This produces a fog that resembles orographic clouds on Earth.

Excitingly, Brown suggests these results are giving Cassini scientists the first possibility of understanding an emerging geological picture of Titan. “Some problems require all the data from all the instruments,” he says. “But we won’t understand Titan geologically until we have data from both instruments at high resolutions.”