ESA Science & Technology - Titan's dunes and other features emerge in new images

Cassini obtained the views during a close flyby of Titan on 25 July, when the spacecraft came as close as 976 kilometres from the giant moon. The spacecraft's radar instrument is able to penetrate the dense, global haze that surrounds Titan, to reveal fine details on the surface.

Flowing dunes of Shangri-La (denoised). Credit: NASA/JPL-Caltech/ASI/Universite Paris-Diderot

One of the new views (along with a short video) shows long, linear dunes, thought to be comprised of grains derived from hydrocarbons that have settled out of Titan's atmosphere. Cassini has shown that dunes of this sort encircle most of Titan's equator. Scientists can use the dunes to learn about winds, the sands they're composed of, and highs and lows in the landscape.

"Dunes are dynamic features. They're deflected by obstacles along the downwind path, often making beautiful, undulating patterns," said Jani Radebaugh, a Cassini radar team associate at Brigham Young University in Provo, Utah, USA.

Another new image shows an area nicknamed the "Xanadu annex" earlier in the mission by members of the Cassini radar team. Cassini's radar had not previously obtained images of this area, but earlier measurements by the spacecraft suggested the terrain might be quite similar to the large region on Titan named Xanadu.

First imaged in 1994 by the NASA/ESA Hubble Space Telescope, Xanadu was the first surface feature to be recognized on Titan. While Hubble was able to see Xanadu's outline, the annex area went unnoticed.

The new Cassini image reveals that the Xanadu annex is, indeed, made up of the same type of mountainous terrains observed in Xanadu and scattered across other parts of Titan.

The 'Xanadu Annex' on Titan (denoised). Credit: NASA/JPL-Caltech/ASI/Université Paris-Diderot

"This 'annex' looks quite similar to Xanadu using our radar, but there seems to be something different about the surface there that masks this similarity when observing at other wavelengths, as with Hubble," said Mike Janssen, a JPL member of the radar team. "It's an interesting puzzle."

Xanadu – and now its annex – remains something of a mystery. Elsewhere on Titan, mountainous terrain appears in small, isolated patches, but Xanadu covers a large area, and scientists have proposed a variety of theories about its formation.

"These mountainous areas appear to be the oldest terrains on Titan, probably remnants of the icy crust before it was covered by organic sediments from the atmosphere," said Rosaly Lopes, also a Cassini radar team member at JPL. "Hiking in these rugged landscapes would likely be similar to hiking in the Badlands of South Dakota."

The 25 July flyby was Cassini's 122nd encounter with Titan since the spacecraft's arrival in the Saturn system in mid-2004. It was also the last time Cassini's radar will image terrain in the far southern latitudes of Titan.

"If Cassini were orbiting Earth instead of Saturn, this would be like getting our last close view of Australia," said Stephen Wall, deputy lead of the Cassini radar team at NASA's Jet Propulsion Laboratory in Pasadena, California.

Cassini's four remaining Titan flybys will focus primarily on the liquid-filled lakes and seas in Titan's far north. The mission will begin its finale in April 2017, with a series of 22 orbits that plunge between the planet and its icy rings.

The Cassini-Huygens mission is a cooperative project of NASA, ESA, and the Italian Space Agency. JPL, a division of Caltech in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington. JPL designed, developed and assembled the Cassini orbiter. The radar instrument was built by JPL and the Italian Space Agency, working with team members from the U.S. and several European countries.

Contact

Preston Dyches
Jet Propulsion Laboratory, Pasadena, California
818-354-7013
preston.dychesjpl.nasa.gov

This article was originally published at: NASA's JPL Cassini website