‘Light Science’ Finds Titan Jet Stream

by Paul Gilster on January 25, 2007

When I interviewed the Jet Propulsion Laboratory’s James Lesh several years ago, he explained how space scientists could use radio signals to do science. It’s the ultimate technique for taking advantage of what’s at hand. If your spacecraft is moving behind a planet it’s investigating as seen from Earth, the changes to its signal as it disappears behind the disk tell you much about the composition of the planetary atmosphere. “One person’s noise,” said Lesh, “is another person’s signal.”

Of course, that kind of work isn’t limited to radio. Twice on November 14, 2003 Titan passed in front of a star, the events separated by just seven and a half hours. As you would expect, the occultation tracks were different, one visible from the Indian Ocean and southern Africa, the other from the Americas and western Europe. The effects of Titan’s atmosphere on the starlight have, in each case, supplied information about the movement of gases around the frigid world.

This work required observations from multiple locations, because what astronomers were looking for was the shape of the light focused by the gaseous lens of the atmosphere. “It is like the light falling through a glass of water and making bright patterns on the table. The focused light is not perfectly round because the glass is not a perfect lens,” says Bruno Sicardy (Observatoire de Paris). The triangular shape observed indicated an expected flattening of the atmosphere at the north pole, where warmer air from the south was cooling and sinking toward the surface.

Occluded light and Titan

Image: This artist’s impression shows the ‘light curve’ produced by a star passing behind Titan. When such occultation events take place, the light from the star is blocked out. Because Titan has a thick atmosphere, the light does not ‘turn off’ straight away. Instead, it drops gradually as the blankets of atmosphere slide in front of the star, as the light-curve drawn here shows. The way the light drops tells astronomers about the atmosphere of Titan. Credit: ESA. Image by C.Carreau.

The other discovery: a fast jet stream moving at about 720 kilometers per hour. The finding was quickly put to practical use, for the team was able to predict a temperature inversion near 510 kilometers altitude. Fourteen months later, the Huygens probe picked up the jolt of that layer on its accelerometers at precisely the suggested altitude, a validation of what James Lesh calls ‘light science.’ And while this finding relied on chance occultations, we’ll see spacecraft use targeted laser signaling for investigations of planetary atmospheres in the not distant future.

The paper on this work is Sicardy et al., “The two Titan stellar occultations of 14 November 2003,” Journal of Geophysical Research Vol. 111, E11S91 (18 November 2006). The abstract is here.

{ 2 comments }

asp06 January 25, 2007 at 10:09

to illustrate this phenomenon :

http://ao.jpl.nasa.gov/Palao/AdditionalResults.html

the first mpeg.

ljk February 1, 2007 at 15:46

Cassini Images Mammoth Cloud Engulfing Titan’s North Pole

A giant cloud half the size of the United States has been imaged on Saturn’s moon Titan by the Cassini spacecraft. The cloud may be responsible for the material that fills the lakes discovered last year by Cassini’s radar instrument.

Cloaked by winter’s shadow, this cloud has now come into view as winter turns to spring.

The cloud extends down to 60 degrees north latitude, is roughly 2,400 kilometers (1,490 miles) in diameter and engulfs almost the entire north pole of Titan.

The new image was acquired on Dec. 29, 2006, by Cassini’s visual and infrared mapping spectrometer. Scientific models predicted this cloud system, but it had never been imaged in such detail before.

The cloud image is available at: http://www.nasa.gov/cassini , http://saturn.jpl.nasa.gov , and http://wwwvims.lpl.arizona.edu .

“We knew this cloud had to be there but were amazed at its size and structure,” said Dr. Christophe Sotin of the University of Nantes, France, a member of the visual and infrared mapping spectrometer team and distinguished visiting scientist at NASA’s Jet Propulsion Laboratory, Pasadena, Calif. “This cloud system may be a key element in the global formation of organics and their interaction with the surface.”

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