Saturn's Moon - Titan - Is Glowing In The Dark From Deep In Its Atmosphere

append delete sky... - Imaging cameras on NASA's Cassini spacecraft has photographed Saturn’s moon Titan “glowing in the dark.”

The images were taken by the Cassini spacecraft while Titan was behind Saturn, in eclipse from the sun.

They present a visible glow emanating from both the top of Titan’s atmosphere and from deep in its atmosphere.

The glow is only a millionth of a watt, and was detected using long exposure photographs.

This set of images from NASA's Cassini spacecraft shows Saturn's moon Titan glowing in the dark. Titan was behind Saturn at the time, in eclipse from the sun. The image on the left is a calibrated, but unprocessed image from Cassini's imaging camera.

The image on the right was processed to exclude reflected light off Saturn and it is clear that even where Titan did not receive any Saturnshine, it is still emitting light. Some light appears to be emanating from high in the atmosphere (noted by the outer dashed line at about 625 miles or 1,000 kilometers in altitude). But more surprisingly, most of it is diffusing up from lower down in the moon's haze, from about 190 miles (300 kilometers) above the surface. Image credit: NASA/JPL-Caltech/SSI

“It turns out that Titan glows in the dark – though very dimly,” said Robert West, lead author of a recent study in the journal Geophysical Research Letters and a Cassini imaging team scientist at NASA’s Jet Propulsion Laboratory.

It’s a little like a neon sign, where electrons generated by electrical power bang into neon atoms and cause them to glow. Here we’re looking at light emitted when charged particles bang into nitrogen molecules in Titan’s atmosphere.

Scientists are studying the input of energy from the sun and charged particles into Titan's atmosphere because it is at the heart of the natural organic chemistry factory that exists in Titan's atmosphere.

"Scientists want to know what galvanizes the chemical reactions forming the heavy molecules that develop into Titan's thick haze of organic chemicals," said Linda Spilker, Cassini project scientist, also at JPL.

This kind of work helps us understand what kind of organic chemistry could have existed on an early Earth.

The airglow, is produced when atoms and molecules are excited by ultraviolet sunlight or electrically charged particles.

Cassini scientists have already seen an airglow from Titan's nitrogen molecules caused by X-rays and ultraviolet radiation from the sun when Titan was illuminated by the sun.

During 2009, Titan passed through Saturn's shadow, offering a unique opportunity for Cassini instruments to observe any luminescence from Titan while in darkness.
Cassini's imaging cameras could see in very dim light by using exposure times of 560 seconds.

Scientists' best guess is that the glow is being caused by deeper-penetrating cosmic rays or by light emitted due to some kind of chemical reaction deep in the atmosphere.

The round form near the center of Titan, as imaged by Cassini in October 2006, may be an old impact basin. Credits: NASA/JPL, Univ. of AZ, ESA, and USGS)

"This is exciting because we've never seen this at Titan before," West said. "It tells us that we don't know all there is to know about Titan and makes it even more mysterious."

Scientists have previously reported that the nightside Venus atmosphere also produces a glow, called the Ashen light. Some have suggested that lightning on Venus is responsible, although that explanation is not universally accepted.

While Cassini's radio wave instrument has detected lightning at Saturn, it has not detected lightning at Titan. Scientists plan to keep looking for clues as Cassini continues to make its way around the Saturn system for another season.

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