Saturn's Aurora

Summary (Aug 06, 2005): New images of Saturn obtained by a University of Colorado at Boulder-led team on June 21 using an instrument on the Cassini spacecraft show auroral emissions at its poles similar to Earth's Northern Lights.

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Saturn's Aurora

based on a CU-Boulder release

New ultraviolet images from Cassini spacecraft show auroral emissions at Saturn's poles. Credit: CU-Boulder

New images of Saturn obtained by a University of Colorado at Boulder-led team on June 21 using an instrument on the Cassini spacecraft show auroral emissions at its poles similar to Earth's Northern Lights.

Taken with the Ultraviolet Imaging Spectrograph aboard the Cassini orbiter, the two UV images, invisible to the human eye, are the first from the Cassini-Huygens mission to capture the entire "oval" of the auroral emissions at Saturn's south pole. They also show similar emissions at Saturn's north pole, according to CU-Boulder Professor Larry Esposito, principal investigator of the UVIS instrument built at CU-Boulder's Laboratory for Atmospheric and Space Physics, and Professor Wayne Pryor of Central Arizona College, a UVIS team member and former CU graduate student.

In the false-color images, blue represents aurora emissions from hydrogen gas excited by electron bombardment, while red-orange represents reflected sunlight. The images show that the aurora lights at the polar regions respond rapidly to changes in the solar wind, said the researchers. Previous images have been taken closer to the equator, making it difficult to see the polar regions.

Earth's northern lights. Jupiter, Saturn, Uranus, and Neptune are four planets in our solar system that experience visual light auroras. Image Credit: Michigan Tech

Major changes in the emissions inside the Saturn south-pole aurora are evident by comparing the two images, which were taken about one hour apart, they said. The brightest spot in the left aurora fades, and a bright spot appears in the middle of the aurora in the second image.

Made by slowly scanning the UVIS instrument across the planet, the images also contain more than 2,000 wavelengths of spectral information within each picture element. Researchers will use the wavelength information to study Saturn's auroras, gases, and hazes and their changing distributions.

The UVIS observation team includes researchers from CU-Boulder, NASA's Jet Propulsion Laboratory, Central Arizona College and the University of Southern California.

Related Web Pages

Cassini
Where is Cassini Now?
Saturn Edition, Astrobiology Magazine
University of Colorado, Boulder
The Martian Aurora
Jovian Lights
Charged Up Over Saturn

Note: Life and Giant Planets

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Saturday, August 06, 2005