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Hot Topic Solar System Saturn Saturn's Rings in Ultraviolet
 
Saturn's Rings in Ultraviolet
based on Univ. Colorado report
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Saturn
Posted:   07/08/04

Summary: Short-wavelength images of Saturn's rings are sensitive to ice content and show that the outer rings are higher in water-ice than inner ones. According to Colorado researchers, these spectra give clues to the ring's origins. The Cassini images in UV are ten times better than the previous best ring snapshots.

Saturn's Rings in Ultraviolet

saturn_magnet
This image shows the outer C and inner B rings respectively from left to right, with the inner B ring beginning a little more than halfway across the image. The general pattern is from "dirty" red particles to the denser ice shown in turquoise as the ringlets spread outward. Banner image: From the inside out, the "Cassini division" in faint red at left is followed by the A ring in its entirety. The A ring begins with a "dirty" interior of red followed by a general pattern of more turquoise as it spreads away from the planet, which indicates denser material made up of ice. The red band roughly three-fourths of the way outward in the A ring is known as the Encke gap Image Credit: NASA/JPL


The best view ever of Saturn's rings in the ultraviolet indicates there is more ice toward the outer part of the rings, hinting at ring origin and evolution, say two University of Colorado at Boulder researchers involved in the Cassini mission.

Researchers from CU-Boulder's Laboratory for Atmospheric and Space Physics, Joshua Colwell and Larry Esposito, said the UV spectra taken during the Cassini spacecraft's orbital insertion June 30 show definite compositional variation in the A, B and C rings.


Esposito, who discovered the F ring around Saturn in 1979 using Pioneer 11 data, is the team leader for Cassini's Ultraviolet Imaging Spectrograph, or UVIS, a $12.5 million instrument riding on the spacecraft. A UVIS team member and ring expert, Colwell created the color-enhanced images from the spectra.

The CU-Boulder built UVIS instrument is capable of resolving the rings to show features up to 60 miles across, roughly 10 times the resolution obtained by the Voyager 2 spacecraft. The instrument was able to resolve the "Cassini division," discovered by Giovanni Domenico Cassini in the 17th century, which separates the A and B rings of Saturn, proving the rings are not one contiguous feature.

The ring system begins from the inside out with the D, C, B and A rings followed by the F, G and E rings. The red in both images indicates sparser ringlets likely made of "dirty," and possibly smaller, particles than in the denser, icier turquoise ringlets.


Related Web Pages

Cassini
Saturn Edition, Astrobiology Magaz.
Cassini Closes In on Saturn
Saturn-- JPL Cassini Main Page
Lord of the Rings
Space Science Institute, Imaging Team Boulder, Colorado
Saturn: The Closest Pass
Voyager Image Query Form
David Seal's JPL site -Solar System Simulator
Gregory Benford's 1970 Essay 'View From Titan'


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