[meteorite-list] Ghostly Spokes in Saturn's Rings Spotted by Cassini

From: Ron Baalke <baalke_at_meteoritecentral.com>
Date: Fri Sep 16 20:50:48 2005
Message-ID: <200509170049.j8H0nbV14931_at_zagami.jpl.nasa.gov>

http://ciclops.org/view.php?id=1456

MEDIA RELATIONS OFFICE
CASSINI IMAGING CENTRAL LABORATORY FOR OPERATIONS (CICLOPS)
SPACE SCIENCE INSTITUTE, BOULDER, COLORADO
http://ciclops.org
media_at_ciclops.org

Preston Dyches (720) 974-5859
CICLOPS/Space Science Institute, Boulder, Colo.

For Immediate Release: September 16, 2005

GHOSTLY SPOKES IN SATURN'S RINGS SPOTTED BY CASSINI

Delighted scientists on the Cassini imaging team will be breaking out
the champagne in celebration of the first Cassini sighting of spokes,
the ghostly radial markings discovered in Saturn's rings by NASA's
Voyager spacecraft 25 years ago.

A sequence of images taken on the unilluminated side of the rings has
captured a few faint, narrow spokes in the outer B ring, about 3,500
kilometers long and about 100 kilometers wide (2,200 miles by 60 miles).
The images show the spokes as they march into the shadow of the planet
on the rings due to their orbital motion.

Dr. Carolyn Porco, Cassini imaging team leader at the Space Science
Institute in Boulder, Colo., and one of the first individuals to study
spokes in Voyager images, was attending the Division of Planetary
Sciences meeting in Cambridge, England, when she was informed of the
discovery by her staff members. "This is really a joy, and very
unexpected," she said. "It takes me back to my early days on the Voyager
mission."

The new Cassini images can be seen at: http://ciclops.org,
http://saturn.jpl.nasa.gov and http://www.nasa.gov/cassini.

According to the latest ideas, the visibility of spokes is believed to
depend on the elevation of the Sun above the rings, the less sunlight,
the more visible the spokes. For this reason, scientists weren't
expecting to see spokes until later in the mission when the sun angle is
low.

"We had convinced ourselves that conditions wouldn't be right for seeing
spokes on the lit side of the rings until about 2007," Porco said. "But
this finding seems to be telling us that conditions on the dark side of
the rings are almost as good right now for seeing spokes."

In Voyager images from 25 years ago, these narrow wedge-shaped features
typically extended 10,000 to 20,000 kilometers (6,200 to 12,400 miles)
radially outward across Saturn's B ring. When seen at low phase angles,
spokes appeared dark; when seen at high phase angles, they appeared
bright. This behavior indicated they were comprised of very small icy
particles, about the size of the wavelength of light. Since Voyager
days, spokes had been seen in images taken by NASA's Hubble Space
Telescope. The new Cassini images were taken at very high solar phase
angles, where small particles can brighten substantially, making them
more visible.

Porco's analysis of spokes in the early 1980s found that these narrow
arrangements of small particles came and went with a period equal to
that of the powerful bursts of radio waves, called Saturn Kilometric
Radiation (SKR), discovered by Voyager and coming from Saturn's magnetic
field. This association indicated that spokes were a phenomenon
involving electromagnetic effects and partly connected to Saturn's
magnetic field.

Of intense interest will be a Cassini determination of the periodicity
in the appearance of spokes. This will require monitoring spoke activity
from a variety of geometries over several years. "Cassini has found that
the SKR period has changed since Voyager, which though hard to believe,
may mean that the rotation of Saturn's interior has changed," said
Porco. "That would be a finding of enormous consequence, so, we'll be
looking very closely to see if the frequency of spoke activity has
changed too."

There is no commonly accepted theory for the creation of spokes. Some
ideas suggest that spokes result from meteoroid impacts onto the rings;
others suggest that they are created by instability in the magnetosphere
near the rings.

Whatever the cause, imaging team members will study the new spoke images
and maintain their vigil for additional spoke sightings. Viewing
conditions on the dayside are expected to improve toward the end of
Cassini's nominal four-year mission, as Saturn continues in its nearly
30-year orbit and the Sun's angle above the rings continues to drop.

The Cassini-Huygens mission is a cooperative project of NASA, the
European Space Agency and the Italian Space Agency. The Jet Propulsion
Laboratory (JPL), a division of the California Institute of Technology
in Pasadena, manages the Cassini-Huygens mission for NASA's Science
Mission Directorate, Washington. The Cassini orbiter and its two onboard
cameras were designed, developed and assembled at JPL. The imaging team
consists of scientists from the U.S., England, France, and Germany. The
imaging operations center and team leader (Dr. C. Porco) are based at
the Space Science Institute in Boulder, Colo.

-end-
Received on Fri 16 Sep 2005 08:49:36 PM PDT