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Cassini Wows The World With Saturn Ring Pictures
The first pictures taken by the Cassini spacecraft after it began orbiting
Saturn show breathtaking detail of Saturn’s rings, and other science measurements
reveal that Saturn’s magnetic field pulsed in size as Cassini approached
the planet.
“For years, we’ve dreamed about getting pictures like this. After
all the planning, waiting and worrying, just seeing these first images makes
it all worthwhile,” said Dr. Charles Elachi, Cassini radar team leader
and director of NASA’s Jet Propulsion Laboratory, Pasadena, CA. “We’re
eager to share these new views and the exciting discoveries ahead with people
around the world.”
The narrow angle camera on Cassini took 61 images soon after the main engine
burn that put Cassini into orbit. The spacecraft was hurtling at 15 kilometers
per second (about 34,000 miles per hour), so only pieces of the rings were
targeted.
“We won’t see the whole puzzle, only pieces, but what we are seeing
is dramatic,” said Dr. Carolyn Porco, Cassini imaging team leader, Space
Science Institute, Boulder, CO. “The images are mind-boggling, just mind-boggling.
I’ve been working on this mission for 14 years and I shouldn’t
be surprised, but it is remarkable how startling it is to see these images
for the
first time.”
After becoming the first spacecraft to enter Saturn's orbit, Cassini sent back this image of a portion of the panet's rings. It shows the sunlit side of the rings.
Some images show patterned density waves in the rings, resembling stripes
of varying width. Another shows a ring’s scalloped edge. “We do not
see individual particles but a collection of particles, like a traffic jam on
a highway,” Porco said. “We see a bunch of particles together, then
it clears up, then there’s traffic again.”
Other instruments on Cassini besides the camera have also been busy collecting
data. The magnetospheric imaging instrument took the first image of Saturn’s
magnetosphere. “With Voyager we inferred what it looked like, in the same
way that a blind man feels an elephant. Now we can see the elephant,” said
Dr. Tom Krimigis of Johns Hopkins Applied Physics Laboratory, laurel, MD, principal
investigator for the magnetospheric imaging instrument. The magnetosphere is
a bubble of energetic particles around the planet shaped by Saturn’s
magnetic field and surrounded by the solar wind of particles speeding outward
from the
sun.
“During approach to Saturn, Cassini was greeted at the gate,” said
Dr. Bill Kurth, deputy principal investigator for the radio and plasma wave science
instrument onboard Cassini. “The bow shock where the solar wind piles into
the planet's magnetosphere was encountered earlier than expected. It was as if
Saturn’s county line had been redrawn, and that was a surprise,” Cassini
first crossed the bow shock about three million kilometers (1.9 million miles)
from Saturn, which is about 50 percent farther from the planet than had been
detected by the Pioneer, Voyager 1 and Voyager 2 spacecraft that flew past
Saturn in 1979, 1980 and 1981.
The location of the bow shock varies with how hard the solar wind is blowing,
Kurth said. As the magnetosphere repeatedly expanded and contracted while
Cassini was approaching Saturn, the spacecraft crossed the bow shock seven
times
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