Go to Science@NASA home page

Saturn Hailstorm

An instrument onboard Cassini recorded a flurry of tiny particles pelting the spacecraft as it crossed Saturn's dusty ring plane.

NASA


Link to story audioListen to this story via streaming audio, a downloadable file, or get help.

see caption

July 9, 2004: When the Cassini spacecraft reached Saturn on June 30th, it dashed through a gap in Saturn's rings ... and then did it again. The double ring crossing was part of a maneuver required to put Cassini in orbit.

Although the ring gaps appeared empty, they weren't. Innumerable bits of ring-dust were waiting for Cassini, and they plowed into the spacecraft at a relative speed of approximately 20 km/s. That's 45,000 mph!


Sign up for EXPRESS SCIENCE NEWS delivery
"When we crossed the ring plane, we had roughly 100,000 total dust hits in less than five minutes," says Cassini science team member Don Gurnett of the University of Iowa. Fortunately the particles were small--"comparable in size to particles in cigarette smoke," he says. And most of the hits were to the spacecraft's tough high-gain antenna.

No damage was done, but it sounded exciting.

Each time a dust particle hit Cassini, the impact produced a puff of plasma--a tiny cloud of ionized gas. Cassini's Radio and Plasma Wave Science (RPWS) instrument was able to count these clouds; there were as many as 680 puffs per second. "We converted these into audible sounds that resemble hail hitting a tin roof," says Gurnett, the intrument's principal investigator. Click to listen: 2 MB Quicktime file.

The spacecraft reported no unusual activity due to the hits and performed flawlessly, successfully going into orbit around Saturn--a thrilling start to Cassini's four-year mission of exploration. More thrills are coming: visit the Cassini home page for updates.

SEND THIS STORY TO A FRIEND


Credits & Contacts
Author: Dr. Tony Phillips
Responsible NASA official: John M. Horack

Production Editor: Dr. Tony Phillips
Curator: Bryan Walls
Media Relations: Steve Roy

The Science and Technology Directorate at NASA's Marshall Space Flight Center sponsors the Science@NASA web sites. The mission of Science@NASA is to help the public understand how exciting NASA research is and to help NASA scientists fulfill their outreach responsibilities.


More Information

Cassini-Huygens Mission Home Page -- (JPL)

Titan's Surface Revealed -- (Science@NASA) Piercing the ubiquitous layer of smog enshrouding Titan, these images from the Cassini visual and infrared mapping spectrometer reveals an exotic surface covered with a variety of materials in the southern hemisphere.

Cassini RPWS: Radio and Plasma Wave Science -- (University of Iowa) home page describing the instrument that recorded the "hailstorm"

Orbital Insertion -- (Planetary Society) a nice overview of events around the time that Cassini reached Saturn

Credits: The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Office of Space Science, Washington, D.C. JPL designed, developed and assembled the Cassini orbiter.


Join our growing list of subscribers - sign up for our express news delivery and you will receive a mail message every time we post a new story!!!

Moresays 'NASA NEWS' Headlines


THE END