Free Newsletter
Register for our Free Newsletters
Newsletter
Zones
Advanced Composites
LeftNav
Aerospace
LeftNav
Amorphous Metal Structures
LeftNav
Analysis and Simulation
LeftNav
Asbestos and Substitutes
LeftNav
Associations, Research Organisations and Universities
LeftNav
Automation Equipment
LeftNav
Automotive
LeftNav
Biomaterials
LeftNav
Building Materials
LeftNav
Bulk Handling and Storage
LeftNav
CFCs and Substitutes
LeftNav
Company
LeftNav
Components
LeftNav
Consultancy
LeftNav
View All
Other Carouselweb publications
Carousel Web
Defense File
New Materials
Pro Health Zone
Pro Manufacturing Zone
Pro Security Zone
Web Lec
Pro Engineering Zone
 
 
 
News

Instrument detects particles near Saturn

University Of Chicago : 27 May, 2007  (Technical Article)
An instrument designed and built at the University of Chicago for the Cassini space probe has discovered dust particles around Enceladus, an ice-covered moon of Saturn that has the distinction of being the most reflective object in the solar system. The particles could indicate the existence of a dust cloud around Enceladus, or they may have originated from Saturn
“We are operating on the plane of the E-ring, and things are very complicated there,” said Thanasis Economou, a Senior Scientist at the University of Chicago’s Enrico Fermi Institute. “It will take a few more flybys to distinguish the dust flux originating from the E-ring as opposed to one around Enceladus.”

The discovery is the first for the Chicago instrument, called the High Rate Detector. “During all this time from Earth to Saturn, we didn’t have any real test of the instrument. I was very happy to see that the instrument performs well after so many years,” Economou said.

Cassini encountered Enceladus at an altitude of 733 miles on Feb. 17. On that date, the Chicago instrument recorded thousands of particle hits during a period of 37 and a half minutes. Cassini executed another flyby of Enceladus at an altitude of 311 miles. “Again we observed a high stream of dust particles,” Economou said.

The largest particles detected by the Chicago instrument measure no more than the diameter of a human hair, too small to pose any danger to Cassini. “Our measurements are important to evaluate any risk to the spacecraft,” Economou said.

The HRD is part of a larger instrument, the Cosmic Dust Analyzer, which with further analysis may be able to determine whether the particles are made of ice or dust. Enceladus measures 310 miles in diameter and reflects nearly 100 percent of the light that hits its ice-covered surface.

“If you look at the surface on Enceladus, it’s very smooth,” Economou said, and varies little in altitude. Scientists have speculated that Enceladus is the source of Saturn’s E-ring, the planet’s widest, stretching 188,000 miles. It is possible, the scientists say, that gravitational interactions between Enceladus and another moon of Saturn have triggered some form of water volcanism.

“The High Rate Detector measurements are extremely important in order to understand the role of Enceladus as the source of the water ice particles in the E-ring,” said Ralf Srama of Germany’s Max Planck Institute for Nuclear Physics, who heads the Cosmic Dust Analyzer science team. This study requires precise measurements of dust density in the Enceladus region, “but without the High Rate Detector this would not be possible,” Srama said.

Enceladus orbits Saturn at a distance of approximately 147,500 miles, almost two-thirds the distance from Earth to the moon. Only one of Saturn’s 31 known moons is closer to the planet.

The HRD was created by Anthony Tuzzolino, Senior Scientist in the Enrico Fermi Institute, under the direction of the late John Simpson, the Arthur Holly Compton Distinguished Service Professor Emeritus in Physics. The HRD was designed to collect data on Saturn’s rings and is capable of counting up to 100,000 impacts per second.

Cassini carries a total of 12 primary instruments that often must compete with one another so that the orbiter is properly oriented for collecting their data. “We did our best in order to make this happen, and the preparations and negotiations for these encounters were enormous,” Srama said. “These were perfect flybys, and we did everything possible.”
Bookmark and Share
 
Home I Editor's Blog I News by Zone I News by Date I News by Category I Special Reports I Directory I Events I Advertise I Submit Your News I About Us I Guides
 
   Â© 2012 NewMaterials.com
Netgains Logo