Saturn Today · About Us · Advertising · Comments Friday, November 16, 2012    
 

Advertisement
spacer
Home | Introduction - Quick Facts - Cassini Mission - Multimedia - News

SpaceRef | SpaceRef Europe - Mars Today - Mars TV

Saturn's Rings

The rings of Saturn have puzzled astronomers since Galileo Galilei discovered them with his telescope in 1610. Detailed study by the Voyager 2 and Voyager 2 spacecraft in the 1980s only increased the mystery.

There are thousands of rings made of up billions of particles of ice and rock. The particles range in size from a grain of sugar to the size of a house. The rings are believe to be pieces of comets, asteroids or shattered moons that broke up before they reached the planet. Each ring orbits at a different speed around the planet. Information from NASA's Cassini mission will help reveal how they formed, how they maintain their orbit and, above all, why they are there in the first place.

spacer
Saturn's rings.
Click for larger image.

While the other three gas planets in the solar system - Jupiter, Uranus and Neptune - have rings orbiting around them, Saturn's are by far the largest and most spectacular. With a thickness of about 1 kilometer (3,200 feet) or less, they span up to 282,000 km (175,000 miles), about three quarters of the distance between the Earth and its moon.

Named alphabetically in the order they were discovered, the rings are relatively close to each other, with the exception of the Cassini Division, a gap measuring 4,700 kilometers (2,920 miles). The main rings are, working outward from the planet, known as C, B, and A. The Cassini Division is the largest gap in the rings and separates Rings B and A. In addition a number of fainter rings have been discovered more recently. The D Ring is exceedingly faint and closest to the planet. The F Ring is a narrow feature just outside the A Ring. Beyond that are two far fainter rings named G and E. The rings show a tremendous amount of structure on all scales; some of this structure is related to gravitational perturbations by Saturn's many moons, but much of it remains unexplained.

To enter Saturn's orbit, Cassini will fly through the gap between the F and the G rings, farther from the planet than the Cassini Division. As a safe measure, during the crossing of the ring plane, instruments and cameras onboard the spacecraft will be shut off temporarily. However, the spectacular crossing into Saturn's orbit will bring incredible information, images and footage, while the instruments onboard will collect unique data that may answer many questions about the rings' composition.

Saturn's Rings
Ring Name: D
Distance*: 67000 km
,500 km

Ring Name: B
Distance*: 92000 km
,500 km
Thickness: 0.1 km - 1 km
Mass: 0.1 kg
Albedo: 0.65

Ring Name: A
Distance*: 122200 km
,600 km
Thickness: 0.1 km - 1 km
Mass: 0.1 kg
Albedo: 0.60

Ring Name: F
Distance*: 140210 km
km - 500 km

Ring Name: G
Distance*: 165800 km
,000 km
Thickness: 100 km - 1,000 km
Mass: 100 kg

Ring Name: E
Distance*: 180000 km
,000 km
Thickness: 1,000 km
Mass: 1,000 kg

* The distance is measured from the planet center to the start of the ring.

Source: NASA

Read a Newsletter Sample

spacer

Saturn Today Home | Introduction - Quick Facts - Cassini Mission - Multimedia - News

Other SpaceRef Sites: SpaceRef - SpaceRef Asia - SpaceRef Canada - SpaceRef Europe - Mars Today
Mars TV - Astrobiology - Space Wire - Space Elevator - Nano2Sol

Copyright © 1999-2012 SpaceRef Interactive Inc. All rights reserved. Privacy Policy
gipoco.com is neither affiliated with the authors of this page nor responsible for its contents. This is a safe-cache copy of the original web site.