The King of Rings

Spitzer_ssc2009-19b_1024

spitzer_ssc2009-19b October 6th, 2009

Credit: NASA/JPL-Caltech

This diagram illustrates the extent of the largest ring around Saturn, discovered by NASA's Spitzer Space Telescope. The ring is huge, and far from the gas planet and the rest of its majestic rings.

The bulk of the ring material starts about six million kilometers (3.7 million miles) away from the planet and extends outward roughly another 12 million kilometers (7.4 million miles). The diameter of the ring is equivalent to 300 Saturns lined up side to side. The ring is thick too -- it's about 20 times as thick as the diameter of the planet. In fact, the entire volume of the ring is big enough to hold one billion Earths!

Saturn's newest halo is tilted at about 27 degrees from the main ring plane and encompasses the orbit of the moon Phoebe. Both the ring and Phoebe orbit in the opposite direction of Saturn's other rings and most of its moons, including Titan and Iapetus.

Why did it take so long to find something so big? The answer is that the ring is very tenuous, made up of a sparse collection of ice and dust particles. If you could transport yourself to the ring, you wouldn't even know you were there because the particles are so far apart. There's not a lot of sunlight out at Saturn, so this small density of particles doesn't reflect much visible light. Spitzer was able to spot the band because it sees infrared light, or heat radiation, from objects. Even though the ring material is very cold, it still gives off heat that Spitzer can see.

The discovery offers a possible solution to the mystery of the moon Iapetus. Years after Giovanni Cassini discovered Iapetus in 1671, he correctly deduced that one side of the moon is white and the other dark in a pattern that some say resembles the yin-yang symbol or a tennis ball. Astronomers think it is possible that the newfound ring, which orbits in the opposite direction of Iapetus, is the cause of the two-faced coloring. As the ring circles around, particles could be drifting inward and splattering the icy moon on the face like bugs on a windshield.

The pictures of Saturn, Phoebe and Iapetus were taken by NASA's Cassini spacecraft. The ring is an artist's illustration.

The size of Phoebe relative to Iapetus has been enlarged to better show Phoebe. Phoebe is about 200 kilometers (124 miles) in diameter, while Iapetus is about 1,500 kilometers (932 miles) across.

Provider: Spitzer Space Telescope

Image Source: http://www.spitzer.caltech.edu/images/2762-ssc2009-19b-The-King-of-Rings

Curator: Spitzer Space Telescope, Pasadena, CA, USA

Image Use Policy: Public Domain

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Image Details Image Details

Image Type
Artwork
Object Name
Saturn Phoebe Iapetus
Subject - Solar System
Planet > Ring
Planet > Type > Gas Giant
Planet > Satellite
Spitzer_ssc2009-19b_1280
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ID
ssc2009-19b
Subject Category
A.1.5.   A.1.1.2.   A.1.4.  
Subject Name
Saturn, Phoebe, Iapetus
Credits
NASA/JPL-Caltech
Release Date
2009-10-06
Lightyears
Redshift
Reference Url
http://www.spitzer.caltech.edu/images/2762-ssc2009-19b-The-King-of-Rings
Type
Artwork
Image Quality
Good
Distance Notes
Facility
Instrument
Color Assignment
Band
Bandpass
Central Wavelength
Start Time
Integration Time
Dataset ID
Notes
Coordinate Frame
Equinox
Reference Value
Reference Dimension
Reference Pixel
Scale
Rotation
Coordinate System Projection:
Quality
FITS Header
Notes
Creator (Curator)
Spitzer Space Telescope
URL
http://www.spitzer.caltech.edu
Name
Email
Telephone
Address
1200 E. California Blvd.
City
Pasadena
State/Province
CA
Postal Code
91125
Country
USA
Rights
Public Domain
Publisher
Spitzer Science Center
Publisher ID
spitzer
Resource ID
ssc2009-19b.tif
Metadata Date
2014-06-13
Metadata Version
1.1
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