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A Saturn moon feeds the planet's rings

The Cassini spacecraft has taken the most detailed temperature measurements to date of Saturn's rings. Data taken by the composite infrared spectrometer instrument on the spacecraft while entering Saturn's orbit show the cool and relatively warm regions of the rings. This false-color image shows that the temperatures on the unlit side of Saturn's rings vary from a relatively warm 110 Kelvin (-261 degrees Fahrenheit, shown in red), to a cool 70 Kelvin (-333 degrees Fahrenheit, shown in blue). The green represents a temperature of 90 Kelvin (-298 degrees Fahrenheit). Water freezes at 273 Kelvin (32 degrees Fahrenheit). (UPI Photo/NASA/JPL)
1 of 2 | The Cassini spacecraft has taken the most detailed temperature measurements to date of Saturn's rings. Data taken by the composite infrared spectrometer instrument on the spacecraft while entering Saturn's orbit show the cool and relatively warm regions of the rings. This false-color image shows that the temperatures on the unlit side of Saturn's rings vary from a relatively warm 110 Kelvin (-261 degrees Fahrenheit, shown in red), to a cool 70 Kelvin (-333 degrees Fahrenheit, shown in blue). The green represents a temperature of 90 Kelvin (-298 degrees Fahrenheit). Water freezes at 273 Kelvin (32 degrees Fahrenheit). (UPI Photo/NASA/JPL) | License Photo

GREENBELT, Md., Feb. 6 (UPI) -- U.S. scientists have determined ice being ejected from geysers on one of Saturn's moons is being captured by one of Saturn's rings.

Observations from the National Aeronautics and Space Administration's Cassini spacecraft show the ice geysers on Enceladus, one of Saturn's smaller moons, travel to the outer edge of Saturn's A-ring. Earlier research had shown the geysers adding material to Saturn's E-ring.

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"Saturn's A-ring and Enceladus are separated by 100,000 kilometers (62,000 miles), yet there's a physical connection between the two," said William Farrell of NASA's Goddard Space Flight Center in Greenbelt, Md. "Prior to Cassini, it was believed that the two bodies were separate and distinct entities, but Cassini's unique observations indicate that Enceladus is actually delivering a portion of its mass directly to the outer edge of the A-ring."

The study found material spewing from Enceladus becomes electrically charged plasma, and is captured by Saturn's magnetic field.

"This is an example of how Saturn's rings mitigate the overall radiation environment around the planet, sponging up low- and high-energy particles," said Farrell.

The study appears in the journal Geophysical Research Letters.

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