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You are here:  Home / Science News / Mystery of Jupiter ring protrusion solved

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Mystery of Jupiter ring protrusion solved

Published: May 12, 2008 at 1:59 PM
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This NASA montage of images of Jupiter and its volcanic moon Io, was taken by the New Horizons spacecraft's flyby in early 2007. The Jupiter image is an infrared color composite taken by the spacecraft's near-infrared imaging spectrometer on Feb. 28, 2007. The Io image, taken on March 1, 2007, is a nearly true-color composite. The image shows a major eruption in progress on Io's night side, at the northern volcano Tvashtar. (UPI Photo/NASA)
This NASA montage of images of Jupiter and its volcanic moon Io, was taken by the New Horizons spacecraft's flyby in early 2007. The Jupiter image is an infrared color composite taken by the spacecraft's near-infrared imaging spectrometer on Feb. 28, 2007. The Io image, taken on March 1, 2007, is a nearly true-color composite. The image shows a major eruption in progress on Io's night side, at the northern volcano Tvashtar. (UPI Photo/NASA)

BALTIMORE, May 12 (UPI) -- German and U.S. scientists say they've determined why dust particles from one of Jupiter's faint rings sometimes travel beyond the rings' normal boundary.

Jupiter has 63 known moons, and the planet's faint rings are produced when debris from space collides with the four moons closest to the planet, researchers said. Although the rings are normally within the orbits of those moons, protrusions of dust sometimes extend beyond the orbit of Thebe -- the most-distant of the four closest moons.

The cause of the protrusions has been a long-standing mystery.

Now, Professor Douglas Hamilton of the University of Maryland and Harald Kruger of the Max-Planck Institute for Solar System Research in Germany say they've solved the mystery. Hamilton and Kruger analyzed data on dust grain sizes, speeds and orbital orientations taken by the spacecraft Galileo as it traversed Jupiter's rings in 2002 and 2003.

As they orbit Jupiter, "dust grains in the rings alternately discharge and charge when they pass through the planet's shadow," said Hamilton. The charged dust particles interact with Jupiter's powerful magnetic field, and "are pushed beyond the expected ring outer boundary," he said.

The study appeared in a recent issue of the journal Nature.



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