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Jupiter's Rings Are Shaped By Interplay Of Sunlight And Shadow

Date:
May 1, 2008
Source:
University of Maryland
Summary:
Astronomers appear to have solved a long-standing mystery about the cause of anomalies in Jupiter's gossamer rings. A faint extension of the outermost ring beyond the orbit of Jupiter's moon Thebe, and other observed deviations from an accepted model of ring formation, result from the interplay of shadow and sunlight on dust particles that make up the rings.

Jupiter's rings consist of bands of widely scattered dust particles generated by the impact of space debris into the planet's small inner moons, Adrastea, Metis, Amalthea and Thebe. This dust is organized into a main ring, an inner halo, and two fainter and more distant gossamer rings. The rings largely are bounded by the orbits of these four moons. However, a faint outward protrusion of dust (not show here) extends beyond the orbit of Thebe.
Credit: Courtesy NASA

Scientists from the University of Maryland and the Max-Planck Institute for Solar System Research in Germany appear to have solved a long-standing mystery about the cause of anomalies in Jupiter's gossamer rings.

In a new study published in the May 1 issue of Nature, they report that a faint extension of the outermost ring beyond the orbit of Jupiter's moon Thebe, and other observed deviations from an accepted model of ring formation, result from the interplay of shadow and sunlight on dust particles that make up the rings.

"It turns out that the outer ring's extended boundary and other oddities in Jupiter's rings really are 'made in the shade,'" said Douglas Hamilton, a professor of astronomy at the University of Maryland. " As they orbit about the planet, dust grains in the rings alternately discharge and charge when they pass through the planet's shadow. These systematic variations in dust particle electric charges interact with the planet's powerful magnetic field. As a result small dust particles are pushed beyond the expected ring outer boundary, and very small grains even change their inclination, or orbital orientation, to the planet."

Hamilton and German co-author Harald Krόger studied for the first time new impact data on dust grain sizes, speeds, and orbital orientations taken by the spacecraft Galileo during its traversal of Jupiter's rings in 2002-2003, as part of its deliberate maneuvering for a death plunge into the planet. Krόger analyzed the new data set and Hamilton created elaborate computer models that matched dust and imaging data on Jupiter's rings and explained the observed eccentricities.

" Within our model we can explain all essential structures of the dust ring we observed, " said Krόger.

According to Hamilton, the mechanisms identified in this paper effect the rings of any planet in any solar system, but the effects may not be as evident as it is at Jupiter. " The icy particles in Saturn's famous rings are too large and heavy to be significantly shaped by this process, which is why similar anomalies are not seen there," he said. " Our findings on the effects of shadow may also shed some light on aspects of planetary formation because electrically charged dust particles must somehow combine into larger bodies from which planets and moons are ultimately formed. "

Jupiter, Galileo and the Mystery of the Rings

Jupiter, the fifth planet from the Sun, has 63 known moons. The dust forming Jupiter's faint rings is produced when bits of space debris smashes into the small inner moons Adrastea, Metis, Amalthea and Thebe (listed closest to farthest). This dust is organized into a main ring, an inner halo, and two fainter and more distant gossamer rings. The rings largely are bounded by the orbits of these four moons, but a faint outward protrusion of dust extending beyond the orbit of Thebe (pronounced The-be) has, until now, mystified scientists.

Italian scientist Galileo Galilei was the first to discover that Jupiter had moons. Galileo first observed the planet's four largest moons in 1610.

On December 7, 1995 NASA's Galileo spacecraft reached Jupiter and began the first of 35 orbits around the planet. Over seven years the spacecraft took some 14, 000 images of Jupiter, its moons and rings. On September 21, 2003 the Galileo spacecraft was put into a controlled dive to end its mission, by plummeting through Jupiter's atmosphere. In addition to its imaging instruments, the spacecraft carried a supersensitive dust detector, which registered thousands of impacts from dust particles on its way through Jupiter's ring system in 2002 and 2003. The Thebe extension was one of the many new discoveries made by the Galileo spacecraft.


Story Source:

The above story is based on materials provided by University of Maryland. Note: Materials may be edited for content and length.


Cite This Page:

University of Maryland. "Jupiter's Rings Are Shaped By Interplay Of Sunlight And Shadow." ScienceDaily. ScienceDaily, 1 May 2008. <www.sciencedaily.com/releases/2008/04/080430134305.htm>.
University of Maryland. (2008, May 1). Jupiter's Rings Are Shaped By Interplay Of Sunlight And Shadow. ScienceDaily. Retrieved July 31, 2014 from www.sciencedaily.com/releases/2008/04/080430134305.htm
University of Maryland. "Jupiter's Rings Are Shaped By Interplay Of Sunlight And Shadow." ScienceDaily. www.sciencedaily.com/releases/2008/04/080430134305.htm (accessed July 31, 2014).

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