Rings Made in the Shade

Summary (May 03, 2008): Scientists may have solved a long-standing mystery about anomalies in Jupiter's rings. The finding provides new information about the Jovian system and may yield clues about planetary formation.

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Rings Made in the Shade

Based on a University of Maryland at College Park news release

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.

Jupiter's rings are seen in a mosaic of five images taken by the Solid State Imaging camera aboard NASA's Galileo spacecraft.
Credit: NASA JPL

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."

Giant Red Spot in background, one of Jupiter's moon in foreground with eclipse shadow cast on gas giant
Credit: NASA/JPL Cassini

Hamilton and German co-author Harald Kruger 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. Kruger 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 Kruger.

According to Hamilton, the mechanisms identified in this paper affect 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."

Understanding the behavior of Jupiter's rings is also important in determining how they interact with the planet's moons. Jupiter is not a planet expected to harbor life, but its moons are of interest to astrobiologists. For instance, Europa is thought to contain a subsurface ocean that could potentially be a habitat for life.

Jupiter, Galileo and the Mystery of the Rings

Life and Giant Planets Briefing
* The surface composition of Europa, one of Jupiter's moons, is water ice
* Surface temperature is -260 F (-162 C)
* This ice layer may be 4 miles (7 km) thick
* Magnetic fluctuations suggest conducting liquid flows
* High tide is 30 meters (or 100 feet)
* On Ganymede, another of Jupiter's moons, the salty ocean may lie beneath an ice layer that is 150 kilometers (90 miles) thick
Credit: NASA

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 (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 (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. It also released a probe that sent back the information on the planet's atmosphere. 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.

The overall Galileo mission was managed by NASA's Jet Propulsion Laboratory (JPL), which also built its main (orbiter) spacecraft.

Related Web Sites

Astrobiology Roadmap Goal 1: Habitable Planets
Astrobiology Roadmap Goal 2: Life in Our Solar System
The End of Galileo
Long Journey's End
Jupter: Moon Festival
Galileo's Spyglass
Swimming a Salty Sea

Note: Life and Giant Planets

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Saturday, May 03, 2008