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2001 News Releases

Galileo Gets One Last Close Encounter with Jupiter's Callisto
May 22, 2001

Landslides inside craters on Jupiter's moon Callisto
Landslides inside craters on Jupiter's moon Callisto
Go to Animation

       On a third and final tour of duty in the Jovian system, NASA's dauntless Galileo spacecraft makes its closest pass yet to Jupiter's outermost large moon.

       Friday, May 25, the orbiter should skim over Callisto, at an altitude of about 123 kilometers, or 76 miles, at 4:24 a.m. PDT. If Callisto were the size of a baseball, that would be just a nickel's thickness away.

       Mission managers expect the pull of the moon's gravity to alter Galileo's orbit around Jupiter. "The main reason we're flying so close to Callisto is to set up flybys of Io," said Dr. Eilene Theilig, Galileo project manager at NASA's Jet Propulsion Laboratory (JPL), Pasadena, Calif. Io is an intensely volcanic moon closer to Jupiter that continually resurfaces itself with fiery eruptions.

       Galileo will pass over polar regions of Io in August and October to help scientists determine if the seething and violent moon generates its own magnetic field. "Since we have to go close to Callisto anyway to get to Io, we'll take advantage of the opportunity for studying Callisto," said JPL's Dr. Torrence Johnson, Galileo project scientist.

       Unlike the planet's other large moons, Callisto, which is about as big as the planet Mercury, appears to be inactive and still bears craters billions of years old.

       Although earlier magnetic studies by Galileo indicated that Callisto may have a liquid saltwater layer deep beneath its surface, Callisto hasn't drawn the excitement generated by Io or its sister moon Europa, which appears to have liquid water closer to its surface, or two-toned Ganymede.

       "Callisto is sort of the ugly duckling of the moons, but it's the one we need to look at to get the bombardment history of the Jovian system," Johnson added. "The craters on Callisto are the visible record of what sizes of comets and other objects have pelted Jupiter and its moons with what frequency over the past four billion years."

       Data from the flyby will be transmitted to Earth over the next two months. Scheduled observations include high-resolution imaging to study the density of small craters and the details of how some features appear to be degraded or eroded, said Dr. Duane Bindschadler, leader of Galileo's science planning team. "Some earlier imaging of Callisto has shown fewer small craters than expected."

       Scientists also plan to snap new pictures of Io, though from a much greater distance than Callisto, and hope to see if a volcanic plume detected near Io's North Pole five months ago is still active. On Aug. 5, Galileo will pass directly over the plume's source area at an altitude of less than 350 kilometers, or about 220 miles.

       Another set of planned observations this week will point at Jupiter. Galileo will make a map of Jupiter's clouds in infrared wavelengths. "One goal is to see if fresh clouds are still being made at the same types of locations they were during similar mapping more than five years ago," said Dr. Kevin Baines, JPL atmospheric scientist. Another is to check for "brown barges," a type of dark cloud that was prominent on Jupiter when NASA's two Voyager spacecraft flew by in 1979, but has not been seen during the years since Galileo began orbiting Jupiter in 1995. Baines believes recent observations from Earth-based telescopes hint at a return of brown barges.

       Galileo's mission was originally scheduled to end in 1997, but has been extended repeatedly as the spacecraft continues to return scientific discoveries. The orbiter has survived more than three times the cumulative radiation exposure it was designed to withstand. Some electronic components have been affected by the radiation, and each swing near Jupiter increases the odds of more serious damage from exposure to the radiation belts around the planet.

       Galileo has made 30 previous flybys of Jupiter's large moons, including seven of Callisto. Before reaching Jupiter, it made close passes of Venus, Earth and two asteroids. After three more encounters with Io and one with the small inner moon Amalthea, Galileo's mission will end in 2003 with a final plunge into the crushing pressure of Jupiter's atmosphere.

       JPL, a division of the California Institute of Technology in Pasadena, manages Galileo for NASA's Office of Space Science, Washington, DC. Additional information about the Galileo, Jupiter and Jupiter's moons is available online at: http://galileo.jpl.nasa.gov.

[NOTE TO BROADCASTERS: A video file with animation to accompany this release will air today on NASA Television at noon, 3 p.m., 6 p.m. and 9 p.m. Eastern Standard Time. NASA Television is broadcast on GE-2, transponder 9C, C-Band, located at 85 degrees West longitude. The frequency is 3880.0 MHz. Polarization is vertical and audio is monaural at 6.8 MHz. For general questions about the NASA Video File, contact: Fred Brown, NASA Television, Washington, D.C. (202) 358- 0713.]


Contact: Guy Webster (818) 354-6278
JPL Media Relations Office

2001-105

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