Spacecraft at Io Sees and Sniffs Tallest Volcanic Plume

Oct. 4, 2001



Contact:
Jet Propulsion Laboratory/Guy Webster (818) 354-6278
University of Arizona/Lori Stiles (520) 626-4402
University of Iowa/Gary Galluzzo (319) 384-0009



Jupiter's moon Io has pulled a surprise on NASA's Galileo spacecraft, hurling up the tallest volcanic plume ever seen, which arose from a previously unknown volcano.

A different volcano had been lofting a plume seven months earlier, but Galileo saw no sign of that plume during its latest Io flyby in early August.

Adding to the surprise, for the first time a Galileo instrument has caught particles freshly released from an eruption, giving scientists a direct sample of Io material to analyze. "This was totally unexpected," said the leader of that experiment, Dr. Louis Frank of the University of Iowa, Iowa City. "We've had wonderful images and other remote sensing of the volcanoes on Io before, but we've never caught the hot breath from one of them until now. Galileo smelled the volcano's strong breath and survived."

The Jupiter-orbiting spacecraft has been gradually transmitting to Earth the new pictures and data from its flight over Io's north pole in early August, said Dr. Eilene Theilig, Galileo project manager at NASA's Jet Propulsion Laboratory, Pasadena, Calif. "Io just keeps amazing everyone," she said. "Now we're eager to see what will be happening there when Galileo flies near Io's south pole in two weeks."

Galileo engineers and scientists had anticipated that the Aug. 6 flyby (Aug. 5, Pacific time) might take the spacecraft right through gases rising from a volcano named Tvashtar near Io's north pole. Tvashtar had been lofting a high plume when last seen seven months earlier by both Galileo and the passing Cassini spacecraft. However, the Tvashtar plume has not been found in images from the August flyby. Researchers were startled to find, instead, that a previously unknown volcano just 600 kilometers (370 miles) from Tvashtar was spewing a grand plume as Galileo passed.

"After not seeing any active plumes at all in Io's high-latitude regions during the first five years of Galileo's tour, we've now seen two this year," said Galileo imaging team member Dr. Alfred McEwen of the University of Arizona, Tucson. The latest appears as a back-lit bulge above Io's surface in two newly released images. A third new image shows a white ring of material from the plume that has fallen back to the moon's surface, painting a circle around the source of the eruption. A fourth shows another new large plume deposit near Io's north pole.

The images are available online from JPL at http://www.jpl.nasa.gov/images/io
and from the University of Arizona at http://pirlwww.lpl.arizona.edu/Galileo/Releases

The new plume rises at least 500 kilometers (more than 300 miles) above ground, McEwen estimated, nearly 10 percent higher than the tallest ever seen before on Io.

Scientists using Galileo's infrared mapping instrument have pinpointed the site of the eruption as a new hot spot at a location that was not known to be an active volcano, said JPL volcanologist Dr. Rosaly Lopes. It was surprising that the site leapt to such intense activity so abruptly with so little evidence of former volcanism, she said.

"Galileo flew between two great volcanoes," Lopes said. "The plume we knew about might have settled down before we got there, but this new one sprang up suddenly."

The particles detected in Galileo's plasma science instrument as the aging spacecraft sped within 194 kilometers (120 miles) of Io's surface likely came from the new hot spot rather than Tvashtar, Frank said. The volcanic material reached the spacecraft no more than a few minutes after rushing out of the source vent on the ground. The particles are apparently snowflakes made of sulfur-dioxide molecules with as many as 15 to 20 molecules clumped together in each flake.

Frank and co-workers will try to wring information from the particle impacts about the temperature and speed of the gas in the plume. "That will get us a step closer to knowing about the newly released material from a volcanic vent," he said.

Galileo is on course to fly about as close to Io again at 0123 Universal Time on Oct. 16 (5:23 p.m. Oct. 16, Pacific Daylight Time). Its trajectory will take it close to Io's south pole, which may provide a look at details of another new hot spot near there identified from infrared mapping data this year. The polar passes in August and this month were also designed to provide data indicating whether Io generates its own magnetic field, as its sibling moon Ganymede does and Earth does.

Io is the innermost of Jupiter's four largest moons and the most volcanically active world in the solar system. Galileo will get its sixth and final encounter with Io in January 2002. It has also flown 27 close approaches to Jupiter's other three large moons: Europa, Ganymede and Callisto. Since it began orbiting Jupiter in 1995, Galileo has survived more than three times the radiation exposure it was designed to withstand. It is still is good overall health, but performance of some instruments has been degraded.

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


IMAGE CAPTION PIA-02591
Hot Spots on Io
October 4, 2001

Volcanic hot spots, including a bright one never seen before, pepper an infrared color-coded image (left) of Jupiter's moon Io, taken by NASA's Galileo spacecraft on Aug. 6, 2001.

The bright, new hot spot (arrow) in Io's high northern latitudes is the source of a towering volcanic plume detected in new images taken by Galileo's camera. Snowflake-like particles of clumped sulfur-dioxide molecules from the plume were caught by the plasma-science instrument onboard the spacecraft.

Beginning about two hours after the spacecraft passed within 194 kilometers (120 miles) of Io's surface, Galileo's near-infrared mapping spectrometer recorded this image of most of the sunlit disc of the large, sizzling moon. The image shows the brightness of features at a wavelength of 4.4 microns, which detects heat from Io's many volcanic eruptions. An earlier image from Galileo's camera showing the same face of Io (right) is included for correlating the heat-sensing infrared data with geological features apparent in visible wavelengths.

Many volcanic hot spots appear in the infrared image as bright regions: yellow to red to white, in order of increasing intensity. The brightest hot spot in the northern hemisphere, indicated by the arrow, was so vigorous at the time of the observation that some pixels (shown in black) were saturated. This hot spot was not a previously known volcano. Io has 108 known hot spots, 10 of which were discovered from this observation. Most of the newly discovered ones are too faint to show up in this map, but their thermal signatures can be detected by examining each location's infrared data at more than one wavelength.

Credit: NASA/JPL/University of Arizona

IMAGE CAPTION PIA-02592
Northern Plume and Plume Deposits on Io
October 4, 2001

Backlit views (left pair) show a giant volcanic plume as a bulge on the crescent edge of Jupiter's moon Io, and more fully lit views (right pair) reveal rings where sulfur-rich plume material has fallen back to the ground, in images captured by NASA's Galileo spacecraft in early August 2001.

Io is the most volcanically active world known. Galileo and NASA's Voyager and Cassini spacecraft have caught several of Io's volcanoes in action lofting plumes of gas and particles high above the large moon's surface. However, none of the plumes seen previously has climbed as high as the one evidenced in three of these pictures.

During its Aug. 6, 2001, close encounter with Io, Galileo flew right through a space where a plume from the Tvashtar volcano near Io's north pole had been active when Galileo and Saturn-bound Cassini imaged Io seven months earlier. To see if the Tvashtar plume was still active in August, scientists used Galileo's camera to acquire images when the spacecraft was nearly on the opposite side of Io from the Sun, so that Io appears as a backlit crescent.

Tvashtar's plume did not show up, but another one did, rising from a previously undiscovered and still unnamed volcano about 600 kilometers (370 miles) south of Tvashtar. The left two images are color coded to reveal the faint outer plume. The bright inner plume rises about 150 kilometers (90 miles) high, and the top of the faint outer plume can be detected at 500 kilometers (310 miles) above the surface, making this the largest plume ever detected on Io. A portion of the plume with intermediate brightness extends north of the eruption's source vent. (The vertical lines, bright spots and short streaks in these two images are noise.)

One of the more fully illuminated color images of Io (second image from right) reveals a bull's-eye ring of new dark and light materials marking the eruption site. No obvious volcanic center had previously been seen at this location, 41 degrees north latitude and 133 degrees west longitude. The bright material of the new plume deposit overlies the red-ring plume deposit encircling the Tvashtar volcano at 63 degees north, 123 degrees west. Tvashtar's ring deposit was first seen in Galileo images taken in late December 2000.

Another new full-disc color image of Io (far right) reveals yet another new plume deposit near Io's north pole, encircling the Dazhbog Patera volcanic site. This red ring has a diameter of about 1,000 kilometers (620 miles), suggesting a plume height of about 300 kilometers (190 miles). This plume deposit was not present in January 2001, so it is evidence of a new eruption.

Io is about the same size as Earth's Moon. All four images have resolutions of 18 to 20 kilometers (11 to 12 miles) per picture element. Unlabeled versions are also available. Click on the thumbnail versions below.

Infrared imagery from Galileo or Earth-based telescopes has detected intense hot spots at the sites of all three of these giant plumes. Giant polar plumes represent a class of eruption seen by the Voyager spacecraft in 1979, but not during Galileo's first five years of orbiting Jupiter. Voyager was unable to measure temperatures or other properties of these eruptions, so scientists are pleased Galileo has survived long enough to do so. Galileo reached Jupiter in late 1995. Its original two-year orbital mission has been extended three times to take advantage of the spacecraft's continuing capability to return valuable scientific information about the Jupiter system.

Credit: NASA/JPL/University of Arizona

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