National Aeronautics and Space Administration Logo
Follow this link to skip to the main content NASA Banner
Solar System Exploration
News & Events
Jupiter's Io Generates Power and Noise, but No Magnetic Field
Jupiter's Io Generates Power and Noise, but No Magnetic Field
10 Dec 2001
(Source: Jet Propulsion Laboratory)

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIFORNIA 91109. TELEPHONE (818) 354-5011
http://www.jpl.nasa.gov

Contact: Guy Webster (818) 354-6278

A great roar of acoustic waves near the north and south poles of Jupiter's moon Io shouts about the power of the volcanic moon.

The wave data, new pictures and other information collected recently by NASA's Galileo spacecraft provide insight into what happens above Io's surface, at its colorful volcanoes and inside its hot belly. Scientists presented the findings Monday at a meeting of the American Geophysical Union in San Francisco.

Galileo, managed by NASA's Jet Propulsion Laboratory, Pasadena, Calif., has been orbiting Jupiter for six years. As it flew near Io's poles in August and October, the density of charged particles it was passing through suddenly increased about tenfold when the spacecraft crossed the path of a magnetic-field connection between Io and Jupiter, reported Dr. Donald Gurnett of the University of Iowa, Iowa City. The waves, indicating the density, travel in a plasma of charged particles, and would be silent to the ear, but Iowa researchers converted them to sound waves to make the patterns audible. Audio clips are available online at http://www.jpl.nasa.gov/videos/io.

"You hear a whistling sound from Jupiter's radio emissions, then, just when you go over the pole, you hear a tremendous roar that starts abruptly, then stops abruptly," Gurnett said. "It's like the noise from a huge electrical power generator." Io actually generates as much wattage as about 1,000 nuclear power plants.

The region of increased density is where electrons and ions come up from Io's tenuous atmosphere and follow a "flux tube" where field lines from Jupiter's strong magnetic field intersect Io. In a 1999 flyby of Io, Galileo had provided some indication of the higher density over the moon's poles. This year's two Io flybys were the first to show that those denser areas coincide with the magnetic-field flux tube, Gurnett said.

Recent magnetic-field measurements tell us something new about the plumes erupting from Io's volcanoes and about the moon's molten core, said Dr. Margaret Kivelson of the University of California, Los Angeles.

Galileo detected electrical currents flowing along magnetic field lines above two areas of volcanic activity on Io, Kivelson said. Material shot high from eruptions is apparently affecting conductivity more than 100 kilometers (about 60 miles) above the surface.

"If this is the mechanism that's producing the currents, it may help us in the search for active plumes," she said.

Galileo's routes near Io's north pole in August and near its south pole in October were chosen for gaining measurements to determine whether Io generates an intrinsic magnetic field of its own within the greater magnetic field generated by Jupiter.

"There's no intrinsic field," Kivelson said. "We can put that question to rest." That means Io's molten iron core does not have the same type of convective overturning by which Earth's molten core generates Earth's magnetic field. Lack of that overturning fits a model of Io's core being heated from the outside, by tidal flexing of the layers around it, rather than being heated from the center.

The heat generated inside Io by the tidal tug of Jupiter makes this moon the most volcanically active world in the solar system. A new color picture of one large volcanic crater, Tupan Patera, shows various red, green, yellow and black surface materials laid down by volcanic interactions of molten rock and sulfur compounds, said Dr. Elizabeth Turtle of the University of Arizona, Tucson. Tupan, named for a Brazilian god of thunder, is one of Io's most persistent volcanoes. Another new image reveals roofed-over portions of a long lava channel, indicating that insulation provided by the cover helped lengthen a large lava flow.

New infrared imagery from Galileo shows that darker areas at Tupan correspond to hotter surface materials, said Dr. Rosaly Lopes of JPL. The infrared data also confirm sulfur- dioxide deposits near the source of a tall plume seen in August above a previously inactive volcano.

New images of Io are available from JPL at http://www.jpl.nasa.gov/images/io and from the University of Arizona Planetary Image Research Laboratory at http://pirlwww.lpl.arizona.edu/missions/Galileo/releases/.

NASA's Jet Propulsion Laboratory, 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.

News Archive Search  Go!
Show  results per page
 
 
Awards and Recognition   Solar System Exploration Roadmap   Contact Us   Site Map   Print This Page
NASA Official: Kristen Erickson
Advisory: Dr. James Green, Director of Planetary Science
Outreach Manager: Alice Wessen
Curator/Editor: Phil Davis
Science Writer: Autumn Burdick
Producer: Greg Baerg
Webmaster: David Martin
> NASA Science Mission Directorate
> Budgets, Strategic Plans and Accountability Reports
> Equal Employment Opportunity Data
   Posted Pursuant to the No Fear Act
> Information-Dissemination Policies and Inventories
> Freedom of Information Act
> Privacy Policy & Important Notices
> Inspector General Hotline
> Office of the Inspector General
> NASA Communications Policy
> USA.gov
> ExpectMore.gov
> NASA Advisory Council
> Open Government at NASA
Last Updated: 10 Dec 2001