MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109 TELEPHONE (818) 354-5011
http://www.jpl.nasa.gov
Contact: Jane Platt
November 4, 1999
New Galileo Images Reveal Hawaiian Style Volcano on Io
A volcanic crater several times larger than one found at Hawaii's Kilauea
volcano has been photographed on Jupiter's moon Io during a close flyby
performed by NASA's Galileo spacecraft.
"It appears that the Prometheus volcano on Io has characteristics
remarkably similar to those of the Kilauea volcano in Hawaii, although
Prometheus is much larger," said Dr. Laszlo Keszthelyi (KEST-ay), a Galileo
research associate at the University of Arizona, Tucson, AZ. "Both
volcanoes are long-lived eruptions, with flows that apparently travel
through lava tubes and produce plumes when they interact with cooler
materials."
The sharp images of Prometheus released today come from two of Galileo's
onboard instruments -- the camera, and the near-infrared mapping
spectrometer which observes in wavelengths not visible to the naked eye.
The images were taken during the close flyby of Io by Galileo on October
10, 1999, and are part of a large batch of data currently being transmitted
to Earth.
"We've been having a feast looking at the material from Io," said Dr.
Rosaly Lopes-Gautier NASA's Jet Propulsion Laboratory, Pasadena, CA. "We
have been waiting for such high-resolution images of Io for more than 10
years." Scientists will present an assortment of new images and describe
their latest discoveries at a press briefing scheduled for November 19 at
NASA Headquarters, Washington, DC.
Prometheus is the "Old Faithful" of Io's many volcanoes. It has been
active during every observation over the past 20 years by NASA's Voyager
and Galileo spacecraft and the Hubble Space Telescope. The new
spectrometer images show two distinct hot spots at Prometheus -- a large
one to the west and a fainter, cooler one to the east. The images reveal
numerous lava flows near the western hot spot and enable scientists to
identify a crater, or caldera, 28 kilometers (17 miles) long and 14
kilometers (9 miles) wide near the hot spot to the east.
Previously, it was thought that the 50 to 100 kilometer- (30 to 60 mile-)
tall plume observed at Prometheus formed where the lava erupts onto the
surface. Now, however, it now appears that the plume forms at the far end
of the lava flows. The caldera and eastern hot spot are thought to be
associated with the vent where the molten rock rises to the surface. It
appears that after the lava reaches the surface, it is transported westward
through lava tubes for about 100 kilometers (60 miles) before breaking out
onto the surface again. Here, numerous lava flows wander across a plain
covered with sulfur dioxide-rich snow. The plume is created by the
interaction of the hot lava with the snow.
This plume feature is just one of several similarities between Prometheus
and Hawaii's Kilauea. Volcanologists say that Prometheus has been erupting
for more than 20 years and Kilauea has been erupting for more than 16
years. The current vent at Kilauea consists of a small lava lake about 100
meters (330 feet) across that produces a relatively small thermal hot spot.
From this vent, lava is transported 10 kilometers (6 miles) in lava tubes
to the Pacific Ocean where large steam plumes are generated by the
interaction between the hot lava and the ocean. Galileo scientists believe
the plume seen on the western end of Prometheus is similar to this Hawaiian
steam plume, except the Ionian plume is composed largely of sulfur dioxide
and rises much higher because of Io's low atmospheric density and gravity.
Another Io flyby, this time at an altitude of 300 kilometers (186 miles),
is planned for November 25 at 8:40 p.m. Pacific Time (11:40 p.m. Eastern
Time). (Times given are in Earth-received time -- or the time when the
signal of the event is received on Earth.) The Io flybys are challenging
and risky, because Io lies in an area of intense radiation from Jupiter's
radiation belts, and that radiation can harm spacecraft components.
Because of the risk, the flybys were scheduled for the final portion of
Galileo's extended mission.
The new Io images are available at http://www.jpl.nasa.gov/pictures/io .
Additional information and pictures taken by Galileo are available at the
mission homepage at http://galileo.jpl.nasa.gov .
The spacecraft has been orbiting Jupiter and its moons for nearly four
years, with its primary mission running from December 1995 until December
1997, followed by its current two-year extended mission. JPL manages the
Galileo mission for NASA's Office of Space Science, Washington, D.C. JPL
is operated for NASA by the California Institute of Technology, Pasadena, CA.
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