|
August 27, 1999: Jupiter's exotic moon Io is often likened
to a pepperoni pizza. Its mozzarella-colored surface is pockmarked
by ruddy volcanic plumes that evoke images of sliced Italian
sausage among imaginative scientists. The strange appearance
of Io's surface is constantly changing as it is formed and reformed
by lava flows of molten silicate rock. What drives this volcanic
powerhouse? The most likely energy source is changing gravitational
tides caused by nearby Jupiter.
Right: This image of Io, captured
by Galileo on July 3, 1999 from a distance of 81,000 miles, is
color balanced to show how that moon would look to the human
eye. [more
information]
On July 3, 1999 Galileo flew closer to Io than it has since entering
orbit around Jupiter in 1995. During the encounter the spacecraft
captured images with a resolution of only 1.3 km per picture
element, giving scientists a detailed view of Io's surface.
The color image above was created by combining data from near-infrared,
green and violet filters in the spacecraft's camera to approximate
what the human eye would see when looking at Io. Comparison of
this image to previous
Galileo images reveals many changes due to the ongoing volcanic
activity. A higher contrast, false color version (below) shows
many small-scale volcanic features which were not recognized
previously.
Above: This false color image shows
small-scale features which were not recognized previously and
which suggest that the lava and sulfurous deposits on Io are
composed of complex mixtures (close-up A). Some of the bright,
whitish, high-latitude (near the top and bottom) deposits have
an ethereal quality like a transparent covering of frost (close-up
B). Bright red areas were seen in previous images only as diffuse
deposits. However, they now appear as both diffuse deposits and
sharp linear features like fissures (close-up C). Some volcanic
centers have bright and colorful flows, perhaps due to flows
of sulfur (rather than silicate) lava (close-up D). In this region
of Io, bright, white material can also be seen to emanate from
linear rifts and cliffs.
Beginning in October 1999, after a series of
four orbit-changing encounters with Callisto spanning May to
September 1999, Galileo is scheduled to make two daring close
approaches to Io, possibly flying through a volcanic plume. The
upcoming encounters are expected to yield images of unprecedented
clarity and detail. The radiation belts of Jupiter are very intense
at Io's distance from the huge planet, and this can disrupt spacecraft
functioning. To insure that Galileo will be able to perform science
observations from this unique vantage point, the Galileo flight
team is preparing contingency plans to protect against radiation-related
problems in the coming months.
Galileo has been orbiting Jupiter and its moons since December
1995. Its primary mission ended in December 1997, but the spacecraft
is currently in the midst of a two-year extended mission.
More information about the Galileo mission is available at: http://www.jpl.nasa.gov/galileo/
JPL manages Galileo for NASA' s Office of Space Science, Washington,
D.C. JPL is a division of the California Institute of Technology,
Pasadena, CA. |