RELEASE DATE:   October 10, 1995
PHOTO RELEASE NO.: STScI-PRC95-37


               HUBBLE DISCOVERS BRIGHT NEW SPOT ON IO


This NASA Hubble Space Telescope pair of images of Jupiter's volcanic
moon Io shows the surprising emergence of a 200-mile diameter large
yellowish-white feature near the center of the moon's disk (photo on
the right).  This is a more dramatic change in 16 months than any seen
over the previous 15 years, say researchers.  They suggest the spot may
be a new class of transient feature on the moon.   For comparison the
photo on the left was taken in March 1994 -- before the spot emerged --
and shows that Io's surface had undergone only subtle changes since it
was last seen close-up by the Voyager 2 probe in 1979.  The new spot
seen in the July 1995 Hubble image replaces a smaller whitish spot seen
in about the same place in the March 1994 image.  Note the much more
subtle changes seen elsewhere on this face of Io over the 16 months
between the images.  Each image is a composite of frames taken at
near-ultraviolet, violet, and yellow wavelengths, with Hubble's Wide
Field and Planetary Camera 2.  "The new spot surrounds the volcano Ra
Patera, which was photographed by Voyager, and is probably composed of
material, probably frozen gas, ejected from Ra Patera by a large
volcanic explosion or fresh lava flows...," according to John Spencer
of Lowell Observatory in Flagstaff, Arizona.  The new bright spot is
also unusual because it is much yellower than other bright regions of
Io, which are whitish in color.  The unusual color may result from the
freshness of the deposit and will probably provide clues as to the
composition of new volcanic materials on Io.   The temperature on Io's
surface is about -150 degrees Celsius (-238 degrees Fahrenheit);
however, "hot spots" associated with volcanic activity may be as warm
as 1,000 degrees Celsius (1,800 degrees Fahrenheit).  Follow-up
observations by Hubble, in coordination with the Galileo spacecraft,
scheduled to arrive at Jupiter and fly by Io in December 1995, will
reveal the evolution and lifetime of the new feature.  Galileo will be
able to see much greater detail on Io in visible light, but will still
rely on information gleaned from Hubble UV observations and Hubble
observations taken at times when Galileo cannot observe Io.  These
further observations should also tell whether astronomers have
witnessed, for the first time, one of the processes which creates the
bright regions on Io.

The research team:  J.R. Spencer (Lowell Observatory); A.S. McEwen
(U.S.  Geological Survey); D.B. Nash (San Juan Capostrano Research
Inst.); M.A. McGrath (STScI); J.T. Clarke, G.E. Ballester (U.
Michigan); P. Sartoretti (NOAO); J.T. Trauger (JPL).

Credit: J. Spencer (Lowell Observatory),  and NASA