Jupiter (Planet) -- Photographs from space; Jupiter probes; Voyager Project
[Illustration: In addition to its giant volcanic plumes or
fountains, Io possesses other indications of current volcanic
activity. One of these takes the form of intermittent blue-white
patches that may be caused by gas venting from the interior. In this
pair of photographs, the same region of the surface is shown about
six hours apart. On the right, there is an arcuate bright gas cloud;
on the left the same region is black. It is believed that the
venting gas is sulfur dioxide, and that the condensation of this gas
produces fine particles of “snow” that look blue. [260-508]]
[Illustration: Some of the most dramatic changes in the surface of
Io between March and July took place in the vicinity of the volcano
Loki, at longitude 310° and latitude 15°N. On the left is a Voyager
1 view; on the right, one from Voyager 2. The “lava lake” associated
with Loki has become less distinct, apparently as a result of
deposits that fell on the northern part of the dark U-shaped
feature. Perhaps the surface had also cooled between these photos.
In the upper left center, a new dark volcanic caldera with bright
spots near it and a large, faint bright ring had appeared by July,
although it was not active at the time Voyager 2 flew by.
[260-687AC]]
No new eruptions were seen by Voyager 2; between them, the two
spacecraft effectively surveyed the whole surface of Io for plumes down
to 40 kilometers height. Interestingly, the smallest plume seen was 70
kilometers high; there appeared to be a real absence of smaller
eruptions.
From the number and size of the observed eruptions, it is possible to
calculate the resurfacing rate for Io due to these plumes. The result is
that each plume is erupting about 10 000 tons of material per second, or
more than 100 billion tons per year. This quantity corresponds to about
10 meters of deposition over the whole surface in a million years. When
additional note is taken of surface flows, the deposition rate could
easily be ten times higher, or 100 meters per million years, in
agreement with the rate estimated from the absence of impact craters.
Energy for the Io Volcanoes
Clearly, something extraordinary is happening to Io to generate the
observed level of volcanism. The primary heat source for the interiors
of the terrestrial planets is the decay of the long-lived radioactive
elements thorium and uranium. But Io would have to be supplied with a
hundred times its quota of these elements to explain the observed
activity.
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