Jupiter (Planet) -- Photographs from space; Jupiter probes; Voyager Project
[Illustration: As Voyager 1 approached Ganymede on March 5, many
strange new surface features became visible. In this frame, taken
from a distance of 250 000 kilometers and showing features as small
as 5 kilometers across, three distinct types of terrain are seen:
polygons of old dark surface, extensive areas of lighter, younger
material, and brilliant white ejecta patterns (probably water-ice)
around fresh craters. The bright rays in the upper part of the
picture are 300-500 kilometers long; at the bottom are several
craters with only faint, muted ejecta patterns. [P-21262C]]
[Illustration: Voyager 1 found that the surface of Ganymede was
geologically very complex. This frame, taken March 5 from a range of
250 000 kilometers, shows a region about 1000 kilometers across
centered near longitude 0° and latitude 20°S. The surface displays
many craters, some (probably the younger ones) with bright ray
systems. Bright grooved bands traverse the surface in various
directions. One of these bands, running in a north-south direction
in the lower left of the picture, is offset along a white line that
may represent a fault. Ganymede is the only Galilean satellite to
show indications of such lateral offsets in the crust. [P-21266]]
The first picture of Amalthea was shown, revealing an elongated, dark,
reddish object about 265 kilometers long. Smith reported: “There is
actually some structure that one can see—a crater—a couple of bright
features for which we have no interpretation and some other evidence of
cratering. It doesn’t look like much, but after all, Amalthea has never
been seen as anything more than a point of light from the Earth, and, in
fact, there are very few people that have even seen it as a point of
light. I doubt that more than one astronomer out of a hundred has
actually seen Amalthea.”
Larry Soderblom introduced new photographs of the satellites. Io still
showed no craters, even at high resolution. The craters that “should”
have been on Io were on Ganymede and Callisto. Ganymede not only had
craters, it had fault lines as well. “There is transverse motion along
these faults. Things get offset, apparently, for hundreds of kilometers.
So it’s the first time we’ve seen major kinds of transverse motion on
the surface of another planet.” Ganymede, in effect, had shown evidence
of having its own icy version of the San Andreas Fault.
[Illustration: Amalthea was thought to be the innermost satellite of
Jupiter until Voyager 2 discovered tiny Adrastea (1979J1). The
Voyager 1 camera revealed Amalthea as an irregular dark reddish
object with dimensions of 270 × 160 kilometers. These three images
have resolutions of (b) 25 kilometers; (c) 13 kilometers; (d) 8
kilometers. [260-503]]
[Illustration: Observation geometry for Amalthea]
[Illustration: (b)]
[Illustration: (c)]
[Illustration: (d)]
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