Apr - May 98
EUROPA:
The Icy Moon
By Mike Carroll
& Friends
Ice,
slush, crystals, bands, plates, and
water???
Europa is probably the
most enigmatic moon in the solar system. Orbiting some 671,000 kilometers from Jupiter,
the 3,100 km diameter moon zips around the great planet in just over three and a half
days.
When two Voyager spacecraft flew by Europa in 1979, they glimpsed a unique worldlet
with mysterious brown fractures across its smooth surface. In some cases, these brown
lines had stripes down the middle, earning the nickname "highways". These
so-called triple bands had an unknown origin, and the baffled scientists hoped more
detailed views from the Galileo orbiter would clear up the mystery. Galileo has given us
spectacular images of Europa and the other Galilean satellites. During its extended
"Galileo Europa Mission" (GEM), the craft promises to show us even more. But the
triple bands are more complex than originally thought. Theories abound, but Ron Greeley
and other planetologists at JPL believe Europas triple bands may form in this way:
(images by Mike Carroll)
a) Bands begin as thin
cracks in the surface. (Figure 1 on the right. Note the "floating iceberg"
formations on the horizon at left.)
b) Liquid water seeps
--or explosively escapes --to the surface and flows outward, building up linear ridges on
either side of the fracture. (Figure 2)
c) As the ridge becomes more massive, the
ice crust cannot support its weight (despite Europas gravity being around half of
the Moons) and more parallel fractures form. These cracks, in turn, go through the
same process until several parallel ridges rise from the surface. (Figure 3. Note the dome
forming in the background, perhaps indicative of volcanism on the ocean floor under the
ice.)
d) The ice crust cannot support any taller structures; the fully formed
triple-band then begins to sink back into the surface, ultimately leaving a smooth,
striped plain. (Figure 4. Note the darkened spots along the crack.)
Those dark spots and the brown bands mentioned above have created a great deal of
speculation. What is causing all the color variations? Could it be geysering or cryo-volcanism of liquid from below? Dale Darby wondered if
radiation from Jupiter would do something to the ice. Could cometary and meteoritic impact
deposit some compounds that melting and/or sublimation could leave behind as stains? Bill
Hartmann speculates that "primordial ice out there has sooty carbonaceous dust in it
that colors it black. On Europa, most present ice probably erupted as liquid and the black
stuff sank out. In general on the Galilean satellites, the black stuff is less volatile
than the ice. Therefore MICROMETEORITE BOMBARDMENT will preferentially tend to sublimate
the ice and leave the black stuff behind. So I have speculated that this is why the
surface layers, especially on Callisto and Ganymede which have more primitive ice, tend to
get darker. Europa, though, may be protected from this mechanism to some degree because it
has pretty clean ice at the surface."
Perhaps the most
intriguing thing about Europa is whats underneath. Models suggest a deep water ocean
(up to 60 km) with active thermal vents on the ocean floor. Could these vents be host to
an alien ecosystem whose organic material is staining the cracks on the surface ice? GEM
will get spectral data of the bands in detail, so we may have more clues soon. Europa is a
beautiful, frozen, and possibly violent world. All in all, it's a great place to paint!

Copyright © 1998
International Association of Astronomical Artists |