Visions
of the Interplanetary Probes
In the end, after the observations of the ancients and the
meticulous mathematics of Kepler, after the comet-frescos
of Giotto and the telescopic discoveries of Galileo, after
Sputnik, Ranger, and all the far-flung probes of four decades
of space flight – we have the stark, spectacular beauty
of the spheres themselves. They’re real, verifiable.
They move kinetically, inexorably. Grouped in wheeling archipelagoes,
or sometimes alone, but always part of a larger system ruled
by the sun’s gravity and light, they’re suspended
in space like weightless jewels. Of the planets, most have
moons. Of the moons, some are bigger than planets. Both moons
and planets can have tenuous atmospheres, or incredibly thick
ones, or none at all. Immense and banded, Jupiter is the
largest by far. Flickering polar auroras, high-speed scudding
clouds, and massive, whirling-dervish storm systems define
its gaseous face. Jupiter’s powerful gravity insures
that its innermost large moon, Io, is unstoppably volcanic
and eerily lurid in its surface coloration. By contrast a
second Jovian moon, Europa, is cool and off-white, a frozen,
cue-ball perfect world. A third satellite, Callisto, has
been ravaged by eons of meteor impacts; battered and pitted,
it doesn’t look at all like either of its sisters.
The proximity of the Jovian moons to each other only accentuates
their odd-ball disparity.
Inwards and closer to the Sun than Jupiter, past the familiar
blue glow of our home world, the hidden topography of cloud-shrouded
Venus ripples and heaves with strange, protuberant forms. First
discerned by the unwavering radar eye of the early 90’s
Magellan space probe, they were quickly dubbed “ticks” and “arachnids” by
planetary scientists, and are almost certainly the result of
sub-surface volcanic activity. Meanwhile our other “terrestrial” neighbor,
Mars, sports seasonal spinning dust devils; they trace spidery
calligraphic streaks in the vicinity of Vallis Marinaris, the
grandest canyon in the Solar System. As wide as the entire
continental United States, this complex of vast and serrated
desert walls was named after its discoverer, the 1971 Mariner
9 probe. And as if all this weren’t already enough, outwards
from Jupiter in the direction of interstellar space, Saturn
hovers like a hallucination. The shimmering ring system of
the second largest planet are sixty feet thick, 155 thousand
miles wide and comprised of innumerable boulders held perpetually
in the grip of the rapidly spinning planet’s gravity.
Saturn looks somehow designed – an object as perfect
as the mathematics within the forces that made it.
How do we know about all this awesome scenery and clockwork
motion? Because it has been photographed, scanned, and parsed
by over a hundred robotic explorers from various nations – though
primarily the United States and the former USSR (see http://www.solarviews.com/eng/craft1.htm) – using
a variety of scientific instruments. (Interestingly, the word “robot” comes
from the Russian “rabotnik,” or worker.) The sum
total of the information which we’ve acquired in the
brief forty years of space exploration so far outstrips all
previous human knowledge of the Solar System as to make the
comparison almost ridiculous – a dime-thin pamphlet next
to a library of encyclopedias. And in the last decade these
discoveries have continued cascading in exponentially. Less
than two years ago, for example, NASA’s recently deceased
Galileo probe revealed that Jupiter has up to nine tiny asteroidal
satellites orbiting it close in. (That venerable spacecraft
finally ended its fourteen year mission by diving into Jupiter
in late September.) Within the last five years, Galileo also
helped planetary geologists to deduce that the spidery network
of cracks splayed across Europa’s ice face gives clear
evidence of a subsurface liquid water ocean. The moon may even
contain several times as much water as Earth – a prospect
which inevitably raises the question of whether life could
have evolved in orbit around Jupiter.
Other recent space probe findings concern Mars, and were conducted
by the camera system of the Mars Global Surveyor and the thermal
imaging system of another orbiting probe, Mars Odyssey. These
two craft revealed that both distinctive gulleys and the thermal
retention properties of parts of the Martian surface give evidence
that this planet, too, most likely has liquid sub-surface water.
Along with Europa, Mars is thus considered a potential host
of extra-terrestrial life.
And this flood of revelations isn’t likely to stop
anytime soon, despite NASA budget cuts and a crises in the
agency due to the recent loss of Space Shuttle Columbia.
In January of 2003, four probes from various nations will
arrive at Mars, where they will join the two US orbiters
currently on-station. Two new NASA missions will deploy rovers;
a European Space Agency mission will leave an orbiter to
circle the planet and send down a small stationary lander;
and a Japanese mission called Nozumi will also go into orbit,
resulting in a record-breaking seven spacecraft active at
the Red Planet simultaneously. And in two years, one of the
largest and most complex interplanetary spacecraft ever conceived,
NASA’s Cassini, will arrive at Saturn after an eight
year flight. This schoolbus-sized robot will study the planet’s
rings and deploy a European-built probe called Huygens, which
will penetrate the clouds of Saturn’s mysterious moon
Titan. This opaque brown sphere appears to be rich in the
same organic chemicals that presaged life on Earth; it may
contain lakes, or even oceans, of liquid methane.
For much of the last decade I’ve been monitoring this
activity as best I can, both by using the Internet and also
by interviewing planetary scientists and the mission directors,
navigators and engineers of NASA’s Jet Propulsion Lab.
As a non-scientist with an interest in the visual arts, much
of my motivation lay in simply being drawn to the more aesthetically
compelling deep-space photographs. I was interested in pictures
capable of inspiring awe, or wonder, and I believe I found
them; many of these shots outstrip the wildest imaginings of
20th century science fiction (and yet they’re real).
I was helped in this research by the existence of large quantities
of photographs on-line – either at public outreach websites
like NASA’s excellent Planetary Photojournal (http://photojournal.jpl.nasa.gov/)
or in more specialized scientific research sites. I started
to log large quantities of time in the latter, and found myself
going through many thousands of raw, unprocessed pictures,
just for the sheer fascination of stumbling on previously unnoticed
views of these alien topographies. Soon I embarked on a book
project to document my findings – something which had
the advantage of giving me both the funding and time to search
for the most ravishing extraterrestrial landscapes I could
find.
Almost all of the photographs in the resulting book, Beyond:
Visions of the Interplanetary Probes, required substantial
amounts of digital processing. Some had never been rendered
into color before. Quite a few are multiple-frame mosaics,
the result of finding remarkable contiguous single frames and
collaging them together. Even the many shots which were picked
up largely pre-processed frequently required hours of work
to make them suitable for publication, either to modify their
colors according to the best information currently available,
or to remove seams between mosaic frames, or to clone over
a speckle of uncorrected bad pixels or other transmission artifacts.
(And some, of course, simply slid into place without needing
additional work—a testament to their talented processors,
who often remain anonymous, with their pictures simply credited
to JPL or NASA.)
As this issue of Smithsonian goes to press, a small squadron
of space probes are in development. These include Messenger,
only the second mission to Mercury, which will fly past the
planet twice before settling into orbit around it in late 2009
after a five-year flight, and the Pluto-Kuiper Express, which
has fought its way back from cancellation and received funding
for a 2006 launch to visit the Solar System’s farthest-flung
and smallest planet. The Express will then proceed to a mysterious
belt of cometary snowballs and—who knows?—abandoned
alien spacecraft beyond Neptune, at the dim edge of interstellar
space.
When they get where they’re going, these and other hardy
robot explorers will continue doing what the other probes have:
they’ll help place us in both space and time, changing
our sense of our position and our possibilities, and revealing
glinting and unexpected new vistas under the dazzling Sun.
--Michael Benson
Ljubljana, Slovenia
September 23, 2003