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Mars exploration has been dogged by disasters. Of 31 robotic missions to the red
planet only 11 have been completely successful. After six initial failures, the
fly-by in 1964 by the Mariner 4 spacecraft paved the way, but the first major
success was the one-billion dollar Viking 1 and 2 landers and orbiters. The first
lander touched down on the western slopes of Chryse Planitia (the Plain of Gold)
in August 1975 and the second in Utopia Planitia of the other side of Mars, close
to the edge of the north polar cap, in September 1975. Both were searching for
water and life. Their cameras revealed a gently rolling freeze-dried ferric-oxide-red
wasteland, with wind-blown fine dust drifting into impact craters and clinging
to eroded rocks, all shivering beneath a thin carbon dioxide atmosphere. The Martian
surface was blasted by cosmic radiation because Mars has only a negligible magnetic
field which is incapable of shielding the planet from incoming ionised particles.
It was also illuminated by life-threatening doses of ultraviolet light. The Martian
soil was apparently antiseptic and organics-free and was rich in peroxides and
superoxides. Cameras on board the Viking probes enabled scientists on Earth to
select specific soil samples from the surroundings. These were then collected
by manipulating scoops and sucked into miniature onboard biology laboratories.
There the soil was exposed to water, and liquid food laced with radioactive carbon.
The results indicated that the planet Mars was lifeless.
Observations of the surrounding landscape continued for six years. Little changed.
The banks of wind-blown Martian dust seemed to be much more permanent than Earth’s
sand dunes. What was really exciting, however, was the simple fact the Earth-made
Viking probes were out there, on the surface of a neighbouring planet, standing
on the soil and observing features in millimetre detail, whilst around them the
wind roared, and the dust hissed, and occasion rumbles from nearby landslides
and active volcanoes rent the thin poisonous air.
On 4 July 1997 Mars Pathfinder, a $250 million, ‘faster, better, cheaper’
mission, landed close to the mouth of a canyon, Ares Vallis, that some 3.6 to
4.5 billion years previously had been carved out by a flash flood of water. A
new epoch of Mars exploration was launched. Mars Pathfinder was carrying with
it Sojourner, a small, 10.6 kg, half a meter long, six-wheeled roving robot. This
could be guided from Earth, rather like a child can guide a radio–controlled
toy car. Sojourner, moved away from Pathfinder at about 0.6 metre per minute and
eventually examined 250 square meters of the nearby soil and rocks. Surprisingly
there was little evidence of chemical diversity. The rocks were volcanic and consisted
of a mixture of basalt and quartz, very similar to the Andes Mountains in South
America.
Sojourner added much excitement and drama to the mission, and showed that a Martian
rover could be effectively driven and manipulated from Earth. This remote robotic
rover could explore the nearby planetary surface effectively, quickly and relatively
cheaply. It could steer round or climb over rocks, and maintain a steady course.
If it fell over, however, there was nobody around to put it back on its wheels
again.
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