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The first detailed topographic maps of Mars were produced with data
from NASA's Mariner 9
orbiter mission of 1971-1972, in which channel and valley networks,
volcanoes, canyons and craters were photographed at reasonable
resolution for the first time. Mariner 9 was also the mission that returned pictures of
layered (possibly sedimentary) terrain in Mars' polar regions. The
channel and valley networks bear such striking similarities to river
valleys and deltas on the Earth that they were assumed to demonstrate
beyond doubt that at some time in its past history, Mars must have had
significant quantities of running water coursing across its
surface. Five years after Mariner 9, in 1976, NASA's two Viking
landers sent back many images of Mars' landscape, showing panoramic
scenes of broken boulders distributed over flat dusty plains.
Viking also measured the elemental composition of both Mars'
atmosphere and surface soils. In combination with the
Mariner data, the Viking results have allowed a picture
of Mars as a rocky planet with a significant and complex geological
history to be built up. The two hemispheres of Mars exhibit very different geological
histories. Most of the northern hemisphere consists of almost flat,
low-lying plains, showing little cratering. In contrast, the terrain
of the southern hemisphere appears more ancient, with cratered
highland regions cross-cut by canyons, channels and valley
networks. But many questions about Mars remain unanswered,
particularly about the fluvial and seismic history of the planet. The Pathfinder
mission of 1997 landed on a rocky plain at the mouth of the Ares
Vallis in Chryse Planitia (19.33°N, 33.55°W). During its month
of operation, it recorded spectacular images of a rock-strewn plain,
with tantalising glimpses of rounded pebbles and possible layered
structures and hollows within some of the rocks. Chemical and image data for rocks and soil were acquired by the
Sojourner rover, a mobile robotic probe. Inferences drawn from
these data are that some of the rocks might be sedimentary, possibly
even conglomerates, thus implying a significant fluvial
history. Paler, almost cream-coloured patches in the soil might be
areas leached by fluid action, hard-grounds
or deposits left after evaporation.
The disordered landscape of partly rounded pebbles and boulders has been
interpreted as the type of landscape remaining after catastrophic flooding, further evidence of the stability of
liquid water at some time in Mars' past. Recent data from the laser altimeter aboard the Mars Global Surveyor have been
interpreted as evidence for a very large ocean across Mars' northern
hemisphere. This spacecraft is currently in orbit around Mars,
producing the most detailed mapping of the surface ever
attempted. |
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Life in the Universe
Exploring the Solar System
Mars
The Features
Space Missions to Mars
Water on Mars?
Life on Mars?
Future Space Missions to Mars
Meteorites from Mars
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Last updated July 25, 2001