A single impact might explain why the Red Planet’s surface looks smoother in the north and rugged and rocky in the south
Web edition
:
Monday, July 7th, 2008

Text Size

SLAM DUNKMars may be home to the solar system’s largest impact crater, hidden below lava. The impact itself, illustrated here, may have given Mars its unusual "two faces" -- af high, cratered crust in the southern hemisphere and smooth, low crust in the north. This illustration was created from Caltech simulations of the impact, one of three recent studies to support the idea that the uneven surface was created by a single impact.M. Marinova et al./Caltech When you look up at the night sky, it's hard to imagine the
violent, chaotic place the solar system was billions of years ago. It looks
quiet and peaceful now, but when the solar system first took shape, asteroids
and other objects regularly slammed into each other, sometimes knocking off
huge chunks of rock. Some of these eventually became moons, and left the
surfaces of the planets forever changed.
Now, scientists say one of these massive collisions knocked
off much of the top layer of the northern hemisphere of Mars, our planetary
neighbor. Their findings answer a question that has long puzzled scientists: Why
do the Red Planet's northern and southern hemispheres look so different from
one another?
The debate started more than 30 years ago, when NASA
scientists launched the Viking spacecraft into orbit around Mars. The
spacecraft sent back the first close-up maps and images anyone had ever seen of
the Martian surface.
Surprisingly, those images showed that northern Mars looks
very different from southern section of the planet. While the north was flat
and smooth, the south was rugged, dotted with craters and mountains. Another
NASA spacecraft, the Mars Global Surveyor, later showed that the planet's crust
is also thicker in the south than in the north. In fact, the entire southern
hemisphere of Mars is about four kilometers higher than the northern
hemisphere.
What could account for these observations? It's been a topic
of debate for decades. Some suggested that processes deep below the planet's
surface gave Mars different kinds of crust in the two hemispheres. Others
thought the impact from many colliding meteorites, comets or other objects
could have shaved off four kilometers of crust from the northern hemisphere
over time. Still another pair of scientists suggested a single impact from just
one object could have created the planet's two faces.
By studying data from two spacecraft, NASA's Mars Odyssey
and the Mars Global Surveyor, a team of planetary scientists was able to look
below the surface of a recent lava flow on the Martian surface. Just like on
Earth, volcanoes periodically spew lava over the planet's surface, and on Mars,
this lava previously blocked scientists' view of the planet's underlying
bedrock.
Below the lava, they found a huge crater the size of Asia,
Australia and Europe combined running the length of the boundary between the
flat northern hemisphere and the bumpy southern hemisphere. It's an important
clue, scientists say.
"Finding this elliptical boundary is a smoking
gun," says Jeffrey Andrews-Hanna, a planetary scientist at the
Massachusetts Institute of Technology. "There is only one known way to get
a shape like this: impact."
The impact theory gets even more support from additional
findings from other scientists.
Two other groups of researchers used computer programs to
predict what kind of impact could have given Mars its dual appearance. They ran
a series of computerized scenarios in which they slammed different objects into
the planet at different speeds and angles.
They estimated that a Pluto-sized object traveling at 32,000
kilometers per hour would have generated enough energy to blast off the crust
of the planet's northern half.
"Something big smacked into Mars and stripped half the
crust off the planet," says Francis Nimmo, a planetary scientist at the
University of California, Santa Cruz who ran some of the computer simulations.
These new observations still do not disprove the idea that
processes deep below the planet's surface could have caused the difference in
the planet's two halves. But, says Steven Squyres, a planetary scientist at
Cornell University, "it's nice to see an old idea dusted off and turned
into something with real physical plausibility."
Found in: Atom & Cosmos
Time to dust off the epicycles of the Greeks, in honor of perturbation theory as an explanation of planetary orbits, and of the indomitable Jerome Y. Lettvin for suggesting that reversion in the 1970s.
Please login or register to participate.