MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109. TELEPHONE (818) 354-5011
http://www.jpl.nasa.gov
IMAGE ADVISORY
October 12, 1998
MARS GLOBAL SURVEYOR CAPTURES DETAILED VIEWS OF OLYMPUS MONS,
KASEI VALLIS RIVER CHANNEL
NASA's Mars Global Surveyor has captured some spectacular
new views of Olympus Mons, the largest volcano in the solar
system, and a system of giant channels on the red planet known as
Kasei Vallis.
The new images are available on the Internet at
http://www.jpl.nasa.gov, http://photojournal.jpl.nasa.gov/, http://mars.jpl.nasa.gov/ and at
http://www.msss.com.
Taken on April 25, 1998, from a distance of about 900
kilometers (560 miles) above the surface, this wide-angle image
of Olympus Mons captures the west side of the volcano on a cool,
crisp winter morning. Olympus Mons is by far the tallest volcano
in the solar system, rising higher than three Mount Everests and
spanning the width of the entire Hawaiian island chain.
The images of Kasei Vallis, a system of giant channels
thought to have been carved by catastrophic floods more than a
billion years ago, illustrate the complexity of the planet's
geologic history. These images were acquired on June 4, 1998, and
reveal details of the 6-kilometer-diameter (4-mile) crater as it
pokes out from beneath an "island" in the valley. The mesa was
created in part by the flood and by its subsequent retreat, which
caused small landslides of the scarp that encircles it. A "mote"
or trench partly encircles the crater to the west and south. This
moat formed when the turbulence of the floodwaters interacting
with the crater rim eroded material in front of and alongside the
crater.
When Mars Global Surveyor reaches its final mapping orbit in
March 1999, the spacecraft's camera will be used to make daily
global maps of Martian clouds and weather systems. The wide-angle
images will resemble weather satellite pictures of Earth and will
help the Mars Global Surveyor science teams plan their
observations and test computer-driven prediction models of
Martian weather.
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