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
Contact: Mary Hardin (818) 354-0344
FOR IMMEDIATE RELEASE
October 5, 2000
GLOBAL SURVEYOR CAPTURES POSTCARD VIEW OF MARTIAN VALLEYS
At the beginning of its fourth year in orbit, NASA's Mars
Global Surveyor spacecraft has snapped a picture-postcard view of
three Martian valleys that is now available on the Internet and
on NASA Television.
The three major valley systems are located east of the
Hellas plains. They are Dao Vallis, Niger Vallis and Harmakhis
Vallis. These valleys are believed by some to have been formed --
at least in part -- by large outbursts of liquid water some time
far back in the Martian past, though there is no way to know
exactly how many hundreds of millions or billions of years ago
this might have occurred. In each valley, water would have flowed
toward the area seen at the bottom of the image. Although their
dimensions vary along their courses, the valleys are all roughly
1 kilometer (0.6 miles) deep and range in width from about 40
kilometers (25 miles) down to about 8 kilometers (5 miles).
The image is located at
http://www.jpl.nasa.gov/pictures/mars or http://www.msss.com or
http://mars.jpl.nasa.gov/mgs .
The images are also available on NASA Television during
today's video file, October 5, at noon Eastern (3 p.m. Pacific
time). NTV is broadcast on GE-2, transponder 9C, C-Band, located
at 85 degrees West longitude. The frequency is 3880.0 MHz.
Polarization is vertical and audio is monaural at 6.8 MHz. See the
schedule at ftp://ftp.hq.nasa.gov/pub/pao/tv-advisory/nasa-tv.txt .
JPL manages the Mars Global Surveyor spacecraft for NASA's
Office of Space Science, Washington, D.C. JPL is a division of
the California Institute of Technology in Pasadena.
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