Summary
This map, compiled photogrammetrically from Viking Orbiter stereo image pairs, is part of a series
of topographic maps of areas of special scientific interest on Mars.
MTM 500k –20/347E OMKT: Abbreviation for Mars Transverse Mercator; 1:500,000 series;
center of sheet latitude 20° S., longitude 347.5° E. in planetocentric coordinate system
(this corresponds to –20/012; latitude 20° S., longitude 12.5° W. in planetographic coordinate
system); orthophotomosaic (OM) with color coded (K) topographic contours and
nomenclature (T) [Greeley and Batson, 1990].
The figure of Mars used for the computation of the map projection is an oblate spheroid (flattening
of 1/176.875) with an equatorial radius of 3396.0 km and a polar radius of 3376.8 km (Kirk and
others, 2000). The datum (the 0–km contour line) for elevations is defined as the equipotential surface
(gravitational plus rotational) whose average value at the equator is equal to the mean radius
as determined by Mars Orbiter Laser Altimeter (Smith and others, 2001).
The image base for this map employs Viking Orbiter images from orbit 651. An orthophotomosaic
was created on the digital photogrammetric workstation using the DTM compiled from stereo
models. Integrated Software for Imagers and Spectrometers (ISIS) (Torson and Becker, 1997) provided
the software to project the orthophotomosaic into the Transverse Mercator Projection.
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First posted April 4, 2004
For questions about the content of this report, contact Mark Rosiek
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