Geologic maps of science study area 3, Olympus Rupes, Mars
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Abstract
This map is one in a series of 1:500,000-scale geologic maps initiated by the National Aeronautics and Space Administration to investigate areas of particular scientific interest on Mars. Olympus Mons is the largest known volcanic construct in the Solar System; it is more than 600 km across and more than 27 km above datum (fig, 1, sheet 1). The volcano and the great scarp that bounds it have been the subject of much scientific controversy. Although it has been possible to generate an empirical model that closely resembles Olympus Mons (fig. 2, sheet 1), the dynamics of scarp formation are still unproven. The scarp area is thus a logical selection as a scientific study area. It has also been designated as a candidate site for a proposed lander/rover/sample-return mission to Mars (fig. 1, sheet 2) not only because the site may provide information about the origins of the scarp and the evolution of Olympus Mons, but also because the rocks of widely diverse ages may be studied from the samples collected from talus at the base of the scarp.
| Publication type | Report |
|---|---|
| Publication Subtype | USGS Numbered Series |
| Title | Geologic maps of science study area 3, Olympus Rupes, Mars |
| Series title | IMAP |
| Series number | 2001 |
| DOI | 10.3133/i2001 |
| Year Published | 1991 |
| Language | English |
| Publisher | U.S. Geological Survey |
| Description | 2 Plates: 45.00 × 37.00 inches and 56.00 × 31.00 inches |
| Other Geospatial | Mars, Olympus Rupes |
| Scale | 502000 |
| Google Analytic Metrics | Metrics page |