Abstract
Olympus Mons, one of the largest known shield volcanoes in the Solar System, covers an area of >3.2 × 105 km2and has a diameter of >600 km, excluding its vast aureole deposits. The structure is five times larger than the largest shield volcano on the Earth. It is situated on the north-west flank of the Tharsis volcanic region, a broad topographic rise on the martian surface. The volcano has three physical subdivisions: the summit caldera, the terraced upper flanks, and the lower flanks, which terminate in a scarp 2–10 km high that nearly surrounds the structure. A large block of images of the Tharsis region, including Olympus Mons, was obtained by the Viking mission1. Here we present a topographic map of Olympus Mons, compiled using various combinations of stereo pairs of these images, together with stereoscopic perspective views generated by image processing techniques.
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Wu, S., Garcia, P., Jordan, R. et al. Topography of the shield volcano, Olympus Mons on Mars. Nature 309, 432–435 (1984). https://doi.org/10.1038/309432a0
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DOI: https://doi.org/10.1038/309432a0
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