On the Martian surface, the mountains are high and the canyons are low. Really, really low.
Not only is the martian volcano Olympus Mons the highest peak in the
Compared to the average shape of Mars, known as the “aeroid,” the canyon floor sinks down about 3.1 miles. Planetary scientists would love to use sea level measurements to describe Martian surface features, but there’s no ocean on the red planet anymore and any signs of an ocean are long since warped by millions of years of surface deformation.
The photo above covers about 7,700 square miles, or about the size of New Jersey, which makes it only a tiny postage stamp of Mars’ deepest, longest and most prominent scar — the 2,500-mile-long Valles Marineris rift valley (below).
Images: 1) Melas Chasma – high-resolution image, ESA/DLR/FU Berlin (G. Neukum), 2) Viking 1 and 2 orbiter image collage of Valles Marineris canyon – high-resolution image. Courtesy NASA/JPL-Caltech
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Authors: Dave Mosher