Cerberus Dorsa
What Cerberus Dorsa is
Cerberus Dorsa is a dorsum — a ridge — on Mars, 623 km across, centred at 13.7° S, 105.3° E in the Mare Tyrrhenum quadrangle. It is the 154th largest named feature on Mars and the 10th largest of its class there.
Where the name comes from
Classical albedo feature name. The International Astronomical Union approved the name in 1982, under the theme it applies to every dorsum on Mars. Of the 36 features of this class catalogued on Mars, the naming categories run Greek (20), Latin (13), Egypt (1), Syria (1).
What it would take to settle Cerberus Dorsa
Mars scores 26.6 as a world. That number is the same for every square metre of it — but sunlight, water, radiation and the ground under your feet are not. This is the same question asked at 13.7° S, 105.3° E.
What this spot has going for it is sunlight — 97% of the sunlight the sunniest latitude on Mars gets. What works against it is water — outside the ice-bearing latitudes.
Computed from Cerberus Dorsa's catalogued latitude, longitude and feature class — 74% of the model's weight had a basis here, and 2 axes were dropped as not applicable to Mars (radiation geometry, earth link). Gravity, pressure, delta-v and distance from the Sun are the same everywhere on Mars and are already counted in the world's own index, not again here.
What this cannot see: elevation. Slope, local shadowing and the polar “peaks of eternal light” — ridge tops near the poles of a barely tilted world that catch sun almost continuously while a crater floor kilometres away never does — need a terrain model this does not have. Where a real mission targets a pole, that is usually why.
What is next to it
The largest dorsum features on Mars
All 36 dorsa on Mars — mapped together, with the naming theme and the size distribution.