Uranius Patera
What Uranius Patera is
Uranius Patera is a patera — an irregular or scalloped-edged crater, usually volcanic — on Mars, 114 km across, centred at 26.3° N, 92.8° W in the Tharsis quadrangle. It is the 585th largest named feature on Mars and the 7th largest of its class there.
Where the name comes from
Classical albedo feature name. The International Astronomical Union approved the name in 1973, under the theme it applies to every patera on Mars. Of the 30 features of this class catalogued on Mars, the naming categories run Greek (20), Latin (8), Hebrew (2).
What it would take to settle Uranius Patera
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 26.3° N, 92.8° W.
What this spot has going for it is sunlight — 91% of the sunlight the sunniest latitude on Mars gets. What works against it is water — outside the ice-bearing latitudes.
Computed from Uranius Patera'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 patera features on Mars
All 30 paterae on Mars — mapped together, with the naming theme and the size distribution.