Eliot Patera
What Eliot Patera is
Eliot Patera is a patera — an irregular or scalloped-edged crater, usually volcanic — on Venus, 116 km across, centred at 39.1° N, 79.0° E in the Tellus Tessera quadrangle. It is the 930th largest named feature on Venus and the 14th largest of its class there.
Where the name comes from
George; (Mary Ann Evans) English writer (1819-1880). The International Astronomical Union approved the name in 1991, under the theme it applies to every patera on Venus. Of the 72 features of this class catalogued on Venus, the naming categories run American (13), Russia (11), Great Britain (5), France (4).
What it would take to settle Eliot Patera
Venus scores 43 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 39.1° N, 79.0° E.
What this spot has going for it is sunlight — 78% of the sunlight the sunniest latitude on Venus gets. What works against it is water — same as everywhere else on this world.
Computed from Eliot 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 Venus (radiation geometry, earth link). Gravity, pressure, delta-v and distance from the Sun are the same everywhere on Venus 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 Venus
All 72 paterae on Venus — mapped together, with the naming theme and the size distribution.