Laverna Dorsa
What Laverna Dorsa is
Laverna Dorsa is a dorsum — a ridge — on Venus, 1,100 km across, centred at 50.0° S, 132.0° E. It is the 152nd largest named feature on Venus and the 27th largest of its class there.
Where the name comes from
Roman darkness and income goddess. The International Astronomical Union approved the name in 1997, under the theme it applies to every dorsum on Venus. Of the 99 features of this class catalogued on Venus, the naming categories run Slavic (9), Siberia (8), Greek (6), Lithuania (5).
What it would take to settle Laverna Dorsa
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 50.0° S, 132.0° E.
What this spot has going for it is known ground — 6,047 km from Vega 2 (1985). What works against it is water — same as everywhere else on this world.
Computed from Laverna 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 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 dorsum features on Venus
All 99 dorsa on Venus — mapped together, with the naming theme and the size distribution.