Dorsum Buckland
What Dorsum Buckland is
Dorsum Buckland is a dorsum — a ridge — on The Moon, 369 km across, centred at 19.4° N, 14.3° E in the Mare Serenitatis quadrangle. It is the 31st largest named feature on The Moon and the 1st largest of its class there.
Where the name comes from
William; British Earth scientist (1784-1856). The International Astronomical Union approved the name in 1976, under the theme it applies to every dorsum on The Moon. Of the 39 features of this class catalogued on The Moon, the naming categories run Great Britain (8), American (6), Germany (5), Switzerland (4).
What it would take to settle Dorsum Buckland
The Moon scores 29.1 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 19.4° N, 14.3° E.
What this spot has going for it is earth link — near side — Earth stands 66° above the horizon and never moves. What works against it is water — outside the ice-bearing latitudes.
Computed from Dorsum Buckland's catalogued latitude, longitude and feature class — 84% of the model's weight had a basis here, and one axis was dropped as not applicable to The Moon (radiation geometry). Gravity, pressure, delta-v and distance from the Sun are the same everywhere on The Moon 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 The Moon
All 39 dorsa on The Moon — mapped together, with the naming theme and the size distribution.