Nakahi Facula
What Nakahi Facula is
Nakahi Facula is a facula — a bright spot — on Mercury, 64 km across, centred at 52.7° S, 17.8° E in the Cyllene quadrangle. It is the 409th largest named feature on Mercury and the 11th largest of its class there.
Where the name comes from
MÄori word for snake. The International Astronomical Union approved the name in 2018, under the theme it applies to every facula on Mercury. Of the 29 features of this class catalogued on Mercury, the naming categories run India (2), Nigeria (2), Philippines (2), Ireland (1).
What it would take to settle Nakahi Facula
Mercury scores 46 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 52.7° S, 17.8° E.
What this spot has going for it is ground — flat ground — the easiest thing to land on and build across. What works against it is water — outside the ice-bearing latitudes.
Computed from Nakahi Facula's catalogued latitude, longitude and feature class — 68% of the model's weight had a basis here, and 3 axes were dropped as not applicable to Mercury (radiation geometry, earth link, known ground). Gravity, pressure, delta-v and distance from the Sun are the same everywhere on Mercury 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 facula features on Mercury
All 29 faculae on Mercury — mapped together, with the naming theme and the size distribution.