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The Moon · Crater · 543rd largest named feature

Al Biruni

Abū ar-Rayhān Muhammad ibn Ahmad al-Birūnī; Persian astronomer, mathematician, geographer (973-1048).

What Al Biruni is

Al Biruni is a crater — a circular depression, almost always an impact scar — on The Moon, 80.4 km across, centred at 18.1° N, 92.6° E in the Joliot quadrangle. It is the 543rd largest named feature on The Moon and the 354th largest of its class there.

Where the name comes from

Abū ar-Rayhān Muhammad ibn Ahmad al-Birūnī; Persian astronomer, mathematician, geographer (973-1048). The International Astronomical Union approved the name in 1970, under the theme it applies to every crater on The Moon. Of the 1615 features of this class catalogued on The Moon, the naming categories run Germany (234), American (229), France (163), Great Britain (160).

Feature class
a circular depression, almost always an impact scar
Diameter
80.4 km
about the width of Yellowstone
Coordinates
18.1° N, 92.6° E
Planetocentric, on The Moon
Name approved
1970
By the IAU Working Group for Planetary System Nomenclature
Quadrangle
Joliot
Map sheet on The Moon
Naming category
Persian
Asia

What it would take to settle Al Biruni

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 18.1° N, 92.6° E.

Settlement difficulty here
29.2/ 100
Typical for this world
The Moon overall
29.1
0.1 harder than the median site
Ranked
1036th
of 2,023 named places on The Moon

What this spot has going for it is sunlight 95% of the sunlight the sunniest latitude on The Moon gets. What works against it is water outside the ice-bearing latitudes.

Computed from Al Biruni'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.

Al Biruni's satellite craters

The IAU names smaller craters around a major one by letter. Al Biruni has 1, and each shares the parent's namesake rather than carrying one of its own.

Al Biruni C 9.5 km

What is next to it

The largest crater features on The Moon

All 1,615 craters on The Moon — mapped together, with the naming theme and the size distribution.