Richardson (lunar crater)
Richardson is a large lunar impact crater on the Moon's far side, just behind the eastern limb, with a diameter of 162.56 km and a center at 30.93° north latitude and 99.89° east longitude.1
| Key fact | Detail |
|---|---|
| Diameter | 162.56 km (Gazetteer boundary; an alternate listed boundary gives 141.00 km)1 |
| Center | 30.93° N, 99.89° E (planetographic, east-positive)1 |
| Named after | Sir Owen Willans Richardson, British quantum physicist and Nobel laureate (1879–1959)2 |
Naming and location
The crater honors Sir Owen Willans Richardson, a British quantum physicist and Nobel laureate (1879–1959); the IAU approved the name in 1979.2 The name should not be confused with living scientists of the same surname: Jacob A. Richardson, for example, is a planetary geologist at NASA's Goddard Space Flight Center who serves as Deputy Lunar Science Lead for the Artemis II mission, but the crater predates that association and commemorates the physicist.3 A separate Richardson crater also exists on Mars, in the planet's south (72°S, 179°E), which is a distinct feature on a different body.4
The USGS Gazetteer of Planetary Nomenclature records the crater's position in planetographic coordinates with east-positive longitudes, giving a center at 30.93° N, 99.89° E and a diameter of 162.56 km; the same entry also lists a second, more detailed boundary polygon with a diameter of 141.00 km centered at 31.10° N, 100.50° E, reflecting the irregular shape of the feature.1
Surface appearance and modification
A comparative morphometric study of lunar craters presented at the 46th Lunar and Planetary Science Conference (2015) measured a shape parameter called S₃, which describes a crater's lumpiness. Among the craters examined, Richardson Crater had the maximum S₃ value, and the study attributed its irregular outline to a post-Maxwell crater event that transformed the boundary into a crescent shape.5
Context in lunar crater studies
Richardson belongs to the population of large far-side craters that could only be compared in detail with near-side craters once spacecraft imaging became available; the USGS photographic and geometric studies of lunar craters note that far-side craters at last could be compared in detail with those on the near side.6 Modern global crater databases, such as the Robbins database of more than a million lunar craters with diameters of 1 km or larger, provide the location and size data on which studies of individual features like Richardson now rely.7
References
- Gazetteer of Planetary Nomenclature: Richardson, Feature ID 5027, USGS
- Gazetteer of Planetary Nomenclature: Moon crater search results, USGS
- Jacob A. Richardson, NASA Sciences and Exploration Directorate
- Water ice in the dark dune spots of Richardson crater on Mars, arXiv
- General statistics of lunar craters, 46th Lunar and Planetary Science Conference (2015), abstract 1709
- Geometric Interpretation of Lunar Craters, USGS Professional Paper 1046-C
- A New Global Database of Lunar Impact Craters >1–2 km, Journal of Geophysical Research: Planets (Robbins, 2019)
Initially written Oct 21, 2026 · Edited: Oct 25, 2026
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