Pythagoras (crater)
![]() Pythagoras shadowed with its central peak seen near the terminator boundary | |
| Coordinates | 63°30′N 62°48′W / 63.5°N 62.8°W |
|---|---|
| Diameter | 130 km |
| Depth | 5.0 km |
| Colongitude | 60° at sunrise |
| Formation | Eratosthenian[1] |
| Eponym | Pythagoras |

(four light spots are blemishes on original)
Pythagoras is a prominent impact crater located near the northwestern limb of the Moon. T. W. Webb described it as "the deepest walled plain" in this quadrant of the visible Moon.[2] It lies just to the northwest of the somewhat larger Babbage. The crater has an oval appearance due to the oblique viewing angle. Only the western face of the interior can be viewed from the Earth, the other side being permanently out of sight.[3]
On the lunar geologic timescale, Pythagoras is a crater of Eratosthenian age.[1] The well-preserved rim of Pythagoras has a wide terrace system, and a slight rampart around the exterior. Although generally circular, the crater outline has a hexagonal form. The floor is flattened, but with an irregular, hilly surface. There is evidence of landslips around the periphery.[4]: 10 In the center is a sharp, mountainous rise with a double peak that ascends 1.5 kilometers above the crater floor. Anorthosite with a very low mafic abundance[5] and the infrared spectrum of pure crystalline plagioclase has been identified in the central peaks.[6]
This crater is named after Greek mathematician and philosopher Pythagoras of Samos (c. 570 – c. 495 BC). Its designation was formally adopted by the International Astronomical Union in 1935.[7] The name was incorporated into lunar nomenclature by Italian astronomer Giovanni Riccioli in 1651.[8]
Satellite craters
By convention these features are identified on lunar maps by placing the letter on the side of the crater midpoint that is closest to Pythagoras.
| Pythagoras[4]: 310 | Latitude | Longitude | Diameter |
|---|---|---|---|
| B | 66.1° N | 73.0° W | 17 km |
| D | 64.5° N | 72.0° W | 30 km |
| G | 67.8° N | 75.3° W | 16 km |
| H | 67.1° N | 73.3° W | 18 km |
| K | 67.3° N | 75.4° W | 12 km |
| L | 67.3° N | 77.6° W | 12 km |
| M | 67.5° N | 81.1° W | 10 km |
| N | 66.6° N | 78.1° W | 14 km |
| P | 65.3° N | 75.2° W | 10 km |
| S | 67.7° N | 64.7° W | 8 km |
| T | 62.5° N | 51.4° W | 6 km |
| W | 63.1° N | 48.9° W | 4 km |
References
- 1 2 Wilhelms, Don E.; McCauley, John F.; Trask, Newell J. (1987). The geologic history of the Moon. USGS Professional Paper 1348. Washington: U.S. Government Printing Office. doi:10.3133/pp1348. Table 12.2.
- ↑ Webb, Rev. T. W. (1962). Celestial Objects for Common Telescopes (6th revised ed.). Dover. pp. 130, 154–159. Reprint: ISBN 978-0-486-20917-3
- ↑ Wood, Chuck (October 9, 2007). "Copernicus on the Limb". Lunar Photo of the Day. Retrieved 2026-05-18.
- 1 2 Bussey, B.; Spudis, P. (2004). The Clementine Atlas of the Moon. New York: Cambridge University Press. ISBN 978-0-521-81528-4.
- ↑ Lemelin, Myriam; et al. (May 2015). "Lunar central peak mineralogy and iron content using the Kaguya Multiband Imager: Reassessment of the compositional structure of the lunar crust". JRG Planets. 120 (5): 869–887. doi:10.1002/2014JE004778.
- ↑ Donaldson Hanna, K. L.; et al. (July 2014). "Global assessment of pure crystalline plagioclase across the Moon and implications for the evolution of the primary crust". Journal of Geophysical Research: Planets. 119 (7): 1516–1545. Bibcode:2014JGRE..119.1516D. doi:10.1002/2013JE004476.
- ↑ "Pythagoras". Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program.
- ↑ Whitaker, Ewen A. (1999). Mapping and Naming the Moon. Cambridge University Press. pp. 60, 214. ISBN 978-0-521-62248-6.
Sources
- Moore, Patrick (2001). On the Moon. Sterling Publishing Co. ISBN 978-0-304-35469-6.
- Price, Fred W. (1988). The Moon Observer's Handbook. Cambridge University Press. ISBN 978-0-521-33500-3.
- Rükl, Antonín (1990). Atlas of the Moon. Kalmbach Books. ISBN 978-0-913135-17-4.
- Wlasuk, Peter T. (2000). Observing the Moon. Springer. ISBN 978-1-85233-193-1.

