Democritus (crater)
![]() Lunar Orbiter 4 image | |
| Coordinates | 62°18′N 35°00′E / 62.3°N 35.0°E |
|---|---|
| Diameter | 37.78 km (23.48 mi)[1] |
| Depth | 2.0 km (1.2 mi) |
| Colongitude | 325° at sunrise |
| Eponym | Democritus |


Democritus is a lunar impact crater that is located on the northern part of the Moon, just to the north of the Mare Frigoris.[2] T. W. Webb described it as "a deep ring-plain".[3] Just to the south of Democritus is the lava-flooded crater Gärtner,[4] which forms a bay on the mare. Directly to the north is Arnold,[2] another flooded formation.
The rim of Democritus is generally sharp-edged and shows little sign of erosion. It forms not quite a circle, with outward notch-like bulges that give it a slightly irregular shape. The inner walls have single or double terraces that lead down to a relatively flat interior floor. Near the midpoint of the crater is a small central peak.[2][5]: 13
This crater is named after the Greek philosopher Democritus (c. 460 – c. 370 BC). Its designation was formally adopted by the International Astronomical Union in 1935.[1] Like many of the craters on the Moon's near side, it was given its name by Giovanni Riccioli, whose 1651 nomenclature system has become standardized.[6]: 212 Earlier lunar cartographers had given the feature different names: Michael van Langren's 1645 map calls it "Alfonsi IX Reg. Cast." after Alfonso IX of León and Castile,[6]: 198 and Johannes Hevelius called it "Mons Bontas".[6]: 202
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 Democritus.[7]
| Democritus[5]: 297 | Latitude | Longitude | Diameter |
|---|---|---|---|
| A | 61.6° N | 32.4° E | 11 km |
| B | 60.1° N | 28.6° E | 12 km |
| D | 62.9° N | 31.2° E | 8 km |
| K | 63.1° N | 40.7° E | 7 km |
| L | 63.4° N | 39.7° E | 18 km |
| M | 63.6° N | 37.1° E | 5 km |
| N | 63.6° N | 34.3° E | 16 km |
The satellite features B includes a permanently shadowed region where the sunlight never reaches.[8]
References
- 1 2 "Democritus". Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program.
- 1 2 3 Moore, Patrick (2001). On the Moon. Sterling Publishing Co. p. 172. ISBN 978-0-304-35469-6.
- ↑ Webb, Rev. T. W. (1962). Celestial Objects for Common Telescopes (6th revised ed.). Dover. pp. 109, 154–159. Reprint: ISBN 978-0-486-20917-3
- ↑ Grego, Peter (2005). The Moon and How to Observe It. Astronomers' Observing Guides Series. London: Springer-Verlag. p. 135. ISBN 1-85233-748-6.
- 1 2 Bussey, B.; Spudis, P. (2004). The Clementine Atlas of the Moon. New York: Cambridge University Press. ISBN 978-0-521-81528-4.
- 1 2 3 Whitaker, Ewen A. (1999). Mapping and Naming the Moon. Cambridge University Press. ISBN 978-0-521-62248-6.
- ↑ Grego, P. (2015). "Satellite Crater". In Hargitai, H.; Kereszturi, Á. (eds.). Encyclopedia of Planetary Landforms. New York, NY: Springer. doi:10.1007/978-1-4614-3134-3_328.
- ↑ McGovern, J. Andrew; et al. (March 2013). "Mapping and characterization of non-polar permanent shadows on the lunar surface". Icarus. 223 (1): 566–581. Bibcode:2013Icar..223..566M. doi:10.1016/j.icarus.2012.10.018.
Sources
- 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.

