Lunar Orbiter 4 image
|Colongitude||9° at sunrise|
Plato is the lava-filled remains of a lunar impact crater on the Moon. It is located on the northeastern shore of the Mare Imbrium, at the western extremity of the Montes Alpes mountain range. In the mare to the south are several rises collectively named the Montes Teneriffe. To the north lies the wide stretch of the Mare Frigoris. East of the crater, among the Montes Alpes, are several rilles collectively named the Rimae Plato.
The age of Plato is about 3.84 billion years, only slightly younger than the Mare Imbrium to the south. The rim is irregular with 2-km-tall jagged peaks that project prominent shadows across the crater floor when the Sun is at a low angle. Sections of the inner wall display signs of past slumping, most notably a large triangular slide along the western side. The rim of Plato is circular, but from the Earth it appears oval due to foreshortening.
The flat floor of Plato has a relatively low albedo, making it appear dark in comparison to the surrounding rugged terrain. The floor is free of significant impact craters and lacks a central peak. However, there are a few small craterlets scattered across the floor.
Plato has developed a reputation for transient lunar phenomena, including flashes of light, unusual colour patterns, and areas of hazy visibility. These anomalies are likely a result of seeing conditions, combined with the effects of different illumination angles of the Sun.
The 17th-century astronomer Hevelius called this feature the 'Greater Black Lake'.
By convention these features are identified on lunar maps by placing the letter on the side of the crater midpoint that is closest to Plato.
|B||53.0° N||17.2° W||13 km|
|C||53.2° N||19.4° W||10 km|
|D||49.6° N||14.5° W||10 km|
|E||49.7° N||16.2° W||7 km|
|F||51.7° N||17.4° W||7 km|
|G||52.1° N||6.3° W||8 km|
|H||55.1° N||2.0° W||11 km|
|J||49.0° N||4.6° W||8 km|
|K||46.8° N||3.3° W||6 km|
|KA||46.8° N||3.6° W||6 km|
|L||51.6° N||4.3° W||10 km|
|M||53.1° N||15.4° W||8 km|
|O||52.3° N||15.4° W||9 km|
|P||51.5° N||15.2° W||8 km|
|Q||54.5° N||4.8° W||8 km|
|R||53.8° N||18.3° W||6 km|
|S||53.8° N||14.9° W||6 km|
|T||54.5° N||11.2° W||8 km|
|U||49.6° N||7.4° W||6 km|
|V||55.8° N||7.4° W||6 km|
|W||57.2° N||17.8° W||4 km|
|X||50.1° N||13.8° W||5 km|
|Y||53.1° N||16.3° W||10 km|
The following craters have been renamed by the IAU:
- Plato A — See Bliss (crater).
Plato in fiction
The crater Plato is the location of an observatory in Arthur C. Clarke's novel Earthlight (1955), of the lunar "warren" Hong Kong Luna in Robert A. Heinlein's novel The Moon Is a Harsh Mistress (1966), and of Moonbase Alpha in the science-fiction TV series Space: 1999.
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- Blue, Jennifer (July 25, 2007). "Gazetteer of Planetary Nomenclature". USGS. Retrieved 2007-08-05.
- Bussey, B.; Spudis, P. (2004). The Clementine Atlas of the Moon. New York: Cambridge University Press. ISBN 978-0-521-81528-4.
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- McDowell, Jonathan (July 15, 2007). "Lunar Nomenclature". Jonathan's Space Report. Retrieved 2007-10-24.
- Menzel, D. H.; Minnaert, M.; Levin, B.; Dollfus, A.; Bell, B. (1971). "Report on Lunar Nomenclature by the Working Group of Commission 17 of the IAU". Space Science Reviews 12 (2): 136–186. Bibcode:1971SSRv...12..136M. doi:10.1007/BF00171763.
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- Rükl, Antonín (1990). Atlas of the Moon. Kalmbach Books. ISBN 978-0-913135-17-4.
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- From LROC: