From Surf Wiki (app.surf) — the open knowledge base
1809 Prometheus
Main-belt asteroid
Main-belt asteroid
| Field | Value |
|---|---|
| minorplanet | yes |
| name | 1809 Prometheus |
| background | #D6D6D6 |
| image | 001809-asteroid shape model (1809) Prometheus.png |
| caption | Shape model of *Prometheus* from its lightcurve |
| discovery_ref | |
| discovered | 24 September 1960 |
| discoverer | C. J. van Houten |
| I. van Houten-G. | |
| T. Gehrels | |
| (Palomar–Leiden survey) | |
| discovery_site | Palomar Obs. |
| mpc_name | (1809) Prometheus |
| alt_names | 2522 P-L |
| 1955 SW1955 VA | |
| 1965 UR | |
| pronounced | |
| adjective | Promethean, -ian |
| named_after | Προμηθεύς *Promētheys* |
| (Greek mythology) | |
| mp_category | main-belt(outer) |
| orbit_ref | |
| epoch | 4 September 2017 (JD 2458000.5) |
| uncertainty | 0 |
| observation_arc | 61.53 yr (22,473 days) |
| aphelion | 3.2256 AU |
| perihelion | 2.6245 AU |
| semimajor | 2.9251 AU |
| eccentricity | 0.1027 |
| period | 5.00 yr (1,827 days) |
| mean_anomaly | 163.57° |
| mean_motion | / day |
| inclination | 3.2585° |
| asc_node | 99.484° |
| arg_peri | 231.33° |
| dimensions | km |
| albedo | |
| abs_magnitude | 11.7 |
I. van Houten-G. T. Gehrels (Palomar–Leiden survey) 1955 SW1955 VA 1965 UR (Greek mythology)
1809 Prometheus is an asteroid from the outer region of the asteroid belt, approximately 14 kilometers in diameter. Discovered during the Palomar–Leiden survey in 1960, it was given the provisional designation and named after Prometheus from Greek mythology.
Orbit and classification
Prometheus orbits the Sun in the outer main-belt at a distance of 2.6–3.2 AU once every 5.00 years (1,827 days). Its orbit has an eccentricity of 0.10 and an inclination of 3° with respect to the ecliptic.
Discovery
It was discovered on 24 September 1960, by the Dutch astronomer couple Ingrid and Cornelis Johannes van Houten at Leiden, on photographic plates taken by Dutch–American astronomer Tom Gehrels at Palomar, California, in the United States. On the same night, the team of astronomers discovered several other minor planets including 1810 Epimetheus.
Prometheus was first identified as at the Hungarian Konkoly Observatory in 1943. In 1955, its first used observation was taken at Goethe Link Observatory, when it was identified as , extending the body's observation arc by 5 years prior to its official discovery observation.
The survey designation "P-L" stands for Palomar–Leiden, named after Palomar Observatory and Leiden Observatory, which collaborated on the fruitful Palomar–Leiden survey in the 1960s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped the photographic plates to Ingrid and Cornelis van Houten at Leiden, where astrometry was carried out. The trio are credited with the discovery of several thousand minor planets.
Naming
This minor planet was named for Prometheus, a Titan from Greek mythology, who stole the fire from the gods. The name has also been given to a moon of Saturn, Prometheus (moon), discovered by the Voyager 1 spacecraft in 1980. The asteroid 1810 Epimetheus is named after his brother. The official was published by the Minor Planet Center on 20 February 1976 (M.P.C. 3934).
Physical characteristics
According to the surveys carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Prometheus measures 14.2 kilometers in diameter, and its surface has an albedo of 0.126. As of 2017, its spectral type, rotation period and shape remain unknown.
References
References
- "Prometheus". [[Oxford University Press]].
- "Promethean". [[Oxford University Press]].
This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.
Ask Mako anything about 1809 Prometheus — get instant answers, deeper analysis, and related topics.
Research with MakoFree with your Surf account
Create a free account to save articles, ask Mako questions, and organize your research.
Sign up freeThis content may have been generated or modified by AI. CloudSurf Software LLC is not responsible for the accuracy, completeness, or reliability of AI-generated content. Always verify important information from primary sources.
Report