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1809 Prometheus

Main-belt asteroid


Main-belt asteroid

FieldValue
minorplanetyes
name1809 Prometheus
background#D6D6D6
image001809-asteroid shape model (1809) Prometheus.png
captionShape model of *Prometheus* from its lightcurve
discovery_ref
discovered24 September 1960
discovererC. J. van Houten
I. van Houten-G.
T. Gehrels
(Palomar–Leiden survey)
discovery_sitePalomar Obs.
mpc_name(1809) Prometheus
alt_names2522 P-L
1955 SW1955 VA
1965 UR
pronounced
adjectivePromethean, -ian
named_afterΠρομηθεύς *Promētheys*
(Greek mythology)
mp_categorymain-belt(outer)
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc61.53 yr (22,473 days)
aphelion3.2256 AU
perihelion2.6245 AU
semimajor2.9251 AU
eccentricity0.1027
period5.00 yr (1,827 days)
mean_anomaly163.57°
mean_motion/ day
inclination3.2585°
asc_node99.484°
arg_peri231.33°
dimensionskm
albedo
abs_magnitude11.7

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

  1. "Prometheus". [[Oxford University Press]].
  2. "Promethean". [[Oxford University Press]].
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