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(6491) 1991 OA

Highly eccentric stony asteroid


Highly eccentric stony asteroid

FieldValue
minorplanetyes
name(6491) 1991 OA
background#FFC2E0
discovery_ref
discovered16 July 1991
discovererH. E. Holt
discovery_sitePalomar Obs.
mpc_name(6491) 1991 OA
mp_categoryNEOAmorPHA
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc24.35 yr (8,895 days)
aphelion3.9772 AU
perihelion1.0227 AU
semimajor2.5000 AU
eccentricity0.5909
period3.95 yr (1,444 days)
mean_anomaly215.03°
mean_motion/ day
inclination5.9464°
asc_node301.90°
arg_peri323.60°
moid0.0420 AU16.4 LD
dimensions0.52 km (derived)
rotationh
albedo0.20 (assumed)
spectral_typeS
abs_magnitude18.7718.9

**** is a highly eccentric, stony asteroid, classified as near-Earth object and potentially hazardous asteroid, approximately half a kilometer in diameter. It was discovered on 16 July 1991, by American astronomer Henry E. Holt at the U.S. Palomar Observatory in California.

Orbit and classification

The S-type body is an Amor asteroid – a subgroup of near-Earth asteroids that approach the orbit of Earth from beyond, but do not cross it. It orbits the Sun at a distance of 1.0–4.0 AU once every 3 years and 11 months (1,444 days). Its orbit has an eccentricity of 0.59 and an inclination of 6° with respect to the ecliptic. Its minimum orbit intersection distance (MOID) with Earth is 0.0420 AU, and on 1 August 2086, it will make a close approach and pass by Earth at a distance of 0.09 AU.

A first precovery was taken at the Australian Siding Spring Observatory in March 1991, extending the asteroid's observation arc by 4 months prior to its discovery.

Physical characteristics

In 2000, a rotational lightcurve was published from photometric observations obtained by the Near-Earth Objects Follow-up Program during the early 1990s. The lightcurve rendered a rotation period of 2.69 hours with an brightness amplitude of 0.08 in magnitude (). The Collaborative Asteroid Lightcurve Link (CALL) assumes an albedo of 0.20 and derives a diameter of 0.53 kilometers, based on an absolute magnitude of 18.77.

Naming

As of 2017, remains unnamed.

References

Info: Wikipedia Source

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.

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