10502 Armaghobs

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10502 Armaghobs
Discovery [1]
Discovered by E. F. Helin
Discovery site Palomar Obs.
Discovery date 22 August 1987
Designations
MPC designation 10502 Armaghobs
Named after
Armagh Observatory
(astronomical observatory)[2]
1987 QF6 · 1980 PJ2
1994 RJ29
Mars-crosser[3]
Orbital characteristics[1]
Epoch 27 June 2015 (JD 2457200.5)
Uncertainty parameter 0
Observation arc 35.33 yr (12,906 days)     
Aphelion 3.0424 AU
Perihelion 1.5759 AU
2.3092 AU
Eccentricity 0.3175
3.51 yr (1,282 days)
281.27°
Inclination 21.936°
170.25°
263.19°
Earth MOID 0.7434 AU
Physical characteristics
Dimensions 2.97 km (calculated)[3]
24.978±0.002 h[4]
0.20 (assumed)[3]
S[3]
15.0[1]

10502 Armaghobs, provisional designation 1987 QF6, is an eccentric asteroid from the inner regions of the asteroid belt, classified as Mars-crossing asteroid, about 3 kilometers in diameter. It was discovered by American female astronomer Eleanor Helin at the U.S. Palomar Observatory in California, on 22 August 1987.[5]

The S-type asteroid orbits the Sun at a distance of 1.6–3.0 AU once every 3 years and 6 months (1,282 days). Its orbit is tilted by 22 degrees to the plane of the ecliptic and shows a notable eccentricity of 0.32.[1] In 2013, a photometric light-curve analysis at the Riverland Dingo Observatory at Moorook, South Australia, has given rotation period of 24.978±0.002 hours with a brightness amplitude of 0.51 in magnitude,[4] while the Collaborative Asteroid Lightcurve Link assumes an albedo of 0.20 for the asteroid's surface, a typical value for bodies with a stony composition.[3]

The minor planet was named after the Armagh Observatory in Northern Ireland. The modern astronomical research institute was founded by Archbishop Richard Robinson in 1790. It is has a rich heritage, that includes T. R. Robinson's cup-anemometer, Dreyer's NGC Catalogue, Lindsay's Armagh-Dunsink-Harvard telescope and the work of the Estonian astronomer E. J. Öpik, after whom the minor planet 2099 Öpik was named.[2]

References

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External links


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