*** Welcome to piglix ***

39890 Bobstephens

39890 Bobstephens
Discovery 
Discovered by P. Pravec
Discovery site Ondřejov Obs.
Discovery date 23 March 1998
Designations
MPC designation (39890) Bobstephens
Named after
Robert D. Stephens (astronomer)
1998 FA3
main-belt · (middle)
Orbital characteristics
Epoch 16 February 2017 (JD 2457800.5)
Uncertainty parameter 0
Observation arc 21.03 yr (7,682 days)
Aphelion 3.1534 AU
Perihelion 2.0295 AU
2.5914 AU
Eccentricity 0.2168
4.17 yr (1,524 days)
154.21°
0° 14m 10.68s / day
Inclination 5.4949°
161.74°
95.738°
Physical characteristics
Dimensions 2.06 km (calculated)
9.55±0.01 h
0.20 (assumed)
S
15.8 · 15.9

39890 Bobstephens, provisional designation 1998 FA3, is a stony asteroid from the middle region of the asteroid belt, approximately 2 kilometers in diameter. It was discovered on 23 March 1998, by Czech astronomer Petr Pravec at Ondřejov Observatory near Prague in the Czech Republic.

Bobstephens is a S-type asteroid and orbits the Sun at a distance of 2.0–3.2 AU once every 4 years and 2 months (1,524 days). Its orbit has an eccentricity of 0.22 and an inclination of 5° with respect to the ecliptic. It was first imaged at Steward Observatory in 1995. This precovery extends the body's observation arc by 3 years prior to its official discovery observation.

In August 2008, a rotational light-curve of Bobstephens was obtained from photometric observations by American amateur astronomer Daniel Coley at the Center for Solar System Studies in California. Light-curve analysis gave a rotation period of 9.55 hours with a brightness variation of 0.20 magnitude (U=2).

The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 2.06 kilometers, using an absolute magnitude of 15.8.

This minor planet was named for well-known Californian amateur astronomer Robert D. Stephens (b. 1955), who is an expert in light-curve photometry of minor planets since 1999. Naming citation was published on 24 July 2002 (M.P.C. 46112).


...
Wikipedia

...