12564 Ikeller, provisional designation 1998 SO49, is a stony Koronian asteroid from the outer region of the asteroid belt, approximately 5 kilometers in diameter.
Discovery[1] | |
---|---|
Discovered by | W. Bickel |
Discovery site | Bergisch Gladbach Obs. |
Discovery date | 22 September 1998 |
Designations | |
(12564) Ikeller | |
Named after | Ingeborg Bickel–Keller (discoverer's wife)[2] |
1998 SO49 · 1988 RA7 1991 EG5 · 1993 SK13 | |
main-belt · Koronis[3] | |
Orbital characteristics[1] | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 27.90 yr (10,190 days) |
Aphelion | 2.9423 AU |
Perihelion | 2.7273 AU |
2.8348 AU | |
Eccentricity | 0.0379 |
4.77 yr (1,743 days) | |
67.076° | |
0° 12m 23.4s / day | |
Inclination | 1.6200° |
180.04° | |
117.88° | |
Physical characteristics | |
Dimensions | 5.17 km (calculated)[3] 5.369±0.259 km[4][5] |
7.0321±0.0196 h (R)[6] 7.0423±0.0196 h (S)[6] | |
0.222±0.049[5] 0.2225±0.0495[4] 0.24 (assumed)[3] | |
S[3] | |
13.6[1][3][4] · 13.644±0.003 (R)[6] · 14.16±0.23[7] · 14.282±0.007 (S)[6] | |
The asteroid was discovered by German amateur astronomer Wolf Bickel at his private Bergisch Gladbach Observatory on 22 September 1998. It was named after the discoverer's wife, Ingeborg Bickel–Keller.[2]
Orbit and classification
Ikeller is a member of the Koronis family, a group of stony asteroids in the outer main-belt named after 158 Koronis. It orbits the Sun at a distance of 2.7–2.9 AU once every 4 years and 9 months (1,743 days). Its orbit has an eccentricity of 0.04 and an inclination of 2° with respect to the ecliptic.[1]
The body's observation arc begins 10 years prior to its official discovery observation, with its identification as 1988 RA7 at ESO's La Silla Observatory in September 1988.[2]
Physical characteristics
According to the survey carried out by the NEOWISE mission of NASA's space-based Wide-field Infrared Survey Explorer, Ikeller measures 5.4 kilometers in diameter and its surface has an albedo of 0.22,[4] while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for Koronian asteroids of 0.24 and thus calculates a smaller diameter of 5.2 kilometers, as the higher the albedo (reflectivity), the smaller a body's diameter at a certain absolute magnitude (brightness).[3]
Lightcurve
In August 2012, a photometric lightcurve of Ikeller was obtained from photometric observations by astronomers at the Palomar Transient Factory in California. Lightcurve analysis gave a rotation period of 7.0423 hours with a brightness variation of 0.44 magnitude (U=2).[6]
Naming
This minor planet was named by the discoverer after his wife, Ingeborg Bickel–Keller (born 1941).[2] The approved naming citation was published by the Minor Planet Center on 16 January 2014 (M.P.C. 86713).[8]
References
External links
- Koronis Family Asteroids Rotation Lightcurve Observing Program, Stephen M. Slivan, 2013
- Asteroid Lightcurve Database (LCDB), query form (info Archived 16 December 2017 at the Wayback Machine)
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (10001)-(15000) – Minor Planet Center
- 12564 Ikeller at AstDyS-2, Asteroids—Dynamic Site
- 12564 Ikeller at the JPL Small-Body Database