12564 Ikeller
| 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 16 February 2017 (JD 2457800.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 26.84 yr (9,802 days) |
| Aphelion | 2.9414 AU |
| Perihelion | 2.7273 AU |
| 2.8343 AU | |
| Eccentricity | 0.0378 |
| 4.77 yr (1,743 days) | |
| 25.904° | |
| 0° 12m 23.76s / day | |
| Inclination | 1.6199° |
| 180.04° | |
| 117.75° | |
| 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] | |
12564 Ikeller, provisional designation 1998 SO49, is a stony Koronis asteroid from the outer region of the asteroid belt, approximately 5 kilometers in diameter. It was discovered by German amateur astronomer Wolf Bickel at his private Bergisch Gladbach Observatory on 22 September 1998.[2]
The S-type asteroid is a member of the Koronis family, which is named after 158 Koronis and consists of about 300 known bodies. 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 a typically low inclination of 2° with respect to the ecliptic.[1] The first precovery was obtained at ESO's La Silla Observatory in 1988, extending the asteroid's observation arc by 10 years prior to its discovery.[2]
According to the survey carried out by the NEOWISE mission of NASA's space-based Wide-field Infrared Survey Explorer, the asteroid measures 5.4 kilometers in diameter and its surface has an albedo of 0.22,[4] while the Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 and thus calculates a smaller diameter of 5.2 kilometers, as the higher the albedo (reflectivity), the smaller the body's diameter at a constant absolute magnitude (brightness).[3] In August 2012, a photometric light-curve analysis at the U.S. Palomar Transient Factory, California, rendered a rotation period of 7.0423±0.0196 hours with a brightness amplitude of 0.44 in magnitude (U=2).[6]
The minor planet was named by the discoverer after his wife, Ingeborg Bickel–Keller (b. 1941).[2] Naming citation was published on 16 January 2014 (M.P.C. 86713).[8]
References
- ^ a b c d "JPL Small-Body Database Browser: 12564 Ikeller (1998 SO49)" (2015-07-12 last obs.). Jet Propulsion Laboratory. Retrieved 4 December 2016.
- ^ a b c d "12564 Ikeller (1998 SO49)". Minor Planet Center. Retrieved 5 April 2016.
- ^ a b c d e f "LCDB Data for (12564) Ikeller". Asteroid Lightcurve Database (LCDB). Retrieved 17 May 2016.
- ^ a b c d Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results". The Astrophysical Journal. 741 (2): 25. arXiv:1109.6407. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. Retrieved 17 May 2016.
- ^ a b Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011). "Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters". The Astrophysical Journal. 741 (2): 20. arXiv:1109.4096. Bibcode:2011ApJ...741...68M. doi:10.1088/0004-637X/741/2/68. Retrieved 4 December 2016.
{{cite journal}}: CS1 maint: multiple names: authors list (link) - ^ a b c d e Waszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015). "Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry". The Astronomical Journal. 150 (3): 35. arXiv:1504.04041. Bibcode:2015AJ....150...75W. doi:10.1088/0004-6256/150/3/75. Retrieved 17 May 2016.
- ^ Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015). "Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results". Icarus. 261: 34–47. arXiv:1506.00762. Bibcode:2015Icar..261...34V. doi:10.1016/j.icarus.2015.08.007. Retrieved 17 May 2016.
- ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 17 May 2016.
External links
- Koronis Family Asteroids Rotation Lightcurve Observing Program, Stephen M. Slivan, 2013
- Asteroid Lightcurve Database (LCDB), query form (info)
- 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 the JPL Small-Body Database
