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12564 Ikeller

From Wikipedia, the free encyclopedia
Stony Koronian asteroid

12564 Ikeller
Discovery[1]
Discovered byW. Bickel
Discovery siteBergisch Gladbach Obs.
Discovery date22 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 arc27.90 yr (10,190 days)
Aphelion2.9423AU
Perihelion2.7273 AU
2.8348 AU
Eccentricity0.0379
4.77yr (1,743 days)
67.076°
0° 12m 23.4s / day
Inclination1.6200°
180.04°
117.88°
Physical characteristics
Dimensions5.17 km(calculated)[3]
5.369±0.259 km[4][5]
7.0321±0.0196h(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 designation1998 SO49, is a stony Koronianasteroid from the outer region of theasteroid belt, approximately 5 kilometers in diameter.

The asteroid was discovered by German amateur astronomerWolf Bickel at his privateBergisch Gladbach Observatory on 22 September 1998. It was named after the discoverer's wife, Ingeborg Bickel–Keller.[2]

Orbit and classification

[edit]

Ikeller is a member of theKoronis family, a group ofstony asteroids in theouter main-belt named after158 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 aneccentricity of 0.04 and aninclination of 2° with respect to theecliptic.[1]

The body'sobservation arc begins 10 years prior to its official discovery observation, with its identification as1988 RA7 at ESO'sLa Silla Observatory in September 1988.[2]

Physical characteristics

[edit]

According to the survey carried out by theNEOWISE mission of NASA's space-basedWide-field Infrared Survey Explorer,Ikeller measures 5.4 kilometers in diameter and its surface has analbedo of 0.22,[4] while theCollaborative 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 certainabsolute magnitude (brightness).[3]

Lightcurve

[edit]

In August 2012, a photometriclightcurve ofIkeller was obtained from photometric observations by astronomers at thePalomar Transient Factory in California. Lightcurve analysis gave arotation period of7.0423 hours with a brightness variation of 0.44magnitude (U=2).[6]

Naming

[edit]

Thisminor planet was named by the discoverer after his wife, Ingeborg Bickel–Keller (born 1941).[2] The approved naming citation was published by theMinor Planet Center on 16 January 2014 (M.P.C. 86713).[8]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 12564 Ikeller (1998 SO49)" (2016-08-03 last obs.).Jet Propulsion Laboratory. Retrieved24 June 2017.
  2. ^abcd"12564 Ikeller (1998 SO49)".Minor Planet Center. Retrieved5 April 2016.
  3. ^abcdef"LCDB Data for (12564) Ikeller". Asteroid Lightcurve Database (LCDB). Retrieved17 May 2016.
  4. ^abcdMainzer, 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. Retrieved17 May 2016.
  5. ^abMasiero, 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. Retrieved4 December 2016.
  6. ^abcdeWaszczak, 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. Retrieved17 May 2016.
  7. ^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. Retrieved17 May 2016.
  8. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved17 May 2016.

External links

[edit]
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