10656 Albrecht
| Discovery [1] | |
|---|---|
| Discovered by |
C. J. van Houten I. van Houten-G. T. Gehrels |
| Discovery site | Palomar Obs. |
| Discovery date | 25 March 1971 |
| Designations | |
| MPC designation | 10656 Albrecht |
Named after |
Carl Albrecht (astronomer)[2] |
|
2213 T-1 · 1990 SZ25 3011 T-2 | |
| main-belt · (outer) [3] | |
| Orbital characteristics [1] | |
| Epoch 16 February 2017 (JD 2457800.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 63.31 yr (23,125 days) |
| Aphelion | 3.4447 AU |
| Perihelion | 2.9071 AU |
| 3.1759 AU | |
| Eccentricity | 0.0846 |
| 5.66 yr (2,067 days) | |
| 277.46° | |
| 0° 10m 26.76s / day | |
| Inclination | 8.5246° |
| 5.2089° | |
| 316.96° | |
| Physical characteristics | |
| Dimensions |
7.057±0.365 km[4][5] 12.83 km (calculated)[3] |
| 14.4899±0.0684 h[6] | |
|
0.057 (assumed)[3] 0.323±0.057[4][5] | |
| C [3] | |
| 12.8[1] · 12.6[4] · 12.737±0.004 (R)[6] · 13.19[3] | |
|
| |
10656 Albrecht, provisional designation 2213 T-1, is a carbonaceous asteroid from the outer region of the asteroid belt, approximately 10 kilometers in diameter. It was discovered on 25 March 1971, by Dutch astronomer couple Ingrid and Cornelis van Houten, on photographic plates taken by Dutch–American astronomer Tom Gehrels at the U.S. Palomar Observatory, California.[7]
The dark C-type asteroid orbits the Sun at a distance of 2.9–3.4 AU once every 5 years and 8 months (2,067 days). Its orbit has an eccentricity of 0.08 and an inclination of 9° with respect to the ecliptic.of 2.9–3.4 AU once every 5 years and 8 months (2,070 days). Its orbit is tilted by 9° to the plane of the ecliptic and shows an eccentricity of 0.09.[1] The first precovery was taken at Palomar Observatory in 1953, extending the asteroid's observation arc by 18 years prior to its discovery.[7]
A rotational light-curve of this asteroid was obtained from photometric observations made at the U.S. Palomar Transient Factory in October 2013. The light-curve gave a rotation period of 14.4899±0.0684 hours with a brightness amplitude of 0.35 in magnitude (U=2).[6]
According to the survey carried out by the NEOWISE mission of NASA's space-based Wide-field Infrared Survey Explorer, the asteroid measures 7.1 kilometers in diameter and its surface has a high albedo of 0.32,[4][5] while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a larger diameter of 12.8 kilometers, based on an absolute magnitude of 13.19.[3]
The special designation T-1 stands for the first Palomar–Leiden Trojan survey, named after the fruitful collaboration of the Palomar and Leiden Observatory in the 1960s and 1970s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped the photographic plates to Cornelis and Ingrid van Houten-Groeneveld at Leiden Observatory where astrometry was carried out. The trio of astronomers are credited with the discovery of 4,620 minor planets.[8]
The minor planet was named in honor of German astronomer Carl Theodor Albrecht (1843–1915), who was instrumental in establishing the International Latitude Service (ILS) in 1899. The ILS was located at the Prussian Geodetic Institute in Berlin. Albrecht was also the first director of the ILS.[2] Naming citation was published on 20 November 2002 (M.P.C. 47167).[9]
References
- 1 2 3 4 "JPL Small-Body Database Browser: 10656 Albrecht (2213 T-1)" (2016-06-09 last obs.). Jet Propulsion Laboratory. Retrieved 4 December 2016.
- 1 2 Schmadel, Lutz D. (2007). Dictionary of Minor Planet Names – (10656) Albrecht. Springer Berlin Heidelberg. p. 741. ISBN 978-3-540-00238-3. Retrieved 7 May 2016.
- 1 2 3 4 5 6 "LCDB Data for (10656) Albrecht". Asteroid Lightcurve Database (LCDB). Retrieved 7 May 2016.
- 1 2 3 4 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 7 May 2016. - 1 2 3 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.
- 1 2 3 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 7 May 2016.
- 1 2 "10656 Albrecht (2213 T-1)". Minor Planet Center. Retrieved 7 May 2016.
- ↑ "Minor Planet Discoverers". Minor Planet Center. 28 December 2015. Retrieved 1 January 2016.
- ↑ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 7 May 2016.
External links
- The International Latitude Service – A Historical Review, Joachim Höpfner
- 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 (10000)-(15000) – Minor Planet Center
- 10656 Albrecht at the JPL Small-Body Database
