8967 Calandra
| Discovery [1] | |
|---|---|
| Discovered by | C. J. van Houten I. van Houten-G. T. Gehrels |
| Discovery site | Palomar Obs. |
| Discovery date | 13 May 1971 |
| Designations | |
| 8967 Calandra | |
Named after | Miliaria calandra (endangered bird)[2] |
| 4878 T-1 · 1978 RM11 1992 EH15 | |
| main-belt · (outer) [3] | |
| Orbital characteristics [1] | |
| Epoch 16 February 2017 (JD 2457800.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 45.49 yr (16,616 days) |
| Aphelion | 3.4085 AU |
| Perihelion | 2.7049 AU |
| 3.0567 AU | |
| Eccentricity | 0.1151 |
| 5.34 yr (1,952 days) | |
| 62.089° | |
| 0° 11m 3.84s / day | |
| Inclination | 9.7428° |
| 170.63° | |
| 171.72° | |
| Physical characteristics | |
| Dimensions | 8.382±0.103 km[4][5] 10.92 km (calculated)[3] |
| 5.2427±0.0036 h[6] | |
| 0.057 (assumed)[3] 0.174±0.030[4][5] | |
| C [3] | |
| 13.1[1] · 13.54[3] · 12.9[4] · 13.086±0.004[6] · 13.30±0.10[7] | |
8967 Calandra, provisional designation 4878 T-1, is a carbonaceous asteroid from the outer region of the asteroid belt, approximately 9 kilometers in diameter. It was discovered on 13 May 1971, by Dutch astronomer couple Ingrid and Cornelis van Houten at Leiden Observatory, on photographic plates taken by Dutch–American astronomer Tom Gehrels at the U.S Palomar Observatory, California.[8]
The dark C-type asteroid orbits the Sun at a distance of 2.7–3.4 AU once every 5 years and 4 months (1,952 days). Its orbit has an eccentricity of 0.12 and an inclination of 10° with respect to the ecliptic.[1] No precoveries were taken prior to its discovery.[8]
In 2011, a photometric light-curve analysis at the U.S. Palomar Transient Factory, California, rendered a rotation period of 5.2427±0.0036 hours with a brightness amplitude of 0.58 in magnitude (U=2).[6] According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, the asteroid measures 8.4 kilometers in diameter and its surface has an albedo of 0.17.[4][5] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and hence calculates a larger diameter of 10.2 kilometers.[3]
The survey 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 at Leiden Observatory where astrometry was carried out. The trio of astronomers are credited with the discovery of 4,620 minor planets.[9]
The minor planet is named for the passerine bird, Miliaria calandra, also known as corn bunting.[2] As of 2015, it is listed as an endangered species on the European Red List of Birds.[10] Naming citation was published on 2 February 1999 (M.P.C. 33794).[11]
References
- ^ a b c d "JPL Small-Body Database Browser: 8967 Calandra (4878 T-1)" (2016-11-08 last obs.). Jet Propulsion Laboratory. Retrieved 4 December 2016.
- ^ a b Schmadel, Lutz D. (2007). Dictionary of Minor Planet Names – (8967) Calandra. Springer Berlin Heidelberg. p. 672. ISBN 978-3-540-00238-3. Retrieved 1 March 2016.
- ^ a b c d e f "LCDB Data for (8967) Calandra". 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 c 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 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.
- ^ a b "8967 Calandra (4878 T-1)". Minor Planet Center. Retrieved 1 March 2016.
- ^ "Minor Planet Discoverers". Minor Planet Center. 24 April 2016. Retrieved 17 May 2016.
- ^ "European Red List of Birds" (PDF). BirdLife International. 2015. p. 58. Retrieved 1 March 2016.
- ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 17 May 2016.
External links
- 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 (5001)-(10000) – Minor Planet Center
- 8967 Calandra at the JPL Small-Body Database
