8967 Calandra

8967 CalandraDiscovery [1]

Discovered by| C. J. van Houten
I. van Houten-G.
T. Gehrels
Discovery site| Palomar Obs.
Discovery date| 13 May 1971
Designations

MPC designation

| (8967) Calandra
Pronunciation| /kəˈlændrə/[4]
Named after| Miliaria calandra
(a species of bunting)[2]

Alternative designations

| 4878 T-1 * 1978 RM11
1992 EH15
Minor planet category| main-belt * (outer) [3]
background
Orbital characteristics [1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc| 45.76 yr (16,714 days)
|{{{apsis}}}|helion}}| 3.4081 AU
|{{{apsis}}}|helion}}| 2.7043 AU

Semi-major axis

| 3.0562 AU
Eccentricity| 0.1151
Orbital period| 5.34 yr (1,952 days)
Mean anomaly| 99.067°
Mean motion| 0° 11m 4.2s / day
Inclination| 9.7428°
Longitude of ascending node| 170.63°

|{{{apsis}}}|helion}}

| 171.63°
Physical characteristics
Dimensions| 8.382±0.103 km[5][6]
10.92 km (calculated)[3]
Rotation period| 5.2427±0.0036 h[7]
Geometric albedo| 0.057 (assumed)[3]
0.174±0.030[5][6]

Spectral type

| C [3]
Absolute magnitude (H)| 13.1[1] * 13.54[3] * 12.9[5] * 13.086±0.004[7] * 13.30±0.10[8]

8967 Calandra, provisional designation 4878 T-1, is a carbonaceous background 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 Palomar Observatory in California.[9] It is named after the corn bunting (Emberiza calandra).[2]

## Contents

* 1 Orbit and classification
* 1.1 Survey designation
* 2 Physical characteristics
* 2.1 Rotation period
* 2.2 Diameter and albedo
* 3 Naming
* 4 References
* 5 External links

## Orbit and classification

Calandra is a non-family asteroid from the main belt's background population. It orbits the Sun in the outer main-belt 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.[9]

### Survey designation

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.[10]

## Physical characteristics

### Rotation period

A photometric lightcurve of Calandra obtained at the Palomar Transient Factory in California in 2011, gave a rotation period of 5.2427±0.0036 hours with a brightness variation of 0.58 magnitude ({{{1}}}).[7]

### Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Calandra measures 8.4 kilometers in diameter and its surface has an albedo of 0.17.[5][6] 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 with an absolute magnitude of 13.54.[3]

## Naming

This minor planet is named for the passerine bird, Miliaria calandra or Emberiza calandra, also known as the corn bunting.[2] It is listed as an endangered species on the European Red List of Birds.[11] The approved naming citation was published by the Minor Planet Center on 2 February 1999 (M.P.C. 33794; 34089).[12]

## References

1. ↑ 1.0 1.1 1.2 1.3 "JPL Small-Body Database Browser: 8967 Calandra (4878 T-1)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2008967.
2. ↑ 2.0 2.1 2.2 Schmadel, Lutz D. (2007). "(8967) Calandra". Dictionary of Minor Planet Names – (8967) Calandra. Springer Berlin Heidelberg. p. 672. doi:10.1007/978-3-540-29925-7_7298. ISBN 978-3-540-00238-3.
3. ↑ 3.0 3.1 3.2 3.3 3.4 3.5 "LCDB Data for (8967) Calandra". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=8967|Calandra.
4. ↑ "calandra". calandra. Oxford University Press. http://www.lexico.com/definition/calandra.
5. ↑ 5.0 5.1 5.2 5.3 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. doi:10.1088/0004-637X/741/2/90. Bibcode: 2011ApJ...741...90M. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...90M. Retrieved 17 May 2016.
6. ↑ 6.0 6.1 6.2 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. doi:10.1088/0004-637X/741/2/68. Bibcode: 2011ApJ...741...68M. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...68M. Retrieved 4 December 2016.
7. ↑ 7.0 7.1 7.2 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. doi:10.1088/0004-6256/150/3/75. Bibcode: 2015AJ....150...75W. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015AJ....150...75W. Retrieved 17 May 2016.
8. ↑ 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. doi:10.1016/j.icarus.2015.08.007. Bibcode: 2015Icar..261...34V. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015Icar..261...34V. Retrieved 17 May 2016.
9. ↑ 9.0 9.1 "8967 Calandra (4878 T-1)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=8967.
10. ↑ "Minor Planet Discoverers". Minor Planet Center. 24 April 2016. https://www.minorplanetcenter.net/iau/lists/MPDiscsNum.html.
11. ↑ "European Red List of Birds". BirdLife International. 2015. p. 58. http://www.birdlife.org/sites/default/files/attachments/RedList - BirdLife publication WEB.pdf.
12. ↑ "MPC/MPO/MPS Archive". Minor Planet Center. https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html.

## 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 AstDyS-2, Asteroids—Dynamic Site
* Ephemeris * Observation prediction * Orbital info * Proper elements * Observational info
* 8967 Calandra at the JPL Small-Body Database
* Close approach * Discovery * Ephemeris * Orbit diagram * Orbital elements * Physical parameters

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