6546 Kaye
Discovery [1] | |
---|---|
Discovered by | A. Mrkos |
Discovery site | Kleť Obs. |
Discovery date | 24 February 1987 |
Designations | |
MPC designation | 6546 Kaye |
Named after | Danny Kaye (actor)[2] |
1987 DY4 · 1978 RF2 1991 XM1 | |
main-belt (outer)[1][3] | |
Orbital characteristics [1] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 37.75 yr (13,789 days) |
Aphelion | 3.5656 AU |
Perihelion | 2.8847 AU |
3.2251 AU | |
Eccentricity | 0.1056 |
5.79 yr (2,116 days) | |
11.833° | |
0° 10m 12.72s / day | |
Inclination | 14.408° |
274.83° | |
272.61° | |
Physical characteristics | |
Dimensions |
±0.174 km 21.624[4] 23.21 km (calculated)[3] ±0.186 km 23.757[5] |
±0.0569 10.0059h (S)[3][6] ±0.0569 h (R) 10.0186[6] | |
0.057 (assumed)[3] ±0.0078 0.0656[5] ±0.015 0.085[4] | |
C [3] | |
11.7[5] 11.9[1][3] ±0.64 11.93[7] ±0.003 (R) 11.986[6] ±0.003 (S) 12.392[6] | |
|
6546 Kaye, provisional designation 1987 DY4, is a carbonaceous asteroid from the outer region of the asteroid belt, approximately 22 kilometers in diameter. It was discovered on 24 February 1987, by Czech astronomer Antonín Mrkos at the South Bohemian Kleť Observatory in the Czech Republic.[8]
The C-type asteroid orbits the Sun at a distance of 2.9–3.6 AU once every 5 years and 9 months (2,116 days). Its orbit has an eccentricity of 0.11 and an inclination of 14° with respect to the ecliptic.[1] It was first identified as "1978 RF2" at Crimea-Nauchnij in 1978, extending the asteroid's observation arc by 9 years prior to its discovery.[8]
In August 2012, two rotational light-curves were obtained for this asteroid from photometric observations at the U.S. Palomar Transient Factory in California. The light-curves gave a rotation period of 10.0059 and 10.0186 hours with a brightness variation of 0.32 and 0.34 magnitude in the R and S-band, respectively (U=2/2).[3][6]
According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, the asteroid measures between 21.6 and 23.8 kilometers in diameter and its surface has an albedo between 0.065 and 0.085.[4][5] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 23.2 kilometers, based on an absolute magnitude of 11.9.[3]
The minor planet was named in memory of American actor and singer David Daniel Kaminsky (1913–1987), known by his screen name as "Danny Kaye". He starred in popular feature films such as The Court Jester (1956), typically playing the role of a gentle bumbler who triumphs eventually. The minor planet's name was suggested by G. V. Williams, who made the identifications for this body.[2] Naming citation was published on 20 June 1997 (M.P.C. 30099).[9]
References
- 1 2 3 4 5 "JPL Small-Body Database Browser: 6546 Kaye (1987 DY4)" (2016-06-09 last obs.). Jet Propulsion Laboratory. Retrieved 4 November 2016.
- 1 2 Schmadel, Lutz D. (2007). Dictionary of Minor Planet Names – (6546) Kaye. Springer Berlin Heidelberg. p. 540. ISBN 978-3-540-00238-3. Retrieved 4 November 2016.
- 1 2 3 4 5 6 7 8 "LCDB Data for (6546) Kaye". Asteroid Lightcurve Database (LCDB). Retrieved 4 November 2016.
- 1 2 3 Masiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos". The Astrophysical Journal. 791 (2): 11. arXiv:1406.6645. Bibcode:2014ApJ...791..121M. doi:10.1088/0004-637X/791/2/121. Retrieved 4 November 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" (PDF). The Astrophysical Journal. 741 (2): 25. arXiv:1109.6407. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. Retrieved 4 November 2016.
- 1 2 3 4 5 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 4 November 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 4 November 2016.
- 1 2 "6546 Kaye (1987 DY4)". Minor Planet Center. Retrieved 4 November 2016.
- ↑ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 4 November 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
- 6546 Kaye at the JPL Small-Body Database