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6546 Kaye

From Wikipedia, the free encyclopedia
Main-belt asteroid

6546 Kaye
Shape model ofKaye from itslightcurve
Discovery[1]
Discovered byA. Mrkos
Discovery siteKleť Obs.
Discovery date24 February 1987
Designations
(6546) Kaye
Named after
Danny Kaye
(American actor and singer)[2]
1987 DY4 · 1978 RF2
1991 XM1
Orbital characteristics[3]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc37.86 yr (13,828 days)
Aphelion3.5611AU
Perihelion2.8844 AU
3.2228 AU
Eccentricity0.1050
5.79yr (2,113 days)
80.178°
0° 10m 13.44s / day
Inclination14.414°
274.80°
272.41°
Physical characteristics
21.624±0.174 km[8]
23.21 km(calculated)[4]
23.757±0.186 km[9]
0.057(assumed)[4]
0.0656±0.0078[9]
0.085±0.015[8]
C(assumed)[4]
11.7[9] · 11.9[1][4] · 11.986±0.003(R)[10] · 12.392±0.003(S)[10]

6546 Kaye (prov. designation:1987 DY4) is a dark and elongatedbackground asteroid from the outer region of theasteroid belt. It was discovered on 24 February 1987, by Czech astronomerAntonín Mrkos at the South BohemianKleť Observatory in the Czech Republic.[3] The presumedC-type asteroid has arotation period of 10.0 hours and measures approximately 22 kilometers (14 miles) in diameter. It was named for American actorDanny Kaye.[2]

Orbit and classification

[edit]

When applying the synthetichierarchical clustering method (HCM) byNesvorný, or the 1995 HCM-analysis byZappalà,[6]Kaye is a non-family asteroid of the main belt'sbackground population,[5][6] while according to another HCM-analysis byMilani andKnežević (AstDyS),[7] it is a core member of theUrsula family (631), a family of 1,500 asteroids with aC- andX-type.[11]: 23 

It orbits the Sun in theouter main-belt at a distance of 2.9–3.6 AU once every 5 years and 9 months (2,113 days). Its orbit has aneccentricity of 0.11 and aninclination of 14° with respect to theecliptic.[1] It was first observed as1978 RF2 atCrimea–Nauchnij in 1978, extending the body'sobservation arc by 9 years prior to its official discovery observation atKleť Observatory.[3]

Naming

[edit]

Thisminor planet was named in memory of American actor and singerDavid Daniel Kaminsky (1911–1987), known by his screen name as "Danny Kaye".[2] Kaye starred in popular feature films such asThe 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] Theapproved naming citation was published by theMinor Planet Center on 20 June 1997 (M.P.C. 30099).[12]

Physical characteristics

[edit]

Rotation period

[edit]

In August 2012, two rotationallightcurves ofKaye were obtained fromphotometric observations at thePalomar Transient Factory in California. Lightcurve analysis gave arotation period of10.0059±0.0569 and10.0186±0.0569 hours with a brightness variation of 0.32 and 0.34magnitude in the R and S-band, respectively (U=2/2).[4][10]

Diameter and albedo

[edit]

According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Kaye measures between 21.6 and 23.8 kilometers in diameter and its surface has analbedo between 0.065 and 0.085.[8][9] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo forcarbonaceous asteroids of 0.057 and calculates a diameter of 23.2 kilometers with anabsolute magnitude of 11.9.[4]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 6546 Kaye (1987 DY4)" (2016-07-18 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 18 September 2020. Retrieved21 June 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(6546) Kaye".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 540.doi:10.1007/978-3-540-29925-7_5941.ISBN 978-3-540-00238-3.
  3. ^abcd"6546 Kaye (1987 DY4)".Minor Planet Center. Retrieved4 November 2016.
  4. ^abcdefgh"LCDB Data for (6546) Kaye". Asteroid Lightcurve Database (LCDB). Retrieved4 November 2016.
  5. ^ab"Asteroid 6546 Kaye".Small Bodies Data Ferret. Retrieved23 March 2020.
  6. ^abcZappalà, V.; Bendjoya, Ph.; Cellino, A.; Farinella, P.; Froeschle, C. (1997)."Asteroid Dynamical Families".NASA Planetary Data System: EAR-A-5-DDR-FAMILY-V4.1. Retrieved15 March 2020. (PDS main page)
  7. ^ab"Asteroid 6546 Kaye – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved23 March 2020.
  8. ^abcMasiero, 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.S2CID 119293330. Retrieved4 November 2016.
  9. ^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.S2CID 118700974.
  10. ^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.S2CID 8342929. Retrieved4 November 2016.
  11. ^Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV. pp. 297–321.arXiv:1502.01628.Bibcode:2015aste.book..297N.doi:10.2458/azu_uapress_9780816532131-ch016.ISBN 9780816532131.S2CID 119280014.
  12. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved4 November 2016.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
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Authority control databasesEdit this at Wikidata
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