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2156 Kate

From Wikipedia, the free encyclopedia
Highly elongated background asteroid

2156 Kate
Shape model ofKate from itslightcurve
Discovery[1]
Discovered byS. Belyavsky
Discovery siteSimeiz Obs.
Discovery date23 September 1917
Designations
(2156) Kate
Named after
Kate Kristensen
(wife of naming astronomer)[2]
A917 SH · 1937 PK
1954 UT2 · 1956 GP
1957 QK · 1969 BE
1970 LK · 1974 RL1
1976 GK1 · 1979 BC
main-belt · (inner)
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc99.61 yr (36,384 days)
Aphelion2.6942AU
Perihelion1.7900 AU
2.2421 AU
Eccentricity0.2016
3.36yr (1,226 days)
264.22°
0° 17m 36.96s / day
Inclination5.3475°
17.175°
4.7281°
Physical characteristics
8.131±0.144 km[3][4]
8.61 km(calculated)[5]
5.62 h[6]
5.62215±0.00005 h[7]
5.6228±0.0003 h[a]
5.623±0.005 h[8]
0.189±0.028[4]
0.20(assumed)[5]
0.2242±0.0353[3]
Tholen =S[1] · A[9]
B–V = 0.916[1]
U–B = 0.525[1]
12.69[1][5][3] · 13.23±1.05[9]

2156 Kate (prov. designation:A917 SH) is a highly elongatedbackground asteroid from the inner regions of theasteroid belt. The asteroid was discovered on 23 September 1917, by Soviet–Russian astronomerSergey Belyavsky at theSimeiz Observatory on the Crimean peninsula.[10] It was named for Kate Kristensen, wife of astronomer L. K. Kristensen.[2] The brightS-type/A-type asteroid has arotation period of 5.6 hours and measures approximately 8 kilometers (5.0 miles) in diameter.

Orbit and classification

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Kate orbits the Sun in theinner main-belt at a distance of 1.8–2.7 AU once every 3 years and 4 months (1,226 days). Its orbit has aneccentricity of 0.20 and aninclination of 5° with respect to theecliptic.[1] As noprecoveries were taken, and no prior identifications were made, the asteroid'sobservation arc begins with its official discovery observation at Simeiz in 1917.[10]

Naming

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Thisminor planet was named after Kate Kristensen, wife of astronomer L. K. Kristensen, who was involved in the body's orbit computation.[2] The official naming citation was published by theMinor Planet Center on 1 April 1980 (M.P.C. 5284).[11]

Physical characteristics

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In theTholen classification,Kate is a commonS-type asteroid.[1] It has also been characterized as a rareA-type asteroid byPan-STARRS' large photometric survey.[9]

Rotation period

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Lightcurve-based 3D-model ofKate

A large number of rotationallightcurves were obtained fromphotometric observations. They gave a well-definedrotation period of 5.620 to 5.623 hours with a brightness variation between 0.5 and 0.9magnitude (U=3/3-).[6][7][8][a]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA's space-basedWide-field Infrared Survey Explorer,Kate measures 8.131 kilometers in diameter and its surface has analbedo of 0.189 and 0.2242, respectively,[3][4] while theCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 8.61 kilometers with anabsolute magnitude of 12.69.[5]

Notes

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  1. ^abDunckel (2011) web: rotation period5.6228±0.0003 hours with a brightness amplitude of0.84 mag. (U=3). Summary figures for (2156) Kate atCollaborative Asteroid Lightcurve Link (CALL)

References

[edit]
  1. ^abcdefgh"JPL Small-Body Database Browser: 2156 Kate (A917 SH)" (2017-05-05 last obs.).Jet Propulsion Laboratory. Retrieved11 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2156) Kate".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 175.doi:10.1007/978-3-540-29925-7_2157.ISBN 978-3-540-00238-3.
  3. ^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. Retrieved1 March 2016.
  4. ^abcMasiero, 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. Retrieved7 December 2016.
  5. ^abcd"LCDB Data for (2156) Kate". Asteroid Lightcurve Database (LCDB). Retrieved1 March 2016.
  6. ^abBinzel, R. P.; Mulholland, J. D. (December 1983)."A photoelectric lightcurve survey of small main belt asteroids".Icarus.56 (3):519–533.Bibcode:1983Icar...56..519B.doi:10.1016/0019-1035(83)90170-7.ISSN 0019-1035. Retrieved1 March 2016.
  7. ^abHanus, J.; Durech, J.; Broz, M.; Warner, B. D.; Pilcher, F.; Stephens, R.; et al. (June 2011)."A study of asteroid pole-latitude distribution based on an extended set of shape models derived by the lightcurve inversion method".Astronomy and Astrophysics.530: 16.arXiv:1104.4114.Bibcode:2011A&A...530A.134H.doi:10.1051/0004-6361/201116738. Retrieved1 March 2016.
  8. ^abKryszczynska, A.; Colas, F.; Polinska, M.; Hirsch, R.; Ivanova, V.; Apostolovska, G.; et al. (October 2012)."Do Slivan states exist in the Flora family?. I. Photometric survey of the Flora region".Astronomy and Astrophysics.546: 51.Bibcode:2012A&A...546A..72K.doi:10.1051/0004-6361/201219199. Retrieved1 March 2016.
  9. ^abcVeres, 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. Retrieved1 March 2016.
  10. ^ab"2156 Kate (A917 SH)".Minor Planet Center. Retrieved1 March 2016.
  11. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved20 May 2016.

External links

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Minor planets
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Distant minor planet
Comets
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Authority control databasesEdit this at Wikidata
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