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4265 Kani

From Wikipedia, the free encyclopedia
Main-belt asteroid

4265 Kani
Shape model ofSalvia from itslightcurve
Discovery[1]
Discovered byY. Mizuno
T. Furuta
Discovery siteKani Obs. (403)
Discovery date8 October 1989
Designations
(4265) Kani
Named after
Kani(Japanese city)[2]
1989 TX · 1940 WM
1955 VJ · 1974 VH2
1983 AP1 · A917 TB
main-belt · (inner)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc76.33 yr (27,880 days)
Aphelion2.9147AU
Perihelion1.9407 AU
2.4277 AU
Eccentricity0.2006
3.78yr (1,382 days)
140.60°
0° 15m 38.16s / day
Inclination4.3567°
127.25°
242.75°
Physical characteristics
14.244±0.160 km[4][5]
15.74±0.76 km[6]
5.72755±0.00005 h[7]
5.727574±0.000001 h[8]
5.7279±0.0001 h[a][9]
5.7285±0.0011 h[10]
0.054±0.006[6]
0.056±0.007[4]
0.0565±0.0074[5]
SMASS =C[1][3]
12.8[5][6] · 12.940±0.006(R)[10] · 13.0[1][3]

4265 Kani (prov. designation:1989 TX) is a darkbackground asteroid from the inner regions of theasteroid belt. It was discovered by Japanese astronomersYoshikane Mizuno andToshimasa Furuta at Kani Observatory (403) on 8 October 1989.[11] The carbonaceousC-type asteroid has arotation period of 5.7 hours and measures approximately 14 kilometers (9 miles) in diameter. It was named for the Japanese city ofKani.[2]

Orbit and classification

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Kani is a non-family asteroid of the main belt'sbackground population when applying thehierarchical clustering method to itsproper orbital elements. It orbits the Sun in theinner main-belt at a distance of 1.9–2.9 AU once every 3 years and 9 months (1,382 days). Its orbit has aneccentricity of 0.20 and aninclination of 4° with respect to theecliptic.[1] The body's first observation atCrimea-Simeis dates back to 1917, while the first used observation was made at Turku in 1940, extending the asteroid'sobservation arc by 49 years prior to its discovery.[11]

Naming

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Thisminor planet was named for the Japanese city ofKani, home of the discoverer, located in the countryside of Japan's Gifu Prefecture, approximately 30 kilometers north of Nagoya, the country's third largest city. Kani is situated on theKiso riverside, which is referred to as theJapan Rhine because of its similarities to the Rhine in Europe.[2] The official naming citation was published by theMinor Planet Center on 11 March 1990 (M.P.C. 16045).[12]

Physical characteristics

[edit]

In the Bus–BinzelSMASS classification,Kani is characterized as a common, carbonaceousC-type asteroid.[1]

Rotation period

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In October 2008, two rotationallightcurves of this asteroid were obtained fromphotometric observations made at the Golden Hill Observatory in Stourton Caundle and the Palmer Divide Observatory in Colorado Springs, Colorado. The lightcurves gave an identicalrotation period of5.7279±0.0001 hours and a brightness variation of 0.75 ± 0.02 inmagnitude (U=3/3).[9][a] Observations at thePalomar Transient Factory and revised shape-models have since confirmed the body's rotation period.[7][10]

Diameter and albedo

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According to the space-based surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer, the asteroid measures 15.7 and 14.2 kilometers in diameter, respectively.[4][5][6] Conversely, theCollaborative Asteroid Lightcurve Link calculates a diameter of only 7.5 kilometers, due to an assumed albedo of 0.20, which is untypically high for acarbonaceous asteroid.[3]

Notes

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  1. ^abPravec (2008):lightcurve plot for (4265) Kani, with a rotation period5.7279±0.0001 hours with a brightness amplitude of0.75 mag. Summary figures atCollaborative Asteroid Lightcurve Link (CALL)

References

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  1. ^abcdef"JPL Small-Body Database Browser: 4265 Kani (1989 TX)" (2017-03-30 last obs.).Jet Propulsion Laboratory. Retrieved20 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(4265) Kani".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 365.doi:10.1007/978-3-540-29925-7_4226.ISBN 978-3-540-00238-3.
  3. ^abcd"LCDB Data for (4265) Kani". Asteroid Lightcurve Database (LCDB). Retrieved7 June 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. Retrieved5 December 2016.
  5. ^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. Retrieved7 June 2016.
  6. ^abcdUsui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey".Publications of the Astronomical Society of Japan.63 (5):1117–1138.Bibcode:2011PASJ...63.1117U.doi:10.1093/pasj/63.5.1117. (online,AcuA catalog p. 153)
  7. ^abHanuš, J.; Ďurech, J.; Oszkiewicz, D. A.; Behrend, R.; Carry, B.; Delbo, M.; et al. (February 2016). "New and updated convex shape models of asteroids based on optical data from a large collaboration network".Astronomy and Astrophysics.586: A108.arXiv:1510.07422.Bibcode:2016A&A...586A.108H.doi:10.1051/0004-6361/201527441.ISSN 0004-6361.
  8. ^Ďurech, J.; Hanuš, J.; Oszkiewicz, D.; Vančo, R. (March 2016). "Asteroid models from the Lowell photometric database".Astronomy and Astrophysics.587: A48.arXiv:1601.02909.Bibcode:2016A&A...587A..48D.doi:10.1051/0004-6361/201527573.ISSN 0004-6361.
  9. ^abMiles, Richard; Warner, Brian D. (April 2009)."The Rotation Period of 4265 Kani and an Example of the Meridian Flip Problem"(PDF).Minor Planet Bulletin.36 (2):66–68.Bibcode:2009MPBu...36...66M.ISSN 1052-8091. Archived fromthe original(PDF) on 6 November 2020. Retrieved19 March 2020.
  10. ^abcWaszczak, 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. Retrieved7 June 2016.
  11. ^ab"4265 Kani (1989 TX)".Minor Planet Center. Retrieved7 June 2016.
  12. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved7 June 2016.

External links

[edit]
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