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4265 Kani

4265 Kani (prov. designation: 1989 TX) is a dark background asteroid from the inner regions of the asteroid belt. It was discovered by Japanese astronomers Yoshikane Mizuno and Toshimasa Furuta at Kani Observatory (403) on 8 October 1989.[11] The carbonaceous C-type asteroid has a rotation period of 5.7 hours and measures approximately 14 kilometers (9 miles) in diameter. It was named for the Japanese city of Kani.[2]

4265 Kani
Shape model of Salvia from its lightcurve
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)
Aphelion2.9147 AU
Perihelion1.9407 AU
2.4277 AU
Eccentricity0.2006
3.78 yr (1,382 days)
140.60°
0° 15m 38.16s / day
Inclination4.3567°
127.25°
242.75°
Physical characteristics
Mean diameter
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]

Orbit and classification edit

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

Naming edit

This minor planet was named for the Japanese city of Kani, 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 the Kiso riverside, which is referred to as the Japan Rhine because of its similarities to the Rhine in Europe.[2] The official naming citation was published by the Minor Planet Center on 11 March 1990 (M.P.C. 16045).[12]

Physical characteristics edit

In the Bus–Binzel SMASS classification, Kani is characterized as a common, carbonaceous C-type asteroid.[1]

Rotation period edit

In October 2008, two rotational lightcurves of this asteroid were obtained from photometric observations made at the Golden Hill Observatory in Stourton Caundle and the Palmer Divide Observatory in Colorado Springs, Colorado. The lightcurves gave an identical rotation period of 5.7279±0.0001 hours and a brightness variation of 0.75 ± 0.02 in magnitude (U=3/3).[9][a] Observations at the Palomar Transient Factory and revised shape-models have since confirmed the body's rotation period.[7][10]

Diameter and albedo edit

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

Notes edit

  1. ^ a b Pravec (2008): lightcurve plot for (4265) Kani, with a rotation period 5.7279±0.0001 hours with a brightness amplitude of 0.75 mag. Summary figures at Collaborative Asteroid Lightcurve Link (CALL)

References edit

  1. ^ a b c d e f "JPL Small-Body Database Browser: 4265 Kani (1989 TX)" (2017-03-30 last obs.). Jet Propulsion Laboratory. Retrieved 20 June 2017.
  2. ^ a b c Schmadel, 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. ^ a b c d "LCDB Data for (4265) Kani". Asteroid Lightcurve Database (LCDB). Retrieved 7 June 2016.
  4. ^ a b c 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. arXiv:1109.4096. Bibcode:2011ApJ...741...68M. doi:10.1088/0004-637X/741/2/68. Retrieved 5 December 2016.
  5. ^ a b c d 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. arXiv:1109.6407. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. Retrieved 7 June 2016.
  6. ^ a b c d Usui, 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. ^ a b Hanuš, 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. ^ a b Miles, Richard; Warner, Brian D. (April 2009). (PDF). Minor Planet Bulletin. 36 (2): 66–68. Bibcode:2009MPBu...36...66M. ISSN 1052-8091. Archived from the original (PDF) on 6 November 2020. Retrieved 19 March 2020.
  10. ^ a b c 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 7 June 2016.
  11. ^ a b "4265 Kani (1989 TX)". Minor Planet Center. Retrieved 7 June 2016.
  12. ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 7 June 2016.

External links edit

  • Lightcurve plot of 4265 Kani, Palmer Divide Observatory, B. D. Warner (2008)
  • Lightcurve Database Query (LCDB), at www.minorplanet.info
  • Dictionary of Minor Planet Names, Google books
  • Asteroids and comets rotation curves, CdR – Geneva Observatory, Raoul Behrend
  • Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
  • 4265 Kani at AstDyS-2, Asteroids—Dynamic Site
    • Ephemeris · Observation prediction · Orbital info · Proper elements · Observational info
  • 4265 Kani at the JPL Small-Body Database  
    • Close approach · Discovery · Ephemeris · Orbit diagram · Orbital elements · Physical parameters

4265, kani, prov, designation, 1989, dark, background, asteroid, from, inner, regions, asteroid, belt, discovered, japanese, astronomers, yoshikane, mizuno, toshimasa, furuta, kani, observatory, october, 1989, carbonaceous, type, asteroid, rotation, period, ho. 4265 Kani prov designation 1989 TX is a dark background asteroid from the inner regions of the asteroid belt It was discovered by Japanese astronomers Yoshikane Mizuno and Toshimasa Furuta at Kani Observatory 403 on 8 October 1989 11 The carbonaceous C type asteroid has a rotation period of 5 7 hours and measures approximately 14 kilometers 9 miles in diameter It was named for the Japanese city of Kani 2 4265 KaniShape model of Salvia from its lightcurveDiscovery 1 Discovered byY MizunoT FurutaDiscovery siteKani Obs 403 Discovery date8 October 1989DesignationsMPC designation 4265 KaniNamed afterKani Japanese city 2 Alternative designations1989 TX 1940 WM1955 VJ 1974 VH2 1983 AP1 A917 TBMinor planet categorymain belt inner 3 Orbital characteristics 1 Epoch 4 September 2017 JD 2458000 5 Uncertainty parameter 0Observation arc76 33 yr 27 880 days Aphelion2 9147 AUPerihelion1 9407 AUSemi major axis2 4277 AUEccentricity0 2006Orbital period sidereal 3 78 yr 1 382 days Mean anomaly140 60 Mean motion0 15m 38 16s dayInclination4 3567 Longitude of ascending node127 25 Argument of perihelion242 75 Physical characteristicsMean diameter14 244 0 160 km 4 5 15 74 0 76 km 6 Synodic rotation period5 72755 0 00005 h 7 5 727574 0 000001 h 8 5 7279 0 0001 h a 9 5 7285 0 0011 h 10 Geometric albedo0 054 0 006 6 0 056 0 007 4 0 0565 0 0074 5 Spectral typeSMASS C 1 3 Absolute magnitude H 12 8 5 6 12 940 0 006 R 10 13 0 1 3 Contents 1 Orbit and classification 2 Naming 3 Physical characteristics 3 1 Rotation period 3 2 Diameter and albedo 4 Notes 5 References 6 External linksOrbit and classification editKani is a non family asteroid of the main belt s background population when applying the hierarchical clustering method to its proper orbital elements It orbits the Sun in the inner main belt at a distance of 1 9 2 9 AU once every 3 years and 9 months 1 382 days Its orbit has an eccentricity of 0 20 and an inclination of 4 with respect to the ecliptic 1 The body s first observation at Crimea Simeis dates back to 1917 while the first used observation was made at Turku in 1940 extending the asteroid s observation arc by 49 years prior to its discovery 11 Naming editThis minor planet was named for the Japanese city of Kani 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 the Kiso riverside which is referred to as the Japan Rhine because of its similarities to the Rhine in Europe 2 The official naming citation was published by the Minor Planet Center on 11 March 1990 M P C 16045 12 Physical characteristics editIn the Bus Binzel SMASS classification Kani is characterized as a common carbonaceous C type asteroid 1 Rotation period edit In October 2008 two rotational lightcurves of this asteroid were obtained from photometric observations made at the Golden Hill Observatory in Stourton Caundle and the Palmer Divide Observatory in Colorado Springs Colorado The lightcurves gave an identical rotation period of 5 7279 0 0001 hours and a brightness variation of 0 75 0 02 in magnitude U 3 3 9 a Observations at the Palomar Transient Factory and revised shape models have since confirmed the body s rotation period 7 10 Diameter and albedo edit According to the space based surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA s Wide field Infrared Survey Explorer the asteroid measures 15 7 and 14 2 kilometers in diameter respectively 4 5 6 Conversely the Collaborative Asteroid Lightcurve Link calculates a diameter of only 7 5 kilometers due to an assumed albedo of 0 20 which is untypically high for a carbonaceous asteroid 3 Notes edit a b Pravec 2008 lightcurve plot for 4265 Kani with a rotation period 5 7279 0 0001 hours with a brightness amplitude of 0 75 mag Summary figures at Collaborative Asteroid Lightcurve Link CALL References edit a b c d e f JPL Small Body Database Browser 4265 Kani 1989 TX 2017 03 30 last obs Jet Propulsion Laboratory Retrieved 20 June 2017 a b c Schmadel 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 a b c d LCDB Data for 4265 Kani Asteroid Lightcurve Database LCDB Retrieved 7 June 2016 a b c 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 arXiv 1109 4096 Bibcode 2011ApJ 741 68M doi 10 1088 0004 637X 741 2 68 Retrieved 5 December 2016 a b c d 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 arXiv 1109 6407 Bibcode 2011ApJ 741 90M doi 10 1088 0004 637X 741 2 90 Retrieved 7 June 2016 a b c d Usui Fumihiko Kuroda Daisuke Muller 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 a b Hanus J Durech 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 amp A 586A 108H doi 10 1051 0004 6361 201527441 ISSN 0004 6361 Durech J Hanus J Oszkiewicz D Vanco R March 2016 Asteroid models from the Lowell photometric database Astronomy and Astrophysics 587 A48 arXiv 1601 02909 Bibcode 2016A amp A 587A 48D doi 10 1051 0004 6361 201527573 ISSN 0004 6361 a b Miles 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 from the original PDF on 6 November 2020 Retrieved 19 March 2020 a b c 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 7 June 2016 a b 4265 Kani 1989 TX Minor Planet Center Retrieved 7 June 2016 MPC MPO MPS Archive Minor Planet Center Retrieved 7 June 2016 External links editLightcurve plot of 4265 Kani Palmer Divide Observatory B D Warner 2008 Lightcurve Database Query LCDB at www minorplanet info Dictionary of Minor Planet Names Google books Asteroids and comets rotation curves CdR Geneva Observatory Raoul Behrend Discovery Circumstances Numbered Minor Planets 1 5000 Minor Planet Center 4265 Kani at AstDyS 2 Asteroids Dynamic Site Ephemeris Observation prediction Orbital info Proper elements Observational info 4265 Kani at the JPL Small Body Database nbsp Close approach Discovery Ephemeris Orbit diagram Orbital elements Physical parameters Retrieved from https en wikipedia org w index php title 4265 Kani amp oldid 1195678524, wikipedia, wiki, book, books, library,

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