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| name = 4265 Kani
| name = 4265 Kani
| background = #FFFFC0
| background = #FFFFC0
| image =
| caption =
| discovery_ref = &thinsp;<ref name="jpldata" />
| discovery_ref = &thinsp;<ref name="jpldata" />
| discovered = 8 October 1989
| discovered = 8 October 1989
| discoverer = [[Yoshikane Mizuno|Y- Mizuno]]<br />[[Toshimasa Furuta|T. Furuta]]
| discoverer = [[Yoshikane Mizuno|Y. Mizuno]], [[Toshimasa Furuta|T. Furuta]]
| discovery_site = [[Kani Observatory]] ([[List of observatory codes|403]])
| discovery_site = [[Kani Observatory]] ({{small|[[IAU code#400–499|403]]}})
| mp_name = 4265 Kani
| mp_name = 4265 Kani
| alt_names = 1989 TX; 1940 WM<br />1955 VJ; {{mp|1974 VH|2}}<br />{{mp|1983 AP|1}}; A917 TB
| alt_names = 1989 TX{{·}}1940 WM<br />1955 VJ{{·}}{{mp|1974 VH|2}}<br />{{mp|1983 AP|1}}{{·}}A917 TB
| named_after = [[Kani, Gifu]]
| named_after = [[Kani, Gifu|Kani]] {{small|(Japanese city)}}<ref name="springer" />
| mp_category = [[main-belt]]
| mp_category = [[main-belt]]{{·}}{{small|(inner)}}&thinsp;<ref name="lcdb" />
| orbit_ref = &thinsp;<ref name="jpldata" />
| orbit_ref = &thinsp;<ref name="jpldata" />
| epoch = 27 June 2015 ([[Julian day|JD]] 2457200.5)
| epoch = 13 January 2016 ([[Julian day|JD]] 2457400.5)
| uncertainty = 0
| uncertainty = 0
| observation_arc = {{nowrap|74.62 yr (27,254 days)}}
| observation_arc = {{nowrap|74.90 yr (27,358 days)&nbsp;&nbsp;&nbsp;&nbsp;}}
| aphelion = 2.9156 [[Astronomical unit|AU]]
| aphelion = 2.9156 [[Astronomical unit|AU]]
| perihelion = 1.9399 AU
| perihelion = 1.9401 AU
| semimajor = 2.4278 AU
| semimajor = 2.4278 AU
| eccentricity = 0.2009
| eccentricity = 0.2009
| period = 3.78 [[Julian year (astronomy)|yr]] (1381.7 days)
| period = 3.78 [[Julian year (astronomy)|yr]] (1,382 days)
| mean_anomaly = 292.09[[degree (angle)|°]]
| mean_anomaly = 344.21[[degree (angle)|°]]
| inclination = 4.3570°
| inclination = 4.3569°
| asc_node = 127.25°
| asc_node = 127.25°
| arg_peri = 242.79°
| arg_peri = 242.77°
| dimensions = {{val|15.74|0.76}} km<ref name="AKARI" /><br />{{val|14.244|0.160}} km<ref name="WISE" /><br />7.46 km {{small|(calculated)}}<ref name="lcdb" />
| moid = 0.9440 AU
| rotation = {{val|5.7279|0.0001}} [[hour|h]]{{efn|name=lcdb-Pravec}}<ref name="Miles-2009" /><br />{{val|5.7285|0.0011}} h<ref name="Waszczak-2015" /><br />{{val|5.72755|0.00005}} h<ref name="Hanus-2015b" />
| dimensions =
| albedo = {{val|0.054|0.006}}<ref name="AKARI" /><br />{{val|0.0565|0.0074}}<ref name="WISE" /><br />0.20 {{small|(assumed)}}<ref name="lcdb" />
| rotation = 5.7279 [[hour|h]]
| spectral_type = [[SMASS classification|SMASS]] = [[C-type asteroid|C]]
| albedo =
| spectral_type = [[C-type asteroid|C]] {{small|([[SMASS]]II)}}
[[C-type asteroid|C]]&thinsp;<ref name="lcdb" />
| abs_magnitude = 13.0<ref name="jpldata" /><ref name="lcdb" /><br />12.8<ref name="AKARI" /><ref name="WISE" /><br />12.94<ref name="Waszczak-2015" />
| abs_magnitude = 13.0 mag
}}
}}


'''4265 Kani''' (1989 TX) is a [[Asteroid belt|main-belt]] [[asteroid]] discovered on October 8, 1989 by [[Yoshikane Mizuno]] and [[Toshimasa Furuta]] at Kani Observatory ([[List of observatory codes|403]]).<ref name="jpldata" />
'''4265 Kani''', provisional designation 1989 TX, is a carbonaceous [[asteroid]] from the inner regions of the [[asteroid belt]], about 14 kilometers in diameter. It was discovered by Japanese astronomers [[Yoshikane Mizuno]] and [[Toshimasa Furuta]] at Kani Observatory ({{small|[[IAU code#400–499|403]]}}) on 8 October 1989.<ref name="MPC-Kani" /> The [[C-type asteroid|C-type]] asteroid orbits the Sun at a distance of 1.9–2.9&nbsp;[[Astronomical unit|AU]] once every 3 years and 9 months (1,382 days). Its orbit shows an [[orbital eccentricity|eccentricity]] of 0.20 and an [[orbital inclination|inclination]] of 4 degrees from the plane of the [[ecliptic]].<ref name="jpldata" />


[[Photometry (astronomy)|Photometric]] observations of this asteroid carried out from Golden Hill Observatory in [[Stourton Caundle]] and Palmer Divide Observatory in [[Colorado Springs, Colorado]] produced a [[light curve]] with a period of 5.7279 ± 0.0002 hours and a brightness variation of 0.75 ± 0.02 in [[Magnitude (astronomy)|magnitude]].<ref name="MilesWarner2009" />
[[Photometry (astronomy)|Photometric]] observations of this asteroid carried out from Golden Hill Observatory in [[Stourton Caundle]] and Palmer Divide Observatory in [[Colorado Springs, Colorado]] produced a [[light-curve]] with a [[rotation period]] for the asteroid of {{val|5.7279|0.0001}} hours and a brightness variation of 0.75 ± 0.02 in [[Magnitude (astronomy)|magnitude]] ({{small|1=[[LCDB quality code|U]]=3-}}).<ref name="Miles-2009" />{{efn|name=lcdb-Pravec}} Observations at the [[Palomar Transient Factory]] and revised shape-models have since confirmed the body's rotation period.<ref name="Waszczak-2015" /><ref name="Hanus-2015b" />

According to the surveys carried out by the Japanese [[Akari (satellite)|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.<ref name="AKARI" /><ref name="WISE" /> 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 [[C-type asteroid|carbonaceous]] asteroids.<ref name="lcdb" />

The minor planet was named for the Japanese city of [[Kani, Gifu|Kani]], a quiet, rural city and home of the discoverer. It is situated about 30 kilometers north of Nagoya, the third largest city in Japan. Kani is located on the banks of the beautiful river Kiso, which is said to resemble the Rhine in Germany.<ref name="springer" />


== References ==
== References ==
{{notelist
|refs=

{{efn|name=lcdb-Pravec|1=Pravec (2008) web: rotation period {{val|5.7279|0.0001}} hours with a brightness amplitude of {{val|0.75}} mag. Summary figures at {{URL|1=http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=4265%7CKani |2=Collaborative Asteroid Lightcurve Link (CALL) for (4265) Kani}}}}

}} <!-- end of notelist -->
{{reflist
{{reflist
|refs=
|refs=


<ref name="jpldata">{{cite web
<ref name="jpldata">{{cite web
|type=2015-07-13 last obs.
|type = 2015-10-25 last obs.
|title=JPL Small-Body Database Browser: 4265 Kani (1989 TX)
|title = JPL Small-Body Database Browser: 4265 Kani (1989 TX)
|url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2004265
|url = http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2004265
|publisher=Jet Propulsion Laboratory
|publisher = Jet Propulsion Laboratory
|accessdate=October 2015}}</ref>
|accessdate = February 2016}}</ref>

<ref name="springer">{{cite book
|title = Dictionary of Minor Planet Names – (4265) Kani
|last = Schmadel | first = Lutz D.
|publisher = Springer Berlin Heidelberg
|page = 365
|date = 2007
|url = http://link.springer.com/referenceworkentry/10.1007/978-3-540-29925-7_4226
|isbn = 978-3-540-00238-3
|accessdate = February 2016}}</ref>

<ref name="MPC-Kani">{{cite web
|title = 4265 Kani (1989 TX)
|work = Minor Planet Center
|url = http://www.minorplanetcenter.net/db_search/show_object?object_id=4265
|accessdate = February 2016}}</ref>

<ref name="lcdb">{{cite web
|title = LCDB Data for (4265) Kani
|publisher = Asteroid Lightcurve Database (LCDB)
|url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=4265%7CKani
|accessdate = February 2016}}</ref>

<ref name="AKARI">{{cite journal
|display-authors = 6
|first1 = Fumihiko |last1 = Usui
|first2 = Daisuke |last2 = Kuroda
|first3 = Thomas G. |last3 = Müller
|first4 = Sunao |last4 = Hasegawa
|first5 = Masateru |last5 = Ishiguro
|first6 = Takafumi |last6 = Ootsubo
|first7 = Daisuke |last7 = Ishihara
|first8 = Hirokazu |last8 = Kataza
|first9 = Satoshi |last9 = Takita
|first10 = Shinki |last10 = Oyabu
|first11 = Munetaka |last11 = Ueno
|first12 = Hideo |last12 = Matsuhara
|first13 = Takashi |last13 = Onaka
|date = October 2011
|title = Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey
|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011PASJ...63.1117U
|journal = Publications of the Astronomical Society of Japan
|volume = 63
|issue = 5
|pages = 1117–1138
|bibcode = 2011PASJ...63.1117U
|doi = 10.1093/pasj/63.5.1117
|access-date= February 2016}}</ref>

<ref name="WISE">{{cite journal
|display-authors = 6
|first1 = A. |last1 = Mainzer
|first2 = T. |last2 = Grav
|first3 = J. |last3 = Masiero
|first4 = E. |last4 = Hand
|first5 = J. |last5 = Bauer
|first6 = D. |last6 = Tholen
|first7 = R. S. |last7 = McMillan
|first8 = T. |last8 = Spahr
|first9 = R. M. |last9 = Cutri
|first10 = E. |last10 = Wright
|first11 = J. |last11 = Watkins
|first12 = W. |last12 = Mo
|first13 = C. |last13 = Maleszewski
|date = November 2011
|title = NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results
|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...90M
|journal = The Astrophysical Journal
|volume = 741
|issue = 2
|page = 25
|bibcode = 2011ApJ...741...90M
|doi = 10.1088/0004-637X/741/2/90
|access-date= February 2016}}</ref>

<ref name="Miles-2009">{{cite journal
|first1 = Richard |last1 = Miles
|first2 = Brian D. |last2 = Warner
|date = April 2009
|title = The Rotation Period of 4265 Kani and an Example of the Meridian Flip Problem
|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2009MPBu...36...66M
|journal = Bulletin of the Minor Planets
|publisher = Section of the Association of Lunar and Planetary Observers
|volume = 36
|issue = 2
|pages = 66–68
|issn = 1052-8091
|bibcode = 2009MPBu...36...66M
|access-date= February 2016}}</ref>

<ref name="Waszczak-2015">{{cite journal
|display-authors = 6
|first1 = Adam |last1 = Waszczak
|first2 = Chan-Kao |last2 = Chang
|first3 = Eran O. |last3 = Ofek
|first4 = Russ |last4 = Laher
|first5 = Frank |last5 = Masci
|first6 = David |last6 = Levitan
|first7 = Jason |last7 = Surace
|first8 = Yu-Chi |last8 = Cheng
|first9 = Wing-Huen |last9 = Ip
|first10 = Daisuke |last10 = Kinoshita
|first11 = George |last11 = Helou
|first12 = Thomas A. |last12 = Prince
|first13 = Shrinivas |last13 = Kulkarni
|date = September 2015
|title = Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry
|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015AJ....150...75W
|journal = The Astronomical Journal
|volume = 150
|issue = 3
|page = 35
|bibcode = 2015AJ....150...75W
|doi = 10.1088/0004-6256/150/3/75
|access-date= February 2016}}</ref>


<ref name="MilesWarner2009">{{citation
<ref name="Hanus-2015b">{{cite journal
|display-authors = 6
| last1 = Miles
| first1 = Richard
|first1 = J. |last1 = Hanus
| last2 = Warner
|first2 = J. |last2 = Durech
|first3 = D. A. |last3 = Oszkiewicz
| first2 = Brian D.
|first4 = R. |last4 = Behrend
| title = The Rotation Period of 4265 Kani and an Example of the Meridian Flip Problem
|first5 = B. |last5 = Carry
| work = Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers
|first6 = M. |last6 = Delbo'
| volume = 36
| issue = 2
|first7 = O. |last7 = Adam
| pages = 66–68
|first8 = V. |last8 = Afonina
|first9 = R. |last9 = Anquetin
|date=April 2009
|first10 = P. |last10 = Antonini
| bibcode = 2009MPBu...36...66M
|first11 = L. |last11 = Arnold
| postscript= .
|first12 = M. |last12 = Audejean
}}</ref>
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|first18 = P. |last18 = Baudouin
|first19 = L. |last19 = Berard
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|first75 = J-P. |last75 = Godard
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|first77 = H. |last77 = Hamanowa
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|first81 = S. |last81 = Heterier
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|first83 = R. |last83 = Hirsch
|first84 = G. |last84 = Hodosan
|first85 = M. |last85 = Hren
|first86 = A. |last86 = Hygate
|first87 = N. |last87 = Innocent
|first88 = H. |last88 = Jacquinot
|first89 = S. |last89 = Jawahar
|first90 = E. |last90 = Jehin
|first91 = L. |last91 = Jerosimic
|first92 = A. |last92 = Klotz
|first93 = W. |last93 = Koff
|first94 = P. |last94 = Korlevic
|first95 = E. |last95 = Kosturkiewicz
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|first99 = O. |last99 = Labrevoir
|first100 = J. |last100 = Lecacheux
|first101 = M. |last101 = Lehký
|first102 = A. |last102 = Leroy
|first103 = B. |last103 = Lesquerbault
|first104 = M. J. |last104 = Lopez-Gonzales
|first105 = M. |last105 = Lutz
|first106 = B. |last106 = Mallecot
|first107 = J. |last107 = Manfroid
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|first110 = A. |last110 = Martin
|first111 = B. |last111 = Modave
|first112 = R. |last112 = Montaigut
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|first114 = E. |last114 = Morelle
|first115 = B. |last115 = Morton
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|first117 = R. |last117 = Naves
|first118 = J. |last118 = Nomen
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|first120 = W. |last120 = Ogloza
|first121 = M. |last121 = Paiella
|first122 = H. |last122 = Pallares
|first123 = A. |last123 = Peyrot
|first124 = F. |last124 = Pilcher
|first125 = J-F. |last125 = Pirenne
|first126 = P. |last126 = Piron
|first127 = M. |last127 = Polinska
|first128 = M. |last128 = Polotto
|first129 = R. |last129 = Poncy
|first130 = J. P. |last130 = Previt
|first131 = F. |last131 = Reignier
|first132 = D. |last132 = Renauld
|first133 = D. |last133 = Ricci
|first134 = F. |last134 = Richard
|first135 = C. |last135 = Rinner
|first136 = V. |last136 = Risoldi
|first137 = D. |last137 = Robilliard
|first138 = D. |last138 = Romeuf
|first139 = G. |last139 = Rousseau
|first140 = R. |last140 = Roy
|first141 = J. |last141 = Ruthroff
|first142 = P. A. |last142 = Salom
|first143 = L. |last143 = Salvador
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|first145 = T. |last145 = Santana-Ros
|first146 = A. |last146 = Scholz
|first147 = G. |last147 = Séné
|first148 = B. |last148 = Skiff
|first149 = K. |last149 = Sobkowiak
|first150 = P. |last150 = Sogorb
|first151 = F. |last151 = Soldán
|first152 = A. |last152 = Spiridakis
|first153 = E. |last153 = Splanska
|first154 = S. |last154 = Sposetti
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|first157 = A. |last157 = Stiepen
|first158 = R. |last158 = Stoss
|first159 = J. |last159 = Strajnic
|first160 = J-P. |last160 = Teng
|first161 = G. |last161 = Tumolo
|first162 = A. |last162 = Vagnozzi
|first163 = B. |last163 = Vanoutryve
|first164 = J. M. |last164 = Vugnon
|first165 = B. D. |last165 = Warner
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|access-date= February 2016}}</ref>


}} <!-- end of reflist -->
}} <!-- end of reflist -->
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[[Category:Numbered asteroids]]
[[Category:Numbered asteroids]]
[[Category:Discoveries by Yoshikane Mizuno|Kani]]
[[Category:Discoveries by Yoshikane Mizuno|Kani]]
[[Category:Discoveries by Toshimasa Furuta|Kani]]
[[Category:Asteroids named for places|Kani]]
[[Category:Asteroids named for places|Kani]]
[[Category:Astronomical objects discovered in 1989|19891008]]
[[Category:Astronomical objects discovered in 1989|19891008]]

Revision as of 08:19, 7 February 2016

4265 Kani
Discovery [1]
Discovered byY. Mizuno, T. Furuta
Discovery siteKani Observatory (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 13 January 2016 (JD 2457400.5)
Uncertainty parameter 0
Observation arc74.90 yr (27,358 days)    
Aphelion2.9156 AU
Perihelion1.9401 AU
2.4278 AU
Eccentricity0.2009
3.78 yr (1,382 days)
344.21°
Inclination4.3569°
127.25°
242.77°
Physical characteristics
Dimensions15.74±0.76 km[4]
14.244±0.160 km[5]
7.46 km (calculated)[3]
5.7279±0.0001 h[a][6]
5.7285±0.0011 h[7]
5.72755±0.00005 h[8]
0.054±0.006[4]
0.0565±0.0074[5]
0.20 (assumed)[3]
SMASS = C C [3]
13.0[1][3]
12.8[4][5]
12.94[7]

4265 Kani, provisional designation 1989 TX, is a carbonaceous asteroid from the inner regions of the asteroid belt, about 14 kilometers in diameter. It was discovered by Japanese astronomers Yoshikane Mizuno and Toshimasa Furuta at Kani Observatory (403) on 8 October 1989.[9] The C-type asteroid orbits the Sun at a distance of 1.9–2.9 AU once every 3 years and 9 months (1,382 days). Its orbit shows an eccentricity of 0.20 and an inclination of 4 degrees from the plane of the ecliptic.[1]

Photometric observations of this asteroid carried out from Golden Hill Observatory in Stourton Caundle and Palmer Divide Observatory in Colorado Springs, Colorado produced a light-curve with a rotation period for the asteroid of 5.7279±0.0001 hours and a brightness variation of 0.75 ± 0.02 in magnitude (U=3-).[6][a] Observations at the Palomar Transient Factory and revised shape-models have since confirmed the body's rotation period.[7][8]

According to the 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] 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 carbonaceous asteroids.[3]

The minor planet was named for the Japanese city of Kani, a quiet, rural city and home of the discoverer. It is situated about 30 kilometers north of Nagoya, the third largest city in Japan. Kani is located on the banks of the beautiful river Kiso, which is said to resemble the Rhine in Germany.[2]

References

  1. ^ a b Pravec (2008) web: rotation period 5.7279±0.0001 hours with a brightness amplitude of 0.75 mag. Summary figures at Collaborative Asteroid Lightcurve Link (CALL) for (4265) Kani
  1. ^ a b c d "JPL Small-Body Database Browser: 4265 Kani (1989 TX)" (2015-10-25 last obs.). Jet Propulsion Laboratory. Retrieved February 2016. {{cite web}}: Check date values in: |accessdate= (help)
  2. ^ a b Schmadel, Lutz D. (2007). Dictionary of Minor Planet Names – (4265) Kani. Springer Berlin Heidelberg. p. 365. ISBN 978-3-540-00238-3. Retrieved February 2016. {{cite book}}: Check date values in: |accessdate= (help)
  3. ^ a b c d e f "LCDB Data for (4265) Kani". Asteroid Lightcurve Database (LCDB). Retrieved February 2016. {{cite web}}: Check date values in: |accessdate= (help)
  4. ^ 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. Retrieved February 2016. {{cite journal}}: Check date values in: |access-date= (help)
  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. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. Retrieved February 2016. {{cite journal}}: Check date values in: |access-date= (help)
  6. ^ a b Miles, Richard; Warner, Brian D. (April 2009). "The Rotation Period of 4265 Kani and an Example of the Meridian Flip Problem". Bulletin of the Minor Planets. 36 (2). Section of the Association of Lunar and Planetary Observers: 66–68. Bibcode:2009MPBu...36...66M. ISSN 1052-8091. Retrieved February 2016. {{cite journal}}: Check date values in: |access-date= (help)
  7. ^ 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. Bibcode:2015AJ....150...75W. doi:10.1088/0004-6256/150/3/75. Retrieved February 2016. {{cite journal}}: Check date values in: |access-date= (help)
  8. ^ a b Hanus, J.; Durech, J.; Oszkiewicz, D. A.; Behrend, R.; Carry, B.; Delbo', M.; et al. (October 2015). "New and updated convex shape models of asteroids based on optical data from a large collaboration network". eprint arXiv:1510.07422. Bibcode:2015arXiv151007422H. Retrieved February 2016. {{cite journal}}: Check date values in: |access-date= (help)
  9. ^ "4265 Kani (1989 TX)". Minor Planet Center. Retrieved February 2016. {{cite web}}: Check date values in: |accessdate= (help)

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