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1185 Nikko

From Wikipedia, the free encyclopedia
Main-belt asteroid

1185 Nikko
Discovery[1]
Discovered byO. Oikawa
Discovery siteTokyo Astronomical Obs. (389)
Discovery date17 November 1927
Designations
(1185) Nikko
Named after
Nikkō(Japanese city)[2]
1927 WC · 1930 SE1
1930 SG1 · 1930 SH1
main-belt · (inner)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc86.78 yr (31,697 days)
Aphelion2.4744AU
Perihelion2.0006 AU
2.2375 AU
Eccentricity0.1059
3.35yr (1,222 days)
280.93°
0° 17m 40.2s / day
Inclination5.7013°
71.904°
1.9614°
Physical characteristics
Dimensions8.347±0.297 km[4]
11.35 km(calculated)[3]
12.56±0.83 km[5]
3.781±0.0326[6]
3.78615±0.00005 h[7]
3.788±0.0326 h[6]
3.7889±0.0004 h[8]
3.79±0.01 h[9]
3.792±0.002h[8]
0.164±0.023[5]
0.20(assumed)[3]
0.370±0.041[4]
S(Tholen)[1] · S(SMASS)[1]
S[3]
B–V = 0.923[1]
U–B = 0.514[1]
11.674±0.002(R)[6] · 11.99±0.33[10] · 12.09[1][3][4][5]

1185 Nikko, provisional designation1927 WC, is a stonyasteroid from the inner regions of theasteroid belt, approximately 10 kilometers in diameter. It was discovered on 17 November 1927 byOkuro Oikawa at the Tokyo Astronomical Observatory, Japan.[11] The asteroid was named after the Japanese city ofNikkō.[2]

Orbit and classification

[edit]

Nikko orbits the Sun in theinner main-belt at a distance of 2.0–2.5 AU once every 3 years and 4 months (1,222 days). Its orbit has aneccentricity of 0.11 and aninclination of 6° with respect to theecliptic.[1]Nikko'sobservation arc begins with its first used observation taken atJohannesburg Observatory in 1930, or 3 years after its official discovery observation at Tokyo.[11]

Physical characteristics

[edit]

In both theTholen andSMASS taxonomy,Nikko is a common stonyS-type asteroid.[1]

Rotation period

[edit]

Between 2004 and 2011, several rotationallightcurves ofNikko were obtained from photometric observations taken by astronomersLaurent Bernasconi,[8] Hiromi and Hiroko Hamanowa,[8] John Menke,[12]Robert Stephens,[9] as well as at thePalomar Transient Factory in California.[6] Lightcurve analysis gave arotation period between 3.781 and 3.792 hours with a brightness variation between 0.26 and 0.50magnitude (U=3/3/3/3-/2/2).[3]

Diameter and albedo

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According to the survey carried out by the JapaneseAkari satellite and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Nikko measures 8.347 and 12.56 kilometers in diameter, and its surface has analbedo of 0.370 and 0.164, respectively.[4][5] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 11.35 kilometers with anabsolute magnitude of 12.09.[3]

Naming

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Thisminor planet was named for the Japanese city ofNikkō, located in the Tochigi Prefecture of central Japan. The tourist resort is known for its Shinto shrine and a UNESCO World Heritage SiteNikkō Tōshō-gū. The official naming citation was published byPaul Herget inThe Names of the Minor Planets in 1955 (H 110).[2][13]

References

[edit]
  1. ^abcdefghi"JPL Small-Body Database Browser: 1185 Nikko (1927 WC)" (2017-07-01 last obs.).Jet Propulsion Laboratory. Retrieved26 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1185) Nikko".Dictionary of Minor Planet Names – (1185) Nikko.Springer Berlin Heidelberg. p. 99.doi:10.1007/978-3-540-29925-7_1186.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (1185) Nikko". Asteroid Lightcurve Database (LCDB). Retrieved12 March 2017.
  4. ^abcdMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012)."Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids".The Astrophysical Journal Letters.759 (1): 5.arXiv:1209.5794.Bibcode:2012ApJ...759L...8M.doi:10.1088/2041-8205/759/1/L8. Retrieved12 March 2017.
  5. ^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)
  6. ^abcdWaszczak, 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. Retrieved12 March 2017.
  7. ^Hanus, 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 & Astrophysics.530: 16.arXiv:1104.4114.Bibcode:2011A&A...530A.134H.doi:10.1051/0004-6361/201116738. Retrieved12 March 2017.
  8. ^abcdBehrend, Raoul."Asteroids and comets rotation curves – (1185) Nikko".Geneva Observatory. Retrieved12 March 2017.
  9. ^abStephens, Robert D. (June 2005)."Rotational periods of 743 Eugenisis, 995 Sternberga, 1185 Nikko 2892 Filipenko, 3144 Brosche, and 3220 Murayama".The Minor Planet Bulletin.32 (2):27–28.Bibcode:2005MPBu...32...27S.ISSN 1052-8091. Retrieved12 March 2017.
  10. ^Veres, 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. Retrieved12 March 2017.
  11. ^ab"1185 Nikko (1927 WC)".Minor Planet Center. Retrieved12 March 2017.
  12. ^Menke, John (December 2005)."Asteroid lightcurve results from Menke Observatory".The Minor Planet Bulletin.32 (4):85–88.Bibcode:2005MPBu...32...85M.ISSN 1052-8091. Retrieved12 March 2017.
  13. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved12 March 2017.

External links

[edit]
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Comets
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