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1088 Mitaka

From Wikipedia, the free encyclopedia
Asteroid

1088 Mitaka
Modelled shape ofMitaka from itslightcurve
Discovery[1]
Discovered byO. Oikawa
Discovery siteTokyo Astronomical Obs.
Discovery date17 November 1927
Designations
(1088) Mitaka
Named after
Mitaka[2](Japanese village)
1927 WA · 1942 FR
1953 VW3 · 1971 BE
A917 RA
Orbital characteristics[3]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc88.22 yr (32,224 days)
Aphelion2.6328AU
Perihelion1.7722 AU
2.2025 AU
Eccentricity0.1954
3.27yr (1,194 days)
200.92°
0° 18m 5.4s / day
Inclination7.6514°
54.495°
319.50°
Physical characteristics
11.33±2.51 km[6]
13.35±0.75 km[7]
15.137±0.131 km[8]
15.957±0.030 km[9]
16.016 km[10]
16.02 km(taken)[11]
3.027±0.003 h[12]
3.0353±0.0005 h[13]
3.035377 h[14]
3.035378±0.000005 h[15]
3.0354±0.0002 h[16]
3.0361±0.0007 h[16]
3.049±0.005h[17]
  • (115.0°, 46.0°) (λ11)[5]
  • (278.0°, −72.0°) (λ22)[5]
0.1549[10]
0.1588±0.0204[9]
0.173±0.025[8]
0.276±0.034[7]
0.37±0.16[6]
11.39[3][7] · 11.55[6] · 11.62[11][9] · 11.62±0.08[10][17]

1088 Mitaka (prov. designation:1927 WA) is a brightbackground asteroid from the inner regions of theasteroid belt. It was discovered on 17 November 1927, by Japanese astronomerOkuro Oikawa at the oldTokyo Astronomical Observatory in Japan.[1] The stonyS-type asteroid has a notably shortrotation period of 3.0 hours and measures approximately 15 kilometers (9.3 miles) in diameter. It was named after the Japanese village ofMitaka.[2]

Orbit and classification

[edit]

Mitaka is a non-family asteroid of the main belt'sbackground population when applying thehierarchical clustering method to itsproper orbital elements.[4][5] It orbits the Sun in theinner asteroid belt at a distance of 1.8–2.6 AU once every 3 years and 3 months (1,194 days). Its orbit has aneccentricity of 0.20 and aninclination of 8° with respect to theecliptic.[3] The asteroid was first observed asA917 RA at theSimeiz Observatory on 11 September 1917. The body'sobservation arc begins at Tokyo in December 1927, one month after its official discovery observation.[1]

Naming

[edit]

Thisminor planet was named after the Japanese village ofMitaka, where the discoveringTokyo Astronomical Observatory was located. Nowadays the city of Mitaka hosts the headquarters of theNational Astronomical Observatory of Japan with theTokyo Photoelectric Meridian Circle, public relation and data centers, and several telescopes. The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 103).[2]

Physical characteristics

[edit]

Mitaka is a common, stonyS-type asteroid in both theTholen and Bus–BinzelSMASS classification.[3][11]

Rotation period and poles

[edit]

Several rotationallightcurves ofMitaka have been obtained fromphotometric observations since 1989.[12][13][16][17] Analysis of the best rated lightcurve by French amateur astronomerPierre Antonini gave arotation period of 3.0361 hours with a consolidated brightness variation of 0.23 to 0.62magnitude (U=3).[11][16]

In 2009 and 2011, modelling ofMitaka's lightcurve using photometric data from theUS Naval Observatory, the Uppsala Asteroid Photometric Catalogue (UAPC), thePalmer Divide Observatory's archive, thePalomar Transient Factory survey, and from individual observers, gave a concurring rotation period of 3.035377 and 3.035378 hours.[14][15] The modeled lightcurves also gave aspin axis of (115.0°, 46.0°) and (278.0°, −72.0°),[14] as well as (280.0°, −71.0°) inecliptic coordinates (λ, β).[15]

Diameter and albedo

[edit]

According to the surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Mitaka measures between 11.33 and 16.016 kilometers in diameter and its surface has analbedo between 0.1549 and 0.37.[6][7][8][9][10] TheCollaborative Asteroid Lightcurve Link adoptsPetr Pravec's revised WISE results with an albedo of 0.1549 and takes a diameter of 16.02 kilometers based on anabsolute magnitude of 11.62.[11]

References

[edit]
  1. ^abcd"1088 Mitaka (1927 WA)".Minor Planet Center. Retrieved27 September 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1088) Mitaka".Dictionary of Minor Planet Names – (1088) Mitaka.Springer Berlin Heidelberg. p. 93.doi:10.1007/978-3-540-29925-7_1089.ISBN 978-3-540-00238-3.
  3. ^abcdefghi"JPL Small-Body Database Browser: 1088 Mitaka (1927 WA)" (2017-07-05 last obs.).Jet Propulsion Laboratory. Retrieved27 September 2017.
  4. ^ab"Asteroid 1088 Mitaka – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved13 March 2020.
  5. ^abcd"Asteroid 1088 Mitaka".Small Bodies Data Ferret. Retrieved13 March 2020.
  6. ^abcdNugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016)."NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos".The Astronomical Journal.152 (3): 12.arXiv:1606.08923.Bibcode:2016AJ....152...63N.doi:10.3847/0004-6256/152/3/63.
  7. ^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)
  8. ^abcMasiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014)."Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos".The Astrophysical Journal.791 (2): 11.arXiv:1406.6645.Bibcode:2014ApJ...791..121M.doi:10.1088/0004-637X/791/2/121.S2CID 119293330. Retrieved27 September 2017.
  9. ^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.S2CID 35447010.
  10. ^abcdPravec, Petr; Harris, Alan W.; Kusnirák, Peter; Galád, Adrián; Hornoch, Kamil (September 2012)."Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations".Icarus.221 (1):365–387.Bibcode:2012Icar..221..365P.doi:10.1016/j.icarus.2012.07.026. Retrieved27 September 2017.
  11. ^abcde"LCDB Data for (1088) Mitaka". Asteroid Lightcurve Database (LCDB). Retrieved27 September 2017.
  12. ^abMacias, Amadeo Aznar (January 2015)."Asteroid Lightcurve Analysis at Isaac Aznar Observatory Aras De Los Olmos, Valencia, Spain".The Minor Planet Bulletin.42 (1):4–6.Bibcode:2015MPBu...42....4M.ISSN 1052-8091. Retrieved27 September 2017.
  13. ^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.
  14. ^abcDurech, J.; Kaasalainen, M.; Warner, B. D.; Fauerbach, M.; Marks, S. A.; Fauvaud, S.; et al. (January 2009)."Asteroid models from combined sparse and dense photometric data"(PDF).Astronomy and Astrophysics.493 (1):291–297.Bibcode:2009A&A...493..291D.doi:10.1051/0004-6361:200810393. Retrieved24 August 2017.
  15. ^abcHanus, 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. Retrieved27 September 2017.
  16. ^abcdBehrend, Raoul."Asteroids and comets rotation curves – (1088) Mitaka".Geneva Observatory. Retrieved27 September 2017.
  17. ^abcWisniewski, W. Z.; Michalowski, T. M.; Harris, A. W.; McMillan, R. S. (March 1995)."Photoelectric Observations of 125 Asteroids".Abstracts of the Lunar and Planetary Science Conference.26: 1511.Bibcode:1995LPI....26.1511W. Retrieved27 September 2017.

External links

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