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4904 Makio

From Wikipedia, the free encyclopedia
Main-belt asteroid

4904 Makio
Discovery[1]
Discovered byY. Mizuno
T. Furuta
Discovery siteKani Obs. (403)
Discovery date21 November 1989
Designations
(4904) Makio
Named after
Makio Akiyama
(Japanese astronomer)[2]
1989 WZ · 1974 TB
1974 WC · 1980 KF2
main-belt · (inner)[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc42.65 yr (15,578 days)
Aphelion2.6986AU
Perihelion2.0785 AU
2.3886 AU
Eccentricity0.1298
3.69yr (1,348 days)
129.31°
0° 16m 1.2s / day
Inclination10.122°
228.94°
266.59°
Physical characteristics
Dimensions6.992±0.044 km[5][6]
9.40 km(calculated)[4]
7.830±0.003h[7]
0.20(assumed)[4]
0.329±0.033[6]
0.3295±0.0326[5]
S[4]
12.5[1][4] · 12.6[5] · 12.70±0.57[8]

4904 Makio, provisional designation1989 WZ, is a stonyasteroid from the inner regions of theasteroid belt, approximately 8 kilometers in diameter. It was discovered by Japanese astronomersYoshikane Mizuno andToshimasa Furuta at Kani Observatory (403) on 21 November 1989.[3] It was named after Japanese astronomerMakio Akiyama.[2]

Orbit and classification

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Makio orbits the Sun in theinner main-belt at a distance of 2.1–2.7 AU once every 3 years and 8 months (1,348 days). Its orbit has aneccentricity of 0.13 and aninclination of 10° with respect to theecliptic.[1]

It was first identified as1974 TB at the ChileanCerro El Roble Station in 1974, extending the body'sobservation arc by 15 years prior to its discovery.[3]

Physical characteristics

[edit]

Makio has been characterized as a commonS-type asteroid.[4]

Rotation period

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A rotationallightcurve ofMakio was obtained fromphotometric observations made by Julian Oey at the Australian Kingsgrove Observatory (E19) in March 2009. Lightcurve analysis gave arotation period of7.830 hours with a small brightness variation of 0.08magnitude, indicative of a spheroidal shape (U=2).[7]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Makio measures 7.0 kilometers in diameter and its surface has analbedo of 0.33,[5][6] while theCollaborative Asteroid Lightcurve Link assumes a standard albedo forstony asteroids of 0.20 and calculates a diameter of 9.4 kilometers with anabsolute magnitude of 12.5.[4]

Naming

[edit]

Thisminor planet was named after Japanese astronomerMakio Akiyama (born 1950), an observer anddiscoverer of minor planets himself at the Susono Observatory (886).[2] The official naming citation was published by theMinor Planet Center on 5 March 1996 (M.P.C. 26763).[9]

References

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  1. ^abcd"JPL Small-Body Database Browser: 4904 Makio (1989 WZ)" (2017-06-05 last obs.).Jet Propulsion Laboratory. Retrieved20 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(4904) Makio".Dictionary of Minor Planet Names – (4904) Makio.Springer Berlin Heidelberg. p. 423.doi:10.1007/978-3-540-29925-7_4794.ISBN 978-3-540-00238-3.
  3. ^abc"4904 Makio (1989 WZ)".Minor Planet Center. Retrieved18 November 2016.
  4. ^abcdefg"LCDB Data for (4904) Makio". Asteroid Lightcurve Database (LCDB). Retrieved18 November 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.
  6. ^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.
  7. ^abOey, Julian (October 2010)."Light Curve Analysis of Asteroids from Leura and Kingsgrove Observatory in the First Half of 2009".The Minor Planet Bulletin.37 (4):135–136.Bibcode:2010MPBu...37..135O.ISSN 1052-8091. Retrieved18 November 2016.
  8. ^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. Retrieved18 November 2016.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved18 November 2016.

External links

[edit]
Minor planets
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