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词条 4904 Makio
释义

  1. Orbit and classification

  2. Physical characteristics

      Rotation period    Diameter and albedo  

  3. Naming

  4. References

  5. External links

{{Infobox planet
| minorplanet = yes
| name = 4904 Makio
| background = #D6D6D6
| image =
| image_size =
| caption =
| discovery_ref =  
| discovered = 21 November 1989
| discoverer = Y. Mizuno
T. Furuta
| discovery_site = Kani Obs. ({{small|403}})
| mpc_name = (4904) Makio
| alt_names = 1989 WZ{{·}}1974 TB
1974 WC{{·}}{{mp|1980 KF|2}}
| pronounced =
| named_after = Makio Akiyama
{{small|(Japanese astronomer)}}[2]
| mp_category = main-belt{{·}}{{small|(inner)}} [3][4]
| orbit_ref =  
| epoch = 4 September 2017 (JD 2458000.5)
| uncertainty = 0
| observation_arc = 42.65 yr (15,578 days)
| aphelion = 2.6986 AU
| perihelion = 2.0785 AU
| semimajor = 2.3886 AU
| eccentricity = 0.1298
| period = 3.69 yr (1,348 days)
| mean_anomaly = 129.31°
| mean_motion = {{Deg2DMS|0.2670|sup=ms}} / day
| inclination = 10.122°
| asc_node = 228.94°
| arg_peri = 266.59°
| dimensions = {{val|6.992|0.044}} km[6][7]
9.40 km {{small|(calculated)}}[4]
| rotation = {{val|7.830|0.003}} h[9]
| albedo = 0.20 {{small|(assumed)}}[4]
{{val|0.329|0.033}}[7]
{{val|0.3295|0.0326}}[6]
| spectral_type = S [4]
| abs_magnitude = 12.5[4]{{·}}12.6[6]{{·}}{{val|12.70|0.57}}[17]
}}4904 Makio, provisional designation {{mp|1989 WZ}}, is a stony asteroid from the inner regions of the asteroid belt, approximately 8 kilometers in diameter. It was discovered by Japanese astronomers Yoshikane Mizuno and Toshimasa Furuta at Kani Observatory ({{small|403}}) on 21 November 1989.[3] It was named after Japanese astronomer Makio Akiyama.[2]

Orbit and classification

Makio orbits the Sun in the inner main-belt at a distance of 2.1–2.7 AU once every 3 years and 8 months (1,348 days). Its orbit has an eccentricity of 0.13 and an inclination of 10° with respect to the ecliptic.

It was first identified as {{mp|1974 TB}} at the Chilean Cerro El Roble Station in 1974, extending the body's observation arc by 15 years prior to its discovery.[3]

Physical characteristics

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

Rotation period

A rotational lightcurve of Makio was obtained from photometric observations made by Julian Oey at the Australian Kingsgrove Observatory ({{small|E19}}) in March 2009. Lightcurve analysis gave a rotation period of {{val|7.830}} hours with a small brightness variation of 0.08 magnitude, indicative of a spheroidal shape ({{small|U=2}}).[9]

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Makio measures 7.0 kilometers in diameter and its surface has an albedo of 0.33,[6][7] while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 9.4 kilometers with an absolute magnitude of 12.5.[4]

Naming

This minor planet was named after Japanese astronomer Makio Akiyama (born 1950), an observer and discoverer of minor planets himself at the Susono Observatory ({{small|886}}).[2] The official naming citation was published by the Minor Planet Center on 5 March 1996 ({{small|M.P.C. 26763}}).[28]

References

1. ^{{cite book |title = Dictionary of Minor Planet Names – (4904) Makio |last = Schmadel | first = Lutz D. |publisher = Springer Berlin Heidelberg |page = 423 |date = 2007 |isbn = 978-3-540-00238-3 |doi = 10.1007/978-3-540-29925-7_4794 |chapter = (4904) Makio }}
2. ^{{cite web |title = 4904 Makio (1989 WZ) |work = Minor Planet Center |url = http://www.minorplanetcenter.net/db_search/show_object?object_id=4904 |accessdate = 18 November 2016}}
3. ^{{cite web |title = MPC/MPO/MPS Archive |work = Minor Planet Center |url = http://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html |accessdate = 18 November 2016}}
4. ^{{cite web |title = LCDB Data for (4904) Makio |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=4904%7CMakio |accessdate = 18 November 2016}}
5. ^{{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 |journal = The Astrophysical Journal |volume = 741 |issue = 2 |page = 25 |bibcode = 2011ApJ...741...90M |doi = 10.1088/0004-637X/741/2/90 |arxiv = 1109.6407 }}
6. ^{{Cite journal |author = Oey, Julian |date = October 2010 |title = Light Curve Analysis of Asteroids from Leura and Kingsgrove Observatory in the First Half of 2009 |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2010MPBu...37..135O |journal = The Minor Planet Bulletin |volume = 37 |issue = 4 |pages = 135–136 |issn = 1052-8091 |bibcode = 2010MPBu...37..135O |access-date= 18 November 2016}}
7. ^{{cite journal |display-authors = 6 |first1 = Peter |last1 = Veres |first2 = Robert |last2 = Jedicke |first3 = Alan |last3 = Fitzsimmons |first4 = Larry |last4 = Denneau |first5 = Mikael |last5 = Granvik |first6 = Bryce |last6 = Bolin |first7 = Serge |last7 = Chastel |first8 = Richard J. |last8 = Wainscoat |first9 = William S. |last9 = Burgett |first10 = Kenneth C. |last10 = Chambers |first11 = Heather |last11 = Flewelling |first12 = Nick |last12 = Kaiser |first13 = Eugen A. |last13 = Magnier |first14 = Jeff S. |last14 = Morgan |first15 = Paul A. |last15 = Price |first16 = John L. |last16 = Tonry |first17 = Christopher |last17 = Waters |date = November 2015 |title = Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015Icar..261...34V |journal = Icarus |volume = 261 |pages = 34–47 |bibcode = 2015Icar..261...34V |doi = 10.1016/j.icarus.2015.08.007 |arxiv = 1506.00762 |access-date= 18 November 2016}}
8. ^{{cite journal |display-authors = 6 |first1 = Joseph R. |last1 = Masiero |first2 = A. K. |last2 = Mainzer |first3 = T. |last3 = Grav |first4 = J. M. |last4 = Bauer |first5 = R. M. |last5 = Cutri |first6 = J. |last6 = Dailey |first7 = P. R. M. |last7 = Eisenhardt |first8 = R. S. |last8 = McMillan |first9 = T. B. |last9 = Spahr |first10 = M. F. |last10 = Skrutskie |first11 = D. |last11 = Tholen |first12 = R. G. |last12 = Walker |first13 = E. L. |last13 = Wright |first14 = E. |last14 = DeBaun |first15 = D. |last15 = Elsbury |first16 = T., IV |last16 = Gautier |first17 = S. |last17 = Gomillion |first18 = A. |last18 = Wilkins |date = November 2011 |title = Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...68M |journal = The Astrophysical Journal |volume = 741 |issue = 2 |page = 20 |bibcode = 2011ApJ...741...68M |doi = 10.1088/0004-637X/741/2/68 |arxiv = 1109.4096 |access-date= 5 December 2016}}
[1][2][3][4][5][6][7][8]

}}

External links

  • Asteroid Lightcurve Database (LCDB), query form (info)
  • [https://books.google.com/books?id=aeAg1X7afOoC&pg Dictionary of Minor Planet Names], Google books
  • Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
  • Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
  • {{JPL small body}}
{{Minor planets navigator|4903 Ichikawa |number=4904 |4905 Hiromi}}{{Small Solar System bodies}}{{DEFAULTSORT:Makio}}

6 : Background asteroids|Discoveries by Yoshikane Mizuno|Discoveries by Toshimasa Furuta|Minor planets named for people|Named minor planets|Astronomical objects discovered in 1989

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