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4672 Takuboku

From Wikipedia, the free encyclopedia
Main-belt asteroid

4672 Takuboku
Discovery [1]
Discovered byS. Ueda
H. Kaneda
Discovery siteKushiro Obs.
Discovery date17 April 1988
Designations
(4672) Takuboku
Named after
Takuboku Ishikawa[1]
(Japanese poet)
1988 HB · 1971 HT
1979 WS7 · 1981 AN3
main-belt[1][2] · (outer)
background[3]
Orbital characteristics[2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc46.11yr (16,841 d)
Aphelion3.3411AU
Perihelion3.0318 AU
3.1864 AU
Eccentricity0.0485
5.69 yr (2,078 d)
45.665°
0° 10m 23.88s / day
Inclination15.530°
91.663°
175.66°
Physical characteristics
Dimensions35.0 km × 35.0 km(occultation)[4]
28.115±0.258 km[5]
35.59±1.9[6]
0.0609±0.007[6]
0.108±0.018[5]
10.90[6]
11.4[2]

4672 Takuboku, provisional designation1988 HB, is a backgroundasteroid from the outer regions of theasteroid belt, approximately 35 kilometers (22 miles) in diameter. It was discovered on 17 April 1988, by Japanese astronomersSeiji Ueda andHiroshi Kaneda at theKushiro Observatory on Hokkaido, Japan. The asteroid was named after the Japanese poetTakuboku Ishikawa.[1] In 2005, measurement of the body'soccultation ellipse also gave 35.0 × 35.0 kilometers.[4]

Orbit and classification

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Takuboku is a non-family asteroid from the main belt'sbackground population.[3] It orbits the Sun in theouter main-belt at a distance of 3.0–3.3 AU once every 5 years and 8 months (2,078 days;semi-major axis of 3.19 AU). Its orbit has aneccentricity of 0.05 and aninclination of 16° with respect to theecliptic.[2]

The body'sobservation arc begins with its first observation as1971 HT atCrimea–Nauchnij in April 1971, or 17 years prior to its official discovery observation at Kushiro.[1]

Physical characteristics

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Takuboku has anabsolute magnitude of between 10.90 and 11.4. As of 2018, no rotationallightcurve ofTakuboku has been obtained fromphotometric observations. The body'srotation period,pole and shape remain unknown.[2]

Diameter and albedo

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According to the surveys carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer and the Infrared Astronomical SatelliteIRAS,Takuboku measures 28.115 and 35.59 kilometers in diameter and its surface has analbedo of 0.108 and 0.0609, respectively.[5][6]

Occultation

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On 13 June 2005,Takubokuocculted 9.3 magnitude star TYC 0312-00789-1, causing a predicted magnitude drop 6.8 during 4.3 seconds. The occultation was visible over the southern island of New Zealand only. Measurement of the asteroid's occultation dimensions 35.0 ×35.0 for its major and minor best-fit ellipse (the fit's quality code is 1).[4][a]

Naming

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Thisminor planet was named after Japanese poetTakuboku Ishikawa (1886–1912) who lived in Japan's lateMeiji-era. He is best known forIchiaku no Suna (A Handful of Sand) a collection of 551 tanka poems published in 1910.[1] The official naming citation was published by theMinor Planet Center on 10 November 1992 (M.P.C. 21131).[7]

Notes

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  1. ^Occultation Prediction Chart: Occultation by (4672) Takuboku - TYC 0312-00789u on 13 June 2005, 11:51 UT

References

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  1. ^abcdef"4672 Takuboku (1988 HB)".Minor Planet Center. Retrieved16 May 2018.
  2. ^abcde"JPL Small-Body Database Browser: 4672 Takuboku (1988 HB)" (2017-06-05 last obs.).Jet Propulsion Laboratory. Retrieved16 May 2018.
  3. ^ab"Asteroid 4672 Takuboku".Small Bodies Data Ferret. Retrieved16 May 2018.
  4. ^abcDunham, D. W.; Herald, D.; Frappa, E.; Hayamizu, T.; Talbot, J.; Timerson, B. (June 2016)."Asteroid Occultations V14.0".NASA Planetary Data System: EAR-A-3-RDR-OCCULTATIONS-V14.0.Bibcode:2016PDSS..243.....D. Retrieved16 May 2018.list andtimings
  5. ^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.
  6. ^abcdTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System.12: IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved22 October 2019.
  7. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved16 May 2018.

External links

[edit]
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