Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

4936 Butakov

From Wikipedia, the free encyclopedia
Main-belt asteroid

4936 Butakov
Discovery[1]
Discovered byL. V. Zhuravleva
Discovery siteCrimean Astrophysical Obs.
Discovery date22 October 1985
Designations
(4936) Butakov
Named after
Grigory Butakov
(Russian admiral)[2]
1985 UY4 · 1978 TK4
1978 VH12
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc66.70 yr (24,364 days)
Aphelion2.5617AU
Perihelion1.9909 AU
2.2763 AU
Eccentricity0.1254
3.43yr (1,254 days)
70.538°
0° 17m 13.2s / day
Inclination5.9129°
155.77°
283.92°
Physical characteristics
Dimensions4.465±0.051[4]
4.867±0.025 km[5]
5.41 km(calculated)[3]
13.828±0.001h[6]
13.9078±0.3029 h[7]
19.200±0.380 h[8]
0.24(assumed)[3]
0.3589±0.0587[5]
0.428±0.076[4]
S[3]
13.5[1][3] · 13.3[5] · 13.400±0.080(R)[8] · 13.418±0.001(R)[7]

4936 Butakov, provisional designation1985 UY4, is a stony Florianasteroid from the inner regions of theasteroid belt, approximately 5 kilometers in diameter. The asteroid was discovered on 22 October 1985, by Soviet–Ukrainian astronomerLyudmila Zhuravleva at theCrimean Astrophysical Observatory in Nauchnyj, on the Crimean peninsula.[9] It was named after Russian admiralGrigory Butakov.[2]

Orbit and classification

[edit]

TheS-type asteroid is a member of theFlora family, one of the largest groups of stony asteroids in the main-belt. It orbits the Sun in theinner main-belt at a distance of 2.0–2.6 AU once every 3 years and 5 months (1,254 days). Its orbit has aneccentricity of 0.13 and aninclination of 6° with respect to theecliptic.[1] The firstprecovery was obtained at the U.S.Goethe Link Observatory in 1950, extending the asteroid'sobservation arc by 35 years prior to its discovery.[9]

Physical characteristics

[edit]

Rotation period

[edit]

According to the survey carried out byNEOWISE mission of NASA's space-basedWide-field Infrared Survey Explorer,Butakov measures 4.5 and 4.9 kilometers in diameter and its surface has a highalbedo of 0.36 and 0.43, respectively,[4][5] while theCollaborative Asteroid Lightcurve Link assumes an intermediate albedo of 0.24 – which derives from8 Flora, the largest member and namesake of this orbital family – and calculates a somewhat larger diameter of 5.4 kilometers.[3]

Diameter and albedo

[edit]

In 2007, a rotationallightcurves ofButakov was obtained at the Carbuncle Hill Observatory which gave arotation period of13.828±0.001 hours with a brightness amplitude of 0.14 inmagnitude (U=2).[6] Two more lightcurves were obtained from photometric observations made at the U.S.Palomar Transient Factory in January and February 2014. They showed arotation period of19.200±0.380 and13.9078±0.3029 hours, respectively, with a corresponding brightness variation of 0.11 and 0.08 in magnitude (U=2/2).[8][7]

Naming

[edit]

Thisminor planet was named in memory of Russian admiralGrigory Butakov (1820–1882), who fought in theCrimean War. In 1856, when the war ended, he becameRear admiral of theBlack Sea Fleet and Naval Governor of Nikolaev and Sevastopol. The minor planet2121 Sevastopol is named after the city on the Crimean peninsula.[2] Butakov is widely credited as being the father of steam-powered ship tactics during the 19th century. The official naming citation was published by theMinor Planet Center on 4 May 1999 (M.P.C. 34620).[10]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 4936 Butakov (1985 UY4)" (2017-03-29 last obs.).Jet Propulsion Laboratory. Retrieved20 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(4936) Butakov".Dictionary of Minor Planet Names – (4936) Butakov.Springer Berlin Heidelberg. p. 425.doi:10.1007/978-3-540-29925-7_4823.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (4936) Butakov". Asteroid Lightcurve Database (LCDB). Retrieved2 May 2016.
  4. ^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. Retrieved5 December 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. Retrieved2 May 2016.
  6. ^abPray, Donald P.; Galad, Adrian; Husarik, Marek; Oey, Julian (March 2008)."Lightcurve Analysis of Fourteen Asteroids".The Minor Planet Bulletin.35 (1):34–36.Bibcode:2008MPBu...35...34P.ISSN 1052-8091. Retrieved2 May 2016.
  7. ^abcWaszczak, 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. Retrieved2 May 2016.
  8. ^abcChang, Chan-Kao;Ip, Wing-Huen; Lin, Hsing-Wen; Cheng, Yu-Chi; Ngeow, Chow-Choong; Yang, Ting-Chang; et al. (August 2015)."Asteroid Spin-rate Study Using the Intermediate Palomar Transient Factory".The Astrophysical Journal Supplement Series.219 (2): 19.arXiv:1506.08493.Bibcode:2015ApJS..219...27C.doi:10.1088/0067-0049/219/2/27. Retrieved2 May 2016.
  9. ^ab"4936 Butakov (1985 UY4)".Minor Planet Center. Retrieved2 May 2016.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved2 May 2016.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
Other
Authority control databasesEdit this at Wikidata
Retrieved from "https://en.wikipedia.org/w/index.php?title=4936_Butakov&oldid=1313081658"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp