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3669 Vertinskij

From Wikipedia, the free encyclopedia
Florian asteroid

3669 Vertinskij
Discovery [1]
Discovered byL. G. Karachkina
Discovery siteCrimean Astrophysical Obs.
Discovery date21 October 1982
Designations
(3669) Vertinskij
Named after
Alexander Vertinsky[1]
(Russian artist)
1982 UO7 · 1972 TE2
1972 XD · 1980 BG3
1984 KJ
main-belt[1][2] · (inner)
Flora[3][4]
Orbital characteristics[2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc67.54yr (24,668 d)
Aphelion2.3704AU
Perihelion2.0574 AU
2.2139 AU
Eccentricity0.0707
3.29 yr (1,203 d)
201.67°
0° 17m 57.12s / day
Inclination4.8271°
90.940°
34.832°
Physical characteristics
6.243±0.087 km[5]
6.467±0.059 km[6]
6.51 km(calculated)[4]
inconclusive[7]
0.2229±0.0273[6]
0.238±0.008[5]
0.24(assumed)[4]
SMASS =S[2][4]
13.1[2][4]
13.2[6]
13.50±0.21[8]

3669 Vertinskij, provisional designation1982 UO7, is a stony Florianasteroid from the inner regions of theasteroid belt, approximately 6.5 kilometers (4 miles) in diameter. It was discovered on 21 October 1982, by Soviet astronomerLyudmila Karachkina at theCrimean Astrophysical Observatory in Nauchnij, on the Crimean peninsula.[1] TheS-type asteroid was named for Russian artistAlexander Vertinsky.[1]

Orbit and classification

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Vertinskij is a member of theFlora family (402),[4][3] a giantasteroid family and the largest family of stony asteroids in the main-belt.[9] It orbits the Sun in theinner asteroid belt at a distance of 2.1–2.4 AU once every 3 years and 3 months (1,203 days;semi-major axis of 2.21 AU). Its orbit has aneccentricity of 0.07 and aninclination of 5° with respect to theecliptic.[2]

The body'sobservation arc begins with aprecovery taken at thePalomar Observatory in November 1949, nearly 33 years prior to its official discovery observation at Nauchnij.[1]

Physical characteristics

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In theSMASS classification,Vertinskij is a common stonyS-type asteroid.[2]

Rotation period

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In December 2015,photometric observations ofVertinskij at theOakley Southern Sky Observatory gave no conclusive results due to excessive noise and/or insufficient data.[7] As of 2018, the body'srotation period,pole and shape remain unknown.[4]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Vertinskij measures between 6.243 and 6.467 kilometers in diameter and its surface has analbedo between 0.2229 and 0.238,[5][6] while theCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, theparent body of the Flora family – and calculates a diameter of 6.51 kilometers based on anabsolute magnitude of 13.1.[4]

Naming

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Thisminor planet was named after Russian artist and poetAlexander Vertinsky (1889–1957). The official naming citation was published by theMinor Planet Center on 12 September 1992 (M.P.C. 20836).[10]

References

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  1. ^abcdef"3669 Vertinskij (1982 UO7)".Minor Planet Center. Retrieved15 May 2018.
  2. ^abcdef"JPL Small-Body Database Browser: 3669 Vertinskij (1982 UO7)" (2017-06-03 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 15 September 2020. Retrieved15 May 2018.
  3. ^ab"Asteroid 3669 Vertinskij".Small Bodies Data Ferret. Retrieved15 May 2018.
  4. ^abcdefgh"LCDB Data for (3669) Vertinskij". Asteroid Lightcurve Database (LCDB). Retrieved15 May 2018.
  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.S2CID 119293330.
  6. ^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. (catalog)
  7. ^abBlack, Sydney; Linville, Dylan; Michalik, Danielle; Wolf, Matthew; Ditteon, Richard (October 2016). "Lightcurve Analysis of Asteroids Observed at the Oakley Southern Sky Observatory: 2015 December - 2016 April".The Minor Planet Bulletin.43 (4):287–289.Bibcode:2016MPBu...43..287B.ISSN 1052-8091.
  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.S2CID 53493339.
  9. ^Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV. pp. 297–321.arXiv:1502.01628.Bibcode:2015aste.book..297N.doi:10.2458/azu_uapress_9780816532131-ch016.ISBN 9780816532131.S2CID 119280014.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved15 May 2018.

External links

[edit]
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