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6537 Adamovich

From Wikipedia, the free encyclopedia
Stony Florian asteroid

6537 Adamovich
Discovery[1]
Discovered byN. Chernykh
Discovery siteCrimean Astrophysical Obs.
Discovery date19 August 1979
Designations
(6537) Adamovich
Named after
Aleksandr Adamovich
(Byelorussian writer)[2]
1979 QK6 · 1985 JQ
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc37.80 yr (13,805 days)
Aphelion2.6055AU
Perihelion1.7518 AU
2.1786 AU
Eccentricity0.1959
3.22yr (1,175 days)
306.60°
0° 18m 23.4s / day
Inclination4.0254°
120.08°
200.65°
Physical characteristics
Dimensions3.22±0.50 km[4]
4.253±0.227 km[5][6]
4.50 km(calculated)[3]
2.4±0.1h[7]
0.170±0.029[5][6]
0.24(assumed)[3]
0.50±0.18[4]
S[3]
13.9[1][3][4] · 13.81±0.14(R)[7] · 13.12±1.33[8] · 14.4[5]

6537 Adamovich, provisional designation1979 QK6, is a stony Florianasteroid from the inner regions of theasteroid belt, approximately 4 kilometers in diameter.

It was discovered on 19 August 1979, by Soviet–Russian astronomerNikolai Chernykh at theCrimean Astrophysical Observatory, Nauchnyj, on the Crimean peninsula.[9] The asteroid was later named after Byelorussian writerAleksandr Adamovich.[2]

Orbit and classification

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Adamovich is aS-type asteroid 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 1.8–2.6 AU once every 3 years and 3 months (1,175 days). Its orbit has aneccentricity of 0.20 and aninclination of 4° with respect to theecliptic.[1]

Physical characteristics

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Lightcurve photometry

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A fragmentary rotationallightcurve ofAdamovich was obtained from photometric observation made at thePalomar Transient Factory in California in February 2013. It showed a provisionalrotation period of2.4±0.1 hours with a brightness amplitude of 0.13magnitude (U=1).[7]

Diameter and albedo

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According to the surveys carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Adamovich measures 3.22 and 4.3 kilometers in diameter and its surface has analbedo of 0.17 and 0.50, respectively.[4][5][6] TheCollaborative Asteroid Lightcurve Link (CALL) assumes analbedo of 0.24 – derived from8 Flora, the largest member and namesake of its orbital family – and calculates a diameter of 4.5 kilometers with anabsolute magnitude of 13.9.[3]

Naming

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Thisminor planet was named in memory ofByelorussian–Russian Aleksandr Mikhajlovich Adamovich (1927–1994), publicist, literary scholar and talented writer, known for his civic responsibility.[2] The official naming citation was published on 4 May 1999 (M.P.C.34624).[10]

References

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  1. ^abcd"JPL Small-Body Database Browser: 6537 Adamovich (1979 QK6)" (2017-06-05 last obs.).Jet Propulsion Laboratory. Retrieved4 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(6537) Adamovich".Dictionary of Minor Planet Names – (6537) Adamovich.Springer Berlin Heidelberg. p. 540.doi:10.1007/978-3-540-29925-7_5936.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (6537) Adamovich". Asteroid Lightcurve Database (LCDB). Retrieved29 April 2016.
  4. ^abcdNugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016)."NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos".The Astronomical Journal.152 (3): 12.arXiv:1606.08923.Bibcode:2016AJ....152...63N.doi:10.3847/0004-6256/152/3/63.
  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.S2CID 35447010. Retrieved29 April 2016.
  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.S2CID 118745497. Retrieved5 December 2016.
  7. ^abcChang, Chan-Kao;Ip, Wing-Huen; Lin, Hsing-Wen; Cheng, Yu-Chi; Ngeow, Chow-Choong; Yang, Ting-Chang; et al. (June 2014)."313 New Asteroid Rotation Periods from Palomar Transient Factory Observations".The Astrophysical Journal.788 (1): 21.arXiv:1405.1144.Bibcode:2014ApJ...788...17C.doi:10.1088/0004-637X/788/1/17.S2CID 51100134. Retrieved10 January 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.S2CID 53493339. Retrieved29 April 2016.
  9. ^"6537 Adamovich (1979 QK6)".Minor Planet Center. Retrieved29 April 2016.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved29 April 2016.

External links

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