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5101 Akhmerov

From Wikipedia, the free encyclopedia
Asteroid

5101 Akhmerov
Discovery[1]
Discovered byL. V. Zhuravleva
Discovery siteCrimean Astrophysical Obs.
Discovery date22 October 1985
Designations
(5101) Akhmerov
Named after
Vadim Akhmerov
(Ukrainiansurgeon)[2]
1985 UB5 · 1969 TQ
main-belt · Eos[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc47.37 yr (17,303 days)
Aphelion3.3535AU
Perihelion2.6561 AU
3.0048 AU
Eccentricity0.1160
5.21yr (1,903 days)
60.772°
0° 11m 21.12s / day
Inclination10.699°
205.91°
174.12°
Physical characteristics
Dimensions11.012±0.228 km[4][5]
12.32 km(calculated)[3]
4.2705±0.0010h[6]
0.14(assumed)[3]
0.192±0.036[4][5]
CX[7] · S[3]
12.2[4] · 12.3[1][3] · 12.36±0.41[7] · 12.925±0.003(S)[6]

5101 Akhmerov, provisional designation1985 UB5, is an Eosasteroid from the outer region of theasteroid belt, about 12 kilometers in diameter. It was discovered on 22 October 1985, by Russian astronomerLyudmila Zhuravleva at theCrimean Astrophysical Observatory in Nauchnyj, on the Crimean peninsula.[8] It was later named for Ukrainian surgeonVadim Akhmerov.[2]

Orbit and classification

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Akhmerov is a member of theEos family (606), the largestasteroid family in theouter main belt consisting of nearly 10,000 asteroids.

It orbits the Sun at a distance of 2.7–3.4 AU once every 5 years and 3 months (1,903 days). Its orbit has aneccentricity of 0.12 and aninclination of 11° with respect to theecliptic.[1] A firstprecovery was obtained at the discovering observatory in 1969, extending the body'sobservation arc by 16 years prior to its official discovery observation.[8]

Physical characteristics

[edit]

PanSTARRS photometric survey has characterizedAkhmerov as a CX-type asteroid, a transitional group between the carbonaceousC-type asteroid and the metallicX-type asteroids.[3][7]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA's space-basedWide-field Infrared Survey Explorer,Akhmerov measures 11.0 kilometers in diameter and its surface has an albedo of 0.19.[4][5] TheCollaborative Asteroid Lightcurve Link (CALL) assumes an albedo of 0.14 – derived from221 Eos, the largest member and namesake of this orbital family – and calculates a diameter of 12.3 kilometers with anabsolute magnitude of 12.3.[3]

Rotation period

[edit]

A rotationallightcurve ofAkhmerov was obtained from photometric observations taken at the U.S.Palomar Transient Factory in September 2011. The lightcurve gave arotation period of4.2705±0.0010 hours with a brightness amplitude of 0.33 inmagnitude (U=2).[6]

Naming

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Thisminor planet was named after Vadim Zinov'evich Akhmerov (born 1929), long-time physician at the maternity hospital inAlushta on the Crimean peninsula.[2] The official naming citation was published by theMinor Planet Center on 4 May 1999 (M.P.C. 34620).[9]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 5101 Akhmerov (1985 UB5)" (2017-02-20 last obs.).Jet Propulsion Laboratory. Retrieved20 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(5101) Akhmerov".Dictionary of Minor Planet Names – (5101) Akhmerov.Springer Berlin Heidelberg. p. 439.doi:10.1007/978-3-540-29925-7_4958.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (5101) Akhmerov". Asteroid Lightcurve Database (LCDB). Retrieved3 May 2016.
  4. ^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. Retrieved3 May 2016.
  5. ^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. Retrieved5 December 2016.
  6. ^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. Retrieved3 May 2016.
  7. ^abcVeres, 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. Retrieved3 May 2016.
  8. ^ab"5101 Akhmerov (1985 UB5)".Minor Planet Center. Retrieved3 May 2016.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved3 May 2016.

External links

[edit]
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