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14335 Alexosipov

From Wikipedia, the free encyclopedia
Main-belt asteroid

14335 Alexosipov
Discovery[1]
Discovered byN. Chernykh
Discovery siteCrimean Astrophysical Obs.
Discovery date3 September 1981
Designations
(14335) Alexosipov
Named after
Alexandr Osipov
(astronomer)[2]
1981 RR3 · 1971 SZ1
1971 TE1
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc45.69 yr (16,689 days)
Aphelion2.7038AU
Perihelion1.7656 AU
2.2347 AU
Eccentricity0.2099
3.34yr (1,220 days)
283.07°
0° 17m 42s / day
Inclination5.9013°
170.12°
181.86°
Earth MOID0.7595 AU
Physical characteristics
Dimensions3.92 km(calculated)[3]
4.176±0.101 km[4][5]
7.18±0.01h[a]
0.24(assumed)[3]
0.279±0.032[4][5]
S[3][6]
14.2[1][3] · 14.20±0.46[6] · 13.9[4]

14335 Alexosipov, provisional designation1981 RR3, is a stony Floraasteroid from the inner regions of theasteroid belt, approximately 4 kilometers in diameter. It was discovered by Soviet–Russian astronomerNikolai Chernykh at theCrimean Astrophysical Observatory in Nauchnyj, on 3 September 1981.[7] The asteroid was named after astronomerAlexandr Osipov.[2]

Orbit and classification

[edit]

Alexosipov is a member of theFlora family, one of the largest groups ofstony asteroids. It orbits the Sun in theinner main-belt at a distance of 1.8–2.7 AU once every 3 years and 4 months (1,220 days). Its orbit has aneccentricity of 0.21 and aninclination of 6° with respect to theecliptic.[1] The firstastrometric observations were already made at the discovering observatory in 1971, 10 years prior to its discovery. However, these observations were not used to extend the asteroid'sobservation arc.[7]

Physical characteristics

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Alexosipov has been characterized as a commonS-type asteroid byPan-STARRS photometric survey.[6]

Rotation period

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A rotationallightcurve ofAlexosipov was obtained from photometric observations made by American astronomerBrian Skiff in October 2011. It gave a well-definedrotation period of7.18±0.01 hours with a low brightness variation of 0.10 inmagnitude (U=3).[a] A low brightness amplitude typically indicates that the body has a nearly spheroidal shape.

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,Alexosipov measures 4.2 kilometers in diameter and its surface has analbedo of 0.279,[4][5] while theCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – which derives from8 Flora, the largest member and namesake of this orbital family – and calculates a diameter of 3.9 kilometers with anabsolute magnitude of 14.2.[3]

Naming

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Thisminor planet was named in memory of astronomer Alexandr Kuzmich Osipov (1920–2004), observer of artificial satellites, the Moon, planets and comets at theAstronomical Observatory of the Kyiv National University in Ukraine. He is described as a skilled teacher for many generations of students.[2] The approved naming citation was published by theMinor Planet Center on 15 December 2005 (M.P.C. 55721).[8]

Notes

[edit]
  1. ^abSkiff (2011) web: rotation period7.18±0.01 hours with a brightness amplitude of0.10 mag. Summary figures for (14335) Alexosipov atCollaborative Asteroid Lightcurve Link (CALL)

References

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  1. ^abcd"JPL Small-Body Database Browser: 14335 Alexosipov (1981 RR3)" (2017-06-02 last obs.).Jet Propulsion Laboratory. Retrieved5 July 2017.
  2. ^abcSchmadel, Lutz D. (2006). "(14335) Alexosipov [2.23, 0.21, 5.9]".Dictionary of Minor Planet Names – (14335) Alexosipov, Addendum to Fifth Edition: 2003–2005.Springer Berlin Heidelberg. p. 85.doi:10.1007/978-3-540-34361-5_848.ISBN 978-3-540-34360-8.
  3. ^abcdef"LCDB Data for (14335) Alexosipov". Asteroid Lightcurve Database (LCDB). Retrieved11 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. Retrieved11 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. Retrieved3 December 2016.
  6. ^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. Retrieved11 May 2016.
  7. ^ab"14335 Alexosipov (1981 RR3)".Minor Planet Center. Retrieved11 May 2016.
  8. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved11 May 2016.

External links

[edit]
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