14335 Alexosipov
| Discovery [1] | |
|---|---|
| Discovered by | N. Chernykh |
| Discovery site | Crimean Astrophysical Obs. |
| Discovery date | 3 September 1981 |
| Designations | |
| MPC designation | 14335 Alexosipov |
Named after |
Alexandr Osipov (astronomer)[2] |
|
1981 RR3 · 1971 SZ1 1971 TE1 | |
| main-belt · Flora [3] | |
| Orbital characteristics [1] | |
| Epoch 16 February 2017 (JD 2457800.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 44.65 yr (16,307 days) |
| Aphelion | 2.7048 AU |
| Perihelion | 1.7664 AU |
| 2.2356 AU | |
| Eccentricity | 0.2099 |
| 3.34 yr (1,221 days) | |
| 224.22° | |
| 0° 17m 41.64s / day | |
| Inclination | 5.9020° |
| 170.13° | |
| 181.73° | |
| Earth MOID | 0.7612 AU |
| Physical characteristics | |
| Dimensions |
3.92 km (calculated)[3] 4.176±0.101 km[4][5] |
| 7.18±0.01 h[lower-alpha 1] | |
|
0.24 (assumed)[3] 0.279±0.032[4][5] | |
| S [6][3] | |
| 14.2[1][3] · 14.20±0.46[6] · 13.9[4] | |
|
| |
14335 Alexosipov, provisional designation 1981 RR3, is a stony Flora asteroid from the inner regions of the asteroid belt, approximately 4 kilometers in diameter. It was discovered by Soviet–Russian astronomer Nikolai Chernykh at the Crimean Astrophysical Observatory in Nauchnyj, on 3 September 1981.[7]
The S-type asteroid is a member of the Flora family, one of the largest groups of stony asteroids in the main-belt. It orbits the Sun at a distance of 1.8–2.7 AU once every 3 years and 4 months (1,221 days). Its orbit has an eccentricity of 0.21 and an inclination of 6° with respect to the ecliptic.[1] The first astrometric 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's observation arc.[7]
A rotational light-curve was obtained from photometric observations made by American astronomer Brian Skiff in October 2011. It gave a well-defined rotation period of 7.18±0.01 hours with a low brightness variation of 0.10 in magnitude (U=3).[lower-alpha 1] A low brightness amplitude typically indicates that the body has a nearly spheroidal shape.
According to the survey carried out by the NEOWISE mission of NASA's space-based Wide-field Infrared Survey Explorer, the asteroid measures 4.2 kilometers in diameter and its surface has an albedo of 0.279,[4][5] while the Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – which derives from 8 Flora, the largest member and namesake of this orbital family – and calculates a diameter of 3.9 kilometers, based on an absolute magnitude of 14.2.[3]
The minor planet was named in memory of astronomer Alexandr Kuzmich Osipov (1920–2004), observer of artificial satellites, the Moon, planets and comets at the Astronomical Observatory of Kyiv National University in Kiev, Ukraine. He is described as a skilled teacher for many generations of students.[2] Naming citation was published on 15 December 2005 (M.P.C. 55721).[8]
References
- 1 2 Skiff (2011) web: rotation period 7.18±0.01 hours with a brightness amplitude of 0.10 mag. Summary figures at Collaborative Asteroid Lightcurve Link (CALL) for (14335) Alexosipov
- 1 2 3 4 "JPL Small-Body Database Browser: 14335 Alexosipov (1981 RR3)" (2016-05-16 last obs.). Jet Propulsion Laboratory. Retrieved 3 December 2016.
- 1 2 Schmadel, Lutz D. (2006). Dictionary of Minor Planet Names – (14335) Alexosipov, Addendum to Fifth Edition: 2003–2005. Springer Berlin Heidelberg. p. 85. ISBN 978-3-540-34360-8. Retrieved 11 May 2016.
- 1 2 3 4 5 6 "LCDB Data for (14335) Alexosipov". Asteroid Lightcurve Database (LCDB). Retrieved 11 May 2016.
- 1 2 3 4 Mainzer, 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. Retrieved 11 May 2016. - 1 2 3 Masiero, 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. Retrieved 3 December 2016.
- 1 2 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. Retrieved 11 May 2016.
- 1 2 "14335 Alexosipov (1981 RR3)". Minor Planet Center. Retrieved 11 May 2016.
- ↑ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 11 May 2016.
External links
- Astronomical Observatory, Kyiv Shevchenko National University
- Asteroid Lightcurve Database (LCDB), query form (info)
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (10001)-(15000) – Minor Planet Center
- 14335 Alexosipov at the JPL Small-Body Database
