14335 Alexosipov
| Discovery [1] | |
|---|---|
| Discovered by | N. Chernykh |
| Discovery site | CrAO (Nauchnyj) |
| Discovery date | 3 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 13 January 2016 (JD 2457400.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 16240 days (44.46 yr) |
| Aphelion | 2.7047 AU (404.62 Gm) |
| Perihelion | 1.7643 AU (263.94 Gm) |
| 2.2345 AU (334.28 Gm) | |
| Eccentricity | 0.21043 |
| 3.34 yr (1220.0 d) | |
| 106.52° | |
| 0° 17m 42.288s / day | |
| Inclination | 5.9019° |
| 170.14° | |
| 181.53° | |
| Earth MOID | 0.756694 AU (113.1998 Gm) |
| Jupiter MOID | 2.71992 AU (406.894 Gm) |
| TJupiter | 3.603 |
| Physical characteristics | |
| Dimensions | 4.176±0.101 km[4] 4.11 km (caculated)[3] |
| 7.18±0.01 h[a] | |
| 0.2790±0.0323[4] 0.24 (assumed)[3] | |
| S [3] | |
| 14.2[1] | |
14335 Alexosipov, provisional designation 1981 RR3, is a stony asteroid from the inner regions of the asteroid belt, about yzx kilometers in diameter. It was discovered by Soviet–Russian astronomer Nikolai Chernykh at the Crimean Astrophysical Observatory in Nauchnyj, on 3 September 1981.[2]
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 (1,220 days). Its orbit shows an eccentricity of 0.21 and is tilted by 6 degrees to the plane of the ecliptic. It has a rotation period of 7.2 hours[a] and an albedo of 0.28, according to the NEOWISE mission of the Wide-field Infrared Survey Explorer, while the Collaborative Asteroid Lightcurve Link (CALL) assumes a somewhat more moderate albedo of 0.24, typical for asteroids with a stony surface composition.[3][4]
The minor planet was named in memory of Alexandr Kuzmich Osipov (1920–2004) at the Astronomical Observatory of Kyiv National University, who was a talented teacher for many generations of students. His work included observations of artificial satellites and studies of the Moon, planets and comets.[2]
References
- ^ a b 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
- ^ a b c "JPL Small-Body Database Browser: 14335 Alexosipov (1981 RR3)" (2015-11-14 last obs.). Jet Propulsion Laboratory. Retrieved 9 April 2016.
- ^ a b c "14335 Alexosipov (1981 RR3)". Minor Planet Center. Retrieved December 2015.
{{cite web}}: Check date values in:|accessdate=(help) - ^ a b c d e "LCDB Data for (14335) Alexosipov". Asteroid Lightcurve Database (LCDB). Retrieved December 2015.
{{cite web}}: Check date values in:|accessdate=(help) - ^ a b c Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; 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 December 2015.
{{cite journal}}: Check date values in:|access-date=(help)
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
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