10258 Sárneczky
| Discovery[1] | |
|---|---|
| Discovered by | G. Kulin |
| Discovery site | Konkoly Obs. |
| Discovery date | 6 January 1940 |
| Designations | |
| (10258) Sárneczky | |
Named after | Krisztián Sárneczky[2] (Hungarian astronomer) |
| 1940 AB · 1988 RZ4 1989 WK7 · 1989 WL6 1998 KD53 | |
| main-belt · (outer) background[3] | |
| Orbital characteristics[1] | |
| Epoch 4 September 2017 (JD 2458000.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 77.74 yr (28,393 days) |
| Aphelion | 3.4567 AU |
| Perihelion | 2.8649 AU |
| 3.1608 AU | |
| Eccentricity | 0.0936 |
| 5.62 yr (2,053 days) | |
| 339.90° | |
| 0° 10m 31.44s / day | |
| Inclination | 14.192° |
| 128.78° | |
| 291.32° | |
| Physical characteristics | |
| Dimensions | 14.275±0.264 km[4] |
| 0.151±0.026[4] | |
| 12.1[1] | |
10258 Sárneczky, provisional designation 1940 AB, is a background asteroid from the outer regions of the asteroid belt, approximately 14 kilometers in diameter. It was discovered on 6 January 1940, by Hungarian astronomer György Kulin at the Konkoly Observatory, near Budapest.[2] The asteroid was named after Hungarian astronomer Krisztián Sárneczky.[2]
Orbit and classification
[edit]Sárneczky is non-family asteroid from the main-belt's background population.[3] It orbits the Sun in the outer asteroid belt at a distance of 2.9–3.5 AU once every 5 years and 7 months (2,053 days). Its orbit has an eccentricity of 0.09 and an inclination of 14° with respect to the ecliptic.[1] The body's observation arc begins with its official discovery observation at Konkoly in 1940.[2]
Physical characteristics
[edit]Diameter and albedo
[edit]According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Sárneczky measures 14.275 kilometers in diameter and its surface has an albedo of 0.151.[4] The asteroid has an absolute magnitude of 12.1.[1]
Rotation period
[edit]As of 2017, no rotational lightcurve of Sárneczky has been obtained from photometric observations. The body's rotation period, shape and poles remain unknown.[5]
Naming
[edit]This minor planet was named after Krisztián Sárneczky (born 1974), a Hungarian amateur astronomer and discoverer of minor planets and supernovae. He is a board member of the Hungarian Astronomical Association (HAA).[2] The official naming citation was published by the Minor Planet Center on 5 October 2017 (M.P.C. 106499).[6]
References
[edit]- ^ a b c d e "JPL Small-Body Database Browser: 10258 Sarneczky (1940 AB)" (2017-10-01 last obs.). Jet Propulsion Laboratory. Retrieved 11 October 2017.
- ^ a b c d e "10258 Sarneczky (1940 AB)". Minor Planet Center. Retrieved 11 October 2017.
- ^ a b "Asteroid 10258 Sarneczky – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved 29 October 2019.
- ^ a b c 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 11 October 2017.
- ^ "LCDB Data for (10258) Sárneczky". Asteroid Lightcurve Database (LCDB). Retrieved 11 October 2017.
- ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 11 October 2017.
External links
[edit]- Asteroid Lightcurve Database (LCDB), query form (info Archived 2017-12-16 at the Wayback Machine)
- 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
- 10258 Sárneczky at the JPL Small-Body Database
