3174 Alcock (prov. designation: 1984 UV) is a carbonaceous Themistian asteroid from the outer region of the asteroid belt. It was discovered by American astronomer Edward Bowell at Lowell's U.S. Anderson Mesa Station in Flagstaff, Arizona, on 26 October 1984.[6] The likely C-type asteroid has a rotation period of 7.1 hours and measures approximately 19 kilometers (12 miles) in diameter. It was named after British amateur astronomer George Alcock (1912–2000).
_Alcock.png) Shape model of Alcock from its lightcurve | |
| Discovery [1] | |
|---|---|
| Discovered by | E. Bowell |
| Discovery site | Anderson Mesa Stn. |
| Discovery date | 26 October 1984 |
| Designations | |
| (3174) Alcock | |
Named after | George Alcock (amateur astronomer)[2] |
| 1984 UV · 1962 YD 1969 BB · 1973 YO1 1975 EO3 · 1978 RB1 1978 TJ3 · 1979 YR8 1980 AH · 1981 GF | |
| main-belt · Themis [3] | |
| Orbital characteristics [1] | |
| Epoch 4 September 2017 (JD 2458000.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 47.71 yr (17,426 days) |
| Aphelion | 3.6932 |
| Perihelion | 2.5991 |
| 3.1462 | |
| Eccentricity | 0.1739 |
| 5.58 yr (2,038 days) | |
| 296.20° | |
| 0° 10m 35.76s / day | |
| Inclination | 2.3715° |
| 72.244° | |
| 4.6082° | |
| Physical characteristics | |
| 18.66±0.80 km[4] 18.71 km (calculated)[3] | |
| 7.05±0.01 h[5] | |
| 0.08 (assumed)[3] 0.102±0.009[4] | |
| C (assumed)[3] | |
| 12.0[1][3] · 11.80[4] | |
Orbit and classification
editThe dark C-type asteroid is a member of the Themis family, a dynamical family of outer-belt asteroids with nearly coplanar ecliptical orbits. It orbits the Sun in the outer main-belt at a distance of 2.6–3.7
Naming
editThis minor planet was named by the discoverer for prolific British amateur astronomer George Alcock (1912–2000), who visually discovered 5 comets and 4 novae.[2] The naming was published by the Minor Planet Center on 5 November 1987 (M.P.C. 12458).[7]
Physical characteristics
editA rotational lightcurve of this asteroid was obtained from photometric observations made by French astronomer René Roy in February 2008. The lightcurve gave a rotation period of 7.05±0.01 hours with a brightness variation of 0.65 in magnitude (U=3-).[5]
According to the spaced-based survey carried out by the Japanese Akari satellite, the asteroid measures 18.66 kilometers in diameter and its surface has an albedo of 0.102,[4] while the Collaborative Asteroid Lightcurve Link assumes an albedo of 0.08 and calculates a diameter of 18.71 kilometers.[3]
References
edit- ^ a b c d "JPL Small-Body Database Browser: 3174 Alcock (1984 UV)" (2016-10-06 last obs.). Jet Propulsion Laboratory. Retrieved 16 June 2017.
- ^ a b Schmadel, Lutz D. (2007). "(3174) Alcock". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 263. doi:10.1007/978-3-540-29925-7_3175. ISBN 978-3-540-00238-3.
- ^ a b c d e f "LCDB Data for (3174) Alcock". Asteroid Lightcurve Database (LCDB). Retrieved 7 May 2016.
- ^ a b c d Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey". Publications of the Astronomical Society of Japan. 63 (5): 1117–1138. Bibcode:2011PASJ...63.1117U. doi:10.1093/pasj/63.5.1117. (online, AcuA catalog p. 153)
- ^ a b Behrend, Raoul. "Asteroids and comets rotation curves – (3174) Alcock". Geneva Observatory. Retrieved 7 May 2016.
- ^ a b "3174 Alcock (1984 UV)". Minor Planet Center. Retrieved 7 May 2016.
- ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 7 May 2016.
External links
edit- Lightcurve Database Query (LCDB), at www.minorplanet.info
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Geneva Observatory, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- 3174 Alcock at AstDyS-2, Asteroids—Dynamic Site
- 3174 Alcock at the JPL Small-Body Database
