6708 Bobbievaile
Discovery [1] | |
---|---|
Discovered by | R. H. McNaught |
Discovery site | Siding Spring Obs. |
Discovery date | 4 January 1989 |
Designations | |
MPC designation | (6708) Bobbievaile |
Named after |
Bobbie Vaile (astrophysicist)[2] |
1989 AA5 · 1979 PF 1989 CM9 · 1994 LB | |
main-belt · (inner)[3] | |
Orbital characteristics [1] | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 37.81 yr (13,811 days) |
Aphelion | 2.8864 AU |
Perihelion | 2.0045 AU |
2.4455 AU | |
Eccentricity | 0.1803 |
3.82 yr (1,397 days) | |
349.25° | |
0° 15m 27.72s / day | |
Inclination | 12.076° |
115.81° | |
193.50° | |
Known satellites | 1 (period: 24.7 h)[4][3] |
Physical characteristics | |
Dimensions | ±0.176 km 8.074[5] |
±0.0004 12.3415h[3] | |
±0.016 0.169[5] | |
S [3] | |
13.1[1] | |
|
6708 Bobbievaile, provisional designation 1989 AA5, is a stony asteroid and asynchronous binary system from the inner regions of the asteroid belt, approximately 8 kilometers in diameter. It was discovered on 4 January 1989, by Australian astronomer Robert McNaught at the Siding Spring Observatory in New South Wales, Australia.[6] It is named after Bobbie Vaile.[2]
Orbit and classification
Bobbievaile is a stony S-type asteroid and orbits the Sun in the inner main-belt at a distance of 2.0–2.9 AU once every 3 years and 10 months (1,397 days). Its orbit has an eccentricity of 0.18 and an inclination of 12° with respect to the ecliptic.[1]
It was first identified as 1979 PF at El Leoncito in 1979, extending the body's observation arc by 10 years prior to its official discovery observation at Siding Spring.[6]
Binary asteroid
On 7 May 2009, it was announced that Bobbievaile was determined to be a binary asteroid based on a series of lightcurve observations. Bobbievaile (the primary) is estimated to have a diameter of ±0.02 km, and its 8.02minor-planet moon (the secondary) to have a diameter of approximately 4.57 km.[7] The primary is probably spherical.
Naming
This minor planet was named in memory of Australian astrophysicist Roberta Anne "Bobbie" Vaile (1959–1996), lecturer at Western Sydney University. She was a SETI enthusiast and participated in both the establishment of the SETI Australia Centre and the conduction of Project Phoenix.[2] The official naming citation was published by the Minor Planet Center on 22 April 1997 (M.P.C. 29671).[8]
References
- 1 2 3 4 "JPL Small-Body Database Browser: 6708 Bobbievaile (1989 AA5)" (2017-06-06 last obs.). Jet Propulsion Laboratory. Retrieved 21 June 2017.
- 1 2 3 Schmadel, Lutz D. (2007). Dictionary of Minor Planet Names – (6708) Bobbievaile. Springer Berlin Heidelberg. p. 551. ISBN 978-3-540-00238-3. Retrieved 13 March 2017.
- 1 2 3 4 "LCDB Data for (6708) Bobbievaile". Asteroid Lightcurve Database (LCDB). Retrieved 13 March 2017.
- ↑ Johnston, Robert. "(6708) Bobbievaile". johnstonsarchive.net. Retrieved 29 May 2015.
- 1 2 Masiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos". The Astrophysical Journal. 791 (2): 11. Bibcode:2014ApJ...791..121M. arXiv:1406.6645 . doi:10.1088/0004-637X/791/2/121. Retrieved 13 March 2017.
- 1 2 "6708 Bobbievaile (1989 AA5)". Minor Planet Center. Retrieved 13 March 2017.
- ↑
- ↑ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 13 March 2017.
External links
- Simostronomy—The Remarkable Bobbie Vaile
- (6708) Bobbievaile, datasheet, johnstonsarchive.net
- Asteroids with Satellites, Robert Johnston, johnstonsarchive.net
- 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 (5001)-(10000) – Minor Planet Center
- 6708 Bobbievaile at the JPL Small-Body Database