Discovery | |
---|---|
Discovered by | Farra d'Isonzo Obs. (inc. Luciano Bittesini) |
Discovery site | Farra d'Isonzo Obs. |
Discovery date | 30 March 1994 |
Designations | |
MPC designation | (8549) Alcide |
Named after | Alcide Bittesini (father of co-discoverer) |
Alternative designations | 1994 FS |
Minor planet category | main-belt · Nysa |
Orbital characteristics | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 23.31 yr (8,514 days) |
Aphelion | 2.8912 AU |
Perihelion | 1.9828 AU |
Semi-major axis | 2.4370 AU |
Eccentricity | 0.1864 |
Orbital period (sidereal) | 3.80 yr (1,390 days) |
Mean anomaly | 318.71° |
Mean motion | 0° 15 32.76 / day |
Inclination | 1.8790° |
Longitude of ascending node | 205.61° |
Argument of perihelion | 64.719° |
Physical characteristics | |
Dimensions | 4.19 km (calculated) 4.341±0.076 km |
Synodic rotation period | 3 h |
Geometric albedo | 0.196±0.012 0.21 (assumed) |
Spectral type | S |
Absolute magnitude (H) | 14.2 · 14.3±0.4 (R) · 14.73±0.25 |
8549 Alcide, provisional designation 1994 FS, is a stony Nysa asteroid from the inner regions of the asteroid belt, approximately 4.2 kilometers in diameter. It was discovered on 30 March 1994, by a group of amateur astronomers at the Farra d'Isonzo Observatory, Italy, near the border to Slovenia. It was named for Alcide Bittesini, father of co-discoverer Luciano Bittesini.
Orbit and classification
Alcide is a member of the stony subgroup of the Nysa family, one of the smaller families in the main-belt, named after its namesake, 44 Nysa. The body orbits the Sun in the inner main-belt at a distance of 2.0–2.9 AU once every 3 years and 10 months (1,390 days). Its orbit has an eccentricity of 0.19 and an inclination of 2° with respect to the ecliptic. Precoveries were taken at Palomar and Steward Observatory (Kitt Peak) just weeks and days prior to the asteroid's official discovery observation at Farra d'Isonzo.
Physical characteristics
Lightcurves
A rotational lightcurve of Alcide was obtained from photometric observations made by astronomer David Polishook at the ground-based Wise Observatory, Israel, in November 2007. The lightcurve gave a rotation period of 3 hours with a brightness amplitude of 0.2 magnitude (U=2-).
Diameter and albedo
According to the survey carried out by the NEOWISE mission of NASA's space-based Wide-field Infrared Survey Explorer, Alcide measures 4.3 kilometers in diameter and its surface has an albedo of 0.195, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.21 and calculates a diameter of 4.2 kilometers with an absolute magnitude of 14.2.
Naming
This minor planet was named for Italian high-school teacher of natural sciences, Alcide Bittesini (1913–1981). He was the father of amateur astronomer Luciano Bittesini, who co-discovered the asteroid with his amateur colleagues at the Farra d'Isonzo Observatory in Italy.
At the age of 9, his father fostered his interest in astronomy, when they observed a comet with a homespun telescope made of a pair of glasses, a tin can and a microscope eyepiece. The official naming citation was published by the Minor Planet Center on 2 February 1999 (M.P.C. 33791).
References
- ^ "JPL Small-Body Database Browser: 8549 Alcide (1994 FS)" (2017-06-05 last obs.). Jet Propulsion Laboratory. Archived from the original on 19 September 2020. Retrieved 22 June 2017.
- ^ Schmadel, Lutz D. (2007). "(8549) Alcide". Dictionary of Minor Planet Names – (8549) Alcide. Springer Berlin Heidelberg. pp. 654–655. doi:10.1007/978-3-540-29925-7_7079. ISBN 978-3-540-00238-3.
- ^ "LCDB Data for (8549) Alcide". Asteroid Lightcurve Database (LCDB). Retrieved 7 May 2016.
- ^ 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 7 May 2016.
- ^ 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 4 December 2016.
- ^ Polishook, D.; Brosch, N. (February 2009). "Photometry and spin rate distribution of small-sized main belt asteroids". Icarus. 199 (2): 319–332. arXiv:0811.1223. Bibcode:2009Icar..199..319P. doi:10.1016/j.icarus.2008.10.020. Retrieved 7 May 2016.
- 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 7 May 2016.
- ^ "8549 Alcide (1994 FS)". Minor Planet Center. Retrieved 7 May 2016.
- "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 7 May 2016.
External links
- Asteroid Lightcurve Database (LCDB), query form (info Archived 16 December 2017 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 (5001)-(10000) – Minor Planet Center
- 8549 Alcide at AstDyS-2, Asteroids—Dynamic Site
- 8549 Alcide at the JPL Small-Body Database
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