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8549 Alcide

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8549 Alcide
Discovery 
Discovered byFarra d'Isonzo Obs.
(inc. Luciano Bittesini)
Discovery siteFarra d'Isonzo Obs.
Discovery date30 March 1994
Designations
MPC designation(8549) Alcide
Named afterAlcide Bittesini
(father of co-discoverer)
Alternative designations1994 FS
Minor planet categorymain-belt · Nysa
Orbital characteristics
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc23.31 yr (8,514 days)
Aphelion2.8912 AU
Perihelion1.9828 AU
Semi-major axis2.4370 AU
Eccentricity0.1864
Orbital period (sidereal)3.80 yr (1,390 days)
Mean anomaly318.71°
Mean motion0° 15 32.76 / day
Inclination1.8790°
Longitude of ascending node205.61°
Argument of perihelion64.719°
Physical characteristics
Dimensions4.19 km (calculated)
4.341±0.076 km
Synodic rotation period3 h
Geometric albedo0.196±0.012
0.21 (assumed)
Spectral typeS
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

  1. ^ "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.
  2. ^ 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.
  3. ^ "LCDB Data for (8549) Alcide". Asteroid Lightcurve Database (LCDB). Retrieved 7 May 2016.
  4. ^ 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.
  5. ^ 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.
  6. ^ 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.
  7. 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.
  8. ^ "8549 Alcide (1994 FS)". Minor Planet Center. Retrieved 7 May 2016.
  9. "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 7 May 2016.

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