10551 Göteborg

10551 Göteborg
Discovery [1]
Discovered by E. W. Elst
Discovery site Caussols Obs. (010)
Discovery date 18 December 1992
Designations
MPC designation 10551 Göteborg
Named after
 Göteborg (Swedish city)[2]
1992 YL2 · 1931 AK
1994 EB3
main-belt · Eos [3]
Orbital characteristics [1]
Epoch 16 February 2017 (JD 2457800.5)
Uncertainty parameter 0
Observation arc 85.42 yr (31,198 days)
Aphelion 3.1822 AU
Perihelion 2.8039 AU
2.9931 AU
Eccentricity 0.0632
5.18 yr (1,891 days)
233.55°
0° 11m 25.08s / day
Inclination 11.382°
93.075°
8.5929°
Physical characteristics
Dimensions 11.53 km (calculated)[3]
15.491±0.101 km[4]
15.689±0.128[5]
335.3458±4.6612 h[6]
0.084±0.010[5]
0.1169±0.0139[4]
0.14 (assumed)[3]
S [3]
11.993±0.005 (R)[6] · 12.0[4] · 12.03±0.33[7] · 12.1[1] · 12.44[3]

    10551 Göteborg, provisional designation 1992 YL2, is a stony Eos asteroid and slow rotator from the outer region of the asteroid belt, about 13 kilometers in diameter. It was discovered on 18 December 1992, by Belgian astronomer Eric Elst at Caussols Observatory in southeastern France.[8]

    The S-type asteroid is a member of the Eos family, an orbital group of more than 4,000 asteroids, which are well known for mostly being of stony composition with a relatively high albedo. It orbits the Sun at a distance of 2.8–3.2 AU once every 5 years and 2 months (1,891 days). Its orbit has an eccentricity of 0.06 and an inclination of 11° with respect to the ecliptic.[1] The first precovery taken at the U.S. Lowell Observatory in 1931, extending the asteroid's observation arc by 61 years prior to its discovery.[8]

    In September 2012, photometric observations at the U.S. Palomar Transient Factory, California, rendered an rotational light-curve that showed a period of 335.3458±4.6612 hours, or 14 days, with a brightness amplitude of 0.70 in magnitude (U=2).[6] A body of this size usually rotates within hours once around its axis. According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, the asteroid measures 15.5 and 15.7 kilometers in diameter and its surface has an albedo of 0.08 and 0.12, respectively,[4] while the Collaborative Asteroid Lightcurve Link assumes an albedo of 0.14 and calculates a diameter of 11.5 kilometers.[3]

    The minor planet is named after Sweden's second-largest city and the largest port in the Nordic countries, Göteborg (Gothenburg), located on the country's southwest coast. Founded in the early 17th century and heavily influenced by the Dutch, the city still has its typical canal system. Later, the Swedes acquired political power over Gothenburg and the city flourished with the development of the Swedish East India Company in the early 18th century.[2] Naming citation was published on 20 March 2000 (M.P.C. 39655).[9]

    References

    1. 1 2 3 4 "JPL Small-Body Database Browser: 10551 Goteborg (1992 YL2)" (2016-06-10 last obs.). Jet Propulsion Laboratory. Retrieved 4 December 2016.
    2. 1 2 Schmadel, Lutz D. (2007). Dictionary of Minor Planet Names – (10551) Göteborg. Springer Berlin Heidelberg. p. 737. ISBN 978-3-540-00238-3. Retrieved 12 April 2016.
    3. 1 2 3 4 5 6 "LCDB Data for (10551) Goteborg". Asteroid Lightcurve Database (LCDB). Retrieved 17 May 2016.
    4. 1 2 3 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:1109.6407Freely accessible. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. Retrieved 17 May 2016.
    5. 1 2 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:1109.4096Freely accessible. Bibcode:2011ApJ...741...68M. doi:10.1088/0004-637X/741/2/68. Retrieved 4 December 2016.
    6. 1 2 3 Waszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015). "Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry". The Astronomical Journal. 150 (3): 35. arXiv:1504.04041Freely accessible. Bibcode:2015AJ....150...75W. doi:10.1088/0004-6256/150/3/75. Retrieved 17 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:1506.00762Freely accessible. Bibcode:2015Icar..261...34V. doi:10.1016/j.icarus.2015.08.007. Retrieved 17 May 2016.
    8. 1 2 "10551 Goteborg (1992 YL2)". Minor Planet Center. Retrieved 12 April 2016.
    9. ↑ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 17 May 2016.

    External links

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