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10208 Germanicus

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10208 Germanicus
Discovery [1]
Discovered byA. Vagnozzi
Discovery siteSanta Lucia Obs.
Discovery date30 August 1997
Designations
(10208) Germanicus
Named after
Germanicus
(Ancient Roman general)[2]
1997 QN1 · 1987 QJ7
1994 WP12
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 16 February 2017 (JD 2457800.5)
Uncertainty parameter 0
Observation arc28.69 yr (10,478 days)
Aphelion2.6847 AU
Perihelion1.7861 AU
2.2354 AU
Eccentricity0.2010
3.34 yr (1,221 days)
292.13°
0° 17m 41.64s / day
Inclination4.5618°
223.63°
115.00°
Earth MOID0.7837 AU
Physical characteristics
Dimensions2.87±0.62 km[4]
3.50 km (taken)[3]
3.503 km[5]
3.552±0.202 km[6][7]
3.1291±0.0002 h[8]
3.3484±0.0001 h[9]
3.3493±0.0006 h[a]
0.1747[5]
0.267±0.027[6][7]
0.36±0.19[4]
S[3]
14.2±0.2 (R)[9] · 14.3[6] · 14.40[4] · 14.5[1] · 14.79±0.139[3][5]

10208 Germanicus, provisional designation 1997 QN1, is a stony binary[10] asteroid from the inner regions of the asteroid belt, approximately 4 kilometers in diameter. It was discovered on 30 August 1997, at the Santa Lucia Stroncone Astronomical Observatory in Stroncone, Italy, and named for Germanicus, an ancient Roman general and nephew of Tiberius.[2] A moon orbits the asteroid with an orbital period of 2 days, 10 hours, and 48 minutes.[10]

Germanicus orbits the Sun at a distance of 1.8–2.7 AU once every 3 years and 4 months (1,221 days). Its orbit has an eccentricity of 0.20 and an inclination of 5° with respect to the ecliptic.[1]

Notes

  1. ^ Pravec (2007) web: rotation period 3.3493±0.0006 hours with a brightness amplitude of 0.12 mag. Summary figures at Collaborative Asteroid Lightcurve Link (CALL) for (10208) Germanicus

References

  1. ^ a b c d "JPL Small-Body Database Browser: 10208 Germanicus (1997 QN1)" (2016-05-03 last obs.). Jet Propulsion Laboratory. Retrieved 31 March 2017.
  2. ^ a b "10208 Germanicus (1997 QN1)". Minor Planet Center. Retrieved 31 March 2017.
  3. ^ a b c d "LCDB Data for (10208) Germanicus". Asteroid Lightcurve Database (LCDB). Retrieved 31 March 2017.
  4. ^ a b c Nugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015). "NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos". The Astrophysical Journal. 814 (2): 13. arXiv:1509.02522. Bibcode:2015ApJ...814..117N. doi:10.1088/0004-637X/814/2/117. Retrieved 31 March 2017.
  5. ^ a b c Pravec, Petr; Harris, Alan W.; Kusnirák, Peter; Galád, Adrián; Hornoch, Kamil (September 2012). "Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations". Icarus. 221 (1): 365–387. Bibcode:2012Icar..221..365P. doi:10.1016/j.icarus.2012.07.026. Retrieved 31 March 2017.
  6. ^ a b c Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results" (PDF). The Astrophysical Journal. 741 (2): 25. arXiv:1109.6407. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. Retrieved 31 March 2017.
  7. ^ a b 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 31 March 2017.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  8. ^ Oey, Julian (January 2016). "Lightcurve Analysis of Asteroids from Blue Mountains Observatory in 2014". The Minor Planet Bulletin. 43 (1): 45–51. Bibcode:2016MPBu...43...45O. ISSN 1052-8091. Retrieved 31 March 2017.
  9. ^ a b Oey, J.; Pravec, P.; Kusnirak, P.; Krugly, Yu.; Chiorny, V.; Ries, J. (September 2007). "(10208) 1997 QN1". Central Bureau Electronic Telegrams (1087). Bibcode:2007CBET.1087....1O. Retrieved 31 March 2017.
  10. ^ a b Johnston, Robert (21 September 2016). "(10208) Germanicus". johnstonsarchive.net. Retrieved 31 March 2017.