Astronomy:210 Isabella

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Short description: Main-belt asteroid
210 Isabella
000210-asteroid shape model (210) Isabella.png
3D convex shape model of 210 Isabella
Discovery
Discovered byJohann Palisa
Discovery date12 November 1879
Designations
(210) Isabella
Pronunciation/ɪzəˈbɛlə/[1]
A879 VA, 1953 EZ1
1962 BF
Minor planet categoryMain belt (Nemesis)
Orbital characteristics[2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc131.26 yr (47943 d)
|{{{apsis}}}|helion}}3.0567 astronomical unit|AU (457.28 Gm)
|{{{apsis}}}|helion}}2.3892 AU (357.42 Gm)
2.7230 AU (407.36 Gm)
Eccentricity0.12257
Orbital period4.49 yr (1641.2 d)
Average Orbital speed18.05 km/s
Mean anomaly153.338°
Mean motion0° 13m 9.66s / day
Inclination5.2600°
Longitude of ascending node32.582°
15.041°
Physical characteristics
Dimensions86.65±2.3 km[2]
73.70 ± 8.47 km[3]
Mass(3.41 ± 1.09) × 1018 kg[3]
Rotation period6.672 h (0.2780 d)
Geometric albedo0.0436±0.002
CF
Apparent magnitude12.2 (peak)
Absolute magnitude (H)9.33


Isabella (minor planet designation: 210 Isabella) is a large and dark asteroid from the central asteroid belt, approximately 80 kilometers in diameter. It was discovered in Pola by Johann Palisa on 12 November 1879. The origin of the name is unknown. The asteroid is probably composed of material similar to carbonaceous chondrites. It is classified as a member of the Nemesis family of asteroids.[4]

References

  1. Isabella (3rd ed.), Oxford University Press, September 2005, http://oed.com/search?searchType=dictionary&q=Isabella  (Subscription or UK public library membership required.)
  2. 2.0 2.1 "210 Isabella". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=210;cad=1. 
  3. 3.0 3.1 Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science 73 (1): 98–118, doi:10.1016/j.pss.2012.03.009, Bibcode2012P&SS...73...98C.  See Table 1.
  4. De León, J.; Pinilla-Alonso, N.; Campins, H.; Licandro, J.; Marzo, G.A. (2012). "Near-infrared spectroscopic survey of B-type asteroids: Compositional analysis". Icarus 218 (1): 196–206. doi:10.1016/j.icarus.2011.11.024. Bibcode2012Icar..218..196D. https://www.researchgate.net/publication/260096891. 

External links