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210 Isabella

From Wikipedia, the free encyclopedia
Main-belt asteroid

210 Isabella
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
Main belt (Nemesis)
Orbital characteristics[2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc131.26 yr (47943 d)
Aphelion3.0567 AU (457.28 Gm)
Perihelion2.3892 AU (357.42 Gm)
2.7230 AU (407.36 Gm)
Eccentricity0.12257
4.493 yr (1,641.2 d)
18.05 km/s
153.338°
0° 13m 9.66s / day
Inclination5.2600°
32.582°
15.041°
Physical characteristics
Dimensions86.65±2.3 km[2]
73.70±8.47 km[3]
Mass(3.41±1.09)×1018 kg[3]
6.672 h (0.2780 d)
0.0436±0.002
CF
12.2 (peak)
9.33

210 Isabella is a large and darkasteroid from the centralasteroid belt, approximately 80 kilometers in diameter. It was discovered inPola byJohann Palisa on 12 November 1879. The origin of the name is unknown. It is orbiting at a distance of2.72 AU from theSun with aneccentricity of 0.12 and aperiod of 4.49 yr. Theorbital plane is inclined at an angle of 5.26° to theplane of the ecliptic.[2]

The asteroid is probably composed of material similar tocarbonaceouschondrites. It is classified as a member of theNemesis family of asteroids.[4] Estimates of the diameter range from 74[3] to 87 km.[2] It is spinning with a period of6.67 h.

References

[edit]
  1. ^"Isabella".Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription orparticipating institution membership required.)
  2. ^abcd"210 Isabella".JPL Small-Body Database.NASA/Jet Propulsion Laboratory. Retrieved12 May 2016.
  3. ^abcCarry, B. (December 2012), "Density of asteroids",Planetary and Space Science,73 (1):98–118,arXiv:1203.4336,Bibcode:2012P&SS...73...98C,doi:10.1016/j.pss.2012.03.009. 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.Bibcode:2012Icar..218..196D.doi:10.1016/j.icarus.2011.11.024.

External links

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