210 Isabella

210 Isabella
3D convex shape model of 210 Isabella
Discovery
Discovered byJohann Palisa
Discovery date12 November 1879
Designations
Pronunciation/ɪzəˈbɛlə/
A879 VA, 1953 EZ1
1962 BF
Main belt (Nemesis)
Orbital characteristics
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
73.70±8.47 km (composite estimate)
Mass(4.5±1.9)×1017 kg
Mean density
1.33 g/cm3
6.672 h (0.2780 d)
0.0436±0.002
CF
12.2 (peak)
9.33

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. It is orbiting at a distance of 2.72 AU from the Sun with an eccentricity of 0.12 and a period of 4.49 yr. The orbital plane is inclined at an angle of 5.26° to the plane of the ecliptic.

The asteroid is probably composed of material similar to carbonaceous chondrites. It is classified as a member of the Nemesis family of asteroids. Estimates of the diameter range from 74 to 87 km. It is spinning with a period of 6.67 h.

Notes

  1. ↑ Calculated from its standard gravitational parameter GM = 0.030±0.013 km3/s2.
  2. ↑ Assuming a diameter of 86.7 km.

References

  1. ↑ "Isabella". Oxford English Dictionary (online ed.). Oxford University Press. (Subscription or participating institution membership required.)
  2. 1 2 3 4 "210 Isabella". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 12 May 2016.
  3. 1 2 Carry, 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. 1 2 Fuentes-Muñoz, Oscar; Farnocchia, Davide; Giorgini, Jon D.; Park, Ryan S. (1 December 2025). "Asteroid Mass Estimation by Mutual Perturbations During Close Encounters After Gaia Focused Product Release". The Astronomical Journal. 170 (6): 353. Bibcode:2025AJ....170..353F. doi:10.3847/1538-3881/ae0cc9. ISSN 0004-6256. S2CID 283347135.
  5. ↑ 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.