Astronomy:211 Isolda

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Short description: Main-belt asteroid
211 Isolda
Орбита астероида 211.png
Orbital diagram
Discovery
Discovered byJohann Palisa
Discovery date10 December 1879
Designations
(211) Isolda
Pronunciation/ɪˈzldə/[1]
Named afterIseult
A879 XA, 1912 AB
1912 BA, 1950 FM
Minor planet categoryMain belt
AdjectivesIsoldian /ɪˈzldiən/[2]
Orbital characteristics[3]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc136.19 yr (49742 d)
|{{{apsis}}}|helion}}3.53270 astronomical unit|AU (528.484 Gm)
|{{{apsis}}}|helion}}2.5514 AU (381.68 Gm)
3.04205 AU (455.084 Gm)
Eccentricity0.16129
Orbital period5.31 yr (1938.0 d)
Average Orbital speed17.08 km/s
Mean anomaly260.142°
Mean motion0° 11m 8.74s / day
Inclination3.8856°
Longitude of ascending node263.644°
173.522°
Physical characteristics
Dimensions143.19±5.1 km[3]
149.81 ± 6.10 km[4]
Mass(4.49 ± 2.43) × 1018 kg[4]
Mean density2.54 ± 1.41 g/cm3[4]
Rotation period18.365 h (0.7652 d)
Geometric albedo0.0602±0.004[3]
0.0598 ± 0.0218[5]
C[5] (Tholen)
Absolute magnitude (H)7.89,[3] 7.90[5]


Isolda (minor planet designation: 211 Isolda) is a very large, dark main-belt asteroid. It is classified as a C-type asteroid and is probably composed of primitive carbonaceous material. The spectra of the asteroid displays evidence of aqueous alteration.[6]

It was discovered by Austrian astronomer Johann Palisa on 10 December 1879, in Pola, and is possibly named after Isolde, heroine of the legend of Tristan and Iseult.[7]

In 2001, the asteroid was detected by radar from the Arecibo Observatory at a distance of 1.78 AU. The resulting data yielded an effective diameter of 143 ± 16 km.[8]

Between 2009 and 2022, 211 Isolda has been observed to occult seven stars.[citation needed]

References

  1. "Isolde". Isolde. Oxford University Press. http://www.lexico.com/definition/Isolde. 
  2. Irene Masing-Delic (1992) Abolishing Death: A Salvation Myth of Russian Twentieth-Century Literature, p. 163
  3. 3.0 3.1 3.2 3.3 "211 Isolda". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=211;cad=1. 
  4. 4.0 4.1 4.2 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.
  5. 5.0 5.1 5.2 Pravec, P. et al. (May 2012), "Absolute Magnitudes of Asteroids and a Revision of Asteroid Albedo Estimates from WISE Thermal Observations", Asteroids, Comets, Meteors 2012, Proceedings of the conference held May 16–20, 2012 in Niigata, Japan 1667 (1667): pp. 6089, Bibcode2012LPICo1667.6089P.  See Table 4.
  6. Fornasier, S. et al. (February 1999), "Spectroscopic comparison of aqueous altered asteroids with CM2 carbonaceous chondrite meteorites", Astronomy and Astrophysics Supplement 135: 65−73, doi:10.1051/aas:1999161, Bibcode1999A&AS..135...65F. 
  7. Schmadel, L. (2003:31). Dictionary of minor planet names. Germany: Springer.
  8. Magri, Christopher et al. (January 2007), "A radar survey of main-belt asteroids: Arecibo observations of 55 objects during 1999 2003", Icarus 186 (1): 126–151, doi:10.1016/j.icarus.2006.08.018, Bibcode2007Icar..186..126M, http://echo.jpl.nasa.gov/asteroids/MBAs/magri.etal.2007.mbas.pdf, retrieved 2015-04-14. 

External links