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654 Zelinda

From Wikipedia, the free encyclopedia
Asteroid in Virgo Cluster

654 Zelinda
Discovery
Discovered byAugust Kopff
Discovery siteHeidelberg
Discovery date4 January 1908
Designations
(654) Zelinda
1908 BM
Orbital characteristics[1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc108.29 yr (39553 d)
Aphelion2.8288 AU (423.18 Gm)
Perihelion1.7653 AU (264.09 Gm)
2.2970 AU (343.63 Gm)
Eccentricity0.23150
1,271.6 d (3.48 yr)
51.9052°
0° 16m 59.196s / day
Inclination18.125°
278.460°
214.008°
Physical characteristics
63.70±1.95 km[1]
63.915±2.615 km[2]
Mass(1.35±0.14)×1018 kg[2]
1.23±0.19 g/cm3[2]
31.735 h (1.3223 d)
0.0425±0.003
8.52

654 Zelinda is aminor planet orbiting theSun that was discovered on 4 January 1908 by German astronomerAugust Kopff. It is orbiting the Sun at a distance of2.297 AU with anorbital eccentricity of 0.23 and aperiod of 3.48 yr.[1] Theorbital plane isinclined at an angle of 18.1° to theplane of the ecliptic. On favorable oppositions, it can be as bright as magnitude 10.0, as observed on January 30, 2016.

In 1988, this object was detected withradar from theArecibo Observatory at a distance of 0.89AU. The measuredradar cross-section was 2,200 km2.[3] Measurements made using theadaptive optics system at theW. M. Keck Observatory give a diameter estimate of 131 km. This is 13% smaller than the diameter estimated from theIRAS observatory measurements. It is roughly triangular in shape,[4] and spins with asynodic rotation period of31.735 h.

References

[edit]
  1. ^abc"654 Zelinda (1908 BM)".JPL Small-Body Database.NASA/Jet Propulsion Laboratory. Retrieved7 May 2016.
  2. ^abcCarry, B. (December 2012), "Density of asteroids",Planetary and Space Science, vol. 73, pp. 98–118,arXiv:1203.4336,Bibcode:2012P&SS...73...98C,doi:10.1016/j.pss.2012.03.009. See Table 1.
  3. ^Ostro, S. J.; et al. (October 1991), "Asteroid radar astrometry",Astronomical Journal, vol. 102, pp. 1490–1502,Bibcode:1991AJ....102.1490O,doi:10.1086/115975.
  4. ^Marchis, F.; et al. (November 2006),"Shape, size and multiplicity of main-belt asteroids. I. Keck Adaptive Optics survey",Icarus, vol. 185, no. 1, pp. 39–63,Bibcode:2006Icar..185...39M,doi:10.1016/j.icarus.2006.06.001,PMC 2600456,PMID 19081813, retrieved27 March 2013.

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