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386 Siegena

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Main-belt asteroid

386 Siegena
A three-dimensional model of 386 Siegena based on its light curve
Discovery
Discovered byMax Wolf
Discovery date1 March 1894
Designations
MPC designation(386) Siegena
Pronunciation/ˈsiːɡənə/ SEE-gə-nə
Named afterSiegen
Alternative designations1894 AY
Minor planet categoryMain belt
AdjectivesSiegenian /siːˈɡɛniən/ see-GHEN-ee-ən
Orbital characteristics
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc122.08 yr (44590 d)
Aphelion3.38983 AU (507.111 Gm)
Perihelion2.40159 AU (359.273 Gm)
Semi-major axis2.89571 AU (433.192 Gm)
Eccentricity0.17064
Orbital period (sidereal)4.93 yr (1799.8 d)
Mean anomaly66.7510°
Mean motion0° 12 0.068 / day
Inclination20.2568°
Longitude of ascending node166.886°
Argument of perihelion219.478°
Physical characteristics
Dimensions165.01±2.7 km
170.35 ± 8.40 km
Mass(8.14 ± 1.58) × 10 kg
Mean density3.14 ± 0.76 g/cm
Synodic rotation period9.763 h (0.4068 d)
Geometric albedo0.0692±0.002
Spectral typeC
Absolute magnitude (H)7.43

386 Siegena is a very large main-belt asteroid. It is classified as a C-type asteroid and is probably composed of primitive carbonaceous material.

It was discovered by Max Wolf on March 1, 1894, in Heidelberg.

During 1999, the asteroid was observed occulting a star. The resulting chords provided a diameter estimate of 174 km.

References

  1. per "siegenite". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)
  2. "Siegenian". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)
  3. ^ "386 Siegena (1894 AY)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 10 May 2016.
  4. ^ Carry, 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.
  5. Shevchenko, Vasilij G.; Tedesco, Edward F. (September 2006), "Asteroid albedos deduced from stellar occultations", Icarus, 184 (1): 211–220, Bibcode:2006Icar..184..211S, doi:10.1016/j.icarus.2006.04.006.

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