Astronomy:386 Siegena

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Short description: Main-belt asteroid
386 Siegena
386Siegena (Lightcurve Inversion).png
A three-dimensional model of 386 Siegena based on its light curve
Discovery
Discovered byMax Wolf
Discovery date1 March 1894
Designations
(386) Siegena
Pronunciation/ˈsɡənə/ SEE-gə-nə[1]
Named afterSiegen
1894 AY
Minor planet categoryMain belt
AdjectivesSiegenian /sˈɡɛniən/ see-GHEN-ee-ən[2]
Orbital characteristics[3]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc122.08 yr (44590 d)
|{{{apsis}}}|helion}}3.38983 astronomical unit|AU (507.111 Gm)
|{{{apsis}}}|helion}}2.40159 AU (359.273 Gm)
2.89571 AU (433.192 Gm)
Eccentricity0.17064
Orbital period4.93 yr (1799.8 d)
Mean anomaly66.7510°
Mean motion0° 12m 0.068s / day
Inclination20.2568°
Longitude of ascending node166.886°
219.478°
Physical characteristics
Dimensions165.01±2.7 km[3]
170.35 ± 8.40 km[4]
Mass(8.14 ± 1.58) × 1018 kg[4]
Mean density3.14 ± 0.76 g/cm3[4]
Rotation period9.763 h (0.4068 d)
Geometric albedo0.0692±0.002
C
Absolute magnitude (H)7.43


Siegena (minor planet designation: 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.[5]

References

  1. per siegenite (3rd ed.), Oxford University Press, September 2005, http://oed.com/search?searchType=dictionary&q=siegenite  (Subscription or UK public library membership required.)
  2. Siegenian (3rd ed.), Oxford University Press, September 2005, http://oed.com/search?searchType=dictionary&q=Siegenian  (Subscription or UK public library membership required.)
  3. 3.0 3.1 "386 Siegena (1894 AY)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=386;cad=1. 
  4. 4.0 4.1 4.2 Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science 73: pp. 98–118, doi:10.1016/j.pss.2012.03.009, Bibcode2012P&SS...73...98C.  See Table 1.
  5. Shevchenko, Vasilij G.; Tedesco, Edward F. (September 2006), "Asteroid albedos deduced from stellar occultations", Icarus 184 (1): 211–220, doi:10.1016/j.icarus.2006.04.006, Bibcode2006Icar..184..211S. 

External links