Astronomy:350 Ornamenta

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Short description: Main-belt asteroid
350 Ornamenta
350Ornamenta (Lightcurve Inversion).png
A three-dimensional model of 350 Ornamenta based on its light curve
Discovery
Discovered byAuguste Charlois
Discovery date14 December 1892
Designations
(350) Ornamenta
Pronunciation/ˌɔːrnəˈmɛntə/
1892 U
Minor planet categoryMain belt
Orbital characteristics[1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc123.34 yr (45051 d)
|{{{apsis}}}|helion}}3.6041 astronomical unit|AU (539.17 Gm)
|{{{apsis}}}|helion}}2.61365 AU (390.996 Gm)
3.10885 AU (465.077 Gm)
Eccentricity0.15929
Orbital period5.48 yr (2002.2 d)
Mean anomaly177.109°
Mean motion0° 10m 47.316s / day
Inclination24.894°
Longitude of ascending node90.106°
338.34°
Physical characteristics
Dimensions118.35±4.5 km
Rotation period9.178 h (0.3824 d)
Geometric albedo0.0566±0.005
C
Absolute magnitude (H)8.37


Ornamenta (minor planet designation: 350 Ornamenta) is a relatively large main-belt asteroid, measuring 118 km in diameter. It is classified as a C-type asteroid and is probably composed of carbonaceous material.

Ornamenta was discovered by Auguste Charlois on December 14, 1892, in Nice, France . It was named in 1905 in honor of Antoinette Horneman, who was a member of the Société astronomique de France.[2]

During 2002, the asteroid was observed occulting a star. The resulting chords provided a diameter estimate of 99.5 km.[3]

This object is the namesake of a family of 14–93 asteroids that share similar spectral properties and orbital elements; hence they may have arisen from the same collisional event. All members have a relatively high orbital inclination.[4]

References

  1. Yeomans, Donald K., "164 Eva", JPL Small-Body Database Browser (NASA Jet Propulsion Laboratory), https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=164, retrieved 11 May 2016. 
  2. Lutz D. Schmadel (2011). Dictionary of Minor Planet Names (Addendum to Fifth Edition: 2006–2008 ed.). Springer. ISBN 978-3-642-01966-1. https://books.google.com/books?id=uwGbkbhMVyAC. 
  3. 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. 
  4. Novaković, Bojan et al. (November 2011), "Families among high-inclination asteroids", Icarus 216 (1): pp. 69–81, doi:10.1016/j.icarus.2011.08.016, Bibcode2011Icar..216...69N. 

External links