350 Ornamenta

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.

350 Ornamenta
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
Main belt
Orbital characteristics[1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc123.34 yr (45051 d)
Aphelion3.6041 AU (539.17 Gm)
Perihelion2.61365 AU (390.996 Gm)
3.10885 AU (465.077 Gm)
Eccentricity0.15929
5.48 yr (2002.2 d)
177.109°
0° 10m 47.316s / day
Inclination24.894°
90.106°
338.34°
Physical characteristics
Dimensions118.35±4.5 km
9.178 h (0.3824 d)
0.0566±0.005
C
8.37

    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, 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.
    3. 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.
    4. Novaković, Bojan; et al. (November 2011), "Families among high-inclination asteroids", Icarus, vol. 216, no. 1, pp. 69–81, arXiv:1108.3740, Bibcode:2011Icar..216...69N, doi:10.1016/j.icarus.2011.08.016.


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