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Eucharis (minor planet designation: 181 Eucharis) is a large, slowly rotating main-belt asteroid that was discovered by French astronomer Pablo Cottenot on February 2, 1878, from Marseille Observatory.[4] It was his only asteroid discovery. This object was named after Eucharis, a Greek nymph.

181 Eucharis
Discovery
Discovered byPablo Cottenot
Discovery date2 February 1878
Designations
MPC designation(181) Eucharis
Pronunciation/ˈjkərɪs/
A906 GA
Main belt
Orbital characteristics[1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc123.63 yr (45157 d)
Aphelion3.7664 AU (563.45 Gm)
Perihelion2.49280 AU (372.918 Gm)
3.12958 AU (468.179 Gm)
Eccentricity0.20347
5.54 yr (2022.2 d)
16.64 km/s
32.3207°
0° 10m 40.879s / day
Inclination18.890°
143.224°
318.943°
Earth MOID1.53686 AU (229.911 Gm)
Jupiter MOID1.47086 AU (220.038 Gm)
TJupiter3.099
Physical characteristics
Dimensions106.66±2.2 km
52.23 h (2.176 d)[1][2]
0.1135±0.0054
S (Tholen)
Xk (Bus)[3]
7.84

In the Tholen classification system, it is categorized as a stony S-type asteroid, while the Bus asteroid taxonomy system lists it as an Xk asteroid.[3] Photometric observations of this asteroid at the Goat Mountain Astronomical Research Station in Rancho Cucamonga, California during 2007 gave a light curve with a leisurely rotation period of 52.23 ± 0.05 hours.[2]

This object is the namesake of a family of 149–778 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.[5]

ReferencesEdit

  1. ^ a b Yeomans, Donald K., "181 Eucharis", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 12 May 2016.
  2. ^ a b Stephens, Robert D. (March 2008), "Long Period Asteroids Observed from GMARS and Santana Observatories", The Minor Planet Bulletin, 35 (1), pp. 21–22, Bibcode:2008MPBu...35...21S.
  3. ^ a b DeMeo, Francesca E.; et al. (July 2009), "An extension of the Bus asteroid taxonomy into the near-infrared" (PDF), Icarus, 202 (1), pp. 160–180, Bibcode:2009Icar..202..160D, doi:10.1016/j.icarus.2009.02.005, archived from the original (PDF) on 2014-03-17, retrieved 2013-04-08. See appendix A.
  4. ^ "Numbered Minor Planets 1–5000", Discovery Circumstances, IAU Minor Planet center, retrieved 2013-04-07.
  5. ^ Novaković, Bojan; et al. (November 2011), "Families among high-inclination asteroids", Icarus, 216 (1), pp. 69–81, arXiv:1108.3740, Bibcode:2011Icar..216...69N, doi:10.1016/j.icarus.2011.08.016.

External linksEdit