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181 Eucharis

From Wikipedia, the free encyclopedia
Main-belt asteroid

181 Eucharis
Orbital diagram
Discovery
Discovered byPablo Cottenot
Discovery date2 February 1878
Designations
(181) Eucharis
Pronunciation/ˈjkərɪs/[1]
Named after
Eucharis
A878 CB; 1906 GA
Main belt
Orbital characteristics[2]
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
5.54yr (2022.2d)
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)[2][3]
0.1135±0.0054
S (Tholen)
Xk (Bus)[4]
7.84

181 Eucharis is a large, slowly rotatingmain-beltasteroid that was discovered byFrenchastronomerPablo Cottenot on February 2, 1878, fromMarseille Observatory.[5] It was his only asteroid discovery. This object was named afterEucharis, anymph from the 17th-century novelLes Aventures de Télémaque.

In theTholen classification system, it is categorized as a stonyS-type asteroid, while the Busasteroid taxonomy system lists it as anXk asteroid.[4]Photometric observations of this asteroid at the Goat Mountain Astronomical Research Station inRancho Cucamonga, California during 2007 gave alight curve with a leisurelyrotation period of 52.23 ± 0.05 hours.[3]

This object is the namesake of afamily of 149–778 asteroids that share similar spectral properties andorbital elements; hence they may have arisen from the same collisional event. All members have a relatively highorbital inclination.[6]

References

[edit]
  1. ^"eucharis".Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription orparticipating institution membership required.)
  2. ^abYeomans, Donald K.,"181 Eucharis",JPL Small-Body Database Browser,NASA Jet Propulsion Laboratory, retrieved12 May 2016.
  3. ^abStephens, Robert D. (March 2008), "Long Period Asteroids Observed from GMARS and Santana Observatories",The Minor Planet Bulletin, vol. 35, no. 1, pp. 21–22,Bibcode:2008MPBu...35...21S.
  4. ^abDeMeo, Francesca E.; et al. (July 2009),"An extension of the Bus asteroid taxonomy into the near-infrared"(PDF),Icarus, vol. 202, no. 1, pp. 160–180,Bibcode:2009Icar..202..160D,doi:10.1016/j.icarus.2009.02.005, archived fromthe original(PDF) on 17 March 2014, retrieved8 April 2013. See appendix A.
  5. ^"Numbered Minor Planets 1–5000",Discovery Circumstances, IAU Minor Planet center, retrieved7 April 2013.
  6. ^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.

External links

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