181 Eucharis
Discovery | |
---|---|
Discovered by | Pablo Cottenot |
Discovery date | February 2, 1878 |
Designations | |
A906 GA | |
Main belt | |
Orbital characteristics[1] | |
Epoch June 14, 2006 (JD 2453900.5) | |
Aphelion | 562.742 Gm (3.762 AU) |
Perihelion | 376.603 Gm (2.517 AU) |
469.672 Gm (3.140 AU) | |
Eccentricity | 0.198 |
2031.902 d (5.56 a) | |
Average orbital speed
|
16.64 km/s |
95.743° | |
Inclination | 18.801° |
143.652° | |
317.284° | |
Physical characteristics | |
Dimensions | 106.0 km |
52.23[2] h | |
Albedo | 0.115 4 |
Spectral type
|
S (Tholen) Xk (Bus)[3] |
7.84 | |
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.
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]
References
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- ↑ 3.0 3.1 Lua error in package.lua at line 80: module 'strict' not found. See appendix A.
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