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185 Eunike

From Wikipedia, the free encyclopedia

185 Eunike
Orbital diagram
Discovery
Discovered byC. H. F. Peters, 1878
Discovery date1 March 1878
Designations
Pronunciation/jˈnk/[1]
Named after
Εὐνίκη Eynīkē
A878 EA
Main belt
AdjectivesEunikean /jnɪˈkən/
Orbital characteristics[2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc131.77 yr (48128 d)
Aphelion3.0924 AU (462.62 Gm)
Perihelion2.3843 AU (356.69 Gm)
2.7383 AU (409.64 Gm)
Eccentricity0.12930
4.53 yr (1655.1 d)
327.48°
0° 13m 3.036s / day
Inclination23.238°
153.84°
224.01°
Earth MOID1.41759 AU (212.068 Gm)
Jupiter MOID2.40697 AU (360.078 Gm)
TJupiter3.222
Physical characteristics
Dimensions157.51±2.6 km[2]
160.61 ± 5.00 km[3]
Mass(3.56 ± 2.61) × 1018 kg[3]
Mean density
1.64 ± 1.21 g/cm3[3]
21.797 h (0.9082 d)[2]
21.812 ± 0.001 hours[4]
0.0638±0.002
C
7.62,[2] 7.45 ± 0.01[4]

185 Eunike is a dark and very large main-belt asteroid. It was discovered by C. H. F. Peters on March 1, 1878, in Clinton, New York and named after Eunike, a Nereid in Greek mythology whose name means 'happy victory'. The name was chosen to celebrate the Treaty of San Stefano (1878).

This object is orbiting the Sun at a distance of 2.74 AU with an eccentricity of 0.129 and an orbital period of 4.53 years. Its orbital plane is inclined at an angle of 23.2° to the plane of the ecliptic. Using infrared measurements, the diameter has been measured at 160.464 km. It has a primitive carbonaceous composition.

Based upon photometric observations made between 2010 and 2014, this asteroid has a rotation period of 21.812±0.001 hours and a brightness variation of 0.08±0.01 in magnitude. At opposition, the absolute magnitude was measured at 7.45±0.01. It displays a hemispheric albedo dichotomy similar to that on 4 Vesta.[4]

As of 17 September 2020, there have been thirteen observed occultations of stars by Eunike.[citation needed]

References

[edit]
  1. Noah Webster (1884) A Practical Dictionary of the English Language
  2. 1 2 3 4 "185 Eunike". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 12 May 2016.
  3. 1 2 3 Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science, vol. 73, pp. 98–118, arXiv:1203.4336, Bibcode:2012P&SS...73...98C, doi:10.1016/j.pss.2012.03.009. See Table 1.
  4. 1 2 3 Pilcher, Frederick; et al. (October 2014), "A Comprehensive Photometric Investigation of 185 Eunike", of the Minor Planets Section of the Association of Lunar and Planetary Observers, 41 (4): 244–250, Bibcode:2014MPBu...41..244P.
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