195 Eurykleia is a fairly large main belt asteroid. It was discovered by the Austrian astronomer Johann Palisa on April 19, 1879, and named after Euryclea, the wet-nurse of Odysseus in The Odyssey.
Discovery | |
---|---|
Discovered by | J. Palisa, 1879 |
Discovery date | 19 April 1879 |
Designations | |
(195) Eurykleia | |
Pronunciation | /jʊrɪˈkliːə/[1] |
A879 HA; 1949 QB2 | |
Main belt | |
Orbital characteristics[2] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 131.99 yr (48,208 d) |
Aphelion | 3.00 AU (449.33 Gm) |
Perihelion | 2.75 AU (411.29 Gm) |
2.88 AU (430.30 Gm) | |
Eccentricity | 0.044205 |
4.88 yr (1,781.9 d) | |
113.56° | |
0° 12m 7.308s / day | |
Inclination | 6.9718° |
6.9930° | |
119.12° | |
Earth MOID | 1.77 AU (264.87 Gm) |
Jupiter MOID | 2.01 AU (300.95 Gm) |
TJupiter | 3.284 |
Physical characteristics | |
42.855±0.85 km | |
16.52178±0.00001 h[3] | |
0.0599±0.002 | |
Ch[3] | |
9.01 | |
This body is orbiting the Sun with a period of 4.88 years and a low eccentricity (ovalness) of 0.04. The orbital plane is inclined by 7° from the plane of the ecliptic. It is spinning with a rotation period of 16.5 hours and varies in brightness with an amplitude of 0.24 magnitude. The cross-section diameter of this body is 43 km. The asteroid has a taxonomic type of Ch in the SMASS classification,[3] which indicates it has a dark surface with a primitive carbonaceous composition.
195 Eurykleia has been observed to occult stars twice, once in 2011 and again in 2021.
References
edit- ^ "Euryclea". Dictionary.com Unabridged (Online). n.d.
- ^ "195 Eurykleia". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 6 May 2016.
- ^ a b c Marciniak, A.; et al. (May 2019). "Thermal properties of slowly rotating asteroids: results from a targeted survey". Astronomy & Astrophysics. 625: 40. arXiv:1905.06056. Bibcode:2019A&A...625A.139M. doi:10.1051/0004-6361/201935129. A139.
External links
edit- 195 Eurykleia at AstDyS-2, Asteroids—Dynamic Site
- 195 Eurykleia at the JPL Small-Body Database