34 Circe
A three-dimensional model of 34 Circe based on its light curve. | |
Discovery | |
---|---|
Discovered by | J. Chacornac |
Discovery date | April 6, 1855 |
Designations | |
Named after | Circe |
1965 JL | |
Main belt | |
Orbital characteristics[1] | |
Epoch November 4, 2013 (JD 2456600.5) | |
Aphelion | 2.967739 AU |
Perihelion | 2.406230 AU |
2.686984 AU | |
Eccentricity | 0.1045 |
4.40 a (1607.332 d) | |
Average orbital speed | 18.12 km/s |
39.80474° | |
Inclination | 5.498° |
184.44157° | |
330.2330° | |
Physical characteristics | |
Dimensions | 113.02 ± 4.90 km[2] |
Mass | (3.66 ± 0.03) × 1018 kg[2] |
Mean density | 4.83 ± 0.63 g/cm3[2] |
~0.0317 m/s² | |
~0.0600 km/s | |
0.5063 d (12.15 h) [1] | |
Albedo | 0.0541 [1] |
Temperature | ~172 K |
Spectral type | C |
8.51 | |
|
34 Circe (/ˈsɜːrsiː/ SUR-see) is a large, very dark main-belt asteroid. It was discovered by French astronomer J. Chacornac on April 6, 1855, and named after Circe, a goddess in Greek mythology.
Photometric observations of this asteroid made during 2007 at the Organ Mesa Observatory in Las Cruces, New Mexico gave an asymmetrical bimodal light curve with a period of 12.176 ± 0.002 hours and a brightness variation of 0.17 ± 0.02 in magnitude.[3]
References
- 1 2 3 Yeomans, Donald K., "34 Circe", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 2013-12-21.
- 1 2 3 Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science, 73, pp. 98–118, arXiv:1203.4336, Bibcode:2012P&SS...73...98C, doi:10.1016/j.pss.2012.03.009. See Table 1.
- ↑ Pilcher, Frederick (September 2008), "Period Determinations for 26 Proserpina, 34 Circe 74 Galatea, 143 Adria, 272 Antonia, 419 Aurelia, and 557 Violetta", The Minor Planet Bulletin, 35 (3), pp. 135–138, Bibcode:2008MPBu...35..135P.
External links
- 34 Circe at the JPL Small-Body Database
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