133 Cyrene

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133 Cyrene
Discovery
Discovered by James Craig Watson
Discovery date August 16, 1873
Designations
Named after
Cyrene (mythology)
A910 NB; 1936 HO;
1948 QC; 1959 UR
Main belt
Orbital characteristics[1]
Epoch July 14, 2004 (JD 2453200.5)
Aphelion 522.169 Gm (3.490 AU)
Perihelion 392.840 Gm (2.626 AU)
457.505 Gm (3.058 AU)
Eccentricity 0.141
1953.456 d (5.35 a)
17.03 km/s
224.793°
Inclination 7.233°
319.246°
291.128°
Physical characteristics
Dimensions 66.6 km
Mass 3.1 × 1017 kg
Mean density
2.0? g/cm³
0.0186 m/s²
0.0352 km/s
12.707[2] h (0.5295 d)
Albedo 0.2563[3]
Temperature ~133 K
Spectral type
S[3]
7.990[4]

133 Cyrene is a fairly large and very bright main-belt asteroid that was discovered by J. C. Watson on August 16, 1873, and named after Cyrene, a nymph, daughter of king Hypseus and beloved of Apollo in Greek mythology.[5] It is classified as an S-type asteroid based upon its spectrum. It is listed as a member of the Hecuba group of asteroids that orbit near the 2:1 mean-motion resonance with Jupiter.[6]

In the Tholen classification system, it is categorized as a stony SR-type asteroid.[7] Photometric observations of this asteroid at the Altimira Observatory in 1985 gave a light curve with a period of 12.707 ± 0.015 hours and a brightness variation of 0.22 in magnitude. This result matches previous measurements reported in 1984 and 2005.[2]

References

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