133 Cyrene

Main-belt asteroid From Wikipedia, the free encyclopedia

133 Cyrene is a fairly large and very bright main-belt asteroid that was discovered by J. C. Watson on 16 August 1873 in Ann Arbor, Michigan, and named after Cyrene, a nymph, daughter of king Hypseus and beloved of Apollo in Greek mythology.[8] 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.[9]

DiscoverysiteAnn Arbor, Michigan, United States
Discoverydate16 August 1873
(133) Cyrene
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133 Cyrene
A 3D lightcurve-derived model of 133 Cyrene.
Discovery[1]
Discovered byJames Craig Watson
Discovery siteAnn Arbor, Michigan, United States
Discovery date16 August 1873
Designations
(133) Cyrene
Pronunciation/sˈrn/[2]
Named after
Cyrene (nymph)
A873 QA · A910 NB · 1936 HO · 1948 QC · 1959 UR[3][a]
Main belt
AdjectivesCyrenean /srɪˈnən/, Cyrenian /sˈrniən/[4]
Orbital characteristics[3]
Epoch 21 November 2025 (JD 2461000.5)
Uncertainty parameter 0
Observation arc152.13 yr (55566 d)
Aphelion7.2245 AU (1,080.77 Gm)
Perihelion2.6736 AU (399.96 Gm)
3.0742 AU (459.89 Gm)
Eccentricity0.1303
5.3902 yr (1968.77 d)
17.03 km/s
219.02°
0° 10m 58.26s / day
Inclination7.2245°
318.67°
291.65°
Earth MOID1.6686 AU (249.62 Gm)
Jupiter MOID1.6595 AU (248.26 Gm)
TJupiter3.205
Physical characteristics
Dimensions66.57±6.0 km
Mass3.1 × 1017 kg
Mean density
2.0? g/cm3
Equatorial surface gravity
0.0186 m/s²
Equatorial escape velocity
0.0352 km/s
12.708 h (0.5295 d)[3]
12.707 h (0.5295 d)[5]
0.2563±0.053[3]
0.2563[6]
Temperature~133 K
S[6]
7.98,[3] 7.990[7]
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    Discovery and naming

    Cyrene was discovered on 16 August 1873 by astronomer James Craig Watson at Ann Arbor, Michigan, United States.[1] Its discovery, alongside that of 132 Aethra, was announced in the journal Astronomische Nachrichten on 30 August.[10] The asteroid was given the name Cyrene after the Greek mythological figure Cyrene, daughter of the Lapithian king Hypseus. With the god Apollo, she bore her two sons Aristaeus and Idmon.[11]:25

    Orbit

    An orbital diagram of 133 Cyrene. The ecliptic grid and the orbits of the inner planets and Jupiter are also shown.

    Cyrene is a main belt asteroid, orbiting the Sun at an average distance—its semi-major axis—of 3.07 astronomical units (AU). Along its 5.39 year long orbit, its distance from the Sun varies from 2.67 AU at perihelion to 3.47 AU at aphelion due to its orbital eccentricity of 0.13. It has an orbital inclination of 7.22° with respect to the ecliptic plane.[3]

    Physical characteristics

    In the Tholen classification system, it is categorized as a stony SR-type asteroid.[12] 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.[5]

    See also

    Minor planets named after figures related to Cyrene:

    Notes

    1. The MPC notates Aethra's retroactive new-style designations as 1873 QA and 1910 NB.[1]

    References

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