Discovery
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Discovered by | J. R. Hind |
Discovery date | December 15, 1852 |
Designations
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Pronunciation | English pronunciation: /θəˈlaɪ.ə/ |
Named after | Thalia |
Alternate name(s) | 1938 CL; 1974 QT2 |
Minor planet category |
Main belt |
Epoch June 14, 2006 (JD 2453900.5) | |
Aphelion | 484.663 Gm (3.240 AU) |
Perihelion | 301.483 Gm (2.015 AU) |
Semi-major axis | 393.073 Gm (2.628 AU) |
Eccentricity | 0.233 |
Orbital period | 1555.679 d (4.26 a) |
Average orbital speed | 18.12 km/s |
Mean anomaly | 328.687° |
Inclination | 10.145° |
Longitude of ascending node | 67.228° |
Argument of perihelion | 59.311° |
Physical characteristics
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Dimensions | 107.5 km |
Mass | 1.3×1018? kg |
Mean density | 2.0? g/cm³ |
Equatorial surface gravity | 0.0300? m/s² |
Escape velocity | 0.0568? km/s |
Rotation period | 0.5128 d (12.308 h) [1] |
Albedo | 0.2536 (geometric)[2] |
Temperature | ~164 K |
Spectral type | S |
Apparent magnitude | 9.11 to 13.19 |
Absolute magnitude (H) | 6.95 |
23 Thalia (Greek: Θάλεια) is a large main-belt asteroid. It was discovered by J. R. Hind on December 15, 1852, at the private observatory of W. Bishop, located in Hyde Park, London, England.[3] Bishop named it after Thalia, the Muse of comedy and pastoral poetry in Greek mythology.[4]
It is categorized as an S-type asteroid consisting of mainly of iron- and magnesium-silicates. This the second most common type of asteroid in the main belt. Based on analysis of the light curve, the object has a sidereal rotation period of 0.513202 ± 0.000002 days. An ellipsoidal model of the light curve gives an a/b ratio of 1.28 ± 0.05.[5]
With a semimajor axis of 2.628, the asteroid is orbiting between the 3:1 and 5:2 Kirkwood gaps in the main belt.[6] Its orbital eccentricity is larger than the median value of 0.07 for the main belt, and the inclination is larger than the median of below 4°. But most of the main-belt asteroids have an eccentricity of no more than 0.4 and an inclination of up to 30°, so the orbit of 23 Thalia is not unusual for a main-belt asteroid.[7]
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