90 Antiope
Antiope (minor planet designation: 90 Antiope) is a double asteroid in the outer asteroid belt. It was discovered on October 1, 1866, by Robert Luther. In 2000, it was found to consist of two almost-equally-sized bodies orbiting each other. At average diameters of about 88 km and 84 km, both components are among the 500 largest asteroids. Antiope is a member of the Themis family of asteroids that share similar orbital elements.
Discovery | |
---|---|
Discovered by | Robert Luther |
Discovery date | October 1, 1866 |
Designations | |
MPC designation | (90) Antiope |
Pronunciation | /ænˈtaɪəpiː/ |
Alternative designations | 1952 BK2 |
Minor planet category | Main belt (Themis family) |
Adjectives | Antiopean |
Orbital characteristics | |
Epoch July 23, 2010 (JD 2455400.5) | |
Aphelion | 545.94 Gm 3.6494 AU |
Perihelion | 398.02 Gm 2.6606 AU |
Semi-major axis | 471.19 Gm 3.1550 AU |
Eccentricity | 0.15670 |
Orbital period (sidereal) | 2046.9 d (5.60 yr) |
Average orbital speed | 16.66 km/s |
Mean anomaly | 304.12° |
Inclination | 2.2195° |
Longitude of ascending node | 70.21° |
242.96° | |
Physical characteristics | |
Dimensions | 93.0×87.0×83.6 km 87.8 ± 1.0 km |
Mass | 8.3×1017 kg (whole system) ~ 4.1−4.2 ×1017 kg (components) |
Mean density | 1.25 ± 0.05 g/cm3 (each) |
Synodic rotation period | 0.687 d (16.50 h) (synchronous) |
0.060 | |
C | |
8.27 (together) 9.02 (each component) | |
Discovery | |
---|---|
Discovered by | W. J. Merline, L. M. Close, J. C. Shelton, C. Dumas, F. Menard, C. R. Chapman, and D. C. Slater |
Discovery date | August 10, 2000 |
Designations | |
Minor planet category | Main belt (Themis family) |
Orbital characteristics | |
Semi-major axis | 171 ± 1 km |
Eccentricity | <0.006 |
Orbital period (sidereal) | 0.687713 ± 0.00004 d (16.5051 ± 0.0001 h) |
Average orbital speed | 18.0 m/s |
Satellite of | Binary with 90 Antiope |
Physical characteristics | |
Dimensions | 89.4×82.8×79.6 km |
Mean diameter | 83.8 ± 1.0 km |
Mass | ~ 8.1−8.5 ×1017 kg |
Equatorial escape velocity | variable; ~ 35−40 m/s |
Synodic rotation period | 0.687 d (16.50 h) (synchronous) |
9.02 | |
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