Antiope (minor planet 90)
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Artist's rendering of the binary asteroid 90 Antiope. Credit: European Southern Observatory
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The first asteroid shown to be a binary system (see binary asteroid); its two components, each about 85 km across, are separated by about 170 km, and appear to be rubble piles consisting of about 30 percent empty space (see rubble-pile asteroid). They complete an orbit around one another every 16.5 hours. Antiope was discovered in 1866 by the German astronomer R. Luther and is a member of the Themis family, located in the outer part of the main asteroid belt.
| spectral class |
C |
| albedo |
0.05 |
| semimajor axis |
3.155 AU |
| perihelion |
2.665 AU |
| aphelion |
3.645 AU |
| eccentricity |
0.155 |
| inclination |
2.2° |
| period |
5.60 years |
Related entry
Antiope in mythology (Encyclopedia of History)
Related category
NOTABLE ASTEROIDS, CENTAURS, AND KUIPER BELT OBJECTS
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