90 Antiope

{| table border="1" cellspacing="0" cellpadding="2" align="right" style="margin-left: 1em"\n|+ 90 Antiope\n|-\n|colspan="2" align="center"|
\n|-\n! bgcolor="#ffc0c0" colspan="2" | Orbital characteristics ¹\n|-\n|Orbit type || Main belt (Themis)\n|-\n|Semimajor axis || 3.157 AU\n|-\n|Perihelion distance || 2.665 AU\n|-\n|Aphelion distance || 3.649 AU\n|-\n|Orbital period || 5.61 years\n|-\n|Inclination || 2.22°\n|-\n|Eccentricity || 0.156\n|-\n! bgcolor="#ffc0c0" colspan="2" | Physical characteristics\n|-\n|Diameter ³ || 85, 85 km\n|-\n|Rotation period ³ || 16.496 hours (sync)\n|-\n|Spectral class ¹ || C\n|-\n|Abs. magnitude ¹ || 8.27\n|-\n|Albedo ⁴ || 0.060\n|-\n! bgcolor="#ffc0c0" colspan="2" | History ²\n|-\n|Discoverer || R. Luther, 1866\n|-\n! bgcolor="#ffc0c0" colspan="2" | Satellites\n|-\n|Designation || S/2000 (90) 1\n|} 90 Antiope is an asteroid discovered on October 1, 1866 by Robert Luther. The 90th asteroid to be discovered, it is named after an Amazon princess, sister of Hippolyte and daughter of Ares, who was taken prisoner by Heracles and later married Theseus. Alternatively, there is another Antiope in Greek legend, a daughter of Nycteus, king of Thebes, and mother of two children by Zeus. Antiope is classified as a member of the Themis family of asteroids. One observed stellar occultation by Antiope has been reported, on (June 11, 1980). In 2000, it was discovered that Antiope is a double asteroid, consisting of two individual bodies about 80 kilometers across and separated by 170 kilometers, orbiting around a common center. A complete revolution takes 16.5 hours. Their composition is C-type, which means that they are dark in colouring with a carbonate composition. The discovery was made with the Keck Telescope at Mauna Kea using adaptive optics, allowing the two components to be resolved.

External links

\n*SWrI Press Release\n*Data from Johnston's Archive Category:Binary asteroids \n