
[After Ophelia, daughter of Polonius in Hamlet by William Shakespeare.]
Discovery image of Ophelia (top of image, outside of rings)
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Discovery
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| Discovered by | Richard J. Terrile / Voyager 2 |
| Discovery date | January 20, 1986 |
| Mean orbit radius | 53,763.390 ± 0.847 km[1] |
| Eccentricity | 0.00992 ± 0.000107[1] |
| Orbital period | 0.37640039 ± 0.00000357 d[1] |
| Inclination | 0.10362 ± 0.055° (to Uranus' equator)[1] |
| Satellite of | Uranus |
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Physical characteristics
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| Dimensions | 54 × 38 × 38 km[2] |
| Mean radius | 21.4 ± 4 km[2][3][4] |
| Surface area | ~6600 km²[a] |
| Volume | ~41,000 km³[a] |
| Mass | ~5.3×1016 kg[a] |
| Mean density | ~1.3 g/cm³ (assumed)[3] |
| Equatorial surface gravity | ~0.0070 m/s²[a] |
| Escape velocity | ~0.018 km/s[a] |
| Rotation period | synchronous[2] |
| Axial tilt | zero[2] |
| Albedo | |
| Temperature | ~64 K[a] |
Ophelia (
/ɵˈfiːliə/ o-FEE-lee-ə) is a moon of Uranus. It was discovered from the images taken by Voyager 2 on January 20, 1986, and was given the temporary designation S/1986 U 8.[6] It was not seen until the Hubble Space Telescope recovered it in 2003.[5][7] Ophelia was named after the daughter of Polonius, Ophelia, in William Shakespeare's play Hamlet. It is also designated Uranus VII.[8]
Other than its orbit,[1] radius of 21 km[2] and geometric albedo of 0.08[5] virtually nothing is known about it. At the Voyager 2 images Ophelia appears as an elongated object, the major axis pointing towards Uranus. The ratio of axes of the Ophelia's prolate spheroid is 0.7 ± 0.3.[2]
Ophelia acts as the outer shepherd satellite for Uranus' Epsilon ring.[9] The orbit of Ophelia is within the synchronous orbit radius of Uranus, and therefore the moon is slowly decaying due to tidal forces.[2]
Explanatory notes
Citations
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