Cordelia (Imaged 24 January 1986) | |
Discovery | |
---|---|
Discovered by | Richard J. Terrile / Voyager 2 |
Discovery date | January 20, 1986 |
Designations | |
Designation | Uranus VI |
Pronunciation | /kɔːrˈdiːliə/[1] |
Adjectives | Cordelian[2] |
Orbital characteristics | |
Mean orbit radius | 49751.722 ± 0.149 km[3] |
Eccentricity | 0.00026 ± 0.000096[3] |
Orbital period | 0.33503384 ± 0.00000058 d[3] |
Inclination | 0.08479 ± 0.031° (to Uranus' equator)[3] |
Satellite of | Uranus |
Group | ring shepherd |
Physical characteristics | |
Dimensions | 50 × 36 × 36 km[4] |
Mean radius | 20.1 ± 3 km[4][5][6] |
Surface area | ~5500 km2[lower-alpha 1] |
Volume | ~38,900 km3[lower-alpha 1] |
Mass | ~4.4×1016 kg[lower-alpha 1] |
Mean density | ~1.3 g/cm3 (assumed)[5] |
~0.0073 m/s2[lower-alpha 1] | |
~0.017 km/s[lower-alpha 1] | |
Rotation period | synchronous[4] |
Axial tilt | zero[4] |
Albedo | |
Physics | ~64 K[lower-alpha 1] |
Cordelia is the innermost known 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 7.[8] It was not detected again until the Hubble Space Telescope observed it in 1997.[7][9] Cordelia takes its name from the youngest daughter of Lear in William Shakespeare's King Lear. It is also designated Uranus VI.[10]
Other than its orbit,[3] radius of 20 km[4] and geometric albedo of 0.08[7] virtually nothing is known about it. In the Voyager 2 images Cordelia appears as an elongated object with its major axis pointing towards Uranus. The ratio of axes of Cordelia's prolate spheroid is 0.7 ± 0.2.[4]
Cordelia acts as the inner shepherd satellite for Uranus' ε ring.[11] Cordelia's orbit is within Uranus' synchronous orbit radius, and is therefore slowly decaying due to tidal deceleration.[4]
Cordelia is very close to a 5:3 orbital resonance with Rosalind.[12]
Explanatory notes
Citations
Original source: https://en.wikipedia.org/wiki/Cordelia (moon).
Read more |