Cupid is an inner satelliteofUranus. It was discovered by Mark R. Showalter and Jack J. Lissauer in 2003 using the Hubble Space Telescope.[6] It was named after a character in William Shakespeare's play Timon of Athens.[7]
 | |
| Discovery | |
|---|---|
| Discovered by | Mark R. Showalter and Jack J. Lissauer |
| Discovery date | August 25, 2003 |
| Designations | |
Designation | Uranus XXVII |
| Pronunciation | /ˈkjuːpəd/ |
| Adjectives | Cupidian /kjuːˈpɪdiən/[1] |
| Orbital characteristics | |
| 74,392 km | |
| Eccentricity | 0.0013 |
| 0.618 d | |
| Inclination | 0.1° (to Uranus' equator) |
| Satellite of | Uranus |
| Physical characteristics | |
| 8.9±0.7 km[4] | |
| ~1,000 km2 | |
| Volume | ~3,000 km3 |
| Mass | ~(1.5–3.5)×1015 kg |
Mean density | 0.5–1.2 g/cm3[5] |
| ~0.0013–0.0029 m/s2 | |
| ~0.0047–0.0072 km/s | |
| synchronous | |
| 0 | |
| Albedo | 0.08 (assumed)[2] |
| Temperature | ~64 K |
It is the smallest known inner Uranian satellite (apart from possibly Mab), crudely estimated to be only about 18 km in diameter. This and the dark surface made it too dim to be detected by the Voyager 2 cameras during its Uranus flyby in 1986.
The orbit of Cupid differs only by 863 km from the orbit of the larger moon Belinda. Unlike Mab and Perdita, Uranian satellites also discovered in 2003, it does not seem to be perturbed.[2] Despite this, it has the least stable orbit of Uranus's inner moons — it is likely to collide with Belinda in the next 100,000–10 million years, due to resonance interactions that cause the smaller Cupid to drift into a more dangerous orbit over this timescale.[5]
Cupid is at most 500 million years old.[3]
Following its discovery, Cupid was given the temporary designation S/2003 U 2.[6] It is also designated Uranus XXVII.[7]
It should not be confused with the asteroid 763 Cupido.