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Miranda, also designated Uranus V, is the smallest and innermost of Uranus's five round satellites. It was discovered by Gerard Kuiper on 16 February 1948 at McDonald Observatory in Texas , and named after Miranda from William Shakespeare 's play The Tempest . [ 9 ]
These lists contain the Sun, the planets, dwarf planets, many of the larger small Solar System bodies (which includes the asteroids), all named natural satellites, and a number of smaller objects of historical or scientific interest, such as comets and near-Earth objects.
S/2023 U 1 is the smallest and faintest natural satellite of Uranus known, with a diameter of around 8–12 km (5–7 mi). It was discovered on 4 November 2023 by Scott S. Sheppard using the 6.5-meter Magellan–Baade Telescope at Las Campanas Observatory, Chile, and later announced on 23 February 2024. [1]
Of the Solar System's eight planets and its nine most likely dwarf planets, six planets and seven dwarf planets are known to be orbited by at least 300 natural satellites, or moons. At least 19 of them are large enough to be gravitationally rounded; of these, all are covered by a crust of ice except for Earth's Moon and Jupiter's Io . [ 1 ]
There may be two additional small (2–7 km in radius) undiscovered shepherd moons located about 100 km exterior to Uranus's α and β rings. [24] At 162 km, Puck is the largest of the inner moons of Uranus and the only one imaged by Voyager 2 in any detail. Puck and Mab are the two outermost inner satellites of Uranus.
Complete list of Saturn's natural satellites. Mimas; Enceladus; Tethys (trojans: Telesto and Calypso) Dione (trojans: Helene and Polydeuces) Rhea. Rings of Rhea; Titan; Hyperion; Iapetus; Phoebe; Shepherd moons; Saturn-crossing minor planets; Uranus. Rings of Uranus; Complete list of Uranus's natural satellites. Miranda; Ariel; Umbriel; Titania ...
Cupid 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 is separated by only 863 km from the orbit of the larger moon Belinda.
Cressida orbits close to a 3:2 resonance with the η ring, one of the rings of Uranus. Perturbations of the ring's shape provide a way to measure the mass of Cressida, which in 2024 was found to be (1.839 ± 0.212) × 10 17 kg. [5] Cressida is one of the few small satellites of Uranus for which the mass has been directly measured. [10] [5]