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On larger amateur telescopes with an objective diameter of between 15 and 23 cm, Uranus appears as a pale cyan disk with distinct limb darkening. With a large telescope of 25 cm or wider, cloud patterns, as well as some of the larger satellites, such as Titania and Oberon, may be visible. [82]
The μ and ν rings of Uranus (R/2003 U1 and U2) in Hubble Space Telescope images from 2005 In 2003–2005, the Hubble Space Telescope detected a pair of previously unknown rings, now called the outer ring system, which brought the number of known Uranian rings to 13. [ 13 ]
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 ]
This discovery image shows the new Uranian moon S/2023 U1 using the Magellan telescope on November 4, 2023. Uranus (upper left) is just off the field of view. ... in diameter and takes nearly nine ...
The James Webb Space Telescope has snapped a glowing new portrait of Uranus that showcases the ice giant’s typically hidden rings, moons, weather and atmosphere — features that were nowhere to ...
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Uranus at European Space Agency; NASA's Uranus fact sheet; Uranus Profile at NASA's Solar System Exploration site; Planets – Uranus A kid's guide to Uranus. Uranus at Jet Propulsion Laboratory's planetary photojournal. (photos) Voyager at Uranus (photos) Uranus (Astronomy Cast homepage) (blog) Uranian system montage (photo) Gray, Meghan ...
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]