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S/2025 U 1
Inner moon of Uranus From Wikipedia, the free encyclopedia
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S/2025 U 1 is one of the smallest known moons of Uranus,[2] with an estimated diameter between 8 and 10 km (5 and 6 mi).[3] It was reported on 19 August 2025 by a team of astronomers led by Maryame El Moutamid,[a] who found the moon in James Webb Space Telescope NIRCam images taken on 2 February 2025.[1][b] It orbits about 56,250 km (34,950 mi) from the center of Uranus (between the orbits of Ophelia and Bianca) with an orbital period of 9.6 hours (0.402 days).[1] Like the other inner moons of Uranus, it follows a nearly circular orbit along Uranus's equatorial plane.[1] Due to its small size, it appears extremely faint with a near-infrared (H-band) apparent magnitude of 25.5—too faint to be seen by the Hubble Space Telescope and the Voyager 2 spacecraft.[1]
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Name
S/2025 U 1 is the provisional designation of this unnamed moon.[2] By convention, the moons of Uranus are named after characters from the plays of William Shakespeare and Alexander Pope.[3] A proper name will be given once it is approved by the International Astronomical Union.[3][2] Co-discoverer Mark R. Showalter has stated in a 2025 NewScientist article that "there have been discussions [of a name for S/2025 U 1] but no shortlist as yet."[2]
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Orbit

S/2025 U 1 is the 14th known member of Uranus's inner moons, which are small moons that orbit interior to the planet's five largest moons (Miranda, Ariel, Umbriel, Titania, and Oberon).[3] S/2025 U 1 follows a nearly circular orbit around Uranus's equatorial plane, at a distance of 56,250 km (34,950 mi) from the planet's center with an orbital period of 9.6 hours (0.402 days).[1] S/2025 U 1 is located outside the edge of Uranus's inner ring system, between the orbits of Ophelia and Bianca.[2] The nearly circular orbit of S/2025 U 1 suggests that it formed near its current location, according to discoverer Maryame El Moutamid.[3]
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Notes
- The full team of researchers involved in the discovery of this moon includes: Maryame El Moutamid, Matthew M. Hedman, Mark R. Showalter, Matthew Tiscareno, Imke de Pater, Jack J. Lissauer, and Damya Souami.[1]
- The NIRCam discovery observations consisted of ten consecutive near-infrared images, each with 40-minute-long exposure times.[3]
References
External links
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