{"schema":"hottub-news/story/v1","story":"st_ibln6pgno5qeis5wz7eq","title":"Inclination of Miranda as a Constraint on the Tidal Dissipation of Uranus","title_en":null,"outlets":1,"brief":null,"page":"https://hottub.news/stories/inclination-of-miranda-as-a-constraint-on-the-tidal-dissipation-of-ibln6pgno5","count":1,"items":[{"id":"n_ibln6pgno5qeis5wz7eq","seq":369760,"kind":"research","title":"Inclination of Miranda as a Constraint on the Tidal Dissipation of Uranus","url":"https://arxiv.org/abs/2609.31580","summary":"arXiv:2609.31580v1 Announce Type: new Abstract: The five major moons of Uranus record a complicated geological history characterized by both tectonic resurfacing and heavy impact cratering, connecting their evolution to dynamical processes in the Solar System. Miranda, the smallest and closest major moon to Uranus, has an unusually large orbital inclination ($4.3^\\circ$) and an remarkable surface geology dominated by coronae and tectonic structures. In this paper we explore…","published":"2026-09-28T04:00:00Z","seen":"2026-09-28T07:43:12Z","lang":"en","source":{"id":"arxiv-astro-ph","name":"arXiv astro-ph (astrophysics)","domain":"arxiv.org","outlet":{"wikidata":"Q118398","name":"arXiv","type":"website","country":"US","designations":["bibliographic database","disciplinary repository","online database","open science tool","preprint server","website"]}},"via":"arxiv-astro-ph","topics":["space","astrophysics","astro-ph.ep"],"authors":["Maryame El Moutamid, Matija \\'Cuk"],"entities":[{"id":"Q5355666","name":"Miranda","type":"place"},{"id":"Q324","name":"Uranus","type":"place"}],"story":"st_ibln6pgno5qeis5wz7eq","category":"science-technology","category_p":0.3799999952316284,"category2":"environment","sentiment":"neutral","tone":-0.09000000357627869,"political":0.2800000011920929}]}