Dynamical Implications of the Recently Detected Feature around Quaoar and Constraints on the Presence of Additional Satellites

A recently reported opaque feature in the Quaoar system, detected during the 2025 June 25 stellar occultation, has been interpreted as either an ∼15 km radius satellite or a dense, sharp-edged arc orbiting at about 5600–5900 km. Here, we investigate both scenarios through numerical integrations that...

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Principais autores:	Gustavo Madeira, Leandro Esteves, Bruno E. Morgado, Paulo V. S. Soares, Silvia M. Giuliatti Winter, Othon C. Winter, Bruno S. Chagas
פורמט:	Artigo
שפה:	Inglês
יצא לאור:	IOP Publishing 2026-01-01
סדרה:	The Planetary Science Journal
נושאים:	Planetary rings Natural satellites (Solar system) Trans-Neptunian objects
גישה מקוונת:	https://doi.org/10.3847/PSJ/ae81a8
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