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The Inner Kernel of the Classical Kuiper Belt

The “kernel” of the classical Kuiper Belt was discovered by Petit et al. as a visual overdensity of objects with low ecliptic inclinations and eccentricities at semimajor axes near ∼44 au. This raises the question—are there other structures present in the classical Kuiper Belt? If there are, cluster...

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Autors principals: Amir Siraj, Christopher F. Chyba, Scott Tremaine
Format: Artigo
Idioma:Inglês
Publicat: IOP Publishing 2025-01-01
Col·lecció:The Astrophysical Journal Letters
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Accés en línia:https://doi.org/10.3847/2041-8213/ae1ca4
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