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Weak S-type asteroids compared to C-type explain the observed size distribution of the main belt

Fuente: arXiv

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Detalles Bibliográficos
Autores principales:	Vávra, Michael, Brož, Miroslav
Formato:	Preprint
Publicado:	2026
Materias:	Earth and Planetary Astrophysics
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

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