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Updated: Dec 23, 2025

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El origen binario amplio de los binarios de contacto del cinturón de Kuiper (2014) MU69

Evgeni Grishin1, Uri Malamud2, Hagai B Perets2

  • 1Physics Department, Technion-Israel Institute of Technology, Haifa, Israel. eugeneg@campus.technion.ac.il.

Nature
|April 24, 2020
PubMed
Resumen

Las perturbaciones semiseculares explican la formación de binarios de contacto oblicuo como Arrokoth. Este proceso, que ocurre en los objetos binarios ultraanchos del cinturón de Kuiper (KBO), conduce a fusiones suaves, reproduciendo las características observadas.

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