Kirkwood, gaps de

Kirkwood, gaps de
Interrupciones en la distribución de asteroides en el cinturón de asteroides ubicado entre las órbitas de Marte y Júpiter, que se producen cuando el período orbital de cualquiera de estos pequeños cuerpos es una fracción simple del período orbital de Júpiter.

Varias zonas de baja densidad en el cinturón de asteroides fueron descubiertas alrededor de 1860 por Daniel Kirkwood (n. 1814–m. 1895), quien explicó estos "gaps como resultado de las perturbaciones de Júpiter. Dedujo que cualquier objeto que orbitara en una de estas regiones sería perturbado de manera regular por la atracción gravitacional del planeta y, como consecuencia, desplazado hacia otra órbita.

Enciclopedia Universal. 2012.

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