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El lado oscuro de los anillos de Urano
Imke de Pater1, H B Hammel, Mark R Showalter
1Astronomy Department, 601 Campbell Hall, University of California, Berkeley, CA 94720, USA. imke@astron.berkeley.edu
Resumen
Urano es el planeta Urano.
Área de la Ciencia:
- Ciencias planetarias Ciencias planetarias.
- La astronomía es la astronomía.
- Sistemas de anillos Sistemas de anillos.
Sus antecedentes:
- Los anillos de Urano fueron descubiertos en 1977.
- Los anillos de Urano se ven típicamente desde un ángulo que oscurece su lado oscuro.
- La orientación edge-on de 2007 ofreció una oportunidad de visualización única.
Objetivo del estudio:
- Para obtener imágenes y analizar el lado oscuro de los anillos de Urano.
- Para evaluar los cambios en la estructura y composición del sistema de anillos.
- Para comparar las observaciones actuales con los datos de la nave espacial Voyager.
Principales métodos:
- Adquisición de imágenes infrarrojas terrestres de los anillos de Urano.
- Análisis de la débil distribución de material del sistema de anillos.
- Comparación de nuevos datos con observaciones históricas.
Principales resultados:
- El lado oscuro de los anillos de Urano reveló un sistema dramáticamente cambiado.
- Se observó una nube extendida de material débil, no asociada con estructuras de anillos conocidas o cinturones de polvo.
- Se observaron diferencias significativas en comparación con las imágenes de la nave espacial Voyager de 1986.
Conclusiones:
- La distribución del polvo en el sistema de anillos de Urano ha sufrido cambios sustanciales desde 1986.
- Estos cambios ocurren en escalas más grandes que las previamente observadas en los sistemas de anillos planetarios.
- El único ángulo de visión de 2007 destacó la evolución dinámica dentro de los anillos de Urano.
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