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Io como fuente de las corrientes de polvo joviano
1Max-Planck-Institute fur Kernphysik, Heidelberg, Germany. Amara.Graps@mpi-hd.mpg.de
Nature
|May 16, 2000
Resumen
Júpiter Júpiter Júpiter es el nombre de Júpiter.
Área de la Ciencia:
- Ciencias planetarias Ciencias planetarias.
- La astronomía es la astronomía.
- Física del espacio Física del espacio
Sus antecedentes:
- Las corrientes de polvo originadas en Júpiter se observaron por primera vez en 1992.
- Estudios previos identificaron fuentes potenciales, incluidos los anillos de Júpiter y el cometa Shoemaker-Levy 9.
Objetivo del estudio:
- Para determinar el origen preciso de las corrientes de polvo de Júpiter.
- Identificar la fuente dominante que contribuye a estas corrientes de polvo.
Principales métodos:
- Análisis de los datos de impacto de polvo recogidos por la nave espacial Galileo.
- Identificación de periodicidades dentro de la señal de impacto de polvo.
Principales resultados:
- El anillo gossamer de Júpiter e Io fueron identificados como las únicas fuentes posibles restantes.
- Se confirmó que los volcanes de Io son la fuente dominante de las corrientes de polvo de Júpiter.
- La actividad volcánica en Io, no el impacto eyecta, es la fuente primaria.
Conclusiones:
- Io es la fuente principal de las corrientes de polvo de Júpiter.
- Los penachos volcánicos en Io son responsables de la generación de estas corrientes de polvo.
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