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Updated: Jun 22, 2026
11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
Observaciones fotométricas de Júpiter a 2400 angstroms desde el cielo
Science (New York, N.Y.)
|November 23, 1979
Resumen
La Voyager 2 es una nave espacial.
Área de la Ciencia:
- Ciencias planetarias Ciencias planetarias.
- Ciencias de la atmósfera Ciencias atmosféricas.
- La detección remota de detección remota.
Sus antecedentes:
- La atmósfera de Júpiter es compleja y dinámica.
- Comprender la composición de la atmósfera es clave para la ciencia planetaria.
Objetivo del estudio:
- Para mapear la composición atmosférica de Júpiter utilizando datos ultravioleta.
- Para identificar los componentes absorbentes en altas latitudes.
Principales métodos:
- Utilizó el instrumento fotopolarimétrico a bordo de la Voyager 2.
- Analizó una franja norte-sur de Júpiter a 2400 angstroms.
Principales resultados:
- Se detectó una fuerte absorción en altas latitudes del norte.
- Se ha identificado un componente molecular o de partículas responsable de la absorción.
- Observó que este constituyente se extendía por encima del nivel de presión de 50 milibares a 65 grados de latitud norte.
Conclusiones:
- Un componente absorbente significativo existe en la atmósfera superior de Júpiter en latitudes altas.
- Este hallazgo proporciona información sobre la dinámica y composición de la atmósfera de Júpiter.
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