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El descubrimiento del sodio en la atmósfera del mercurio
Resumen
Mercurio Mercurio Mercurio Mercurio es Mercurio.
Área de la Ciencia:
- Ciencias planetarias Ciencias planetarias.
- Ciencias de la atmósfera Ciencias atmosféricas.
- La espectroscopia es una técnica de espectroscopia.
Sus antecedentes:
- La atmósfera de Mercurio es tenue y su composición ha sido parcialmente estudiada.
- Misiones anteriores como la Mariner 10 identificaron el helio como un componente importante.
Objetivo del estudio:
- Para investigar la composición de la atmósfera de Mercurio.
- Para cuantificar la abundancia de vapor de sodio en la atmósfera de Mercurio.
Principales métodos:
- Análisis del espectro de Mercurio en las líneas D de Fraunhofer de sodio.
- Medición de las características de emisión atribuidas a la dispersión resonante de la luz solar.
Principales resultados:
- Las fuertes características de emisión indican la presencia de vapor de sodio.
- Se estima que la abundancia total de sodio en la columna es de 8,1 x 10^11 átomos/cm^2,2.
- La densidad superficial del sodio es de aproximadamente 1,5 x 10^5 átomos/cm^3, comparable a la del helio.
Conclusiones:
- El vapor de sodio es un componente importante de la atmósfera de Mercurio.
- La dispersión resonante de la luz solar es la fuente de la emisión de sodio observada.
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