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Updated: Jul 3, 2026
11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
Reflexión y variaciones de color en Mercurio: procesos de regolito y heterogeneidad de composición
Mark S Robinson1, Scott L Murchie, David T Blewett
1School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287, USA. robinson@ser.asu.edu
Science (New York, N.Y.)
|July 5, 2008
Resumen
Las imágenes multiespectral de la nave espacial MESSENGER revelan Mercurio.
Área de la Ciencia:
- Ciencias planetarias Ciencias planetarias.
- La detección remota con sensores.
- Mercurio Geología Geología de Mercurio.
Sus antecedentes:
- La superficie de Mercurio exhibe una baja reflectancia general.
- Estudios previos habían identificado amplias variaciones espectrales.
Objetivo del estudio:
- Caracteriza las unidades de superficie de Mercurio utilizando imágenes multispectrales.
- Identificar materiales geológicos distintos basados en sus propiedades espectrales.
Principales métodos:
- Análisis de imágenes multiespectrales de la nave espacial MESSENGER (0,4 1,0 micrómetros).
- Clasificación de las unidades de superficie basadas en la reflectancia y la pendiente espectral.
Principales resultados:
- Se identificaron tres unidades a gran escala: llanuras lisas de mayor reflexión (volcánicas), material de menor reflexión (minerales opacos) y terreno intermedio (corteza superior).
- Las unidades distintas incluyen eyecciones frescas del cráter, depósitos del suelo del cráter y materiales de depresión sin borde.
Conclusiones:
- La composición de la superficie de Mercurio es diversa, con distintas unidades vinculadas a procesos geológicos.
- El análisis espectral proporciona información sobre la composición de la corteza terrestre y la historia volcánica.
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