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Venus: resultados preliminares de imágenes topográficas y de superficie del orbitador pionero
Science (New York, N.Y.)
|July 6, 1979
Resumen
El mapeador de radar Pioneer Venus revela tres grandes rasgos elevados de la superficie venusiana. Estos incluyen una meseta elevada masiva y una región volcánica brillante de radar, junto con cráteres de impacto potenciales.
Área de la Ciencia:
- Ciencias planetarias Ciencias planetarias.
- Geología Geología Geología.
- Radar Astronomía y Astronomía por el Radar
Sus antecedentes:
- Anteriores observaciones de radar basadas en la Tierra insinuaban características significativas de la superficie de Venus.
- La misión Pioneer Venus tenía como objetivo mapear y analizar la superficie venusiana con mayor detalle.
Objetivo del estudio:
- Para analizar las características de la superficie de Venus previamente identificadas utilizando el mapeador de radar Pioneer Venus.
- Para caracterizar la topografía, el origen y la composición de estas características.
Principales métodos:
- Utilizó el mapeador de radar Pioneer Venus para imágenes de alta resolución y análisis topográfico.
- Compiló imágenes de dispersión de radar para crear una visión completa de la región ecuatorial norte.
Principales resultados:
- Se han confirmado tres grandes rasgos de superficie elevados a 5-10 km por encima del terreno circundante.
- Identificó una gran meseta tectónicamente elevada con crestas de radar brillantes de posible origen volcánico o tectónico.
- Caracterizó una tercera característica brillante de radar como material potencialmente volcánico a lo largo de una zona de falla y observó depresiones circulares posiblemente de impactos meteoríticos.
Conclusiones:
- El mapeador de radar Pioneer Venus proporcionó detalles sin precedentes sobre la topografía y la geología de Venus.
- Las características identificadas sugieren una significativa actividad tectónica y volcánica en Venus.
- Un análisis más detallado de los datos de radar puede revelar más sobre los procesos de impacto en Venus.
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