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12:35
Atomically Traceable Nanostructure Fabrication
Published on: July 17, 2015
Comienza la exploración intensiva de Titán.
1Solar System Exploration Division, NASA, Goddard Space Flight Center, Greenbelt, MD 20771, USA. paul.r.mahaffy@nasa.gov
Resumen
El orbitador Cassini fue lanzado.
Área de la Ciencia:
- Ciencias planetarias Ciencias planetarias.
- Química de la atmósfera La química de la atmósfera
- Física del plasma es la física del plasma.
Sus antecedentes:
- Titán, la luna más grande de Saturno, posee una densa atmósfera de nitrógeno.
- La atmósfera de Titán es lo suficientemente fría como para precipitar metano, impulsando la química de hidrocarburos y nitrilo.
- Esta química produce la neblina naranja característica de Titán.
Objetivo del estudio:
- Para analizar los datos del primer sobrevuelo de la Cassini Orbiter por la atmósfera superior de Titán.
- Para investigar el campo magnético y el entorno de plasma de Titán.
- Para revelar nuevos conocimientos sobre la dinámica atmosférica, la química y la geología de la superficie de Titán.
Principales métodos:
- Recopilación de datos de sobrevuelo de naves espaciales por el Orbitador Cassini.
Principales resultados:
- Se obtuvieron nuevos datos sobre el campo magnético y el entorno de plasma de Titán.
- Se revelaron nuevos aspectos de la dinámica atmosférica y la química de Titán.
- Las observaciones iniciales sugieren una superficie compleja, geológicamente joven, formada por procesos fluidos.
Conclusiones:
- El primer sobrevuelo de la Cassini sobre Titán proporcionó datos cruciales sobre su atmósfera y su entorno.
- Las condiciones atmosféricas únicas de Titán apoyan procesos químicos y geológicos complejos.
- La Luna exhibe características de un mundo dinámico y geológicamente activo.

