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Estados Unidos – 18/Ene/2022
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La UNAM participa en un programa internacional de Cartografía de Galaxias Cercanas en el Observatorio Apache Point, conocido como “MaNGA” (Mapping Nearby Galaxies at APO), que ha mapeado aproximadamente 10 mil galaxias cercanas a la Vía Láctea en el observatorio de Nuevo México, Estados Unidos, mediante un telescopio de 2.5 metros.
Es posible gracias a programas anteriores que analizaron cientos de ellas y forma parte, junto con “MaNGA”, del Sondeo Digital del Cielo Sloan, un proyecto internacional de investigación que inició en el año 2000 auspiciado por la Fundación Alfred P. Sloan.En el proyecto participan instituciones de Estados Unidos, Gran Bretaña, Alemania, España, China, Chile y México, entre otros.
Para su funcionamiento es fundamental una sofisticada técnica llamada espectroscopía de campo integral, la cual permite estudiar objetos del espacio sobre un campo de visión bidimensional; es decir, analiza cubos con tres dimensiones: dos espaciales y una espectral, explicó el investigador del Instituto de Astronomía (IA) de la UNAM y colaborador del proyecto, Sebastián Francisco Sánchez Sánchez.
Su uso es cada vez más frecuente porque permite investigar la morfología o forma de objetos extensos y sus propiedades espectrales de manera simultánea.
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