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The Satellite Cluster, C50 // Serge Sankov
In the heart of the Rosette Nebula lies the Satellite Cluster (NGC 2244). This is an extremely young star cluster at only 5 million years old. The brightest stars among them, over 400,000 times brighter than the Sun, are responsible for lighting up the gas around them.
La nebulosa Roseta es una región H II grande y circular, ubicada en el borde de una gigantesca nube molecular en la constelación del Unicornio, situada en la banda de la Vía Láctea. El cúmulo abierto NGC 2244 (Caldwell 50) está estrechamente asociado con la nebulosa, en virtud de que las estrellas del cúmulo se han formado de la materia de la misma.
The Rosette Nebula (also known as Caldwell 49) is a large spherical ionized atomic hhydrogen region (H II region) that is circular in appearance and located near one end of a giant molecular cloud in the Monoceros region of the Milky Way Galaxy. The open cluster NGC 2244 (Caldwell 50) is closely associated with the nebulosity, the stars of the cluster having been formed from the nebula’s matter…
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