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Hubble observes a dwarf galaxy with a bright nebula
The starry mist streaking across this image obtained by the Hubble Space Telescope is the central part of the dwarf galaxy known as NGC 2366. The most obvious feature in this galaxy is a large nebula visible in the upper-left part of the image, called NGC 2363.
The nearby yellowish swirl is not in fact part of the nebula. It is a spiral galaxy much further away, whose light is shining right through NGC 2366. This is possible because galaxies are not solid objects. While we see the stars because they shine brightly, galaxies are overwhelmingly made up of the empty space between them.
Due to the burst of star formation that the galaxy has undergone in recent cosmic time, NGC 2366 is home to numerous gigantic blue stars. A new generation of these stellar titans has lit up the nebula NGC 2363 as their ultraviolet radiation excites the hydrogen gas. Imaged through green and infrared filters, the nebula take on a blueish tinge in this image, though the actual colour is a shade of red.
The splendid interconnected objects of NGC 2366 and NGC 2363 are located about 10 million light-years away in the constellation of Camelopardalis.
