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Myriad of Stars in Spiral Galaxy NGC 300


What appear as individual grains of sand on a beach in the image obtained with NASA's Hubble Space Telescope are actually myriads of stars embedded deep in the heart of the nearby galaxy NGC 300. The Hubble telescope's exquisite resolution enables it to see the stars as individual points of light, despite the fact that the galaxy is millions of light-years away. NGC 300 is a spiral galaxy much like our own Milky Way galaxy. It is a member of a nearby group of galaxies known as the Sculptor group, named for the southern constellation where they can be found. The distance to NGC 300 is 6.5 million light-years making it one of the Milky Way's closer neighbors. At this distance the brightest individual stars can be picked out even from ground-based images. With a resolution some 10 times better than ground-based telescopes, Hubble's Advanced Camera for Surveys ACS) resolves many more stars in this galaxy than have ever been seen before.



The color composite was made from filtered images taken in blue, green, and infrared light. Hot, young blue stars appear in clusters that form in the galaxy's spiral arms. Ribbons of deep red stars mark the location of gauzy curtains of dust that partially hide the light of the stars behind them. Near the center of the image is the bright and compact nucleus of the galaxy where even the ACS loses the ability to separate the densely packed stars.


Credit: NASA, ESA, and The Hubble Heritage Team (AURA/STScI)

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