📍 NGC 346
➡️ 210,000 light-years
🏠 Small Magellanic Cloud
Nestled within one of our Milky Way’s closest galaxy neighbors, the Small Magellanic Cloud, the star cluster NGC 346 is home to hot stars that unleash a torrent of radiation and energetic outflows. This erodes the denser portions of gas and dust in the surrounding nebula, N66.
Dozens of hot, high-mass stars shine in NGC 346. They might look a little unusual in this new view because Hubble captured them with its unique ability to observe in ultraviolet light.
Ultraviolet light helps astronomers understand more about star formation and evolution. These specific observations were gathered to learn more about how star formation shapes the interstellar medium, which is the gas distributed throughout seemingly empty space, in a low-metallicity galaxy like the SMC.
Astronomers call any element heavier than hydrogen and helium “metals,” and the SMC contains fewer metals when compared to most parts of our Milky Way. This condition makes it an excellent example of a galaxy similar to those that existed in our early universe, when very few heavy elements were around to incorporate.
Image credit: NASA, ESA, and C. Murray (Space Telescope Science Institute); Image Processing: Gladys Kober (NASA/Catholic University of America)
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