Facts about Pinwheel Galaxy
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Intense star formation occurs within the Pinwheel Galaxy's spiral arms, where massive young stars produce brilliant blue light and ionized hydrogen gas creates distinctive reddish H-alpha emission regions.
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Hubble Space Telescope observations revealed that the Pinwheel Galaxy's disk contains younger, bluer stars in its spiral arms compared to the older, redder stars populating its central bulge.
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The Pinwheel Galaxy's outer regions rotate at unexpectedly high speeds, suggesting the presence of substantial dark matter halos surrounding this spiral system.
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Eleven spiral arms extend from the Pinwheel Galaxy's central region, a notably high number compared to the Milky Way's typical two to four main arms.
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During the 2011 supernova SN 2011fe, the Pinwheel Galaxy brightened considerably, allowing astronomers to refine distance measurements to this nearby spiral galaxy.
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M101, the Pinwheel Galaxy's official designation, contains an estimated one trillion stars distributed across its grand design spiral structure.
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Approximately 21 million light-years away, the Pinwheel Galaxy spans roughly 170,000 light-years across, making it nearly twice the diameter of the Milky Way.