Celestial hemisphere:  Northern  ·  Constellation: Canes Venatici (CVn)  ·  Contains:  M 63  ·  NGC 5055  ·  Sunflower Galaxy
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Sunflower Galaxy, Darius Kopriva
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Sunflower Galaxy, Darius Kopriva
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Description

Messier 63, also known as the Sunflower Galaxy, is a stunning spiral galaxy located approximately 37 million light-years away from Earth in the constellation Canes Venatici. It was first discovered by the French astronomer Pierre Méchain in 1779 and later added to the Messier Catalog by Charles Messier himself.

One of the most striking features of Messier 63 is its beautiful spiral arms that resemble the pattern of a sunflower, hence its popular name. These arms are filled with numerous bright, young blue stars, which give the galaxy a vibrant appearance. The interstellar dust and gas present in the arms also create lanes of dark dust, adding further contrast to the galaxy's structure.

The Sunflower Galaxy has a relatively small and compact nucleus compared to other spiral galaxies, and it is believed to contain a supermassive black hole at its center. This black hole exerts a gravitational pull on the surrounding stars and gas, contributing to the dynamics of the galaxy.

With an apparent magnitude of around 9.3, Messier 63 is visible through amateur telescopes under dark skies. It spans approximately 100,000 light-years in diameter, making it similar in size to our Milky Way galaxy. Its proximity and relatively bright appearance make it a popular target for astrophotography enthusiasts.

Overall, Messier 63, the Sunflower Galaxy, stands out as a captivating example of a spiral galaxy, showcasing the intricate beauty of the cosmos and providing a window into the vastness of our universe.

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Sunflower Galaxy, Darius Kopriva

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Southern Hemisphere Astro