Celestial hemisphere:  Northern  ·  Constellation: Coma Berenices (Com)  ·  Contains:  HD111813  ·  NGC 4725
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NGC 4725, Ron Stanley
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NGC 4725

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NGC 4725, Ron Stanley
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NGC 4725

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Description

NGC 4725 is a barred spiral galaxy located about 40 million light-years away in the constellation Coma Berenices. Unlike our Milky Way galaxy with multiple spiral arms, NGC 4725 has a unique structure with only one prominent arm winding out from a central ring. This single arm is packed with young, blue star clusters and reddish star-forming regions, while the yellowish central bar features an older stellar population.

This galaxy is classified as an intermediate spiral due to its arm structure and the presence of a weak to moderate bar. Interestingly, NGC 4725 is also considered a double-barred spiral, a characteristic shared by roughly a third of all barred spirals. The galactic disk is tilted at an angle of 46 degrees relative to our line of sight, offering us a good view of its internal structure.

At the heart of NGC 4725 lies a bright nucleus, suspected to harbor a supermassive black hole. This galactic center is likely quite active, influencing the galaxy's environment and potentially contributing to the warping observed in its spiral arm. NGC 4725 is the brightest member of the Coma I Group, a collection of galaxies within the Coma-Sculptor Cloud. However, it's relatively isolated from its neighbors, adding to its unique characteristics. Astronomers believe NGC 4725 might be interacting with another nearby spiral galaxy, NGC 4747, which could explain some of the distortions observed in its structure.

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NGC 4725, Ron Stanley