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Elliptical galaxy NGC 1275 in Perseus

IMAGE number
PIX5620129
Image title
Elliptical galaxy NGC 1275 in Perseus
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Image description

Detailed observations of NGC 1275 indicate that the dusty material belongs to a spiral system seen nearly edge - on in the foreground. The second galaxy, lying beyond the first, is actually a giant elliptical with peculiar faint spiral structure in its nucleus. These galaxies are believed to be colliding at over 6 million miles per hour. NGC 1275 is about 230 million light - years away in the constellation Perseus. Embedded in the center of a large cluster of galaxies known as the Perseus Cluster, it is also known to emit a powerful signal at both X - ray and radio frequencies. The galaxy collision causes the gas and dust already existing in the central bright galaxy to swirl into the center of the object. The X - ray and radio emission indicates the probable existence of a black hole at the bright galaxy's center. While the dark dusty material in the Hubble image falls inward, NGC 1275 displays intricate filamentary structures at a much larger scale outside the image. This is a typical feature of bright cluster galaxies

Photo credit
Photo © NASA/Hubble heritage team/Novapix / Bridgeman Images
Image keywords
astronomy / star / astronomy / giant

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Largest available format 2641 × 2674 px 1 MB
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