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Center of the Andromede Galaxy (M31) - Center of the Andromeda galaxy - The Andromede...

IMAGE number
PIX4608823
Image title
Center of the Andromede Galaxy (M31) - Center of the Andromeda galaxy - The Andromede galaxy is located about 2 million years ago - light from Earth. Like the lactee path, the Andromede galaxy belongs to the local group. This image obtained from the 2.5m Isaac Newton telescope of La Palma shows the nucleus of the galaxy. This nucleus is double, probably the vestige of a collision with another galaxy. At the heart of the nearby spiral galaxy M31 is a tiny, bright nucleus, seen to be slightly elongated on this colour picture. Hubble Space Telescope pictures show the nucleus to be a double structure, possibly the remains of the nucleus of another galaxy which has now been almost completely absorbed in M31. Around the binary nucleus swirls a huge cloud of mostly old, faint stars. This not only reveals the inner nucleus but also shows traces of dust which seem to stream into the bright central part of the galaxy. Studies of the stars around the nucleus strongly suggest that at the heart of M31 there lurks a black hole, accelerating stars close to it to abnormally high velocities. Similar effects are seen in the Milky Way, but in our galaxy the nucleus is hidden at optical wavelengths, so observations are made in the infrared and at radio wavelengths
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Image description

Center of the Andromede Galaxy (M31) - Center of the Andromeda galaxy - The Andromede galaxy is located about 2 million years ago - light from Earth. Like the lactee path, the Andromede galaxy belongs to the local group. This image obtained from the 2.5m Isaac Newton telescope of La Palma shows the nucleus of the galaxy. This nucleus is double, probably the vestige of a collision with another galaxy. At the heart of the nearby spiral galaxy M31 is a tiny, bright nucleus, seen to be slightly elongated on this colour picture. Hubble Space Telescope pictures show the nucleus to be a double structure, possibly the remains of the nucleus of another galaxy which has now been almost completely absorbed in M31. Around the binary nucleus swirls a huge cloud of mostly old, faint stars. This not only reveals the inner nucleus but also shows traces of dust which seem to stream into the bright central part of the galaxy. Studies of the stars around the nucleus strongly suggest that at the heart of M31 there lurks a black hole, accelerating stars close to it to abnormally high velocities. Similar effects are seen in the Milky Way, but in our galaxy the nucleus is hidden at optical wavelengths, so observations are made in the infrared and at radio wavelengths

Photo credit
Photo © IAC/RGO/David Malin Images/Novapix / Bridgeman Images
Image keywords
astronomy / kernel / star / astronomy / galaxy / spiral galaxy / palma / star / Novapix / astronomy / galaxy / nucleus / andromeda / andromede / Galaxy Spiral / m31 / Ngc 224

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Largest available format 2646 × 3307 px 2 MB
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