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News Release 142 of 964

January 11, 2012 10:45 AM (EST)

News Release Number: STScI-2012-04

Hubble Zooms in on Double Nucleus in Andromeda Galaxy

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Image: Hubble Zooms in on Double Nucleus in Andromeda Galaxy

Hubble Zooms in on Double Nucleus in Andromeda GalaxySTScI-PRC2012-04

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ABOUT THIS IMAGE:

A new Hubble Space Telescope image centers on the 100-million-solar-mass black hole at the hub of the neighboring spiral galaxy M31, or the Andromeda galaxy, one of the few galaxies outside the Milky Way visible to the naked eye and the only other giant galaxy in the Local Group.

This is the sharpest visible-light image ever made of the nucleus of an external galaxy.

The event horizon, the closest region around the black hole where light can still escape, is too small to be seen, but it lies near the middle of a compact cluster of blue stars at the center of the image. The compact cluster of blue stars is surrounded by the larger "double nucleus" of M31, discovered with the Hubble Space Telescope in 1992. The double nucleus is actually an elliptical ring of old reddish stars in orbit around the black hole but more distant than the blue stars. When the stars are at the farthest point in their orbit they move slower and give the illusion of a second nucleus.

The blue stars surrounding the black hole are no more than 200 million years old, and therefore must have formed near the black hole in an abrupt burst of star formation. Massive blue stars are so short-lived that they would not have enough time to migrate to the black hole if they were formed elsewhere.

Astronomers are trying to understand how apparently young stars were formed so deep inside the black hole's gravitational grip and how they survive in an extreme environment.

The fact that young stars are also closely bound to the central black hole in our Milky Way galaxy suggests this may be a common phenomenon in spiral galaxies.

Tod R. Lauer of the National Optical Astronomy Observatory in Tucson, Ariz., assembled this image of the nuclear region by taking several blue and ultraviolet light exposures of the nucleus with Hubble's Advanced Camera for Surveys high-resolution channel during September 2005 and February 2006, each time slightly moving the telescope to change how the camera sampled the region. By combining these pictures, he was able to construct an ultra-sharp view of the galaxy's core.

Lauer is presenting these Hubble observations today at the meeting of the American Astronomical Society in Austin, Texas.

The image of the Andromeda galaxy was taken on Jan. 13, 2001, with the WIYN/KPNO 0.9-meter Mosaic I by T. Rector and B. Wolpa of the National Optical Astronomy Observatory in Tucson, Ariz.

For more information, contact:

Ray Villard
Space Telescope Science Institute, Baltimore, Md.
410-338-4514
villard@stsci.edu

Tod R. Lauer
National Optical Astronomy Observatory, Tucson, Ariz. 5
20-318-8290
lauer@noao.edu

Object Names: M31, NGC 224, Andromeda Galaxy

Image Type: Astronomical/Annotated

Hubble Image Credit: NASA, ESA, and T. Lauer (National Optical Astronomy Observatory)

NEWS RELEASE IMAGES

The above montage includes these images:

Center of M31 Image Type: Astronomical Center of M31 Ground-based Image of Andromeda Galaxy, M31 Image Type: Astronomical/Annotated Ground-based Image of Andromeda Galaxy, M31

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