Hubble image archive
Monster Galaxy Lacks a Bright Core
The giant elliptical galaxy in the center of this image, taken by NASA's Hubble Space Telescope, is the most massive and brightest member of the galaxy cluster Abell 2261.Spanning a little more than one million light-years, the galaxy is about 10 times the diameter of our Milky W...
- Date
- Jan 1, 2012
- Mission
- Hubble Space Telescope
- Archive ID
- hubblesite-images-2012-24-3049-image
The giant elliptical galaxy in the center of this image, taken by NASA's Hubble Space Telescope, is the most massive and brightest member of the galaxy cluster Abell 2261.
Spanning a little more than one million light-years, the galaxy is about 10 times the diameter of our Milky Way galaxy. The bloated galaxy is a member of an unusual class of galaxies with a diffuse core filled with a fog of starlight. Normally, astronomers would expect to see a concentrated peak of light around a central black hole. The Hubble observations revealed that the galaxy's puffy core, measuring about 10,000 light-years, is the largest yet seen.
The observations present a mystery, and studies of this galaxy may provide insight into how black hole behavior may shape the cores of galaxies.
Astronomers used Hubble's Advanced Camera for Surveys and Wide Field Camera 3 to measure the amount of starlight across the galaxy, dubbed A2261-BCG. Abell 2261 is located three billion light-years away.
The observations were taken March to May 2011. The Abell 2261 cluster is part of a multi-wavelength survey called the Cluster Lensing And Supernova survey with Hubble (CLASH).
Credits
Credit: NASA, ESA, M. Postman (STScI), T. Lauer (NOAO), and the CLASH teamImage Details
| About The Object | |
|---|---|
| Object Name | Abell 2261, A2261-BCG |
| Object Description | Elliptical Galaxy |
| R.A. Position | 17h 22m 28.34s |
| Dec. Position | 32° 9' 12.66" |
| Constellation | Hercules |
| Distance | 3 billion light-years (920 megaparsecs) |
| About The Data | |
| Data Description | The image was created from Hubble data from proposal : M. Postman (STScI) et al. |
| Instrument | HST>ACS/WFC, and HST>WFC3/IR |
| Exposure Dates | March - May 2011, Exposure Time: 13 hours |
| Filters | ACS/WFC: F435W (B), F475W (g), F606W (V) + F625W (r) + F775W (i), F814W (I), and F850LP (z); WFC3/IR: F105W (Y), F110W (YJ), F125W (J), F140W (JH), and F160W (H) |
| About The Image | |
| Color Info | This image is a composite of separate exposures acquired by the ACS instrument. Several filters were used to sample various wavelengths. The color results from assigning different hues (colors) to each monochromatic (grayscale) image associated with an individual filter. In this case, the assigned colors are: Blue: ACS/WFC F435W (B) + F475W (g) Green: ACS/WFC F606W (V) + F625W (r) + F775W (i) Red: ACS/WFC F814W (I) + F850LP (z), WFC3/IR F105W (Y) + F110W (YJ) + F125W (J) + F140W (JH) + F160W (H) |
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Image and source material are credited to the official mission archive linked below.
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