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About the Image
- Date
- 2007-05-28
- ID
- ssc2007-10a1
- Type
- Observation
- Credit
- NASA/JPL-Caltech/L. Jenkins (GSFC)
About the Object
- Name
- Coma Cluster
- Type
- Galaxy > Type > Elliptical
- Galaxy > Size > Giant
- Galaxy > Size > Dwarf
- Galaxy > Grouping > Cluster
- Distance
- 320,000,000 Light Years
- Redshift
- 0.231
Color Mapping
| Band | Wavelength | Telescope |
| Optical | 550 nm | SDSS |
| Optical | 700 nm | SDSS |
| Optical | 900 nm | SDSS |
| Infrared | 3.6 µm | Spitzer IRAC |
| Infrared | 4.5 µm | Spitzer IRAC |
| Infrared | 8.0 µm | Spitzer IRAC |
Astrometrics
- Position (undefined)
- RA = 13h 0m 33.5s
- Dec = 28° 5' 57.0"
- Field of View
- 41.7 x 36.2 arcminutes
- Orientation
- North is 11.8° right of vertical
- Constellation
- Coma Berenices
Dwarf Galaxies in the Coma Cluster
This mosaic of the central region of the Coma cluster combines infrared and visible-light images to reveal thousands of faint objects (green). Follow-up observations showed that many of these objects, which appear here as faint green smudges, are dwarf galaxies belonging to the cluster. Two large elliptical galaxies, NGC 4889 and NGC 4874, dominate the cluster's center. The mosaic combines visible-light data from the Sloan Digital Sky Survey (color coded blue) with long- and short-wavelength infrared views (red and green, respectively) from NASA's Spitzer Space Telescope.
Related Media
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