Archivo de imágenes de Hubble
Masa del cúmulo de galaxias Abell 520 (HST WFPC2)
This image shows the location of most of the mass in merging galaxy cluster Abell 520's core, which is dominated by dark matter. Dark matter is an invisible substance that makes up most of the universe's mass. The dark-matter map was derived from Hubble Wide Field Planetary Camer...
- Fecha
- Jan 1, 2012
- Misión
- Hubble Space Telescope
- ID de archivo
- hubblesite-images-2012-10-2991-image
This image shows the location of most of the mass in merging galaxy cluster Abell 520's core, which is dominated by dark matter. Dark matter is an invisible substance that makes up most of the universe's mass. The dark-matter map was derived from Hubble Wide Field Planetary Camera 2 observations, by detecting how light from distant objects is distorted by the cluster galaxies, an effect called gravitational lensing.
Abell 520 resides 2.4 billion light-years away.
Credits
NASA, ESA, and M.J. Jee (University of California, Davis)Detalles de la imagen
| About The Object | |
|---|---|
| Object Name | Abell 520 |
| Object Description | Merging Galaxy Cluster |
| R.A. Position | 04h 54m 18.98s |
| Dec. Position | 02° 56' 48.8" |
| Constellation | Orion |
| Distance | 2.4 billion light-years (740 million parsecs) |
| About The Data | |
| Data Description | The image was created from Hubble data from proposal : J. Dalcanton (University of Washington, Seattle), A. Mahdavi (San Francisco State University), H. Hoekstra (Leiden Observatory), and A. Babul (University of Victoria, BC). The science paper is led by M.J. Jee (University of California, Davis). |
| Instrument | HST>WFPC2 |
| Filters | HST/WFPC2 F814W (I) |
| About The Image | |
| Color Info | Blue: HST/WFPC2 F814W (I) |
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Fuente
La imagen y el material de referencia se acreditan al archivo oficial de la misión enlazado a continuación.
Ver en NASA.gov