Archivo de imágenes de Hubble
Abell 1689 Hubble ACS/WFC
CreditsNASA, ESA, E. Jullo (Jet Propulsion Laboratory), P. Natarajan (Yale University), and J.-P. Kneib (Laboratoire d'Astrophysique de Marseille, CNRS, France); Acknowledgment: H. Ford and N. Benitez (Johns Hopkins University), and T. Broadhurst (Tel Aviv University)
- Fecha
- Jan 1, 2010
- Misión
- Hubble Space Telescope
- ID de archivo
- hubblesite-images-2010-26-2758-image
Credits
NASA, ESA, E. Jullo (Jet Propulsion Laboratory), P. Natarajan (Yale University), and J.-P. Kneib (Laboratoire d'Astrophysique de Marseille, CNRS, France);Acknowledgment: H. Ford and N. Benitez (Johns Hopkins University), and T. Broadhurst (Tel Aviv University)
Detalles de la imagen
| About The Object | |
|---|---|
| Object Name | Abell 1689 |
| Object Description | Galaxy Cluster |
| R.A. Position | 13h 11m 29.5s |
| Dec. Position | -1° 20' 17.01" |
| Constellation | Virgo |
| Distance | The distance to the lensing cluster is 2.2 billion light-years (675 megaparsecs). The distance to the lensed galaxy is about 12.8 billion light-years. |
| About The Data | |
| Data Description | ACS/WFC data of Abell 1689 were observed with the HST proposal : H. Ford and N. Benitez (Johns Hopkins University), and T. Broadhurst (Tel Aviv University). The science team for this release includes: E. Jullo (Jet Propulsion Laboratory), P. Natarajan (Yale University), J.-P. Kneib (Laboratoire d'Astrophysique de Marseille, CNRS, France), A. D'Aloisio (Yale University), M. Limousin (Laboratoire d'Astrophysique de Marseille and University of Copenhagen, Denmark), J. Richard (Durham University, U.K.), and C. Schimd (Laboratoire d'Astrophysique de Marseille, CNRS, France). |
| Instrument | HST>ACS/WFC |
| Exposure Dates | June 12-21, 2002, Exposure Time: 10.5 hours |
| Filters | F475W (g) F775W (i) F850LP (z) |
| About The Image | |
| Color Info | Blue: F475W (g) Green: F775W (i) Red: F850LP (z) |
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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
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