File:Gravitational Lens in Galaxy Cluster AC 114 (1992-25-79).tiff
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DescriptionGravitational Lens in Galaxy Cluster AC 114 (1992-25-79).tiff |
English: The NASA Hubble Space Telescope photograph (left) shows a pair of L-shaped images with striking mirror-symmetry. These are thought to arise from a very distant galaxy seen through a cluster of foreground galaxies (right). The gravity of the galaxy cluster acts as a natural magnifying glass, bending and focusing the light of the more distant source into several images, each of which is apparently larger and brighter than would otherwise be the case. This rare combination of Hubble's powerful telescope mirrors and the natural telephoto lens gives astronomers unprecedented information on the nature of very distant galaxies, and on the distribution and nature of matter in the foreground cluster. The two compact objects in the center of the HST image are thought to be unrelated galaxies in the foreground cluster. |
Date | 8 October 1992 (upload date) |
Source | Gravitational Lens in Galaxy Cluster AC 114 |
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Public domainPublic domainfalsefalse |
This file is in the public domain because it was created by NASA and ESA. NASA Hubble material (and ESA Hubble material prior to 2009) is copyright-free and may be freely used as in the public domain without fee, on the condition that only NASA, STScI, and/or ESA is credited as the source of the material. This license does not apply if ESA material created after 2008 or source material from other organizations is in use. The material was created for NASA by Space Telescope Science Institute under Contract NAS5-26555, or for ESA by the Hubble European Space Agency Information Centre. Copyright statement at hubblesite.org or 2008 copyright statement at spacetelescope.org. For material created by the European Space Agency on the spacetelescope.org site since 2009, use the {{ESA-Hubble}} tag. |
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Horizontal resolution | 2,700 dpi |
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Data arrangement | chunky format |