File:B324 Pan-STARRS.jpg
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This is a file from the Wikimedia Commons. The description on its description page there is shown below.
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Summary
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English: This image shows the luminous YHG B324 located in the Triangulum Galaxy 2.7 million light years away. |
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| Source | https://ps1images.stsci.edu/cgi-bin/ps1cutouts?pos=01%3A33%3A55.93272+%2B30%3A45%3A30.4452&filter=color&filter=g&filter=r&filetypes=stack&auxiliary=data&size=400&output_size=1024&verbose=0&autoscale=99.500000&catlist= |
| Author | The Pan-STARRS1 Surveys (PS1) and the PS1 public science archive have been made possible through contributions by the Institute for Astronomy, the University of Hawaii, the Pan-STARRS Project Office, the Max-Planck Society and its participating institutes, the Max Planck Institute for Astronomy, Heidelberg and the Max Planck Institute for Extraterrestrial Physics, Garching, The Johns Hopkins University, Durham University, the University of Edinburgh, the Queen's University Belfast, the Harvard-Smithsonian Center for Astrophysics, the Las Cumbres Observatory Global Telescope Network Incorporated, the National Central University of Taiwan, the Space Telescope Science Institute, the National Aeronautics and Space Administration under Grant No. NNX08AR22G issued through the Planetary Science Division of the NASA Science Mission Directorate, the National Science Foundation Grant No. AST-1238877, the University of Maryland, Eotvos Lorand University (ELTE), the Los Alamos National Laboratory, and the Gordon and Betty Moore Foundation. |
Licensing
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This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.) |  |
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| Date/Time | Dimensions | User | Comment | |
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| current | 06:57, 26 November 2023 | 1,024 × 1,024 (100 KB) | Diamantinasaurus | Uploaded a work by The Pan-STARRS1 Surveys (PS1) and the PS1 public science archive have been made possible through contributions by the Institute for Astronomy, the University of Hawaii, the Pan-STARRS Project Office, the Max-Planck Society and its participating institutes, the Max Planck Institute for Astronomy, Heidelberg and the Max Planck Institute for Extraterrestrial Physics, Garching, The Johns Hopkins University, Durham University, the University of Edinburgh, the Queen's University... |
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