File:Hubble NGC1792.jpg
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Size of this preview: 611 × 600 pixels. Other resolutions: 245 × 240 pixels | 489 × 480 pixels | 783 × 768 pixels | 1,044 × 1,024 pixels | 2,087 × 2,048 pixels | 4,000 × 3,925 pixels.
Original file (4,000 × 3,925 pixels, file size: 1.33 MB, MIME type: image/jpeg)
Summary
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English: A Hubble image of galaxy NGC1792 using old data as well as newer data from 2025. |
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| Source | https://science.nasa.gov/missions/hubble/hubble-spots-a-storm-of-new-stars/ |
| Author | ESA/Hubble & NASA, D. Thilker, F. Belfiore, J. Lee and the PHANGS-HST Team |
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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Warnings:
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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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File history
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 21:16, 17 February 2026 | | 4,000 × 3,925 (1.33 MB) | wikimediacommons>BardTheRambler | Uploaded a work by ESA/Hubble & NASA, D. Thilker, F. Belfiore, J. Lee and the PHANGS-HST Team from https://science.nasa.gov/missions/hubble/hubble-spots-a-storm-of-new-stars/ with UploadWizard |
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