File:R Aquarii (heic2413a).jpg
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Summary
[edit]DescriptionR Aquarii (heic2413a).jpg |
English: This image features R Aquarii, a symbiotic binary star that lies only roughly 1,000 light-years from Earth in the constellation Aquarius. This is a type of binary star system consisting of a white dwarf and a red giant that is surrounded by a large, dynamic nebula.[Image description: A bright binary star surrounded by a nebula. The star, in the centre, is a large white spot surrounded by a circular glow. It has a large, X-shaped set of diffraction spikes around it. The nebula extends far above, below, left and right of the star in long, arcing shapes made of thin, multicoloured filaments — mostly red and greenish colours, but lit in a bright cyan near the star where its light illuminates the gas.] |
Date | 16 October 2024 (upload date) |
Source | R Aquarii |
Author | NASA, ESA, M. Stute, M. Karovska, D. de Martin & M. Zamani (ESA/Hubble) |
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Licensing
[edit]ESA/Hubble images, videos and web texts are released by the ESA under the Creative Commons Attribution 4.0 International license and may on a non-exclusive basis be reproduced without fee provided they are clearly and visibly credited. Detailed conditions are below; see the ESA copyright statement for full information. For images created by NASA or on the hubblesite.org website, or for ESA/Hubble images on the esahubble.org site before 2009, use the {{PD-Hubble}} tag.
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 09:01, 17 October 2024 | 3,067 × 2,332 (2.36 MB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://cdn.esahubble.org/archives/images/large/heic2413a.jpg via Commons:Spacemedia |
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Source | ESA/Hubble |
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Credit/Provider | NASA, ESA, M. Stute, M. Karovska, D. de Martin & M. Zamani (ESA/Hubble) |
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Image title |
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Date and time of data generation | 16:00, 16 October 2024 |
Contact information |
ESA Office, Space Telescope Science Institute, 3700 San Martin Dr Baltimore, MD, 21218 United States |
Keywords | R Aqr |
IIM version | 4 |