File:Betelgeuse radio.jpg
Betelgeuse_radio.jpg (236 × 236 pixels, file size: 6 KB, MIME type: image/jpeg)
Summary[edit | edit source]
The asymmetric structure of Betelgeuse in radio waves is likely due to activity in the outer atmosphere of the star.
Licensing[edit | edit source]
Description |
The asymmetric structure of Betelgeuse in radio waves is likely due to activity in the outer atmosphere of the star. |
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Source |
The image appears on a website entitled, "Betelgeuse (Red giant)" at url=http://hubblesite.org/explore_astronomy/black_holes/encyc_mod1_q5.html. |
Date |
31 December 2015 (upload date) |
Author |
NRAO/AUI |
Rationale |
No free use or Public Domain image known to show the asymmetric structure of Betelgeuse in radio waves is likely due to activity in the outer atmosphere of the star. Per NRAO/AUI restriction to education, teaching and research. Commons checked. |
Permission |
Fair Use |
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File history
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 23:44, 31 December 2015 | 236 × 236 (6 KB) | Marshallsumter (discuss | contribs) | The asymmetric structure of Betelgeuse in radio waves is likely due to activity in the outer atmosphere of the star. Category:Stars images |
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