File:Artist’s impression of the active galactic nucleus of Messier 77 (eso2203d).jpg
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Summary[edit]
DescriptionArtist’s impression of the active galactic nucleus of Messier 77 (eso2203d).jpg |
English: This illustration shows what the core of Messier 77 might look like. As other active galactic nuclei, the central region of Messier 77 is powered by a black hole that is surrounded by a thin accretion disc, which itself is surrounded by a thick ring or torus of gas and dust. In the case of Messier 77, this thick ring completely obscures our view of the supermassive black hole. This active galactic nucleus is also believed to have jets, as well as dusty winds, that flow out of the region around the black hole perpendicularly to the accretion disc around it. |
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Date | 16 February 2022 (upload date) | ||
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Author | ESO/M. Kornmesser and L. Calçada | ||
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Licensing[edit]
This media was created by the European Southern Observatory (ESO).
Their website states: "Unless specifically noted, the images, videos, and music distributed on the public ESO website, along with the texts of press releases, announcements, pictures of the week, blog posts and captions, are licensed under a Creative Commons Attribution 4.0 International License, and may on a non-exclusive basis be reproduced without fee provided the credit is clear and visible." To the uploader: You must provide a link (URL) to the original file and the authorship information if available. | |
This file is licensed under the Creative Commons Attribution 4.0 International license.
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 17:13, 20 August 2023 | 5,000 × 3,438 (2.5 MB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://cdn.eso.org/images/large/eso2203d.jpg via Commons:Spacemedia |
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Metadata
This file contains additional information such as Exif metadata which may have been added by the digital camera, scanner, or software program used to create or digitize it. If the file has been modified from its original state, some details such as the timestamp may not fully reflect those of the original file. The timestamp is only as accurate as the clock in the camera, and it may be completely wrong.
Credit/Provider | ESO/M. Kornmesser and L. Calçada |
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Source | European Southern Observatory |
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Date and time of data generation | 17:00, 16 February 2022 |
Software used | Adobe Photoshop 22.5 (20210825.orig.371 f9e5e2d) (Windows) |
File change date and time | 18:07, 27 January 2022 |
Date and time of digitizing | 19:05, 27 January 2022 |
Date metadata was last modified | 19:07, 27 January 2022 |
Unique ID of original document | xmp.did:288de469-4bf4-224a-b4c2-352e5f649d7d |
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Contact information |
Karl-Schwarzschild-Strasse 2 Garching bei München, None, D-85748 Germany |
IIM version | 4 |