File:Mini-Jet Found Near Milky Way’s Supermassive Black Hole.jpg
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DescriptionMini-Jet Found Near Milky Way’s Supermassive Black Hole.jpg |
English: Hubble has found circumstantial evidence that the black hole is still smoldering long after the earlier outburst. Hubble astronomers' evidence is like doing an archeological dig to try and peer through the interstellar pollution of dense sheets of dust and gas between Earth and the galactic center, 27,000 light-years away. Hubble photographed a bright knot of gas that has been impacted by an invisible jet from the black hole, that is merely 15 light-years from it. The black hole must have shown brilliantly billions of years ago as a quasar (quasi-stellar object), when our young galaxy was feeding on lots of infalling gas. But after all this time the black hole still goes through fits and starts, and is not ready for napping as long as there is a snack around. This image presents a composite view of X-rays, molecular gas, and warm ionized gas near the galactic center. The graphic of a translucent, vertical white fan is added to show the suggested axis of a mini-jet from the supermassive black hole at the galaxy’s heart. The orange-colored features are of glowing hydrogen gas. One such feature, at the top tip of the jet is interpreted as a hydrogen cloud that has been hit by the outflowing jet. The jet scatters off the cloud into tendrils that flow northward. Farther down near the black hole are X-ray observations of superheated gas colored blue and molecular gas in green. These data are evidence that the black hole occasionally accretes stars or gas clouds, and ejects some of the superheated material along its spin axis. |
Date | (released) |
Source | https://esahubble.org/images/opo2162a/; see also https://www.flickr.com/photos/europeanspaceagency/51738072670/ |
Author | NASA, ESA, Gerald Cecil (UNC-Chapel Hill), J. DePasquale (STScI) |
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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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This file is licensed under the Creative Commons Attribution 4.0 International license.
Attribution: NASA, ESA, Gerald Cecil (UNC-Chapel Hill), J. DePasquale (STScI)
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 18:38, 23 December 2021 | 2,678 × 3,310 (3.23 MB) | Pandreve (talk | contribs) | Uploaded a work by NASA, ESA, Gerald Cecil (UNC-Chapel Hill), J. DePasquale (STScI) from https://esahubble.org/images/opo2162a/ with UploadWizard |
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Author | Space Telescope Science Institut |
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Credit/Provider | NASA, ESA, Gerald Cecil (UNC-Chapel Hill), J. DePasquale (STScI) |
Source | ESA/Hubble |
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Date and time of data generation | 19:00, 9 December 2021 |
JPEG file comment | This is a composite of view of X-rays and warm ionized gas near the galactic center. The graphic of a translucent, vertical white fan is added to show the suggested axis of a mini-jet from the supermassive black hole at the galaxy’s heart. The orange colored features are of glowing hydrogen gas. One such feature, at the top tip of the jet is interpreted at a hydrogen cloud that has been hit by the outflowing jet. The jet scatters off the cloud into tendrils that flow northward. Farther down near the black hole are X-ray observations of superheated gas colored green and blue. These date are circumstantial evidence that the black hole occasionally accretes stars or gas clouds, and ejects some of the superheated material along its spin axis. |
Software used | Adobe Photoshop 22.4 (Macintosh) |
File change date and time | 17:18, 30 November 2021 |
Date and time of digitizing | 11:16, 2 November 2021 |
Date metadata was last modified | 12:56, 30 November 2021 |
Unique ID of original document | xmp.did:ce1e7ec5-d2b9-464b-bf03-9e966d23b8ad |
Keywords | Sgr A* |
Contact information | outreach@stsci.edu
ESA Office, Space Telescope Science Institute, 3700 San Martin Dr Baltimore, MD, 21218 United States |
IIM version | 4 |
Structured data
9 December 2021
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