File:Host Galaxies of Calcium-Rich Supernovae.jpg
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[edit]DescriptionHost Galaxies of Calcium-Rich Supernovae.jpg |
English: These Hubble Space Telescope images show elliptical galaxies with dark, wispy dust lanes, the signature of a recent galaxy merger. The dust is the only relic of a smaller galaxy that was consumed by the larger elliptical galaxy.
The "X" in the images marks the location of supernova explosions that are associated with the galaxies. Each supernova may have been gravitationally kicked out of its host galaxy by a pair of central supermassive black holes. When two galaxies merge, so do their supermassive black holes. Astronomers suggest the supernovae were stars that were once part of double-star systems. These systems wandered too close to the binary black holes, which ejected them from their galaxies. Eventually, the stars in each system moved close enough together to trigger a supernova blast. These outcast supernovae are located at various distances from their home galaxies. SN 2000ds (left) is at least 12,000 light-years from its galaxy, NGC 2768; SN 2005cz (right) is at least 7,000 light-years from its galaxy, NGC 4589. NGC 2768 resides 75 million light-years from Earth, and NGC 4589 is 108 million light-years away. The supernovae are part of a census of 13 supernovae to determine why they detonated outside the cozy confines of galaxies. The study is based on archived images made by several telescopes, including Hubble. Both galaxies were observed by Hubble's Advanced Camera for Surveys. The image of NGC 4589 was taken on Nov. 11, 2006, and the image of NGC 2768 on May 31, 2002. |
Date | |
Source | http://www.spacetelescope.org/images/opo1528a/ |
Author | NASA, ESA, and R. Foley (University of Illinois) |
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[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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current | 14:45, 15 December 2019 | 2,888 × 1,765 (1.82 MB) | BevinKacon (talk | contribs) | Cropped 4 % horizontally, 26 % vertically using CropTool with lossless mode. removing blank area | |
14:41, 15 December 2019 | 3,000 × 2,400 (1.77 MB) | BevinKacon (talk | contribs) | actual size from source | ||
08:35, 17 August 2015 | 1,280 × 1,024 (143 KB) | Jmencisom (talk | contribs) | User created page with UploadWizard |
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Credit/Provider | NASA, ESA, and R. Foley (University of Illinois) |
Source | ESA/Hubble |
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Date and time of data generation | 18:11, 14 August 2015 |
Software used | Adobe Photoshop CS6 (Macintosh) |
Unique ID of original document | xmp.did:6D60F9EED12468118083E6573332D06C |
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Contact information |
http://www.spacetelescope.org/ Karl-Schwarzschild-Strasse 2 Garching bei München, None, D-85748 Germany |
IIM version | 4 |