File:Dark Matter in the Belly of the Whale - Flickr - europeanspaceagency.jpg
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Summary[edit]
DescriptionDark Matter in the Belly of the Whale - Flickr - europeanspaceagency.jpg |
This image, taken with the NASA/ESA Hubble Space Telescope, focuses on an object named UGC 695, which is located 30 million light-years away within the constellation Cetus (The Sea Monster), also known as The Whale. UGC 695 is a low-surface-brightness (LSB) galaxy. These galaxies are so faint that their brightness is less than the background brightness of Earth’s atmosphere, which makes them tricky to observe. This low brightness is the result of the relatively small number of stars within them — most of the baryonic matter in these galaxies exists in the form of huge clouds of gas and dust. The stars are also distributed over a relatively large area. LSB galaxies, like dwarf galaxies, have a high fraction of dark matter relative to the number of stars they contain. Astronomers still debate about how LSB galaxies formed in the first place. Credits: ESA/Hubble & NASA, D. Calzetti; CC BY 4.0 |
Date | Taken on 13 September 2019, 10:09 |
Source | Dark Matter in the Belly of the Whale |
Author | European Space Agency |
Flickr tags InfoField | ugc 695 , esa , european space agency , space , universe , cosmos , space science , science , space technology , tech , technology , hst , hubble space telescope , galaxy , supernova , nasa , dark matter , lsb galaxies , lsb , cetus |
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This image was originally posted to Flickr by europeanspaceagency at https://flickr.com/photos/37472264@N04/48725975902. It was reviewed on 20 August 2020 by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc-by-2.0. |
20 August 2020
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current | 00:50, 20 August 2020 | 3,113 × 2,000 (5.26 MB) | Red panda bot (talk | contribs) | In Flickr Explore: 2019-09-13 |
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Credit/Provider | ESA/Hubble & NASA, D. Calzetti |
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Source | ESA/Hubble |
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Image title |
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Date and time of data generation | 06:00, 9 September 2019 |
JPEG file comment | This image, taken with the NASA/ESA Hubble Space Telescope, focuses on an object named UGC 695, which is located 30 million light-years away within the constellation Cetus (The Sea Monster), also known as The Whale. UGC 695 is a low-surface-brightness (LSB) galaxy. These galaxies are so faint that their brightness is less than the background brightness of Earth’s atmosphere, which makes them tricky to observe. This low brightness is the result of the relatively small number of stars within them — most of the baryonic matter in these galaxies exists in the form of huge clouds of gas and dust. The stars are also distributed over a relatively large area. LSB galaxies, like dwarf galaxies, have a high fraction of dark matter relative to the number of stars they contain. Astronomers still debate about how LSB galaxies formed in the first place. |
Software used | Adobe Photoshop CC (Windows) |
Date and time of digitizing | 18:54, 11 March 2019 |
File change date and time | 12:05, 16 May 2019 |
Date metadata was last modified | 12:05, 16 May 2019 |
Unique ID of original document | xmp.did:27fea783-9828-2f4b-b701-2dc54a1b9131 |
Keywords | UGC 695 |
Contact information |
Karl-Schwarzschild-Strasse 2 Garching bei München, None, D-85748 Germany |