Файл:Hubble explores explosive aftermath in NGC 298 (potw2322a).jpg
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Цуьнах лаьцнаHubble explores explosive aftermath in NGC 298 (potw2322a).jpg |
English: The spiral galaxy NGC 298 basks in this image from the NASA/ESA Hubble Space Telescope. NGC 298 lies around 89 million light-years away in the constellation Cetus, and appears isolated in this image — only a handful of distant galaxies and foreground stars accompany the lonely galaxy. While NGC 298 seems peaceful, in 1986 it was host to one of astronomy's most extreme events: a catastrophic stellar explosion known as a Type II supernova. Hubble’s Advanced Camera for Surveys captured NGC 298 as part of an investigation into the origins of Type II supernovae. All Type II supernovae are produced by the collapse and subsequent explosion of young, massive stars, but they can produce a spectacular diversity of brightnesses and spectral features. Astronomers suspect that the diversity of this cosmic firework show might be due to gas and dust being stripped from the stars that will eventually produce Type II supernovae. Observing the region surrounding supernova explosions can reveal traces of the progenitor star’s history preserved in this lost mass, as well as revealing any companion stars that survived the supernova. Hubble used the brief periods between scheduled observations to explore the aftermath of a number of Type II supernovae, hoping to piece together the relationship between Type II supernovae and the stellar systems which give rise to them.[Image description: A spiral galaxy. It is tilted diagonally, and slightly towards the viewer, making its core and disc separately visible. Its disc is speckled by small stars, has threads of dark reddish dust and bubbles of bright, glowing gas. The core shines brightly in a warmer colour. Several tiny stars and small galaxies are included in the black background.] |
Терахь | шeран 29 май (дата загрузки) |
Хьост | Hubble explores explosive aftermath in NGC 298 |
Автор | ESA/Hubble & NASA, C. Kilpatrick |
Кхин версеш |
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Лицензи
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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3694 пиксель
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3 483 833 байт
контрольная сумма оьрсийн
892515269110291c48078f16de4c4dd1e8d47dc4
29 май 2023
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Терахь/Хан | Жима | Файлан барам | Декъашхо | Билгалдаккхар | |
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карара | 2023, 29 май, 04:46 | 3694 × 2865 (3,32 Мб) | OptimusPrimeBot | #Spacemedia - Upload of https://cdn.spacetelescope.org/archives/images/large/potw2322a.jpg via Commons:Spacemedia |
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Хьост | ESA/Hubble |
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Кхоьхьург, хьа делла сурт | ESA/Hubble & NASA, C. Kilpatrick |
Йоцца цӀе |
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Суьртан цӏе |
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Лелоран биллам |
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Оригиналан терахь а, хан а | 2023, 29 май, 06:00 |
JPEG-файлан билгалдаккхар | The spiral galaxy NGC 298 basks in the centre of this image from the NASA/ESA Hubble Space Telescope. NGC 298 lies around 89 million light-years away in the constellation Cetus, and appears isolated in this image — only a handful of distant galaxies and foreground stars accompany the lonely galaxy. While NGC 298 seems peaceful, in 1986 it was host to one of astronomy's most extreme events: a catastrophic stellar explosion known as a Type II supernova. Hubble’s Advanced Camera for Surveys captured NGC 298 as part of an investigation into the origins of Type II supernovae. All Type II supernovae are produced by the collapse and subsequent explosion of young, massive stars, but they can produce a spectacular diversity of brightnesses and spectral features. Astronomers suspect that the diversity of this cosmic firework show might be due to gas and dust being stripped from the stars that will eventually produce Type II supernovae. Observing the region surrounding supernova explosions can reveal traces of the progenitor star’s history preserved in this lost mass, as well as revealing any companion stars that survived the supernova. Hubble used the brief periods between scheduled observations to explore the aftermath of a number of Type II supernovae, hoping to piece together the relationship between Type II supernovae and the stellar systems which give rise to them. [Image description: A spiral galaxy. It is tilted diagonally, and slightly towards the viewer, making its core and disc separately visible. Its disc is speckled by small stars, has threads of dark reddish dust and bubbles of bright, glowing gas. The core shines brightly in a warmer colour. Several tiny stars and small galaxies are included in the black background.] |
Лелина программа | Adobe Photoshop 24.5 (Windows) |
Файлан хийцам бина терахь а, хан а | 2023, 26 май, 21:34 |
Оцифровк йина терахь а, хан а | 2023, 22 март, 11:28 |
ТӀаьххьара метахаамаш хийцина терахь | 2023, 26 май, 23:34 |
ДӀадолалун документан ша тайпа ID | xmp.did:b7b101fd-b26c-3e4b-877e-cb70f3914bfc |
Коьрта дешнаш | NGC 298 |
Контактан хаам |
ESA Office, Space Telescope Science Institute, 3700 San Martin Dr Baltimore, MD, 21218 United States |
Верси IIM | 4 |