File:Caldwell 23 - 2.jpg
原始檔案 (3,847 × 3,995 像素,檔案大小:17.94 MB,MIME 類型:image/jpeg)
摘要
描述Caldwell 23 - 2.jpg |
English: If we could travel across space and time to see our own galaxy from the outside looking in, it would probably look a lot like Caldwell 23. This spiral galaxy, also cataloged as NGC 891, is about 35 million light-years away from Earth in the constellation Andromeda. Sir Patrick Moore, creator of the Caldwell catalog, once said the full galaxy looks like “two fried eggs clapped back to back.” In this Hubble image, taken in visible and infrared light using the Advanced Camera for Surveys, the “yolk” portion of the galaxy is out of the picture beyond the lower left corner. A few foreground stars from the Milky Way shine brightly, while more-distant galaxies can be seen in the lower right corner of the image.
Astronomers used Hubble’s observations of Caldwell 23 to learn more about the structure and evolution of spiral galaxies. One of their findings helped identify the source of Caldwell 23’s galactic “halo.” The halo surrounds the galaxy and primarily contains old stars, some of which are grouped together in large, sphere-shaped collections called globular clusters. The source of this halo material has been unclear, since theoretically it could either originate in the galaxy or be gravitationally pulled in from the area surrounding the galaxy. Scientists using Hubble found that Caldwell 23’s halo is similar in composition to other material in the galaxy, which suggests that the halo material was expelled from within the galaxy. This Hubble image shows wispy tendrils of dust and gas branching off from the plane of the galaxy into the halo. Astronomers believe these structures formed as material was ejected outward by supernovae or intense star formation activity. When massive stars light up at birth or explode at death, they produce powerful winds that can blow dust and gas over hundreds of light-years of space. Caldwell 23 was discovered by astronomer William Herschel in October 1784. The galaxy has a magnitude of 10, so use a telescope to see it, away from any sources of light pollution. Under ideal conditions you can make out the galaxy’s central dark lane. Autumn night skies in the Northern Hemisphere will provide the best view. In the Southern Hemisphere, look for Caldwell 23 in the springtime. For more information about Hubble’s observations of Caldwell 23, see: www.spacetelescope.org/images/potw1220a/ hubblesite.org/contents/news-releases/1999/news-1999-10.html Credit: ESA/Hubble & NASA; Acknowledgement: Nick Rose For Hubble's Caldwell catalog site and information on how to find these objects in the night sky, visit: www.nasa.gov/content/goddard/hubble-s-caldwell-catalog |
日期 | |
來源 | https://www.flickr.com/photos/144614754@N02/49164938063/ |
作者 | NASA Hubble |
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這幅圖片原始出處為Flickr的https://flickr.com/photos/144614754@N02/49164938063 ,作者為NASA Hubble 。經機器人FlickreviewR 2在2020年2月23日審查後確定為採用cc-by-2.0的協議授權使用。 |
2020年2月23日
沒有維基數據項目的某些值
創用CC姓名標示2.0通用版 繁體中文 (已轉換拼寫)
14 5 2012
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18,809,716 位元組
3,995 像素
3,847 像素
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目前 | 2020年2月23日 (日) 20:05 | 3,847 × 3,995(17.94 MB) | Killarnee | User created page with UploadWizard |
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詮釋資料
此檔案中包含其他資訊,這些資訊可能是由數位相機或掃描器在建立或數位化過程中所新增的。若檔案自原始狀態已被修改,一些詳細資料可能無法完整反映出已修改的檔案。
資料產生的日期時間 | 2012年5月14日 (一) 10:00 |
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簡稱 | Edge-on beauty |
製作/提供者 | ESA/Hubble & NASA Acknowledgemen |
來源 | ESA/Hubble |
影像標題 | Visible in the constellation of Andromeda, NGC 891 is located approximately 30 million light-years away from Earth. The NASA/ESA Hubble Space Telescope turned its powerful wide field Advanced Camera for Surveys towards this spiral galaxy and took this close-up of its northern half. The galaxy's central bulge is just out of the image on the bottom left. The galaxy, spanning some 100 000 light-years, is seen exactly edge-on, and reveals its thick plane of dust and interstellar gas. While initially thought to look like our own Milky Way if seen from the side, more detailed surveys revealed the existence of filaments of dust and gas escaping the plane of the galaxy into the halo over hundreds of light-years. They can be clearly seen here against the bright background of the galaxy halo, expanding into space from the disc of the galaxy. Astronomers believe these filaments to be the result of the ejection of material due to supernovae or intense stellar formation activity. By lighting up when they are born, or exploding when they die, stars cause powerful winds that can blow dust and gas over hundreds of light-years in space. A few foreground stars from the Milky Way shine brightly in the image, while distant elliptical galaxies can be seen in the lower right of the image. NGC 891 is part of a small group of galaxies bound together by gravity. A version of this image was entered into the Hubble’s Hidden Treasures Image Processing Competition by contestant Nick Rose. Hidden Treasures is an initiative to invite astronomy enthusiasts to search the Hubble archive for stunning images that have never been seen by the general public. |
出版商 | ESA/Hubble |
使用條款 |
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JPEG 檔案備註 | Visible in the constellation of Andromeda, NGC 891 is located approximately 30 million light-years away from Earth. The NASA/ESA Hubble Space Telescope turned its powerful wide field Advanced Camera for Surveys towards this spiral galaxy and took this close-up of its northern half. The galaxy's central bulge is just out of the image on the bottom left. The galaxy, spanning some 100 000 light-years, is seen exactly edge-on, and reveals its thick plane of dust and interstellar gas. While initially thought to look like our own Milky Way if seen from the side, more detailed surveys revealed the existence of filaments of dust and gas escaping the plane of the galaxy into the halo over hundreds of light-years. They can be clearly seen here against the bright background of the galaxy halo, expanding into space from the disc of the galaxy. Astronomers believe these filaments to be the result of the ejection of material due to supernovae or intense stellar formation activity. By lighting up when they are born, or exploding when they die, stars cause powerful winds that can blow dust and gas over hundreds of light-years in space. A few foreground stars from the Milky Way shine brightly in the image, while distant elliptical galaxies can be seen in the lower right of the image. NGC 891 is part of a small group of galaxies bound together by gravity. A version of this image was entered into the Hubble’s Hidden Treasures Image Processing Competition by contestant Nick Rose. Hidden Treasures is an initiative to invite astronomy enthusiasts to search the Hubble archive for stunning images that have never been seen by the general public. |
方位 | 標準 |
水平解析度 | 72 dpi |
垂直解析度 | 72 dpi |
使用軟體 | Adobe Photoshop CS5 Windows |
檔案修改日期時間 | 2012年2月13日 (一) 16:18 |
亮度與彩度位置 | 中間 |
Exif 版本 | 2.31 |
數位化的日期時間 | 2012年1月30日 (一) 22:27 |
每像素內含 |
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支援的 Flashpix 版本 | 1 |
色彩空間 | 顏色未校準 |
IIM 版本 | 4 |
關鍵字 | NGC 891 |
每像素位元 |
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高度 | 3,995 px |
寬度 | 3,847 px |
像素合成 | RGB |
像素數量 | 3 |
聯絡資訊 |
http://www.spacetelescope.org/ Karl-Schwarzschild-Strasse 2 Garching bei München, , D-85748 Germany |
媒體類型 | Observation |
詮釋資料最後修改日期 | 2012年2月13日 (一) 17:18 |
原始文件唯一識別碼 | uuid:C26DB2EB884BE11180F4ED18AB6954A9 |
版權狀態 | 版權狀態不明 |