File:Caldwell 23 - 2.jpg
原始文件 (3,847 × 3,995像素,文件大小:17.94 MB,MIME类型: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 | |
来源 | https://www.flickr.com/photos/144614754@N02/49164938063/ |
作者 | NASA Hubble |
许可协议
这幅图片原始出处为Flickr的https://flickr.com/photos/144614754@N02/49164938063 ,作者为NASA Hubble 。经机器人FlickreviewR 2在2020年2月23日审查后确定为采用cc-by-2.0的协议授权使用。 |
2020年2月23日
某些值没有维基数据项目
14 5 2012
image/jpeg
18,809,716 字节
3,995 像素
3,847 像素
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数据生成日期时间 | 2012年5月14日 (一) 10:00 |
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简短标题 | Edge-on beauty |
提供者 | ESA/Hubble & NASA Acknowledgemen |
来源 | ESA/Hubble |
图像标题 | 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 |
使用条款 |
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JPEG文件备注 | 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. |
方向 | 正常 |
水平分辨率 | 72 dpi |
垂直分辨率 | 72 dpi |
使用软件 | Adobe Photoshop CS5 Windows |
文件修改日期时间 | 2012年2月13日 (一) 16:18 |
YCbCr位置 | 中间 |
Exif版本 | 2.31 |
数字化日期时间 | 2012年1月30日 (一) 22:27 |
每个色彩组分意义 |
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支持的Flashpix版本 | 1 |
色彩空间 | 未标定 |
IIM版本 | 4 |
关键词 | NGC 891 |
每色彩组分位数 |
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高度 | 3,995 px |
宽度 | 3,847 px |
像素构成 | RGB |
色彩组分数 | 3 |
联系信息 |
-{R|http://www.spacetelescope.org/}- Karl-Schwarzschild-Strasse 2 Garching bei München, , D-85748 Germany |
媒体文件类型 | Observation |
元数据最后修改日期 | 2012年2月13日 (一) 17:18 |
原始文件唯一ID | uuid:C26DB2EB884BE11180F4ED18AB6954A9 |
著作权状况 | 著作权状况未设置 |