File:NGC 4861 - HST- Potw1704a.tif
![File:NGC 4861 - HST- Potw1704a.tif](https://upload.wikimedia.org/wikipedia/commons/thumb/e/ee/NGC_4861_-_HST-_Potw1704a.tif/lossy-page1-750px-NGC_4861_-_HST-_Potw1704a.tif.jpg?20170123113607)
原始文件 (3,885 × 3,107像素,文件大小:69.11 MB,MIME类型:image/tiff)
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[编辑]描述NGC 4861 - HST- Potw1704a.tif |
English: The lesser-known constellation of Canes Venatici (The Hunting Dogs), is home to a variety of deep-sky objects — including this beautiful galaxy, known as NGC 4861. Astronomers are still debating on how to classify it: While its physical properties — such as mass, size and rotational velocity — indicate it to be a spiral galaxy, its appearance looks more like a comet with its dense, luminous “head” and dimmer “tail” trailing behind. Features more fitting with a dwarf irregular galaxy.
Although small and messy, galaxies like NGC 4861 provide astronomers with interesting opportunities for study. Small galaxies have lower gravitational potentials, which simply means that it takes less energy to move stuff about inside them than it does in other galaxies. As a result, moving in, around, and through such a tiny galaxy is quite easy to do, making them far more likely to be suffused with streams and outflows of speedy charged particles known as galactic winds, which can flood such galaxies with little effort. These galactic winds can be powered by the ongoing process of star formation, which involves huge amounts of energy. New stars are springing into life within the bright, colourful ‘head’ of NGC 4861 and ejecting streams of high-speed particles as they do so, which flood outwards to join the wider galactic wind. While NGC 4861 would be a perfect candidate to study such winds, recent studies did not find any galactic winds in it. Credit: ESA/Hubble & NASA Coordinates Position (RA): 12 59 2.76 Position (Dec): 34° 51' 46.80" Field of view: 3.24 x 2.59 arcminutes Orientation: North is 80.3° right of vertical Colours & filters Band Wavelength Telescope Optical V 606 nm Hubble Space Telescope ACS Optical V 606 nm Hubble Space Telescope ACS Optical I 814 nm Hubble Space Telescope ACS Optical NII 658 nm Hubble Space Telescope WFC3 Optical SII 673 nm Hubble Space Telescope WFC3 Optical I 814 nm Hubble Space Telescope ACS. |
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来源 | http://spacetelescope.org/images/potw1704a/ http://spacetelescope.org/static/archives/images/original/potw1704a.tif |
作者 | Credit: ESA/Hubble & NASA |
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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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宽度 | 3,885 px |
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高度 | 3,107 px |
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压缩方案 | 未压缩 |
像素构成 | RGB |
图像数据位置 | 27,030 |
方向 | 正常 |
色彩组分数 | 3 |
每带行数 | 3,107 |
每压缩带字节数 | 72,424,170 |
水平分辨率 | 72 dpi |
垂直分辨率 | 72 dpi |
数据排布 | 大块格式 |
使用软件 | Adobe Photoshop CC 2015 (Windows) |
文件修改日期时间 | 2016年7月22日 (五) 12:34 |
色彩空间 | 未标定 |