File:Caldwell 80 - 3.jpg
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Summary
[edit]DescriptionCaldwell 80 - 3.jpg |
English: This Hubble image shows off 2 million members of the biggest and brightest ball of stars in our galaxy. Caldwell 80, also known as NGC 5139 and commonly called Omega Centauri, is home to around 10 million stars. Located about 17,000 light-years away from Earth toward the Centaurus constellation, the cluster has a diameter of about 450 light-years. This image, taken with the Advanced Camera for Surveys in 2002, covers a region only about 50 light-years across.
Globular clusters like this one are spherical groups of mostly old, low-mass stars that are bound together by gravity. Omega Centauri has always been a bit of a black sheep since it has several characteristics that set it apart. In addition to it being the most massive globular cluster in our galaxy, it also includes stars of various ages, whereas other globular clusters typically contain stars from only one generation. What’s more, observations using Hubble and ground-based telescopes indicate that there is a black hole at the center of the cluster. This suggests that Omega Centauri may not be a globular cluster after all — it might actually be a dwarf galaxy that has somehow been stripped of its outer stars. Omega Centauri has been known since at least the time of the ancient astronomer Ptolemy, though he thought the cluster was a star. English astronomer Edmund Halley classified it as a nebulous object in 1677. Omega Centauri was finally correctly identified as a star cluster by another English astronomer, John Herschel, in 1836. With a magnitude of 3.7, Omega Centauri is often considered the most dazzling globular cluster in the sky. It’s so bright that it can easily be seen with the unaided eye, though binoculars or a telescope will reveal an especially breathtaking spectacle. The cluster is a favorite observing target for amateur astronomers, but it is only visible to observers at low northern latitudes and south of the equator. Autumn skies in the Southern Hemisphere will present the best opportunity to observe it. For more information about Hubble’s observations of Caldwell 80, see: hubblesite.org/contents/news-releases/2008/news-2008-14.h... hubblesite.org/contents/news-releases/2001/news-2001-33.h... hubblesite.org/contents/media/images/2009/25/2609-Image.html Credit: NASA, ESA and the Hubble Heritage Team (STScI/AURA); Acknowledgment: A. Cool (San Francisco State University) and J. Anderson (STScI) 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 |
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Source | https://www.flickr.com/photos/144614754@N02/49214013287/ |
Author | NASA Hubble |
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This image was originally posted to Flickr by NASA Hubble at https://flickr.com/photos/144614754@N02/49214013287 (archive). It was reviewed on 23 February 2020 by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc-by-2.0. |
23 February 2020
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Orientation | Normal |
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Horizontal resolution | 400 dpi |
Vertical resolution | 400 dpi |
Software used | Adobe Photoshop CS3 Macintosh |
File change date and time | 09:18, 27 March 2008 |
Y and C positioning | Centered |
Exif version | 2.31 |
Date and time of digitizing | 09:18, 27 March 2008 |
Meaning of each component |
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Supported Flashpix version | 1 |
Color space | Uncalibrated |
Image width | 4,000 px |
Image height | 3,650 px |
Bits per component |
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Height | 3,650 px |
Width | 4,000 px |
Pixel composition | RGB |
Number of components | 3 |
Date metadata was last modified | 05:18, 27 March 2008 |
IIM version | 2 |