File:Famous Supernova Reveals Clues About Crucial Cosmic Distance Markers (9934095563).jpg
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DescriptionFamous Supernova Reveals Clues About Crucial Cosmic Distance Markers (9934095563).jpg |
Description: Over 400 years ago, Johannes Kepler and many others witnessed the appearance of a new "star" in the sky. Today, this object is known as the Kepler supernova remnant. Previously, astronomers have deduced that the Kepler remnant comes from a so-called Type Ia supernova, which is the result of a thermonuclear explosion of a white dwarf. New data from Chandra suggest that this white dwarf exploded after pulling material from a companion red giant star, and not from the merger with another white dwarf. In this image, data from Chandra are colored red, green, and blue to show low, medium, and high-energy X-rays that have been combined with an optical image of the field. Creator: Chandra X-ray Observatory Center Date Created: March 18, 2013 Repository: Smithsonian Astrophysical Observatory Image ID: kepler_xray Permanent URL: chandra.harvard.edu/photo/2013/kepler/ View more collections from the Smithsonian Institution. |
Date | |
Source | Famous Supernova Reveals Clues About Crucial Cosmic Distance Markers |
Author | Smithsonian Institution from United States |
Permission (Reusing this file) |
Smithsonian Institution @ Flickr Commons |
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This image was taken from Flickr's The Commons. The uploading organization may have various reasons for determining that no known copyright restrictions exist, such as: No known copyright restrictionsNo restrictionshttps://www.flickr.com/commons/usage/false
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This image was originally posted to Flickr by Smithsonian Institution at https://flickr.com/photos/25053835@N03/9934095563. It was reviewed on 14 September 2016 by FlickreviewR and was confirmed to be licensed under the terms of the No known copyright restrictions. |
14 September 2016
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current | 06:18, 14 September 2016 | 3,000 × 2,006 (814 KB) | Vanished Account Byeznhpyxeuztibuo (talk | contribs) | Transferred from Flickr via Flickr2Commons |
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This file contains additional information such as Exif metadata which may have been added by the digital camera, scanner, or software program used to create or digitize it. If the file has been modified from its original state, some details such as the timestamp may not fully reflect those of the original file. The timestamp is only as accurate as the clock in the camera, and it may be completely wrong.
Image title |
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Source | Chandra X-ray Observatory |
Headline | The remains of a stellar explosion that appear in Earth's sky in 1604. |
Credit/Provider | X-ray: NASA/CXC/NCSU/M.Burkey et al; Optical: DSS |
Short title |
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Usage terms | |
Date and time of data generation | 18 March 2013 |
Width | 3,600 px |
Height | 2,407 px |
Bits per component |
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Compression scheme | LZW |
Pixel composition | RGB |
Orientation | Normal |
Number of components | 3 |
Horizontal resolution | 300 dpi |
Vertical resolution | 300 dpi |
Data arrangement | chunky format |
Software used | Adobe Photoshop CS6 (Macintosh) |
File change date and time | 09:03, 25 September 2013 |
Exif version | 2.21 |
Color space | sRGB |
Date metadata was last modified | 05:03, 25 September 2013 |
Date and time of digitizing | 07:48, 8 August 2012 |
Unique ID of original document | xmp.did:404FE6011920681180838656C119EA5F |
Keywords | Kepler's Supernova Remnant |
Contact information | cxcpub@cfa.harvard.edu
60 Garden St. Cambridge, MA, 02138 USA |
IIM version | 4 |