File:Remnant of an Explosion With a Powerful Kick? (7064827397).jpg
Original file (3,600 × 3,058 pixels, file size: 309 KB, MIME type: image/jpeg)
Captions
Summary
[edit]DescriptionRemnant of an Explosion With a Powerful Kick? (7064827397).jpg |
Description: A supernova remnant located about 14,700 light years from Earth toward the center of the Milky Way. G350.1+0.3 is a young and exceptionally bright supernova remnant in our Galaxy. While many supernova remnants are nearly circular, G350.1+0.3 is strikingly asymmetrical as seen in a new composite image of X-rays from Chandra (gold) and infrared data from Spitzer (light blue). Astronomers think that this bizarre shape is due to the stellar debris field expanding into a nearby cloud of cold molecular gas. With an age of between 600 and 1,200 years old, G350.1+0.3 is in the same time frame as other famous supernovas that formed the Crab and SN 1006 supernova remnants. However, it is unlikely that anyone on Earth would have seen the explosion because of the obscuring gas and dust that lies along our line of sight to the remnant. Creator/Photographer: Chandra X-ray Observatory NASA's Chandra X-ray Observatory, which was launched and deployed by Space Shuttle Columbia on July 23, 1999, is the most sophisticated X-ray observatory built to date. The mirrors on Chandra are the largest, most precisely shaped and aligned, and smoothest mirrors ever constructed. Chandra is helping scientists better understand the hot, turbulent regions of space and answer fundamental questions about origin, evolution, and destiny of the Universe. The images Chandra makes are twenty-five times sharper than the best previous X-ray telescope. NASA's Marshall Space Flight Center in Huntsville, Ala., manages the Chandra program for NASA's Science Mission Directorate in Washington. The Smithsonian Astrophysical Observatory controls Chandra science and flight operations from the Chandra X-ray Center in Cambridge, Massachusetts. Medium: Chandra telescope x-ray Date: 2012 Image ID: 500 Persistent URL: chandra.harvard.edu/photo/2012/g350/ Repository: Smithsonian Astrophysical Observatory Gift line: X-ray: NASA/CXC/SAO/I.Lovchinsky et al, IR: NASA/JPL-Caltech View more collections from the Smithsonian Institution. |
Date | |
Source | Remnant of an Explosion With a Powerful Kick? |
Author | Smithsonian Institution from United States |
Permission (Reusing this file) |
Smithsonian Institution @ Flickr Commons |
Licensing
[edit]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
More information can be found at https://flickr.com/commons/usage/. Please add additional copyright tags to this image if more specific information about copyright status can be determined. See Commons:Licensing for more information. |
This image was originally posted to Flickr by Smithsonian Institution at https://flickr.com/photos/25053835@N03/7064827397. 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
File history
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 06:41, 14 September 2016 | 3,600 × 3,058 (309 KB) | Vanished Account Byeznhpyxeuztibuo (talk | contribs) | Transferred from Flickr via Flickr2Commons |
You cannot overwrite this file.
File usage on Commons
There are no pages that use this file.
Metadata
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.
JPEG file comment | G350.1+0.3 is a young and exceptionally bright supernova remnant in our Galaxy. While many supernova remnants are nearly circular, G350.1+0.3 is strikingly asymmetrical as seen in a new composite image of X-rays from Chandra (gold) and infrared data from Spitzer (light blue). Astronomers think that this bizarre shape is due to the stellar debris field expanding into a nearby cloud of cold molecular gas. With an age of between 600 and 1,200 years old, G350.1+0.3 is in the same time frame as other famous supernovas that formed the Crab and SN 1006 supernova remnants. However, it is unlikely that anyone on Earth would have seen the explosion because of the obscuring gas and dust that lies along our line of sight to the remnant. |
---|