File:Hubble Supernova Bubble Resembles Holiday Ornament (27747558060).jpg
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[edit]DescriptionHubble Supernova Bubble Resembles Holiday Ornament (27747558060).jpg |
A delicate sphere of gas, photographed by NASA's Hubble Space Telescope, floats serenely in the depths of space. The pristine shell, or bubble, is the result of gas that is being shocked by the expanding blast wave from a supernova. Called SNR 0509-67.5 (or SNR 0509 for short), the bubble is the visible remnant of a powerful stellar explosion in the Large Magellanic Cloud (LMC), a small galaxy about 160,000 light-years from Earth. Ripples in the shell's surface may be caused by either subtle variations in the density of the ambient interstellar gas, or possibly driven from the interior by pieces of the ejecta. The bubble-shaped shroud of gas is 23 light-years across and is expanding at more than 11 million miles per hour (5,000 kilometers per second). Astronomers have concluded that the explosion was one of an especially energetic and bright variety of supernovae. Known as Type Ia, such supernova events are thought to result from a white dwarf star in a binary system that robs its partner of material, takes on much more mass than it is able to handle, and eventually explodes. Hubble's Advanced Camera for Surveys observed the supernova remnant on Oct. 28, 2006, with a filter that isolates light from glowing hydrogen seen in the expanding shell. These observations were then combined with visible-light images of the surrounding star field that were imaged with Hubble's Wide Field Camera 3 on Nov. 4, 2010. With an age of about 400 years as seen from Earth, the supernova might have been visible to southern hemisphere observers around the year 1600. However, there are no known records of a "new star" in the direction of the LMC near that time. A more recent supernova in the LMC, SN 1987A, did catch the eye of Earth viewers and continues to be studied with ground- and space-based telescopes, including Hubble. For more information, visit: <a href="http://hubblesite.org/news_release/news/2010-27" rel="nofollow">hubblesite.org/news_release/news/2010-27</a> Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA) Acknowledgment: J. Hughes (Rutgers University) |
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Source | Hubble Supernova Bubble Resembles Holiday Ornament |
Author | NASA Hubble Space Telescope |
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This image was originally posted to Flickr by NASA Hubble at https://flickr.com/photos/144614754@N02/27747558060 (archive). It was reviewed on 13 July 2018 by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc-by-2.0. |
13 July 2018
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current | 15:50, 13 July 2018 | 2,942 × 2,287 (8.15 MB) | Hiàn (alt) (talk | contribs) | Transferred from Flickr via #flickr2commons |
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Author | Space Telescope Science Institute Office of Public Outreach |
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Image title |
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Publisher | STScI |
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Short title |
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Credit/Provider | NASA, ESA, and the Hubble Heritage Team (STScI/AURA) |
Headline | NASA's Hubble Space Telescope has imaged a pristine bubble of shocked gas from the expanding blast wave from a supernova. Called SNR 0509-67.5, the bubble is the visible remnant of a powerful stellar explosion in the Large Magellanic Cloud (LMC), a small galaxy about 160,000 light-years from Earth. |
Source | STScI |
Usage terms | |
Online copyright statement | http://hubblesite.org/copyright/ |
Date and time of data generation | 14 December 2010 |
Contact information | outreach@stsci.edu
3700 San Martin Drive Baltimore, MD, 21218 USA |
Keywords | SNR 0509 |
Type of media | Observation |
Date and time of digitizing | 07:36, 16 November 2010 |
Software used | Adobe Photoshop CS5 Macintosh |
Date metadata was last modified | 6 April 2015 |
File change date and time | 12:54, 24 March 2014 |
Unique ID of original document | xmp.did:79DB22F72A20681197A5FD446F4C3A60 |