File:RCW 86.jpg
Summary
<a href="//commons.wikimedia.org/wiki/Category:Infrared" title="Category:Infrared">Infrared</a> images from NASA's Spitzer Space Telescope and Wide-field Infrared Survey Explorer (WISE) are combined in this image of RCW 86, the dusty remains of the oldest documented example of an exploding star, or supernova. It shows <a href="//commons.wikimedia.org/wiki/Light" title="Light">light</a> from both the remnant itself and unrelated background light from our <a href="//commons.wikimedia.org/wiki/Category:Milky_Way_Galaxy" title="Category:Milky Way Galaxy">Milky Way galaxy</a>. The colours in the image allow astronomers to distinguish between the remnant and galactic background, and determine exactly which structures belong to the remnant. <a href="//commons.wikimedia.org/wiki/Category:Dust" title="Category:Dust">Dust</a> associated with the blast wave of the supernova appears <a href="//commons.wikimedia.org/wiki/Red" class="mw-redirect" title="Red">red</a> in this image, while dust in the background appears <a href="//commons.wikimedia.org/wiki/Yellow" class="mw-redirect" title="Yellow">yellow</a> and <a href="//commons.wikimedia.org/wiki/Green" title="Green">green</a>. Stars in the field of view appear <a href="//commons.wikimedia.org/wiki/Blue" title="Blue">blue</a>. By determining the <a href="//commons.wikimedia.org/wiki/Category:Temperature" title="Category:Temperature">temperature</a> of the dust in the red circular <a href="//commons.wikimedia.org/wiki/Shell" title="Shell">shell</a> of the supernova remnant, which marks the extent to which the blast wave from the supernova has travelled since the explosion, astronomers were able to determine the density of the material there, and conclude that RCW 86 must have exploded into a large, wind-blown cavity. The infrared images, when combined with optical and <a href="//commons.wikimedia.org/wiki/X-ray" title="X-ray">X-ray</a> <a href="//commons.wikimedia.org/wiki/Category:Data" title="Category:Data">data</a>, clearly indicate that the source of the mysterious object seen in the <a href="//commons.wikimedia.org/wiki/Sky" title="Sky">sky</a> over 1,800 years ago must have been a Type Ia supernova.
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 22:11, 17 January 2017 | 2,811 × 2,154 (639 KB) | 127.0.0.1 (talk) | <a href="//commons.wikimedia.org/wiki/Category:Infrared" title="Category:Infrared">Infrared</a> images from NASA's Spitzer Space Telescope and Wide-field Infrared Survey Explorer (WISE) are combined in this image of RCW 86, the dusty remains of the oldest documented example of an exploding star, or supernova. It shows <a href="//commons.wikimedia.org/wiki/Light" title="Light">light</a> from both the remnant itself and unrelated background light from our <a href="//commons.wikimedia.org/wiki/Category:Milky_Way_Galaxy" title="Category:Milky Way Galaxy">Milky Way galaxy</a>. The colours in the image allow astronomers to distinguish between the remnant and galactic background, and determine exactly which structures belong to the remnant. <a href="//commons.wikimedia.org/wiki/Category:Dust" title="Category:Dust">Dust</a> associated with the blast wave of the supernova appears <a href="//commons.wikimedia.org/wiki/Red" class="mw-redirect" title="Red">red</a> in this image, while dust in the background appears <a href="//commons.wikimedia.org/wiki/Yellow" class="mw-redirect" title="Yellow">yellow</a> and <a href="//commons.wikimedia.org/wiki/Green" title="Green">green</a>. Stars in the field of view appear <a href="//commons.wikimedia.org/wiki/Blue" title="Blue">blue</a>. By determining the <a href="//commons.wikimedia.org/wiki/Category:Temperature" title="Category:Temperature">temperature</a> of the dust in the red circular <a href="//commons.wikimedia.org/wiki/Shell" title="Shell">shell</a> of the supernova remnant, which marks the extent to which the blast wave from the supernova has travelled since the explosion, astronomers were able to determine the density of the material there, and conclude that RCW 86 must have exploded into a large, wind-blown cavity. The infrared images, when combined with optical and <a href="//commons.wikimedia.org/wiki/X-ray" title="X-ray">X-ray</a> <a href="//commons.wikimedia.org/wiki/Category:Data" title="Category:Data">data</a>, clearly indicate that the source of the mysterious object seen in the <a href="//commons.wikimedia.org/wiki/Sky" title="Sky">sky</a> over 1,800 years ago must have been a Type Ia supernova. |
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