| M57 The Ring Nebula Widefield |
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| Written by keith grice |
| Sunday, 10 July 2011 18:23 |
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The star at the center of the Ring nebula has a surface temperature of 216,000 degrees Farenheit or 120,000 degrees Celsius. Our own star, the Sun, is expected to undergo the same process in a couple of billion years. Planetary nebulae do not last long at all in cosmic terms, the shell of gas expands and diffuses, becoming invisible, and the star turns into a white dwarf Planetary nebula are shells of gas shed by stars late in their life cycles after using up all of their nuclear fuel. The star then ejects a significant portion of its mass in a gaseous shell, which is illuminated by its extremely hot central star, which is just the core left from the original star. This widefield image was taken with a Canon 40D DSLR fitted with a light pollution filter and 8" F/5 Ritchey Cretien Astrograph. Exposure settings are 22 x 3mins @ ISO 1600 captured in Nebulosity, aligned and stacked. Image saved as a Tiff file and processed in Photoshop CS5.
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| Last Updated on Sunday, 10 July 2011 18:44 |





