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Deskripsyon
English: Mira A is a red giant variable star in the constellation Cetus. This ultraviolet-wavelength image mosaic, taken by NASA's Galaxy Evolution Explorer, shows a comet-like "tail" stretching 13 Light-years across space. The "tail" consists of hydrogen gas blown off of the star, with the material at the furthest end of the "tail" having been emitted about 30,000 years ago. The tail-like configuration of the emitted material appears to result from Mira's uncommonly high speed relative to the Milky Way galaxy's ambient gas-- about 130 kilometers per second.Mira itself is seen as a small white dot inside a blue bulb. You could also see many stars and galaxies at the image.
Gigikanan http://www.galex.caltech.edu/media/glx2007-04r_img01.html
Tagsulat NASA
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Mira.jpg
Mira-uv-bow-shock-tail-vertical.jpg

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Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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kasamtangan04:40, 21 Marso 2010Thumbnail sa bersyon sa 04:40, 21 Marso 20102,500 × 625 (1.31 MB)Ohms Law Bot{{BotMoveToCommons|1=en.wikipedia|day=21|month=March|year=2010}} == Summary == :Mira A is a red giant variable star in the constellation Cetus. This ultraviolet-wavelength image mosaic, taken by NASA's Galaxy Evolution Explorer, s

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