  
                 
                
            May 7, 2010 - Menkhib and the California Nebula 
            This infrared  image from NASA’s WISE (Wide-field Infrared Survey Explorer) features one of  the bright stars in the constellation Perseus, named Menkhib (the bright star  in the upper left near the red dust cloud) along with a large star forming  cloud catalogued as NGC 1499, or more commonly called the California Nebula (running  diagonally through the image). 
            Menkhib is one  of the hottest stars visible in the night sky; its surface temperature is about  37,000 Kelvin (about 66,000 degrees Fahrenheit – over 6 times hotter than the  Sun). Because of its high temperature it appears blue-white to the human eye  (almost all stars appear bluish to WISE).  It has about 40 times the mass of the Sun and  gives off 330,000 times the amount of light. Menkhib is a runaway star, and the  fast stellar wind it blows is piling up in front of it to create a shock wave  in the gas and dust surrounding it in the space between the stars. This shock  wave is heating up the dust within and WISE sees it as the red cloud in the  upper left of the image.  
            Menkhib is  part of an association of very hot stars that were born from the California  Nebula only a few million years ago. These stars are lighting up the nebula;  heating and ionizing it. In visible light, the ionized gas glows red, while in  infrared light we see the heated dust (which appears in green and red in this  image from WISE). The California Nebula gets its name due to a resemblance to  the shape of the U.S. State of California (which you can just make out as  outlined by the green dust if you rotate the image by a little more than 90  degrees clockwise). The entire California Nebula stretches across about 100  light-years, and we see about 80% of it in this view. 
            Menkhib and  the California Nebula are about 1,800 light-years away from Earth. This is within  the same spur of the Orion spiral arm of the Milky Way in which we are located. 
            All four  infrared detectors aboard WISE were used to make this image. Color is  representational: blue and cyan represent infrared light at wavelengths of 3.4  and 4.6 microns, which is dominated by light from stars. Green and red  represent light at 12 and 22 microns, which is mostly light from warm dust.  
          Image Credit: NASA/JPL-Caltech/WISE Team 
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