This planetary nebula, known as NGC 650 or the Little Dumbbell, is about 2,500 light-years from Earth in the Perseus constellation. Unlike the other spherical nebulas, it has a bipolar or butterfly shape due to a "waist," or disk, of thick material, running from lower left to upper right. Fast winds blow material away from the star, above and below this dusty disk. The ghoulish green and red clouds are from glowing hydrogen molecules, with the green area being hotter than the red.
In this image, infrared light at wavelengths of 3.6 microns is rendered in blue, 4.5 microns in green, and 8.0 microns in red.
NASA/JPL-Caltech/J. Hora (Harvard-Smithsonian CfA)
<a rel="nofollow" class="external free" href="http://www.spitzer.caltech.edu/images/5686-sig13-015-Little-Dumbbell-Nebula">http://www.spitzer.caltech.edu/images/5686-sig13-015-Little-Dumbbell-Nebula</a>