U Camelopardalis [ http://en.wikipedia.org/wiki/U_Camelopardalis ] is a star on the brink. The carbon star -- 1,500 light years away from us, in the Camelopardalis constellation [ http://en.wikipedia.org/wiki/Camelopardalis_%28constellation%29 ] -- is nearing the end of its life. And as stars run low on fuel, they become unstable. U Cam has an atmosphere that contains more carbon than oxygen -- and, due to its low surface gravity, as much as half of U Cam's total mass can be lost to the forces of stellar winds.
In the picture above, the explosion of gas makes U Cam seem much larger than it actually is. (The gas is the murky halo around the bright-white star itself.) And the brightness of the explosion, NASA notes, saturated the Hubble camera's receptors -- meaning that U Cam, the sneezy, wheezy carbon star, is actually much daintier than the image above suggests.