(See description below)
Camelopardalis, or U Cam for short, is a star nearing the end of
its life. As it begins to run low on fuel, it is becoming unstable. Every few
thousand years, it coughs out a nearly spherical shell of gas as a layer of
helium around its core begins to fuse. The gas ejected in the star’s latest
eruption is clearly visible in this picture as a faint bubble of gas surrounding
U Cam is an example of a carbon star. This is a rare type of star whose atmosphere contains more carbon than oxygen. Due to its low surface gravity, typically as much as half of the total mass of a carbon star may be lost by way of powerful stellar winds. Located in the constellation of Camelopardalis (The Giraffe), near the North Celestial Pole, U Cam itself is actually much smaller than it appears in Hubble’s picture. In fact, the star would easily fit within a single pixel at the center of the image. Its brightness, however, is enough to saturate the camera's receptors, making the star look much bigger than it really is.
The shell of gas, which is both much larger and much fainter than its parent star, is visible in intricate detail in Hubble’s portrait. While phenomena that occur at the ends of stars’ lives are often quite irregular and unstable, the shell of gas expelled from U Cam is almost perfectly spherical.
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