Death star

Star around the nucleus of the helium layer melting Camelopardalis U sing every several thousand years will jet out of a nearly spherical shell of gas

                                                         The human cornea

Beijing, July 13, the Hubble Space Telescope captured a distant death star "last breath" - about to burn out the star core, the shape resembles the human cornea. As star's nuclear fuel is exhausted, around the ring is also clearly visible.This is moving towards the dying star called the the Camelopardalis U-Star, the great distances from Earth, usually expressed as a pixel photo. However, the Camelopardalis U stars nuclear exhaled gas shell brightness is extremely high, able to capture spectacular photos under a scene so that the sensors of the Hubble Space Telescope.The Camelopardalis U star is in the final stages of life. With fuel is exhausted, the star is more unstable. Star around the nucleus of the helium layer melting Camelopardalis U sing every several thousand years will jet out of a nearly spherical shell of gas. In photographs taken by the Hubble telescope, the Camelopardalis U star gas jet is clearly visible, showing as a surround the Camelopardalis U Star dark bubbles.The Camelopardalis U star is a carbon star, which is a rare stellar atmosphere of carbon than oxygen. Due to the low surface gravity, the quality of the carbon star is usually half the form of strong stellar winds disappear. The Camelopardalis U star is located in Camelopardalis near the north celestial pole. Photographs taken by the Hubble Space Telescope, this in the center of the picture stars account for only one pixel, high brightness of the gas shell, Camelopardalis U star in the photo look bigger. Compared with the parent star, the gas shell is larger, but lower brightness, visible in photographs taken by the Hubble telescope. This phenomenon is often erratic and unstable, but it the Camelopardalis U star ejected gas shells but was almost perfectly spherical.