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Sooty Nebula Around a Sun Like Star.

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planetary nebula.
Subaru telescope captured this image of a dusty planetary nebula.

The Subaru telescope captured this image of a dusty planetary nebula surrounding a star similar to our own Sun at the end of its life. Located 5,000 light-years away from Earth in the constellation of Cygnus, the nebula is very similar to the more famous Ring Nebula. When they reach the end of their lives, stars like our own Sun shed layers of gas and dust which pile up around the star, and are pushed outward. In this nebula, the material has reached a distance of 100 times the size of our Solar System.

The Coronagraphic Imager with Adaptive Optics (CIAO) on the Subaru telescope captured this near-infrared (wavelengths of 1.25 - 2.2 microns) image of a star at the end of its life. BD +303639 is a planetary nebula, similar to the Ring Nebula in the constellation Lyra, the Harp. It is about five thousand light years from Earth in the direction of the constellation Cygnus, the Swan. The surface of the star in the center of the nebula sizzles at a temperature of forty two thousand degrees Kelvin, and shines fifty thousand times brighter than our Sun.

At the end of their lives, comparatively lightweight stars like our Sun shed dust and gas which pile around the star. BD +303639 rapidly puffed off its outer layers about nine hundred years ago. This material, weighing almost a quarter of the Sun, has now expanded into a shell one hundred times more extended than the Solar System. The central star illuminates the material which looks like a life preserver from our point of view.

With visible light we can only see the light from the central star scattering off the dust. In Infrared light, we can also see light emitted by the dust itself. CIAO used a technique called adaptive optics, which removes the twinkle of light due to turbulence in Earth's atmosphere, to obtain an extraordinarily sharp image of the dust surrounding the star. (Note 1)

Spectra of the central star from the Subaru telescope's High Dispersion Sepctrogrtaph indicates that the sizzling at the star's surface is generating large quantities of carbon. This carbon is a likely ingredient of the dust surrounding the star.

Shedding of material is an integral part of the life of stars. "Although Astronomers have been studying the dust and gas surrounding stars of different ages and types, we are only beginning to be able to observe and understand detailed structures such those in BD +303639," says Dr. Koji Murakawa, an Astronomer at the Netherlands Foundation for Research in Astronomy. Murakawa adds that "images like these give us precious insight into the last moments in a stars life."

Note 1: The coronagraph, a device that blocks the light from a bright central star, was not used to obtain this image.

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