Vega, Brightest Star In the Constellation Lyra


NASA's Spitzer Space Telescope recently captured these images of the star Vega, located 25 light years away in the constellation Lyra. Spitzer was able to detect the heat radiation from the cloud of dust around the star and found that the debris disc is much larger than previously thought. This side by side comparison, taken by Spitzer's multiband imaging photometer, shows the warm infrared glows from dust particles orbiting the star at wavelengths of 24 microns (figure 1 in blue) and 70 microns (figure 32in red). Both images show a very large, circular and smooth debris disc. The disc radius extends to at least 815 astronomical units. Scientists compared the surface brightness of the disc in the infrared wavelengths to determine the temperature distribution of the disc and then infer the corresponding particle size in the disc. These fine dust particles originate from collisions of embryonic planets near the star at a radius of approximately 90 astronomical units, and are then blown away by Vega's intense radiation. The mass and short lifetime of these small particles indicate that the disc detected by Spitzer is the aftermath of a large and relatively recent collision, involving bodies perhaps as big as the planet Pluto. The images are 3 arcminutes on each side. North is oriented upward and east is to the left. Spitzer Space Telescope Mission, Image taken with the Multiband Imaging Photometer (MIPS).


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Keywords: astronomical, astronomy, body, brightest, celestial, comparison, constellation, deep, heavenly, imaging, lyra, mips, mission, multiband, object, photometer, science, sky, space, spitzer, sst, star, telescope, vega