Rigel A is classified as a blue-white [[supergiant]] of spectral class B8 Iab. The star contains some 17 times the mass of our [[Sun]]. While the radius of Rigel is estimated to be 74 times that of the Sun, so large, that is Rigel was at the center of our solar system, it would extend to the orbit of [[Mercury]].<ref name="illinois">http://www.astro.illinois.edu/~jkaler/sow/rigel.html</ref> The star has 40,000 times the Sun's visual luminosity.<ref name="illinois">http://www.astro.illinois.edu/~jkaler/sow/rigel.html</ref> Much of Rigel's radiation however, is in the [[ultraviolet]], when this is accounted for, the star's total luminosity is 150,000 times of the Sun's.<ref name="star">http://www.nasa.gov/worldbook/star_worldbook.html</ref> | Rigel A is classified as a blue-white [[supergiant]] of spectral class B8 Iab. The star contains some 17 times the mass of our [[Sun]]. While the radius of Rigel is estimated to be 74 times that of the Sun, so large, that is Rigel was at the center of our solar system, it would extend to the orbit of [[Mercury]].<ref name="illinois">http://www.astro.illinois.edu/~jkaler/sow/rigel.html</ref> The star has 40,000 times the Sun's visual luminosity.<ref name="illinois">http://www.astro.illinois.edu/~jkaler/sow/rigel.html</ref> Much of Rigel's radiation however, is in the [[ultraviolet]], when this is accounted for, the star's total luminosity is 150,000 times of the Sun's.<ref name="star">http://www.nasa.gov/worldbook/star_worldbook.html</ref> |