Daftar bintang terbesar: Perbedaan antara revisi

| [[Betelgeuse]] ''(Alpha Orionis)'' || 950–1.000<ref>A NEW VLA-HIPPARCOS DISTANCE TO BETELGEUSE AND ITS IMPLICATIONS. Graham M. Harper et al 2008 The Astronomical Journal 135 1430-1440 doi: 10.1088/0004-6256/135/4/1430 [http://www.iop.org/EJ/abstract/1538-3881/135/4/1430/]</ref> atau 880–988<ref>Jim Kaler. 2009-06-26. [http://www.astro.uiuc.edu/~kaler/sow/betelgeuse.html Betelgeuse ] {{Webarchive|url=https://web.archive.org/web/20081216023607/http://www.astro.uiuc.edu/~kaler/sow/betelgeuse.html |date=2008-12-16 }} "0.047 seconds of arc, from which we find a true radius of between 4.1 (compromise distance) and 4.6 (larger distance) AU, … extended atmosphere, and the pulsations make it difficult to locate an actual "surface" to tell just how large the star actually is. … "size" of the star depends on the color of observation. Long-wave infrared … up to 5 AU and greater, … shorter-wave infrared … 3 AU. … Betelgeuse to be shrinking … not even round, but somewhat oval"</ref>

* [http://www.lowell.edu/press_room/releases/recent_releases/largest_star_rls.html '''Lowell Observatory''' Astronomers Identify Largest Stars Known] {{Webarchive|url=https://web.archive.org/web/20050119220417/http://www.lowell.edu/press_room/releases/recent_releases/largest_star_rls.html |date=2005-01-19 }}