Daftar bintang terbesar: Perbedaan antara revisi

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! style="background-color:#EFEFEF; white-space: nobr;" | Nama

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|[[Stephenson 2-18]]

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| [[VY Canis Majoris]] || 1.420

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| [[VV Cephei|VV Cephei A]] || 1.050<ref>{{cite journal |author=Habets, G. M. H. J.; Heintze, J. R. W. |title=Empirical bolometric corrections for the main-sequence |journal=Astronomy and Astrophysics Supplement |volume=46 |month=November |year=1981 |pages=193–237 |accessdate=2010-03-14 |url=http://adsabs.harvard.edu/abs/1981A&AS...46..193H}} Page 225 "Table IV" #178</ref>–1.900<ref name="Kaler">{{cite web

|accessdate=2010-03-15

}}</ref>

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| [[Mu Cephei]] || 1.400<ref name="Levesque2005">{{cite web

|accessdate=2010-07 16

}}</ref>

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| [[RW Cephei]] || 1.260–1.610{{Citation needed|date=December 2009}}

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| [[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 ] "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>

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| [[Antares]] ''(Alpha Scorpii)'' || 883<ref name="foot">approximately 800, derived from the 1990 lunar occultation measurement of apparent diameter of 43.1 milliarcsec (up to ±1 milliarcsec error) (http://adsabs.harvard.edu/abs/1990A&A...230..355R page 361) together with 1997 parallax of 5.40 [1.68] milliarcsec ([http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Antares&submit=SIMBAD+search SIMBAD] citing [http://astrobib.u-strasbg.fr:2008/cgi-bin/cdsbib?1997A%26A...323L..49P Hipparcos]). The parallax gives a derived distance from 460 to 877 light years. This in turn yields an actual diameter from 653 to 1,246 solar radius. An average of 800 is used here.</ref>

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| [[UY Scuti]] || 755

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| [[V382 Carinae]] || 747

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| [[S Pegasi]] || 580<ref>http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=10781</ref>

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| [[T Cephei]] || 540<ref>http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=9837</ref>

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| [[S Orionis]] || 530<ref>http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=2512</ref>

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| [[W Hydrae]] || 520<ref>http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=6127</ref>

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| [[R Cassiopeiae]] || 500<ref>http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=10947</ref>

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| [[Chi Cygni]] || 470<ref>http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=9107</ref>

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| [[Alpha Herculis]] ''(Ras Algethi)'' || 460

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| [[Rho Cassiopeiae]] || 450

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| [[Mira|Mira A]] ''(Omicron Ceti)'' || 400<ref>http://www.eso.org/~mwittkow/publications/conferences/SPIECWo5491199.pdf</ref>

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| [[V509 Cassiopeiae]] || 400<ref>[http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=10628]</ref>–900<ref name="Nugent">{{cite web |first=Richard |last=Nugent |publisher=weblore.com |url=http://www.weblore.com/richard/garnet_star.htm |title=The Garnet Star |quote=DIAM .. m Cep 1224 ... V509 CAS 910 ... V382 CAR 747 |accessdate=2009-12-04}}</ref>

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| [[S Doradus]] || 100–380<ref>

| accessdate=2009-03-25 | bibcode=1995ASPC...83..176L

}}</ref>

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| [[R Doradus]] || 370

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| [[HR Carinae]] || 350

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| [[R Leonis]] || 350<ref>http://arxiv.org/abs/astro-ph/0411133</ref>

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| [[Pistol Star|The Pistol Star]] || 340

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| [[Alpha Draconis]] ''(Thuban)'' || 265

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| [[119 Tauri]] ''("Ruby Star")''<ref>[http://jumk.de/astronomie/big-stars/119-tauri.shtml "Big and Giant Stars"]</ref> || 255<ref>http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=2526</ref>

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| [[La Superba]] ''([[Y Canum Venaticorum]])'' || 225

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| [[Deneb]] ''(Alpha Cygni)'' || 220

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| [[Delta Canis Majoris]] ''(Wezen)'' || 215±66<ref>{{cite journal|last= Davis J, Booth AJ, Ireland MJ, Jacob AP, North JR, Owens SM, Robertson JG, Tango WJ, Tuthill PG|year=2007|first1= J.|pages= 151|last2= Booth|first2= A. J.|last3= Ireland|first3= M. J.|last4= Jacob|first4= A. P.|last5= North|first5= J. R.|last6= Owens|first6= S. M.|last7= Robertson|first7= J. G.|last8= Tango|first8= W. J.|last9= Tuthill|first9= P. G.|volume= 24|title=The Emergent Flux and Effective Temperature of Delta Canis Majoris|journal= Publications of the Astronomical Society of Australia|doi=10.1071/AS07017|url=http://arxiv.org/abs/0709.3873v1|accessdate=28 May 2010}}</ref>

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| [[Zeta Aurigae]] || 200<ref>[http://www.hposoft.com/EAur09/ZetaAurigae.html]</ref>

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| [[Eta Carinae]] || 85–195<ref>http://etacar.umn.edu/etainfo/basic/</ref>

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| [[Epsilon Aurigae]] A || 175

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| [[Epsilon Carinae]] || 153

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| [[LBV 1806-20]] || 150

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| [[Epsilon Pegasi]] ''(Enif)'' || 150

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| [[Gamma Crucis]] ''(Gacrux)'' || 113<ref>Gamma Crucis by Jim Kaler]</ref>

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| [[Gamma Andromedae]] || 83

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| [[Rigel]] ''(Beta Orionis)'' || 78

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| [[Alpha Leporis]] ''(Arneb)'' || 77

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| [[R Coronae Borealis]] || 65

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| [[Canopus]] ''(Alpha Carinae)'' || 65

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| [[Delta Orionis]] ''(Mintaka)'' || 60

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| [[Alpha Persei]] ''(Mirfak)'' || 60

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| [[Zeta Geminorum]] ''(Mekbuda)'' || 60

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| [[Eta Aquilae]] || 60

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| [[Gamma Draconis]] ''(Eltanin)'' || 50

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| [[Aldebaran]] ''(Alpha Tauri)'' || 43<ref>http://adsabs.harvard.edu/abs/2005astro.ph..2181R</ref>

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| [[Beta Ursae Minoris]] ''(Kochab)'' || 41

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| [[Beta Draconis]] ''(Rastaban)'' || 40

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| [[Zeta Orionis]] ''(Alnitak)'' || 20

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| [[Zeta Puppis]] ''(Naos)'' || 18.6

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| [[Beta Cygni]] A1 ''(Albireo)'' || 16

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