|
! style="background-color:#FFDEAD;" colspan="2" | [[Jari-jari Matahari|Radii Matahari]]<br />([[Matahari]] = 1)
|-
|[[UY Scuti]]
| [[VY Canis Majoris]] || 1.800–2.100<ref name="Choi"> ▼|1.516-1.900
{{cite web
|
|title=Distance to VY VMa with VERA
|publisher=Publications Astronomical Society of Japan
|author=K. Yoon Choi
|url=http://adsabs.harvard.edu/abs/2008PASJ...60.1007C
|accessdate=2010-07 16
}}</ref>
|-
| [[WOHV838 G64Monocerotis]] || 1.900-2.000<ref570 atau name="Levesque2009">380
|
{{cite web
|title=WOH G64: The Largest Star Known?
|publisher=Astronomical Journal
|author=E. M. Levesque
|url=http://adsabs.harvard.edu/abs/2009AJ....137.4744L
|accessdate=2010-07 16
}}</ref>
|-
| [[WOH G64]] ||1.540
| [[VV Cephei|VV Cephei A]] || 1.600<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
|title=VV CEP (VV Cephei)
|publisher=University of Illinois
|author=Professor James B. (Jim) Kaler
|url=http://www.astro.uiuc.edu/~kaler/sow/vvcep.html
|accessdate=2010-03-15
}}</ref>
|-
| [[MuV354 Cephei]] || 1.650<ref name="Levesque2005">520
{{cite web
|title=The Effective Temperature Scale of Galactic Red Supergiants: Cool, but Not as Cool As We Thought
|publisher=Astrophysical Journal
|author=E. M. Levesque
|url=http://iopscience.iop.org/0004-637X/628/2/973/fulltext
|accessdate=2010-07 16
}}</ref>
|-
| [[KW Sagittarii]] || 1.460 {{Citation needed|date=December 2009}}▼| [[V838 Monocerotis]] || 1.570 atau 800<ref>[[V838 Monocerotis]]</ref>
|-
| [[V354KY CepheiCygni]] || 1.520{{Citation420 needed|date=Decemberatau 2009}}2.850
|-
▲| [[VY Canis Majoris]] || 1. 800–2.100<ref name="Choi">420
| [[RW Cephei]] || 1.260–1.610{{Citation needed|date=December 2009}}
|-
| [[VV Cephei|VV Cephei A]] ||1.050-1.900
▲| [[KW Sagittarii]] || 1.460{{Citation needed|date=December 2009}}
|-
| [[RW Cephei]] ||1.260
| [[KY Cygni]] || 1.420 atau 1.440{{Citation needed|date=December 2009}}
|-
| [[Mu Cephei]] ||980
|-
| [[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>
|-
| [[Antares]] ''(Alpha Scorpii)'' ||883
| [[Antares]] ''(Alpha Scorpii)'' || 800<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>
|-
| [[V382 Carinae]] || 747
| 