Lys van grootste sterre: Verskil tussen weergawes
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|[[Stephenson 2-18|{{nowrap|Stephenson 2-18}}]] || 2 150 || Geleë naby die massiewe oop sterreswerm Stephenson 2, waar 26 rooisuperreuse voorkom.
|<ref name="thomas">{{Cite journal|last1=Fok|first1=Thomas K. T|last2=Nakashima|first2=Jun-ichi|last3=Yung|first3=Bosco H. K|last4=Hsia|first4=Chih-Hao|last5=Deguchi|first5=Shuji|s2cid=53393926|year=2012|title=Maser Observations of Westerlund 1 and Comprehensive Considerations on Maser Properties of Red Supergiants Associated with Massive Clusters|journal=The Astrophysical Journal|volume=760|issue=1|pages=65|arxiv=1209.6427|bibcode=2012ApJ...760...65F|doi=10.1088/0004-637X/760/1/65}}</ref>
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| [[Saturnus|Sauturnus se wentelbaan]] || 1 940 - 2 169 || <small>Aangedui vir verwysing</small> ||
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| [[UY Scuti]] || 1 708 || Foutmarge in die groottevasstelling: ± 192 sonradiusse. Op sy kleinste sal hy so groot soos V354 Cephei wees (sien onder).
|<ref name="torres2013">{{Cite journal | last1 = Arroyo-Torres | first1 = B. | last2 = Wittkowski | first2 = M. | last3 = Marcaide | first3 = J. M. | last4 = Hauschildt | first4 = P. H. | title = The atmospheric structure and fundamental parameters of the red supergiants AH Scorpii, UY Scuti, and KW Sagittarii | doi = 10.1051/0004-6361/201220920 | journal = Astronomy & Astrophysics | volume = 554 | pages = A76 | year = 2013 | pmid = | pmc = | bibcode = 2013A&A...554A..76A |arxiv = 1305.6179 }}</ref>
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