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St2-18 memiliki ketidakpastian jarak >50%, yang sangat memengaruhi luminositasnya, dan juga ukurannya. Batas teoritis radius bintang adalah 1500-1800 jari-jari matahari, jadi ukuran ini kemungkinan besar tidak benar.
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Baris 28:
([[Matahari]] = 1)
!Keterangan
|-▼
|[[Stephenson 2-18]]
|2.150<ref name="thomas"/>▼
|Bintang terbesar di jagat raya (sebelumnya UY Scuti)
|-Super raksasa merah
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Baris 41 ⟶ 37:
|accessdate=2010-07 16
}}</ref>
|Mungkin bintang terbesar yang diketahui.<ref name="Levesque2009" /><ref>{{Cite journal|last=Jones|first=O. C.|last2=Woods|first2=P. M.|last3=Kemper|first3=F.|last4=Kraemer|first4=K. E.|last5=Sloan|first5=G. C.|last6=Srinivasan|first6=S.|last7=Oliveira|first7=J. M.|last8=Van Loon|first8=J. Th.|last9=Boyer|first9=M. L.|date=2017-09|title=The SAGE-Spec Spitzer Legacy program: the life-cycle of dust and gas in the Large Magellanic Cloud. Point source classification – III|url=https://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/stx1101|journal=Monthly Notices of the Royal Astronomical Society|language=en|volume=470|issue=3|pages=3250–3282|doi=10.1093/mnras/stx1101|issn=0035-8711}}</ref><ref>{{Cite journal|last=de Wit|first=S.|last2=Bonanos|first2=A. Z.|last3=Tramper|first3=F.|last4=Yang|first4=M.|last5=Maravelias|first5=G.|last6=Boutsia|first6=K.|last7=Britavskiy|first7=N.|last8=Zapartas|first8=E.|date=2023-01-01|title=Properties of luminous red supergiant stars in the Magellanic Clouds|url=https://ui.adsabs.harvard.edu/abs/2023A&A...669A..86D|journal=Astronomy and Astrophysics|volume=669|pages=A86|doi=10.1051/0004-6361/202243394|issn=0004-6361}}</ref>
|▼
|-
|RSGC1-F01
| [[KY Cygni]]|| 1.420<ref name=":0">{{Cite journal|last=Levesque|first=Emily M.|last2=Massey|first2=Philip|last3=Olsen|first3=K. A. G.|last4=Plez|first4=Bertrand|last5=Josselin|first5=Eric|last6=Maeder|first6=Andre|last7=Meynet|first7=Georges|date=2005-08|title=The Effective Temperature Scale of Galactic Red Supergiants: Cool, But Not As Cool As We Thought|url=http://arxiv.org/abs/astro-ph/0504337|journal=The Astrophysical Journal|volume=628|issue=2|pages=973–985|doi=10.1086/430901|issn=0004-637X}}</ref>▼
| [[KW Sagittarii]]|| 1.009 ± 142450<ref>{{Cite journal|last=Arroyo-TorresDecin|first=B.Leen|last2=WittkowskiRichards|first2=Anita M. S.|last3=MarcaideMarchant|first3=J. M.Pablo|last4=HauschildtSana|first4=P. H.Hugues|date=20132024-0601|title=TheALMA atmosphericdetection structureof andCO fundamentalrotational parametersline emission in red supergiant stars of the redmassive supergiantsyoung AHstar Sco,cluster UYRSGC1 Sct-- andDetermination KWof Sgra new mass-loss rate prescription for red supergiants|url=http://arxiv.org/abs/13052303.617909385|journal=Astronomy & Astrophysics|volume=554681|pages=A76A17|doi=10.1051/0004-6361/201220920202244635|issn=0004-6361}}</ref>▼
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Baris 49 ⟶ 46:
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|[[AH Scorpii]]
| [[Mu Cephei]] || 1.259<ref>{{Cite journal|last=Josselin|first=E.|last2=Plez|first2=B.|date=2007-07|title=Atmospheric dynamics and the mass loss process in red supergiant stars|url=http://arxiv.org/abs/0705.0266|journal=Astronomy & Astrophysics|volume=469|issue=2|pages=671–680|doi=10.1051/0004-6361:20066353|issn=0004-6361}}</ref> – 1.420<ref name=":0" />▼
▲|21.150411<ref name="thomas:1" />
|
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|[[S Persei]]
|1.212<ref>{{Cite journal|last=Thompson|first=R. R.|last2=Creech-Eakman|first2=M. J.|date=2003-12-01|title=Interferometric observations of the supergiant S Persei: Evidence for axial symmetry and the warm molecular layer|url=https://ui.adsabs.harvard.edu/abs/2003AAS...203.4907T|volume=203|pages=49.07}}</ref> – 1.364<ref>{{Cite web|last=Norris|first=Ryan P.|date=2019|title=Seeing Stars Like Never Before: A Long-term Interferometric Imaging Survey of Red Supergiants|url=https://core.ac.uk/download/pdf/225164189.pdf|website=Georgia State University}}</ref>
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|[[VX Sagittarii]]
| [[V354 Cephei]] || 1.139<ref>{{Cite journal|last=Verhoelst|first=T.|last2=Zypen|first2=N. Van der|last3=Hony|first3=S.|last4=Decin|first4=L.|last5=Cami|first5=J.|last6=Eriksson|first6=K.|date=2009-04-01|title=The dust condensation sequence in red supergiant stars|url=https://www.aanda.org/articles/aa/abs/2009/16/aa9063-07/aa9063-07.html|journal=Astronomy & Astrophysics|language=en|volume=498|issue=1|pages=127–138|doi=10.1051/0004-6361/20079063|issn=0004-6361}}</ref>▼
|1.356<ref>{{Cite journal|last=Tabernero|first=H. M.|last2=Dorda|first2=R.|last3=Negueruela|first3=I.|last4=Marfil|first4=E.|date=2021-02-01|title=The nature of VX Sagitarii - Is it a TŻO, a RSG, or a high-mass AGB star?|url=https://www.aanda.org/articles/aa/abs/2021/02/aa39236-20/aa39236-20.html|journal=Astronomy & Astrophysics|language=en|volume=646|pages=A98|doi=10.1051/0004-6361/202039236|issn=0004-6361}}</ref>–1.480<ref>{{Cite journal|last=Wallström|first=S. H. J.|last2=Danilovich|first2=T.|last3=Müller|first3=H. S. P.|last4=Gottlieb|first4=C. A.|last5=Maes|first5=S.|last6=Sande|first6=M. Van de|last7=Decin|first7=L.|last8=Richards|first8=A. M. S.|last9=Baudry|first9=A.|date=2024-01-01|title=ATOMIUM: Molecular inventory of 17 oxygen-rich evolved stars observed with ALMA|url=https://www.aanda.org/articles/aa/abs/2024/01/aa47632-23/aa47632-23.html|journal=Astronomy & Astrophysics|language=en|volume=681|pages=A50|doi=10.1051/0004-6361/202347632|issn=0004-6361}}</ref>
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▲| [[KYMu CygniCephei]] || 1.259<ref>{{Cite journal|last=Josselin|first=E.|last2=Plez|first2=B.|date=2007-07|title=Atmospheric dynamics and the mass loss process in red supergiant stars|url=http://arxiv.org/abs/0705.0266|journal=Astronomy & Astrophysics|volume=469|issue=2|pages=671–680|doi=10.1051/0004-6361:20066353|issn=0004-6361}}</ref> – 1.420<ref name=":0">{{Cite journal|last=Levesque|first=Emily M.|last2=Massey|first2=Philip|last3=Olsen|first3=K. A. G.|last4=Plez|first4=Bertrand|last5=Josselin|first5=Eric|last6=Maeder|first6=Andre|last7=Meynet|first7=Georges|date=2005-08|title=The Effective Temperature Scale of Galactic Red Supergiants: Cool, But Not As Cool As We Thought|url=http://arxiv.org/abs/astro-ph/0504337|journal=The Astrophysical Journal|volume=628|issue=2|pages=973–985|doi=10.1086/430901|issn=0004-637X}}</ref>
|[[HR 5171|V766 Centauri]] Aa▼
▲|
|1.060 — 1.160<ref>{{Cite journal|last=van Genderen|first=A. M.|last2=Lobel|first2=A.|last3=Nieuwenhuijzen|first3=H.|last4=Henry|first4=G. W.|last5=de Jager|first5=C.|last6=Blown|first6=E.|last7=Di Scala|first7=G.|last8=van Ballegoij|first8=E. J.|date=2019-11|title=Pulsations, eruptions, and evolution of four yellow hypergiants|url=http://arxiv.org/abs/1910.02460|journal=Astronomy & Astrophysics|volume=631|pages=A48|doi=10.1051/0004-6361/201834358|issn=0004-6361}}</ref>▼
▲|-
| [[V354 Cephei]] || 1.245<ref name=":2">{{Cite journal|last=Healy|first=Sarah|last2=Horiuchi|first2=Shunsaku|last3=Molla|first3=Marta Colomer|last4=Milisavljevic|first4=Dan|last5=Tseng|first5=Jeff|last6=Bergin|first6=Faith|last7=Weil|first7=Kathryn|last8=Tanaka|first8=Masaomi|date=2024-03-23|title=Red Supergiant Candidates for Multimessenger Monitoring of the Next Galactic Supernova|url=http://arxiv.org/abs/2307.08785|journal=Monthly Notices of the Royal Astronomical Society|volume=529|issue=4|pages=3630–3650|doi=10.1093/mnras/stae738|issn=0035-8711}}</ref>
|-▼
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|[[WOH S264]]
|1.210<ref><nowiki>https://arxiv.org/abs/2405.11019</nowiki></ref>
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Baris 67 ⟶ 72:
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▲|[[HR 5171|V766 Centauri]] Aa
| [[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
▲|1.060 — 1.160<ref>{{Cite journal|last=van Genderen|first=A. M.|last2=Lobel|first2=A.|last3=Nieuwenhuijzen|first3=H.|last4=Henry|first4=G. W.|last5=de Jager|first5=C.|last6=Blown|first6=E.|last7=Di Scala|first7=G.|last8=van Ballegoij|first8=E. J.|date=2019-11|title=Pulsations, eruptions, and evolution of four yellow hypergiants|url=http://arxiv.org/abs/1910.02460|journal=Astronomy & Astrophysics|volume=631|pages=A48|doi=10.1051/0004-6361/201834358|issn=0004-6361}}</ref>
|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
|archive-date=2009-02-01
|archive-url=https://web.archive.org/web/20090201112518/http://www.astro.uiuc.edu/~kaler/sow/vvcep.html
|dead-url=yes
}}</ref>
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|-
|[[KY Cygni]]
▲| [[KW Sagittarii]]|| 1.009 ± 142<ref>{{Cite journal|last=Arroyo-Torres|first=B.|last2=Wittkowski|first2=M.|last3=Marcaide|first3=J. M.|last4=Hauschildt|first4=P. H.|date=2013-06|title=The atmospheric structure and fundamental parameters of the red supergiants AH Sco, UY Sct and KW Sgr|url=http://arxiv.org/abs/1305.6179|journal=Astronomy & Astrophysics|volume=554|pages=A76|doi=10.1051/0004-6361/201220920|issn=0004-6361}}</ref>
▲| [[V354 Cephei]] || 1.139033<ref>{{Cite journal|last=VerhoelstComerón|first=TF.|last2=ZypenDjupvik|first2=NA. Van derA.|last3=HonySchneider|first3=SN.|last4=DecinPasquali|first4=L.|last5=Cami|first5=J.|last6=Eriksson|first6=KA.|date=20092020-0412-01|title=The dusthistorical condensationrecord sequenceof inmassive redstar supergiantformation starsin Cygnus|url=https://wwwui.aandaadsabs.org/articles/aaharvard.edu/abs/2009/16/aa9063-07/aa9063-072020A&A...644A.html.62C|journal=Astronomy &and Astrophysics|language=en|volume=498|issue=1644|pages=127–138A62|doi=10.1051/0004-6361/20079063202039188|issn=0004-6361}}</ref>
|
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▲| [[MuKW CepheiSagittarii]] || 1.259009 ± 142<ref name=":1">{{Cite journal|last=JosselinArroyo-Torres|first=EB.|last2=PlezWittkowski|first2=BM.|last3=Marcaide|first3=J. M.|last4=Hauschildt|first4=P. H.|date=20072013-0706|title=AtmosphericThe dynamicsatmospheric structure and fundamental parameters of the massred losssupergiants processAH inSco, redUY Sct and supergiantKW starsSgr|url=http://arxiv.org/abs/07051305.02666179|journal=Astronomy & Astrophysics|volume=469|issue=2554|pages=671–680A76|doi=10.1051/0004-6361:20066353/201220920|issn=0004-6361}}</ref> – 1.420<ref name=":0" />
| [[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/]{{Pranala mati|date=Agustus 2021|bot=InternetArchiveBot|fix-attempted=yes}}</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>
|
|bintang paling terang ke-10 di langit malam.▼
|-
| [[UY Scuti]] || 755909<ref name=":2" />▼
| [[RW Cephei]] || 900–1760<ref>{{Cite journal|last=Anugu|first=Narsireddy|last2=Baron|first2=Fabien|last3=Gies|first3=Douglas R.|last4=Lanthermann|first4=Cyprien|last5=Schaefer|first5=Gail H.|last6=Shepard|first6=Katherine A.|last7=Brummelaar|first7=Theo ten|last8=Monnier|first8=John D.|last9=Kraus|first9=Stefan|date=2023-07|title=The Great Dimming of the Hypergiant Star RW Cephei: CHARA Array Images and Spectral Analysis|url=https://dx.doi.org/10.3847/1538-3881/ace59d|journal=The Astronomical Journal|language=en|volume=166|issue=2|pages=78|doi=10.3847/1538-3881/ace59d|issn=1538-3881}}</ref>▼
|
|-
▲ |title=[[VV CEP (Cephei|VV Cephei) A]]
▲| [[UY Scuti]] || 755
|779.27<ref>{{Cite journal|last=Baines|first=Ellyn K.|last2=Armstrong|first2=J. Thomas|last3=Clark|first3=James H.|last4=Gorney|first4=Jim|last5=Hutter|first5=Donald J.|last6=Jorgensen|first6=Anders M.|last7=Kyte|first7=Casey|last8=Mozurkewich|first8=David|last9=Nisley|first9=Ishara|date=2021-10|title=Angular Diameters and Fundamental Parameters of Forty-four Stars from the Navy Precision Optical Interferometer|url=https://dx.doi.org/10.3847/1538-3881/ac2431|journal=The Astronomical Journal|language=en|volume=162|issue=5|pages=198|doi=10.3847/1538-3881/ac2431|issn=1538-3881}}</ref>
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▲| [[RW Cephei]] || 900–1760<ref>{{Cite journal|last=Anugu|first=Narsireddy|last2=Baron|first2=Fabien|last3=Gies|first3=Douglas R.|last4=Lanthermann|first4=Cyprien|last5=Schaefer|first5=Gail H.|last6=Shepard|first6=Katherine A.|last7=Brummelaar|first7=Theo ten|last8=Monnier|first8=John D.|last9=Kraus|first9=Stefan|date=2023-07|title=The Great Dimming of the Hypergiant Star RW Cephei: CHARA Array Images and Spectral Analysis|url=https://dx.doi.org/10.3847/1538-3881/ace59d|journal=The Astronomical Journal|language=en|volume=166|issue=2|pages=78|doi=10.3847/1538-3881/ace59d|issn=1538-3881}}</ref>
|
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| [[Betelgeuse]] ''(Alpha Orionis)''|| 764<ref>{{Cite journal|last=Joyce|first=Meridith|last2=Leung|first2=Shing-Chi|last3=Molnár|first3=László|last4=Ireland|first4=Michael|last5=Kobayashi|first5=Chiaki|last6=Nomoto|first6=Ken'ichi|date=2020-10-01|title=Standing on the Shoulders of Giants: New Mass and Distance Estimates for Betelgeuse through Combined Evolutionary, Asteroseismic, and Hydrodynamic Simulations with MESA|url=https://ui.adsabs.harvard.edu/abs/2020ApJ...902...63J|journal=The Astrophysical Journal|volume=902|pages=63|doi=10.3847/1538-4357/abb8db|issn=0004-637X}}</ref>
▲|bintang paling terang ke-10 di langit malam.
|-
| [[Antares]] ''(Alpha Scorpii)'' || 680<ref>{{Cite journal|last=Ohnaka|first=Keiichi|last2=Hofmann|first2=Karl-Heinz|last3=Schertl|first3=Dieter|last4=Weigelt|first4=Gerd|last5=Baffa|first5=Carlo|last6=Chelli|first6=Alain|last7=Petrov|first7=Romain|last8=Robbe-Dubois|first8=Sylvie|date=2013-07|title=High spectral resolution imaging of the dynamical atmosphere of the red supergiant Antares in the CO first overtone lines with VLTI/AMBER|url=http://arxiv.org/abs/1304.4800|journal=Astronomy & Astrophysics|volume=555|pages=A24|doi=10.1051/0004-6361/201321063|issn=0004-6361}}</ref>
|bintang paling terang ke-15 di langit malam.
|-
| [[Rho Cassiopeiae]] || 450▼
|636–981<ref>{{Cite journal|last=van Genderen|first=A. M.|last2=Lobel|first2=A.|last3=Nieuwenhuijzen|first3=H.|last4=Henry|first4=G. W.|last5=de Jager|first5=C.|last6=Blown|first6=E.|last7=Di Scala|first7=G.|last8=van Ballegoij|first8=E. J.|date=2019-11-01|title=Pulsations, eruptions, and evolution of four yellow hypergiants|url=https://ui.adsabs.harvard.edu/abs/2019A&A...631A..48V|journal=Astronomy and Astrophysics|volume=631|pages=A48|doi=10.1051/0004-6361/201834358|issn=0004-6361}}</ref>
|
|-
| [[S Pegasi]] || 580<ref>http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=10781</ref>
Baris 117 ⟶ 126:
| [[V838 Monocerotis]]|| 467<ref>{{Cite journal|last=Kamiński|first=Tomek|last2=Tylenda|first2=Romuald|last3=Kiljan|first3=Aleksandra|last4=Schmidt|first4=Mirek|last5=Lisiecki|first5=Krzysztof|last6=Melis|first6=Carl|last7=Frankowski|first7=Adam|last8=Joshi|first8=Vishal|last9=Menten|first9=Karl M.|date=2021-11-01|title=V838 Monocerotis as seen by ALMA: A remnant of a binary merger in a triple system|url=https://ui.adsabs.harvard.edu/abs/2021A&A...655A..32K|journal=Astronomy and Astrophysics|volume=655|pages=A32|doi=10.1051/0004-6361/202141526|issn=0004-6361}}</ref>
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▲|-
▲| [[Rho Cassiopeiae]] || 450
|-
| [[Mira|Mira A]] ''(Omicron Ceti)'' || 400<ref>http://www.eso.org/~mwittkow/publications/conferences/SPIECWo5491199.pdf</ref>
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