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Baris 1:
{{Daftar tidak lengkap}}
Berikut adalah '''daftar bintang terbesar''':
{{distinguish|Daftar bintang paling masif}}
{{short description|Artikel daftar Wikipedia}}
[[Berkas:Star-sizes.jpg|500px|thumb|right|Ukuran relatif [[planet]] di [[Tata Surya]] dan beberapa [[bintang]] terkenal:
{{ordered list
| [[Merkurius (planet)|Merkurius]] < [[Mars]] < [[Venus]] < [[Bumi]]
| [[Bumi]] < [[Neptunus]] < [[Uranus]] < [[Saturnus]] < [[Jupiter]]
| [[Jupiter]] < [[Wolf 359]] < [[Matahari]] < [[Sirius A]]
| [[Sirius A]] < [[Pollux (bintang)|Pollux]] < [[Arcturus]] < [[Aldebaran]]
| [[Aldebaran]] < [[Rigel A]] < [[Antares A]] < [[Betelgeuse]]| [[Betelgeuse]] < [[Mu Cephei]] < [[VV Cephei A]] < [[VY Canis Majoris]]
}}
]]
Di bawah ini adalah '''daftar bintang terbesar''' yang diketahui saat ini, diurutkan berdasarkan [[radius]]. Satuan pengukuran yang digunakan adalah [[radius matahari|jari-jari Matahari]] (kira-kira {{convert|1|solar radius|km mi|0|abbr=on|disp=out|lk=on}}).
 
Ketidakpastian besar tetap ada pada keanggotaan dan urutan daftar, terutama ketika mendapatkan berbagai parameter yang digunakan dalam penghitungan, seperti bintang [[luminositas]] dan [[suhu efektif]]. Seringkali jari-jari bintang hanya dapat dinyatakan sebagai rata-rata atau dalam rentang nilai yang besar. Nilai untuk radius bintang sangat bervariasi di berbagai sumber dan untuk metode observasi yang berbeda.
 
Diameter sudut banyak bintang dapat diukur secara langsung menggunakan [[Interferometri optik astronomi|interferometri bintang]]. Metode lain dapat menggunakan [[okultasi]] bulan atau dari [[biner gerhana]], yang dapat digunakan untuk menguji metode tidak langsung untuk menemukan jari-jari bintang. Hanya beberapa bintang [[supergiant]] berguna yang dapat disembunyikan oleh Bulan, termasuk [[Antares]] A (Alpha Scorpii A). Contoh biner gerhana adalah [[Epsilon Aurigae]] (Almaaz), [[VV Cephei]], dan [[V766 Centauri]] (HR 5171). Pengukuran diameter sudut bisa jadi tidak konsisten karena batas atmosfer yang sangat tipis ([[Opasitas (optik)|opasitas]]) berbeda-beda bergantung pada panjang gelombang cahaya di mana [[bintang]] diamati.
 
__TOC__
 
== Daftar ==
<!-- Jangan dilepas; daftar ini tidak akan lengkap sampai kita memetakan alam semesta yang diketahui. -->
{| class="wikitable sortable"
|+Daftar bintang terbesar
|-
! style="background-color:#EFEFEF; white-space: nobr;" | Nama
! style="background-color:#FFDEAD;" colspan="2" | Ukuran dalam satuan [[Jari-jari Matahari|Radii Matahari]]<br />
([[Matahari]] = 1)
!Keterangan
|-
|[[Stephenson 2-18]]
| [[VY Canis Majoris]] || 1.800–2.100<ref name="Choi">
|2.150<ref name="thomas"/>
{{cite web
|Bintang terbesar di jagat raya (sebelumnya UY Scuti)
|title=Distance to VY VMa with VERA
|-Super raksasa merah
|publisher=Publications Astronomical Society of Japan
|author=K. Yoon Choi
|url=http://adsabs.harvard.edu/abs/2008PASJ...60.1007C
|accessdate=2010-07 16
}}</ref>
|-
| [[WOH G64]] || 1.900-2.000540<ref name="Levesque2009">{{cite web
{{cite web
|title=WOH G64: The Largest Star Known?
|publisher=Astronomical Journal
Baris 24 ⟶ 41:
|accessdate=2010-07 16
}}</ref>
|
|-
| [[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>
| [[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
|-
| [[VY Canis Majoris]] || 1.420<ref>{{Cite journal|last=Wittkowski|first=M.|last2=Hauschildt|first2=P. H.|last3=Torres|first3=B. Arroyo|last4=Marcaide|first4=J. M.|date=2012-04|title=Fundamental properties and atmospheric structure of the red supergiant VY CMa based on VLTI/AMBER spectro-interferometry|url=http://arxiv.org/abs/1203.5194|journal=Astronomy & Astrophysics|volume=540|pages=L12|doi=10.1051/0004-6361/201219126|issn=0004-6361}}</ref><ref>{{Cite journal|last=Gordon|first=Michael S.|last2=Jones|first2=Terry J.|last3=Humphreys|first3=Roberta M.|last4=Ertel|first4=Steve|last5=Hinz|first5=Philip M.|last6=Hoffmann|first6=William F.|date=2019-01-18|title=Thermal Emission in the Southwest Clump of VY CMa|url=https://doi.org/10.3847/1538-3881/aaf5cb|journal=The Astronomical Journal|volume=157|issue=2|pages=57|doi=10.3847/1538-3881/aaf5cb|issn=1538-3881}}</ref>
|
|-
| [[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" />
|
|-
|[[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>
|
|-
| [[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>
|
|-
|[[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>
|
|-
|[[MY Cephei]]
|1.134<ref>{{Cite journal|last=Beasor|first=Emma R.|last2=Davies|first2=Ben|date=2018-03-01|title=The evolution of red supergiant mass-loss rates|url=https://ui.adsabs.harvard.edu/abs/2018MNRAS.475...55B|journal=Monthly Notices of the Royal Astronomical Society|volume=475|pages=55–62|doi=10.1093/mnras/stx3174|issn=0035-8711}}</ref>
|
|-
| [[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
|title=VV CEP (VV Cephei)
|publisher=University of Illinois
Baris 32 ⟶ 73:
|url=http://www.astro.uiuc.edu/~kaler/sow/vvcep.html
|accessdate=2010-03-15
|archive-date=2009-02-01
}}</ref>
|archive-url=https://web.archive.org/web/20090201112518/http://www.astro.uiuc.edu/~kaler/sow/vvcep.html
|dead-url=yes
}}</ref>
|
|-
| [[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>
| [[Mu Cephei]] || 1.650<ref name="Levesque2005">
|
{{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>
|-
| [[V838 Monocerotis]] || 1.570 atau 800<ref>[[V838 Monocerotis]]</ref>
|-
| [[V354 Cephei]] || 1.520{{Citation needed|date=December 2009}}
|-
| [[RW Cephei]] || 1.260–1.610{{Citation needed|date=December 2009}}
|-
| [[KW Sagittarii]] || 1.460{{Citation needed|date=December 2009}}
|-
| [[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>
| [[KY Cygni]] || 1.420 atau 1.440{{Citation needed|date=December 2009}}
|bintang paling terang ke-10 di langit malam.
|-
| [[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>
| [[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>
|
|-
| [[UY Scuti]] || 755
| [[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>
|
|-
| [[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>
| [[V382 Carinae]] || 747
|bintang paling terang ke-15 di langit malam.
|-
| [[S Pegasi]] || 580<ref>http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=10781</ref>
|
|-
| [[{{ill|T Cephei]] |en}}|| 540<ref>http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=9837</ref>
|
|-
| [[S Orionis]] || 530<ref>http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=2512</ref>
|
|-
| [[{{ill|W Hydrae]] |en}}|| 520<ref>http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=6127</ref>
|
|-
| [[{{Ill|R Cassiopeiae]] |en}}|| 500<ref>http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=10947</reFref>
|
|-
| [[V382 Carinae]] || 485<ref>{{Cite journal|last=Groenewegen|first=M. A. T.|date=2020-03|title=Analysing the spectral energy distributions of Galactic classical Cepheids|url=http://arxiv.org/abs/2002.02186|journal=Astronomy & Astrophysics|volume=635|pages=A33|doi=10.1051/0004-6361/201937060|issn=0004-6361}}</ref>
| [[Chi Cygni]] || 470<ref>http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=9107</ref>
|Hypergiant paling terang di langit.
|-
| {{ill|Chi Cygni|en}} || 470<ref>http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=9107</ref>
| [[Alpha Herculis]] ''(Ras Algethi)'' || 460
|
|-
| [[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>
|
|-
| [[Rho Cassiopeiae]] || 450
|-
| [[Mira|Mira A]] ''(Omicron Ceti)'' || 400<ref>http://www.eso.org/~mwittkow/publications/conferences/SPIECWo5491199.pdf</ref>
|
|-
| [[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 |archive-date=2012-05-19 |archive-url=https://web.archive.org/web/20120519234705/http://www.weblore.com/richard/garnet_star.htm |dead-url=yes }}</ref>
|
|-
| [[S Doradus]] || 100–380<ref>
Baris 91 ⟶ 138:
| accessdate=2009-03-25 | bibcode=1995ASPC...83..176L
}}</ref>
|-
| [[R Doradus]] || 370
|-
| [[HR Carinae]] || 350
|
|-
| [[R Doradus]] || 298 ± 21<ref>{{Cite journal|last=Ohnaka|first=Keiichi|last2=Weigelt|first2=Gerd|last3=Hofmann|first3=Karl-Heinz|date=2019-09-01|title=Infrared Interferometric Three-dimensional Diagnosis of the Atmospheric Dynamics of the AGB Star R Dor with VLTI/AMBER|url=https://ui.adsabs.harvard.edu/abs/2019ApJ...883...89O|journal=The Astrophysical Journal|volume=883|pages=89|doi=10.3847/1538-4357/ab3d2a|issn=0004-637X}}</ref>
| [[R Leonis]] || 350<ref>http://arxiv.org/abs/astro-ph/0411133</ref>
|
|-
| [[Alpha Herculis]] ''(Ras Algethi)'' || 284 ± 60<ref>{{Cite journal|last=Moravveji|first=Ehsan|last2=Guinan|first2=Edward F.|last3=Khosroshahi|first3=Habib G.|last4=Wasatonic|first4=Rick|date=2013-11-01|title=The Age and The Mass of The \alpha Herculis Triple-Star System From A MESA Grid of rotating stars with 1.3|url=http://arxiv.org/abs/1308.1632|journal=The Astronomical Journal|volume=146|issue=6|pages=148|doi=10.1088/0004-6256/146/6/148|issn=0004-6256}}</ref>
| [[Pistol Star|The Pistol Star]] || 340
|
|-
| [[Eta Carinae]] || 240<ref>{{Cite journal|last=Gull|first=Theodore R.|last2=Damineli|first2=Augusto|date=2009-11|title=Eta Carinae in the Context of the Most Massive Stars|url=http://arxiv.org/abs/0910.3158|journal=Proceedings of the International Astronomical Union|volume=5|issue=H15|pages=373–398|doi=10.1017/S1743921310009890|issn=1743-9213}}</ref> (60 – 881)<ref>{{Cite journal|last=Hillier|first=D. John|last2=Davidson|first2=K.|last3=Ishibashi|first3=K.|last4=Gull|first4=T.|date=2001-06-01|title=On the Nature of the Central Source in η Carinae|url=https://ui.adsabs.harvard.edu/abs/2001ApJ...553..837H|journal=The Astrophysical Journal|volume=553|pages=837–860|doi=10.1086/320948|issn=0004-637X}}</ref>
| [[Alpha Draconis]] ''(Thuban)'' || 265
|
|-
| {{Ill|La Superba|en}}|| 225
| [[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>
|
|-
| [[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>
| [[La Superba]] ''([[Y Canum Venaticorum]])'' || 225
|bintang paling terang ke-36 di langit malam.
|-
| [[Epsilon Pegasi]] ''(Enif)'' || 211<ref>{{Cite journal|last=Stock|first=S.|last2=Reffert|first2=S.|last3=Quirrenbach|first3=A.|date=2018-05-01|title=VizieR Online Data Catalog: Stellar parameters of 372 giant stars (Stock+, 2018)|url=https://ui.adsabs.harvard.edu/abs/2018yCat..36160033S|journal=VizieR Online Data Catalog|pages=J/A+A/616/A33|doi=10.26093/cds/vizier.36160033}}</ref>
| [[Deneb]] ''(Alpha Cygni)'' || 220
|
|-
| [[Deneb]] ''(Alpha Cygni)'' || 203 ± 17<ref>{{Cite journal|last=Schiller|first=Florian|last2=Przybilla|first2=Norbert|date=2008-03|title=Quantitative spectroscopy of Deneb|url=http://arxiv.org/abs/0712.0040|journal=Astronomy & Astrophysics|volume=479|issue=3|pages=849–858|doi=10.1051/0004-6361:20078590|issn=0004-6361}}</ref>
| [[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>
|bintang paling terang ke-19 di langit malam.
|-
| [[Zeta Aurigae]] || 200<ref>{{Cite web |url=http://www.hposoft.com/EAur09/ZetaAurigae.html] |title=Salinan arsip |access-date=2010-10-07 |archive-date=2012-03-21 |archive-url=https://web.archive.org/web/20120321213715/http://www.hposoft.com/EAur09/ZetaAurigae.html |dead-url=yes }}</ref>
|
|-
| [[Epsilon Aurigae]] A || 143 – 358<ref>{{Cite journal|last=Kloppenborg|first=Brian|last2=Stencel|first2=Robert|last3=Monnier|first3=John D.|last4=Schaefer|first4=Gail|last5=Baron|first5=Fabien|last6=Tycner|first6=Chris|last7=Zavala|first7=Robert T.|last8=Hutter|first8=Donald|last9=Zhao|first9=Ming|date=2015-09-21|title=Interferometry of $\epsilon$ Aurigae: Characterization of the asymmetric eclipsing disk|url=http://arxiv.org/abs/1508.01909|journal=The Astrophysical Journal Supplement Series|volume=220|issue=1|pages=14|doi=10.1088/0067-0049/220/1/14|issn=1538-4365}}</ref>
| [[Eta Carinae]] || 85–195<ref>http://etacar.umn.edu/etainfo/basic/</ref>
|-
| [[Epsilon Aurigae]] A || 175
|-
| [[Epsilon Carinae]] || 153
|Bintang paling terang ke-39 di langit malam.
|-
| [[{{Ill|LBV 1806-20]] |en}}|| 150
|-
| [[Epsilon Pegasi]] ''(Enif)'' || 150
|-
| [[Gamma Crucis]] ''(Gacrux)'' || 113<ref>Gamma Crucis by Jim Kaler]</ref>
|
|-
| [[Gamma Andromedae]] || 8380
|
|-
| [[Rigel]] ''(Beta Orionis)'' || 78.9<ref>{{Cite journal|last=Moravveji|first=Ehsan|last2=Guinan|first2=Edward F.|last3=Shultz|first3=Matt|last4=Williamson|first4=Michael H.|last5=Moya|first5=Andres|date=2012-03-10|title=Asteroseismology of the Nearby SN-II Progenitor: Rigel Part I. The MOST High Precision Photometry and Radial Velocity Monitoring|url=http://arxiv.org/abs/1201.0843|journal=The Astrophysical Journal|volume=747|issue=2|pages=108|doi=10.1088/0004-637X/747/2/108|issn=0004-637X}}</ref>
| [[Rigel]] ''(Beta Orionis)'' || 78
|Bintang paling terang ke-7 di langit malam.
|-
| [[Alpha Leporis]] ''(Arneb)'' || 7775
|
|-
| [[Canopus]] ''(Alpha Carinae)''|| 73.3<ref>{{Cite journal|last=de Souza|first=A. Domiciano|last2=Zorec|first2=J.|last3=Millour|first3=F.|last4=Bouquin|first4=J.-B. Le|last5=Spang|first5=A.|last6=Vakili|first6=F.|date=2021-10|title=Refined fundamental parameters of Canopus from combined near-IR interferometry and spectral energy distribution|url=http://arxiv.org/abs/2109.07153|journal=Astronomy & Astrophysics|volume=654|pages=A19|doi=10.1051/0004-6361/202140478|issn=0004-6361}}</ref>
| [[R Coronae Borealis]] || 65
|bintang paling terang ke-2 di langit malam.
|-
| [[Alpha Persei]] ''(Mirfak)''|| 68<ref>{{Cite journal|last=Nordgren|first=Tyler E.|last2=Germain|first2=M. E.|last3=Benson|first3=J. A.|last4=Mozurkewich|first4=D.|last5=Sudol|first5=J. J.|last6=Elias|first6=N. M., II|last7=Hajian|first7=Arsen R.|last8=White|first8=N. M.|last9=Hutter|first9=D. J.|date=1999-12-01|title=Stellar Angular Diameters of Late-Type Giants and Supergiants Measured with the Navy Prototype Optical Interferometer|url=https://ui.adsabs.harvard.edu/abs/1999AJ....118.3032N|journal=The Astronomical Journal|volume=118|pages=3032–3038|doi=10.1086/301114|issn=0004-6256}}</ref>
| [[Canopus (star)|Canopus]] ''(Alpha Carinae)'' || 65
|bintang paling terang ke-35 di langit malam.
|-
| [[Albireo]] (Beta Cygni Aa'')''|| 62<ref>{{Cite journal|last=Drimmel|first=Ronald|last2=Sozzetti|first2=Alessandro|last3=Schroeder|first3=Klaus-Peter|last4=Bastian|first4=Ulrich|last5=Pinamonti|first5=Matteo|last6=Jack|first6=Dennis|last7=Huerta|first7=Missael A. Hernandez|date=2021-01-28|title=A celestial matryoshka: Dynamical and spectroscopic analysis of the Albireo system|url=http://arxiv.org/abs/2012.01277|journal=Monthly Notices of the Royal Astronomical Society|volume=502|issue=1|pages=328–350|doi=10.1093/mnras/staa4038|issn=0035-8711}}</ref>
| [[Delta Orionis]] ''(Mintaka)'' || 60
|
|-
| [[Zeta Geminorum]] ''(Mekbuda)''|| 65.24<ref>{{Cite journal|last=Groenewegen|first=M. A. T.|date=2007-11-01|title=The projection factor, period-radius relation, and surface-brightness colour relation in classical cepheids|url=https://ui.adsabs.harvard.edu/abs/2007A&A...474..975G|journal=Astronomy and Astrophysics|volume=474|pages=975–981|doi=10.1051/0004-6361:20078225|issn=0004-6361}}</ref>
| [[Alpha Persei]] ''(Mirfak)'' || 60
|
|-
| [[Alpha Hydrae]] ''(Alphard)''|| 50.5<ref>{{Cite journal|last=da Silva|first=L.|last2=Girardi|first2=L.|last3=Pasquini|first3=L.|last4=Setiawan|first4=J.|last5=von der Luhe|first5=O.|last6=de Medeiros|first6=J. R.|last7=Hatzes|first7=A.|last8=Dollinger|first8=M. P.|last9=Weiss|first9=A.|date=2006-11|title=Basic physical parameters of a selected sample of evolved stars|url=http://arxiv.org/abs/astro-ph/0608160|journal=Astronomy & Astrophysics|volume=458|issue=2|pages=609–623|doi=10.1051/0004-6361:20065105|issn=0004-6361}}</ref>
| [[Zeta Geminorum]] ''(Mekbuda)'' || 60
|-
| [[Eta Aquilae]] || 60
|-
| [[Gamma Draconis]] ''(Eltanin)'' || 50
|-
| [[Aldebaran]] ''(Alpha Tauri)'' || 43<ref>http://adsabs.harvard.edu/abs/2005astro.ph..2181R</ref>
|Bintang paling terang ke-14 di langit malam.
|-
| [[{{ill|Beta Ursae Minoris]]|en}} ''(Kochab)'' || 41
|
|-
|[[Polaris]]
| [[Beta Draconis]] ''(Rastaban)'' || 40
|37.5<ref>{{Cite journal|last=Fadeyev|first=Yu A.|date=2015-05-01|title=Evolutionary status of Polaris|url=http://arxiv.org/abs/1502.06463|journal=Monthly Notices of the Royal Astronomical Society|volume=449|issue=1|pages=1011–1017|doi=10.1093/mnras/stv412|issn=1365-2966}}</ref>
|
|-
|[[Arcturus]]
|25.4<ref>{{Cite journal|last=Ramirez|first=I.|last2=Prieto|first2=C. Allende|date=2011-12-20|title=Fundamental Parameters and Chemical Composition of Arcturus|url=http://arxiv.org/abs/1109.4425|journal=The Astrophysical Journal|volume=743|issue=2|pages=135|doi=10.1088/0004-637X/743/2/135|issn=0004-637X}}</ref>
|Bintang paling terang ke-4 di langit malam.
|-
| [[Zeta Orionis]] ''(Alnitak)'' || 20
|bintang paling terang ke-32 di langit malam.
|-
| [[Mintaka]] ''(Delta Orionis)''|| 16.5<ref>{{Cite journal|last=Shenar|first=T.|last2=Oskinova|first2=L.|last3=Hamann|first3=W. -R.|last4=Corcoran|first4=M. F.|last5=Moffat|first5=A. F. J.|last6=Pablo|first6=H.|last7=Richardson|first7=N. D.|last8=Waldron|first8=W. L.|last9=Huenemoerder|first9=D. P.|date=2015-08-01|title=A Coordinated X-Ray and Optical Campaign of the Nearest Massive Eclipsing Binary, δ Orionis Aa. IV. A Multiwavelength, Non-LTE Spectroscopic Analysis|url=https://ui.adsabs.harvard.edu/abs/2015ApJ...809..135S|journal=The Astrophysical Journal|volume=809|pages=135|doi=10.1088/0004-637X/809/2/135|issn=0004-637X}}</ref>
|
|-
| [[Zeta Puppis]] ''(Naos)''|| 14 – 26<ref>{{Cite journal|last=Schilbach|first=E.|last2=Röser|first2=S.|date=2008-10-01|title=On the origin of field O-type stars|url=https://ui.adsabs.harvard.edu/abs/2008A&A...489..105S|journal=Astronomy and Astrophysics|volume=489|pages=105–114|doi=10.1051/0004-6361:200809936|issn=0004-6361}}</ref>
|
|-
|[[Beta Geminorum|Pollux]]
| [[Zeta Puppis]] ''(Naos)'' || 18.6
|9.06<ref>{{Cite journal|last=Baines|first=Ellyn K.|last2=Armstrong|first2=J. Thomas|last3=Schmitt|first3=Henrique R.|last4=Zavala|first4=R. T.|last5=Benson|first5=James A.|last6=Hutter|first6=Donald J.|last7=Tycner|first7=Christopher|last8=van Belle|first8=Gerard T.|date=2017-12-20|title=Fundamental Parameters of 87 Stars from the Navy Precision Optical Interferometer|url=http://arxiv.org/abs/1712.08109|journal=The Astronomical Journal|volume=155|issue=1|pages=30|doi=10.3847/1538-3881/aa9d8b|issn=1538-3881}}</ref>
|Bintang paling terang ke-17 di langit malam.
|-
|[[Sirius]] A
| [[Beta Cygni]] A1 ''(Albireo)'' || 16
|1.711<ref>{{Cite journal|last=Liebert|first=James|last2=Young|first2=Patrick A.|last3=Arnett|first3=David|last4=Holberg|first4=J. B.|last5=Williams|first5=Kurtis A.|date=2005-09-01|title=The Age and Progenitor Mass of Sirius B|url=http://arxiv.org/abs/astro-ph/0507523|journal=The Astrophysical Journal|volume=630|issue=1|pages=L69–L72|doi=10.1086/462419|issn=0004-637X}}</ref>
|Bintang paling terang di langit malam.
|}
 
== Lihat pula ==
{{Portal|Bintang}}
{{cmn|colwidth=18em|
* [[Rasi bintang]]
* [[Daftar bintang]]
* [[Daftar bintang paling masif]]
* [[Daftar bintang paling bercahaya]]
* [[Daftar bintang terpanas]]
* [[Daftar lubang hitam paling masif]]
* [[Daftar nebula terbesar]]
* [[Daftar galaksi terbesar]]
* [[Daftar struktur kosmik terbesar]]
* [[Daftar planet ekstrasurya terbesar]]
* [[Daftar bintang yang ekstrim]]
* [[Bintang]]
}}
 
== Referensi ==
{{wikiportal|Astronomi}}
{{Reflist}}
 
== Pranala luar ==
* [http://www.giantstars.de/ '''Giant Stars''' An interactive website comparing the Earth and the Sun to some of the largest known stars]
* [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 }}
* [http://news.bbc.co.uk/2/hi/science/nature/4164365.stm '''BBC News''' Three largest stars identified]
* [http://www.youtube.com/watch?v=Tfs1t-2rrOM Star Size comparison movie]
* [http://video.google.com/videoplay?docid=-3974466981713172831&sourceid=Himself '''Google Video''' Planets and stars drawn to scale] {{Webarchive|url=https://web.archive.org/web/20090107210444/http://video.google.com/videoplay?docid=-3974466981713172831&sourceid=Himself |date=2009-01-07 }}
* [http://www.universetoday.com/2008/04/06/what-is-the-biggest-star-in-the-universe/ '''Universe Today''' What is the Biggest Star in the Universe?]
 
[[Kategori:Daftar bintang]]
 
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[[en:List of largest known stars]]
[[es:Anexo:Estrellas más grandes conocidas]]
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[[fi:Luettelo suurimmista tähdistä]]
[[fr:Liste des étoiles géantes (par taille décroissante)]]
[[gl:Lista das estrelas máis grandes coñecidas]]
[[it:Lista delle stelle più grandi conosciute]]
[[ja:直径の大きい恒星の一覧]]
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[[pl:Lista największych gwiazd]]
[[pt:Anexo:Lista das maiores estrelas conhecidas]]
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