Wikipedia

Daftar bintang terbesar: Perbedaan antara revisi

Jelajahi riwayat secara interaktif
← Revisi sebelumnya
Konten dihapus Konten ditambahkan
VisualTeks wiki
Tidak ada ringkasan suntingan
Tag: Suntingan perangkat seluler Suntingan peramban seluler
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.
Tag: VisualEditor Suntingan perangkat seluler Suntingan peramban seluler
 
(27 revisi perantara oleh 11 pengguna tidak ditampilkan)
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
|-
|-Super raksasa merah
|[[UY Scuti]]
|1.516--1.900
|Bintang terbesar di jagat raya
|-Red supergiant
| [[V838 Monocerotis]] || 1.570 atau 800<ref>[[V838 Monocerotis]]</ref>
|
|-
| [[WOH G64]] || 1.540<ref name="Levesque2009">{{cite web
Baris 21 ⟶ 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
|1.450<ref>{{Cite journal|last=Decin|first=Leen|last2=Richards|first2=Anita M. S.|last3=Marchant|first3=Pablo|last4=Sana|first4=Hugues|date=2024-01|title=ALMA detection of CO rotational line emission in red supergiant stars of the massive young star cluster RSGC1 -- Determination of a new mass-loss rate prescription for red supergiants|url=http://arxiv.org/abs/2303.09385|journal=Astronomy & Astrophysics|volume=681|pages=A17|doi=10.1051/0004-6361/202244635|issn=0004-6361}}</ref>
|
|-
| [[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>
| [[V354 Cephei]] || 1.520{{Citation needed|date=December 2009}}
|
|-
|[[AH Scorpii]]
| [[KW Sagittarii]] || 1.460{{Citation needed|date=December 2009}}
|1.411<ref name=":1" />
|
|-
|[[S Persei]]
| [[KY Cygni]] || 1.420{{Citation needed|date=December 2009}}
|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>
|
|-
|[[VX Sagittarii]]
| [[VY Canis Majoris]] || 1.420
|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>
|
|-
| [[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">{{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]] || 1.050<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
|author=Professor James B. (Jim) Kaler
|url=http://www.astro.uiuc.edu/~kaler/sow/vvcep.html
|accessdate=2010-03-15
}}</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>
| [[Mu Cephei]] || 1.400<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>
|-
|[[WOH S264]]
| [[RW Cephei]] || 1.260–1.610{{Citation needed|date=December 2009}}
|1.210<ref><nowiki>https://arxiv.org/abs/2405.11019</nowiki></ref>
|
|-
|[[MY Cephei]]
| [[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>
|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>
|
|-
|[[HR 5171|V766 Centauri]] Aa
| [[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>
|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>
|
|-
| [[V382KY CarinaeCygni]] || 747
|1.033<ref>{{Cite journal|last=Comerón|first=F.|last2=Djupvik|first2=A. A.|last3=Schneider|first3=N.|last4=Pasquali|first4=A.|date=2020-12-01|title=The historical record of massive star formation in Cygnus|url=https://ui.adsabs.harvard.edu/abs/2020A&A...644A..62C|journal=Astronomy and Astrophysics|volume=644|pages=A62|doi=10.1051/0004-6361/202039188|issn=0004-6361}}</ref>
|
|-
| [[KW Sagittarii]]|| 1.009 ± 142<ref name=":1">{{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>
|
|-
| [[UY Scuti]]|| 909<ref name=":2" />
|
|-
|[[VV Cephei|VV Cephei A]]
|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>
|
|-
| [[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)''|| 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]]
|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>
|
|-
| [[{{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 90 ⟶ 145:
| 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>
|-
| [[La Superba]] ''([[Y Canum Venaticorum]])'' || 225
|-
| [[Deneb]] ''(Alpha Cygni)'' || 220
|-
| [[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-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>
| [[Zeta Aurigae]] || 200<ref>http://www.hposoft.com/EAur09/ZetaAurigae.html]</ref>
|
|-
| [[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>
| [[Eta Carinae]] || 85–195<ref>http://etacar.umn.edu/etainfo/basic/</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 || 175
|
|-
| [[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>
|
|-
| [[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)'' || 18.6
|
|-
| [[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 Cygni]] A1 ''(Albireo)'' || 16
|
|-
|[[Beta Geminorum|Pollux]]
|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
|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?]
 
Diperoleh dari "https://wiki-indonesia.club/wiki/Daftar_bintang_terbesar"