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Daftar bintang terbesar

Dari Wikipedia bahasa Indonesia, ensiklopedia bebas
Artikel ini bukan mengenai Daftar bintang paling masif.
Ukuran relatif planet di Tata Surya dan beberapa bintang terkenal:

Di bawah ini adalah daftar bintang terbesar yang diketahui saat ini, diurutkan berdasarkan radius. Satuan pengukuran yang digunakan adalah jari-jari Matahari (kira-kira 695.700 km; 432.288 mi).

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 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) berbeda-beda bergantung pada panjang gelombang cahaya di mana bintang diamati.

Daftar

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Daftar bintang terbesar
Nama Ukuran dalam satuan Radii Matahari

(Matahari = 1)

Keterangan
WOH G64 1.540[1] Mungkin bintang terbesar yang diketahui.[1][2][3]
RSGC1-F01 1.450[4]
VY Canis Majoris 1.420[5][6]
AH Scorpii 1.411[7]
S Persei 1.364[8]
VX Sagittarii 1.356[9]–1.480[10]
Mu Cephei 1.259[11] – 1.420[12]
V354 Cephei 1.245[13]
WOH S264 1.210[14]
MY Cephei 1.134[15]
V766 Centauri Aa 1.060 — 1.160[16]
KY Cygni 1.033[17]
KW Sagittarii 1.009 ± 142[7]
UY Scuti 909[13]
VV Cephei A 779.27[18]
RW Cephei 900–1760[19]
Betelgeuse (Alpha Orionis) 764[20] bintang paling terang ke-10 di langit malam.
Antares (Alpha Scorpii) 680[21] bintang paling terang ke-15 di langit malam.
Rho Cassiopeiae 636–981[22]
S Pegasi 580[23]
T Cephei [en] 540[24]
S Orionis 530[25]
W Hydrae [en] 520[26]
R Cassiopeiae [en] 500[27]
V382 Carinae 485[28] Hypergiant paling terang di langit.
Chi Cygni [en] 470[29]
V838 Monocerotis 467[30]
Mira A (Omicron Ceti) 400[31]
V509 Cassiopeiae 400[32]–900[33]
S Doradus 100–380[34]
HR Carinae 350
R Doradus 298 ± 21[35]
Alpha Herculis (Ras Algethi) 284 ± 60[36]
Eta Carinae 240[37] (60 – 881)[38]
La Superba [en] 225
Delta Canis Majoris (Wezen) 215±66[39] bintang paling terang ke-36 di langit malam.
Epsilon Pegasi (Enif) 211[40]
Deneb (Alpha Cygni) 203 ± 17[41] bintang paling terang ke-19 di langit malam.
Zeta Aurigae 200[42]
Epsilon Aurigae A 143 – 358[43]
Epsilon Carinae 153 Bintang paling terang ke-39 di langit malam.
LBV 1806-20 [en] 150
Gamma Crucis (Gacrux) 113[44]
Gamma Andromedae 80
Rigel (Beta Orionis) 78.9[45] Bintang paling terang ke-7 di langit malam.
Alpha Leporis (Arneb) 75
Canopus (Alpha Carinae) 73.3[46] bintang paling terang ke-2 di langit malam.
Alpha Persei (Mirfak) 68[47] bintang paling terang ke-35 di langit malam.
Albireo (Beta Cygni Aa) 62[48]
Zeta Geminorum (Mekbuda) 65.24[49]
Alpha Hydrae (Alphard) 50.5[50]
Aldebaran (Alpha Tauri) 43[51] Bintang paling terang ke-14 di langit malam.
Beta Ursae Minoris [en] (Kochab) 41
Polaris 37.5[52]
Arcturus 25.4[53] 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[54]
Zeta Puppis (Naos) 14 – 26[55]
Pollux 9.06[56] Bintang paling terang ke-17 di langit malam.
Sirius A 1.711[57] Bintang paling terang di langit malam.

Lihat pula

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Referensi

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  1. ^ a b E. M. Levesque. "WOH G64: The Largest Star Known?". Astronomical Journal. Diakses tanggal 2010-07 16. 
  2. ^ Jones, O. C.; Woods, P. M.; Kemper, F.; Kraemer, K. E.; Sloan, G. C.; Srinivasan, S.; Oliveira, J. M.; Van Loon, J. Th.; Boyer, M. L. (2017-09). "The SAGE-Spec Spitzer Legacy program: the life-cycle of dust and gas in the Large Magellanic Cloud. Point source classification – III". Monthly Notices of the Royal Astronomical Society (dalam bahasa Inggris). 470 (3): 3250–3282. doi:10.1093/mnras/stx1101. ISSN 0035-8711. 
  3. ^ de Wit, S.; Bonanos, A. Z.; Tramper, F.; Yang, M.; Maravelias, G.; Boutsia, K.; Britavskiy, N.; Zapartas, E. (2023-01-01). "Properties of luminous red supergiant stars in the Magellanic Clouds". Astronomy and Astrophysics. 669: A86. doi:10.1051/0004-6361/202243394. ISSN 0004-6361. 
  4. ^ Decin, Leen; Richards, Anita M. S.; Marchant, Pablo; Sana, Hugues (2024-01). "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". Astronomy & Astrophysics. 681: A17. doi:10.1051/0004-6361/202244635. ISSN 0004-6361. 
  5. ^ Wittkowski, M.; Hauschildt, P. H.; Torres, B. Arroyo; Marcaide, J. M. (2012-04). "Fundamental properties and atmospheric structure of the red supergiant VY CMa based on VLTI/AMBER spectro-interferometry". Astronomy & Astrophysics. 540: L12. doi:10.1051/0004-6361/201219126. ISSN 0004-6361. 
  6. ^ Gordon, Michael S.; Jones, Terry J.; Humphreys, Roberta M.; Ertel, Steve; Hinz, Philip M.; Hoffmann, William F. (2019-01-18). "Thermal Emission in the Southwest Clump of VY CMa". The Astronomical Journal. 157 (2): 57. doi:10.3847/1538-3881/aaf5cb. ISSN 1538-3881. 
  7. ^ a b Arroyo-Torres, B.; Wittkowski, M.; Marcaide, J. M.; Hauschildt, P. H. (2013-06). "The atmospheric structure and fundamental parameters of the red supergiants AH Sco, UY Sct and KW Sgr". Astronomy & Astrophysics. 554: A76. doi:10.1051/0004-6361/201220920. ISSN 0004-6361. 
  8. ^ Norris, Ryan P. (2019). "Seeing Stars Like Never Before: A Long-term Interferometric Imaging Survey of Red Supergiants" (PDF). Georgia State University. 
  9. ^ Tabernero, H. M.; Dorda, R.; Negueruela, I.; Marfil, E. (2021-02-01). "The nature of VX Sagitarii - Is it a TŻO, a RSG, or a high-mass AGB star?". Astronomy & Astrophysics (dalam bahasa Inggris). 646: A98. doi:10.1051/0004-6361/202039236. ISSN 0004-6361. 
  10. ^ Wallström, S. H. J.; Danilovich, T.; Müller, H. S. P.; Gottlieb, C. A.; Maes, S.; Sande, M. Van de; Decin, L.; Richards, A. M. S.; Baudry, A. (2024-01-01). "ATOMIUM: Molecular inventory of 17 oxygen-rich evolved stars observed with ALMA". Astronomy & Astrophysics (dalam bahasa Inggris). 681: A50. doi:10.1051/0004-6361/202347632. ISSN 0004-6361. 
  11. ^ Josselin, E.; Plez, B. (2007-07). "Atmospheric dynamics and the mass loss process in red supergiant stars". Astronomy & Astrophysics. 469 (2): 671–680. doi:10.1051/0004-6361:20066353. ISSN 0004-6361. 
  12. ^ Levesque, Emily M.; Massey, Philip; Olsen, K. A. G.; Plez, Bertrand; Josselin, Eric; Maeder, Andre; Meynet, Georges (2005-08). "The Effective Temperature Scale of Galactic Red Supergiants: Cool, But Not As Cool As We Thought". The Astrophysical Journal. 628 (2): 973–985. doi:10.1086/430901. ISSN 0004-637X. 
  13. ^ a b Healy, Sarah; Horiuchi, Shunsaku; Molla, Marta Colomer; Milisavljevic, Dan; Tseng, Jeff; Bergin, Faith; Weil, Kathryn; Tanaka, Masaomi (2024-03-23). "Red Supergiant Candidates for Multimessenger Monitoring of the Next Galactic Supernova". Monthly Notices of the Royal Astronomical Society. 529 (4): 3630–3650. doi:10.1093/mnras/stae738. ISSN 0035-8711. 
  14. ^ https://arxiv.org/abs/2405.11019
  15. ^ Beasor, Emma R.; Davies, Ben (2018-03-01). "The evolution of red supergiant mass-loss rates". Monthly Notices of the Royal Astronomical Society. 475: 55–62. doi:10.1093/mnras/stx3174. ISSN 0035-8711. 
  16. ^ van Genderen, A. M.; Lobel, A.; Nieuwenhuijzen, H.; Henry, G. W.; de Jager, C.; Blown, E.; Di Scala, G.; van Ballegoij, E. J. (2019-11). "Pulsations, eruptions, and evolution of four yellow hypergiants". Astronomy & Astrophysics. 631: A48. doi:10.1051/0004-6361/201834358. ISSN 0004-6361. 
  17. ^ Comerón, F.; Djupvik, A. A.; Schneider, N.; Pasquali, A. (2020-12-01). "The historical record of massive star formation in Cygnus". Astronomy and Astrophysics. 644: A62. doi:10.1051/0004-6361/202039188. ISSN 0004-6361. 
  18. ^ Baines, Ellyn K.; Armstrong, J. Thomas; Clark, James H.; Gorney, Jim; Hutter, Donald J.; Jorgensen, Anders M.; Kyte, Casey; Mozurkewich, David; Nisley, Ishara (2021-10). "Angular Diameters and Fundamental Parameters of Forty-four Stars from the Navy Precision Optical Interferometer". The Astronomical Journal (dalam bahasa Inggris). 162 (5): 198. doi:10.3847/1538-3881/ac2431. ISSN 1538-3881. 
  19. ^ Anugu, Narsireddy; Baron, Fabien; Gies, Douglas R.; Lanthermann, Cyprien; Schaefer, Gail H.; Shepard, Katherine A.; Brummelaar, Theo ten; Monnier, John D.; Kraus, Stefan (2023-07). "The Great Dimming of the Hypergiant Star RW Cephei: CHARA Array Images and Spectral Analysis". The Astronomical Journal (dalam bahasa Inggris). 166 (2): 78. doi:10.3847/1538-3881/ace59d. ISSN 1538-3881. 
  20. ^ Joyce, Meridith; Leung, Shing-Chi; Molnár, László; Ireland, Michael; Kobayashi, Chiaki; Nomoto, Ken'ichi (2020-10-01). "Standing on the Shoulders of Giants: New Mass and Distance Estimates for Betelgeuse through Combined Evolutionary, Asteroseismic, and Hydrodynamic Simulations with MESA". The Astrophysical Journal. 902: 63. doi:10.3847/1538-4357/abb8db. ISSN 0004-637X. 
  21. ^ Ohnaka, Keiichi; Hofmann, Karl-Heinz; Schertl, Dieter; Weigelt, Gerd; Baffa, Carlo; Chelli, Alain; Petrov, Romain; Robbe-Dubois, Sylvie (2013-07). "High spectral resolution imaging of the dynamical atmosphere of the red supergiant Antares in the CO first overtone lines with VLTI/AMBER". Astronomy & Astrophysics. 555: A24. doi:10.1051/0004-6361/201321063. ISSN 0004-6361. 
  22. ^ van Genderen, A. M.; Lobel, A.; Nieuwenhuijzen, H.; Henry, G. W.; de Jager, C.; Blown, E.; Di Scala, G.; van Ballegoij, E. J. (2019-11-01). "Pulsations, eruptions, and evolution of four yellow hypergiants". Astronomy and Astrophysics. 631: A48. doi:10.1051/0004-6361/201834358. ISSN 0004-6361. 
  23. ^ http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=10781
  24. ^ http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=9837
  25. ^ http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=2512
  26. ^ http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=6127
  27. ^ http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=10947
  28. ^ Groenewegen, M. A. T. (2020-03). "Analysing the spectral energy distributions of Galactic classical Cepheids". Astronomy & Astrophysics. 635: A33. doi:10.1051/0004-6361/201937060. ISSN 0004-6361. 
  29. ^ http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=9107
  30. ^ Kamiński, Tomek; Tylenda, Romuald; Kiljan, Aleksandra; Schmidt, Mirek; Lisiecki, Krzysztof; Melis, Carl; Frankowski, Adam; Joshi, Vishal; Menten, Karl M. (2021-11-01). "V838 Monocerotis as seen by ALMA: A remnant of a binary merger in a triple system". Astronomy and Astrophysics. 655: A32. doi:10.1051/0004-6361/202141526. ISSN 0004-6361. 
  31. ^ http://www.eso.org/~mwittkow/publications/conferences/SPIECWo5491199.pdf
  32. ^ [1]
  33. ^ Nugent, Richard. "The Garnet Star". weblore.com. Diarsipkan dari versi asli tanggal 2012-05-19. Diakses tanggal 2009-12-04. DIAM .. m Cep 1224 ... V509 CAS 910 ... V382 CAR 747 
  34. ^ Lamers, H. J. G. L. M. (February 6–10, 1995). "Observations and Interpretation of Luminous Blue Variables". Cape Town, South Africa: Astronomical Society of the Pacific: 176–191. Bibcode:1995ASPC...83..176L. Diakses tanggal 2009-03-25. 
  35. ^ Ohnaka, Keiichi; Weigelt, Gerd; Hofmann, Karl-Heinz (2019-09-01). "Infrared Interferometric Three-dimensional Diagnosis of the Atmospheric Dynamics of the AGB Star R Dor with VLTI/AMBER". The Astrophysical Journal. 883: 89. doi:10.3847/1538-4357/ab3d2a. ISSN 0004-637X. 
  36. ^ Moravveji, Ehsan; Guinan, Edward F.; Khosroshahi, Habib G.; Wasatonic, Rick (2013-11-01). "The Age and The Mass of The \alpha Herculis Triple-Star System From A MESA Grid of rotating stars with 1.3". The Astronomical Journal. 146 (6): 148. doi:10.1088/0004-6256/146/6/148. ISSN 0004-6256. 
  37. ^ Gull, Theodore R.; Damineli, Augusto (2009-11). "Eta Carinae in the Context of the Most Massive Stars". Proceedings of the International Astronomical Union. 5 (H15): 373–398. doi:10.1017/S1743921310009890. ISSN 1743-9213. 
  38. ^ Hillier, D. John; Davidson, K.; Ishibashi, K.; Gull, T. (2001-06-01). "On the Nature of the Central Source in η Carinae". The Astrophysical Journal. 553: 837–860. doi:10.1086/320948. ISSN 0004-637X. 
  39. ^ Davis J, Booth AJ, Ireland MJ, Jacob AP, North JR, Owens SM, Robertson JG, Tango WJ, Tuthill PG, J.; Booth, A. J.; Ireland, M. J.; Jacob, A. P.; North, J. R.; Owens, S. M.; Robertson, J. G.; Tango, W. J.; Tuthill, P. G. (2007). "The Emergent Flux and Effective Temperature of Delta Canis Majoris". Publications of the Astronomical Society of Australia. 24: 151. doi:10.1071/AS07017. Diakses tanggal 28 May 2010. 
  40. ^ Stock, S.; Reffert, S.; Quirrenbach, A. (2018-05-01). "VizieR Online Data Catalog: Stellar parameters of 372 giant stars (Stock+, 2018)". VizieR Online Data Catalog: J/A+A/616/A33. doi:10.26093/cds/vizier.36160033. 
  41. ^ Schiller, Florian; Przybilla, Norbert (2008-03). "Quantitative spectroscopy of Deneb". Astronomy & Astrophysics. 479 (3): 849–858. doi:10.1051/0004-6361:20078590. ISSN 0004-6361. 
  42. ^ "Salinan arsip". Diarsipkan dari versi asli tanggal 2012-03-21. Diakses tanggal 2010-10-07. 
  43. ^ Kloppenborg, Brian; Stencel, Robert; Monnier, John D.; Schaefer, Gail; Baron, Fabien; Tycner, Chris; Zavala, Robert T.; Hutter, Donald; Zhao, Ming (2015-09-21). "Interferometry of $\epsilon$ Aurigae: Characterization of the asymmetric eclipsing disk". The Astrophysical Journal Supplement Series. 220 (1): 14. doi:10.1088/0067-0049/220/1/14. ISSN 1538-4365. 
  44. ^ Gamma Crucis by Jim Kaler]
  45. ^ Moravveji, Ehsan; Guinan, Edward F.; Shultz, Matt; Williamson, Michael H.; Moya, Andres (2012-03-10). "Asteroseismology of the Nearby SN-II Progenitor: Rigel Part I. The MOST High Precision Photometry and Radial Velocity Monitoring". The Astrophysical Journal. 747 (2): 108. doi:10.1088/0004-637X/747/2/108. ISSN 0004-637X. 
  46. ^ de Souza, A. Domiciano; Zorec, J.; Millour, F.; Bouquin, J.-B. Le; Spang, A.; Vakili, F. (2021-10). "Refined fundamental parameters of Canopus from combined near-IR interferometry and spectral energy distribution". Astronomy & Astrophysics. 654: A19. doi:10.1051/0004-6361/202140478. ISSN 0004-6361. 
  47. ^ Nordgren, Tyler E.; Germain, M. E.; Benson, J. A.; Mozurkewich, D.; Sudol, J. J.; Elias, N. M., II; Hajian, Arsen R.; White, N. M.; Hutter, D. J. (1999-12-01). "Stellar Angular Diameters of Late-Type Giants and Supergiants Measured with the Navy Prototype Optical Interferometer". The Astronomical Journal. 118: 3032–3038. doi:10.1086/301114. ISSN 0004-6256. 
  48. ^ Drimmel, Ronald; Sozzetti, Alessandro; Schroeder, Klaus-Peter; Bastian, Ulrich; Pinamonti, Matteo; Jack, Dennis; Huerta, Missael A. Hernandez (2021-01-28). "A celestial matryoshka: Dynamical and spectroscopic analysis of the Albireo system". Monthly Notices of the Royal Astronomical Society. 502 (1): 328–350. doi:10.1093/mnras/staa4038. ISSN 0035-8711. 
  49. ^ Groenewegen, M. A. T. (2007-11-01). "The projection factor, period-radius relation, and surface-brightness colour relation in classical cepheids". Astronomy and Astrophysics. 474: 975–981. doi:10.1051/0004-6361:20078225. ISSN 0004-6361. 
  50. ^ da Silva, L.; Girardi, L.; Pasquini, L.; Setiawan, J.; von der Luhe, O.; de Medeiros, J. R.; Hatzes, A.; Dollinger, M. P.; Weiss, A. (2006-11). "Basic physical parameters of a selected sample of evolved stars". Astronomy & Astrophysics. 458 (2): 609–623. doi:10.1051/0004-6361:20065105. ISSN 0004-6361. 
  51. ^ http://adsabs.harvard.edu/abs/2005astro.ph..2181R
  52. ^ Fadeyev, Yu A. (2015-05-01). "Evolutionary status of Polaris". Monthly Notices of the Royal Astronomical Society. 449 (1): 1011–1017. doi:10.1093/mnras/stv412. ISSN 1365-2966. 
  53. ^ Ramirez, I.; Prieto, C. Allende (2011-12-20). "Fundamental Parameters and Chemical Composition of Arcturus". The Astrophysical Journal. 743 (2): 135. doi:10.1088/0004-637X/743/2/135. ISSN 0004-637X. 
  54. ^ Shenar, T.; Oskinova, L.; Hamann, W. -R.; Corcoran, M. F.; Moffat, A. F. J.; Pablo, H.; Richardson, N. D.; Waldron, W. L.; Huenemoerder, D. P. (2015-08-01). "A Coordinated X-Ray and Optical Campaign of the Nearest Massive Eclipsing Binary, δ Orionis Aa. IV. A Multiwavelength, Non-LTE Spectroscopic Analysis". The Astrophysical Journal. 809: 135. doi:10.1088/0004-637X/809/2/135. ISSN 0004-637X. 
  55. ^ Schilbach, E.; Röser, S. (2008-10-01). "On the origin of field O-type stars". Astronomy and Astrophysics. 489: 105–114. doi:10.1051/0004-6361:200809936. ISSN 0004-6361. 
  56. ^ Baines, Ellyn K.; Armstrong, J. Thomas; Schmitt, Henrique R.; Zavala, R. T.; Benson, James A.; Hutter, Donald J.; Tycner, Christopher; van Belle, Gerard T. (2017-12-20). "Fundamental Parameters of 87 Stars from the Navy Precision Optical Interferometer". The Astronomical Journal. 155 (1): 30. doi:10.3847/1538-3881/aa9d8b. ISSN 1538-3881. 
  57. ^ Liebert, James; Young, Patrick A.; Arnett, David; Holberg, J. B.; Williams, Kurtis A. (2005-09-01). "The Age and Progenitor Mass of Sirius B". The Astrophysical Journal. 630 (1): L69–L72. doi:10.1086/462419. ISSN 0004-637X. 

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