Lompat ke isi

Daftar bintang terbesar: Perbedaan antara revisi

Dari Wikipedia bahasa Indonesia, ensiklopedia bebas
Konten dihapus Konten ditambahkan
NFarras (bicara | kontrib)
Tidak ada ringkasan suntingan
Tidak ada ringkasan suntingan
Tag: Suntingan perangkat seluler Suntingan peramban seluler
Baris 11: Baris 11:
|2.150<ref name="thomas"/>
|2.150<ref name="thomas"/>
|Bintang terbesar di jagat raya (sebelumnya UY Scuti)
|Bintang terbesar di jagat raya (sebelumnya UY Scuti)
|-Super raksasa merah
|-Red supergiant
|-
|-
|LGGS J004520.67+414717.3
| [[WY Velorum]] || 2.028<ref>{{Cite journal|last=Cruzalèbes|first=P|last2=Petrov|first2=R G|last3=Robbe-Dubois|first3=S|last4=Varga|first4=J|last5=Burtscher|first5=L|last6=Allouche|first6=F|last7=Berio|first7=P|last8=Hofmann|first8=K-H|last9=Hron|first9=J|date=2019-12-11|title=A catalogue of stellar diameters and fluxes for mid-infrared interferometry★|url=https://academic.oup.com/mnras/article/490/3/3158/5583026|journal=Monthly Notices of the Royal Astronomical Society|language=en|volume=490|issue=3|pages=3158–3176|doi=10.1093/mnras/stz2803|issn=0035-8711}}</ref>
|2.126
|Bintang yang terletak di [[Galaksi Andromeda]]
|-
|[[WY Velorum]] || 2.028<ref>{{Cite journal|last=Cruzalèbes|first=P|last2=Petrov|first2=R G|last3=Robbe-Dubois|first3=S|last4=Varga|first4=J|last5=Burtscher|first5=L|last6=Allouche|first6=F|last7=Berio|first7=P|last8=Hofmann|first8=K-H|last9=Hron|first9=J|date=2019-12-11|title=A catalogue of stellar diameters and fluxes for mid-infrared interferometry★|url=https://academic.oup.com/mnras/article/490/3/3158/5583026|journal=Monthly Notices of the Royal Astronomical Society|language=en|volume=490|issue=3|pages=3158–3176|doi=10.1093/mnras/stz2803|issn=0035-8711}}</ref>
|
|
|-
|-

Revisi per 17 Agustus 2020 05.21

Berikut adalah daftar bintang terbesar:

Nama Ukuran dalam satuan Radii Matahari

(Matahari = 1)

Keterangan
Stephenson 2-18 2.150[1] Bintang terbesar di jagat raya (sebelumnya UY Scuti)
LGGS J004520.67+414717.3 2.126 Bintang yang terletak di Galaksi Andromeda
WY Velorum 2.028[2]
V838 Monocerotis 1.570 atau 800[3]
WOH G64 1.540[4]
V354 Cephei 1.520[butuh rujukan]
KW Sagittarii 1.460[butuh rujukan]
KY Cygni 1.420[butuh rujukan]
VY Canis Majoris 1.420
VV Cephei A 1.050[5]–1.900[6]
Mu Cephei 1.400[7]
RW Cephei 1.260–1.610[butuh rujukan]
Betelgeuse (Alpha Orionis) 950–1.000[8] atau 880–988[9]
Antares (Alpha Scorpii) 883[10]
UY Scuti 755
V382 Carinae 747
S Pegasi 580[11]
T Cephei 540[12]
S Orionis 530[13]
W Hydrae 520[14]
R Cassiopeiae 500[15]
Chi Cygni 470[16]
Alpha Herculis (Ras Algethi) 460
Rho Cassiopeiae 450
Mira A (Omicron Ceti) 400[17]
V509 Cassiopeiae 400[18]–900[19]
S Doradus 100–380[20]
R Doradus 370
HR Carinae 350
R Leonis 350[21]
The Pistol Star 340
Alpha Draconis (Thuban) 265
119 Tauri ("Ruby Star")[22] 255[23]
La Superba (Y Canum Venaticorum) 225
Deneb (Alpha Cygni) 220
Delta Canis Majoris (Wezen) 215±66[24]
Zeta Aurigae 200[25]
Eta Carinae 85–195[26]
Epsilon Aurigae A 175
Epsilon Carinae 153
LBV 1806-20 150
Epsilon Pegasi (Enif) 150
Gamma Crucis (Gacrux) 113[27]
Gamma Andromedae 83
Rigel (Beta Orionis) 78
Alpha Leporis (Arneb) 77
R Coronae Borealis 65
Canopus (Alpha Carinae) 65
Delta Orionis (Mintaka) 60
Alpha Persei (Mirfak) 60
Zeta Geminorum (Mekbuda) 60
Eta Aquilae 60
Gamma Draconis (Eltanin) 50
Aldebaran (Alpha Tauri) 43[28]
Beta Ursae Minoris (Kochab) 41
Beta Draconis (Rastaban) 40
Zeta Orionis (Alnitak) 20
Zeta Puppis (Naos) 18.6
Beta Cygni A1 (Albireo) 16

Referensi

  1. ^ Kesalahan pengutipan: Tag <ref> tidak sah; tidak ditemukan teks untuk ref bernama thomas
  2. ^ Cruzalèbes, P; Petrov, R G; Robbe-Dubois, S; Varga, J; Burtscher, L; Allouche, F; Berio, P; Hofmann, K-H; Hron, J (2019-12-11). "A catalogue of stellar diameters and fluxes for mid-infrared interferometry★". Monthly Notices of the Royal Astronomical Society (dalam bahasa Inggris). 490 (3): 3158–3176. doi:10.1093/mnras/stz2803. ISSN 0035-8711. 
  3. ^ V838 Monocerotis
  4. ^ E. M. Levesque. "WOH G64: The Largest Star Known?". Astronomical Journal. Diakses tanggal 2010-07 16. 
  5. ^ Habets, G. M. H. J.; Heintze, J. R. W. (1981). "Empirical bolometric corrections for the main-sequence". Astronomy and Astrophysics Supplement. 46: 193–237. Diakses tanggal 2010-03-14.  Page 225 "Table IV" #178
  6. ^ Professor James B. (Jim) Kaler. "VV CEP (VV Cephei)". University of Illinois. Diakses tanggal 2010-03-15. 
  7. ^ E. M. Levesque. "The Effective Temperature Scale of Galactic Red Supergiants: Cool, but Not as Cool As We Thought". Astrophysical Journal. Diakses tanggal 2010-07 16. 
  8. ^ 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 [1]
  9. ^ Jim Kaler. 2009-06-26. 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"
  10. ^ 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 (SIMBAD citing 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.
  11. ^ http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=10781
  12. ^ http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=9837
  13. ^ http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=2512
  14. ^ http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=6127
  15. ^ http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=10947
  16. ^ http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=9107
  17. ^ http://www.eso.org/~mwittkow/publications/conferences/SPIECWo5491199.pdf
  18. ^ [2]
  19. ^ Nugent, Richard. "The Garnet Star". weblore.com. Diakses tanggal 2009-12-04. DIAM .. m Cep 1224 ... V509 CAS 910 ... V382 CAR 747 
  20. ^ 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. 
  21. ^ http://arxiv.org/abs/astro-ph/0411133
  22. ^ "Big and Giant Stars"
  23. ^ http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=2526
  24. ^ 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. 
  25. ^ [3]
  26. ^ http://etacar.umn.edu/etainfo/basic/
  27. ^ Gamma Crucis by Jim Kaler]
  28. ^ http://adsabs.harvard.edu/abs/2005astro.ph..2181R

Pranala luar