Daftar bintang terbesar: Perbedaan antara revisi
Konten dihapus Konten ditambahkan
k Membatalkan 1 suntingan oleh 210.55.76.21 (bicara) ke revisi terakhir oleh EmausBot. (Twinkle 🗳️) |
VY Canis Majoris bukan bintang terbesar. Ada bintang lain yang lebih besar daripada itu. |
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Baris 7:
! style="background-color:#FFDEAD;" colspan="2" | [[Jari-jari Matahari|Radii Matahari]]<br />([[Matahari]] = 1)
|-
|[[UY Scuti]]
| [[VY Canis Majoris]] || 1.800–2.100<ref name="Choi">▼
|1.516--1.900
|-▼
| [[V838 Monocerotis]] || 1.570 atau 800<ref>[[V838 Monocerotis]]</ref>▼
|-
| [[WOH G64]] || 1.
|title=WOH G64: The Largest Star Known?
|publisher=Astronomical Journal
Baris 24 ⟶ 21:
|accessdate=2010-07 16
}}</ref>
|-
| [[V354 Cephei]] || 1.520{{Citation needed|date=December 2009}}▼
| [[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">▼
|
|-
| [[KW Sagittarii]] || 1.460{{Citation needed|date=December 2009}}▼
|
|-
|
|-
|-
▲| [[VV Cephei|VV Cephei A]] || 1.
|title=VV CEP (VV Cephei)
|publisher=University of Illinois
Baris 34 ⟶ 42:
}}</ref>
|-
| [[Mu Cephei]] || 1.
|title=The Effective Temperature Scale of Galactic Red Supergiants: Cool, but Not as Cool As We Thought
|publisher=Astrophysical Journal
Baris 42 ⟶ 49:
|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}}
▲|-
▲| [[KY Cygni]] || 1.420 atau 1.440{{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/]</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>
|-
| [[Antares]] ''(Alpha Scorpii)'' ||
|-
| [[V382 Carinae]] || 747
| |||