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List of the largest known stars: galactic pending additions
[a]
Star name
Solar radii (
Sun = 1)
Method
[b]
Notes
Radii that were stated in the paper
U Arietis
801± 205
[1]
AD
RT Ophiuchi
801± 217
[1]
AD
UU Pegasi
742± 193
[1]
AD
V Camelopardalis
716± 185
[1]
AD
RR Aquilae
648± 169
[1]
AD
RR Persei
599± 161
[1]
AD
R Cassiopeiae
593± 181
[1]
AD
S Serpentis
583± 172 – 601± 159
[1]
AD
RS Virginis
577± 155
[1]
AD
RU Herculis
572± 147
[1]
AD
R Leonis Minoris
569± 146
[1]
AD
S Orionis
545± 142
[1]
AD
R Draconis
511± 142
[1]
AD
DG Cygni
499± 140
[1]
AD
V Cassiopeiae
472± 129
[1]
AD
Mira (ο Ceti)
468± 120 – 482± 124
[1]
AD
S Coronae Borealis
457± 116
[1]
AD
S Pegasi
459± 135 – 574± 154
[1]
AD
R Pegasi
455± 119 – 476± 122
[1]
AD
U Herculis
431± 114 – 453± 117
[1]
AD
T Cassiopeiae
416± 108
[1]
AD
Y Cassiopeiae
413± 110
[1]
AD
R Aquarii
412± 106 – 438± 114
[1]
AD
R Leonis
409± 105
[1]
AD
R Aurigae
407± 105
[1]
AD
U Orionis
370± 96
[1]
AD
BG Serpentis
354± 99
[1]
AD
S Herculis
354± 124
[1]
AD
R Serpentis
328± 86
[1]
AD
U Persei
325± 94 – 352± 101
[1]
AD
Z Pegasi
310± 92
[1]
AD
RT Aquilae
305± 79
[1]
AD
X Ophiuchi
298± 78 – 314± 81
[1]
AD
S Ursae Minoris
296± 82
[1]
AD
R Canum Venaticorum
279± 75 – 322± 82
[1]
AD
R Aquilae
259± 67 – 328± 85
[1]
AD
BG Cygni
236± 76
[1]
AD
Radii that were calculated manually
Stephenson 2-18
2,150
[2]
L/Teff
MY Cephei
2,061
[3]
L/Teff
NML Cygni (V1489 Cygni)
1,639(–2,770)
[4]
L/Teff
RSGC1-F01
1,530
[3]
L/Teff
RSGC1 -F04
1,422
[3]
L/Teff
RSGC1 -F06
1,382
[3]
L/Teff
Stephenson 2 -3
1,301
[3]
L/Teff
Stephenson 2 -11
1,300
[3]
L/Teff
RSGC1 -F10
1,246
[3]
L/Teff
RSGC1 -F05
1,185
[3]
L/Teff
EV Carinae
1,165
[5]
L/Teff
RSGC1 -F08
1,150
[3]
L/Teff
RSGC1-F02
1,128
[3]
L/Teff
S Persei
1,109
[2]
L/Teff
W Persei
1,011
[2]
L/Teff
RSGC1 -F11
1,032
[3]
L/Teff
RSGC1 -F13
1,017
[3]
L/Teff
RSGC1 -F07
1,006
[3]
L/Teff
RSGC1 -F09
996
[3]
L/Teff
RSGC1 -F12
955
[3]
L/Teff
RSGC1 -F03
942
[3]
L/Teff
Stephenson 2 -14
911
[3]
L/Teff
SU Persei
863
[2]
L/Teff
Stephenson 2 -4
855
[3]
L/Teff
AD Persei
812
[2]
L/Teff
V441 Persei
799
[2]
L/Teff
BU Persei
795
[2]
L/Teff
V648 Cassiopeiae
778
[2]
L/Teff
YZ Persei
758
[2]
L/Teff
GP Cassiopeiae
751
[2]
L/Teff
RSGC3 -3
735
[3]
L/Teff
Stephenson 2 -5
730
[3]
L/Teff
RSGC3 -15
728
[3]
L/Teff
KK Persei
724
[2]
L/Teff
XX Persei
710
[2]
L/Teff
Mercer 8 -6
708
[2]
L/Teff
RSGC3 -16
682
[3]
L/Teff
RSGC1 -F14
662
[3]
L/Teff
Stephenson 2 DFK 23
661
[3]
L/Teff
The star has a peculiar SED and is potentially not a member.
RSGC3 -13
655
[3]
L/Teff
Stephenson 2 -1
635
[3]
L/Teff
Mercer 8 -1
620
[2]
L/Teff
PR Persei
603
[2]
L/Teff
Stephenson 2 DFK 6
592
[3]
L/Teff
Stephenson 2 -8
576
[2]
L/Teff
RSGC3 -4
575
[3]
L/Teff
Stephenson 2 -2
569
[3]
L/Teff
V778 Cassiopeiae
549
[2]
L/Teff
Stephenson 2 DFK 18
531
[3]
L/Teff
NGC 7419 BNSW e
528
[3]
L/Teff
Mercer 8 -5
522
[2]
L/Teff
FZ Persei
501
[2]
L/Teff
RSGC3 -5
500
[3]
L/Teff
Stephenson 2 DFK 13
499
[3]
L/Teff
Mercer 8 -2
498
[2]
L/Teff
Stephenson 2 -26
496
[2]
L/Teff
RSGC3 -1
494
[3]
L/Teff
V605 Cassiopeiae
490
[2]
L/Teff
V439 Persei
479
[2]
L/Teff
RSGC3 -14
474
[3]
L/Teff
Mercer 8 -4
458
[2]
L/Teff
NGC 7419 BNSW c
455
[3]
L/Teff
Stephenson 2 DFK 17
451
[3]
L/Teff
HD 236947
431
[2]
L/Teff
Stephenson 2 DFK 14
422
[3]
L/Teff
RSGC1 -F15
410
[3]
L/Teff
RSGC3 -2
393
[3]
L/Teff
RSGC3 -7
393
[3]
L/Teff
NGC 7419 BNSW d
390
[3]
L/Teff
V403 Persei
389
[2]
L/Teff
RSGC3 -9
386
[3]
L/Teff
BD+59 372
380
[2]
L/Teff
V550 Persei
371
[2]
L/Teff
Stephenson 2 DFK 52
357
[3]
L/Teff
The star has a peculiar SED.
PP Persei
352
[2]
L/Teff
Mercer 8 -3
351
[2]
L/Teff
RSGC3 -6
342
[3]
L/Teff
RSGC3 -11
342
[3]
L/Teff
RSGC3 -8
310
[3]
L/Teff
Stephenson 2 DFK 15
288
[3]
L/Teff
NGC 7419 BNSW a
273
[3]
L/Teff
RSGC3 -12
271
[3]
L/Teff
RSGC3 -10
231
[3]
L/Teff
^
a
b So far these values are very far from final and they will definetly change some time in the future.
^ Methods for calculating the radius:
^ Methods for calculating the radius:
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ak van Belle, G. T.; Thompson, R. R.; Creech-Eakman, M. J. (September 2002). "Angular Size Measurements of Mira Variable Stars at 2.2 Microns. II". The Astronomical Journal . 124 : 1706–1715.
arXiv :
astro-ph/0210167 .
Bibcode :
2002AJ....124.1706V .
doi :
10.1086/342282 .
ISSN
0004-6256 .
^
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ad Fok, Thomas K. T.; Nakashima, Jun-ichi; Yung, Bosco H. K.; Hsia, Chih-Hao; Deguchi, Shuji (November 2012). "Maser Observations of Westerlund 1 and Comprehensive Considerations on Maser Properties of Red Supergiants Associated with Massive Clusters". The Astrophysical Journal . 760 : 65.
arXiv :
1209.6427 .
Bibcode :
2012ApJ...760...65F .
doi :
10.1088/0004-637X/760/1/65 .
ISSN
0004-637X .
^
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ay Humphreys, Roberta M.; Helmel, Greta; Jones, Terry J.; Gordon, Michael S. (September 2020). "Exploring the Mass-loss Histories of the Red Supergiants". The Astronomical Journal . 160 : 145.
arXiv :
2008.01108 .
Bibcode :
2020AJ....160..145H .
doi :
10.3847/1538-3881/abab15 .
ISSN
0004-6256 . {{
cite journal }}
: CS1 maint: unflagged free DOI (
link )
^ Zhang, B.; Reid, M. J.; Menten, K. M.; Zheng, X. W.; Brunthaler, A. (August 2012). "The distance and size of the red hypergiant NML Cygni from VLBA and VLA astrometry". Astronomy and Astrophysics . 544 : A42.
arXiv :
1207.1850 .
Bibcode :
2012A&A...544A..42Z .
doi :
10.1051/0004-6361/201219587 .
ISSN
0004-6361 .
^ van Loon, J. Th.; Cioni, M. -R. L.; Zijlstra, A. A.; Loup, C. (July 2005). "An empirical formula for the mass-loss rates of dust-enshrouded red supergiants and oxygen-rich Asymptotic Giant Branch stars". Astronomy and Astrophysics . 438 : 273–289.
arXiv :
astro-ph/0504379 .
Bibcode :
2005A&A...438..273V .
doi :
10.1051/0004-6361:20042555 .
ISSN
0004-6361 .
^ Matsuura, Mikako; Sargent, B.; Swinyard, Bruce; Yates, Jeremy; Royer, P.; Barlow, M. J.; Boyer, Martha; Decin, L.; Khouri, Theo; Meixner, Margaret; van Loon, Jacco Th. (November 2016). "The mass-loss rates of red supergiants at low metallicity: detection of rotational CO emission from two red supergiants in the Large Magellanic Cloud". Monthly Notices of the Royal Astronomical Society . 462 : 2995–3005.
arXiv :
1608.01729 .
Bibcode :
2016MNRAS.462.2995M .
doi :
10.1093/mnras/stw1853 .
ISSN
0035-8711 .
^ Levesque, Emily M.; Massey, Philip; Plez, Bertrand; Olsen, Knut A. G. (June 2009). "The Physical Properties of the Red Supergiant WOH G64: The Largest Star Known?". The Astronomical Journal . 137 : 4744–4752.
arXiv :
0903.2260 .
Bibcode :
2009AJ....137.4744L .
doi :
10.1088/0004-6256/137/6/4744 .
ISSN
0004-6256 .