List of largest known stars facts for kids
The largest stars known are truly enormous, much bigger than our own Sun! Imagine stars so big that if our Sun were a tiny pebble, these giants would be like huge boulders or even mountains. Scientists measure their size by comparing them to the Sun's radius. One solar radius is about 695,700 kilometers (432,280 miles).

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What Makes a Star Big?
Stars get their huge size from different things. The biggest stars are often called red supergiants. These are old stars that have used up most of their fuel. When this happens, they swell up to incredible sizes, becoming much cooler and redder.
Sometimes, stars can suddenly grow even bigger for a short time! This happens during events like "luminous red novae" or "LBV eruptions." During these events, a star can expand super fast, reaching thousands of times the Sun's radius in just a few months. That's even bigger than the largest red supergiants!
Scientists also think that some of the very first stars in the universe, called "Population III" stars, might have been super-duper massive. These early stars might have grown into "red supergiant protostars" that were tens of thousands of times bigger than our Sun! They would have been as big as some of the largest black holes we know today.
How Do We Measure Stars?
It's tricky to measure the exact size of a star, especially when they are so far away! One way is to measure their "angular diameter." This is how big a star looks from Earth. It's like holding a coin far away – it looks small, but it's still the same size. Scientists use special telescopes that combine light from different places, called stellar interferometers, to get a clearer view.
Another way to measure stars is when they pass in front of the Moon (called a lunar occultation) or when they are part of a binary star system where one star passes in front of another.
However, even with these methods, it's hard to be perfectly accurate. Stars have thin outer layers, and their edges can look different depending on the type of light we use to observe them. Also, many giant stars change their size over time, like a beating heart, which makes it even harder to get one exact measurement. So, the sizes you see in these lists are often averages or within a range of possible values.
Things to Remember About Star Sizes
Measuring the exact size of the biggest stars is really tough, and there can be some errors. Here are a few reasons why:
- Most star sizes are estimated using math formulas that connect a star's brightness and its surface temperature.
- Knowing the exact distance to a star is hard, and any mistake in distance affects the size calculation.
- Many supergiant stars have huge, cloudy atmospheres or are hidden by dust, which makes it hard to see their true surface.
- These giant stars often change their size over months or years, like variable stars. This means their brightness changes too, making it tricky to pin down their exact size.
- It's much easier to measure stars that are part of star clusters or binary systems because their distances are better known.
- Stars in other galaxies might behave a bit differently than those in our Milky Way. For example, some red supergiants in the Magellanic Clouds might have slightly different temperatures or brightness limits.
All the sizes in these lists have some uncertainty, and scientists are always working to get more accurate numbers!
Lists of the Largest Stars
Here are some of the biggest stars we know, grouped by the galaxy they are in. The sizes are given in "solar radii," meaning how many times bigger they are than our Sun.
Milky Way Galaxy
This list shows some of the largest known stars in our home galaxy, the Milky Way.
Star name | Solar radii (Sun = 1) |
Method | Notes | ||||
---|---|---|---|---|---|---|---|
Orbit of Saturn | 2,047–2,049.9 | Listed for comparison, this is how big Saturn's orbit is! | |||||
WOH G64 (For comparison) | 1,540 ± 77 | L/Teff | Found in the Large Magellanic Cloud. It might be the largest star known anywhere. | ||||
Theoretical limit of star size (Milky Way) | ~1,500 | Scientists think stars bigger than this might be too unstable to form. | |||||
RSGC1-F01 | 1,436, 1,450, 1,530+330 −424 |
L/Teff | |||||
VY Canis Majoris | 1,420±120 | AD | An extremely large red hypergiant. It's possibly the biggest star in the Milky Way. | ||||
CM Velorum | 1,416.24+0.40 −0.96 |
L/Teff | |||||
AH Scorpii | 1,411±124 | AD | |||||
Stephenson 2 DFK 2 | 1,301+259 −325 |
L/Teff | |||||
CD-26 5055 | 1,280+20 −123 |
L/Teff | |||||
AS Cephei | 1,263+19 −9 |
L/Teff | |||||
Westerlund 1 W237 (Westerlund 1 BKS B) | 1,241±70 | L/Teff | |||||
S Persei | 1,212 – 1,364±6 | AD | |||||
IRC -10414 | ~1,200 | L/Teff | |||||
V517 Monocerotis | 1,196+80 −159 |
L/Teff | |||||
PZ Cassiopeiae | 1,190±238(–1,940±388), 1,364 | L/Teff | |||||
GCIRS 7 | 1,170±60–1,368, 1,359 | AD & L/Teff | |||||
Westerlund 1 W26 (Westerlund 1 BKS AS) | 1,165±58–1,221±120 | L/Teff | |||||
HD 143183 | 1,147 | L/Teff | |||||
V354 Cephei | 1,139 | L/Teff | |||||
VX Sagitarii | 1,120 – 1,550, 1,200, 1,356, 1,400 | L/Teff | One of the largest stars known. | ||||
Orbit of Jupiter | 1,114.5–1,115.8 | Listed for comparison, this is how big Jupiter's orbit is! | |||||
RW Cygni | 1,103+251 −177 |
AD | |||||
RT Carinae | 1,090±218 | L/Teff | |||||
UU Persei | 1,079+9 −8 |
L/Teff | |||||
LL Pegasi | 1,074 | L/Teff | |||||
V396 Centauri | 1,070±214–1,145.31 | L/Teff & ? | |||||
HD 126577 | 1,066+9 −32 |
L/Teff | |||||
V766 Centauri Aa | 1,060–1,160 | ? | A rare variable yellow hypergiant. | ||||
VV Cephei A | 1,050 | AD | One of the largest stars known. | ||||
BC Cygni | 1,031–1,187+34 −37 |
L/Teff | |||||
KY Cygni | 1,032–(1,420±284–2,850±570) | L/Teff | |||||
V602 Carinae | 1,015 – 1,050±165 | AD | |||||
CK Carinae | 1,013–1,060±212 | L/Teff | |||||
KW Sagittarii | 1,009±142 | AD | |||||
V349 Carinae | 1,002+12 −74 |
L/Teff | |||||
μ Cephei (Herschel's Garnet Star) | 972±228, 1,000 – 1,200, 1,259, 1,420, 1,500 | AD | One of the largest stars known. | ||||
Stephenson 2 DFK 5 | 911 | L/Teff | |||||
RW Cephei | 900–1,760, 940 | AD & L/Teff | |||||
NSV 25875 | 891 | L/Teff | |||||
Trumpler 27 MMU 1 | 875.86+5.5 −11.83 |
L/Teff | |||||
V437 Scuti | 874 | L/Teff | |||||
V669 Cassiopeiae | 859 | L/Teff | |||||
Westerlund 1 W20 (Westerlund 1 BKS D) | 858±48 | L/Teff | |||||
Stephenson 2 DFK 3 | 855 | L/Teff | |||||
BI Cygni | 851–1,240±248 | L/Teff | |||||
V1185 Scorpii | 830 | L/Teff | |||||
6 Geminorum | 821 | L/Teff | |||||
AZ Cygni | 814+175 −124–911+57 −50 |
AD | |||||
U Arietis | 801±205 | AD | |||||
RT Ophiuchi | 801±217 | AD | |||||
BO Carinae | 790±158 | L/Teff | |||||
SU Persei | 780±156–1,139+34 −23 |
L/Teff | |||||
GP Cassiopeiae | 771.74+0.23 −0.86 |
L/Teff | |||||
RS Persei | 770±30 | AD | |||||
V355 Cephei | 770±154 | L/Teff | |||||
GU Cephei A | 767 | ? | |||||
Betelgeuse (α Orionis) | 764+116 −62, 944 ± 157, 1,021, 1,074+232 −165, 1,259, 1,268, 1,285, ~1,300, 1,409+319 −229 |
? | One of the brightest stars in the night sky and one of the largest known. Its size changed during a "great dimming" event in 2020. | ||||
HD 303250 | 750±150 | L/Teff | |||||
UU Pegasi | 742±193 | AD | |||||
Stephenson 2 DFK 10 | 730 | L/Teff | |||||
Westerlund 1 W75 (Westerlund 1 BKS E) | 722±36 | L/Teff | |||||
V Camelopardalis | 716±185 | AD | |||||
V923 Centauri | 716 | ? | |||||
S Canis Minoris | 710 | ||||||
V528 Carinae | 700±140 | L/Teff | The following well-known stars are listed for comparison. | ||||
Antares A (α Scorpii) | 680 | AD | A very bright star and one of the largest known. | ||||
119 Tauri (CE Tauri, Ruby Star) | 587 – 593 | AD | |||||
CW Leonis | 560 | L/Teff | The closest carbon star. | ||||
Unurgunite (σ Canis Majoris) | 420±84 | L/Teff | |||||
V838 Monocerotis | 364 | L/Teff | During a special event in 2002, this star's radius might have grown to 3,190 times the Sun's size! | ||||
La Superba (Y Canum Venaticorum) | 342 | AD | |||||
Mira A (ο Ceti) | 332–402 | AD | |||||
Orbit of Mars | 322–323.1 | Listed for comparison, this is how big Mars's orbit is! | |||||
Pistol Star (V4647 Sagittarii) | 306 | ? | |||||
R Doradus | 298±21 | AD | This star looks the biggest in our sky, even though it's not the largest in real size. | ||||
Rasalgethi A (α Herculis) | 284±60 (264–303) | L/Teff | |||||
Cygnus OB2#12 | 246 | ? | One of the heaviest and brightest stars known. | ||||
η Carinae | 240 | ? | During a huge eruption in 1843, this star's radius might have grown to 4,319–6,032 times the Sun's size. | ||||
Wezen (δ Canis Majoris) | 215±66 | AD | A bright star in the night sky. | ||||
Orbit of Earth (~1 AU) | 214 | Listed for comparison, this is how big Earth's orbit is! | |||||
Deneb (α Cygni) | 203±17 | ? | A bright star in the night sky. |
Magellanic Clouds
The Magellanic Clouds are two small galaxies close to our Milky Way.
Star name | Solar radii (Sun = 1) |
Galaxy | Method | Notes
L/Teff |
|||||
---|---|---|---|---|---|---|---|---|---|
WOH G64 | 1,540 ± 77 | Large Magellanic Cloud | L/Teff | This star is surrounded by a huge cloud of dust. It might be the largest star known. | |||||
IRAS 05280–6910 | 1,367 | Large Magellanic Cloud | L/Teff | The reddest object in the Large Magellanic Cloud. | |||||
IRAS 05346-6949 | 1,211 | Large Magellanic Cloud | L/Teff | This star is losing a lot of its material every year, more than any other star. | |||||
HV 2242 | 1,160 – 1,180 | Large Magellanic Cloud | L/Teff | ||||||
W60 B90 (WOH S264) | 1,149–1,390+130 −110 |
Large Magellanic Cloud | L/Teff | Scientists are still studying its exact size. | |||||
MSX SMC 018 | 1,119 | Small Magellanic Cloud | L/Teff | ||||||
WOH S338 | 1,100 | Large Magellanic Cloud | L/Teff | ||||||
IRAS 04516-6902 | 1,085 – 1,283 | Large Magellanic Cloud | L/Teff | ||||||
MSX LMC 589 | 1,051 | Large Magellanic Cloud | L/Teff | ||||||
IRAS 05402-6956 | 1,032 | Large Magellanic Cloud | L/Teff | ||||||
IRAS 04509-6922 | (1,027-2,249)–1,187 | Large Magellanic Cloud | L/Teff | ||||||
UCAC2 2674864 (HV 2834) | 990+115 −100 |
Large Magellanic Cloud | L/Teff | ||||||
HV 2362 | 982 – 1,030 | Large Magellanic Cloud | L/Teff | ||||||
MG73 59 | 979 | Large Magellanic Cloud | L/Teff | A yellow supergiant. | |||||
HD 268757 | 979 | Large Magellanic Cloud | L/Teff | A G8 yellow hypergiant. | |||||
WOH S457 | 902±45 | Large Magellanic Cloud | L/Teff | ||||||
IRAS 04498-6842 (LI-LMC 60) | (898-1,660) – 1,137 – 1,765, 1,224 | Large Magellanic Cloud | L/Teff | ||||||
HV 12185 | 890+55 −65 |
Large Magellanic Cloud | L/Teff | ||||||
HV 12793 | 880+45 −65 |
Large Magellanic Cloud | L/Teff | ||||||
WOH S57 | 875+70 −60 |
Large Magellanic Cloud | L/Teff | ||||||
SP77 28-2 | 825±60 | Large Magellanic Cloud | L/Teff | ||||||
SP77 22-9 | 823 – 850 | Large Magellanic Cloud | L/Teff | ||||||
Z Doradus | 824±108–956 | Large Magellanic Cloud | L/Teff | ||||||
HD 269723 | 814–829 | Large Magellanic Cloud | L/Teff | A yellow hypergiant. | |||||
PMMR 116 | 717 | Small Magellanic Cloud | L/Teff | ||||||
MSX SMC 055 | 702–1,557+215 −130 |
Small Magellanic Cloud | L/Teff | The following well-known stars are listed for comparison. | |||||
HV 2112 | 675 – 1,193 | Small Magellanic Cloud | L/Teff | Once thought to be a very strange type of star called a Thorne–Żytkow object. | |||||
HV 11417 | 673–798 | Small Magellanic Cloud | L/Teff | Another candidate for a Thorne-Zytkow object. | |||||
HD 269953 | 647–720 | Large Magellanic Cloud | L/Teff | A yellow hypergiant. | |||||
HD 33579 | 471 | Large Magellanic Cloud | L/Teff | The brightest star in the Large Magellanic Cloud. | |||||
S Doradus | 100 | Large Magellanic Cloud | L/Teff | A luminous blue variable star. | |||||
HD 37974 | 99 | Large Magellanic Cloud | L/Teff | An unusual blue hypergiant with a large dusty disk around it. | |||||
R136a1 | 42.7+1.6 −0.9 |
Large Magellanic Cloud | L/Teff | One of the brightest and heaviest stars known. | |||||
BAT 99-98 | 37.5 | Large Magellanic Cloud | L/Teff | Another very bright and heavy star. | |||||
HD 5980 A | 24 | Small Magellanic Cloud | L/Teff | A luminous blue variable and one of the brightest stars. |
Andromeda (M31) and Triangulum (M33) Galaxies
These are two other large galaxies in our Local Group of galaxies.
Star name | Solar radii (Sun = 1) |
Galaxy | Method | Notes | |||||
---|---|---|---|---|---|---|---|---|---|
WOH G64 (For comparison) | 1540 ± 77 | Large Magellanic Cloud | L/Teff | Located in the Large Magellanic Cloud. Possibly the largest known star. | |||||
LGGS J013418.56+303808.6 | 1,363 | Triangulum Galaxy | L/Teff | ||||||
LGGS J004124.80+411634.7 | 1,240 | Andromeda Galaxy | L/Teff | ||||||
LGGS J013349.86+303246.1 | 710–795 | Triangulum Galaxy | L/Teff | A yellow supergiant. | |||||
LGGS J004255.95+404857.5 | 785 | Andromeda Galaxy | L/Teff | The following well-known stars are listed for comparison. | |||||
Var 83 | 150 | Triangulum Galaxy | L/Teff | A luminous blue variable and one of the brightest stars in M33. |
Other Galaxies (within the Local Group)
These are other galaxies that are part of our Local Group, a cluster of galaxies that includes the Milky Way.
Star name | Solar radii (Sun = 1) |
Galaxy | Method | Notes |
---|---|---|---|---|
WOH G64 (For comparison) | 1540 ± 77 | Large Magellanic Cloud | L/Teff | Located in the Large Magellanic Cloud. Possibly the largest known star. |
Sextans A 10 | 995±130 | Sextans A | L/Teff | |
WLM 02 | 883+284 −167 |
WLM | L/Teff | |
Sextans A 5 | 870±145 | Sextans A | L/Teff | |
Sextans A 7 | 710±100 | Sextans A | L/Teff |
Outside the Local Group
These stars are in galaxies much farther away from us.
Star name | Solar radii (Sun = 1) |
Galaxy | Group | Method | Notes |
---|---|---|---|---|---|
WOH G64 (For comparison) | 1540 ± 77 | Large Magellanic Cloud | L/Teff | Located in the Large Magellanic Cloud. Possibly the largest known star. | |
SPIRITS 14atl | 1,134–1,477 | Messier 83 | Centaurus A/M83 Group | L/Teff | |
SPIRITS 15ahp | 1,098 | NGC 2403 | M81 Group | L/Teff | |
Quyllur | 965 | L/Teff | This is likely the first red supergiant star found at very far distances, discovered by the James Webb Space Telescope. | ||
The following well-known stars are listed for comparison. | |||||
Godzilla | 430–2,365 | Sunburst galaxy | L/Teff | The brightest star known. | |
Mothra | 271 | L/Teff | A binary star system very far away. | ||
NGC 2363-V1 | 194–356 | NGC 2366 | M81 Group | L/Teff |
Transient Events
Sometimes, stars can temporarily become much larger during special events like red novae (a type of star explosion) or LBV eruptions (when a very bright star suddenly gets even brighter).
Star or transient event name | Solar radii (Sun = 1) |
Year | Galaxy | Group | Method | Notes |
---|---|---|---|---|---|---|
AT 2017jfs | 33,000 | 2017 | NGC 4470 | L/Teff | ||
SNhunt151 | 16,700 | 2014 | UGC 3165 | LDC 331 | L/Teff | |
SN 2015bh | 16,400±2,600 | 2015 | NGC 2770 | LDC 616 | L/Teff | |
AT 2018hso | 10,350 | 2018 | NGC 3729 | M109 Group | L/Teff | |
M51 OT2019-1 | 5,500 | 2019 | Whirlpool Galaxy | M51 Group | L/Teff | |
η Carinae | 4,319 – 6,032 | 1845 | Milky Way | Local Group | L/Teff | During its huge outburst, this star became the second brightest in the sky! |
AT 2010dn | 4,130 | 2010 | NGC 3180 | LDC 743 | L/Teff | |
SN 2011fh | 3,980 | 2011 | NGC 4806 | Abell 3528 | L/Teff | |
AT 2014ej | 3,600 | 2014 | NGC 7552 | Grus Quartet | L/Teff | |
V838 Monocerotis | 3,190 | 2002 | Milky Way | Local Group | L/Teff | |
SN2008S | 3,020 | 2008 | NGC 6946 | NGC 6946 Group | L/Teff | |
SNhunt120 | 2,900 | 2012 | NGC 5775 | Virgo Cluster | L/Teff | |
AT 2017be | 2,000 | 2017 | NGC 2537 | L/Teff | ||
WOH G64 (For comparison) | 1540 ± 77 | Large Magellanic Cloud | L/Teff | Located in the Large Magellanic Cloud. Possibly the largest known star. | ||
PHL 293B star | 1,348 – 1,463 | 2002 | PHL 293B | L/Teff | ||
SNhunt248 | ~850 | 2014 | NGC 5806 | NGC 5846 Group | L/Teff | |
R71 | 500 | 2012 | Large Magellanic Cloud | Local Group | L/Teff | |
SN 2000ch | 500 | 2000 | NGC 3432 | LDC 743 | L/Teff | |
Godzilla | 430 – 2,365 | 2015 | Sunburst galaxy | ? | ||
AT 2016blu | ~330 | 2012 – 2022 | NGC 4559 | Coma I Group | L/Teff | This star had many outbursts over ten years. |
Images for kids
See also
- Constellation
- Lists of stars
- List of most massive stars
- List of most luminous stars
- List of hottest stars
- List of coolest stars
- List of most massive black holes
- List of largest nebulae
- List of largest galaxies
- List of largest cosmic structures
- List of largest exoplanets
- List of star extremes
- Star