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List of smallest known stars
This is a list of the smallest known stars, brown dwarfs and stellar remnants, sorted by increasing size. The list is divided into sublists, and contain notable objects up to 350,000 km in radius, or 0.50 R☉, as well as all red dwarfs smaller than 0.1 R☉ and all neutron stars with accurately measured radii.
Partial list containing stars up to 0.0014 R☉.
| Star name | Star radius, kilometres | Star class | Notes | References |
|---|---|---|---|---|
| SGR J1935+2154 | 4.35+1.95−1.35 | Magnetar | Has one potential planet. | |
| RX J0720.4−3125 | 4.50+0.08−0.09 – 5.38+0.13−0.14 | Neutron star | ||
| Hercules X-1 | 8.10±0.41 | Pulsar | ||
| LMC X-4 | 8.301±0.2 | |||
| Centaurus X-3 | 9.178±0.130 | |||
| Vela X-1 | 9.56±0.0 | |||
| HESS J1731-347 | 10.40+0.86−0.78 | Neutron star | Lightest neutron star ever discovered, at a mass of 0.77 M☉. | |
| PSR J0348+0432 A | 11–15 | Pulsar | Has a white dwarf companion. | |
| PSR J0437−4715 | >11.1 | Most stable known natural clock. | ||
| GW170817 A | 11.9±0.4 | |||
| GW170817 B | 11.9±0.4 | |||
| PSR J1906+0746 | 11.99–12.85 | |||
| PSR J0205+6449 | 12 | Pulsar | Pulsar located in the supernova remnant 3C 58. | |
| RX J1856.5−3754 | 12.1+1.3−1.6 | Neutron star | Nearest known neutron star. | |
| PSR J2043+1711 | 12.13–12.96 | Pulsar | ||
| PSR J1933-6211 | 12.15–12.98 | |||
| PSR J0952–0607 A | 12.245+0.685−0.315 | Most massive neutron star so far discovered. | ||
| 4U 1702−429 | 12.4±0.4 | Neutron star | ||
| Vela pulsar | 12.52–13.30 | Pulsar | ||
| PSR J1614−2230 | 13±2 | |||
| PSR J0348+0432 | 13±2 | |||
| PSR J0740+6620 | 13.7+2.6−1.5 | |||
| ZTF J1406+1422 A | 14 | Neutron star | Has a substellar companion orbiting it closely. | |
| PSR J1748−2446Ad | 16 | Pulsar | Fasted spinning neutron star, it is constrained to a small size to avoid being torn apart, located in the star cluster Terzan 5, and potentially the largest known pulsar. |
Partial list containing stars from 0.0014 to 0.0718 R☉.
Partial list containing stars from 0.0718 to 0.18 R☉.
Partial list containing stars from 0.18 to 0.287 R☉.
Partial list containing stars from 0.29 to 0.395 solar radii.
Partial list containing stars from 0.395 to 0.5 solar radii.
| Star name | Star radius, kilometres | Star radius, R☉ | Star class | Notes | References |
|---|---|---|---|---|---|
| Gliese 570 C | 277,300 | 0.399 ± 0.028 | Red dwarf | ||
| Asellus Primus B (Theta Boötis B) | 279,180 | 0.4013±0.012 | |||
| GJ 3293 | 281,100 | 0.404±0.027 | |||
| Gliese 623 A | 280,900 | 0.404 ± 0.024 | |||
| Alpha Trianguli C | 282,500 | 0.406±0.012 | |||
| Gliese 908 (Lalande 46650) | 284,540 | 0.409±0.023 | |||
| EQ Pegasi A | 284,540 | 0.409±0.016 | Has one confirmed exoplanet. | ||
| Gliese 163 | 284,540 | 0.409+0.017−0.016 | |||
| SDSS J001820.5−093939.2 | 285,930 | 0.411+0.090−0.011 | F-type star | Among the most metal-poor stars. | |
| Gliese 806 | 288,300 | 0.4144±0.0038 | Red dwarf | Has three confirmed exoplanets. | |
| Gliese 317 | 290,110 | 0.4170±0.0013 | Has two confirmed exoplanets. | ||
| Gliese 687 | 291,290 | 0.4187+0.0066−0.0063 | |||
| QS Virginis B | 292,000 | 0.42±0.02 | |||
| TOI-700 | 292,000 | 0.420±0.031 | |||
| Gliese 180 | 294,210 | 0.4229±0.0047 | Has two confirmed exoplanets and one unconfirmed. | ||
| AD Leonis | 294,490 | 0.4233±0.0057 | |||
| Gliese 686 | 297,060 | 0.427±0.013 | |||
| Chi Ceti Bb | 298,460 | 0.429±0.017 | |||
| GJ 3634 | 300,000 | 0.43±0.03 | Has one confirmed exoplanet. | ||
| Iota Ursae Majoris B | 300,000 | 0.43 | |||
| U Geminorum B | 300,000 | 0.43±0.06 | |||
| Gliese 436 | 300,540 | 0.432±0.011 | Has one confirmed exoplanet. | ||
| Gliese 393 | 300,540 | 0.432±0.025 | |||
| Sigma Coronae Borealis C | 304,020 | 0.437±0.020 | |||
| Kappa1 Apodis B | 306,000 | 0.44±0.06 | Subdwarf O star | ||
| WR 93b | 306,000 | 0.44 | Wolf-Rayet | ||
| Gliese 832 | 307,500 | 0.442±0.018 | Red dwarf | ||
| Alpha Caeli B | 313,000 | 0.45 | |||
| Gliese 367 (Anañuca) | 317,930 | 0.457±0.013 | Has three confirmed exoplanets. | ||
| Gliese 588 | 320,000 | 0.46±0.019 | |||
| Iota Ursae Majoris C | 320,000 | 0.46 | |||
| HD 147379 B | 320,000 | 0.460±0.008 | |||
| Gliese 849 | 322,800 | 0.464±0.018 | |||
| BAT99-123 (Brey 93) | 327,000 | 0.47 | Wolf-Rayet | ||
| Gliese 176 | 329,760 | 0.474±0.015 | Red dwarf | ||
| Lacaille 9352 | 329,760 | 0.474±0.008 | |||
| Tau Boötis B | 333,900 | 0.48±0.05 | |||
| Gliese 752 A | 334,630 | 0.481±0.014 | |||
| UScoCTIO 108 A | 336,720 | 0.484 | Brown dwarf | ||
| Gliese 526 | 338,810 | 0.487±0.008 | Red dwarf | ||
| UX Ursae Majoris B | 345,070–484,900 | 0.496–0.697 | |||
| Theta Persei Ab | 346,500 | 0.498±0.017 | |||
| GJ 3470 (Kaewkosin) | 347,150 | 0.499±0.021 | |||
| Kappa Reticuli B | 347,900 | 0.50 | |||
| TOI-2119 | 347,900 | 0.500±0.015 | |||
| Gliese 22 A | ~350,000 | ~0.5 |
| Type | Star name | RadiusSolar radii(Sun = 1) | RadiusJupiter radii(Jupiter = 1) | RadiusEarth radii(Earth = 1) | Radius(km / mi) | Date | Notes | References |
|---|---|---|---|---|---|---|---|---|
| Red dwarf | EBLM J0555−57Ab | 0.084 | 0.84 | 9.41 | 60,000 km (37,000 mi) | 2017 | The red dwarf stars are considered the smallest stars known, and representative of the smallest star possible. | |
| Brown dwarf | ZTF J1406+1422 B | 0.029 | 0.282 | 3.16 | 20,200 kilometres (12,600 mi) | 2022 | Brown dwarfs are not massive enough to build up the pressure in the central regions to allow nuclear fusion of hydrogen into helium. They are best described as extremely massive gas giants that were not able to ignite into a hydrogen-fusing star. | |
| White dwarf | ZTF J1901+1458 | 0.0031 | 0.030 | 0.34 | 2,140 km (1,330 mi) | 2021 | White dwarfs are stellar remnants produced when a star with around 8 solar masses or less sheds its outer layers into a planetary nebula. The leftover core becomes the white dwarf. It is thought that white dwarfs cool down over quadrillions of years to produce a black dwarf. | |
| Neutron star | RX J0720.4−3125 | 0.0000064683 – 0.0000077332 | 0.00006294 – 0.00007525 | 0.0007055 – 0.0008435 | 4.50+0.08−0.09 – 5.38+0.13−0.14 | 2012 | Neutron stars are stellar remnants produced when stars with around 9 solar masses or more explode in supernovae at the ends of their lives. They are usually produced by stars with less than 20 solar masses, although a more massive star may produce a neutron star in certain cases. |
Red dwarfs are considered the smallest stars known that are active fusion stars, and are the smallest stars possible that is not a brown dwarf.
| Star name | Date | RadiusSolar radii(Sun = 1) | RadiusJupiter radii(Jupiter = 1) | Radiuskm(mi) | Notes | |
|---|---|---|---|---|---|---|
| EBLM J0555−57Ab | 2017- | 0.084 | 0.84 | 60,000 km (37,000 mi) | This star has a size comparable to that of Saturn. | |
| 2MASS J0523−1403 | 2013-2017 | 0.102 | 1.01 | 70,600 km (43,900 mi) | Lowest mass main sequence star as of 2020. | |
| OGLE-TR-122B | 2005-2013 | 0.117 | 1.16 | 81,100 km (50,400 mi) |
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