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, as well as all red dwarfs smaller than and all neutron stars with accurately measured radii.
0 to 1,000 km
Partial list containing stars up to 0.0014.| Star name | Star radius, kilometres | Star class | Notes | References |
| SGR J1935+2154 | Magnetar | |||
| RX J0720.4−3125 | – | Neutron star | ||
| LMC X-4 | Pulsar | |||
| Hercules X-1 | Pulsar | |||
| Centaurus X-3 | Pulsar | |||
| Vela X-1 | Pulsar | |||
| HESS J1731-347 | Neutron star | Lightest neutron star ever discovered, at a mass of. | ||
| PSR J0348+0432 A | Pulsar | Has a white dwarf companion. | ||
| PSR J0437−4715 | >11.1 | Pulsar | Most stable known natural clock. | |
| GW170817 A | Pulsar | |||
| GW170817 B | Pulsar | |||
| PSR J1906+0746 | Pulsar | |||
| RX J1856.5−3754 | Neutron star | |||
| PSR J2043+1711 | Pulsar | |||
| PSR J1933-6211 | Pulsar | |||
| PSR J0952–0607 A | Pulsar | Most massive neutron star so far discovered. | ||
| Neutron star | ||||
| Vela pulsar | Pulsar | |||
| PSR J1614−2230 | Pulsar | |||
| PSR J0348+0432 | Pulsar | |||
| PSR J0740+6620 | Pulsar | |||
| 14 | Neutron star | Has a substellar companion orbiting it closely. |
1,000 to 50,000 km
Partial list containing stars from 0.0014 to 0.0718.| Star name | Star radius, kilometres | Star radius, | Star class | Notes | References |
| ZTF J1901+1458 | 2,140 | The most massive white dwarf so far discovered, around 1.3 times more massive than the Sun, close to the mass limit of any white dwarf, and is also a candidate white dwarf pulsar. | |||
| RE J0317-853 | 0.0032 | Also among the most massive white dwarfs. | |||
| WD1 | 2,230 | An ultramassive white dwarf ejected from the Hyades. At a mass of, it is possibly the most massive known white dwarf consistent with single-star evolution. | |||
| T Coronae Borealis | 0.0045 | Expected to become a nova in the near future, its apparent magnitude may increase up to 2.0. | |||
| Janus | A white dwarf with a side of hydrogen and another side of helium. | ||||
| Wolf 1130 B | 0.005 | Nearest candidate for a supernova, a type Ia supernova. | |||
| HD 49798 B | 3,580 | ||||
| BPM 37093 | |||||
| IK Pegasi B | 0.006 | ||||
| U Geminorum A | |||||
| WD 2317+1830 | |||||
| BW Sculptoris | |||||
| Sirius B | Nearest white dwarf | ||||
| GRW +70 8247 ' | |||||
| Gamma Cassiopeiae Ab | |||||
| AN Ursae Majoris | 6,300 | ||||
| Gliese 915 | |||||
| LP 658-2 | |||||
| BZ Ursae Majoris A | 6,880 | ||||
| AE Aquarii A | 0.01 | First discovered white dwarf pulsar. | |||
| AR Scorpii A | 7,000 | A white dwarf pulsar. It is often mistaken as the first discovered white dwarf pulsar. | |||
| QS Virginis A | |||||
| YZ Leonis Minoris | 0.01 | ||||
| GW Librae | |||||
| WZ Sagittae | |||||
| MY Apodis | |||||
| OY Carinae A | 0.011 | ||||
| TMTS J0526+5934 A | 0.011 | ||||
| G 99-47 | 7,650 | ||||
| EX Hydrae | 0.011 | ||||
| RX Andromedae | |||||
| van Maanen 2 | Third-closest white dwarf. | ||||
| Stein 2051 B | |||||
| G 107-70 B | |||||
| Ross 548 ' | |||||
| 39 Ceti B ' | 0.012 | ||||
| Mira B ' | 0.012 | ||||
| WD 1054−226 | |||||
| Gliese 440 | Fourth-closest white dwarf. | ||||
| Procyon B | Second-closest white dwarf. | ||||
| GD 165 A | |||||
| Epsilon2 Arae C | |||||
| WD 0806−661 ' | Has one confirmed exoplanet. | ||||
| SW Ursae Majoris | |||||
| Epsilon Reticuli B | – | 0.0129–0.0141 | |||
| G 29-38 | |||||
| AM Herculis A | |||||
| 40 Eridani B | First white dwarf to be discovered and the fifth-closest one. | ||||
| TY Coronae Borealis | |||||
| HD 147513 B | |||||
| GD 358 ' | 0.0132 | ||||
| Wolf 489 | |||||
| GALEX J2339−0424 | |||||
| G 107-70 A | |||||
| Wolf 1346 | |||||
| WD 1032+011 A | |||||
| Gliese 318 | |||||
| RR Caeli A | 0.01568 | ||||
| HL Tau 76 | 0.0162 | ||||
| PG 1159-035 | or | 0.0232 or | PG 1159 star | PG 1159 stars are pre-white dwarfs. | |
| WD 2226−210 | White dwarf | Located in Helix Nebula | |||
| WD 0032−317 A | White dwarf | ||||
| Feige 55 | White dwarf | ||||
| 0.029 | Brown dwarf | with an orbital period of 62 minutes and a dayside surface temperature of, comparable to A-type stars such as Vega and Sirius. | |||
| KPD 0005+5106 | Pre-white dwarf | Has one unconfirmed exoplanet. | |||
| AG Pegasi B | 0.06 | White dwarf | In a symbiotic binary with AG Peg A, has underwent many mass transfer events, varying in radius, luminosity and temperature. | ||
| Regulus Ab | Pre-white dwarf | ||||
| PSR J0348+0432 B | White dwarf | Orbiting a pulsar. | |||
| TMTS J0526+5934 B | Subdwarf B star | Smallest known non-degenerate star. | |||
| WISEA 1810−1010 | Brown dwarf |
50,000 to 125,000 km
Partial list containing stars from 0.0718 to 0.18.125,000 to 200,000 km
Partial list containing stars from 0.18 to 0.287.200,000 to 275,000 km
Partial list containing stars from 0.29 to 0.395 solar radii.275,000 to 350,000 km
Partial list containing stars from 0.395 to 0.5 solar radii.Smallest stars by type
| Type | Radius | Radius | Radius | Radius | Date | Notes | References | |
| Red dwarf | EBLM J0555−57Ab | 0.084 | 0.84 | 9.41 | 2017 | The red dwarf stars are considered the smallest stars known, and representative of the smallest star possible. | ||
| Brown dwarf | 0.029 | 0.282 | 3.16 | 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 | 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 | 0.00000646830.0000077332 | 0.000062940.00007525 | 0.00070550.0008435 | – | 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. |
Timeline of smallest red dwarf star recordholders
Red dwarfs are considered the smallest star known that are active fusion stars, and are the smallest stars possible that is not a brown dwarf.| Date | Radius | Radius | Radius km | Notes | ||
| 0.084 | 0.84 | This star has a size comparable to that of Saturn. | ||||
| 0.102 | 1.01 | Lowest mass main sequence star as of 2020. | ||||
| 0.117 | 1.16 |