This is a list of notable brown dwarfs. These are objects that have masses between heavy gas giants and low-mass stars. The first isolated brown dwarf discovered was Teide 1 in 1995. The first brown dwarf discovered orbiting a star was Gliese 229 B, also discovered in 1995. The first brown dwarf found to have a planet was 2M1207, discovered in 2004., more than 2,800 brown dwarfs have been identified. An isolated object with less than about 13 Jupiter masses is technically a sub-brown dwarf or rogue planet.
Because the mass of a brown dwarf is between that of a planet and that of a star, they have also been called planetars or hyperjovians. Various catalog designations have been used to name brown dwarfs. Brown dwarfs with names ending in a letter such as B, C, or D are in orbit around a primary star; those with names ending in a lower-case letter such as b, c, or d, may be exoplanets (see Exoplanet naming convention).
Some exoplanets, especially those detected by radial velocity, can turn out to be brown dwarfs if their mass is higher than originally thought: most have only known minimum masses because the inclination of their orbit is not known. Examples include HD 114762 b (>11.68 MJ), Pi Mensae b (>10.312 MJ), and NGC 2423-3 b (>10.6 MJ).
A complete list of more than 3000 ultracool dwarfs, which includes brown dwarfs and low-mass stars, is being maintained by astronomers. It is called the UltracoolSheet. The same team also produced a list of 1000 ultracool dwarfs with their mass being determined.
Sorted by increasing right ascension of the parent star. Brown dwarfs within a system sorted by increasing orbital period.
Some brown dwarfs listed could still be massive planets.
Star | Constellation | Right ascension | Declination | App. mag. | Distance (ly) | Spectral type | Brown dwarf | Mass (MJ) | Radius (RJ) | Orbital period (d) | Semimajor axis (AU) | Ecc. | Discovery year | |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
5.88 | 36.1 | K0V+T7.5 | B | 45.96 ±4.05 | 0.85 | 476 | 2006 | |||||||
6.77 | 66 | G9V+L8 | 880 | 2001 | ||||||||||
HD 63754 | Puppis | 6.55 | 163.6 | G0V + L/T | b | 81.9 | 0.86 | 26,791 | 16.9 | 0.26 | 2024 | |||
12.36 | 538 | K7+M8 | b | 17 | 2.2 | 440 | 2008 | |||||||
HD 984 | Cetus | 7.32 | 149.1 | F7V | b | 61 | 1.576 | 51,100 | 28 | 0.76 | 2015 | |||
5.02 | 58.3 | G2+G2+L8 | C | 44.00 ±6.46 | 0.95 | 3600 | 2010 | |||||||
11.77 | 50.2 | M2.5+L3β | b | 31.66 ±7.19 | 1.18 | 300 | 1998 | |||||||
5.64 | 19.0 | K4V+ M1V+M3V | D | 32.54 ±6.01 | 0.93 | 1500 | 2000 | |||||||
13.1 | 155.3 | M3V+T3.5 | b | 11 | 2000 | 2006 | ||||||||
5.74 | 126.2 | F7IV | B | 2000 | ||||||||||
6.70 | 337.25 | B9Vne | b | 20 | 6.5? | 2005 | ||||||||
58.3 | G0V+T2.5 | B | 17.06 ±6.9 | 1.14 | 795 | 2006 | ||||||||
473 | M7 | b | 14 | 670 | 2007 | |||||||||
12.33 | 139 | K1IV+M2 | 18.4 | 1.3283 | 0.0177 | 0.081 | 2004 | |||||||
CoRoT-15 | 22 | F7V | b | 63.4 | 1.12 | 3.06036 | 0.045 | 0 | 2010 | |||||
4.73 | 25.11 | F8.5V | b | 37 | 3.98 | 0.06 | 0 | 1931 | ||||||
4.63 | 43.9 | F8V | 13.98 | 237.7 | 0.822 | 0.224 | 1999 | |||||||
6.36 | 51.9 | G8V+T9 | 23 | 96 | 21 | 2009 | ||||||||
4.40 | 302 | K2III | b | 18.1 | 305 | 2004 | ||||||||
10.62 | 698 | G4 | 15.2 | 428.5 | 1.186 | 0.691 | 2009 | |||||||
8.74 | 163 | G5V | 14.3 | 465.1 | 1.13 | 0.067 | 2009 | |||||||
7.57 | 603.4 | K2II | 14 | 471.6 | 1.85 | 0.28 | 2005 | |||||||
6.31 | 124.75 | F7V | b | 14 | 639 | 1.58 | 2005 | |||||||
10.2 | 31.5 | M3V+M8.5 | Ba + Bb | 116 | 870 | 0.87 | 0.317 | 1988 | ||||||
7.29 | 146.77 | G2V | b | 40 | 1471.7 | 2.5 | 0.37 | 1996 | ||||||
20.1 | 522 | M6.5 | b | 18 | 1590.9 | 1 | 0.49 | 2007 | ||||||
CoRoT-20 | 14.66 | 4000 | G2V | 17 | 1675 | 2.9 | 0.6 | 2010 | ||||||
6.92 | 123.5 | G5 | c | 34 | 1739.5 | 2.87 | 0.228 | 2001 | ||||||
5.94 | 138 | G4IV | c | 37 | 2174.3 | 3.68 | 0.36 | 2002 | ||||||
4.69 | 11.8 | K5V+T1V+T6V | 28 | 5478.75 | 2.65 | 2003 | ||||||||
10.9 | 590 | sdB+M | b | 19.23 | 5786 | 5.30 | 0.46 | 2008 | ||||||
9.72 | 37.55 | M0V+T8.5p | c | 10.29 ±2.46 | 1.15 | 33081 | 1100 | 2010 | ||||||
7.88 | 136 | G5V+T9 | C | 60 | 73000 | 20 | 2006 | |||||||
8.14 | 19 | M1V+T6.5 | B | 40 | 73050 | 40 | 1995 | |||||||
Octans | 11.82 | 111 | M1V+L3γ | 13.3 ± 1.7 | 328725000 | 6900 | 2009 | |||||||
4.69 | 11.8 | K5V+T1V+T6V | 47 | 1532899.8 | 2003 | |||||||||
8.13 | 180.8 | G3V | b | 18.15 | 1951 | 3.17 | 0.638 | 2008 | ||||||
6.94 | 171 | F9V | 42 | 1209 | 1.45 | 0.352 | 2002 | |||||||
8.07 | 156.42 | G0V | b | 46 | 147.94 | 0.54 | 0.61 | 1996 | ||||||
11.4 | 400 | K7eV+M9e | 1–42 | 1.8 | 103 | 2005 | ||||||||
9.18 | 101.95 | K2V | 15.0 | 8.428198 | 0.0751 | 0.277 | 2000 | |||||||
3.33 | 152.8 | K0III | b | 21.9 | 536 | 0.13 | 2004 | |||||||
6.89 | 127.52 | G4IV | 46 | 108.55 | 0.46 | 0.55 | 2000 | |||||||
17.4 | 12.57 | M8.5V | B | 40-50 | 4.1 | 2006 | ||||||||
13.3 | 2220 | G0V | 21.66 | 1.01 | 4.2568 | 0.057 | 0 | 2008 | ||||||
V921 Scorpii[1] | Scorpius | 11.0 | 4833 | B0IVe | b | 60 | 835 | 2019 | ||||||
5.80 | 57.7 | G1V+L4-5 | B | 65 | 14 | 2002 | ||||||||
4.65 | 220 | A3V+L5 | B | 55 | 910 | 2014 | ||||||||
8.08 | 151.14 | G6V | b | 17.4 | 255.87 | 0.83 | 0.435 | 2000 | ||||||
Koenigstuhl1 | Phoenix | 15.3 | 87.4 | M5.5V+L0.6V | B | 51.88 ±3.6 | 1.18 | 2083.4 | 1998 | |||||
HD 126053 | Virgo | 6.3 | 56.9 | G1+T8p | B | 34.29 ±18.38 | 0.91 | 2630 | 2012 | |||||
47 Ophiuchi | Ophiuchus | 4.5 | 105.3 | F3+L5.5 | B | 69.66 ±0.88 | 0.93 | 8850 | 2014 | |||||
Wolf 1130 | Cygnus | 13.9 | 54.1 | sdM3+ONe+sdT8 | C | 44.9 | 0.82 | 3150 | 2013 |
A stellar remnant can be for example a white dwarf, a pulsar or a black hole. Objects with a mass of a brown dwarf, but with a history of mass-transfer might not be brown dwarfs. If they exist as a period bouncer around a white dwarf they are thought to once have been stars and are today "brown dwarf-like objects". Objects around black widow pulsars on the other hand are thought to be white dwarfs that lost mass to the pulsar and therefore will differ in composition and density compared to brown dwarfs. This list is sorted after the discovery year.
Star | Constellation | Right ascension | Declination | App. mag. | Distance (ly) | Spectral type | Brown dwarf | Mass (MJ) | Radius (RJ) | Orbital period (d) | Semimajor axis (AU) | Ecc. | Discovery year | |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
14.6 | 103 | D4A+L4 | B | 76.12 ±1.04 | 0.91 | 123 | 1988 | |||||||
WD 0137-349 | Sculptor | 15.33 | 330 | DA+L8 | B | 53 | 0.0803 | 0.0030 | 0 | 2006 | ||||
PHL 5038 | Aquarius | 17.3 | 240 | DAZ+L8-9 | B | 73 | 66 | 2006 | ||||||
SDSS J1433 (mass transfer) | Boötes | 18.9 | 760 | WD+L1 | B | 58 ±8 | 0.054 | 2008/2016 | ||||||
SDSS 1557 | Serpens | 18.6 | 500 | DAZ+L4 | B | 0.095 | 0.003 | 2011/2017 | ||||||
QZ Librae (mass transfer) | Libra | 18.8 | 649 | WD+T? | B | 25-61 | 0.064 | 2018 | ||||||
BW Sculptoris (mass transfer) | Sculptor | 16.5 | 305 | D+T | B | 53.4 ±6.3 | 0.054 | 0.0027 | 1997/2023 |
Sorted by increasing right ascension of the parent star. Brown dwarfs within a system sorted by increasing orbital period.
Some brown dwarfs listed could still be massive planets.
Star | Constellation | Right ascension | Declination | App. mag. | Distance (ly) | Spectral type | Brown dwarf | Mass (MJ) | Radius (RJ) | Orbital period (d) | Semimajor axis (AU) | Ecc. | Discovery year | |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
12.90 | 48 | M4 | b | 64 | 73 | 0.27 | 1998 | |||||||
9.75 | 652 | K2II | 21.42 | 379.63 | 1.45 | 0.15 | 2009 | |||||||
5.16 | 655.58 | K5III | c | 60 | 650 | 2.5 | 1996 | |||||||
5.54 | 42.1 | G9 | b | 17.2 | 2752 | 0.38 | 2007 | |||||||
7.25 | 220 | G5V | 18.4 | 2900 | >0.25 | 2007 | ||||||||
10.38 | 326 | M2.5V | b | 16 | ~5500 | 0 | 2008 |
Data updated from and merged from previous tables
Brown dwarf | Constellation | Right ascension | Declination | App. mag. | Distance (ly) | Spectral type | Mass (MJ) | Radius (RJ) | Discovery year | |
---|---|---|---|---|---|---|---|---|---|---|
2MASS 0036+1821 | Pisces | 12.47 | 28.6 | L3.5 | 42 | 0.94 | 2000 | |||
CFBDS J005910.90–011401.3 | Cetus | 18.08 | 30 | T8.5 | 23 | 2013 | ||||
DENIS-P J020529.0−115925A | Cetus | 65 | L5.5 | 1997 | ||||||
DENIS-P J020529.0−115925B | Cetus | 65 | L8 | 1997 | ||||||
DENIS-P J020529.0−115925C | Cetus | 65 | T0 | 1997 | ||||||
2MASS J02431371−2453298 | Fornax | 35 | T6 | 33 | 0.99 | 2002 | ||||
WISE J0254+0223 | Cetus | 16.01 | 24 | T8 | 65 | 1.9 | n/a | |||
DEN 0255-4700 | Eridanus | 22.92 | 16.2 | L8 | 80 | 0.97 | 2006 | |||
LP 944-20 | Fornax | 10.725 | 20.9 | M9β | 73 | 1.43 | n/a | |||
2MASP J0345432+254023 | 88 | L0 | 74 | 1.05 | 1997 | |||||
Teide 1 | Taurus | 380 | M8 | 55 | 3.78 | 1995 | ||||
2MASS J03552337+1133437 | Taurus | 14.05 | 29.8 | L5γ | 20 | 1.32 | 2006 | |||
2MASS J04151954−0935066 | Eridanus | 15.7 | 18.6 | T8 | 30 | 0.95 | 2002 | |||
Eridanus | 29.5 | L6.5 | 48 | 0.97 | 2003 | |||||
2MASS J04414489+2301513 | 470 | M8.5 | 19 | 2010 | ||||||
2MASS J0523−1403 | Lepus | 40 | L2.5 | 68 | 1.01 | n/a | ||||
2MASS 0532+8246 | Camelopardalis | 81 | L7 | 83 | 2018 | |||||
UGPS J072227.51-054031.2 | Monoceros | 13.4 | T9 | 26 | 0.98 | 2010 | ||||
DENIS J081730.0-615520 | Carina | 13.6 | 16.1 | T6 | 44 | 0.94 | 2010 | |||
DENIS J082303.1−491201A | Vela | 67 | L1.5 | 44 | 2006 | |||||
DENIS J082303.1−491201B | Vela | 67 | L5.5 | 28 | 2006 | |||||
2MASSW J0920122+351742 | Lynx | 95 | L6.5 | 2000 | ||||||
2MASSI J0937347+293142 | Leo | 20.0 | T6p | 42 | 0.94 | 2002 | ||||
2MASS 0939−2448 | Antlia | 16.83 | 17.4 | T8 | 32 | 0.95 | 2005 | |||
Luhman 16B | Vela | 6.516 | T1 | 43 | 1.02 | 2013 | ||||
Luhman 16A | Vela | 6.516 | L8 | 40 | 1.01 | 2013 | ||||
DENIS-P J1058.7−1548 | Crater | 14.155 | 49 | L3 | 64 | 1.00 | 1997 | |||
Cha 110913-773444 | Chamaeleon | 21.59 | 163 | L | 8 | 1.8 | 2005 | |||
OTS 44 | Chamaeleon | 554 | M9.5V | 15 | 2005 | |||||
2MASS J11145133−2618235 | Hydra | 15.86 | 18.2 | T7.5 | 33 | 0.96 | 2005 | |||
DENIS-P J1228.2-1547 | Corvus | 14.38 | 66 | L5 | 1999 | |||||
2M 1237+6526 | Draco | 16.05 | 45.6 | T6.5 | 41 | 0.94 | 2003 | |||
Kelu-1A | Hydra | 61 | L2 | 63 | 0.98 | 1997 | ||||
Kelu-1B | Hydra | 61 | L4 | 58 | 0.98 | 1997 | ||||
LHS 2924 | Boötes | 19.74 | 38.5 | M9V | 76 | 1.06 | ||||
CFBDSIR 1458+10A | Boötes | 19.83 | 104 | T9 | 11.1 | 1.5 | 2010 | |||
CFBDSIR 1458+10B | Boötes | 21.85 | 104 | Y0 | 9 | 1.3 | 2010 | |||
TVLM 513-46546 | Boötes | 15.09 | 35.1 | M8.5V | 75 | 1.05 | n/a | |||
2MASS 1503+2525 | Boötes | 20.7 | T5 | 44 | 0.94 | 2003 | ||||
2MASS 1507−1627 | Libra | 19 | 23.9 | L5 | 60 | 0.99 | 2000 | |||
SDSSp J162414.37+002915.6 | Serpens | 36 | T6 | 43 | 0.94 | 1999 | ||||
LSR J1835+3259 | Lyra | 18.27 | 18.5 | M8.5 | 77 | 1.07 | 2003 | |||
PSO J318.5−22 | Capricornus | 80 | L7VL-G | 6.5 | 1.53 | 2013 | ||||
2MASS J21392676+0220226 | Aquarius | 14.71 | 32.1 | T1.5 | 46 | 0.96 | n/a | |||
2MASS J22282889-4310262 | Grus | 15.66 | 35 | T6 | 42 | 0.94 | 2013 | |||
WISE 0146+4234 | Andromeda | 18.71 | 20.5 | Y0 | 2010 | |||||
WISE 0226-0211 | Cetus | 18.94 | 91 | T7 | 2010 | |||||
WISE 0313+7807 | Cepheus | 17.65 | 28 | T8.5 | 2010 | |||||
WISE 0316+4307 | Perseus | 106.3 | T8 | 2010 | ||||||
WISE 0350-5658 | Reticulum | 22.8 | 17.7 | Y1 | 2010 | |||||
WISE 0359-5401 | Reticulum | 21.56 | 19.2 | Y0 | 2010 | |||||
WISE 0410+1502 | Taurus | 19.25 | 20 | Y0 | 6 | 1.17 | 2010 | |||
WISE 0458+6434A | Camelopardalis | 17.50 | 35.9 | T8.5 | 15 | 4.2 | 2010 | |||
WISE 0458+6434B | Camelopardalis | 18.48 | 35.9 | T9.5 | 10 | 3.8 | 2010 | |||
WISE 0535-7500 | Mensa | 21.1 | 47 | Y1 | 2010 | |||||
WISE 0607+2429 | Gemini | 14.22 | 25.4 | L8 | 2010 | |||||
WISE 0647-6232 | Pictor | 22.65 | 28 | Y1 | 2010 | |||||
WISE 0713-2917 | Canis Major | 19.64 | 23.2 | Y0 | 2010 | |||||
WISE 0734-7157 | Volans | 20.41 | 34.9 | Y0 | 2010 | |||||
WISE 1217+1626A | Coma Berenices | 18.59 | 34.2 | T9 | 12 | 2010 | ||||
WISE 1217+1626B | Coma Berenices | 20.26 | 34.2 | Y0 | 6 | 2010 | ||||
WISE 1405+5534 | Ursa Major | 20.2 | 25.3 | Y0 pec | 30 | 0.86 | 2010 | |||
WISE 1506+7027 | Ursa Minor | 14.33 | 11.1 | T6 | 2010 | |||||
WISE 1541-2250 | Libra | 21.16 | 20 | Y0.5 | 2010 | |||||
WISE 1639-6847 | Triangulum Australe | 16.3 | Y0 | 2010 | ||||||
WISE 1711+3500 | Hercules | 17.89 | 60.3 | T8 | 2010 | |||||
WISE 1738+2732 | Hercules | 19.47 | 20 | Y0 | 2010 | |||||
WISE 1741+2553 | Hercules | 16.53 | 18.9 | T9 | 2010 | |||||
WISE 1828+2650 | Lyra | 23.57 | 36 | Y2 | 2010 | |||||
WISE 1841+7000 | Draco | 17.24 | 131.1 | T5 | 2010 | |||||
WISE 1952+7240 | Draco | 15.09 | 44.4 | T4 | 2010 | |||||
WISE 2056+1459 | Delphinus | 19.21 | 24.5 | Y0 | 2010 | |||||
WISE 2220-3628 | Grus | 20.38 | 26.4 | Y0 | 2010 | |||||
WISEA 1101+5400 | Ursa Major | 11h 01m 25.95s | +54° 00′ 52.8″ | 111 | T5.5 | 2017 | ||||
2M1510 | Libra | 15h 10m 47.47s | −28° 18′ 18.3″ | 120 | M9γ+M9γ | 2002 |