List of brown dwarfs explained

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.

Confirmed brown dwarfs orbiting primary stars

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.

StarConstellationRight
ascension
DeclinationApp.
mag.
Distance (ly)Spectral
type
Brown dwarfMass
(MJ)
Radius
(RJ)
Orbital
period

(d)
Semimajor
axis
(AU)
Ecc.Discovery
year
5.88 36.1 K0V+T7.5B 45.96 ±4.050.85476 2006
6.77 66 G9V+L88802001
HD 63754Puppis6.55163.6G0V + L/Tb81.90.8626,79116.90.262024
12.36 538 K7+M8b 17 2.2 440 2008
HD 984Cetus7.32149.1F7Vb611.57651,100280.762015
5.02 58.3 G2+G2+L8C 44.00 ±6.460.953600 2010
11.77 50.2 M2.5+L3βb 31.66 ±7.191.18300 1998
5.64 19.0 K4V+
M1V+M3V
D 32.54 ±6.010.931500 2000
13.1 155.3 M3V+T3.5b 11 2000 2006
5.74 126.2 F7IVB 2000
6.70 337.25 B9Vneb 20 6.5? 2005
58.3 G0V+T2.5B 17.06 ±6.91.14795 2006
473 M7b 14 670 2007
12.33 139 K1IV+M218.4 1.3283 0.0177 0.081 2004
CoRoT-1522 F7Vb63.41.123.060360.04502010
4.73 25.11 F8.5Vb 37 3.98 0.06 0 1931
4.63 43.9 F8V13.98 237.7 0.822 0.224 1999
6.36 51.9 G8V+T923 96 21 2009
4.40 302 K2IIIb 18.1 305 2004
10.62 698 G415.2 428.5 1.186 0.691 2009
8.74 163 G5V14.3 465.1 1.13 0.067 2009
7.57 603.4 K2II14 471.6 1.85 0.28 2005
6.31 124.75 F7Vb 14 639 1.58 2005
10.2 31.5 M3V+M8.5Ba + Bb 116 870 0.87 0.317 1988
7.29 146.77 G2Vb 40 1471.7 2.5 0.37 1996
20.1 522 M6.5b 18 1590.9 1 0.49 2007
CoRoT-2014.66 4000G2V1716752.90.62010
6.92 123.5 G5c 34 1739.5 2.87 0.228 2001
5.94 138 G4IVc 37 2174.3 3.68 0.36 2002
4.69 11.8 K5V+T1V+T6V28 5478.75 2.65 2003
10.9 590 sdB+Mb 19.23 5786 5.30 0.46 2008
9.72 37.55 M0V+T8.5pc 10.29 ±2.461.1533081 11002010
7.88 136 G5V+T9C 60 73000202006
8.14 19 M1V+T6.5 B 40 73050 40 1995
Octans11.82 111 M1V+L3γ 13.3 ± 1.7 328725000 6900 2009
4.69 11.8 K5V+T1V+T6V47 1532899.8 2003
8.13 180.8 G3Vb 18.15 1951 3.17 0.638 2008
6.94 171 F9V42 1209 1.45 0.352 2002
8.07 156.42 G0Vb 46 147.94 0.54 0.61 1996
11.4 400 K7eV+M9e1–42 1.8 103 2005
9.18 101.95 K2V15.0 8.428198 0.0751 0.277 2000
3.33 152.8 K0IIIb 21.9 536 0.13 2004
6.89 127.52 G4IV46 108.55 0.46 0.55 2000
17.4 12.57 M8.5VB 40-50 4.1 2006
13.3 2220 G0V21.66 1.01 4.2568 0.057 0 2008
V921 Scorpii[1] Scorpius11.04833B0IVeb608352019
5.80 57.7 G1V+L4-5B 65 14 2002
4.65 220 A3V+L5B 55 910 2014
8.08 151.14 G6Vb 17.4 255.87 0.83 0.435 2000
Koenigstuhl1Phoenix15.387.4M5.5V+L0.6VB51.88 ±3.61.182083.41998
HD 126053Virgo6.356.9G1+T8pB34.29 ±18.380.9126302012
47 OphiuchiOphiuchus4.5105.3F3+L5.5B69.66 ±0.880.9388502014
Wolf 1130Cygnus13.954.1sdM3+ONe+sdT8C44.90.8231502013

Confirmed brown dwarf orbiting stellar remnants

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.

StarConstellationRight
ascension
DeclinationApp.
mag.
Distance (ly)Spectral
type
Brown dwarfMass
(MJ)
Radius
(RJ)
Orbital
period

(d)
Semimajor
axis
(AU)
Ecc.Discovery
year
14.6 103 D4A+L4B 76.12 ±1.040.91123 1988
WD 0137-349Sculptor15.33330DA+L8B530.08030.003002006
PHL 5038Aquarius17.3240DAZ+L8-9B73662006
SDSS J1433 (mass transfer)Boötes18.9760WD+L1B58 ±80.0542008/2016
SDSS 1557Serpens18.6500DAZ+L4B0.0950.0032011/2017
QZ Librae (mass transfer)Libra18.8649WD+T?B25-610.0642018
BW Sculptoris (mass transfer)Sculptor16.5305D+TB53.4 ±6.30.0540.00271997/2023

Unconfirmed brown dwarfs

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.

StarConstellationRight
ascension
DeclinationApp.
mag.
Distance (ly)Spectral
type
Brown dwarfMass
(MJ)
Radius
(RJ)
Orbital
period

(d)
Semimajor
axis
(AU)
Ecc.Discovery year
12.90 48 M4b 64 73 0.27 1998
9.75 652 K2II21.42 379.63 1.45 0.15 2009
5.16 655.58 K5IIIc 60 650 2.5 1996
5.54 42.1 G9b 17.2 2752 0.38 2007
7.25 220 G5V18.4 2900 >0.25 2007
10.38 326 M2.5Vb 16 ~5500 0 2008

Field brown dwarfs

Data updated from and merged from previous tables

Brown dwarfConstellationRight
ascension
DeclinationApp.
mag.
Distance (ly)Spectral
type
Mass
(MJ)
Radius
(RJ)
Discovery
year
2MASS 0036+1821Pisces12.4728.6L3.5420.942000
CFBDS J005910.90–011401.3Cetus18.0830T8.5232013
DENIS-P J020529.0−115925ACetus65L5.51997
DENIS-P J020529.0−115925BCetus65L81997
DENIS-P J020529.0−115925CCetus65T01997
2MASS J02431371−2453298Fornax35T6330.992002
WISE J0254+0223Cetus16.0124T8651.9n/a
DEN 0255-4700Eridanus22.9216.2L8800.972006
LP 944-20Fornax10.72520.9M9β731.43n/a
2MASP J0345432+25402388L0741.051997
Teide 1Taurus380M8553.781995
2MASS J03552337+1133437Taurus14.0529.8L5γ201.322006
2MASS J04151954−0935066Eridanus15.718.6T8300.952002
Eridanus29.5L6.5480.972003
2MASS J04414489+2301513470M8.5192010
2MASS J0523−1403Lepus40L2.5681.01n/a
2MASS 0532+8246Camelopardalis81L7832018
UGPS J072227.51-054031.2Monoceros13.4T9260.982010
DENIS J081730.0-615520Carina13.616.1T6440.942010
DENIS J082303.1−491201AVela67L1.5442006
DENIS J082303.1−491201BVela67L5.5282006
2MASSW J0920122+351742Lynx95L6.52000
2MASSI J0937347+293142Leo20.0T6p420.942002
2MASS 0939−2448Antlia16.8317.4T8320.952005
Luhman 16BVela6.516T1431.022013
Luhman 16AVela6.516L8401.012013
DENIS-P J1058.7−1548Crater14.15549L3641.001997
Cha 110913-773444Chamaeleon21.59163L81.82005
OTS 44Chamaeleon554M9.5V152005
2MASS J11145133−2618235Hydra15.8618.2T7.5330.962005
DENIS-P J1228.2-1547Corvus14.3866L51999
2M 1237+6526Draco16.0545.6T6.5410.942003
Kelu-1AHydra61L2630.981997
Kelu-1BHydra61L4580.981997
LHS 2924Boötes19.7438.5M9V761.06
CFBDSIR 1458+10ABoötes19.83104T911.11.52010
CFBDSIR 1458+10BBoötes21.85104Y091.32010
TVLM 513-46546Boötes15.0935.1M8.5V751.05n/a
2MASS 1503+2525Boötes20.7T5440.942003
2MASS 1507−1627Libra1923.9L5600.992000
SDSSp J162414.37+002915.6Serpens36T6430.941999
LSR J1835+3259Lyra18.2718.5M8.5771.072003
PSO J318.5−22Capricornus80L7VL-G6.51.532013
2MASS J21392676+0220226Aquarius14.7132.1T1.5460.96n/a
2MASS J22282889-4310262Grus15.6635T6420.942013
WISE 0146+4234Andromeda18.7120.5Y02010
WISE 0226-0211Cetus18.9491T72010
WISE 0313+7807Cepheus17.6528T8.52010
WISE 0316+4307Perseus106.3T82010
WISE 0350-5658Reticulum22.817.7Y12010
WISE 0359-5401Reticulum21.5619.2Y02010
WISE 0410+1502Taurus19.2520Y061.172010
WISE 0458+6434ACamelopardalis17.5035.9T8.5154.22010
WISE 0458+6434BCamelopardalis18.4835.9T9.5103.82010
WISE 0535-7500Mensa21.147Y12010
WISE 0607+2429Gemini14.2225.4L82010
WISE 0647-6232Pictor22.6528Y12010
WISE 0713-2917Canis Major19.6423.2Y02010
WISE 0734-7157Volans20.4134.9Y02010
WISE 1217+1626AComa Berenices18.5934.2T9122010
WISE 1217+1626BComa Berenices20.2634.2Y062010
WISE 1405+5534Ursa Major20.225.3Y0 pec300.862010
WISE 1506+7027Ursa Minor14.3311.1T62010
WISE 1541-2250Libra21.1620Y0.52010
WISE 1639-6847Triangulum Australe16.3Y02010
WISE 1711+3500Hercules17.8960.3T82010
WISE 1738+2732Hercules19.4720Y02010
WISE 1741+2553Hercules16.5318.9T92010
WISE 1828+2650Lyra23.5736Y22010
WISE 1841+7000Draco17.24131.1T52010
WISE 1952+7240Draco15.0944.4T42010
WISE 2056+1459Delphinus19.2124.5Y02010
WISE 2220-3628Grus20.3826.4Y02010
WISEA 1101+5400Ursa Major11h 01m 25.95s+54° 00′ 52.8″111T5.52017
2M1510Libra15h 10m 47.47s−28° 18′ 18.3″120M9γ+M9γ2002

See also

External links

Notes and References

  1. Web site: Martin . Pierre-Yves . 2022 . Planet V921 Sco b . 2024-01-01 . exoplanet.eu . en.
  2. Web site: L 34-26. 2021-07-16. sim-basic.