List of least massive stars
From Wikipedia, the free encyclopedia
|
|
This article needs additional citations for verification. (April 2009) |
This is a list of the least-massive stars known. The list is ordered by solar mass and Jovian mass.
This list includes brown dwarfs and red dwarfs. The name of each brown dwarf has background color brown, and the names of and red dwarfs are against a background of red or orange, depending on whether they are cooler class M or warmer class M. (The objects are not actually these colors.)
Although brown dwarfs lack sufficient mass to ignite core hydrogen fusion (75-87 Jupiters, depending on metallicity), the smallest true stars (red dwarfs) can have such cool atmospheric temperatures (below 4,000 K), that it is difficult to distinguish them from brown dwarfs.
A star's mass cannot be lower than 13 Jupiter masses, because below this critical point the core does not get hot enough by gravitational pressure to start the fusion of deuterium. According to the brown dwarf interior models, typical conditions in the core for density, temperature, and pressure are expected to be the following:
A brown dwarf, therefore, is heavier than a gas-giant planet, but not quite massive enough to be a star.
The colour code for the table below is as follows: Brown = Brown Dwarf, Pink = Red Dwarf, Orange: Stars of stellar class "K".
| Star name | Solar Mass | Jupiter Mass |
|---|---|---|
| Jupiter (as reference) | 0.00096 | 1 |
| ---------------- | ----- | -- |
| OTS 44 | 0.013 | 15 |
| Oph1622 A | 0.014 | 15.5 |
| Oph1622 B | 0.016 | 17.5 |
| Gliese 229B | 0.021 | 25 |
| 2M1207 | 0.021 | 25 |
| Epsilon Indi BB | 0.024 | 28 |
| HD 98230B | 0.037 | 39 |
| Teide 1 | 0.041 | 43 |
| Epsilon Indi BA | 0.045 | 47 |
| Gliese 570D | 0.050 | 52 |
| LP 944-020 | 0.056 | 58 |
| 2MASS 0415-0935 | 0.060 | 63 |
| DENIS 1048-0039 | 0.065 | 68 |
| 2MASS 1835+3259 | 0.070 | 75 |
| DENIS 0255-4700 | 0.070 | 75 |
| V1581 Cygni C | 0.074 | 79 |
| 2MASS 0532+8246 | 0.077 | 81 |
| LHS 3003 (GJ 3877) | 0.077 | 81 |
| Gliese 165B | 0.080 | 84 |
| Gliese 623B | 0.080 | 84 |
| LHS 1070B | 0.080 | 84 |
| LHS 1070C | 0.080 | 84 |
| Ross 614B | 0.080 | 84 |
| Teegarden's Star | 0.080 | 84 |
| Van Biesbroeck's Star (VB 10) | 0.080 | 84 |
| Gl 105C | 0.082 | 86 |
| LHS 292 | 0.083 | 87 |
| LP 731-058 | 0.083 | 87 |
| DX Cancri | 0.087 | 91 |
| Van Briesboeck 8 (VB 8) | 0.088 | 92 |
| AB Doradus C | 0.089 | 93 |
| OGLE-TR-122b | 0.091 | 96 |
| Wolf 359 | 0.1 | 105 |
| ---------------- | ----- | -- |
| Sun (as reference) | 1 | 1042 |
Cha 110913-773444
The object Cha 110913-773444 is sometimes referred to as being the smallest brown dwarf, but its mass is too light for this (8 times Jupiter's mass). It is even less massive than some known exoplanets. Therefore it can better be seen as a so-called sub-brown dwarf or a planemo. Some stars are listed as red dwarfs although they should be listed as brown dwarfs due to their mass, and vice versa.
See also
|
||||||||||||||||||||||||||||||||||||||||||||







