This is a list of exceptional red dwarfs.
![]() | This article may require cleanup to meet Wikipedia's quality standards. The specific problem is: Many sections need to be filled in or if too hard to fill in, delete the section header. (October 2018) |
![]() |
Look up red dwarf in Wiktionary, the free dictionary. |
![]() |
Wikimedia Commons has media related to Red dwarfs. |
This is a list of red dwarfs that currently hold records.
Record Title | Star | Date | Data | Notes | |
---|---|---|---|---|---|
First discovered | Lacaille 8760 | 1753 | Originally listed in a 1763 catalog that was published posthumously by Abbé Nicolas Louis de Lacaille.
Further information: § List of the earliest red dwarfs discovered |
[1] | |
First discovered with planet(s) | Gliese 876 | 1998 | Gliese 876 b | See also: List of exoplanet firsts
The Jovian planet was the first discovered around a red dwarf. |
[2][3] |
First discovered with giant planet(s) | Gliese 876 | 1998 | Gliese 876 b | The giant planet was the first planet discovered around a red dwarf. | [2][3] |
First discovered with terrestrial planet(s) | Kepler-42 (KOI-961) |
2012 | KOI-961 b KOI-961 c KOI-961 d |
3 terrestrial planets were discovered around KOI-961 in 2012, the first terrestrial planets found to orbit a red dwarf. | [4] |
Record Title | Star | Date | Data | Notes | |
---|---|---|---|---|---|
Least voluminous | EBLM J0555-57Ab | 2017 | r= 59,000 km (37,000 mi) | Further information: § List of least voluminous red dwarfs |
[5][6][7] |
Most voluminous | V358 Boo | 2020 | 3.73 R☉ | Further information: § List of most voluminous red dwarfs |
[8] |
Least massive | 2MASS J0523-1403 | 2015 | 67.54±12.79 MJ | Further information: § List of least massive red dwarfs |
[9] |
Most massive | Lacaille 8760 | 3.91 M☉ | Further information: § List of most massive red dwarfs |
[8] | |
Least distant | Proxima Centauri | 1917 | 4.2 ly (1.3 pc) | Further information: § List of nearest red dwarfs
This is also known as Alpha Centauri C and is a member of the α Cen trinary system. It is the nearest neighbouring star to the Sun. |
[10] |
Most distant | UDF 3561 | 2010 | 202,000 ly
(62,000 pc) |
Further information: § List of furthest red dwarfs |
[11] |
Least luminous | 2MASS J0523-1403 | Further information: § List of least luminous red dwarfs |
[9] | ||
Most luminous | Further information: § List of most luminous red dwarfs |
||||
Dimmest | Further information: § List of dimmest red dwarfs |
||||
Brightest | Lacaille 8760 | V= 6.69 | Further information: § List of brightest red dwarfs
Also called AX Microscopii. This is the 24th closest star to the Sun, and also intrinsically luminous for red dwarfs, having spectral class M0. |
[12][13] | |
Youngest | See T Tauri star | Further information: § List of youngest red dwarfs |
|||
Oldest | Further information: § List of oldest red dwarfs |
||||
This is a list of red dwarfs with names that are not systematically designated.
Star | Naming | Notes | |
---|---|---|---|
Proxima Centauri | Named for being the closest neighbouring star to Earth's Sun | Lies within the Alpha Centauri star system | [10] |
Barnard's Star | Named after its discoverer, E. E. Barnard | Second closest neighbouring star system to Earth, after α Cen. Also the star with the highest proper motion. | [14] |
van Biesbroeck's star | Named for its discoverer, George van Biesbroeck | Was once the least luminous, and, lowest mass, known star. | [15] |
Kapteyn's star | Named for the astronomer who discovered it had gone missing, Jacobus Kapteyn | Was once the star with the highest proper motion, thus making it move away from its recorded position in the sky and go "missing". | [14] |
Teegarden's Star | Named after the lead investigator astrophysicist who discovered it, Bonnard J. Teegarden, through a datacrunching search of archived data. | ||
Star | Distance ly (pc) |
Notes | ||
---|---|---|---|---|
1 | Proxima Centauri | 4.2 ly (1.3 pc) | Part of the α Cen trinary system, the closest neighbouring star system. It is also the nearest neighbouring star. | [10] |
2 | Barnard's Star | 5.95 ly (1.82 pc) | Second closest neighbouring star system | [16] |
3 | Wolf 359 | 7.86 ly (2.41 pc) | Also called CN Leonis | |
4 | Lalande 21185 | 8.3 ly (2.5 pc) | ||
5 | Luyten 726-8 | 8.7 ly (2.7 pc) | This is a binary star system with two red dwarfs | |
6 | Ross 154 | 9.68 ly (2.97 pc) | [citation needed] | |
Star | Radius Solar radii (Sun = 1) |
Radius Jupiter radii (Jupiter = 1) |
Radius km (mi) |
Notes | ||
---|---|---|---|---|---|---|
1 | EBLM J0555-57Ab | 0.084 | 0.84 | 59,000 km (37,000 mi) | This star is slightly larger than the planet Saturn. | [5][6][7] |
2 | 2MASS J0523-1403 | 0.086 | 0.86 | 60,000 km (37,000 mi) | [17][18][19] | |
This is a list of titleholders of being the red dwarf with the smallest volume, and its succession over time.
Star | Date | Radius Solar radii (Sun = 1) |
Radius Jupiter radii (Jupiter = 1) |
Radius km (mi) |
Notes | |
---|---|---|---|---|---|---|
EBLM J0555-57Ab | 2017— | 0.084 | 0.84 | 59,000 km (37,000 mi) | This star is slightly larger than the planet Saturn. | [5][6][7] |
2MASS J0523-1403 | 2013-2017 | 0.086 | 0.86 | 60,000 km (37,000 mi) | [17][18][19] | |
OGLE-TR-122B | 2005-2013 | 0.120 | 1.16 | 81,100 km (50,400 mi) | [20][21][22] | |
{{cite journal}}
: CS1 maint: uses authors parameter (link){{cite magazine}}
: Cite magazine requires |magazine=
(help)
Stars | |||||||
---|---|---|---|---|---|---|---|
Formation |
| ||||||
Evolution |
| ||||||
Classification |
| ||||||
Nucleosynthesis | |||||||
Structure |
| ||||||
Properties |
| ||||||
Star systems | |||||||
Earth-centric observations |
| ||||||
Lists |
| ||||||
Related |
| ||||||