View source for List of smallest known stars

{{Short description|None}}
This is a list of [[stars]], [[neutron stars]], [[white dwarfs]] and [[brown dwarfs]] which are the least voluminous known (the smallest stars by volume).

==List==
{{incomplete list|date=January 2015}}

===Notable small stars===
This is a list of small stars that are notable for characteristics that are not separately listed.

{| class="wikitable sortable"
|-
!| Star name !! Star mean radius, [[kilometres]] !! Star class !! Notes !! References
|-
|[[SGR 1935+2154]]
|4.35
|[[soft gamma repeater]]
|
| <ref> {{Cite arXiv|last=Shao|first=Yixuan|date=2024|title=GTC Optical/NIR upper limits and NICER X-ray analysis of SGR J1935+2154 for the outburst in 2022|eprint=2410.00635|class=astrophysics}} </ref>
|-
|[[RX J0720.4−3125]]
|{{val|4.50|0.08|0.09}}{{snd}}{{val|5.38|0.13|0.14}}
| rowspan="1" |[[Neutron star]]
|Neutron stars are stellar remnants produced when a star of around 8–9 solar masses or more explodes in a supernova at the end of its life. They are usually produced by stars of less than 20 solar masses, although a more massive star may produce a neutron star in certain cases.
|<ref name="Hohle">{{cite journal|display-authors= 4|author= Hohle, M.M.|author2= Haberl, F.|author3= Vink, J.|author4= de Vries, C.P.|author5= Turolla, R.|author6= Zane, S.|author7= Méndez, M. |title = The Continued Spectral and Temporal Evolution of RX J0720.4-3125 | journal = [[Monthly Notices of the Royal Astronomical Society]] |volume = 423 |issue = 2 |pages= 1194–99 |bibcode=2012MNRAS.423.1194H |arxiv = 1203.3708 |doi = 10.1111/j.1365-2966.2012.20946.x |year= 2012|doi-access= free|s2cid= 55696761}}</ref>
|-
|[[4U 1820-30]]
|9.1
|[[Pulsar]]
|
|<ref name=Wanas2024>{{Cite journal|last1=Wanas|first1=M. I.|last2=Ammar|first2=Samah A.|last3=Foda|first3=Mona M.|date=July 2024|title=Structure of compact stars: A pure geometric approach|journal=New Astronomy|volume=109|url=https://www.sciencedirect.com/science/article/abs/pii/S1384107624000150|bibcode=2024NewA..10902201W|doi=10.1016/j.newast.2024.102201|issn=1384-1076}}</ref>
|-
|[[PSR B1257+12|Lich Pulsar]] ''(PSR B1257+12)''
|10
| rowspan="3" |[[Pulsar]]
|Orbited by three planets.
|<ref name="pulsar">{{Cite web |url=http://www.phy.cuhk.edu.hk/opus/comments_2011/hckrep.pdf |title=Archived copy |access-date=2017-10-26 |archive-date=2019-02-12 |archive-url=https://web.archive.org/web/20190212190344/http://www.phy.cuhk.edu.hk/opus/comments_2011/hckrep.pdf |url-status=dead }}</ref>
|-
|[[Crab Pulsar]] ''(PSR B0531+21)''
|10
|Relatively young at 7200 (or 970 relative to Earth) years old as of May 2024.
|<ref>{{cite web|url=https://www.google.com/search?q=psr+b0531+21+radius|title=psr b0531 21 radius - Google Search|website=www.google.com|access-date=2018-09-04}}</ref>
|-
|[[Geminga]]
|10
|
|<ref>{{cite encyclopedia|url=https://www.britannica.com/place/Geminga|title=Geminga {{!}} pulsar|encyclopedia=Encyclopedia Britannica|access-date=2018-09-05}}</ref>
|-
|[[XTE J1739-285]]
|10.9
|[[Pulsar]] ([[quark star]]?)
|
|<ref>{{cite journal|last1=Zhang|first1=C. M.|last2=Yin|first2=H. X.|last3=Zhao|first3=Y. H.|last4=Wei|first4=Y. C.|last5=Li|first5=X. D.|date=October 2007|title=Does Sub-millisecond Pulsar XTE J1739-285 Contain a Low Magnetic Neutron Star or Quark Star ?|journal=Publications of the Astronomical Society of the Pacific|volume=119|issue=860|pages=1108–1113|doi=10.1086/522796|issn=0004-6280|arxiv=0708.3566|bibcode=2007PASP..119.1108Z|s2cid=15651718 }}</ref>
|-
|[[PSR J1906+0746]]
|11.99{{snd}}12.85
| rowspan="6" |[[Pulsar]]
|
|<ref name=Sen2024/>
|-
|[[PSR J2043+1711]]
|12.13{{snd}}12.96
|
|<ref name=Sen2024/>
|-
|[[PSR J1933–6211]]
|12.15{{snd}}12.98
|
|<ref name=Sen2024/>
|-
|[[Vela Pulsar|Vela pulsar]]
|12.52{{snd}}13.30
|
|<ref name=Sen2024>{{Cite arXiv|last1=Sen|first1=Debashree|last2=Guha|first2=Atanu|date=21 February 2024|title=Estimating the dark matter halo velocity and surface temperature of some known pulsars due to dark matter capture|class=hep-ph |eprint=2402.13795}}</ref>
|-
|[[PSR J0348+0432|PSR J0348+0432 A]]
|13 ± 2
|Orbited by a white dwarf star (see below)
|<ref name="ReferenceA">{{cite journal|last1=Antoniadis|first1=J.|last2=Freire|first2=P. C. C.|last3=Wex|first3=N.|last4=Tauris|first4=T. M.|last5=Lynch|first5=R. S.|last6=Van Kerkwijk|first6=M. H.|last7=Kramer|first7=M.|last8=Bassa|first8=C.|last9=Dhillon|first9=V. S.|year=2013|title=A Massive Pulsar in a Compact Relativistic Binary|journal=Science|volume=340|issue=6131|pages=1233232|arxiv=1304.6875|bibcode=2013Sci...340..448A|doi=10.1126/science.1233232|pmid=23620056|last10=Driebe|first10=T.|last11=Hessels|first11=J. W. T.|last12=Kaspi|first12=V. M.|last13=Kondratiev|first13=V. I.|last14=Langer|first14=N.|last15=Marsh|first15=T. R.|last16=McLaughlin|first16=M. A.|last17=Pennucci|first17=T. T.|last18=Ransom|first18=S. M.|last19=Stairs|first19=I. H.|last20=Van Leeuwen|first20=J.|last21=Verbiest|first21=J. P. W.|last22=Whelan|first22=D. G.|citeseerx=10.1.1.769.4180|s2cid=15221098 }}</ref>
|-
|[[PSR J1614−2230]]
|13 ± 2
|
|<ref>{{Cite journal |last1=Demorest |first1=Paul |last2=Pennucci |first2=Tim |last3=Ransom |first3=Scott |last4=Roberts |first4=Mallory |last5=Hessels |first5=Jason |date=October 2010 |title=Shapiro delay measurement of a two solar mass neutron star |journal=Nature |volume=467 |issue=7319 |pages=1081–1083 |doi=10.1038/nature09466 |pmid=20981094 |arxiv=1010.5788 |issn=0028-0836}}</ref>
|-
|[[GX 13+1]]
|≲14.50
|[[Neutron star]]
|
|<ref name=Giridharan2024>{{Cite journal|last1=Giridharan|first1=L.|last2=Thomas|first2=Neal Titus|last3=Gudennavar|first3=S. B.|last4=Bubbly|first4=S. G.|date=21 December 2023|title=Spectral and temporal features of GX 13+1 as revealed by AstroSat|journal=Monthly Notices of the Royal Astronomical Society|volume=527|issue=4|pages=11855–11865|url=https://academic.oup.com/mnras/article/527/4/11855/7491082|doi=10.1093/mnras/stad3941|issn=0035-8711|doi-access=free}}</ref>
|-
|[[PSR J1748-2446ad]]
|<16
|[[Pulsar]]
|Fastest-spinning pulsar known.
|<ref>{{cite web|url=https://www.pinterest.com/pin/116952921557434940/?lp=true|title=PSR J1748-2446ad is the fastest-spinning pulsar known, at 716 Hz, or 716 times a second. This pulsar was discovered by Jason W. T. Hessels... {{!}} Astro Sci {{!}} Pinterest|website=Pinterest|access-date=2018-09-16}}</ref>
|-
|[[RX J1856.5−3754]]
|19
|[[Neutron star]]
|Closest neutron star discovered to date.
|<ref>{{Cite journal |last1=Ho |first1=Wynn C. G. |last2=Kaplan |first2=David L. |last3=Chang |first3=Philip |last4=van Adelsberg |first4=Matthew |last5=Potekhin |first5=Alexander Y. |date=2007-03-01 |title=Magnetic Hydrogen Atmosphere Models and the Neutron Star RX J1856.5-3754 |journal=Monthly Notices of the Royal Astronomical Society |volume=375 |issue=3 |pages=821–830 |doi=10.1111/j.1365-2966.2006.11376.x |arxiv=astro-ph/0612145 |bibcode=2007MNRAS.375..821H |issn=0035-8711|doi-access=free }}</ref>
|-
|[[PSR B1620-26]]
|24
|[[Pulsar]]
|An exoplanet orbits PSR B1620-26 and its white dwarf companion (see below) in a [[Circumbinary planet|circumbinary]] orbit.
|
|-
|[[HD 49798]]
|1,600
| rowspan="42" |[[White dwarf]]
|One of the smallest white dwarf stars known.
|<ref name=":0">{{Cite journal|date=April 10, 2021|title=New X-ray observations of the hot subdwarf binary HD 49798/RX J0648.0–4418|url=https://academic.oup.com/mnras/article-abstract/504/1/920/6219849|journal=Monthly Notices of the Royal Astronomical Society|pages=920–925|doi=10.1093/mnras/stab1004|arxiv=2104.03867|last1=Mereghetti |first1=S. |last2=Pintore |first2=F. |last3=Rauch |first3=T. |last4=La Palombara |first4=N. |last5=Esposito |first5=P. |last6=Geier |first6=S. |last7=Pelisoli |first7=I. |last8=Rigoselli |first8=M. |last9=Schaffenroth |first9=V. |last10=Tiengo |first10=A. |volume=504 |doi-access=free }}</ref>
|-
|[[ZTF J1901+1458]]
|1,809
|Currently the most massive white dwarf known.
|<ref>{{Cite journal|last1=Caiazzo|first1=Ilaria|last2=Burdge|first2=Kevin|last3=Fuller|first3=James|last4=Heyl|first4=Jeremy|last5=Kulkarni|first5=Shri|last6=Prince|first6=Thomas|last7=Richer|first7=Harvey|last8=Schwab|first8=Josiah|last9=Andreoni|first9=Igor|date=2020-11-09|title=A moon-sized, highly magnetised and rapidly rotating white dwarf may be headed toward collapse|url=http://dx.doi.org/10.21203/rs.3.rs-99143/v1|access-date=2020-11-29|doi=10.21203/rs.3.rs-99143/v1 |s2cid=234924493 }}</ref>
|-
|[[Janus (star)|Janus]]
|3,400
|A white dwarf with a side of hydrogen and another side of helium.
|<ref>{{Cite journal |last1=Caiazzo |first1=Ilaria |last2=Burdge |first2=Kevin B. |last3=Tremblay |first3=Pier-Emmanuel |last4=Fuller |first4=James |last5=Ferrario |first5=Lilia |last6=Gänsicke |first6=Boris T. |last7=Hermes |first7=J. J. |last8=Heyl |first8=Jeremy |last9=Kawka |first9=Adela |last10=Kulkarni |first10=S. R. |last11=Marsh |first11=Thomas R. |last12=Mróz |first12=Przemek |last13=Prince |first13=Thomas A. |last14=Richer |first14=Harvey B. |last15=Rodriguez |first15=Antonio C. |date=2023-08-01 |title=A rotating white dwarf shows different compositions on its opposite faces |url=https://ui.adsabs.harvard.edu/abs/2023Natur.620...61C |journal=Nature |volume=620 |issue=7972 |pages=61–66 |doi=10.1038/s41586-023-06171-9 |pmid=37468630 |issn=0028-0836|arxiv=2308.07430 |bibcode=2023Natur.620...61C }}</ref>
|-
|[[Wolf 1130]] B
|3,480
|
|<ref>{{Citation |last1=Mace |first1=Gregory N. |title=Wolf 1130: A Nearby Triple System Containing a Cool, Ultramassive White Dwarf |date=2018-02-13 |doi=10.3847/1538-4357/aaa8dd |last2=Mann |first2=Andrew W. |last3=Skiff |first3=Brian A. |last4=Sneden |first4=Christopher |last5=Kirkpatrick |first5=Davy |last6=Schneider |first6=Adam C. |last7=Kidder |first7=Benjamin |last8=Gosnell |first8=Natalie M. |last9=Kim |first9=Hwihyun|journal=The Astrophysical Journal |volume=854 |issue=2 |page=145 |doi-access=free |arxiv=1802.04803 |bibcode=2018ApJ...854..145M }}</ref>
|-
|[[IK Pegasi]] B
|4,174
|The nearest [[supernova]] candidate. ([[Type Ia supernova|Type Ia]])
|<ref>{{Cite journal |last1=Barstow |first1=M. A. |last2=Holberg |first2=J. B. |last3=Koester |first3=D. |date=1994-10-01 |title=Extreme-ultraviolet spectrophotometry of HD 15638 and HR 8210 (IK Peg). |journal=Monthly Notices of the Royal Astronomical Society |volume=270 |issue=3 |pages=516–522 |doi=10.1093/mnras/270.3.516 |doi-access=free |bibcode=1994MNRAS.270..516B |issn=0035-8711}}</ref>
|-
|[[Sirius B]]
| 5,466
| Historically first detected white dwarf star
| <ref>{{cite journal |jstor= 40678784|title= Temperature, radius, and rotational velocity of Sirius B |author1=Peter Thejll |author2=Harry L. Shipman |journal= Publications of the Astronomical Society of the Pacific |volume= 98 |number= 608 |publication-date= October 1986 |pages= 922–926 |issn= 0004-6280 |doi= 10.1086/131845 |bibcode= 1986PASP...98..922T |year= 1986 |doi-access= free }}</ref>
|-
|[[LB 1497]]
|5,494.5
|
|<ref>{{cite journal|last1=Wegner|first1=Gary|last2=Reid|first2=I. N.|last3=McMahan|first3=Robert K. Jr. |date=July 1991|title=Gravitational redshift for the Pleiad white dwarf LB 1497|journal=The Astrophysical Journal|volume=376|pages=186|doi=10.1086/170266|issn=0004-637X|bibcode=1991ApJ...376..186W}}</ref>
|-
|[[40 Eridani]] B
|5,547.5
|
|
|-
|[[U Geminorum]] white dwarf
|5,565
|
|<ref name=":13">{{Cite journal |last1=Naylor |first1=T. |last2=Allan |first2=A. |last3=Long |first3=K. S. |date=August 2005 |title=The masses, radii and luminosities of the components of U Geminorum |journal=Monthly Notices of the Royal Astronomical Society |volume=361 |issue=3 |pages=1091–1101 |doi=10.1111/j.1365-2966.2005.09262.x|doi-access=free |arxiv=astro-ph/0506351 |bibcode=2005MNRAS.361.1091N |hdl=10871/20279 |hdl-access=free }}</ref>
|-
|[[BPM 37093]]
|5,750
|
|<ref>{{Cite web |title=V* V886 Cen |url=https://www.montrealwhitedwarfdatabase.org/WDs/V*%20V886%20Cen/V*%20V886%20Cen.html |access-date=2024-05-30 |website=Montreal White Dwarf Database}}</ref>{{efn | Applying the [[Stefan–Boltzmann law]] with a nominal [[sun|solar]] [[effective temperature]] of 5,772&nbsp;[[Kelvin|K]]:
:<math>\sqrt{\biggl(\frac{5,772}{10,780}\biggr)^4 \cdot 10^{-3.08}} = 0.008268\ R_\odot</math>.}}
|-
|[[GRW +70 8247|Gliese 742]] ''(GRW +70 8247)''
|5,950
|
|<ref>{{Cite web |title=GJ 742 |url=https://www.montrealwhitedwarfdatabase.org/WDs/GJ%20742/GJ%20742.html |access-date=2024-05-30 |website=Montreal White Dwarf Database}}</ref>{{efn | Applying the [[Stefan–Boltzmann law]] with a nominal [[sun|solar]] [[effective temperature]] of 5,772&nbsp;[[Kelvin|K]]:
:<math>\sqrt{\biggl(\frac{5,772}{11,880}\biggr)^4 \cdot 10^{-2.88}} = 0.00857\ R_\odot</math>.}}
|-
|[[WD 2359−434|Gliese 915]] ''(WD 2359-434)''
|6,748.3
|
|<ref name=":18">{{Cite journal |last1=Subasavage |first1=John P. |last2=Jao |first2=Wei-Chun |last3=Henry |first3=Todd J. |last4=Bergeron |first4=P. |last5=Dufour |first5=P. |last6=Ianna |first6=Philip A. |last7=Costa |first7=Edgardo |last8=Mendez |first8=Rene A. |date=2009-06-01 |title=The Solar Neighborhood. XXI. Parallax Results from the CTIOPI 0.9m Program: 20 New Members of the 25 Parsec White Dwarf Sample |journal=The Astronomical Journal |volume=137 |issue=6 |pages=4547–4560 |doi=10.1088/0004-6256/137/6/4547 |arxiv=0902.0627 |bibcode=2009AJ....137.4547S |s2cid=14696597 |issn=0004-6256}}</ref>
|-
|[[AE Aquarii]] A
|6,950
|
|<ref name="Ishida">{{cite journal | url=http://xmm.esac.esa.int/external/xmm_science/x-ray-symposium/172852_mi_aeaquarii.pdf | display-authors=1 | last1=Itoh | first1=Kei | last2=Okada | first2=Shunsaku | last3=Ishida | first3=Manabu | last4=Kunieda | first4=Hideyo | title=Density diagnostics of the hot plasma in AE Aquarii with XMM-NEWTON | journal=The Astrophysical Journal | volume=639 | pages=397–404 | date=2005 | issue=1 | doi=10.1086/499152 | bibcode=2006ApJ...639..397I | arxiv=astro-ph/0412559 | s2cid=14578720 | access-date=2009-11-15 | archive-date=2011-07-19 | archive-url=https://web.archive.org/web/20110719102610/http://xmm.esac.esa.int/external/xmm_science/x-ray-symposium/172852_mi_aeaquarii.pdf | url-status=dead }}</ref>
|-
|[[AR Scorpii]]
|6,950
|
|<ref>{{Cite journal |last1=Singh |first1=K. K. |last2=Meintjes |first2=P. J. |last3=Yadav |first3=K. K. |date=2021-03-22 |title=Properties of white dwarf in the binary system AR Scorpii and its observed features |journal=Modern Physics Letters A |volume=36 |issue=13 |language=en |doi=10.1142/S0217732321500966|arxiv=2103.11602v1 |bibcode=2021MPLA...3650096S |s2cid=232307204 }}</ref>
|-
|[[G 29-38]]
|6,950
|
|<ref>{{Cite journal |last1=Reach |first1=William T. |last2=Lisse |first2=Carey |last3=von Hippel |first3=Ted |last4=Mullally |first4=Fergal |date=2009-03-01 |title=The Dust Cloud around the White Dwarf G 29-38. II. Spectrum from 5 to 40 μm and Mid-Infrared Photometric Variability |url=https://ui.adsabs.harvard.edu/abs/2009ApJ...693..697R |journal=The Astrophysical Journal |volume=693 |issue=1 |pages=697–712 |doi=10.1088/0004-637X/693/1/697 |arxiv=0810.3276 |bibcode=2009ApJ...693..697R |s2cid=12832891 |issn=0004-637X}}</ref>
|-
|[[LP 145-141]]
|6,950
|4th nearest white dwarf.<ref>{{Cite journal |last1=Sion |first1=Edward M. |last2=Holberg |first2=Jay B. |last3=Oswalt |first3=Terry D. |last4=McCook |first4=George P. |last5=Wasatonic |first5=Richard |date=2009-12-01 |title=The White Dwarfs within 20 Parsecs of the Sun: Kinematics and Statistics |journal=The Astronomical Journal |volume=138 |issue=6 |pages=1681–1689 |doi=10.1088/0004-6256/138/6/1681 |arxiv=0910.1288 |bibcode=2009AJ....138.1681S |issn=0004-6256|doi-access=free }}</ref>
|
|-
|[[PSR B1620-26|WD B1620−26]] <br />''(PSR B1620-26 B)''
|6,950
|An exoplanet orbits WD B1620−26 and its pulsar companion (see above) in a [[Circumbinary planet|circumbinary]] orbit.
|
|-
|[[Van Maanen's Star]] <br />''(Van Maanen 2)''
|6,950
|{{nowrap|3rd nearest white dwarf.}}
|<ref>{{Cite journal |last1=Kervella |first1=Pierre |last2=Arenou |first2=Frédéric |last3=Thévenin |first3=Frédéric |date=2022-01-01 |title=Stellar and substellar companions from Gaia EDR3 - Proper-motion anomaly and resolved common proper-motion pairs |url=https://www.aanda.org/articles/aa/abs/2022/01/aa42146-21/aa42146-21.html |journal=Astronomy & Astrophysics |language=en |volume=657 |pages=A7 |doi=10.1051/0004-6361/202142146 |arxiv=2109.10912 |bibcode=2022A&A...657A...7K |issn=0004-6361}}</ref>
|-
|[[WD 0810–353]]
|6,950
|
|<ref>{{cite journal | arxiv=2109.10912 | doi=10.1051/0004-6361/202142146 | title=Stellar and substellar companions from ''Gaia'' EDR3 | date=2022 | last1=Kervella | first1=Pierre | last2=Arenou | first2=Frédéric | last3=Thévenin | first3=Frédéric | journal=Astronomy & Astrophysics | volume=657 | pages=A7 | bibcode=2022A&A...657A...7K }}</ref>
|-
|[[YZ Leonis Minoris]] A
|6,950
|
|<ref>{{Cite journal |last1=Sengupta |first1=Sujan |last2=Taam |first2=Ronald E. |date=2011-09-02 |title=Theoretical Spectra of the Am Canum Venaticorum Binary System SDSS J0926+3624: Effects of Irradiation Onto the Donor Star |url=https://dx.doi.org/10.1088/0004-637X/739/1/34 |journal=The Astrophysical Journal |language=en |volume=739 |issue=1 |pages=34 |doi=10.1088/0004-637X/739/1/34 |arxiv=1107.1444 |bibcode=2011ApJ...739...34S |issn=0004-637X}}</ref>
|-
|[[QS Virginis]] A
|7,658
|
|<ref name=":17">{{Cite journal |last1=O'Donoghue |first1=D. |last2=Koen |first2=C. |last3=Kilkenny |first3=D. |last4=Stobie |first4=R. S. |last5=Koester |first5=D. |last6=Bessell |first6=M. S. |last7=Hambly |first7=N. |last8=MacGillivray |first8=H. |date=October 2003 |title=The DA+dMe eclipsing binary EC13471-1258: its cup runneth over...just |journal=Monthly Notices of the Royal Astronomical Society |volume=345 |issue=2 |pages=506–528 |doi=10.1046/j.1365-8711.2003.06973.x |doi-access=free |arxiv=astro-ph/0307144 |bibcode=2003MNRAS.345..506O |issn=0035-8711}}</ref>
|-
|[[Stein 2051]] B
|7,930
|
|<ref>{{Cite journal |last1=Sahu |first1=Kailash C. |last2=Anderson |first2=Jay |last3=Casertano |first3=Stefano |last4=Bond |first4=Howard E. |last5=Bergeron |first5=Pierre |last6=Nelan |first6=Edmund P. |last7=Pueyo |first7=Laurent |last8=Brown |first8=Thomas M. |last9=Bellini |first9=Andrea |last10=Levay |first10=Zoltan G. |last11=Sokol |first11=Joshua |last12=Dominik |first12=Martin |last13=Calamida |first13=Annalisa |last14=Kains |first14=Noé |last15=Livio |first15=Mario |date=2017-06-09 |title=Relativistic deflection of background starlight measures the mass of a nearby white dwarf star |journal=Science |volume=356 |issue=6342 |pages=1046–1050 |doi=10.1126/science.aal2879 |pmid=28592430 |arxiv=1706.02037 |bibcode=2017Sci...356.1046S |issn=0036-8075|doi-access=free }}</ref>
|-
|[[Ross 548]] ''(ZZ Ceti)''
|8,209
|
|<ref name=":6" />
|-
|[[CR Boötis]] A
|8,350
|
|<ref name=Boneva_et_al_2021>{{citation | postscript=.
 | title=Mid-Cycle Observations of CR Boo and Estimation of the System's Parameters
 | display-authors=1 | last1=Boneva | first1=Daniela
 | last2=Boeva | first2=Svetlana | last3=Nikolov | first3=Yanko
 | last4=Cvetković | first4=Zorica | last5=Zamanov | first5=Radoslav
 | journal=Data
 | date=August 2021 | volume=5
 | issue=4
 | page=113
 | doi=10.3390/data5040113
 | arxiv=2108.10421 | doi-access=free
 }}</ref>
|-
|[[DQ Herculis]] A
|8,420
|A slow, bright [[nova]] that reached peak brightness on {{Nowrap|22 December 1934}} with an [[apparent magnitude]] of 1.5.<ref>{{Cite journal |date=1935-02-01 |title=Notes from Pacific Coast Observatories |url=https://ui.adsabs.harvard.edu/abs/1935PASP...47...47. |journal=Publications of the Astronomical Society of the Pacific |volume=47 |issue=275 |pages=47 |doi=10.1086/124534 |bibcode=1935PASP...47...47. |issn=0004-6280}}</ref>
|<ref>{{Cite journal |last1=Saito |first1=R. K. |last2=Baptista |first2=R. |last3=Horne |first3=K. |last4=Martell |first4=P. |date=2010-05-07 |title=Spectral Mapping of the Intermediate Polar Dq Herculis |url=https://doi.org/10.1088/0004-6256/139/6/2542 |journal=The Astronomical Journal |volume=139 |issue=6 |pages=2542–2556 |doi=10.1088/0004-6256/139/6/2542 |arxiv=1005.1612 |bibcode=2010AJ....139.2542S |s2cid=118447217 |issn=0004-6256}}</ref>
|-
|[[Procyon]] B
|8,595
|Second nearest white dwarf.
|<ref>{{Cite journal |last1=Provencal |first1=J. L. |last2=Shipman |first2=H. L. |last3=Koester |first3=Detlev |last4=Wesemael |first4=F. |last5=Bergeron |first5=P. |date=2002-03-20 |title=Procyon B: Outside the Iron Box |journal=The Astrophysical Journal |volume=568 |issue=1 |pages=324–334 |doi=10.1086/338769 |bibcode=2002ApJ...568..324P |issn=0004-637X|doi-access=free }}</ref>
|-
|[[GD 165]] A
|8,626.5
|
|<ref name=":6">{{Cite journal |last1=Giammichele |first1=N. |last2=Fontaine |first2=G. |last3=Brassard |first3=P. |last4=Charpinet |first4=S. |date=2016-03-01 |title=A New Analysis of the Two Classical ZZ Ceti White Dwarfs GD 165 and Ross 548. II. Seismic Modeling |journal=The Astrophysical Journal Supplement Series |volume=223 |issue=1 |pages=10 |doi=10.3847/0067-0049/223/1/10 |bibcode=2016ApJS..223...10G |s2cid=124354534 |issn=0067-0049 |doi-access=free }}</ref>
|-
|[[ESO 439-26]]
|8,775.5
|Faintest known white dwarf.<ref>{{cite journal|last1=Ruiz|first1=María Teresa|last2=Bergeron|first2=P.|last3=Leggett|first3=S. K.|last4=Anguita|first4=Claudio|date=1995-12-20|title=The Extremely Low Luminosity White Dwarf ESO 439−26|journal=The Astrophysical Journal|volume=455|issue=2|pages=L159|doi=10.1086/309845|issn=0004-637X|bibcode=1995ApJ...455L.159R|doi-access=free}}</ref>
|
|-
|[[Gliese 293]]
|8,900{{Efn|From surface gravity and mass|name=Gliese 293 radius}}
|
|<ref name=":18" />
|-
|[[Wolf 489]]
|9,044
|
|<ref>{{Cite journal |last1=Holberg |first1=J. B. |last2=Sion |first2=E. M. |last3=Oswalt |first3=T. |last4=McCook |first4=G. P. |last5=Foran |first5=S. |last6=Subasavage |first6=John P. |date=2008-04-01 |title=A New Look at the Local White Dwarf Population |url=https://ui.adsabs.harvard.edu/abs/2008AJ....135.1225H |journal=The Astronomical Journal |volume=135 |issue=4 |pages=1225–1238 |doi=10.1088/0004-6256/135/4/1225 |bibcode=2008AJ....135.1225H |s2cid=122855486 |issn=0004-6256}}</ref>
|-
|[[HD 44120]] C
|9,044
|
|<ref>{{Cite journal |last1=Bédard |first1=Antoine |last2=Bergeron |first2=Pierre |last3=Fontaine |first3=Gilles |date=2017-10-09 |title=Measurements of Physical Parameters of White Dwarfs: A Test of the Mass-Radius Relation |journal=The Astrophysical Journal |volume=848 |issue=1 |pages=11 |doi=10.3847/1538-4357/aa8bb6 |arxiv=1709.02324 |bibcode=2017ApJ...848...11B |issn=1538-4357|doi-access=free }}</ref>
|-
|[[WD 1856+534]]
|9,113.67
|
|<ref>{{Cite journal |last1=Vanderburg |first1=Andrew |last2=Rappaport |first2=Saul A. |last3=Xu |first3=Siyi |last4=Crossfield |first4=Ian |last5=Becker |first5=Juliette C. |last6=Gary |first6=Bruce |last7=Murgas |first7=Felipe |last8=Blouin |first8=Simon |last9=Kaye |first9=Thomas G. |last10=Palle |first10=Enric |last11=Melis |first11=Carl |last12=Morris |first12=Brett |last13=Kreidberg |first13=Laura |last14=Gorjian |first14=Varoujan |last15=Morley |first15=Caroline V. |date=2020-09-17 |title=A Giant Planet Candidate Transiting a White Dwarf |journal=Nature |volume=585 |issue=7825 |pages=363–367 |doi=10.1038/s41586-020-2713-y |pmid=32939071 |arxiv=2009.07282 |bibcode=2020Natur.585..363V |hdl=1721.1/129733 |s2cid=221738865 |issn=0028-0836}}</ref>
|-
|[[Epsilon Reticuli]] B
|9,185
|
|<ref>{{Cite journal |last1=Farihi |first1=J. |last2=Burleigh |first2=M. R. |last3=Holberg |first3=J. B. |last4=Casewell |first4=S. L. |last5=Barstow |first5=M. A. |date=2011-11-01 |title=Evolutionary Constraints on the Planet-Hosting Subgiant Epsilon Reticulum from its White Dwarf Companion |journal=Monthly Notices of the Royal Astronomical Society |volume=417 |issue=3 |pages=1735–1741 |doi=10.1111/j.1365-2966.2011.19354.x|arxiv=1104.0925 |doi-access=free }}</ref>
|-
|[[KOI-256]] B
|9,350
|
|<ref>{{Cite journal |last1=Muirhead |first1=Philip S. |last2=Vanderburg |first2=Andrew |last3=Shporer |first3=Avi |last4=Becker |first4=Juliette |last5=Swift |first5=Jonathan J. |last6=Lloyd |first6=James P. |last7=Fuller |first7=Jim |last8=Zhao |first8=Ming |last9=Hinkley |first9=Sasha |last10=Pineda |first10=J. Sebastian |last11=Bottom |first11=Michael |last12=Howard |first12=Andrew W. |last13=von Braun |first13=Kaspar |last14=Boyajian |first14=Tabetha S. |last15=Law |first15=Nicholas |date=2013-04-02 |title=Characterizing the Cool KOIs. V. KOI-256: A Mutually Eclipsing Post-Common Envelope Binary |journal=The Astrophysical Journal |volume=767 |issue=2 |pages=111 |doi=10.1088/0004-637X/767/2/111 |arxiv=1304.1165 |bibcode=2013ApJ...767..111M |issn=0004-637X}}</ref>
|-
|[[RR Caeli]] white dwarf
|10,908.5
|
|<ref>{{Cite journal |last1=Parsons |first1=S. G. |last2=Gänsicke |first2=B. T. |last3=Marsh |first3=T. R. |last4=Ashley |first4=R. P. |last5=Bours |first5=M. C. P. |last6=Breedt |first6=E. |last7=Burleigh |first7=M. R. |last8=Copperwheat |first8=C. M. |last9=Dhillon |first9=V. S. |last10=Green |first10=M. |last11=Hardy |first11=L. K. |last12=Hermes |first12=J. J. |last13=Irawati |first13=P. |last14=Kerry |first14=P. |last15=Littlefair |first15=S. P. |date=October 2017 |title=Testing the white dwarf mass-radius relationship with eclipsing binaries |journal=Monthly Notices of the Royal Astronomical Society |volume=470 |issue=4 |pages=4473–4492 |doi=10.1093/mnras/stx1522 |doi-access=free |arxiv=1706.05016 |issn=0035-8711|hdl=2117/113341 |hdl-access=free }}</ref>
|-
|[[WD 1145+017]]
|13,926.84
|Host star of one of the [[List of smallest exoplanets|smallest exoplanets]].
|<ref name="discovery">{{cite journal |title= A disintegrating minor planet transiting a white dwarf |author1=Andrew Vanderburg |author2=John Asher Johnson |author3=Saul Rappaport |author4=Allyson Bieryla |author5=Jonathan Irwin |author6=John Arban Lewis |author7=David Kipping |author8=Warren R. Brown |author9=Patrick Dufour |author10=David R. Ciardi |author11=Ruth Angus |author12=Laura Schaefer |author13=David W. Latham |author14=David Charbonneau |author15=Charles Beichman |author16=Jason Eastman |author17=Nate McCrady |author18=Robert A. Wittenmyer |author19=Jason T. Wright |arxiv= 1510.06387 |bibcode= 2015Natur.526..546V |doi= 10.1038/nature15527 |url= https://www.cfa.harvard.edu/~avanderb/wd1145_017.pdf |date= 11 June 2015 |publication-date= 22 October 2015 |journal= Nature |volume= 526 |issue=7574 |pages= 546–549 |pmid=26490620|s2cid=4451207 }}</ref>
|-
|[[NN Serpentis]] white dwarf
|14,679.5
|
|<ref>{{Cite journal |last1=Parsons |first1=S. G. |last2=Marsh |first2=T. R. |last3=Copperwheat |first3=C. M. |last4=Dhillon |first4=V. S. |last5=Littlefair |first5=S. P. |last6=Gansicke |first6=B. T. |last7=Hickman |first7=R. |date=March 2010 |title=Precise mass and radius values for the white dwarf and low mass M dwarf in the pre-cataclysmic binary NN Serpentis |journal=Monthly Notices of the Royal Astronomical Society |volume=402 |issue=4 |pages=2591–2608 |doi=10.1111/j.1365-2966.2009.16072.x|arxiv=0909.4307 |bibcode=2010MNRAS.402.2591P |doi-access=free }}</ref>
|-
|[[Beta Crateris]] B
|18,800
|
|<ref>{{Cite journal |last1=Holberg |first1=J. B. |last2=Oswalt |first2=T. D. |last3=Sion |first3=E. M. |last4=Barstow |first4=M. A. |last5=Burleigh |first5=M. R. |date=2013-11-01 |title=Where are all the Sirius-Like Binary Systems? |journal=Monthly Notices of the Royal Astronomical Society |volume=435 |issue=3 |pages=2077–2091 |doi=10.1093/mnras/stt1433 |doi-access=free |arxiv=1307.8047 |bibcode=2013MNRAS.435.2077H |issn=1365-2966}}</ref>
|-
|[[Feige 55]]
|19,450
|
|<ref>{{Cite web |title=Feige 55 |url=https://www.montrealwhitedwarfdatabase.org/WDs/Feige%2055/Feige%2055.html |access-date=2024-05-30 |website=Montreal White Dwarf Database}}</ref>{{efn | Applying the [[Stefan–Boltzmann law]] with a nominal [[sun|solar]] [[effective temperature]] of 5,772&nbsp;[[Kelvin|K]]:
:<math>\sqrt{\biggl(\frac{5,772}{58,280}\biggr)^4 \cdot 10^{0.91}} = 0.02796\ R_\odot</math>.}}
|-
|Central star of the [[Dumbbell Nebula]]
|38,265
|
|<ref>{{Cite journal |last1=Benedict |first1=G. Fritz |last2=McArthur |first2=B. E. |last3=Fredrick |first3=L. W. |last4=Harrison |first4=T. E. |last5=Skrutskie |first5=M. F. |last6=Slesnick |first6=C. L. |last7=Rhee |first7=J. |last8=Patterson |first8=R. J. |last9=Nelan |first9=E. |last10=Jefferys |first10=W. H. |last11=van Altena |first11=W. |last12=Montemayor |first12=T. |last13=Shelus |first13=P. J. |last14=Franz |first14=O. G. |last15=Wasserman |first15=L. H. |date=November 2003 |title=Astrometry with Hubble Space Telescope: A Parallax of the Central Star of the Planetary Nebula NGC 6853 |journal=The Astronomical Journal |volume=126 |issue=5 |pages=2549–2556 |doi=10.1086/378603 |arxiv=astro-ph/0307449 |bibcode=2003AJ....126.2549B |issn=0004-6256|doi-access=free }}</ref>
|-
|[[KPD 0005+5106]]
|41,045
|
|<ref>{{Cite journal |last1=Chu |first1=You-Hua |last2=Toalá |first2=Jesús A. |last3=Guerrero |first3=Martín A. |last4=Bauer |first4=Florian F. |last5=Bilikova |first5=Jana |last6=Gruendl |first6=Robert A. |date=2021-04-01 |title=Hard X-Ray Emission Associated with White Dwarfs. IV. Signs of Accretion from Substellar Companions |journal=The Astrophysical Journal |volume=910 |issue=2 |pages=119 |doi=10.3847/1538-4357/abe5a5 |doi-access=free |arxiv=2102.05035 |bibcode=2021ApJ...910..119C |issn=0004-637X}}</ref>
|-
|[[PSR J0348+0432|PSR J0348+0432 B]]
|45,268
|A white dwarf that orbits its pulsar companion (see above)
|<ref name="ReferenceA" />
|-
|[[TMTS J052610.43+593445.1]]
|45,916
|[[Subdwarf B star|B-type subdwarf]]
|Smallest known non-degenerate star.
|<ref>https://www.researchgate.net/publication/375515291_A_seven-Earth-radius_helium-burning_star_inside_a_205-min_verification_binary_of_GWs {{Bare URL inline|date=August 2024}}</ref>
|-
|[[WISEA 1810−1010]]
|46,840
| rowspan="2" |[[Brown dwarf]]
|Smallest known brown dwarf.
|<ref name=":11">{{Cite journal |last1=Lodieu |first1=N. |last2=Osorio |first2=M. R. Zapatero |last3=Martín |first3=E. L. |last4=López |first4=R. Rebolo |last5=Gauza |first5=B. |date=2022-07-01 |title=Physical properties and trigonometric distance of the peculiar dwarf WISE J181005.5−101002.3 |url=https://www.aanda.org/articles/aa/abs/2022/07/aa43516-22/aa43516-22.html |journal=Astronomy & Astrophysics |language=en |volume=663 |pages=A84 |doi=10.1051/0004-6361/202243516 |arxiv=2206.13097 |bibcode=2022A&A...663A..84L |issn=0004-6361|doi-access=free }}</ref>
|-
|{{ill|EPIC 201702477|fr}}
|54,120
|
|<ref name=":4">{{Cite journal |last1=Bayliss |first1=D. |last2=Hojjatpanah |first2=S. |last3=Santerne |first3=A. |last4=Dragomir |first4=D. |last5=Zhou |first5=G. |last6=Shporer |first6=A. |last7=Colón |first7=K. D. |last8=Almenara |first8=J. |last9=Armstrong |first9=D. J. |last10=Barrado |first10=D. |last11=Barros |first11=S. C. C. |last12=Bento |first12=J. |last13=Boisse |first13=I. |last14=Bouchy |first14=F. |last15=Brown |first15=D. J. A. |date=2017-01-01 |title=EPIC 201702477b: A Transiting Brown Dwarf from K2 in a 41 day Orbit |journal=The Astronomical Journal |volume=153 |issue=1 |pages=15 |doi=10.3847/1538-3881/153/1/15 |arxiv=1606.04047 |bibcode=2017AJ....153...15B |hdl=1721.1/109493 |s2cid=31951035 |issn=0004-6256 |doi-access=free }}</ref>
|-
|[[BE Ursae Majoris]] A
|54,250
|[[O-type subdwarf]]
|
|<ref>{{Cite journal |last1=Ferguson |first1=Donald H. |last2=Liebert |first2=James |last3=Haas |first3=Stefan |last4=Napiwotzki |first4=Ralf |last5=James |first5=Thomas A. |date=1999-06-01 |title=Masses and Other Parameters of the Post-Common Envelope Binary BE Ursae Majoris |journal=The Astrophysical Journal |volume=518 |issue=2 |pages=866–872 |doi=10.1086/307289 |bibcode=1999ApJ...518..866F |issn=0004-637X|hdl=2299/1230 |hdl-access=free }}</ref>
|-
|[[LP 40-365]]
|54,250
|[[White dwarf]]
|A white dwarf that might have formed in a [[Type Ia supernova#Type Iax|type Iax supernova]]. Range of values of 40,350 to 82,095 km
|<ref>{{Cite journal |last1=Vennes |first1=S. |last2=Nemeth |first2=P. |last3=Kawka |first3=A. |last4=Thorstensen |first4=J. R. |last5=Khalack |first5=V. |last6=Ferrario |first6=L. |last7=Alper |first7=E. H. |date=2017-08-01 |title=An unusual white dwarf star may be a surviving remnant of a subluminous Type Ia supernova |bibcode=2017Sci...357..680V |journal=Science |volume=357 |issue=6352 |pages=680–683 |doi=10.1126/science.aam8378 |pmid=28818942 |arxiv=1708.05568 |issn=0036-8075}}</ref>

|-
|[[Epsilon Indi]] Ba
|55,656
| rowspan="8" |[[Brown dwarf]]
|
|<ref name=":5">{{Cite journal |last1=King |first1=Robert R. |last2=McCaughrean |first2=Mark J. |last3=Homeier |first3=Derek |last4=Allard |first4=France |last5=Scholz |first5=Ralf-Dieter |last6=Lodieu |first6=Nicolas |date=February 2010 |title=Epsilon Indi Ba, Bb: a detailed study of the nearest known brown dwarfs |journal=Astronomy and Astrophysics |volume=510 |pages=A99 |doi=10.1051/0004-6361/200912981 |arxiv=0911.3143 |s2cid=53550866 |issn=0004-6361}}</ref>
|-
|[[LHS 6343]] C
|55,978
|
|<ref name=":9">{{Cite journal |last1=Montet |first1=Benjamin T. |last2=Johnson |first2=John Asher |last3=Muirhead |first3=Philip S. |last4=Villar |first4=Ashley |author-link4=V. Ashley Villar |last5=Vassallo |first5=Corinne |last6=Baranec |first6=Christoph |last7=Law |first7=Nicholas M. |last8=Riddle |first8=Reed |last9=Marcy |first9=Geoffrey W. |last10=Howard |first10=Andrew W. |last11=Isaacson |first11=Howard |date=2015-02-20 |title=Characterizing the Cool KOIs. VII. Refined Physical Properties of the Transiting Brown Dwarf LHS 6343 C |journal=The Astrophysical Journal |volume=800 |issue=2 |pages=134 |arxiv=1411.4047 |bibcode=2015ApJ...800..134M |doi=10.1088/0004-637X/800/2/134 |issn=1538-4357 |s2cid=555496}}</ref>
|-
|[[Epsilon Indi]] Bb
|57,050
|
|<ref name=":5" />
|-
|[[54 Piscium]] B
|57,050
|
|<ref>{{Cite journal |last1=Luhman |first1=K. L. |last2=Patten |first2=B. M. |last3=Marengo |first3=M. |last4=Schuster |first4=M. T. |last5=Hora |first5=J. L. |last6=Ellis |first6=R. G. |last7=Stauffer |first7=J. R. |last8=Sonnett |first8=S. M. |last9=Winston |first9=E. |last10=Gutermuth |first10=R. A. |last11=Megeath |first11=S. T. |last12=Backman |first12=D. E. |last13=Henry |first13=T. J. |last14=Werner |first14=M. W. |last15=Fazio |first15=G. G. |date=January 2007 |title=Discovery of Two T Dwarf Companions with the Spitzer Space Telescope |journal=The Astrophysical Journal |volume=654 |issue=1 |pages=570–579 |doi=10.1086/509073 |arxiv=astro-ph/0609464 |bibcode=2007ApJ...654..570L |s2cid=11576708 |issn=0004-637X}}</ref>
|-
|[[2MASS J11263991−5003550|2MASS J1126−5003]]
|57,193.5
|
|<ref>{{Cite journal |last1=Vos |first1=Johanna M. |last2=Allers |first2=Katelyn N. |last3=Biller |first3=Beth A. |date=2017-06-15 |title=The Viewing Geometry of Brown Dwarfs Influences Their Observed Colors and Variability Amplitudes |journal=The Astrophysical Journal |language=en |volume=842 |issue=2 |pages=78 |doi=10.3847/1538-4357/aa73cf |arxiv=1705.06045 |bibcode=2017ApJ...842...78V |issn=1538-4357|doi-access=free }}</ref>
|-
|[[UGPS J0521+3640]]
|57,193.5
|
|
|-
|[[Wolf 1130]] C
|58,625
|
|<ref>{{Cite journal |last1=Zhang |first1=Zhoujian |last2=Liu |first2=Michael C. |last3=Best |first3=William M. J. |last4=Dupuy |first4=Trent J. |last5=Siverd |first5=Robert J. |date=2021-04-01 |title=The Hawaii Infrared Parallax Program. V. New T-dwarf Members and Candidate Members of Nearby Young Moving Groups |journal=The Astrophysical Journal |volume=911 |issue=1 |pages=7 |doi=10.3847/1538-4357/abe3fa |doi-access=free |arxiv=2102.05045 |bibcode=2021ApJ...911....7Z |issn=0004-637X}}</ref>
|-
|[[Gliese 570]] D
|59,350 to 66,090
|
|<ref name=saumon>{{Cite journal |last1=Saumon |first1=D. |last2=Marley |first2=M. S. |last3=Cushing |first3=M. C. |last4=Leggett |first4=S. K. |last5=Roellig |first5=T. L. |last6=Lodders |first6=K. |last7=Freedman |first7=R. S. |date=2006-08-10 |title=Ammonia as a tracer of chemical equilibrium in the T7.5 dwarf Gliese 570D |arxiv=astro-ph/0605563 |journal=The Astrophysical Journal |volume=647 |issue=1 |pages=552–557 |doi=10.1086/505419 |bibcode=2006ApJ...647..552S |issn=0004-637X}}</ref>
|-
||[[EBLM J0555-57Ab]]|| 60,000
|[[Red dwarf]]|| This red dwarf has a size comparable to that of the planet [[Saturn]]. As of 2019, it is the second lightest hydrogen-fusing star known, marginally heavier (0.0777-0.0852{{Solar mass}}) than the [[2MASS J0523-1403]]. Although its mass is comparable to that of TRAPPIST-1, its radius is 1/3 smaller. ||<ref name="cnet-2017-07-11">{{cite news |url= https://www.cnet.com/news/smallest-star-eblm-j0555-57ab-space-alien-life-cambridge-trappist-1/ |title= Saturn-sized star is the smallest ever discovered |author= Eric Mack |date= 11 July 2017 |publisher= cnet }}</ref><ref name="Cambridge-2017-smallest-ever-star-discovered-by-astronomers">{{cite web |url= https://www.cam.ac.uk/research/news/smallest-ever-star-discovered-by-astronomers |title= Smallest-ever star discovered by astronomers |date= 2017 |publisher= University of Cambridge }}</ref><ref name="2017arXiv170608781V">{{cite journal |title= The EBLM project; III. A Saturn-size low-mass star at the hydrogen-burning limit |author1= Alexander von Boetticher |author2=Amaury H.M.J. Triaud |author3=Didier Queloz |author4=Sam Gill |author5=Monika Lendl |author6=Laetitia Delrez |author7=David R. Anderson |author8=Andrew Collier Cameron |author9=Francesca Faedi |author10=Michaël Gillon |author11=Yilen Gómez Maqueo Chew |author12=Leslie Hebb |author13=Coel Hellier |author14=Emmanuël Jehin |author15=Pierre F.L. Maxted |author16=David V. Martin |author17=Francesco Pepe |author18=Don Pollacco |author19=Damien Ségransan|author20=Barry Smalley |author21=Stéphane Udry |author22=Richard West |arxiv= 1706.08781 |journal= Astronomy & Astrophysics |volume= 604 |pages= L6 |id= EBLM_III |date= 12 June 2017 |bibcode= 2017A&A...604L...6V |doi= 10.1051/0004-6361/201731107 |s2cid= 54610182 |display-authors=1}}</ref>
|-
|[[Luhman 16]] A
|60,768
|[[Brown dwarf]]
|Luhman 16 A and Luhman 16 B are the closest brown dwarf stars to Earth, and the third-nearest star system to the Solar System.
|{{efn|From : {{resize|75%|<math>R = \sqrt \frac{L}{ 4 \pi  \sigma {T_e}^4} </math>}}, where {{small|<math>L</math>}}  is the luminosity, {{small|<math>R</math>}}  is the radius, {{small|<math>T_e</math>}} is the effective surface temperature and {{small|<math>\sigma </math>}} is the [[Stefan–Boltzmann constant]].|name="RadiusCalculationFromLuminosityandTemperature"}}
|-
|| {{vanchor|SSSPM J0829-1309}} || 61,300
|[[Red dwarf]]|| An L2 dwarf that is fusing hydrogen. Similarly to 2MASS J0523-1403, SSSPM J0829-1309 is one of the least luminous and massive hydrogen-fusing stars, and is smaller than Jupiter.|| <ref name="2014AJ....147...94D">{{cite journal |author1=Sergio B. Dieterich9 |author2=Todd J. Henry |author3=Wei-Chun Jao |author4=Jennifer G. Winters |author5=Altonio D. Hosey |author6=Adric R. Riedel |author7=John P. Subasavage |title= The Solar Neighborhood XXXII. The Hydrogen Burning Limit |journal= The Astronomical Journal |volume= 147 |issue= 5 |id= 94 |page= 25 |date= May 2014 |doi= 10.1088/0004-6256/147/5/94 |bibcode= 2014AJ....147...94D |arxiv= 1312.1736 |s2cid=21036959 }}</ref><ref name="SSSPM J0829-1309">{{Cite web|url=https://inspirehep.net/literature/593466|title = SSSPM J0829-1309: A New nearby L dwarf detected in superCOSMOS Sky Surveys|website=inspirehep.net|access-date=November 21, 2021}}</ref>
|-
|[[WISE 1405+5534]]
|61,483
| rowspan="9" |[[Brown dwarf]]
|
|<ref name=":15">{{Cite journal |last1=Cushing |first1=Michael C. |last2=Kirkpatrick |first2=J. Davy |last3=Gelino |first3=Christopher R. |last4=Griffith |first4=Roger L. |last5=Skrutskie |first5=Michael F. |last6=Mainzer |first6=Amanda K.|author6-link=Amy Mainzer |last7=Marsh |first7=Kenneth A. |last8=Beichman |first8=Charles A. |last9=Burgasser |first9=Adam J. |last10=Prato |first10=Lisa A. |last11=Simcoe |first11=Robert A. |last12=Marley |first12=Mark S. |last13=Saumon |first13=D. |last14=Freedman |first14=Richard S. |last15=Eisenhardt |first15=Peter R. |date=2011-08-23 |title=The Discovery of Y Dwarfs Using Data from the Wide-field Infrared Survey Explorer (WISE) |journal=The Astrophysical Journal |volume=743 |issue=1 |page=50 |language=en |doi=10.1088/0004-637X/743/1/50|arxiv=1108.4678v1 |bibcode=2011ApJ...743...50C |s2cid=286881 }}</ref>
|-
|[[2MASS J09393548−2448279|2MASS 0939-2448]] B
|62,600
|
|<ref>{{Cite journal |last1=Leggett |first1=S. K. |last2=Cushing |first2=M. C. |last3=Saumon |first3=D. |last4=Marley |first4=M. S. |last5=Roellig |first5=T. L. |last6=Warren |first6=S. J. |last7=Burningham |first7=B. |last8=Jones |first8=H. R. A. |last9=Kirkpatrick |first9=J. D. |last10=Lodieu |first10=N. |last11=Lucas |first11=P. W. |last12=Mainzer |first12=A. K. |author12-link=Amy Mainzer|last13=Martin |first13=E. L. |last14=McCaughrean |first14=M. J. |last15=Pinfield |first15=D. J. |date=2009-04-20 |title=The Physical Properties of Four ~600K T Dwarfs |journal=The Astrophysical Journal |volume=695 |issue=2 |pages=1517–1526 |doi=10.1088/0004-637X/695/2/1517 |arxiv=0901.4093 |bibcode=2009ApJ...695.1517L |s2cid=44050900 |issn=0004-637X}}</ref>
|-
|[[WISE 0855−0714]]
|63,500
|Coolest known brown dwarf.
|<ref name="Luhman2024">{{cite journal |last1=Luhman |first1=K. L. |last2=Tremblin |first2=P. |last3=Alves de Oliveira |first3=C. |last4=Birkmann |first4=S. M. |last5=Baraffe |first5=I. |last6=Chabrier |first6=G. |last7=Manjavacas |first7=E. |last8=Parker |first8=R. J. |last9=Valenti |first9=J. |display-authors=2 |date=January 2024 |title=JWST/NIRSpec Observations of the Coldest Known Brown Dwarf |journal=[[The Astronomical Journal]] |volume=167 |issue=1 |pages=5 |arxiv=2311.17316 |bibcode=2024AJ....167....5L |doi=10.3847/1538-3881/ad0b72 |issn=0004-6256 |doi-access=free}}</ref>{{efn | Applying the [[Stefan–Boltzmann law]] with a nominal [[sun|solar]] [[effective temperature]] of 5,772&nbsp;[[Kelvin|K]]:
:<math>\sqrt{\biggl(\frac{5,772}{285}\biggr)^4 \cdot 10^{-7.305}} = 0.091298\ R_\odot</math>.}}
|- )
|[[2MASS J02431371−2453298|2MASS 0243−2453]]
|64,000
|
|<ref>{{Cite journal |last1=Burgasser |first1=Adam J. |last2=Burrows |first2=Adam |last3=Kirkpatrick |first3=J. Davy |date=2006-03-10 |title=A Method for Determining the Physical Properties of the Coldest Known Brown Dwarfs |journal=The Astrophysical Journal |volume=639 |issue=2 |pages=1095–1113 |doi=10.1086/499344 |arxiv=astro-ph/0510707 |bibcode=2006ApJ...639.1095B |issn=0004-637X|doi-access=free }}</ref>
|-
|[[W1906+40]]
|64,350
|In 2015 it was shown to have on its surface a storm the size of [[Jupiter]]'s [[Great Red Spot]]. 
|
|-
|[[2MASS J03480772−6022270|2MASS J0348−6022]]
|64,700
|
|<ref>{{Cite journal |last1=Tannock |first1=Megan E. |last2=Metchev |first2=Stanimir |last3=Heinze |first3=Aren |last4=Miles-Páez |first4=Paulo A. |last5=Gagné |first5=Jonathan |last6=Burgasser |first6=Adam |last7=Marley |first7=Mark S. |last8=Apai |first8=Dániel |last9=Suárez |first9=Genaro |last10=Plavchan |first10=Peter |date=2021-05-01 |title=Weather on Other Worlds. V. The Three Most Rapidly Rotating Ultra-Cool Dwarfs |journal=The Astronomical Journal |volume=161 |issue=5 |pages=224 |doi=10.3847/1538-3881/abeb67 |arxiv=2103.01990 |bibcode=2021AJ....161..224T |issn=0004-6256|doi-access=free }}</ref>
|-
|[[SDSS J1416+1348]] A
|65,772.5
|
|<ref>{{Cite journal |last1=Gonzales |first1=Eileen C. |last2=Burningham |first2=Ben |last3=Faherty |first3=Jacqueline K. |last4=Cleary |first4=Colleen |last5=Visscher |first5=Channon |last6=Marley |first6=Mark S. |last7=Lupu |first7=Roxana |last8=Freedman |first8=Richard |date=2020-12-01 |title=Retrieval of the d/sdL7+T7.5p Binary SDSS J1416+1348AB |journal=The Astrophysical Journal |volume=905 |issue=1 |pages=46 |doi=10.3847/1538-4357/abbee2 |arxiv=2010.01224 |bibcode=2020ApJ...905...46G |issn=0004-637X|doi-access=free }}</ref>
|-
|[[WISEPC J205628.90+145953.3]]
|66,487.5
|
|<ref name=":15" />
|-
|[[WISE 1738+2732]]
|66,487.5
|
|<ref name=":15" />
|-
|[[SCR 1845−6357]] A
|66,790
|[[Red dwarf]]
|
|
|-
|[[2MASS 0937+2931]]
|67,200
| rowspan="10" |[[Brown dwarf]]
|
|<ref name="Fundamental Parameters and Spectral" />
|-
|[[WISE 0359−5401]]
|67,200
|In June 2023, it became the first Y-dwarf with a [[spectral energy distribution]] measured by the [[James Webb Space Telescope]].
|<ref>{{Cite journal |last1=Beiler |first1=Samuel A. |last2=Cushing |first2=Michael C. |last3=Kirkpatrick |first3=J. Davy |last4=Schneider |first4=Adam C. |last5=Mukherjee |first5=Sagnick |last6=Marley |first6=Mark S. |date=2023-07-01 |title=The First JWST Spectral Energy Distribution of a Y Dwarf |journal=The Astrophysical Journal |volume=951 |issue=2 |pages=L48 |doi=10.3847/2041-8213/ace32c |doi-access=free |arxiv=2306.11807 |bibcode=2023ApJ...951L..48B |issn=0004-637X}}</ref><ref>{{Citation |last1=Leggett |first1=S. K. |title=The First Y Dwarf Data From JWST Show That Dynamic and Diabatic Processes Regulate Cold Brown Dwarf Atmospheres |date=2023-09-25 |arxiv=2309.14567 |last2=Tremblin |first2=Pascal|journal=The Astrophysical Journal |volume=959 |issue=2 |page=86 |doi=10.3847/1538-4357/acfdad |doi-access=free |bibcode=2023ApJ...959...86L }}</ref>
|-
|[[2MASS J22282889–4310262]]
|67,200
|
|<ref>{{Cite journal |last1=Vos |first1=Johanna M. |last2=Biller |first2=Beth A. |last3=Allers |first3=Katelyn N. |last4=Faherty |first4=Jacqueline K. |last5=Liu |first5=Michael C. |last6=Metchev |first6=Stanimir |last7=Eriksson |first7=Simon |last8=Manjavacas |first8=Elena |last9=Dupuy |first9=Trent J. |last10=Janson |first10=Markus |last11=Radigan-Hoffman |first11=Jacqueline |last12=Crossfield |first12=Ian |last13=Bonnefoy |first13=Mickael |last14=Best |first14=William M. J. |last15=Homeier |first15=Derek |date=2020-06-24 |title=Spitzer Variability Properties of Low-Gravity L Dwarfs |journal=The Astronomical Journal |volume=160 |issue=1 |pages=38 |doi=10.3847/1538-3881/ab9642 |arxiv=2005.12854 |bibcode=2020AJ....160...38V |issn=1538-3881 |doi-access=free }}</ref>
|-
|[[SDSS J1416+1348]] B
|67,200
|
|<ref>{{Cite journal |last1=Gonzales |first1=Eileen C. |last2=Burningham |first2=Ben |last3=Faherty |first3=Jacqueline K. |last4=Cleary |first4=Colleen |last5=Visscher |first5=Channon |last6=Marley |first6=Mark S. |last7=Lupu |first7=Roxana |last8=Freedman |first8=Richard |date=2020-12-01 |title=Retrieval of the d/sdL7+T7.5p Binary SDSS J1416+1348AB |journal=The Astrophysical Journal |volume=905 |issue=1 |pages=46 |doi=10.3847/1538-4357/abbee2 |arxiv=2010.01224 |bibcode=2020ApJ...905...46G |issn=0004-637X|doi-access=free }}</ref>
|-
|[[DENIS J081730.0−615520]]
|67,200
|
|<ref name="Fundamental Parameters and Spectral" />
|-
|[[WISE 2150–7520 AB|WISE 2150–7520]] B
|67,900
|
|<ref name=":20">{{Cite journal |last1=Faherty |first1=Jacqueline K. |last2=Goodman |first2=Sam |last3=Caselden |first3=Dan |last4=Colin |first4=Guillaume |last5=Kuchner |first5=Marc J. |last6=Meisner |first6=Aaron M. |last7=Gagné |first7=Jonathan |last8=Schneider |first8=Adam C. |last9=Gonzales |first9=Eileen C. |last10=Bardalez Gagliuffi |first10=Daniella C. |last11=Logsdon |first11=Sarah E. |last12=Allers |first12=Katelyn |last13=Burgasser |first13=Adam J. |date=2020-02-01 |title=WISE 2150-7520AB: A Very Low-mass, Wide Comoving Brown Dwarf System Discovered through the Citizen Science Project Backyard Worlds: Planet 9 |journal=The Astrophysical Journal |volume=889 |issue=2 |pages=176 |doi=10.3847/1538-4357/ab5303 |doi-access=free |arxiv=1911.04600 |bibcode=2020ApJ...889..176F |issn=0004-637X}}</ref>
|-
|[[Kelu-1]] B
|67,900
|
|
|-
|[[Kelu-1]] A
|68,180
|
|
|-
|[[LHS 1070]] C
|68,180
|Certainly a [[brown dwarf]] based on its mass<ref name="kohler">{{Cite journal |last1=Köhler |first1=R. |last2=Ratzka |first2=T. |last3=Leinert |first3=Ch |date=2012-05-01 |title=Orbits and masses in the multiple system LHS 1070 |url=https://www.aanda.org/articles/aa/abs/2012/05/aa18707-11/aa18707-11.html |journal=Astronomy & Astrophysics |language=en |volume=541 |pages=A29 |doi=10.1051/0004-6361/201118707 |arxiv=1203.6270 |bibcode=2012A&A...541A..29K |issn=0004-6361}}</ref>
|<ref name="lhs1070">{{Citation |last1=Rajpurohit |first1=A. S. |title=The very low mass multiple system LHS\,1070 -- a testbed for model atmospheres for the lower end of the main sequence |date=2012-08-02 |doi=10.1051/0004-6361/201219029 |last2=Reyle |first2=C. |last3=Schultheis |first3=M. |last4=Leinert |first4=Ch |last5=Allard |first5=F. |last6=Homeier |first6=D. |last7=Ratzka |first7=T. |last8=Abraham |first8=P. |last9=Moster |first9=B.|journal=Astronomy & Astrophysics |volume=545 |pages=A85 |arxiv=1208.0452 |bibcode=2012A&A...545A..85R }}</ref>
|-
|[[DENIS 0255−4700]]
|69,570
|
|<ref>{{Cite journal |last1=Stephens |first1=D. C. |last2=Leggett |first2=S. K. |last3=Cushing |first3=Michael C. |last4=Marley |first4=Mark S. |last5=Saumon |first5=D. |last6=Geballe |first6=T. R. |last7=Golimowski |first7=David A. |last8=Fan |first8=Xiaohui |last9=Noll |first9=K. S. |date=2009-09-01 |title=The 0.8-14.5 micron Spectra of Mid-L to Mid-T Dwarfs: Diagnostics of Effective Temperature, Grain Sedimentation, Gas Transport, and Surface Gravity |journal=The Astrophysical Journal |volume=702 |issue=1 |pages=154–170 |doi=10.1088/0004-637X/702/1/154 |issn=0004-637X|arxiv=0906.2991 |s2cid=118650774 }}</ref>
|-
|[[R Aquarii]] B
|69,570
|[[White dwarf]]
|Part of a [[symbiotic binary]] star system containing a [[red giant]] and a white dwarf.
|<ref>{{Cite journal |last1=Burgarella |first1=D. |last2=Vogel |first2=M. |last3=Paresce |first3=F. |date=1992-08-01 |title=R Aquarii : an attempt at a unified model. |url=https://ui.adsabs.harvard.edu/abs/1992A&A...262...83B |journal=Astronomy and Astrophysics |volume=262 |pages=83–96 |bibcode=1992A&A...262...83B |issn=0004-6361}}</ref>
|-
|[[HD 114762]] B
|69,570
|[[Red dwarf]]
|
|<ref>{{Cite journal |last1=Bowler |first1=Brendan P. |last2=Liu |first2=Michael C. |last3=Cushing |first3=Michael C. |date=2009-12-01 |title=The Benchmark Ultracool Subdwarf HD 114762B: A Test of Low-Metallicity Atmospheric and Evolutionary Models |journal=The Astrophysical Journal |volume=706 |issue=2 |pages=1114–1135 |doi=10.1088/0004-637X/706/2/1114 |arxiv=0910.1604 |bibcode=2009ApJ...706.1114B |issn=0004-637X|doi-access=free }}</ref>
|-
|[[2MASS J0407+1546]]
|69,570
|rowspan="2"|[[Brown dwarf]]
|
|<ref>{{Cite journal |last1=Tannock |first1=Megan E. |last2=Metchev |first2=Stanimir |last3=Heinze |first3=Aren |last4=Miles-Páez |first4=Paulo A. |last5=Gagné |first5=Jonathan |last6=Burgasser |first6=Adam |last7=Marley |first7=Mark S. |last8=Apai |first8=Dániel |last9=Suárez |first9=Genaro |last10=Plavchan |first10=Peter |date=2021-05-01 |title=Weather on Other Worlds. V. The Three Most Rapidly Rotating Ultra-Cool Dwarfs |journal=The Astronomical Journal |volume=161 |issue=5 |pages=224 |doi=10.3847/1538-3881/abeb67 |doi-access=free |arxiv=2103.01990 |bibcode=2021AJ....161..224T |issn=0004-6256}}</ref>
|-
|[[HN Pegasi]] B
|70,265
|
|<ref>{{Cite journal |last1=Leggett |first1=S. K. |last2=Saumon |first2=D. |last3=Albert |first3=Loic |last4=Cushing |first4=Michael C. |last5=Liu |first5=Michael C. |last6=Luhman |first6=K. L. |last7=Marley |first7=M. S. |last8=Kirkpatrick |first8=J. Davy |last9=Roellig |first9=Thomas L. |last10=Allers |first10=K. N. |date=August 2008 |title=HN Peg B: A Test of Models of the L to T Dwarf Transition |journal=The Astrophysical Journal |volume=682 |issue=2 |pages=1256–1263 |doi=10.1086/589146 |arxiv=0804.1386 |bibcode=2008ApJ...682.1256L |issn=0004-637X}}</ref>
|-
|| [[2MASS J0523-1403]] || 70,600
|[[Red dwarf]]||As in 2019, with mass {{val|67.54|12.79}}{{Jupiter mass}} (0.0523-0.0767{{Solar mass}}) is the lowest known mass hydrogen-burning star.  ||<ref name="SnT-2013-12-23">{{cite news |url= http://www.skyandtelescope.com/astronomy-news/new-cutoff-for-star-sizes/ |title= New Cutoff for Star Sizes |author= John Bochanski |date= 23 December 2013 |publisher= Sky and Telescope }}</ref><ref name="2014AJ....147...94D" /><ref name="Fundamental Parameters and Spectral">{{cite journal|arxiv=1508.01767|doi=10.1088/0004-637X/810/2/158|title=Fundamental Parameters and Spectral Energy Distributions of Young and Field Age Objects with Masses Spanning the Stellar to Planetary Regime|journal=The Astrophysical Journal|volume=810|issue=2|pages=158|year=2015|last1=Filippazzo|first1=Joseph C.|last2=Rice|first2=Emily L.|last3=Faherty|first3=Jacqueline|author3-link=Jackie Faherty|last4=Cruz|first4=Kelle L.|last5=Van Gordon|first5=Mollie M.|last6=Looper|first6=Dagny L.|last7=Kramer|first7=Michael|last8=Bassa|first8=Cees|last9=Dhillon|first9=Vik S.|last10=Driebe|first10=Thomas|last11=Hessels|first11=Jason W. T.|last12=Kaspi|first12=Victoria M.|last13=Kondratiev|first13=Vladislav I.|last14=Langer|first14=Norbert|last15=Marsh|first15=Thomas R.|last16=McLaughlin|first16=Maura A.|last17=Pennucci|first17=Timothy T.|last18=Ransom|first18=Scott M.|last19=Stairs|first19=Ingrid H.|author20=Joeri van Leeuwen|last21=Verbiest|first21=Joris P. W.|last22=Whelan|first22=David G.|bibcode=2015ApJ...810..158F|s2cid=89611607 }}</ref>
|-
|[[GD 165]] B
|71,492
| rowspan="3" |[[Brown dwarf]]
|
|<ref>{{Cite journal |last1=Filippazzo |first1=Joseph C. |last2=Rice |first2=Emily L. |last3=Faherty |first3=Jacqueline |last4=Cruz |first4=Kelle L. |last5=Van Gordon |first5=Mollie M. |last6=Looper |first6=Dagny L. |date=2015-09-10 |title=Fundamental Parameters and Spectral Energy Distributions of Young and Field Age Objects with Masses Spanning the Stellar to Planetary Regime |journal=The Astrophysical Journal |volume=810 |issue=2 |pages=158 |doi=10.1088/0004-637X/810/2/158 |arxiv=1508.01767 |bibcode=2015ApJ...810..158F |s2cid=89611607 |issn=1538-4357}}</ref>
|-
|[[15 Sagittae]] B
|71,492
|
|<ref>{{Cite journal |last1=Crepp |first1=Justin R. |last2=Johnson |first2=John Asher |last3=Fischer |first3=Debra A. |last4=Howard |first4=Andrew W. |last5=Marcy |first5=Geoffrey W. |last6=Wright |first6=Jason T. |last7=Isaacson |first7=Howard |last8=Boyajian |first8=Tabetha |last9=von Braun |first9=Kaspar |last10=Hillenbrand |first10=Lynne A. |last11=Hinkley |first11=Sasha |last12=Carpenter |first12=John M. |last13=Brewer |first13=John M. |date=2012-06-01 |title=The Dynamical Mass and Three-Dimensional Orbit of HR7672B: A Benchmark Brown Dwarf with High Eccentricity |journal=The Astrophysical Journal |volume=751 |issue=2 |pages=97 |doi=10.1088/0004-637X/751/2/97 |arxiv=1112.1725 |bibcode=2012ApJ...751...97C |issn=0004-637X}}</ref>
|-
|[[DENIS-P J1058.7−1548]]
|71,492
|
|<ref>{{Cite journal |last1=Vos |first1=Johanna M. |last2=Biller |first2=Beth A. |last3=Allers |first3=Katelyn N. |last4=Faherty |first4=Jacqueline K. |last5=Liu |first5=Michael C. |last6=Metchev |first6=Stanimir |last7=Eriksson |first7=Simon |last8=Manjavacas |first8=Elena |last9=Dupuy |first9=Trent J. |last10=Janson |first10=Markus |last11=Radigan-Hoffman |first11=Jacqueline |last12=Crossfield |first12=Ian |last13=Bonnefoy |first13=Mickael |last14=Best |first14=William M. J. |last15=Homeier |first15=Derek |date=2020-06-24 |title=Spitzer Variability Properties of Low-Gravity L Dwarfs |journal=The Astronomical Journal |volume=160 |issue=1 |pages=38 |doi=10.3847/1538-3881/ab9642 |arxiv=2005.12854 |bibcode=2020AJ....160...38V |hdl=1721.1/132407.2 |s2cid=218889787 |issn=1538-3881 |doi-access=free }}</ref>
|-
|[[LHS 2924]]
|71,657
|[[Red dwarf]]
|
|<ref>{{Cite journal |last1=Tsuji |first1=Takashi |last2=Nakajima |first2=Tadashi |date=2016-02-01 |title=Near-infrared spectroscopy of M dwarfs. III. Carbon and oxygen abundances in late M dwarfs, including the dusty rapid rotator 2MASSI J1835379+325954† |url=https://ui.adsabs.harvard.edu/abs/2016PASJ...68...13T |journal=Publications of the Astronomical Society of Japan |volume=68 |issue=1 |pages=13 |doi=10.1093/pasj/psv119 |arxiv=1511.04682 |bibcode=2016PASJ...68...13T |issn=0004-6264}}</ref>
|-
|[[2MASS J00361617+1821104|2MASS 0036+1821]]
|72,200
| rowspan="6" |[[Brown dwarf]]
|
|<ref name="Fundamental Parameters and Spectral" />
|-
|[[CoRoT-3b|CoRoT-3 b]]
|72,200
|
|<ref>{{Cite journal |last1=Deleuil |first1=M. |last2=Deeg |first2=H. J. |last3=Alonso |first3=R. |last4=Bouchy |first4=F. |last5=Rouan |first5=D. |last6=Auvergne |first6=M. |last7=Baglin |first7=A. |last8=Aigrain |first8=S. |last9=Almenara |first9=J. M. |last10=Barbieri |first10=M. |last11=Barge |first11=P. |last12=Bruntt |first12=H. |last13=Bordé |first13=P. |last14=Collier Cameron |first14=A. |last15=Csizmadia |first15=Sz. |date=2008-12-01 |title=Transiting exoplanets from the CoRoT space mission . VI. CoRoT-Exo-3b: the first secure inhabitant of the brown-dwarf desert |url=https://ui.adsabs.harvard.edu/abs/2008A&A...491..889D |journal=Astronomy and Astrophysics |volume=491 |issue=3 |pages=889–897 |doi=10.1051/0004-6361:200810625 |arxiv=0810.0919 |bibcode=2008A&A...491..889D |issn=0004-6361}}</ref>
|-
|[[LHS 1070]] B
|72,350
|Likely a brown dwarf based on its mass<ref name="kohler" />
|<ref name="lhs1070" />
|-
|[[UGPS 0722-05]]
|72,850
|Possibly a [[rogue planet]]
|<ref>{{Cite journal |last1=Dupuy |first1=Trent J. |last2=Kraus |first2=Adam L. |date=2013-09-27 |title=Distances, Luminosities, and Temperatures of the Coldest Known Substellar Objects |journal=Science |volume=341 |issue=6153 |pages=1492–1495 |doi=10.1126/science.1241917 |pmid=24009359 |issn=0036-8075|arxiv=1309.1422 |bibcode=2013Sci...341.1492D |s2cid=30379513 }}</ref>
|-
|[[WISE 2150–7520 AB|WISE 2150–7520]] A
|73,635
|
|<ref name=":20" />
|-
|[[Luhman 16]] B
|74,350
|Luhman 16 B and Luhman 16 A are the closest brown dwarf stars to Earth, and the third-nearest star system to the Solar System.
|{{efn|name="RadiusCalculationFromLuminosityandTemperature"}}
|-
|[[DENIS J1048−3956]]
|75,135.5
|rowspan="4" |[[Red dwarf]]
|
|<ref>{{Cite journal |last1=Lienhard |first1=F. |last2=Queloz |first2=D. |last3=Gillon |first3=M. |last4=Burdanov |first4=A. |last5=Delrez |first5=L. |last6=Ducrot |first6=E. |last7=Handley |first7=W. |last8=Jehin |first8=E. |last9=Murray |first9=C. A. |last10=Triaud |first10=A. H. M. J. |last11=Gillen |first11=E. |last12=Mortier |first12=A. |last13=Rackham |first13=B. V. |date=2020-09-21 |title=Global Analysis of the TRAPPIST Ultra-Cool Dwarf Transit Survey |journal=Monthly Notices of the Royal Astronomical Society |volume=497 |issue=3 |pages=3790–3808 |doi=10.1093/mnras/staa2054 |doi-access=free |arxiv=2007.07278 |issn=0035-8711}}</ref>
|-
|[[DX Cancri]]
|76,527
|
|<ref>{{Cite journal |last1=Morin |first1=J. |last2=Donati |first2=J. F. |last3=Petit |first3=P. |last4=Delfosse |first4=X. |last5=Forveille |first5=T. |last6=Jardine |first6=M. M. |date=2010-07-20 |title=Large-scale magnetic topologies of late M dwarfs |journal=Monthly Notices of the Royal Astronomical Society |volume=407 |issue=4 |pages=2269–2286 |doi=10.1111/j.1365-2966.2010.17101.x|doi-access=free |arxiv=1005.5552 |bibcode=2010MNRAS.407.2269M |s2cid=119192200 }}</ref>
|-
|[[LHS 292]]
|76,527
|
|<ref>{{Cite journal |last1=Morin |first1=J. |last2=Donati |first2=J. F. |last3=Petit |first3=P. |last4=Delfosse |first4=X. |last5=Forveille |first5=T. |last6=Jardine |first6=M. M. |date=2010-07-20 |title=Large-scale magnetic topologies of late M dwarfs |journal=Monthly Notices of the Royal Astronomical Society |volume=407 |issue=4 |pages=2269–2286 |doi=10.1111/j.1365-2966.2010.17101.x|arxiv=1005.5552 |bibcode=2010MNRAS.407.2269M |doi-access=free }}</ref>
|-
|[[TVLM 513-46546]]
|76,527
|Has one confirmed exoplanet
|
|-
|[[Gliese 229]] B
|79,000
| rowspan="3" |[[Brown dwarf]]
|
|
|-
|[[HR 2562 b|HR 2562 B]]
|79,350
|Its mass is quite uncertain, at {{val|29|15|ul=Jupiter mass}} .<ref>{{Cite journal |last1=Sutlieff |first1=Ben J. |last2=Bohn |first2=Alexander J. |last3=Birkby |first3=Jayne L. |last4=Kenworthy |first4=Matthew A. |last5=Morzinski |first5=Katie M. |last6=Doelman |first6=David S. |last7=Males |first7=Jared R. |last8=Snik |first8=Frans |last9=Close |first9=Laird M. |last10=Hinz |first10=Philip M. |last11=Charbonneau |first11=David |date=2021-07-24 |title=High-contrast observations of brown dwarf companion HR 2562 B with the vector Apodizing Phase Plate coronagraph |journal=Monthly Notices of the Royal Astronomical Society |volume=506 |issue=3 |pages=3224–3238 |doi=10.1093/mnras/stab1893 |doi-access=free |arxiv=2106.14890 |issn=0035-8711}}</ref> It is cited by the [[NASA Exoplanet Archive]] as the most massive exoplanet known.<ref>{{Cite web |title=Planetary Systems |url=https://exoplanetarchive.ipac.caltech.edu/cgi-bin/TblView/nph-tblView?app=ExoTbls&config=PS |access-date=2023-12-30 |website=exoplanetarchive.ipac.caltech.edu}}</ref>
|<ref>{{Cite journal |last1=Konopacky |first1=Quinn M. |last2=Rameau |first2=Julien |last3=Duchene |first3=Gaspard |last4=Filippazzo |first4=Joseph C. |last5=Godfrey |first5=Paige A. Giorla |last6=Marois |first6=Christian |last7=Nielsen |first7=Eric L. |last8=Pueyo |first8=Laurent |last9=Rafikov |first9=Roman R. |last10=Rice |first10=Emily L. |last11=Wang |first11=Jason J. |last12=Ammons |first12=S. Mark |last13=Bailey |first13=Vanessa P. |last14=Barman |first14=Travis S. |last15=Bulger |first15=Joanna |date=2016-09-14 |title=Discovery of a Substellar Companion to the Nearby Debris Disk Host HR 2562 |journal=The Astrophysical Journal |volume=829 |issue=1 |pages=L4 |doi=10.3847/2041-8205/829/1/L4 |doi-access=free |arxiv=1608.06660 |bibcode=2016ApJ...829L...4K |issn=2041-8213}}</ref>
|-
|[[KELT-1]] B
|79,350
|
|<ref>{{Cite journal |last1=Siverd |first1=Robert J. |last2=Beatty |first2=Thomas G. |last3=Pepper |first3=Joshua |last4=Eastman |first4=Jason D. |last5=Collins |first5=Karen |last6=Bieryla |first6=Allyson |last7=Latham |first7=David W. |last8=Buchhave |first8=Lars A. |last9=Jensen |first9=Eric L. N. |last10=Crepp |first10=Justin R. |last11=Street |first11=Rachel |last12=Stassun |first12=Keivan G. |last13=Gaudi |first13=B. Scott |last14=Berlind |first14=Perry |last15=Calkins |first15=Michael L. |date=2012-12-20 |title=KELT-1b: A Strongly Irradiated, Highly Inflated, Short Period, 27 Jupiter-mass Companion Transiting a mid-F Star |journal=The Astrophysical Journal |volume=761 |issue=2 |pages=123 |doi=10.1088/0004-637X/761/2/123 |arxiv=1206.1635 |bibcode=2012ApJ...761..123S |issn=0004-637X}}</ref>
|-
|| [[OGLE-TR-122B]] || 81,100
|[[Red dwarf]]|| This was once the smallest known actively fusing star, when found in 2005, through 2013. It is the smallest eclipsing red dwarf, and smallest observationally measured diameter. || <ref name="Space-2005-03-03">{{cite news |url= http://www.space.com/840-newfound-star-smaller-planets.html |title= Newfound Star Smaller than Some Planets |author= Robert Roy Britt |date= 3 March 2005 |publisher= Space.com }}</ref><ref name="SpaceAnswers-SmallestStar-2013-03-22">{{cite web |url= http://www.spaceanswers.com/deep-space/what-is-the-smallest-star/ |title= What is the smallest star? |author1= Jonathan O'Callaghan |author2= Josh Barker (National Space Centre) |date= 22 March 2013 |publisher= SpaceAnswers.com }}</ref><ref name="2005A&A...433L..21P">{{cite journal |title= A planet-sized transiting star around OGLE-TR-122. Accurate mass and radius near the hydrogen-burning limit |arxiv= astro-ph/0501611 |doi= 10.1051/0004-6361:200500025 |bibcode= 2005A&A...433L..21P |author1=Pont, F. |author2=Melo, C. H. F. |author3=Bouchy, F. |author4=Udry, S. |author5=Queloz, D. |author6=Mayor, M. |author7=Santos, N. C. |publication-date= April 2005 |journal= Astronomy and Astrophysics |volume= 433 |issue= 2 |page= L21–L24 |date= 27 January 2005 |s2cid= 14799999 }}</ref>
|-
|[[CoRoT-15b]]
|82,200
|[[Brown dwarf]]
|
|<ref>{{Cite journal |last1=Bouchy |first1=F. |last2=Deleuil |first2=M. |last3=Guillot |first3=T. |last4=Aigrain |first4=S. |last5=Carone |first5=L. |last6=Cochran |first6=W. D. |date=January 2011 |title=Transiting exoplanets from the CoRoT space mission. XV. CoRoT-15b: a brown dwarf transiting companion |journal=Astronomy & Astrophysics |volume=525 |pages=A68 |doi=10.1051/0004-6361/201015276 |arxiv=1010.0179 |bibcode=2011A&A...525A..68B |issn=0004-6361|doi-access=free }}</ref>
|-
|[[VB 10]]
|82,300
| rowspan="6" | [[Red dwarf]]
|It was the smallest known star from 1948 to 1981.
|<ref name=":3" />
|-
||[[TRAPPIST-1]]|| 82,925|| Hosts a planetary system with at least seven rocky planets. ||<ref>{{Cite journal |last1=Agol |first1=Eric |last2=Dorn |first2=Caroline |last3=Grimm |first3=Simon L. |last4=Turbet |first4=Martin |last5=Ducrot |first5=Elsa |last6=Delrez |first6=Laetitia |last7=Gillon |first7=Michaël |last8=Demory |first8=Brice-Olivier |last9=Burdanov |first9=Artem |last10=Barkaoui |first10=Khalid |last11=Benkhaldoun |first11=Zouhair |last12=Bolmont |first12=Emeline |last13=Burgasser |first13=Adam |last14=Carey |first14=Sean |last15=Wit |first15=Julien de |date=2021-01-22 |title=Refining the Transit-timing and Photometric Analysis of TRAPPIST-1: Masses, Radii, Densities, Dynamics, and Ephemerides |journal=The Planetary Science Journal |language=en |volume=2 |issue=1 |pages=1 |doi=10.3847/PSJ/abd022 |arxiv=2010.01074 |bibcode=2021PSJ.....2....1A |issn=2632-3338|doi-access=free }}</ref>
|-
|[[LHS 2090]]
|83,500
|
|<ref>{{Cite journal |last1=Fouqué |first1=Pascal |last2=Moutou |first2=Claire |last3=Malo |first3=Lison |last4=Martioli |first4=Eder |last5=Lim |first5=Olivia |last6=Rajpurohit |first6=Arvind |last7=Artigau |first7=Etienne |last8=Delfosse |first8=Xavier |last9=Donati |first9=Jean-François |last10=Forveille |first10=Thierry |last11=Morin |first11=Julien |last12=Allard |first12=France |last13=Delage |first13=Raphaël |last14=Doyon |first14=René |last15=Hébrard |first15=Elodie |date=2018-04-01 |title=SPIRou Input Catalogue: Global properties of 440 M dwarfs observed with ESPaDOnS at CFHT |journal=Monthly Notices of the Royal Astronomical Society |volume=475 |issue=2 |pages=1960–1986 |doi=10.1093/mnras/stx3246 |doi-access=free |issn=0035-8711|arxiv=1712.04490 }}</ref>
|-
|[[Teegarden's Star]]
|83,500
|Has two potentially habitable planets.
|<ref>{{Citation |last1=Dreizler |first1=S. |title=Teegarden's Star revisited: A nearby planetary system with at least three planets |date=2024-02-01 |arxiv=2402.00923 |last2=Luque |first2=R. |last3=Ribas |first3=I. |last4=Koseleva |first4=V. |last5=Ruh |first5=H. L. |last6=Nagel |first6=E. |last7=Pozuelos |first7=F. J. |last8=Zechmeister |first8=M. |last9=Reiners |first9=A.|journal=Astronomy and Astrophysics |volume=684 |doi=10.1051/0004-6361/202348033 |bibcode=2024A&A...684A.117D }}</ref>
|-
|[[V1054 Ophiuchi|VB 8]]
|84,450
|
|<ref name=":3" />
|-
|[[SPECULOOS-3]]
|85,570
|Second-smallest star known to host a transiting exoplanet after TRAPPIST-1<ref name="speculoos3b" />
|<ref name="speculoos3b">{{Cite journal |last1=Gillon |first1=Michaël |last2=Pedersen |first2=Peter P. |last3=Rackham |first3=Benjamin V. |last4=Dransfield |first4=Georgina |last5=Ducrot |first5=Elsa |last6=Barkaoui |first6=Khalid |last7=Burdanov |first7=Artem Y. |last8=Schroffenegger |first8=Urs |last9=Gómez Maqueo Chew |first9=Yilen |last10=Lederer |first10=Susan M. |last11=Alonso |first11=Roi |last12=Burgasser |first12=Adam J. |last13=Howell |first13=Steve B. |last14=Narita |first14=Norio |last15=de Wit |first15=Julien |date=2024-05-15 |title=Detection of an Earth-sized exoplanet orbiting the nearby ultracool dwarf star SPECULOOS-3 |url=https://www.nature.com/articles/s41550-024-02271-2 |journal=Nature Astronomy |volume=8 |issue=7 |language=en |pages=865–878 |doi=10.1038/s41550-024-02271-2 |arxiv=2406.00794 |bibcode=2024NatAs...8..865G |issn=2397-3366}}</ref>
|-
|[[2MASS 0939-2448]] A
|87,220
| rowspan="2" |[[Brown dwarf]]
|
|<ref>{{Cite journal |last1=Line |first1=Michael R. |last2=Marley |first2=Mark S. |last3=Liu |first3=Michael C. |last4=Burningham |first4=Ben |last5=Morley |first5=Caroline V. |last6=Hinkel |first6=Natalie R. |last7=Teske |first7=Johanna |last8=Fortney |first8=Jonathan J. |last9=Lupu |first9=Roxana |last10=Freedman |first10=Richard |date=2017-10-13 |title=Uniform Atmospheric Retrieval Analysis of Ultracool Dwarfs II: Properties of 11 T-dwarfs |journal=The Astrophysical Journal |volume=848 |issue=2 |pages=83 |doi=10.3847/1538-4357/aa7ff0 |arxiv=1612.02809 |bibcode=2017ApJ...848...83L |s2cid=53053922 |issn=1538-4357 |doi-access=free }}</ref>
|-
|[[Teide 1]]
|88,130
|The first brown dwarf to be verified, in 1995.
|<ref>{{Cite journal |last1=Rebolo |first1=R. |last2=Martin |first2=E. L. |last3=Basri |first3=G. |last4=Marcy |first4=G. W. |last5=Osorio |first5=M. R. Zapatero |date=1996-09-20 |title=Brown Dwarfs in the Pleiades Cluster Confirmed by the Lithium Test |journal=The Astrophysical Journal |volume=469 |issue=1 |pages=L53–L56 |doi=10.1086/310263|arxiv=astro-ph/9607002 |bibcode=1996ApJ...469L..53R }}</ref>{{efn | Applying the [[Stefan–Boltzmann law]] with a nominal [[sun|solar]] [[effective temperature]] of 5,772&nbsp;[[Kelvin|K]]:
:<math>\sqrt{\biggl(\frac{5,772}{2,600}\biggr)^4 \cdot 10^{-3.18}} = 0.12668\ R_\odot</math>.}}
|-
|[[Gliese 412]] B
|90,400
|[[Red dwarf]]
|
|<ref name=":1">{{Cite journal |last1=Mann |first1=Andrew W. |last2=Feiden |first2=Gregory A. |last3=Gaidos |first3=Eric |last4=Boyajian |first4=Tabetha |last5=von Braun |first5=Kaspar |date=2015-05-01 |title=How to Constrain Your M Dwarf: measuring effective temperature, bolometric luminosity, mass, and radius |journal=The Astrophysical Journal |volume=804 |issue=1 |pages=64 |doi=10.1088/0004-637X/804/1/64 |arxiv=1501.01635 |bibcode=2015ApJ...804...64M |issn=0004-637X|hdl=2152/34940 |s2cid=19269312 |hdl-access=free }}</ref>
|-
|[[CFBDSIR 1458+10]] B
|90,450
|[[Brown dwarf]]
|
|
|-
|[[CWISE J124909.08+362116.0]]
|93,200{{Efn|1=Calculated using the mass and a surface gravity of 5.1 using the following equation:<br />log(R/{{solar radius}}) = 2.22 + 0.5{{*}}log(M/{{solar mass}}) - 0.5{{*}}log ''g''}}
| rowspan="7" |[[Red dwarf]]
|A high-velocity star travelling the Milky Way at 456 km/s.
|<ref>{{Cite journal |last1=Burgasser |first1=Adam J. |title=Discovery of a Hypervelocity L Subdwarf at the Star/Brown Dwarf Mass Limit |date=2024-07-11 |arxiv=2407.08578 |last2=Gerasimov |first2=Roman |last3=Kremer |first3=Kyle |last4=Brooks |first4=Hunter |last5=Alvarado III |first5=Efrain |last6=Schneider |first6=Adam C. |last7=Meisner |first7=Aaron M. |last8=Theissen |first8=Christopher A. |last9=Softich |first9=Emma|journal=The Astrophysical Journal |volume=971 |issue=1 |pages=L25 |doi=10.3847/2041-8213/ad6607 |doi-access=free |bibcode=2024ApJ...971L..25B }}</ref>
|-
|[[Gliese 1002]]
|95,310
|Has two confirmed exoplanets
|<ref>{{Cite journal |last1=Mascareño |first1=A. Suárez |last2=González-Álvarez |first2=E. |last3=Osorio |first3=M. R. Zapatero |last4=Lillo-Box |first4=J. |last5=Faria |first5=J. P. |last6=Passegger |first6=V. M. |last7=Hernández |first7=J. I. González |last8=Figueira |first8=P. |last9=Sozzetti |first9=A. |last10=Rebolo |first10=R. |last11=Pepe |first11=F. |last12=Santos |first12=N. C. |last13=Cristiani |first13=S. |last14=Lovis |first14=C. |last15=Silva |first15=A. M. |date=2022-11-28 |title=Two temperate Earth-mass planets orbiting the nearby star GJ1002 |journal=Astronomy & Astrophysics |volume=670 |pages=A5 |doi=10.1051/0004-6361/202244991 |arxiv=2212.07332 |issn=0004-6361|doi-access=free |bibcode=2023A&A...670A...5S }}</ref>
|-
|[[LHS 1070]] A
|97,400
|
|<ref name="lhs1070"/>
|-
|[[LHS 3154]]
|97,400
|Has one confirmed exoplanet
|<ref>{{Citation |last1=Stefansson |first1=Gudmundur |title=An extreme test case for planet formation: a close-in Neptune orbiting an ultracool star |date=2023-03-23 |arxiv=2303.13321 |last2=Mahadevan |first2=Suvrath |last3=Miguel |first3=Yamila |last4=Robertson |first4=Paul |last5=Delamer |first5=Megan |last6=Kanodia |first6=Shubham |last7=Cañas |first7=Caleb |last8=Winn |first8=Joshua |last9=Ninan |first9=Joe}}</ref>
|-
|[[Wolf 424]] B
|97,400
|
|<ref name=":16" />
|-
|| [[Wolf 359]]|| 100,180.8 || Fifth-nearest star system to the Solar System. Has one unconfirmed exoplanet|| <ref name=":3" />
|-
|[[NN Serpentis]] red dwarf
|103,660
|
|<ref name="aaa364_217">{{citation |last1=Delfosse |first1=Xavier |title=Accurate masses of very low mass stars. IV. Improved mass-luminosity relations |date=December 2000 |journal=Astronomy and Astrophysics |volume=364 |pages=217–224 |arxiv=astro-ph/0010586 |bibcode=2000A&A...364..217D |display-authors=1 |last2=Forveille |first2=Thierry |last3=Ségransan |first3=Damien |last4=Beuzit |first4=Jean-Luc |last5=Udry |first5=Stéphane |last6=Perrier |first6=Christian |last7=Mayor |first7=Michel}}</ref>
|-
|[[CFBDSIR 1458+10]] A
|104,350
|[[Brown dwarf]]
|
|
|-
|[[NY Virginis]] A
|105,050
|[[Subdwarf B star|B-type subdwarf]]
|
|<ref>{{Cite journal |last1=Charpinet |first1=S. |last2=Van Grootel |first2=V. |last3=Reese |first3=D. |last4=Fontaine |first4=G. |last5=Green |first5=E. M. |last6=Brassard |first6=P. |last7=Chayer |first7=P. |date=2008-10-01 |title=Testing the forward modeling approach in asteroseismology. II. Structure and internal dynamics of the hot B subdwarf component in the close eclipsing binary system PG 1336-018 |url=https://ui.adsabs.harvard.edu/abs/2008A&A...489..377C |journal=Astronomy and Astrophysics |volume=489 |issue=1 |pages=377–394 |doi=10.1051/0004-6361:200809907 |bibcode=2008A&A...489..377C |hdl=2268/109085 |issn=0004-6361|hdl-access=free }}</ref>
|-
|[[Gliese 1061]]
|105,746.4
| rowspan="7" | [[Red dwarf]]
|Has three confirmed exoplanets, two of them are in the habitable zone.
|<ref name=":3" />
|-
|[[LP 890-9]]
|106,580
|Has two confirmed exoplanets, one of them (LP 890-9c) is in the habitable zone.
|<ref name=":14">{{Cite journal |last1=Delrez |first1=L. |last2=Murray |first2=C. A. |last3=Pozuelos |first3=F. J. |last4=Narita |first4=N. |last5=Ducrot |first5=E. |last6=Timmermans |first6=M. |last7=Watanabe |first7=N. |last8=Burgasser |first8=A. J. |last9=Hirano |first9=T. |last10=Rackham |first10=B. V. |last11=Stassun |first11=K. G. |last12=Van Grootel |first12=V. |last13=Aganze |first13=C. |last14=Cointepas |first14=M. |last15=Howell |first15=S. |date=November 2022 |title=Two temperate super-Earths transiting a nearby late-type M dwarf |journal=Astronomy & Astrophysics |volume=667 |pages=A59 |doi=10.1051/0004-6361/202244041 |arxiv=2209.02831 |bibcode=2022A&A...667A..59D |issn=0004-6361}}</ref>
|-
|[[Proxima Centauri]] <br />''(Alpha Centauri C)''
|107,277
|Nearest star and nearest stellar system to the Sun. Has one confirmed potentially habitable exoplanet, one unconfirmed exoplanet and one disputed exoplanet
|<ref>{{Cite journal |last1=Kervella |first1=P. |last2=Thévenin |first2=F. |last3=Lovis |first3=C. |date=February 2017 |title=Proxima's orbit around Alpha Centauri |journal=Astronomy & Astrophysics |volume=598 |pages=L7 |doi=10.1051/0004-6361/201629930 |arxiv=1611.03495 |bibcode=2017A&A...598L...7K |s2cid=50867264 |issn=0004-6361}}</ref>
|-
|{{nowrap|[[Luyten 726-8]] B}} {{nowrap|''(UV Ceti)''}}
|110,615
|The archetypal type of the [[flare star]]s, and the eight-nearest star system to the Solar System.
|<ref name=":12">{{Cite journal |last1=Kervella |first1=P. |last2=Mérand |first2=A. |last3=Ledoux |first3=C. |last4=Demory |first4=B.-O. |last5=Bouquin |first5=J.-B. Le |date=September 2016 |title=The red dwarf pair GJ65AB: inflated, spinning twins of Proxima |journal=Astronomy & Astrophysics |volume=593 |pages=A127 |doi=10.1051/0004-6361/201628631 |arxiv=1607.04351 |issn=0004-6361|doi-access=free |bibcode=2016A&A...593A.127K }}</ref>
|-
|[[GL Virginis]]
|111,300
|
|<ref>{{Cite journal |last1=Reiners |first1=A. |last2=Basri |first2=G. |last3=Browning |first3=M. |date=2009-02-01 |title=Evidence for Magnetic Flux Saturation in Rapidly Rotating M Stars |url=https://ui.adsabs.harvard.edu/abs/2009ApJ...692..538R |journal=The Astrophysical Journal |volume=692 |issue=1 |pages=538–545 |doi=10.1088/0004-637X/692/1/538 |arxiv=0810.5139 |bibcode=2009ApJ...692..538R |issn=0004-637X}}</ref>
|-
|[[NY Virginis]] B
|111,300
|
|<ref>{{Cite journal |last1=Vučković |first1=M. |last2=Aerts |first2=C. |last3=Östensen |first3=R. |last4=Nelemans |first4=G. |last5=Hu |first5=Haili |last6=Jeffery |first6=C. S. |last7=Dhillon |first7=V. S. |last8=Marsh |first8=T. R. |date=2007-08-01 |title=The binary properties of the pulsating subdwarf B eclipsing binary PG 1336-018 (NY Virginis) |journal=Astronomy and Astrophysics |volume=471 |issue=2 |pages=605–615 |doi=10.1051/0004-6361:20077179 |arxiv=0706.3363 |bibcode=2007A&A...471..605V |issn=0004-6361|doi-access=free }}</ref>
|-
|[[TZ Arietis]]
|112,000
|Has one confirmed exoplanet
|<ref name="Houdebine 56">{{Cite journal |last1=Houdebine |first1=Eric R. |last2=Mullan |first2=D. J. |last3=Doyle |first3=J. G. |last4=de La Vieuville |first4=Geoffroy |last5=Butler |first5=C. J. |last6=Paletou |first6=F. |date=2019-07-10 |title=The Mass-Activity relationships in M and K dwarfs. I. Stellar parameters of our sample of M and K dwarfs |journal=The Astronomical Journal |volume=158 |issue=2 |pages=56 |doi=10.3847/1538-3881/ab23fe |arxiv=1905.07921 |bibcode=2019AJ....158...56H |issn=1538-3881|doi-access=free }}</ref>
|-
|[[HD 984]] B
|112,700
|[[Brown dwarf]]
|
|<ref>{{Cite journal |last1=Johnson-Groh |first1=Mara |last2=Marois |first2=Christian |last3=De Rosa |first3=Robert J. |last4=Nielsen |first4=Eric L. |last5=Rameau |first5=Julien |last6=Blunt |first6=Sarah |last7=Vargas |first7=Jeffrey |last8=Ammons |first8=S. Mark |last9=Bailey |first9=Vanessa P. |last10=Barman |first10=Travis S. |last11=Bulger |first11=Joanna |last12=Chilcote |first12=Jeffrey K. |last13=Cotten |first13=Tara |last14=Doyon |first14=René |last15=Duchêne |first15=Gaspard |date=2017-04-01 |title=Integral Field Spectroscopy of the Low-mass Companion HD 984 B with the Gemini Planet Imager |journal=The Astronomical Journal |volume=153 |issue=4 |pages=190 |doi=10.3847/1538-3881/aa6480 |doi-access=free |arxiv=1703.02607 |bibcode=2017AJ....153..190J |issn=0004-6256}}</ref>{{efn | name=radius | Applying the [[Stefan–Boltzmann law]] with a nominal [[sun|solar]] [[effective temperature]] of 5,772&nbsp;[[Kelvin|K]]:
:<math>\sqrt{\biggl(\frac{5,772}{2,730}\biggr)^4 \cdot 10^{-2.88}} = 0.162\ R_\odot</math>.}}
|-
|{{nowrap|[[Luyten 726-8]] A}} {{nowrap|''(BL Ceti)''}}
|114,790
| rowspan="4" | [[Red dwarf]]
|Luyten 726-8 A and B are the eight-nearest star system to the Solar System.
|<ref name=":12" />
|-
|[[YZ Ceti]]
|116,877.5
|Has three confirmed exoplanets
|<ref>{{Cite journal |last1=Astudillo-Defru |first1=N. |last2=Díaz |first2=R. F. |last3=Bonfils |first3=X. |last4=Almenara |first4=J. M. |last5=Delisle |first5=J.-B. |last6=Bouchy |first6=F. |last7=Delfosse |first7=X. |last8=Forveille |first8=T. |last9=Lovis |first9=C. |last10=Mayor |first10=M. |last11=Murgas |first11=F. |last12=Pepe |first12=F. |last13=Santos |first13=N. C. |last14=Ségransan |first14=D. |last15=Udry |first15=S. |date=2017-08-10 |title=The HARPS search for southern extra-solar planets XLII. A system of Earth-mass planets around the nearby M dwarf YZ Ceti |journal=Astronomy and Astrophysics |volume=605 |language=en |doi=10.1051/0004-6361/201731581|arxiv=1708.03336v2 |bibcode=2017A&A...605L..11A |s2cid=119393757 }}</ref>
|-
|[[LP 791-18]] ''(TOI-736)''
|118,270
|Has three confirmed exoplanets
|<ref>{{Cite journal |last1=Crossfield |first1=Ian J. M. |last2=Waalkes |first2=William |last3=Newton |first3=Elisabeth R. |last4=Narita |first4=Norio |last5=Muirhead |first5=Philip |last6=Ment |first6=Kristo |last7=Matthews |first7=Elisabeth |last8=Kraus |first8=Adam |last9=Kostov |first9=Veselin |last10=Kosiarek |first10=Molly R. |last11=Kane |first11=Stephen R. |last12=Isaacson |first12=Howard |last13=Halverson |first13=Sam |last14=Gonzales |first14=Erica |last15=Everett |first15=Mark |date=2019-09-19 |title=A Super-Earth and Sub-Neptune Transiting the Late-type M Dwarf LP 791-18 |journal=The Astrophysical Journal Letters |volume=883 |issue=1 |pages=L16 |doi=10.3847/2041-8213/ab3d30 |doi-access=free |arxiv=1906.09267 |bibcode=2019ApJ...883L..16C |issn=2041-8205}}</ref>
|-
|[[HR 858]] B
|118,270
|
|<ref>{{Cite journal |last1=Vanderburg |first1=Andrew |last2=Huang |first2=Chelsea X. |last3=Rodriguez |first3=Joseph E. |last4=Becker |first4=Juliette C. |last5=Ricker |first5=George R. |last6=Vanderspek |first6=Roland K. |last7=Latham |first7=David W. |last8=Seager |first8=Sara |last9=Winn |first9=Joshua N. |last10=Jenkins |first10=Jon M. |last11=Addison |first11=Brett |last12=Bieryla |first12=Allyson |last13=Briceño |first13=Cesar |last14=Bowler |first14=Brendan P. |last15=Brown |first15=Timothy M. |date=2019-08-10 |title=TESS Spots a Compact System of Super-Earths around the Naked-Eye Star HR 858 |journal=The Astrophysical Journal Letters |volume=881 |issue=1 |pages=L19 |doi=10.3847/2041-8213/ab322d |doi-access=free |arxiv=1905.05193 |bibcode=2019ApJ...881L..19V |issn=2041-8205}}</ref>
|-
| [[UY Sextantis]]|| 118,270  || [[Subdwarf B star|B-type subdwarf]]|| || <ref>{{Cite journal |last1=Reed |first1=M. D. |last2=Yeager |first2=M. |last3=Vos |first3=J. |last4=Telting |first4=J. H. |last5=Østensen |first5=R. H. |last6=Slayton |first6=A. |last7=Baran |first7=A. S. |last8=Jeffery |first8=C. S. |date=2020-03-01 |title=K2 observations of the pulsating subdwarf B stars UY Sex and V1405 Ori |journal=Monthly Notices of the Royal Astronomical Society |volume=492 |issue=4 |pages=5202–5217 |doi=10.1093/mnras/staa144 |bibcode=2020MNRAS.492.5202R |issn=0035-8711|doi-access=free }}</ref>
|-
|[[Wolf 424]] A
|118,270
| rowspan="1" |[[Red dwarf]]
|
|<ref name=":16" />
|-
|[[Z Andromedae]] B
|118,270{{snd}}250,450
| rowspan="1" |[[White dwarf]]
|
|<ref name="fekel">{{cite journal |last1=Fekel |first1=Francis C |last2=Hinkle |first2=Kenneth H |last3=Joyce |first3=Richard R |last4=Skrutskie |first4=Michael F |year=2000 |title=Infrared Spectroscopy of Symbiotic Stars. II. Orbits for Five S-Type Systems with Two-Year Periods |journal=The Astronomical Journal |volume=120 |issue=6 |pages=3255 |bibcode=2000AJ....120.3255F |doi=10.1086/316872 |doi-access=free}}</ref>
|-
|[[Kepler-42]]
|121,750
| rowspan="7" |[[Red dwarf]]
|Has three confirmed exoplanets
|<ref>{{Cite journal |last1=Mann |first1=Andrew W. |last2=Dupuy |first2=Trent |last3=Muirhead |first3=Philip S. |last4=Johnson |first4=Marshall C. |last5=Liu |first5=Michael C. |last6=Ansdell |first6=Megan |last7=Dalba |first7=Paul A. |last8=Swift |first8=Jonathan J. |last9=Hadden |first9=Sam |date=2017-05-25 |title=The Gold Standard: Accurate Stellar and Planetary Parameters for Eight Kepler M dwarf Systems Enabled by Parallaxes |journal=The Astronomical Journal |volume=153 |issue=6 |pages=267 |doi=10.3847/1538-3881/aa7140 |arxiv=1705.01545 |bibcode=2017AJ....153..267M |s2cid=119325474 |issn=1538-3881 |doi-access=free }}</ref>
|-
|{{nowrap|[[EZ Aquarii]] A}} {{nowrap|''(Luyten 789-6 A)''}}
|121,750
|
|<ref name=":16">{{Cite journal |last=Routley |first=Nick |date=June 26, 2020 |title=The 44 Closest Stars and How They Compare to our Sun |url=https://www.visualcapitalist.com/the-44-closest-stars-and-how-they-compare-to-our-sun/ |journal=Visual Capitalist}}</ref>
|-
|[[HW Virginis]] B
|121,835
|
|<ref name="Brown-Sevilla 2122–2135">{{Cite journal |last1=Brown-Sevilla |first1=S. B. |last2=Nascimbeni |first2=V. |last3=Borsato |first3=L. |last4=Tartaglia |first4=L. |last5=Nardiello |first5=D. |last6=Granata |first6=V. |last7=Libralato |first7=M. |last8=Damasso |first8=M. |last9=Piotto |first9=G. |last10=Pollacco |first10=D. |last11=West |first11=R. G. |last12=Colombo |first12=L. S. |last13=Cunial |first13=A. |last14=Piazza |first14=G. |last15=Scaggiante |first15=F. |date=2021-07-19 |title=A new photometric and dynamical study of the eclipsing binary star HW Virginis |journal=Monthly Notices of the Royal Astronomical Society |volume=506 |issue=2 |pages=2122–2135 |doi=10.1093/mnras/stab1843 |doi-access=free |arxiv=2106.15632 |issn=0035-8711}}</ref>
|-
|[[Gliese 1151]]
|123,900
|Has one confirmed exoplanet
|<ref>{{Cite journal |last1=Blanco-Pozo |first1=J. |last2=Perger |first2=M. |last3=Damasso |first3=M. |last4=Escudé |first4=G. Anglada |last5=Ribas |first5=I. |last6=Baroch |first6=D. |last7=Caballero |first7=J. A. |last8=Cifuentes |first8=C. |last9=Jeffers |first9=S. V. |last10=Lafarga |first10=M. |last11=Kaminski |first11=A. |last12=Kaur |first12=S. |last13=Nagel |first13=E. |last14=Perdelwitz |first14=V. |last15=Pérez-Torres |first15=M. |date=March 2023 |title=The CARMENES search for exoplanets around M dwarfs. A long-period planet around GJ 1151 measured with CARMENES and HARPS-N data |journal=Astronomy & Astrophysics |volume=671 |pages=A50 |doi=10.1051/0004-6361/202245053 |arxiv=2301.04442 |bibcode=2023A&A...671A..50B |issn=0004-6361|doi-access=free }}</ref>
|-
|[[AB Doradus]] C
|124,100
|Very low-mass star ({{solar mass|0.09}})
|<ref>{{Cite journal |last1=Close |first1=Laird M. |last2=Thatte |first2=Niranjan |last3=Nielsen |first3=Eric L. |last4=Abuter |first4=Roberto |last5=Clarke |first5=Fraser |last6=Tecza |first6=Matthias |date=2007-08-01 |title=New Photometry and Spectra of AB Doradus C: An Accurate Mass Determination of a Young Low-Mass Object with Theoretical Evolutionary Tracks |url=https://ui.adsabs.harvard.edu/abs/2007ApJ...665..736C |journal=The Astrophysical Journal |volume=665 |issue=1 |pages=736–743 |doi=10.1086/518207 |arxiv=astro-ph/0703564 |bibcode=2007ApJ...665..736C |issn=0004-637X}}</ref>{{efn | Applying the [[Stefan–Boltzmann law]] with a nominal [[sun|solar]] [[effective temperature]] of 5,772&nbsp;[[Kelvin|K]]:
:<math>\sqrt{\biggl(\frac{5,772}{2,925}\biggr)^4 \cdot 0.0021} = 0.1784\ R_\odot</math>.}}
|-
|[[Groombridge 34|GQ And]] ''(Groombridge 34 B)''
|125,200
|
|<ref>{{Cite journal |last1=Pinamonti |first1=M. |last2=Damasso |first2=M. |last3=Marzari |first3=F. |last4=Sozzetti |first4=A. |last5=Desidera |first5=S. |last6=Maldonado |first6=J. |last7=Scandariato |first7=G. |last8=Affer |first8=L. |last9=Lanza |first9=A. F. |last10=Bignamini |first10=A. |last11=Bonomo |first11=A. S. |last12=Borsa |first12=F. |last13=Claudi |first13=R. |last14=Cosentino |first14=R. |last15=Giacobbe |first15=P. |date=September 2018 |title=The HADES RV Programme with HARPS-N@TNG VIII. Gl15A: A multiple wide planetary system sculpted by binary interaction |journal=Astronomy & Astrophysics |volume=617 |pages=A104 |doi=10.1051/0004-6361/201732535 |arxiv=1804.03476 |bibcode=2018A&A...617A.104P |issn=0004-6361|doi-access=free }}</ref>
|-
|[[Wolf 1069]]
|126,130
|Has one confirmed potentially habitable exoplanet
|<ref>{{Cite journal |last1=Kossakowski |first1=D. |last2=Kürster |first2=M. |last3=Trifonov |first3=T. |last4=Henning |first4=Th |last5=Kemmer |first5=J. |last6=Caballero |first6=J. A. |last7=Burn |first7=R. |last8=Sabotta |first8=S. |last9=Crouse |first9=J. S. |last10=Fauchez |first10=T. J. |last11=Nagel |first11=E. |last12=Kaminski |first12=A. |last13=Herrero |first13=E. |last14=Rodríguez |first14=E. |last15=González-Álvarez |first15=E. |date=February 2023 |title=The CARMENES search for exoplanets around M dwarfs, Wolf 1069 b: Earth-mass planet in the habitable zone of a nearby, very low-mass star |journal=Astronomy & Astrophysics |volume=670 |pages=A84 |doi=10.1051/0004-6361/202245322 |arxiv=2301.02477 |bibcode=2023A&A...670A..84K |issn=0004-6361}}</ref>
|-
|[[HW Virginis]] A
|127,404.6
|[[Subdwarf B star|B-type subdwarf]]
|
|<ref name="Brown-Sevilla 2122–2135" />
|-
|[[Gliese 3323]]
|129,539.5
| rowspan="6" |[[Red dwarf]]
|Has two confirmed exoplanets
|<ref name=":8">{{Cite journal |last1=Schweitzer |first1=Andreas |last2=Passegger |first2=V. M. |last3=Cifuentes |first3=C. |last4=Bejar |first4=V. J. S. |last5=Cortes-Contreras |first5=M. |last6=Caballero |first6=J. A. |last7=del Burgo |first7=C. |last8=Czesla |first8=S. |last9=Kuerster |first9=M. |last10=Montes |first10=D. |last11=Osorio |first11=M. R. Zapatero |last12=Ribas |first12=I. |last13=Reiners |first13=A. |last14=Quirrenbach |first14=A. |last15=Amado |first15=P. J. |date=May 2019 |title=The CARMENES search for exoplanets around M dwarfs: Different roads to radii and masses of the target stars |journal=Astronomy & Astrophysics |volume=625 |pages=A68 |arxiv=1904.03231 |bibcode=2019A&A...625A..68S |doi=10.1051/0004-6361/201834965 |issn=0004-6361}}</ref>
|-
|[[Barnard's Star]]
|130,100
|The star with the highest proper motion,<ref>{{Cite journal |last1=Vallenari |first1=A. |last2=Brown |first2=A. G. A. |last3=Prusti |first3=T. |date=2022-06-13 |title=Gaia Data Release 3. Summary of the content and survey properties |url=https://www.aanda.org/articles/aa/abs/forth/aa43940-22/aa43940-22.html |journal=Astronomy & Astrophysics |volume=674 |pages=A1 |language=en |doi=10.1051/0004-6361/202243940 |s2cid=244398875 |issn=0004-6361|arxiv=2208.00211 |bibcode=2023A&A...674A...1G }}</ref> and the second-nearest star system to the Solar system. Has a planet, [[Barnard b|Barnard's Star b / Barnard b]].<ref>{{cite journal |last1=González Hernández |first1=J. I. |last2=Suárez Mascareño |first2=A. |last3=Silva |first3=A. M. |last4=Stefanov |first4=A. K. |last5=Faria |first5=J. P. |last6=Tabernero |first6=H. M. |last7=Sozzetti |first7=A. |last8=Rebolo |first8=R. |last9=Pepe |first9=F. |last10=Santos |first10=N. C. |last11=Cristiani |first11=S. |last12=Lovis |first12=C. |last13=Dumusque |first13=X. |last14=Figueira |first14=P. |last15=Lillo-Box |first15=J. |display-authors=1 |date=October 2024 |title=A sub-Earth-mass planet orbiting Barnard's star |journal=Astronomy & Astrophysics |volume=690 |arxiv=2410.00569 |bibcode=2024A&A...690A..79G |doi=10.1051/0004-6361/202451311 |id=A79 |first16=N. |last16=Nari |first17=S. |last17=Benatti |first18=M. J. |last18=Hobson |first19=A. |last19=Castro-González |first20=R. |last20=Allart |first21=V. M. |last21=Passegger |first22=M.-R. |last22=Zapatero Osorio |first23=V. |last23=Adibekyan |first24=Y. |last24=Alibert |first25=C. |last25=Allende Prieto |first26=F. |last26=Bouchy |first27=M. |last27=Damasso |first28=V. |last28=D'Odorico |first29=P. |last29=Di Marcantonio |first30=D. |last30=Ehrenreich |first31=G. |last31=Lo Curto |first32=R. |last32=Génova Santos |first33=C. J. A. P. |last33=Martins |first34=A. |last34=Mehner |first35=G. |last35=Micela |first36=P. |last36=Molaro |first37=N. |last37=Nunes15 |first38=E. |last38=Palle |first39=S. G. |last39=Sousa |first40=S. |last40=Udry|pages=A79 }}</ref>
|<ref name=":3" />
|-
|{{nowrap|[[LHS 3844|Batsũ̀]] ''(LHS 3844)''}}
|131,500
|Has one confirmed exoplanet
|<ref>{{Cite journal |last1=Vanderspek |first1=Roland |last2=Huang |first2=Chelsea X. |last3=Vanderburg |first3=Andrew |last4=Ricker |first4=George R. |last5=Latham |first5=David W. |last6=Seager |first6=Sara |last7=Winn |first7=Joshua N. |last8=Jenkins |first8=Jon M. |last9=Burt |first9=Jennifer |last10=Dittmann |first10=Jason |last11=Newton |first11=Elisabeth |last12=Quinn |first12=Samuel N. |last13=Shporer |first13=Avi |last14=Charbonneau |first14=David |last15=Irwin |first15=Jonathan |date=2019-01-25 |title=TESS Discovery of an ultra-short-period planet around the nearby M dwarf LHS 3844 |journal=The Astrophysical Journal |volume=871 |issue=2 |pages=L24 |doi=10.3847/2041-8213/aafb7a |arxiv=1809.07242 |bibcode=2019ApJ...871L..24V |issn=2041-8213 |doi-access=free }}</ref>
|-
|[[Ross 248]]
|132,200
|Tenth-nearest star system to the Solar System.
|<ref name=":1" />
|-
|[[GJ 1128|Gliese 1128]]
|132,200
|
|<ref>{{Cite journal |last1=Houdebine |first1=Eric R. |last2=Mullan |first2=D. J. |last3=Doyle |first3=J. G. |last4=de La Vieuville |first4=Geoffroy |last5=Butler |first5=C. J. |last6=Paletou |first6=F. |date=2019-07-10 |title=The Mass-Activity relationships in M and K dwarfs. I. Stellar parameters of our sample of M and K dwarfs |journal=The Astronomical Journal |volume=158 |issue=2 |pages=56 |doi=10.3847/1538-3881/ab23fe |doi-access=free |arxiv=1905.07921 |bibcode=2019AJ....158...56H |issn=1538-3881}}</ref>
|-
|[[Alpha Mensae]] B
|132,200
|
|<ref>{{Cite journal |last1=Chontos |first1=Ashley |last2=Huber |first2=Daniel |last3=Berger |first3=Travis A. |last4=Kjeldsen |first4=Hans |last5=Serenelli |first5=Aldo M. |last6=Aguirre |first6=Victor Silva |last7=Ball |first7=Warrick H. |last8=Basu |first8=Sarbani |last9=Bedding |first9=Timothy R. |last10=Chaplin |first10=William J. |last11=Claytor |first11=Zachary R. |last12=Corsaro |first12=Enrico |last13=García |first13=Rafael A. |last14=Howell |first14=Steve B. |last15=Lundkvist |first15=Mia S. |date=2021-12-01 |title=TESS Asteroseismology of $\alpha$ Mensae: Benchmark Ages for a G7 Dwarf and its M-dwarf Companion |journal=The Astrophysical Journal |volume=922 |issue=2 |pages=229 |doi=10.3847/1538-4357/ac1269 |arxiv=2012.10797 |bibcode=2021ApJ...922..229C |issn=0004-637X|doi-access=free }}</ref>
|-
|[[WD 2134−125]], central star of {{Ill|NGC 7094|fr}}
|{{convert|{{solar radius calculator|type=logLT|3.77|115000|decimals=8}}|solar radius|km|disp=number|sigfig=3}}
|[[White dwarf]]
|
|<ref>{{Cite journal |last1=Löbling |first1=L |last2=Rauch |first2=T |last3=Miller Bertolami |first3=M M |last4=Todt |first4=H |last5=Friederich |first5=F |last6=Ziegler |first6=M |last7=Werner |first7=K |last8=Kruk |first8=J W |date=2019-10-11 |title=Spectral analysis of the hybrid PG 1159-type central stars of the planetary nebulae Abell 43 and NGC 7094 |url=https://academic.oup.com/mnras/article/489/1/1054/5538811 |journal=Monthly Notices of the Royal Astronomical Society |volume=489 |issue=1 |pages=1054–1071 |doi=10.1093/mnras/stz1994 |doi-access=free |issn=0035-8711|arxiv=1907.07049 }}</ref>{{efn|Applying the [[Stefan–Boltzmann law]] with a nominal [[sun|solar]] [[effective temperature]] of 5,772&nbsp;[[Kelvin|K]]:
:<math>\sqrt{\biggl(\frac{5,772}{115,000}\biggr)^4 \cdot 10^{3.77}} = 0.1933\ R_\odot</math>.}}
|-
|[[Ross 128]]
|136,844
| rowspan="4" |[[Red dwarf]]
|Has one confirmed potentially habitable exoplanet
|<ref>{{Cite journal |last1=Mann |first1=Andrew W. |last2=Feiden |first2=Gregory A. |last3=Gaidos |first3=Eric |last4=Boyajian |first4=Tabetha |last5=von Braun |first5=Kaspar |date=2015-05-01 |title=How to Constrain Your M Dwarf: measuring effective temperature, bolometric luminosity, mass, and radius |journal=The Astrophysical Journal |volume=804 |issue=1 |pages=64 |doi=10.1088/0004-637X/804/1/64 |arxiv=1501.01635 |bibcode=2015ApJ...804...64M |s2cid=19269312 |issn=0004-637X}}</ref>
|-
|[[LTT 1445]] C
|137,050
|
|<ref name="Winters 152">{{Cite journal |last1=Winters |first1=Jennifer G. |last2=Medina |first2=Amber A. |last3=Irwin |first3=Jonathan M. |last4=Charbonneau |first4=David |last5=Astudillo-Defru |first5=Nicola |last6=Horch |first6=Elliott P. |last7=Eastman |first7=Jason D. |last8=Vrijmoet |first8=Eliot |last9=Henry |first9=Todd J. |last10=Diamond-Lowe |first10=Hannah |last11=Winston |first11=Elaine |last12=Barclay |first12=Thomas |last13=Bonfils |first13=Xavier |last14=Ricker |first14=George R. |last15=Vanderspek |first15=Roland |date=2019-09-23 |title=Three Red Suns in the Sky: A Transiting, Terrestrial Planet in a Triple M Dwarf System at 6.9 Parsecs |journal=The Astronomical Journal |volume=158 |issue=4 |pages=152 |doi=10.3847/1538-3881/ab364d |arxiv=1906.10147 |issn=1538-3881|doi-access=free |bibcode=2019AJ....158..152W }}</ref>
|-
|[[Ross 154]]
|139,140
|Ninth-nearest star system to our Solar System.
|<ref name=":3" />
|-
|[[Gliese 1062]]
|141,000
|Other sources cites 258,800&nbsp;km (0.372 {{Solar radius|link=y}})<ref>{{Cite journal |last=Houdebine |first=E. R. |date=2010-09-01 |title=Observation and modelling of main-sequence star chromospheres - XIV. Rotation of dM1 stars |journal=Monthly Notices of the Royal Astronomical Society |volume=407 |issue=3 |pages=1657–1673 |doi=10.1111/j.1365-2966.2010.16827.x |doi-access=free |bibcode=2010MNRAS.407.1657H |issn=0035-8711}}</ref> and 285,935&nbsp;km (0.411 {{Solar radius}})<ref>{{Cite journal |last=Houdebine |first=E. R. |date=2010-08-25 |title=Observation and modelling of main-sequence star chromospheres - XIV. Rotation of dM1 stars★ |journal=Monthly Notices of the Royal Astronomical Society |volume=407 |issue=3 |pages=1657–1673 |doi=10.1111/j.1365-2966.2010.16827.x |doi-access=free |bibcode=2010MNRAS.407.1657H |issn=0035-8711}}</ref>
|<ref>{{Cite journal |last1=Kesseli |first1=Aurora Y. |last2=Kirkpatrick |first2=J. Davy |last3=Fajardo-Acosta |first3=Sergio B. |last4=Penny |first4=Matthew T. |last5=Gaudi |first5=B. Scott |last6=Veyette |first6=Mark |last7=Boeshaar |first7=Patricia C. |last8=Henderson |first8=Calen B. |last9=Cushing |first9=Michael C. |last10=Calchi-Novati |first10=Sebastiano |last11=Shvartzvald |first11=Yossi |last12=Muirhead |first12=Philip S. |date=2019-01-21 |title=Radii of 88 M Subdwarfs and Updated Radius Relations for Low-Metallicity M Dwarf Stars |journal=The Astronomical Journal |volume=157 |issue=2 |pages=63 |doi=10.3847/1538-3881/aae982 |doi-access=free |arxiv=1810.07702 |bibcode=2019AJ....157...63K |issn=1538-3881}}</ref>
|-
|[[Kepler-70]]
|141,225
|[[Subdwarf B star|B-type subdwarf]]
|Has two unconfirmed exoplanets, which may be the hottest exoplanets known.
|<ref>{{Cite encyclopedia |last=DEDIEU |first=cyril |title=Notes for Planet KOI-55 b |url=https://exoplanet.eu/catalog/koi_55_b--1037/ |archive-url=https://web.archive.org/web/20231222025555/https://exoplanet.eu/catalog/koi_55_b--1037/ |archive-date=2023-12-22  |url-status=live |encyclopedia=[[Extrasolar Planets Encyclopaedia]] |access-date=2022-11-12 }}</ref>
|-
|[[RR Caeli]] red dwarf
|141,225
| rowspan="6" |[[Red dwarf]]
|
|
|-
|[[Gliese 1214]]
|141,922
|Has a confirmed exoplanet
|<ref name=":3" />
|-
|[[Gliese 754]]
|142,618.5
|
|<ref>{{Cite journal |last1=Newton |first1=Elisabeth R. |last2=Mondrik |first2=Nicholas |last3=Irwin |first3=Jonathan |last4=Winters |first4=Jennifer G. |last5=Charbonneau |first5=David |date=2018-10-18 |title=New rotation period measurements for M dwarfs in the southern hemisphere: an abundance of slowly rotating, fully convective stars |journal=The Astronomical Journal |volume=156 |issue=5 |pages=217 |doi=10.3847/1538-3881/aad73b |arxiv=1807.09365 |bibcode=2018AJ....156..217N |s2cid=119209638 |issn=1538-3881 |doi-access=free }}</ref>
|-
|[[LHS 1140]]
|142,618.5
|Has two confirmed exoplanets
|<ref name=":3" />
|-
|[[EZ Aquarii]] B {{Nowrap|''(Luyten 789-6 B)''}}
|146,100
|
|<ref>{{Cite journal |last1=Torres |first1=G. |last2=Andersen |first2=J. |last3=Gimenez |first3=A. |date=February 2010 |title=Accurate masses and radii of normal stars: modern results and applications |journal=The Astronomy and Astrophysics Review |volume=18 |issue=1–2 |pages=67–126 |doi=10.1007/s00159-009-0025-1 |issn=0935-4956|arxiv=0908.2624 |bibcode=2010A&ARv..18...67T }}</ref>
|-
|[[Gliese 1132]]
|149,575
|Has two confirmed exoplanets
|<ref name=":3" />
|-
|[[LSR J1835+3259]]
|150,133
| rowspan="2" |[[Brown dwarf]]
|
|<ref>{{Cite journal |last1=Berdyugina |first1=S. V. |last2=Harrington |first2=D. M. |last3=Kuzmychov |first3=O. |last4=Kuhn |first4=J. R. |last5=Hallinan |first5=G. |last6=Kowalski |first6=A. F. |last7=Hawley |first7=S. L. |date=2017-09-20 |title=First Detection of a Strong Magnetic Field on a Bursty Brown Dwarf: Puzzle Solved |journal=The Astrophysical Journal |volume=847 |issue=1 |pages=61 |doi=10.3847/1538-4357/aa866b |arxiv=1709.02861 |bibcode=2017ApJ...847...61B |s2cid=118904301 |issn=1538-4357 |doi-access=free }}</ref>
|-
|{{nowrap|[[CT Chamaeleontis]] B ''(CT Cha B)''}}
|157,300
|Either [[exoplanet|planet]] or brown dwarf
|<ref>{{Cite Exoplanet Archive|title=CT Cha|access-date=May 30, 2024}}</ref>
|-
|[[Fomalhaut]] C
|160,000
|[[Red dwarf]]
|
|<ref>{{Cite journal |last1=Mamajek |first1=Eric E. |last2=Bartlett |first2=Jennifer L. |last3=Seifahrt |first3=Andreas |last4=Henry |first4=Todd J. |last5=Dieterich |first5=Sergio B. |last6=Lurie |first6=John C. |last7=Kenworthy |first7=Matthew A. |last8=Jao |first8=Wei-Chun |last9=Riedel |first9=Adric R. |last10=Subasavage |first10=John P. |last11=Winters |first11=Jennifer G. |last12=Finch |first12=Charlie T. |last13=Ianna |first13=Philip A. |last14=Bean |first14=Jacob |date=2013-12-01 |title=The Solar Neighborhood. XXX. Fomalhaut C |url=https://ui.adsabs.harvard.edu/abs/2013AJ....146..154M |journal=The Astronomical Journal |volume=146 |issue=6 |pages=154 |doi=10.1088/0004-6256/146/6/154 |arxiv=1310.0764 |bibcode=2013AJ....146..154M |issn=0004-6256}}</ref>{{efn | Applying the [[Stefan–Boltzmann law]] with a nominal [[sun|solar]] [[effective temperature]] of 5,772&nbsp;[[Kelvin|K]]:
:<math>\sqrt{\biggl(\frac{5,772}{3,132}\biggr)^4 \cdot 0.004603} = 0.23\ R_\odot</math>.}}
|-
|[[V391 Pegasi]]
|160,000
|[[Subdwarf B star|B-type subdwarf]]
|Has one exoplanet candidate
|<ref>{{Cite journal |last1=Silvotti |first1=R. |last2=Schuh |first2=S. |last3=Kim |first3=S.-L. |last4=Lutz |first4=R. |last5=Reed |first5=M. |last6=Benatti |first6=S. |last7=Janulis |first7=R. |last8=Lanteri |first8=L. |last9=Ostensen |first9=R. |last10=Marsh |first10=T. R. |last11=Dhillon |first11=V. S. |last12=Paparo |first12=M. |last13=Molnar |first13=L. |date=March 2018 |title=The sdB pulsating star V391 Peg and its putative giant planet revisited after 13 years of time-series photometric data |journal=Astronomy & Astrophysics |volume=611 |pages=A85 |doi=10.1051/0004-6361/201731473 |arxiv=1711.10942 |bibcode=2018A&A...611A..85S |issn=0004-6361}}</ref>
|-
|[[Kepler-1649]]
|161,400
| rowspan="3" |[[Red dwarf]]
|Has two confirmed exoplanets
|<ref>{{Cite web |title=Kepler-1649 {{!}} NASA Exoplanet Archive |url=https://exoplanetarchive.ipac.caltech.edu/overview/Kepler-1649 |access-date=2023-01-15 |website=exoplanetarchive.ipac.caltech.edu}}</ref>
|-
|[[LTT 1445]] B
|164,185
|
|<ref name="Winters 152" />
|-
|[[CM Draconis]] B ''(CM Dra B)''
|166,700
|
|<ref>{{Cite journal |last1=Morales |first1=J. C. |last2=Ribas |first2=I. |last3=Jordi |first3=C. |last4=Torres |first4=G. |last5=Gallardo |first5=J. |last6=Guinan |first6=E. F. |last7=Charbonneau |first7=D. |last8=Wolf |first8=M. |last9=Latham |first9=D. W. |last10=Anglada-Escudé |first10=G. |last11=Bradstreet |first11=D. H. |last12=Everett |first12=M. E. |last13=O'Donovan |first13=F. T. |last14=Mandushev |first14=G. |last15=Mathieu |first15=R. D. |date=2009-02-01 |title=Absolute properties of the low-mass eclipsing binary CM Draconis |journal=The Astrophysical Journal |volume=691 |issue=2 |pages=1400–1411 |doi=10.1088/0004-637X/691/2/1400 |arxiv=0810.1541 |bibcode=2009ApJ...691.1400M |s2cid=3752277 |issn=0004-637X}}</ref>
|-
|[[Kepler-429]]
|167,000
|[[Subdwarf B star|B-type subdwarf]]
|Has three exoplanet candidates
|<ref>{{Cite journal |last1=Mathur |first1=Savita |last2=Huber |first2=Daniel |last3=Batalha |first3=Natalie M. |last4=Ciardi |first4=David R. |last5=Bastien |first5=Fabienne A. |last6=Bieryla |first6=Allyson |last7=Buchhave |first7=Lars A. |last8=Cochran |first8=William D. |last9=Endl |first9=Michael |last10=Esquerdo |first10=Gilbert A. |last11=Furlan |first11=Elise |last12=Howard |first12=Andrew W. |last13=Howell |first13=Steve B. |last14=Isaacson |first14=Howard |last15=Latham |first15=David W. |date=2017-03-30 |title=Revised Stellar Properties of Kepler Targets for the Q1-17 (DR25) Transit Detection Run |journal=The Astrophysical Journal Supplement Series |volume=229 |issue=2 |pages=30 |doi=10.3847/1538-4365/229/2/30 |doi-access=free |arxiv=1609.04128 |bibcode=2017ApJS..229...30M |issn=1538-4365}}</ref>
|-
|[[Kruger 60]] B
|167,000
|rowspan="3"|[[Red dwarf]]
|
|<ref name=":2">{{Cite journal |last1=Fracassini |first1=L. E. Pasinetti |last2=Pastori |first2=L. |last3=Covino |first3=S. |last4=Pozzi |first4=A. |date=February 2001 |title=Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third Edition - Comments and Statistics |journal=Astronomy and Astrophysics |volume=367 |issue=2 |pages=521–524 |doi=10.1051/0004-6361:20000451 |arxiv=astro-ph/0012289 |bibcode=2001A&A...367..521P |s2cid=425754 |issn=0004-6361}}</ref>
|-
|[[Ross 695]]
|167,000
|
|<ref name=":10">{{Cite journal |last1=Maldonado |first1=J. |last2=Affer |first2=L. |last3=Micela |first3=G. |last4=Scandariato |first4=G. |last5=Damasso |first5=M. |last6=Stelzer |first6=B. |last7=Barbieri |first7=M. |last8=Bedin |first8=L. R. |last9=Biazzo |first9=K. |last10=Bignamini |first10=A. |last11=Borsa |first11=F. |last12=Claudi |first12=R. U. |last13=Covino |first13=E. |last14=Desidera |first14=S. |last15=Esposito |first15=M. |date=May 2015 |title=Stellar parameters of early M dwarfs from ratios of spectral features at optical wavelengths |journal=Astronomy & Astrophysics |volume=577 |pages=A132 |doi=10.1051/0004-6361/201525797 |arxiv=1503.03010 |bibcode=2015A&A...577A.132M |issn=0004-6361|doi-access=free }}</ref>
|-
|[[TOI-715]]
|167,000
|Has one confirmed, potentially habitable exoplanet
|<ref>{{Cite journal |last1=Dransfield |first1=Georgina |last2=Timmermans |first2=Mathilde |last3=Triaud |first3=Amaury H. M. J. |last4=Dévora-Pajares |first4=Martín |last5=Aganze |first5=Christian |last6=Barkaoui |first6=Khalid |last7=Burgasser |first7=Adam J. |last8=Collins |first8=Karen A. |last9=Cointepas |first9=Marion |last10=Ducrot |first10=Elsa |last11=Günther |first11=Maximilian N. |last12=Howell |first12=Steve B. |last13=Murray |first13=Catriona A. |last14=Niraula |first14=Prajwal |last15=Rackham |first15=Benjamin V. |date=2024-01-01 |title=A 1.55 R⊕ habitable-zone planet hosted by TOI-715, an M4 star near the ecliptic South Pole |journal=Monthly Notices of the Royal Astronomical Society |volume=527 |issue=1 |pages=35–52 |doi=10.1093/mnras/stad1439 |doi-access=free |arxiv=2305.06206 |bibcode=2024MNRAS.527...35D |issn=0035-8711}}</ref>
|-
|[[2M1207]] A
|173,925
|[[Brown dwarf]]
|Has one confirmed exoplanet
|<ref>{{Cite journal |last1=Mohanty |first1=Subhanjoy |last2=Jayawardhana |first2=Ray |last3=Huélamo |first3=Nuria |last4=Mamajek |first4=Eric |date=2007-03-01 |title=The Planetary Mass Companion 2MASS 1207-3932B: Temperature, Mass, and Evidence for an Edge-on Disk |journal=The Astrophysical Journal |volume=657 |issue=2 |pages=1064–1091 |doi=10.1086/510877 |arxiv=astro-ph/0610550 |bibcode=2007ApJ...657.1064M |issn=0004-637X|doi-access=free }}</ref>
|-
| [[CM Draconis]] A ''(CM Dra A)''
| 176,000
| rowspan="74" |[[Red dwarf]]
|
| <ref name="2009ApJ...691.1400M">{{cite journal |author1=J.C. Morales |author2=I. Ribas |author3=C. Jordi |author4=G. Torres |author5=J. Gallardo |author6=E.F. Guinan |author7=D. Charbonneau |author8=M. Wolf |author9=D.W. Latham |author10=G. Anglada-Escudé |author11=D.H. Bradstreet |author12=M.E. Everett |author13=F.T. O'Donovan |author14=G. Mandushev |author15=R.D. Mathieu |year=2009 |title=Absolute properties of the low-mass eclipsing binary CM Draconis |journal=The Astrophysical Journal |publication-date=February 2009 |volume=691 |issue=2 |pages=1400–1411 |arxiv=0810.1541 |bibcode=2009ApJ...691.1400M |doi=10.1088/0004-637X/691/2/1400 |orig-year=8 October 2008 |s2cid=3752277}}</ref>
|-
|[[DG Canum Venaticorum]]
|176,000
|
|<ref>{{Cite journal |last1=Houdebine |first1=E. R. |last2=Mullan |first2=D. J. |last3=Paletou |first3=F. |last4=Gebran |first4=M. |date=2016-05-01 |title=Rotation-Activity Correlations in K and M Dwarfs. I. Stellar Parameters and Compilations of v sin I and P/sin I for a Large Sample of Late-K and M Dwarfs |journal=The Astrophysical Journal |volume=822 |issue=2 |pages=97 |doi=10.3847/0004-637X/822/2/97 |doi-access=free |arxiv=1604.07920 |bibcode=2016ApJ...822...97H |issn=0004-637X}}</ref>
|-
|[[Gliese 625]]
|177,400
|
|<ref>{{Cite journal |last1=Khata |first1=Dhrimadri |last2=Mondal |first2=Soumen |last3=Das |first3=Ramkrishna |last4=Ghosh |first4=Supriyo |last5=Ghosh |first5=Samrat |date=2020-04-01 |title=Understanding the physical properties of young M dwarfs: NIR spectroscopic studies |journal=Monthly Notices of the Royal Astronomical Society |volume=493 |issue=3 |pages=4533–4550 |doi=10.1093/mnras/staa427 |doi-access=free |arxiv=2002.05762 |bibcode=2020MNRAS.493.4533K |issn=0035-8711}}</ref>
|-
|[[Gliese 12]]
|182,065
|Has one known exoplanet
|<ref>{{Cite journal |last1=Kuzuhara |first1=Masayuki |last2=Fukui |first2=Akihiko |last3=Livingston |first3=John H. |last4=Caballero |first4=José A. |last5=de Leon |first5=Jerome P. |last6=Hirano |first6=Teruyuki |last7=Kasagi |first7=Yui |last8=Murgas |first8=Felipe |last9=Narita |first9=Norio |last10=Omiya |first10=Masashi |last11=Orell-Miquel |first11=Jaume |last12=Palle |first12=Enric |last13=Changeat |first13=Quentin |last14=Esparza-Borges |first14=Emma |last15=Harakawa |first15=Hiroki |date=2024-05-23 |title=Gliese 12 b: A Temperate Earth-sized Planet at 12 pc Ideal for Atmospheric Transmission Spectroscopy |journal=The Astrophysical Journal Letters |volume=967 |issue=2 |pages=L21 |doi=10.3847/2041-8213/ad3642 |doi-access=free |arxiv=2405.14708 |bibcode=2024ApJ...967L..21K |issn=2041-8205}}</ref>
|-
|[[AM Herculis]] red dwarf
|180,882
|
|<ref>{{Cite journal |last1=Dai |first1=Zhibin |last2=Qian |first2=Shengbang |last3=Li |first3=Linjia |date=2013-08-26 |title=Updated photometry and orbital period analysis for the polar \objectname{am herculis} on the upper edge of the period gap |journal=The Astrophysical Journal |volume=774 |issue=2 |pages=153 |doi=10.1088/0004-637X/774/2/153 |arxiv=1307.5135 |issn=0004-637X|doi-access=free }}</ref>
|-
|[[55 Cancri]] B
|186,447.5
|
|<ref>{{Cite journal |last1=von Braun |first1=Kaspar |last2=Boyajian |first2=Tabetha S. |last3=Brummelaar |first3=Theo A. ten |last4=Kane |first4=Stephen R. |last5=van Belle |first5=Gerard T. |last6=Ciardi |first6=David R. |last7=Raymond |first7=Sean N. |last8=Lopez-Morales |first8=Mercedes |last9=McAlister |first9=Harold A. |last10=Schaefer |first10=Gail |last11=Ridgway |first11=Stephen T. |last12=Sturmann |first12=Laszlo |last13=Sturmann |first13=Judit |last14=White |first14=Russel |last15=Turner |first15=Nils H. |date=2011-10-10 |title=55 Cancri: Stellar Astrophysical Parameters, a Planet in the Habitable Zone, and Implications for the Radius of a Transiting Super-Earth |journal=The Astrophysical Journal |volume=740 |issue=1 |pages=49 |doi=10.1088/0004-637X/740/1/49 |arxiv=1106.1152 |bibcode=2011ApJ...740...49V |s2cid=2856228 |issn=0004-637X}}</ref>
|-
|[[LTT 1445]] A
|188,500
|Has three confirmed exoplanets, one of them is in the habitable zone
|<ref>{{cite journal | arxiv=2307.02970 | author1=Emily K Pass | author2=Jennifer G Winters | last3=Charbonneau | first3=David | last4=Balkanski | first4=Aurelia | last5=Lewis | first5=Nikole | last6=Lally | first6=Maura | author7=Jacob L Bean | last8=Cloutier | first8=Ryan | author9=Jason D Eastman | title=HST/WFC3 Light Curve Supports a Terrestrial Composition for the Closest Exoplanet to Transit an M Dwarf | journal=The Astronomical Journal | date=2023 | volume=166 | issue=4 | page=171 | doi=10.3847/1538-3881/acf561 | bibcode=2023AJ....166..171P | doi-access=free }}</ref>
|-
|[[Struve 2398]] B
|189,925
|
|<ref name=":1" />
|-
|[[Gliese 105]] B ''{{Nowrap|(268 G. Ceti B)}}''
|193,405
|
|<ref name=":1" />
|-
|[[LHS 475]]
|194,030.5
|Has one confirmed exoplanet
|<ref>{{Cite journal |last1=Lustig-Yaeger |first1=J. |last2=Fu |first2=G. |last3=May |first3=E. M. |last4=Ceballos |first4=K. N. Ortiz |last5=Moran |first5=S. E. |last6=Peacock |first6=S. |last7=Stevenson |first7=K. B. |last8=López-Morales |first8=M. |last9=MacDonald |first9=R. J. |last10=Mayorga |first10=L. C. |last11=Sing |first11=D. K. |last12=Sotzen |first12=K. S. |last13=Valenti |first13=J. A. |last14=Adams |first14=J. |last15=Alam |first15=M. K. |date=2023-01-10 |title=A JWST transmission spectrum of the nearby Earth-sized exoplanet LHS 475 B |journal=Nature Astronomy |volume=7 |issue=11 |pages=1317–1328 |doi=10.1038/s41550-023-02064-z |arxiv=2301.04191 |bibcode=2023NatAs...7.1317L }}</ref>
|-
|[[HR 7703]] B
|194,800
|
|<ref name=":2" />
|-
|[[Gliese 445]]
|198,275
|
|<ref>{{Cite journal |last1=Houdebine |first1=Éric R. |last2=Mullan |first2=D. J. |last3=Doyle |first3=J. G. |last4=de La Vieuville |first4=Geoffroy |last5=Butler |first5=C. J. |last6=Paletou |first6=F. |date=2019-07-10 |title=The Mass–Activity Relationships in M and K Dwarfs. I. Stellar Parameters of Our Sample of M and K Dwarfs* |journal=The Astronomical Journal |volume=158 |issue=2 |pages=56 |doi=10.3847/1538-3881/ab23fe |doi-access=free |arxiv=1905.07921 |bibcode=2019AJ....158...56H |issn=0004-6256}}</ref>
|-
|[[Mu Cassiopeiae]] Ab
|201,750
|
|<ref>{{Cite journal |last1=Drummond |first1=Jack D. |last2=Christou |first2=Julian C. |last3=Fugate |first3=Robert Q. |date=1995-09-01 |title=Full Adaptive Optics Images of ADS 9731 and MU Cassiopeiae: Orbits and Masses |url=https://ui.adsabs.harvard.edu/abs/1995ApJ...450..380D |journal=The Astrophysical Journal |volume=450 |pages=380 |doi=10.1086/176148 |bibcode=1995ApJ...450..380D |issn=0004-637X}}</ref>
|-
|| [[Kapteyn's Star]] || 202,448.7 || This is the closest halo star to the Sun. || <ref>{{Cite journal |last1=Guinan |first1=Edward F. |last2=Engle |first2=Scott G. |last3=Durbin |first3=Allyn |date=2016-04-13 |title=Living with a Red Dwarf: Rotation and X-ray and Ultraviolet Properties of the Halo Population Kapteyn's Star |journal=The Astrophysical Journal |volume=821 |issue=2 |pages=81 |doi=10.3847/0004-637X/821/2/81 |arxiv=1602.01912 |bibcode=2016ApJ...821...81G |s2cid=119283541 |issn=1538-4357 |doi-access=free }}</ref>
|-
|[[Stein 2051]] A
|203,150
|
|<ref>{{Cite journal |last1=Khata |first1=Dhrimadri |last2=Mondal |first2=Soumen |last3=Das |first3=Ramkrishna |last4=Ghosh |first4=Supriyo |last5=Ghosh |first5=Samrat |date=2020-04-11 |title=Understanding Physical Properties of Young M-dwarfs: NIR spectroscopic studies |journal=Monthly Notices of the Royal Astronomical Society |volume=493 |issue=3 |pages=4533–4550 |doi=10.1093/mnras/staa427 |doi-access=free |issn=0035-8711|arxiv=2002.05762 |bibcode=2020MNRAS.493.4533K }}</ref>
|-
|[[HN Librae]]
|208,000
|Has one confirmed planet and one unconfirmed
|<ref>{{Cite journal |last1=González-Álvarez |first1=E. |last2=Kemmer |first2=J. |last3=Chaturvedi |first3=P. |last4=Caballero |first4=J. A. |last5=Quirrenbach |first5=A. |last6=Amado |first6=P. J. |last7=Béjar |first7=V. J. S. |last8=Cifuentes |first8=C. |last9=Herrero |first9=E. |last10=Kossakowski |first10=D. |last11=Reiners |first11=A. |last12=Ribas |first12=I. |last13=Rodríguez |first13=E. |last14=Rodríguez-López |first14=C. |last15=Sanz-Forcada |first15=J. |date=July 2023 |title=The CARMENES search for exoplanets around M dwarfs. A sub-Neptunian mass planet in the habitable zone of HN Lib |journal=Astronomy & Astrophysics |volume=675 |pages=A141 |doi=10.1051/0004-6361/202346276 |arxiv=2305.19677 |bibcode=2023A&A...675A.141G |issn=0004-6361}}</ref>
|-
|[[Gliese 402]]
|208,700
|
|
|-
|[[L 98-59]]
|210,800
|Has four confirmed exoplanets and one unconfirmed
|<ref>{{Cite journal |last1=Demangeon |first1=Olivier D. S. |last2=Osorio |first2=M. R. Zapatero |last3=Alibert |first3=Y. |last4=Barros |first4=S. C. C. |last5=Adibekyan |first5=V. |last6=Tabernero |first6=H. M. |last7=Antoniadis-Karnavas |first7=A. |last8=Camacho |first8=J. D. |last9=Mascareño |first9=A. Suárez |last10=Oshagh |first10=M. |last11=Micela |first11=G. |last12=Sousa |first12=S. G. |last13=Lovis |first13=C. |last14=Pepe |first14=F. A. |last15=Rebolo |first15=R. |date=September 2021 |title=Warm terrestrial planet with half the mass of Venus transiting a nearby star |journal=Astronomy & Astrophysics |volume=653 |pages=A41 |doi=10.1051/0004-6361/202140728 |arxiv=2108.03323 |bibcode=2021A&A...653A..41D |issn=0004-6361}}</ref>
|-
|[[Gliese 581]]
|215,650
|Has three confirmed exoplanets
|<ref name=":3" />
|-
|[[40 Eridani]] C
|215,650
|
|<ref>{{Cite web |title=Catalogue of nearest stars until 10pc |url=https://cdsarc.cds.unistra.fr/viz-bin/cat/V/101 |access-date=2023-11-05 |website=cdsarc.cds.unistra.fr |language=en}}</ref>
|-
|[[Wolf 1061]]
|221,900
|Has three confirmed exoplanets
|<ref name=":3" />
|-
|[[Gliese 3929]]
|222,600
|Has two confirmed exoplanets
|<ref>{{Cite journal |last1=Beard |first1=Corey |last2=Robertson |first2=Paul |last3=Kanodia |first3=Shubham |last4=Lubin |first4=Jack |last5=Cañas |first5=Caleb I. |last6=Gupta |first6=Arvind F. |last7=Holcomb |first7=Rae |last8=Jones |first8=Sinclaire |last9=Libby-Roberts |first9=Jessica E. |last10=Lin |first10=Andrea S. J. |last11=Mahadevan |first11=Suvrath |last12=Stefánsson |first12=Guðmundur |last13=Bender |first13=Chad F. |last14=Blake |first14=Cullen H. |last15=Cochran |first15=William D. |date=2022-09-01 |title=GJ 3929: High Precision Photometric and Doppler Characterization of an Exo-Venus and its Hot, Mini-Neptune-mass Companion |journal=The Astrophysical Journal |volume=936 |issue=1 |pages=55 |doi=10.3847/1538-4357/ac8480 |doi-access=free |arxiv=2207.10672 |bibcode=2022ApJ...936...55B |issn=0004-637X}}</ref>
|-
|[[Xi Ursae Majoris]] Ab
|222,600
|
|<ref>{{Cite journal |title=Nearby stars of the Galactic disc and halo – IV |journal=Monthly Notices of the Royal Astronomical Society | year=2008 |doi=10.1111/j.1365-2966.2007.12671.x| last1=Fuhrmann | first1=Klaus | volume=384 | issue=1 | pages=173–224 | bibcode=2008MNRAS.384..173F | s2cid=85444248 | doi-access=free }}</ref>
|-
|[[Kepler-296]] B
|224,000
|
|<ref>{{Cite journal |last1=Barclay |first1=Thomas |last2=Quintana |first2=Elisa V. |last3=Adams |first3=Fred C. |last4=Ciardi |first4=David R. |last5=Huber |first5=Daniel |last6=Foreman-Mackey |first6=Daniel |last7=Montet |first7=Benjamin T. |last8=Caldwell |first8=Douglas |date=2015-08-01 |title=The Five Planets in the Kepler-296 Binary System All Orbit the Primary: A Statistical and Analytical Analysis |url=https://ui.adsabs.harvard.edu/abs/2015ApJ...809....7B |journal=The Astrophysical Journal |volume=809 |issue=1 |pages=7 |doi=10.1088/0004-637X/809/1/7 |arxiv=1505.01845 |bibcode=2015ApJ...809....7B |issn=0004-637X}}</ref>
|-
|[[YZ Canis Minoris]]
|225,400
|
|<ref name="Houdebine 56" />
|-
|[[LHS 1678]]
|228,285
|Has three known exoplanets
|<ref>{{Cite journal |last1=Silverstein |first1=Michele L. |last2=Schlieder |first2=Joshua E. |last3=Barclay |first3=Thomas |last4=Hord |first4=Benjamin J. |last5=Jao |first5=Wei-Chun |last6=Vrijmoet |first6=Eliot Halley |last7=Henry |first7=Todd J. |last8=Cloutier |first8=Ryan |last9=Kostov |first9=Veselin B. |last10=Kruse |first10=Ethan |last11=Winters |first11=Jennifer G. |last12=Irwin |first12=Jonathan M. |last13=Kane |first13=Stephen R. |last14=Stassun |first14=Keivan G. |last15=Huang |first15=Chelsea |date=2022-04-01 |title=The LHS 1678 System: Two Earth-Sized Transiting Planets and an Astrometric Companion Orbiting an M Dwarf Near the Convective Boundary at 20 pc |journal=The Astronomical Journal |volume=163 |issue=4 |pages=151 |doi=10.3847/1538-3881/ac32e3 |doi-access=free |arxiv=2110.12079 |bibcode=2022AJ....163..151S |issn=0004-6256}}</ref>
|-
|[[Wolf 437]] ''(Gar)''
|228,190
|Has one confirmed exoplanet
|<ref>{{Cite journal |last1=Trifonov |first1=T. |last2=Caballero |first2=J. A. |last3=Morales |first3=J. C. |last4=Seifahrt |first4=A. |last5=Ribas |first5=I. |last6=Reiners |first6=A. |last7=Bean |first7=J. L. |last8=Luque |first8=R. |last9=Parviainen |first9=H. |last10=Pallé |first10=E. |last11=Stock |first11=S. |last12=Zechmeister |first12=M. |last13=Amado |first13=P. J. |last14=Anglada-Escudé3 |first14=G. |last15=Azzaro |first15=M. |date=2021-03-05 |title=A nearby transiting rocky exoplanet that is suitable for atmospheric investigation |journal=Science |volume=371 |issue=6533 |pages=1038–1041 |doi=10.1126/science.abd7645 |pmid=33674491 |arxiv=2103.04950 |bibcode=2021Sci...371.1038T |issn=0036-8075}}</ref>
|-
|[[Gliese 1]]
|229,580
|
|<ref>{{Cite journal |last1=Maldonado |first1=J. |last2=Micela |first2=G. |last3=Baratella |first3=M. |last4=D'Orazi |first4=V. |last5=Affer |first5=L. |last6=Biazzo |first6=K. |last7=Lanza |first7=A. F. |last8=Maggio |first8=A. |last9=Hernández |first9=J. I. González |last10=Perger |first10=M. |last11=Pinamonti |first11=M. |last12=Scandariato |first12=G. |last13=Sozzetti |first13=A. |last14=Locci |first14=D. |last15=Di Maio |first15=C. |date=December 2020 |title=HADES RV Programme with HARPS-N at TNG XII. The abundance signature of M dwarf stars with planets |journal=Astronomy & Astrophysics |volume=644 |pages=A68 |doi=10.1051/0004-6361/202039478 |arxiv=2010.14867 |bibcode=2020A&A...644A..68M |issn=0004-6361}}</ref>
|-
|[[Wolf 1130]] A
|229,580
|
|<ref>{{Cite journal |last1=Honaker |first1=Easton J. |last2=Mace |first2=Gregory N. |last3=Han |first3=Eunkyu |last4=Hussaini |first4=Maryam |last5=Lubar |first5=Emily |date=2020-11-01 |title=TESS Photometry of the Precataclysmic Variable Wolf 1130AB |journal=Research Notes of the American Astronomical Society |volume=4 |issue=11 |pages=197 |doi=10.3847/2515-5172/abc6a4 |doi-access=free |bibcode=2020RNAAS...4..197H |issn=2515-5172}}</ref>
|-
|[[Gliese 357]]
|231,650
|Has three confirmed exoplanets
|<ref name=":19" />
|-
|[[Gliese 667]] C
|231,650
|Has two confirmed exoplanets
|<ref name=":3" />
|-
|[[Kepler-47]] B
|235,150
|There are three exoplanets orbiting Kepler-47 B and its companion, Kepler-47 A, in a [[Circumbinary planet|circumbinary]] orbit.
|<ref>{{Cite journal |last1=Orosz |first1=Jerome A. |last2=Welsh |first2=William F. |last3=Carter |first3=Joshua A. |last4=Fabrycky |first4=Daniel C. |last5=Cochran |first5=William D. |last6=Endl |first6=Michael |last7=Ford |first7=Eric B. |last8=Haghighipour |first8=Nader |last9=MacQueen |first9=Phillip J. |last10=Mazeh |first10=Tsevi |last11=Sanchis-Ojeda |first11=Roberto |last12=Short |first12=Donald R. |last13=Torres |first13=Guillermo |last14=Agol |first14=Eric |last15=Buchhave |first15=Lars A. |date=2012-09-21 |title=Kepler-47: A Transiting Circumbinary Multi-Planet System |journal=Science |volume=337 |issue=6101 |pages=1511–1514 |doi=10.1126/science.1228380 |pmid=22933522 |arxiv=1208.5489 |bibcode=2012Sci...337.1511O |issn=0036-8075}}</ref><ref>{{Cite journal |last1=Orosz |first1=Jerome A. |last2=Welsh |first2=William F. |last3=Haghighipour |first3=Nader |last4=Quarles |first4=Billy |last5=Short |first5=Donald R. |last6=Mills |first6=Sean M. |last7=Satyal |first7=Suman |last8=Torres |first8=Guillermo |last9=Agol |first9=Eric |last10=Fabrycky |first10=Daniel C. |last11=Jontof-Hutter |first11=Daniel |last12=Windmiller |first12=Gur |last13=Müller |first13=Tobias W. A. |last14=Hinse |first14=Tobias C. |last15=Cochran |first15=William D. |date=2019-05-01 |title=Discovery of a Third Transiting Planet in the Kepler-47 Circumbinary System |journal=The Astronomical Journal |volume=157 |issue=5 |pages=174 |doi=10.3847/1538-3881/ab0ca0 |doi-access=free |arxiv=1904.07255 |bibcode=2019AJ....157..174O |issn=0004-6256}}</ref>
|-
|[[Luyten's Star]] ''(Gliese 273)''
|243,500
|Has two confirmed exoplanets and other two unconfirmed
|<ref name="apjss141">{{cite journal|title=Radial Velocities for 889 Late-Type Stars|date=August 2002|last1=Nidever|last2=Marcy|last3=Butler|last4=Fischer|last5=Vogt|first1=David L.|first2=Geoffrey W.|first3=R. Paul|first4=Debra A.|first5=Steven S.|journal=The Astrophysical Journal Supplement Series|volume=141|issue=2|pages=503–522|arxiv=astro-ph/0112477|bibcode=2002ApJS..141..503N|doi=10.1086/340570|s2cid=51814894 |display-authors=1}}</ref>
|-
|[[Kruger 60]] A
|243,500
|
|<ref name=":2" />
|-
|[[Struve 2398]] A
|246,300
|
|<ref name=":3" />
|-
|[[EV Lacertae]]
|250,500
|On 25 April 2008, a record-setting [[stellar flare]] was observed on its surface by [[NASA]]'s [[Neil Gehrels Swift Observatory|Swift]], that was thousands of times more powerful than any solar flare.<ref>{{Cite web |title=Pipsqueak Star Unleashes Monster Flare - NASA |url=https://www.nasa.gov/image-article/pipsqueak-star-unleashes-monster-flare/ |access-date=2024-01-12 |language=en-US}}</ref>
|<ref>{{Cite journal |last1=Phan-Bao |first1=N. |last2=Martin |first2=E. L. |last3=Donati |first3=J.-F. |last4=Lim |first4=J. |date=2006-07-20 |title=Magnetic fields in M dwarfs: rapid magnetic field variability in EV Lac |journal=The Astrophysical Journal |volume=646 |issue=1 |pages=L73–L76 |doi=10.1086/506591 |arxiv=astro-ph/0603480 |bibcode=2006ApJ...646L..73P |s2cid=18410819 |issn=0004-637X}}</ref>
|-
|[[Theta Cygni]] B
|250,500
|
|<ref>{{Cite journal |last1=Guzik |first1=J. A. |last2=Houdek |first2=G. |last3=Chaplin |first3=W. J. |last4=Smalley |first4=B. |last5=Kurtz |first5=D. W. |last6=Gilliland |first6=R. L. |last7=Mullally |first7=F. |last8=Rowe |first8=J. F. |last9=Bryson |first9=S. T. |last10=Still |first10=M. D. |last11=Antoci |first11=V. |last12=Appourchaux |first12=T. |last13=Basu |first13=S. |last14=Bedding |first14=T. R. |last15=Benomar |first15=O. |date=2016-10-21 |title=Detection of Solar-Like Oscillations, Observational Constraints, and Stellar Models for $\theta$ Cyg, the Brightest Star Observed by the {\it Kepler} Mission |journal=The Astrophysical Journal |volume=831 |issue=1 |pages=17 |doi=10.3847/0004-637X/831/1/17 |arxiv=1607.01035 |issn=1538-4357 |doi-access=free }}</ref>
|-
|[[Gliese 251]]
|253,235
|Has one confirmed exoplanet
|<ref>{{Cite journal |last1=Stock |first1=S. |last2=Nagel |first2=E. |last3=Kemmer |first3=J. |last4=Passegger |first4=V. M. |last5=Reffert |first5=S. |last6=Quirrenbach |first6=A. |last7=Caballero |first7=J. A. |last8=Czesla |first8=S. |last9=Béjar |first9=V. J. S. |last10=Cardona |first10=C. |last11=Díez-Alonso |first11=E. |last12=Herrero |first12=E. |last13=Lalitha |first13=S. |last14=Schlecker |first14=M. |last15=Tal-Or |first15=L. |date=November 2020 |title=The CARMENES search for exoplanets around M dwarfs. Three temperate to warm super-Earths |journal=Astronomy & Astrophysics |volume=643 |pages=A112 |doi=10.1051/0004-6361/202038820 |arxiv=2010.00474 |bibcode=2020A&A...643A.112S |issn=0004-6361}}</ref>
|-
|[[DT Virginis]] B ''(Ross 458)''
|256,000
|
|<ref>{{Cite journal |last1=Khata |first1=Dhrimadri |last2=Mondal |first2=Soumen |last3=Das |first3=Ramkrishna |last4=Ghosh |first4=Supriyo |last5=Ghosh |first5=Samrat |date=2020-04-11 |title=Understanding Physical Properties of Young M-dwarfs: NIR spectroscopic studies |journal=Monthly Notices of the Royal Astronomical Society |volume=493 |issue=3 |pages=4533–4550 |doi=10.1093/mnras/staa427 |doi-access=free |arxiv=2002.05762 |bibcode=2020MNRAS.493.4533K |issn=0035-8711}}</ref>
|-
|[[AT Microscopii]] B ''(AT Mic B)''
|257,400
|
|<ref name=":7">{{Cite web |title=ISDB search results |url=http://www.stellar-database.com/Scripts/search_star.exe?Name=AT+Microscopii |access-date=2023-02-02 |website=www.stellar-database.com}}</ref>
|-
|[[Regulus]] C
|257,400
|
|<ref>{{Cite journal |last1=Johnson |first1=H. M. |last2=Wright |first2=C. D. |date=1983-11-01 |title=Predicted infrared brightness of stars within 25 parsecs of the sun. |url=https://ui.adsabs.harvard.edu/abs/1983ApJS...53..643J |journal=The Astrophysical Journal Supplement Series |volume=53 |pages=643–711 |doi=10.1086/190905 |bibcode=1983ApJS...53..643J |issn=0067-0049}}</ref>
|-
|[[Gliese 876]] ''(Ross 780)''
|258,800
|Has four confirmed exoplanets
|<ref name=":3" />
|-
|[[LHS 6343]] A ''(KOI-959 A)''
|259,495
|
|<ref name=":9" />
|-
|[[LTT 3780]] ''(TOI-732)''
|260,190
|Has two confirmed exoplanets
|<ref>{{Cite journal |last1=Cloutier |first1=Ryan |last2=Eastman |first2=Jason D. |last3=Rodriguez |first3=Joseph E. |last4=Astudillo-Defru |first4=Nicola |last5=Bonfils |first5=Xavier |last6=Mortier |first6=Annelies |last7=Watson |first7=Christopher A. |last8=Stalport |first8=Manu |last9=Pinamonti |first9=Matteo |last10=Lienhard |first10=Florian |last11=Harutyunyan |first11=Avet |last12=Damasso |first12=Mario |last13=Latham |first13=David W. |last14=Collins |first14=Karen A. |last15=Massey |first15=Robert |date=2020-07-01 |title=A pair of TESS planets spanning the radius valley around the nearby mid-M dwarf LTT 3780 |journal=The Astronomical Journal |volume=160 |issue=1 |pages=3 |doi=10.3847/1538-3881/ab91c2 |doi-access=free |arxiv=2003.01136 |bibcode=2020AJ....160....3C |issn=0004-6256}}</ref>
|-
|[[TOI-270]]
|263,000
|Has three confirmed exoplanets
|<ref>{{Cite journal |last1=Van Eylen |first1=Vincent |last2=Astudillo-Defru |first2=N. |last3=Bonfils |first3=X. |last4=Livingston |first4=J. |last5=Hirano |first5=T. |last6=Luque |first6=R. |last7=Lam |first7=K. W. F. |last8=Justesen |first8=A. B. |last9=Winn |first9=J. N. |last10=Gandolfi |first10=D. |last11=Nowak |first11=G. |last12=Palle |first12=E. |last13=Albrecht |first13=S. |last14=Dai |first14=F. |last15=Estrada |first15=B. Campos |date=2021-08-24 |title=Masses and compositions of three small planets orbiting the nearby M dwarf L231-32 (TOI-270) and the M dwarf radius valley |journal=Monthly Notices of the Royal Astronomical Society |pages=stab2143 |doi=10.1093/mnras/stab2143 |doi-access=free |arxiv=2101.01593 |issn=0035-8711}}</ref>
|-
|[[Gliese 412]] A
|264,400
|
|<ref name=":1" />
|-
|[[KIC 4150611]] Ab2
|264,400
|
|<ref name=kemp/>
|-
|[[Groombridge 34|GX And]] ''(Groombridge 34 A)''
|267,800
|Has two confirmed exoplanets
|<ref name=":3">{{Cite journal |last1=Pineda |first1=J. Sebastian |last2=Youngblood |first2=Allison |last3=France |first3=Kevin |date=2021-09-01 |title=The M-dwarf Ultraviolet Spectroscopic Sample I. Determining Stellar Parameters for Field Stars |journal=The Astrophysical Journal |volume=918 |issue=1 |pages=40 |doi=10.3847/1538-4357/ac0aea |issn=0004-637X|arxiv=2106.07656 |bibcode=2021ApJ...918...40P |s2cid=235435757 |doi-access=free }}</ref>
|-
|[[L 34-26]]
|270,000
|It hosts the exoplanet with the longest known orbital period, [[COCONUTS-2b]], which takes about 1.1 million years to complete an orbit around its star.<ref>{{Cite web |title=Exoplanet-catalog |url=https://exoplanets.nasa.gov/exoplanet-catalog/7945/coconuts-2-b/ |access-date=2023-09-25 |website=Exoplanet Exploration: Planets Beyond our Solar System |language=en}}</ref>
|<ref>{{Cite journal |last1=Zhang |first1=Zhoujian |last2=Liu |first2=Michael C. |last3=Claytor |first3=Zachary R. |last4=Best |first4=William M. J. |last5=Dupuy |first5=Trent J. |last6=Siverd |first6=Robert J. |date=2021-08-01 |title=The Second Discovery from the COol Companions ON Ultrawide orbiTS (COCONUTS) Program: A Cold Wide-Orbit Exoplanet around a Young Field M Dwarf at 10.9 pc |journal=The Astrophysical Journal Letters |volume=916 |issue=2 |pages=L11 |doi=10.3847/2041-8213/ac1123 |arxiv=2107.02805 |issn=2041-8205|doi-access=free |bibcode=2021ApJ...916L..11Z }}</ref>
|-
|[[Gliese 908]] ''(BR Piscium)''
|271,323
|
|<ref name=":10" />
|-
|[[Gliese 1252]]
|272,000
|Has one confirmed exoplanet, an [[Ultra-short period planet|ultra-short-period planet]] with a daytime temperature measured at 1140&nbsp;°C.<ref>{{Cite journal |last1=Crossfield |first1=Ian J. M. |last2=Malik |first2=Matej |last3=Hill |first3=Michelle L. |last4=Kane |first4=Stephen R. |last5=Foley |first5=Bradford |last6=Polanski |first6=Alex S. |last7=Coria |first7=David |last8=Brande |first8=Jonathan |last9=Zhang |first9=Yanzhe |last10=Wienke |first10=Katherine |last11=Kreidberg |first11=Laura |last12=Cowan |first12=Nicolas B. |last13=Dragomir |first13=Diana |last14=Gorjian |first14=Varoujan |last15=Mikal-Evans |first15=Thomas |date=September 2022 |title=GJ 1252b: A Hot Terrestrial Super-Earth with No Atmosphere |journal=The Astrophysical Journal Letters |language=en |volume=937 |issue=1 |pages=L17 |doi=10.3847/2041-8213/ac886b |doi-access=free |arxiv=2208.09479 |bibcode=2022ApJ...937L..17C |issn=2041-8205}}</ref>
|<ref>{{Cite journal |last1=Shporer |first1=Avi |last2=Collins |first2=Karen A. |last3=Astudillo-Defru |first3=Nicola |last4=Irwin |first4=Jonathan |last5=Bonfils |first5=Xavier |last6=Collins |first6=Kevin I. |last7=Matthews |first7=Elisabeth |last8=Winters |first8=Jennifer G. |last9=Anderson |first9=David R. |last10=Armstrong |first10=James D. |last11=Charbonneau |first11=David |last12=Cloutier |first12=Ryan |last13=Daylan |first13=Tansu |last14=Gan |first14=Tianjun |last15=Günther |first15=Maximilian N. |date=2020-02-10 |title=GJ 1252 b: A 1.2 R<sub>⊕</sub> Planet Transiting an M3 Dwarf at 20.4 pc |journal=The Astrophysical Journal Letters |volume=890 |issue=1 |pages=L7 |doi=10.3847/2041-8213/ab7020 |doi-access=free |arxiv=1912.05556 |bibcode=2020ApJ...890L...7S |issn=2041-8205}}</ref>
|-
|[[HIP 79431|Sharjah]] ''(HIP 79431)''
|272,000
|Has one confirmed exoplanet. Other sources cites radius of {{Nowrap|307,500 km}} (0.442 {{Solar radius|link=y}})<ref>{{Cite journal |last1=Tsuji |first1=Takashi |last2=Nakajima |first2=Tadashi |date=2014-10-01 |title=Near Infrared Spectroscopy of M Dwarfs. I. CO Molecule as an Abundance Indicator of Carbon |journal=Publications of the Astronomical Society of Japan |volume=66 |issue=5 |pages=98 |doi=10.1093/pasj/psu078 |arxiv=1407.5829 |issn=2053-051X}}</ref> and {{Nowrap|375,680 km}} (0.54 {{Solar radius|link=}})<ref>{{Cite journal |last1=Stassun |first1=Keivan G. |last2=Collins |first2=Karen A. |last3=Gaudi |first3=B. Scott |date=2017-03-03 |title=Accurate, Empirical Radii and Masses of Planets and their Host Stars with Gaia Parallaxes |journal=The Astronomical Journal |volume=153 |issue=3 |pages=136 |doi=10.3847/1538-3881/aa5df3 |doi-access=free |arxiv=1609.04389 |bibcode=2017AJ....153..136S |issn=1538-3881}}</ref>
|<ref>{{Cite journal |last1=Doyle |first1=L. |last2=Ramsay |first2=G. |last3=Doyle |first3=J. G. |last4=Wu |first4=K. |last5=Scullion |first5=E. |date=2018-10-21 |title=Investigating the Rotational Phase of Stellar Flares on M dwarfs Using K2 Short Cadence Data |journal=Monthly Notices of the Royal Astronomical Society |volume=480 |issue=2 |pages=2153–2164 |doi=10.1093/mnras/sty1963 |arxiv=1807.08592 |issn=0035-8711|doi-access=free }}</ref>
|-
|[[Lalande 21185]]
|273,500
|Sixth-nearest star system to the Solar System. Has two confirmed exoplanets and one unconfirmed
|<ref name="2009A&A...505..205D">{{cite journal |last1=Demory |first1=Brice-Olivier |last2=Ségransan |first2=Damien |last3=Forveille |first3=Thierry |last4=Queloz |first4=Didier |last5=Beuzit |first5=Jean-Luc |last6=Delfosse |first6=Xavier |last7=Di Folco |first7=Emmanuel |last8=Kervella |first8=Pierre |last9=Le Bouquin |first9=Jean-Baptiste |last10=Perrier |first10=Christian |last11=Benisty |first11=Myriam |last12=Duvert |first12=Gilles |last13=Hofmann |first13=Karl-Heinz |last14=Lopez |first14=Bruno |last15=Petrov |first15=Romain |date=October 2009 |title=Mass-radius relation of low and very low-mass stars revisited with the VLTI |journal=Astronomy and Astrophysics |volume=505 |issue=1 |pages=205–215 |arxiv=0906.0602 |bibcode=2009A&A...505..205D |doi=10.1051/0004-6361/200911976 |s2cid=14786643}}</ref>
|-
|[[LHS 6343]] B
|274,100
|
|<ref name=":9" />
|-
|[[Gliese 22]] B
|274,100
|
|<ref>{{Cite journal |last1=Newton |first1=Elisabeth R. |last2=Irwin |first2=Jonathan |last3=Charbonneau |first3=David |last4=Berlind |first4=Perry |last5=Calkins |first5=Michael L. |last6=Mink |first6=Jessica |date=2017-01-04 |title=The H$\alpha$ emission of nearby M dwarfs and its relation to stellar rotation |journal=The Astrophysical Journal |volume=834 |issue=1 |pages=85 |doi=10.3847/1538-4357/834/1/85 |doi-access=free |arxiv=1611.03509 |bibcode=2017ApJ...834...85N |issn=1538-4357}}</ref>
|-
|[[Gliese 179]]
|278,300
|Has two confirmed exoplanets
|<ref name=":8" />
|-
|[[HIP 57050]]
|278,300
|Has two confirmed exoplanets
|<ref>{{Cite journal |last1=Haghighipour |first1=Nader |last2=Vogt |first2=Steven S. |last3=Butler |first3=R. Paul |last4=Rivera |first4=Eugenio J. |last5=Laughlin |first5=Greg |last6=Meschiari |first6=Stefano |last7=Henry |first7=Gregory W. |date=2010-05-20 |title=The Lick-Carnegie Exoplanet Survey: A Saturn-Mass Planet in the Habitable Zone of the Nearby M4V Star HIP 57050 |journal=The Astrophysical Journal |volume=715 |issue=1 |pages=271–276 |doi=10.1088/0004-637X/715/1/271 |arxiv=1004.4608 |bibcode=2010ApJ...715..271H |issn=0004-637X}}</ref>
|-
|[[KOI-4777]]
|278,300
|Has one confirmed exoplanet
|<ref>{{Cite journal |last1=Cañas |first1=Caleb I. |author2-link=Suvrath Mahadevan |last2=Mahadevan |first2=Suvrath |last3=Cochran |first3=William D. |last4=Bender |first4=Chad F. |last5=Feigelson |first5=Eric D. |last6=Harman |first6=C. E. |last7=Kopparapu |first7=Ravi Kumar |last8=Caceres |first8=Gabriel A. |last9=Diddams |first9=Scott A. |last10=Endl |first10=Michael |last11=Ford |first11=Eric B. |last12=Halverson |first12=Samuel |last13=Hearty |first13=Fred |last14=Jones |first14=Sinclaire |last15=Kanodia |first15=Shubham |date=2022-01-01 |title=A Hot Mars-sized Exoplanet Transiting an M Dwarf |journal=The Astronomical Journal |volume=163 |issue=1 |pages=3 |doi=10.3847/1538-3881/ac3088 |arxiv=2112.03958 |bibcode=2022AJ....163....3C |issn=0004-6256|doi-access=free }}</ref>
|-
|[[Gliese 163]]
|284,550
|Has five confirmed exoplanets
|<ref name=":3" />
|-
|[[AT Microscopii]] A ''(AT Mic A)''
|285,250
|
|<ref name=":7" />
|-
|[[Gliese 588]]
|292,200
|
|<ref>{{Cite journal |journal=Monthly Notices of the Royal Astronomical Society |doi=10.1093/mnras/stx1140|title=High-cadence spectroscopy of M-dwarfs – II. Searching for stellar pulsations with HARPS |year=2017 |last1=Berdiñas |first1=Z. M. |last2=Rodríguez-López |first2=C. |last3=Amado |first3=P. J. |last4=Anglada-Escudé |first4=G. |last5=Barnes |first5=J. R. |last6=MacDonald |first6=J. |last7=Zechmeister |first7=M. |last8=Sarmiento |first8=L. F. |volume=469 |issue=4 |pages=4268–4282 |doi-access=free |arxiv=1705.04690 }}</ref>
|-
|[[Gliese 686]]
|292,200
|Has a confirmed exoplanet
|<ref>{{Cite journal |last1=Affer |first1=L. |last2=Damasso |first2=M. |last3=Micela |first3=G. |last4=Poretti |first4=E. |last5=Scandariato |first5=G. |last6=Maldonado |first6=J. |last7=Lanza |first7=A. F. |last8=Covino |first8=E. |last9=Rubio |first9=A. Garrido |last10=Hernandez |first10=J. I. Gonzalez |last11=Gratton |first11=R. |last12=Leto |first12=G. |last13=Maggio |first13=A. |last14=Perger |first14=M. |last15=Sozzetti |first15=A. |date=February 2019 |title=HADES RV program with HARPS-N at TNG. IX. A super-Earth around the M dwarf Gl686 |journal=Astronomy & Astrophysics |volume=622 |pages=A193 |doi=10.1051/0004-6361/201834868 |arxiv=1901.05338 |bibcode=2019A&A...622A.193A |issn=0004-6361|doi-access=free }}</ref>
|-
|[[KIC 4150611]] Ab1
|292,200
|
|<ref name=kemp>{{cite journal | arxiv=2406.04131 | last1=Kemp | first1=Alex | last2=Tkachenko | first2=Andrew | last3=Torres | first3=Guillermo | last4=Pavlovski | first4=Kresimir | last5=IJspeert | first5=Luc | last6=Serebriakova | first6=Nadya | last7=Conroy | first7=Kyle | author8=Timothy van Reeth | last9=Latham | first9=David | last10=Prsa | first10=Andrej | last11=Aerts | first11=Conny | title=KIC 4150611: A quadruply eclipsing heptuple star system with a ''g'' -mode period-spacing pattern | journal=Astronomy & Astrophysics | date=2024 | volume=689 | pages=A164 | doi=10.1051/0004-6361/202450390 }}</ref>
|-
|[[TOI 700]]
|292,200
|Has four confirmed exoplanets
|<ref>{{Cite journal |last1=Gilbert |first1=Emily A. |last2=Barclay |first2=Thomas |last3=Schlieder |first3=Joshua E. |last4=Quintana |first4=Elisa V. |last5=Hord |first5=Benjamin J. |last6=Kostov |first6=Veselin B. |last7=Lopez |first7=Eric D. |last8=Rowe |first8=Jason F. |last9=Hoffman |first9=Kelsey |last10=Walkowicz |first10=Lucianne M. |last11=Silverstein |first11=Michele L. |last12=Rodriguez |first12=Joseph E. |last13=Vanderburg |first13=Andrew |last14=Suissa |first14=Gabrielle |last15=Airapetian |first15=Vladimir S. |date=2020-08-14 |title=The First Habitable Zone Earth-sized Planet from TESS. I: Validation of the TOI-700 System |journal=The Astronomical Journal |volume=160 |issue=3 |pages=116 |doi=10.3847/1538-3881/aba4b2 |arxiv=2001.00952 |bibcode=2020AJ....160..116G |s2cid=209862554 |issn=1538-3881 |doi-access=free }}</ref>
|-
|[[QS Virginis]] B
|292,404
|
|<ref name=":17" />
|-
|[[Gliese 180]]
|294,211.5
|Has two confirmed exoplanets
|<ref name=":8" />
|-
|[[AD Leonis]] ''(Gliese 388)''
|294,500
|
|<ref>{{Cite journal |last1=Kossakowski |first1=D. |last2=Kürster |first2=M. |last3=Henning |first3=Th |last4=Trifonov |first4=T. |last5=Caballero |first5=J. A. |last6=Lafarga |first6=M. |last7=Bauer |first7=F. F. |last8=Stock |first8=S. |last9=Kemmer |first9=J. |last10=Jeffers |first10=S. V. |last11=Amado |first11=P. J. |last12=Pérez-Torres |first12=M. |last13=Béjar |first13=V. J. S. |last14=Cortés-Contreras |first14=M. |last15=Ribas |first15=I. |date=2022-10-01 |title=The CARMENES search for exoplanets around M dwarfs - Stable radial-velocity variations at the rotation period of AD Leonis: A test case study of current limitations to treating stellar activity |url=https://www.aanda.org/articles/aa/abs/2022/10/aa43773-22/aa43773-22.html |journal=Astronomy & Astrophysics |language=en |volume=666 |pages=A143 |doi=10.1051/0004-6361/202243773 |arxiv=2209.05814 |bibcode=2022A&A...666A.143K |issn=0004-6361}}</ref>
|-
|[[Gliese 408]]
|299,150
|
|<ref name=":2" />
|-
|[[Gliese 3634]]
|299,150
|Has a confirmed exoplanet
|<ref>{{Cite encyclopedia |title=The Extrasolar Planet Encyclopaedia — Catalog Listing |url=https://exoplanet.eu/catalog/?f=%27GJ%203634%27+in+name/ |access-date=2023-01-10 |encyclopedia=[[Extrasolar Planets Encyclopaedia]] | date=1995 }}</ref>
|-
|[[Gliese 569]] A
|299,150
|
|<ref>{{Cite journal |last1=Lund |first1=K. |last2=Jardine |first2=M. |last3=Russell |first3=A. J. B. |last4=Donati |first4=J. -F. |last5=Fares |first5=R. |last6=Folsom |first6=C. P. |last7=Jeffers |first7=S. V. |last8=Marsden |first8=S. C. |last9=Morin |first9=J. |last10=Petit |first10=P. |last11=See |first11=V. |date=2021-04-01 |title=Field linkage and magnetic helicity density |journal=Monthly Notices of the Royal Astronomical Society |volume=502 |issue=4 |pages=4903–4910 |doi=10.1093/mnras/stab305 |doi-access=free |arxiv=2102.11238 |bibcode=2021MNRAS.502.4903L |issn=0035-8711}}</ref>
|-
|[[U Geminorum]] red dwarf
|299,150
|
|<ref name=":13" />
|-
|[[Gliese 436]]
|300,542
|Has a confirmed exoplanet
|<ref name=":3" />
|-
|[[Sigma Coronae Borealis]] C
|304,000
|
|<ref>{{Cite journal |last1=Mann |first1=Andrew W. |last2=Feiden |first2=Gregory A. |last3=Gaidos |first3=Eric |last4=Boyajian |first4=Tabetha |last5=von Braun |first5=Kaspar |date=2015-05-01 |title=How to Constrain Your M Dwarf: measuring effective temperature, bolometric luminosity, mass, and radius |journal=The Astrophysical Journal |volume=804 |issue=1 |pages=64 |doi=10.1088/0004-637X/804/1/64 |arxiv=1501.01635 |bibcode=2015ApJ...804...64M |issn=0004-637X|hdl=2152/34940 |hdl-access=free }}</ref>
|-
|[[HD 260655]] ''(TOI-4599)''
|305,400
|Has two confirmed exoplanets
|<ref>{{Cite journal |last1=Luque |first1=R. |last2=Fulton |first2=B. J. |last3=Kunimoto |first3=M. |last4=Amado |first4=P. J. |last5=Gorrini |first5=P. |last6=Dreizler |first6=S. |last7=Hellier |first7=C. |last8=Henry |first8=G. W. |last9=Molaverdikhani |first9=K. |last10=Morello |first10=G. |last11=Peña-Moñino |first11=L. |last12=Pérez-Torres |first12=M. |last13=Pozuelos |first13=F. J. |last14=Shan |first14=Y. |last15=Anglada-Escudé |first15=G. |date=August 2022 |title=The HD 260655 system: Two rocky worlds transiting a bright M dwarf at 10 pc |journal=Astronomy & Astrophysics |volume=664 |pages=A199 |doi=10.1051/0004-6361/202243834 |arxiv=2204.10261 |bibcode=2022A&A...664A.199L |issn=0004-6361}}</ref>
|-
|[[WR 93b]]
|306,108
|[[Wolf–Rayet star|Wolf-Rayet]]
|
|<ref>{{Cite journal |last1=Sander |first1=A. |last2=Hamann |first2=W. -R. |last3=Todt |first3=H. |date=2012-04-01 |title=The Galactic WC stars. Stellar parameters from spectral analyses indicate a new evolutionary sequence |url=https://ui.adsabs.harvard.edu/abs/2012A&A...540A.144S |journal=Astronomy and Astrophysics |volume=540 |pages=A144 |doi=10.1051/0004-6361/201117830 |arxiv=1201.6354 |bibcode=2012A&A...540A.144S |s2cid=119182468 |issn=0004-6361}}</ref>
|-
|[[Gliese 832]]
|307,500
| rowspan="8" |[[Red dwarf]]
|Has two exoplanets
|<ref name=":3" />
|-
|[[Gliese 877]]
|307,500
|
|<ref name=":19">{{Cite journal |last1=Houdebine |first1=E. R. |last2=Mullan |first2=D. J. |last3=Paletou |first3=F. |last4=Gebran |first4=M. |date=2016-05-11 |title=The Rotation-Activity Correlations in K and M dwarfs. I. Stellar parameters, compilations of $v\sin i$ and $P/\sin i$ for a large sample of late-K and M dwarfs |journal=The Astrophysical Journal |volume=822 |issue=2 |pages=97 |doi=10.3847/0004-637X/822/2/97 |arxiv=1604.07920 |s2cid=119118088 |issn=1538-4357 |doi-access=free |bibcode=2016ApJ...822...97H }}</ref>
|-
|[[Gliese 393]]
|310,212.5
|
|<ref name=":8" />
|-
|[[Tabby's Star]] B ''(KIC 8462852 B)''
|313,065
|
|<ref>{{Cite journal |last1=Pearce |first1=Logan A. |last2=Kraus |first2=Adam L. |last3=Dupuy |first3=Trent J. |last4=Mann |first4=Andrew W. |last5=Huber |first5=Daniel |date=2021-03-01 |title=Boyajian's Star B: The co-moving stellar companion to KIC 8462852 |journal=The Astrophysical Journal |volume=909 |issue=2 |pages=216 |doi=10.3847/1538-4357/abdd33 |arxiv=2101.06313 |issn=0004-637X|doi-access=free }}</ref>
|-
|[[Gliese 367|Añañuca]] ''(Gliese 367)''
|317,935
|Has three confirmed exoplanets
|<ref>{{Cite journal |last1=Lam |first1=Kristine W. F. |last2=Csizmadia |first2=Szilárd |last3=Astudillo-Defru |first3=Nicola |last4=Bonfils |first4=Xavier |last5=Gandolfi |first5=Davide |last6=Padovan |first6=Sebastiano |last7=Esposito |first7=Massimiliano |last8=Hellier |first8=Coel |last9=Hirano |first9=Teruyuki |last10=Livingston |first10=John |last11=Murgas |first11=Felipe |last12=Smith |first12=Alexis M. S. |last13=Collins |first13=Karen A. |last14=Mathur |first14=Savita |last15=Garcia |first15=Rafael A. |date=2021-12-03 |title=GJ 367b: A dense ultra-short period sub-Earth planet transiting a nearby red dwarf star |journal=Science |volume=374 |issue=6572 |pages=1271–1275 |doi=10.1126/science.aay3253 |pmid=34855492 |arxiv=2112.01309 |bibcode=2021Sci...374.1271L |issn=0036-8075}}</ref>
|-
|[[Gliese 849]]
|322,800
|Has two confirmed exoplanets
|<ref name=":3" />
|-
|[[K2-18]] ''(EPIC 201912552)''
|326,300
|Has two confirmed exoplanets
|<ref>{{Cite journal |last1=Cloutier |first1=R. |last2=Astudillo-Defru |first2=N. |last3=Doyon |first3=R. |last4=Bonfils |first4=X. |last5=Almenara |first5=J. M. |last6=Bouchy |first6=F. |last7=Delfosse |first7=X. |last8=Forveille |first8=T. |last9=Lovis |first9=C. |last10=Mayor |first10=M. |last11=Menou |first11=K. |last12=Murgas |first12=F. |last13=Pepe |first13=F. |last14=Santos |first14=N. C. |last15=Udry |first15=S. |date=January 2019 |title=Confirmation of the radial velocity super-Earth K2-18c with HARPS and CARMENES |journal=Astronomy & Astrophysics |volume=621 |pages=A49 |doi=10.1051/0004-6361/201833995 |arxiv=1810.04731 |bibcode=2019A&A...621A..49C |issn=0004-6361}}</ref>
|-
|[[Gliese 521]]
|327,000
|
|<ref>{{Cite journal |last1=Maldonado |first1=J. |last2=Scandariato |first2=G. |last3=Stelzer |first3=B. |last4=Biazzo |first4=K. |last5=Lanza |first5=A. F. |last6=Maggio |first6=A. |last7=Micela |first7=G. |last8=González-Álvarez |first8=E. |last9=Affer |first9=L. |last10=Claudi |first10=R. U. |last11=Cosentino |first11=R. |last12=Damasso |first12=M. |last13=Desidera |first13=S. |last14=Hernández |first14=J. I. González |last15=Gratton |first15=R. |date=February 2017 |title=The HADES RV Programme with HARPS-N@TNG. III. Flux-flux and activity-rotation relationships of early-M dwarfs |journal=Astronomy & Astrophysics |volume=598 |pages=A27 |doi=10.1051/0004-6361/201629223 |arxiv=1610.05906 |bibcode=2017A&A...598A..27M |issn=0004-6361|doi-access=free }}</ref>
|-
|[[BAT99-123]] ''(Brey 93)''
|327,000
|[[Wolf-Rayet star|Wolf-Rayet]]
|First WO star discovered in the [[Large Magellanic Cloud]].
|<ref>{{Cite journal |last1=Tramper |first1=F. |last2=Straal |first2=S. M. |last3=Sanyal |first3=D. |last4=Sana |first4=H. |last5=de Koter |first5=A. |last6=Gräfener |first6=G. |last7=Langer |first7=N. |last8=Vink |first8=J. S. |last9=de Mink |first9=S. E. |last10=Kaper |first10=L. |date=September 2015 |title=Massive stars on the verge of exploding: the properties of oxygen sequence Wolf-Rayet stars |journal=Astronomy & Astrophysics |volume=581 |pages=A110 |doi=10.1051/0004-6361/201425390 |arxiv=1507.00839 |bibcode=2015A&A...581A.110T |issn=0004-6361}}</ref>
|-
|[[Lacaille 9352]] ''(Gliese 887)''
|329,750
|[[Red dwarf]]
|Has two confirmed exoplanets and one unconfirmed
|<ref name=":3" />
|-
|}

=== Smallest stars by type ===

{| class="wikitable sortable"
|+'''List of the smallest stars by star type'''
|-
!| Type
!| {{nowrap|Star name}}
!| Radius<br />{{nowrap|[[Solar radius|Solar radii]]}}<br /><small>{{nowrap|1=([[Sun]] = 1)}}</small>
!| Radius<br />{{nowrap|[[Jupiter radius|Jupiter radii]]}}<br /><small>{{nowrap|1=([[Jupiter]] = 1)}}</small>
!| Radius<br />{{nowrap|[[Earth radius|Earth radii]]}}<br /><small>{{nowrap|1=([[Earth]] = 1)}}</small>
!| Radius<br /><small>{{nowrap|([[kilometre|km]] / [[statute mile|mi]])}}</small>
!| Date
!width=100%| Notes
!|References
|-
|| [[Red dwarf]]
|| [[EBLM J0555-57Ab]]
|| 0.084
|| 0.84
|| 9.41
|| {{convert|60000|km|mi|abbr=on}}
|| 2017
|| The red dwarf stars are considered the smallest stars known, and representative of the smallest star possible.
|| <ref name=cnet-2017-07-11/><ref name=Cambridge-2017-smallest-ever-star-discovered-by-astronomers/><ref name=2017arXiv170608781V/>
|-
|| [[Brown dwarf]]
||[[WISEA 1810−1010]]
|| 0.067
|| 0.655
|| 7.29
|| {{convert|46840|km|mi|abbr=on}}
||
|| 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.
|| <ref name=":11" />
|-
|| [[White dwarf]]
|| [[HD 49798]]
|| 0.0023
|| 0.023
|| 0.25
|| {{convert|1600|km|mi|abbr=on}}
|| 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.
|| <ref name=":0" />
|-
|| [[Neutron star]]
||{{Nowrap|[[RX J0720.4−3125]]}}
|| 0.0000064683{{Snd}}0.0000077332
|| 0.00006294{{Snd}}0.00007525
|| 0.0007055{{Snd}}0.0008435
||{{val|4.50|0.08|0.09}}{{snd}}{{val|5.38|0.13|0.14}}
|| 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.
||<ref name="Hohle" />
|-
|}

===Timeline of smallest red dwarf star recordholders===
[[Red dwarf]]s are considered the smallest star known that are active fusion stars, and are the smallest stars possible that is not a [[brown dwarf]].

{| class="wikitable sortable"
|+ '''List of smallest red dwarf titleholders'''
|-
!| {{nowrap|Star name}}
!| Date
!| Radius<br />{{nowrap|[[Solar radius|Solar radii]]}}<br /><small>{{nowrap|1=([[Sun]] = 1)}}</small>
!| Radius<br />{{nowrap|[[Jupiter radius|Jupiter radii]]}}<br /><small>{{nowrap|1=([[Jupiter]] = 1)}}</small>
!| Radius<br />km<br />(mi)
!width=100%| Notes
!|
|-
|| {{nowrap|[[EBLM J0555-57Ab]]}}
|| {{nowrap|2017-}}
|| 0.084
|| 0.84
|| {{convert|60000|km|mi|abbr=on}}
|| This star has a size comparable to that of [[Saturn]].
|| <ref name="cnet-2017-07-11" /><ref name="Cambridge-2017-smallest-ever-star-discovered-by-astronomers" /><ref name="2017arXiv170608781V" />
|-
|| {{nowrap|[[2MASS J0523-1403]]}}
|| {{nowrap|2013-2017}}
|| 0.102
|| 1.01
|| {{convert|70600|km|mi|abbr=on}}
|| Lowest mass main sequence star as of 2020.
|| <ref name=SnT-2013-12-23/><ref name=2014AJ....147...94D/><ref name="NOAO-pr1311">{{cite web|first=Katy|last=Garmany|title=NOAO/SOAR: Where do stars end and brown dwarfs begin?|url=http://www.noao.edu/news/2013/pr1311.php|publisher=National Optical Astronomy Observatory|access-date=14 December 2013}}</ref><ref name="Fundamental Parameters and Spectral"/>
|-
|| {{nowrap|[[OGLE-TR-122B]]}}
|| {{nowrap|2005-2013}}
|| 0.117
|| 1.16
|| {{convert|81100|km|mi|abbr=on}}
||
|| <ref name=Space-2005-03-03/><ref name=SpaceAnswers-SmallestStar-2013-03-22/><ref name=2005A&A...433L..21P/>
|-
|}

== Notes ==
{{notelist|30em}}

== References ==
{{reflist}}
<references group="note" />
{{star}}
{{Portal bar|Astronomy|Spaceflight|Outer space|Solar System}}

[[Category:Lists of stars|Volume, least]]
[[Category:Smallest things|S]]