Editing List of nearest stars

{{Short description|Stars and brown dwarfs within 20 light years of the Solar System}}
{{Use dmy dates |date=September 2021}}
[[File:Nearest_stars_rotating_red-green.gif|alt=Rotating 3D image of the nearest stars|300px|thumb|upright=2|Animated 3D map of the nearest stars, centered on the Sun. {{3d glasses|color=red green}}]]
[[File:Angular map of fusors around Sol within 9ly (large).png|300px|thumb|upright=2|A radar map of all known stellar and [[substellar]] objects within 9 light years (ly), arranged clockwise in [[hour angle|hours]] of [[right ascension]], and  marked by distance (▬) and position (◆). Distances are marked outward from the [[Sun|Sun (Sol)]], with concentric circles indicating the distance in one ly steps. Positions are marked inward from their distance markings, connected by lines according to their [[declination]]s (doted when positive), representing the [[Circular arc|arcs]] of the declinations viewed edge-on. For within 12 ly see [[commons:File:Angular_map_of_fusors_around_Sol_within_12ly_(large).png|this map]].]]

<!-- Current distances (first table) -->
This list covers all known [[star]]s, [[white dwarf]]s, [[brown dwarf]]s, and [[sub-brown dwarf]]s within {{convert|20|ly|pc|abbr=off|sigfig=3|lk=on}} of the [[Sun]]. So far, 131 such objects have been found.  Only [[List of nearest bright stars|22 are bright enough]] to be visible without a telescope, for which the star's visible light needs to reach or exceed the dimmest brightness visible to the [[naked eye]] from Earth, 6.5 [[apparent magnitude]].<ref name="Weaver1947">{{cite journal
|last=Weaver |first=Harold F.
|title=The Visibility of Stars Without Optical Aid
|journal=Publications of the Astronomical Society of the Pacific
|date=1947
|volume=59
|issue=350
|pages=232–243
|bibcode=1947PASP...59..232W
|doi=10.1086/125956|doi-access=
}}</ref>

The known 131 objects are bound in 94 [[stellar systems]]. Of those, 103 are [[main sequence stars]]: 80 [[red dwarf]]s and 23 "typical" stars having greater mass. Additionally, astronomers have found 6 [[white dwarf]]s (stars that have exhausted all fusible hydrogen), 21 brown dwarfs, as well as 1 sub-brown dwarf, [[WISE 0855−0714]] (possibly a [[rogue planet]]). The closest system is [[Alpha Centauri]], with [[Proxima Centauri]] as the closest star in that system, at 4.2465 light-years from Earth. The brightest, most massive and most luminous object among those 131 is [[Sirius A]], which is also the brightest star in Earth's [[night sky]]; its white dwarf companion Sirius B is the hottest object among them. The largest object within the 20 light-years is [[Procyon]].

The [[Solar System]], and the other stars/dwarfs listed here, are currently moving within (or near) the [[Local Interstellar Cloud]], roughly {{convert|30|ly|pc|1|lk=on}} across. The Local Interstellar Cloud is, in turn, contained inside the [[Local Bubble]], a cavity in the interstellar medium about {{convert|300|ly|pc|1|lk=on}} across.  It contains [[Ursa Major Moving Group|Ursa Major]] and the [[Hyades (star cluster)|Hyades]] [[star cluster]], among others. The Local Bubble also contains the neighboring [[G-Cloud]], which contains the stars [[Alpha Centauri]] and [[Altair]]. In the [[Solar System#Galactic context|galactic context]], the Local Bubble is a small part of the [[Orion Arm]], which contains most stars that we can see without a telescope. The Orion Arm is one of the [[spiral arms]] of our [[Milky Way galaxy]].

==Astrometrics==
<!-- Notes on methodology -->
The easiest way to determine stellar distance to the Sun for objects at these distances is [[parallax]], which measures how much stars appear to move against background objects over the course of Earth's orbit around the Sun. As a [[parsec]] (parallax-second) is defined by the distance of an object that would appear to move exactly one [[second of arc]] against background objects, stars less than 5 parsecs away will have measured parallaxes of over 0.2 arcseconds, or 200 milliarcseconds. Determining past and future positions relies on accurate [[astrometric]] measurements of their parallax and total [[proper motion]]s (how far they move across the sky due to their actual velocity relative to the Sun), along with [[spectroscopic]]ally determined [[radial velocities]] (their speed directly towards or away from us, which combined with proper motion defines their true movement through the sky relative to the Sun). Both of these measurements are subject to increasing and significant errors over very long time spans, especially over the several thousand-year time spans it takes for stars to noticeably move relative to each other.<ref name="Matthews1994">{{cite journal
|title=The Close Approach of Stars in the Solar Neighborhood
|last1=Matthews |first1=R. A.
|year=1994
|journal=Quarterly Journal of the Royal Astronomical Society
|volume=35
|page=1
|bibcode=1994QJRAS..35....1M}}</ref>

<!-- Past/Future distances (second table) -->
Based on results from the [[Gaia (spacecraft)|Gaia]] telescope's second data release from April 2018, an estimated 694 stars will approach the Solar System to less than 5 [[parsec]]s in the next 15 million years. Of these, 26 have a good probability to come within {{convert|1.0|pc|ly|abbr=off|sigfig=2}} and another 7 within {{convert|0.5|pc|ly|abbr=off|sigfig=2}}.<ref name="Bailer2018">{{Cite journal|last1=Bailer-Jones|first1=C. A. L.
|last2=Rybizki|first2=J.
|last3=Andrae|first3=R.
|last4=Fouesnea|first4=M.
|title=New stellar encounters discovered in the second Gaia data release
|journal=Astronomy & Astrophysics
|volume=616
|issue=37
|pages=A37
|arxiv=1805.07581
|doi=10.1051/0004-6361/201833456
|year=2018
|bibcode=2018A&A...616A..37B
|s2cid=56269929
}}</ref> This number is likely much higher, due to the sheer number of stars needed to be surveyed; a star approaching the Solar System 10 million years ago, moving at a typical Sun-relative 20–200 kilometers per second, would be 600–6,000 light-years from the Sun at present day, with millions of stars closer to the Sun. The closest encounter to the Sun so far predicted is the low-mass orange dwarf star [[Gliese 710]] / HIP 89825 with roughly 60% the mass of the Sun.<ref name="Hall2018">{{cite web|title=Known Close Stellar Encounters Surge in Number
|author= Hall, Shannon
|publisher=Sky and Telescope
|date=28 May 2018
|url=http://www.skyandtelescope.com/astronomy-news/close-stellar-encounters-surge/
|access-date=2 June 2018}}</ref> It is currently predicted to pass {{val|0.1696|0.0065|u=ly}} ({{val|10635|500}} [[Astronomical unit|au]]) from the Sun in {{val|1.290|0.04}} million years from the present, close enough to significantly disturb the Solar System's [[Oort cloud]].<ref name="resultsGaiaDR3">{{cite journal 
|last1=de la Fuente Marcos |first1=Raúl
|last2=de la Fuente Marcos |first2=Carlos
|title=An Update on the Future Flyby of Gliese 710 to the Solar System Using Gaia DR3: Flyby Parameters Reproduced, Uncertainties Reduced
|journal=[[Research Notes of the AAS]]
|volume= 6
|issue= 6
|pages= 136
|year = 2022
|arxiv=
|bibcode=2022RNAAS...6..136D
|doi= 10.3847/2515-5172/ac7b95|doi-access=free }}</ref>

[[File:Stars-within-11-light-years2.webm|thumb|upright=1.3|Stars within {{nowrap|11 ly}}.]]
[[File:12lightyears.gif|thumb|upright=1.3|Stars and star systems within {{nowrap|12.5 ly}}.]]

==List==
<!--PLEASE NOTE: The various values for the stars, to preserve one's ability to sort various parts of the table, will be organized as such:

#/distance/system/star: no sort
stellar class: 3-digit 0-padded spectral type in intervals of 10: A0 = 000, A5 = 005, F5 = 015, etc.
A0 = 000, F0 = 010, G0 = 020, K0 = 030, M0 = 040, L0 = 050, T0 = 060, Y0 = 070, D0 = 080
apparent magnitude/absolute magnitude: 2-digit 0-padded value.

-->
{{sticky header}}
{| class="wikitable sortable sticky-header-multi" style="font-size:1.00em; line-height:1.5em;"
|+Key
|-
| style="background-color: lightblue"| {{Hash-tag|alt=visible to naked eye}}
|Visible to the unaided eye ([[apparent magnitude]] of +6.5 or brighter)
|-
| style="background-color: lightgreen"| {{Dollar sign}}
|[[List of nearest bright stars|Luminous star]] ([[absolute magnitude]] of +8.5 or brighter)
|-
| style="background-color:#F5F5DC"| {{Double-dagger|alt=white dwarf}}
|[[White dwarf]]
|-
| style="background-color:#D8BD98"| §
|[[Brown dwarf]]
|-
| style="background-color:#C67B30"| {{&}}
|[[Sub-brown dwarf]] or [[rogue planet]]
|-
| style="background-color: pink"| {{Asterisk}}
|Nearest in constellation
|}

The [[Stellar classification|classes]] of the stars and brown dwarfs are shown in the color of their spectral types (these colors are derived from conventional names for the spectral types and do not necessarily represent the star's observed color). Many brown dwarfs are not listed by [[visible spectrum|visual magnitude]] but are listed by near-infrared [[J band (infrared)|J band]] [[Magnitude (astronomy)|apparent magnitude]] due to how dim (and often invisible) they are in visible color bands (U, B or V). Absolute magnitude (with electromagnetic wave, 'light' band denoted in subscript) is a measurement at a 10-parsec distance across imaginary empty space devoid of all its sparse dust and gas. Some of the [[parallax]]es and resultant distances are rough measurements.<ref name="RECONS">{{cite journal
|date=September 17, 2007
|title=The One Hundred Nearest Star Systems
|journal=Research Consortium on Nearby Stars
|url=http://www.astro.gsu.edu/RECONS/TOP100.posted.htm
|access-date=2007-11-06}}</ref>
{{clear}}
{| class="wikitable sortable mw-collapsible sticky-header-multi" style="font-size: 90%; position:relative" 
|+Known systems within {{convert|20|ly|pc|abbr=off|sigfig=3}}
<span style="font-size:111.11111%;position:absolute;right:0px;top:0px">[[List of star systems within 20–25 light-years|→]]</span><span style="font-size:111.11111%;position:absolute;right:0px;bottom:-18px">[[List of star systems within 20–25 light-years|→]]</span>
! class="unsortable" colspan="2" |Designation
! rowspan="2" data-sort-type="number" |<small>[[Distance]]<br>([[light-year|ly]])<ref name=distfn>From parallax.</ref></small>
! rowspan="2" |<div style="position:absolute;transform: translate(-35%,-50%) rotate(270deg);;"><small>[[Constellation]]</small></div>
! rowspan="2" |<small>[[Right ascension|RA]]/[[Declination|Dec]]<br>([[Epoch (astronomy)|Ep.]] & [[Equinox (celestial coordinates)|Eq.]] [[J2000]])<ref name=RECONS/></small>
! rowspan="2" |<small>[[Stellar classification|Stellar<br>class]]</small>
! rowspan="2" |Mass ([[Solar mass|<var>M</var><sub>☉</sub>]])
! colspan="2" |<small>Magnitude ({{nowrap|m<sub>[[UBV photometric system|V]]</sub><ref name=RECONS/> or m<sub>[[J band (infrared)|J]]</sub>}})</small>
! rowspan="2" |<small>[[Stellar parallax|Parallax]]<br>([[milliarcsecond|mas]])</small><br><ref name="RECONS"/><ref name=plxfn group=note>Parallaxes given by RECONS are a weighted mean of values in the sources given, as well as measurements by the RECONS program.</ref>
! rowspan="2" |Notes and [[#References|additional<br>references]]
|-class="unsortable"
![[Star system|System]]
!Name
! data-sort-type="number" |<small>[[Apparent magnitude|App.]]</small>
! data-sort-type="number" |<small>[[Absolute magnitude|Abs.]]</small>
|-
| [[Solar System]]
| style="background-color: lightgreen" | [[Sun]] (Sol){{Dollar sign}}
| 0.0000158
| {{TableTBA|N/A}}
| {{TableTBA|N/A}}
| style="background: {{star-color|G}};" | [[G-type main-sequence star|G2V]]<ref name=RECONS/>
|1
| style="background: lightblue;" | −26.74{{Hash-tag|alt=visible to naked eye}}
| 4.85
| {{TableTBA|N/A}}
|[[List of gravitationally rounded objects of the Solar System#Planets|eight recognized planets]] and more [[dwarf planet]]s
|-
| rowspan="3" | [[Alpha Centauri]]
| [[Proxima Centauri|Proxima&nbsp;Centauri]] (C, V645&nbsp;Centauri)
| 4.2465<br>{{±|0.0003}}
| rowspan="3" style="background-color: pink" | [[Centaurus|Cen]]{{Asterisk}}
| {{RA|14|29|43.0}}<br>{{DEC|−62|40|46}}
| style="background: {{star-color|M}};" | [[red dwarf|M5.5Ve]]
|0.122
| 11.09
| 15.53
| 768.0665<br>{{±|0.0499}}<ref name="GaiaEDR3">{{cite Gaia EDR3}}</ref>
| [[flare star]], one confirmed planet ([[Proxima b|b]], 2016, and two candidate planets, ([[Proxima Centauri d|d]], 2022)<ref name="Suárez MascareñoFaria2020">{{cite journal|last1=Suárez Mascareño|first1=A.|last2=Faria|first2=J. P.|last3=Figueira|first3=P.|last4=Lovis|first4=C.|last5=Damasso|first5=M.|last6=González Hernández|first6=J. I.|last7=Rebolo|first7=R.|last8=Cristiano|first8=S.|last9=Pepe|first9=F.|last10=Santos|first10=N. C.|last11=Zapatero Osorio|first11=M. R.|last12=Adibekyan|first12=V.|last13=Hojjatpanah|first13=S.|last14=Sozzetti|first14=A.|last15=Murgas|first15=F.|last16=Abreu|first16=M.|display-authors=2|title=Revisiting Proxima with ESPRESSO|journal=Astronomy & Astrophysics|year=2020|volume=639|pages=A77|issn=0004-6361|arxiv=2005.12114|doi=10.1051/0004-6361/202037745|bibcode=2020A&A...639A..77S|doi-access=free }}</ref><ref name="Faria2022">{{cite journal|last1=Faria|first1=J. P.|last2=Suárez Mascareño|first2=A.|last3=Figueira|first3=P.|last4=Silva|first4=A. M.|last5=Damasso|first5=M.|last6=Demangeon|first6=O.|last7=Pepe|first7=F.|last8=Santos|first8=N. C.|last9=Rebolo|first9=R.|last10=Cristiani|first10=S.|last11=Adibekyan|first11=V.|last12=Alibert|first12=Y.|last13=Allart|first13=R.|last14=Barros|first14=S. C. C.|last15=Cabral|first15=A.|last16=D’Odorico|first16=V.|last17=Di Marcantonio|first17=P.|last18=Dumusque|first18=X.|last19=Ehrenreich|first19=D.|last20=González Hernández|first20=J. I.|last21=Hara|first21=N.|last22=Lillo-Box|first22=J.|last23=Lo Curto|first23=G.|last24=Lovis|first24=C.|last25=Martins|first25=C. J. A. P.|last26=Mégevand|first26=D.|last27=Mehner|first27=A.|last28=Micela|first28=G.|last29=Molaro|first29=P.|last30=Nunes|first30=N. J.|last31=Pallé|first31=E.|last32=Poretti|first32=E.|last33=Sousa|first33=S. G.|last34=Sozzetti|first34=A.|last35=Tabernero|first35=H.|last36=Udry|first36=S.|last37=Zapatero Osorio|first37=M. R. |display-authors=3|title=A candidate short-period sub-Earth orbiting Proxima Centauri|journal=Astronomy & Astrophysics|publisher=EDP Sciences|volume=658|year=2022 |doi=10.1051/0004-6361/202142337|doi-access=free|page=A115|arxiv=2202.05188 |bibcode=2022A&A...658A.115F |url=https://www.eso.org/public/archives/releases/sciencepapers/eso2202/eso2202a.pdf}}</ref> and ([[Proxima Centauri c|c]], 2019)<ref name="nationalgeographic">{{cite web| url=https://www.nationalgeographic.com/science/2019/04/proxima-c-new-super-earth-may-orbit-star-next-door-proxima-centauri/| archive-url=https://web.archive.org/web/20190413130915/https://www.nationalgeographic.com/science/2019/04/proxima-c-new-super-earth-may-orbit-star-next-door-proxima-centauri/| url-status=dead| archive-date=13 April 2019|title=A new super-Earth may orbit the star next door|last=Drake |first=Nadia|author-link=Nadia Drake |date=12 April 2019|website=[[National Geographic]]|access-date= 21 April 2019 }}  [https://www.youtube.com/watch?v=EkqpBW4h44c Video of discovery being discussed (accidentally announced?)]</ref><ref name="ArtigauCadieux2022">{{cite journal|last1=Artigau|first1=Étienne|last2=Cadieux|first2=Charles|last3=Cook|first3=Neil J.|last4=Doyon|first4=René|last5=Vandal|first5=Thomas|last6=Donati|first6=Jean-Françcois|last7=Moutou|first7=Claire|last8=Delfosse|first8=Xavier|last9=Fouqué|first9=Pascal|last10=Martioli|first10=Eder|last11=Bouchy|first11=François|last12=Parsons|first12=Jasmine|last13=Carmona|first13=Andres|last14=Dumusque|first14=Xavier|last15=Astudillo-Defru|first15=Nicola|last16=Bonfils|first16=Xavier|last17=Mignon|first17=Lucille|display-authors=5|title=Line-by-line velocity measurements, an outlier-resistant method for precision velocimetry|journal=The Astronomical Journal|volume=164:84|issue=3|pages=18pp|arxiv=2207.13524|bibcode=2022AJ....164...84A|doi=10.3847/1538-3881/ac7ce6|doi-access=free|date=June 23, 2022|publication-date=August 8, 2022}}</ref>
|-
| style="background-color: lightgreen" | Rigil&nbsp;Kentaurus (A){{Dollar sign}}
| rowspan="2" | 4.3441<br>{{±|0.0022}}
| {{RA|14|39|36.5}}<br>{{DEC|−60|50|02}}
| style="background: {{star-color|G}};" | [[G-type main-sequence star|G2V]]<ref name=RECONS/>
|1.079
| style="background: lightblue;" | 0.01{{Hash-tag|alt=visible to naked eye}}
| 4.38
| rowspan="2"| 750.81<br>{{±|0.38}}<ref name="Akeson2021">{{cite journal|doi=10.3847/1538-3881/abfaff|bibcode=2021AJ....162...14A|arxiv=2104.10086|title=Precision Millimeter Astrometry of the α Centauri AB System|journal= The Astronomical Journal|volume=162|last1=Akeson|first1=Rachel|last2=Beichman|first2=Charles|last3=Kervella|first3=Pierre|last4=Fomalont|first4=Edward|last5=Benedict|first5=G. Fritz|date=20 April 2021|issue=1 |page=14 |s2cid=233307418 |doi-access=free }}</ref>
| one directly imaged habitable-zone planet candidate ([[Candidate 1]]) (2021)
|-
| style="background-color: lightgreen" | Toliman (B){{Dollar sign}}
| {{RA|14|39|35.1}}<br>{{DEC|−60|50|14}}
| style="background: {{star-color|K}};" | [[K-type main-sequence star|K1V]]<ref name=RECONS/>
|0.909
| style="background: lightblue;" | 1.34{{Hash-tag|alt=visible to naked eye}}
| 5.71
| planet [[Alpha Centauri Bb|b]] refuted in 2015
|-
| colspan="2" | [[Barnard's Star]] (BD+04°3561a)
| 5.9629<br>{{±|0.0004}}
| style="background-color: pink" | [[Ophiuchus|Oph]]{{Asterisk}}
| {{RA|17|57|48.5}}<br>{{DEC|+04|41|36}}
| style="background: {{star-color|M}};" |[[red dwarf|M4.0Ve]]
|0.144
| 9.53
| 13.22
| 546.9759<br>{{±|0.0401}}<ref name="GaiaEDR3"/>
| flare star, largest-known [[proper motion]],<ref name="EEB">{{cite journal
| first=E. E. | last=Barnard
| author-link=Edward Emerson Barnard | date=1916
| title=A small star with large proper motion
| journal=Astronomical Journal | volume=29 | issue=695
| page=181 | bibcode = 1916AJ.....29..181B
| doi = 10.1086/104156 }}</ref> four confirmed planets (d, [[Barnard's Star b|b]], c, and e)<ref name="GonzálezHernández2024">{{cite journal|title=A sub-Earth-mass planet orbiting Barnard's star|first1=J. I.|last1=González Hernández|first2=A.|last2=Suárez Mascareño|first3=A. M.|last3=Silva|first4=A. K.|last4=Stefanov|first5=J. P.|last5=Faria|first6=H. M.|last6=Tabernero|first7=A.|last7=Sozzetti|first8=R.|last8=Rebolo|first9=F.|last9=Pepe|first10=N. C.|last10=Santos|first11=S.|last11=Cristiani|first12=C.|last12=Lovis|first13=X.|last13=Dumusque|first14=P.|last14=Figueira|first15=J.|last15=Lillo-Box|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|display-authors=1|journal=Astronomy & Astrophysics|volume=690|date=October 2024|pages=A79 |doi=10.1051/0004-6361/202451311|arxiv=2410.00569}}</ref><ref>{{cite web |last1=Basant |first1=Ritvik |last2=Luque |first2=Rafael |last3=Bean |first3=Jacob |last4=Seifahrt |first4=Andreas |last5=Brady |first5=Madison |last6=Zhao |first6=Lily |last7=Brown |first7=Nina |last8=Das |first8=Tanya |last9=Stürmer |first9=Julian |last10=Kasper |first10=David |last11=Gupta |first11=Rohan |last12=Stefánsson |first12=Guđmundur |title=Four Sub-Earth Planets Orbiting Barnard's Star from MAROON-X and ESPRESSO |url=https://iopscience.iop.org/article/10.3847/2041-8213/adb8d5 |website=IOPscience |publisher=American Astronomical Society |access-date=14 March 2025}}</ref>
|-
| rowspan="2" | [[Luhman 16]]<br>(WISE 1049−5319)
| style="background: #D8BD98"| A§
| rowspan="2" | 6.5029<br>{{±|0.0011}}
| rowspan="2" style="background-color: pink" | [[Vela (constellation)|Vel]]{{Asterisk}}
| rowspan="2" | {{RA|10|49|18.9}}<br>{{DEC|−53|19|10}}
| style="background: {{star-color|L}};" | [[Brown dwarf#Spectral class L|L8±1]]<ref name="1049primary">{{cite journal|last=Luhman|first=K. L.|year=2013|title=Discovery of a Binary Brown Dwarf at 2 Parsecs from the Sun|journal=The Astrophysical Journal Letters|volume=767|issue=1|page=L1|arxiv=1303.2401|bibcode=2013ApJ...767L...1L|doi=10.1088/2041-8205/767/1/L1|s2cid=8419422}}</ref>
|0.032
| 10.7 J
| 14.2 J
| rowspan="2" | 501.557<br>{{±|0.082}}<ref>{{cite journal |last1=Lazorenko |first1=P. F. |last2=Sahlmann |first2=J. |title=Updated astrometry and masses of the LUH 16 brown dwarf binary |journal=Astronomy & Astrophysics |volume=618 |pages=A111 |date=23 August 2018 |arxiv=1808.07835 |doi=10.1051/0004-6361/201833626 |bibcode=2018A&A...618A.111L |s2cid=119540451 }}</ref>
| rowspan="2" | nearest [[brown dwarf]]s
|-
| style="background: #D8BD98" | B§
| style="background: {{star-color|T}};" | [[Brown dwarf#Spectral class T|T1±2]]<ref name=1049primary/>
|0.027
| 
| 
|-
| style="background: #C67B30" colspan="2" | [[WISE 0855−0714]]{{&}}
| 7.430<br>{{±|0.041}}
| style="background-color: pink" | [[Hydra (constellation)|Hya]]{{Asterisk}}
| {{RA|08|55|10.8}}<br>{{DEC|-07|14|43}}
|style="background: {{star-color|Y}};" | [[Brown dwarf#Spectral class Y|Y4]] 
|0.003-0.010
| 25.0 J
| 28.2 J
| 439.0<br>{{±|2.4}}<ref name="Kirkpatrick2021"/>
| [[sub-brown dwarf]]
|- 
| colspan="2" | [[Wolf 359]] (CN&nbsp;Leonis)
| 7.8558<br>{{±|0.0013}}
| style="background-color: pink" | [[Leo (constellation)|Leo]]{{Asterisk}}
| {{RA|10|56|29.2}}<br>{{DEC|+07|00|53}}
| style="background: {{star-color|M}};" | [[red dwarf|M6.0V]]<ref name=RECONS/>
|0.090
| 13.44
| 16.55
| 415.1794<br>{{±|0.0684}}<ref name="GaiaEDR3"/>
| flare star, has 1 candidate & 1 refuted planet<ref name="Frequency of planets orbiting M dwa">{{cite arXiv|last1=Tuomi|first1=M.|last2=el|first2=al.|date=2019-06-11|title=Frequency of planets orbiting M dwarfs in the Solar neighbourhood |class=astro-ph.EP|language=en|eprint=1906.04644}}</ref><ref name=lafarga2021>{{cite journal |bibcode=2021A&A...652A..28L |title=The CARMENES search for exoplanets around M dwarfs. Mapping stellar activity indicators across the M dwarf domain |last1=Lafarga |first1=M. |last2=Ribas |first2=I. |last3=Reiners |first3=A. |last4=Quirrenbach |first4=A. |last5=Amado |first5=P. J. |last6=Caballero |first6=J. A. |last7=Azzaro |first7=M. |last8=Béjar |first8=V. J. S. |last9=Cortés-Contreras |first9=M. |last10=Dreizler |first10=S. |last11=Hatzes |first11=A. P. |last12=Henning |first12=Th. |last13=Jeffers |first13=S. V. |last14=Kaminski |first14=A. |last15=Kürster |first15=M. |last16=Montes |first16=D. |last17=Morales |first17=J. C. |last18=Oshagh |first18=M. |last19=Rodríguez-López |first19=C. |last20=Schöfer |first20=P. |last21=Schweitzer |first21=A. |last22=Zechmeister |first22=M. |journal=Astronomy and Astrophysics |year=2021 |volume=652 |page=652 |doi=10.1051/0004-6361/202140605 |arxiv=2105.13467 |s2cid=235248016 }}</ref>
|-
| colspan="2" | [[Lalande 21185]] (BD+36°2147, [[Gliese Catalogue of Nearby Stars|Gliese]]&nbsp;411, HD&nbsp;95735)
| 8.3044<br>{{±|0.0007}}
| style="background-color: pink" | [[Ursa Major|UMa]]{{Asterisk}}
| {{RA|11|03|20.2}}<br>{{DEC|+35|58|12}}
| style="background: {{star-color|M}};" | [[red dwarf|M2.0V]]<ref name=RECONS/>
|0.390
| 7.47
| 10.44
| 392.7529<br>{{±|0.0321}}<ref name="GaiaEDR3"/>
| two known planets (2019, 2021)<ref name=Hurt2021>{{citation|arxiv=2107.09087|year=2021|title=Confirmation of the Long-Period Planet Orbiting Gliese 411 and the Detection of a New Planet Candidate|last1=Hurt|first1=Spencer A.|last2=Fulton|first2=Benjamin|last3=Isaacson|first3=Howard|last4=Rosenthal|first4=Lee J.|last5=Howard|first5=Andrew W.|last6=Weiss|first6=Lauren M.|last7=Petigura|first7=Erik A.|doi=10.3847/1538-3881/ac5c47|journal=The Astronomical Journal|volume=163|issue=5|page=218|bibcode=2022AJ....163..218H |s2cid=236134034 |doi-access=free }}</ref>
|-
| rowspan="2" | [[Sirius]] (Alpha&nbsp;Canis&nbsp;Majoris)
| style="background-color: lightgreen" | A{{Dollar sign}}
| rowspan="2" | 8.7094<br>{{±|0.0054}}
| rowspan="2" style="background-color: pink" | [[Canis Major|CMa]]{{Asterisk}}
| rowspan="2" | {{RA|06|45|08.9}}<br>{{DEC|−16|42|58}}
| style="background: {{star-color|A}}" | [[A-type main-sequence star|A1V]]<ref name=RECONS/>
|2.063
| style="background: lightblue;" | −1.46{{Hash-tag|alt=visible to naked eye}}
| 1.42
| rowspan="2" | 374.4896<br>{{±|0.2313}}<ref name="GaiaEDR3"/>
| rowspan="2" | brightest star in the night sky
|-
| style="background: #F5F5DC" | B{{Double-dagger|alt=white dwarf}}
| style="background: #F5F5DC" | [[White dwarf|DA2]]<ref name=RECONS/>
|1.018
| 8.44
| 11.34
|-
| rowspan="2" | [[Gliese 65]] (Luyten 726–8)
| A (BL&nbsp;Ceti)
| rowspan="2" | 8.724<br>{{±|0.012}}
| rowspan="2" style="background-color: pink" | [[Cetus|Cet]]{{Asterisk}}
| rowspan="2" | {{RA|01|39|01.3}}<br>{{DEC|−17|57|01}}
| style="background: {{star-color|M}};" | [[red dwarf|M5.5Ve]]
|0.102
| 12.54
| 15.40
| rowspan="2" | 373.8443<br>{{±|0.5009}}<ref name="GaiaEDR3"/>
| rowspan="2" |flare star (Archetypal member), has 1 candidate planet<ref name="GRAVITY2024">{{cite journal |collaboration=GRAVITY Collaboration |last1=Abuter |first1=R. |last2=Amorim |first2=A. |last3=Benisty |first3=M. |last4=Berger |first4=J.-P. |last5=Bonnet |first5=H. |last6=Bourdarot |first6=G. |last7=Bourget |first7=P. |last8=Brandner |first8=W. |display-authors=1 |date=May 2024 |title=Astrometric detection of a Neptune-mass candidate planet in the nearest M-dwarf binary system GJ65 with VLTI/GRAVITY |journal=[[Astronomy & Astrophysics]] |volume=685 |issue= |pages=L9 |doi=10.1051/0004-6361/202449547 |arxiv=2404.08746 |bibcode=2024A&A...685L...9G}}</ref>
|-
| B (UV&nbsp;Ceti)
| style="background: {{star-color|M}};" | [[red dwarf|M6.0Ve]]
|0.100
| 12.99
| 15.85
|-
| colspan="2" | [[Ross 154]] (V1216&nbsp;Sagittarii)
| 9.7063<br>{{±|0.0009}}
| style="background-color: pink" | [[Sagittarius (constellation)|Sgr]]{{Asterisk}}
| {{RA|18|49|49.4}}<br>{{DEC|−23|50|10}}
| style="background: {{star-color|M}};" | [[red dwarf|M3.5Ve]]
|0.17
| 10.43
| 13.07
| 336.0266<br>{{±|0.0317}}<ref name="GaiaEDR3"/>
| flare star
|-
| colspan="2" | [[Ross 248]] (HH&nbsp;Andromedae)
| 10.3057<br>{{±|0.0014}}
| style="background-color: pink" | [[Andromeda (constellation)|And]]{{Asterisk}}
| {{RA|23|41|54.7}}<br>{{DEC|+44|10|30}}
| style="background: {{star-color|M}};" | [[red dwarf|M5.5Ve]]
|0.136
| 12.29
| 14.79
| 316.4812<br>{{±|0.0444}}<ref name="GaiaEDR3"/>
| flare star
|-
| colspan="2" style="background-color: lightgreen" | [[Epsilon Eridani]] (Ran){{Dollar sign}}
| 10.4749<br>{{±|0.0037}}
| style="background-color: pink" | [[Eridanus (constellation)|Eri]]{{Asterisk}}
| {{RA|03|32|55.8}}<br>{{DEC|−09|27|30}}
| style="background: {{star-color|K}};" | [[K-type main-sequence star|K2V]]<ref name=RECONS/>
|0.820
| style="background: lightblue;" | 3.73{{Hash-tag|alt=visible to naked eye}}
| 6.19
| 311.37<br>{{±|0.11}}<ref name=aj132_2206>{{citation
| last1=Benedict | first1=G. Fritz
| last2=McArthur | first2=Barbara E.
| last3=Gatewood | first3=George
| last4=Nelan | first4=Edmund
| last5=Cochran | first5=William D.
| last6=Hatzes | first6=Artie
| last7=Endl | first7=Michael
| last8=Wittenmyer | first8=Robert
| last9=Baliunas | first9=Sallie L.
| last10=Walker | first10=Gordon A. H. | last11=Yang | first11=Stephenson | last12=Kürster | first12=Martin | last13=Els | first13=Sebastian | last14=Paulson | first14=Diane B. |date=November 2006 | title=The extrasolar planet e Eridani b – orbit and mass | journal=The Astronomical Journal | volume=132 | issue=5 | pages=2206–2218 | bibcode=2006AJ....132.2206B | doi=10.1086/508323 | arxiv=astro-ph/0610247 | s2cid=18603036 | postscript=. }}</ref>
| three circumstellar disks,<br>one confirmed planet ([[Epsilon Eridani b|AEgir]], 2000) and one candidate ([[Epsilon Eridani c|c]], 2002)<ref>{{citation | display-authors=1| last1=Janson | first1=M.| last2=Reffert | first2=S.| last3=Brandner | first3=W.| last4=Henning | first4=T.| last5=Lenzen | first5=R.| last6=Hippler | first6=S.| title=A comprehensive examination of the ε Eridani system. Verification of a 4 micron narrow-band high-contrast imaging approach for planet searches | journal=Astronomy & Astrophysics | volume=488 | issue=2 | pages=771–780 | date=September 2008 | bibcode=2008A&A...488..771J | doi=10.1051/0004-6361:200809984 | arxiv=0807.0301 | s2cid=119113471 }}</ref>
|-
| colspan="2" | [[Lacaille 9352]] (Gliese&nbsp;887)
| 10.7241<br>{{±|0.0007}}
| style="background-color: pink" | [[Piscis Austrinus|PsA]]{{Asterisk}}
| {{RA|23|05|52.0}}<br>{{DEC|−35|51|11}}
| style="background: {{star-color|M}};" | [[red dwarf|M0.5V]]
|0.486
| 7.34
| 9.75
| 304.1354<br>{{±|0.0200}}<ref name="GaiaEDR3"/>
|flare star,<ref name="Loyd2020">{{cite journal|last=Loyd|first=R. O. Parke|last2=Shkolnik|first2=Evgenya L.|last3=France|first3=Kevin| last4=Wood|first4=Brian E.|last5=Youngblood|first5=Allison|display-authors=1|title=When “Boring” Stars Flare: The Ultraviolet Activity of GJ 887, a Bright M Star Hosting Newly Discovered Planets|journal=Research Notes of the AAS|volume=4|issue=7|date=July 2020|doi=10.3847/2515-5172/aba94a|doi-access=free|page=119}}</ref> two planets, b and c, with equivocal evidence for a third in the habitable zone (2020)<ref name="Jeffers Dreizler Barnes Haswell pp. 1477–1481">{{citation |arxiv=2006.16372 |title=A multiple planet system of super-Earths orbiting the brightest red dwarf star GJ887 |year=2020 |doi=10.1126/science.aaz0795 |last1=Jeffers |first1=S. V. |last2=Dreizler |first2=S. |last3=Barnes |first3=J. R. |last4=Haswell |first4=C. A. |last5=Nelson |first5=R. P. |last6=Rodríguez |first6=E. |last7=López-González |first7=M. J. |last8=Morales |first8=N. |last9=Luque |first9=R. |last10=Zechmeister |first10=M. |last11=Vogt |first11=S. S. |last12=Jenkins |first12=J. S. |last13=Pallé |first13=E. |last14=Berdi Ñas |first14=Z. M.|last15=Coleman |first15=G. A. L. |last16=Díaz |first16=M. R. |last17=Ribas |first17=I. |last18=Jones |first18=H. R. A.|last19=Butler |first19=R. P. |last20=Tinney |first20=C. G. |last21=Bailey |first21=J. |last22=Carter |first22=B. D. |last23=o'Toole |first23=S. |last24=Wittenmyer |first24=R. A. |last25=Crane |first25=J. D. |last26=Feng |first26=F. |last27=Shectman |first27=S. A. |last28=Teske |first28=J. |last29=Reiners |first29=Ansgar |last30=Amado |first30=P. J.|s2cid=220075207 |journal=Science |volume=368 |issue=6498 |pages=1477–1481 |pmid=32587019 |bibcode=2020Sci...368.1477J |display-authors=9}}</ref>
|-
| colspan="2" | [[Ross 128]] (FI&nbsp;Virginis)
| 11.0074<br>{{±|0.0011}}
| style="background-color: pink" | [[Virgo (constellation)|Vir]]{{Asterisk}}
| {{RA|11|47|44.4}}<br>{{DEC|+00|48|16}}
| style="background: {{star-color|M}};" | [[red dwarf|M4.0Vn]]
|0.168
| 11.13
| 13.51
| 296.3053<br>{{±|0.0302}}<ref name="GaiaEDR3"/>
| flare star, one planet ([[Ross 128 b|b]]) (2017)<ref name="Atlantic">{{cite web|last1= ESO|title=A temperate exo-Earth around a quiet M dwarf at 3.4 parsecs|url=https://www.eso.org/public/archives/releases/sciencepapers/eso1736/eso1736a.pdf|access-date=15 November 2017}}</ref>
|-
| rowspan="3" | [[EZ Aquarii]]<br>(Gliese&nbsp;866, Luyten&nbsp;789-6)
| A
| rowspan="3" | 11.109<br>{{±|0.034}}
| rowspan="3" style="background-color: pink" | [[Aquarius (constellation)|Aqr]]{{Asterisk}}
| rowspan="3" | {{RA|22|38|33.4}}<br>{{DEC|−15|17|57}}
| style="background: {{star-color|M}};" | [[red dwarf|M5.0Ve]]
|0.11
| 13.33
| 15.64
| rowspan="3" | 293.60<br>{{±|0.9}}<ref name="Torres2009">{{cite journal|last1=Torres|first1=G.|last2=Andersen|first2=J.|last3=Giménez|first3=A.|title=Accurate masses and radii of normal stars: modern results and applications|journal=The Astronomy & Astrophysics Review|year=2010|volume=18|issue=1–2|pages=67–126|doi=10.1007/s00159-009-0025-1|arxiv=0908.2624|bibcode=2010A&ARv..18...67T|s2cid=14006009}}</ref>
| rowspan="3" | A & B flare stars
|-
| B
| style="background: {{star-color|M}};" | [[red dwarf|M?]]
|0.11
| 13.27
| 15.58
|-
| C
| style="background: {{star-color|M}};" | [[red dwarf|M?]]
|0.10
| 14.03
| 16.34
|-
| rowspan="2" | [[Procyon]] (Alpha&nbsp;Canis&nbsp;Minoris)
| style="background-color: lightgreen" | A{{Dollar sign}}
| rowspan="2" | 11.402<br>{{±|0.032}}
| rowspan="2" style="background-color: pink" | [[Canis Minor|CMi]]{{Asterisk}}
| rowspan="2" | {{RA|07|39|18.1}}<br>{{DEC|+05|13|30}}
| style="background: {{star-color|F}}" | [[F-type main-sequence star|F5IV–V]]<ref name=RECONS/>
|1.499
| style="background: lightblue;" | 0.38{{Hash-tag|alt=visible to naked eye}}
| 2.66
| rowspan="2" | 286.05<br>{{±|0.81}}<br><ref name="Y">[[General Catalogue of Trigonometric Parallaxes]].</ref><ref name="H">[[Hipparcos Catalogue]].</ref>
| rowspan="2" |
|-
| style="background: #F5F5DC" | B{{Double-dagger|alt=white dwarf}}
| style="background: #F5F5DC" | [[White dwarf|DQZ]]<ref name=RECONS/>
|0.602
| 10.70
| 12.98
|-
| rowspan="2" | [[61 Cygni]]
| style="background-color: lightgreen" | A (BD+38°4343){{Dollar sign}}
| rowspan="2" | 11.4039<br>{{±|0.0012}}
| rowspan="2" style="background-color: pink" | [[Cygnus (constellation)|Cyg]]{{Asterisk}}
| {{RA|21|06|53.9}}<br>{{DEC|+38|44|58}}
| style="background: {{star-color|K}};" | [[K-type main-sequence star|K5.0V]]<ref name=RECONS/> 
|0.70
| style="background: lightblue;" | 5.21{{Hash-tag|alt=visible to naked eye}}
| 7.49
| rowspan="2" | 286.0054<br>{{±|0.0289}}<ref name="GaiaEDR3"/>
| rowspan="2" | first star (besides Sun) to have its distance measured.<ref>{{cite journal | last=Bessel | first=F. W. | title=Bestimmung der Entfernung des 61sten Sterns des Schwans. Von Herrn Geheimen - Rath und Ritter Bessel | journal=Astronomische Nachrichten | date=1839 | volume=16 | issue=5–6 | pages=65–96 | language=de | bibcode=1838AN.....16...65B | quote=(page 92) Ich bin daher der Meinung, daß nur die jährliche Parallaxe = 0"3136 als das Resultat der bisherigen Beobachtungen zu betrachten ist | doi=10.1002/asna.18390160502 | url=https://zenodo.org/record/1424605 }} A parallax of 313.6 mas yields a distance of 10.4 light years</ref> <br> B flare star, with possible planet or brown dwarf.<ref name="KervellaArenou2018">{{cite journal|last1=Kervella|first1=Pierre|last2=Arenou|first2=Frédéric|last3=Mignard|first3=François|last4=Thévenin|first4=Frédéric|display-authors=2|title=Stellar and substellar companions of nearby stars from Gaia DR2|journal=Astronomy & Astrophysics|volume=623|year=2019|pages=A72|doi=10.1051/0004-6361/201834371|bibcode=2019A&A...623A..72K |doi-access=free|s2cid=119491061|quote="This PMa offset between 61 Cyg A and B points at the possible presence of a third body in the system, likely orbiting around 61 Cyg B."|arxiv=1811.08902}}</ref> <br> Possible circumstellar disk.
|-
| style="background-color: lightgreen" | B (BD+38°4344){{Dollar sign}}
| {{RA|21|06|55.3}}<br>{{DEC|+38|44|31}}
| style="background: {{star-color|K}};" | [[K-type main-sequence star|K7.0V]]<ref name=RECONS/> 
|0.63
| style="background: lightblue;" | 6.03{{Hash-tag|alt=visible to naked eye}}
| 8.31
|-
| rowspan="2" | [[Struve 2398]]<br>(Gliese&nbsp;725, BD+59°1915)
| A (HD&nbsp;173739)
| rowspan="2" | 11.4908<br>{{±|0.0009}}
| rowspan="2" style="background-color: pink" | [[Draco (constellation)|Dra]]{{Asterisk}}
| {{RA|18|42|46.7}}<br>{{DEC|+59|37|49}}
| style="background: {{star-color|M}};" | [[red dwarf|M3.0V]]<ref name=RECONS/>
|0.334
| 8.90
| 11.16
| rowspan="2" | 283.8401<br>{{±|0.0220}}<ref name="GaiaEDR3"/>
| rowspan="2" | flare stars, star B has 2 candidate planets<ref name="Frequency of planets orbiting M dwa"/>
|-
| B (HD&nbsp;173740)
| {{RA|18|42|46.9}}<br>{{DEC|+59|37|37}}
| style="background: {{star-color|M}};" | [[red dwarf|M3.5V]]<ref name=RECONS/>
|0.248
| 9.69
| 11.95
|-
| rowspan="2" | [[Groombridge 34]]<br>(Gliese&nbsp;15)
| A (GX&nbsp;Andromedae)
| rowspan="2" | 11.6191<br>{{±|0.0008}}
| rowspan="2" | [[Andromeda (constellation)|And]]
| rowspan="2" | {{RA|00|18|22.9}}<br>{{DEC|+44|01|23}}
| style="background: {{star-color|M}};" | [[red dwarf|M1.5V]]<ref name=RECONS/> <!--previous: M3.0V-->
|0.38
| 8.08
| 10.32
| rowspan="2" | 280.7068<br>{{±|0.0203}}<ref name="GaiaEDR3"/>
| flare star, two known planets ([[Gliese 15 Ab|Ab]], 2014, and [[Gliese 15 Ac|Ac]], 2018)<ref name=Pinamonti2018>{{cite journal|bibcode=2018A&A...617A.104P|title=The HADES RV Programme with HARPS-N at TNG. VIII. GJ15A: A multiple wide planetary system sculpted by binary interaction|journal=Astronomy and Astrophysics|volume=617|pages=A104|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.|last16=González-Álvarez|first16=E.|last17=González Hernández|first17=J. I.|last18=Gratton|first18=R.|last19=Leto|first19=G.|last20=Malavolta|first20=L.|last21=Martinez Fiorenzano|first21=A.|last22=Micela|first22=G.|last23=Molinari|first23=E.|last24=Pagano|first24=I.|last25=Pedani|first25=M.|last26=Perger|first26=M.|last27=Piotto|first27=G.|last28=Rebolo|first28=R.|last29=Ribas|first29=I.|last30=Suárez Mascareño|first30=A.|display-authors=29|year=2018|arxiv=1804.03476|doi=10.1051/0004-6361/201732535|s2cid=54990041}}</ref>
|-
| B (GQ&nbsp;Andromedae)
| style="background: {{star-color|M}};" | [[red dwarf|M3.5V]]<ref name=RECONS/>
|0.15
| 11.06
| 13.30
| flare star
|-
| colspan="2" | [[DX Cancri]] (G&nbsp;51-15)
| 11.6797<br>{{±|0.0027}}
| style="background-color: pink" | [[Cancer (constellation)|Cnc]]{{Asterisk}}
| {{RA|08|29|49.5}}<br>{{DEC|+26|46|37}}
| style="background: {{star-color|M}};" | [[red dwarf|M6.5Ve]]
|0.09
| 14.78
| 16.98
| 279.2496<br>{{±|0.0637}}<ref name="GaiaEDR3"/>
| flare star
|-
| rowspan="3" | [[Epsilon Indi]]<br>(CPD−57°10015)
| style="background-color: lightgreen" | A{{Dollar sign}}
| rowspan="3" | 11.8670<br>{{±|0.0041}}
| rowspan="3" style="background-color: pink" | [[Indus (constellation)|Ind]]{{Asterisk}}
| {{RA|22|03|21.7}}<br>{{DEC|−56|47|10}}
| style="background: {{star-color|K}};" | [[K-type main-sequence star|K5Ve]]<ref name=RECONS/>
|0.754
| style="background: lightblue;" | 4.69{{Hash-tag|alt=visible to naked eye}}
| 6.89
| rowspan="3" | 274.8431<br>{{±|0.0956}}<ref name="GaiaEDR3"/>
| one planet (Ab) (2018)<ref name="Feng2019">{{Citation | title=Detection of the nearest Jupiter analog in radial velocity and astrometry data | first1=Fabo | last1=Feng | first2=Guillem | last2=Anglada-Escudé | first3=Mikko | last3=Tuomi | first4=Hugh R. A. | last4=Jones | first5=Julio | last5=Chanamé | first6=Paul R. | last6=Butler | first7=Markus | last7=Janson | journal=[[Monthly Notices of the Royal Astronomical Society]] | arxiv=1910.06804 | date=14 October 2019 | volume=490 | issue=4 | pages=5002–5016 | doi=10.1093/mnras/stz2912 | doi-access=free | bibcode=2019MNRAS.490.5002F | s2cid=204575783 }}</ref>
|-
| style="background: #D8BD98"| Ba§
| rowspan="2" | {{RA|22|04|10.5}}<br>{{DEC|−56|46|58}}
| style="background: {{star-color|T}};" | [[Brown dwarf#Spectral class T|T1.0V]]
|0.065
| 12.3 J<ref name="DwarfArchives">{{cite web
 |title=DwarfArchives.org: Photometry, spectroscopy, and astrometry of M, L, and T dwarfs
 |publisher=caltech.edu
 |author=Chris Gelino, [[J. Davy Kirkpatrick|Davy Kirkpatrick]], Adam Burgasser
 |url=http://ldwarf.ipac.caltech.edu/archive/version5/viewlist.php?table=ltdwarf&format=text
 |access-date=2012-06-10
 |archive-date=13 November 2013
 |archive-url=https://web.archive.org/web/20131113142759/http://ldwarf.ipac.caltech.edu/archive/version5/viewlist.php?table=ltdwarf&format=text
 |url-status=dead
 }} [http://spider.ipac.caltech.edu/staff/davy/ARCHIVE/index.shtml (main page)] {{Webarchive|url=https://web.archive.org/web/20190511221033/http://spider.ipac.caltech.edu/staff/davy/ARCHIVE/index.shtml |date=11 May 2019 }}</ref>
| 14.5 J
|
|-
| style="background: #D8BD98"| Bb§
| style="background: {{star-color|T}};" | [[Brown dwarf#Spectral class T|T6.0V]]
|0.050
| 13.2 J<ref name="DwarfArchives"/>
| 15.4 J
|
|-
| colspan="2" style="background-color: lightgreen" | [[Tau Ceti]] (BD−16°295){{Dollar sign}}
| 11.9118<br>{{±|0.0074}}
| [[Cetus|Cet]]
| {{RA|01|44|04.1}}<br>{{DEC|−15|56|15}}
| style="background: {{star-color|G}};" | [[G-type main-sequence star|G8.5Vp]]<ref name=RECONS/>
|0.783
|style="background: lightblue;" | 3.49{{Hash-tag|alt=visible to naked eye}}
| 5.68
| 273.8097<br>{{±|0.1701}}<ref name="GaiaEDR3"/>
| debris disk,<br> and evidence for four planets ([[Tau Ceti e|e]], [[Tau Ceti f|f]], g, and h) (2012, 2017),<br> and further four suspected planets (b, c, d, and "i") (2012, 2019)
|-
| colspan="2" | [[GJ 1061]] (LHS&nbsp;1565)
| 11.9839<br>{{±|0.0014}}
| style="background-color: pink" | [[Horologium (constellation)|Hor]]{{Asterisk}}
| {{RA|03|35|59.7}}<br>{{DEC|−44|30|45}}
| style="background: {{star-color|M}};" | [[red dwarf|M5.5V]]<ref name=RECONS/>
|0.113
| 13.09
| 15.26
| 272.1615<br>{{±|0.0316}}<ref name="GaiaEDR3"/>
| has 3 known planets (2019)<ref>{{Cite journal |journal=[[Monthly Notices of the Royal Astronomical Society]]
|last1=Dreizler |first1=S.
|last2=Jeffers |first2=S. V.
|last3=Rodríguez |first3=E.
|last4=Zechmeister |first4=M.
|last5=Barnes |first5 = J.R.
|last6=Haswell |first6=C.A.
|last7=Coleman |first7=G. A. L.
|last8=Lalitha |first8=S.
|last9=Hidalgo Soto |first9=D.
|last10=Strachan |first10=J.B.P.
|last11=Hambsch |first11=F-J.
|last12=López-González |first12=M. J.
|last13=Morales |first13=N.
|last14=Rodríguez López |first14=C.
|last15=Berdiñas |first15=Z. M.
|last16=Ribas |first16=I.
|last17=Pallé |first17=E.
|last18=Reiners |first18=Ansgar
|last19=Anglada-Escudé |first19=G.
|date=2019-08-13 |title=Red Dots: A temperate 1.5 Earth-mass planet in a compact multi-terrestrial planet system around GJ1061 |doi=10.1093/mnras/staa248 |arxiv=1908.04717| s2cid=199551874 |language=en |volume=493 |issue=1 |pages=536–550|doi-access=free |bibcode=2020MNRAS.493..536D }}</ref><ref name=henry1997>{{cite journal | last1 = Henry | first1 = Todd J. | last2 = Ianna | first2 = Philip A. | last3 = Kirkpatrick | first3 = J. Davy | last4 = Jahreiss | first4 = Hartmut | date = July 1997 | title = The solar neighborhood IV: discovery of the twentieth nearest star | journal = The Astronomical Journal | volume = 114 | issue = 1 | pages = 388–395 | doi = 10.1086/118482 | bibcode=1997AJ....114..388H}}</ref><ref name=henry2006>{{cite journal | last1 = Henry | first1 = Todd J. | last2 = Jao | first2 = Wei-Chun | last3 = Subasavage | first3 = John P. | last4 = Beaulieu | first4 = Thomas D. | last5 = Ianna | first5 = Philip A. | last6 = Costa | first6 = Edgardo | last7 = Méndez | first7 = René A. | date = December 2006 | title = The Solar Neighborhood. XVII. Parallax Results from the CTIOPI 0.9 m Program: 20 New Members of the RECONS 10 Parsec Sample | journal = The Astronomical Journal | volume = 132 | issue = 6| pages = 2360–2371 | doi = 10.1086/508233 | bibcode=2006AJ....132.2360H|arxiv = astro-ph/0608230  | s2cid = 15002841 }}</ref>
|-
| colspan="2" | [[YZ Ceti]] (LHS&nbsp;138)
| 12.1222<br>{{±|0.0015}}
| [[Cetus|Cet]]
| {{RA|01|12|30.6}}<br>{{DEC|−16|59|56}}
| style="background: {{star-color|M}};" | [[red dwarf|M4.5V]]<ref name=RECONS/>
|0.130
| 12.02
| 14.17
| 269.0573<br>{{±|0.0337}}<ref name="GaiaEDR3"/>
| flare star, three planets (b, c, and d) (2017)<ref>{{cite journal |doi=10.1051/0004-6361/201731581 |bibcode=2017A&A...605L..11A |arxiv=1708.03336 |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 & Astrophysics |volume=605 |pages=L11 |last1=Astudillo-Defru |first1=Nicola |last2=Díaz |first2=Rodrigo F. |last3=Bonfils |first3=Xavier |last4=Almenara |first4=José M. |last5=Delisle |first5=Jean-Baptiste |last6=Bouchy |first6=François |last7=Delfosse |first7=Xavier |last8=Forveille |first8=Thierry |last9=Lovis |first9=Christophe |last10=Mayor |first10=Michel |last11=Murgas |first11=Felipe |last12=Pepe |first12=Francesco |last13=Santos |first13=Nuno C. |last14=Ségransan |first14=Damien |last15=Udry |first15=Stéphane |last16=Wünsche |first16=Anaël |year=2017 |s2cid=119393757 }}</ref>
|-
| colspan="2" | [[Luyten's Star]] (BD+05°1668)
| 12.3485<br>{{±|0.0019}}
| [[Canis Minor|CMi]]
| {{RA|07|27|24.5}}<br>{{DEC|+05|13|33}}
| style="background: {{star-color|M}};" | [[red dwarf|M3.5Vn]]
|0.26
| 9.86
| 11.97
| 264.1269<br>{{±|0.0413}}<ref name="GaiaEDR3"/>
| two planets ([[Luyten b|b]], c) (2017)<ref>{{cite journal | doi=10.1051/0004-6361/201630153 
 | last1=Astudillo-Defru | first1=Nicola | last2=Forveille | first2=Thierry
 | last3=Bonfils  | first3=Xavier        | last4=Ségransan  | first4=Damien
 | last5=Bouchy   | first5=François      | last6=Delfosse   | first6=Xavier
 | last7=Lovis    | first7=Christophe    | last8=Mayor      | first8=Michel
 | last9=Murgas   | first9=Felipe        | last10=Pepe      | first10=Francesco
 | last11=Santos  | first11=Nuno C.      | last12=Udry      | first12=Stéphane
 | last13=Wünsche | first13=Anaël | display-authors=6
 | year=2017
 | title=The HARPS search for southern extra-solar planets. XLI. A dozen planets around the M&nbsp;dwarfs GJ&nbsp;3138, GJ&nbsp;3323, GJ&nbsp;273, GJ&nbsp;628, and GJ&nbsp;3293
 | journal=Astronomy and Astrophysics
 | volume=602  | at=A88
 | arxiv=1703.05386  | bibcode=2017A&A...602A..88A | s2cid=119418595
 | url=https://www.aanda.org/articles/aa/full_html/2017/06/aa30153-16/aa30153-16.html
}}</ref> and two suspected planets (d, e) (2019)<ref name="Pozuelos2020">{{cite journal|last1=Pozuelos|first1=Francisco J.|last2=13 more |display-authors=1|title=GJ 273: on the formation, dynamical evolution, and habitability of a planetary system hosted by an M dwarf at 3.75 parsec|journal=Astronomy & Astrophysics|volume=641|year=2020|pages=A23|doi=10.1051/0004-6361/202038047|arxiv=2006.09403|bibcode=2020A&A...641A..23P|s2cid=219721292}}</ref>
|-
| colspan="2" | [[Teegarden's Star]] (SO025300.5+165258)
| 12.4970<br>{{±|0.0045}}
| style="background-color: pink" | [[Aries (constellation)|Ari]]{{Asterisk}}
| {{RA|02|53|00.9}}<br>{{DEC|+16|52|53}}
| style="background: {{star-color|M}};" | [[red dwarf|M6.5V]]
|0.08
| 15.14
| 17.22
| 260.9884<br>{{±|0.0934}}<ref name="GaiaEDR3"/>
| has 3 known planets (2019, 2024)<ref>{{cite journal |last1=Caballero |first1=J. A. |last2=Reiners |first2=Ansgar |last3=Ribas |first3=I. |last4=Dreizler |first4=S. |last5=Zechmeister |first5=M. |display-authors=etal |date=12 June 2019 |title=The CARMENES search for exoplanets around M dwarfs. Two temperate Earth-mass planet candidates around Teegarden's Star |url=https://www.aanda.org/articles/aa/pdf/forth/aa35460-19.pdf |journal=Astronomy & Astrophysics |volume=627 |pages=A49 |language=en |doi=10.1051/0004-6361/201935460 |arxiv=1906.07196 |issn=0004-6361 |bibcode=2019A&A...627A..49Z |s2cid=189999121 }}</ref><ref name="Dreizler2024">{{cite journal |last1=Dreizler |first1=S. |last2=Luque |first2=R. |display-authors=etal |date=April 2024 |title=Teegarden's Star revisited: A nearby planetary system with at least three planets |journal=[[Astronomy & Astrophysics]] |volume=684 |issue= |pages=A117 |doi=10.1051/0004-6361/202348033 |arxiv=2402.00923 |bibcode=2024A&A...684A.117D}}</ref>
|-
| colspan="2" | [[Kapteyn's Star]] (CD−45°1841)
| 12.8308<br>{{±|0.0008}}
| style="background-color: pink" | [[Pictor|Pic]]{{Asterisk}}
| {{RA|05|11|40.6}}<br>{{DEC|−45|01|06}}
| style="background: {{star-color|M}};" | [[red dwarf|M1.5]][[subdwarf#Cool subdwarfs|VI]]<ref name=RECONS/> <!--Current RECONS link gives "M2.0VI"--><!--previous: sdM0VI-->
|0.281
| 8.84
| 10.87
| 254.1986<br>{{±|0.0168}}<ref name="GaiaEDR3"/>
| two refuted planets (b and c) (2014)<ref name="Kapteyn-discovery">{{cite journal|title=Two planets around Kapteyn's star : a cold and a temperate super-Earth orbiting the nearest halo red-dwarf |date=2014|arxiv=1406.0818|doi=10.1093/mnrasl/slu076 |volume=443 |journal=Monthly Notices of the Royal Astronomical Society: Letters |pages=L89–L93|bibcode = 2014MNRAS.443L..89A |hdl=2299/19219 |last1=Anglada-Escude|first1=G.|doi-access=free |s2cid=67807856|display-authors=etal}}</ref><ref name="BortleFausey2021">{{cite journal|last1=Bortle|first1=Anna|last2=Fausey|first2=Hallie|last3=Ji|first3=Jinbiao|last4=Dodson-Robinson|first4=Sarah|last5=Ramirez Delgado|first5=Victor|last6=Gizis|first6=John|display-authors=1|title=A Gaussian Process Regression Reveals No Evidence for Planets Orbiting Kapteyn's Star|journal=The Astronomical Journal|volume=161|issue=5|year=2021|pages=230|arxiv=2103.02709|doi=10.3847/1538-3881/abec89|bibcode=2021AJ....161..230B|s2cid=232110395 |doi-access=free }}</ref>
|-
| colspan="2" | [[Lacaille 8760]] (AX&nbsp;Microscopii)
| 12.9472<br>{{±|0.0018}}
| style="background-color: pink" | [[Microscopium|Mic]]{{Asterisk}}
| {{RA|21|17|15.3}}<br>{{DEC|−38|52|03}}
| style="background: {{star-color|M}};" | [[red dwarf|M0.0V]]<ref name=RECONS/> <!--previous: M2Ve-->
|0.60
| 6.67
| 8.69
| 251.9124<br>{{±|0.0352}}<ref name="GaiaEDR3"/>
| brightest [[M dwarf]] star in night sky, flare star
|-
| rowspan="2" | [[SCR 1845−6357]]
| A
| rowspan=2 | 13.0638<br>{{±|0.0070}}
| rowspan="2" style="background-color: pink" | [[Pavo (constellation)|Pav]]{{Asterisk}}
| {{RA|18|45|05.3}}<br>{{DEC|−63|57|48}}
| style="background: {{star-color|M}};" | [[red dwarf|M8.5V]]<ref name=RECONS/>
|0.07
| 17.39
| 19.41
| rowspan=2 | 249.6651<br>{{±|0.1330}}<ref name="GaiaEDR3"/>
| rowspan=2 | <ref name=henry2006/>
|-
| style="background: #D8BD98"| B§
| {{RA|18|45|02.6}}<br>{{DEC|−63|57|52}}
| style="background: {{star-color|T}};" | [[Brown dwarf#Spectral class T|T6]]<ref name=nearmt>{{Cite journal |bibcode = 2007A&A...471..655K|title = The very nearby M/T dwarf binary SCR 1845-6357|journal = Astronomy & Astrophysics|volume = 471|issue = 2|pages = 655|last1 = Kasper|first1 = M.|last2 = Biller|first2 = B. A.|last3 = Burrows|first3 = A.|last4 = Brandner|first4 = W.|last5 = Budaj|first5 = J.|last6 = Close|first6 = L. M.|year = 2007|arxiv = 0706.3824|doi = 10.1051/0004-6361:20077881|s2cid = 1860702}}</ref>
|0.03<ref name="RECONS" />
| 13.3 J<ref name="DwarfArchives"/>
| 15.3 J
|-
| rowspan="2" | [[Kruger 60]]<br>(BD+56°2783)
| A
| rowspan="2" | 13.0724<br>{{±|0.0052}}
| rowspan="2" style="background-color: pink" | [[Cepheus (constellation)|Cep]]{{Asterisk}}
| rowspan="2" | {{RA|22|27|59.5}}<br>{{DEC|+57|41|45}}
| style="background: {{star-color|M}};" | [[red dwarf|M3.0V]]<ref name="RECONS"/>
|0.271
| 9.79
| 11.76
| rowspan="2" | 249.5<br>{{±|0.1}}<ref name="GaiaDR2">{{cite Gaia DR2}}</ref>
| rowspan="2" | B flare star
|-
| B (DO&nbsp;Cephei)
| style="background: {{star-color|M}};" | [[red dwarf|M4.0V]]<ref name="RECONS"/>
|0.176
| 11.41
| 13.38
|-
| colspan="2" | [[DENIS J1048−3956|DENIS&nbsp;J1048−3956]]
| 13.1932<br>{{±|0.0027}}
| style="background-color: pink" | [[Antlia|Ant]]{{Asterisk}}
| {{RA|10|48|14.7}}<br>{{DEC|−39|56|06}}
| style="background: {{star-color|M}};" | [[red dwarf|M8.5V]]<ref name="RECONS"/>
|0.08
| 17.39
| 19.37
| 247.2156<br>{{±|0.0512}}<ref name="GaiaEDR3"/>
| <ref>{{Cite journal |bibcode = 2005AJ....129.1954J|title = The Solar Neighborhood. XIII. Parallax Results from the CTIOPI 0.9 Meter Program: Stars with μ >= 1.0" yr<suP>−1</SUP> (MOTION Sample)|journal = The Astronomical Journal|volume = 129|issue = 4|pages = 1954|last1 = Jao|first1 = Wei-Chun|last2 = Henry|first2 = Todd J.|last3 = Subasavage|first3 = John P.|last4 = Brown|first4 = Misty A.|last5 = Ianna|first5 = Philip A.|last6 = Bartlett|first6 = Jennifer L.|author6-link=Jennifer Bartlett (astronomer)|last7 = Costa|first7 = Edgardo|last8 = Méndez|first8 = René A.|year = 2005|doi = 10.1086/428489|arxiv = astro-ph/0502167|s2cid = 16164903}}</ref><ref name="costa2005">{{Cite journal |bibcode = 2005AJ....130..337C|title = The Solar Neighborhood. XIV. Parallaxes from the Cerro Tololo Inter-American Observatory Parallax Investigation-First Results from the 1.5 m Telescope Program|journal = The Astronomical Journal|volume = 130|issue = 1|pages = 337|last1 = Costa|first1 = Edgardo|last2 = Méndez|first2 = René A.|last3 = Jao|first3 = W. -C.|last4 = Henry|first4 = Todd J.|last5 = Subasavage|first5 = John P.|last6 = Brown|first6 = Misty A.|last7 = Ianna|first7 = Philip A.|last8 = Bartlett|first8 = Jennifer|author8-link=Jennifer Bartlett (astronomer)|year = 2005|doi = 10.1086/430473|doi-access = free}}</ref>
|-
| rowspan="2" | [[Ross 614]]<br>(V577&nbsp;Monocerotis, Gliese 234)
| A (LHS&nbsp;1849)
| rowspan="2" | 13.363<br>{{±|0.040}}
| rowspan="2" style="background-color: pink" | [[Monoceros (constellation)|Mon]]{{Asterisk}}
| rowspan="2" | {{RA|06|29|23.4}}<br>{{DEC|−02|48|50}}
| style="background: {{star-color|M}};" | [[red dwarf|M4.5V]]<ref name="RECONS"/>
|0.223
| 11.15
| 13.09
| rowspan="2" | 244.07<br>{{±|0.73}}<ref name="Gatewood">{{cite journal
| title=An Astrometric Study of the Low-Mass Binary Star Ross 614
| author=George Gatewood
| author-link=George Gatewood
| display-authors=etal
| url=http://www.iop.org/EJ/article/1538-3881/125/3/1530/202454.web.pdf?request-id=b6f1cb86-b810-4d37-8eb5-4adea768585d
| date=2003
| journal=[[The Astronomical Journal]]
| volume=125
| issue=3
| pages=1530–1536
| doi=10.1086/346143
| bibcode=2003AJ....125.1530G
| s2cid=119597659
| access-date=15 March 2022
| archive-date=19 December 2021
| archive-url=https://web.archive.org/web/20211219130826/https://www.iop.org/EJ/article/1538-3881/125/3/1530/202454.web.pdf?request-id=b6f1cb86-b810-4d37-8eb5-4adea768585d
| url-status=dead
}}</ref>
| rowspan="2" | A flare star
|-
| B (LHS&nbsp;1850)
| style="background: {{star-color|M}};" | [[red dwarf|M5.5V]]
|0.111
| 14.23
| 16.17
|-
| colspan="2" style="background: #D8BD98" |[[UGPS J0722-0540]]§
| 13.43<br>{{±|0.13}}
| [[Monoceros (constellation)|Mon]]
| {{RA|07|22|27.3}}<br>{{DEC|–05|40|30}}
| style="background: {{star-color|T}};" | [[brown dwarf#Spectral class T|T9]]<ref name="RECONS"/>
|0.010-0.025
| 16.52 J<ref>{{Cite journal | arxiv=1004.0317 | title=The discovery of a very cool, very nearby brown dwarf in the Galactic plane | date=2010 | last1=Bailer-Jones | first1=C. A. L. | last2=Rybizki | first2=J. | last3=Andrae | first3=R. | last4=Fouesneau | first4=M. | journal=Monthly Notices of the Royal Astronomical Society | volume=408 | issue=1 | pages=L56 | doi=10.1111/j.1745-3933.2010.00927.x | doi-access=free | bibcode=2010MNRAS.408L..56L | s2cid=16032606 }}</ref>
| 18.45 J
| 242.8<br>{{±|2.4}}<ref name="Leggett2012">{{cite journal  |last=Leggett |first=Sandy K.  |author2=Saumon, Didier  |author3=Marley, Mark S. |author4=Lodders, Katharina|author4-link=Katharina Lodders |author5=Canty, J. |author6=Lucas, Philip W. |author7=Smart, Richard L. |author8=Tinney, Chris G. |author9=Homeier, Derek |author10=Allard, France |author11=Burningham, Ben |author12=Day-Jones, Avril |author13=Fegley, Bruce  |author14=Ishii, Miki  |author15=Jones, Hugh R. A. |author16=Marocco, Federico |author17=Pinfield, David J. |author18=Tamura, Motohide |title=The Properties of the 500 K Dwarf UGPS J072227.51-054031.2 and a Study of the Far-red Flux of Cold Brown Dwarfs |date=2012 |journal=[[The Astrophysical Journal]] |volume=748 |issue=2 |pages=74 |arxiv=1201.2973 |doi=10.1088/0004-637X/748/2/74 |bibcode=2012ApJ...748...74L |s2cid=14171934 }}</ref>
| <ref name="Lucas2010v2">{{cite arXiv |title=Discovery of a very cool brown dwarf amongst the ten nearest stars to the Solar System|date=2010|eprint=1004.0317v1 |class=astro-ph.SR|last1=Bailer-Jones|first1=C. A. L.|last2=Rybizki|first2=J.|last3=Andrae|first3=R.|last4=Fouesneau|first4=M.}}</ref>
|-
| colspan="2" | [[Wolf 1061]] (Gliese 628, BD−12°4523)
| 14.0500<br>{{±|0.0016}}
| [[Ophiuchus|Oph]]
| {{RA|16|30|18.1}}<br>{{DEC|−12|39|45}}
| style="background: {{star-color|M}};" | [[red dwarf|M3.0V]]<ref name="RECONS"/>
|0.294
| 10.07
| 11.93
| 232.1390<br>{{±|0.0268}}<ref name="GaiaEDR3"/>
| three planets ([[Wolf 1061 b|b]], [[Wolf 1061 c|c]], and [[Wolf 1061 d|d]]) (2015)<ref>{{cite web
 | url =http://phys.org/news/2015-12-nearby-star-hosts-closest-alien.html
 | title =Nearby star hosts closest alien planet in the 'habitable zone'
 | date =December 16, 2015
 | website =[[Phys.org]]
 | access-date =2015-12-16
 | quote =The planet, more than four times the mass of the Earth, is one of three that the team detected around a red dwarf star called Wolf 1061.}}</ref>
|-
| colspan="2" style="background: #F5F5DC" | [[Van Maanen's Star]] (Gliese 35, LHS&nbsp;7){{Double-dagger|alt=white dwarf}}
| 14.0718<br>{{±|0.0011}}
| style="background-color: pink" | [[Pisces (constellation)|Psc]]{{Asterisk}}
| {{RA|00|49|09.9}}<br>{{DEC|+05|23|19}}
| style="background: #F5F5DC" | [[White dwarf|DZ7]]<ref name="RECONS"/>
|0.67
| 12.38
| 14.21
| 231.7800<br>{{±|0.0183}}<ref name="GaiaEDR3"/>
| closest-known free-floating white dwarf,<br>third-known white dwarf<br>possible debris disk (1917)
|-
| colspan="2" | [[Gliese 1]] (CD−37°15492)
| 14.1747<br>{{±|0.0022}}
| style="background-color: pink" | [[Sculptor (constellation)|Scl]]{{Asterisk}}
| {{RA|00|05|24.4}}<br>{{DEC|−37|21|27}}
| style="background: {{star-color|M}};" | [[red dwarf|M1.5 V]]<ref name="RECONS"/>
|0.45-0.48
| 8.55
| 10.35
| 230.0970<br>{{±|0.0362}}<ref name="GaiaEDR3"/>
| 
|-
| colspan="2" | [[TZ Arietis]] (Gliese 83.1, L 1159–16)
| 14.5780<br>{{±|0.0046}}
| [[Aries (constellation)|Ari]]
| {{RA|02|00|13.2}}<br>{{DEC|+13|03|08}}
| style="background: {{star-color|M}};" | [[red dwarf|M4.5V]]<ref name="RECONS"/>
|0.14
| 12.27
| 14.03
| 223.7321<br>{{±|0.0699}}<ref name="GaiaEDR3"/>
| flare star, has one confirmed planet (b)<ref name=Quirrenbach2022>{{citation |postscript=. | arxiv=2203.16504| last1=Quirrenbach| first1=A.| last2=Passegger| first2=V. M.| last3=Trifonov| first3=T.| last4=Amado| first4=P. J.| last5=Caballero| first5=J. A.| last6=Reiners| first6=A.| last7=Ribas| first7=I.| last8=Aceituno| first8=J.| last9=Bejar| first9=V. J. S.| last10=Chaturvedi| first10=P.| last11=Gonzalez-Cuesta| first11=L.| last12=Henning| first12=T.| last13=Herrero| first13=E.| last14=Kaminski| first14=A.| last15=Kuerster| first15=M.| last16=Lalitha| first16=S.| last17=Lodieu| first17=N.| last18=Lopez-Gonzalez| first18=M. J.| last19=Montes| first19=D.| last20=Palle| first20=E.| last21=Perger| first21=M.| last22=Pollacco| first22=D.| last23=Reffert| first23=S.| last24=Rodriguez| first24=E.| last25=Rodriguez Lopez| first25=C.| last26=Shan| first26=Y.| last27=Tal-Or| first27=L.| last28=Zapatero Osorio| first28=M. R.| last29=Zechmeister| first29=M.|display-authors=1| title=The CARMENES search for exoplanets around M dwarfs| journal=Astronomy & Astrophysics| year=2022| volume=663| pages=A48| doi=10.1051/0004-6361/202142915| s2cid=247835988 |bibcode=2022A&A...663A..48Q}}</ref>
|-
| rowspan="2" | [[Wolf 424]]<br>(FL&nbsp;Virginis, LHS&nbsp;333, Gliese 473)
| A
| rowspan="2" | 14.595<br>{{±|0.031}}
| rowspan="2" | [[Virgo (constellation)|Vir]]
| rowspan="2" | {{RA|12|33|17.2}}<br>{{DEC|+09|01|15}}
| style="background: {{star-color|M}};" | [[red dwarf|M5.5Ve]]
|0.143
| 13.18
| 14.97
| rowspan="2" | 223.4775<br>{{±|0.4665}}<ref name="GaiaEDR3"/>
| rowspan="2" | flare stars
|-
| B
| style="background: {{star-color|M}};" | [[red dwarf|M7Ve]]
|0.131
| 13.17
| 14.96
|-
| colspan="2" | [[Gliese 687]] (LHS&nbsp;450, BD+68°946)
| 14.8395<br>{{±|0.0014}}
| [[Draco (constellation)|Dra]]
| {{RA|17|36|25.9}}<br>{{DEC|+68|20|21}}
| style="background: {{star-color|M}};" | [[red dwarf|M3.0V]]<ref name="RECONS"/>
|0.401
| 9.17
| 10.89
| 219.7898<br>{{±|0.0210}}<ref name="GaiaEDR3"/>
| possible flare star, two planets (b) (2014)<ref name="GJ687b-discovery">[http://www.oklo.org/GL687.pdf The Lick–Carnegie exoplanet survey: Gliese 687 b: A Neptune-mass planet orbiting a nearby red dwarf] {{webarchive|url=https://web.archive.org/web/20140327221259/http://www.oklo.org/GL687.pdf |date=March 27, 2014 }}</ref> and (c) (2020)<ref name=Feng2020>{{citation|arxiv=2008.07998|title=Search for Nearby Earth Analogs. III. Detection of ten new planets, three planet candidates, and confirmation of three planets around eleven nearby M dwarfs|year=2020|last1=Feng|first1=Fabo|last2=Shectman|first2=Stephen A.|last3=Clement|first3=Matthew S.|last4=Vogt|first4=Steven S.|last5=Tuomi|first5=Mikko|last6=Teske|first6=Johanna K.|last7=Burt|first7=Jennifer|last8=Crane|first8=Jeffrey D.|last9=Holden|first9=Bradford|author10=Sharon Xuesong Wang|last11=Thompson|first11=Ian B.|last12=Diaz|first12=Matias R.|last13=Paul Butler|first13=R.|doi=10.3847/1538-4365/abb139|s2cid=221150644|volume=250|journal=The Astrophysical Journal Supplement Series|issue=2 |page=29 |doi-access=free |bibcode=2020ApJS..250...29F }}  Accepted for publication by [[The Astrophysical Journal Supplement Series|ApJS]]</ref>
|-
| colspan="2" | [[Gliese 674]] (LHS&nbsp;449)
| 14.8492<br>{{±|0.0018}}
| style="background-color: pink" | [[Ara (constellation)|Ara]]{{Asterisk}}
| {{RA|17|28|39.9}}<br>{{DEC|−46|53|43}}
| style="background: {{star-color|M}};" | [[red dwarf|M3.0V]]<ref name="RECONS"/>
|0.35
| 9.38
| 11.09
| 219.6463<br>{{±|0.0262}}<ref name="GaiaEDR3"/>
| one planet (b) (2007)<ref>{{cite encyclopedia|url=http://exoplanet.eu/star.php?st=GJ+674|archive-url=https://web.archive.org/web/20070702185803/http://exoplanet.eu/star.php?st=GJ+674|url-status=dead|archive-date=2 July 2007|encyclopedia=[[Extrasolar Planets Encyclopaedia]]|title=The Extrasolar Planet Encyclopaedia — Catalog Listing}}</ref>
|-
| colspan="2" | [[LHS 292]] (LP&nbsp;731-58)
| 14.8706<br>{{±|0.0041}}
| style="background-color: pink" | [[Sextans|Sex]]{{Asterisk}}
| {{RA|10|48|12.6}}<br>{{DEC|−11|20|14}}
| style="background: {{star-color|M}};" | [[red dwarf|M6.5V]]<ref name="RECONS"/>
|0.08
| 15.60
| 17.32
| 219.3302<br>{{±|0.0602}}<ref name="GaiaEDR3"/>
| flare star
|-
| colspan="2" style="background: #F5F5DC" | [[Gliese 440]] (WD&nbsp;1142-645, LP 145-141){{Double-dagger|alt=white dwarf}}
| 15.1226<br>{{±|0.0013}}
| style="background-color: pink" | [[Musca|Mus]]{{Asterisk}}
| {{RA|11|45|42.9}}<br>{{DEC|−64|50|29}}
| style="background: #F5F5DC" | [[White dwarf|DQ6]]<ref name="RECONS"/>
|0.75
| 11.50
| 13.18
| 215.6753<br>{{±|0.0181}}<ref name="GaiaEDR3"/>
| 
|-
| rowspan="3" | [[GJ 1245]]
| A (G&nbsp;208-44&nbsp;A)
| rowspan="3" | 15.2001<br>{{±|0.0034}}
| rowspan="3" | [[Cygnus (constellation)|Cyg]]
| {{RA|19|53|54.2}}<br>{{DEC|+44|24|55}}
| style="background: {{star-color|M}};" | [[red dwarf|M5.5V]]<ref name="RECONS"/>
|0.11
| 13.46
| 15.17
| rowspan="3" | 214.5745<br>{{±|0.0476}}<ref name="GaiaEDR3"/>
| rowspan="3" | flare stars
|-
| B (G&nbsp;208-45)
| {{RA|19|53|55.2}}<br>{{DEC|+44|24|56}}
| style="background: {{star-color|M}};" | [[red dwarf|M6.0V]]<ref name="RECONS"/>
|0.10
| 14.01
| 15.72
|-
| C (G&nbsp;208-44&nbsp;B)
| {{RA|19|53|54.2}}<br>{{DEC|+44|24|55}}
| style="background: {{star-color|M}};" | [[red dwarf|M5.5]]
|0.07
| 16.75
| 18.46
|-
| colspan="2" style="background: #D8BD98" | [[WISEPA J174124.26+255319.5|WISE 1741+2553]]§
| 15.22<br>{{±|0.20}}
| style="background-color: pink" | [[Hercules (constellation)|Her]]{{Asterisk}}
| {{RA|17|41|24.2}}<br>{{DEC|+25|53|19}}
| style="background: {{star-color|T}};" | [[Brown dwarf#Spectral class T|T9]]
| 
| 16.53 J
| 18.18 J
| 214.3<br>{{±|2.8}}<ref name="Kirkpatrick2019">{{Cite journal
 | doi = 10.3847/1538-4365/aaf6af
| title = Preliminary Trigonometric Parallaxes of 184 Late-T and Y Dwarfs and an Analysis of the Field Substellar Mass Function into the "Planetary" Mass Regime
| journal = [[The Astrophysical Journal Supplement]]
| volume = 240
| issue = 19
| year = 2019
| last1 = Kirkpatrick | first1 = J. Davy
| last2 = Martin | first2 = Emily C.
| last3 = Smart | first3 = Richard L.
| last4 = Cayago | first4 = Alfred J.
| last5 = Beichman | first5 = Charles A.
| last6 = Marocco | first6 = Federico
| last7 = Gelino | first7 = Christopher R.
| last8 = Faherty | first8 = Jacqueline K.
| last9 = Cushing | first9 = Michael C.
| last10 = Schneider | first10 = Adam C.
| last11 = Mace | first11 = Gregory N.
| last12 = Tinney | first12 = Christopher G.
| last13 = Wright | first13 = Edward L.
| last14 = Lowrance | first14 = Patrick J.
| last15 = Ingalls | first15 = James G.
| last16 = Vrba | first16 = Frederick J.
| last17 = Munn | first17 = Jeffrey A.
| last18 = Dahm | first18 = Scott E.
| last19 = McLean | first19 = Ian S. 
| page = 19
|arxiv = 1812.01208 |bibcode = 2019ApJS..240...19K | s2cid = 119451195
| doi-access = free
}}</ref>
|
|-
| colspan="2" | [[Gliese 876]] (Ross&nbsp;780)
| 15.2382<br>{{±|0.0025}}
| [[Aquarius (constellation)|Aqr]]
| {{RA|22|53|16.7}}<br>{{DEC|−14|15|49}}
| style="background: {{star-color|M}};" | [[red dwarf|M3.5V]]<ref name="RECONS"/>
|0.37
| 10.17
| 11.81
| 214.0380<br>{{±|0.0356}}<ref name="GaiaEDR3"/>
| four planets ([[Gliese 876 d|d]] (2005), [[Gliese 876 c|c]] (2001), [[Gliese 876 b|b]] (1998), and [[Gliese 876 e|e]] (2010))<ref>{{cite journal| last1=Rivera | first1=Eugenio J.| last2=Laughlin | first2=Gregory| last3=Butler | first3=R. Paul| last4=Vogt | first4=Steven S.| last5=Haghighipour | first5=Nader| last6=Meschiari | first6=Stefano| display-authors=1| title=The Lick-Carnegie Exoplanet Survey: A Uranus-mass Fourth Planet for GJ 876 in an Extrasolar Laplace Configuration| journal=The Astrophysical Journal| volume=719| issue=1| pages=890–899| date=July 2010 | doi=10.1088/0004-637X/719/1/890| bibcode=2010ApJ...719..890R | arxiv=1006.4244| s2cid=118707953}}</ref>
|-
| colspan="2" style="background: #D8BD98" | [[WISE 1639−6847]]§
| 15.336<br>{{±|0.066}}
| style="background-color: pink" | [[Triangulum Australe|TrA]]{{Asterisk}}
| {{RA|16|39|40.9}}<br>{{DEC|-68|47|46}}
| style="background: {{star-color|Y}};" | [[brown dwarf#Spectral class Y|Y0.5]]
|
| 20.57 J
| 22.10 J
| 212.67<br>{{±|0.91}}<ref name="Fontanive2024">{{cite arXiv |last1=Fontanive |first1=Clémence |last2=Bedin |first2=Luigi R. |last3=Albert |first3=Loïc |last4=Gagliuffi |first4=Daniella C. Bardalez |title=The Y Dwarf Population with HST: unlocking the secrets of our coolest neighbours -- II. Parallaxes and Proper Motions |date=21 December 2024 |class=astro-ph.SR |eprint=2412.16679}}</ref>
|
|-
| colspan="2" | [[LHS 288]] (Luyten&nbsp;143-23)
| 15.7586<br>{{±|0.0034}}
| style="background-color: pink" | [[Carina (constellation)|Car]]{{Asterisk}}
| {{RA|10|44|21.2}}<br>{{DEC|−61|12|36}}
| style="background: {{star-color|M}};" | [[red dwarf|M5.5V]]<ref name="RECONS"/>
|0.11<ref name="RECONS" />
| 13.90
| 15.51
| 206.9698<br>{{±|0.0448}}<ref name="GaiaEDR3"/>
| 
|-
| colspan="2" | [[GJ 1002]]
| 15.8060<br>{{±|0.0036}}
| [[Cetus|Cet]]
| {{RA|00|06|43.8}}<br>{{DEC|−07|32|22}}
| style="background: {{star-color|M}};" | [[red dwarf|M5.5V]]<ref name="RECONS"/>
|0.11
| 13.76
| 15.40
| 206.3500<br>{{±|0.0474}}<ref name="GaiaEDR3"/>
| two known planets (b & c, 2022)<ref name="SuárezMascareño2022">{{cite journal |last1=Suárez Mascareño |first1=A. |last2=González-Alvarez |first2=E. |display-authors=etal |date=November 2022 |title=Two temperate Earth-mass planets orbiting the nearby star GJ 1002 |journal=[[Astronomy & Astrophysics]] |volume= 670|issue= |pages= A5|doi=10.1051/0004-6361/202244991 |arxiv=2212.07332|bibcode=2023A&A...670A...5S |s2cid=254353639 }}</ref>
|-
| colspan="2" style="background: #D8BD98" | [[DENIS 0255−4700|DENIS&nbsp;0255−4700]]§
| 15.877<br>{{±|0.014}}
| [[Eridanus (constellation)|Eri]]
| {{RA|02|55|03.7}}<br>{{DEC|−47|00|52}}
| style="background: {{star-color|L}};" | [[Brown dwarf#Spectral class L|L7.5V]]<ref name="RECONS"/>
|0.025-0.065
| 22.92
| 24.44
| 205.4251<br>{{±|0.1857}}<ref name="GaiaEDR3"/>
| <ref name="costa2005"/>
|-
| colspan="2" style="background-color: lightgreen" | [[Groombridge 1618]] (Gliese 380){{Dollar sign}}
| 15.8857<br>{{±|0.0017}}
| [[Ursa Major|UMa]]
| {{RA|10|11|22.1}}<br>{{DEC|+49|27|15}}
| style="background: {{star-color|K}};" | [[K-type main-sequence star|K7.0V]]<ref name="RECONS"/>
|0.67
| 6.59
| 8.16
| 205.3148<br>{{±|0.0224}}<ref name="GaiaEDR3"/>
| flare star, one suspected debris disk
|-
| rowspan="2" | [[Gliese 412]]
| A
| rowspan="2" | 15.9969<br>{{±|0.0026}}
| rowspan="2" | [[Ursa Major|UMa]]
| {{RA|11|05|28.6}}<br>{{DEC|+43|31|36}}
| style="background: {{star-color|M}};" | [[red dwarf|M1.0V]]<ref name="RECONS"/>
|0.48
| 8.77
| 10.34
| rowspan="2" | 203.8876<br>{{±|0.0332}}<ref name="GaiaEDR3"/>
|
|-
| B (WX&nbsp;Ursae&nbsp;Majoris)
| {{RA|11|05|30.4}}<br>{{DEC|+43|31|18}}
| style="background: {{star-color|M}};" | [[red dwarf|M5.5V]]<ref name="RECONS"/>
|0.10
| 14.48
| 16.05
| flare star
|-
| colspan="2" | [[AD Leonis]]
| 16.1939<br>{{±|0.0024}}
| [[Leo (constellation)|Leo]]
| {{RA|10|19|36.4}}<br>{{DEC|+19|52|10}}
| style="background: {{star-color|M}};" | [[red dwarf|M3.0V]]<ref name="RECONS"/>
|0.39-0.42
| 9.32
| 10.87
| 201.4064<br>{{±|0.0296}}<ref name="GaiaEDR3"/>
| flare star, one refuted planet (b<ref name="Frequency of planets orbiting M dwa"/> in 2020)<ref name=GAPS2020>{{cite journal|last1=Carleo |first1=I.|last2=29 more |display-authors=1|year=2020|title=The GAPS Programme at TNG&nbsp;XXI – A GIARPS case-study of known young planetary candidates: Confirmation of HD&nbsp;285507&nbsp;b and refutation of AD&nbsp;Leo&nbsp;b|journal=Astronomy & Astrophysics|volume=A5|page=638|doi=10.1051/0004-6361/201937369|arxiv=2002.10562 |bibcode=2020A&A...638A...5C|s2cid=211296466}}</ref>
|-
| colspan="2" | [[Gliese 832]]
| 16.2005<br>{{±|0.0019}}
| style="background-color: pink" | [[Grus (constellation)|Gru]]{{Asterisk}}
| {{RA|21|33|34.0}}<br>{{DEC|−49|00|32}}
| style="background: {{star-color|M}};" | [[red dwarf|M1.5 V]]<ref name="RECONS"/>
|0.45
| 8.66
| 10.20
| 201.3252<br>{{±|0.0237}}<ref name="GaiaEDR3"/>
| possible flare star, two planets; one confirmed ([[Gliese 832 b|b]] (2008)),<ref>{{cite journal | last=Bailey |first=Jeremy | display-authors=etal | title=A Jupiter-like Planet Orbiting the Nearby M Dwarf GJ832 | doi=10.1088/0004-637X/690/1/743 | bibcode=2009ApJ...690..743B | journal=The Astrophysical Journal | volume=690 | issue=1 | pages=743–747 | arxiv=0809.0172 | year=2009 |s2cid=17172233 }}</ref> and the other now refuted ([[Gliese 832 c|c]] (2014))<ref>{{Cite journal|arxiv=1406.5587|title= GJ 832c: A super-earth in the habitable zone|journal= The Astrophysical Journal|volume= 791|issue= 2|pages= 114|last1=  Wittenmyer|first1= R. A.|last2= Tuomi |display-authors=etal |year= 2014|doi= 10.1088/0004-637X/791/2/114|bibcode=2014ApJ...791..114W|s2cid= 12157837}}</ref><ref name="Gorrini Astudillo-Defru Dreizler Damasso 2022 p=A64">{{cite journal | last1=Gorrini | first1=P. | last2=Astudillo-Defru | first2=N. | last3=Dreizler | first3=S. | last4=Damasso | first4=M. | last5=Díaz | first5=R. F. | last6=Bonfils | first6=X. | last7=Jeffers | first7=S. V. | last8=Barnes | first8=J. R. | last9=Del Sordo | first9=F. | last10=Almenara | first10=J.-M. | last11=Artigau | first11=E. | last12=Bouchy | first12=F. | last13=Charbonneau | first13=D. | last14=Delfosse | first14=X. | last15=Doyon | first15=R. | last16=Figueira | first16=P. | last17=Forveille | first17=T. | last18=Haswell | first18=C. A. | last19=López-González | first19=M. J. | last20=Melo | first20=C. | last21=Mennickent | first21=R. E. | last22=Gaisné | first22=G. | last23=Morales | first23=N. Morales | last24=Murgas | first24=F. | last25=Pepe | first25=F. | last26=Rodríguez | first26=E. | last27=Santos | first27=N. C. | last28=Tal-Or | first28=L. | last29=Tsapras | first29=Y. | last30=Udry | first30=S.|display-authors=3 | title=Detailed stellar activity analysis and modelling of GJ 832 | journal=Astronomy & Astrophysics | publisher=EDP Sciences | volume=664 | year=2022 | issn=0004-6361 | doi=10.1051/0004-6361/202243063 |doi-access=free | page=A64| arxiv=2206.07552 | bibcode=2022A&A...664A..64G }}</ref>
|-
| colspan = '2' | [[Gliese 682]] (CD-44 11909)
| 16.3328<br>{{±|0.0026}}
| style="background-color: pink" | [[Scorpius|Sco]]{{Asterisk}}
| {{RA|17|37|03.7}}<br>{{DEC|–44|19|09}}
| style="background: {{star-color|M}};" | [[red dwarf|M4 V]]
| 0.27
| 10.95
| 12.45
| 199.6944<br>{{±|0.0312}}<ref name="GaiaEDR3"/>
| has two disputed planets
|-
| rowspan='3' | [[40 Eridani|Omicron<sup>2</sup> Eridani]]<br />(40&nbsp;Eridani, Gliese&nbsp;166)
 | style="background-color: lightgreen" | Keid (A){{Dollar sign}}
| rowspan="3" |16.3330<br>{{±|0.0042}}
| rowspan='3' |[[Eridanus (constellation)|Eri]]
|{{RA|04|15|16.3}}<br>{{DEC|-07|39|10}}
| style="background: {{star-color|K}};" | [[K-type main-sequence star|K0.5 V]]
| 0.84
| style="background: lightblue;" | 4.43{{Hash-tag|alt=visible to naked eye}}
| 5.93
| rowspan="3" |199.6911<br>{{±|0.0512}}<ref name="GaiaEDR3"/>
| has one refuted planet
|-
 | style="background: #F5F5DC" | B{{Double-dagger|alt=white dwarf}}
| {{RA|04|15|21.8}}<br>{{DEC|−07|39|29}}
| style="background: #F5F5DC" | [[White dwarf|DA4]]
| 0.573
| 9.52
| 11.02
|
|-
 | C
| {{RA|04|15|21.5}}<br>{{DEC|−07|39|22}}
| style="background: {{star-color|M}};" | [[red dwarf|M4 V]]
| 0.2036
| 11.24
| 12.74
|
|-
| colspan = '2' | [[EV Lacertae]]
| 16.4761<br>{{±|0.0018}}
| style="background-color: pink" | [[Lacerta|Lac]]{{Asterisk}}
| {{RA|22|46|49.7}}<br>{{DEC|+44|20|02}}
| style="background: {{star-color|M}};" | [[red dwarf|M3.5 V]]
| 0.35
| 10.22
| 11.70
| 197.9573<br>{{±|0.0220}}<ref name="GaiaEDR3"/>
| record setting stellar flare observed
|-
| rowspan='2' | [[70 Ophiuchi]] (Gliese&nbsp;702)
 | style="background-color: lightgreen" | A{{Dollar sign}}
| rowspan='2' | 16.7074<br>{{±|0.0087}}
| rowspan='2' | [[Ophiuchus|Oph]]
| {{RA|18|05|27.4}}<br>{{DEC|+02|29|59}}
| style="background: {{star-color|K}};" | [[K-type main-sequence star|K0 V]]
| 0.90
| style="background: lightblue;" | 4.21{{Hash-tag|alt=visible to naked eye}}
| 5.66
| rowspan='2' | 195.2166<br>{{±|0.1012}}<ref name="GaiaDR2">{{cite Gaia DR2}}</ref>
| rowspan="2" |
|-
 | style="background-color: lightgreen" | B{{Dollar sign}}
| {{RA|18|05|27.5}}<br>{{DEC|+02|29|56}}
| style="background: {{star-color|K}};" | [[K-type main-sequence star|K5 V]]
| 0.70
| style="background: lightblue;" | 6.01{{Hash-tag|alt=visible to naked eye}}
| 7.46
|-
| colspan = '2' style="background-color: lightgreen" | [[Altair]] (Alpha&nbsp;Aquilae){{Dollar sign}}
| 16.730<br>{{±|0.049}}
| style="background-color: pink" | [[Aquila (constellation)|Aql]]{{Asterisk}}
| {{RA|19|50|47.0}}<br>{{DEC|+08|52|06}}
| style="background: {{star-color|A}}" | [[A-type main-sequence star|A7 IV-Vn]]
| 1.79
| style="background: lightblue;" | 0.77{{Hash-tag|alt=visible to naked eye}}
| 2.22
| 194.95<br>{{±|0.57}}<ref name=aaa474_2_653>{{citation | last1=van Leeuwen | first1=F. | title=Validation of the new Hipparcos reduction | journal=Astronomy and Astrophysics | volume=474 | issue=2 |date=November 2007 | pages=653–664 | doi=10.1051/0004-6361:20078357 | bibcode=2007A&A...474..653V | arxiv=0708.1752 | s2cid=18759600 }}</ref>
|
|-
| rowspan='2' | [[G 9-38|EI Cancri]] (GJ&nbsp;1116, {{nowrap|G 9-38}})
 | A
| rowspan='2' | 16.800<br>{{±|0.011}}
| rowspan='2' | [[Cancer (constellation)|Cnc]] 
| rowspan='2' | {{RA|08|58|15.2}}<br>{{DEC|+19|45|47}}
| style="background: {{star-color|M}};" | [[red dwarf|M5.5 V]]
| 0.12
| 14.06
| 15.50
| rowspan='2' | 194.1443<br>{{±|0.1228}}<ref name="GaiaEDR3"/>
| rowspan="2" |
|-
 | B
| style="background: {{star-color|M}};" | [[red dwarf|M V]]
| 0.10
| 14.92
| 16.36
|-
| colspan = '2' style="background: #D8BD98" | [[WISE 1506+7027|WISE J150649.97+702736.1]]§
| 16.856<br>{{±|0.052}}
| style="background-color: pink" | [[Ursa Minor|UMi]]{{Asterisk}}
| {{RA|15|06|52.4}}<br>{{DEC|+70|27|25}}
| style="background: {{star-color|T}};" | [[Brown dwarf#Spectral class T|T6]]
|
| 13.74 J
| 15.17 J
| 193.5<br>{{±|0.6}}<ref name="Kirkpatrick2019"/>
|
|-
| colspan = '2' | [[GJ 3379]] ({{nowrap|G 99-49}})
| 16.9861<br>{{±|0.0027}}
| style="background-color: pink" | [[Orion (constellation)|Ori]]{{Asterisk}}
| {{RA|06|00|03.5}}<br>{{DEC|+02|42|24}}
| style="background: {{star-color|M}};" | [[red dwarf|M3.5 V]]
| 0.2312
| 11.31
| 12.73
| 192.0135<br>{{±|0.0310}}<ref name="GaiaEDR3"/>
|
|-
| colspan = '2' style="background: #D8BD98" | [[DENIS J081730.0−615520]]§
| 17.002<br>{{±|0.037}}
| [[Carina (constellation)|Car]]
| {{RA|08|17|30.1}}<br>{{DEC|−61|55|16}}
| style="background: {{star-color|T}};" | [[Brown dwarf#Spectral class T|T6]]
| 0.015
| 13.61 J
| 15.03 J
| 191.8362<br>{{±|0.4186}}<ref name="GaiaEDR3"/>
|
|-
| colspan = '2' | [[Gliese 445]] (LHS&nbsp;2459, {{nowrap|G 254-29}})
| 17.1368<br>{{±|0.0017}}
| style="background-color: pink" | [[Camelopardalis|Cam]]{{Asterisk}}
| {{RA|11|47|41.4}}<br>{{DEC|+78|41|28}}
| style="background: {{star-color|M}};" | [[red dwarf|M3.5 V]]
| 0.14
| 10.79
| 12.19
| 190.3251<br>{{±|0.0194}}<ref name="GaiaEDR3"/>
|
|-
| colspan = '2' | [[2MASS J15404342−5101357]]
| 17.3738<br>{{±|0.0046}}
| style="background-color: pink" | [[Norma (constellation)|Nor]]{{Asterisk}}
| {{RA|15|40|43.5}}<br>{{DEC|-51|01|36}}
| style="background: {{star-color|M}};" | [[red dwarf|M7 V]]
| 0.090
| 15.26
| 16.63
| 187.7290<br>{{±|0.0496}}<ref name="GaiaEDR3"/>
|  
|-
| rowspan='2' | [[2MASS J09393548−2448279|2MASS 0939−2448]]
| style="background: #D8BD98" | A§
| rowspan='2' | 17.41<br>{{±|0.44}}
| rowspan='2' | [[Antlia|Ant]]
| rowspan='2' | {{RA|09|39|35.5}}<br>{{DEC|−24|48|28}}
| style="background: {{star-color|T}};" | [[Brown dwarf#Spectral class T|T8 V]]
| 0.019–0.048
| 15.61 J
| 16.97 J
| rowspan='2' | 187.3<br>{{±|4.6}}<ref name="Burgasser2008">{{cite journal |last1=Burgasser |first1=Adam J. |last2=Tinney |first2=C. G.  |last3=Cushing |first3=Michael C. |last4=Saumon |first4=Didier |last5=Marley |first5=Mark S. |last6=Bennett |first6=Clara S. |last7=Kirkpatrick |first7=J. Davy |title=2MASS J09393548-2448279: The Coldest and Least Luminous Brown Dwarf Binary Known? |date=2008 |journal=[[The Astrophysical Journal]] |volume=689 | issue=1 | pages=L53–L56  |doi=10.1086/595747 |bibcode=2008ApJ...689L..53B|url=https://authors.library.caltech.edu/13440/1/BURapjl08.pdf |doi-access=free }}</ref>
| rowspan='2' | binary brown dwarf 
|-
| style="background: #D8BD98" | B§
| style="background: {{star-color|T}};" | [[Brown dwarf#Spectral class T|T8 V]]
| 0.019–0.038
| 
|
|-
| colspan = '2' | [[GJ 3323]] (LHS 1723, {{nowrap|LP 656-38}})
| 17.5309<br>{{±|0.0026}}
| [[Eridanus (constellation)|Eri]]
| {{RA|05|01|57.4}}<br>{{DEC|−06|56|46}}
| style="background: {{star-color|M}};" | [[red dwarf|M4 V]]
| 0.1705
| 12.22
| 13.57
| 186.0466<br>{{±|0.0277}}<ref name="GaiaEDR3"/>
| has two known planets
|-
| colspan = '2' | [[Gliese 526]] (Wolf&nbsp;498, HD&nbsp;119850)
|17.7263<br>{{±|0.0024}}
| style="background-color: pink" | [[Boötes|Boo]]{{Asterisk}}
| {{RA|13|45|43.8}}<br>{{DEC|+14|53|29}}
| style="background: {{star-color|M}};" | [[red dwarf|M1 V]]
| 0.28
| 8.46
| 9.78
| 183.9962<br>{{±|0.0253}}<ref name="GaiaEDR3"/>
|
|-
| colspan = '2' style="background: #D8BD98" | [[WISE 0350−5658]]§
| 17.84<br>{{±|0.30}}
| style="background-color: pink" | [[Reticulum|Ret]]{{Asterisk}}
| {{RA|03|50|00.3}}<br>{{DEC|-56|58|30}}
| style="background: {{star-color|Y}};" | [[Brown dwarf#Spectral class Y|Y1]]
|
| 22.47 J
| 23.70 J
| 182.9<br>{{±|3.1}}<ref name="Fontanive2024"/>
|
|-
| rowspan='2' | [[Stein 2051]] (Gliese&nbsp;169.1, {{nowrap|G 175-34}})
 | A
| rowspan='2' | 17.9925<br>{{±|0.0020}}
| rowspan='2' | [[Camelopardalis|Cam]]
| {{RA|04|31|11.5}}<br>{{DEC|+58|58|37}}
| style="background: {{star-color|M}};" | [[red dwarf|M4 V]]
| 0.252
| 11.04
| 12.33
| rowspan='2' | 181.2730<br>{{±|0.0203}}<ref name="GaiaEDR3"/>
| rowspan="2" |
|-
 | style="background: #F5F5DC" | B{{Double-dagger|alt=white dwarf}}
| {{RA|04|31|12.6}}<br>{{DEC|+58|58|41}}
| style="background: #F5F5DC" | [[White dwarf|DC5]]
| 0.675
| 12.43
| 13.72
|-
| colspan = '2' style="background: #D8BD98" | [[2MASS J11145133−2618235]]§
| 18.20<br>{{±|0.14}}
| [[Hydra (constellation)|Hya]]
| {{RA|11|14|51.3}}<br>{{DEC|−26|18|24}}
| style="background: {{star-color|T}};" | [[Brown dwarf#Spectral class T|T7.5]]
| 0.029–0.048
| 15.86 J
| 17.12 J
| 179.2<br>{{±|1.4}}<ref name="Dupuy &amp; Liu2012">{{cite journal  |last1=Dupuy |first1=Trent J.  |last2=Liu |first2=Michael C.  |title=The Hawaii Infrared Parallax Program. I. Ultracool Binaries and the L/T Transition  |year=2012  |journal=[[The Astrophysical Journal Supplement]]  |volume=201 | issue=2 | pages=19  |arxiv=1201.2465  |doi=10.1088/0067-0049/201/2/19  |bibcode=2012ApJS..201...19D|s2cid=119256363 }}</ref>
|
|-
| colspan = '2' | [[Gliese 251]] (Wolf&nbsp;294, HD&nbsp;265866)
| 18.2146<br>{{±|0.0028}}
| style="background-color: pink" | [[Gemini (constellation)|Gem]]{{Asterisk}}
| {{RA|06|54|49.0}}<br>{{DEC|+33|16|05}}
| style="background: {{star-color|M}};" | [[red dwarf|M3 V]]
| 0.360
| 10.02
| 11.29
| 179.0629<br>{{±|0.0280}}<ref name="GaiaEDR3"/>
| has one known planet
|-
| colspan = '2' | [[LP 816-60]]
| 18.3305<br>{{±|0.0038}}
| style="background-color: pink" | [[Capricornus|Cap]]{{Asterisk}}
| {{RA|20|52|33.0}}<br>{{DEC|-16|58|29}}
| style="background: {{star-color|M}};" | [[red dwarf|M3.5 V]]
| 0.224
| 11.50
| 12.75
| 177.9312<br>{{±|0.0365}}<ref name="GaiaEDR3"/>
|
|-
| colspan = '2' | [[LSR J1835+3259]]
| 18.5534<br>{{±|0.0049}}
| style="background-color: pink" | [[Lyra|Lyr]]{{Asterisk}}
| {{RA|18|35|37.9}}<br>{{DEC|+32|59|55}}
| style="background: {{star-color|M}};" | [[red dwarf|M8.5 V]]
| 0.053
| 18.27
| 19.50
| 175.7930<br>{{±|0.0468}}<ref name="GaiaEDR3"/>
|
|-
| colspan = '2' | [[Gliese 205]] (Wolf&nbsp;1453, HD&nbsp;36395)
| 18.6042<br>{{±|0.0022}}
| [[Orion (constellation)|Ori]]
| {{RA|05|31|27.4}}<br>{{DEC|−03|40|38}}
| style="background: {{star-color|M}};" | [[red dwarf|M1 V]]
| 0.556
| 7.95
| 9.17
| 175.3131<br>{{±|0.0204}}<ref name="GaiaEDR3"/>
| 
|-
| colspan = '2' style="background: #D8BD98" | [[2MASS J04151954−0935066]]§
| 18.62<br>{{±|0.18}}
| [[Eridanus (constellation)|Eri]]
| {{RA|04|15|19.5}}<br>{{DEC|−09|35|07}}
| style="background: {{star-color|T}};" | [[Brown dwarf#Spectral class T|T8]]
| 0.03
| 15.34 J
| 16.56 J
| 175.2<br>{{±|1.7}}<ref name="Dupuy &amp; Liu2012"/>
|
|-
| rowspan='3' | [[Gliese 229]] (HD&nbsp;42581)
 | A
| rowspan='3' | 18.7906<br>{{±|0.0018}}
| rowspan='3' style="background-color: pink" | [[Lepus (constellation)|Lep]]{{Asterisk}}
| rowspan='3' | {{RA|06|10|34.6}}<br>{{DEC|−21|51|53}}
| style="background: {{star-color|M}};" | [[red dwarf|M1.5 V]]
| 0.579
| 8.14
| 9.34
| rowspan='3' | 173.5740<br>{{±|0.0170}}<ref name="GaiaEDR3"/>
| rowspan="3" | <ref name="Xuan2024">{{Cite journal |last1=Xuan |first1=Jerry W. |last2=Mérand |first2=A. |last3=Thompson |first3=W. |last4=Zhang |first4=Y. |last5=Lacour |first5=S. |last6=Blakely |first6=D. |last7=Mawet |first7=D. |last8=Oppenheimer |first8=R. |last9=Kammerer |first9=J. |last10=Batygin |first10=K. |last11=Sanghi |first11=A. |last12=Wang |first12=J. |last13=Ruffio |first13=J.-B. |last14=Liu |first14=M. C. |last15=Knutson |first15=H. |date=2024-10-16 |title=The cool brown dwarf Gliese 229 B is a close binary |journal=Nature |volume=634 |issue=8036 |language=en |pages=1070–1074 |arxiv=2410.11953 |doi=10.1038/s41586-024-08064-x |pmid=39415016 |bibcode=2024Natur.634.1070X |issn=1476-4687}}</ref>
|-
 | style="background: #D8BD98" | Ba§
| style="background: {{star-color|T}};" | [[Brown dwarf#Spectral class T|T7]]
| 0.036
| rowspan=2 | 14.01 J
| rowspan=2 | 15.21 J
|-
 | style="background: #D8BD98" | Bb§
| style="background: {{star-color|T}};" | [[Brown dwarf#Spectral class T|T8]]
| 0.033
|-
| colspan = '2' style="background-color: lightgreen" | [[Sigma Draconis|Alsafi]] (Sigma Draconis){{Dollar sign}}
| 18.7993<br>{{±|0.0081}}
| [[Draco (constellation)|Dra]]
| {{RA|19|32|21.6}}<br>{{DEC|+69|39|40}}
| style="background: {{star-color|G}};" | [[G-type main-sequence star|G9 V]]
| 0.85
| style="background: lightblue;" | 4.67{{Hash-tag|alt=visible to naked eye}}
| 5.87
| 173.4939<br>{{±|0.0748}}<ref name="GaiaEDR3"/>
| 
|-
| colspan = '2' | [[Ross 47]] (Gliese&nbsp;213)
| 18.8883<br>{{±|0.0031}}
| [[Orion (constellation)|Ori]]
| {{RA|05|42|09.3}}<br>{{DEC|+12|29|21}}
| style="background: {{star-color|M}};" | [[red dwarf|M4 V]]
| 0.35
| 11.57
| 12.76
| 172.6762<br>{{±|0.0286}}<ref name="GaiaEDR3"/>
|
|-
| colspan = '2' style="background: #D8BD98" | [[WISE 1541−2250]]§
| 18.93<br>{{±|0.17}}
| [[Libra (constellation)|Lib]]
| {{RA|15|41|51.6}}<br>{{DEC|−22|50|25}}
| style="background: {{star-color|Y}};" | [[Brown dwarf#Spectral class Y|Y0.5]] 
| 0.011
| 20.99 J
| 22.10 J
| 172.3<br>{{±|1.6}}<ref name="Fontanive2024"/>
|
|-
| rowspan='4' | [[Gliese 570]]<br />(Lalande&nbsp;27173, 33&nbsp;G.&nbsp;Librae)
 | style="background-color: lightgreen" | A{{Dollar sign}}
| rowspan='4' | 19.1987<br>{{±|0.0074}}
| rowspan='4' style="background-color: pink" | [[Libra (constellation)|Lib]]{{Asterisk}}
| rowspan='4' | {{RA|14|57|28.0}}<br>{{DEC|-21|24|56}}
| style="background: {{star-color|K}};" | [[K-type main-sequence star|K4 V]]
| 0.802
| style="background: lightblue;" | 5.64{{Hash-tag|alt=visible to naked eye}}
| 6.79
| rowspan='4' | 169.8843<br>{{±|0.0653}}<ref name="GaiaEDR3"/>
| rowspan='4' |
|-
 | B
| style="background: {{star-color|M}};" | [[red dwarf|M1.5 V]]
| 0.55
| 8.30
| 9.45
|-
 | C
| style="background: {{star-color|M}};" | [[red dwarf|M]]
| 0.35
| 9.96
| 11.11
|-
 | style="background: #D8BD98" | D§
| style="background: {{star-color|T}};" | [[Brown dwarf#Spectral class T|T7.5]]
| 0.05
| 15.32 J
| 16.47 J
|-
| colspan = '2' | [[Gliese 693]] (Luyten 205–128)
| 19.2078<br>{{±|0.0053}}
| [[Pavo (constellation)|Pav]]
| {{RA|17|46|32.4}}<br>{{DEC|-57|19|09}}
| style="background: {{star-color|M}};" | [[red dwarf|M3 V]]
| 0.26
| 10.76
| 11.91
| 169.8042<br>{{±|0.0465}}<ref name="GaiaEDR3"/>
|  
|-
| colspan = '2' | [[Gliese 754]] (Luyten 347–14)
| 19.2724<br>{{±|0.0067}}
| style="background-color: pink" | [[Telescopium|Tel]]{{Asterisk}}
| {{RA|19|20|48.0}}<br>{{DEC|−45|33|30}}
| style="background: {{star-color|M}};" | [[red dwarf|M4 V]]
| 0.173
| 12.23
| 13.37
| 169.2351<br>{{±|0.0588}}<ref name="GaiaEDR3"/>
| has one candidate planet
|-
| colspan = '2' | [[Gliese 908]] (Lalande&nbsp;46650, BR&nbsp;Piscium)
| 19.2745<br>{{±|0.0032}}
| [[Pisces (constellation)|Psc]]
| {{RA|23|49|12.5}}<br>{{DEC|+02|24|04}}
| style="background: {{star-color|M}};" | [[red dwarf|M1 V]]
| 0.37
| 8.98
| 10.12
| 169.2163<br>{{±|0.0281}}<ref name="GaiaEDR3"/>
|  
|-
| rowspan='2' | [[Gliese 752]] (Wolf&nbsp;1055, HD&nbsp;180617)
 | A
| rowspan='2' | 19.2922<br>{{±|0.0027}}
| rowspan='2' | [[Aquila (constellation)|Aql]]
| {{RA|19|16|55.3}}<br>{{DEC|+05|10|08}}
| style="background: {{star-color|M}};" | [[red dwarf|M2.5 V]]
| 0.46
| 9.10
| 10.24
| rowspan='2' | 169.0615<br>{{±|0.0239}}<ref name="GaiaEDR3"/>
| has one known planet
|-
 | [[VB 10|B]] {{Nowrap|(VB 10)}}
| {{RA|19|16|57.6}}<br>{{DEC|+05|09|02}}
| style="background: {{star-color|M}};" | [[red dwarf|M8 V]]
| 0.075
| 17.45
| 18.59
| very small and very dim red dwarf 
|-
| colspan = '2' | [[Gliese 588]] (CD-40 9712)
| 19.2996<br>{{±|0.0031}}
| style="background-color: pink" | [[Lupus (constellation)|Lup]]{{Asterisk}}
| {{RA|15|32|12.9}}<br>{{DEC|-41|16|32}}
| style="background: {{star-color|M}};" | [[red dwarf|M2.5 V]]
| 0.43
| 9.31
| 10.45
| 168.9965<br>{{±|0.0270}}<ref name="GaiaEDR3"/>
| has two candidate planets
|-
| rowspan='2' | [[Eta Cassiopeiae]] (Gliese&nbsp;34)
 | style="background-color: lightgreen" | Achird (A){{Dollar sign}}
| rowspan='2' | 19.3314<br>{{±|0.0025}}
| rowspan='2' style="background-color: pink" | [[Cassiopeia (constellation)|Cas]]{{Asterisk}}
| rowspan='2' | {{RA|00|49|06.3}}<br>{{DEC|+57|48|55}}
| style="background: {{star-color|G}};" | [[G-type main-sequence star|G3 V]]
| 0.972
| style="background: lightblue;" | 3.46{{Hash-tag|alt=visible to naked eye}}
| 4.60
| rowspan='2' | 168.7186<br>{{±|0.0216}}<ref name="GaiaEDR3"/>
| rowspan="2" |
|-
 | B
| style="background: {{star-color|K}};" | [[K-type main-sequence star|K7 V]]
| 0.57
| 7.51
| 8.65
|-
| rowspan='3' | [[36 Ophiuchi]] (Gliese&nbsp;663)
 | style="background-color: lightgreen" | Guniibuu (A){{Dollar sign}}
| rowspan='3' | 19.4185<br>{{±|0.0036}}
| rowspan='3' | [[Ophiuchus|Oph]]
| {{RA|17|15|20.9}}<br>{{DEC|-26|36|09}}
| style="background: {{star-color|K}};" | [[K-type main-sequence star|K1.5 V]]
| 0.85
| style="background: lightblue;" | 5.07{{Hash-tag|alt=visible to naked eye}}
| 6.20
| rowspan='3' | 167.9617<br>{{±|0.0311}}<ref name="GaiaEDR3"/>
| rowspan='3' |
|-
 | style="background-color: lightgreen" | B{{Dollar sign}}
| {{RA|17|15|21.0}}<br>{{DEC|-26|36|10}}
| style="background: {{star-color|K}};" | [[K-type main-sequence star|K1 V]]
| 0.85
| style="background: lightblue;" | 5.08{{Hash-tag|alt=visible to naked eye}}
| 6.21
|-
 | style="background-color: lightgreen" | C{{Dollar sign}}
| {{RA|17|16|13.4}}<br>{{DEC|-26|32|46}}
| style="background: {{star-color|K}};" | [[K-type main-sequence star|K5 V]]
| 0.71
| style="background: lightblue;" | 6.32{{Hash-tag|alt=visible to naked eye}}
| 7.45
|-
| colspan = '2' | [[YZ Canis Minoris]] (Ross&nbsp;882, Gliese&nbsp;285)
| 19.5330<br>{{±|0.0040}}
| [[Canis Minor|CMi]]
| {{RA|07|44|40.2}}<br>{{DEC|+03|33|09}}
| style="background: {{star-color|M}};" | [[red dwarf|M4 V]]
| 0.308
| 11.19
| 12.30
| 166.9769<br>{{±|0.0343}}<ref name="GaiaEDR3"/>
|  
|-
| rowspan='2' | [[GJ 1005]] ({{nowrap|Luyten 722-22}}, {{nowrap|G 158-50}}) 
 | A
| rowspan="2" | 19.577<br>{{±|0.035}}
| rowspan="2" | [[Cetus|Cet]]
| rowspan="2" | {{RA|00|15|28.1}}<br>{{DEC|-16|08|02}}
| style="background: {{star-color|M}};" | [[red dwarf|M3.5 V]]
| 0.179
| 11.60
| 12.71
| rowspan="2" | 166.6<br>{{±|0.3}}<ref name=Benedict>{{cite journal|bibcode=2016AJ....152..141B|doi=10.3847/0004-6256/152/5/141|arxiv=1608.04775|title=The Solar Neighborhood. XXXVII. The Mass–Luminosity Relation for Main-Sequence M Dwarfs|journal=The Astronomical Journal|volume=152|issue=5|pages=141|year=2016|last1=Benedict|first1=G. F.|last2=Henry|first2=T. J.|last3=Franz|first3=O. G.|last4=McArthur|first4=B. E.|last5=Wasserman|first5=L. H.|last6=Jao|first6=Wei-Chun|last7=Cargile|first7=P. A.|last8=Dieterich|first8=S. B.|last9=Bradley|first9=A. J.|last10=Nelan|first10=E. P.|last11=Whipple|first11=A. L.|s2cid=54029447 |doi-access=free }}</ref>
| rowspan="2" | distance uncertain: 16.28±0.75, 17.91±0.67, 17.0±1.5, 16.26±0.76, 17.26, 19.695±0.095 ly{{Citation needed|date=March 2025}}
|-
 | B
| style="background: {{star-color|M}};" | [[red dwarf|M V]]
| 0.112
| 14.02
| 15.13
|-
| rowspan='2' | [[HR 7703]] (279&nbsp;G.&nbsp;Sagittarii, HD&nbsp;191408, Gliese&nbsp;783, {{nowrap|IRAS 20079-3614}})
 | style="background-color: lightgreen" | A{{Dollar sign}}
| rowspan='2' | 19.609<br>{{±|0.013}}
| rowspan='2' | [[Sagittarius (constellation)|Sgr]]
| rowspan='2' | {{RA|20|11|11.93}}<br>{{DEC|–36|06|04}}
| style="background: {{star-color|K}};" | [[K-type main-sequence star|K2.5 V]]
| 0.65
| style="background: lightblue;" | 5.31{{Hash-tag|alt=visible to naked eye}}
| 6.41
| rowspan='2' | 166.3272<br>{{±|0.1065}}<ref name="GaiaEDR3"/>
| rowspan='2' |
|-
 | B
| style="background: {{star-color|M}};" | [[red dwarf|M4 V]]
| 0.24
| 11.50
| 12.60
|-
| colspan = '2' style="background-color: lightgreen" | [[82 G. Eridani]] (e&nbsp;Eridani, Gliese&nbsp;139, HD&nbsp;20794){{Dollar sign}}
| 19.7045<br>{{±|0.0093}}
| [[Eridanus (constellation)|Eri]]
| {{RA|03|19|55.7}}<br>{{DEC|−43|04|11}}
| style="background: {{star-color|G}};" | [[G-type main-sequence star|G8 V]]
| 0.70
| style="background: lightblue;" | 4.26{{Hash-tag|alt=visible to naked eye}}
| 5.35
| 165.5242<br>{{±|0.0784}}<ref name="GaiaEDR3"/>
|has three confirmed planets, three candidate planets, hot and cold dust disks
|-
| rowspan='2' | [[Gliese 268]] (Ross&nbsp;986, QY&nbsp;Aurigae)
 | A
| rowspan='2' | 19.7414<br>{{±|0.0076}}
| rowspan='2' style="background-color: pink" | [[Auriga (constellation)|Aur]]{{Asterisk}}
| rowspan='2' | {{RA|07|10|01.8}}<br>{{DEC|+38|31|46}}
| style="background: {{star-color|M}};" | [[red dwarf|M4.5 V]]
| 0.226
| 12.05
| 13.14
| rowspan='2' | 165.2147<br>{{±|0.0636}}<ref name="GaiaEDR3"/>
| rowspan='2' |  
|-
 | B
| style="background: {{star-color|M}};" | [[red dwarf|M V]]
| 0.192
| 12.45
| 13.54
|-
| colspan = '2' style="background-color: lightgreen" | [[Delta Pavonis]]{{Dollar sign}}
| 19.893<br>{{±|0.015}}
| [[Pavo (constellation)|Pav]]
| {{RA|20|08|43.6}}<br>{{DEC|−66|10|55}}
| style="background: {{star-color|G}};" | [[G-type main-sequence star|G8 IV]]
| 1.051
| style="background: lightblue;" | 3.55{{Hash-tag|alt=visible to naked eye}}
| 4.62
| 163.9544<br>{{±|0.1222}}<ref name="GaiaEDR3"/>
| has one candidate planet
|-
| colspan = '2' style="background: #D8BD98" | [[SIMP J013656.5+093347]]§
| 19.955<br>{{±|0.057}}
| [[Pisces (constellation)|Psc]]
| {{RA|01|36|56.5}}<br>{{DEC|+09|33|47}}
| style="background: {{star-color|T}};" | [[Brown dwarf#Spectral class T|T2.5]]
| 0.012
| 13.25 J
| 14.32 J
| 163.4478<br>{{±|0.4629}}<ref name="GaiaEDR3"/>
| rogue planet, 12.7 MJ 
|-
| colspan = '2' style="background: #D8BD98" | [[2MASS J09373487+2931409|2MASS 0937+2931]]§
| 19.96<br>{{±|0.22}}
| [[Leo (constellation)|Leo]]
| {{RA|09|37|34.9}}<br>{{DEC|+29|31|41}}
| style="background: {{star-color|T}};" | [[Brown dwarf#Spectral class T|T7]]
| 0.040
| 14.65 J
| 15.71 J
| 163.39<br>{{±|1.76}}<ref name="Schilbach2009">{{cite journal  |last=Schilbach |first=E.  |author2=Röser, S. |author3=Scholz, R.-D.  |title=Trigonometric parallaxes of ten ultracool subdwarfs  |year=2009  |journal=[[Astronomy and Astrophysics]]  |volume=493 | issue=2 | pages=L27–L30  |arxiv=0811.4136  |doi=10.1051/0004-6361:200811281  |bibcode=2009A&A...493L..27S|s2cid=17774863 }}</ref>
| 
|- class="unsortable"
![[Stellar system|System]]
!<small>Star or (sub-) brown dwarf</small>
! rowspan="2" |<small>[[Distance]]<br>([[light-year|ly]] [[margin of error|(±err)]])<ref name=distfn/></small>
! rowspan="2" |<div style="position:absolute;transform: translate(-30%,-50%) rotate(270deg);;">[[Constellation]]</div>
! rowspan="2" |<small>Coordinates:<br>[[Right ascension|RA]],&nbsp;[[Declination|Dec]]<br>([[Epoch (astronomy)#Julian years and J2000|Ep&nbsp;J2000]], [[Equinox|Eq]]&nbsp;J2000)<ref name=RECONS/></small>
! rowspan="2" |<small>[[Stellar classification|Stellar<br>class]]</small>
! rowspan="2" |Mass<br>[[Solar mass|<var>M</var><sub>☉</sub>]]
! data-sort-type="number" |<small>[[Apparent magnitude|App.]]</small>
! data-sort-type="number" |<small>[[Absolute magnitude|Abs.]]</small>
! rowspan="2" |<small>[[Stellar parallax|Parallax]]<br>([[milliarcsecond|mas]]<br>[[margin of error|(±err)]])</small><br><ref name="RECONS"/><ref name=plxfn group=note>Parallaxes given by RECONS are a weighted mean of values in the sources given, as well as measurements by the RECONS program.</ref>
! rowspan="2" |Notes and [[#References|additional<br>references]]
|-class="unsortable"
! colspan="2" |<small>Designation</small>
! colspan="2" |<small>Magnitude ({{nowrap|m<sub>[[UBV photometric system|V]]</sub><ref name=RECONS/> or m<sub>[[J band (infrared)|J]]</sub>}})</small>
|}

==Distant future and past encounters==
[[File:NearSunStarsSimple.jpg|right|thumb|350px|alt=Graph of the distances of various stars from the Sun during the past 20,000 to future 80,000 years.|Distances of the nearest stars from 20,000 years ago until 80,000 years in the future]]
[[File:Sun_in_orbit_around_Galactic_Centre.gif|thumb|350px|Visualisation of the [[orbit of the Sun]] (yellow dot and white curve) around the [[Galactic Centre]] (GC) in the last [[galactic year]]. The red dots correspond to the positions of the stars studied by the [[European Southern Observatory]] in a monitoring programme.<ref>{{cite web|title=Milky Way Past Was More Turbulent Than Previously Known | url= http://www.eso.org/public/news/eso0411/ |work=ESO News|publisher = [[European Southern Observatory]] |date = 2004-04-06 |quote= After more than 1,000 nights of observations spread over 15 years, they have determined the spatial motions of more than 14,000 solar-like stars residing in the neighbourhood of the Sun.}}</ref>]]

Over long periods of time, the slow independent motion of stars change in both relative position and in their distance from the observer. This can cause other currently distant stars to fall within a stated range, which may be readily calculated and predicted using accurate [[astrometric]] measurements of [[parallax]] and total [[proper motion]]s, along with [[spectroscopic]]ally determined [[radial velocities]]. Although extrapolations can be made into the past or future, they are subject to increasingly significant cumulative errors over very long periods.<ref name="Matthews1994"/> Inaccuracies of these measured parameters make determining the true minimum distances of any encountering stars or brown dwarfs fairly difficult.<ref>See also: [[Stellar kinematics]].</ref>

One of the first stars known to approach the Sun particularly close is [[Gliese 710]]. The star, whose mass is roughly half that of the Sun, is currently 62 light-years from the Solar System. It was first noticed in 1999 using data from the [[Hipparcos]] satellite, and was estimated to pass less than {{Convert|1.3|ly|pc}} from the Sun in 1.4 million years.<ref>{{cite journal |last1=García-Sánchez |first1=Joan |last2=Preston |first2=Robert A. |last3=Jones |first3=Dayton L. |last4=Weissman |first4=Paul R. |last5=Lestrade |first5=Jean-François |last6=Latham |first6=David W. |last7=Stefanik |first7=Robert P. |title=Stellar Encounters with the Oort Cloud Based on ''Hipparcos'' Data |journal=The Astronomical Journal |date=February 1999 |volume=117 |issue=2 |pages=1042–1055 |doi=10.1086/300723 |bibcode=1999AJ....117.1042G |s2cid=122929693 |doi-access=free }}</ref> With the release of [[Gaia (spacecraft)|''Gaia'']]'s observations of the star, it has since been refined to a much closer {{convert|0.178|ly|pc}}, close enough to significantly disturb objects in the [[Oort cloud]], which extends {{convert|1.2|ly|pc}} from the Sun.<ref>{{cite journal |last1=Bailer-Jones |first1=C. A. L. |last2=Rybizki |first2=J. |last3=Andrae |first3=R. |last4=Fouesneau |first4=M. |title=New stellar encounters discovered in the second data release |journal=Astronomy & Astrophysics |date=13 August 2018 |volume=616 |pages=A37 |doi=10.1051/0004-6361/201833456 |arxiv=1805.07581 |bibcode=2018A&A...616A..37B |s2cid=56269929 }}</ref>

''Gaia''{{'s}} third data release has provided updated values for many of the candidates in the table below.<ref name="BailerJones2022">{{cite journal | last1=Bailer-Jones | first1=C. A. L. | date=13 July 2022 | title=Stars that approach within one parsec of the Sun: New and more accurate encounters identified in Gaia Data Release 3  | journal=The Astrophysical Journal Letters | volume= 935| issue= 1| page= 152| arxiv=2207.06258  | bibcode=2022ApJ...935L...9B | doi=10.3847/2515-5172/ac842b | s2cid=251154282 | url= | doi-access=free }}</ref><ref name="Bobylev2022">{{cite journal | last1=Bobylev | first1=Vadim | last2=Bajkova  | first2=Anisa  | date=14 July 2022 | title=Search for Close Stellar Encounters with the Solar System Based on Data from the Gaia DR3 Catalogue  | journal=Astronomy Letters | volume=48 | issue=9 | pages=542–549 | doi=10.1134/S1063773722080011 | arxiv=2206.14443| bibcode=2022AstL...48..542B | s2cid=256832377 }}</ref><ref name="Gliese710GaiaDR3">{{cite journal |last1=de la Fuente Marcos |first1=Raúl
|last2=de la Fuente Marcos |first2=Carlos |date=28 June 2022 |title=An Update on the Future Flyby of Gliese 710 to the Solar System Using Gaia DR3: Flyby Parameters Reproduced, Uncertainties Reduced |journal=[[Research Notes of the AAS]] |volume= 6 |issue= 6 |pages= 136 |arxiv=
|bibcode=2022RNAAS...6..136D |doi= 10.3847/2515-5172/ac7b95|doi-access=free }}</ref><ref name="ClosestPast">{{cite journal | last1=de la Fuente Marcos | first1=Carlos | last2=de la Fuente Marcos | first2=Raúl | date=28 July 2022 | title=The Closest Past Flyby of a Known Star to the Solar System: HD 7977, UCAC4 237-008148 or WISE J072003.20-084651.2? | journal=[[Research Notes of the AAS]] | volume=6 | issue=7 | pages=152 | arxiv= | bibcode=2022RNAAS...6..152D | doi=10.3847/2515-5172/ac842b | s2cid=251154282 | doi-access=free }}</ref>

<!--Comment: These examples are all from one source Matthews (1994). This section does require more source references-->
{| class="wikitable sortable sticky-header-multi" style="text-align:center"
|+Stars that are known to have passed or will pass within 5 light-years of the Sun in the past or future<ref name="Bobylev:arXiv1003.2160">Table 3, {{cite journal |last=Bobylev |first=Vadim V. | date=March 2010 |title=Searching for Stars Closely Encountering with the Solar System |journal=Astronomy Letters |volume=36 |issue=3 |pages=220–226 |doi=10.1134/S1063773710030060 |arxiv=1003.2160 |bibcode=2010AstL...36..220B|s2cid=118374161 }}</ref><ref>{{cite journal|title=New stellar encounters discovered in the second Gaia data release|journal=Astronomy & Astrophysics|volume=616|issue=37|pages=A37|last1=Bailer-Jones|first1=C. A. L.|last2=Rybizki|first2=J.|last3=Andrae|first3=R.|last4=Fouesneau|first4=M.|date=19 May 2018|arxiv=1805.07581|doi=10.1051/0004-6361/201833456|bibcode=2018A&A...616A..37B|s2cid=56269929 }}</ref><ref>{{cite journal |last1=Bobylev |first1=Vadim |last2=Bajkova |first2=Anisa |title=Search for Close Stellar Encounters with the Solar System Based on Data from the Gaia DR3 Catalogue |journal=Astronomy Letters |date=29 June 2022 |volume=48 |issue=9 |pages=542–549 |doi=10.1134/S1063773722080011 |arxiv=2206.14443 |bibcode=2022AstL...48..542B |s2cid=256832377 }}</ref>
! Star name
! Minimum distance<br>([[light-year]]s)
! Date of approach<br>in thousands of years<!--this is the date of approach. NOT how many years away. Barnard's star will approach us in 9,700 years, not 11,700.-->
! Current distance<br>(light-years)
! [[Stellar classification]]
! Mass in [[solar mass|M<sub>☉</sub>]]
! Current<br>[[apparent magnitude]]
! Current [[Constellation]]
! Current<br>[[Right ascension|Right&nbsp;ascension]]
! Current<br>[[Declination]]
|-
| [[Gliese 710]]
| {{val|0.167|0.012}}
| {{val|1296|24|23}}
| {{val|62.248|0.020}}
| K7V
| 0.4–0.6
| {{sort|09.6|9.6}}
| [[Serpens]]
| {{RA|18|19|50.843}}
| {{DEC|−01|56|18.98}}
|-<!--OMITTED FOR HUGE RV
| WD 0810-353
| {{val|0.3702|0.0085|0.0082}}
| {{val|31.24|0.66|0.63}}
| {{val|36.4394|0.0063}}
| WD
| 0.65
| {{sort|14.5|14.5}}
| [[Puppis]]
| {{RA|08|12|27.066}}
| {{DEC|-35|29|43.32}}-->
|-
| [[HD 7977]]
| {{val|0.478|0.104|0.078}}
| {{val|-2764|28|29}}
| {{val|246.74|0.60}}
| G0V
| ~1.2
| {{sort|09.04|9.04}}
| [[Cassiopeia (constellation)|Cassiopeia]]
| {{RA|01|20|31.597}}
| {{DEC|+61|52|57.08}}
|-<!--STARS MEASURED BY BAILER-JONES+ (2018) MAY BE FALSE POSITIVES. FALSE POSITIVE STARS ARE OMITTED-->
| [[Scholz's Star]] and companion brown dwarf 
| {{val|0.82|0.37|0.22}}
| {{val|-78.5|0.7}}
| {{val|22.2|0.2}}
| A: M9V<br/>B: T5
| A: 0.095<br>B: 0.063
| {{sort|18.3|18.3}}
| [[Monoceros]]
| {{RA|07|20|03.20}}
| {{DEC|-08|46|51.2}} <!--2MASS J0610-4246 (AKA Gaia DR2 5571232118090082816) is not included despite appearing in several papers, because it has a low-mass companion with a much higher proper motion that averages to a much more distant approach-->
|-
| 2MASS J0628+1845
| {{val|1.61|0.28|0.24}}
| {{val|1720|150|130}}
| {{val|272.28|0.80}}
| M2.5V
| 0.28
| {{sort|16.2|16.2}}
| [[Gemini (constellation)|Gemini]]
| {{RA|06|28|11.593}}
| {{DEC|+18|45|12.91}}
|-
| 2MASS J0805+4624
| {{val|1.610|0.099|0.092}}
| {{val|-363|13|14}}
| {{val|238.1|1.0}}
| M3V
| 0.25
| {{sort|17.0|17.0}}
| [[Lynx (constellation)|Lynx]]
| {{RA|08|05|29.038}}
| {{DEC|+46|24|51.78}}
|-
| CD-69 2001
| {{val|1.616|0.070|0.068}}
| {{val|-1907|10}}
| {{val|332.61|0.55}}
| K4V
| 0.61
| {{sort|11.13|11.13}}
| [[Indus (constellation)|Indus]]
| {{RA|21|40|31.514}}
| {{DEC|-69|25|14.58}}
|-
| HD 49995
| {{val|1.70|0.23|0.20}}
| {{val|-4034|94|98}}
| {{val|439.74|0.59}}
| A: F3V<br/>B: M1V
| A: 1.48<br/>B: 0.49
| 8.78
| [[Canis Major]]
| {{RA|06|50|20.810}}
| {{DEC|-18|37|30.58}}
|-
| 2MASS J0621-0101
| {{val|1.71|0.46|0.39}}
| {{val|-3206|68|66}}
| {{val|428.8|3.1}}
| G5V
| 0.96
| 11.9
| [[Orion (constellation)|Orion]]
| {{RA|06|21|34.807}}
| {{DEC|-01|01|55.01}}
|-<!-- the object at 17 40 14.405 -23 37 53.28 is in a highly contaminated part of the galactic center and isn't included, with an approach of 1.75 +0.26 -0.23 LY-->
| LSPM J2146+3813
| {{val|1.8557|0.0048}}
| {{val|84.59|0.19}}
| {{val|22.9858|0.0034}}
| M5V
| ~0.15
| {{sort|10.82|10.82}}
| [[Cygnus (constellation)|Cygnus]]
| {{RA|21|46|22.285}}
| {{DEC|+38|13|03.12}}
|-
| 2MASS J0455+1144
| {{val|1.94|0.16|0.15}}
| {{val|1702|58|54}}
| {{val|349.50|0.80}}
| M0V
| 0.50
| {{sort|15.3|15.3}}
| [[Orion (constellation)|Orion]]
| {{RA|04|55|21.427}}
| {{DEC|+11|44|41.25}}
|-
| 2MASS J0734-0637
| {{val|1.950|0.021}}
| {{val|-554.6|3.3}}
| {{val|130.66|0.12}}
| M0V
| 0.50
| {{sort|12.9|12.9}}
| [[Monoceros]]
| {{RA|07|34|39.097}}
| {{DEC|-06|37|12.21}}
|-
| 2MASS J1151-0313
| {{val|1.98|0.20|0.18}}
| {{val|1017|60|54}}
| {{val|125.88|0.41}}
| M3.5V
| 0.23
| {{sort|15.3|15.3}}
| [[Virgo (constellation)|Virgo]]
| {{RA|11|51|37.434}}
| {{DEC|-03|13|45.24}}
|-
| UCAC4 076–006432
| {{val|2.042|0.034|0.033}}
| {{val|-893.8|7.9|8.0}}
| {{val|212.41|0.15}}
| mid K
| ~0.6
| {{sort|12.69|12.69}}
| [[Mensa (constellation)|Mensa]]
| {{RA|06|34|29.385}}
| {{DEC|-74|49|47.12}}
|-<!--UCAC4 574-064555 is not included despite giving a close approach of 2.15 +0.84 -0.74 due to having a highly uncertain solution in Gaia eDR3 which might change-->
| 2MASS J0120+4739
| {{val|2.25|0.17|0.15}}
| {{val|473|27|25}}
| {{val|237.56|0.66}}
| M3.5V
| 0.25
| {{sort|16.5|16.5}}
| [[Andromeda (constellation)|Andromeda]]
| {{RA|01|20|04.561}}
| {{DEC|+47|39|46.56}}
|-
| TYC 6760–1510–1
| {{val|2.46|0.19|0.18}}
| {{val|-1708|44|47}}
| {{val|102.89|0.16}}
| M1.5V
| 0.58
| {{sort|11.5|11.5}}
| [[Hydra (constellation)|Hydra]]
| {{RA|15|00|09.536}}
| {{DEC|-29|05|27.67}}
|-
| UCAC2 15719371
| {{val|2.46|0.10}}
| {{val|-4282|70|73}}
| {{val|280.80|0.26}}
| K4V
| 0.66
| {{sort|12.58|12.58}}
| [[Antlia]]
| {{RA|09|44|09.884}}
| {{DEC|-37|45|31.09}}
|-<!-- EGGR 290 at 2.514 +0.065 -0.062 is omitted for unreasonable RV-->
| TYC 1662–1962–1
| {{val|2.637|0.055|0.054}}
| {{val|-1536.6|9.0|9.1}}
| {{val|286.51|0.40}}
| Early K
| ~0.8
| {{sort|10.95|10.95}}
| [[Vulpecula]]
| {{RA|21|14|32.911}}
| {{DEC|+21|53|32.76}}
|-
| HD 179939
| {{val|2.65|0.17}}
| {{val|3020|25}}
| {{val|334.32|0.88}}
| A3V
| 1.7
| {{sort|07.23|7.23}}
| [[Aquila (constellation)|Aquila]]
| {{RA|19|14|10.043}}
| {{DEC|+07|45|50.72}}
|-
| BD-21 1529
| {{val|2.701|0.059|0.058}}
| {{val|-1660.1|6.3}}
| {{val|368.48|0.56}}
| G5V
| ~0.95
| {{sort|09.67|9.67}}
| [[Canis Major]]
| {{RA|06|37|48.004}}
| {{DEC|-21|22|21.94}}
|-
| 2MASS J1310-1307
| {{val|2.79|0.59|0.47}}
| {{val|-1520|150|190}} 
| {{val|433.0|2.6}}
| M2.5V
| 0.34
| {{sort|16.3|16.3}}
| [[Virgo (constellation)|Virgo]]
| {{RA|13|10|30.804}}
| {{DEC|-13|07|33.55}}
|-
| UPM J1121-5549
| {{val|2.803|0.020}}
| {{val|-282.5|1.6|1.7}}
| {{val|72.498|0.029}}
| M3V
| 0.29
| {{sort|13.5|13.5}}
| [[Centaurus]]
| {{RA|11|21|18.136}}
| {{DEC|-55|49|17.77}}
|-
| UCAC4 464–006057
| {{val|2.812|0.052|0.051}}
| {{val|932|11}}
| {{val|101.570|0.086}}
| Early M
| ~0.4
| {{sort|11.73|11.73}}
| [[Taurus (constellation)|Taurus]]
| {{RA|04|09|02.050}}
| {{DEC|+02|45|38.32}}
|-<!-- 10 15 33.832 -23 40 14.02 (approach 2.815 +0.101 -0.096) was omitted for an impossible RV of over 700 km/s-->
| UCAC4 213–008644
| {{val|2.91|0.13|0.12}}
| {{val|-306|12|13}}
| {{val|80.987|0.048}}
| M5.0
| 0.17
| {{sort|16.4|16.4}}
| [[Puppis]]
| {{RA|06|21|54.714}}
| {{DEC|-47|25|31.33}}
|-
| GJ 3649
| {{val|3.016|0.024}}
| {{val|-520.4|3.1}}
| {{val|54.435|0.023}}
| M1
| 0.49
| {{sort|10.85|10.85}}
| [[Leo (constellation)|Leo]]
| {{RA|11|12|38.97}}
| {{DEC|+18|56|05.4}}
|-
| [[Ross 248]]
| {{val|3.0446|0.0077}}
| {{val|38.500|0.096}}
| {{val|10.3057|0.0014}}
| M6V
| 0.136
| {{sort|12.29|12.29}}
| [[Andromeda (constellation)|Andromeda]]
| {{RA|23|41|54.99}}
| {{DEC|+44|10|40.8}}
|-
| 2MASS J1921-1244
| {{val|3.08|0.21|0.19}}
| {{val|-3490|120|130}}
| {{val|376.46|0.73}}
| K6V
| 0.69
| {{sort|12.46|12.46}}
| [[Sagittarius (constellation)|Sagittarius]]
| {{RA|19|21|58.124}}
| {{DEC|-12|43|58.61}}
|-
| [[Proxima Centauri]]
| {{val|3.123|0.015}}
| {{val|28.65|0.27}}
| {{val|4.24646|0.00028}}
| M5Ve
| 0.15
| {{sort|11.05|11.05}}
| [[Centaurus]]
| {{RA|14|29|42.949}}
| {{DEC|−62|40|46.14}}
|-
| TYC 9387–2515–1
| {{val|3.220|0.081|0.079}}
| {{val|-1509.1|8.6|8.7}}
| {{val|401.96|0.54}}
| K1V
| 0.86
| {{sort|11.45|11.45}}
| [[Mensa (constellation)|Mensa]]
| {{RA|06|18|54.643}}
| {{DEC|-80|19|16.54}}
|-
| [[Alpha Centauri]] AB
| {{val|3.242|0.060}}
| {{val|29.63|1.00|0.98}}
| {{val|4.321|0.024}}
| A:&nbsp;G2V<br>B:&nbsp;K1V
| A:&nbsp;1.100<br>B:&nbsp;0.907<ref name=eso0307>{{Cite web|url=https://www.eso.org/public/news/eso0307/|title=A Family Portrait of the Alpha Centauri System - VLT Interferometer Studies the Nearest Stars|publisher=[[European Southern Observatory]]|language=en-GB|date=15 March 2003|access-date=24 January 2011}}</ref>
| A:&nbsp;-0.01<br>B:&nbsp;+1.33
| [[Centaurus]]
| {{RA|14|39|36.495}}
| {{DEC|−60|50|02.31}}
|-
| [[Gliese 445]]
| {{val|3.3400|0.0051}}
| {{val|46.341|0.065}}
| {{val|17.1368|0.0017}}
| M4
| 0.15?
| {{sort|10.8|10.8}}
| [[Camelopardalis]]
| {{RA|11|47|41.377}}
| {{DEC|+78|41|28.18}}
|-
| 2MASS J1638-6355
| {{val|3.37|0.29|0.28}}
| {{val|-1428|21|22}}
| {{val|468.5|4.2}}
| K2V
| 0.82
| {{sort|12.44|12.44}}
| [[Triangulum Australe]]
| {{RA|16|38|21.759}}
| {{DEC|-63|55|13.16}}
|-
| 2MASS J0542+3217
| {{val|3.43|0.75|0.71}}
| {{val|5823|89|87}}
| {{val|884.6|2.4}}
| A: G4V<br/>B: K0V
| A: 1.01<br/>B: 0.85
| {{sort|12.80|12.80}}
| [[Auriga (constellation)|Auriga]]
| {{RA|05|42|38.349}}
| {{DEC|+32|17|29.85}}
|-
| 2MASS J0625-2408
| {{val|3.700|0.082|0.080}}
| {{val|-1874|14}}
| {{val|534.88|0.93}}
| K/M
| ~0.5
| {{sort|12.91|12.91}}
| [[Canis Major]]
| {{RA|06|25|42.744}}
| {{DEC|-24|08|35.02}}
|-
| [[Barnard's Star]]
| {{val|3.7682|0.0031}}
| {{val|11.735|0.013}}
| {{val|5.96290|0.00044}}
| sdM4
| 0.144
| {{sort|09.54|9.54}}
| [[Ophiuchus]]
| {{RA|17|57|48.498}}
| {{DEC|+04|41|36.25}}
|-
| BD+05 1792
| {{val|3.965|0.040}}
| {{val|-962.7|3.0}}
| {{val|239.73|0.33}}
| G2V
| 1.07
| {{sort|08.58|8.58}}
| [[Gemini (constellation)|Gemini]]
| {{RA|07|48|07.037}}
| {{DEC|+05|27|22.51}}
|-
| 2MASS J2241-2759
| {{val|4.05|0.16}}
| {{val|-2810|37|38}}
| {{val|411.06|0.76}}
| K7V
| ~0.5
| {{sort|12.28|12.28}}
| [[Piscis Austrinus]]
| {{RA|22|41|50.996}}
| {{DEC|-27|59|47.04}}
|-
| 2MASS J1724-0522
| {{val|4.15|0.26|0.25}}
| {{val|3058|54|52}}
| {{val|489.5|1.3}}
| K0V
| 0.86
| {{sort|12.73|12.73}}
| [[Ophiuchus]]
| {{RA|17|24|55.056}}
| {{DEC|-05|22|11.45}}
|-
| StKM 1–554
| {{val|4.217|0.036|0.035}}
| {{val|-549.9|2.9|3.0}}
| {{val|151.97|0.19}}
| M0V
| 0.65
| {{sort|12.17|12.17}}
| [[Orion (constellation)|Orion]]
| {{RA|05|14|01.871}}
| {{DEC|+05|22|56.26}}
|-
| [[GJ 3379]]
| {{val|4.227|0.024}}
| {{val|-157.43|0.93|0.94}}
| {{val|16.9861|0.0027}}
| M3.5V
| 0.19
| {{sort|11.31|11.31}}
| [[Orion (constellation)|Orion]]
| {{RA|06|00|03.824}}
| {{DEC|+02|42|22.97}}
|-
| 2MASS J1936+3627
| {{val|4.23|0.62|0.57}}
| {{val|3830|120|110}}
| {{val|671.6|3.4}}
| G5.5V
| 0.95
| 12.2
| [[Cygnus (constellation)|Cygnus]]
| {{RA|19|36|57.294}}
| {{DEC|+36|27|57.71}}
|-
| 2MASS J0710+5228
| {{val|4.303|0.039}}
| {{val|507.6|3.8|3.7}}
| {{val|90.949|0.050}}
| M3V
| 0.33
| {{sort|12.52|12.52}}
| [[Lynx (constellation)|Lynx]]
| {{RA|07|10|52.167}}
| {{DEC|+52|28|18.49}}
|-
| HD 146248
| {{val|4.341|0.040|0.039}}
| {{val|-1141.5|3.7}}
| {{val|334.87|0.47}}
| G2/3IV
| 1.23
| {{sort|09.47|9.47}}
| [[Triangulum Australe]]
| {{RA|16|19|27.875}}
| {{DEC|-64|50|34.38}}
|-
| 2MASS J1724+0355
| {{val|4.37|0.12}}
| {{val|1991|38|37}}
| {{val|254.99|0.26}}
| G8V
| 0.85
| {{sort|12.54|12.54}}
| [[Ophiuchus]]
| {{RA|17|24|34.633}}
| {{DEC|+03|55|26.75}}
|-
| StKM 1–1456
| {{val|4.396|0.043}}
| {{val|1240.2|6.9|6.8}}
| {{val|144.934|0.095}}
| A: K5V<br/>B: M8V
| A: 0.81<br/>B: 0.09
| {{sort|10.58|10.58}}
| [[Hercules (constellation)|Hercules]]
| {{RA|17|17|31.118}}
| {{DEC|+15|34|55.35}}
|-
| [[Zeta Leporis]]
| {{val|4.43|0.33|0.30}}
| {{val|-878|42|46}}
| {{val|72.81|0.40}}
| A2Vann
| 2.0
| {{sort|03.55|3.55}}
| [[Lepus (constellation)|Lepus]]
| {{RA|05|46|57.341}}
| {{DEC|−14|49|19.02}}
|-
| [[Lalande 21185]]
| {{val|4.6807|0.0055}}
| {{val|21.973|0.033}}
| {{val|8.30437|0.00068}}
| M2V
| 0.39
| {{sort|07.52|7.52}}
| [[Ursa Major]]
| {{RA|11|03|20.194}}
| {{DEC|+35|58|11.55}}
|-
| HD 68814
| {{val|4.724|0.090|0.089}}
| {{val|-2242|13}}
| {{val|259.85|0.30}}
| G6V
| 0.98
| {{sort|09.57|9.57}}
| [[Hydra (constellation)|Hydra]]
| {{RA|08|13|57.112}}
| {{DEC|-04|03|12.56}}
|-
| 2MASS J1941-4602
| {{val|4.814|0.050|0.049}}
| {{val|-456.5|4.1|4.2}}
| {{val|66.848|0.033}}
| M4-M6
| ~0.15
| {{sort|12.4|12.4}}
| [[Telescopium (constellation)|Telescopium]]
| {{RA|19|41|53.18}}
| {{DEC|-46|02|31.4}}
|-<!--Gaia DR2 5828371157273738368 is not included because of a potential white dwarf companion with high proper motion uncertainty influencing the total system motion-->
|}

{{wide image|Objects_between_sun_and_alpha_centauri.jpg|2500px|
Schematic view to scale of past and future close approaches of stars to the Sun (Up to 4.5 light-years)}}

==See also==
{{col div|colwidth=30em}}
* [[Interstellar travel]]
* [[Location of Earth]]
* [[The Magnificent Seven (neutron stars)|The Magnificent Seven]]
* [[Nearby Stars Database]]
* [[Solar System#Galactic context]]
* [[Stars in fiction]]
{{colend}}

===Related lists===
{{col div|colwidth=30em}}
* [[List of stars with resolved images]]
* [[List of brightest stars]]
* [[List of star systems within 20–25 light-years]]
* [[List of star systems within 25–30 light-years]]
* [[List of star systems within 30–35 light-years]]
* [[List of star systems within 35–40 light-years]]
* [[List of star systems within 40–45 light-years]]
* [[List of star systems within 45–50 light-years]]
* [[List of star systems within 50–55 light-years]]
* [[List of star systems within 55–60 light-years]]
* [[List of star systems within 60–65 light-years]]
* [[List of star systems within 65–70 light-years]]
* [[List of star systems within 70–75 light-years]]
* [[List of star systems within 75–80 light-years]]
* [[List of star systems within 80–85 light-years]]
* [[List of star systems within 85–90 light-years]]
*[[List of star systems within 90–95 light-years]]
*[[List of star systems within 95–100 light-years]]
*[[List of nearest giant stars]]
*[[List of nearest supergiants]]
* [[List of nearest bright stars]]
** [[Historical brightest stars]]
* [[List of nearest exoplanets]]
* [[List of nearest terrestrial exoplanet candidates]]
* [[List of nearest stars by spectral type]]
* [[List of nearby stellar associations and moving groups]]
* [[List of star-forming regions in the Local Group]]
* [[Lists of stars]]
* [[List of Solar System objects by greatest aphelion]]
* [[List of trans-Neptunian objects]]
* [[List of nearest known black holes]]
{{colend}}

==Notes==
{{reflist |group=note}}

==References==
{{Reflist|30em|refs=

<ref name="Kirkpatrick2021">{{Cite journal|last1=Kirkpatrick|first1=J. Davy|last2=Gelino|first2=Christopher R.|last3=Faherty|first3=Jacqueline K.|author3-link=Jackie Faherty|last4=Meisner|first4=Aaron M.|last5=Caselden|first5=Dan|last6=Schneider|first6=Adam C.|last7=Marocco|first7=Federico|last8=Cayago|first8=Alfred J.|last9=Smart|first9=R. L.|last10=Eisenhardt|first10=Peter R.|last11=Kuchner|first11=Marc J.|last12=Wright|first12=Edward L.|last13=Cushing|first13=Michael C.|last14=Allers|first14=Katelyn N.|last15=Bardalez Gagliuffi|first15=Daniella C.|last16=Burgasser|first16=Adam J.|last17=Gagne|first17=Jonathan|last18=Logsdon|first18=Sarah E.|last19=Martin|first19=Emily C.|last20=Ingalls|first20=James G.|last21=Lowrance|first21=Patrick J.|last22=Abrahams|first22=Ellianna S.|last23=Aganze|first23=Christian|last24=Gerasimov|first24=Roman|last25=Gonzales|first25=Eileen C.|last26=Hsu|first26=Chih-Chun|last27=Kamraj|first27=Nikita|last28=Kiman|first28=Rocio|last29=Rees|first29=Jon|last30=Theissen|first30=Christopher|display-authors=2|title=The Field Substellar Mass Function Based on the Full-sky 20 pc Census of 525 L, T, and Y Dwarfs|journal=The Astrophysical Journal Supplement Series|year=2021|volume=253|issue=1|page=7|doi=10.3847/1538-4365/abd107|arxiv=2011.11616|bibcode=2021ApJS..253....7K|s2cid=227126954 |doi-access=free }}</ref>

}}

==External links==
*[http://www.astro.gsu.edu/RECONS/TOP100.posted.htm "The 100 nearest star systems"], ''[[Research Consortium on Nearby Stars]]'' 
*{{cite web
 |title       = NStars database
 |website        = [[Northern Arizona University]]
 |url         = http://nstars.nau.edu
 |access-date  = 2005-10-24
 |url-status     = dead
 |archive-url  = https://web.archive.org/web/20051030160049/http://nstars.nau.edu/
 |archive-date = October 30, 2005
 |df          = mdy-all
}}
*{{Cite APOD
|title=Map of the 25 nearest star systems
|date=March 18, 2001
|access-date=2005-10-24}}
*{{cite web
|title=Notable Nearby Stars
|website=SolStation
|url=http://www.solstation.com/stars.htm
|access-date=2005-10-24}}
*{{cite web
|title=Cool stars in the solar Neighbourhood
|website=D. Montes, UCM
|url=http://www.ucm.es/info/Astrof/invest/actividad/cool_NS.html
|access-date=2005-11-14}}
*[http://adsabs.harvard.edu/abs/1994QJRAS..35....1M The dynamics of the closest stars]
*{{cite web
|author=Takeda, G.
|author2=E. B. Ford |author3=A. Sills |author4=F. A. Rasio |author5=D. A. Fischer |author6=J. A. Valenti
 |date=2006
|url=http://exoplanets.org/SPOCS_evol.html
|title=Structure and Evolution of Nearby Stars with Planets II. Physical Properties of ~ 1000 Cool Stars from the SPOCS Catalog
|publisher=California & Carnegie Planet Search
|access-date=2006-10-13
}}
*[http://www.bodurov.com/NearestStars/ Nearest Stars 3D View]
*Table 4 "The Census of Stars and Brown Dwarfs within 8 Parsecs of the Sun" in {{Cite journal |arxiv=1205.2122|last1=Bailer-Jones|first1=C. A. L.|display-authors=etal|title=Further Defining Spectral Type "Y" and Exploring the Low-mass End of the Field Brown Dwarf Mass Function|journal=The Astrophysical Journal|volume=753|issue=2|pages=156|year=2012|doi=10.1088/0004-637X/753/2/156|bibcode=2012ApJ...753..156K|s2cid=119279752}}

{{star}}
{{Nearest star systems}}
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[[Category:Lists of stars|nearest stars and brown dwarfs]]
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[[Category:Lists by distance|nearest stars and brown dwarfs]]