View source for User:Jelle Gouw/sandbox

{{User sandbox}}
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==Discord Roles==
{| class="wikitable" style="text-align: center; width: 200px;"
 |-
 ! Level || Colour
 |-
 | style="width: 10%;" | <code>5</code> || style="background: #FFB3BC" | Thales
 |-
 | style="width: 10%;" | <code>10</code> || style="background: #ff4040" | Ptolemy
 |-
 | style="width: 10%;" | <code>15</code> || style="background: #FFB384" | Copernicus
 |-
 | style="width: 10%;" | <code>20</code> || style="background: #F4973A" | Da Vinci
 |-
 | style="width: 10%;" | <code>25</code> || style="background: #fff2a1" | Galileo
 |-
 | style="width: 10%;" | <code>30</code> || style="background: #ffe46f" | Kepler
 |-
 | style="width: 10%;" | <code>35</code> || style="background: #80ff80" | Newton
 |-
 | style="width: 10%;" | <code>40</code> || style="background: #4edd4e" | Herschel
 |-
 | style="width: 10%;" | <code>45</code> || style="background: #48bb48" | Darwin
 |-
 | style="width: 10%;" | <code>50</code> || style="background: #80b0ff" | Einstein
 |-
 | style="width: 10%;" | <code>55</code> || style="background: #6080ff" | Curie
 |-
 | style="width: 10%;" | <code>60</code> || style="background: #4040ff" | Planck
 |-
 | style="width: 10%;" | <code>65</code> || style="background: #f3caff" | Hubble
 |-
 | style="width: 10%;" | <code>70</code> || style="background: #ebaaff" | Dyson
 |-
 | style="width: 10%;" | <code>75</code> || style="background: #d88fff" | Hawking
 |-
|}

{| class="wikitable" style="text-align: center; width: 200px;"
 |-
 ! Level || Colour
 |-
 | style="width: 10%;" | <code>5</code> || style="background: #ffffff" | Thales
 |-
 | style="width: 10%;" | <code>10</code> || style="background: #fffdd0" | Ptolemy
 |-
 | style="width: 10%;" | <code>15</code> || style="background: #fff2a1" | Copernicus
 |-
 | style="width: 10%;" | <code>20</code> || style="background: #ffe46f" | Da Vinci
 |-
 | style="width: 10%;" | <code>25</code> || style="background: #ffbd6f" | Galileo
 |-
 | style="width: 10%;" | <code>30</code> || style="background: #ffa040" | Kepler
 |-
 | style="width: 10%;" | <code>35</code> || style="background: #ff8050" | Newton
 |-
 | style="width: 10%;" | <code>40</code> || style="background: #ff6060" | Herschel
 |-
 | style="width: 10%;" | <code>45</code> || style="background: #ff4080" | Darwin
 |-
 | style="width: 10%;" | <code>50</code> || style="background: #cad7ff" | Einstein
 |-
 | style="width: 10%;" | <code>55</code> || style="background: #aabfff" | Planck
 |-
 | style="width: 10%;" | <code>60</code> || style="background: #8a9fff" | Hubble
 |-
 | style="width: 10%;" | <code>65</code> || style="background: #f3caff" | Dyson
 |-
 | style="width: 10%;" | <code>70</code> || style="background: #ebaaff" | Hawking
 |-
 | style="width: 10%;" | <code>75</code> || style="background: #d88fff" | Elon
 |-
 | || 
 |-
 | style="width: 10%;" | <code>N/A</code> || style="background: #dc143c" | N/A
 |-
 | style="width: 10%;" | <code>N/A</code> || style="background: #9366b4" | N/A
 |-
 | style="width: 10%;" | <code>N/A</code> || style="background: #C6005B" | N/A
 |-
 | style="width: 10%;" | <code>N/A</code> || style="background: #CCFFCC" | N/A
 |-
 | style="width: 10%;" | <code>N/A</code> || style="background: #b8f4bb" | N/A
 |-
 | style="width: 10%;" | <code>N/A</code> || style="background: #88df8d" | N/A
 |-
 | style="width: 10%;" | <code>N/A</code> || style="background: #68bf6d" | N/A
 |-
 | style="width: 10%;" | <code>MOD</code> || style="background: #00aa00" | Moderator
 |-
|}

== De Lijst==
deze lijst bied een overzicht van [[ster|sterren]] (inclusief [[bruine dwerg]]en) geordend op afstand van de zon.

{| style="font-size: 100%; text-align: center;" class="sortable wikitable" border = "1" 
! rowspan="2" |#
! rowspan="2" data-sort-type="number" |<small>[[Distance]]<ref name=distfn>From parallax.</ref><br>[[Light-year]]s [[margin of error|(±err)]]</small>
! class="unsortable" colspan="3" |<small>Designation</small>
! rowspan="2" |<small>[[Stellar classification|Stellar class]]</small>
! rowspan="2" data-sort-type="number"  |<small>[[Apparent magnitude]] ({{nowrap|m<sub>[[UBV photometric system|V]]</sub> or m<sub>[[J band|J]]</sub>}})</small>
! rowspan="2" data-sort-type="number"  |<small>[[Absolute magnitude]] ({{nowrap|M<sub>[[UBV photometric system|V]]</sub> or M<sub>[[J band|J]]</sub>}})</small>
! class="unsortable" style="background: #FFC" colspan="2" |<small>[[Epoch (astronomy)|Epoch]] [[J2000.0]]</small>
! rowspan="2" |<small>[[Stellar parallax|Parallax]]<ref name="RECONS"/><ref name=plxfn>Parallaxes given by RECONS are a weighted mean of values in the sources given, as well as measurements by the RECONS program.</ref><br>[[milliarcsecond|mas]][[margin of error|(±err)]]</small>
! rowspan="2" |<small>Discovery date<ref name=discfn>Before 1900: earliest certain recorded observation. 1900–1930: first catalogued. After 1930: earliest trigonometric or spectroscopic parallax.</ref></small>
! rowspan="2" |<small>[[#References|Additional<br>references]]</small>
|-class="unsortable"
!<small>[[Stellar system|System]]</small>
!<small>[[Star]]</small>
!<small>Star #</small>
!<small>[[Right ascension]]<ref name=RECONS/></small>
!<small>[[Declination]]<ref name=RECONS/></small>
|-
|
| 0
| [[Solar System]]
| [[Sun]]
|
| style="background: {{star-color|G}};" | [[G-type main-sequence star|G2V]]<ref name=RECONS/>
| style="background: lightblue;" | −26.74<ref name=RECONS/>
| 4.85<ref name=RECONS/>
| —
| —
| —
| —
| has eight planets
|-
| rowspan="3" | 1
| 4.2421(16)
| rowspan="3" | [[Alpha Centauri]]<br>(Rigil&nbsp;Kentaurus)
| [[Proxima Centauri|Proxima&nbsp;Centauri]] (V645&nbsp;Centauri)
| 1
| style="background: {{star-color|M}};" | [[red dwarf|M5.5Ve]]
| 11.09<ref name=RECONS />
| 15.53<ref name=RECONS />
| {{RA|14|29|43.0}}
| {{DEC|−62|40|46}}
|align=left | 768.87(029)<ref name="Y">[[General Catalogue of Trigonometric Parallaxes]].</ref><ref name="H">[[Hipparcos Catalogue]].</ref>
| 1915
| <ref name="B">Burgasser et al. 2000</ref>
|-
| rowspan="2" | 4.3650(68)
| α&nbsp;Centauri&nbsp;A (HD&nbsp;128620)
| 2
| style="background: {{star-color|G}};" | [[G-type main-sequence star|G2V]]<ref name=RECONS />
| style="background: lightblue;" | 0.01<ref name=RECONS />
| 4.38<ref name=RECONS />
| {{RA|14|39|36.5}}
| {{DEC|−60|50|02}}
| rowspan="2" align=left | 747.23(117)<ref name="Y"/><ref name="S">[http://adsabs.harvard.edu/abs/1999A%26A...341..121S Visual binary orbits and masses post Hipparcos], Staffan Söderhjelm, ''Astronomy and Astrophysics'' '''341''' (January 1999), pp. 121&ndash;140.</ref>
| 
|
|-
| α&nbsp;Centauri&nbsp;B (HD&nbsp;128621)
| 2
| style="background: {{star-color|K}};" | [[K-type main-sequence star|K1V]]<ref name=RECONS />
| style="background: lightblue;" | 1.34<ref name=RECONS />
| 5.71<ref name=RECONS />
| {{RA|14|39|35.1}}
| {{DEC|−60|50|14}}
| 1689
| has one suspected planet<ref>[http://www.nature.com/news/the-exoplanet-next-door-1.11605 "The exoplanet next door: Earth-sized world discovered in nearby α Centauri star system".] Eric Hand, ''Nature'', October 16, 2012. Accessed October 16, 2012.</ref>
|-
| 2
| 5.9630(109)
| colspan="2" | [[Barnard's Star|Barnard's&nbsp;Star]] (BD+04°3561a)
| 4
| style="background: {{star-color|M}};" | M4.0Ve
| 9.53<ref name=RECONS />
| 13.22<ref name=RECONS />
| {{RA|17|57|48.5}}
| {{DEC|+04|41|36}}
|align=left | 546.98(1&nbsp;00)<ref name="Y"/><ref name="H"/>
| 1916
| largest known [[proper motion]]<ref name="EEB">{{cite journal
 | first=E. E. | last=Barnard
 | authorlink=Edward Emerson Barnard | year=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>
|-
| rowspan="2" | 3
| rowspan="2" | 6.59(7)
| style="background: #C67B30"  rowspan="2" | [[Luhman 16]]<br>(WISE 1049−5319)
| style="background: #C67B30"| Luhman 16A
| 5
| style="background: {{star-color|L}};" | [[Brown dwarf|L8±1]]<ref name="1049primary">{{cite journal
 | first=K. L. | last=Luhman
 | title=Discovery of a Binary Brown Dwarf at 2 Parsecs from the Sun
 | journal=Astrophysical Journal Letters (to be published)
 | url=http://science.psu.edu/alert/photos/research-photos/astro/Luhman_ApJL_32013.pdf
 }}</ref>
| 10.7 J
| 14.2 J
| rowspan="2" | {{RA|10|49|15.57}}
| rowspan="2" | {{DEC|−53|19|06}}
| rowspan="2" align=left | 495 (5)<ref name=1049primary />
| rowspan="2" | 2013
| rowspan="2" | has one suspected planet<ref>http://arxiv.org/abs/1312.1303</ref>
|-
| style="background: #C67B30" | Luhman 16B
| 5
| style="background: {{star-color|T}};" | [[Brown dwarf|T1±2]]<ref name=1049primary/>
| 
| 
|-
| 4
| 7.2(6)<ref name="Luhman20140421">{{cite journal |title=Discovery of a ~250 K Brown Dwarf at 2 pc from the Sun |journal=[[The Astrophysical Journal Letters]] |first=K. L. |last=Luhman |volume=786 |issue=2 |page=L18 |date=21 April 2014 |doi=10.1088/2041-8205/786/2/L18|arxiv = 1404.6501 |bibcode = 2014ApJ...786L..18L }}</ref> 
| style="background: #C67B30" colspan="2" | [[WISE 0855−0714]]
| 7
|style="background: {{star-color|Y}};" | [[Brown dwarf#Spectral class Y|Y]] 
| 
| 
| {{RA|08|55|10.83}}
| {{DEC|-07|14|42.5}}
|
| 2014
| may be a rogue planet
|- 
| 5
| 7.7825(390)
| colspan="2" | [[Wolf 359|Wolf&nbsp;359]] (CN&nbsp;Leonis)
| 8
| style="background: {{star-color|M}};" | M6.0V<ref name=RECONS />
| 13.44<ref name=RECONS />
| 16.55<ref name=RECONS />
| {{RA|10|56|29.2}}
| {{DEC|+07|00|53}}
|align=left | 419.10(210)<ref name="Y" />
| 1919
| 
|-
| 6
| 8.2905(148)
| colspan="2" | [[Lalande 21185|Lalande&nbsp;21185]] (BD+36°2147)
| 9
| style="background: {{star-color|M}};" | M2.0V<ref name=RECONS />
| 7.47<ref name=RECONS />
| 10.44<ref name=RECONS />
| {{RA|11|03|20.2}}
| {{DEC|+35|58|12}}
|align=left | 393.42(070)<ref name="Y"/><ref name="H"/>
| 1801
| 
|-
| rowspan="2" | 7
| rowspan="2" | 8.5828(289)
| rowspan="2" | [[Sirius]]<br>(α&nbsp;Canis&nbsp;Majoris)
| Sirius A
| 10
| style="background: {{star-color|A}}" | [[A-type main-sequence star|A1V]]<ref name=RECONS />
| style="background: lightblue;" | −1.46<ref name=RECONS />
| 1.42<ref name=RECONS />
| rowspan="2" | {{RA|06|45|08.9}}
| rowspan="2" | {{DEC|−16|42|58}}
| rowspan="2" align=left | 380.02(128)<ref name="Y"/><ref name="H"/>
| 
| rowspan="2" | brightest star in the night sky
|-
| Sirius&nbsp;B
| 10
| style="background: F0F0F0" | [[White dwarf|DA2]]<ref name=RECONS />
| 8.44<ref name=RECONS />
| 11.34<ref name=RECONS />
| 1844
|-
| rowspan="2" | 8
| rowspan="2" | 8.7280(631)
| rowspan="2" | [[Luyten 726-8|Luyten&nbsp;726-8]]
| Luyten&nbsp;726-8&nbsp;A (BL&nbsp;Ceti)
| 12
| style="background: {{star-color|M}};" | M5.5Ve
| 12.54<ref name=RECONS />
| 15.40<ref name=RECONS />
| rowspan="2" | {{RA|01|39|01.3}}
| rowspan="2" | {{DEC|−17|57|01}}
| rowspan="2" align=left | 373.70(270)<ref name="Y"/>
| rowspan="2" |1949
| rowspan="2" |
|-
| Luyten&nbsp;726-8&nbsp;B (UV&nbsp;Ceti)
| 12
| style="background: {{star-color|M}};" | M6.0Ve
| 12.99<ref name=RECONS />
| 15.85<ref name=RECONS />
|-
| 9
| 9.6813(512)
| colspan="2" | [[Ross 154|Ross&nbsp;154]] (V1216&nbsp;Sagittarii)
| 14
| style="background: {{star-color|M}};" | M3.5Ve
| 10.43<ref name=RECONS />
| 13.07<ref name=RECONS />
| {{RA|18|49|49.4}}
| {{DEC|−23|50|10}}
|align=left | 336.90(178)<ref name="Y"/><ref name="H"/>
| 1925
| 
|-
| 10
| 10.322(36)
| colspan="2" | [[Ross 248|Ross&nbsp;248]] (HH&nbsp;Andromedae)
| 15
| style="background: {{star-color|M}};" | M5.5Ve
| 12.29<ref name=RECONS />
| 14.79<ref name=RECONS />
| {{RA|23|41|54.7}}
| {{DEC|+44|10|30}}
|align=left | 316.00(110)<ref name="Y"/>
| 1925
| 
|-
| 11
| 10.522(27)
| colspan="2" | [[Epsilon Eridani|Epsilon&nbsp;Eridani]] (BD−09°697)
| 16
| style="background: {{star-color|K}};" | [[K-type main-sequence star|K2V]]<ref name=RECONS />
| style="background: lightblue;" | 3.73<ref name=RECONS />
| 6.19<ref name=RECONS />
| {{RA|03|32|55.8}}
| {{DEC|−09|27|30}}
|align=left | 309.99(079)<ref name="Y"/><ref name="H"/>
| 150
| at least one planet<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 and 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 }}</ref>
|-
| 12
| 10.742(31)
| colspan="2" | [[Lacaille 9352|Lacaille&nbsp;9352]] (CD−36°15693)
| 17
| style="background: {{star-color|M}};" | M1.5Ve
| 7.34<ref name=RECONS />
| 9.75<ref name=RECONS />
| {{RA|23|05|52.0}}
| {{DEC|−35|51|11}}
|align=left | 303.64(087)<ref name="Y"/><ref name="H"/>
| 1753
| 
|-
| 13
| 10.919(49)
| colspan="2" | [[Ross 128|Ross&nbsp;128]] (FI&nbsp;Virginis)
| 18
| style="background: {{star-color|M}};" | M4.0Vn
| 11.13<ref name=RECONS />
| 13.51<ref name=RECONS />
| {{RA|11|47|44.4}}
| {{DEC|+00|48|16}}
|align=left | 298.72(135)<ref name="Y"/><ref name="H"/>
| 1925
| 
|-
| 14
| 11.089<ref name="Marsh2012">{{cite journal
 | last=Marsh |first=Kenneth A.
 | author2=Wright, Edward L.
 | author3=Kirkpatrick, J. Davy
 | author4=Gelino, Christopher R.
 | author5=Cushing, Michael C.
 | author6=Griffith, Roger L.
 | author7=Skrutskie, Michael F.
 | author8=Eisenhardt, Peter R.
 | date=2013
 | title=Parallaxes and Proper Motions of Ultracool Brown Dwarfs of Spectral Types Y and Late T
 | journal=[[The Astrophysical Journal]]
 | volume=762 | issue=2 | pages=119
 | arxiv=1211.6977
 | bibcode=2013ApJ...762..119M
 | doi=10.1088/0004-637X/762/2/119
}}</ref>
| style="background: #C67B30" colspan="2" | [[WISE 1506+7027]]
| 19
| style="background: {{star-color|T}};" | [[Brown dwarf|T6]]
| 14.3 J
| 16.6 J
|| {{RA|15|06|49.9}}
|| {{DEC|+70|27|36}}
|align=left | 310(042)<ref name="Marsh2012"/>
| 2011
| 
|-
| rowspan="3" | 15
| rowspan="3" | 11.266(171)
| rowspan="3" | [[EZ Aquarii|EZ&nbsp;Aquarii]]<br>(Gliese&nbsp;866, Luyten&nbsp;789-6)
| EZ&nbsp;Aquarii&nbsp;A
| 20
| style="background: {{star-color|M}};" | M5.0Ve
| 13.33<ref name=RECONS />
| 15.64<ref name=RECONS />
| rowspan="3" | {{RA|22|38|33.4}}
| rowspan="3" | {{DEC|−15|17|57}}
| rowspan="3" align=left | 289.50(440)<ref name="Y"/>
| 1937
| rowspan="3" |
|-
| EZ&nbsp;Aquarii&nbsp;B
| 20
| style="background: {{star-color|M}};" | M?
| 13.27<ref name=RECONS />
| 15.58<ref name=RECONS />
| -
|-
| EZ&nbsp;Aquarii&nbsp;C
| 20
| style="background: {{star-color|M}};" | M?
| 14.03<ref name=RECONS />
| 16.34<ref name=RECONS />
| 1995
|-
| rowspan="2" | 16
| rowspan="2" | 11.402(32)
| rowspan="2" | [[Procyon]]<br>(α&nbsp;Canis&nbsp;Minoris)
| Procyon&nbsp;A
| 23
| style="background: {{star-color|F}}" | F5V–IV<ref name=RECONS />
| style="background: lightblue;" | 0.38<ref name=RECONS />
| 2.66<ref name=RECONS />
| rowspan="2" | {{RA|07|39|18.1}}
| rowspan="2" | {{DEC|+05|13|30}}
| rowspan="2" align=left | 286.05(081)<ref name="Y"/><ref name="H"/>
| 
| rowspan="2" |
|-
| Procyon&nbsp;B
| 23
| style="background: #F0F0F0" | [[White dwarf|DQZ]]<ref name=RECONS />
| 10.70<ref name=RECONS />
| 12.98<ref name=RECONS />
| 1844
|-
| rowspan="2" | 17
| rowspan="2" | 11.403(22)
| rowspan="2" | [[61 Cygni|61&nbsp;Cygni]]
| 61&nbsp;Cygni&nbsp;A (BD+38°4343)
| 25
| style="background: {{star-color|K}};" | [[K-type main-sequence star|K5.0V]]<ref name=RECONS /> <!--previous: K3.5Ve-->
| style="background: lightblue;" | 5.21<ref name=RECONS />
| 7.49<ref name=RECONS />
| {{RA|21|06|53.9}}
| {{DEC|+38|44|58}}
| rowspan="2" align=left | 286.04(056)<ref name="Y"/><ref name="H"/>
| 1725
| rowspan="2" | first star (other than the 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 | year=1839 | volume=16 | issue=5-6 | pages=65 | language=German | bibcode=1839AN.....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 }} A parallax of 313.6 mas yields a distance of 10.4 light years</ref>
|-
| 61&nbsp;Cygni&nbsp;B (BD+38°4344)
| 25
| style="background: {{star-color|K}};" | [[K-type main-sequence star|K7.0V]]<ref name=RECONS /> <!--previous: K4.7Ve-->
| style="background: lightblue;" | 6.03<ref name=RECONS />
| 8.31<ref name=RECONS />
| {{RA|21|06|55.3}}
| {{DEC|+38|44|31}}
| -
|-
| rowspan="2" | 18
| rowspan="2" | 11.525(69)
| rowspan="2" | [[Struve 2398|Struve&nbsp;2398]]<br>(Gliese&nbsp;725, BD+59°1915)
| Struve&nbsp;2398&nbsp;A (HD&nbsp;173739)
| 27
| style="background: {{star-color|M}};" | M3.0V<ref name=RECONS />
| 8.90<ref name=RECONS />
| 11.16<ref name=RECONS />
| {{RA|18|42|46.7}}
| {{DEC|+59|37|49}}
| rowspan="2" align=left | 283.00(169)<ref name="Y"/><ref name="H"/>
| 1835
| rowspan="2" |
|-
| Struve&nbsp;2398&nbsp;B (HD&nbsp;173740)
| 27
| style="background: {{star-color|M}};" | M3.5V<ref name=RECONS />
| 9.69<ref name=RECONS />
| 11.95<ref name=RECONS />
| {{RA|18|42|46.9}}
| {{DEC|+59|37|37}}
| 1835
|-
| rowspan="2" | 19
| rowspan="2" | 11.624(39)
| rowspan="2" | [[Groombridge 34|Groombridge&nbsp;34]]<br>(Gliese&nbsp;15)
| Groombridge&nbsp;34&nbsp;A (GX&nbsp;Andromedae)
| 29
| style="background: {{star-color|M}};" | M1.5V<ref name=RECONS /> <!--previous: M3.0V-->
| 8.08<ref name=RECONS />
| 10.32<ref name=RECONS />
| rowspan="2" | {{RA|0|18|22.9}}
| rowspan="2" | {{DEC|+44|01|23}}
| rowspan="2" align=left | 280.59(095)<ref name="Y"/><ref name="H"/>
| 1813
| has one planet<ref>[http://arxiv.org/abs/1408.5645 "The NASA-UC-UH Eta-Earth Program: IV. A Low-mass Planet Orbiting an M Dwarf 3.6 PC from Earth".] Andrew W. Howard, Geoffrey W. Marcy, Debra A. Fischer, Howard Isaacson, Philip S. Muirhead, Gregory W. Henry, Tabetha S. Boyajian, Kaspar von Braun, Juliette C. Becker, Jason T. Wright, John Asher Johnson. Accessed August 26, 2014.</ref>
|-
| Groombridge&nbsp;34&nbsp;B (GQ&nbsp;Andromedae)
| 29
| style="background: {{star-color|M}};" | M3.5V<ref name=RECONS />
| 11.06<ref name=RECONS />
| 13.30<ref name=RECONS />
| -
|
|-
| rowspan="3" | 20
| rowspan="3" | 11.824(30)
| rowspan="3" | [[Epsilon Indi|Epsilon&nbsp;Indi]]<br>(CPD−57°10015)
| Epsilon Indi A
| 31
| style="background: {{star-color|K}};" | [[K-type main-sequence star|K5Ve]]<ref name=RECONS />
| style="background: lightblue;" | 4.69<ref name=RECONS />
| 6.89<ref name=RECONS />
| {{RA|22|03|21.7}}
| {{DEC|−56|47|10}}
| rowspan="3" align=left | 275.84(069)<ref name="Y"/><ref name="H"/>
| 1597
| one suspected planet<ref name="Zechmeister et al">{{cite journal | title=The planet search programme at the ESO CES and HARPS. IV. The search for Jupiter analogues around solar-like stars | display-authors=9<!--Reducible--> | last1=Zechmeister | first1=M. | last2=Kürster | first2=M | last3=Endl | first3=M. | last4=Lo Curto | first4=G. | last5=Hartman | first5=H. | last6=Nilsson | first6=H. | last7=Henning | first7=T. | last8=Hatzes | first8=A. | last9=Cochran | first9=W. D. | journal=Astronomy and Astrophysics | date=April 2013 | volume=552 | pages=pp62 | doi=10.1051/0004-6361/201116551 | bibcode=2013A&A...552A..78Z | arxiv = 1211.7263 | url =}}</ref>
|-
| style="background: #C67B30"| Epsilon&nbsp;Indi&nbsp;Ba
| 31
| style="background: {{star-color|T}};" | [[Brown dwarf|T1.0V]]
| 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
  |accessdate=2012-06-10}} [http://spider.ipac.caltech.edu/staff/davy/ARCHIVE/index.shtml (main page)]</ref>
| 
| rowspan="2" | {{RA|22|04|10.5}}
| rowspan="2" | {{DEC|−56|46|58}}
| Jan 2003
|
|-
| style="background: #C67B30"| Epsilon&nbsp;Indi&nbsp;Bb
| 31
| style="background: {{star-color|T}};" | [[Brown dwarf|T6.0V]]
| 13.2 J<ref name="DwarfArchives"/>
| 
| Aug 2003
|
|-
| 21
| 11.826(129)
| colspan="2" | [[DX Cancri|DX&nbsp;Cancri]] (G&nbsp;51-15)
| 34
| style="background: {{star-color|M}};" | M6.5Ve
| 14.78<ref name=RECONS />
| 16.98<ref name=RECONS />
| {{RA|08|29|49.5}}
| {{DEC|+26|46|37}}
|align=left | 275.80(300)<ref name=Y />
| 1972
| 
|-
| 22
| 11.887(33)
| colspan="2" | [[Tau Ceti|Tau&nbsp;Ceti]] (BD−16°295)
| 35
| style="background: {{star-color|G}};" | [[G-type main-sequence star|G8Vp]]<ref name=RECONS />
|style="background: lightblue;" | 3.49<ref name=RECONS />
| 5.68<ref name=RECONS />
| {{RA|01|44|04.1}}
| {{DEC|−15|56|15}}
|align=left | 274.39(076)<ref name="Y"/><ref name="H"/>
| 150
| possibly five planets
|-
| 23
| 11.991(57)
| colspan="2" | [[GJ 1061]] (LHS&nbsp;1565)
| 36
| style="background: {{star-color|M}};" | M5.5V<ref name=RECONS />
| 13.09<ref name=RECONS />
| 15.26<ref name=RECONS />
| {{RA|03|35|59.7}}
| {{DEC|−44|30|45}}
|align=left | 272.01(130)<ref name="recent">Systems with their first accurate trigonometric parallaxes measured by RECONS</ref>
| 1995
| <ref name=henry1997>[http://adsabs.harvard.edu/abs/1997AJ....114..388H The solar neighborhood IV: discovery of the twentieth nearest star], Todd J. Henry, Philip A. Ianna, J. Davy Kirkpatrick, Hartmut Jahreiss, ''The Astronomical Journal'' '''114''', #1 (July 1997), pp. 388&ndash;395. {{doi|10.1086/118482}}</ref><ref name=henry2006>[http://adsabs.harvard.edu/abs/2006AJ....132.2360H The Solar Neighborhood. XVII. Parallax Results from the CTIOPI 0.9 m Program: 20 New Members of the RECONS 10 Parsec Sample], Todd J. Henry, Wei-Chun Jao, John P. Subasavage, Thomas D. Beaulieu, Philip A. Ianna, Edgardo Costa, René A. Méndez, ''The Astronomical Journal'' '''132''', #6 (December 2006), pp. 2360&ndash;2371. {{doi|10.1086/508233}}</ref>
|-
| 24
| 12.068<ref name="Marsh2012"/><!--3.7pc x 3.26156 = 12.067772ly-->
| style="background: #C67B30" colspan="2" | [[WISE 0350−5658]]
| 37
| style="background: {{star-color|Y}};" | [[Brown dwarf#Spectral class Y|Y1]]
| 22.8 J<ref name="Kirkpatrick2012v1">{{cite arXiv |last=Kirkpatrick |first=J. Davy |authors=Gelino; Cushing; Mace; Griffith; Skrutskie; Marsh; Wright; Eisenhardt; McLean; Mainzer; Burgasser; Tinney; Parker; Salter |title=Further Defining Spectral Type "Y" and Exploring the Low-mass End of the Field Brown Dwarf mass Function |year=2012 |eprint=1205.2122 |version=v1 |class=astro-ph.SR}}</ref>
| 
|| {{RA|03|50|00.32}}
|| {{DEC|−56|58|30.2}}
|align=left | 291(050)<ref name="Marsh2012"/>
| 2011
| 
|-
| 25
| 12.132(133)
| colspan="2" | [[YZ Ceti|YZ&nbsp;Ceti]] (LHS&nbsp;138)
| 38
| style="background: {{star-color|M}};" | M4.5V<ref name=RECONS />
| 12.02<ref name=RECONS />
| 14.17<ref name=RECONS />
| {{RA|01|12|30.6}}
| {{DEC|−16|59|56}}
|align=left | 268.84(295)<ref name="Y"/><ref name="H"/>
| 1961
| 
|-
| 26
| 12.366(59)
| colspan="2" | [[Luyten's Star|Luyten's&nbsp;Star]] (BD+05°1668)
| 39
| style="background: {{star-color|M}};" | M3.5Vn
| 9.86<ref name=RECONS />
| 11.97<ref name=RECONS />
| {{RA|07|27|24.5}}
| {{DEC|+05|13|33}}
|align=left | 263.76(125)<ref name="Y"/><ref name="H"/>
| 1935
| 
|-
| 27
| 12.514(129)
| style="background: #C67B30" colspan="2" | [[Teegarden's star|Teegarden's&nbsp;star]] (SO025300.5+165258)
| 40
| style="background: {{star-color|M}};" | M6.5V
| 15.14<ref name=RECONS />
| 17.22<ref name=RECONS />
| {{RA|02|53|00.9}}
| {{DEC|+16|52|53}}
|align=left | 260.63(269)<ref name=recent />
| 2003
| possible planetary system<ref name=henry2006 /><ref name=ROPS>{{cite journal | url=http://mnras.oxfordjournals.org/content/424/1/591 |title=ROPS: A New Search for Habitable Earths in the Southern Sky  |author=Barnes, J. R. et al. |year=2012|journal=[[Monthly Notices of the Royal Astronomical Society]] |volume=424|issue=1 |pages=591–604 |doi=10.1111/j.1365-2966.2012.21236.x |bibcode=2012MNRAS.424..591B|arxiv = 1204.6283 }}</ref>
|-
| rowspan="2" | 28
| rowspan=2 | 12.571(54)
| rowspan="2" | [[SCR 1845-6357|SCR&nbsp;1845-6357]]
| SCR&nbsp;1845-6357&nbsp;A
| 41
| style="background: {{star-color|M}};" | M8.5V<ref name=RECONS />
| 17.39
| 19.41
| {{RA|18|45|05.3}}
| {{DEC|−63|57|48}}
| rowspan=2 align=left | 259.45(111)<ref name="recent"/>
| 2004
| rowspan=2 | <ref name=henry2006 />
|-
| style="background: #C67B30"| SCR&nbsp;1845-6357&nbsp;B
| 41
| style="background: {{star-color|T}};" | [[Brown dwarf|T6]]<ref name=nearmt>[http://adsabs.harvard.edu/abs/2007A%26A...471..655K The very nearby M/T dwarf binary SCR 1845-6357], Markus Kasper, Beth A. Biller, Adam Burrows, Wolfgang Brandner, Jano Budaj, and Laird M. Close, ''Astronomy and Astrophysics'' '''471''', #2 (August 2007), pp. 655&ndash;659. {{doi|10.1051/0004-6361:20077881}}</ref>
| 13.3 J<ref name="DwarfArchives"/>
| 
| {{RA|18|45|02.6}}
| {{DEC|−63|57|52}}
| 2006
|-
| 29
| 12.777(43)
| colspan="2" | [[Kapteyn's Star|Kapteyn's&nbsp;Star]] (CD−45°1841)
| 43
| style="background: {{star-color|M}};" | M1.5V<ref name=RECONS /> <!--previous: sdM0VI-->
| 8.84<ref name=RECONS />
| 10.87<ref name=RECONS />
| {{RA|05|11|40.6}}
| {{DEC|−45|01|06}}
|align=left | 255.27(086)<ref name="Y"/><ref name="H"/>
| 1898
| has two known planets<ref name="Kapteyn-discovery">{{cite arXiv|title=Two planets around Kapteyn's star : a cold and a temperate super-Earth orbiting the nearest halo red-dwarf|author=Guillem Anglada-Escudé, Pamela Arriagada, Mikko Tuomi, Mathias Zechmeister, James S. Jenkins, Aviv Ofir, Stefan Dreizler, Enrico Gerlach, Chris J. Marvin, Ansgar Reiners, Sandra V. Jeffers, R. Paul Butler, Steven S. Vogt, Pedro J. Amado, Cristina Rodríguez-López, Zaira M. Berdiñas, Julian Morin, Jeff D. Crane, Stephen A. Shectman, Ian B. Thompson, Matías Díaz, Eugenio Rivera, Luis F. Sarmiento, Hugh R.A. Jones|year=2014|eprint=1406.0818|class=astro-ph.EP|accessdate=2014-06-29}}</ref>
|-
| 30
| 12.870(57)
| colspan="2" | [[Lacaille 8760|Lacaille&nbsp;8760]] (AX&nbsp;Microscopii)
| 44
| style="background: {{star-color|M}};" | M0.0V<ref name=RECONS /> <!--previous: M2Ve-->
| 6.67<ref name=RECONS />
| 8.69<ref name=RECONS />
| {{RA|21|17|15.3}}
| {{DEC|−38|52|03}}
|align=left | 253.43(112)<ref name="Y"/><ref name="H"/>
| 1753
| 
|-
| rowspan="2" | 31
| rowspan="2" | 13.149(74)
| rowspan="2" | [[Kruger 60|Kruger&nbsp;60]]<br>(BD+56°2783)
| Kruger&nbsp;60&nbsp;A
| 45
| style="background: {{star-color|M}};" | M3.0V<ref name=RECONS />
| 9.79<ref name=RECONS />
| 11.76<ref name=RECONS />
| rowspan="2" | {{RA|22|27|59.5}}
| rowspan="2" | {{DEC|+57|41|45}}
| rowspan="2" align=left | 248.06(139)<ref name="Y"/><ref name="S"/>
| 1880
| rowspan="2" |
|-
| Kruger&nbsp;60&nbsp;B (DO&nbsp;Cephei)
| 45
| style="background: {{star-color|M}};" | M4.0V<ref name=RECONS />
| 11.41<ref name=RECONS />
| 13.38<ref name=RECONS />
| 1890?
|-
| 32
| 13.167(82)
| style="background: #C67B30" colspan="2" | [[DEN 1048-3956|DEN&nbsp;1048-3956]]
| 47
| style="background: {{star-color|M}};" | M8.5V<ref name=RECONS />
| 17.39<ref name=RECONS />
| 19.37<ref name=RECONS />
| {{RA|10|48|14.7}}
| {{DEC|−39|56|06}}
|align=left | 247.71(155)<ref name="recent"/>
| 2001
| <ref>[http://adsabs.harvard.edu/abs/2005AJ....129.1954J The Solar Neighborhood. XIII. Parallax Results from the CTIOPI 0.9 Meter Program: Stars with μ >= 1.0" yr<sup>-1</sup> (Motion sample)], Wei-Chun Jao, Todd J. Henry, John P. Subasavage, Misty A. Brown, Philip A. Ianna, Jennifer L. Bartlett, Edgardo Costa, René A. Méndez, ''The Astronomical Journal'' '''129''', #4 (April 2005), pp. 1954&ndash;1967. {{doi|10.1086/428489}}</ref><ref name=costa2005>[http://adsabs.harvard.edu/abs/2005AJ....130..337C The Solar Neighborhood. XIV. Parallaxes from the Cerro Tololo Inter-American Observatory Parallax Investigation&mdash;First Results from the 1.5 m Telescope Program], Edgardo Costa, René A. Méndez, W.-C. Jao, Todd J. Henry, John P. Subasavage, Misty A. Brown, Philip A. Ianna, and Jennifer Bartlett, ''The Astronomical Journal'' '''130''', #1 (July 2005), pp. 337&ndash;349. {{doi|10.1086/430473}}</ref>
|-
| 33
| 13.259
| style="background: #C67B30" colspan="2" |[[UGPS J072227.51-054031.2|UGPS 0722-05]] 
| 48
| style="background: {{star-color|T}};" | T9<ref name=RECONS /> <!--previous: M2Ve-->
| 16.52 J<ref>{{Cite arXiv | eprint=1004.0317v2 | author1=Lucas | author2=Tinney | author3=Ben Burningham | author4=Leggett | author5=Pinfield | author6=Richard Smart | author7=Jones | author8=Federico Marocco | author9=Barber | title=The discovery of a very cool, very nearby brown dwarf in the Galactic plane | class=astro-ph.SR | year=2010 }}</ref>
| 
| {{RA|07|22|27.3}}
| {{DEC|–05|40|30}}
|align=left | 246 
| 2010
| <ref name="Lucas2010v2">{{cite arXiv|last=Lucas |first=Philip W.|author2=Tinney; Burningham; Leggett; Pinfield; Smart; et al.  |title=Discovery of a very cool brown dwarf amongst the ten nearest stars to the Solar System|year=2010|eprint=1004.0317  |version=v1|class=astro-ph.SR}}</ref>
|-
| rowspan="2" | 34
| rowspan="2" | 13.349(110)
| rowspan="2" | [[Ross 614|Ross&nbsp;614]]<br>(V577&nbsp;Monocerotis, Gliese 234)
| Ross&nbsp;614A (LHS&nbsp;1849)
| 49
| style="background: {{star-color|M}};" | M4.5V<ref name=RECONS/>
| 11.15<ref name=RECONS />
| 13.09<ref name=RECONS />
| rowspan="2" | {{RA|06|29|23.4}}
| rowspan="2" | {{DEC|−02|48|50}}
| rowspan="2" align=left | 244.34(201)<ref name="Y"/><ref name="S"/>
| 1927
| rowspan="2" |
|-
| Ross&nbsp;614B (LHS&nbsp;1850)
| 49
| style="background: {{star-color|M}};" | M5.5V
| 14.23<ref name=RECONS />
| 16.17<ref name=RECONS />
| 1936
|-
| 35
| 13.820(98)
| colspan="2" | [[Wolf&nbsp;1061]] (Gliese 628, BD−12°4523)
| 51
| style="background: {{star-color|M}};" | M3.0V<ref name=RECONS />
| 10.07<ref name=RECONS />
| 11.93<ref name=RECONS />
| {{RA|16|30|18.1}}
| {{DEC|−12|39|45}}
|align=left | 236.01(167)<ref name="Y"/><ref name="H"/>
| 1919
| 
|-
| 36
| 14.066(109)
| colspan="2" | [[Van Maanen's star]] (Gliese 35, LHS&nbsp;7)
| 52
| style="background: #F0F0F0" | [[White dwarf|DZ7]]<ref name=RECONS />
| 12.38<ref name=RECONS />
| 14.21<ref name=RECONS />
| {{RA|00|49|09.9}}
| {{DEC|+05|23|19}}
|align=left | 231.88(179)<ref name="Y"/><ref name="H"/>
| 1896
| 
|-
| 37
| 14.231(66)
| colspan="2" | [[Gliese 1]] (CD−37°15492)
| 53
| style="background: {{star-color|M}};" |  M1.5 V <ref name=RECONS />
| 8.55<ref name=RECONS />
| 10.35<ref name=RECONS />
| {{RA|00|05|24.4}}
| {{DEC|−37|21|27}}
|align=left | 229.20(107)<ref name="Y"/><ref name="H"/>
| 1884
| 
|-
| rowspan="2" | 38
| rowspan="2" | 14.312(289)
| rowspan="2" | [[Wolf 424|Wolf&nbsp;424]]<br>(FL&nbsp;Virginis, LHS&nbsp;333, Gliese 473)
| Wolf&nbsp;424&nbsp;A
| 54
| style="background: {{star-color|M}};" | M5.5Ve
| 13.18<ref name=RECONS />
| 14.97<ref name=RECONS />
| rowspan="2" | {{RA|12|33|17.2}}
| rowspan="2" | {{DEC|+09|01|15}}
| rowspan="2" align=left | 227.90(460)<ref name="Y"/>
| 
| rowspan="2" |
|-
| Wolf&nbsp;424&nbsp;B
| 54
| style="background: {{star-color|M}};" | M7Ve
| 13.17<ref name=RECONS />
| 14.96<ref name=RECONS />
| 
|-
| 39
| 14.4
| colspan="2" | [[2MASS J154043.42-510135.7]]
| 56
| style="background: {{star-color|M}};" | M7V
| 15.26
| 17.04
| {{RA|15|40|43.42}}
| {{DEC|-51|01|35.7}}
|align=left | 224.80(290)
| 2014
| <ref>http://arxiv.org/abs/1405.5439</ref>
|-
| 40
| 14.509(187)
| colspan="2" | [[L 1159-16|L&nbsp;1159-16]] (TZ Arietis, Gliese 83.1)
| 57
| style="background: {{star-color|M}};" | M4.5V<ref name=RECONS />
| 12.27<ref name=RECONS />
| 14.03<ref name=RECONS />
| {{RA|02|00|13.2}}
| {{DEC|+13|03|08}}
|align=left | 224.80(290)<ref name="Y"/>
| 
| 
|-
| 41
| 14.793(55)
| colspan="2" | [[Gliese 687]] (LHS&nbsp;450, BD+68°946)
| 58
| style="background: {{star-color|M}};" | M3.0V<ref name=RECONS />
| 9.17<ref name=RECONS />
| 10.89<ref name=RECONS />
| {{RA|17|36|25.9}}
| {{DEC|+68|20|21}}
|align=left | 220.49(082)<ref name="Y"/><ref name="H"/>
| 
| has one known planet<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]</ref>
|-
| 42
| 14.805(242)
| colspan="2" | [[LHS 292|LHS&nbsp;292]] (LP&nbsp;731-58)
| 59
| style="background: {{star-color|M}};" | M6.5V<ref name=RECONS />
| 15.60<ref name=RECONS />
| 17.32<ref name=RECONS />
| {{RA|10|48|12.6}}
| {{DEC|−11|20|14}}
|align=left | 220.30(360)<ref name="Y"/>
| 
| 
|-
| 43
| 14.809(107)
| colspan="2" | [[Gliese 674]] (LHS&nbsp;449)
| 60
| style="background: {{star-color|M}};" | M3.0V<ref name=RECONS />
| 9.38<ref name=RECONS />
| 11.09<ref name=RECONS />
| {{RA|17|28|39.9}}
| {{DEC|−46|53|43}}
|align=left | 220.25(159)<ref name="Y"/><ref name="H"/>
| 
| has one known planet<ref>http://exoplanet.eu/star.php?st=GJ+674</ref>
|-
| rowspan="3" | 44
| rowspan="3" | 14.812(67)
| rowspan="3" | [[G 208-44/208-45|G 208-44<br/>G 208-45]]<br/>(GJ 1245)
| G&nbsp;208-44&nbsp;A (V1581&nbsp;Cyg)
| 61
| style="background: {{star-color|M}};" | M5.5V<ref name=RECONS />
| 13.46<ref name=RECONS />
| 15.17<ref name=RECONS />
| {{RA|19|53|54.2}}
| {{DEC|+44|24|55}}
| rowspan="3" align=left | 220.20(100)<ref name="Y"/>
| 
| rowspan="3" |
|-
| G&nbsp;208-45
| 61
| style="background: {{star-color|M}};" | M6.0V<ref name=RECONS />
| 14.01<ref name=RECONS />
| 15.72<ref name=RECONS />
| {{RA|19|53|55.2}}
| {{DEC|+44|24|56}}
| 
|-
| G&nbsp;208-44&nbsp;B
| 61
| style="background: {{star-color|M}};" | M5.5
| 16.75<ref name=RECONS />
| 18.46<ref name=RECONS />
| {{RA|19|53|54.2}}
| {{DEC|+44|24|55}}
| 
|-
| 45
| 15.060(140)
| colspan="2" | [[LP 145-141]] (WD&nbsp;1142-645, Gliese 440)
| 64
| style="background: #F0F0F0" | [[White dwarf|DQ6]]<ref name=RECONS />
| 11.50<ref name=RECONS />
| 13.18<ref name=RECONS />
| {{RA|11|45|42.9}}
| {{DEC|−64|50|29}}
|align=left | 216.57(201)<ref name="Y"/><ref name="H"/>
| 
| 
|-
| 46
| 15.313(259)
| colspan="2" | [[GJ 1002]]
| 65
| style="background: {{star-color|M}};" | M5.5V<ref name=RECONS />
| 13.76<ref name=RECONS />
| 15.40<ref name=RECONS />
| {{RA|00|06|43.8}}
| {{DEC|−07|32|22}}
|align=left | 213.00(360)<ref name="Y"/>
| 
| 
|-
| 47
| 15.342(141)
| colspan="2" | [[Gliese 876]] (Ross&nbsp;780)
| 66
| style="background: {{star-color|M}};" | M3.5V<ref name=RECONS />
| 10.17<ref name=RECONS />
| 11.81<ref name=RECONS />
| {{RA|22|53|16.7}}
| {{DEC|−14|15|49}}
|align=left | 212.59(196)<ref name="Y"/><ref name="H"/>
| 
| has four known planets<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}}</ref>
|-
| 48
| 15.610(204)
| colspan="2" | [[LHS 288|LHS&nbsp;288]] (Luyten&nbsp;143-23)
| 67
| style="background: {{star-color|M}};" | M5.5V<ref name=RECONS />
| 13.90<ref name=RECONS />
| 15.51<ref name=RECONS />
| {{RA|10|44|21.2}}
| {{DEC|−61|12|36}}
|align=left | 208.95(273)<ref name="recent"/>
| 
| <ref name=henry2006 />
|-
| rowspan="2" | 49
| rowspan="2" | 15.832(83)
| rowspan="2" | [[Gliese 412]]
| Gliese 412&nbsp;A
| 68
| style="background: {{star-color|M}};" | M1.0V<ref name=RECONS />
| 8.77<ref name=RECONS />
| 10.34<ref name=RECONS />
| {{RA|11|05|28.6}}
| {{DEC|+43|31|36}}
| rowspan="2" align=left | 206.02(108)<ref name="Y"/><ref name="H"/>
| 
| rowspan="2" |
|-
| Gliese 412&nbsp;B (WX&nbsp;Ursae&nbsp;Majoris)
| 68
| style="background: {{star-color|M}};" | M5.5V<ref name=RECONS />
| 14.48<ref name=RECONS />
| 16.05<ref name=RECONS />
| {{RA|11|05|30.4}}
| {{DEC|+43|31|18}}
| 
|-
| 50
| 15.848(52)
| colspan="2" | [[Groombridge 1618|Groombridge&nbsp;1618]] (Gliese 380)
| 70
| style="background: {{star-color|K}};" | [[K-type main-sequence star|K7.0V]]<ref name=RECONS />
| 6.59<ref name=RECONS />
| 8.16<ref name=RECONS />
| {{RA|10|11|22.1}}
| {{DEC|+49|27|15}}
|align=left | 205.81(067)<ref name="Y"/><ref name="H"/>
| 
| 
|-
| 51
| 15.942(218)
| colspan="2" | [[AD Leonis|AD&nbsp;Leonis]]
| 71
| style="background: {{star-color|M}};" | M3.0V<ref name=RECONS />
| 9.32<ref name=RECONS />
| 10.87<ref name=RECONS />
| {{RA|10|19|36.4}}
| {{DEC|+19|52|10}}
|align=left | 204.60(280)<ref name="Y"/>
| 
| 
|-
| 52
| 16.067<ref name="Kirkpatrick2012v1"/>
| style="background: #C67B30" colspan="2" | [[DENIS J081730.0-615520]]
| 72
| style="background: {{star-color|T}};" | [[Brown dwarf#Spectral class T|T6]]
| 
| 
|| {{RA|08|17|30.096}}
|| {{DEC|-61|55|15.802}}
| 203 <ref name="Kirkpatrick2012v1" />
| 2010
| 
|-
| 53
| 16.085(105)
| colspan="2" | [[Gliese 832]]
| 73
| style="background: {{star-color|M}};" | M1.5 V<ref name=RECONS />
| 8.66<ref name=RECONS />
| 10.20<ref name=RECONS />
| {{RA|21|33|34.0}}
| {{DEC|−49|00|32}}
|align=left | 202.78(132)<ref name="Y"/><ref name="H"/>
| 
| has two known planets<ref>{{cite journal | author=Bailey, Jeremy et al. | 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&ndash;747 | year=2008 | accessdate=2008-09-02 | arxiv=0809.0172 }}</ref><ref>http://arxiv.org/abs/1406.5587</ref>
|-
| 54
| 16.197(313)
| style="background: #C67B30" colspan="2" | [[DEN 0255-4700|DEN&nbsp;0255-4700]]
| 74
| style="background: {{star-color|L}};" | [[Brown dwarf|L7.5V]]<ref name=RECONS />
| 22.92<ref name=RECONS />
| 24.44<ref name=RECONS />
| {{RA|02|55|03.7}}
| {{DEC|−47|00|52}}
|align=left | 201.37(389)<ref name="recent"/>
| 
| <ref name=costa2005 />
|-
| rowspan="3" | 54
| rowspan="3" | 16.26
| rowspan="3" | [[40 Eridani]]
| 40&nbsp;Eridani&nbsp;A
| 75
| style="background: {{star-color|K}};" | K1.V
| 11.17
| 5.92
| {{RA|04|15|16.320}} 
| {{DEC|−07|39|10.34}}
| 
| 
| 
|-
| 40&nbsp;Eridani&nbsp;B
| 75
| style="background: {{star-color|D}};" | [[witte dwerg | DA.4.V]]
| 11.17
| 11.01
| {{RA|04|15|16.320}} 
| {{DEC|−07|39|10.34}}
|
|
| 
|-
| 40&nbsp;Eridani&nbsp;C
| 75
| style="background: {{star-color|M}};" | M4.5
| 11.17
| 12.66
| {{RA|04|15|16.320}} 
| {{DEC|−07|39|10.34}}
| 
| 
| 
|-
| 55
| 16.3
| style="background: #C67B30" colspan="2" | [[WISE J0521+1025]]
| 78
| style="background: {{star-color|L}};" | [[Bruine dwerg|L7.5]]
| 14
| 
| {{RA|05|21|26.349}}
| {{DEC|10|25|27.41}}
| 
| Okt 2012
| 
|- 
| 56
| 16.3
| style="background: #C67B30" colspan="2" | [[WISE 1639-1847]]
| 79
| style="background: {{star-color|Y}};" | [[Bruine dwerg|Y0.5]]
| 14
| 
| {{RA|16|39|40.83}}
| {{DEC|-68|47|38.6}}
| 200
| 2012
|
|-
| 57
| 16.46
| colspan="2" | [[EV Lacertae]]
| 80
| style="background: {{star-color|M}};" | M3.5V
| 10.09
| 
| {{RA|22|46|49.7323}}
| {{DEC|+44|20|02.368}}
|
| 
| 
|-
| rowspan="2" | 58
| rowspan="2" | 16.58
| rowspan="2" | [[70 Ophiuchi]]
| 70&nbsp;Ophiuchi&nbsp;A
| 81
| style="background: {{star-color|K}};" | K0.V
| style="background: lightblue;" | 4.03
| 5.48
| {{RA|18|05|27.371}}
| {{DEC|+02|29|59.32}}
|
| 
| 
|-
| 70&nbsp;Ophiuchi&nbsp;B
| 81
| style="background: {{star-color|K}};" | K4.V
| style="background: lightblue;" | 6
| 7.51
| {{RA|18|05|27.421}}
| {{DEC|+02|29|56.42}}
|
| 
|
|-
| 59
| 16.60
| colspan="2" | [[Gliese 682]]
| 83
| style="background: {{star-color|M}};" | M3.5V
| 10.96
| 12,45
| {{RA|17|37|03.6613}}
| {{DEC|–44|19|09.18}}
|
|
| 
|-
| 60
| 16.73
| colspan="2" | [[Altair]]
| 84
| style="background: {{star-color|A}};" | A7.V
| style="background: lightblue;" | 0.77
| 2,21
| {{RA|19|50|46.99855}}
| {{DEC|+08|52|05.9563}}
|
|
| 
|-
| rowspan="2" | 61
| rowspan="2" | 17.05
| rowspan="2" | [[Gliese 1116]]
| Gliese&nbsp;1116&nbsp;A
| 85
| style="background: {{star-color|M}};" | M8.V
| 14.06
| 14.92
| 
| 
|
| 
| 
|-
| Gliese&nbsp;1116&nbsp;B
| 85
| style="background: {{star-color|M}};" | M5.5V
| 14.06
| 14.92
| 
| 
|
| 
|
|-
| 62
| 17.10
| colspan="2" | [[Gliese 3379]]
| 87
| style="background: {{star-color|M}};" | M3.5V
| 11.33
| 12,68
| {{RA|06|00|3.495}}
| {{DEC|+02|42|23.67}}
|
|
| 
|-
| 63
| 17.36
| colspan="2" | [[LHS 1723]]
| 88
| style="background: {{star-color|M}};" | M4.5V
| 12.15
| 13,46
| 
| 
|
|
| 
|-
| rowspan="2" | 64
| rowspan="2" | 17.41
| style="background: #C67B30"  rowspan="2" | [[2MASS 0939-2448]]
| style="background: #C67B30"  | 2MASS&nbsp;0939-2448&nbsp;A
| 89
| style="background: {{star-color|T}};" | [[Bruine dwerg|T8]]
| 15.96
| 
| {{RA|09|39|35.48}}
| {{DEC|-24|48|27.9}}
|
| 2005
| 
|-
| style="background: #C67B30"  |  2MASS&nbsp;0939-2448&nbsp;B
| 89
| style="background: {{star-color|T}};" | [[Bruine dwerg|T8]]
| 15.96
| 
| {{RA|09|39|35.48}}
| {{DEC|-24|48|27.9}} 
|
| 2005 
|
|-
| 65
| 17.42
| colspan="2" | [[Gliese 445]]
| 91
| style="background: {{star-color|M}};" | M3.5V
| 10.78
| 
| {{RA|11|47|41.3771}}
| {{DEC|+78|41|28.178}}
|
|
| 
|-
| 66
| 17.66
| colspan="2" | [[Wolf 498]]
| 92
| style="background: {{star-color|M}};" | M.V
| 8.46
| 9,78
| 
| 
|
|
| 
|-
| rowspan="2" | 67
| rowspan="2" | 17.91
| rowspan="2" | [[Stein 2051]]
| Stein&nbsp;2051&nbsp;A
| 93
| style="background: {{star-color|M}};" | M4.V
| 11.08
| 12.37
| 
| 
|
| 
| 
|-
| Stein&nbsp;2051&nbsp;B
| 93
| style="background: {{star-color|D}};" | [[Witte dwerg|DC5]]
| 12.44
| 13.73
| 
| 
|
| 
|
|-
| 68
| 18.10
| style="background: #C67B30" colspan="2" | [[WISE 1741+2553]]
| 95
| style="background: {{star-color|T}};" | [[Bruine dwerg|T9]]
| 16.63
| 
| {{RA|17|41|24.22}}
| {{DEC|25|53|18.96}}
|
|
| 
|-
| 69
| 18.20
| style="background: #C67B30" colspan="2" | [[2MASS 1114-2618]]
| 96
| style="background: {{star-color|T}};" | [[Bruine dwerg|T7.5]]
| 15.55
| 
| {{RA|11|14|51.337}}
| {{DEC|-26|18|23.56}}
|
|
| 
|-
| 70
| 18.31
| colspan="2" | [[Gliese 251]]
| 97
| style="background: {{star-color|M}};" | M4.V
| 9.89
| 11,18
| 
| 
|
|
| 
|-
| 71
| 18.48
| style="background: #C67B30" colspan="2" | [[2MASS 1835+3259]]
| 98
| style="background: {{star-color|M}};" | [[Bruine dwerg|M8.5]]
| 16.28
| 
| {{RA|18|35|37.902}}
| {{DEC|+32|59|54.59}}
|
|
| 
|-
| 72
| 18.53
| colspan="2" | [[Gliese 205]]
| 99
| style="background: {{star-color|M}};" | M1.5
| 7.97
| 9.19
| 
|
| 
|
| 
|-
| 73
| 18.60
| colspan="2" | [[L 449-1]]
| 100
| style="background: {{star-color|M}};" | M3.0
| 
| 
| 
|
| 
|
| 
|-
| 74
| 18.62
| style="background: #C67B30" colspan="2" | [[2MASS 0415-0935]]
| 101
| style="background: {{star-color|T}};" | [[Bruine dwerg|T8.V]]
| 15.343
| 
| {{RA|04|15|19.54}}
| {{DEC|−09|35|06.6}}
|
|
| 
|-
| 75
| 18.63
| colspan="2" | [[LP 816-060]]
| 102
| style="background: {{star-color|M}};" | M5.V
| 11.41
| 12.71
| 
| 
|
|
| 
|-
| 76
| 18.77
| colspan="2" | [[Alsafi]] (Sigma Draconis)
| 103
| style="background: {{star-color|G}};" | G9.V
| style="background: lightblue;" | 4.674
| 5.87
| {{RA|19|32|21.59026}}
| {{DEC|+69|39|40.2354}}
|
| 
| 
|-
| rowspan="2" | 77
| rowspan="2" | 18.77
| rowspan="2" | [[Gliese 229]]
| Gliese&nbsp;229&nbsp;A
| 104
| style="background: {{star-color|M}};" | M1.V
| 8.14
| 
| {{RA|06|10|34.6154}}
| {{DEC|−21|51|52.715}}
|
| 
| 
|-
| style="background: #C67B30"  |  [[Gliese 229B]]
| 104
| style="background: {{star-color|T}};" | [[Bruine dwerg|T7]]
| 
| 
| {{RA|06|10|34.6154}}
| {{DEC|−21|51|52.715}}
|
| 1994 
|
|-
| rowspan="4" | 78
| rowspan="4" | 19.00
| rowspan="4" | [[Gliese 570]]
| Gliese&nbsp;570&nbsp;A
| 106
| style="background: {{star-color|K}};" | K4.V
| style="background: lightblue;" |5.64
| 6.79
| {{RA|14|57|28.00144}} 
| {{DEC|-21|24|55.7131}}
| 
| 
| 
|-
| Gliese&nbsp;570&nbsp;B
| 106
| style="background: {{star-color|M}};" | M1.V
| 8.07
| 9.21
| {{RA|14|57|28.00144}} 
| {{DEC|-21|24|55.7131}}
|
|
| 
|-
| Gliese&nbsp;570&nbsp;C
| 106
| style="background: {{star-color|M}};" | M3.V
| 9.90
| 11.05
| {{RA|14|57|28.00144}} 
| {{DEC|-21|24|55.7131}}
| 
| 
| 
|-
| style="background: #C67B30" | Gliese&nbsp;570&nbsp;D
| 106
| style="background: {{star-color|M}};" | [[bruine dwerg|T7.V]]
| 
| 
| {{RA|14|57|28.00144}} 
| {{DEC|-21|24|55.7131}}
| 
| jan 2000 
| 
|-
| 79
| 19.02
| colspan="2" | [[Ross 47]] 
| 110
| style="background: {{star-color|M}};" | M4.V
| 11.56
| 12.75
| 
| 
|
| 
| 
|-
| 80
| 19.06
| colspan="2" | [[Gliese 693]] 
| 111
| style="background: {{star-color|M}};" | M3.5V
| 10.75
| 11.93
| 
| 
|
| 
| 
|-
| rowspan="2" | 81
| rowspan="2" | 19.06
| rowspan="2" | [[Gliese 752]]
| Gliese&nbsp;752&nbsp;A
| 112
| style="background: {{star-color|M}};" | M2.5
| 9.13
| 10.13
| {{RA|19|16|55.257}}
| {{DEC|+05|10|08.05}}
| 164.3
| 
| 
|-
| Gliese 752B
| 112
| style="background: {{star-color|M}};" | M1.V
| 17.30
| 18.7
| {{RA|19|16|57.62}}
| {{DEC|+05|09|02.2}}
| 
|  
|
|-
| 82
| 19.20
| style="background: #C67B30" colspan="2" | [[WISE 0359-5401]]
| 114
| style="background: {{star-color|Y}};" | [[Bruine dwerg|Y0.V]]
| 21.94
| 
| {{RA|03|59|34.06}}
| {{DEC|-54|01|54.6}}
|
|
| 
|-
| 83
| 19.28
| colspan="2" | [[Gliese 754]] 
| 115
| style="background: {{star-color|M}};" | M4.5V
| 12.23
| 13.37
| 
| 
|
| 
| 
|-
| 84
| 19.35
| colspan="2" | [[Gliese 588]] 
| 116
| style="background: {{star-color|M}};" | M3.V
| 9.31
| 10.41
| 
| 
|
| 
| 
|-
| rowspan="2" | 85
| rowspan="2" | 19.37
| rowspan="2" | [[Gliese 1005]]
| Gliese&nbsp;1005&nbsp;A
| 117
| style="background: {{star-color|M}};" | M2.V
| 12.03
| 13.41
| 
| 
| 
| 
| 
|-
| Gliese 1005B
| 117
| style="background: {{star-color|M}};" | M6.V
| 14.30
| 15.7
| 
| 
| 
|  
|
|-
| 86
| 19.41
| colspan="2" | [[Gliese 908]] 
| 119
| style="background: {{star-color|M}};" | M2.V
| 8.98
| 10.1
| 
| 
|
| 
| 
|-
| rowspan="2" | 87
| rowspan="2" | 19.42
| rowspan="2" | [[Achird]] (Eta Cassiopeiae)
| Eta&nbsp;Cassiopeiae&nbsp;A
| 120
| style="background: {{star-color|G}};" | G0.V
| style="background: lightblue;" | 3.44
| 
| {{RA|00|49|06.29070}}
| {{DEC|+57|48|54.6758}}
| 
| 
| 
|-
| Eta CassiopeiaeB
| 120
| style="background: {{star-color|K}};" | K7.V
| 7.51
| 
| {{RA|00|49|06.29070}}
| {{DEC|+57|48|54.6758}} 
| 
|  
|
|-
| rowspan="3" | 88
| rowspan="3" | 19.47
| rowspan="3" | [[36 Ophiuchi]]
| 36&nbsp;Ophiuchi&nbsp;A
| 122
| style="background: {{star-color|K}};" | K2.V
| style="background: lightblue;" | 5.08
| 
| {{RA|17|15|20.851}}
| {{DEC| -26|36|09.04}}
| 167.1
| 
| 
|-
| 36&nbsp;Ophiuchi&nbsp;B
| 122
| style="background: {{star-color|K}};" | K1.V
| style="background: lightblue;" | 5.08
| 
| {{RA|17|15|20.978}}
| {{DEC| -26|36|10.18}}
| 167.1
|
| 
|-
| 36&nbsp;Ophiuchi&nbsp;C
| 122
| style="background: {{star-color|K}};" | K5.V
| 6.34
| 
| {{RA|17|16|13.3624}}
| {{DEC| -26|32|46.129}}
| 167.1
| 
| 
|-
| 89
| 19.51
| colspan="2" | [[YZ Canis Minoris]] 
| 125
| style="background: {{star-color|M}};" | M4.5V
| 11.19
| 12.31
| {{RA|07|44|40.17401}}
| {{DEC|03|33|08.8350}}
|
| 
| 
|-
| 90
| 19.6
| colspan="2" | [[2MASS 0533-4257]] 
| 126
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
|
| 
| 
|-
| rowspan="2" | 91
| rowspan="2" | 19.6
| rowspan="2" | [[2MASS 1845-1409]]
| 2MASS&nbsp;1845-1409&nbsp;A
| 127
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
| 
| 
|-
| 2MASS 1845-1409B
| 127
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
|  
|
|-
| rowspan="2" | 92
| rowspan="2" | 19.62
| rowspan="2" | [[HR 7703]]
| HR&nbsp;7703&nbsp;A
| 129
| style="background: {{star-color|K}};" | K2.V
| style="background: lightblue;" | 5.31 
| 6.40
| {{RA|20|11|11.94}}
| {{DEC|–36|06|04.4}}
| 166.25
| 
| 
|-
| HR 7703B
| 129
| style="background: {{star-color|M}};" | M3.5V
| 11.5
| 12.6
| {{RA|20|11|11.94}}
| {{DEC|–36|06|04.4}}
| 166.25
|  
|
|-
| 93
| 19.71
| colspan="2" | [[82 G. Eridani]] 
| 131
| style="background: {{star-color|G}};" | G8.V
| style="background: lightblue;" | 4.254
| 5.34
| {{RA|03|19|55.65093}}
| {{DEC|−43|04|11.2175}}
| 165.47
| 
| heeft 3 planeten 
|-
| 94
| 19.80
| colspan="2" | [[G 240-72]] 
| 132
| style="background: {{star-color|D}};" | [[witte dwerg|DQP.90]]
| 14.15
| 15.23
| {{RA|17|48|08.17}}
| {{DEC|+70|52|35.3}}
| 164.7
| 
| 
|-
| rowspan="2" | 96
| rowspan="2" | 19.92
| rowspan="2" | [[Gliese 338]]
| Gliese&nbsp;338&nbsp;A
| 134
| style="background: {{star-color|M}};" | M4.V
| 9.4 
| 10.95
| 
| 
| 
| 
| 
|-
| Gliese 338B
| 134
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
|  
|
|-
| rowspan="2" | 97
| rowspan="2" | 19.96
| rowspan="2" | [[Gliese 268]]
| Gliese&nbsp;268&nbsp;A
| 136
| style="background: {{star-color|M}};" | M4.V
| 12.05 
| 
| 
| 
| 
| 
| 
|-
| Gliese 268B
| 136
| style="background: {{star-color|M}};" | M.V
| 12.45
| 
| 
| 
| 
|  
|
|-
| 98
| 19.20
| style="background: #C67B30" colspan="2" | [[2MASS 0937+2931]]
| 138
| style="background: {{star-color|T}};" | [[Bruine dwerg|T6]]
| 
| 
| {{RA|09|37|34.9}}
| {{DEC|29|31|41}}
| 163.49
| 2002
| 
|-
| 99
| 20.22
| colspan="2" | [[Gliese 784]]
| 139
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
| 
| 
|-
| 100
| 20.29
| colspan="2" | [[HR Librae]]
| 140
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
| 
| 
|-
| 101
| 20.38
| colspan="2" | [[Gliese 581]]
| 141
| style="background: {{star-color|M}};" | M.V
| 10.57
| 11.6
| {{RA|15|19|26.8250}}
| {{DEC|−07|43|20.209}}
| 161.91
| 
| heeft zes planeten
|-
| rowspan="2" | 102
| rowspan="2" | 20.40
| rowspan="2" | [[EQ Pegasi]]
| EQ&nbsp;Pegasi&nbsp;A
| 142
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
| 
| 
|-
| EQ PegasiB
| 142
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
|  
|
|-
| 103
| 20.50
| style="background: #C67B30" colspan="2" | [[WISE 0146+4234]]
| 144
| style="background: {{star-color|Y}};" | [[Bruine dwerg|Y0]]
| 18.71
| 
| {{RA|15|03|19.613}}
| {{DEC|42|34|10}}
| 
| 
| 
|-
| 104
| 20.75
| style="background: #C67B30" colspan="2" | [[2MASS 1503+2525]]
| 145
| style="background: {{star-color|T}};" | [[bruine dwerg|T5.5]]
| 18.71
| 
| {{RA|15|03|19.613}}
| {{DEC|25|25|19.68}}
| 157.2
| 
| 
|-
| 105
| 20.8
| colspan="2" | [[LHS 2090]]
| 146
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
| 
| 
|-
| 106
| 20.89
| colspan="2" | [[LP 658-2]]
| 147
| style="background: {{star-color|D}};" | [[witte dwerg|DZ.11.8]]
| 13.99
| 15.44
| {{RA|05|55|09.53}}
| {{DEC|−04|10|07.1}}
| 
| 
| 
|-
| 107
| 20.8
| colspan="2" | [[LHS 337]]
| 148
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
| 
| 
|-
| rowspan="2" | 108
| rowspan="2" | 20.90
| rowspan="2" | [[Furuhjelm 46]]
| Furuhjelm&nbsp;46&nbsp;A
| 149
| style="background: {{star-color|M}};" | M.V
| 10.02
| 
| {{RA|10|56|28.99}}
| {{DEC|+07|00|52.0}} 
| 167.29
| 
| 
|-
| Furuhjelm 46B
| 149
| style="background: {{star-color|M}};" | M.V
| 10.25
| 
| {{RA|10|56|28.99}}
| {{DEC|+07|00|52.0}}
| 167.29
|  
|
|-
| 109
| 20.9
| colspan="2" | [[G 180-060]]
| 151
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
| 
| 
|-
| 110
| 20.9
| style="background: #C67B30" colspan="2" | [[SIMP 0136+0933]]
| 152
| style="background: {{star-color|T}};" | [[bruine dwerg| T2.5]]
| 12.771
| 
| {{RA|01|36|57}}
| {{DEC|+09|33|47.3}}
| 156.25
| 2006
| 
|-
| rowspan="5" | 111
| rowspan="5" | 21.05
| rowspan="5" | [[V1054 Ophiuchi]]
| V1054&nbsp;Ophiuchi&nbsp;A
| 153
| style="background: {{star-color|M}};" | M3.V
| 10.69
| 9.74
| {{RA|16|55|32.0}} 
| {{DEC|-08|21|30|21.05}}
| 
| 
| 
|-
| V1054&nbsp;Ophiuchi&nbsp;Ba
| 153
| style="background: {{star-color|M}};" | M3.Ve
| 11.79
| 10.34
| {{RA|16|55|32.0}} 
| {{DEC|-08|21|30|21.05}}
|
|
| 
|-
| V1054&nbsp;Ophiuchi&nbsp;Bb
| 153
| style="background: {{star-color|M}};" | M3.Ve
| 11.79
| 10.84
| {{RA|16|55|32.0}} 
| {{DEC|-08|21|30|21.05}}
| 
| 
| 
|-
| Gliese 643
| 153
| style="background: {{star-color|M}};" | M3.5V
| 12.69
| 11.74
| {{RA|16|55|32.0}} 
| {{DEC|-08|21|30|21.05}}
| 
| 
| 
|-
| V1054 C
| 153
| style="background: {{star-color|M}};" | M7.0V
| 17.75
| 16.80
| {{RA|16|55|32.0}} 
| {{DEC|-08|21|30|21.05}}
| 
| 
| 
|-
| 112
| 21.3
| colspan="2" | [[LP 71-82]] 
| 158
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
| 
| 
|-
| 113
| 21.3
| colspan="2" | [[G 161-71]] 
| 159
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
| 
| 
|-
| 114
| 21.3
| colspan="2" | [[Gliese 625]] 
| 160
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
| 
| 
|-
| 115
| 21.3
| colspan="2" | [[Gliese 1128]] 
| 161
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
| 
| 
|-
| 116
| 21.3
| colspan="2" | [[GL Virginis]] 
| 162
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
| 
| 
|-
| 117
| 21.34
| colspan="2" | [[HR 8832]] 
| 163
| style="background: {{star-color|K}};" | K3.V
| style="background: lightblue;"  | 5.574
| 6.50
| {{RA|23|13|16.97632}}
| {{DEC|+57|10|06.0823}}
| 152.76
| 
| 
|-
| 118
| 21.4
| colspan="2" | [[LHS 3003]] 
| 164
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
| 
| 
|-
| 119
| 21.8
| colspan="2" | [[Gliese 408]] 
| 165
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
| 
| 
|-
| 120
| 21.8
| colspan="2" | [[Gliese 408]] 
| 166
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
| 
| 
|-
| rowspan="2" | 121
| rowspan="2" | 21.89
| rowspan="2" | [[Xi Boötis]]
| Xi&nbsp;Boötis&nbsp;A
| 167
| style="background: {{star-color|G}};" | G8.Ve
| style="background: lightblue;" | 4.70
| 5.54
| {{RA|14|51|23.37993}} 
| {{DEC|+19|06|01.6994}}
| 148.98
| 
| 
|-
| Xi&nbsp;Boötis&nbsp;B
| 167
| style="background: {{star-color|K}};" | K4.Ve
| 6.97
| 7.81
| {{RA|14|51|23.37993}} 
| {{DEC|+19|06|01.6994}}
| 148.98
|
| 
|-
| 122
| 21.9
| colspan="2" | [[SCR J1546-5534]] 
| 169
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
| 
| 
|-
| rowspan="2" | 123
| rowspan="2" | 21.9
| rowspan="2" | [[Gliese 829]]
| Gliese&nbsp;829&nbsp;A
| 170
| style="background: {{star-color|M}};" | M.V
| 
| 
|  
| 
| 
| 
| 
|-
| Gliese&nbsp;829&nbsp;B
| 170
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
|
| 
|-
| rowspan="3" | 124
| rowspan="3" | 22.1
| rowspan="3" | [[G 41-14]]
| G&nbsp;41-14&nbsp;A
| 172
| style="background: {{star-color|M}};" | M.V
| 
| 
|  
| 
| 
| 
| 
|-
| G&nbsp;41-14&nbsp;B
| 172
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
|
| 
|-
| G&nbsp;41-14&nbsp;C
| 172
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
|
| 
|-
| 122
| 22.2
| colspan="2" | [[EE Leonis]] 
| 175
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
| 
| 
|-
| rowspan="2" | 123
| rowspan="2" | 22.3
| rowspan="2" | [[Gliese 880]]
| Gliese&nbsp;880&nbsp;A
| 176
| style="background: {{star-color|M}};" | M.V
| 
| 
|  
| 
| 
| 
| 
|-
| Gliese&nbsp;880&nbsp;B
| 176
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
|
| 
|-
| 124
| 22.3
| colspan="2" | [[Gliese 299]] 
| 178
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
| 
| 
|-
| 125
| 22.6
| style="background: #C67B30" colspan="2" | [[WISE 2054+1459]]
| 179
| style="background: {{star-color|Y}};" | [[bruine dwerg| Y0]]
| 17.1
| 
| {{RA|20|56|28.88}}
| {{DEC|14|59|53.68}}
| 144
| 2011
| 
|-
| rowspan="3" | 126
| rowspan="3" | 22.7
| rowspan="3" | [[LP 771-095]]
| LP&nbsp;771-095&nbsp;A
| 180
| style="background: {{star-color|M}};" | M.V
| 
| 
|  
| 
| 
| 
| 
|-
| LP&nbsp;771-095&nbsp;B
| 180
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
|
| 
|-
| LP&nbsp;771-095&nbsp;C
| 180
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
|
| 
|-
| 127
| 22.7
| colspan="2" | [[Gliese 1068]] 
| 183
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
| 
| 
|-
| 128
| 22.8
| colspan="2" | [[2MASS 2036-3607]]
| 184
| style="background: {{star-color|M}};" | M.V
| 
| 
|  
| 
| 
| 
| 
|-
| rowspan="2" | 129
| rowspan="2" | 22.8
| rowspan="2" | [[L 369-44]]
| L&nbsp;369-44&nbsp;A
| 185
| style="background: {{star-color|M}};" | M.V
| 
| 
|  
| 
| 
| 
| 
|-
| L&nbsp;369-44&nbsp;B
| 185
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
|
| 
|-
| 130
| 22.8
| colspan="2" | [[2MASS 1852-3730]]
| 187
| style="background: {{star-color|M}};" | M.V
| 
| 
|  
| 
| 
| 
| 
|-
| rowspan="2" | 131
| rowspan="2" | 22.8
| rowspan="2" | [[G 161-7]]
| G&nbsp;161-7&nbsp;A
| 188
| style="background: {{star-color|M}};" | M.V
| 
| 
|  
| 
| 
| 
| 
|-
| G&nbsp;161-7&nbsp;B
| 188
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
|
| 
|-
| 132
| 22.8
| style="background: #C67B30" colspan="2" | [[WISE 1928+2356]]
| 190
| style="background: {{star-color|T}};" | [[bruine dwerg| T]]
| 
| 
| 
| 
| 
| 
| 
|-
| rowspan="2" | 133
| rowspan="2" | 23.0
| rowspan="2" | [[Gliese 809]]
| Gliese&nbsp;809&nbsp;A
| 191
| style="background: {{star-color|M}};" | M.V
| 
| 
|  
| 
| 
| 
| 
|-
| Gliese&nbsp;809&nbsp;B
| 191
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
|
| 
|-
| 134
| 23.0
| colspan="2" | [[Gliese 393]]
| 193
| style="background: {{star-color|M}};" | M.V
| 
| 
|  
| 
| 
| 
| 
|-
| rowspan="2" | 135
| rowspan="2" | 23.1
| rowspan="2" | [[Gliese 54]]
| Gliese&nbsp;54&nbsp;A
| 194
| style="background: {{star-color|M}};" | M.V
| 
| 
|  
| 
| 
| 
| 
|-
| Gliese&nbsp;54&nbsp;B
| 194
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
|
| 
|-
| 136
| 23.1
| style="background: #C67B30" colspan="2" | [[WISE 0713+2917]]
| 196
| style="background: {{star-color|Y}};" | [[bruine dwerg| Y0]]
| 20.06
| 
| {{RA|07|13|22.55}}
| {{DEC|-29|17|51.9}}
| 
| 
| 
|-
| 137
| 23.2
| style="background: #C67B30" colspan="2" | [[WISE 0005+3737]]
| 197
| style="background: {{star-color|T}};" | [[bruine dwerg| T9]]
| 
| 
| {{RA|00|05|17.48}}
| {{DEC|37|37|20.5}}
| 
| 
| 
|-
| rowspan="3" | 138
| rowspan="3" | 23.42
| rowspan="3" | [[HR 753]]
| HR&nbsp;753&nbsp;A
| 198
| style="background: {{star-color|K}};" | K3.V
| style="background: lightblue;"  | 5.82
| 6.49
| {{RA|02|36|04.89}}
| {{DEC|+06|53|12.7}}
| 139.27
| 
| 
|-
| HR&nbsp;753&nbsp;B
| 198
| style="background: {{star-color|M}};" | M3.5V
| 11.66
| 12.34
| {{RA|02|36|15.0}} 
| {{DEC|+06|52|18}}
| 139.27
|
| 
|-
| HR&nbsp;753&nbsp;C
| 198
| style="background: {{star-color|M}};" | M7.V
| 16.9
| 17.58
| {{RA|02|35|58.8}}
| {{DEC|+06|52|00}} 
| 139.27
|
| 
|-
| 139
| 23.5
| colspan="2" | [[SCR J0740-4257]]
| 201
| style="background: {{star-color|M}};" | M.V
| 
| 
|  
| 
| 
| 
| 
|-
| 140
| 23.5
| colspan="2" | [[L 43-72]]
| 202
| style="background: {{star-color|M}};" | M.V
| 
| 
|  
| 
| 
| 
| 
|-
| rowspan="3" | 141
| rowspan="3" | 23.60
| rowspan="3" | [[Gliese 667]]
| Gliese&nbsp;667&nbsp;A
| 203
| style="background: {{star-color|K}};" | K3.V
| style="background: lightblue;"  | 5.91
| 7.07
| {{RA|17|18|57.16483}}
| {{DEC|−34|59|23.1416}}
| 146.29
| 
| 
|-
| Gliese&nbsp;667&nbsp;B
| 203
| style="background: {{star-color|K}};" | K5.V
| 7.20
| 8.02
| {{RA|17|18|57.16483}}
| {{DEC|−34|59|23.1416}}
| 146.29
|
| 
|-
| Gliese&nbsp;667&nbsp;C
| 203
| style="background: {{star-color|M}};" | M1.5V
| 10.20
| 11.03
| {{RA|17|18|57.16483}}
| {{DEC|−34|59|23.1416}}
| 146.29
|
| heeft zeven planeten
|-
| 142
| 23.6
| colspan="2" | [[Gliese 1286]]
| 206
| style="background: {{star-color|M}};" | M.V
| 
| 
|  
| 
| 
| 
| 
|-
| 143
| 23.6
| colspan="2" | [[Gliese 4063]]
| 207
| style="background: {{star-color|M}};" | M.V
| 
| 
|  
| 
| 
| 
| 
|-
| 143
| 23.7
| colspan="2" | [[Gliese 4053]]
| 208
| style="background: {{star-color|M}};" | M.V
| 
| 
|  
| 
| 
| 
| 
|-
| 144
| 23.91
| style="background: #C67B30" colspan="2" | [[2MASS 1507-1627]]
| 209
| style="background: {{star-color|L}};" | [[bruine dwerg |L5]]
| 11.895
| 
| {{RA|15|07|47.69}}
| {{DEC|−16|27|38.6}}
| 136.4
| 
| 
|-
| 145
| 24.1
| style="background: #C67B30" colspan="2" | [[WISE 0049-2151]]
| 210
| style="background: {{star-color|T}};" | [[bruine dwerg |T8.5]]
| 
| 
| {{RA|00|49|45.61}}
| {{DEC|21|51|20}}
| 136.4
| 2012
| 
|-
| 146
| 24.2
| style="background: #C67B30" colspan="2" | [[WISE 0254+0223]]
| 211
| style="background: {{star-color|T}};" | [[bruine dwerg |T8]]
| 15.916
| 
| {{RA|02|54|09.62}}
| {{DEC|02|23|58.85}}
| 135
| 2011
| 
|-
| rowspan="2" | 147
| rowspan="2" | 24.28
| rowspan="2" | [[Gliese 3991]]
| Gliese&nbsp;3991&nbsp;A
| 212
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
| 
| 
|-
| Gliese&nbsp;3991&nbsp;B
| 212
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
|
| 
|-
| 148
| 24.29
| colspan="2" | [[Gliese 4248]]
| 214
| style="background: {{star-color|M}};" | M.V
| 
| 
|  
| 
| 
| 
| 
|-
| 159
| 24.3
| colspan="2" | [[Gliese 4274]]
| 215
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
| 
| 
|-
| 150
| 24.31
| colspan="2" | [[HD 4628]]
| 216
| style="background: {{star-color|K}};" | K2.V
| style="background: lightblue;"  | 5.75
| 5.88
| {{RA|00|48|22.98}}
| {{DEC|+05|16|50.2}}
| 134.14
| 
| 
|-
| 151
| 24.33
| colspan="2" | [[Beta Hydri]]
| 217
| style="background: {{star-color|G}};" | G2.IV
| style="background: lightblue;" | 2.80
| 3.45
| {{RA|00|25|45.07036}}
| {{DEC|–77|15|15.2860}}
| 134.07
| 
| 
|-
| 152
| 24.5
| colspan="2" | [[Gliese 109]]
| 218
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
| 
| 
|-
| 153
| 24.57
| colspan="2" | [[107 Piscium]]
| 219
| style="background: {{star-color|K}};" | K1.V
| style="background: lightblue;" | 5.14 
| 5.87
| {{RA|01|42|29.7619}}
| {{DEC|+20|16|06.616}}
| 133.92
| 
| 
|-
| 154
| 24.6
| colspan="2" | [[Gliese 1224]]
| 220
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
| 
| 
|-
| rowspan="2" | 155
| rowspan="2" | 24.62
| rowspan="2" | [[Mu Cassiopeiae]]
| Mu&nbsp;Cassiopeiae&nbsp;A
| 221
| style="background: {{star-color|G}};" | G5.VI
| style="background: lightblue;" | 5.159 
| 5.77
| {{RA|01|08|16.39470}}
| {{DEC|+54|55|13.2264}}
| 132.38
| 
| 
|-
| Mu&nbsp;Cassiopeiae&nbsp;B
| 221
| style="background: {{star-color|M}};" | M5.V
| 11
| 11.6
| {{RA|01|08|16.39470}}
| {{DEC|+54|55|13.2264}}
| 132.38
|
| 
|-
| 156
| 24.7
| colspan="2" | [[Gliese 3378]]
| 223
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
| 
| 
|-
| 157
| 24.7
| style="background: #C67B30" colspan="2" | [[WISE 0410+1502]]
| 224
| style="background: {{star-color|Y}};" | [[bruine dwerg |Y0]]
| 19.15
| 
| {{RA|04|10|22.79}}
| {{DEC|15|02|47.47}}
| 132
| 2011
| 
|-
| 158
| 24.97
| colspan="2" | [[Gliese 514]]
| 225
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
| 
| 
|-
| 159
| 25.04
| colspan="2" | [[Vega]]
| 226
| style="background: {{star-color|A}};" | A1.V
| style="background: lightblue;" | 0.03
| 0.58
| {{RA|18|36|56.33635}}
| {{DEC|+38|47|01.2802}}
| 130.23
| 
| 
|-
| 160
| 25.12
| colspan="2" | [[Gliese 673]]
| 227
| style="background: {{star-color|K}};" | K.V
| 7.492
| 8.06
| {{RA|17|25|45.23266}}
| {{DEC|+02|06|41.1208}}
| 129.86
| 
| 
|-
| rowspan="3" | 161
| rowspan="3" | 25.13
| rowspan="3" | [[Fomalhaut]]
| Fomalhaut&nbsp;A
| 228
| style="background: {{star-color|A}};" | A3.V
| style="background: lightblue;"  | 1.16
| 1.72
| {{RA|22|57|39.0465}}
| {{DEC|−29|37|20.050}}
| 129.81
| 
| heeft een planeet
|-
| Fomalhaut&nbsp;B
| 228
| style="background: {{star-color|K}};" | K5.V
| 6.48
| 7.08
| {{RA|22|56|24.05327}}   
| {{DEC|−31|33|56.0351}}
| 131.42
|
| LET OP! 24.82 lichtjaar
|-
| Fomalhaut&nbsp;C
| 228
| style="background: {{star-color|M}};" | M4.V
| 
| 
| 
| 
| 
|
| LET OP! 24.70 lichtjaar
|-
| rowspan="3" | 162
| rowspan="3" | 25.2
| rowspan="3" | [[LHS 1070]]
| LHS&nbsp;1070&nbsp;A
| 231
| style="background: {{star-color|M}};" | M.V
| 
| 
| 
| 
| 
| 
| 
|-
| LHS&nbsp;1070&nbsp;A
| 231
| style="background: {{star-color|M}};" | M.V
| 
|
|   
| 
| 
|
| 
|-
| LHS&nbsp;1070&nbsp;A
| 231
| style="background: {{star-color|M}};" | M.V
| 
|
|   
| 
| 
|
| 
|-
|}