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Lyn 1:
[[Lêer:Morgan-Keenan spectral classification.png|thumb|350px|Morgan-Keenan-Kellman-spektraaltipes van [[hoofreeks]]sterre.]]
[[Lêer:RedDwarfNASA-hue-shifted.jpg|thumb|240px|’n Kunstenaarsvoorstelling van ’n [[rooi dwerg]]ster, die algemeenste soort ster in die [[Sonnestelsel]] en die [[heelal]].]]
 
Hierdie '''lys van die naaste sterre''' bevat al die sterre en [[bruin dwerg]]sterre binne ’n afstand van 5 [[parsek]] (16,3 [[ligjare]]) van die [[Sonnestelsel]] af, gerangskik volgens toenemende afstand.
Lyn 12:
 
==Lys==
Sterre op die lys hier onder wat met die blote oog van die Aarde af gesien kan word, se skynbare magnitude het ’n ligblou agtergrond. Die [[Sterreklassifikasie|sterklas]] van die sterre en bruin dwerge word volgens die kleur van hul [[spektraaltipe]] aangegee (die kleure is afgelei van konvensionele name vir die spektraaltipes en is nie die stersterre se presiese sigbare kleur nie). Baie bruin sterre is nie volgens hul visuelesigbarelig-spektrum spektruk(m<sub>V</sub>) geklassifiseer nie, maar volgens hul infrarooi-magnitude (m<sub>J</sub>). Van die [[parallaks]]e en afstande is voorlopige waardes.<ref name="RECONS">{{cite journal | last = Research Consortium on Nearby Stars | first = Georgia State University | date = 2007-09-17 | title = The One Hundred Nearest Star Systems | journal = [http://www.chara.gsu.edu/RECONS/ RECONS] | url = http://www.chara.gsu.edu/RECONS/TOP100.posted.htm | accessdate = 2007-11-06}}</ref>
{| style="font-size: 100%; text-align: center;" class="sortable wikitable" border = "1"
! rowspan="2" |#
Lyn 61:
| α&nbsp;Centauri&nbsp;A (HD&nbsp;128620)
| 2
| style="background: #fff4ea;" | [[G V star|G2V]]<ref name=RECONS />
| style="background: lightblue;" | 0,01<ref name=RECONS />
| 4,38<ref name=RECONS />
Lyn 72:
| α&nbsp;Centauri&nbsp;B (HD&nbsp;128621)
| 2
| style="background: #ffd2a1;" | [[K V star|K1V]]<ref name=RECONS />
| style="background: lightblue;" | 1,34<ref name=RECONS />
| 5,71<ref name=RECONS />
Lyn 78:
| {{Dek|−60|50|14}}
|
| hashet oneeen knownbekende planetplaneet<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;Starse Ster]] (BD+04°3561a)
| 4
| style="background: #ffcc6f;" | M4.0Ve
Lyn 91:
|align=left | 546,98(1&nbsp;00)<ref name="Y"/><ref name="H"/>
| 1916
| largestgrootste knownbekende [[proper motioneiebeweging]]<ref name="EEB">{{cite journal
| first=E. E. | last=Barnard
| authorlink=Edward Emerson Barnard | year=1916
Lyn 101:
| rowspan="2" | 3
| rowspan="2" | 6,52(49)
| style="background: #D99058" rowspan="2" | [[WISE 1049-5319]]
| style="background: #D99058"| WISE 1049-5319 A
| 5
| style="background: #E6B2B2;" | [[Brown dwarf|L8]]
| 10,7 J
|
Lyn 116:
}}</ref>
| rowspan="2" | 2013
| rowspan="2" | nearestnaaste knownbekende brownbruin dwarfdwerg
|-size
| style="background: #D99058" | WISE 1049-5319 B
| 5
| style="background: #FFB6C1;" | [[Brown dwarf|L9/T0]]?
|
|
Lyn 126:
| 4
| 7,7825(390)
| colspan="2" | [[Wolf 359|Wolf&nbsp;359]] (CN&nbsp;Leonis)
| 7
| style="background: #ffcc6f;" | M6.0V<ref name=RECONS />
Lyn 139:
| 5
| 8,2905(148)
| colspan="2" | [[Lalande 21185|Lalande&nbsp;21185]] (BD+36°2147)
| 8
| style="background: #ffcc6f;" | M2.0V<ref name=RECONS />
Lyn 155:
| Sirius A
| 9
| style="background: #f8f7ff" | [[A V star|A1V]]<ref name=RECONS />
| style="background: lightblue;" | −1,46<ref name=RECONS />
| 1,42<ref name=RECONS />
Lyn 162:
| rowspan="2" align=left | 380,02(128)<ref name="Y"/><ref name="H"/>
| —
| rowspan="2" | brightesthelderste starster inaan thedie night skynaghemel
|-
| Sirius&nbsp;B
| 9
| style="background:#f8f7ff" | [[White dwarf|DA2]]<ref name=RECONS />
| 8,44<ref name=RECONS />
| 11,34<ref name=RECONS />
Lyn 173:
| rowspan="2" | 7
| rowspan="2" | 8,7280(631)
| rowspan="2" | [[Luyten 726-8|Luyten&nbsp;726-8]]
| Luyten&nbsp;726-8&nbsp;A (BL&nbsp;Ceti)
| 11
Lyn 194:
| 8
| 9,6813(512)
| colspan="2" | [[Ross 154|Ross&nbsp;154]] (V1216&nbsp;Sagittarii)
| 13
| style="background: #ffcc6f;" | M3.5Ve
Lyn 207:
| 9
| 10,322(36)
| colspan="2" | [[Ross 248|Ross&nbsp;248]] (HH&nbsp;Andromedae)
| 14
| style="background: #ffcc6f;" | M5.5Ve
Lyn 220:
| 10
| 10,521
| style="background: #D99058" colspan="2" | [[WISE 1506+7027]]
| 15
| style="background: #FFB6C1;" | [[Brown dwarf|T6]]
| 14,3 J
|
Lyn 233:
| 11
| 10,522(27)
| colspan="2" | [[Epsilon Eridani|Epsilon&nbsp;Eridani]] (BD−09°697)
| 16
| style="background: #ffd2a1;" | [[K V star|K2V]]<ref name=RECONS />
| style="background: lightblue;" | 3,73<ref name=RECONS />
| 6,19<ref name=RECONS />
Lyn 242:
|align=left | 309,99(079)<ref name="Y"/><ref name="H"/>
|
| believedhet toglo have2 two planetsplanete<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 | month=September | year=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: #ffcc6f;" | M1.5Ve
Lyn 259:
| 13
| 10,919(49)
| colspan="2" | [[Ross 128|Ross&nbsp;128]] (FI&nbsp;Virginis)
| 18
| style="background: #ffcc6f;" | M4.0Vn
Lyn 272:
| 14
| 11,208
| style="background: #D99058" colspan="2" | [[WISE 0350-5658]]
| 19
| style="background: #CC99CC;" | [[Brown dwarf#Spectral class Y|Y1]]
| >22,8 J
|
Lyn 285:
| 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
Lyn 313:
| rowspan="2" | 16
| rowspan="2" | 11,402(32)
| rowspan="2" | [[Procyon]]<br>(α&nbsp;Canis&nbsp;Minoris)
| Procyon&nbsp;A
|23
Lyn 327:
| Procyon&nbsp;B
| 23
| style="background: #f8f7ff" | [[White dwarf|DQZ]]<ref name=RECONS />
| 10,70<ref name=RECONS />
| 12,98<ref name=RECONS />
Lyn 334:
| 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: #ffd2a1;" | [[K V star|K5.0V]]<ref name=RECONS /> <!--previous: K3.5Ve-->
| style="background: lightblue;" | 5,21<ref name=RECONS />
| 7,49<ref name=RECONS />
Lyn 344:
| rowspan="2" align=left | 286,04(056)<ref name="Y"/><ref name="H"/>
|
| rowspan="2" | firsteerste starster (othernaas thandie Sun)Son towaarvan havedie itsafstand distancegemeet measuredis<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: #ffd2a1;" | [[K V star|K7.0V]]<ref name=RECONS /> <!--previous: K4.7Ve-->
| style="background: lightblue;" | 6,03<ref name=RECONS />
| 8,31<ref name=RECONS />
Lyn 357:
| 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
Lyn 380:
| 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
Lyn 401:
| 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: #ffd2a1;" | [[K V star|K5Ve]]<ref name=RECONS />
| style="background: lightblue;" | 4,69<ref name=RECONS />
| 6,89<ref name=RECONS />
Lyn 415:
| style="background: #D99058"| Epsilon&nbsp;Indi&nbsp;Ba
| 31
| style="background: #FFB6C1;" | [[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
Lyn 429:
| style="background: #D99058"| Epsilon&nbsp;Indi&nbsp;Bb
| 31
| style="background: #FFB6C1;" | [[Brown dwarf|T6.0V]]
| 13,2 J<ref name="DwarfArchives"/>
|
| AugustAugustus 2003
|-
| 21
| 11,826(129)
| colspan="2" | [[DX Cancri|DX&nbsp;Cancri]] (G&nbsp;51-15)
| 34
| style="background: #ffcc6f;" | M6.5Ve
Lyn 449:
| 22
| 11,887(33)
| colspan="2" | [[Tau Ceti|Tau&nbsp;Ceti]] (BD−16°295)
| 35
| style="background: #fff4ea;" | [[G V star|G8Vp]]<ref name=RECONS />
|style="background: lightblue;" | 3,49<ref name=RECONS />
| 5,68<ref name=RECONS />
Lyn 458:
|align=left | 274,39(076)<ref name="Y"/><ref name="H"/>
|
| naaste G-tipe ster; het glo 5 planete
| nearest G-type single star and believed to have five planets
|-
| 23
| 11,991(57)
| colspan="2" | [[GJ 1061]] (LHS&nbsp;1565)
| 36
| style="background: #ffcc6f;" | M5.5V<ref name=RECONS />
Lyn 469:
| {{RK|03|35|59,7}}
| {{Dek|−44|30|45}}
|align=left | 272,01(130)
|align=left | 272,01(130)<ref name="recent">Systems with their first accurate trigonometric parallaxes measured by RECONS</ref>
|
| <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 (JulyJulie 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
| 12,132(133)
| colspan="2" | [[YZ Ceti|YZ&nbsp;Ceti]] (LHS&nbsp;138)
| 37
| style="background: #ffcc6f;" | M4.5V<ref name=RECONS />
Lyn 488:
| 25
| 12,366(59)
| colspan="2" | [[Luyten's Star|Luyten's&nbsp;Star]]se Ster (BD+05°1668)
| 38
| style="background: #ffcc6f;" | M3.5Vn
Lyn 501:
| 26
| 12,514(129)
| style="background: #D99058" colspan="2" | [[Teegarden's star|Teegarden's&nbsp;star]]se Ster (SO025300.5+165258)
| 39
| style="background: #ffcc6f;" | M6.5V
Lyn 508:
| {{RK|02|53|00,9}}
| {{Dek|+16|52|53}}
|align=left | 260,63(269)<ref name=recent />Stelsels waarvan die eerste akkurate trigonometriese parallakse deur RECONS gemeet is</ref>
| 2003
| <ref name=henry2006 />
Lyn 514:
| rowspan="2" | 27
| rowspan=2 | 12,571(54)
| rowspan="2" | [[SCR 1845-6357|SCR&nbsp;1845-6357]]
| SCR&nbsp;1845-6357&nbsp;A
| 40
Lyn 528:
| style="background: #D99058"| SCR&nbsp;1845-6357&nbsp;B
| 40
| style="background: #FFB6C1;" | [[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 (AugustAugustus 2007), pp. 655&ndash;659. {{doi|10.1051/0004-6361:20077881}}</ref>
| 13.3 J<ref name="DwarfArchives"/>
|
Lyn 537:
| 28
| 12,777(43)
| colspan="2" | [[Kapteyn's Star|Kapteyn's&nbsp;Star]]se Ster (CD−45°1841)
| 42
| style="background: #ffcc6f;" | M1.5V<ref name=RECONS /> <!--previous: sdM0VI-->
Lyn 550:
| 29
| 12,870(57)
| colspan="2" | [[Lacaille 8760|Lacaille&nbsp;8760]] (AX&nbsp;Microscopii)
| 43
| style="background: #ffcc6f;" | M0.0V<ref name=RECONS /> <!--previous: M2Ve-->
Lyn 563:
| 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
Lyn 584:
| 32
| 13,167(82)
| style="background: #D99058" colspan="2" | [[DEN 1048-3956|DEN&nbsp;1048-3956]]
| 47
| style="background: #ffcc6f;" | M8.5V<ref name=RECONS />
Lyn 597:
| 33
| 13,259
| style="background: #D99058" colspan="2" |[[UGPS J072227.51-054031.2|UGPS 0722-05]]
| 48
| style="background: #FFB6C1;" | T9<ref name=RECONS /> <!--previous: M2Ve-->
Lyn 610:
| 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
Lyn 631:
| 35
| 13,820(98)
| colspan="2" | [[Wolf&nbsp;1061]] (Gliese 628, BD−12°4523)
| 51
| style="background: #ffcc6f;" | M3.0V<ref name=RECONS />
Lyn 644:
| 36
| 13,998
| style="background: #D99058" colspan="2" | [[WISE 0410+1502]]
| 52
| style="background: #CC99CC;" | [[Brown dwarf#Spectral class Y|Y0]]
| 19,3 J
|
Lyn 657:
| 37
| 14,066(109)
| colspan="2" | [[Van Maanen's starse Ster]] (Gliese 35, LHS&nbsp;7)
| 53
| style="background: #f8f7ff" | [[White dwarf|DZ7]]<ref name=RECONS />
| 12,38<ref name=RECONS />
| 14,21<ref name=RECONS />
Lyn 670:
| 38
| 14,231(66)
| colspan="2" | [[Gliese &nbsp;1]] (CD−37°15492)
| 54
| style="background: #ffcc6f;" | M3.0V<ref name=RECONS />
Lyn 683:
| rowspan="2" | 39
| 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
| 55
Lyn 704:
| 40
| 14,509(187)
| colspan="2" | [[TZ Arietis|TZ&nbsp;Arietis]] (Gliese 83.1, Luyten&nbsp;1159-16)
| 57
| style="background: #ffcc6f;" | M4.5V<ref name=RECONS />
Lyn 717:
| 41
| 14,793(55)
| colspan="2" | [[Gliese &nbsp;687]] (LHS&nbsp;450, BD+68°946)
| 58
| style="background: #ffcc6f;" | M3.0V<ref name=RECONS />
Lyn 730:
| 42
| 14,805(242)
| colspan="2" | [[LHS 292|LHS&nbsp;292]] (LP&nbsp;731-58)
| 59
| style="background: #ffcc6f;" | M6.5V<ref name=RECONS />
Lyn 743:
| 43
| 14,809(107)
| colspan="2" | [[Gliese &nbsp;674]] (LHS&nbsp;449)
| 60
| style="background: #ffcc6f;" | M3.0V<ref name=RECONS />
Lyn 752:
|align=left | 220,25(159)<ref name="Y"/><ref name="H"/>
|
| hashet oneeen knownbekende planetplaneet<ref>http://exoplanet.eu/star.php?st=GJ+674</ref>
|-
| rowspan="3" | 44
| rowspan="3" | 14,812(67)
| rowspan="3" | [[GJ &nbsp;1245]]
| GJ&nbsp;1245&nbsp;A
| 61
Lyn 788:
| 45
| 15,060(140)
| colspan="2" | [[Gliese &nbsp;440]] (WD&nbsp;1142-645)
| 64
| style="background: #f8f7ff" | [[White dwarf|DQ6]]<ref name=RECONS />
| 11,50<ref name=RECONS />
| 13,18<ref name=RECONS />
Lyn 801:
| 46
| 15,313(259)
| colspan="2" | [[GJ &nbsp;1002]]
| 65
| style="background: #ffcc6f;" | M5.5V<ref name=RECONS />
Lyn 823:
|align=left | 212,59(196)<ref name="Y"/><ref name="H"/>
|
| hashet four4 knownbekende planetsplanete<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| month=July| year=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: #ffcc6f;" | M5.5V<ref name=RECONS />
Lyn 840:
| 49
| 15,757
| style="background: #D99058" colspan="2" | [[WISE 1405+5534]]
| 68
| style="background: #CC99CC;" | [[Brown dwarf#Spectral class Y|Y0p]]
| 20,09 J
|
Lyn 853:
| rowspan="2" | 50
| rowspan="2" | 15,832(83)
| rowspan="2" | [[Gliese 412]]
| Gliese 412&nbsp;A
| 69
Lyn 876:
| 51
| 15,848(52)
| colspan="2" | [[Groombridge 1618|Groombridge&nbsp;1618]] (Gliese 380)
| 71
| style="background: #ffd2a1;" | [[K V star|K7.0V]]<ref name=RECONS />
| 6,59<ref name=RECONS />
| 8,16<ref name=RECONS />
Lyn 889:
| 52
| 15,942(218)
| colspan="2" | [[AD Leonis|AD&nbsp;Leonis]]
| 72
| style="background: #ffcc6f;" | M3.0V<ref name=RECONS />
Lyn 902:
| 53
| 16,067
| style="background: #D99058" colspan="2" | [[DENIS J081730.0-615520]]
| 73
| style="background: #FFB6C1;" | [[BrownBruin dwarf#Spectral class Tdwerg|T6]]
|
|
Lyn 915:
| 54
| 16,085(105)
| colspan="2" | [[Gliese 832]]
| 74
| style="background: #ffcc6f;" | M3.0V<ref name=RECONS />
Lyn 924:
|align=left | 202,78(132)<ref name="Y"/><ref name="H"/>
|
| hashet one1 knownbekende planetplaneet<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>
|-
| 55
| 16,195(338)
| style="background: #D99058" colspan="2" | [[LP 944-020|LP&nbsp;944-020]]
| 75
| style="background: #ffcc6f;" | M9.0V<ref name=RECONS />
Lyn 941:
| 56
| 16,197(313)
| style="background: #D99058" colspan="2" | [[DEN 0255-4700|DEN&nbsp;0255-4700]]
| 76
| style="background: #E6B2B2;" | [[BrownBruin dwarfdwerg|L7.5V]]<ref name=RECONS />
| 22,92<ref name=RECONS />
| 24,44<ref name=RECONS />
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