{{위키데이터 속성 추적}}
[[파일:RedDwarfNASA.jpg|250px|오른쪽|섬네일|우리 [[태양계]]에서 가까운 별들 중 대다수를 차지하는 것들은 [[적색 왜성]]이다.]]
아래 표의 '''가까운 항성 목록'''은 [[지구]]로부터 5파섹(16.308광년) 이내에 있는 [[항성]]들을 가까운 것으로부터 순서대로 정렬한 것이다. 이 거리 내에 있는 [[항성계]]는 50개이며, 항성은 65개(우리 [[태양]]을 포함하여), [[갈색 왜성]](발견된 것)은 4개가 있다.

맨눈으로 볼 수 없는<ref>{{저널 인용
 | 성=Weaver | 이름=Harold F.
 | 제목=The Visibility of Stars Without Optical Aid
 | 저널=Publications of the Astronomical Society of the Pacific
 | 연도=1947 | volume=59 | issue=350 | 쪽=232–243
 | url=http://adsabs.harvard.edu/abs/1947PASP...59..232W}}</ref> 항성들은 <span style="background: lightblue">청록색</span>으로 표시했다.(겉보기 등급이 6.5보다 큰 경우임.) 분광형 박스의 배경색은 실제 사람이 눈으로 보았을 때의 색깔이 아니라, 학문적으로 정해 놓은 색채로 실제와는 차이가 있다.

우리 태양은 65개의 항성들 중 네 번째로 밝은 별이다.

일부 시차 및 거리는 [[RECONS]]에서 측정한 자료이다.<ref name="RECONS">{{저널 인용 | 성 = Research Consortium on Nearby Stars | 이름 = Georgia State University | 연도 = 2007-09-17 | 제목 = The One Hundred Nearest Star Systems | 저널 = RECONS | url = http://www.chara.gsu.edu/RECONS/TOP100.posted.htm |  = 2007-11-06 | 확인날짜 = 2012-05-13 | 보존url = https://web.archive.org/web/20120513202710/http://www.chara.gsu.edu/RECONS/TOP100.posted.htm | 보존날짜 = 2012-05-13 | url-status = dead }}</ref>

== 목록 ==
해당 문서는 [[주계열]] 문서의 항성 매개변수 항목에 따라 작성되었다.
{| style="font-size: 100%; text-align: center;" class="wikitable" border = "1"
! rowspan="2" |#
! colspan="2" |<small>명칭</small>
! rowspan="2" |<small>[[항성 분류|분광형]]</small>
! rowspan="2" |<small>[[겉보기등급|''m'']]<sub>[[존슨의 UBV 시스템|''V'']]</sub></small>
! rowspan="2" |<small>[[절대등급|''M'']]<sub>[[존슨의 UBV 시스템|''V'']]</sub></small>
! rowspan="2" |<small>[[유효온도|''T<sub>eff</sub>'']]<br />[[켈빈|K]][[오차 범위|(±err)]]</small>
! style="background: #FFC" colspan="2" |<small>[[역기점]] J2000.0</small>
! rowspan="2" |<small>[[시차]]<ref name="RECONS"/><ref name=plxfn>RECONS가 보유하고 있는 시차값은 RECONS 프로그램 측정 도구를 이용하여 도출한 것이다.</ref><br />[[초 (각도)|초각]][[오차 범위|(±err)]]</small>
! rowspan="2" |<small>[[거리]]<ref name=distfn>시차로 구한 값임.</ref><br />[[광년]][[오차 범위|(±err)]]</small>
! rowspan="2" |<small>[[#참고 문헌|참고<br />문헌]]</small>
|-
!<small>[[행성계]] 또는 [[항성계]]</small>
!<small>[[항성]]</small>
!<small>[[적경]]<ref name=RECONS /></small>
!<small>[[적위]]<ref name=RECONS /></small>
|-
|style="background: #FFFFFF;" |
|style="background: #FFFFFF;" | [[태양계]]
|style="background: #FFFFFF;" | [[태양]]
| style="background: #f0f5ff;" | [[G형 주계열성|G2V]]<ref name=RECONS />
| −26.72<ref name=RECONS />
| 4.85<ref name=RECONS />
| align=left | &nbsp;5,778<ref>[http://nssdc.gsfc.nasa.gov/planetary/factsheet/sunfact.html Sun Fact Sheet], NASA.</ref>
| {{RA|0|0|0}} ~ {{RA|23|59|59}}
| {{DEC|-90|0}} ~ {{DEC|+90|0}}
| 180°
| 0.0000158(3)<br />또는 약<br /> [[광분|8.317광분]], 또는 1[[천문단위|AU]]
|
|-
| style="background: #FFFFFF;" rowspan="3" | 1
| style="background: #FFFFFF;" rowspan="3" | [[센타우루스자리 알파|알파 센타우리]]<br />(리길 켄타우루스, 톨리만)
| style="background: lightblue;" | [[센타우루스자리 프록시마|프록시마 센타우리]] (센타우루스자리 V645)
| style="background: #ffa040;" | [[적색 왜성|M5.5Ve]]
| 11.09<ref name=RECONS />
| 15.53<ref name=RECONS />
|  align=left | &nbsp;3,040<ref name="ESO2003" />
| {{RA|14|29|43.0}}
| {{DEC|−62|40|46}}
| align=left | 0.768&nbsp;87(0&nbsp;29)″<ref name="Y">General Catalogue of Trigonometric Parallaxes.</ref><ref name="H">[[히파르코스 성표]].</ref>
| 4.2421(16)
|<ref name="B">Burgasser et al. 2000</ref>
|-
|style="background: #FFFFFF;" | 센타우루스자리 알파 A (HD 128620)
| style="background: #f0f5ff;" | [[G형 주계열성|G2V]]<ref name=RECONS />
| 0.01<ref name=RECONS />
| 4.38<ref name=RECONS />
| align=left | &nbsp;5,790<ref name="ESO2003">{{뉴스 인용
 |저자       = Kervella, Pierre; Thevenin, Frederic
 |제목       = A Family Portrait of the Alpha Centauri System: VLT Interferometer Studies the Nearest Stars
 |작품       = ESO Press Release 05/03
 |출판사    = ESO
 |연도 = 2003-03-15
 |url          = http://www.eso.org/public/outreach/press-rel/pr-2003/pr-05-03.html
 |확인날짜 = 2009-12-06
 |보존url    = https://web.archive.org/web/20080616125016/http://www.eso.org/public/outreach/press-rel/pr-2003/pr-05-03.html
 |보존날짜 = 2008-06-16
 |url-status = dead
}}</ref>
| {{RA|14|39|36.5}}
| {{DEC|−60|50|02}}
| rowspan="2" align=left | 0.747&nbsp;23(1&nbsp;17)″<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''' (1999-01), pp. 121–140.</ref>
| rowspan="2" | 4.3650(68)
| rowspan="2" | 
|-
|style="background: #FFFFFF;" | 센타우루스자리 알파 B (HD 128621)
| style="background: #fffeed;" | [[K형 주계열성|K0V]]<ref name=RECONS />
| 1.34<ref name=RECONS />
| 5.71<ref name=RECONS />
| align=left | &nbsp;5,260<ref name="ESO2003" />
| {{RA|14|39|35.1}}
| {{DEC|−60|50|14}}
|-
| style="background: lightblue;" | 2
| colspan="2" style="background: lightblue;" | [[바너드 별]] (BD+04°3561a)
| style="background: #ffa040;" | M4.0Ve
| 9.53<ref name=RECONS />
| 13.22<ref name=RECONS />
| align=left | &nbsp;3,134(102)<ref>[http://adsabs.harvard.edu/abs/2004AJ....127.2909D Barnard's Star and the M Dwarf Temperature Scale], P. C. Dawson and M. M. de Robertis, ''The Astronomical Journal'' '''127''', #5 (May 2004), pp. 2909–2914. {{doi|10.1086/383289}}</ref>
| {{RA|17|57|48.5}}
| {{DEC|+04|41|36}}
| align=left | 0.546&nbsp;98(1&nbsp;00)″<ref name="Y"/><ref name="H"/>
| 5.9630(109)
| 
|-
| style="background: lightblue;" | 3
| colspan="2" style="background: lightblue;" | [[볼프 359]] (사자자리 CN)
| style="background: #ffa040;" | M6.0V<ref name=RECONS />
| 13.44<ref name=RECONS />
| 16.55<ref name=RECONS />
| align=left | &nbsp;2,800(100)<ref name="aaa447">{{저널 인용
 | 저자=Ya. V. Pavlenko, H. R. A. Jones, Yu. Lyubchik, J. Tennyson, and D. J. Pinfield
 | 제목=Spectral energy distribution for GJ406
 | 저널=Astronomy and Astrophysics
 | 연도=2006 | 발행월=02 | volume=447 | issue=2 | 쪽=709–717
 | url=http://adsabs.harvard.edu/abs/2006A&A...447..709P
 | doi=10.1051/0004-6361:20052979 }}</ref>
| {{RA|10|56|29.2}}
| {{DEC|+07|00|53}}
|align=left |  0.419&nbsp;10(2&nbsp;10)″<ref name="Y" />
| 7.7825(390)
| 
|-
| style="background: lightblue;" | 4
| colspan="2" style="background: lightblue;" | [[랄랑드 21185]] (BD+36°2147)
| style="background: #ffa040;" | M2.0V<ref name=RECONS />
| 7.47<ref name=RECONS />
| 10.44<ref name=RECONS />
| align=left | &nbsp;3,400<ref>[http://adsabs.harvard.edu/abs/2002A&A...396..967P Carbon monoxide bands in M dwarfs], Y. V. Pavlenko and H. R. A. Jones, ''Astronomy and Astrophysics'' '''396''' (December 2002), pp. 967–975.  {{doi|10.1051/0004-6361:20021454}}</ref>
| {{RA|11|03|20.2}}
| {{DEC|+35|58|12}}
| align=left | 0.393&nbsp;42(0&nbsp;70)″<ref name="Y"/><ref name="H"/>
| 8.2905(148)
| 
|-
| rowspan="2" style="background: #FFFFFF;"  | 5
| rowspan="2" style="background: #FFFFFF;"  | [[시리우스]]<br />(큰개자리 알파)
|style="background: FFFFFF;" | 시리우스 A
| style="background: #7ca5ff;" | [[A형 주계열성|A1V]]<ref name=RECONS />
| −1.43<ref name=RECONS />
| 1.47<ref name=RECONS />
| align=left | &nbsp;9,940(210)<ref>[http://adsabs.harvard.edu/abs/2004IAUS..224....1A The physical properties of normal A stars], Saul J. Adelman, pp. 1–11, ''The A-Star Puzzle'', ''Proceedings of the International Astronomical Union'', edited by J. Zverko, J. Ziznovsky, S. J. Adelman, and W. W. Weiss, Cambridge, UK: Cambridge University Press, 2004. {{doi|10.1017/S1743921304004314}}</ref>
| rowspan="2" | {{RA|06|45|08.9}}
| rowspan="2" | {{DEC|−16|42|58}}
| rowspan="2" align=left | 0.380&nbsp;02(1&nbsp;28)″<ref name="Y"/><ref name="H"/>
| rowspan="2" | 8.5828(289)
| rowspan="2" | 
|-
| style="background: lightblue;" | 시리우스 B
| style="background: F0F0F0" | [[백색 왜성|DA2]]<ref name=RECONS />
| 8.44<ref name=RECONS />
| 11.34<ref name=RECONS />
| align=left | 25,000(200)<ref>[http://adsabs.harvard.edu/abs/2005ApJ...630L..69L The Age and Progenitor Mass of Sirius B], James Liebert, Patrick A. Young, David Arnett, J.B. Holberg, and Kurtis A. Williams, ''The Astrophysical Journal'' '''630''', #1 (2005년 9월), pp. L69–L72.</ref>
|-
| rowspan="2" style="background: lightblue;" | 6
| rowspan="2" style="background: lightblue;" | [[루이텐 726-8]]
| style="background: lightblue;" | 루이텐 726-8&nbsp;A (고래자리 BL)
| style="background: #ffa040;" | M5.5Ve
| 12.54<ref name=RECONS />
| 15.40<ref name=RECONS />
| align=left | &nbsp;2,670
| rowspan="2" | {{RA|01|39|01.3}}
| rowspan="2" | {{DEC|−17|57|01}}
| rowspan="2" align=left  | 0.373&nbsp;70(2&nbsp;70)″<ref name="Y"/>
| rowspan="2" | 8.7280(631)
| rowspan="2" | 
|-
| style="background: lightblue;" | 루이텐 726-8&nbsp;B (고래자리 UV)
| style="background: #ffa040;" | M6.0Ve
| 12.99<ref name=RECONS />
| 15.85<ref name=RECONS />
| align=left | ~2,600
|-
| style="background: lightblue;" | 7
| colspan="2" style="background: lightblue;" | [[로스 154]] (궁수자리 V1216)
| style="background: #ffa040;" | M3.5Ve
| 10.43<ref name=RECONS />
| 13.07<ref name=RECONS />
| align=left | &nbsp;2,700
| {{RA|18|49|49.4}}
| {{DEC|−23|50|10}}
| align=left | 0.336&nbsp;90(1&nbsp;78)″<ref name="Y"/><ref name="H"/>
| 9.6813(512)
| 
|-
| style="background: lightblue;" | 8
| colspan="2" style="background: lightblue;" | [[로스 248]] (안드로메다자리 HH)
| style="background: #ffa040;" | M5.5Ve
| 12.29<ref name=RECONS />
| 14.79<ref name=RECONS />
| ''?''
| {{RA|23|41|54.7}}
| {{DEC|+44|10|30}}
| align=left | 0.316&nbsp;00(1&nbsp;10)″<ref name="Y"/>
| 10.322(36)
| 
|-
| 9
| colspan="2" | [[에리다누스자리 엡실론]] (BD−09°697)
| style="background: #fff4af;" | [[K형 주계열성|K2V]]<ref name=RECONS />
| 3.73<ref name=RECONS />
| 6.19<ref name=RECONS />
| align=left | &nbsp;5,100
| {{RA|03|32|55.8}}
| {{DEC|−09|27|30}}
|align=left |  0.309&nbsp;99(0&nbsp;79)″<ref name="Y"/><ref name="H"/>
| 10.522(27)
| 
|-
| style="background: lightblue;" | 10
| colspan="2" style="background: lightblue;" | [[라카유 9352]] (CD−36°15693)
| style="background: #ffa040;" | M1.5Ve
| 7.34<ref name=RECONS />
| 9.75<ref name=RECONS />
| align=left | &nbsp;3,340
| {{RA|23|05|52.0}}
| {{DEC|−35|51|11}}
| align=left | 0.303&nbsp;64(0&nbsp;87)″<ref name="Y"/><ref name="H"/>
| 10.742(31)
| 
|-
| style="background: lightblue;" | 11
| colspan="2" style="background: lightblue;" | [[로스 128]] (처녀자리 FI)
| style="background: #ffa040;" | M4.0Vn
| 11.13<ref name=RECONS />
| 13.51<ref name=RECONS />
| align=left | &nbsp;2,800
| {{RA|11|47|44.4}}
| {{DEC|+00|48|16}}
| align=left | 0.298&nbsp;72(1&nbsp;35)″<ref name="Y"/><ref name="H"/>
| 10.919(49)
| 
|-
| rowspan="3" style="background: lightblue;" | 12
| rowspan="3" style="background: lightblue;" | [[물병자리 EZ]]<br />(글리제 866, 루이텐 789-6)
| style="background: lightblue;" | 물병자리 EZ A
| style="background: #ffa040;" | M5.0Ve
| 13.33<ref name=RECONS />
| 15.64<ref name=RECONS />
| ''?''
| rowspan="3" | {{RA|22|38|33.4}}
| rowspan="3" | {{DEC|−15|18|07}}
| rowspan="3" align=left | 0.289&nbsp;50(4&nbsp;40)″<ref name="Y"/>
| rowspan="3" | 11.266(171)
| rowspan="3" | 
|-
| style="background: lightblue;" | 물병자리 EZ B
| style="background: #ffa040;" | M?
| 13.27<ref name=RECONS />
| 15.58<ref name=RECONS />
| ''?''
|-
| style="background: lightblue;" | 물병자리 EZ C
| style="background: #ffa040;" | M?
| 14.03<ref name=RECONS />
| 16.34<ref name=RECONS />
| ''?''
|-
| rowspan="2" | 13
| rowspan="2" | [[프로키온]]<br />(작은개자리 알파)
| 프로키온 A
| style="background: #d4e4ff" | F5V-IV<ref name=RECONS />
| 0.38<ref name=RECONS />
| 2.66<ref name=RECONS />
| align=left | &nbsp;6,650
| rowspan="2" | {{RA|07|39|18.1}}
| rowspan="2" | {{DEC|+05|13|30}}
| rowspan="2" align=left | 0.286&nbsp;05(0&nbsp;81)″<ref name="Y"/><ref name="H"/>
| rowspan="2" | 11.402(32)
| rowspan="2" | 
|-
| style="background: lightblue;" | 프로키온 B
| style="background: #F0F0F0" | [[백색 왜성|DA]]<ref name=RECONS />
| 10.70<ref name=RECONS />
| 12.98<ref name=RECONS />
| align=left | &nbsp;9,700
|-
| rowspan="2" | 14
| rowspan="2" | [[백조자리 61]]
| 백조자리 61 A (BD+38°4343)
| style="background: #ffe46f;" | [[K형 주계열성|K5.0V]]<ref name=RECONS />
| 5.21<ref name=RECONS />
| 7.49<ref name=RECONS />
| align=left | &nbsp;4,640
| {{RA|21|06|53.9}}
| {{DEC|+38|44|58}}
| rowspan="2" align=left | 0.286&nbsp;04(0&nbsp;56)″<ref name="Y"/><ref name="H"/>
| rowspan="2" | 11.403(22)
| rowspan="2" | 
|-
| 백조자리 61 B (BD+38°4344)
| style="background: #ffe46f;" | [[K형 주계열성|K7.0V]]<ref name=RECONS />
| 6.03<ref name=RECONS />
| 8.31<ref name=RECONS />
| align=left | &nbsp;4,440
| {{RA|21|06|55.3}}
| {{DEC|+38|44|31}}
|-
| rowspan="2" style="background: lightblue;" | 15
| rowspan="2" style="background: lightblue;" | [[스트루베 2398]]<br />(글리제 725, BD+59°1915)
| style="background: lightblue;" | 스트루베 2398 A (HD 173739)
| style="background: #ffa040;" | 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 | 0.283&nbsp;00(1&nbsp;69)″<ref name="Y"/><ref name="H"/>
| rowspan="2" | 11.525(69)
| rowspan="2" | 
|-
| style="background: lightblue;" | 스트루베 2398 B (HD 173740)
| style="background: #ffa040;" | M3.5V<ref name=RECONS />
| 9.69<ref name=RECONS />
| 11.95<ref name=RECONS />
| ''?''
| {{RA|18|42|46.9}}
| {{DEC|+59|37|37}}
|-
| rowspan="2" style="background: lightblue;" | 16
| rowspan="2" style="background: lightblue;" | [[그룸브리지 34|그룸브리지&nbsp;34]]<br />(글리제 15)
| style="background: lightblue;" | 그룸브리지&nbsp;34&nbsp;A (안드로메다자리 GX)
| style="background: #ffa040;" | M1.5V<ref name=RECONS />
| 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 | 0.280&nbsp;59(0&nbsp;95)″<ref name="Y"/><ref name="H"/>
| rowspan="2" | 11.624(39)
| rowspan="2" | 
|-
| style="background: lightblue;" | 그룸브리지&nbsp;34&nbsp;B (안드로메다자리 GQ)
| style="background: #ffa040;" | M3.5V<ref name=RECONS />
| 11.06<ref name=RECONS />
| 13.30<ref name=RECONS />
| ''?''
|-
| rowspan="3" | 17
| rowspan="3" | [[인디언자리 엡실론]]<br />(CPD−57°10015)
| 인디언자리 엡실론 A
| style="background: #ffe46f;" | [[K형 주계열성|K5Ve]]<ref name=RECONS />
| 4.69<ref name=RECONS />
| 6.89<ref name=RECONS />
| align=left | &nbsp;4,280
| {{RA|22|03|21.7}}
| {{DEC|−56|47|10}}
| rowspan="3" align=left  | 0.275&nbsp;84(0&nbsp;69)″<ref name="Y"/><ref name="H"/>
| rowspan="3" | 11.824(30)
| rowspan="3" | 
|-
| style="background: lightblue;" | 인디언자리 엡실론 Ba
| style="background: #a00000;" | [[갈색 왜성|T1.0V]]
| >23
| >25
| align=left | &nbsp;1,280
| rowspan="2" | {{RA|22|04|10.5}}
| rowspan="2" | {{DEC|−56|46|58}}
|-
| style="background: lightblue;" | 인디언자리 엡실론 Bb
| style="background: #700000;" | [[갈색 왜성|T6.0V]]
| >23
| >25
| align=left | &nbsp;&nbsp;&nbsp;850
|-
| style="background: lightblue;" | 18
| colspan="2" style="background: lightblue;" | [[게자리 DX]] (G&nbsp;51-15)
| style="background: #ffa040;" | M6.5Ve
| 14.78<ref name=RECONS />
| 16.98<ref name=RECONS />
| ''?''
| {{RA|08|29|49.5}}
| {{DEC|+26|46|37}}
| align=left | 0.275&nbsp;80(3&nbsp;00)″<ref name=Y />
| 11.826(129)
| 
|-
| 19
| colspan="2" | [[고래자리 타우]] (BD−16°295)
| style="background: #ffffff;" | [[G형 주계열성|G8Vp]]<ref name=RECONS />
| 3.49<ref name=RECONS />
| 5.68<ref name=RECONS />
| align=left | &nbsp;5,344
| {{RA|01|44|04.1}}
| {{DEC|−15|56|15}}
| align=left |  0.274&nbsp;39(0&nbsp;76)″<ref name="Y"/><ref name="H"/>
| 11.887(33)
| 
|-
| style="background: lightblue;" | 20
| colspan="2" style="background: lightblue;" | [[글리제 1061]] (LHS&nbsp;1565)
| style="background: #ffa040;" | 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 | 0.272&nbsp;01(1&nbsp;30)″<ref name="recent">RECONS가 이 항성계의 시차를 삼각법을 이용하여 최초로 정확하게 쟀다.</ref>
| 11.991(57)
|<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. 388–395.  {{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. 2360–2371.  {{doi|10.1086/508233}}</ref>
|-
| style="background: lightblue;" | 21
| colspan="2" style="background: lightblue;" | [[고래자리 YZ]] (LHS&nbsp;138)
| style="background: #ffa040;" | 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 | 0.268&nbsp;84(2&nbsp;95)″<ref name="Y"/><ref name="H"/>
| 12.132(133)
| 
|-
| style="background: lightblue;" | 22
| colspan="2" style="background: lightblue;" | [[루이텐의 별]] (BD+05°1668)
| style="background: #ffa040;" | M3.5Vn
| 9.86<ref name=RECONS />
| 11.97<ref name=RECONS />
| ''?''
| {{RA|07|27|24.5}}
| {{DEC|+05|13|33}}
| align=left | 0.263&nbsp;76(1&nbsp;25)″<ref name="Y"/><ref name="H"/>
| 12.366(59)
| 
|-
| style="background: lightblue;" | 23
| colspan="2" style="background: lightblue;" | [[티가든의 별]] (SO025300.5+165258)
| style="background: #ffa040;" | M6.5V
| 15.14<ref name=RECONS />
| 17.22<ref name=RECONS />
| ''?''
| {{RA|02|53|00.9}}
| {{DEC|+16|52|53}}
| align=left | 0.260&nbsp;63(2&nbsp;69)″<ref name=recent />
| 12.514(129)
|<ref name=henry2006 />
|-
| rowspan="2" style="background: lightblue;" | 24
| rowspan="2" style="background: lightblue;" | [[SCR 1845-6357]]
| style="background: lightblue;" | SCR&nbsp;1845-6357&nbsp;A
| style="background: #ffa040;" | M8.5V<ref name=RECONS />
| 17.39
| 19.41
| ''?''
|  {{RA|18|45|05.3}}
|  {{DEC|−63|57|48}}
| rowspan=2 align=left | 0.259&nbsp;45(1&nbsp;11)″<ref name="recent"/>
| rowspan=2 | 12.571(54)
| rowspan=2 |<ref name=henry2006 />
|-
| style="background: lightblue;" | SCR&nbsp;1845-6357&nbsp;B
| style="background: #700000;" | [[갈색 왜성|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. 655–659. {{doi|10.1051/0004-6361:20077881}}</ref>
| ''?''
| ''?''
| align=left | &nbsp;&nbsp;&nbsp;950<ref name=nearmt />
|  {{RA|18|45|02.6}}
|  {{DEC|−63|57|52}}
|-
| style="background: lightblue;" | 25
| colspan="2" style="background: lightblue;" | [[카프타인의 별]] (CD−45°1841)
| style="background: #ffa040;" | M1.5V<ref name=RECONS />
| 8.84<ref name=RECONS />
| 10.87<ref name=RECONS />
| align=left | &nbsp;3,800
| {{RA|05|11|40.6}}
| {{DEC|−45|01|06}}
| align=left | 0.255&nbsp;27(0&nbsp;86)″<ref name="Y"/><ref name="H"/>
| 12.777(43)
| 
|-
| style="background: lightblue;" | 26
| colspan="2" style="background: lightblue;" | [[라카유 8760]] (현미경자리 AX)
| style="background: #ffa040;" | M0.0V<ref name=RECONS />
| 6.67<ref name=RECONS />
| 8.69<ref name=RECONS />
| align=left | &nbsp;3,340
| {{RA|21|17|15.3}}
| {{DEC|−38|52|03}}
| align=left | 0.253&nbsp;43(1&nbsp;12)″<ref name="Y"/><ref name="H"/>
| 12.870(57)
| 
|-
| rowspan="2" style="background: lightblue;" | 27
| rowspan="2" style="background: lightblue;" | [[크루거 60]]<br />(BD+56°2783)
| style="background: lightblue;" | 크루거 60 A
| style="background: #ffa040;" | M3.0V<ref name=RECONS />
| 9.79<ref name=RECONS />
| 11.76<ref name=RECONS />
| align=left | &nbsp;3,180
| rowspan="2" | {{RA|22|27|59.5}}
| rowspan="2" | {{DEC|+57|41|45}}
| rowspan="2" align=left | 0.248&nbsp;06(1&nbsp;39)″<ref name="Y"/><ref name="S"/>
| rowspan="2" | 13.149(74)
| rowspan="2" | 
|-
| style="background: lightblue;" | 크루거 60 B (세페우스자리 DO)
| style="background: #ffa040;" | M4.0V<ref name=RECONS />
| 11.41<ref name=RECONS />
| 13.38<ref name=RECONS />
| align=left | &nbsp;2,890
|-
| style="background: lightblue;" | 28
| colspan="2" style="background: lightblue;" | [[DEN 1048-3956]]
| style="background: #ffa040;" | 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 | 0.247&nbsp;71(1&nbsp;55)″<ref name="recent"/>
| 13.167(82)
|<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. 1954–1967.  {{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—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. 337–349. {{doi|10.1086/430473}}</ref>
|-
| rowspan="2" style="background: lightblue;" | 29
| rowspan="2" style="background: lightblue;" | [[로스 614]]<br />(외뿔소자리 V577, 글리제 234)
| style="background: lightblue;" | 로스 614A (LHS 1849)
| style="background: #ffa040;" | 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 | 0.244&nbsp;34(2&nbsp;01)″<ref name="Y"/><ref name="S"/>
| rowspan="2" | 13.349(110)
| rowspan="2" | 
|-
| style="background: lightblue;" | 로스 614B (LHS 1850)
| style="background: #ffa040;" | M5.5V
| 14.23<ref name=RECONS />
| 16.17<ref name=RECONS />
| ''?''
|-
| style="background: lightblue;" | 30
| colspan="2" style="background: lightblue;" | [[글리제 628]] (울프 1061, BD−12°4523)
| style="background: #ffa040;" | 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 | 0.236&nbsp;01(1&nbsp;67)″<ref name="Y"/><ref name="H"/>
| 13.820(98)
| 
|-
| style="background: lightblue;" | 31
| colspan="2" style="background: lightblue;" | [[반 마넨의 별]] (글리제 35, LHS&nbsp;7)
| style="background: #F0F0F0" | [[백색 왜성|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 | 0.231&nbsp;88(1&nbsp;79)″<ref name="Y"/><ref name="H"/>
| 14.066(109)
| 
|-
| style="background: lightblue;" | 32
| colspan="2" style="background: lightblue;" | [[글리제 1]] (CD−37°15492)
| style="background: #ffa040;" | M3.0V<ref name=RECONS />
| 8.55<ref name=RECONS />
| 10.35<ref name=RECONS />
| ''?''
| {{RA|00|05|24.4}}
| {{DEC|−37|21|27}}
| align=left | 0.229&nbsp;20(1&nbsp;07)″<ref name="Y"/><ref name="H"/>
| 14.231(66)
| 
|-
| rowspan="2" style="background: lightblue;" | 33
| rowspan="2" style="background: lightblue;" | [[울프 424]]<br />(처녀자리 FL, LHS 333, 글리제 473)
| style="background: lightblue;" | 울프 424&nbsp;A
| style="background: #ffa040;" | 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 | 0.227&nbsp;90(4&nbsp;60)″<ref name="Y"/>
| rowspan="2" | 14.312(289)
| rowspan="2" |
|-
| style="background: lightblue;" | 울프 424&nbsp;B
| style="background: #ffa040;" | M7Ve
| 13.17<ref name=RECONS />
| 14.96<ref name=RECONS />
| ''?''
|-
| style="background: lightblue;" | 34
| colspan="2" style="background: lightblue;" | [[양자리 TZ]] (글리제 83.1, 루이텐 1159-16)
| style="background: #ffa040;" | 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 | 0.224&nbsp;80(2&nbsp;90)″<ref name="Y"/>
| 14.509(187)
| 
|-
| style="background: lightblue;" | 35
| colspan="2" style="background: lightblue;" | [[글리제 687]] (LHS&nbsp;450, BD+68°946)
| style="background: #ffa040;" | 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 | 0.220&nbsp;49(0&nbsp;82)″<ref name="Y"/><ref name="H"/>
| 14.793(55)
| 
|-
| style="background: lightblue;" | 36
| colspan="2" style="background: lightblue;" | [[LHS 292]] (LP&nbsp;731-58)
| style="background: #ffa040;" | 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 | 0.220&nbsp;30(3&nbsp;60)″<ref name="Y"/>
| 14.805(242)
| 
|-
| style="background: lightblue;" | 37
| colspan="2" style="background: lightblue;" | [[글리제 674]] (LHS&nbsp;449)
| style="background: #ffa040;" | 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 | 0.220&nbsp;25(1&nbsp;59)″<ref name="Y"/><ref name="H"/>
| 14.809(107)
| 
|-
| rowspan="3" style="background: lightblue;" | 38
| rowspan="3" style="background: lightblue;" | [[글리제 1245]]
| style="background: lightblue;" | 글리제 1245&nbsp;A
| style="background: #ffa040;" | 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 | 0.220&nbsp;20(1&nbsp;00)″<ref name="Y"/>
| rowspan="3" | 14.812(67)
| rowspan="3" | 
|-
| style="background: lightblue;" | 글리제 1245&nbsp;B
| style="background: #ffa040;" | M6.0V<ref name=RECONS />
| 14.01<ref name=RECONS />
| 15.72<ref name=RECONS />
| ''?''
| {{RA|19|53|55.2}}
| {{DEC|+44|24|56}}
|-
| style="background: lightblue;" | 글리제 1245&nbsp;C
| style="background: #ffa040;" | M?
| 16.75<ref name=RECONS />
| 18.46<ref name=RECONS />
| ''?''
| {{RA|19|53|54.2}}
| {{DEC|+44|24|55}}
|-
| style="background: lightblue;" | 39
| colspan="2" style="background: lightblue;" | [[글리제 440]] (WD&nbsp;1142-645)
| style="background: #F0F0F0" | [[백색 왜성|DQ6]]<ref name=RECONS />
| 11.50<ref name=RECONS />
| 13.18<ref name=RECONS />
| align=left | &nbsp;7,500
| {{RA|11|45|42.9}}
| {{DEC|−64|50|29}}
|align=left |  0.216&nbsp;57(2&nbsp;01)″<ref name="Y"/><ref name="H"/>
| 15.060(140)
| 
|-
| style="background: lightblue;" | 40
| colspan="2" style="background: lightblue;" | [[글리제 1002]]
| style="background: #ffa040;" | 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 | 0.213&nbsp;00(3&nbsp;60)″<ref name="Y"/>
| 15.313(259)
| 
|-
| style="background: lightblue;" | 41
| colspan="2" style="background: lightblue;" | [[글리제 876|로스 780]] (글리제 876)
| style="background: #ffa040;" | M3.5V<ref name=RECONS />
| 10.17<ref name=RECONS />
| 11.81<ref name=RECONS />
| align=left | &nbsp;3,480
| {{RA|22|53|16.7}}
| {{DEC|−14|15|49}}
| align=left | 0.212&nbsp;59(1&nbsp;96)″<ref name="Y"/><ref name="H"/>
| 15.342(141)
| 
|-
| style="background: lightblue;" | 42
| colspan="2" style="background: lightblue;" | [[LHS 288|LHS&nbsp;288]] (루이텐 143-23)
| style="background: #ffa040;" | 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 | 0.208&nbsp;95(2&nbsp;73)″<ref name="recent"/>
| 15.610(204)
|<ref name=henry2006 />
|-
| rowspan="2" style="background: lightblue;" | 43
| rowspan="2" style="background: lightblue;" | [[글리제 412]]
| style="background: lightblue;" | 글리제 412&nbsp;A
| style="background: #ffa040;" | 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 | 0.206&nbsp;02(1&nbsp;08)″<ref name="Y"/><ref name="H"/>
| rowspan="2" | 15.832(83)
| rowspan="2" | 
|-
| style="background: lightblue;" | 글리제 412&nbsp;B (큰곰자리 WX)
| style="background: #ffa040;" | M5.5V<ref name=RECONS />
| 14.48<ref name=RECONS />
| 16.05<ref name=RECONS />
| ''?''
| {{RA|11|05|30.4}}
| {{DEC|+43|31|18}}
|-
| style="background: lightblue;" | 44
| colspan="2" style="background: lightblue;" | [[그룸브리지 1618|그룸브리지&nbsp;1618]] (글리제 380)
| style="background: #ffe46f;" | [[K형 주계열성|K7.0V]]<ref name=RECONS />
| 6.59<ref name=RECONS />
| 8.16<ref name=RECONS />
| align=left | &nbsp;4,000
| {{RA|10|11|22.1}}
| {{DEC|+49|27|15}}
|align=left |  0.205&nbsp;81(0&nbsp;67)″<ref name="Y"/><ref name="H"/>
| 15.848(52)
| 
|-
| style="background: lightblue;" | 45
| colspan="2" style="background: lightblue;" | [[글리제 388]]
| style="background: #ffa040;" | 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 | 0.204&nbsp;60(2&nbsp;80)″<ref name="Y"/>
| 15.942(218)
|
|-
| style="background: lightblue;" | 46
| colspan="2" style="background: lightblue;" | [[글리제 832]]
| style="background: #ffa040;" | M3.0V<ref name=RECONS />
| 8.66<ref name=RECONS />
| 10.20<ref name=RECONS />
| ''?''
| {{RA|21|33|34.0}}
| {{DEC|−49|00|32}}
| align=left | 0.202&nbsp;78(1&nbsp;32)″<ref name="Y"/><ref name="H"/>
| 16.085(105)
| 
|-
| style="background: lightblue;" | 47
| colspan="2" style="background: lightblue;" | [[LP 944-020|LP&nbsp;944-020]]
| style="background: #ffa040;" | M9.0V<ref name=RECONS />
| 18.50<ref name=RECONS />
| 20.02<ref name=RECONS />
| ''?''
| {{RA|03|39|35.2}}
| {{DEC|−35|25|41}}
| align=left | 0.201&nbsp;40(4&nbsp;20)″<ref name="T">[http://cdsads.u-strasbg.fr/abs/1996MNRAS.281..644T CCD astrometry of southern very low-mass stars], C. G. Tinney, ''Monthly Notices of the Royal Astronomical Society'' '''281''', #2 (July 1996), pp. 644–658.</ref>
| 16.195(338)
| 
|-
| style="background: lightblue;" | 48
| colspan="2" style="background: lightblue;" | [[DEN 0255-4700|DEN&nbsp;0255-4700]]
| style="background: #F00000;" | [[갈색 왜성|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 | 0.201&nbsp;37(3&nbsp;89)″<ref name="recent"/>
| 16.197(313)
|<ref name=costa2005 />
|-
!colspan="11"|시차 오차 범위 = 0.200″
|-
| style="background: lightblue;" | 49
| colspan="2" style="background: lightblue;" | [[글리제 682]]
| style="background: #ffa040;" | M4.5V<ref name=RECONS />
| 10.95<ref name=RECONS />
| 12.45<ref name=RECONS />
| ''?''
| {{RA|17|37|03.7}}
| {{DEC|−44|19|09}}
| align=left | 0.199&nbsp;65(2&nbsp;30)″<ref name="Y"/><ref name="H"/>
| 16.337(188)
| 
|-
! rowspan="2" |#
!<small>[[항성계]]</small>
!<small>[[항성]]</small>
! rowspan="2" |<small>[[항성 분류|분광형]]</small>
! rowspan="2" |<small>[[겉보기등급|''m'']]<sub>[[존슨의 UBV 시스템|''V'']]</small>
! rowspan="2" |[[절대등급|''M'']]<sub>[[존슨의 UBV 시스템|''V'']]
! rowspan="2" |<small>[[유효온도|''T<sub>eff</sub>'']]<br />[[켈빈|K]][[오차 범위|(±err)]]</small>
!<small>[[적경]]<ref name=RECONS /></small>
!<small>[[적위]]<ref name=RECONS /></small>
! rowspan="2" |<small>[[시차]]<ref name="RECONS"/><ref name=plxfn /><br />[[초 (각도)|초각]][[오차 범위|(±err)]]</small>
! rowspan="2" |<small>[[거리]]<ref name=distfn /><br />[[광년]][[오차 범위|(±err)]]</small>
! rowspan="2" |<small>[[#참고 문헌|참고<br />문헌]]</small>
|-
! colspan="2" |<small>명칭</small>
! style="background: #FFC" colspan="2" |<small>[[역기점]] J2000.0</small>
|}

== 입체 지도 ==
다음 지도는 태양으로부터 14광년 이내에 있는 32개 항성계를 입체적으로 표시한 그림이다. [[이중성]] 또는 [[다중성|삼중성]]들은 별들이 차곡차곡 쌓여 있는 모습으로 표현되어 있으나, 실제 이들은 매우 가깝게 붙어 있기 때문에 하나의 별로 보인다. 항성의 색은 상기 표의 분광형 색채와 동일하다.
[[파일:Nearby Stars (14ly Radius) ko.svg|가운데|800px]]

== 각주 ==
{{각주|2}}

== 같이 보기 ==
* [[가까운 밝은 별 목록]]
* [[RECONS]]
* [[항성]]
* [[반지름순 별 목록]]
* [[질량이 큰 별 목록]]
* [[겉보기등급 순 항성 목록]]
* [[절대등급 순 항성 목록]]

{{0–5광년 안에 있는 천체들}}
{{5–10광년 안에 있는 천체들}}
{{10–15광년 안에 있는 천체들}}

[[분류:국부 거품]]
[[분류:항성 목록]]
[[분류:항성 목록]]
[[분류:거리에 따른 목록]]