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فهرست ستارگان نزدیک: تفاوت میان نسخه‌ها

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جز ←‏فهرست: حذف عبارت جادویی مدیاویکی با استفاده از AWB
خط ۵:
{| style="font-size: 100%; text-align: center;" class="wikitable" border = "1"
! rowspan="2" |#
! colspan="2" |<small>نامگذاریsmallBBBBنامگذاری</small>smallBBBB
! rowspan="2" |<small>smallBBBB[[رده‌بندی ستارگان|رده‌بندی]]</small>smallBBBB
! rowspan="2" |<small>smallBBBB[[قدر ظاهری|''m'']]<sub>subBBBB[[سیستم فتومتریک UBV|''V'']]</sub>subBBBB</small>smallBBBB
! rowspan="2" |<small>smallBBBB[[قدر مطلق (اخترشناسی)|''M'']]<sub>subBBBB[[سیستم فتومتریک UBV|''V'']]</sub>subBBBB</small>smallBBBB
! rowspan="2" |<small>smallBBBB[[دمای موثر|''T<sub>effsubBBBBeff</sub>subBBBB'']]{{سخ}}[[کلوین|K]][[margin of error|(±err)]]</small>smallBBBB
! style="background: #FFC" colspan="2" |<small>smallBBBB[[مبدا (ستاره‌شناسی)|مبدا]] [[مبدأ (ستاره‌شناسی)]]</small>smallBBBB
! rowspan="2" |<small>smallBBBB[[اختلاف منظر]]<refAAAA name="RECONS">BBBB{{یادکرد|فصل=|کتاب=|ناشر= |چاپ= |شهر= |کوشش= |ویرایش= |سال=|شابک=|نویسنده=Research Consortium on Nearby Stars, {{چر}}Georgia State University |نویسندگان سایر بخش‌ها=|ترجمه=|صفحه= |زبان=en |مقاله= [http://www.chara.gsu.edu/RECONS/TOP100.posted.htm The One Hundred Nearest Star Systems] |ژورنال= [http://www.chara.gsu.edu/RECONS/ RECONS] |نشریه=|تاریخ=2007-Sep 17 |دوره= |شماره= |شاپا=}} Retrieved on 2007-11-06.</ref><refrefBBBBAAAA name=plxfn>ParallaxesplxfnBBBBParallaxes given by RECONS are a weighted mean of values in the sources given, as well as measurements by the RECONS program.</ref>refBBBB{{سخ}}[[ثانیه قوسی]][[margin of error|(±err)]]</small>smallBBBB
! rowspan="2" |<small>smallBBBB[[فاصله]]<refAAAA name=distfn>ازdistfnBBBBاز روی اختلاف منظر محاسبه می‌شود.</ref>refBBBB{{سخ}}[[سال نوری]]s[[margin of error|(±err)]]</small>smallBBBB
! rowspan="2" |<small>smallBBBB[[#References|Additional{{سخ}}references]]</small>smallBBBB
|-
!<small>smallBBBB[[سامانه ستاره‌ای|سامانه]]</small>smallBBBB
!<small>smallBBBB[[ستاره]]</small>smallBBBB
!<small>smallBBBB[[بعد]]<refAAAA name=RECONS/>BBBB</small>smallBBBB
!<small>smallBBBB[[میل]]<refAAAA name=RECONS/>BBBB</small>smallBBBB
|-
|style="background: #FFFFFF;" |
|style="background: #FFFFFF;" | [[منظومه خورشیدی]]
|style="background: #FFFFFF;" | [[خورشید]] (Sol)
| style="background: {{star-color|G}};" | [[ستاره نوع جی|G2V]]<refAAAA name=RECONS/>BBBB
| −26.72<ref72AAAA name=RECONS/>BBBB
| 4.85<ref85AAAA name=RECONS/>BBBB
| align=left | &nbsp;5,778<ref>778AAAABBBB[http://nssdc.gsfc.nasa.gov/planetary/factsheet/sunfact.html Sun Fact Sheet], NASA. Accessed on line [[۸ نوامبر]], [[2007]].</ref>refBBBB
| —
| —
خط ۳۷:
| style="background: #E0E0FF;" | [[پروکسیما قنطورس]] (V645&nbsp;Centauri)
| style="background: {{star-color|M}};" | [[کوتوله سرخ|M5.5Ve]]
| 11.09<ref09AAAA name=RECONS/>BBBB
| 15.53<ref53AAAA name=RECONS/>BBBB
| align=left | &nbsp;3,040<ref040AAAA name="ESO2003"/>BBBB
| {{RA|14|29|43.0}}
| {{DEC|−62|40|46}}
| align=left | 0.768&nbsp;87(0&nbsp;29)″<ref″AAAA name="Y">BBBB[[کاتالوگ ستاره‌ای]].</ref><refrefBBBBAAAA name="H">BBBB[[کاتالوگ ابرخس]].</ref>refBBBB
| 4.2421(16)
| <refAAAA name="B">BurgasserBBBBBurgasser et al. 2000</ref>refBBBB
|-
|style="background: #FFFFFF;" | α&nbsp;Centauri&nbsp;A (HD&nbsp;128620)
| style="background: {{star-color|G}};" | [[ستاره نوع جی|G2V]]<refAAAA name=RECONS/>BBBB
| 0.01<ref01AAAA name=RECONS/>BBBB
| 4.38<ref38AAAA name=RECONS/>BBBB
| align=left | &nbsp;5,790<ref790AAAA name="ESO2003">BBBB{{یادکرد|فصل=|کتاب=|ناشر= |چاپ= |شهر= |کوشش= |ویرایش= ESO Press Release 05/03 |سال=|شابک=|نویسنده= Kervella, Pierre; Thevenin, Frederic|نویسندگان سایر بخش‌ها=|ترجمه=|صفحه= |زبان=en |مقاله= [http://www.eso.org/public/outreach/press-rel/pr-2003/pr-05-03.html A Family Portrait of the Alpha Centauri System: VLT Interferometer Studies the Nearest Stars] |ژورنال= |نشریه=ESO |تاریخ=[[۱۵ مارس|March 15]], [[۲۰۰۳ (میلادی)|2003]] |دوره= |شماره= |شاپا=}} Retrieved on 2007-11-08.</ref>refBBBB
| {{RA|14|39|36.5}}
| {{DEC|−60|50|02}}
| rowspan="2" align=left | 0.747&nbsp;23(1&nbsp;17)″<ref″AAAA name="Y"/><refBBBBAAAA name="S">BBBB[http://adsabs.harvard.edu/abs/1999A&A...341..121S Visual binary orbits and masses post Hipparcos], Staffan Söderhjelm, ''Astronomy and Astrophysics'' '''341''' (January 1999), pp. 121–140.</ref>refBBBB
| rowspan="2" | 4.3650(68)
| rowspan="2" |
|-
|style="background: #FFFFFF;" | α&nbsp;Centauri&nbsp;B (HD&nbsp;128621)
| style="background: {{star-color|K}};" | [[K V star|K0V]]<refAAAA name=RECONS/>BBBB
| 1.34<ref34AAAA name=RECONS/>BBBB
| 5.71<ref71AAAA name=RECONS/>BBBB
| align=left | &nbsp;5,260<ref260AAAA name="ESO2003"/>BBBB
| {{RA|14|39|35.1}}
| {{DEC|−60|50|14}}
خط ۶۸:
| colspan="2" style="background: #E0E0FF;" | [[ستاره بارنارد]] (BD+04°3561a)
| style="background: {{star-color|M}};" | M4.0Ve
| 9.53<ref53AAAA name=RECONS/>BBBB
| 13.22<ref22AAAA name=RECONS/>BBBB
| align=left | &nbsp;3,134(102)<ref>AAAABBBB[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>refBBBB
| {{RA|17|57|48.5}}
| {{DEC|+04|41|36}}
| align=left | 0.546&nbsp;98(1&nbsp;00)″<ref″AAAA name="Y"/><refBBBBAAAA name="H"/>BBBB
| 5.9630(109)
|
خط ۷۹:
| style="background: #E0E0FF;" | 3
| colspan="2" style="background: #E0E0FF;" | [[ولف ۳۵۹|Wolf&nbsp;359]] (CN&nbsp;Leonis)
| style="background: {{star-color|M}};" | M6.0V<ref0VAAAA name=RECONS/>BBBB
| 13.44<ref44AAAA name=RECONS/>BBBB
| 16.55<ref55AAAA name=RECONS/>BBBB
| align=left | &nbsp;2,800(100)<refAAAA name="aaa447">BBBB{{یادکرد|فصل=|کتاب=|ناشر= |چاپ= |شهر= |کوشش= |ویرایش= |سال=|شابک=|نویسنده= Ya. V. Pavlenko, H. R. A. Jones, Yu. Lyubchik, J. Tennyson, and D. J. Pinfield|نویسندگان سایر بخش‌ها=|ترجمه=|صفحه=709–717 |زبان=en |مقاله= [http://adsabs.harvard.edu/abs/2006A&A...447..709P Spectral energy distribution for GJ406] |ژورنال= Astronomy and Astrophysics |نشریه=|تاریخ= {{{day}}} February {{چر}}2006 |دوره=447 |شماره= 2 |شاپا= [[Digital object identifier|doi]]: <span class="neverexpand">BBBB[http://dx.doi.org/%7B%7Burlencode:10.1051/0004-6361:20052979}} {{#tag:<nowiki|>10.1051/0004-6361:20052979}}</nowiki>]</span>spanBBBB}}</ref>refBBBB
| {{RA|10|56|29.2}}
| {{DEC|+07|00|53}}
|align=left | 0.419&nbsp;10(2&nbsp;10)″<ref″AAAA name="Y"/>BBBB
| 7.7825(390)
|
خط ۹۱:
| style="background: #E0E0FF;" | 4
| colspan="2" style="background: #E0E0FF;" | [[Lalande 21185|Lalande&nbsp;21185]] (BD+36°2147)
| style="background: {{star-color|M}};" | M2.0V<ref0VAAAA name=RECONS/>BBBB
| 7.47<ref47AAAA name=RECONS/>BBBB
| 10.44<ref44AAAA name=RECONS/>BBBB
| align=left | &nbsp;3,400<ref>400AAAABBBB[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>refBBBB
| {{RA|11|03|20.2}}
| {{DEC|+35|58|12}}
| align=left | 0.393&nbsp;42(0&nbsp;70)″<ref″AAAA name="Y"/><refBBBBAAAA name="H"/>BBBB
| 8.2905(148)
|
خط ۱۰۴:
| rowspan="2" style="background: #FFFFFF;" | [[شباهنگ (ستاره)]]{{سخ}}(α&nbsp;Canis&nbsp;Majoris)
|style="background: #FFFFFF;" | Sirius A
| style="background: {{star-color|A}}" | [[A V star|A1V]]<refAAAA name=RECONS/>BBBB
| −1.43<ref43AAAA name=RECONS/>BBBB
| 1.47<ref47AAAA name=RECONS/>BBBB
| align=left | &nbsp;9,940(210)<ref>TableAAAABBBBTable 2, [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>refBBBB
| 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″AAAA name="Y"/><refBBBBAAAA name="H"/>BBBB
| rowspan="2" | 8.5828(289)
| rowspan="2" |
|-
| style="background: #E0E0FF;" | Sirius&nbsp;B
| style="background: F0F0F0" | [[کوتوله سفید|DA2]]<refAAAA name=RECONS/>BBBB
| 8.44<ref44AAAA name=RECONS/>BBBB
| 11.34<ref34AAAA name=RECONS/>BBBB
| align=left | 25,000(200)<ref>AdoptedAAAABBBBAdopted value, [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 (September 2005), pp. L69–L72.</ref>refBBBB
|-
| rowspan="2" style="background: #E0E0FF;" | 6
خط ۱۲۴:
| style="background: #E0E0FF;" | Luyten&nbsp;726-8&nbsp;A (BL&nbsp;Ceti)
| style="background: {{star-color|M}};" | M5.5Ve
| 12.54<ref54AAAA name=RECONS/>BBBB
| 15.40<ref40AAAA name=RECONS/>BBBB
| 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″AAAA name="Y"/>BBBB
| rowspan="2" | 8.7280(631)
| rowspan="2" |
خط ۱۳۵:
| style="background: #E0E0FF;" | Luyten&nbsp;726-8&nbsp;B (UV&nbsp;Ceti)
| style="background: {{star-color|M}};" | M6.0Ve
| 12.99<ref99AAAA name=RECONS/>BBBB
| 15.85<ref85AAAA name=RECONS/>BBBB
| align=left | ~2,600
|-
خط ۱۴۲:
| colspan="2" style="background: #E0E0FF;" | [[روس ۱۵۴|Ross&nbsp;154]] (V1216&nbsp;Sagittarii)
| style="background: {{star-color|M}};" | M3.5Ve
| 10.43<ref43AAAA name=RECONS/>BBBB
| 13.07<ref07AAAA name=RECONS/>BBBB
| align=left | &nbsp;2,700
| {{RA|18|49|49.4}}
| {{DEC|−23|50|10}}
| align=left | 0.336&nbsp;90(1&nbsp;78)″<ref″AAAA name="Y"/><refBBBBAAAA name="H"/>BBBB
| 9.6813(512)
|
خط ۱۵۴:
| colspan="2" style="background: #E0E0FF;" | [[روس ۲۴۸|Ross&nbsp;248]] (HH&nbsp;Andromedae)
| style="background: {{star-color|M}};" | M5.5Ve
| 12.29<ref29AAAA name=RECONS/>BBBB
| 14.79<ref79AAAA name=RECONS/>BBBB
| {{?}}
| {{RA|23|41|54.7}}
| {{DEC|+44|10|30}}
| align=left | 0.316&nbsp;00(1&nbsp;10)″<ref″AAAA name="Y"/>BBBB
| 10.322(36)
|
خط ۱۶۵:
| 9
| colspan="2" | [[اپسیلون جوی]] (BD−09°697)
| style="background: {{star-color|K}};" | [[K V star|K2V]]<refAAAA name=RECONS/>BBBB
| 3.73<ref73AAAA name=RECONS/>BBBB
| 6.19<ref19AAAA name=RECONS/>BBBB
| align=left | &nbsp;5,100
| {{RA|03|32|55.8}}
| {{DEC|−09|27|30}}
|align=left | 0.309&nbsp;99(0&nbsp;79)″<ref″AAAA name="Y"/><refBBBBAAAA name="H"/>BBBB
| 10.522(27)
|
خط ۱۷۸:
| colspan="2" style="background: #E0E0FF;" | [[Lacaille 9352|Lacaille&nbsp;9352]] (CD−36°15693)
| style="background: {{star-color|M}};" | M1.5Ve
| 7.34<ref34AAAA name=RECONS/>BBBB
| 9.75<ref75AAAA name=RECONS/>BBBB
| align=left | &nbsp;3,340
| {{RA|23|05|52.0}}
| {{DEC|−35|51|11}}
| align=left | 0.303&nbsp;64(0&nbsp;87)″<ref″AAAA name="Y"/><refBBBBAAAA name="H"/>BBBB
| 10.742(31)
|
خط ۱۹۰:
| colspan="2" style="background: #E0E0FF;" | [[روس ۱۲۸|Ross&nbsp;128]] (FI&nbsp;Virginis)
| style="background: {{star-color|M}};" | M4.0Vn
| 11.13<ref13AAAA name=RECONS/>BBBB
| 13.51<ref51AAAA name=RECONS/>BBBB
| align=left | &nbsp;2,800
| {{RA|11|47|44.4}}
| {{DEC|+00|48|16}}
| align=left | 0.298&nbsp;72(1&nbsp;35)″<ref″AAAA name="Y"/><refBBBBAAAA name="H"/>BBBB
| 10.919(49)
|
خط ۲۰۲:
| rowspan="3" style="background: #E0E0FF;" | [[ای‌زد دلو|EZ&nbsp;Aquarii]]{{سخ}}(GJ&nbsp;866, Luyten&nbsp;789-6)
| style="background: #E0E0FF;" | EZ&nbsp;Aquarii&nbsp;A
<!--DDDD-It is also known as
[[Henry-Lee Giclas|G]] 156-031,
[[کاتالوگ ستاره‌ای|GCTP]] 5475.00,
[[Luyten Half-Second catalogue|LHS]] 68 and
Luyten 0789-006.--->EEEE
| style="background: {{star-color|M}};" | M5.0Ve
| 13.33<ref33AAAA name=RECONS/>BBBB
| 15.64<ref64AAAA name=RECONS/>BBBB
| {{?}}
| 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″AAAA name="Y"/>BBBB
| rowspan="3" | 11.266(171)
| rowspan="3" |
خط ۲۱۹:
| style="background: #E0E0FF;" | EZ&nbsp;Aquarii&nbsp;B
| style="background: {{star-color|M}};" | M?
| 13.27<ref27AAAA name=RECONS/>BBBB
| 15.58<ref58AAAA name=RECONS/>BBBB
| {{?}}
|-
| style="background: #E0E0FF;" | EZ&nbsp;Aquarii&nbsp;C
| style="background: {{star-color|M}};" | M?
| 14.03<ref03AAAA name=RECONS/>BBBB
| 16.34<ref34AAAA name=RECONS/>BBBB
| {{?}}
|-
خط ۲۳۲:
| rowspan="2" | [[شعرای شامی]]{{سخ}}(α&nbsp;Canis&nbsp;Minoris)
| Procyon&nbsp;A
| style="background: {{star-color|F}}" | F5V-IV<refIVAAAA name=RECONS/>BBBB
| 0.38<ref38AAAA name=RECONS/>BBBB
| 2.66<ref66AAAA name=RECONS/>BBBB
| 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″AAAA name="Y"/><refBBBBAAAA name="H"/>BBBB
| rowspan="2" | 11.402(32)
| rowspan="2" |
|-
| style="background: #E0E0FF;" | Procyon&nbsp;B
| style="background: #F0F0F0" | [[کوتوله سفید|DA]]<refAAAA name=RECONS/>BBBB
| 10.70<ref70AAAA name=RECONS/>BBBB
| 12.98<ref98AAAA name=RECONS/>BBBB
| align=left | &nbsp;9,700
|-
خط ۲۵۱:
| rowspan="2" | [[۶۱ ماکیان|61&nbsp;Cygni]]
| 61&nbsp;Cygni&nbsp;A (BD+38°4343)
| style="background: {{star-color|K}};" | [[K V star|K5.0V]]<refAAAA name=RECONS/>BBBB <!--previousDDDDprevious: K3.5Ve-->5VeEEEE
| 5.21<ref21AAAA name=RECONS/>BBBB
| 7.49<ref49AAAA name=RECONS/>BBBB
| 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″AAAA name="Y"/><refBBBBAAAA name="H"/>BBBB
| rowspan="2" | 11.403(22)
| rowspan="2" |
|-
| 61&nbsp;Cygni&nbsp;B (BD+38°4344)
| style="background: {{star-color|K}};" | [[K V star|K7.0V]]<refAAAA name=RECONS/>BBBB <!--previousDDDDprevious: K4.7Ve-->7VeEEEE
| 6.03<ref03AAAA name=RECONS/>BBBB
| 8.31<ref31AAAA name=RECONS/>BBBB
| align=left | &nbsp;4,440
| {{RA|21|06|55.3}}
خط ۲۷۲:
| rowspan="2" style="background: #E0E0FF;" | [[Struve 2398|Struve&nbsp;2398]]{{سخ}}(GJ&nbsp;725, BD+59°1915)
| style="background: #E0E0FF;" | Struve&nbsp;2398&nbsp;A (HD&nbsp;173739)
| style="background: {{star-color|M}};" | M3.0V<ref0VAAAA name=RECONS/>BBBB
| 8.90<ref90AAAA name=RECONS/>BBBB
| 11.16<ref16AAAA name=RECONS/>BBBB
| {{?}}
| {{RA|18|42|46.7}}
| {{DEC|+59|37|49}}
| rowspan="2" align=left | 0.283&nbsp;00(1&nbsp;69)″<ref″AAAA name="Y"/><refBBBBAAAA name="H"/>BBBB
| rowspan="2" | 11.525(69)
| rowspan="2" |
خط ۲۸۴:
| style="background: #E0E0FF;" | Struve&nbsp;2398&nbsp;B (HD&nbsp;173740)
 
| style="background: {{star-color|M}};" | M3.5V<ref5VAAAA name=RECONS/>BBBB
| 9.69<ref69AAAA name=RECONS/>BBBB
| 11.95<ref95AAAA name=RECONS/>BBBB
| {{?}}
| {{RA|18|42|46.9}}
خط ۲۹۴:
| rowspan="2" style="background: #E0E0FF;" | [[گروم‌بریج ۳۴|Groombridge&nbsp;34]]{{سخ}}(GJ&nbsp;15)
| style="background: #E0E0FF;" | Groombridge&nbsp;34&nbsp;A (GX&nbsp;Andromedae)
<!--DDDD-It is also known as
[[Henry Draper catalogue|HD]] 1326,
[[Bonner Durchmusterung|BD]]+43°44,
خط ۳۰۰:
[[کاتالوگ ستاره‌ای|GCTP]] 49.00A,
[[Luyten Half-Second catalogue|LHS]] 3 and
[[Alexander N. Vyssotsky|Vyssotsky]] 85.--->EEEE
| style="background: {{star-color|M}};" | M1.5V<ref5VAAAA name=RECONS/>BBBB <!--previousDDDDprevious: M3.0V-->0VEEEE
| 8.08<ref08AAAA name=RECONS/>BBBB
| 10.32<ref32AAAA name=RECONS/>BBBB
| {{?}}
| 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″AAAA name="Y"/><refBBBBAAAA name="H"/>BBBB
| rowspan="2" | 11.624(39)
| rowspan="2" |
|-
| style="background: #E0E0FF;" | Groombridge&nbsp;34&nbsp;B (GQ&nbsp;Andromedae)
<!--DDDD-It is also known as
[[Henry-Lee Giclas|G]] 171-048 and
[[Luyten Half-Second catalogue|LHS]] 4.--->EEEE
| style="background: {{star-color|M}};" | M3.5V<ref5VAAAA name=RECONS/>BBBB
| 11.06<ref06AAAA name=RECONS/>BBBB
| 13.30<ref30AAAA name=RECONS/>BBBB
| {{?}}
|-
خط ۳۲۳:
| rowspan="3" | [[اپسیلون هندی|Epsilon&nbsp;Indi]]{{سخ}}(CPD−57°10015)
| Epsilon Indi A
| style="background: {{star-color|K}};" | [[K V star|K5Ve]]<refAAAA name=RECONS/>BBBB
| 4.69<ref69AAAA name=RECONS/>BBBB
| 6.89<ref89AAAA name=RECONS/>BBBB
| 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″AAAA name="Y"/><refBBBBAAAA name="H"/>BBBB
| rowspan="3" | 11.824(30)
| rowspan="3" |
خط ۳۳۵:
| style="background: #E0E0FF;" | Epsilon&nbsp;Indi&nbsp;Ba
| style="background: {{star-color|T}};" | [[کوتوله قهوه‌ای|T1.0V]]
|BBBB23
|>23
|BBBB25
|>25
| align=left | &nbsp;1,280
| rowspan="2" | {{RA|22|04|10.5}}
خط ۳۴۳:
| style="background: #E0E0FF;" | Epsilon&nbsp;Indi&nbsp;Bb
| style="background: {{star-color|T}};" | [[کوتوله قهوه‌ای|T6.0V]]
|BBBB23
|>23
|BBBB25
|>25
| align=left | &nbsp;&nbsp;&nbsp;850
|-
| style="background: #E0E0FF;" | 18
| colspan="2" style="background: #E0E0FF;" | [[دی‌ایکس خرچنگ|DX&nbsp;Cancri]] (G&nbsp;51-15)
<!--DDDD-It is also known as
[[Henry-Lee Giclas|G]] 051-015,
[[کاتالوگ ستاره‌ای|GCTP]] 2016.01 and
[[Luyten Half-Second catalogue|LHS]] 248.--->EEEE
| style="background: {{star-color|M}};" | M6.5Ve
| 14.78<ref78AAAA name=RECONS/>BBBB
| 16.98<ref98AAAA name=RECONS/>BBBB
| {{?}}
| {{RA|08|29|49.5}}
| {{DEC|+26|46|37}}
| align=left | 0.275&nbsp;80(3&nbsp;00)″<ref″AAAA name=Y/>BBBB
| 11.826(129)
|
خط ۳۶۵:
| 19
| colspan="2" | [[تاو نهنگ|Tau&nbsp;Ceti]] (BD−16°295)
| style="background: {{star-color|G}};" | [[ستاره نوع جی|G8Vp]]<refAAAA name=RECONS/>BBBB
| 3.49<ref49AAAA name=RECONS/>BBBB
| 5.68<ref68AAAA name=RECONS/>BBBB
| align=left | &nbsp;5,344
| {{RA|01|44|04.1}}
| {{DEC|−15|56|15}}
| align=left | 0.274&nbsp;39(0&nbsp;76)″<ref″AAAA name="Y"/><refBBBBAAAA name="H"/>BBBB
| 11.887(33)
|
خط ۳۷۷:
| style="background: #E0E0FF;" | 20
| colspan="2" style="background: #E0E0FF;" | [[جی‌جی ۱۰۶۱|GJ&nbsp;1061]] (LHS&nbsp;1565)
| style="background: {{star-color|M}};" | M5.5V<ref5VAAAA name=RECONS/>BBBB
| 13.09<ref09AAAA name=RECONS/>BBBB
| 15.26<ref26AAAA name=RECONS/>BBBB
| {{?}}
| {{RA|03|35|59.7}}
| {{DEC|−44|30|45}}
| align=left | 0.272&nbsp;01(1&nbsp;30)″<ref″AAAA name="recent">SystemsBBBBSystems with their first accurate trigonometric parallaxes measured by RECONS</ref>refBBBB
| 11.991(57)
| <refAAAA name=henry1997>henry1997BBBB[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><refrefBBBBAAAA name=henry2006>henry2006BBBB[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>refBBBB
|-
| style="background: #E0E0FF;" | 21
| colspan="2" style="background: #E0E0FF;" | [[وای‌زد نهنگ|YZ&nbsp;Ceti]] (LHS&nbsp;138)
<!--DDDD-It is also known as
[[Henry-Lee Giclas|G]] 268-135,
[[کاتالوگ ستاره‌ای|GCTP]] 248.01,
[[Luyten Half-Second catalogue|LHS]] 138,
Luyten 0725-032 and
[[Luyten Two-Tenths catalogue|LTT]] 670.--->EEEE
| style="background: {{star-color|M}};" | M4.5V<ref5VAAAA name=RECONS/>BBBB
| 12.02<ref02AAAA name=RECONS/>BBBB
| 14.17<ref17AAAA name=RECONS/>BBBB
| {{?}}
| {{RA|01|12|30.6}}
| {{DEC|−16|59|56}}
| align=left | 0.268&nbsp;84(2&nbsp;95)″<ref″AAAA name="Y"/><refBBBBAAAA name="H"/>BBBB
| 12.132(133)
|
خط ۴۰۸:
| colspan="2" style="background: #E0E0FF;" | [[Luyten's Star|Luyten's&nbsp;Star]] (BD+05°1668)
| style="background: {{star-color|M}};" | M3.5Vn
| 9.86<ref86AAAA name=RECONS/>BBBB
| 11.97<ref97AAAA name=RECONS/>BBBB
| {{?}}
| {{RA|07|27|24.5}}
| {{DEC|+05|13|33}}
| align=left | 0.263&nbsp;76(1&nbsp;25)″<ref″AAAA name="Y"/><refBBBBAAAA name="H"/>BBBB
| 12.366(59)
|
خط ۴۲۰:
| colspan="2" style="background: #E0E0FF;" | [[ستاره باغ چای|Teegarden's&nbsp;star]] (SO025300.5+165258)
| style="background: {{star-color|M}};" | M6.5V
| 15.14<ref14AAAA name=RECONS/>BBBB
| 17.22<ref22AAAA name=RECONS/>BBBB
| {{?}}
| {{RA|02|53|00.9}}
| {{DEC|+16|52|53}}
| align=left | 0.260&nbsp;63(2&nbsp;69)″<ref″AAAA name=recent/>BBBB
| 12.514(129)
| <refAAAA name=henry2006/>BBBB
|-
| rowspan="2" style="background: #E0E0FF;" | 24
| rowspan="2" style="background: #E0E0FF;" | [[اس‌سی‌آر ۱۸۴۵-۶۳۵۷|SCR&nbsp;1845-6357]]
| style="background: #E0E0FF;" | SCR&nbsp;1845-6357&nbsp;A
| style="background: {{star-color|M}};" | M8.5V<ref5VAAAA name=RECONS/>BBBB
| 17.39
| 19.41
خط ۴۳۸:
| {{RA|18|45|05.3}}
| {{DEC|−63|57|48}}
| rowspan=2 align=left | 0.259&nbsp;45(1&nbsp;11)″<ref″AAAA name="recent"/>BBBB
| rowspan=2 | 12.571(54)
| rowspan=2 | <refAAAA name=henry2006/>BBBB
|-
| style="background: #E0E0FF;" | SCR&nbsp;1845-6357&nbsp;B
| style="background: {{star-color|T}};" | [[کوتوله قهوه‌ای|T6]]<refAAAA name=nearmt>nearmtBBBB[http://adsabs.harvard.edu/abs/2007A&A...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>refBBBB
| {{?}}
| {{?}}
| align=left | &nbsp;&nbsp;&nbsp;950<ref950AAAA name=nearmt/>BBBB
| {{RA|18|45|02.6}}
| {{DEC|−63|57|52}}
خط ۴۵۲:
| style="background: #E0E0FF;" | 25
| colspan="2" style="background: #E0E0FF;" | [[ستاره کاپتین|Kapteyn's&nbsp;Star]] (CD−45°1841)
| style="background: {{star-color|M}};" | M1.5V<ref5VAAAA name=RECONS/>BBBB <!--previousDDDDprevious: sdM0VI-->sdM0VIEEEE
| 8.84<ref84AAAA name=RECONS/>BBBB
| 10.87<ref87AAAA name=RECONS/>BBBB
| align=left | &nbsp;3,800
| {{RA|05|11|40.6}}
| {{DEC|−45|01|06}}
| align=left | 0.255&nbsp;27(0&nbsp;86)″<ref″AAAA name="Y"/><refBBBBAAAA name="H"/>BBBB
| 12.777(43)
|
خط ۴۶۴:
| style="background: #E0E0FF;" | 26
| colspan="2" style="background: #E0E0FF;" | [[Lacaille 8760|Lacaille&nbsp;8760]] (AX&nbsp;Microscopii)
<!--DDDD-It is also known as
[[Henry Draper catalogue|HD]] 202560,
[[Cordoba Durchmusterung|CD]]−39°14192,
[[کاتالوگ ستاره‌ای|GCTP]] 5117.00,
[[Luyten Half-Second catalogue|LHS]] 66 and UGPMF 518.--->EEEE
| style="background: {{star-color|M}};" | M0.0V<ref0VAAAA name=RECONS/>BBBB <!--previousDDDDprevious: M2Ve-->M2VeEEEE
| 6.67<ref67AAAA name=RECONS/>BBBB
| 8.69<ref69AAAA name=RECONS/>BBBB
| align=left | &nbsp;3,340
| {{RA|21|17|15.3}}
| {{DEC|−38|52|03}}
| align=left | 0.253&nbsp;43(1&nbsp;12)″<ref″AAAA name="Y"/><refBBBBAAAA name="H"/>BBBB
| 12.870(57)
|
خط ۴۸۲:
| rowspan="2" style="background: #E0E0FF;" | [[کروگر ۶۰|Kruger&nbsp;60]]{{سخ}}(BD+56°2783)
| style="background: #E0E0FF;" | Kruger&nbsp;60&nbsp;A
| style="background: {{star-color|M}};" | M3.0V<ref0VAAAA name=RECONS/>BBBB
| 9.79<ref79AAAA name=RECONS/>BBBB
| 11.76<ref76AAAA name=RECONS/>BBBB
| 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″AAAA name="Y"/><refBBBBAAAA name="S"/>BBBB
| rowspan="2" | 13.149(74)
| rowspan="2" |
|-
| style="background: #E0E0FF;" | Kruger&nbsp;60&nbsp;B (DO&nbsp;Cephei)
| style="background: {{star-color|M}};" | M4.0V<ref0VAAAA name=RECONS/>BBBB
| 11.41<ref41AAAA name=RECONS/>BBBB
| 13.38<ref38AAAA name=RECONS/>BBBB
| align=left | &nbsp;2,890
|-
| style="background: #E0E0FF;" | 28
| colspan="2" style="background: #E0E0FF;" | [[دی‌ای‌ان ۱۰۴۸-۳۹۵۶|DEN&nbsp;1048-3956]]
| style="background: {{star-color|M}};" | M8.5V<ref5VAAAA name=RECONS/>BBBB
| 17.39<ref39AAAA name=RECONS/>BBBB
| 19.37<ref37AAAA name=RECONS/>BBBB
| {{?}}
| {{RA|10|48|14.7}}
| {{DEC|−39|56|06}}
| align=left | 0.247&nbsp;71(1&nbsp;55)″<ref″AAAA name="recent"/>BBBB
| 13.167(82)
| <ref>AAAABBBB[http://adsabs.harvard.edu/abs/2005AJ....129.1954J The Solar Neighborhood. XIII. Parallax Results from the CTIOPI 0.9 Meter Program: Stars with μ>μBBBB= 1.0" yr<sup>supBBBB-1</sup>supBBBB (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><refrefBBBBAAAA name=costa2005>costa2005BBBB[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>refBBBB
|-
| rowspan="2" style="background: #E0E0FF;" | 29
| rowspan="2" style="background: #E0E0FF;" | [[روس ۶۱۴|Ross&nbsp;614]]{{سخ}}(V577&nbsp;Monocerotis, GJ&nbsp;234)
| style="background: #E0E0FF;" | Ross&nbsp;614A (LHS&nbsp;1849)
<!--DDDD-It is also known as
[[Henry-Lee Giclas|G]] 106-049,
[[کاتالوگ ستاره‌ای|GCTP]] 1509.00 and
[[Luyten Half-Second catalogue|LHS]] 1849.--->EEEE
| style="background: {{star-color|M}};" | M4.5V<ref5VAAAA name=RECONS/>BBBB
| 11.15<ref15AAAA name=RECONS/>BBBB
| 13.09<ref09AAAA name=RECONS/>BBBB
| {{?}}
| 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″AAAA name="Y"/><refBBBBAAAA name="S"/>BBBB
| rowspan="2" | 13.349(110)
| rowspan="2" |
|-
| style="background: #E0E0FF;" | Ross&nbsp;614B (LHS&nbsp;1850)
<!--DDDD-It is also known as
[[Luyten Half-Second catalogue|LHS]] 1850.--->EEEE
| style="background: {{star-color|M}};" | M5.5V
| 14.23<ref23AAAA name=RECONS/>BBBB
| 16.17<ref17AAAA name=RECONS/>BBBB
| {{?}}
|-
| style="background: #E0E0FF;" | 30
| colspan="2" style="background: #E0E0FF;" | [[ولف ۱۰۶۱|Gl&nbsp;628]] (Wolf&nbsp;1061, BD−12°4523)
<!--DDDD-It is also known as
[[Bonner Durchmusterung|BD]]−12°4523,
[[Henry-Lee Giclas|G]] 153-058,
[[کاتالوگ ستاره‌ای|GCTP]] 3746.00,
[[Luyten Half-Second catalogue|LHS]] 419 and
[[Alexander N. Vyssotsky|Vyssotsky]] 164.--->EEEE
| style="background: {{star-color|M}};" | M3.0V<ref0VAAAA name=RECONS/>BBBB
| 10.07<ref07AAAA name=RECONS/>BBBB
| 11.93<ref93AAAA name=RECONS/>BBBB
| {{?}}
| {{RA|16|30|18.1}}
| {{DEC|−12|39|45}}
| align=left | 0.236&nbsp;01(1&nbsp;67)″<ref″AAAA name="Y"/><refBBBBAAAA name="H"/>BBBB
| 13.820(98)
|
خط ۵۵۵:
| style="background: #E0E0FF;" | 31
| colspan="2" style="background: #E0E0FF;" | [[Van Maanen's Star|Van&nbsp;Maanen's&nbsp;Star]] (Gl&nbsp;35, LHS&nbsp;7)
| style="background: #F0F0F0" | [[کوتوله سفید|DZ7]]<refAAAA name=RECONS/>BBBB
| 12.38<ref38AAAA name=RECONS/>BBBB
| 14.21<ref21AAAA name=RECONS/>BBBB
| {{?}}
| {{RA|00|49|09.9}}
| {{DEC|+05|23|19}}
| align=left | 0.231&nbsp;88(1&nbsp;79)″<ref″AAAA name="Y"/><refBBBBAAAA name="H"/>BBBB
| 14.066(109)
|
خط ۵۶۸:
| colspan="2" style="background: #E0E0FF;" | [[گلیز ۱|Gl&nbsp;1]] (CD−37°15492)
 
| style="background: {{star-color|M}};" | M3.0V<ref0VAAAA name=RECONS/>BBBB
| 8.55<ref55AAAA name=RECONS/>BBBB
| 10.35<ref35AAAA name=RECONS/>BBBB
| {{?}}
| {{RA|00|05|24.4}}
| {{DEC|−37|21|27}}
| align=left | 0.229&nbsp;20(1&nbsp;07)″<ref″AAAA name="Y"/><refBBBBAAAA name="H"/>BBBB
| 14.231(66)
|
خط ۵۸۳:
 
| style="background: {{star-color|M}};" | M5.5Ve
| 13.18<ref18AAAA name=RECONS/>BBBB
| 14.97<ref97AAAA name=RECONS/>BBBB
| {{?}}
| rowspan="2" | {{RA|12|33|17.2}}
| rowspan="2" | {{DEC|+09|01|15}}
| rowspan="2" align=left | 0.227&nbsp;90(4&nbsp;60)″ <refAAAA name="Y"/>BBBB
| rowspan="2" | 14.312(289)
| rowspan="2" |
خط ۵۹۴:
| style="background: #E0E0FF;" | Wolf&nbsp;424&nbsp;B
| style="background: {{star-color|M}};" | M7Ve
| 13.17<ref17AAAA name=RECONS/>BBBB
| 14.96<ref96AAAA name=RECONS/>BBBB
| {{?}}
|-
| style="background: #E0E0FF;" | 34
| colspan="2" style="background: #E0E0FF;" | [[تی‌زد بره|TZ&nbsp;Arietis]] (GJ&nbsp;83.1, Luyten&nbsp;1159-16)
| style="background: {{star-color|M}};" | M4.5V<ref5VAAAA name=RECONS/>BBBB
| 12.27<ref27AAAA name=RECONS/>BBBB
| 14.03<ref03AAAA name=RECONS/>BBBB
| {{?}}
| {{RA|02|00|13.2}}
| {{DEC|+13|03|08}}
| align=left | 0.224&nbsp;80(2&nbsp;90)″<ref″AAAA name="Y"/>BBBB
| 14.509(187)
|
خط ۶۱۲:
| style="background: #E0E0FF;" | 35
| colspan="2" style="background: #E0E0FF;" | [[گلیز ۶۸۷|Gl&nbsp;687]] (LHS&nbsp;450, BD+68°946)
| style="background: {{star-color|M}};" | M3.0V<ref0VAAAA name=RECONS/>BBBB
| 9.17<ref17AAAA name=RECONS/>BBBB
| 10.89<ref89AAAA name=RECONS/>BBBB
| {{?}}
| {{RA|17|36|25.9}}
| {{DEC|+68|20|21}}
| align=left | 0.220&nbsp;49(0&nbsp;82)″<ref″AAAA name="Y"/><refBBBBAAAA name="H"/>BBBB
| 14.793(55)
|
خط ۶۲۴:
| style="background: #E0E0FF;" | 36
| colspan="2" style="background: #E0E0FF;" | [[ال‌اچ‌اس ۲۹۲|LHS&nbsp;292]] (LP&nbsp;731-58)
| style="background: {{star-color|M}};" | M6.5V<ref5VAAAA name=RECONS/>BBBB
| 15.60<ref60AAAA name=RECONS/>BBBB
| 17.32<ref32AAAA name=RECONS/>BBBB
| {{?}}
| {{RA|10|48|12.6}}
| {{DEC|−11|20|14}}
| align=left | 0.220&nbsp;30(3&nbsp;60)″<ref″AAAA name="Y"/>BBBB
| 14.805(242)
|
خط ۶۳۶:
| style="background: #E0E0FF;" | 37
| colspan="2" style="background: #E0E0FF;" | [[گلیز ۶۷۴|Gl&nbsp;674]] (LHS&nbsp;449)
| style="background: {{star-color|M}};" | M3.0V<ref0VAAAA name=RECONS/>BBBB
| 9.38<ref38AAAA name=RECONS/>BBBB
| 11.09<ref09AAAA name=RECONS/>BBBB
| {{?}}
| {{RA|17|28|39.9}}
| {{DEC|−46|53|43}}
| align=left | 0.220&nbsp;25(1&nbsp;59)″<ref″AAAA name="Y"/><refBBBBAAAA name="H"/>BBBB
| 14.809(107)
|
خط ۶۴۹:
| rowspan="3" style="background: #E0E0FF;" | [[جی‌جی ۱۲۴۵|GJ&nbsp;1245]]
| style="background: #E0E0FF;" | GJ&nbsp;1245&nbsp;A
| style="background: {{star-color|M}};" | M5.5V<ref5VAAAA name=RECONS/>BBBB
| 13.46<ref46AAAA name=RECONS/>BBBB
| 15.17<ref17AAAA name=RECONS/>BBBB
| {{?}}
| {{RA|19|53|54.2}}
| {{DEC|+44|24|55}}
| rowspan="3" align=left | 0.220&nbsp;20(1&nbsp;00)″<ref″AAAA name="Y"/>BBBB
| rowspan="3" | 14.812(67)
| rowspan="3" |
|-
| style="background: #E0E0FF;" | GJ&nbsp;1245&nbsp;B
| style="background: {{star-color|M}};" | M6.0V<ref0VAAAA name=RECONS/>BBBB
| 14.01<ref01AAAA name=RECONS/>BBBB
| 15.72<ref72AAAA name=RECONS/>BBBB
| {{?}}
| {{RA|19|53|55.2}}
خط ۶۶۹:
| style="background: #E0E0FF;" | GJ&nbsp;1245&nbsp;C
| style="background: {{star-color|M}};" | M?
| 16.75<ref75AAAA name=RECONS/>BBBB
| 18.46<ref46AAAA name=RECONS/>BBBB
| {{?}}
| {{RA|19|53|54.2}}
خط ۶۷۷:
| style="background: #E0E0FF;" | 39
| colspan="2" style="background: #E0E0FF;" | [[جی‌جی ۴۴۰|GJ&nbsp;440]] (WD&nbsp;1142-645)
| style="background: #F0F0F0" | [[کوتوله سفید|DQ6]]<refAAAA name=RECONS/>BBBB
| 11.50<ref50AAAA name=RECONS/>BBBB
| 13.18<ref18AAAA name=RECONS/>BBBB
| align=left | &nbsp;7,500
| {{RA|11|45|42.9}}
| {{DEC|−64|50|29}}
|align=left | 0.216&nbsp;57(2&nbsp;01)″<ref″AAAA name="Y"/><refBBBBAAAA name="H"/>BBBB
| 15.060(140)
|
خط ۶۸۹:
| style="background: #E0E0FF;" | 40
| colspan="2" style="background: #E0E0FF;" | [[جی‌جی ۱۰۰۲|GJ&nbsp;1002]]
| style="background: {{star-color|M}};" | M5.5V<ref5VAAAA name=RECONS/>BBBB
| 13.76<ref76AAAA name=RECONS/>BBBB
| 15.40<ref40AAAA name=RECONS/>BBBB
| {{?}}
| {{RA|00|06|43.8}}
| {{DEC|−07|32|22}}
| align=left | 0.213&nbsp;00(3&nbsp;60)″<ref″AAAA name="Y"/>BBBB
| 15.313(259)
|
خط ۷۰۱:
| style="background: #E0E0FF;" | 41
| colspan="2" style="background: #E0E0FF;" | [[گلیز ۸۷۶|Ross&nbsp;780]] (GJ&nbsp;876)
| style="background: {{star-color|M}};" | M3.5V<ref5VAAAA name=RECONS/>BBBB
| 10.17<ref17AAAA name=RECONS/>BBBB
| 11.81<ref81AAAA name=RECONS/>BBBB
| align=left | &nbsp;3,480
| {{RA|22|53|16.7}}
| {{DEC|−14|15|49}}
| align=left | 0.212&nbsp;59(1&nbsp;96)″<ref″AAAA name="Y"/><refBBBBAAAA name="H"/>BBBB
| 15.342(141)
|
خط ۷۱۳:
| style="background: #E0E0FF;" | 42
| colspan="2" style="background: #E0E0FF;" | [[ال‌اچ‌اس ۲۸۸|LHS&nbsp;288]] (Luyten&nbsp;143-23)
| style="background: {{star-color|M}};" | M5.5V<ref5VAAAA name=RECONS/>BBBB
| 13.90<ref90AAAA name=RECONS/>BBBB
| 15.51<ref51AAAA name=RECONS/>BBBB
| {{?}}
| {{RA|10|44|21.2}}
| {{DEC|−61|12|36}}
| align=left | 0.208&nbsp;95(2&nbsp;73)″<ref″AAAA name="recent"/>BBBB
| 15.610(204)
| <refAAAA name=henry2006/>BBBB
|-
| rowspan="2" style="background: #E0E0FF;" | 43
| rowspan="2" style="background: #E0E0FF;" | [[گلیز ۴۱۲|GJ&nbsp;412]]
| style="background: #E0E0FF;" | GJ&nbsp;412&nbsp;A
| style="background: {{star-color|M}};" | M1.0V<ref0VAAAA name=RECONS/>BBBB
| 8.77<ref77AAAA name=RECONS/>BBBB
| 10.34<ref34AAAA name=RECONS/>BBBB
| {{?}}
| {{RA|11|05|28.6}}
| {{DEC|+43|31|36}}
| rowspan="2" align=left | 0.206&nbsp;02(1&nbsp;08)″<ref″AAAA name="Y"/><refBBBBAAAA name="H"/>BBBB
| rowspan="2" | 15.832(83)
| rowspan="2" |
|-
| style="background: #E0E0FF;" | GJ&nbsp;412&nbsp;B (WX&nbsp;Ursae&nbsp;Majoris)
| style="background: {{star-color|M}};" | M5.5V<ref5VAAAA name=RECONS/>BBBB
| 14.48<ref48AAAA name=RECONS/>BBBB
| 16.05<ref05AAAA name=RECONS/>BBBB
| {{?}}
| {{RA|11|05|30.4}}
خط ۷۴۶:
| style="background: #E0E0FF;" | 44
| colspan="2" style="background: #E0E0FF;" | [[گروم‌بریج ۱۶۱۸|Groombridge&nbsp;1618]] (GJ&nbsp;380)
| style="background: {{star-color|K}};" | [[K V star|K7.0V]]<refAAAA name=RECONS/>BBBB
| 6.59<ref59AAAA name=RECONS/>BBBB
| 8.16<ref16AAAA name=RECONS/>BBBB
| align=left | &nbsp;4,000
| {{RA|10|11|22.1}}
| {{DEC|+49|27|15}}
|align=left | 0.205&nbsp;81(0&nbsp;67)″<ref″AAAA name="Y"/><refBBBBAAAA name="H"/>BBBB
| 15.848(52)
|
خط ۷۵۸:
| style="background: #E0E0FF;" | 45
| colspan="2" style="background: #E0E0FF;" | [[ای‌دی شیر|GJ&nbsp;388]]
| style="background: {{star-color|M}};" | M3.0V<ref0VAAAA name=RECONS/>BBBB
| 9.32<ref32AAAA name=RECONS/>BBBB
| 10.87<ref87AAAA name=RECONS/>BBBB
| {{?}}
| {{RA|10|19|36.4}}
| {{DEC|+19|52|10}}
| align=left | 0.204&nbsp;60(2&nbsp;80)″<ref″AAAA name="Y"/>BBBB
| 15.942(218)
|
خط ۷۷۰:
| style="background: #E0E0FF;" | 46
| colspan="2" style="background: #E0E0FF;" | [[گلیز ۸۳۲|GJ&nbsp;832]]
| style="background: {{star-color|M}};" | M3.0V<ref0VAAAA name=RECONS/>BBBB
| 8.66<ref66AAAA name=RECONS/>BBBB
| 10.20<ref20AAAA name=RECONS/>BBBB
| {{?}}
| {{RA|21|33|34.0}}
| {{DEC|−49|00|32}}
| align=left | 0.202&nbsp;78(1&nbsp;32)″<ref″AAAA name="Y"/><refBBBBAAAA name="H"/>BBBB
| 16.085(105)
|
خط ۷۸۲:
| style="background: #E0E0FF;" | 47
| colspan="2" style="background: #E0E0FF;" | [[ال‌پی ۹۴۴-۰۲۰|LP&nbsp;944-020]]
| style="background: {{star-color|M}};" | M9.0V<ref0VAAAA name=RECONS/>BBBB
| 18.50<ref50AAAA name=RECONS/>BBBB
| 20.02<ref02AAAA name=RECONS/>BBBB
| {{?}}
| {{RA|03|39|35.2}}
| {{DEC|−35|25|41}}
| align=left | 0.201&nbsp;40(4&nbsp;20)″<ref″AAAA name="T">BBBB[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>refBBBB
| 16.195(338)
|
خط ۷۹۴:
| style="background: #E0E0FF;" | 48
| colspan="2" style="background: #E0E0FF;" | [[دی‌ای‌ان ۰۲۵۵-۴۷۰۰|DEN&nbsp;0255-4700]]
| style="background: {{star-color|L}};" | [[کوتوله قهوه‌ای|L7.5V]]<refAAAA name=RECONS/>BBBB
| 22.92<ref92AAAA name=RECONS/>BBBB
| 24.44<ref44AAAA name=RECONS/>BBBB
| {{?}}
| {{RA|02|55|03.7}}
| {{DEC|−47|00|52}}
| align=left | 0.201&nbsp;37(3&nbsp;89)″<ref″AAAA name="recent"/>BBBB
| 16.197(313)
| <refAAAA name=costa2005/>BBBB
|-
| style="background: #E0E0FF;" | 49
| colspan="2" style="background: #E0E0FF;" | [[گلیز ۶۸۲|GJ&nbsp;682]]
| style="background: {{star-color|M}};" | M4.5V<ref5VAAAA name=RECONS/>BBBB
| 10.95<ref95AAAA name=RECONS/>BBBB
| 12.45<ref45AAAA name=RECONS/>BBBB
| {{?}}
| {{RA|17|37|03.7}}
| {{DEC|−44|19|09}}
| align=left | 0.199&nbsp;65(2&nbsp;30)″<ref″AAAA name="Y"/><refBBBBAAAA name="H"/>BBBB
| 16.337(188)
|
|-
! rowspan="2" |#
!<small>smallBBBB[[سامانه ستاره‌ای|System]]</small>smallBBBB
!<small>smallBBBB[[ستاره]]</small>smallBBBB
! rowspan="2" |<small>smallBBBB[[رده‌بندی ستارگان|Stellar class]]</small>smallBBBB
! rowspan="2" |<small>smallBBBB[[قدر ظاهری|''m'']]<sub>subBBBB[[UBV photometric system|''V'']]</sub>subBBBB</small>smallBBBB
! rowspan="2" |<small>smallBBBB[[قدر مطلق (ستاره‌شناسی)|''M'']]<sub>subBBBB[[UBV photometric system|''V'']]</sub>subBBBB</small>smallBBBB
! rowspan="2" |<small>smallBBBB[[Effective temperature|''T<sub>effsubBBBBeff</sub>subBBBB'']]{{سخ}}[[کلوین|K]][[margin of error|(±err)]]</small>smallBBBB
!<small>smallBBBB[[بعد (ستاره‌شناسی)|RA]]<refAAAA name=RECONS/>BBBB</small>smallBBBB
!<small>smallBBBB[[میل (ستاره‌شناسی)|Dec]]<refAAAA name=RECONS/>BBBB</small>smallBBBB
! rowspan="2" |<small>smallBBBB[[اختلاف منظر]]<refAAAA name="RECONS"/><refBBBBAAAA name=plxfn/>BBBB{{سخ}}[[دقیقه قوسی|Arcseconds]][[margin of error|(±err)]]</small>smallBBBB
! rowspan="2" |<small>smallBBBB[[فاصله]]<refAAAA name=distfn/>BBBB{{سخ}}[[سال نوری|Light-years]][[margin of error|(±err)]]</small>smallBBBB
! rowspan="2" |<small>smallBBBB[[#References|Additional{{سخ}}references]]</small>smallBBBB
|-
! colspan="2" |<small>DesignationsmallBBBBDesignation</small>smallBBBB
! style="background: #FFC" colspan="2" |<small>smallBBBB[[مبدأ (ستاره‌شناسی)|Epoch]] J2000.0</small>smallBBBB
|}
 
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