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فهرست ستارگان نزدیک: تفاوت میان نسخه‌ها

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ربات‌ها، مدیران رباتیک
۴٬۴۱۱٬۲۶۸ ویرایش‌ها
جز ←‏فهرست: دارای عبارت جادویی، + ماژول ابرابزار با استفاده از AWB
خط ۸:
! colspan="2" |<small>نامگذاری</small>
! rowspan="2" |<small>[[رده‌بندی ستارگان|رده‌بندی]]</small>
! rowspan="2" |<small>''''[[قدر ظاهری|''m'']]''<sub>[[سیستم فتومتریک UBV|V]]''</sub></small>
! rowspan="2" |<small>''''[[قدر مطلق (اخترشناسی)|''M'']]''<sub>[[سیستم فتومتریک UBV|V]]''</sub></small>
! rowspan="2" |<small>[[دمای موثر|''T<sub>eff</sub>'']]{{سخ}}[[کلوین|K]][[margin of error|(±err)]]</small>
! style="background: #FFC" colspan="2" |<small>[[مبدأ (ستاره‌شناسی)|مبدا]] [[مبدأ (ستاره‌شناسی)]]</small>
خط ۱۸:
!<small>[[سامانه ستاره‌ای|سامانه]]</small>
!<small>[[ستاره]]</small>
!<small>[[بعد]]<ref name=RECONS /></small>
!<small>[[میل]]<ref name=RECONS /></small>
|-
|style="background: #FFFFFF;" |
|style="background: #FFFFFF;" | [[منظومه خورشیدی]]
|style="background: #FFFFFF;" | [[خورشید]] (Sol)
| style="background: {{star-color|G}};" | [[ستاره نوع جی|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. Accessed on line [[۸ نوامبر]]، [[2007]].</ref>
| —
| —
خط ۳۵:
|-
| style="background: #FFFFFF;" rowspan="3" | ۱
| style="background: #FFFFFF;" rowspan="3" | [[آلفا قنطورس]]{{سخ}}(Rigil&nbsp; Kentaurus; Toliman)
| style="background: #E0E0FF;" | [[پروکسیما قنطورس]] (V645&nbsp; Centauri)
| style="background: {{star-color|M}};" | [[کوتوله سرخ|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|−۶۲|۴۰|۴۶}}
| align=left | 0.768&nbsp; 87(0&nbsp; 29)″<ref name="Y">[[کاتالوگ ستاره‌ای]].</ref><ref name="H">[[کاتالوگ ابرخس]].</ref>
| ۴٫۲۴۲1(16)
|<ref name="B">Burgasser et al. 2000</ref>
|-
|style="background: #FFFFFF;" | α&nbsp; Centauri&nbsp; A (HD&nbsp; 128620)
| style="background: {{star-color|G}};" | [[ستاره نوع جی|G2V]]<ref name=RECONS />
| 0.01<ref name=RECONS />
| 4.38<ref name=RECONS />
| align=left | &nbsp;5,790<ref name="ESO2003">{{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>
| {{RA|14|39|36.5}}
| {{DEC|−۶۰|۵۰|۰۲}}
| rowspan="2" align=left | 0.747&nbsp; 23(1&nbsp; 17)″<ref name="Y" /><ref name="S">[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>
| rowspan="2" | ۴٫۳۶۵0(68)
| rowspan="2" |
|-
|style="background: #FFFFFF;" | α&nbsp; Centauri&nbsp; B (HD&nbsp; 128621)
| style="background: {{star-color|K}};" | [[K V star|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|−۶۰|۵۰|۱۴}}
خط ۶۹:
| colspan="2" style="background: #E0E0FF;" | [[ستاره بارنارد]] (BD+04°3561a)
| style="background: {{star-color|M}};" | 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" />
| ۵٫۹۶۳0(109)
|
|-
| style="background: #E0E0FF;" | ۳
| colspan="2" style="background: #E0E0FF;" | [[ولف ۳۵۹|Wolf&nbsp; 359]] (CN&nbsp; Leonis)
| style="background: {{star-color|M}};" | M6.0V<ref name=RECONS />
| 13.44<ref name=RECONS />
| 16.55<ref name=RECONS />
| align=left | &nbsp;2,800(100)<ref name="aaa447">{{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"> [http://dx.doi.org/%7B%7Burlencode:10.1051/0004-6361:20052979}} <nowiki>10.1051/0004-6361:20052979</nowiki>]</span>}}</ref>
| {{RA|10|56|29.2}}
| {{DEC|+07|00|53}}
|align=left | 0.419&nbsp; 10(2&nbsp; 10)″<ref name="Y" />
| ۷٫۷۸۲5(390)
|
|-
| style="background: #E0E0FF;" | ۴
| colspan="2" style="background: #E0E0FF;" | [[Lalande 21185|Lalande&nbsp;21185]] (BD+36°۲۱۴۷)
| style="background: {{star-color|M}};" | 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" />
| ۸٫۲۹۰5(148)
|
|-
| rowspan="2" style="background: #FFFFFF;" | ۵
| 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]]<ref name=RECONS />
| −1.43<ref name=RECONS />
| 1.47<ref name=RECONS />
| align=left | &nbsp;9,940(210)<ref>Table 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>
| rowspan="2" | {{RA|06|45|08.9}}
| rowspan="2" | {{DEC|−۱۶|۴۲|۵۸}}
| rowspan="2" align=left | 0.380&nbsp; 02(1&nbsp; 28)″<ref name="Y" /><ref name="H" />
| rowspan="2" | ۸٫۵۸۲8(289)
| rowspan="2" |
|-
| style="background: #E0E0FF;" | Sirius&nbsp; B
| style="background: F0F0F0" | [[کوتوله سفید|DA2]]<ref name=RECONS />
| 8.44<ref name=RECONS />
| 11.34<ref name=RECONS />
| align=left | 25,000(200)<ref>Adopted 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>
|-
| rowspan="2" style="background: #E0E0FF;" | ۶
| rowspan="2" style="background: #E0E0FF;" | [[Luyten 726-8|Luyten&nbsp;726-8]]
| style="background: #E0E0FF;" | Luyten&nbsp; 726-8&nbsp; A (BL&nbsp; Ceti)
| style="background: {{star-color|M}};" | 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|−۱۷|۵۷|۰۱}}
| rowspan="2" align=left | 0.373&nbsp; 70(2&nbsp; 70)″<ref name="Y" />
| rowspan="2" | ۸٫۷۲۸0(631)
| rowspan="2" |
|-
| style="background: #E0E0FF;" | Luyten&nbsp; 726-8&nbsp; B (UV&nbsp; Ceti)
| style="background: {{star-color|M}};" | M6.0Ve
| 12.99<ref name=RECONS />
| 15.85<ref name=RECONS />
| align=left | ~۲٬۶۰۰
|-
| style="background: #E0E0FF;" | ۷
| colspan="2" style="background: #E0E0FF;" | [[روس ۱۵۴|Ross&nbsp; 154]] (V1216&nbsp; Sagittarii)
| style="background: {{star-color|M}};" | M3.5Ve
| 10.43<ref name=RECONS />
| 13.07<ref name=RECONS />
| align=left | &nbsp;2,700
| {{RA|18|49|49.4}}
| {{DEC|−۲۳|۵۰|۱۰}}
| align=left | 0.336&nbsp; 90(1&nbsp; 78)″<ref name="Y" /><ref name="H" />
| ۹٫۶۸۱3(512)
|
|-
| style="background: #E0E0FF;" | ۸
| colspan="2" style="background: #E0E0FF;" | [[روس ۲۴۸|Ross&nbsp; 248]] (HH&nbsp; Andromedae)
| 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 | 0.316&nbsp; 00(1&nbsp; 10)″<ref name="Y" />
| ۱۰٫۳۲2(36)
|
خط ۱۶۶:
| ۹
| colspan="2" | [[اپسیلون جوی]] (BD−۰۹°۶۹۷)
| style="background: {{star-color|K}};" | [[K V star|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|−۰۹|۲۷|۳۰}}
|align=left | 0.309&nbsp; 99(0&nbsp; 79)″<ref name="Y" /><ref name="H" />
| ۱۰٫۵۲2(27)
|
|-
| style="background: #E0E0FF;" | ۱۰
| colspan="2" style="background: #E0E0FF;" | [[Lacaille 9352|Lacaille&nbsp;9352]] (CD−۳۶°۱۵۶۹۳)
| style="background: {{star-color|M}};" | M1.5Ve
| 7.34<ref name=RECONS />
| 9.75<ref name=RECONS />
| align=left | &nbsp;3,340
| {{RA|23|05|52.0}}
| {{DEC|−۳۵|۵۱|۱۱}}
| align=left | 0.303&nbsp; 64(0&nbsp; 87)″<ref name="Y" /><ref name="H" />
| ۱۰٫۷۴2(31)
|
|-
| style="background: #E0E0FF;" | ۱۱
| colspan="2" style="background: #E0E0FF;" | [[روس ۱۲۸|Ross&nbsp; 128]] (FI&nbsp; Virginis)
| style="background: {{star-color|M}};" | 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" />
| ۱۰٫۹۱9(49)
|
|-
| rowspan="3" style="background: #E0E0FF;" | ۱۲
| 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
<!---It is also known as
[[Henry-Lee Giclas|G]] 156-031,
خط ۲۰۹:
Luyten 0789-006. --->
| 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|−۱۵|۱۸|۰۷}}
| rowspan="3" align=left | 0.289&nbsp; 50(4&nbsp; 40)″<ref name="Y" />
| rowspan="3" | ۱۱٫۲۶6(171)
| rowspan="3" |
|-
| style="background: #E0E0FF;" | EZ&nbsp; Aquarii&nbsp; B
| style="background: {{star-color|M}};" | M?
| 13.27<ref name=RECONS />
| 15.58<ref name=RECONS />
| {{?}}
|-
| style="background: #E0E0FF;" | EZ&nbsp; Aquarii&nbsp; C
| style="background: {{star-color|M}};" | M?
| 14.03<ref name=RECONS />
| 16.34<ref name=RECONS />
| {{?}}
|-
| rowspan="2" | ۱۳
| rowspan="2" | [[شعرای شامی]]{{سخ}}(α&nbsp; Canis&nbsp; Minoris)
| Procyon&nbsp; A
| style="background: {{star-color|F}}" | 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" | ۱۱٫۴۰2(32)
| rowspan="2" |
|-
| style="background: #E0E0FF;" | Procyon&nbsp; B
| style="background: #F0F0F0" | [[کوتوله سفید|DA]]<ref name=RECONS />
| 10.70<ref name=RECONS />
| 12.98<ref name=RECONS />
| align=left | &nbsp;9,700
|-
| rowspan="2" | ۱۴
| rowspan="2" | [[۶۱ ماکیان|61&nbsp; Cygni]]
| 61&nbsp; Cygni&nbsp; A (BD+۳۸°۴۳۴۳)
| style="background: {{star-color|K}};" | [[K V star|K5.0V]]<ref name=RECONS /> <!--previous: K3.5Ve-->
| 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" | ۱۱٫۴۰3(22)
| rowspan="2" |
|-
| 61&nbsp; Cygni&nbsp; B (BD+۳۸°۴۳۴۴)
| style="background: {{star-color|K}};" | [[K V star|K7.0V]]<ref name=RECONS /> <!--previous: K4.7Ve-->
| 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: #E0E0FF;" | ۱۵
| rowspan="2" style="background: #E0E0FF;" | [[Struve 2398|Struve&nbsp;2398]]{{سخ}}(GJ&nbsp; 725, BD+59°۱۹۱۵)
| style="background: #E0E0FF;" | Struve&nbsp; 2398&nbsp; A (HD&nbsp; 173739)
| 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 | 0.283&nbsp; 00(1&nbsp; 69)″<ref name="Y" /><ref name="H" />
| rowspan="2" | ۱۱٫۵۲5(69)
| rowspan="2" |
|-
| style="background: #E0E0FF;" | Struve&nbsp; 2398&nbsp; B (HD&nbsp; 173740)
 
| 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}}
خط ۲۹۳:
|-
| rowspan="2" style="background: #E0E0FF;" | ۱۶
| 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)
<!---It is also known as
[[Henry Draper catalogue|HD]] 1326,
خط ۳۰۲:
[[Luyten Half-Second catalogue|LHS]] 3 and
[[Alexander N. Vyssotsky|Vyssotsky]] 85. --->
| 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 | 0.280&nbsp; 59(0&nbsp; 95)″<ref name="Y" /><ref name="H" />
| rowspan="2" | ۱۱٫۶۲4(39)
| rowspan="2" |
|-
| style="background: #E0E0FF;" | Groombridge&nbsp; 34&nbsp; B (GQ&nbsp; Andromedae)
<!---It is also known as
[[Henry-Lee Giclas|G]] 171-048 and
[[Luyten Half-Second catalogue|LHS]] 4. --->
| style="background: {{star-color|M}};" | M3.5V<ref name=RECONS />
| 11.06<ref name=RECONS />
| 13.30<ref name=RECONS />
| {{?}}
|-
| rowspan="3" | ۱۷
| rowspan="3" | [[اپسیلون هندی|Epsilon&nbsp; Indi]]{{سخ}}(CPD−۵۷°۱۰۰۱۵)
| Epsilon Indi A
| style="background: {{star-color|K}};" | [[K V star|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|−۵۶|۴۷|۱۰}}
| rowspan="3" align=left | 0.275&nbsp; 84(0&nbsp; 69)″<ref name="Y" /><ref name="H" />
| rowspan="3" | ۱۱٫۸۲4(30)
| rowspan="3" |
|-
| style="background: #E0E0FF;" | Epsilon&nbsp; Indi&nbsp; Ba
| style="background: {{star-color|T}};" | [[کوتوله قهوه‌ای|T1.0V]]
|>۲۳
|>۲۵
| align=left | &nbsp;1,280
| rowspan="2" | {{RA|22|04|10.5}}
| rowspan="2" | {{DEC|−۵۶|۴۶|۵۸}}
|-
| style="background: #E0E0FF;" | Epsilon&nbsp; Indi&nbsp; Bb
| style="background: {{star-color|T}};" | [[کوتوله قهوه‌ای|T6.0V]]
|>۲۳
|>۲۵
| align=left | &nbsp;&nbsp;&nbsp;850
|-
| style="background: #E0E0FF;" | ۱۸
| colspan="2" style="background: #E0E0FF;" | [[دی‌ایکس خرچنگ|DX&nbsp; Cancri]] (G&nbsp; 51-15)
<!---It is also known as
[[Henry-Lee Giclas|G]] 051-015,
خط ۳۵۵:
[[Luyten Half-Second catalogue|LHS]] 248. --->
| 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 | 0.275&nbsp; 80(3&nbsp; 00)″<ref name=Y />
| ۱۱٫۸۲6(129)
|
|-
| ۱۹
| colspan="2" | [[تاو نهنگ|Tau&nbsp; Ceti]] (BD−۱۶°۲۹۵)
| style="background: {{star-color|G}};" | [[ستاره نوع جی|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|−۱۵|۵۶|۱۵}}
| align=left | 0.274&nbsp; 39(0&nbsp; 76)″<ref name="Y" /><ref name="H" />
| ۱۱٫۸۸7(33)
|
|-
| style="background: #E0E0FF;" | ۲۰
| colspan="2" style="background: #E0E0FF;" | [[جی‌جی ۱۰۶۱|GJ&nbsp; 1061]] (LHS&nbsp; 1565)
| 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|−۴۴|۳۰|۴۵}}
| align=left | 0.272&nbsp; 01(1&nbsp; 30)″<ref name="recent">Systems with their first accurate trigonometric parallaxes measured by RECONS</ref>
| ۱۱٫۹۹1(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: #E0E0FF;" | ۲۱
| colspan="2" style="background: #E0E0FF;" | [[وای‌زد نهنگ|YZ&nbsp; Ceti]] (LHS&nbsp; 138)
<!---It is also known as
[[Henry-Lee Giclas|G]] 268-135,
خط ۳۹۶:
Luyten 0725-032 and
[[Luyten Two-Tenths catalogue|LTT]] 670. --->
| 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|−۱۶|۵۹|۵۶}}
| align=left | 0.268&nbsp; 84(2&nbsp; 95)″<ref name="Y" /><ref name="H" />
| ۱۲٫۱۳2(133)
|
|-
| style="background: #E0E0FF;" | ۲۲
| colspan="2" style="background: #E0E0FF;" | [[Luyten's Star|Luyten's&nbsp;Star]] (BD+05°۱۶۶۸)
| 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 | 0.263&nbsp; 76(1&nbsp; 25)″<ref name="Y" /><ref name="H" />
| ۱۲٫۳۶6(59)
|
|-
| style="background: #E0E0FF;" | ۲۳
| colspan="2" style="background: #E0E0FF;" | [[ستاره باغ چای|Teegarden's&nbsp; star]] (SO025300.5+165258)
| 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 | 0.260&nbsp; 63(2&nbsp; 69)″<ref name=recent />
| ۱۲٫۵۱4(129)
|<ref name=henry2006 />
|-
| rowspan="2" style="background: #E0E0FF;" | ۲۴
| 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<ref name=RECONS />
| ۱۷٫۳۹
| ۱۹٫۴۱
خط ۴۳۹:
| {{RA|18|45|05.3}}
| {{DEC|−۶۳|۵۷|۴۸}}
| rowspan=2 align=left | 0.259&nbsp; 45(1&nbsp; 11)″<ref name="recent" />
| rowspan=2 | ۱۲٫۵۷1(54)
| rowspan=2 |<ref name=henry2006 />
|-
| style="background: #E0E0FF;" | SCR&nbsp; 1845-6357&nbsp; B
| style="background: {{star-color|T}};" | [[کوتوله قهوه‌ای|T6]]<ref name=nearmt>[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>
| {{?}}
| {{?}}
| align=left | &nbsp;&nbsp;&nbsp;950<ref name=nearmt />
| {{RA|18|45|02.6}}
| {{DEC|−۶۳|۵۷|۵۲}}
|-
| style="background: #E0E0FF;" | ۲۵
| colspan="2" style="background: #E0E0FF;" | [[ستاره کاپتین|Kapteyn's&nbsp; Star]] (CD−۴۵°۱۸۴۱)
| style="background: {{star-color|M}};" | M1.5V<ref name=RECONS /> <!--previous: sdM0VI-->
| 8.84<ref name=RECONS />
| 10.87<ref name=RECONS />
| align=left | &nbsp;3,800
| {{RA|05|11|40.6}}
| {{DEC|−۴۵|۰۱|۰۶}}
| align=left | 0.255&nbsp; 27(0&nbsp; 86)″<ref name="Y" /><ref name="H" />
| ۱۲٫۷۷7(43)
|
|-
| style="background: #E0E0FF;" | ۲۶
| colspan="2" style="background: #E0E0FF;" | [[Lacaille 8760|Lacaille&nbsp;8760]] (AX&nbsp; Microscopii)
<!---It is also known as
[[Henry Draper catalogue|HD]] 202560,
خط ۴۷۰:
[[کاتالوگ ستاره‌ای|GCTP]] 5117.00,
[[Luyten Half-Second catalogue|LHS]] 66 and UGPMF 518. --->
| style="background: {{star-color|M}};" | M0.0V<ref name=RECONS /> <!--previous: M2Ve-->
| 6.67<ref name=RECONS />
| 8.69<ref name=RECONS />
| align=left | &nbsp;3,340
| {{RA|21|17|15.3}}
| {{DEC|−۳۸|۵۲|۰۳}}
| align=left | 0.253&nbsp; 43(1&nbsp; 12)″<ref name="Y" /><ref name="H" />
| ۱۲٫۸۷0(57)
|
|-
| rowspan="2" style="background: #E0E0FF;" | ۲۷
| rowspan="2" style="background: #E0E0FF;" | [[کروگر ۶۰|Kruger&nbsp; 60]]{{سخ}}(BD+56°۲۷۸۳)
| style="background: #E0E0FF;" | Kruger&nbsp; 60&nbsp; A
| style="background: {{star-color|M}};" | 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" | ۱۳٫۱۴9(74)
| rowspan="2" |
|-
| style="background: #E0E0FF;" | Kruger&nbsp; 60&nbsp; B (DO&nbsp; Cephei)
| style="background: {{star-color|M}};" | M4.0V<ref name=RECONS />
| 11.41<ref name=RECONS />
| 13.38<ref name=RECONS />
| align=left | &nbsp;2,890
|-
| style="background: #E0E0FF;" | ۲۸
| colspan="2" style="background: #E0E0FF;" | [[دی‌ای‌ان ۱۰۴۸-۳۹۵۶|DEN&nbsp; 1048-3956]]
| 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|−۳۹|۵۶|۰۶}}
| align=left | 0.247&nbsp; 71(1&nbsp; 55)″<ref name="recent" />
| ۱۳٫۱۶7(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: #E0E0FF;" | ۲۹
| 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)
<!---It is also known as
[[Henry-Lee Giclas|G]] 106-049,
[[کاتالوگ ستاره‌ای|GCTP]] 1509.00 and
[[Luyten Half-Second catalogue|LHS]] 1849. --->
| 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|−۰۲|۴۸|۵۰}}
| rowspan="2" align=left | 0.244&nbsp; 34(2&nbsp; 01)″<ref name="Y" /><ref name="S" />
| rowspan="2" | ۱۳٫۳۴9(110)
| rowspan="2" |
|-
| style="background: #E0E0FF;" | Ross&nbsp; 614B (LHS&nbsp; 1850)
<!---It is also known as
[[Luyten Half-Second catalogue|LHS]] 1850. --->
| style="background: {{star-color|M}};" | M5.5V
| 14.23<ref name=RECONS />
| 16.17<ref name=RECONS />
| {{?}}
|-
| style="background: #E0E0FF;" | ۳۰
| colspan="2" style="background: #E0E0FF;" | [[ولف ۱۰۶۱|Gl&nbsp; 628]] (Wolf&nbsp; 1061, BD−۱۲°۴۵۲۳)
<!---It is also known as
[[Bonner Durchmusterung|BD]]−۱۲°۴۵۲۳,
خط ۵۴۴:
[[Luyten Half-Second catalogue|LHS]] 419 and
[[Alexander N. Vyssotsky|Vyssotsky]] 164. --->
| 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|−۱۲|۳۹|۴۵}}
| align=left | 0.236&nbsp; 01(1&nbsp; 67)″<ref name="Y" /><ref name="H" />
| ۱۳٫۸۲0(98)
|
|-
| style="background: #E0E0FF;" | ۳۱
| 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]]<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" />
| ۱۴٫۰۶6(109)
|
|-
| style="background: #E0E0FF;" | ۳۲
| colspan="2" style="background: #E0E0FF;" | [[گلیز ۱|Gl&nbsp; 1]] (CD−۳۷°۱۵۴۹۲)
 
| style="background: {{star-color|M}};" | M3.0V<ref name=RECONS />
| 8.55<ref name=RECONS />
| 10.35<ref name=RECONS />
| {{?}}
| {{RA|00|05|24.4}}
| {{DEC|−۳۷|۲۱|۲۷}}
| align=left | 0.229&nbsp; 20(1&nbsp; 07)″<ref name="Y" /><ref name="H" />
| ۱۴٫۲۳1(66)
|
|-
| rowspan="2" style="background: #E0E0FF;" | ۳۳
| rowspan="2" style="background: #E0E0FF;" | [[ولف ۴۲۴|Wolf&nbsp; 424]]{{سخ}}(FL&nbsp; Virginis, LHS&nbsp; 333, GJ&nbsp; 473)
| style="background: #E0E0FF;" | Wolf&nbsp; 424&nbsp; A
 
| 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 | 0.227&nbsp; 90(4&nbsp; 60)″<ref name="Y" />
| rowspan="2" | ۱۴٫۳۱2(289)
| rowspan="2" |
|-
| style="background: #E0E0FF;" | Wolf&nbsp; 424&nbsp; B
| style="background: {{star-color|M}};" | M7Ve
| 13.17<ref name=RECONS />
| 14.96<ref name=RECONS />
| {{?}}
|-
| style="background: #E0E0FF;" | ۳۴
| 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<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" />
| ۱۴٫۵۰9(187)
|
|-
| style="background: #E0E0FF;" | ۳۵
| colspan="2" style="background: #E0E0FF;" | [[گلیز ۶۸۷|Gl&nbsp; 687]] (LHS&nbsp; 450, BD+68°۹۴۶)
| 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 | 0.220&nbsp; 49(0&nbsp; 82)″<ref name="Y" /><ref name="H" />
| ۱۴٫۷۹3(55)
|
|-
| style="background: #E0E0FF;" | ۳۶
| colspan="2" style="background: #E0E0FF;" | [[ال‌اچ‌اس ۲۹۲|LHS&nbsp; 292]] (LP&nbsp; 731-58)
| 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|−۱۱|۲۰|۱۴}}
| align=left | 0.220&nbsp; 30(3&nbsp; 60)″<ref name="Y" />
| ۱۴٫۸۰5(242)
|
|-
| style="background: #E0E0FF;" | ۳۷
| colspan="2" style="background: #E0E0FF;" | [[گلیز ۶۷۴|Gl&nbsp; 674]] (LHS&nbsp; 449)
| 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|−۴۶|۵۳|۴۳}}
| align=left | 0.220&nbsp; 25(1&nbsp; 59)″<ref name="Y" /><ref name="H" />
| ۱۴٫۸۰9(107)
|
|-
| rowspan="3" style="background: #E0E0FF;" | ۳۸
| 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<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" | ۱۴٫۸۱2(67)
| rowspan="3" |
|-
| style="background: #E0E0FF;" | GJ&nbsp; 1245&nbsp; B
| 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}}
|-
| style="background: #E0E0FF;" | GJ&nbsp; 1245&nbsp; C
| style="background: {{star-color|M}};" | M?
| 16.75<ref name=RECONS />
| 18.46<ref name=RECONS />
| {{?}}
| {{RA|19|53|54.2}}
خط ۶۷۷:
|-
| style="background: #E0E0FF;" | ۳۹
| colspan="2" style="background: #E0E0FF;" | [[جی‌جی ۴۴۰|GJ&nbsp; 440]] (WD&nbsp; 1142-645)
| style="background: #F0F0F0" | [[کوتوله سفید|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|−۶۴|۵۰|۲۹}}
|align=left | 0.216&nbsp; 57(2&nbsp; 01)″<ref name="Y" /><ref name="H" />
| ۱۵٫۰۶0(140)
|
|-
| style="background: #E0E0FF;" | ۴۰
| colspan="2" style="background: #E0E0FF;" | [[جی‌جی ۱۰۰۲|GJ&nbsp; 1002]]
| 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|−۰۷|۳۲|۲۲}}
| align=left | 0.213&nbsp; 00(3&nbsp; 60)″<ref name="Y" />
| ۱۵٫۳۱3(259)
|
|-
| style="background: #E0E0FF;" | ۴۱
| colspan="2" style="background: #E0E0FF;" | [[گلیز ۸۷۶|Ross&nbsp; 780]] (GJ&nbsp; 876)
| style="background: {{star-color|M}};" | 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|−۱۴|۱۵|۴۹}}
| align=left | 0.212&nbsp; 59(1&nbsp; 96)″<ref name="Y" /><ref name="H" />
| ۱۵٫۳۴2(141)
|
|-
| style="background: #E0E0FF;" | ۴۲
| colspan="2" style="background: #E0E0FF;" | [[ال‌اچ‌اس ۲۸۸|LHS&nbsp; 288]] (Luyten&nbsp; 143-23)
| 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|−۶۱|۱۲|۳۶}}
| align=left | 0.208&nbsp; 95(2&nbsp; 73)″<ref name="recent" />
| ۱۵٫۶۱0(204)
|<ref name=henry2006 />
|-
| rowspan="2" style="background: #E0E0FF;" | ۴۳
| 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<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" | ۱۵٫۸۳2(83)
| rowspan="2" |
|-
| style="background: #E0E0FF;" | GJ&nbsp; 412&nbsp; B (WX&nbsp; Ursae&nbsp; Majoris)
| 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}}
خط ۷۴۶:
|-
| style="background: #E0E0FF;" | ۴۴
| colspan="2" style="background: #E0E0FF;" | [[گروم‌بریج ۱۶۱۸|Groombridge&nbsp; 1618]] (GJ&nbsp; 380)
| style="background: {{star-color|K}};" | [[K V star|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" />
| ۱۵٫۸۴8(52)
|
|-
| style="background: #E0E0FF;" | ۴۵
| colspan="2" style="background: #E0E0FF;" | [[ای‌دی شیر|GJ&nbsp; 388]]
| 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 | 0.204&nbsp; 60(2&nbsp; 80)″<ref name="Y" />
| ۱۵٫۹۴2(218)
|
|-
| style="background: #E0E0FF;" | ۴۶
| colspan="2" style="background: #E0E0FF;" | [[گلیز ۸۳۲|GJ&nbsp; 832]]
| style="background: {{star-color|M}};" | M3.0V<ref name=RECONS />
| 8.66<ref name=RECONS />
| 10.20<ref name=RECONS />
| {{?}}
| {{RA|21|33|34.0}}
| {{DEC|−۴۹|۰۰|۳۲}}
| align=left | 0.202&nbsp; 78(1&nbsp; 32)″<ref name="Y" /><ref name="H" />
| ۱۶٫۰۸5(105)
|
|-
| style="background: #E0E0FF;" | ۴۷
| colspan="2" style="background: #E0E0FF;" | [[ال‌پی ۹۴۴-۰۲۰|LP&nbsp; 944-020]]
| style="background: {{star-color|M}};" | M9.0V<ref name=RECONS />
| 18.50<ref name=RECONS />
| 20.02<ref name=RECONS />
| {{?}}
| {{RA|03|39|35.2}}
| {{DEC|−۳۵|۲۵|۴۱}}
| 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>
| ۱۶٫۱۹5(338)
|
|-
| style="background: #E0E0FF;" | ۴۸
| colspan="2" style="background: #E0E0FF;" | [[دی‌ای‌ان ۰۲۵۵-۴۷۰۰|DEN&nbsp; 0255-4700]]
| style="background: {{star-color|L}};" | [[کوتوله قهوه‌ای|L7.5V]]<ref name=RECONS />
| 22.92<ref name=RECONS />
| 24.44<ref name=RECONS />
| {{?}}
| {{RA|02|55|03.7}}
| {{DEC|−۴۷|۰۰|۵۲}}
| align=left | 0.201&nbsp; 37(3&nbsp; 89)″<ref name="recent" />
| ۱۶٫۱۹7(313)
|<ref name=costa2005 />
|-
| style="background: #E0E0FF;" | ۴۹
| colspan="2" style="background: #E0E0FF;" | [[گلیز ۶۸۲|GJ&nbsp; 682]]
| style="background: {{star-color|M}};" | M4.5V<ref name=RECONS />
| 10.95<ref name=RECONS />
| 12.45<ref name=RECONS />
| {{?}}
| {{RA|17|37|03.7}}
| {{DEC|−۴۴|۱۹|۰۹}}
| align=left | 0.199&nbsp; 65(2&nbsp; 30)″<ref name="Y" /><ref name="H" />
| ۱۶٫۳۳7(188)
|
خط ۸۲۱:
!<small>[[ستاره]]</small>
! rowspan="2" |<small>[[رده‌بندی ستارگان|Stellar class]]</small>
! rowspan="2" |<small>''''[[قدر ظاهری|''m'']]''<sub>[[UBV photometric system|V]]''</sub></small>
! rowspan="2" |<small>''''[[قدر مطلق (ستاره‌شناسی)|''M'']]''<sub>[[UBV photometric system|V]]''</sub></small>
! rowspan="2" |<small>[[Effective temperature|''T<sub>eff</sub>'']]{{سخ}}[[کلوین|K]][[margin of error|(±err)]]</small>
!<small>[[بعد (ستاره‌شناسی)|RA]]<ref name=RECONS /></small>
!<small>[[میل (ستاره‌شناسی)|Dec]]<ref name=RECONS /></small>
! rowspan="2" |<small>[[اختلاف منظر]]<ref name="RECONS" /><ref name=plxfn />{{سخ}}[[دقیقه قوسی|Arcseconds]][[margin of error|(±err)]]</small>
! rowspan="2" |<small>[[فاصله]]<ref name=distfn />{{سخ}}[[سال نوری|Light-years]][[margin of error|(±err)]]</small>
! rowspan="2" |<small>[[#References|Additional{{سخ}}references]]</small>
|-
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