恒星距离列表

1、恒星距离列表维基百科，自由的百科全书恒星距离列表 是依据距离的增加由近而远排列，最远的距离是5秒差距（16.308光年）。在这个距离内，包括 太阳系在内，已知的恒星系有 50个，共有65颗恒星和 4颗棕矮星。列于表内的恒星和棕矮星，刷上浅蓝色的是 视星等大于6.5不能以裸眼直接看见的。恒星和棕矮星的光谱则直接刷上相对应光谱的颜色（这些颜色是光谱呈现的颜色， 不是观测时实际见到的颜色）。有些视差和距离是RECONS测量的结果1，可能只是初步的测量数据。目录隐藏1恒星距离表2近距离恒星图3相关条目4参考资料5外部链接编辑恒星距离表名称TeffK（ 士 err）历元J2000.0距离同附 加#系统恒

2、星恒星类形mvMVrA1Dec1视差12” （士 err）光年（士 err）参 考 资 料太阳系太阳G2V1-26.72 14.8515,7784一一180°0.0000158（3）or approx.8光分半人马座15."114h 2-62o0.768 87比邻星M5.11.3,0409m 4340'464.2428(V645 Ce n tauri)5Ve09535.0 s(0 29) 671(16)半人马座a14h 3-60o1(Rigil K en taurus半人马座G2V0.04.35,7909m 3650'02a A(HD 128620)1181

3、5.5 s0.747 23Tolima n)4.365(117) 0(68)半人马座14h 3-60o69a BKOV1.35.75,2609m 35. s50'14(HD 128614115.121)17h 5+04°4M4.9.513.3,1347m 481'360.546 985.963巴纳德1120VeJ122(102).5ff(1 00) 0(109星(BD+04 3561a)3067)10h 5+07°0M6.16.2,800_m _ _6 290'530.419 107.782Wolf 359(CN Leo ni13.551(100)

4、113s)0V144.2 s(2 10) 65(390)11h 0+35°5M2.10.3m 208'120.393 428.290Lala nde 21185 (BD+17.413,400436°2147)0V74412.2 sff(0 70) 675(148)天狼星AA1V1-1./q11.4719,940(210) 106h 4-16o天狼星43735m 0842'580.380 028.5825（大犬座.9 sff(1 28) ” 8(289a )da28.411. 34125,000(200) 1467)天狼星B141鲁鲁15.01h 3-17o0

5、.373 708.728M5.12.4016坦 726-8坦 726-85Ve542,6709m 0157'01(2 70) 60(631A （鲸鱼J.3 s)座BL)鲁坦 726-815.M6.12.851B （鲸鱼12,6000Ve99座UV)18h 4-23°13.9m 4950'100.336 909.681Ross 154 (V1216 SaM3.10.07175Ve c12,700.4 sff(1 78) 3(512gittani)4367)23h 4+44°114.1m 540'300.316 008Ross 248 (HH Andro

6、M5.12.1791?.7 sff(1 10) 10.32medae)5Ve2962(36)03h 3-09o波江座K2V2m 5527'300.309 993.76.110.529Epsilo n(BD-09°61J15,100.8 sff(0 79) 2(27)396797)23h 0-35o5m 5251'110.303 641Lacaille 9352(CD -M1.7.39.7s10.74036° 15693)5Ve4513,340.0ff(0 87) 672(31)11h 4+00°413.7m 448'160.298 721R

7、oss 128 (FI VirgiM4.11.5112,80010.911OVn13.4 sff(1 35)"9(49)nis)15.EZ AquarM5.13.164?EZ Aquarii A0Ve33_ h 22 3-15 18'ii(GJ 866,15.*m _ _8 33070.289 5011.261EZ AquarM?13.LC16(171)2鲁坦 789-6ii B2758?.4 s(4 40) 6)16.EZ AquarM?14.03341?ii C1南河三南河三AF5V0.32.607h 3+05°10.286 0511.403（小犬座-IV 86

8、16,6509m 183'30(0 81) 2(32)a )1.1 sff67南河三BdA110.70112. 9819,70061 Cyg ni21h 0+38°4K5.5.27.4m6 53A4'581(BD+38°0V11914,640.9 s天鹅座4343)0.286 041(0 56) 11.404613(22)61 Cyg niK7. 0V16.08.321h 06m 55+38°467B4'31(BD+38°3114,440.3 sff4344)Struve 218h 4+59°3398 AM3.8.911

9、.2m 467'491610V11?.7 sffStruve 2(HD 1737039839)0.283 001(GJ 725,(1 69) 11.5255(69)BD+59 1915)Struve 2M3.11.18h 42m 46+59°7'33767398 B9.69515V191?.9 sff(HD 173740)GroombriM1.110.dge 34 A (GX An dr5V18.081321?0h 18 m+44°01Groombriomedae)22.91'230.280 5911.62dge 34s(0 95) 64(39)(G

10、J 15)GroombriM3.13.67dge 34 B (GQ An dr omedae)5V111.061301?22h 0-56o3m 2147'10Epsilo nK5V4.66.84,2801J1J1.7 sEpsilo nIndi Ae990.275 841Indi(0 69) 11.82(CPD- 5722h 07Epsilo nT1.-56o674(30)° 10015)Indi Ba0V>23>251,2804m 1046'58.5 sffEpsilo nT6.850>23 >25Indi Bb0V08h 2+26°

11、;416.9m 496'370.275 8011.821DX Ca ncri(G 51-15M6.14.9818)5Verc1?.5 sff(3 00)6(129786)01h 4-15oTau Ceti (G8V4m 0456'150.274 391BD- 16°23.45.611.8891J1J15,344.1 sff(0 76) 7(33)95)p986703h 3-44oM5.15.5m 5930'450.272 0116213.26111.9910GJ 1061 (LHS 1565)5V1cc1?.7 sff(1 30) 1(57)09157h01

12、1-16o21M4.12.0214.2m 3059'560.268 8412.13YZ Ceti (LHS 138)5V1171?.6 sff(2 95) 672(133)07h 2+05°111.7m 243'330.263 762鲁坦M3.9.897112.362星(BD+05 1668)5Vn61?.5 sff(1 25) 676(59)02h 5+16°517.3m 002'530.260 6312.51172Teeqarden's star(M6.15.cc14(1291422?.9 s(2 69) ”3S0025300.5+165

13、258)5V15)J18h 4-63oSCR 1845M8.17.19.5m 0557'485V1?s.3ffSCR 1845-6357 A39410.259 45172(1 11) 12.5718h 44-6357SCR 1845T61950-63 57'o52151(54)m5 02-6357 B8?18.6 sff2H Th/ 卡普:坦M1.8.810.3,80005h 1-45o0.255 2712.775V1871m5星(CD -45° 1841)41 4001'06(0 86) 7(43)M0. 0V1.6 sff6726Lacaille 8760

14、(AXMicroscopii)6.678.6913,34021h 1 7m 15.3 s-3852'ffo030.253 43(1 12) 6712.870(57)M3.11.Kruger 6C A0V19.77613,18022h 2+57°42Kruger 600 A97m 591'450.248 0613.147(BD+56°Kruger 6M4.13.5 sff(1 39) 699(74)2783)0 B0V111.13812,890(DO Ceph41ei)10h 4-39oM8.19.8m 1456'060.247 71192DEN 10

15、48-39565V117.一1371?.7 sff(1 55) 13.162839157(82)0Ross 614M4.13.Ross 614A(LHS 1845V111.115091?06h 2-02o2(V577 Mo9)9m 2348'500.244 34, 13.34no ceroti.4 sff(2 01)9(1109s,Ross 61416.69)GJ 234)BM5.14.23171?(LHS 1855V0)16h 3-12oM3.11.0m 1839'450.236 013Gl 628 (Wolf 1061,0V110.1931?s.1ff(1 67) 13.8

16、20BD12°4523)07670(98)00h 4+05°2DZ7114.9m 093'190.231 8814.063Van Maa nen's Star12.21111cc1?.9 sff(1 79) 6(109(Gl 35, LHS 7)3867)M3.10.00h 0-37o0.229 203Gl 1 (CD -37° 1549218.51m14.2320Vl135?5 2421'27(1 07) ” 1(66)5.4 sff67Wolf 424Wolf 424(FL Virg in is, 3LHS 333,GJ 473)Wol

17、f 4243 TZ Arietis (GJ 83.4 1, Luyte n 1159-16)3 Gl 687 (LHS 450,5BD+68 946)3 LHS 292 (LP 731-586 )3 Gl 674 (LHS 449)3GJ 12458GJ 1245GJ 1245GJ 124513.18114.12h 3971?+09°03m 1715.2 sff14.13.961171?02h 0+13°012._114.0m 133'08031?.2 sff2717h 3+68°29.17110. 891?6m 25.9 s0'ff2110h 4

18、-11o15.17.3218m 1220'14"1?.6 sff6017h 2-46o9.311. 0918m 3953'4381?.9 sffh19 5+44°213.15. 1713m 544'55461?.2 sff19h 5+44°214.15.7213m 554'561?.2 sff0118.19h 5+44°216.1461?3m 544'5575.2 sffM5.5VeM7Ve0.220 25M?OVM3.,1M6. 5V1M3. 0V1M4.5V1M6. 0V1(1 59) 670.227 90 (

19、4 60) 60.224 80(2 90) ”60.220 49(0 82)670.220 30(3 60) ”6M5. 5V10.220 20(1 00) 614.312(289)14.509(187)14.793(55)14.805(242)14.809(107)14.812(67)11h 4-64odq613.5m 4250'290.216 5715.063GJ 440 (WD 1142-6411.1817,50010(14091"1.9 sff(2 01) 5)5067)00h 0-07oM5.15.6m 4332'220.213 0015.314GJ 100

20、25V113.r J1401?.8 sff(3 60) ” 3(2590766)22h 5-14oM3.10.11.3m 1615'490.212 5915.344111Ross 780(GJ 876)5V1813,480.7 sff(1 96) 2(1411767)10h 4-61oM5.15.4m 2112'360.208 9515.61174LHS 288 (Luyte n 14113.125Vcc151?.2 sff(2 73) ” 0(2043-23)9015)11h 0+43°3M1.8.77110.5m 281'36GJ 412 A0V1341?

21、.6 sff0.206 024GJ 412(1 08) 15.83311h 02(83)GJ 412 B+43°367(WX UrsaM5.14.16.5m 301'18亠 15V48105?.4 sffe Majoris)10h 1+49°2K7.1m 22.1 s7'150.205 814Groombridge 1618(0V16.518.114,000ff(0 67) ” 15.844GJ 380)96678(52)10h 1+19°5M3.10.9m 362'100.204 6015.9445GJ 3880V19.32871?.4

22、sff(2 80) 62(218)_ . h _21 3-49 °4M3.0V18.610.2013m 3400'320.202 7816.086GJ 832.1?.0 sff(1 32)5(105667)03h 3-35 °4M9.18.J120.9m 3525'410.201 4016.19LP 944-0200V1021?.2 s(4 20) 5(33875021)02h 5-47 °L7.24.5m 0300'520.201 3716.192048DEN 0255-47005V122.921441?.7 s(3 89) 157(31

23、3)h17 3-44 °49M4.10.95112.7m 0319'090.199 6516.33GJ 6825V1451?.7 s(2 30) 677(188)系统恒星ra!11f 1DecParan 11距离同附Teff加恒星光年参#类型mvMVK( 士 er考名称r)历元 J2000.0Arcsec onds(士 err(士 err)资料编辑近距离恒星图下图是距离太阳在 14光年以内的32颗恒星位置图， 双星和三合星会以实际的数量推叠，但真实的位置是以最靠近中心平面的那一颗为准，颜色则与上面的表相对应。显示查？论？编恒星距离列表编辑相关条目天文学星际旅行最近的星系列表邻

24、近恒星资料视差RECONS - Research Con sortium on Nearby StarsResearchCon sortium on Nearby StarsNEAREST STAR SY STEMS 2007-09-17 2007-11-06.2.0 2.12. 八 Parallaxes give n by,GSU. THE ONE HUNDRED.RECONS .RECONS are a weighted恒星恒星列表 恒星距离列表 恒星亮度列表 恒星光度列表 巨大恒星列表 巨大质量恒星列表编辑参考资料1.000 1.001 1.002 1.003 1.004 1.005 1

25、.006 1.007 1.008 1.009 1.010 1.011 1.0121. 八1.013 1.014 1.015 1.016 1.017 1.018 1.019 1.020 1.021 1.022 1.0231.024 1.025 1.026 1.027 1.028 1.029 1.030 1.031 1.032 1.033 1.034 1.035 1.036 1.037 1.038 1.0391.040 1.041 1.042 1.043 1.044 1.045 1.046 1.0471.048 1.049 1.050 1.051 1.052 1.053 1.054 1.055 1

26、.056 1.057 1.058 1.059 1.060 1.061 1.062 1.063 1.064 1.065 1.0661.067 1.068 1.069 1.070 1.0711.072 1.073 1.074 1.075 1.076 1.077 1.078 1.079 1.080 1.081 1.082 1.083 1.084 1.085 1.086 1.087 1.088 1.089 1.090 1.091 1.092 1.0931.094 1.0951.096 1.097 1.098 1.099 1.100 1.101 1.102 1.103 1.104 1.105 1.106

27、 1.107 1.108 1.109 1.110 1.111 1.112 1.113 1.114 1.115 1.116 1.117 1.118 1.1191.1201.121 1.122 1.123 1.124 1.125 1.126 1.127 1.128 1.129 1.130 1.131 1.132 1.133 1.134 1.135 1.136 1.137 1.138 1.139 1.140 1.141 1.142 1.1431.144 1.145 1.146 1.1471.148 1.149 1.150 1.151 1.152 1.153 1.154 1.155 1.156 1.1

28、57 1.158 1.159 1.160 1.161 1.162 1.163 1.164 1.165 1.166 1.1671.168 1.169 1.170 1.171 1.172 1.173 1.1741.175 1.176 1.177 1.178 1.179 1.180 1.181 1.182 1.183 1.184mean of values in the sources give n, as well as measureme nts by the RECONS program.3.0 3.13. 八 From parallax.4. 八 Sun Fact Sheet , NASA.

29、 Accessed on line 2007-11-08.5 0 5 15 25. 人Kervella, Pierre; Theve nin, Frederic. A FamilyPortrait of the Alpha Cen tauri System: VLT In terferometerStudies the Nearest Stars . ESO Press Release 05/03.ESO. 2003-03-15 2007-11-08.6.00 6.01 6.02 6.03 6.04 6.05 6.06 6.07 6.08 6.09 6.10 6.11 6.12 6.13 6.

30、14 6.156. A6.16 6.17 6.18 6.19 6.20 6.21 6.22 6.23 6.24 6.25 6.26 6.27 6.286.29 6.30 6.31 6.327.8.9.10.11.12.13.14.15.16.6.33 6.34 6.35 6.36 6.37 6.38 6.39 6.40 6.41 6.42 小小Gen eral Catalogue ofTrig ono metric Parallaxes.7.00 7.01 7.02 7.03 7.04 7.05 7.06 7.07 7.08 7.09 7.10 7.11 7.12 7.13 7.14 7.15

31、 A7.16 7.17 7.18 7.19 7.20 7.21 7.22 7.23 7.24 7.25 7.26 7.27 7.28HipparcosCatalogue .9.0 9.1 9.2a Burgasser et al. 2000Visual binary orbits and masses post HipparcosStaffan S? derhjelm, Astronomy andAstrophysics 341 (Ja nuary 1999), pp. 12140.a Barnard's Star and the M Dwarf Temperature Scale ,

32、 P. C. Dawso n and M. M. de Robertis,The Astro nomicalJournal 127 , #5 (May 2004), pp.2909 2914. DOI:10.1086/383289a Ya. V. Pavle nko, H. R. A. Jon es, Yu. Lyubchik, J.Tennyson, and D. J. Pin field.Spectral en ergy distributi onfor GJ406 . Astronomy and Astrophysics. February 2006, 447 (2):709 -717.

33、 doi:10.1051/0004-6361:20052979.a Carbon monoxide bands in M dwarfs , Y. V. Pavlenkoand H. R. A. Jon es, Astro nomy andAstrophysics 396 (December 2002), pp.967 -975. D0I:10.1051/0004-6361:20021454a Table 2, The physical properties of normal A stars , Saul J. Adelma n, pp. 1 T1, The A-Star Puzzle , P

34、roceedi ngs of the In ter nati onal Astr ono mical Un io n , edited by J. Zverko, J. Ziznovsky, S. J. Adelman, and W. W. Weiss, Cambridge, UK: Cambridge Uni versity Press,2004. D0I:10.1017/S1743921304004314a Adopted value, The Age and Proge nitor Mass of Sirius B, James Liebert, Patrick A. You ng, D

35、avid Ar nett, J.B. Holberg, and Kurtis A. Williams, The Astrophysical Journal 630 , #1 (September 2005), pp. L6972.15.0 15.1 15.2 15.3 15.4 15.5、Systems with their first accuratetrigo no metric parallaxes measured by RECONSa The solar neighborhood IV: discovery of the twentieth nearest star , Todd J

36、. Henry, Philip A. Ianna, J. Davy Kirkpatrick, Hartmut Jahreiss, The Astr ono micalJournal 114 , #1 (July 1997), pp.388 -395. DOI:10.1086/11848217 0 17 1 17 2 17 317. 人The Solar Neighborhood. X VII. ParallaxResults from the CTIOPI 0.9 m Program: 20 New Members of the RECONS 10 Parsec Sample , Todd J. Henry, Wei-Chu n Jao, Joh n P. Subasavage, Thomas D. Beaulieu, Philip A. Ianna, Edgardo Costa, RenA. eMe ndez, The Astronomical Journal 132 , #6 (December2006) , pp. 2360-2371. DOI:10.1086/50823318 0 18 118. 人The very nearby M/T dwarf bin ar