This list is accurate as of 01 January 2008.
Red entries are systems with their first accurate trigonometric parallaxes measured by RECONS.
RECONS has made the first accurate distance measurements for 12 of the nearest 100 systems, and 29 of the 249 total systems within 10 parsecs.
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CNS NAME # comp LHS RA DEC proper motion trigonometric Spectral V Mv mass notes Common Name
2000.0 "/yr angle parallax Type estimate
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)
_______________________________________________________________________________________________________________________________________________________________________________________________
SUN (8) ---------- ----------- ----- ------- ----- ----- G2 V N -26.72 4.85 1.00 * 8 planets
1. GJ 551 - 49 14 29 43.0 -62 40 46 H 3.853 281.5 H 0.76887 0.00029 YHB* M5.5 V * 11.09 15.53 0.11 separation 7849" Proxima Centauri
GJ 559 A 3 50 14 39 36.5 -60 50 02 H 3.710 277.5 H 0.74723 0.00117 YS G2 V N 0.01 4.38 1.14 alpha Centauri A
GJ 559 B - 51 14 39 35.1 -60 50 14 H 3.724 284.8 H 0.74723 0.00117 K0 V N 1.34 5.71 0.92 orbit 18" alpha Centauri B
2. GJ 699 1 57 17 57 48.5 +04 41 36 H 10.358 355.6 H 0.54698 0.00100 YH M4.0 V * 9.53 13.22 0.17 Barnard's Star
3. GJ 406 1 36 10 56 29.2 +07 00 53 N 4.696 234.6 N 0.41910 0.00210 Y M6.0 V * 13.44 16.55 0.09 Wolf 359
4. GJ 411 1 37 11 03 20.2 +35 58 12 H 4.802 186.9 H 0.39342 0.00070 YH M2.0 V * 7.47 10.44 0.46 Lalande 21185
5. GJ 244 A 2 219 06 45 08.9 -16 42 58 H 1.339 204.1 H 0.38002 0.00128 YH A1 V N -1.43 1.47 1.99 Sirius
GJ 244 B - 06 45 08.9 -16 42 58 1.339 204.1 0.38002 0.00128 DA2 N 8.44 11.34 0.5 * orbit 8" Sirius B
6. GJ 65 A 2 9 01 39 01.3 -17 57 01 N 3.368 080.4 N 0.37370 0.00270 Y M5.5 V * 12.54 15.40 0.11 BL Ceti
GJ 65 B - 10 01 39 01.3 -17 57 01 3.368 080.4 0.37370 0.00270 M6.0 V * 12.99 15.85 0.10 orbit < 2" UV Ceti
7. GJ 729 1 3414 18 49 49.4 -23 50 10 H 0.666 106.8 H 0.33690 0.00178 YH M3.5 V * 10.43 13.07 0.17 Ross 154
8. GJ 905 1 549 23 41 54.7 +44 10 30 N 1.617 177.0 N 0.31600 0.00110 Y M5.5 V * 12.29 14.79 0.12 Ross 248
9. GJ 144 2 1557 03 32 55.8 -09 27 30 H 0.977 271.1 H 0.30999 0.00079 YH K2 V N 3.73 6.19 0.85 cold dust epsilon Eridani
GJ 144 P1 - 03 32 55.8 -09 27 30 0.977 271.1 0.30999 0.00079 planet - orbit < 2"
10. GJ 887 1 70 23 05 52.0 -35 51 11 H 6.896 078.9 H 0.30364 0.00087 YH M1.5 V * 7.34 9.75 0.53 Lacaille 9352
11. GJ 447 1 315 11 47 44.4 +00 48 16 H 1.361 153.6 H 0.29872 0.00135 YH M4.0 V * 11.13 13.51 0.16 Ross 128
12. GJ 866 A 3 68 22 38 33.4 -15 18 07 N 3.254 046.6 N 0.28950 0.00440 Y M5.0 V J* 13.33 15.64 0.11 EZ Aquarii A
GJ 866 B - 22 38 33.4 -15 18 07 3.254 046.6 0.28950 0.00440 ------ - 13.27 15.58 0.11 orbit < 2" EZ Aquarii B
GJ 866 C - 22 38 33.4 -15 18 07 3.254 046.6 0.28950 0.00440 ------ - 14.03 16.34 0.10 orbit < 2" EZ Aquarii C
13. GJ 280 A 2 233 07 39 18.1 +05 13 30 H 1.259 214.7 H 0.28605 0.00081 YH F5 IV-V N 0.38 2.66 1.57 Procyon
GJ 280 B - 07 39 18.1 +05 13 30 1.259 214.7 0.28605 0.00081 DA N 10.70 12.98 0.5 * orbit 4" Procyon B
14. GJ 820 A 2 62 21 06 53.9 +38 44 58 H 5.281 051.9 H 0.28604 0.00056 YHH K5.0 V * 5.21 7.49 0.70 61 Cygni A
GJ 820 B - 63 21 06 55.3 +38 44 31 H 5.172 052.6 H 0.28604 0.00056 K7.0 V * 6.03 8.31 0.63 orbit 25" 61 Cygni B
15. GJ 725 A 2 58 18 42 46.7 +59 37 49 H 2.238 323.6 H 0.28300 0.00169 YHH M3.0 V * 8.90 11.16 0.35
GJ 725 B - 59 18 42 46.9 +59 37 37 H 2.313 323.0 H 0.28300 0.00169 M3.5 V * 9.69 11.95 0.26 orbit 14"
16. GJ 15 A 2 3 00 18 22.9 +44 01 23 H 2.918 081.9 H 0.28059 0.00095 YH M1.5 V * 8.08 10.32 0.49 GX Andromedae
GJ 15 B - 4 00 18 22.9 +44 01 23 2.918 081.9 0.28059 0.00095 M3.5 V * 11.06 13.30 0.16 orbit 41" GQ Andromedae
17. GJ 845 A 3 67 22 03 21.7 -56 47 10 H 4.704 122.7 H 0.27584 0.00069 YH K5 Ve N 4.69 6.89 0.77 epsilon Indi A
GJ 845 B - 22 04 10.5 -56 46 58 S 4.823 121.1 S 0.27584 0.00069 T1.0 M 0.04 : separation 402" epsilon Indi B
GJ 845 C - 22 04 10.5 -56 46 58 S 4.823 121.1 S 0.27584 0.00069 T6.0 M 0.03 : separation < 2" epsilon Indi C
18. GJ 1111 1 248 08 29 49.5 +26 46 37 N 1.290 242.2 N 0.27580 0.00300 Y M6.5 V * 14.78 16.98 0.09 DX Cancri
19. GJ 71 1 146 01 44 04.1 -15 56 15 H 1.922 296.4 H 0.27439 0.00076 YH G8 Vp N 3.49 5.68 0.92 tau Ceti
20. GJ 1061 1 1565 03 35 59.7 -44 30 45 * 0.826 117.7 * 0.27201 0.00130 ** M5.5 V * 13.09 15.26 0.11 Henry et al. 1997, Henry et al. 2006
21. GJ 54.1 1 138 01 12 30.6 -16 59 56 H 1.372 061.9 H 0.26884 0.00295 YH M4.5 V * 12.02 14.17 0.14 YZ Ceti
22. GJ 273 1 33 07 27 24.5 +05 13 33 H 3.738 171.2 H 0.26376 0.00125 YH M3.5 V * 9.86 11.97 0.26 Luyten's Star
23. SO 0253+1652 1 02 53 00.9 +16 52 53 * 5.106 138.2 * 0.26063 0.00269 * M7.0 V * 15.14 17.22 0.08 Henry et al. 2006
24. SCR 1845-6357 A 2 18 45 05.3 -63 57 48 * 2.664 076.6 * 0.25945 0.00111 * M8.5 V * 17.40J 19.42 0.07 Henry et al. 2006
SCR 1845-6357 B - 18 45 02.6 -63 57 52 2.664 076.6 0.25945 0.00111 T Biller et al. 2006
25. GJ 191 1 29 05 11 40.6 -45 01 06 H 8.670 131.4 H 0.25527 0.00086 YH M1.5 V * 8.84 10.87 0.39 Kapteyn's Star
26. GJ 825 1 66 21 17 15.3 -38 52 03 H 3.455 250.6 H 0.25343 0.00112 YH M0.0 V * 6.67 8.69 0.60 AX Microscopii
27. GJ 860 A 2 3814 22 27 59.5 +57 41 45 H 0.990 241.6 H 0.24806 0.00139 YS M3.0 V * 9.79 11.76 0.28 Kruger 60 A
GJ 860 B - 3815 22 27 59.5 +57 41 45 0.990 241.6 0.24806 0.00139 M4.0 V * 11.41 13.38 0.16 orbit 2" Kruger 60 B
28. DEN 1048-3956 1 10 48 14.7 -39 56 06 D 1.530 229.2 * 0.24771 0.00155 ** M8.5 V * 17.39 19.37 0.07 Jao et al. 2005, Costa et al. 2005
29. GJ 234 A 2 1849 06 29 23.4 -02 48 50 H 0.930 131.7 H 0.24434 0.00201 YS M4.5 V J* 11.15 13.09 0.17 Ross 614 A
GJ 234 B - 1850 06 29 23.4 -02 48 50 0.930 131.7 0.24434 0.00201 ------ - 14.23 16.17 0.10 orbit < 2" Ross 614 B
30. GJ 628 1 419 16 30 18.1 -12 39 45 H 1.189 184.5 H 0.23601 0.00167 YH M3.0 V * 10.07 11.93 0.26 Wolf 1061
31. GJ 35 1 7 00 49 09.9 +05 23 19 H 2.978 155.5 H 0.23188 0.00179 YH DZ7 N 12.38 14.21 0.5 * WD 0046+051
32. GJ 1 1 1 00 05 24.4 -37 21 27 H 6.100 112.5 H 0.22920 0.00107 YH M3.0 V * 8.55 10.35 0.48
33. GJ 473 A 2 333 12 33 17.2 +09 01 15 N 1.811 277.4 N 0.22790 0.00460 Y M5.5 V J* 13.18 14.97 0.12 Wolf 424 A
GJ 473 B - 12 33 17.2 +09 01 15 1.811 277.4 0.22790 0.00460 ------ - 13.17 14.96 0.12 orbit < 2" Wolf 424 B
34. GJ 83.1 1 11 02 00 13.2 +13 03 08 N 2.097 147.8 N 0.22480 0.00290 Y M4.5 V * 12.27 14.03 0.14 TZ Arietis
35. GJ 687 1 450 17 36 25.9 +68 20 21 H 1.309 194.2 H 0.22049 0.00082 YH M3.0 V * 9.17 10.89 0.39
36. LHS 292 1 292 10 48 12.6 -11 20 14 N 1.644 158.5 N 0.22030 0.00360 Y M6.5 V * 15.60 17.32 0.08
37. GJ 674 2 449 17 28 39.9 -46 53 43 H 1.050 146.9 H 0.22025 0.00159 YH M3.0 V * 9.38 11.09 0.36
GJ 674 P1 - 17 28 39.9 -46 53 43 1.050 146.9 0.22025 0.00159 planet - orbit < 2"
38. GJ 1245 A 3 3494 19 53 54.2 +44 24 55 N 0.731 143.1 N 0.22020 0.00100 Y M5.5 V J* 13.46 15.17 0.11 G 208-044 A
GJ 1245 B - 3495 19 53 55.2 +44 24 56 N 0.731 143.1 0.22020 0.00100 M6.0 V * 14.01 15.72 0.10 separation 8" G 208-045
GJ 1245 C - 19 53 54.2 +44 24 55 0.731 143.1 0.22020 0.00100 ------ - 16.75 18.46 0.07 orbit < 2" G 208-044 B
39. GJ 440 1 43 11 45 42.9 -64 50 29 H 2.688 097.4 H 0.21657 0.00201 YH DQ6 N 11.50 13.18 0.5 * WD 1142-645
40. GJ 1002 1 2 00 06 43.8 -07 32 22 N 2.041 203.6 N 0.21300 0.00360 Y M5.5 V * 13.76 15.40 0.11
41. GJ 876 A 4 530 22 53 16.7 -14 15 49 H 1.174 125.1 H 0.21259 0.00196 YH M3.5 V J* 10.17 11.81 0.27 Ross 780
GJ 876 P1 - 22 53 16.7 -14 15 49 1.174 125.1 0.21259 0.00196 planet - orbit < 2"
GJ 876 P2 - 22 53 16.7 -14 15 49 1.174 125.1 0.21259 0.00196 planet - orbit < 2"
GJ 876 P3 - 22 53 16.7 -14 15 49 1.174 125.1 0.21259 0.00196 planet - orbit < 2"
42. LHS 288 1 288 10 44 21.2 -61 12 36 * 1.643 347.7 * 0.20895 0.00273 * M5.5 V * 13.90 15.51 0.11 Henry et al. 2006
43. GJ 412 A 2 38 11 05 28.6 +43 31 36 H 4.511 282.1 H 0.20602 0.00108 YH M1.0 V * 8.77 10.34 0.48
GJ 412 B - 39 11 05 30.4 +43 31 18 H 4.531 281.9 N 0.20602 0.00108 M5.5 V * 14.48 16.05 0.10 separation 28" WX Ursae Majoris
44. GJ 380 1 280 10 11 22.1 +49 27 15 H 1.452 249.7 H 0.20581 0.00067 YH K7.0 V * 6.59 8.16 0.64
45. GJ 388 1 5167 10 19 36.4 +19 52 10 N 0.506 264.0 N 0.20460 0.00280 Y M3.0 V * 9.32 10.87 0.39
46. GJ 832 1 3685 21 33 34.0 -49 00 32 H 0.819 183.2 H 0.20278 0.00132 YH M3.0 V * 8.66 10.20 0.50
47. LP 944-020 1 03 39 35.2 -35 25 41 N 0.439 047.6 N 0.20140 0.00420 T M9.0 V * 18.50 20.02 0.07
48. DEN 0255-4700 1 02 55 03.7 -47 00 52 * 1.149 119.5 * 0.20137 0.00389 * L7.5 V 22.92 24.44 0.07 Costa et al. 2005
49. GJ 682 1 451 17 37 03.7 -44 19 09 H 1.176 217.1 H 0.19965 0.00230 YH M4.5 V * 10.95 12.45 0.21
50. GJ 166 A 3 23 04 15 16.3 -07 39 10 H 4.088 213.2 H 0.19900 0.00077 YH K1 Ve N 4.43 5.92 0.89 omicron 2 Eridani
GJ 166 B - 24 04 15 22.0 -07 39 35 H 4.073 212.4 N 0.19900 0.00077 DA4 N 9.52 11.01 0.5 * separation 83"
GJ 166 C - 25 04 15 22.0 -07 39 35 4.073 212.4 0.19900 0.00077 M4.5 V * 11.19 12.68 0.20 orbit 7"
51. GJ 873 1 3853 22 46 49.7 +44 20 02 H 0.841 236.9 H 0.19804 0.00161 YH M3.5 V * 10.22 11.70 0.29 EV Lacertae
52. GJ 702 A 2 458 18 05 27.3 +02 30 00 H 0.971 172.6 H 0.19596 0.00087 YS K0 Ve N 4.20 5.66 0.92 70 Ophiuchi A
GJ 702 B - 459 18 05 27.3 +02 30 00 0.971 172.6 0.19596 0.00087 K5 Ve N 6.05 7.51 0.70 orbit 5" 70 Ophiuchi B
53. GJ 768 1 3490 19 50 47.0 +08 52 06 H 0.661 054.3 H 0.19497 0.00086 YH A7 IV-V N 0.77 2.22 1.71 Altair
54. GJ 1116 A 2 2076 08 58 14.9 +19 45 43 N 0.874 267.7 N 0.19120 0.00250 Y M5.5 V J* 14.06 15.47 0.11 EI Cancri
GJ 1116 B - 2077 08 58 14.9 +19 45 49 N 0.874 267.7 0.19120 0.00250 ------ - 14.92 16.33 0.10 separation < 2"
55. G 099-049 1 06 00 03.5 +02 42 24 * 0.313 097.5 * 0.19093 0.00189 * M3.5 V * 11.31 12.71 0.19 Henry et al. 2006
56. LHS 1723 1 1723 05 01 57.4 -06 56 47 * 0.769 226.9 * 0.18792 0.00126 * M4.5 V * 12.22 13.59 0.15 Henry et al. 2006
57. GJ 445 1 2459 11 47 41.4 +78 41 28 H 0.885 057.1 H 0.18584 0.00139 YH M3.5 V * 10.79 12.14 0.24
58. GJ 526 1 47 13 45 43.8 +14 53 29 H 2.298 129.3 H 0.18421 0.00116 YH M1.5 V * 8.46 9.79 0.53 Wolf 498
59. LP 816-060 1 20 52 33.0 -16 58 29 H 0.308 275.7 H 0.18215 0.00368 H m * 11.41 12.71 0.19
60. GJ 169.1 A 2 26 04 31 11.8 +58 58 38 H 2.427 147.6 H 0.18063 0.00078 YH M4.0 V * 11.04 12.32 0.22 Stein 2051
GJ 169.1 B - 27 04 31 11.8 +58 58 38 2.427 147.6 0.18063 0.00078 DC5 N 12.44 13.72 0.5 * separation 8"
61. GJ 251 1 1879 06 54 49.0 +33 16 05 H 0.831 241.3 H 0.17958 0.00161 YH M3.0 V * 10.02 11.29 0.33
62. 2MA 1835+3259 1 18 35 37.9 +32 59 54 M 0.759 186.1 U 0.17650 0.00050 U M8.5 V 18.27 19.50 0.07 Reid et al. 2003
63. GJ 205 1 30 05 31 27.4 -03 40 38 H 2.228 160.0 H 0.17517 0.00105 YH M1.5 V * 7.95 9.17 0.57 Wolf 1453
64. 2MA 0415-0935 1 04 15 19 -09 35 M 2.255 076.5 U 0.17434 0.00276 U T8.5V Vrba et al. 2004
65. GJ 764 1 477 19 32 21.6 +69 39 40 H 1.839 161.0 H 0.17359 0.00041 YH K0 V N 4.68 5.88 0.89 sigma Draconis
66. GJ 229 A 2 1827 06 10 34.6 -21 51 53 H 0.727 190.9 H 0.17317 0.00110 YH M1.0 V * 8.12 9.31 0.56
GJ 229 B - 06 10 34.6 -21 51 53 0.727 190.9 0.17317 0.00110 T6.0 V G 0.05 * separation 8"
67. GJ 693 1 454 17 46 34.2 -57 19 09 H 1.756 219.6 H 0.17169 0.00214 YH M4.0 V * 10.75 11.92 0.26
68. GJ 752 A 2 473 19 16 55.3 +05 10 08 H 1.452 203.5 H 0.17101 0.00062 YH M3.0 V * 9.11 10.28 0.49 Wolf 1055
GJ 752 B - 474 19 16 58.3 +05 09 01 H 1.461 203.1 N 0.17101 0.00062 M8.0 V * 17.50 18.67 0.07 separation 74" van Biesbroeck 10
69. GJ 213 1 31 05 42 09.3 +12 29 22 H 2.542 128.2 H 0.17037 0.00309 YH M4.0 V * 11.51 12.67 0.20 Ross 47
70. GJ 570 A 4 387 14 57 28.0 -21 24 56 H 2.012 149.1 H 0.16985 0.00082 YHS K5 Ve N 5.75 6.90 0.76
GJ 570 B - 386 14 57 26.5 -21 24 41 H 1.937 149.4 H 0.16985 0.00082 M1.0 V J* 8.28 9.43 0.55 separation 22"
GJ 570 C - 14 57 26.5 -21 24 41 1.937 149.4 0.16985 0.00082 ------ - 10.05 11.20 0.35 orbit < 2"
GJ 570 D - 14 57 15.0 -21 21 50 B 2.012 149.1 0.16985 0.00082 T8.0 V G 0.05 * separation 258"
71. GJ 754 1 60 19 20 48.0 -45 33 27 N 2.945 167.3 N 0.16903 0.00155 * M4.5 V * 12.23 13.37 0.16 Jao et al. 2005
72. GJ 908 1 550 23 49 12.5 +02 24 04 H 1.388 134.2 H 0.16851 0.00140 YH M1.0 V * 8.99 10.12 0.51
73. GJ 34 A 2 123 00 49 06.3 +57 48 55 H 1.223 117.2 H 0.16838 0.00059 YH G3 V N 3.45 4.58 1.11 eta Cassiopei A
GJ 34 B - 122 00 49 06.3 +57 48 55 1.223 117.2 0.16838 0.00059 K7.0 V * 7.51 8.64 0.60 orbit 12" eta Cassiopei B
74. GJ 588 1 397 15 32 12.9 -41 16 32 H 1.564 228.9 H 0.16836 0.00138 YH M3.0 V * 9.31 10.44 0.46
75. GJ 1005 A 2 1047 00 15 28.1 -16 08 02 H 0.955 130.3 H 0.16806 0.00082 YSE M4.0 V J* 11.58 12.93 0.18
GJ 1005 B - 00 15 28.1 -16 08 02 0.955 130.3 0.16806 0.00082 ------ - 14.33 15.68 0.11 orbit < 2"
76. GJ 285 1 1943 07 44 40.2 +03 33 09 H 0.568 217.4 H 0.16754 0.00228 YH M4.0 V * 11.19 12.31 0.23 Ross 882
77. GJ 663 A 3 437 17 15 21.0 -26 36 10 H 1.238 202.5 H 0.16751 0.00075 YHYH K1 Ve N 5.07 6.19 0.85 36 Ophiuchi A
GJ 663 B - 438 17 15 21.0 -26 36 10 1.238 202.5 0.16751 0.00075 K1 Ve N 5.08 6.20 0.85 orbit 14" 36 Ophiuchi B
GJ 664 - 439 17 16 13.4 -26 32 46 H 1.222 203.1 H 0.16751 0.00075 K5 Ve N 6.33 7.45 0.71 separation 732" 36 Ophiuchi C
78. GJ 783 A 2 486 20 11 11.9 -36 06 04 H 1.640 163.8 H 0.16533 0.00090 YH K3 V N 5.32 6.41 0.82
GJ 783 B - 487 20 11 11.9 -36 06 04 1.640 163.8 0.16533 0.00090 M4.0 V * 11.50 12.59 0.20 separation 7"
79. GJ 139 1 19 03 19 55.6 -43 04 11 H 3.124 076.6 H 0.16501 0.00055 YH G5 V N 4.26 5.35 0.97 82 Eridani
80. GJ 1221 1 455 17 48 06.7 +70 52 29 N 1.651 311.0 N 0.16470 0.00240 Y DXP9 N 14.12 15.20 0.5 *
81. GJ 780 1 485 20 08 43.6 -66 10 55 H 1.656 133.0 H 0.16378 0.00065 YH G8 V N 3.56 4.63 1.10 delta Pavonis
82. GJ 268 A 2 226 07 10 01.8 +38 31 46 H 1.045 204.9 H 0.16293 0.00177 YH M4.5 V J* 12.05 13.11 0.17 QY Aurigae A
GJ 268 B - 07 10 01.8 +38 31 46 1.045 204.9 0.16293 0.00177 ------ - 12.45 13.51 0.16 orbit < 2" QY Aurigae B
83. GJ 555 1 2945 14 34 16.8 -12 31 10 H 0.694 329.0 H 0.16286 0.00261 YH M3.5 V * 11.31 12.37 0.22 HN Librae
84. 2MA 0937+2931 1 09 37 34 +29 31 M 1.622 143.1 M 0.16284 0.00388 U T6.0 V Vrba et al. 2004
85. GJ 338 A 2 260 09 14 22.8 +52 41 12 H 1.634 249.8 H 0.16213 0.00237 YHH M0.0 V * 7.62 8.67 0.60
GJ 338 B - 261 09 14 24.7 +52 41 11 H 1.684 247.1 H 0.16213 0.00237 K7.0 V * 7.71 8.76 0.60 orbit 17"
86. GJ 784 1 3531 20 13 53.4 -45 09 50 H 0.794 101.6 H 0.16118 0.00107 YH M0.0 V * 7.96 9.00 0.58
87. GJ 581 4 394 15 19 26.8 -07 43 20 H 1.229 265.4 H 0.15929 0.00210 YH M2.5 V * 10.56 11.57 0.30 Wolf 562
GJ 581 P1 - 15 19 26.8 -07 43 20 1.229 265.4 0.15929 0.00210 planet - orbit < 2"
GJ 581 P2 - 15 19 26.8 -07 43 20 1.229 265.4 0.15929 0.00210 planet - orbit < 2"
GJ 581 P3 - 15 19 26.8 -07 43 20 1.229 265.4 0.15929 0.00210 planet - orbit < 2"
88. GJ 896 A 2 3965 23 31 52.2 +19 56 14 H 0.558 096.4 H 0.15772 0.00243 YH M3.5 V * 10.26 11.25 0.34 EQ Pegasi
GJ 896 B - 3966 23 31 52.2 +19 56 14 0.558 096.4 0.15772 0.00243 M4.5 V * 12.40 13.39 0.16 orbit 7"
89. LHS 2090 1 2090 09 00 23.6 +21 50 05 * 0.774 221.2 * 0.15687 0.00267 * M6.0 V * 16.10 17.07 0.09 Henry et al. 2006
90. LHS 337 1 337 12 38 49.1 -38 22 54 * 1.464 206.4 * 0.15678 0.00199 * M4.0 V * 12.75 13.73 0.15 Henry et al. 2006
91. GJ 661 A 2 433 17 12 07.9 +45 39 57 H 1.625 168.4 H 0.15632 0.00128 YS M3.0 V J* 9.93 10.90 0.39
GJ 661 B - 434 17 12 07.9 +45 39 57 1.625 168.4 0.15632 0.00128 ------ - 10.35 11.32 0.33 orbit < 2"
92. LHS 3003 1 3003 14 56 38.5 -28 09 51 N 0.965 210.1 N 0.15630 0.00300 Y M7.0 V * 17.05 18.02 0.08
93. G 180-060 1 16 31 18.4 +40 51 54 N 0.358 330.0 N 0.15600 0.00400 D m+ N 14.79 15.76 0.10
94. GJ 223.2 1 32 05 55 09.7 -04 10 17 N 2.377 166.6 N 0.15500 0.00210 Y DZ9 N 14.45 15.40 0.5 * WD 0552-041
95. GJ 644 A 5 428 16 55 28.8 -08 20 11 H 1.208 223.3 H 0.15497 0.00056 YSYH M2.5 V J* 9.72 10.67 0.43 Wolf 630 A
GJ 644 B - 16 55 28.8 -08 20 11 1.208 223.3 0.15497 0.00056 ------ - 10.54 11.49 0.31 orbit < 2" Wolf 630 B
GJ 644 C - 429 16 55 35.8 -08 23 40 H 1.190 222.5 N 0.15497 0.00056 M7.0 V * 16.80 17.75 0.08 separation 221" van Biesbroeck 8
GJ 644 D - 16 55 28.8 -08 20 11 1.208 223.3 0.15497 0.00056 ------ - 10.63 11.58 0.30 orbit < 2" Wolf 630 C
GJ 643 - 427 16 55 25.2 -08 19 21 H 1.210 222.3 H 0.15497 0.00056 M3.5 V * 11.74 12.69 0.19 separation 72" Wolf 629
96. GJ 892 1 71 23 13 17.0 +57 10 06 H 2.095 081.9 H 0.15341 0.00054 YH K3 V N 5.56 6.49 0.81
97. GJ 1128 1 271 09 42 46.4 -68 53 06 1.121 356.7 * 0.15305 0.00241 * M4.5 V * 12.74 13.66 0.15 Jao et al. 2005
98. GJ 1156 1 324 12 19 00.3 +11 07 31 N 1.301 279.1 N 0.15290 0.00300 Y M5.0 V * 13.80 14.72 0.12 GL Virginis
99. GJ 625 1 16 25 24.6 +54 18 15 H 0.465 111.5 H 0.15179 0.00101 YH M1.5 V * 10.10 11.01 0.37
100. GJ 408 1 11 00 04.3 +22 49 59 H 0.510 236.7 H 0.15016 0.00149 YH M2.5 V * 10.02 10.90 0.39 Ross 104
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FORMER TOP 100 MEMBERS PUSHED OUT BY NEW MEMBERS
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GJ 829 A 2 508 21 29 36.8 +17 38 36 H 1.076 069.5 H 0.14825 0.00173 YH M3.5 V J* 11.06 11.91 0.26 Ross 775 A
GJ 829 B - 21 29 36.8 +17 38 36 1.076 069.5 0.14825 0.00173 ------ - 11.06 11.91 0.26 orbit < 2" Ross 775 B
G 041-014 A 3 08 58 56.3 +08 28 26 * 0.503 130.0 * 0.14766 0.00198 * M4.5 V J* 11.9 12.8 0.19 Henry et al. 2006
G 041-014 B - 08 58 56.3 +08 28 26 * 0.503 130.0 * 0.14766 0.00198 * ------ - 12.1 13.0 0.17
G 041-014 C - 08 58 56.3 +08 28 26 * 0.503 130.0 * 0.14766 0.00198 * ------ - 12.3 13.1 0.17
GJ 566 A 2 14 51 23.4 +19 06 02 H 0.169 115.0 H 0.14757 0.00072 YS G8 Ve N 4.70 5.54 0.94 ksi Bootis A
GJ 566 B - 14 51 23.4 +19 06 02 0.169 115.0 0.14757 0.00072 K4 Ve N 6.97 7.81 0.67 orbit 5" ksi Bootis B
GJ 402 1 294 10 50 52.1 +06 48 29 H 1.150 225.1 N 0.14701 0.00544 YH M4.0 V * 11.67 12.51 0.21 EE Leonis
GJ 299 1 35 08 11 57.5 +08 46 28 N 5.211 167.1 N 0.14630 0.00310 Y M4.0 V * 12.82 13.65 0.15 Ross 619
GJ 880 1 533 22 56 34.8 +16 33 12 H 1.071 254.7 H 0.14579 0.00113 YH M1.5 V * 8.66 9.48 0.55 Ross 671
LP 771-095 A 3 03 01 51.4 -16 35 36 * 0.477 234.4 * 0.14468 0.00252 * M3.0 V * 11.22 12.03 0.25 Henry et al. 2006
LP 771-095 B - 03 01 51.0 -16 35 31 * 0.479 235.5 * 0.14468 0.00252 * M3.5 VJ * 11.77 12.58 separation 7" LP 771-096
LP 771-095 C - 03 01 51.0 -16 35 31 * 0.479 235.5 * 0.14468 0.00252 * ------ - 12.63 13.44 separation < 2"
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FORMER TOP 100 MEMBERS PUSHED OUT BY NEW RECONS PARALLAXES
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GJ 300 1 1989 08 12 40.8 -21 33 10 N 0.707 177.5 N 0.16990 0.01500 Y M3.5 V * 12.07 13.22 0.17 0.12010 0.00110 * Henry et al. 2006
GJ 2130 A 3 17 46 12.6 -32 06 13 H 0.324 188.9 H 0.16177 0.01129 H M2 V N 10.49 11.53 0.30 0.07145 0.00264 * Henry et al. 2006
GJ 2130 B - 17 46 14.4 -32 06 08 H 0.281 196.0 H 0.16177 0.01129 H M2 VJ N 11.75 12.79 0.19 separation 21"
GJ 2130 C - 17 46 14.4 -32 06 08 0.281 196.0 0.16177 0.01129 H ------ - 12.75 13.79 0.15 orbit < 2"
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PARALLAX REFERENCES
E = Hershey
H = Hipparcos
S = Soderjhelm 1999
T = Tinney 1996
U = United States Naval Observatory (USNO)
Y = Yale Parallax Catalog
* = RECONS program (see Jao et al. 2005 and Henry et al. 2006 for background)
OTHER REFERENCES
B = Burgasser et al. 2000
D = Ducourant et al. 1998
G = Geballe et al. 2002
N = Catalog of Nearby Stars (CNS) by Gliese & Jahreiss 1957, 1969, 1979, 1991
O = Oppenheimer et al. 1995
S = Scholz et al. 2003
* = RECONS program (see Henry et al. 1997 and Henry et al. 2006 for background)
COLUMNS
(1) name as given in the Catalog of Nearby Stars (1991) by Gliese and Jahreiss
(2) number of known components in the system
(3) name as given in the Luyten Half Second Catalog, which provides finder charts for faint, high proper motion stars
(4) Right Ascension on the sky, in hours, minutes, seconds
(5) Declination on the sky, in degrees, arcminutes, arcseconds
(6) magnitude of proper motion (in arcseconds/year) and direction of proper motion (in degrees, where 0 is north and 90 is east)
(7) trigonometric parallax, in arcseconds -- the values listed include determinations from various sources with weighted means calculated;
to determine the distance in light years use (3.26/parallax)
(8) stellar spectral type and luminosity class -- types are (blue-white) O,B,A,F,G,K,M (red) main sequence stars and types beginning
with "D" are white dwarfs; luminosity class V is a normal, main sequence star
(9) V magnitude is a measure of brightness at wavelengths centered near 5500 Angstroms, similar to the the color of light to which
human eyes are most sensitive; larger positive numbers are fainter stars, where each factor of 2.5 in brightness is one magnitude;
under good sky conditions, the eye is sensitive to magnitudes as faint as V = 6
(10) Mv is the absolute magnitude of the star and mimics the brightness it would have at the standard distance of 10 parsecs; as with
the V magnitude, larger positive numbers are fainter stars
(11) the estimated mass (in units of the Sun's mass) is based upon the Mv value and the empirical mass-luminosity relations of Henry and
McCarthy (1993) and Henry et al. (1999) -- values that have an asterisk (*) after them are not from the relations, given that the objects
are too faint for the relations (fainter than Mv = 20.00), are white dwarfs (for which 0.5 is always listed), or in the case of the Sun,
which defines the yscale at 1.000 Msun