This list is accurate as of January 1, 2000.
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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 (10) ---------- ----------- ----- ------- ----- ----- G2 V N -26.72 4.85 1.000* 9 planets
1. Gl 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 1.144 Alpha Centauri A #fff5f2
Gl 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 0.916 orbit 18" Alpha Centauri B #ffeedd
Gl 551 - 49 14 29 43.0 -62 40 46 H 3.853 281.5 H 0.77199 0.00225 YH M5.5 V * 11.09 15.53 0.107 separation 7849" Proxima Centauri #ffcc6f (M5.5V fudged as M5V)
2. Gl 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 0.166 Barnard's Star #ffc97f
3. Gl 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 0.092 Wolf 359 #ffc370
4. Gl 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 0.464 Lalande 21185 #ffc483
5. Gl 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 1.991 Sirius #b5c7ff
Gl 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 #a8bdff (DA2 fudged as D?2)
6. Gl 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 0.109 #ffcc6f (M5.5V fudged as M5V)
Gl 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 0.102 orbit < 2" UV Ceti #ffc370
7. Gl 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 0.171 Ross 154 #ffce81 (M3.5V fudged as M3V)
8. Gl 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 0.121 Ross 248 #ffcc6f (M5.5V fudged as M5V)
9. Gl 144 1 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 0.850 cold dust epsilon Eridani #ffe3c4
10. Gl 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 0.529 Lacaille 9352 #ffcc8e (M1.5V fudged as M1V)
11. Gl 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 0.156 Ross 128 #ffc97f
12. Gl 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 0.105 EZ Aquarii #ffcc6f
Gl 866 B - 22 38 33.4 -15 18 07 3.254 046.6 0.28950 0.00440 ------ - 13.27 15.58 0.106 orbit < 2"
Gl 866 C - 22 38 33.4 -15 18 07 3.254 046.6 0.28950 0.00440 ------ - 14.03 16.34 0.095 orbit < 2"
13. Gl 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 1.569 Procyon #f1efff (F5IV-V fudged as F5IV)
Gl 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"
14. Gl 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 0.703 61 Cygni #ffd2a1
Gl 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 0.630 orbit 25" #ffc78e
15. Gl 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 0.351 #ffce81
Gl 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 0.259 orbit 14" #ffce81 (M3.5V fudged as M3V)
16. Gl 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 0.486 #ffcc8e (M1.5V fudged as M1V)
Gl 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 0.163 orbit 41" #ffce81 (M3.5V fudged as M3V)
17. Gl 845 1 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 0.766 epsilon Indi #ffd2a1 (K5Ve fudged as K5V)
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 0.087 DX Cancri #ffc370 (M6.5V fudged as M6V)
19. Gl 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 0.921 tau Ceti #ffedde (G8Vp fudged as G8V)
20. GJ 1061 1 1565 03 36 00.0 -44 30 46 N 0.831 118.8 N 0.27340 0.00520 * M5.5 V * 13.03 15.21 0.113 RECONS 1 #ffcc6f (M5.5V fudged as M5V)
21. Gl 54.1 1 138 01 12 30.6 -16 59 57 H 1.372 061.9 H 0.26884 0.00295 YH M4.5 V * 12.02 14.17 0.136 YZ Ceti #ffc97f (M4.5V fudged as M4V)
22. Gl 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 0.257 Luyten's Star #ffce81 (M3.5V fudged as M3V)
23. Gl 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 0.393 Kapteyn's Star #ffcc8e (M1.5V fudged as M1V)
24. Gl 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 0.600 AX Microscopium #ffc38b
25. Gl 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 0.279 Kruger 60 #ffce81
Gl 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 0.160 orbit 2" #ffc97f
26. Gl 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 0.170 Ross 614 #ffc97f (M4.5V fudged as M4V)
Gl 234 B - 1850 06 29 23.4 -02 48 50 0.930 131.7 0.24434 0.00201 ------ - 14.23 16.17 0.097 orbit < 2"
27. Gl 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 0.261 #ffce81
28. Gl 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 * #f3f3ff (DZ7 fudged as D?7)
29. Gl 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 0.481 #ffce81
30. Gl 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 0.118 Wolf 424 #ffcc6f (M5.5V fudged as M5V)
Gl 473 B - 12 33 17.2 +09 01 15 1.811 277.4 0.22790 0.00460 ------ - 13.17 14.96 0.118 orbit < 2"
31. Gl 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 0.140 #ffc97f (M4.5V fudged as M4V)
32. LHS 288 1 288 10 44 31.8 -61 11 38 N 1.657 348.1 N 0.22250 0.01130 Y M5.5 V * 13.92 15.66 0.105 #ffcc6f (M5.5V fudged as M5V)
33. Gl 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 0.390 #ffce81
34. 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 0.083 #ffc370 (M6.5V fudged as M6V)
35. Gl 674 1 449 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 0.361 #ffce81
36. 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 0.114 G 208-44A #ffcc6f (M5.5V fudged as M5V)
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 0.104 separation 8" G 208-45 #ffc370
GJ 1245 C - 19 53 54.2 +44 24 55 0.731 143.1 0.22020 0.00100 ------ - 16.75 18.46 0.074 orbit < 2" G 208-44B
37. Gl 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 * #e0e6ff (DQ6 fudged as D?6)
38. 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 0.109 #ffcc6f (M5.5V fudged as M5V)
39. Gl 876 A 2 530 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 0.273 #ffce81 (M3.5V fudged as M3V)
Gl 876 B - 22 53 16.7 -14 15 49 1.174 125.1 0.21259 0.00196 planet? - 0.003* orbit < 2"
40. Gl 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 0.483 #ffcc8e
Gl 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 0.099 separation 28" WX Ursae Majoris #ffcc6f (M5.5V fudged as M5V)
41. Gl 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 0.642 #ffc78e
42. Gl 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 0.393 #ffce81
43. Gl 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 0.503 #ffce81
44. 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 0.066* #ffc66d (M9.0V fudged as M8V)
45. Gl 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 0.213 #ffc97f (M4.5V fudged as M4V)
46. Gl 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 0.887 omicron 2 Eridani #ffe0bc (K1Ve fudged as K1V)
Gl 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" #c0cfff (DA4 fudged as D?4)
Gl 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 0.195 orbit 7" #ffc97f (M4.5V fudged as M4V)
47. Gl 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 0.285 EV Lacertae #ffce81 (M3.5V fudged as M3V)
48. Gl 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 0.924 #ffeedd (K0Ve fudged as K0V)
Gl 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 0.701 orbit 5" #ffd2a1 (K5Ve fudged as K5V)
49. Gl 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 1.710 Altair #c0cfff (A7IV-V fudged as A7IV)
50. 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 0.108 #ffcc6f (M5.5V fudged as M5V)
GJ 1116 B - 2077 08 58 14.9 +19 45 49 N 0.874 267.7 0.19120 0.00250 ------ - 14.92 16.33 0.095 separation < 2"
51. G 099-049 1 06 00 03.6 +02 42 20 N 0.241 108.0 N 0.18620 0.01010 Y M3.5 V * 11.33 12.68 0.195 #ffce81 (M3.5V fudged as M3V)
52. Gl 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 0.240 #ffce81 (M3.5V fudged as M3V)
53. GJ 1005 A 2 1047 00 15 28.1 -16 08 02 H 0.955 130.3 H 0.18582 0.00297 YS M4.0 V J* 11.58 12.93 0.177 #ffc97f
GJ 1005 B - 00 15 28.1 -16 08 02 0.955 130.3 0.18582 0.00297 ------ - 14.33 15.68 0.105 orbit < 2"
54. Gl 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 0.526 #ffcc8e (M1.5V fudged as M1V)
55. 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 0.193
56. Gl 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 0.224 Stein 2051 #ffc97f
Gl 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" #cfdaff (DC5 fudged as D?5)
57. Gl 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 0.334 #ffce81
58. Gl 754 1 60 19 20 48.0 -45 33 27 N 2.945 167.3 N 0.17520 0.01010 Y M4.5 V * 12.23 13.45 0.158 #ffc97f (M4.5V fudged as M4V)
59. Gl 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 0.566 #ffcc8e (M1.5V fudged as M1V)
60. Gl 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 0.892 #ffeedd
61. Gl 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 0.556 #ffcc8e
Gl 229 B - 06 10 34.6 -21 51 53 0.727 190.9 0.17317 0.00110 BD O 0.050* separation 8"
62. Gl 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 0.262 #ffc97f
63. Gl 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 0.494 #ffce81
Gl 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 0.073 separation 74" van Biesbroeck 10 #ffc66d
64. Gl 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 0.196 #ffc97f
65. Gl 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 0.166 #ffce81 (M3.5V fudged as M3V)
66. Gl 570 A 3 387 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 0.764 #ffd2a1 (K5Ve fudged as K5V)
Gl 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 0.548 separation 22" #ffcc8e
Gl 570 C - 14 57 26.5 -21 24 41 1.937 149.4 0.16985 0.00082 ------ - 10.05 11.20 0.346 orbit < 2"
67. Gl 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 0.507 #ffcc8e
68. Gl 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 1.105 eta Cassiopeiae #fff5f2 (G3V fudged as G2V)
Gl 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 0.604 orbit 12" #ffc78e
69. Gl 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 0.464 #ffce81
70. Gl 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 0.225 #ffc97f
71. Gl 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 0.850 #ffe0bc (K1Ve fudged as K1V)
Gl 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 0.849 orbit 14" #ffe0bc (K1Ve fudged as K1V)
Gl 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 0.707 separation 732" #ffd2a1 (K5Ve fudged as K5V)
72. Gl 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 0.822 #ffdec3
Gl 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 0.202 separation 7" #ffc97f
73. Gl 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 0.971 #fff4ea
74. 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 * #ffefe1 (DXP9 fudged as D?9)
75. Gl 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 1.095 #ffedde
76. Gl 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 0.170 #ffc97f (M4.5V fudged as M4V)
Gl 268 B - 07 10 01.8 +38 31 46 1.045 204.9 0.16293 0.00177 ------ - 12.45 13.51 0.156 orbit < 2"
77. Gl 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 0.220 #ffce81 (M3.5V fudged as M3V)
78. Gl 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 0.601 #ffc38b
Gl 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 0.595 orbit 17" #ffc78e
79. 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 0.304 #ffc483
GJ 2130 B - 17 46 14.4 -32 06 08 H 0.281 196.0 H 0.16177 0.01129 M2 V N 11.75 12.79 0.187 separation 21" #ffc483
GJ 2130 C - 17 46 14.4 -32 06 08 0.281 196.0 0.16177 0.01129 ------ - 12.75 13.79 0.147 orbit < 2"
80. Gl 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 0.577 #ffc38b
81. Gl 581 1 394 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 0.300 #ffc483 (M2.5V fudged as M2V)
82. Gl 896 A 4 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 0.339 #ffce81 (M3.5V fudged as M3V)
Gl 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 0.160 orbit 7" #ffc97f (M4.5V fudged as M4V)
Gl 896 C - 23 31 52.2 +19 56 14 0.558 096.4 0.15772 0.00243 ------ - 13.26 14.25 0.134 orbit < 2"
Gl 896 D - 23 31 52.2 +19 56 14 0.558 096.4 0.15772 0.00243 ------ - 15.40 16.39 0.094 orbit < 2"
83. Gl 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 0.389 #ffce81
Gl 661 B - 434 17 12 07.9 +45 39 57 1.625 168.4 0.15632 0.00128 ------ - 10.35 11.32 0.330 orbit < 2"
84. 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 0.077 #ffc370 (M7.0V fudged as M6V)
85. 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 0.103
86. Gl 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 * #ffefe1 (DZ9 fudged as D?9)
87. Gl 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 0.425 #ffc483 (M2.5V fudged as M2V)
Gl 644 B - 16 55 28.8 -08 20 11 1.208 223.3 0.15497 0.00056 ------ - 10.54 11.49 0.309 orbit < 2"
Gl 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 0.080 separation 221" van Biesbroeck 8 #ffc370 (M7.0V fudged as M6V)
Gl 644 D - 16 55 28.8 -08 20 11 1.208 223.3 0.15497 0.00056 ------ - 10.63 11.58 0.299 orbit < 2"
Gl 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 0.194 separation 72" #ffce81 (M3.5V fudged as M3V)
88. Gl 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 0.812 #ffdec3
89. 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 0.123 #ffcc6f
90. Gl 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 0.372 #ffcc8e (M1.5V fudged as M1V)
91. Gl 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 0.389 #ffc483 (M2.5V fudged as M2V)
92. Gl 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 0.263 #ffce81 (M3.5V fudged as M3V)
Gl 829 B - 21 29 36.8 +17 38 36 1.076 069.5 0.14825 0.00173 ------ - 11.06 11.91 0.263 orbit < 2"
93. Gl 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 0.942 #ffedde (G8Ve fudged as G8V)
Gl 566 B - 14 51 23.4 +19 06 02 0.169 115.0 0.14757 0.00072 K4 Ve N 6.97 7.81 0.673 orbit 5" #ffd8b5 (K4Ve fudged as K4V)
94. Gl 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 0.208 Wolf 358 #ffc97f
95. Gl 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 0.151 #ffc97f
96. Gl 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 0.545 #ffcc8e (M1.5V fudged as M1V)
97. Gl 809 1 3595 20 53 19.8 +62 09 16 H 0.774 179.9 H 0.14158 0.00075 YH M0.0 V * 8.56 9.32 0.556 #ffc38b
98. Gl 293 1 34 07 53 14.7 -67 47 31 N 2.041 135.6 N 0.14120 0.00840 Y DQ9 N 14.08 14.83 0.5 * #ffefe1 (DQ9 fudged as D?9)
99. GJ 1286 1 546 23 35 10.7 -02 23 25 N 1.157 137.4 N 0.13830 0.00350 Y M5.5 V * 14.67 15.37 0.110 #ffcc6f (M5.5V fudged as M5V)
100. Gl 667 A 3 442 17 18 57.2 -34 59 24 H 1.153 094.5 H 0.13822 0.00070 YS K3 V N 6.27 6.97 0.757 #ffdec3
Gl 667 B - 17 18 57.2 -34 59 24 1.153 094.5 0.13822 0.00070 K5 V N 7.27 7.97 0.658 orbit < 2" #ffd2a1
Gl 667 C - 443 17 18 58.3 -34 59 41 H 1.180 098.3 N 0.13822 0.00070 M2.5 V * 10.26 10.96 0.380 separation 31" #ffc483 (M2.5V fudged as M2V)
____________________________________________________________________________________________________________________________________________________________________
REFERENCES
D = Ducourant et al 1998
H = Hipparcos
N = Nearby Star Catalog
O = Oppenheimer et al 1995
S = Soderjhelm 1999
T = Tinney 1996
Y = Yale Parallax Catalog
* = RECONS program (see Henry et al 1997)
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 hours, minutes, seconds
(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 (2000) -- 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
As of January 1, 2000, the complete sample of objects outside our solar system known within 10 parsecs (32.6 light years) includes
315 objects in 227 systems. The census includes 163 single stars, 46 doubles, 13 triples, 4 quadruples and 1 quintuple. There is
one brown dwarf known (Gl 229B) and one probable extrasolar planet (Gl 876B) in the sample.
For questions or comments, please contact Dr. Todd J. Henry at [email protected]