This list is accurate as of 01 January 2012.
Red entries are systems with their first accurate trigonometric parallaxes (errors less than 10 milliarcseconds) measured by RECONS.
RECONS has made the first accurate distance measurements for 12 of the nearest 100 systems, and 32 of the 259 total systems within 10 parsecs.
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CNS NAME # obj 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 1+8P ---------- ----------- ----- ------- ----- ----- G2.0 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 0.76885 0.00029 YHB* M5.0 V * 11.05 15.48 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 G2.0 V G 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 0.54551 0.00029 YHB M3.5 V * 9.57 13.25 0.16 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 M5.5 V * 13.53 16.64 0.09 Wolf 359
4. GJ 411 1 37 11 03 20.2 +35 58 12 H 4.802 186.9 H 0.39325 0.00057 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 A1.0 V G -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 1.00 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 * 12.61 15.47 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 * 13.06 15.93 0.10 orbit < 2" UV Ceti
7. GJ 729 1 3414 18 49 49.4 -23 50 10 H 0.666 106.8 H 0.33722 0.00197 YH M3.5 V * 10.44 13.08 0.17 Ross 154
8. GJ 905 1 549 23 41 54.7 +44 10 30 N 1.617 177.0 N 0.31637 0.00055 YGG M5.5 V * 12.29 14.79 0.12 Ross 248
9. GJ 144 1+1P 1557 03 32 55.8 -09 27 30 H 0.977 271.1 H 0.31122 0.00009 YHB K2.0 V G 3.73 6.20 0.85 cold dust epsilon Eridani
GJ 144 P1 - 03 32 55.8 -09 27 30 0.977 271.1 0.31122 0.00009 planet - orbit < 2"
10. GJ 887 1 70 23 05 52.0 -35 51 11 H 6.896 078.9 H 0.30508 0.00070 YH M1.0 V * 7.34 9.76 0.53 Lacaille 9352
11. GJ 447 1 315 11 47 44.4 +00 48 16 H 1.361 153.6 H 0.29814 0.00137 YH M4.0 V * 11.16 13.53 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 VJ * 13.03 15.33 0.11 EZ Aquarii A
GJ 866 B - 22 38 33.4 -15 18 07 3.254 046.6 0.28950 0.00440 M V - 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 M V - 15.07 17.37 0.08 orbit < 2" EZ Aquarii C
13. GJ 820 A 2 62 21 06 53.9 +38 44 58 H 5.281 051.9 H 0.28608 0.00048 YHH K5.0 V * 5.20 7.48 0.70 61 Cygni A
GJ 820 B - 63 21 06 55.3 +38 44 31 H 5.172 052.6 H 0.28608 0.00048 K7.0 V * 6.03 8.31 0.63 orbit 25" 61 Cygni B
14. GJ 280 A 2 233 07 39 18.1 +05 13 30 H 1.259 214.7 H 0.28517 0.00064 YHGGi F5 IV-V G 0.37 2.65 1.57 Procyon
GJ 280 B - 07 39 18.1 +05 13 30 1.259 214.7 0.28517 0.00064 DQZ Pl 10.70 12.98 0.5 * orbit 4" Procyon B
15. GJ 725 A 2 58 18 42 46.7 +59 37 49 H 2.238 323.6 H 0.28383 0.00146 YHH M3.0 V * 8.90 11.17 0.35
GJ 725 B - 59 18 42 46.9 +59 37 37 H 2.313 323.0 H 0.28383 0.00146 M3.5 V * 9.69 11.96 0.26 orbit 14"
16. GJ 15 A 2 3 00 18 22.9 +44 01 23 H 2.918 081.9 H 0.27987 0.00060 YHG M1.5 V * 8.08 10.31 0.49 GX Andromedae
GJ 15 B - 4 00 18 22.9 +44 01 23 2.918 081.9 0.27987 0.00060 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 0.27607 0.00028 YH K4.0 V G 4.68 6.89 0.77 epsilon Indi A
GJ 845 B - 22 04 10.5 -56 46 58 S 4.823 121.1 S 0.27607 0.00028 T1.0 V 0.03 * separation 402" epsilon Indi B
GJ 845 C - 22 04 10.5 -56 46 58 S 4.823 121.1 S 0.27607 0.00028 T6.0 V 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 M6.0 V * 14.90 17.10 0.09 DX Cancri
19. GJ 71 1 146 01 44 04.1 -15 56 15 H 1.922 296.4 H 0.27397 0.00017 YH G8.5 V G 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 ** M5.0 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 0.26908 0.00299 YH M4.0 V * 12.10 14.25 0.13 YZ Ceti
22. GJ 273 1 33 07 27 24.5 +05 13 33 H 3.738 171.2 H 0.26623 0.00066 YHG M3.5 V * 9.85 11.98 0.26 Luyten's Star
23. SCR 1845-6357 A 2 18 45 05.3 -63 57 48 * 2.664 076.6 * 0.25950 0.00111 *De M8.5 V * 17.40J 19.47 0.07 Henry et al. 2006
SCR 1845-6357 B - 18 45 02.6 -63 57 52 2.664 076.6 0.25950 0.00111 T6.0 V 0.03 * Biller et al. 2006
24. SO 0253+1652 1 02 53 00.9 +16 52 53 * 5.106 138.2 * 0.25941 0.00089 *GTe M6.5 V * 15.14 17.21 0.08 Henry et al. 2006
25. GJ 191 1 29 05 11 40.6 -45 01 06 H 8.670 131.4 H 0.25567 0.00091 YH M2.0 VI * 8.85 10.89 0.39 Kapteyn's Star
26. GJ 825 1 66 21 17 15.3 -38 52 03 H 3.455 250.6 H 0.25344 0.00080 YH K9.0 V * 6.67 8.69 0.60 AX Microscopii
27. DEN 1048-3956 1 10 48 14.7 -39 56 06 1.530 229.2 * 0.24853 0.00118 **De M8.5 V * 17.39 19.37 0.07 Jao et al. 2005, Costa et al. 2005
28. 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
29. GJ 234 A 2 1849 06 29 23.4 -02 48 50 H 0.930 131.7 H 0.24444 0.00092 YSG M4.5 VJ * 11.18 13.12 0.17 Ross 614 A
GJ 234 B - 1850 06 29 23.4 -02 48 50 0.930 131.7 0.24444 0.00092 M V - 14.26 16.20 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 0.23438 0.00150 YH M3.5 V * 10.10 11.95 0.26 Wolf 1061
31. GJ 35 1 7 00 49 09.9 +05 23 19 H 2.978 155.5 H 0.23270 0.00181 YH DZ7 N 12.40 14.23 0.5 * van Maanen's Star
32. GJ 1 1 1 00 05 24.4 -37 21 27 H 6.100 112.5 H 0.23032 0.00090 YH M1.5 V * 8.54 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 M5.0 VJ * 13.25 15.03 0.12 Wolf 424 A
GJ 473 B - 12 33 17.2 +09 01 15 1.811 277.4 0.22790 0.00460 M V - 13.24 15.02 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 M4.0 V * 12.31 14.07 0.14 TZ Arietis
35. GJ 687 1 450 17 36 25.9 +68 20 21 H 1.309 194.2 H 0.22047 0.00083 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 * 15.73 17.45 0.08
37. 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 VJ * 13.46 15.18 0.11 G 208-044 A
GJ 1245 C - 19 53 54.2 +44 24 55 0.731 143.1 0.22020 0.00100 M V - 16.75 18.47 0.07 orbit < 2" G 208-044 B
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
38. GJ 674 1+1P 449 17 28 39.9 -46 53 43 H 1.050 146.9 H 0.22011 0.00139 YH M2.5 V * 9.37 11.08 0.36
GJ 674 P1 - 17 28 39.9 -46 53 43 1.050 146.9 0.22011 0.00139 planet - orbit < 2"
39. GJ 440 1 43 11 45 42.9 -64 50 29 H 2.688 097.4 H 0.21612 0.00109 YH* DQ6 N 11.50 13.17 0.5 * WD 1142-645
40. GJ 876 A 1+4P 530 22 53 16.7 -14 15 49 H 1.174 125.1 H 0.21447 0.00057 YHB M3.5 V * 10.18 11.84 0.27 Ross 780
GJ 876 P1 - 22 53 16.7 -14 15 49 1.174 125.1 0.21447 0.00057 planet - orbit < 2"
GJ 876 P2 - 22 53 16.7 -14 15 49 1.174 125.1 0.21447 0.00057 planet - orbit < 2"
GJ 876 P3 - 22 53 16.7 -14 15 49 1.174 125.1 0.21447 0.00057 planet - orbit < 2"
GJ 876 P4 - 22 53 16.7 -14 15 49 1.174 125.1 0.21447 0.00057 planet - orbit < 2"
41. GJ 1002 1 2 00 06 43.8 -07 32 22 N 2.041 203.6 N 0.21300 0.00360 Y M5.0 V * 13.77 15.41 0.11
42. LHS 288 1 288 10 44 21.2 -61 12 36 * 1.643 347.7 * 0.20970 0.00265 *Y M5.5 V * 13.92 15.53 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 0.20567 0.00093 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 0.20567 0.00093 M5.5 V * 14.44 16.01 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 0.20553 0.00049 YH K7.0 V * 6.59 8.15 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 M2.5 V * 9.29 10.87 0.39
46. GJ 832 1+1P 3685 21 33 34.0 -49 00 32 H 0.819 183.2 H 0.20203 0.00100 YH M1.5 V * 8.66 10.19 0.50
GJ 832 P1 - 21 33 34.0 -49 00 32 0.819 183.2 0.20203 0.00100 planet - orbit < 2" Bailey et al. 2009
47. LP 944-020 1 03 39 35.2 -35 25 41 N 0.439 047.6 N 0.20140 0.00421 T M9.0 V * 18.69 20.21 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 0.05 * Costa et al. 2005
49. GJ 166 A 3 23 04 15 16.3 -07 39 10 H 4.088 213.2 H 0.20065 0.00023 YH K0.5 V G 4.43 5.94 0.89 omicron 2 Eridani
GJ 166 B - 24 04 15 22.0 -07 39 35 H 4.073 212.4 N 0.20065 0.00023 DA4 N 9.52 11.03 0.5 * separation 83"
GJ 166 C - 25 04 15 22.0 -07 39 35 4.073 212.4 0.20065 0.00023 M4.0 V * 11.24 12.75 0.18 orbit 7"
50. GJ 873 1 3853 22 46 49.7 +44 20 02 H 0.841 236.9 H 0.19821 0.00084 YHG M3.5 V * 10.22 11.71 0.28 EV Lacertae
51. GJ 682 1 451 17 37 03.7 -44 19 09 H 1.176 217.1 H 0.19809 0.00206 YH M4.0 V * 10.95 12.43 0.20
52. GJ 702 A 2 458 18 05 27.3 +02 30 00 H 0.971 172.6 H 0.19596 0.00087 YS K0.0 V G 4.21 5.67 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 V N 6.01 7.47 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 0.19540 0.00046 YHG 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 VJ * 14.06 15.46 0.11 EI Cancri
GJ 1116 B - 2077 08 58 14.9 +19 45 49 N 0.874 267.7 0.19120 0.00250 M V - 14.92 16.32 0.10 separation < 2"
55. G 099-049 1 06 00 03.5 +02 42 24 * 0.313 097.5 * 0.19077 0.00186 *Y 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 * M4.0 V * 12.22 13.59 0.15 Henry et al. 2006
57. 2MA 0939-2448 1 09 39 35.5 -24 48 28 M 1.192 151.2 T 0.18730 0.00460 T T8.0 V 0.03 * Burgasser et al. 2008
58. GJ 445 1 2459 11 47 41.4 +78 41 28 H 0.885 057.1 H 0.18726 0.00164 YH M3.5 V * 10.79 12.15 0.24
59. GJ 526 1 47 13 45 43.8 +14 53 29 H 2.298 129.3 H 0.18472 0.00074 YHG M1.0 V * 8.46 9.79 0.53 Wolf 498
60. GJ 169.1 A 2 26 04 31 11.8 +58 58 38 H 2.427 147.6 H 0.18052 0.00078 YH M4.0 V * 11.04 12.32 0.20 Stein 2051
GJ 169.1 B - 27 04 31 11.8 +58 58 38 2.427 147.6 0.18052 0.00078 DC5 N 12.43 13.71 0.5 * separation 8"
61. GJ 251 1 1879 06 54 49.0 +33 16 05 H 0.831 241.3 H 0.17811 0.00143 YH M3.0 V * 10.02 11.27 0.34
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 0.17599 0.00104 YH M1.0 V * 7.95 9.18 0.57 Wolf 1453
64. LP 816-060 1 20 52 33.0 -16 58 29 H 0.308 275.7 H 0.17503 0.00340 H M3.5 V * 11.50 12.72 0.19
65. 2MA 0415-0935 1 04 15 19.5 -09 35 07 M 2.255 076.5 U 0.17434 0.00276 U T8.0 V 0.03 * Vrba et al. 2004
66. GJ 764 1 477 19 32 21.6 +69 39 40 H 1.839 161.0 H 0.17379 0.00018 YH G9.0 V G 4.67 5.87 0.89 sigma Draconis
67. GJ 229 A 2 1827 06 10 34.6 -21 51 53 H 0.727 190.9 H 0.17377 0.00097 YH M1.5 V * 8.14 9.34 0.56
GJ 229 B - 06 10 34.6 -21 51 53 0.727 190.9 0.17377 0.00097 T6.0 V 0.03 * separation 8"
68. GJ 213 1 31 05 42 09.3 +12 29 22 H 2.542 128.2 H 0.17150 0.00100 YHG M4.0 V * 11.57 12.74 0.18 Ross 47
69. GJ 693 1 454 17 46 34.2 -57 19 09 H 1.756 219.6 H 0.17110 0.00222 YH M3.0 V * 10.76 11.93 0.26
70. GJ 752 A 2 473 19 16 55.3 +05 10 08 H 1.452 203.5 H 0.17096 0.00052 YHTTPo M2.5 V * 9.10 10.26 0.50 Wolf 1055
GJ 752 B - 474 19 16 58.3 +05 09 01 H 1.461 203.1 N 0.17096 0.00052 M8.0 V * 17.45 18.61 0.07 separation 74" van Biesbroeck 10
71. GJ 570 A 4 387 14 57 28.0 -21 24 56 H 2.012 149.1 H 0.17062 0.00067 YHS K4.0 V G 5.64 6.80 0.78
GJ 570 B - 386 14 57 26.5 -21 24 41 H 1.937 149.4 H 0.17062 0.00067 M1.5 VJ * 8.30 9.46 0.55 separation 22"
GJ 570 C - 14 57 26.5 -21 24 41 1.937 149.4 0.17062 0.00067 M V - 9.96 11.12 0.36 orbit < 2"
GJ 570 D - 14 57 15.0 -21 21 50 2.012 149.1 0.17062 0.00067 T7.0 V 0.03 * separation 258"
72. GJ 754 1 60 19 20 48.0 -45 33 27 N 2.945 167.3 N 0.16917 0.00153 *Y M4.0 V * 12.23 13.37 0.16 Jao et al. 2005
73. GJ 588 1 397 15 32 12.9 -41 16 32 H 1.564 228.9 H 0.16852 0.00127 YH M2.5 V * 9.31 10.44 0.46
74. GJ 1005 A 2 1047 00 15 28.1 -16 08 02 H 0.955 130.3 H 0.16835 0.00090 YSHe M3.5 VJ * 11.60 12.73 0.18
GJ 1005 B - 00 15 28.1 -16 08 02 0.955 130.3 0.16835 0.00090 M V - 14.02 15.15 0.11 orbit < 2"
75. GJ 34 A 2 123 00 49 06.3 +57 48 55 H 1.223 117.2 H 0.16823 0.00046 YH G3 V N 3.46 4.59 1.11 eta Cassiopei A
GJ 34 B - 122 00 49 06.3 +57 48 55 1.223 117.2 0.16823 0.00046 K7.0 V * 7.21 8.34 0.60 orbit 12" eta Cassiopei B
76. GJ 663 A 3 437 17 15 21.0 -26 36 10 H 1.238 202.5 H 0.16812 0.00040 YYHH K1.5 VJ G 5.07 6.20 0.85 36 Ophiuchi A
GJ 663 B - 438 17 15 21.0 -26 36 10 1.238 202.5 0.16812 0.00040 K V - 5.08 6.21 0.85 orbit 14" 36 Ophiuchi B
GJ 664 - 439 17 16 13.4 -26 32 46 H 1.222 203.1 H 0.16812 0.00040 K5.0 V G 6.32 7.45 0.71 separation 732" 36 Ophiuchi C
77. GJ 908 1 550 23 49 12.5 +02 24 04 H 1.388 134.2 H 0.16802 0.00118 YH M1.0 V * 8.98 10.11 0.51
78. GJ 285 1 1943 07 44 40.2 +03 33 09 H 0.568 217.4 H 0.16719 0.00205 YH M4.0 V * 11.19 12.31 0.20 Ross 882
79. GJ 783 A 2 486 20 11 11.9 -36 06 04 H 1.640 163.8 H 0.16626 0.00027 YH K2.5 V G 5.31 6.42 0.82
GJ 783 B - 487 20 11 11.9 -36 06 04 1.640 163.8 0.16626 0.00027 M4.0 V * 11.50 12.61 0.19 separation 7"
80. GJ 139 1 19 03 19 55.6 -43 04 11 H 3.124 076.6 H 0.16547 0.00019 YH G8.0 V G 4.26 5.35 0.97 82 Eridani
81. GJ 1221 1 455 17 48 06.7 +70 52 29 N 1.651 311.0 N 0.16470 0.00240 Y DXP9 N 14.22 15.30 0.5 *
82. GJ 338 A 2 260 09 14 22.8 +52 41 12 H 1.634 249.8 H 0.16373 0.00252 YHH M0.0 V * 7.64 8.71 0.60
GJ 338 B - 261 09 14 24.7 +52 41 11 H 1.684 247.1 H 0.16373 0.00252 K7.0 V * 7.70 8.77 0.60 orbit 17"
83. GJ 780 1 485 20 08 43.6 -66 10 55 H 1.656 133.0 H 0.16371 0.00017 YH G8.0 IV G 3.55 4.62 1.10 delta Pavonis
84. GJ 268 A 2 226 07 10 01.8 +38 31 46 H 1.045 204.9 H 0.16341 0.00178 YH M4.5 VJ * 12.05 13.12 0.17 QY Aurigae A
GJ 268 B - 07 10 01.8 +38 31 46 1.045 204.9 0.16341 0.00178 M V - 12.45 13.52 0.16 orbit < 2" QY Aurigae B
85. 2MA 0937+2931 1 09 37 34.9 +29 31 41 M 1.622 143.1 U 0.16330 0.00160 USc T6.0 V 0.03 * Vrba et al. 2004
86. GJ 784 1 3531 20 13 53.4 -45 09 50 H 0.794 101.6 H 0.16135 0.00099 YH M0.0 V * 7.95 8.99 0.58
87. GJ 555 1 2945 14 34 16.8 -12 31 10 H 0.694 329.0 H 0.16078 0.00198 YH* M4.0 V * 11.32 12.35 0.20 HN Librae
88. GJ 896 A 2 3965 23 31 52.2 +19 56 14 H 0.558 096.4 H 0.15988 0.00153 YHW M3.5 V * 10.27 11.29 0.33 EQ Pegasi
GJ 896 B - 3966 23 31 52.2 +19 56 14 0.558 096.4 0.15988 0.00153 M4.5 V * 12.21 13.43 0.16 orbit 7"
89. GJ 581 1+4P 394 15 19 26.8 -07 43 20 H 1.229 265.4 H 0.15780 0.00176 YH* M3.0 V * 10.57 11.56 0.30 Wolf 562
GJ 581 P1 - 15 19 26.8 -07 43 20 1.229 265.4 0.15780 0.00176 planet - orbit < 2" Bonfils et al. 2005
GJ 581 P2 - 15 19 26.8 -07 43 20 1.229 265.4 0.15780 0.00176 planet - orbit < 2" Udry et al. 2007
GJ 581 P3 - 15 19 26.8 -07 43 20 1.229 265.4 0.15780 0.00176 planet - orbit < 2" Udry et al. 2007
GJ 581 P4 - 15 19 26.8 -07 43 20 1.229 265.4 0.15780 0.00176 planet - orbit < 2" Mayor et al. 2009
90. LHS 2090 1 2090 09 00 23.6 +21 50 05 * 0.774 221.2 * 0.15687 0.00267 * M6.0 V * 16.10 17.08 0.09 Henry et al. 2006
91. 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
92. 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 VJ * 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 M V - 10.35 11.32 0.33 orbit < 2"
93. GJ 223.2 1 32 05 55 09.7 -04 10 17 N 2.377 166.6 N 0.15605 0.00075 Y** DZ9 N 14.47 15.44 0.5 * WD 0552-041
94. G 180-060 1 16 31 18.4 +40 51 54 N 0.358 330.0 N 0.15600 0.00400 Du M5.0 V 14.76 15.73 0.10
95. GJ 644 A 5 428 16 55 28.8 -08 20 11 H 1.208 223.3 H 0.15496 0.00052 YYHS* M2.5 VJ * 9.72 10.67 0.42 Wolf 630 A
GJ 644 B - 16 55 28.8 -08 20 11 1.208 223.3 0.15496 0.00052 M V - 10.37 11.32 0.33 orbit < 2" Wolf 630 B
GJ 644 D - 16 55 28.8 -08 20 11 1.208 223.3 0.15496 0.00052 M V - 10.87 11.82 0.27 orbit < 2" Wolf 630 C
GJ 644 C - 429 16 55 35.8 -08 23 40 H 1.190 222.5 N 0.15496 0.00052 M7.0 V * 16.78 17.73 0.08 separation 221" van Biesbroeck 8
GJ 643 - 427 16 55 25.2 -08 19 21 H 1.210 222.3 H 0.15496 0.00052 M3.0 V * 11.80 12.75 0.18 separation 72" Wolf 629
96. GJ 625 1 16 25 24.6 +54 18 15 H 0.465 111.5 H 0.15314 0.00092 YH M1.5 V * 10.10 11.03 0.37
97. GJ 1128 1 271 09 42 46.4 -68 53 06 1.121 356.7 * 0.15305 0.00241 * M4.0 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 M4.5 V * 13.80 14.72 0.12 GL Virginis
99. GJ 892 1 71 23 13 17.0 +57 10 06 H 2.095 081.9 H 0.15284 0.00028 YH K3.0 V G 5.57 6.49 0.81
100. LHS 3003 1 3003 14 56 38.5 -28 09 51 N 0.965 210.1 N 0.15249 0.00202 YT* M7.0 V * 17.05 17.97 0.08
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FORMER TOP 100 MEMBERS PUSHED OUT BY NEW MEMBERS
_______________________________________________________________________________________________________________________________________________________________________________________________
101. GJ 408 1 11 00 04.3 +22 49 59 H 0.510 236.7 H 0.14932 0.00158 YH M2.5 V * 10.02 10.89 0.39 Ross 104
102. GJ 829 A 2 508 21 29 36.8 +17 38 36 H 1.076 069.5 H 0.14901 0.00169 YH M3.0 VJ * 11.05 11.92 0.26 Ross 775 A
GJ 829 B - 21 29 36.8 +17 38 36 1.076 069.5 0.14901 0.00169 M V - 11.05 11.92 0.26 orbit < 2" Ross 775 B
103. G 041-014 A 3 08 58 56.3 +08 28 26 * 0.503 130.0 * 0.14766 0.00198 * M3.5 VJ * 11.94 12.79 0.18 Henry et al. 2006
G 041-014 B - 08 58 56.3 +08 28 26 * 0.503 130.0 * 0.14766 0.00198 * M V - 12.14 12.99 0.17
G 041-014 C - 08 58 56.3 +08 28 26 * 0.503 130.0 * 0.14766 0.00198 * M V - 12.28 13.13 0.17
104. GJ 566 A 2 14 51 23.4 +19 06 02 H 0.169 115.0 H 0.14757 0.00072 YS G7.0 V G 4.67 5.51 0.94 ksi Bootis A
GJ 566 B - 14 51 23.4 +19 06 02 0.169 115.0 0.14757 0.00072 K4 V N 6.94 7.78 0.67 orbit 5" ksi Bootis B
105. GJ 402 1 294 10 50 52.1 +06 48 29 H 1.150 225.1 N 0.14715 0.00298 YH M4.0 V * 11.65 12.49 0.20 EE Leonis
106. GJ 880 1 533 22 56 34.8 +16 33 12 H 1.071 254.7 H 0.14637 0.00095 YH M1.5 V * 8.65 9.48 0.55 Ross 671
107. 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
108. LP 771-095 A 3 03 01 51.4 -16 35 36 * 0.477 234.4 * 0.14381 0.00249 **H M2.5 V * 11.22 12.01 0.25 Henry et al. 2006
LP 771-095 B - 03 01 51.0 -16 35 31 * 0.479 235.5 * 0.14381 0.00249 **H M3.5 VJ * 11.79 12.58 0.19 separation 7" LP 771-096
LP 771-095 C - 03 01 51.0 -16 35 31 * 0.479 235.5 * 0.14381 0.00249 **H M V - 12.65 13.44 0.16 separation < 2"
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FORMER TOP 100 CANDIDATES EXCUSED BY NEW RECONS PARALLAXES
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XXX. 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
XXX. 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 0.18 separation 21"
GJ 2130 C - 17 46 14.4 -32 06 08 0.281 196.0 0.16177 0.01129 H M V - 12.75 13.79 0.15 orbit < 2"
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PARALLAX REFERENCES
* = RECONS program (see Jao et al. 2005 and Henry et al. 2006 for background)
B = Benedict (various)
De = Deacon (various)
Du = Ducourant et al. 1998
G = Gatewood (various)
Gi = Girard et al. 2000
He = Hershey 1998
H = Hipparcos, where for 2010 we have updated the 1997 Hipparcos parallaxes with the 2007 van Leeuwen values
Po = Pravdo et al. 2009
Sc = Schilbach et al. 2009
S = Soderjhelm 1999
T = Tinney (various)
Te = Teegarden et al. 2004
U = United States Naval Observatory (USNO) program
W = Weis et al. 1999
Y = Yale Parallax Catalog
REFERENCES FOR POSITIONS, PROPER MOTIONS, AND SPECTRAL TYPES
* = RECONS program (see Henry et al. 1997 and Henry et al. 2006 for background)
G = Gray et al. 2003
H = Hipparcos
M = 2MASS
N = Catalog of Nearby Stars (CNS) by Gliese & Jahreiss 1957, 1969, 1979, 1991
Pl = Provencal et al. (2002)
S = Scholz et al. 2003
T = Tinney (various)
U = United States Naval Observatory (USNO) program
O = Oppenheimer et al. 1995
COLUMNS
(1) name as given in the Catalog of Nearby Stars (1991) by Gliese and Jahreiss
(2) number of known objects in the system, where +nP represents the number (n) of planets
(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 of 1.00 Msun) 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 = 20.5, where 0.05 or 0.03 is assigned, depending on the spectral
type), or are white dwarfs (for which 0.5 is typically listed)