THE ONE HUNDRED NEAREST STAR SYSTEMS

brought to you by RECONS (Research Consortium On Nearby Stars)

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                     
                                                                                                                                              
_______________________________________________________________________________________________________________________________________________________________________________________________

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"

_______________________________________________________________________________________________________________________________________________________________________________________________

FORMER TOP 100 CANDIDATES EXCUSED BY NEW RECONS PARALLAXES
_______________________________________________________________________________________________________________________________________________________________________________________________


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"          

_______________________________________________________________________________________________________________________________________________________________________________________________

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)