Adopted distance estimates
Object | Parallax, mas | Distance, pc | Distance, ly | Distance, Pm | Source | ||
---|---|---|---|---|---|---|---|
Systems with an F-type main-sequence star (yellow-white dwarf) as primary member. | |||||||
Procyon | 285.93±0.88 | 3.497±0.011 | 11.41+0.04 −0.03 |
107.9±0.3 | Perryman et al. (1997)[1] | ||
Systems with a G-type main-sequence star (yellow dwarf) as primary member. | |||||||
Tau Ceti | 273.96±0.17 | 3.6502±0.0023 | 11.905±0.007 | 112.63±0.07 | van Leeuwen (2007)[2] | ||
Systems with a K-type main-sequence star (orange dwarf) as primary member. | |||||||
Epsilon Eridani | 311.37±0.1 | 3.2116±0.001 | 10.475±0.003 | 99.1±0.03 | Benedict et al. (2006)[3] | ||
61 Cygni | 285.88±0.54 | 3.498±0.007 | 11.409±0.022 | 107.94±0.2 | van Leeuwen (2007) (B)[4] | ||
Epsilon Indi | 276.06±0.28 | 3.622±0.004 | 11.815±0.012 | 111.78±0.11 | van Leeuwen (2007)[5] | ||
Systems with an M-type main-sequence star (red dwarf) as primary member. | |||||||
Ross 248 | 316.72±0.72 | 3.157±0.007 | 10.298±0.023 | 97.43±0.22 | Gatewood (2008)[6] | ||
Lacaille 9352 | 305.26±0.70 | 3.276+0.008 −0.007 |
10.685+0.025 −0.024 |
101.08±0.23 | van Leeuwen (2007)[7] | ||
Ross 128 | 298.2±1.7 | 3.353±0.019 | 10.94±0.06 | 103.5±0.6 | van Altena et al. (1995)[8] | ||
EZ Aquarii | 294.3±3.5 | 3.4±0.04 | 11.08±0.13 | 104.8+1.3 −1.2 |
Gliese & Jahreiß (1991)[9] | ||
Struve 2398 | 286.1±1.8 | 3.495±0.022 | 11.4±0.07 | 107.9±0.7 | Gliese & Jahreiß (1991)[10] | ||
Groombridge 34 | 278.76±0.77 | 3.587±0.01 | 11.7±0.03 | 110.69+0.31 −0.3 |
van Leeuwen (2007)[11] | ||
SIPS 1259-4336 | 276±41 | 3.6+0.6 −0.5 |
11.8+2.1 −1.5 |
111.8+19.5 −14.5 |
Deacon et al. (2005)[12] | ||
DX Cancri | 275.8±3.0 | 3.63±0.04 | 11.83±0.13 | 111.9±1.2 | Gliese & Jahreiß (1991)[13] | ||
GJ 1061 | 270.86±1.29 | 3.692+0.018 −0.017 |
12.04±0.06 | 113.9±0.5 | Lurie et al. (2014)[14] | ||
YZ Ceti | 267.4±3.0 | 3.74±0.04 | 12.2±0.14 | 115.4±1.3 | Gliese & Jahreiß (1991)[15] | ||
Luyten's Star | 267.36±0.79 | 3.74±0.011 | 12.2±0.04 | 115.4±0.3 | Gatewood (2008)[6] | ||
Kapteyn's Star | 255.26±0.86 | 3.918±0.013 | 12.78±0.04 | 120.9±0.4 | Perryman et al. (1997)[16] | ||
Lacaille 8760 | 253.41±0.80 | 3.946±0.012 | 12.87±0.04 | 121.8±0.4 | van Leeuwen (2007)[17] | ||
Kruger 60 | 247.5±1.5 | 4.04+0.025 −0.024 |
13.18±0.08 | 124.7±0.8 | Söderhjelm (1999) [18] | ||
Ross 614 | 244.07±0.73 | 4.097±0.012 | 13.36±0.04 | 126.4±0.4 | Gatewood et al. (2003) (weighted mean)[19] | ||
Wolf 1061 | 232.98±1.60 | 4.292+0.03 −0.029 |
14±0.1 | 132.4±0.9 | van Leeuwen (2007)[20] | ||
Wolf 424 | 232.2±4.3 | 4.31±0.08 | 14.05+0.27 −0.26 |
132.9+2.5 −2.4 |
Gliese & Jahreiß (1991)[21] | ||
Gliese 1 | 230.42±0.90 | 4.34±0.017 | 14.15±0.06 | 133.9±0.5 | van Leeuwen (2007)[22] | ||
TZ Arietis | 224.8±2.9 | 4.45±0.06 | 14.51+0.19 −0.18 |
137.3+1.8 −1.7 |
van Altena et al. (1995)[23] | ||
LHS 292 | 221.0±3.6 | 4.52±0.07 | 14.76±0.24 | 139.6+2.3 −2.2 |
Gliese & Jahreiß (1991)[24] | ||
Gliese 687 | 220.85±0.92 | 4.528±0.019 | 14.77±0.06 | 139.7±0.6 | Perryman et al. (1997)[25] | ||
Gliese 674 | 220.24±1.42 | 4.541±0.029 | 14.81+0.1 −0.09 |
140.1±0.9 | van Leeuwen (2007)[26] | ||
G 208-44/208-45 | 220.2±1.0 | 4.541±0.021 | 14.81±0.07 | 140.1±0.6 | van Altena et al. (1995)[27] | ||
Systems with a white dwarf star as primary member. | |||||||
van Maanen's star | 232.5±1.9 | 4.3+0.04 −0.03 |
14.03+0.12 −0.11 |
132.7±1.1 | van Altena et al. (1995)[28] | ||
Systems with an M-type brown dwarf as primary member. | |||||||
SCR 1845-6357 | 259.45±1.11 | 3.854+0.017 −0.016 |
12.57±0.05 | 118.9±0.5 | Henry et al. (2006)[29] | ||
Teegarden's star | 259.25±0.94 | 3.857±0.014 | 12.58±0.05 | 119±0.4 | Gatewood et al. (2009)[30] | ||
DEN 1048-3956 | 248.08±0.61 | 4.031±0.01 | 13.15±0.03 | 124.38±0.31 | Lurie et al. (2014)[14] | ||
2M1540 | 228±24 | 4.4+0.5 −0.4 |
14.3+1.7 −1.4 |
135.3+15.9 −12.9 |
Pérez Garrido et al. (2014)[31] | ||
Systems with a T-type brown dwarf as primary member. | |||||||
WISE 1506+7027 | 310±42 | 3.4+0.7 −0.4 |
11.1+2.3 −1.3 |
Marsh et al. (2013)[32] | |||
UGPS 0722-05 | 242.8±2.4 | 4.12±0.04 | 13.43±0.13 | 127.1+1.3 −1.2 |
Leggett et al. (2012)[33] | ||
Systems with a Y-type brown dwarf as primary member. | |||||||
WISE 0350-5658 | 291±50 | 3.7+1.6 −0.4 |
12.1+5.2 −1.3 |
Marsh et al. (2013)[32] | |||
For other distance estimates see articles on these objects. |
See also
|
References
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