Draft:List of nearest stars by spectral type
This is a list of the nearest stars separated by spectral type.
List of nearest M-type stars[edit]
This is a list of M-type stars within 12 light years.
Name | Distance (ly) | Spectral type | Stellar radius (R☉) | Stellar mass (M☉) | Apparent magnitude (V) | Absolute magnitude (V) | Notes | |
---|---|---|---|---|---|---|---|---|
Proxima Centauri | 4.24[1] | M5.5Ve[1] | 0.1542 ± 0.0045[2] | 0.1221 ± 0.0022[2] | 10.43 – 11.1[3] | 15.6[4] | Also the nearest star to the Solar System. | |
Barnard's Star | 5.96 | M4.0V[5] | 0.187 ± 0.001[6] | 0.161[6] | 9.511[7] | 13.21[7] | Also the second-nearest stellar system to the Solar System. | |
Wolf 359 | 7.856±0.001 | M6V[8] | 0.144 ± 0.004[6] | 0.11 ± 0.003[6] | 13.507[9] | 16.614[10] | Also the fourth-nearest stellar system to the Solar System. | |
Lalande 21185 | 8.034[11] | M2V[12] | 0.392 ± 0.004[6] | 0.389 ± 0.008[6] | 7.52[13] | 10.48[14] | Also the fifth-nearest stellar system to our Solar System. | |
Luyten 726-8 | B | 8.72±0.01 | M6V[15] | 0.159 ± 0.006[16] | 0.1195 ± 0.0043[16] | 12.8[10] | 15.7[10] | Also known as UV Ceti. |
A | 8.87±0.02 | M5.5V[15] | 0.165 ± 0.006[16] | 0.1225 ± 0.0043[16] | The archetype of the flare stars. Also known as BL Ceti | |||
Ross 154 | 9.706[17] | M3.5V[18] | 0.200 ± 0.008[6] | 0.177 ± 0.004[6] | 10.44[18] | 13.07[18] | ||
Ross 248 | 10.306[19] | M6V[20] | 0.19[21] | 0.145[21] | 12.23 – 12.34[18] | 14.79[22] | ||
Lacaille 9352 | 10.74[11] | M0.5V[23] | 0.474 ± 0.008[6] | 0.479+0.011 −0.010[6] |
7.34[24] | 9.8[25] | ||
Ross 128 | 11.007±0.001 | M4V[26] | 0.198 ± 0.007[6] | 0.176 ± 0.004[6] | 11.13[18] | 13.53[18] | ||
EZ Aquarii | A | 11.11 | M5V[18] | 0.175[27] | 0.1187 ± 0.0011[28] | 13.03[18] | 15.33[18] | |
B | 0.21 ± 0.04[28] | 0.1145 ± 0.0012[28] | 13.27[18] | 15.58[18] | ||||
C | 0.093[28] | 12.38[18] | 17.37[18] | |||||
Struve 2398 | A | 11.4908[17] | M3V[21] | 0.354 ± 0.003[6] | 0.336 ± 0.007[6] | 8.94 | ||
B | 11.491[17] | M3.5V[21] | 0.273 ± 0.011[21] | 0.248 ± 0.235[21] | 9.7[29] | |||
Groombridge 34 | A | 11.6191±0.0008[17] | M1.4V[21] | 0.385 ± 0.002[21] | 0.393+0.009 −0.008[21] |
8.119[21] | ||
B | 11.62[17] | M4.1V[21] | 0.18 ± 0.03[30] | 0.15 ± 0.02[30] | 11.007[21] | |||
DX Cancri | 11.68 | M6.5V[31] | 0.11[32] | 0.09[33] | 14.81[34] | 16.98[18] | ||
GJ 1061 | 11.984[35] | M5.5V[35] | 0.152 ± 0.007[6] | 0.125 ± 0.003[6] | 13.03[35] | 15.26[36] | ||
YZ Ceti | 12.122±0.002 | M4Ve | 0.168 ± 0.009[29] | 0.13 ± 0.013[37] | 12.03 – 12.18[38] | 14.3[39] | ||
Luyten's Star | 12.348±0.002 | M3.5V[18] | 0.293 ± 0.007[40] | 0.29[40] | 0.987[41] | 11.94[41] | ||
Teegarden's Star | 12.497±0.004[42] | M7V[39] | 0.107 ± 0.004[43] | 0.093 ± 0.003[43] | 15.13[44] | 17.2[45] | ||
Kapteyn's Star | 12.83 [46] | M1.5V[47][23] or sdM1[7] | 0.291 ± 0.025[47] | 0.281 ± 0.014[47] | 8.853 ± 0.008[47] | 10.89[7] | ||
Lacaille 8760 | 12.947 | M0Ve[48] | 0.51[49] | 0.6[18] | 6.67[18] | 8.69[18] | Brightest red dwarf in the sky. |
List of nearest K-type stars[edit]
This is a list of K-type stars within 30 light years.
Name | Distance (ly) | Spectral type | Stellar radius (R☉) | Stellar mass (M☉) | Apparent magnitude (V) | Absolute magnitude (V) | Notes | |
---|---|---|---|---|---|---|---|---|
Alpha Centauri B (Toliman) | 4.344 | K1V[50] | 0.8591 ± 0.0036[51] | 0.9092 ± 0.0025[51] | 1.33[52] | 5.71[53] | Also the 2nd/3rd nearest individual star to the Solar System. Named Toliman. | |
Epsilon Eridani (Ran) | 10.475 | K2V[54] | 0.735 ± 0.005[23] | 0.82 ± 0.02[55][56] | 3.736[57] | 6.19[18] | Also the tenth-nearest star system to our Solar System. Has one confirmed exoplanet | |
61 Cygni | A | 11.404 | K5V[58] | 0.665 ± 0.005[59] | 0.7[60] | 5.21[61] | 7.506[62] | The first star to have its distance to Earth measured after the Sun. Also the 15th nearest stellar system to our solar system. |
B | K7V[58] | 0.595 ± 0.008[59] | 0.63[60] | 6.05[63] | 8.228[62] | |||
Epsilon Indi A | 11.867 | K5V[23] | 0.711 ± 0.005[64] | 0.754 ± 0.038[21] | 4.83[11] | 6.89[65] | Also the 19th nearest star system to our Solar System. Has one confirmed exoplanet and 2 brown dwarfs. | |
Groombridge 1618 | 15.886 | K7.5Ve[66] | 0.605 ± 0.02[67] | 0.67 ± 0.033[67] | 6.6[68] | 8.11[69] | ||
40 Eridani A | 16.33[17] | K0.5V[54] | 0.812 ± 0.017[70] | 0.78 ± 0.08[70] | 4.43[11] | 5.93[69] | Part of a triple star system | |
70 Ophiuchi | A | 16.68 | K0V[71] | 0.91 ± 0.03[71] | 0.9 ± 0.03[72] | 4.13[73] | 5.49[69] | |
B | 16.707 | K4V[71] | 0.7 ± 0.07[72] | 6.07[73] | ||||
Sigma Draconis (Alsafi) | 18.799 | K0V[74] | 0.776 ± 0.008[75] | 0.85+0.01 −0.03[76] |
4.674[77] | 5.89[78] | ||
Gliese 570 A | 19.199[79] | K4V[79] | 0.739 ± 0.019[23] | 0.82 ± 0.04[23] | 5.7[79] | 6.89[69] | Part of a quadruple star system | |
Eta Cassiopeiae B | 19.42[11] | K7V[72] | 0.66[14] | 0.57[72] | 7.51[72] | Part of a binary star system | ||
36 Ophiuchi | A | 19.41 | K2V[80] | 0.817 ± 0.016[23] | 0.85 | 5.08[80] | Also known as Guniibuu | |
B | K1V[80] | 0.81 | 5.03[80] | |||||
C | 19.418±0.004 | K5V[80] | 0.72 | 0.71 | 6.34[80] | |||
HR 7703 A | 19.61 | K2.5V[54] | 0.66[81] | 0.65[81] | 5.31[82] | 6.53[83] | Part of a binary system | |
ADS 7251 B | 20.658±0.003 | K7V[15] | 0.58 ± 0.03[84] | 0.64 ± 0.07[84] | 7.7[23] | Part of a binary star system | ||
HD 219134 | 21.336 | K3V[85] | 0.778 ± 0.005[86] | 0.81 ± 0.03[86] | 5.574[77] | Has six known exoplanets | ||
Xi Boötis B | 23.011±0.008 | K4Ve[87] | 0.61[88] | 0.66 ± 0.07[88] | 6.8[87] | Part of a binary star system | ||
268 G. Ceti A | 23.58 | K3V[89] | 0.65 ± 0.053[89] | 0.7 ± 0.1[90] | 5.83[89] | Part of a trinary stellar system also known as Gliese 105 | ||
Gliese 667 | A | 23.623±0.005 | K3V[91][92] | 0.76[91] | 0.73[93] | 5.91[91] | Part of a triple star system | |
B | K5V[91][92] | 0.7[91] | 0.69[93] | 7.2[91] | ||||
HD 4628 | 24.25±0.01[94] | K2.5V[54] | 0.749 ± 0.051[89] | 0.7 ± 0.1[95] | 5.74[96] | |||
TW Piscis Austrini | 24.793±0.005 | K5Vp[54] | 0.629 ± 0.051[23] | 0.725 ± 0.036[23] | 5.44 – 6.51[97] | Also known as Fomalhaut B. Part of a triple star system | ||
107 Piscium | 24.8±0.03[94] | K1V[74] | 0.82 ± 0.03[98] | 0.86[98] | 5.14 — 5.26[99] | |||
Gliese 673 | 25.157±0.003 | K7V[7] | 0.564[89] | 7.492[7] | ||||
p Eridani | A | 26.710±0.008 | K2V[54] | 0.75[17] | 0.78[100] | 5.76[101] | ||
B | 26.733±0.007 | 0.77[17] | 0.77[100] | 5.87[101] | ||||
Gliese 884 | 26.85[102] | K7V[102] | 0.67[102] | 0.63[102] | 7.9[102] | |||
Chi Draconis B | 27.17±0.03 | K0V[28] | 0.73 ± 0.11[28] | 0.748 ± 0.017[28] | 3.57 (combined)[103] | Part of a binary star system | ||
HR 1614 | 28.4±0.1[11] | K3V[104] | 0.78+0.03 −0.02[49] |
0.838+0.034 −0.033[49] |
6.208[104] | |||
HD 50281 | 28.54±0.01 | K3.5V[105] | 0.73+0.01 −0.02[94] |
0.79[106] | 6.58[107] | |||
HD 192310 | 28.74±0.01 | K2+ V[108] | 0.79 – 0.85[91] | 0.78 ± 0.04[109] | 5.73[108] | |||
AK Leporis | 29±0.004 | K2V[110] | 0.8[17] | 6.141[111] | ||||
Delta Eridani (Rana) | 29.49±0.08[11] | K0 IV[112] | 2.327 ± 0.029[71] | 1.33 ± 0.07[71] | 3.51 – 3.56[3] |
List of nearest G-type stars[edit]
This is a list of G-type stars within 40 light years.
Name | Distance (ly) | Spectral type | Stellar radius (R☉) | Stellar mass (M☉) | Apparent magnitude (V) | Absolute magnitude (V) | Notes | |
---|---|---|---|---|---|---|---|---|
Sun | 1.58 × 10-5 (149,600,000 km) | G2V | -26.74[113] | 4.83[113] | The star at the centre of the Solar System. | |||
Alpha Centauri A (Rigil Kentaurus) | 4.344±0.002 | G2V[50] | 1.2175 ± 0.0055[51] | 1.0788 ± 0.0029[51] | 0.01[52] | 4.38[53] | It is the 2nd/3rd nearest individual star to the Solar System, and the fourth-brightest individual star in the night sky. Has one candidate exoplanet. | |
Tau Ceti | 11.912±0.007 | G8V[74] | 0.793 ± 0.004[114] | 0.783 ± 0.012[114] | 3.5[114] | 5.68[114] | Also the 20nd nearest star system to the Solar System. Has one confirmed exoplanet. | |
Eta Cassiopeiae A (Achird) | 19.42[11] | G0V[115] | 1.0386 ± 0.0038[116] | 0.972 ± 0.012[75] | 3.44[108] | 4.57[69] | Part of a binary star system | |
82 G. Eridani | 19.704±0.009 | G6V[74] | 0.92[14] | 0.7[117] | 4.254 | 5.34[69] | Has two confirmed exoplanets and one unconfirmed | |
Delta Pavonis | 19.89[17] | G8 IV[54] | 1.197 ± 0.016[64] | 1.051 ± 0.062[118] | 3.56[119] | 4.62[69] | The nearest undisputed subgiant. | |
Xi Boötis A | 22.027[120] | G8Ve[120] | 0.817 ± 0.007[88] | 0.88 ± 0.03[88] | 4.7[120] | 5.54[121] | Part of a binary star system | |
Beta Hydri | 24.33[11] | G2 IV[122] | 1.809 ± 0.015[123] | 1.08 ± 0.03[122] | 2.8[108] | 3.45[124] | ||
Mu Cassiopeiae Aa (Marfak) | 25.03±0.08 | G5Vb[74] | 0.789 ± 0.008[125] | 0.744 ± 0.0122[125] | 5.14[126] | 5.78[127] | Part of a binary star system | |
Mu Herculis Aa | 27.11±0.04 | G5IV[128] | 1.73 ± 0.02[129] | 1.11 ± 0.01[129] | 3.417[11] | 3.82[129] | Part of a quadruple star system | |
Chara | 27.63±0.04[17] | G0V[130] | 1.123 ± 0.028[75] | 0.97 ± 0.04[130] | 4.25[130] | 4.64[69] | ||
61 Virginis | 27.84±0.03 | G7V[105] | 0.9867 ± 0.0048[131] | 0.93[131] | 4.74 | 5.07[69] | Has three confirmed exoplanets | |
Chi1 Orionis A | 28.26±0.07 | G0V[74] | 0.979 ± 0.009[75] | 1.01[132] | 4.38 – 4.41[133] | 4.82[121] | ||
41 G. Arae A | 28.67±0.02 | G8V[134] | 0.79[49] | 0.81[49] | 5.61 | 5.74[69] | Part of a binary star system | |
Xi Ursae Majoris Ba | 29 | G2V[74] | 0.92 ± 0.04[135] | 0.86[135] | 4.264[136] | 4.66[a] | Part of a quadruple star system | |
Groombridge 1830 (Argelander's Star) | 29.93[94] | G8VIp[137] | 0.681 ± 0.006[75] | 0.661[49] | 6.44[68] | 6.64[69] | ||
Beta Comae Berenices | 29.95±0.1 | G0V[138] | 1.106 ± 0.011[75] | 1.15[49] | 4.26[108] | 4.46[69] | ||
HD 102365 A | 30.4±0.02 | G2V[54] | 0.96[49] | 0.889[49] | 4.88[82] | 5.07[69] | Part of a binary star system | |
61 Ursae Majoris | 31.24±0.04[94] | G8V[139] | 0.86 ± 0.02[140] | 0.93 ± 0.02[141] | 5.35[142] | 5.53[121] | ||
Alpha Mensae A | 33.31±0.02 | G7V[54] | 0.96 ± 0.013[143] | 0.964 ± 0.037[143] | 5.09 | 5.03[69] | Part of a binary star system | |
Iota Persei | 34.38±0.08[11] | G0V[74] or F9.5V[54] | 1.412 ± 0.009[75] | 1.35 ± 0.08[144] | 4.062[145] | 3.94[69] | ||
Zeta Herculis A | 35±0.2[11] | G7V[128] | 0.915 – 0.92[146] | 0.98 ± 0.02[146] | 2.81 (combined)[108] | 2.65 (combined)[147] | Part of a binary star system | |
Delta Trianguli A | 35.2±0.1 | G0V[148] | 0.98[91] | 1[149] | 4.865[69] | 4.69[69] | Part of a binary star system | |
11 Leonis Minoris A | 36.54±0.08 | G8V[150] | 1.0029 ± 0.0158[116] | 0.964[116] | 5.54[151] | 5.25[121] | Part of a binary star system | |
Eta Boötis A (Muphrid) | 37.2±0.5[11] | G0IV[152] | 2.672 ± 0.028[153] | 1.71 ± 0.05[153] | 2.68[69] | 2.41[103] | Part of a binary star system | |
Lambda Serpentis | 38.87±0.07[17] | G0V[154] | 1.06 ± 0.152[89] | 1.14[144] | 4.43[155] | 4.01[69] | ||
Zeta Reticuli | A | 39.27±0.03 | G3-5V[156] | 0.92[49] | 0.958[49] | 5.52[82] | 5.11[69] | |
B | 39.29±0.09 | G2V[156] | 0.99[49] | 0.985[49] | 5.22[82] | 4.83[69] | ||
85 Pegasi A | 39.5±0.4[157] | G5Vb | 0.91 | 0.88 | 5.75 | 5.32[69] | Part of a binary star system |
List of nearest F-type stars[edit]
This is a list of F-type stars within 45 light years.
Name | Distance (ly) | Spectral type | Stellar radius (R☉) | Stellar mass (M☉) | Apparent magnitude (V) | Absolute magnitude (V) | Notes | |
---|---|---|---|---|---|---|---|---|
Procyon A | 11.46±0.05[11] | F5IV-V[158] | 2.048 ± 0.025[158] | 1.499 ± 0.031[159] | 0.34[158] | 2.66[22] | Part of a binary star system. Eight-brightest star in the night sky. | |
Pi3 Orionis (Tabit) | 26.32±0.04[11] | F6V[137] | 1.323 ± 0.004[75] | 1.236[49] | 3.16[137] | 3.65[69] | ||
Chi Draconis A | 27.17±0.03 | F7V[28] | 1.2 ± 0.09[28] | 1.029 ± 0.06[28] | 3.57[103] | 4.04[103] | Part of a binary system | |
Zeta Tucanae | 28.01±0.04[11] | F9.5V[54] | 1.08 ± 0.08[81] | 0.99 ± 0.02[109] | 4.23 | 4.67[121] | ||
Xi Ursae Majoris A (Alula Australis) | 29±1 | F8.5:V[74] | 1.02 ± 0.04[98] | 0.97[98] | 4.264[136] | 4.66[b] | Part of a five-star system | |
Gamma Leporis | 29.12±0.05 | F6V[160] | 1.33 ± 0.04[161] | 1.23 ± 0.05[161] | 3.587[162] | 3.84[69] | ||
Gamma Pavonis | 30.21±0.05[11] | F9 V Fe-1.4 CH-0.7[54] | 1.15 ± 0.04[71] | 1.21 ± 0.12[71] | 4.22[163] | 4.40[69] | ||
Zeta Herculis A | 35±0.2[11] | F9IV[128] | 2.56 – 2.61[164] | 1.45 ± 0.1[164] | 2.81[108] | 2.65[165] | ||
Beta Virginis (Zavijava) | 35.65±0.09[11] | F9V[166] | 1.681 ± 0.008[75] | 1.413 ± 0.061[167] | 3.604[168] | 3.41[69] | ||
Theta Persei A | 36.29±0.09 | F8V[169] | 1.319 ± 0.011[75] | 1.138 ± 0.01[75] | 4.11[89] | 3.88[69] | ||
Gamma Serpentis | 36.7±0.07[11] | F6V[170] | 1.55 ± 0.05[71] | 1.3 ± 0.15[71] | 3.85[170] | 3.60[69] | ||
Zeta Doradus A | 37.91±0.07 | F7V | 1.07+0.02 −0.07[171] |
1.07[172] | 4.8191[11] | 4.38[173] | ||
Gamma Virginis (Porrima) | A | 38.1±0.3 | F0V[174] | 1.56[175] | 3.4[175] | 3[175] | ||
B | 1.5[175] | 3.5[175] | 3.1[175] | |||||
Iota Pegasi A | 38.5±0.2 | F5V | 1.526 ± 0.068 | 1.33 | 3.84 | 3.49 | ||
Zeta Trianguli Australis A | 39.5±0.2 | F9V[54] | 1.12[176] | 4.90[96] | 4.49[69] | Part of a binary star system | ||
Beta Trianguli Australis | 40.37±0.08 | F1V[54] | 1.976 ± 0.021[64] | 1.56[177] | 2.85[178] | 2.37[107] | ||
Theta Ursae Majoris | 43.96±0.08 | F6IV | 2.365 ± 0.008 | 1.41 | 3.166 | 2.43 | ||
Upsilon Andromedae A (Titawin) | 44±0.1 | F8V | 1.48 ± 0.087 | 1.27 ± 0.06 | 4.10 | 3.44 |
List of nearest A-type stars[edit]
This is a list of A-type stars within 60 light years.
Name | Distance (ly) | Spectral type | Stellar radius (R☉) | Stellar mass (M☉) | Apparent magnitude (V) | Absolute magnitude (V) | Notes | |
---|---|---|---|---|---|---|---|---|
Sirius A | 8.6±0.04 | A0mA1Va[105] | 1.711[179] | 2.063 ± 0.023[180] | -1.46 [181] | 1.43[182] | Also the sixth-nearest stellar system to the Solar System and the brightest star in the night sky. | |
Altair | 16.7[183] | A7Vn[105] | 2.01 – 1.57[184] | 1.86 ± 0.03[184] | 0.76[52] | 2.22[185] | 12th brightest star in the night sky. | |
Vega | 25.04±0.07 | A0Va[105] | 2.818 – 2.362[186] | 2.135 ± 0.074[186] | 0.026[187] | 0.582[188] | Fifth-brightest star in the night sky. | |
Fomalhaut A | 25.13±0.09[189] | A3V[23] | 1.842 ± 0.019[190] | 1.92 ± 0.02[190] | 1.16[52] | 1.72[190] | 18th brightest star in the night sky. Part of a triple star system. | |
Denebola | 35.9±0.2[11] | A3Va[105] | 1.728[191] | 1.78[191] | 2.14[192] | 1.93[107] | ||
Delta Capricorni (Deneb Algedi) | 38.7±0.09 | A7m III[193] | 1.91[194] | 2[194] | 2.81[193] | 2.48[107] | Part of a binary star system | |
Iota Ursae Majoris A (Talitha) | 47.3±0.1 | A7V(n)[195] | 1.7 ± 0.1 | 3.14[108] | 2.31[107] | Part of a quadruple star system | ||
Alpha Ophiuchi A (Rasalhague) | 48.6±0.8 | A5IVnn[196] | 2.6[170] | 2.4+0.23 −0.37[197] |
2.07[108] | 1.248[198] | Part of a binary star system. | |
Alderamin | 49.05±0.08 | A8Vn[105] or A7IV-V[199] | 2.823 × 2.175[199] | 2 ± 0.15[199] | 2.5141[11] | 1.57[200] | ||
Castor | Aa | 51±3 | A1V[201] | 2.089[202] | 2.37[202] | 1.93[73] | 0.986[203] | Part of a sextuple star system. |
Ba | Am[201] | 1.648[202] | 1.79[202] | 2.97[73] | 1.886[203] | |||
Delta Leonis (Zosma) | 58.4±0.3[11] | A4V[204] | 2.14 ± 0.04[205] | 2.2[206] | 2.56[207] | 1.29[107] | ||
Iota Centauri | 58.6[11] | A2V[54] | 2.5[208] | 2.73[108] | 1.47[107] | |||
Beta Arietis A (Sheratan) | 59.6±0.8 | A5V[209] | 2.34 ± 0.1[210] | 2.655[162] | 1.59[182] | Part of a binary star system |
List of nearest B-type stars[edit]
This is a list of B-type stars within 200 light years.
Name | Distance (ly) | Spectral type | Stellar radius (R☉) | Stellar mass (M☉) | Apparent magnitude (V) | Absolute magnitude (V) | Notes | |
---|---|---|---|---|---|---|---|---|
Regulus A | 79.3±0.7 | B8IVn[89] | 4.35 ± 0.1[211] | 3.8[170] | 1.40[89] | -0.57[107] | Part of a binary star system. Also the 20th brightest star in the night sky. | |
Algol Aa1 | 90±3[11] | B8V[212] | 2.73 ± 0.2[213] | 3.17 ± 0.21[213] | 2.12 (combined)[52] | -0.07[214] | ||
Alpheratz A | 97±1 | B8IV-VHgMn[215] | 2.7 ± 0.4[216] | 3.8 ± 0.2[216] | 2.22 | -0.19[217] | Part of a binary star system | |
Alnair | 101±0.7 | B6V[54] or B7IV[151] | 3.4[218] | 4[170] | 1.74[219] | -0.72[107] | 31st brightest star in the night sky. | |
Alkaid | 103.9±0.8[11] | B3V[166] | 3.4[220] | 6.1 ± 0.1[221] | 1.86[52] | -0.67[107] | 40th brightest star in the night sky. | |
Alpha Pegasi (Markab) | 133±1 | B9V[222], B9.5III[223] or A0IV[224] | 4.62 ± 0.29[225] | 3.5[226] | 2.48[108] | -0.718[227] | ||
Beta Tauri (Elnath) | 134±2 | B7III[228] | 4.2[220] | 5 ± 0.1[229] | 1.65[52] | -1.42[107] | 27th brightest star in the night sky. | |
Achernar | 139±3[11] | B3Vpe[230] | 9.16 – 6.78[231] | 6[232] | 0.40 – 0.46[233] | -2.7[234] | 9th brightest star in the night sky. | |
Epsilon Sagittarii A (Kaus Australis) | 143±2[11] | B9.5III[235] | 6.8[236] | 3.515 ± 0.038[237] | 1.85[108] | -1.41[237] | 38th brightest star in the night sky. | |
Gamma Corvi A (Gienah) | 154±1[11] | B8III[238] | 4.2+0.4 −0.3[229] |
2.585[57] | -0.79[107] | |||
Beta Canis Minoris (Gomeisa) | 160±10 | B8Ve[239] | 3.5[240] | 3.5[239] | 2.84 – 2.92[233] | -0.59[107] | ||
Kappa Andromedae | 168±2 | B9IVn[204] | 2.29 ± 0.06[241] | 2.768+1 −1.09[242] |
4.139[243] | 0.59[107] | Has one confirmed exoplanet or brown dwarf | |
Alpha Pavonis A (Peacock) | 179±5[11] | B3V[244] | 4.83[245] | 5.91[177] | 1.94[178] | -1.762[246] | 44th brightest star in the night sky. | |
Kappa1 Lupi | 180±5[11] | B9.5Vne[247] | 2.3[91] | 2.89 ± 0.03[248] | 3.86 | |||
Alpha Sagittarii (Rukbat) | 182±2 | B8V[249] | 2.35[c] | 2.95[177] | 3.97[108] | 0.23[107] | ||
Beta Librae (Zubeneschamali) | 185±2 | B8V[229] | 4.9 ± 0.3[d] | 3.5+0.3 −0.2[229] |
2.61[207] | -1.16 |
List of nearest O-type stars[edit]
This is a list of O-type stars within 1,500 light years.
Name | Distance (ly) | Spectral type | Stellar radius (R☉) | Stellar mass (M☉) | Apparent magnitude (V) | Absolute magnitude (V) | Notes | |
---|---|---|---|---|---|---|---|---|
Zeta Ophiuchi | 366±8[11] | O9.5V[251] | 8.5[252] | 20.2[253] | 2.56 – 2.58[3] | -4.2[254] | ||
Zeta Puppis (Naos) | 1080±40 | O4If(n)p[255] | 14 – 26[256] | 56.1[257] | 2.24 – 2.26[258] | -6.23[257] | One of the most massive stars visible to the naked eye. | |
Mintaka | 1200[259] | O9.5II[259] | 16.5[259] | 24[259] | 2.5[260] | -5.8[261] | Part of a multiple star system | |
Gamma Velorum A | 1236±13[262] | O7.5III[263] | 17 ± 2[264] | 28.5 ± 1.1[264] | 1.83 (combined)[52] | -5.63[264] | 30th brightest star in the night sky. | |
Alnitak | 1260±180[265] | O9.5lab[265] | 20 ± 3.2[265] | 33 ± 10[265] | 2.08[265] | -6[265] | Part of a triple star system | |
Sigma Orionis Aa | 1263±4.3[266] | O9.5V[267] | 5.6[266] | 16[266] | 4.07 (combined)[268] | -3.49[269] | Part of a quintuple star system | |
Meissa A | ~1300[270] | O8III((f))[255] | 13.4[271] | 27.9 ± 3.3[221] | 3.7[272] | -4.25 | Part of a multiple star system | |
Mu Columbae | ~1300 | O9.5V[273] | 6.58[274] | 16[274] | 5.18[52] | -3.64[274] | ||
AE Aurigae | 1320±40 | O9.5V[255] | 7.47[275] | 23[275] | 5.96[52] (5.78 – 6.08)[233] | |||
Theta1 Orionis C1 | 1340±65[276] | O7Vp[277] | 10.6 ± 1.5[278] | 33 ± 5[279] | 5.13[52] | -4.9[278] | Part of a binary star system | |
Iota Orionis Aa1 (Haytsa) | 1343+45.6 −42.3[280] |
O9III[281] | 8.3[282] | 23.1[282] | 2.77 (combined)[178] | Part of a multiple star system |
Notes[edit]
- ^ Calculated from the bolometric magnitude 4.54 ± 0.06 and the bolometric correction −0.12 ± 0.05 using the formula: BC = Mbol − MV
- ^ Calculated from the bolometric magnitude 4.54 ± 0.06 and the bolometric correction −0.12 ± 0.05 using the formula: BC = Mbol − MV
- ^ Radius calculated using a effective temperature of 12 387 K and a luminosity of 117 L☉.[177]
- ^ Calculated using an angular diameter of 0.801 Milliarcseconds.[250]
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{{cite book}}
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: CS1 maint: multiple names: authors list (link) - ^ a b Marchenko, Sergey V.; Rauw, Gregor; Antokhina, Eleonora A.; Antokhin, Igor I.; Ballereau, Dominique; Chauville, Jacques; Corcoran, Michael F.; Costero, Rafael; Echevarria, Juan; Eversberg, Thomas; Gayley, Ken G.; Koenigsberger, Gloria; Miroshnichenko, Anatoly S.; Moffat, Anthony F. J.; Morrell, Nidia I. (September 2000). "Coordinated monitoring of the eccentric O-star binary Iota Orionis: optical spectroscopy and photometry". Monthly Notices of the Royal Astronomical Society. 317 (2): 333–342. Bibcode:2000MNRAS.317..333M. doi:10.1046/j.1365-8711.2000.03542.x. ISSN 0035-8711.