Talaan ng malalapit na bituin
(Idinirekta mula sa Talaan ng mga malalapit na bituin)
Naglalaman ang talaang ito ng lahat ng natuklasang mga bituin at tsokolateng duwende na may layong hanggang 5 parsec (16.3 sinag-taon), mula sa Sistemang Solar. Karagdagan sa Sistemang Solar, mayroon pang karagdagang 54 sistemang bituin na kasalukuyang natuklasang makikita sa parehong layo. These systems contain a total of Naglalaman ang mga sistemang ito ng may kabuuang 56 hydrogen-fusing na bituin (46 doon ay pulang duwende), 14 tsokolateng duwende, at 4 na puting duwende. Kahit na may relatibong kalapitan ang mga bagay na ito sa Mundo, siyam lamang dito ang may maliwanag na kalakhan na hindi bababa sa 6.5. Ibig sabihin nito, 12% lamang sa mga bagay ang maaaring makita ng mga mata.[1] Bukod sa Araw, tatlo lamang ang first-magnitude stars: Alpha Centauri, Sirius, at Procyon. Makikita lahat ng mga bagay na ito sa Local Bubble, isang rehiyong makikita sa Orion–Cygnus Arm ng Daang Magatas.
Talaan
baguhinMay magaang na asul sa ibaba ang mga bituin makikita ng mata na walang instrumentong ginagamit. Ilan sa parallax at layo ay nasa panimulang pagsusukat.[2]
| # | Layo[3] Sinag-taon (±err) |
Designasyon | Uri | Maliwanag na kalakhan (mV o mJ) | Lubusang kalakhan (MV o MJ) | Epoch J2000.0 | Parallax[2][4] mas(±err) |
Petsa ng pagkatuklas[5] | Karagdagang talababa | |||
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Sistema | Bituin | # ng bituin | Kanang asensiyon[2] | Deklinasyon[2] | ||||||||
| 0 | Sistemang Solar | Sun | G2V[2] | −26.74[2] | 4.85[2] | — | — | — | — | mayroong walong planeta | ||
| 1 | 4.2421(16) | Alpha Centauri (Rigil Kentaurus) |
Proxima Centauri (V645 Centauri) | 1 | M5.5Ve | 11.09[2] | 15.53[2] | 14h 29m 43.0s | −62° 40′ 46″ | 768.87(029)[6][7] | 1915 | [8] |
| 4.3650(68) | α Centauri A (HD 128620) | 2 | G2V[2] | 0.01[2] | 4.38[2] | 14h 39m 36.5s | −60° 50′ 02″ | 747.23(117)[6][9] | ||||
| α Centauri B (HD 128621) | 2 | K1V[2] | 1.34[2] | 5.71[2] | 14h 39m 35.1s | −60° 50′ 14″ | 1689 | mayroong isang suspetsang planeta[10] | ||||
| 2 | 5.9630(109) | Barnard's Star (BD+04°3561a) | 4 | M4.0Ve | 9.53[2] | 13.22[2] | 17h 57m 48.5s | +04° 41′ 36″ | 546.98(1 00)[6][7] | 1916 | pinakamalaking proper motion[11] | |
| 3 | 6.59(7) | Luhman 16 (WISE 1049−5319) |
Luhman 16A | 5 | L8±1[12] | 10.7 J | 14.2 J | 10h 49m 15.57s | −53° 19′ 06″ | 495 (5)[12] | 2013 | mayroong isang suspetsang planeta[13] |
| Luhman 16B | 5 | T1±2[12] | ||||||||||
| 4 | 7.2(6)[14] | WISE 0855−0714 | 7 | Y | 08h 55m 10.83s | -07° 14′ 42.5″ | 2014 | posibleng isang planeta | ||||
| 5 | 7.7825(390) | Wolf 359 (CN Leonis) | 8 | M6.0V[2] | 13.44[2] | 16.55[2] | 10h 56m 29.2s | +07° 00′ 53″ | 419.10(210)[6] | 1919 | ||
| 6 | 8.2905(148) | Lalande 21185 (BD+36°2147) | 9 | M2.0V[2] | 7.47[2] | 10.44[2] | 11h 03m 20.2s | +35° 58′ 12″ | 393.42(070)[6][7] | 1801 | ||
| 7 | 8.5828(289) | Sirius (α Canis Majoris) |
Sirius A | 10 | A1V[2] | −1.46[2] | 1.42[2] | 06h 45m 08.9s | −16° 42′ 58″ | 380.02(128)[6][7] | pinakamaliwanag na bituin sa himpapawid | |
| Sirius B | 10 | DA2[2] | 8.44[2] | 11.34[2] | 1844 | |||||||
| 8 | 8.7280(631) | Luyten 726-8 | Luyten 726-8 A (BL Ceti) | 12 | M5.5Ve | 12.54[2] | 15.40[2] | 01h 39m 01.3s | −17° 57′ 01″ | 373.70(270)[6] | 1949 | |
| Luyten 726-8 B (UV Ceti) | 12 | M6.0Ve | 12.99[2] | 15.85[2] | ||||||||
| 9 | 9.6813(512) | Ross 154 (V1216 Sagittarii) | 14 | M3.5Ve | 10.43[2] | 13.07[2] | 18h 49m 49.4s | −23° 50′ 10″ | 336.90(178)[6][7] | 1925 | ||
| 10 | 10.322(36) | Ross 248 (HH Andromedae) | 15 | M5.5Ve | 12.29[2] | 14.79[2] | 23h 41m 54.7s | +44° 10′ 30″ | 316.00(110)[6] | 1925 | ||
| 11 | 10.522(27) | Epsilon Eridani (BD−09°697) | 16 | K2V[2] | 3.73[2] | 6.19[2] | 03h 32m 55.8s | −09° 27′ 30″ | 309.99(079)[6][7] | 150 | mayroong isang planeta[15] | |
| 12 | 10.742(31) | Lacaille 9352 (CD−36°15693) | 17 | M1.5Ve | 7.34[2] | 9.75[2] | 23h 05m 52.0s | −35° 51′ 11″ | 303.64(087)[6][7] | 1753 | ||
| 13 | 10.919(49) | Ross 128 (FI Virginis) | 18 | M4.0Vn | 11.13[2] | 13.51[2] | 11h 47m 44.4s | +00° 48′ 16″ | 298.72(135)[6][7] | 1925 | ||
| 14 | 11.089[16] | WISE 1506+7027 | 19 | T6 | 14.3 J | 16.6 J | 15h 06m 49.9s | +70° 27′ 36″ | 310(042)[16] | 2011 | ||
| 15 | 11.266(171) | EZ Aquarii (Gliese 866, Luyten 789-6) |
EZ Aquarii A | 20 | M5.0Ve | 13.33[2] | 15.64[2] | 22h 38m 33.4s | −15° 17′ 57″ | 289.50(440)[6] | 1937 | |
| EZ Aquarii B | 20 | M? | 13.27[2] | 15.58[2] | - | |||||||
| EZ Aquarii C | 20 | M? | 14.03[2] | 16.34[2] | 1995 | |||||||
| 16 | 11.402(32) | Procyon (α Canis Minoris) |
Procyon A | 23 | F5V–IV[2] | 0.38[2] | 2.66[2] | 07h 39m 18.1s | +05° 13′ 30″ | 286.05(081)[6][7] | ||
| Procyon B | 23 | DQZ[2] | 10.70[2] | 12.98[2] | 1844 | |||||||
| 17 | 11.403(22) | 61 Cygni | 61 Cygni A (BD+38°4343) | 25 | K5.0V[2] | 5.21[2] | 7.49[2] | 21h 06m 53.9s | +38° 44′ 58″ | 286.04(056)[6][7] | 1725 | unang bituin (bukod sa Araw) na nasukat ang layo[17] |
| 61 Cygni B (BD+38°4344) | 25 | K7.0V[2] | 6.03[2] | 8.31[2] | 21h 06m 55.3s | +38° 44′ 31″ | - | |||||
| 18 | 11.525(69) | Struve 2398 (Gliese 725, BD+59°1915) |
Struve 2398 A (HD 173739) | 27 | M3.0V[2] | 8.90[2] | 11.16[2] | 18h 42m 46.7s | +59° 37′ 49″ | 283.00(169)[6][7] | 1835 | |
| Struve 2398 B (HD 173740) | 27 | M3.5V[2] | 9.69[2] | 11.95[2] | 18h 42m 46.9s | +59° 37′ 37″ | 1835 | |||||
| 19 | 11.624(39) | Groombridge 34 (Gliese 15) |
Groombridge 34 A (GX Andromedae) | 29 | M1.5V[2] | 8.08[2] | 10.32[2] | 0h 18m 22.9s | +44° 01′ 23″ | 280.59(095)[6][7] | 1813 | mayroong isang planeta[18] |
| Groombridge 34 B (GQ Andromedae) | 29 | M3.5V[2] | 11.06[2] | 13.30[2] | - | |||||||
| 20 | 11.824(30) | Epsilon Indi (CPD−57°10015) |
Epsilon Indi A | 31 | K5Ve[2] | 4.69[2] | 6.89[2] | 22h 03m 21.7s | −56° 47′ 10″ | 275.84(069)[6][7] | 1597 | mayroong isang suspetsang planeta[19] |
| Epsilon Indi Ba | 31 | T1.0V | 12.3 J[20] | 22h 04m 10.5s | −56° 46′ 58″ | Jan 2003 | ||||||
| Epsilon Indi Bb | 31 | T6.0V | 13.2 J[20] | Aug 2003 | ||||||||
| 21 | 11.826(129) | DX Cancri (G 51-15) | 34 | M6.5Ve | 14.78[2] | 16.98[2] | 08h 29m 49.5s | +26° 46′ 37″ | 275.80(300)[6] | 1972 | ||
| 22 | 11.887(33) | Tau Ceti (BD−16°295) | 35 | G8Vp[2] | 3.49[2] | 5.68[2] | 01h 44m 04.1s | −15° 56′ 15″ | 274.39(076)[6][7] | 150 | mayroong limang posibleng planeta | |
| 23 | 11.991(57) | GJ 1061 (LHS 1565) | 36 | M5.5V[2] | 13.09[2] | 15.26[2] | 03h 35m 59.7s | −44° 30′ 45″ | 272.01(130)[21] | 1995 | [22][23] | |
| 24 | 12.068[16] | WISE 0350−5658 | 37 | Y1 | 22.8 J[24] | 03h 50m 00.32s | −56° 58′ 30.2″ | 291(050)[16] | 2011 | |||
| 25 | 12.132(133) | YZ Ceti (LHS 138) | 38 | M4.5V[2] | 12.02[2] | 14.17[2] | 01h 12m 30.6s | −16° 59′ 56″ | 268.84(295)[6][7] | 1961 | ||
| 26 | 12.366(59) | Luyten's Star (BD+05°1668) | 39 | M3.5Vn | 9.86[2] | 11.97[2] | 07h 27m 24.5s | +05° 13′ 33″ | 263.76(125)[6][7] | 1935 | ||
| 27 | 12.514(129) | Teegarden's star (SO025300.5+165258) | 40 | M6.5V | 15.14[2] | 17.22[2] | 02h 53m 00.9s | +16° 52′ 53″ | 260.63(269)[21] | 2003 | posibleng isang sistemang planetaryo[23][25] | |
| 28 | 12.571(54) | SCR 1845-6357 | SCR 1845-6357 A | 41 | M8.5V[2] | 17.39 | 19.41 | 18h 45m 05.3s | −63° 57′ 48″ | 259.45(111)[21] | 2004 | [23] |
| SCR 1845-6357 B | 41 | T6[26] | 13.3 J[20] | 18h 45m 02.6s | −63° 57′ 52″ | 2006 | ||||||
| 29 | 12.777(43) | Kapteyn's Star (CD−45°1841) | 43 | M1.5V[2] | 8.84[2] | 10.87[2] | 05h 11m 40.6s | −45° 01′ 06″ | 255.27(086)[6][7] | 1898 | may dalawang natuklasang planeta[27] | |
| 30 | 12.870(57) | Lacaille 8760 (AX Microscopii) | 44 | M0.0V[2] | 6.67[2] | 8.69[2] | 21h 17m 15.3s | −38° 52′ 03″ | 253.43(112)[6][7] | 1753 | ||
| 31 | 13.149(74) | Kruger 60 (BD+56°2783) |
Kruger 60 A | 45 | M3.0V[2] | 9.79[2] | 11.76[2] | 22h 27m 59.5s | +57° 41′ 45″ | 248.06(139)[6][9] | 1880 | |
| Kruger 60 B (DO Cephei) | 45 | M4.0V[2] | 11.41[2] | 13.38[2] | 1890? | |||||||
| 32 | 13.167(82) | DEN 1048-3956 | 47 | M8.5V[2] | 17.39[2] | 19.37[2] | 10h 48m 14.7s | −39° 56′ 06″ | 247.71(155)[21] | 2001 | [28][29] | |
| 33 | 13.259 | UGPS 0722-05 | 48 | T9[2] | 16.52 J[30] | 07h 22m 27.3s | –05° 40′ 30″ | 246 | 2010 | [31] | ||
| 34 | 13.349(110) | Ross 614 (V577 Monocerotis, Gliese 234) |
Ross 614A (LHS 1849) | 49 | M4.5V[2] | 11.15[2] | 13.09[2] | 06h 29m 23.4s | −02° 48′ 50″ | 244.34(201)[6][9] | 1927 | |
| Ross 614B (LHS 1850) | 49 | M5.5V | 14.23[2] | 16.17[2] | 1936 | |||||||
| 35 | 13.820(98) | Wolf 1061 (Gliese 628, BD−12°4523) | 51 | M3.0V[2] | 10.07[2] | 11.93[2] | 16h 30m 18.1s | −12° 39′ 45″ | 236.01(167)[6][7] | 1919 | ||
| 36 | 14.066(109) | Van Maanen's star (Gliese 35, LHS 7) | 52 | DZ7[2] | 12.38[2] | 14.21[2] | 00h 49m 09.9s | +05° 23′ 19″ | 231.88(179)[6][7] | 1896 | ||
| 37 | 14.231(66) | Gliese 1 (CD−37°15492) | 53 | M1.5 V [2] | 8.55[2] | 10.35[2] | 00h 05m 24.4s | −37° 21′ 27″ | 229.20(107)[6][7] | 1884 | ||
| 38 | 14.312(289) | Wolf 424 (FL Virginis, LHS 333, Gliese 473) |
Wolf 424 A | 54 | M5.5Ve | 13.18[2] | 14.97[2] | 12h 33m 17.2s | +09° 01′ 15″ | 227.90(460)[6] | ||
| Wolf 424 B | 54 | M7Ve | 13.17[2] | 14.96[2] | ||||||||
| 39 | 14.4 | 2MASS J154043.42-510135.7 | 56 | M7V | 15.26 | 17.04 | 15h 40m 43.42s | -51° 01′ 35.7″ | 224.80(290) | 2014 | [32] | |
| 40 | 14.509(187) | L 1159-16 (TZ Arietis, Gliese 83.1) | 57 | M4.5V[2] | 12.27[2] | 14.03[2] | 02h 00m 13.2s | +13° 03′ 08″ | 224.80(290)[6] | |||
| 41 | 14.793(55) | Gliese 687 (LHS 450, BD+68°946) | 58 | M3.0V[2] | 9.17[2] | 10.89[2] | 17h 36m 25.9s | +68° 20′ 21″ | 220.49(082)[6][7] | mayroong isang planeta[33] | ||
| 42 | 14.805(242) | LHS 292 (LP 731-58) | 59 | M6.5V[2] | 15.60[2] | 17.32[2] | 10h 48m 12.6s | −11° 20′ 14″ | 220.30(360)[6] | |||
| 43 | 14.809(107) | Gliese 674 (LHS 449) | 60 | M3.0V[2] | 9.38[2] | 11.09[2] | 17h 28m 39.9s | −46° 53′ 43″ | 220.25(159)[6][7] | mayroong isang planeta[34] | ||
| 44 | 14.812(67) | G 208-44 G 208-45 (GJ 1245) |
G 208-44 A (V1581 Cyg) | 61 | M5.5V[2] | 13.46[2] | 15.17[2] | 19h 53m 54.2s | +44° 24′ 55″ | 220.20(100)[6] | ||
| G 208-45 | 61 | M6.0V[2] | 14.01[2] | 15.72[2] | 19h 53m 55.2s | +44° 24′ 56″ | ||||||
| G 208-44 B | 61 | M5.5 | 16.75[2] | 18.46[2] | 19h 53m 54.2s | +44° 24′ 55″ | ||||||
| 45 | 15.060(140) | LP 145-141 (WD 1142-645, Gliese 440) | 64 | DQ6[2] | 11.50[2] | 13.18[2] | 11h 45m 42.9s | −64° 50′ 29″ | 216.57(201)[6][7] | |||
| 46 | 15.313(259) | GJ 1002 | 65 | M5.5V[2] | 13.76[2] | 15.40[2] | 00h 06m 43.8s | −07° 32′ 22″ | 213.00(360)[6] | |||
| 47 | 15.342(141) | Gliese 876 (Ross 780) | 66 | M3.5V[2] | 10.17[2] | 11.81[2] | 22h 53m 16.7s | −14° 15′ 49″ | 212.59(196)[6][7] | mayroong apat na planeta[35] | ||
| 48 | 15.610(204) | LHS 288 (Luyten 143-23) | 67 | M5.5V[2] | 13.90[2] | 15.51[2] | 10h 44m 21.2s | −61° 12′ 36″ | 208.95(273)[21] | [23] | ||
| 49 | 15.832(83) | Gliese 412 | Gliese 412 A | 68 | M1.0V[2] | 8.77[2] | 10.34[2] | 11h 05m 28.6s | +43° 31′ 36″ | 206.02(108)[6][7] | ||
| Gliese 412 B (WX Ursae Majoris) | 68 | M5.5V[2] | 14.48[2] | 16.05[2] | 11h 05m 30.4s | +43° 31′ 18″ | ||||||
| 50 | 15.848(52) | Groombridge 1618 (Gliese 380) | 70 | K7.0V[2] | 6.59[2] | 8.16[2] | 10h 11m 22.1s | +49° 27′ 15″ | 205.81(067)[6][7] | |||
| 51 | 15.942(218) | AD Leonis | 71 | M3.0V[2] | 9.32[2] | 10.87[2] | 10h 19m 36.4s | +19° 52′ 10″ | 204.60(280)[6] | |||
| 52 | 16.067[24] | DENIS J081730.0-615520 | 72 | T6 | 08h 17m 30.096s | -61° 55′ 15.802″ | 203 [24] | 2010 | ||||
| 53 | 16.085(105) | Gliese 832 | 73 | M1.5 V[2] | 8.66[2] | 10.20[2] | 21h 33m 34.0s | −49° 00′ 32″ | 202.78(132)[6][7] | mayroong dalawang planeta[36][37] | ||
| 54 | 16.197(313) | DEN 0255-4700 | 74 | L7.5V[2] | 22.92[2] | 24.44[2] | 02h 55m 03.7s | −47° 00′ 52″ | 201.37(389)[21] | [29] | ||
| # | Layo[3] Sinag-taon (±err) |
Uri | Bituin | Star # | Stellar class | Apparent magnitude (mV or mJ) | Absolute magnitude (MV or MJ) | Right ascension[2] | Declination[2] | Parallax[2][4] mas(±err) |
Discovery date | Additional references |
| Designation | Epoch J2000.0 | |||||||||||
Talababa
baguhin- ↑ Weaver, Harold F. (1947). "The Visibility of Stars Without Optical Aid". Publications of the Astronomical Society of the Pacific. 59 (350): 232–243. Bibcode:1947PASP...59..232W. doi:10.1086/125956.
{{cite journal}}: CS1 maint: date auto-translated (link) - ↑ 2.000 2.001 2.002 2.003 2.004 2.005 2.006 2.007 2.008 2.009 2.010 2.011 2.012 2.013 2.014 2.015 2.016 2.017 2.018 2.019 2.020 2.021 2.022 2.023 2.024 2.025 2.026 2.027 2.028 2.029 2.030 2.031 2.032 2.033 2.034 2.035 2.036 2.037 2.038 2.039 2.040 2.041 2.042 2.043 2.044 2.045 2.046 2.047 2.048 2.049 2.050 2.051 2.052 2.053 2.054 2.055 2.056 2.057 2.058 2.059 2.060 2.061 2.062 2.063 2.064 2.065 2.066 2.067 2.068 2.069 2.070 2.071 2.072 2.073 2.074 2.075 2.076 2.077 2.078 2.079 2.080 2.081 2.082 2.083 2.084 2.085 2.086 2.087 2.088 2.089 2.090 2.091 2.092 2.093 2.094 2.095 2.096 2.097 2.098 2.099 2.100 2.101 2.102 2.103 2.104 2.105 2.106 2.107 2.108 2.109 2.110 2.111 2.112 2.113 2.114 2.115 2.116 2.117 2.118 2.119 2.120 2.121 2.122 2.123 2.124 2.125 2.126 2.127 2.128 2.129 2.130 2.131 2.132 2.133 2.134 2.135 2.136 2.137 2.138 2.139 2.140 2.141 2.142 2.143 2.144 2.145 2.146 2.147 2.148 2.149 2.150 2.151 2.152 2.153 2.154 2.155 2.156 2.157 2.158 2.159 2.160 2.161 2.162 2.163 2.164 2.165 2.166 2.167 2.168 2.169 2.170 2.171 2.172 2.173 2.174 2.175 2.176 2.177 2.178 2.179 Research Consortium on Nearby Stars, GSU (2007-09-17). "The One Hundred Nearest Star Systems". RECONS. Nakuha noong 2007-11-06.
{{cite journal}}: Check|first=value (tulong); External link in|journal= - ↑ 3.0 3.1 From parallax.
- ↑ 4.0 4.1 Parallaxes given by RECONS are a weighted mean of values in the sources given, as well as measurements by the RECONS program.
- ↑ Before 1900: earliest certain recorded observation. 1900–1930: first catalogued. After 1930: earliest trigonometric or spectroscopic parallax.
- ↑ 6.00 6.01 6.02 6.03 6.04 6.05 6.06 6.07 6.08 6.09 6.10 6.11 6.12 6.13 6.14 6.15 6.16 6.17 6.18 6.19 6.20 6.21 6.22 6.23 6.24 6.25 6.26 6.27 6.28 6.29 6.30 6.31 6.32 6.33 6.34 6.35 6.36 6.37 6.38 6.39 6.40 6.41 General Catalogue of Trigonometric Parallaxes.
- ↑ 7.00 7.01 7.02 7.03 7.04 7.05 7.06 7.07 7.08 7.09 7.10 7.11 7.12 7.13 7.14 7.15 7.16 7.17 7.18 7.19 7.20 7.21 7.22 7.23 7.24 7.25 7.26 7.27 Hipparcos Catalogue.
- ↑ Burgasser et al. 2000
- ↑ 9.0 9.1 9.2 Visual binary orbits and masses post Hipparcos, Staffan Söderhjelm, Astronomy and Astrophysics 341 (January 1999), pp. 121–140.
- ↑ "The exoplanet next door: Earth-sized world discovered in nearby α Centauri star system". Eric Hand, Nature, October 16, 2012. Accessed October 16, 2012.
- ↑ Barnard, E. E. (1916). "A small star with large proper motion". Astronomical Journal. 29 (695): 181. Bibcode:1916AJ.....29..181B. doi:10.1086/104156.
{{cite journal}}: CS1 maint: date auto-translated (link) - ↑ 12.0 12.1 12.2 Luhman, K. L. "Discovery of a Binary Brown Dwarf at 2 Parsecs from the Sun" (PDF). Astrophysical Journal Letters (to be published).[patay na link]
- ↑ http://arxiv.org/abs/1312.1303
- ↑ Luhman, K. L. (21 Abril 2014). "Discovery of a ~250 K Brown Dwarf at 2 pc from the Sun". The Astrophysical Journal Letters. 786 (2): L18. arXiv:1404.6501. Bibcode:2014ApJ...786L..18L. doi:10.1088/2041-8205/786/2/L18.
{{cite journal}}: CS1 maint: date auto-translated (link) - ↑ Janson, M.; atbp. (Setyembre 2008), "A comprehensive examination of the ε Eridani system. Verification of a 4 micron narrow-band high-contrast imaging approach for planet searches", Astronomy and Astrophysics, 488 (2): 771–780, arXiv:0807.0301, Bibcode:2008A&A...488..771J, doi:10.1051/0004-6361:200809984
{{citation}}: CS1 maint: date auto-translated (link) - ↑ 16.0 16.1 16.2 16.3 Padron:Rr/2012arXiv1211.6977M
- ↑ Bessel, F. W. (1839). "Bestimmung der Entfernung des 61sten Sterns des Schwans. Von Herrn Geheimen - Rath und Ritter Bessel". Astronomische Nachrichten (sa wikang Aleman). 16 (5–6): 65. Bibcode:1839AN.....16...65B. doi:10.1002/asna.18390160502.
(page 92) Ich bin daher der Meinung, daß nur die jährliche Parallaxe = 0"3136 als das Resultat der bisherigen Beobachtungen zu betrachten ist
{{cite journal}}: CS1 maint: date auto-translated (link) A parallax of 313.6 mas yields a distance of 10.4 light years - ↑ "The NASA-UC-UH Eta-Earth Program: IV. A Low-mass Planet Orbiting an M Dwarf 3.6 PC from Earth". Andrew W. Howard, Geoffrey W. Marcy, Debra A. Fischer, Howard Isaacson, Philip S. Muirhead, Gregory W. Henry, Tabetha S. Boyajian, Kaspar von Braun, Juliette C. Becker, Jason T. Wright, John Asher Johnson. Accessed August 26, 2014.
- ↑ Zechmeister, M.; Kürster, M; Endl, M.; Lo Curto, G.; Hartman, H.; Nilsson, H.; Henning, T.; Hatzes, A.; Cochran, W. D. (Abril 2013). "The planet search programme at the ESO CES and HARPS. IV. The search for Jupiter analogues around solar-like stars". Astronomy and Astrophysics. 552: pp62. arXiv:1211.7263. Bibcode:2013A&A...552A..78Z. doi:10.1051/0004-6361/201116551.
{{cite journal}}:|pages=has extra text (tulong); Invalid|display-authors=9(tulong)CS1 maint: date auto-translated (link) - ↑ 20.0 20.1 20.2 Chris Gelino, Davy Kirkpatrick, Adam Burgasser. "DwarfArchives.org: Photometry, spectroscopy, and astrometry of M, L, and T dwarfs". caltech.edu. Inarkibo mula sa orihinal noong 2013-11-13. Nakuha noong 2012-06-10.
{{cite web}}: CS1 maint: date auto-translated (link) CS1 maint: multiple names: mga may-akda (link) (main page) Naka-arkibo 2019-05-11 sa Wayback Machine. - ↑ 21.0 21.1 21.2 21.3 21.4 21.5 Systems with their first accurate trigonometric parallaxes measured by RECONS
- ↑ The solar neighborhood IV: discovery of the twentieth nearest star, Todd J. Henry, Philip A. Ianna, J. Davy Kirkpatrick, Hartmut Jahreiss, The Astronomical Journal 114, #1 (July 1997), pp. 388–395. doi:10.1086/118482
- ↑ 23.0 23.1 23.2 23.3 The Solar Neighborhood. XVII. Parallax Results from the CTIOPI 0.9 m Program: 20 New Members of the RECONS 10 Parsec Sample, Todd J. Henry, Wei-Chun Jao, John P. Subasavage, Thomas D. Beaulieu, Philip A. Ianna, Edgardo Costa, René A. Méndez, The Astronomical Journal 132, #6 (December 2006), pp. 2360–2371. doi:10.1086/508233
- ↑ 24.0 24.1 24.2 Kirkpatrick, J. Davy (2012). "Further Defining Spectral Type "Y" and Exploring the Low-mass End of the Field Brown Dwarf mass Function". arXiv:1205.2122 [astro-ph.SR].
{{cite arXiv}}: Unknown parameter|authors=ignored (tulong); Unknown parameter|version=ignored (tulong)CS1 maint: date auto-translated (link) - ↑ Barnes, J. R.; atbp. (2012). "ROPS: A New Search for Habitable Earths in the Southern Sky". Monthly Notices of the Royal Astronomical Society. 424 (1): 591–604. arXiv:1204.6283. Bibcode:2012MNRAS.424..591B. doi:10.1111/j.1365-2966.2012.21236.x.
{{cite journal}}: Explicit use of et al. in:|author=(tulong)CS1 maint: date auto-translated (link) - ↑ The very nearby M/T dwarf binary SCR 1845-6357, Markus Kasper, Beth A. Biller, Adam Burrows, Wolfgang Brandner, Jano Budaj, and Laird M. Close, Astronomy and Astrophysics 471, #2 (August 2007), pp. 655–659. doi:10.1051/0004-6361:20077881
- ↑ Guillem Anglada-Escudé, Pamela Arriagada, Mikko Tuomi, Mathias Zechmeister, James S. Jenkins, Aviv Ofir, Stefan Dreizler, Enrico Gerlach, Chris J. Marvin, Ansgar Reiners, Sandra V. Jeffers, R. Paul Butler, Steven S. Vogt, Pedro J. Amado, Cristina Rodríguez-López, Zaira M. Berdiñas, Julian Morin, Jeff D. Crane, Stephen A. Shectman, Ian B. Thompson, Matías Díaz, Eugenio Rivera, Luis F. Sarmiento, Hugh R.A. Jones (2014). "Two planets around Kapteyn's star : a cold and a temperate super-Earth orbiting the nearest halo red-dwarf". arXiv:1406.0818 [astro-ph.EP].
{{cite arXiv}}: Unknown parameter|accessdate=ignored (tulong)CS1 maint: date auto-translated (link) CS1 maint: multiple names: mga may-akda (link) - ↑ The Solar Neighborhood. XIII. Parallax Results from the CTIOPI 0.9 Meter Program: Stars with μ >= 1.0" yr-1 (Motion sample), Wei-Chun Jao, Todd J. Henry, John P. Subasavage, Misty A. Brown, Philip A. Ianna, Jennifer L. Bartlett, Edgardo Costa, René A. Méndez, The Astronomical Journal 129, #4 (April 2005), pp. 1954–1967. doi:10.1086/428489
- ↑ 29.0 29.1 The Solar Neighborhood. XIV. Parallaxes from the Cerro Tololo Inter-American Observatory Parallax Investigation—First Results from the 1.5 m Telescope Program, Edgardo Costa, René A. Méndez, W.-C. Jao, Todd J. Henry, John P. Subasavage, Misty A. Brown, Philip A. Ianna, and Jennifer Bartlett, The Astronomical Journal 130, #1 (July 2005), pp. 337–349. doi:10.1086/430473
- ↑ Lucas; Tinney; Ben Burningham; Leggett; Pinfield; Richard Smart; Jones; Federico Marocco; Barber (2010). "The discovery of a very cool, very nearby brown dwarf in the Galactic plane". arXiv:1004.0317v2 [astro-ph.SR].
{{cite arXiv}}: CS1 maint: date auto-translated (link) - ↑ Lucas, Philip W.; Tinney; Burningham; Leggett; Pinfield; Smart; atbp. (2010). "Discovery of a very cool brown dwarf amongst the ten nearest stars to the Solar System". arXiv:1004.0317 [astro-ph.SR].
{{cite arXiv}}: Explicit use of et al. in:|author2=(tulong); Unknown parameter|version=ignored (tulong)CS1 maint: date auto-translated (link) CS1 maint: multiple names: mga may-akda (link) - ↑ http://arxiv.org/abs/1405.5439
- ↑ "The Lick–Carnegie exoplanet survey: Gliese 687 b: A Neptune-mass planet orbiting a nearby red dwarf" (PDF). Inarkibo mula sa orihinal (PDF) noong 2014-03-27. Nakuha noong 2014-12-07.
{{cite web}}: CS1 maint: date auto-translated (link) - ↑ http://exoplanet.eu/star.php?st=GJ+674
- ↑ Rivera, Eugenio J.; atbp. (Hulyo 2010). "The Lick-Carnegie Exoplanet Survey: A Uranus-mass Fourth Planet for GJ 876 in an Extrasolar Laplace Configuration". The Astrophysical Journal. 719 (1): 890–899. arXiv:1006.4244. Bibcode:2010ApJ...719..890R. doi:10.1088/0004-637X/719/1/890.
{{cite journal}}: CS1 maint: date auto-translated (link) - ↑ Bailey, Jeremy; atbp. (2008). "A Jupiter-like Planet Orbiting the Nearby M Dwarf GJ832". The Astrophysical Journal. 690 (1): 743–747. arXiv:0809.0172. Bibcode:2009ApJ...690..743B. doi:10.1088/0004-637X/690/1/743.
{{cite journal}}:|access-date=requires|url=(tulong); Explicit use of et al. in:|author=(tulong)CS1 maint: date auto-translated (link) - ↑ http://arxiv.org/abs/1406.5587
Mga kawing panlabas
baguhin- "The 100 nearest star systems", Research Consortium on Nearby Stars
- "NStars database". Northern Arizona University. Inarkibo mula sa orihinal noong 2005-10-30. Nakuha noong 2005-10-24.
{{cite web}}: CS1 maint: date auto-translated (link) - "Map of the 25 nearest star systems". NASA. Nakuha noong 2005-10-24.
{{cite web}}: CS1 maint: date auto-translated (link) - "Notable Nearby Stars". SolStation. Nakuha noong 2005-10-24.
{{cite web}}: CS1 maint: date auto-translated (link) - "Cool stars in the solar Neighbourhood". D. Montes, UCM. Nakuha noong 2005-11-14.
{{cite web}}: CS1 maint: date auto-translated (link) - The dynamics of the closest stars
- Takeda, G.; E. B. Ford; A. Sills; F. A. Rasio; D. A. Fischer; J. A. Valenti (2006). "Structure and Evolution of Nearby Stars with Planets II. Physical Properties of ~ 1000 Cool Stars from the SPOCS Catalog". California & Carnegie Planet Search. Nakuha noong 2006-10-13.
{{cite web}}: CS1 maint: date auto-translated (link) - Nearest Stars 3D View
- Table 4 "The Census of Stars and Brown Dwarfs within 8 Parsecs of the Sun" in Kirkpatrick et al. (2012) Further Defining Spectral Type “Y” and Exploring the Low-mass End of the Field Brown Dwarf Mass Function, http://arxiv.org/pdf/1205.2122v1.pdf