Lis bintang pinih nampek

jmpl|Peta konformal jarak miwah sudut objek luar angkasa sané magenah ring jarak 12 taun cahaya saking Matahari.

Puniki suratan indik lis bintang sané pinih nampek ring jarak  saking Tata Surya. Jantos mangkin, 76 bintang sakadi punika sampun kapanggihin, miwah wantah sia sané cukup terang mangda prasida kacingakin antuk teleskop. Cahya sané kanten patut nyantos utawi langkungan ring tingkat kecerahan paling redup, inggih punika nilai magnitudo semu 6,5 mangda prasida kacingakin antuk mata telanjang saking Bumi.

 Lis 
#PenandaanSoroh bintangmVMVTeffK(±batas kesalahan)Epos J2000.0ParalaksParalaks yang diberikan RECONS adalah min nilai bagi sumber diberi, begitu juga pengukuran oleh program RECONS,mili detik busur(±batas kesalahan)JarakDari paralaks,Tahun cahaya(±batas kesalahan)ReferensitambahanSistemBintangPKPen Tata Surya Matahari (Sol) G2V −26,72 4,85  5,778Sun Fact Sheet, NASA,  Accessed on line November 8, 2007,  — — 180° 0,0000158(3)atau8 menit cahaya 1  Alpha Centauri(Rigil Kentaurus; Toliman) Proxima Centauri (V645 Centauri) M5,5Ve 11,09 15,53  3,040   0,768 87(0 29)″Katalog Am Paralaks Trigonometri,Katalog Hipparcos, 4,2421(16) Burgasser et al, 2000 α Centauri A (HD 128620) G2V 0,01 4,38  5,790   0,747 23(1 17)″Visual binary orbits and masses post Hipparcos, Staffan Söderhjelm, Astronomy and Astrophysics 341 (January 1999), pp, 121–140,  4,3650(68)  α Centauri B (HD 128621) K0V 1,34 5,71  5,260   2 Bintang Barnard (BD+04°3561a) M4,0Ve 9,53 13,22  3,134(102)Barnard's Star and the M Dwarf Temperature Scale, P, C, Dawson and M, M, de Robertis, The Astronomical Journal 127, #5 (May 2004), pp, 2909–2914,    0,546 98(1 00)″ 5,9630(109)  3 Wolf 359 (CN Leonis) M6,0V 13,44 16,55  2,800(100)    0,419 10(2 10)″ 7,7825(390)  4 Lalande 21185 (BD+36°2147) M2,0V 7,47 10,44  3,400Carbon monoxide bands in M dwarfs, Y, V, Pavlenko and H, R, A, Jones, Astronomy and Astrophysics 396 (December 2002), pp, 967–975,     0,393 42(0 70)″ 8,2905(148)  5 Sirius(α Canis Majoris) Sirius A  A1V −1,43 1,47  9,940(210)Table 2, The physical properties of normal A stars, Saul J, Adelman, pp, 1–11, The A-Star Puzzle, Proceedings of the International Astronomical Union, edited by J, Zverko, J, Ziznovsky, S, J, Adelman, and W, W, Weiss, Cambridge, UK: Cambridge University Press, 2004,    0,380 02(1 28)″ 8,5828(289)  Sirius B DA2 8,44 11,34 25,000(200)Adopted value, The Age and Progenitor Mass of Sirius B, James Liebert, Patrick A, Young, David Arnett, J,B, Holberg, and Kurtis A, Williams, The Astrophysical Journal 630, #1 (September 2005), pp, L69–L72, 6 Luyten 726-8 Luyten 726-8 A (BL Ceti) M5,5Ve 12,54 15,40  2,670   0,373 70(2 70)″ 8,7280(631)  Luyten 726-8 B (UV Ceti) M6,0Ve 12,99 15,85 ~2,600 7 Ross 154 (V1216 Sagittarii) M3,5Ve 10,43 13,07  2,700   0,336 90(1 78)″ 9,6813(512)  8 Ross 248 (HH Andromedae) M5,5Ve 12,29 14,79    0,316 00(1 10)″ 10,322(36)  9 Epsilon Eridani (BD−09°697) K2V 3,73 6,19  5,100    0,309 99(0 79)″ 10,522(27)  10 Lacaille 9352 (CD−36°15693) M1,5Ve 7,34 9,75  3,340   0,303 64(0 87)″ 10,742(31)  11 Ross 128 (FI Virginis) M4,0Vn 11,13 13,51  2,800   0,298 72(1 35)″ 10,919(49)  12 EZ Aquarii(GJ 866, Luyten 789-6) EZ Aquarii A M5,0Ve 13,33 15,64    0,289 50(4 40)″ 11,266(171)  EZ Aquarii B M? 13,27 15,58  EZ Aquarii C M? 14,03 16,34  13 Procyon(α Canis Minoris) Procyon A  F5V-IV 0,38 2,66  6,650   0,286 05(0 81)″ 11,402(32)  Procyon B DA 10,70 12,98  9,700 14 61 Cygni 61 Cygni A (BD+38°4343) K5,0V  5,21 7,49  4,640   0,286 04(0 56)″ 11,403(22)  61 Cygni B (BD+38°4344) K7,0V  6,03 8,31  4,440   15 Struve 2398(GJ 725, BD+59°1915) Struve 2398 A (HD 173739) M3,0V 8,90 11,16    0,283 00(1 69)″ 11,525(69)  Struve 2398 B (HD 173740) M3,5V 9,69 11,95    16 Groombridge 34(GJ 15) Groombridge 34 A (GX Andromedae) M1,5V  8,08 10,32    0,280 59(0 95)″ 11,624(39)  Groombridge 34 B (GQ Andromedae) M3,5V 11,06 13,30  17 Epsilon Indi(CPD−57°10015) Epsilon Indi A K5Ve 4,69 6,89  4,280   0,275 84(0 69)″ 11,824(30)  Epsilon Indi Ba T1,0V >23 >25  1,280   Epsilon Indi Bb T6,0V >23 >25    850 18 DX Cancri (G 51-15) M6,5Ve 14,78 16,98    0,275 80(3 00)″ 11,826(129)  19 Tau Ceti (BD−16°295) G8Vp 3,49 5,68  5,344    0,274 39(0 76)″ 11,887(33)  20 GJ 1061 (LHS 1565) M5,5V 13,09 15,26    0,272 01(1 30)″Systems with their first accurate trigonometric parallaxes measured by RECONS 11,991(57) 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,  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,   21 YZ Ceti (LHS 138) M4,5V 12,02 14,17    0,268 84(2 95)″ 12,132(133)  22 Bintang Luyten (BD+05°1668) M3,5Vn 9,86 11,97    0,263 76(1 25)″ 12,366(59)  23 Bintang Teegarden (SO025300,5+165258) M6,5V 15,14 17,22    0,260 63(2 69)″ 12,514(129)  24 SCR 1845-6357 SCR 1845-6357 A M8,5V 17,39 19,41      0,259 45(1 11)″ 12,571(54)  SCR 1845-6357 B T6The 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,       950     25 Bintang Kapteyn (CD−45°1841) M1,5V  8,84 10,87  3,800   0,255 27(0 86)″ 12,777(43)  26 Lacaille 8760 (AX Microscopii) M0,0V  6,67 8,69  3,340   0,253 43(1 12)″ 12,870(57)  27 Kruger 60(BD+56°2783) Kruger 60 A M3,0V 9,79 11,76  3,180   0,248 06(1 39)″ 13,149(74)  Kruger 60 B (DO Cephei) M4,0V 11,41 13,38  2,890 28 DEN 1048-3956 M8,5V 17,39 19,37    0,247 71(1 55)″ 13,167(82) 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,  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,  29 Ross 614(V577 Monocerotis, GJ 234) Ross 614A (LHS 1849) M4,5V 11,15 13,09    0,244 34(2 01)″ 13,349(110)  Ross 614B (LHS 1850) M5,5V 14,23 16,17  30 Gl 628 (Wolf 1061, BD−12°4523) M3,0V 10,07 11,93    0,236 01(1 67)″ 13,820(98)  31 Bintang Van Maanen (Gl 35, LHS 7) DZ7 12,38 14,21    0,231 88(1 79)″ 14,066(109)  32 Gl 1 (CD−37°15492) M3,0V 8,55 10,35    0,229 20(1 07)″ 14,231(66)  33 Wolf 424(FL Virginis, LHS 333, GJ 473) Wolf 424 A M5,5Ve 13,18 14,97    0,227 90(4 60)″  14,312(289) Wolf 424 B M7Ve 13,17 14,96  34 TZ Arietis (GJ 83,1, Luyten 1159-16) M4,5V 12,27 14,03    0,224 80(2 90)″ 14,509(187)  35 Gl 687 (LHS 450, BD+68°946) M3,0V 9,17 10,89    0,220 49(0 82)″ 14,793(55)  36 LHS 292 (LP 731-58) M6,5V 15,60 17,32    0,220 30(3 60)″ 14,805(242)  37 Gl 674 (LHS 449) M3,0V 9,38 11,09    0,220 25(1 59)″ 14,809(107)  38 GJ 1245 GJ 1245 A M5,5V 13,46 15,17    0,220 20(1 00)″ 14,812(67)  GJ 1245 B M6,0V 14,01 15,72    GJ 1245 C M? 16,75 18,46    39 GJ 440 (WD 1142-645) DQ6 11,50 13,18  7,500    0,216 57(2 01)″ 15,060(140)  40 GJ 1002 M5,5V 13,76 15,40    0,213 00(3 60)″ 15,313(259)  41 Ross 780 (GJ 876) M3,5V 10,17 11,81  3,480   0,212 59(1 96)″ 15,342(141)  42 LHS 288 (Luyten 143-23) M5,5V 13,90 15,51    0,208 95(2 73)″ 15,610(204)  43 GJ 412 GJ 412 A M1,0V 8,77 10,34    0,206 02(1 08)″ 15,832(83)  GJ 412 B (WX Ursae Majoris) M5,5V 14,48 16,05    44 Groombridge 1618 (GJ 380) K7,0V 6,59 8,16  4,000    0,205 81(0 67)″ 15,848(52)  45 GJ 388 M3,0V 9,32 10,87    0,204 60(2 80)″ 15,942(218) 46 GJ 832 M3,0V 8,66 10,20    0,202 78(1 32)″ 16,085(105)  47 LP 944-020 M9,0V 18,50 20,02    0,201 40(4 20)″CCD astrometry of southern very low-mass stars, C, G, Tinney, Monthly Notices of the Royal Astronomical Society 281, #2 (July 1996), pp, 644–658, 16,195(338)  48 DEN 0255-4700 L7,5V 22,92 24,44    0,201 37(3 89)″ 16,197(313)  49 GJ 682 M4,5V 10,95 12,45    0,199 65(2 30)″ 16,337(188) #SistemBintangKelas bintangmVMVTeffK(±err)PKPenParalaksarka saat(±err)JarakTahun cahaya(±err)ReferensitambahanPenandaanEpos J2000.0

 Lihat pula 
 Magnitudo absolut
 Magnitudo semu
 Daftar bintang paling terang
 Daftar bintang terbesar

 Referensi 

 Pranala luar 
 "The 100 nearest star systems", Research Consortium on Nearby Stars





 The dynamics of the closest stars

 Nearest Stars 3D View

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