Daftar bintang terdekat
Berikut adalah daftar bintang terdekat dari Bumi:
# | Penandaan | Kelas bintang | mV | MV | Teff K(±batas kesalahan) |
Epos J2000.0 | Paralaks[1][2] Arka saat(±batas kesalahan) |
Jarak[3] Tahun cahaya(±batas kesalahan) |
Rujukan tambahan | ||
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Sistem | Bintang | PK[1] | Pen[1] | ||||||||
Tata Surya | Matahari (Sol) | G2V[1] | −26,72[1] | 4,85[1] | 5,778[4] | — | — | 180° | 0,0000158(3) atau anggaran 8 menit cahaya |
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1 | Alpha Centauri (Rigil Kentaurus; Toliman) |
Proxima Centauri (V645 Centauri) | M5,5Ve | 11,09[1] | 15,53[1] | 3,040[5] | 14j 29m 43,0d | −62° 40′ 46″ | 0,768 87(0 29)″[6][7] | 4,2421(16) | [8] |
α Centauri A (HD 128620) | G2V[1] | 0,01[1] | 4,38[1] | 5,790[5] | 14j 39m 36,5d | −60° 50′ 02″ | 0,747 23(1 17)″[6][9] | 4,3650(68) | |||
α Centauri B (HD 128621) | K0V[1] | 1,34[1] | 5,71[1] | 5,260[5] | 14j 39m 35,1d | −60° 50′ 14″ | |||||
2 | Bintang Barnard (BD+04°3561a) | M4,0Ve | 9,53[1] | 13,22[1] | 3,134(102)[10] | 17j 57m 48,5d | +04° 41′ 36″ | 0,546 98(1 00)″[6][7] | 5,9630(109) | ||
3 | Wolf 359 (CN Leonis) | M6,0V[1] | 13,44[1] | 16,55[1] | 2,800(100)[11] | 10j 56m 29,2d | +07° 00′ 53″ | 0,419 10(2 10)″[6] | 7,7825(390) | ||
4 | Lalande 21185 (BD+36°2147) | M2,0V[1] | 7,47[1] | 10,44[1] | 3,400[12] | 11j 03m 20,2d | +35° 58′ 12″ | 0,393 42(0 70)″[6][7] | 8,2905(148) | ||
5 | Sirius (α Canis Majoris) |
Sirius A | A1V[1] | −1,43[1] | 1,47[1] | 9,940(210)[13] | 06j 45m 08,9d | −16° 42′ 58″ | 0,380 02(1 28)″[6][7] | 8,5828(289) | |
Sirius B | DA2[1] | 8,44[1] | 11,34[1] | 25,000(200)[14] | |||||||
6 | Luyten 726-8 | Luyten 726-8 A (BL Ceti) | M5,5Ve | 12,54[1] | 15,40[1] | 2,670 | 01j 39m 01,3d | −17° 57′ 01″ | 0,373 70(2 70)″[6] | 8,7280(631) | |
Luyten 726-8 B (UV Ceti) | M6,0Ve | 12,99[1] | 15,85[1] | ~2,600 | |||||||
7 | Ross 154 (V1216 Sagittarii) | M3,5Ve | 10,43[1] | 13,07[1] | 2,700 | 18j 49m 49,4d | −23° 50′ 10″ | 0,336 90(1 78)″[6][7] | 9,6813(512) | ||
8 | Ross 248 (HH Andromedae) | M5,5Ve | 12,29[1] | 14,79[1] | ? | 23j 41m 54,7d | +44° 10′ 30″ | 0,316 00(1 10)″[6] | 10,322(36) | ||
9 | Epsilon Eridani (BD−09°697) | K2V[1] | 3,73[1] | 6,19[1] | 5,100 | 03j 32m 55,8d | −09° 27′ 30″ | 0,309 99(0 79)″[6][7] | 10,522(27) | ||
10 | Lacaille 9352 (CD−36°15693) | M1,5Ve | 7,34[1] | 9,75[1] | 3,340 | 23j 05m 52,0d | −35° 51′ 11″ | 0,303 64(0 87)″[6][7] | 10,742(31) | ||
11 | Ross 128 (FI Virginis) | M4,0Vn | 11,13[1] | 13,51[1] | 2,800 | 11j 47m 44,4d | +00° 48′ 16″ | 0,298 72(1 35)″[6][7] | 10,919(49) | ||
12 | EZ Aquarii (GJ 866, Luyten 789-6) |
EZ Aquarii A | M5,0Ve | 13,33[1] | 15,64[1] | ? | 22j 38m 33,4d | −15° 18′ 07″ | 0,289 50(4 40)″[6] | 11,266(171) | |
EZ Aquarii B | M? | 13,27[1] | 15,58[1] | ? | |||||||
EZ Aquarii C | M? | 14,03[1] | 16,34[1] | ? | |||||||
13 | Procyon (α Canis Minoris) |
Procyon A | F5V-IV[1] | 0,38[1] | 2,66[1] | 6,650 | 07j 39m 18,1d | +05° 13′ 30″ | 0,286 05(0 81)″[6][7] | 11,402(32) | |
Procyon B | DA[1] | 10,70[1] | 12,98[1] | 9,700 | |||||||
14 | 61 Cygni | 61 Cygni A (BD+38°4343) | K5,0V[1] | 5,21[1] | 7,49[1] | 4,640 | 21j 06m 53,9d | +38° 44′ 58″ | 0,286 04(0 56)″[6][7] | 11,403(22) | |
61 Cygni B (BD+38°4344) | K7,0V[1] | 6,03[1] | 8,31[1] | 4,440 | 21j 06m 55,3d | +38° 44′ 31″ | |||||
15 | Struve 2398 (GJ 725, BD+59°1915) |
Struve 2398 A (HD 173739) | M3,0V[1] | 8,90[1] | 11,16[1] | ? | 18j 42m 46,7d | +59° 37′ 49″ | 0,283 00(1 69)″[6][7] | 11,525(69) | |
Struve 2398 B (HD 173740) | M3,5V[1] | 9,69[1] | 11,95[1] | ? | 18j 42m 46,9d | +59° 37′ 37″ | |||||
16 | Groombridge 34 (GJ 15) |
Groombridge 34 A (GX Andromedae) | M1,5V[1] | 8,08[1] | 10,32[1] | ? | 0j 18m 22,9d | +44° 01′ 23″ | 0,280 59(0 95)″[6][7] | 11,624(39) | |
Groombridge 34 B (GQ Andromedae) | M3,5V[1] | 11,06[1] | 13,30[1] | ? | |||||||
17 | Epsilon Indi (CPD−57°10015) |
Epsilon Indi A | K5Ve[1] | 4,69[1] | 6,89[1] | 4,280 | 22j 03m 21,7d | −56° 47′ 10″ | 0,275 84(0 69)″[6][7] | 11,824(30) | |
Epsilon Indi Ba | T1,0V | >23 | >25 | 1,280 | 22j 04m 10,5d | −56° 46′ 58″ | |||||
Epsilon Indi Bb | T6,0V | >23 | >25 | 850 | |||||||
18 | DX Cancri (G 51-15) | M6,5Ve | 14,78[1] | 16,98[1] | ? | 08j 29m 49,5d | +26° 46′ 37″ | 0,275 80(3 00)″[6] | 11,826(129) | ||
19 | Tau Ceti (BD−16°295) | G8Vp[1] | 3,49[1] | 5,68[1] | 5,344 | 01j 44m 04,1d | −15° 56′ 15″ | 0,274 39(0 76)″[6][7] | 11,887(33) | ||
20 | GJ 1061 (LHS 1565) | M5,5V[1] | 13,09[1] | 15,26[1] | ? | 03j 35m 59,7d | −44° 30′ 45″ | 0,272 01(1 30)″[15] | 11,991(57) | [16][17] | |
21 | YZ Ceti (LHS 138) | M4,5V[1] | 12,02[1] | 14,17[1] | ? | 01j 12m 30,6d | −16° 59′ 56″ | 0,268 84(2 95)″[6][7] | 12,132(133) | ||
22 | Bintang Luyten (BD+05°1668) | M3,5Vn | 9,86[1] | 11,97[1] | ? | 07j 27m 24,5d | +05° 13′ 33″ | 0,263 76(1 25)″[6][7] | 12,366(59) | ||
23 | Bintang Teegarden (SO025300,5+165258) | M6,5V | 15,14[1] | 17,22[1] | ? | 02j 53m 00,9d | +16° 52′ 53″ | 0,260 63(2 69)″[15] | 12,514(129) | [17] | |
24 | SCR 1845-6357 | SCR 1845-6357 A | M8,5V[1] | 17,39 | 19,41 | ? | 18j 45m 05,3d | −63° 57′ 48″ | 0,259 45(1 11)″[15] | 12,571(54) | [17] |
SCR 1845-6357 B | T6[18] | ? | ? | 950[18] | 18j 45m 02,6d | −63° 57′ 52″ | |||||
25 | Bintang Kapteyn (CD−45°1841) | M1,5V[1] | 8,84[1] | 10,87[1] | 3,800 | 05j 11m 40,6d | −45° 01′ 06″ | 0,255 27(0 86)″[6][7] | 12,777(43) | ||
26 | Lacaille 8760 (AX Microscopii) | M0,0V[1] | 6,67[1] | 8,69[1] | 3,340 | 21j 17m 15,3d | −38° 52′ 03″ | 0,253 43(1 12)″[6][7] | 12,870(57) | ||
27 | Kruger 60 (BD+56°2783) |
Kruger 60 A | M3,0V[1] | 9,79[1] | 11,76[1] | 3,180 | 22j 27m 59,5d | +57° 41′ 45″ | 0,248 06(1 39)″[6][9] | 13,149(74) | |
Kruger 60 B (DO Cephei) | M4,0V[1] | 11,41[1] | 13,38[1] | 2,890 | |||||||
28 | DEN 1048-3956 | M8,5V[1] | 17,39[1] | 19,37[1] | ? | 10j 48m 14,7d | −39° 56′ 06″ | 0,247 71(1 55)″[15] | 13,167(82) | [19][20] | |
29 | Ross 614 (V577 Monocerotis, GJ 234) |
Ross 614A (LHS 1849) | M4,5V[1] | 11,15[1] | 13,09[1] | ? | 06j 29m 23,4d | −02° 48′ 50″ | 0,244 34(2 01)″[6][9] | 13,349(110) | |
Ross 614B (LHS 1850) | M5,5V | 14,23[1] | 16,17[1] | ? | |||||||
30 | Gl 628 (Wolf 1061, BD−12°4523) | M3,0V[1] | 10,07[1] | 11,93[1] | ? | 16j 30m 18,1d | −12° 39′ 45″ | 0,236 01(1 67)″[6][7] | 13,820(98) | ||
31 | Bintang Van Maanen (Gl 35, LHS 7) | DZ7[1] | 12,38[1] | 14,21[1] | ? | 00j 49m 09,9d | +05° 23′ 19″ | 0,231 88(1 79)″[6][7] | 14,066(109) | ||
32 | Gl 1 (CD−37°15492) | M3,0V[1] | 8,55[1] | 10,35[1] | ? | 00j 05m 24,4d | −37° 21′ 27″ | 0,229 20(1 07)″[6][7] | 14,231(66) | ||
33 | Wolf 424 (FL Virginis, LHS 333, GJ 473) |
Wolf 424 A | M5,5Ve | 13,18[1] | 14,97[1] | ? | 12j 33m 17,2d | +09° 01′ 15″ | 0,227 90(4 60)″ [6] | 14,312(289) | |
Wolf 424 B | M7Ve | 13,17[1] | 14,96[1] | ? | |||||||
34 | TZ Arietis (GJ 83,1, Luyten 1159-16) | M4,5V[1] | 12,27[1] | 14,03[1] | ? | 02j 00m 13,2d | +13° 03′ 08″ | 0,224 80(2 90)″[6] | 14,509(187) | ||
35 | Gl 687 (LHS 450, BD+68°946) | M3,0V[1] | 9,17[1] | 10,89[1] | ? | 17j 36m 25,9d | +68° 20′ 21″ | 0,220 49(0 82)″[6][7] | 14,793(55) | ||
36 | LHS 292 (LP 731-58) | M6,5V[1] | 15,60[1] | 17,32[1] | ? | 10j 48m 12,6d | −11° 20′ 14″ | 0,220 30(3 60)″[6] | 14,805(242) | ||
37 | Gl 674 (LHS 449) | M3,0V[1] | 9,38[1] | 11,09[1] | ? | 17j 28m 39,9d | −46° 53′ 43″ | 0,220 25(1 59)″[6][7] | 14,809(107) | ||
38 | GJ 1245 | GJ 1245 A | M5,5V[1] | 13,46[1] | 15,17[1] | ? | 19j 53m 54,2d | +44° 24′ 55″ | 0,220 20(1 00)″[6] | 14,812(67) | |
GJ 1245 B | M6,0V[1] | 14,01[1] | 15,72[1] | ? | 19j 53m 55,2d | +44° 24′ 56″ | |||||
GJ 1245 C | M? | 16,75[1] | 18,46[1] | ? | 19j 53m 54,2d | +44° 24′ 55″ | |||||
39 | GJ 440 (WD 1142-645) | DQ6[1] | 11,50[1] | 13,18[1] | 7,500 | 11j 45m 42,9d | −64° 50′ 29″ | 0,216 57(2 01)″[6][7] | 15,060(140) | ||
40 | GJ 1002 | M5,5V[1] | 13,76[1] | 15,40[1] | ? | 00j 06m 43,8d | −07° 32′ 22″ | 0,213 00(3 60)″[6] | 15,313(259) | ||
41 | Ross 780 (GJ 876) | M3,5V[1] | 10,17[1] | 11,81[1] | 3,480 | 22j 53m 16,7d | −14° 15′ 49″ | 0,212 59(1 96)″[6][7] | 15,342(141) | ||
42 | LHS 288 (Luyten 143-23) | M5,5V[1] | 13,90[1] | 15,51[1] | ? | 10j 44m 21,2d | −61° 12′ 36″ | 0,208 95(2 73)″[15] | 15,610(204) | [17] | |
43 | GJ 412 | GJ 412 A | M1,0V[1] | 8,77[1] | 10,34[1] | ? | 11j 05m 28,6d | +43° 31′ 36″ | 0,206 02(1 08)″[6][7] | 15,832(83) | |
GJ 412 B (WX Ursae Majoris) | M5,5V[1] | 14,48[1] | 16,05[1] | ? | 11j 05m 30,4d | +43° 31′ 18″ | |||||
44 | Groombridge 1618 (GJ 380) | K7,0V[1] | 6,59[1] | 8,16[1] | 4,000 | 10j 11m 22,1d | +49° 27′ 15″ | 0,205 81(0 67)″[6][7] | 15,848(52) | ||
45 | GJ 388 | M3,0V[1] | 9,32[1] | 10,87[1] | ? | 10j 19m 36,4d | +19° 52′ 10″ | 0,204 60(2 80)″[6] | 15,942(218) | ||
46 | GJ 832 | M3,0V[1] | 8,66[1] | 10,20[1] | ? | 21j 33m 34,0d | −49° 00′ 32″ | 0,202 78(1 32)″[6][7] | 16,085(105) | ||
47 | LP 944-020 | M9,0V[1] | 18,50[1] | 20,02[1] | ? | 03j 39m 35,2d | −35° 25′ 41″ | 0,201 40(4 20)″[21] | 16,195(338) | ||
48 | DEN 0255-4700 | L7,5V[1] | 22,92[1] | 24,44[1] | ? | 02j 55m 03,7d | −47° 00′ 52″ | 0,201 37(3 89)″[15] | 16,197(313) | [20] | |
49 | GJ 682 | M4,5V[1] | 10,95[1] | 12,45[1] | ? | 17j 37m 03,7d | −44° 19′ 09″ | 0,199 65(2 30)″[6][7] | 16,337(188) | ||
# | Sistem | Bintang | Kelas bintang | mV | MV | Teff K(±err) |
PK[1] | Pen[1] | Paralaks[1][2] arka saat(±err) |
Jarak[3] Tahun cahaya(±err) |
Rujukan tambahan |
Penandaan | Epos J2000.0 |
Catatan kaki
- ^ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag ah ai aj ak al am an ao ap aq ar as at au av aw ax ay az ba bb bc bd be bf bg bh bi bj bk bl bm bn bo bp bq br bs bt bu bv bw bx by bz ca cb cc cd ce cf cg ch ci cj ck cl cm cn co cp cq cr cs ct cu cv cw cx cy cz da db dc dd de df dg dh di dj dk dl dm dn do dp dq dr ds dt du dv dw dx dy dz ea eb ec ed ee ef eg eh ei ej ek el em en eo ep eq er es et eu ev ew ex ey ez fa fb fc fd fe ff fg fh fi fj fk fl fm fn fo fp fq fr fs ft fu fv fw fx fy fz ga gb Research Consortium on Nearby Stars, GSU (2007-09-17). "The One Hundred Nearest Star Systems". RECONS. Diakses tanggal 2007-11-06. Hapus pranala luar di parameter
|journal=
(bantuan) - ^ a b Paralaks yang diberikan RECONS adalah min nilai bagi sumber diberi, begitu juga pengukuran oleh program RECONS,
- ^ a b Dari paralaks,
- ^ Sun Fact Sheet, NASA, Accessed on line November 8, 2007,
- ^ a b c Kervella, Pierre; Thevenin, Frederic (15 Mac 2003). "A Family Portrait of the Alpha Centauri System: VLT Interferometer Studies the Nearest Stars" Periksa nilai
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(bantuan). ESO Press Release 05/03. ESO. Diakses tanggal 2007-11-08. - ^ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag ah ai aj ak al am an ao ap aq Katalog Am Paralaks Trigonometri,
- ^ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac Katalog Hipparcos,
- ^ Burgasser et al, 2000
- ^ a b c Visual binary orbits and masses post Hipparcos, Staffan Söderhjelm, Astronomy and Astrophysics 341 (January 1999), pp, 121–140,
- ^ 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, DOI:10,1086/383289
- ^ Ya, V, Pavlenko, H, R, A, Jones, Yu, Lyubchik, J, Tennyson, and D, J, Pinfield (2006). "Spectral energy distribution for GJ406" Periksa nilai
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(bantuan). Astronomy and Astrophysics. 447 (2): 709–717. doi:10,1051/0004-6361:20052979 Periksa nilai|doi=
(bantuan). - ^ Carbon monoxide bands in M dwarfs, Y, V, Pavlenko and H, R, A, Jones, Astronomy and Astrophysics 396 (December 2002), pp, 967–975, DOI:10,1051/0004-6361:20021454
- ^ 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, DOI:10,1017/S1743921304004314
- ^ 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,
- ^ a b c d e f 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
- ^ a b c d 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
- ^ a b 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
- ^ 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
- ^ a b 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
- ^ 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,
Pranala luar
- "The 100 nearest star systems", Research Consortium on Nearby Stars
- "NStars database". NAU. Diakses tanggal 2005-10-24.
- "Map of the 25 nearest star systems". NASA. Diakses tanggal 2005-10-24.
- "Notable Nearby Stars". SolStation. Diakses tanggal 2005-10-24.
- "Cool stars in the solar Neighbourhood". D. Montes, UCM. Diakses tanggal 2005-11-14.
- The dynamics of the closest stars
- Takeda, G. (2006). "Structure and Evolution of Nearby Stars with Planets II. Physical Properties of ~ 1000 Cool Stars from the SPOCS Catalog". California & Carnegie Planet Search. Diakses tanggal 2006-10-13.
- Nearest Stars 3D View