Sekolapedia

Portal Sekolah di Indonesia

Popular Articles
Daftar Sekolah
Ensiklopedia
Kode Pos

×

Ensiklopedia

Home
Ensiklopedia

Ensiklopedi – Sekolapedia

Tekan Enter untuk memulai pencarian cepat.

Kembali ke Ensiklopedia Arsip Wikipedia Indonesia

Daftar bintang terdekat

Berikut adalah daftar bintang terdekat dalam jarak 5,0 parsec (16,3 tahun cahaya) dari Tata Surya. Sejauh ini, 76 bintang seperti itu telah ditemukan, dan hanya sembilan yang cukup terang untuk terlihat tanpa teleskop. Cahaya tampak perlu mencapai atau melebihi tingkat kecerahan paling redup, yaitu nilai magnitudo semu sebesar 6,5 agar dapat dilihat dengan mata telanjang dari Bumi.^[1]

Daftar

#	Penandaan		Kelas bintang	m_V	M_V	T_eff K (±batas kesalahan)	Epos J2000.0		Paralaks^[2]^[3] mili detik busur (±batas kesalahan)	Jarak^[4] Tahun cahaya (±batas kesalahan)	Referensi tambahan
#	Sistem	Bintang	Kelas bintang	m_V	M_V	T_eff K (±batas kesalahan)	PK^[2]	Pen^[2]	Paralaks^[2]^[3] mili detik busur (±batas kesalahan)	Jarak^[4] Tahun cahaya (±batas kesalahan)	Referensi tambahan
	Tata Surya	Matahari (Sol)	G2V^[2]	−26,72^[2]	4,85^[2]	5,778^[5]	—	—	180°	0,0000158(3) atau 8 menit cahaya
1	Alpha Centauri (Rigil Kentaurus; Toliman)	Proxima Centauri (V645 Centauri)	M5,5Ve	11,09^[2]	15,53^[2]	3,040^[6]	14^j 29^m 43,0^d	−62° 40′ 46″	0,768 87(0 29)″^[7]^[8]	4,2421(16)	^[9]
		α Centauri A (HD 128620)	G2V^[2]	0,01^[2]	4,38^[2]	5,790^[6]	14^j 39^m 36,5^d	−60° 50′ 02″	0,747 23(1 17)″^[7]^[10]	4,3650(68)
		α Centauri B (HD 128621)	K0V^[2]	1,34^[2]	5,71^[2]	5,260^[6]	14^j 39^m 35,1^d	−60° 50′ 14″	0,747 23(1 17)″^[7]^[10]	4,3650(68)
2	Bintang Barnard (BD+04°3561a)		M4,0Ve	9,53^[2]	13,22^[2]	3,134(102)^[11]	17^j 57^m 48,5^d	+04° 41′ 36″	0,546 98(1 00)″^[7]^[8]	5,9630(109)
3	Wolf 359 (CN Leonis)		M6,0V^[2]	13,44^[2]	16,55^[2]	2,800(100)^[12]	10^j 56^m 29,2^d	+07° 00′ 53″	0,419 10(2 10)″^[7]	7,7825(390)
4	Lalande 21185 (BD+36°2147)		M2,0V^[2]	7,47^[2]	10,44^[2]	3,400^[13]	11^j 03^m 20,2^d	+35° 58′ 12″	0,393 42(0 70)″^[7]^[8]	8,2905(148)
5	Sirius (α Canis Majoris)	Sirius A	A1V^[2]	−1,43^[2]	1,47^[2]	9,940(210)^[14]	06^j 45^m 08,9^d	−16° 42′ 58″	0,380 02(1 28)″^[7]^[8]	8,5828(289)
5	Sirius (α Canis Majoris)	Sirius B	DA2^[2]	8,44^[2]	11,34^[2]	25,000(200)^[15]	06^j 45^m 08,9^d	−16° 42′ 58″	0,380 02(1 28)″^[7]^[8]	8,5828(289)
6	Luyten 726-8	Luyten 726-8 A (BL Ceti)	M5,5Ve	12,54^[2]	15,40^[2]	2,670	01^j 39^m 01,3^d	−17° 57′ 01″	0,373 70(2 70)″^[7]	8,7280(631)
6	Luyten 726-8	Luyten 726-8 B (UV Ceti)	M6,0Ve	12,99^[2]	15,85^[2]	~2,600	01^j 39^m 01,3^d	−17° 57′ 01″	0,373 70(2 70)″^[7]	8,7280(631)
7	Ross 154 (V1216 Sagittarii)		M3,5Ve	10,43^[2]	13,07^[2]	2,700	18^j 49^m 49,4^d	−23° 50′ 10″	0,336 90(1 78)″^[7]^[8]	9,6813(512)
8	Ross 248 (HH Andromedae)		M5,5Ve	12,29^[2]	14,79^[2]	?	23^j 41^m 54,7^d	+44° 10′ 30″	0,316 00(1 10)″^[7]	10,322(36)
9	Epsilon Eridani (BD−09°697)		K2V^[2]	3,73^[2]	6,19^[2]	5,100	03^j 32^m 55,8^d	−09° 27′ 30″	0,309 99(0 79)″^[7]^[8]	10,522(27)
10	Lacaille 9352 (CD−36°15693)		M1,5Ve	7,34^[2]	9,75^[2]	3,340	23^j 05^m 52,0^d	−35° 51′ 11″	0,303 64(0 87)″^[7]^[8]	10,742(31)
11	Ross 128 (FI Virginis)		M4,0Vn	11,13^[2]	13,51^[2]	2,800	11^j 47^m 44,4^d	+00° 48′ 16″	0,298 72(1 35)″^[7]^[8]	10,919(49)
12	EZ Aquarii (GJ 866, Luyten 789-6)	EZ Aquarii A	M5,0Ve	13,33^[2]	15,64^[2]	?	22^j 38^m 33,4^d	−15° 18′ 07″	0,289 50(4 40)″^[7]	11,266(171)
		EZ Aquarii B	M?	13,27^[2]	15,58^[2]	?
		EZ Aquarii C	M?	14,03^[2]	16,34^[2]	?
13	Procyon (α Canis Minoris)	Procyon A	F5V-IV^[2]	0,38^[2]	2,66^[2]	6,650	07^j 39^m 18,1^d	+05° 13′ 30″	0,286 05(0 81)″^[7]^[8]	11,402(32)
13	Procyon (α Canis Minoris)	Procyon B	DA^[2]	10,70^[2]	12,98^[2]	9,700	07^j 39^m 18,1^d	+05° 13′ 30″	0,286 05(0 81)″^[7]^[8]	11,402(32)
14	61 Cygni	61 Cygni A (BD+38°4343)	K5,0V^[2]	5,21^[2]	7,49^[2]	4,640	21^j 06^m 53,9^d	+38° 44′ 58″	0,286 04(0 56)″^[7]^[8]	11,403(22)
14	61 Cygni	61 Cygni B (BD+38°4344)	K7,0V^[2]	6,03^[2]	8,31^[2]	4,440	21^j 06^m 55,3^d	+38° 44′ 31″	0,286 04(0 56)″^[7]^[8]	11,403(22)
15	Struve 2398 (GJ 725, BD+59°1915)	Struve 2398 A (HD 173739)	M3,0V^[2]	8,90^[2]	11,16^[2]	?	18^j 42^m 46,7^d	+59° 37′ 49″	0,283 00(1 69)″^[7]^[8]	11,525(69)
15	Struve 2398 (GJ 725, BD+59°1915)	Struve 2398 B (HD 173740)	M3,5V^[2]	9,69^[2]	11,95^[2]	?	18^j 42^m 46,9^d	+59° 37′ 37″	0,283 00(1 69)″^[7]^[8]	11,525(69)
16	Groombridge 34 (GJ 15)	Groombridge 34 A (GX Andromedae)	M1,5V^[2]	8,08^[2]	10,32^[2]	?	0^j 18^m 22,9^d	+44° 01′ 23″	0,280 59(0 95)″^[7]^[8]	11,624(39)
16	Groombridge 34 (GJ 15)	Groombridge 34 B (GQ Andromedae)	M3,5V^[2]	11,06^[2]	13,30^[2]	?	0^j 18^m 22,9^d	+44° 01′ 23″	0,280 59(0 95)″^[7]^[8]	11,624(39)
17	Epsilon Indi (CPD−57°10015)	Epsilon Indi A	K5Ve^[2]	4,69^[2]	6,89^[2]	4,280	22^j 03^m 21,7^d	−56° 47′ 10″	0,275 84(0 69)″^[7]^[8]	11,824(30)
		Epsilon Indi Ba	T1,0V	>23	>25	1,280	22^j 04^m 10,5^d	−56° 46′ 58″
		Epsilon Indi Bb	T6,0V	>23	>25	850	22^j 04^m 10,5^d	−56° 46′ 58″
18	DX Cancri (G 51-15)		M6,5Ve	14,78^[2]	16,98^[2]	?	08^j 29^m 49,5^d	+26° 46′ 37″	0,275 80(3 00)″^[7]	11,826(129)
19	Tau Ceti (BD−16°295)		G8Vp^[2]	3,49^[2]	5,68^[2]	5,344	01^j 44^m 04,1^d	−15° 56′ 15″	0,274 39(0 76)″^[7]^[8]	11,887(33)
20	GJ 1061 (LHS 1565)		M5,5V^[2]	13,09^[2]	15,26^[2]	?	03^j 35^m 59,7^d	−44° 30′ 45″	0,272 01(1 30)″^[16]	11,991(57)	^[17]^[18]
21	YZ Ceti (LHS 138)		M4,5V^[2]	12,02^[2]	14,17^[2]	?	01^j 12^m 30,6^d	−16° 59′ 56″	0,268 84(2 95)″^[7]^[8]	12,132(133)
22	Bintang Luyten (BD+05°1668)		M3,5Vn	9,86^[2]	11,97^[2]	?	07^j 27^m 24,5^d	+05° 13′ 33″	0,263 76(1 25)″^[7]^[8]	12,366(59)
23	Bintang Teegarden (SO025300,5+165258)		M6,5V	15,14^[2]	17,22^[2]	?	02^j 53^m 00,9^d	+16° 52′ 53″	0,260 63(2 69)″^[16]	12,514(129)	^[18]
24	SCR 1845-6357	SCR 1845-6357 A	M8,5V^[2]	17,39	19,41	?	18^j 45^m 05,3^d	−63° 57′ 48″	0,259 45(1 11)″^[16]	12,571(54)	^[18]
24	SCR 1845-6357	SCR 1845-6357 B	T6^[19]	?	?	950^[19]	18^j 45^m 02,6^d	−63° 57′ 52″	0,259 45(1 11)″^[16]	12,571(54)	^[18]
25	Bintang Kapteyn (CD−45°1841)		M1,5V^[2]	8,84^[2]	10,87^[2]	3,800	05^j 11^m 40,6^d	−45° 01′ 06″	0,255 27(0 86)″^[7]^[8]	12,777(43)
26	Lacaille 8760 (AX Microscopii)		M0,0V^[2]	6,67^[2]	8,69^[2]	3,340	21^j 17^m 15,3^d	−38° 52′ 03″	0,253 43(1 12)″^[7]^[8]	12,870(57)
27	Kruger 60 (BD+56°2783)	Kruger 60 A	M3,0V^[2]	9,79^[2]	11,76^[2]	3,180	22^j 27^m 59,5^d	+57° 41′ 45″	0,248 06(1 39)″^[7]^[10]	13,149(74)
27	Kruger 60 (BD+56°2783)	Kruger 60 B (DO Cephei)	M4,0V^[2]	11,41^[2]	13,38^[2]	2,890	22^j 27^m 59,5^d	+57° 41′ 45″	0,248 06(1 39)″^[7]^[10]	13,149(74)
28	DEN 1048-3956		M8,5V^[2]	17,39^[2]	19,37^[2]	?	10^j 48^m 14,7^d	−39° 56′ 06″	0,247 71(1 55)″^[16]	13,167(82)	^[20]^[21]
29	Ross 614 (V577 Monocerotis, GJ 234)	Ross 614A (LHS 1849)	M4,5V^[2]	11,15^[2]	13,09^[2]	?	06^j 29^m 23,4^d	−02° 48′ 50″	0,244 34(2 01)″^[7]^[10]	13,349(110)
29	Ross 614 (V577 Monocerotis, GJ 234)	Ross 614B (LHS 1850)	M5,5V	14,23^[2]	16,17^[2]	?	06^j 29^m 23,4^d	−02° 48′ 50″	0,244 34(2 01)″^[7]^[10]	13,349(110)
30	Gl 628 (Wolf 1061, BD−12°4523)		M3,0V^[2]	10,07^[2]	11,93^[2]	?	16^j 30^m 18,1^d	−12° 39′ 45″	0,236 01(1 67)″^[7]^[8]	13,820(98)
31	Bintang Van Maanen (Gl 35, LHS 7)		DZ7^[2]	12,38^[2]	14,21^[2]	?	00^j 49^m 09,9^d	+05° 23′ 19″	0,231 88(1 79)″^[7]^[8]	14,066(109)
32	Gl 1 (CD−37°15492)		M3,0V^[2]	8,55^[2]	10,35^[2]	?	00^j 05^m 24,4^d	−37° 21′ 27″	0,229 20(1 07)″^[7]^[8]	14,231(66)
33	Wolf 424 (FL Virginis, LHS 333, GJ 473)	Wolf 424 A	M5,5Ve	13,18^[2]	14,97^[2]	?	12^j 33^m 17,2^d	+09° 01′ 15″	0,227 90(4 60)″ ^[7]	14,312(289)
33	Wolf 424 (FL Virginis, LHS 333, GJ 473)	Wolf 424 B	M7Ve	13,17^[2]	14,96^[2]	?	12^j 33^m 17,2^d	+09° 01′ 15″	0,227 90(4 60)″ ^[7]	14,312(289)
34	TZ Arietis (GJ 83,1, Luyten 1159-16)		M4,5V^[2]	12,27^[2]	14,03^[2]	?	02^j 00^m 13,2^d	+13° 03′ 08″	0,224 80(2 90)″^[7]	14,509(187)
35	Gl 687 (LHS 450, BD+68°946)		M3,0V^[2]	9,17^[2]	10,89^[2]	?	17^j 36^m 25,9^d	+68° 20′ 21″	0,220 49(0 82)″^[7]^[8]	14,793(55)
36	LHS 292 (LP 731-58)		M6,5V^[2]	15,60^[2]	17,32^[2]	?	10^j 48^m 12,6^d	−11° 20′ 14″	0,220 30(3 60)″^[7]	14,805(242)
37	Gl 674 (LHS 449)		M3,0V^[2]	9,38^[2]	11,09^[2]	?	17^j 28^m 39,9^d	−46° 53′ 43″	0,220 25(1 59)″^[7]^[8]	14,809(107)
38	GJ 1245	GJ 1245 A	M5,5V^[2]	13,46^[2]	15,17^[2]	?	19^j 53^m 54,2^d	+44° 24′ 55″	0,220 20(1 00)″^[7]	14,812(67)
		GJ 1245 B	M6,0V^[2]	14,01^[2]	15,72^[2]	?	19^j 53^m 55,2^d	+44° 24′ 56″
		GJ 1245 C	M?	16,75^[2]	18,46^[2]	?	19^j 53^m 54,2^d	+44° 24′ 55″
39	GJ 440 (WD 1142-645)		DQ6^[2]	11,50^[2]	13,18^[2]	7,500	11^j 45^m 42,9^d	−64° 50′ 29″	0,216 57(2 01)″^[7]^[8]	15,060(140)
40	GJ 1002		M5,5V^[2]	13,76^[2]	15,40^[2]	?	00^j 06^m 43,8^d	−07° 32′ 22″	0,213 00(3 60)″^[7]	15,313(259)
41	Ross 780 (GJ 876)		M3,5V^[2]	10,17^[2]	11,81^[2]	3,480	22^j 53^m 16,7^d	−14° 15′ 49″	0,212 59(1 96)″^[7]^[8]	15,342(141)
42	LHS 288 (Luyten 143-23)		M5,5V^[2]	13,90^[2]	15,51^[2]	?	10^j 44^m 21,2^d	−61° 12′ 36″	0,208 95(2 73)″^[16]	15,610(204)	^[18]
43	GJ 412	GJ 412 A	M1,0V^[2]	8,77^[2]	10,34^[2]	?	11^j 05^m 28,6^d	+43° 31′ 36″	0,206 02(1 08)″^[7]^[8]	15,832(83)
43	GJ 412	GJ 412 B (WX Ursae Majoris)	M5,5V^[2]	14,48^[2]	16,05^[2]	?	11^j 05^m 30,4^d	+43° 31′ 18″	0,206 02(1 08)″^[7]^[8]	15,832(83)
44	Groombridge 1618 (GJ 380)		K7,0V^[2]	6,59^[2]	8,16^[2]	4,000	10^j 11^m 22,1^d	+49° 27′ 15″	0,205 81(0 67)″^[7]^[8]	15,848(52)
45	GJ 388		M3,0V^[2]	9,32^[2]	10,87^[2]	?	10^j 19^m 36,4^d	+19° 52′ 10″	0,204 60(2 80)″^[7]	15,942(218)
46	GJ 832		M3,0V^[2]	8,66^[2]	10,20^[2]	?	21^j 33^m 34,0^d	−49° 00′ 32″	0,202 78(1 32)″^[7]^[8]	16,085(105)
47	LP 944-020		M9,0V^[2]	18,50^[2]	20,02^[2]	?	03^j 39^m 35,2^d	−35° 25′ 41″	0,201 40(4 20)″^[22]	16,195(338)
48	DEN 0255-4700		L7,5V^[2]	22,92^[2]	24,44^[2]	?	02^j 55^m 03,7^d	−47° 00′ 52″	0,201 37(3 89)″^[16]	16,197(313)	^[21]
49	GJ 682		M4,5V^[2]	10,95^[2]	12,45^[2]	?	17^j 37^m 03,7^d	−44° 19′ 09″	0,199 65(2 30)″^[7]^[8]	16,337(188)
#	Sistem	Bintang	Kelas bintang	m_V	M_V	T_eff K (±err)	PK^[2]	Pen^[2]	Paralaks^[2]^[3] arka saat (±err)	Jarak^[4] Tahun cahaya (±err)	Referensi tambahan
#	Penandaan		Kelas bintang	m_V	M_V	T_eff K (±err)	Epos J2000.0		Paralaks^[2]^[3] arka saat (±err)	Jarak^[4] Tahun cahaya (±err)	Referensi tambahan

Lihat pula

Magnitudo absolut
Magnitudo semu
Daftar bintang paling terang
Daftar bintang terbesar

Referensi

↑ 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.
1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 55 56 57 58 59 60 61 62 63 64 65 66 67 68 69 70 71 72 73 74 75 76 77 78 79 80 81 82 83 84 85 86 87 88 89 90 91 92 93 94 95 96 97 98 99 100 101 102 103 104 105 106 107 108 109 110 111 112 113 114 115 116 117 118 119 120 121 122 123 124 125 126 127 128 129 130 131 132 133 134 135 136 137 138 139 140 141 142 143 144 145 146 147 148 149 150 151 152 153 154 155 156 157 158 159 160 161 162 163 164 165 166 167 168 169 170 171 172 173 174 175 176 177 178 179 180 181 182 183 184 Research Consortium on Nearby Stars, GSU (2007-09-17). "The One Hundred Nearest Star Systems". RECONS. Diakses tanggal 6 November 2007. ;
1 2 Paralaks yang diberikan RECONS adalah min nilai bagi sumber diberi, begitu juga pengukuran oleh program RECONS,
1 2 Dari paralaks,
↑ Sun Fact Sheet, NASA, Accessed on line November 8, 2007,
1 2 3 Kervella, Pierre; Thevenin, Frederic (15 Mac 2003). "A Family Portrait of the Alpha Centauri System: VLT Interferometer Studies the Nearest Stars". ESO Press Release 05/03. ESO. Diakses tanggal 2007-11-08. Pemeliharaan CS1: Banyak nama: authors list (link)
1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 Katalog Am Paralaks Trigonometri,
1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 Katalog Hipparcos,
↑ Burgasser et al, 2000
1 2 3 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". Astronomy and Astrophysics. 447 (2): 709–717. doi:10,1051/0004-6361:20052979. ; Pemeliharaan CS1: Banyak nama: authors list (link)
↑ 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,
1 2 3 4 5 6 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
1 2 3 4 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
1 2 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
1 2 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. Diarsipkan dari asli tanggal 2005-10-30. 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

Sumber data: id.wikipedia.org via REST API v1

Search