Lys van naaste sterre

in Wikipedia, die vrye ensiklopedie
Spring na: navigasie, soek
Morgan-Keenan-Kellman-spektraaltipes van hoofreekssterre.

Hierdie lys van die naaste sterre bevat al die sterre en bruin dwergsterre binne ’n afstand van 5 parsek (16,3 ligjare) van die Sonnestelsel af, gerangskik volgens toenemende afstand.

Benewens die Sonnestelsel is daar nog 55 stelsels van sterre wat sover bekend binne dié afstand lê. Die stelsels bevat altesaam 56 waterstofverbrandende sterre, 15 bruin dwerge en 4 wit dwerge. Ondanks hul relatiewe nabyheid aan die Aarde, het net nege van hulle ’n skynbare magnitude van minder as 6,5, wat beteken net sowat 13% van die voorwerpe kan met die blote oog gesien word.[1] Benenewens die Son is daar net drie sterre van die eerste magnitude: Alpha Centauri, Sirius en Procyon. Al dié voorwerpe lê in die Lokale Borrel, ’n streek in die Orion-Cygnus-arm van die Melkweg.

Lys[wysig]

Sterre op die lys hier onder wat met die blote oog van die Aarde af gesien kan word, se skynbare magnitude het ’n ligblou agtergrond. Die sterklas van die sterre en bruin dwerge word volgens die kleur van hul spektraaltipe aangegee (die kleure is afgelei van konvensionele name vir die spektraaltipes en is nie die sterre se presiese sigbare kleur nie). Bruin dwerge se name het ’n bruin agtergrond. Baie van hulle is nie volgens hul sigbarelig-spektrum (mV) geklassifiseer nie, maar volgens hul infrarooi-magnitude (mJ). Van die parallakse en afstande is voorlopige waardes.[2]

# Afstand[3]
ligjare (±err)
Naam Sterklas Skynbare magnitude (mV of mJ) Absolute magnitude (MV of MJ) Epog J2000.0 Parallaks[2][4]
mbs
(±err)
Ontdek Notas
Stelsel Ster Ster # Regte klimming[2] Deklinasie[2]
0 Sonnestelsel Son G2V[2] −26,74[2] 4,85[2] het agt planete
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)[5][6] 1915 [7]
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)[5][8]
α Centauri B (HD 128621) 2 K1V[2] 1,34[2] 5,71[2] 14h 39m 35,1s −60° 50′ 14″ het een bekende planeet[9]
2 5,9630(109) Barnard se Ster (BD+04°3561a) 4 M4.0Ve 9,53[2] 13,22[2] 17h 57m 48,5s +04° 41′ 36″ 546,98(1 00)[5][6] 1916 grootste bekende eiebeweging[10]
3 6,52(49) WISE 1049-5319 WISE 1049-5319 A 5 L8 10,7 J 10h 49m 15,57s −53° 19′ 06″ 496 (37)[11] 2013 naaste bekende bruin dwerg
WISE 1049-5319 B 5 L9/T0?
4 7,7825(390) Wolf 359 (CN Leonis) 7 M6.0V[2] 13,44[2] 16,55[2] 10h 56m 29,2s +07° 00′ 53″ 419,10(210)[5]
5 8,2905(148) Lalande 21185 (BD+36°2147) 8 M2.0V[2] 7,47[2] 10,44[2] 11h 03m 20,2s +35° 58′ 12″ 393,42(070)[5][6]
6 8,5828(289) Sirius
(α Canis Majoris)
Sirius A 9 A1V[2] −1,46[2] 1,42[2] 06h 45m 08,9s −16° 42′ 58″ 380,02(128)[5][6] helderste ster aan die naghemel
Sirius B 9 DA2[2] 8,44[2] 11,34[2] 1844
7 8,7280(631) Luyten 726-8 Luyten 726-8 A (BL Ceti) 11 M5.5Ve 12,54[2] 15,40[2] 01h 39m 01,3s −17° 57′ 01″ 373,70(270)[5] 1948
Luyten 726-8 B (UV Ceti) 11 M6.0Ve 12,99[2] 15,85[2]
8 9,6813(512) Ross 154 (V1216 Sagittarii) 13 M3.5Ve 10,43[2] 13,07[2] 18h 49m 49,4s −23° 50′ 10″ 336,90(178)[5][6]
9 10,322(36) Ross 248 (HH Andromedae) 14 M5.5Ve 12,29[2] 14,79[2] 23h 41m 54,7s +44° 10′ 30″ 316,00(110)[5]
10 10,521 WISE 1506+7027 15 T6 14,3 J 15h 06m 49,9s +70° 27′ 36″ 310(042) 2011
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)[5][6] het glo 2 planete[12]
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)[5][6]
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)[5][6]
14 11,208 WISE 0350-5658 19 Y1 >22,8 J 03h 50m −56° 58′ 291(050) 2012
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° 18′ 07″ 289,50(440)[5]
EZ Aquarii B 20 M? 13,27[2] 15,58[2]
EZ Aquarii C 20 M? 14,03[2] 16,34[2]
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)[5][6]
Procyon B 23 DQZ[2] 10,70[2] 12,98[2]
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)[5][6] eerste ster naas die Son waarvan die afstand gemeet is[13]
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)[5][6]
Struve 2398 B (HD 173740) 27 M3.5V[2] 9,69[2] 11,95[2] 18h 42m 46,9s +59° 37′ 37″
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)[5][6]
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)[5][6]
Epsilon Indi Ba 31 T1.0V 12,3 J[14] 22h 04m 10,5s −56° 46′ 58″ 2003
Epsilon Indi Bb 31 T6.0V 13,2 J[14] 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)[5]
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)[5][6] naaste G-tipe ster; het glo 5 planete
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) [15][16]
24 12,132(133) YZ Ceti (LHS 138) 37 M4.5V[2] 12,02[2] 14,17[2] 01h 12m 30,6s −16° 59′ 56″ 268,84(295)[5][6]
25 12,366(59) Luyten se Ster (BD+05°1668) 38 M3.5Vn 9,86[2] 11,97[2] 07h 27m 24,5s +05° 13′ 33″ 263,76(125)[5][6]
26 12,514(129) Teegarden se Ster (SO025300.5+165258) 39 M6.5V 15,14[2] 17,22[2] 02h 53m 00,9s +16° 52′ 53″ 260,63(269)[17] 2003 [16]
27 12,571(54) SCR 1845-6357 SCR 1845-6357 A 40 M8.5V[2] 17,39 19,41 18h 45m 05,3s −63° 57′ 48″ 259,45(111)[17] [16]
SCR 1845-6357 B 40 T6[18] 13.3 J[14] 18h 45m 02,6s −63° 57′ 52″
28 12,777(43) Kapteyn se Ster (CD−45°1841) 42 M1.5V[2] 8,84[2] 10,87[2] 05h 11m 40,6s −45° 01′ 06″ 255,27(086)[5][6]
29 12,870(57) Lacaille 8760 (AX Microscopii) 43 M0.0V[2] 6,67[2] 8,69[2] 21h 17m 15,3s −38° 52′ 03″ 253,43(112)[5][6]
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)[5][8]
Kruger 60 B (DO Cephei) 45 M4.0V[2] 11,41[2] 13,38[2]
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)[17] [19][20]
33 13,259 UGPS 0722-05 48 T9[2] 16,52 J 07h 22m 27,3s –05° 40′ 30″ 246 2010
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)[5][8] 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)[5][6]
36 13,998 WISE 0410+1502 52 Y0 19,3 J 04h 10m 22,79s +15° 02′ 47″ 233(056) 2011
37 14,066(109) Van Maanen se Ster (Gliese 35, LHS 7) 53 DZ7[2] 12,38[2] 14,21[2] 00h 49m 09,9s +05° 23′ 19″ 231,88(179)[5][6] 1917
38 14,231(66) Gliese 1 (CD−37°15492) 54 M3.0V[2] 8,55[2] 10,35[2] 00h 05m 24,4s −37° 21′ 27″ 229,20(107)[5][6]
39 14,312(289) Wolf 424
(FL Virginis, LHS 333, Gliese 473)
Wolf 424 A 55 M5.5Ve 13,18[2] 14,97[2] 12h 33m 17,2s +09° 01′ 15″ 227,90(460)[5]
Wolf 424 B 55 M7Ve 13,17[2] 14,96[2]
40 14,509(187) TZ Arietis (Gliese 83.1, Luyten 1159-16) 57 M4.5V[2] 12,27[2] 14,03[2] 02h 00m 13,2s +13° 03′ 08″ 224,80(290)[5]
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)[5][6]
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)[5]
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)[5][6] het een bekende planeet[21]
44 14,812(67) GJ 1245 GJ 1245 A 61 M5.5V[2] 13,46[2] 15,17[2] 19h 53m 54,2s +44° 24′ 55″ 220,20(100)[5]
GJ 1245 B 61 M6.0V[2] 14,01[2] 15,72[2] 19h 53m 55,2s +44° 24′ 56″
GJ 1245 C 61 M5.5 16,75[2] 18,46[2] 19h 53m 54,2s +44° 24′ 55″
45 15,060(140) Gliese 440 (WD 1142-645) 64 DQ6[2] 11,50[2] 13,18[2] 11h 45m 42,9s −64° 50′ 29″ 216,57(201)[5][6]
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)[5]
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)[5][6] het 4 bekende planete[22]
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)[17] [16]
49 15,757 WISE 1405+5534 68 Y0p 20,09 J 14h 05m +55° 34′ 207 2011
50 15,832(83) Gliese 412 Gliese 412 A 69 M1.0V[2] 8,77[2] 10,34[2] 11h 05m 28,6s +43° 31′ 36″ 206,02(108)[5][6]
Gliese 412 B (WX Ursae Majoris) 69 M5.5V[2] 14,48[2] 16,05[2] 11h 05m 30,4s +43° 31′ 18″
51 15,848(52) Groombridge 1618 (Gliese 380) 71 K7.0V[2] 6,59[2] 8,16[2] 10h 11m 22,1s +49° 27′ 15″ 205,81(067)[5][6]
52 15,942(218) AD Leonis 72 M3.0V[2] 9,32[2] 10,87[2] 10h 19m 36,4s +19° 52′ 10″ 204,60(280)[5]
53 16,067 DENIS J081730.0-615520 73 T6 08h 17m -61° 55′ 203 2010
54 16,085(105) Gliese 832 74 M3.0V[2] 8,66[2] 10,20[2] 21h 33m 34,0s −49° 00′ 32″ 202,78(132)[5][6] het 1 bekende planeet[23]
55 16,195(338) LP 944-020 75 M9.0V[2] 18,50[2] 20,02[2] 03h 39m 35,2s −35° 25′ 41″ 201,40(420)[24]
56 16,197(313) DEN 0255-4700 76 L7.5V[2] 22,92[2] 24,44[2] 02h 55m 03,7s −47° 00′ 52″ 201,37(389)[17] [20]
# Afstand[3]
ligjare
(±err)
Stelsel Ster Ster # Sterklas Skynbare magnitude (mV of mJ) Absolute magnitude (mV of mJ) Regte klimming[2] Deklinasie[2] Parallaks[2][4]
milliboogsek.
(±err)
Ontdek Notas
Naam Epog J2000.0

Die toekoms[wysig]

Die afstand van die naaste sterre van 20 000 jaar gelede tot oor 80 000.

Ross 248, tans op ’n afstand van 10,3 ligjare, het ’n radiale snelheid van −81 km/s. In sowat 31 000 jaar kan dit vir verskeie millennia die naaste ster aan die Son wees met ’n afstand van 3,02 ligjare oor 36 000 jaar.[25] Gliese 445, tans 17,6 ligjare van die Son af, het ’n radiale snelheid van −119 km/s. In sowat 40 000 years sal dit vir ’n paar duisend jaar die naaste ster wees.[25]

Verwysings[wysig]

  1. Weaver, Harold F. (1947). “The Visibility of Stars Without Optical Aid”. Publications of the Astronomical Society of the Pacific 59 (350): 232–243. DOI:10.1086/125956.
  2. 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 2,180 2,181 2,182 Research Consortium on Nearby Stars, Georgia State University (2007-09-17). “The One Hundred Nearest Star Systems”. RECONS. Besoek op 2007-11-06.
  3. 3,0 3,1 Van parallaks.
  4. 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.
  5. 5,00 5,01 5,02 5,03 5,04 5,05 5,06 5,07 5,08 5,09 5,10 5,11 5,12 5,13 5,14 5,15 5,16 5,17 5,18 5,19 5,20 5,21 5,22 5,23 5,24 5,25 5,26 5,27 5,28 5,29 5,30 5,31 5,32 5,33 5,34 5,35 5,36 5,37 5,38 5,39 5,40 5,41 General Catalogue of Trigonometric Parallaxes.
  6. 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 Hipparcos Catalogue.
  7. Burgasser et al. 2000
  8. 8,0 8,1 8,2 Visual binary orbits and masses post Hipparcos, Staffan Söderhjelm, Astronomy and Astrophysics 341 (January 1999), pp. 121–140.
  9. "The exoplanet next door: Earth-sized world discovered in nearby α Centauri star system". Eric Hand, Nature, October 16, 2012. Accessed October 16, 2012.
  10. Edward Emerson Barnard (1916). “A small star with large proper motion”. Astronomical Journal 29 (695). DOI:10.1086/104156.
  11. Luhman, K. L.. “Discovery of a Binary Brown Dwarf at 2 Parsecs from the Sun”. Astrophysical Journal Letters (to be published).
  12. Janson, M. et al. (September 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, doi:10.1051/0004-6361:200809984, Bibcode2008A&A...488..771J 
  13. Bessel, F. W. (1839). “Bestimmung der Entfernung des 61sten Sterns des Schwans. Von Herrn Geheimen - Rath und Ritter Bessel” (in German). Astronomische Nachrichten 16 (5-6): 65. DOI:10.1002/asna.18390160502. A parallax of 313.6 mas yields a distance of 10.4 light years
  14. 14,0 14,1 14,2 Chris Gelino, Davy Kirkpatrick, Adam Burgasser. “DwarfArchives.org: Photometry, spectroscopy, and astrometry of M, L, and T dwarfs”. caltech.edu. URL besoek op 2012-06-10. (main page)
  15. 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 (Julie 1997), pp. 388–395. doi:10.1086/118482
  16. 16,0 16,1 16,2 16,3 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
  17. 17,0 17,1 17,2 17,3 17,4 Stelsels waarvan die eerste akkurate trigonometriese parallakse deur RECONS gemeet is
  18. 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 (Augustus 2007), pp. 655–659. doi:10.1051/0004-6361:20077881
  19. 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
  20. 20,0 20,1 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
  21. http://exoplanet.eu/star.php?st=GJ+674
  22. (July 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. DOI:10.1088/0004-637X/719/1/890.
  23. Bailey, Jeremy et al. (2008). “A Jupiter-like Planet Orbiting the Nearby M Dwarf GJ832”. The Astrophysical Journal 690 (1): 743–747. DOI:10.1088/0004-637X/690/1/743. Besoek op 2008-09-02.
  24. 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.
  25. 25,0 25,1 The Close Approach of Stars in the Solar Neighborhood


Soorte sterre en sterregroepe
HD 820.jpg
 Sterre   SterDwergsterWit dwergSwart dwergRooi dwergGeel dwergBruin dwergSubdwergReusesterHelder reusSuperreusHiperreusSubreusRooi reusBlou reusNeutronsterPulsarBlou dwaalsterCepheïedVeranderlike sterNovaOpvlamsterRR Lyrae-sterWolf-RayetsterT Tauri-sterHerbig Ae/Be-sterPoolster
 Sterregroepe   DubbelsterX-straaldubbelsterVeelvoudige sterSterreswermSterrestroomSterrestelselMelkwegSterrestelselswermSuperswerm
 Verwante voorwerpe   SupernovaNewelPlanetêre newelMessier-voorwerpHeelalMultiversumSterrebeeldAsterismeSterreklassifikasieSwartkolkSuperholteInterstellêre mediumMolekulêre wolk
 Lyste   Lys van sterrekundige katalogusseLys van naaste sterreLys van grootste sterreLys van gewone name van sterre