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Lys van naaste sterre: Verskil tussen weergawes

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Lyn 1:
[[Lêer:Morgan-Keenan spectral classification.png|thumb|350px300px|Morgan-Keenan-Kellman-spektraaltipes van [[hoofreeks]]sterre.]]
 
Hierdie '''lys van die naaste sterre''' bevat al die sterre en [[bruin dwerg]]sterre binne ’n afstand van 5 [[parsek]] (16,3 [[ligjare]]) van die [[Sonnestelsel]] af, gerangskik volgens toenemende afstand.
Lyn 49:
| Proxima Centauri (V645 Centauri)
| 1
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M5.5Ve]]
| 11,09<ref name=RECONS />
| 15,53<ref name=RECONS />
Lyn 61:
| α&nbsp;Centauri&nbsp;A (HD&nbsp;128620)
| 2
| style="background: #fff4ea;" | [[Sterreklassifikasie#Spektraaltipes|G2V]]<ref name=RECONS />
| style="background: lightblue;" | 0,01<ref name=RECONS />
| 4,38<ref name=RECONS />
Lyn 72:
| α&nbsp;Centauri&nbsp;B (HD&nbsp;128621)
| 2
| style="background: #ffd2a1;" | [[Sterreklassifikasie#Spektraaltipes|K1V]]<ref name=RECONS />
| style="background: lightblue;" | 1,34<ref name=RECONS />
| 5,71<ref name=RECONS />
Lyn 84:
| colspan="2" | [[Barnard se Ster]] (BD+04°3561a)
| 4
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M4.0Ve]]
| 9,53<ref name=RECONS />
| 13,22<ref name=RECONS />
Lyn 101:
| rowspan="2" | 3
| rowspan="2" | 6,52(49)
| style="background: #D99058C3B091" rowspan="2" | WISE 1049-5319
| style="background: #D99058C3B091"| WISE 1049-5319 A
| 5
| style="background: #E6B2B2;" | [[Bruin dwerg|L8]]
| 10,7 J
|
Lyn 118:
| rowspan="2" | naaste bekende bruin dwerg
|-size
| style="background: #D99058C3B091" | WISE 1049-5319 B
| 5
| style="background: #FFB6C1;" | [[Bruin dwerg|L9/T0]]?
|
|
Lyn 128:
| colspan="2" | Wolf&nbsp;359 (CN&nbsp;Leonis)
| 7
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M6.0V]]<ref name=RECONS />
| 13,44<ref name=RECONS />
| 16,55<ref name=RECONS />
Lyn 141:
| colspan="2" | Lalande&nbsp;21185 (BD+36°2147)
| 8
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M2.0V]]<ref name=RECONS />
| 7,47<ref name=RECONS />
| 10,44<ref name=RECONS />
Lyn 155:
| Sirius A
| 9
| style="background: #f8f7ff" | [[Sterreklassifikasie#Spektraaltipes|A1V]]<ref name=RECONS />
| style="background: lightblue;" | −1,46<ref name=RECONS />
| 1,42<ref name=RECONS />
Lyn 166:
| Sirius&nbsp;B
| 9
| style="background:#f8f7ff" | [[Wit dwerg|DA2]]<ref name=RECONS />
| 8,44<ref name=RECONS />
| 11,34<ref name=RECONS />
Lyn 176:
| Luyten&nbsp;726-8&nbsp;A (BL&nbsp;Ceti)
| 11
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M5.5Ve]]
| 12,54<ref name=RECONS />
| 15,40<ref name=RECONS />
Lyn 187:
| Luyten&nbsp;726-8&nbsp;B (UV&nbsp;Ceti)
| 11
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M6.0Ve]]
| 12,99<ref name=RECONS />
| 15,85<ref name=RECONS />
|
|-
| 8
Line 196 ⟶ 195:
| colspan="2" | Ross&nbsp;154 (V1216&nbsp;Sagittarii)
| 13
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M3.5Ve]]
| 10,43<ref name=RECONS />
| 13,07<ref name=RECONS />
Line 209 ⟶ 208:
| colspan="2" | Ross&nbsp;248 (HH&nbsp;Andromedae)
| 14
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M5.5Ve]]
| 12,29<ref name=RECONS />
| 14,79<ref name=RECONS />
Line 220 ⟶ 219:
| 10
| 10,521
| style="background: #D99058C3B091" colspan="2" | WISE 1506+7027
| 15
| style="background: #FFB6C1;" | [[Bruin dwerg|T6]]
| 14,3 J
|
Line 235 ⟶ 234:
| colspan="2" | Epsilon&nbsp;Eridani (BD−09°697)
| 16
| style="background: #ffd2a1;" | [[Sterreklassifikasie#Spektraaltipes|K2V]]<ref name=RECONS />
| style="background: lightblue;" | 3,73<ref name=RECONS />
| 6,19<ref name=RECONS />
Line 248 ⟶ 247:
| colspan="2" | Lacaille&nbsp;9352 (CD−36°15693)
| 17
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M1.5Ve]]
| 7,34<ref name=RECONS />
| 9,75<ref name=RECONS />
Line 261 ⟶ 260:
| colspan="2" | Ross&nbsp;128 (FI&nbsp;Virginis)
| 18
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M4.0Vn]]
| 11,13<ref name=RECONS />
| 13,51<ref name=RECONS />
Line 272 ⟶ 271:
| 14
| 11,208
| style="background: #D99058C3B091" colspan="2" | WISE 0350-5658
| 19
| style="background: #CC99CC;" | [[Bruin dwerg|Y1]]
| >22,8 J
|
Line 288 ⟶ 287:
| EZ&nbsp;Aquarii&nbsp;A
| 20
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M5.0Ve]]
| 13,33<ref name=RECONS />
| 15,64<ref name=RECONS />
Line 299 ⟶ 298:
| EZ&nbsp;Aquarii&nbsp;B
| 20
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M]]?
| 13,27<ref name=RECONS />
| 15,58<ref name=RECONS />
Line 306 ⟶ 305:
| EZ&nbsp;Aquarii&nbsp;C
| 20
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M]]?
| 14,03<ref name=RECONS />
| 16,34<ref name=RECONS />
Line 316 ⟶ 315:
| Procyon&nbsp;A
|23
| style="background: #f8f7ff" | [[Sterreklassifikasie#Spektraaltipes|F5V–IV]]<ref name=RECONS />
| style="background: lightblue;" | 0,38<ref name=RECONS />
| 2,66<ref name=RECONS />
Line 327 ⟶ 326:
| Procyon&nbsp;B
| 23
| style="background: #f8f7ff" | [[Wit dwerg|DQZ]]<ref name=RECONS />
| 10,70<ref name=RECONS />
| 12,98<ref name=RECONS />
Line 337 ⟶ 336:
| 61&nbsp;Cygni&nbsp;A (BD+38°4343)
|25
| style="background: #ffd2a1;" | [[Sterreklassifikasie#Spektraaltipes|K5.0V]]<ref name=RECONS /> <!--previous: K3.5Ve-->
| style="background: lightblue;" | 5,21<ref name=RECONS />
| 7,49<ref name=RECONS />
Line 348 ⟶ 347:
| 61&nbsp;Cygni&nbsp;B (BD+38°4344)
|25
| style="background: #ffd2a1;" | [[Sterreklassifikasie#Spektraaltipes|K7.0V]]<ref name=RECONS /> <!--previous: K4.7Ve-->
| style="background: lightblue;" | 6,03<ref name=RECONS />
| 8,31<ref name=RECONS />
Line 360 ⟶ 359:
| Struve&nbsp;2398&nbsp;A (HD&nbsp;173739)
| 27
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M3.0V]]<ref name=RECONS />
| 8,90<ref name=RECONS />
| 11,16<ref name=RECONS />
Line 371 ⟶ 370:
| Struve&nbsp;2398&nbsp;B (HD&nbsp;173740)
| 27
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M3.5V]]<ref name=RECONS />
| 9,69<ref name=RECONS />
| 11,95<ref name=RECONS />
Line 383 ⟶ 382:
| Groombridge&nbsp;34&nbsp;A (GX&nbsp;Andromedae)
| 29
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M1.5V]]<ref name=RECONS /> <!--previous: M3.0V-->
| 8,08<ref name=RECONS />
| 10,32<ref name=RECONS />
Line 394 ⟶ 393:
| Groombridge&nbsp;34&nbsp;B (GQ&nbsp;Andromedae)
| 29
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M3.5V]]<ref name=RECONS />
| 11,06<ref name=RECONS />
| 13,30<ref name=RECONS />
Line 413 ⟶ 412:
| rowspan="3" |
|-
| style="background: #D99058C3B091"| Epsilon&nbsp;Indi&nbsp;Ba
| 31
| style="background: #FFB6C1;" | [[Bruin dwerg|T1.0V]]
| 12,3 J<ref name="DwarfArchives">{{cite web
|title=DwarfArchives.org: Photometry, spectroscopy, and astrometry of M, L, and T dwarfs
Line 427 ⟶ 426:
| January 2003
|-
| style="background: #D99058C3B091"| Epsilon&nbsp;Indi&nbsp;Bb
| 31
| style="background: #FFB6C1;" | [[Bruin dwerg|T6.0V]]
| 13,2 J<ref name="DwarfArchives"/>
|
Line 438 ⟶ 437:
| colspan="2" | DX&nbsp;Cancri (G&nbsp;51-15)
| 34
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M6.5Ve]]
| 14,78<ref name=RECONS />
| 16,98<ref name=RECONS />
Line 451 ⟶ 450:
| colspan="2" | Tau&nbsp;Ceti (BD−16°295)
| 35
| style="background: #fff4ea;" | [[Sterreklassifikasie#Spektraaltipes|G8Vp]]<ref name=RECONS />
|style="background: lightblue;" | 3,49<ref name=RECONS />
| 5,68<ref name=RECONS />
Line 464 ⟶ 463:
| colspan="2" | GJ 1061 (LHS&nbsp;1565)
| 36
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M5.5V]]<ref name=RECONS />
| 13,09<ref name=RECONS />
| 15,26<ref name=RECONS />
Line 477 ⟶ 476:
| colspan="2" | YZ&nbsp;Ceti (LHS&nbsp;138)
| 37
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M4.5V]]<ref name=RECONS />
| 12,02<ref name=RECONS />
| 14,17<ref name=RECONS />
Line 490 ⟶ 489:
| colspan="2" | Luyten se Ster (BD+05°1668)
| 38
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M3.5Vn]]
| 9,86<ref name=RECONS />
| 11,97<ref name=RECONS />
Line 501 ⟶ 500:
| 26
| 12,514(129)
| style="background: #D99058C3B091" colspan="2" | Teegarden se Ster (SO025300.5+165258)
| 39
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M6.5V]]
| 15,14<ref name=RECONS />
| 17,22<ref name=RECONS />
Line 517 ⟶ 516:
| SCR&nbsp;1845-6357&nbsp;A
| 40
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M8.5V]]<ref name=RECONS />
| 17,39
| 19,41
Line 526 ⟶ 525:
| rowspan=2 | <ref name=henry2006 />
|-
| style="background: #D99058C3B091"| SCR&nbsp;1845-6357&nbsp;B
| 40
| style="background: #FFB6C1;" | [[Bruin dwerg|T6]]<ref name=nearmt>[http://adsabs.harvard.edu/abs/2007A%26A...471..655K 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&ndash;659. {{doi|10.1051/0004-6361:20077881}}</ref>
| 13.3 J<ref name="DwarfArchives"/>
|
Line 539 ⟶ 538:
| colspan="2" | Kapteyn se Ster (CD−45°1841)
| 42
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M1.5V]]<ref name=RECONS /> <!--previous: sdM0VI-->
| 8,84<ref name=RECONS />
| 10,87<ref name=RECONS />
Line 552 ⟶ 551:
| colspan="2" | Lacaille&nbsp;8760 (AX&nbsp;Microscopii)
| 43
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M0.0V]]<ref name=RECONS /> <!--previous: M2Ve-->
| 6,67<ref name=RECONS />
| 8,69<ref name=RECONS />
Line 566 ⟶ 565:
| Kruger&nbsp;60&nbsp;A
| 45
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M3.0V]]<ref name=RECONS />
| 9,79<ref name=RECONS />
| 11,76<ref name=RECONS />
Line 577 ⟶ 576:
| Kruger&nbsp;60&nbsp;B (DO&nbsp;Cephei)
| 45
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M4.0V]]<ref name=RECONS />
| 11,41<ref name=RECONS />
| 13,38<ref name=RECONS />
Line 584 ⟶ 583:
| 32
| 13,167(82)
| style="background: #D99058C3B091" colspan="2" | DEN&nbsp;1048-3956
| 47
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M8.5V]]<ref name=RECONS />
| 17,39<ref name=RECONS />
| 19,37<ref name=RECONS />
Line 597 ⟶ 596:
| 33
| 13,259
| style="background: #D99058C3B091" colspan="2" | UGPS 0722-05
| 48
| style="background: #FFB6C1;" | [[Bruin dwerg|T9]]<ref name=RECONS /> <!--previous: M2Ve-->
| 16,52 J
|
Line 613 ⟶ 612:
| Ross&nbsp;614A (LHS&nbsp;1849)
| 49
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M4.5V]]<ref name=RECONS/>
| 11,15<ref name=RECONS />
| 13,09<ref name=RECONS />
Line 624 ⟶ 623:
| Ross&nbsp;614B (LHS&nbsp;1850)
| 49
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M5.5V]]
| 14,23<ref name=RECONS />
| 16,17<ref name=RECONS />
Line 633 ⟶ 632:
| colspan="2" | Wolf&nbsp;1061 (Gliese 628, BD−12°4523)
| 51
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M3.0V]]<ref name=RECONS />
| 10,07<ref name=RECONS />
| 11,93<ref name=RECONS />
Line 644 ⟶ 643:
| 36
| 13,998
| style="background: #D99058C3B091" colspan="2" | WISE 0410+1502
| 52
| style="background: #CC99CC;" | [[Bruin dwerg|Y0]]
| 19,3 J
|
Line 659 ⟶ 658:
| colspan="2" | [[Van Maanen se Ster]] (Gliese 35, LHS&nbsp;7)
| 53
| style="background: #f8f7ff" | [[Wit dwerg|DZ7]]<ref name=RECONS />
| 12,38<ref name=RECONS />
| 14,21<ref name=RECONS />
Line 672 ⟶ 671:
| colspan="2" | Gliese&nbsp;1 (CD−37°15492)
| 54
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M3.0V]]<ref name=RECONS />
| 8,55<ref name=RECONS />
| 10,35<ref name=RECONS />
Line 686 ⟶ 685:
| Wolf&nbsp;424&nbsp;A
| 55
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M5.5Ve]]
| 13,18<ref name=RECONS />
| 14,97<ref name=RECONS />
Line 697 ⟶ 696:
| Wolf&nbsp;424&nbsp;B
| 55
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M7Ve]]
| 13,17<ref name=RECONS />
| 14,96<ref name=RECONS />
Line 706 ⟶ 705:
| colspan="2" | TZ&nbsp;Arietis (Gliese 83.1, Luyten&nbsp;1159-16)
| 57
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M4.5V]]<ref name=RECONS />
| 12,27<ref name=RECONS />
| 14,03<ref name=RECONS />
Line 719 ⟶ 718:
| colspan="2" | Gliese&nbsp;687 (LHS&nbsp;450, BD+68°946)
| 58
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M3.0V]]<ref name=RECONS />
| 9,17<ref name=RECONS />
| 10,89<ref name=RECONS />
Line 732 ⟶ 731:
| colspan="2" | LHS&nbsp;292 (LP&nbsp;731-58)
| 59
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M6.5V]]<ref name=RECONS />
| 15,60<ref name=RECONS />
| 17,32<ref name=RECONS />
Line 745 ⟶ 744:
| colspan="2" | Gliese&nbsp;674 (LHS&nbsp;449)
| 60
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M3.0V]]<ref name=RECONS />
| 9,38<ref name=RECONS />
| 11,09<ref name=RECONS />
Line 759 ⟶ 758:
| GJ&nbsp;1245&nbsp;A
| 61
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M5.5V]]<ref name=RECONS />
| 13,46<ref name=RECONS />
| 15,17<ref name=RECONS />
Line 770 ⟶ 769:
| GJ&nbsp;1245&nbsp;B
| 61
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M6.0V]]<ref name=RECONS />
| 14,01<ref name=RECONS />
| 15,72<ref name=RECONS />
Line 779 ⟶ 778:
| GJ&nbsp;1245&nbsp;C
| 61
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M5.5]]
| 16,75<ref name=RECONS />
| 18,46<ref name=RECONS />
Line 790 ⟶ 789:
| colspan="2" | Gliese&nbsp;440 (WD&nbsp;1142-645)
| 64
| style="background: #f8f7ff" | [[Wit dwerg|DQ6]]<ref name=RECONS />
| 11,50<ref name=RECONS />
| 13,18<ref name=RECONS />
Line 803 ⟶ 802:
| colspan="2" | GJ&nbsp;1002
| 65
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M5.5V]]<ref name=RECONS />
| 13,76<ref name=RECONS />
| 15,40<ref name=RECONS />
Line 816 ⟶ 815:
| colspan="2" | [[Gliese 876]] (Ross&nbsp;780)
| 66
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M3.5V]]<ref name=RECONS />
| 10,17<ref name=RECONS />
| 11,81<ref name=RECONS />
Line 829 ⟶ 828:
| colspan="2" | LHS&nbsp;288 (Luyten&nbsp;143-23)
| 67
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M5.5V]]<ref name=RECONS />
| 13,90<ref name=RECONS />
| 15,51<ref name=RECONS />
Line 840 ⟶ 839:
| 49
| 15,757
| style="background: #D99058C3B091" colspan="2" | WISE 1405+5534
| 68
| style="background: #CC99CC;" | [[Bruin dwerg|Y0p]]
| 20,09 J
|
Line 856 ⟶ 855:
| Gliese 412&nbsp;A
| 69
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M1.0V]]<ref name=RECONS />
| 8,77<ref name=RECONS />
| 10,34<ref name=RECONS />
Line 867 ⟶ 866:
| Gliese 412&nbsp;B (WX&nbsp;Ursae&nbsp;Majoris)
| 69
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M5.5V]]<ref name=RECONS />
| 14,48<ref name=RECONS />
| 16,05<ref name=RECONS />
Line 878 ⟶ 877:
| colspan="2" | Groombridge&nbsp;1618 (Gliese 380)
| 71
| style="background: #ffd2a1;" | [[Sterreklassifikasie#Spektraaltipes|K7.0V]]<ref name=RECONS />
| 6,59<ref name=RECONS />
| 8,16<ref name=RECONS />
Line 891 ⟶ 890:
| colspan="2" | AD&nbsp;Leonis
| 72
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M3.0V]]<ref name=RECONS />
| 9,32<ref name=RECONS />
| 10,87<ref name=RECONS />
Line 902 ⟶ 901:
| 53
| 16,067
| style="background: #D99058C3B091" colspan="2" | DENIS J081730.0-615520
| 73
| style="background: #FFB6C1;" | [[Bruin dwerg|T6]]
Line 917 ⟶ 916:
| colspan="2" | Gliese 832
| 74
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M3.0V]]<ref name=RECONS />
| 8,66<ref name=RECONS />
| 10,20<ref name=RECONS />
Line 928 ⟶ 927:
| 55
| 16,195(338)
| style="background: #D99058C3B091" colspan="2" | LP&nbsp;944-020
| 75
| style="background: #ffcc6f;" | [[Sterreklassifikasie#Spektraaltipes|M9.0V]]<ref name=RECONS />
| 18,50<ref name=RECONS />
| 20,02<ref name=RECONS />
Line 941 ⟶ 940:
| 56
| 16,197(313)
| style="background: #D99058C3B091" colspan="2" | DEN&nbsp;0255-4700
| 76
| style="background: #E6B2B2;" | [[Bruin dwerg|L7.5V]]<ref name=RECONS />
Ontsluit van "https://af.wikipedia.org/wiki/Lys_van_naaste_sterre"