Wysiging soos op 10:40, 9 Maart 2013 wysig Addbot (besprekings \| bydraes) 27 847 edits k Verplasing van 59 interwikiskakels wat op Wikidata beskikbaar is op d:q10934 ← Ouer wysiging		Wysiging soos op 17:06, 8 April 2013 wysig maak ongedaan BurgertB (besprekings \| bydraes) Administrateurs 65 312 edits kassie Nuwer wysiging →
Lyn 1: {{Inligtingskas newel ~~{{Inligtingskas2~~ \|~~naam~~ naam= Krap-newel \|~~beeld~~ beeld= Crab Nebula.jpg▼ ~~\|kleur = #CEDAF2~~ \|~~beeld_onderskrif~~ onderskrif= M1, die Krap-newel▼ ▲\|beeld = Crab Nebula.jpg \|1 soort= [[~~Newel#Soorte newels~~Supernova\|Supernova-oorblyfsel]] ▼ ~~\|beeld_wydte = 250px~~ \|2 sterrebeeld= [[Bul (sterrebeeld)\|Bul]]▼ ▲\|beeld_onderskrif = M1, die Krap-newel \| messier= Messier 1 ~~\|beeld2 =~~ \| tipe= ~~\|beeld2_wydte =~~ \|3 RK= 05<sup>h</sup> 34<sup>m</sup>31,94<sup>s</sup>▼ ~~\|beeld2_onderskrif =~~ \|4 Dek= +22º 00' 52,2"▼ ~~\|opskrif1 = Soort~~ \| magnitude= ▲\|1 = [[Newel#Soorte newels\|Supernova-oorblyfsel]] \| skynmagnitude= 8,4 ~~\|opskrif2 = Sterrebeeld~~ \| absolute magnitude= −3,1 ▲\|2 = [[Bul (sterrebeeld)\|Bul]] \| afstand= 6 500 ~~\|opskrif3 = Regte klimming~~ \| ouderdom= ▲\|3 = 05<sup>h</sup> 34<sup>m</sup>31,94<sup>s</sup> \|7 grootte= 420" × 290"▼ ~~\|opskrif4 = Deklinasie~~ \| sterre= ▲\|4 = +22º 00' 52,2" \| rooiverskuiwing= ~~\|opskrif5 = Afstand~~ \| kenmerke= Optiese [[pulsar]] ~~\|5 = 6,5 ± 1,6 [[ligjare\|kilo-ligjare]] (2,0 ± 0,5 [[parsek\|kilo-parsek]])<ref name="Kaplanetal2008">~~ \| massa= ~~{{cite journal~~ \|9 name= ~~Messier 1, M1,~~ NGC 1952, Sharpless 244▼ ~~\| last1 = Kaplan \| first1 = D. L.~~ \| koo= {{Lug2\|5\|34\|31.97\|+\|22\|00\|52.1\|6500}} ~~\| last2 = Chatterjee \| first2 = S.~~ }} ▼ ~~\| last3 = Gaensler \| first3 = B. M.~~ ~~\| last4 = Anderson \| first4 = J.~~ ~~\| year = 2008~~ ~~\| title = A Precise Proper Motion for the Crab Pulsar, and the Difficulty of Testing Spin-Kick Alignment for Young Neutron Stars~~ ~~\| journal = Astrophysical Journal~~ ~~\| volume = 677~~ ~~\| issue = 2 \| page = 1201~~ ~~\| arxiv = 0801.1142~~ ~~\| doi = 10.1086/529026 \| bibcode=2008ApJ...677.1201K~~ ~~}}</ref>~~ ~~\|opskrif6 = Oënskynlike magnitude~~ ~~\|6 = +8,4 [[Magnitude\|mag]]~~ ~~\|opskrif7 = Oënskynlike grootte~~ ▲\|7 = 420" × 290" ~~\|opskrif8 = Radius~~ ~~\|8 = 5,5 ligjare (1,7 parsek)~~ ~~\|opskrif9 = Ander name~~ ▲\|9 = Messier 1, M1, NGC 1952, Sharpless 244 ~~\|opskrif10 =~~ ~~\|10 =~~ ~~\|opskrif11 =~~ ~~\|11 =~~ ~~\|opskrif12 =~~ ~~\|12 =~~ ~~\|opskrif13 =~~ ~~\|13 =~~ ~~\|opskrif14 =~~ ~~\|14 =~~ ~~\|opskrif15 =~~ ~~\|15 =~~ ~~\|opskrif16 =~~ ~~\|16 =~~ ~~\|opskrif17 =~~ ~~\|17 =~~ ~~\|opskrif18 =~~ ~~\|18 =~~ ~~\|opskrif19 =~~ ~~\|19 =~~ ~~\|opskrif20 =~~ ~~\|20 =~~ ▲}} Die '''Krap-newel''' (ook bekend as '''Messier 1''' of '''NGC 1952''') is ’n [[Newel#Soorte newels\|Supernova-oorblyfsel]] en [[pulsar]]wind-[[newel]] in die [[sterrebeeld]] [[Bul (sterrebeeld)\|Bul]]. Dit is in 1731 deur [[John Bevis]] waargeneem; dit stem ooreen met die helder [[supernova]] [[SN 1054]] wat in 1054 gesien is deur Arabiese, Sjinese en Japannese sterrekundiges.

Krap-newel: Verskil tussen weergawes