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- ...also causes the outer parts of the star to explode violently, causing the supernova brightness rise. ===Core collapse supernova===4 KB (664 words) - 16:43, 28 November 2010
- 867 bytes (132 words) - 15:04, 19 July 2010
- 394 bytes (68 words) - 05:35, 19 July 2010
- | pagename = Supernova | abc = Supernova2 KB (324 words) - 05:32, 19 July 2010
- {{r|Supernova type I}} {{r|Supernova type II}}982 bytes (156 words) - 06:05, 19 July 2010
Page text matches
- ...va Story'' (Plenum Press, New York, 1988) - Although focused on the famous supernova 1987A and other supernovae, this lucid popular science volume also has some281 bytes (37 words) - 09:57, 9 March 2008
- #Redirect [[Nova (astronomy)#Supernova]]40 bytes (4 words) - 11:41, 2 November 2008
- #Redirect [[Nova (astronomy)#Supernova]]40 bytes (4 words) - 13:23, 9 March 2008
- the remnant of a [[star]] that had sufficient mass to explode in a supernova, but not so much mass that it forms a [[black hole]] instead of a neutron s192 bytes (33 words) - 15:40, 25 January 2023
- {{r|Supernova type I}} {{r|Supernova type II}}982 bytes (156 words) - 06:05, 19 July 2010
- ...also causes the outer parts of the star to explode violently, causing the supernova brightness rise. ===Core collapse supernova===4 KB (664 words) - 16:43, 28 November 2010
- I'm not sure about redirecting [[supernova]] here. Isn't there enough distinct information about this particular type ...these type of redirect with time. Note that in Related Atricles subpages supernova can exist with its own unique definition and it will be identified as a red3 KB (534 words) - 03:51, 19 July 2010
- <code><nowiki>{{pl|Supernova}}</nowiki></code> produces: {{pl|Supernova}}2 KB (266 words) - 15:36, 24 January 2011
- ...star is the remnant of a [[star]] that had sufficient mass to explode in a supernova, but not so much mass that it forms a [[black hole]] instead of a neutron s415 bytes (69 words) - 15:39, 25 January 2023
- ...magnitudes. They are currently regarded as a separate kind of objects. The supernova explosions are caused by the collapse of a white dwarf or a degenerate star {{main|Supernova}}6 KB (1,048 words) - 17:23, 26 July 2010
- | pagename = Supernova | abc = Supernova2 KB (324 words) - 05:32, 19 July 2010
- * [[Supernova]]e are exhibiting similar brightness increases but are much brighter. They688 bytes (92 words) - 05:21, 19 July 2010
- {{r|Supernova}}678 bytes (86 words) - 07:00, 30 August 2024
- ...va article is a redirect as follows ''<nowiki>#Redirect [[Nova (astronomy)#Supernova]]</nowiki>'': ::2) and a definition does exist at [[Supernova/Definition]].12 KB (1,720 words) - 13:43, 12 March 2010
- ...IUE, including [[planet]]s, [[comet]]s, [[star]]s, [[interstellar gas]], [[supernova]]e, [[Aurora|planetary aurorae]], [[Galaxy|galaxies]], and [[quasar]]s. ...t identification of the progenitor of any supernova in history ([[SN 1987A|Supernova 1987A]])7 KB (1,080 words) - 07:01, 2 September 2024
- * [[Supernova]], <s>now a redirect to be remade and populated</s>, now a new article, nee3 KB (374 words) - 04:49, 22 November 2023
- == kepplers supernova ==10 KB (1,596 words) - 16:10, 18 January 2010
- There have not been any recorded observations of [[supernova]]e in NGC 221. In 1998 a [[nova]] was recorded about 53ˡˡ south and west3 KB (484 words) - 13:33, 29 October 2011
- |Supernova (final stage) |Type II Supernova15 KB (2,142 words) - 21:59, 7 November 2008
- ===Supernova of 1572=== ..." star (we now know that [[SN 1572|Tycho's star in Cassiopeia]] was a [[supernova]] 7500 light years from earth). This discovery was decisive for his choice23 KB (3,568 words) - 10:30, 2 April 2024