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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
- 394 bytes (68 words) - 05:35, 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) - 13:23, 9 March 2008
- #Redirect [[Nova (astronomy)#Supernova]]40 bytes (4 words) - 11:41, 2 November 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
- ...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
- * [[Supernova]]e are exhibiting similar brightness increases but are much brighter. They688 bytes (92 words) - 05:21, 19 July 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 (1,076 words) - 09:16, 6 March 2024
- 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
- ===Time dilation in supernova light curves===17 KB (2,731 words) - 19:52, 26 October 2020
- ...ynthesis before being ejected into interstellar space by stellar winds and supernova explosions.7 KB (987 words) - 10:12, 30 May 2009
- ...ease in astronomical and astrological work and publications. Tycho Brahe's supernova was significant because it encouraged astronomers in the 16th-century to qu23 KB (3,546 words) - 19:39, 25 September 2020
- ...steadily enriched by heavier elements. These are introduced as a result of supernova explosions, stellar winds and the expulsion of the outer envelope of evolve8 KB (1,199 words) - 20:34, 8 June 2010
- ...to explain accelerating cosmological expansion.<ref>[http://snap.lbl.gov/ SuperNova Acceleration Probe] Lawrence Berkeley National Lab</ref>18 KB (2,817 words) - 20:15, 27 October 2020
- Not counting the occasional [[supernova]], the first variable star to be identified was Mira or ''ο Ceti'' which w {{main|supernova}}18 KB (2,830 words) - 10:19, 9 June 2008
- ...result of collapsing matter following the explosion of large stars into [[supernova|supernovae]]. Therefore, the mass of a black hole is often depicted in term9 KB (1,324 words) - 08:30, 31 July 2023