Search results
Jump to navigation
Jump to search
Page title matches
- ...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) - 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
- ...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
- ...but uses the [[Supernova/Definition]]. The key is the redirect set up at [[Supernova]]. [[User:Chris Day|Chris Day]] 23:48, 1 November 2008 (UTC) ...The existence of the supernova definition is independent of whether or not supernova were a subhead (superhead?) of nova. <small>Howard C. Berkowitz 00:48, 2 N52 KB (8,701 words) - 18:02, 1 April 2024
- ...igh energy photons, from relatively normal stars to explosive phenomena ([[supernova|supernovae]], [[gamma ray burst|gamma ray bursts]]), to [[galaxy cluster|cl ...d; a second astronomical source whose neutrino emission was observed was [[supernova]] 1987A. Prospects for the observation of neutrinos from several kinds of a46 KB (6,796 words) - 10:08, 28 February 2024
- ...y rare occurrence.<ref>[http://chandra.harvard.edu/resources/illustrations/supernova.html Supernovas and remnants] Chandra X-ray Observatory</ref>14 KB (2,338 words) - 10:18, 23 November 2011
- ...ease in astronomical and astrological work and publications. Tycho Brahe's supernova was significant because it encouraged astronomers in the 16th-century to qu51 KB (8,075 words) - 05:28, 17 October 2013
- ...around a protogalaxy as it starts to contract. These huge stars quickly [[supernova]], releasing heavy elements into the [[interstellar medium]]. Within the ne17 KB (2,688 words) - 22:56, 16 January 2021
- ...samples of these are man-made and radioactive, though some are created in supernova explosions for very brief periods. Non-radioactive elements are stable, and39 KB (5,559 words) - 09:16, 6 March 2024
- ...Sun formed within a [[star cluster]], and in range of a number of nearby [[supernova]]e explosions. The shock wave from these supernovae may have triggered the ...and larger, comet-like bodies.<ref> {{cite web |year= 2005| author=|title= Supernova Explosion May Have Caused Mammoth Extinction| work=Physorg.com|url=http://w76 KB (11,605 words) - 21:48, 1 September 2020
- <blockquote>...heavier atomic nuclei, left from a supernova, are not at thermodynamic equilibrium. Decay of these nuclei is a powerful150 KB (22,449 words) - 05:42, 6 March 2024
- ...family: Gill Sans MT, Trebuchet MS;">...heavier atomic nuclei, left from a supernova, are not at thermodynamic equilibrium. Decay of these nuclei is a powerful194 KB (28,649 words) - 05:43, 6 March 2024