Talk:Supergiant: Difference between revisions
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Closing requested move; moved using rmCloser |
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{{Vital article|level=4|topic=Science|class=C|subpage=Physics}} |
{{Vital article|level=4|topic=Science|class=C|subpage=Physics}} |
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{{WikiProject Astronomy|class=C|importance=Top}} |
{{WikiProject Astronomy|class=C|importance=Top}} |
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{{old move|date=29 July 2021|from=Supergiant star|destination=Supergiant|result=moved|link=Special:Permalink/1036151798#Requested move 29 July 2021}} |
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== Images, anyone? == |
== Images, anyone? == |
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== Requested move 29 July 2021 == |
== Requested move 29 July 2021 == |
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<div class="boilerplate" style="background-color: #efe; margin: 0; padding: 0 10px 0 10px; border: 1px dotted #aaa;"><!-- Template:RM top --> |
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{{requested move/dated|multiple=yes |
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:''The following is a closed discussion of a [[Wikipedia:Requested moves|requested move]]. <span style="color:red">'''Please do not modify it.'''</span> Subsequent comments should be made in a new section on the talk page. Editors desiring to contest the closing decision should consider a [[Wikipedia:move review|move review]] after discussing it on the closer's talk page. No further edits should be made to this discussion. '' |
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|current1=Supergiant star|new1=Supergiant|current2=Blue supergiant star|new2=Blue supergiant|current3=Yellow supergiant star|new3=Yellow supergiant|current4=Red supergiant star|new4=Red supergiant|}} |
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The result of the move request was: '''moved.''' <small>([[Wikipedia:Requested moves/Closing instructions#Closure by a page mover|closed by non-admin page mover]])</small> [[User:Lennart97|Lennart97]] ([[User talk:Lennart97|talk]]) 09:47, 5 August 2021 (UTC) |
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* [[:Supergiant star]] → {{no redirect|Supergiant}} |
* [[:Supergiant star]] → {{no redirect|Supergiant}} |
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*'''Support''' per nom. '''[[User:Lugnuts|<font color="002bb8">Lugnuts</font>]]''' <sup>[[User talk:Lugnuts|Fire Walk with Me]]</sup> 06:38, 29 July 2021 (UTC) |
*'''Support''' per nom. '''[[User:Lugnuts|<font color="002bb8">Lugnuts</font>]]''' <sup>[[User talk:Lugnuts|Fire Walk with Me]]</sup> 06:38, 29 July 2021 (UTC) |
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*'''Support''', brevity and common name. [[User:Randy Kryn|Randy Kryn]] ([[User talk:Randy Kryn|talk]]) 11:13, 29 July 2021 (UTC) |
*'''Support''', brevity and common name. [[User:Randy Kryn|Randy Kryn]] ([[User talk:Randy Kryn|talk]]) 11:13, 29 July 2021 (UTC) |
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<div style="padding-left: 1.6em; font-style: italic; border-top: 1px solid #a2a9b1; margin: 0.5em 0; padding-top: 0.5em">The discussion above is closed. <b style="color: #FF0000;">Please do not modify it.</b> Subsequent comments should be made on the appropriate discussion page. No further edits should be made to this discussion.</div><!-- from [[Template:Archive bottom]] --> |
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Revision as of 09:47, 5 August 2021
Astronomy C‑class Top‑importance | ||||||||||
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On 29 July 2021, it was proposed that this article be moved from Supergiant star to Supergiant. The result of the discussion was moved. |
Images, anyone?
Does anyone have an image of a supergiant?
How are Supergiants formed?
It doesn't say how supergiants formed.
pretty much like any other star, but with...more gas available. — Preceding unsigned comment added by 24.18.8.160 (talk) 06:19, 24 January 2013 (UTC)
- This reply really misses the point. Supergiants are indeed more massive than most stars, but there are equally (and more!) massive stars which are not supergiants. The article fails to really express why, how, or when supergiants form, or really to give a meaningful summary of where supergiants fit into the grand scheme of things. The stellar evolution article does explain this, but if that is to be the excuse for lack of information here, then people need to be very clearly directed to where they can find the information. Lithopsian (talk) 12:15, 24 January 2013 (UTC)
What is the energy source of a supergiant?
It doesn't say.
Is it helium fusion? If so, is it via the triple-alpha process? SolomonFreer 04:51, 3 November 2007 (UTC)
supergiants can burn pretty much anything. Hydrogen, helium, carbon, even iron(?)...I'd add it to the article itself, but I don't have a good reference to use. — Preceding unsigned comment added by 24.18.8.160 (talk) 06:20, 24 January 2013 (UTC)
- Again, the response fails to understand or answer the question. Supergiants can't burn "anything". They form very specifically because a star has started to burn elements heavier than hydrogen. They *might* still be burning hydrogen in a shell outside the core, but most certainly they are burning something else in the core. In almost all cases this is helium (although note that burning helium in the core isn't sufficient to create a supergiant), but in the most massive stars it can be heavier elements for a brief period. Again, the stellar evolution article explains this reasonably well. The supernova article also describes some of the later stages in the life of a massive star. Lithopsian (talk) 12:20, 24 January 2013 (UTC)
Core Helium
Shouldn't it be a "Helium core" instead of "core helium?
21:07, 4 February 2017 (UTC)
Good pick-up. Fixed. Arianewiki1 (talk) 05:54, 4 June 2017 (UTC)
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Requested move 29 July 2021
- The following is a closed discussion of a requested move. Please do not modify it. Subsequent comments should be made in a new section on the talk page. Editors desiring to contest the closing decision should consider a move review after discussing it on the closer's talk page. No further edits should be made to this discussion.
The result of the move request was: moved. (closed by non-admin page mover) Lennart97 (talk) 09:47, 5 August 2021 (UTC)
- Supergiant star → Supergiant
- Blue supergiant star → Blue supergiant
- Yellow supergiant star → Yellow supergiant
- Red supergiant star → Red supergiant
– "Supergiant star" is superfluous, and is more frequently known as just "supergiant" (Google Ngrams for plural). –LaundryPizza03 (dc̄) 03:07, 29 July 2021 (UTC)
- @Bear-rings: renamed these article in 2017. I wasn't keen on the idea at the time. Lithopsian (talk) 20:21, 29 July 2021 (UTC)
- Support per nom. Lugnuts Fire Walk with Me 06:38, 29 July 2021 (UTC)
- Support, brevity and common name. Randy Kryn (talk) 11:13, 29 July 2021 (UTC)