Editing Talk:1123: The Universal Label
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::Actually, the amount of energy in any grocery or non-grocery (even in explosives) is significally lower that the amount of energy in hydrogen used for their creation. Sure, you need energy to grow crops, but where does that energy come from? Hydrogen fusion in Sun - which is first step of creating the carbon the crop is from (not the same crop, of course). -- [[User:Hkmaly|Hkmaly]] ([[User talk:Hkmaly|talk]]) 09:12, 19 October 2012 (UTC) | ::Actually, the amount of energy in any grocery or non-grocery (even in explosives) is significally lower that the amount of energy in hydrogen used for their creation. Sure, you need energy to grow crops, but where does that energy come from? Hydrogen fusion in Sun - which is first step of creating the carbon the crop is from (not the same crop, of course). -- [[User:Hkmaly|Hkmaly]] ([[User talk:Hkmaly|talk]]) 09:12, 19 October 2012 (UTC) | ||
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So when [http://xkcd.com/282/ Mussolini made the trains run on thyme] he was really making them run on hydrogen '''and''' time?--[[User:Pmakholm|Pmakholm]] ([[User talk:Pmakholm|talk]]) 08:18, 19 October 2012 (UTC) | So when [http://xkcd.com/282/ Mussolini made the trains run on thyme] he was really making them run on hydrogen '''and''' time?--[[User:Pmakholm|Pmakholm]] ([[User talk:Pmakholm|talk]]) 08:18, 19 October 2012 (UTC) | ||
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[http://en.wikipedia.org/wiki/P-process] | [http://en.wikipedia.org/wiki/P-process] | ||
:The fusion of heavier elements is still fusion, even if it takes a supernova to make it happen. Nothing in the cartoon suggests that only the fusion reactions found in stable stars apply, and even more complicated processes (fusion+fission, whatever) involves matter that ultimately has a hydrogen pedigree. (I am, however, intrigued by the comment about helium and lithium in the early universe. I have some of those around here somewhere.) [[Special:Contributions/208.54.40.210|208.54.40.210]] 21:02, 19 October 2012 (UTC) | :The fusion of heavier elements is still fusion, even if it takes a supernova to make it happen. Nothing in the cartoon suggests that only the fusion reactions found in stable stars apply, and even more complicated processes (fusion+fission, whatever) involves matter that ultimately has a hydrogen pedigree. (I am, however, intrigued by the comment about helium and lithium in the early universe. I have some of those around here somewhere.) [[Special:Contributions/208.54.40.210|208.54.40.210]] 21:02, 19 October 2012 (UTC) | ||
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Another pun? | Another pun? | ||
--[[Special:Contributions/178.26.107.37|178.26.107.37]] 23:08, 19 October 2012 (UTC) | --[[Special:Contributions/178.26.107.37|178.26.107.37]] 23:08, 19 October 2012 (UTC) | ||
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