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	<id>https://energyeducation.ca/wiki/index.php?action=history&amp;feed=atom&amp;title=Mass-energy_equivalence</id>
	<title>Mass-energy equivalence - Revision history</title>
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	<updated>2026-04-03T20:32:07Z</updated>
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	<entry>
		<id>https://energyeducation.ca/wiki/index.php?title=Mass-energy_equivalence&amp;diff=5596&amp;oldid=prev</id>
		<title>Jmdonev: 1 revision imported</title>
		<link rel="alternate" type="text/html" href="https://energyeducation.ca/wiki/index.php?title=Mass-energy_equivalence&amp;diff=5596&amp;oldid=prev"/>
		<updated>2017-08-29T01:47:38Z</updated>

		<summary type="html">&lt;p&gt;1 revision imported&lt;/p&gt;
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				&lt;td colspan=&quot;1&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;1&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 01:47, 29 August 2017&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-notice&quot; lang=&quot;en&quot;&gt;&lt;div class=&quot;mw-diff-empty&quot;&gt;(No difference)&lt;/div&gt;
&lt;/td&gt;&lt;/tr&gt;&lt;/table&gt;</summary>
		<author><name>Jmdonev</name></author>
	</entry>
	<entry>
		<id>https://energyeducation.ca/wiki/index.php?title=Mass-energy_equivalence&amp;diff=5595&amp;oldid=prev</id>
		<title>Jmdonev at 06:57, 27 August 2017</title>
		<link rel="alternate" type="text/html" href="https://energyeducation.ca/wiki/index.php?title=Mass-energy_equivalence&amp;diff=5595&amp;oldid=prev"/>
		<updated>2017-08-27T06:57:30Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 06:57, 27 August 2017&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l1&quot;&gt;Line 1:&lt;/td&gt;
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&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[Category:Done &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;2015&lt;/del&gt;-07-&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;24&lt;/del&gt;]]  &lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[Category:Done &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;2017&lt;/ins&gt;-07-&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;01&lt;/ins&gt;]]  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[File:sunsun.jpg|300px|thumb|Figure 1. The sun produces its energy by the conversion of mass into energy through the process of nuclear [[fusion]].&amp;lt;ref&amp;gt;Wikimedia Commons [Online], Available: https://upload.wikimedia.org/wikipedia/commons/3/35/The_Sun_in_extreme_ultraviolet.jpg&amp;lt;/ref&amp;gt;]]&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[File:sunsun.jpg|300px|thumb|Figure 1. The sun produces its energy by the conversion of mass into energy through the process of nuclear [[fusion]].&amp;lt;ref&amp;gt;Wikimedia Commons [Online], Available: https://upload.wikimedia.org/wikipedia/commons/3/35/The_Sun_in_extreme_ultraviolet.jpg&amp;lt;/ref&amp;gt;]]&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;onlyinclude&amp;gt;&#039;&#039;&#039;Mass-energy equivalence&#039;&#039;&#039; is the famous concept in physics represented mathematically by &amp;lt;&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;m&lt;/del&gt;&amp;gt;E=mc^2&amp;lt;/&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;m&lt;/del&gt;&amp;gt;, which states that [[mass]] and [[energy]] are one and the same.&amp;lt;/onlyinclude&amp;gt;&amp;lt;ref name=Knight&amp;gt;R. D. Knight, &quot;Relativity&quot; in &#039;&#039;Physics for Scientists and Engineers: A Strategic Approach,&#039;&#039; 3nd ed. San Francisco, U.S.A.: Pearson Addison-Wesley, 2008, ch.37, sec. 10, pp.1172-1176 &amp;lt;/ref&amp;gt;&amp;lt;ref name=Hawkes&amp;gt;Hawkes et al, &quot;Deformation and Elasticity,&quot; in &#039;&#039;Physics for Scientists and Engineers,&#039;&#039; 1st ed. Toronto: Cengage, 2014, pp. 265-268.&amp;lt;/ref&amp;gt;  This idea was not actually put forth by Einstein, but he was the first to describe an accurate relationship for it in his theory of special relativity, where he first wrote down this famous equation. The &amp;lt;&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;m&lt;/del&gt;&amp;gt;c^2&amp;lt;/&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;m&lt;/del&gt;&amp;gt; term is a tremendously large quantity, so this means that a small amount of mass corresponds to a large amount of energy. This equation is only representative of an object at rest, so this energy is called the &quot;rest energy&quot; of an object. The full equation Einstein wrote down includes the energy of a moving object, but the simplified version is still profound.&amp;lt;ref name=Knight/&amp;gt;  &lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;onlyinclude&amp;gt;&#039;&#039;&#039;Mass-energy equivalence&#039;&#039;&#039; is the famous concept in physics represented mathematically by &amp;lt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;math&lt;/ins&gt;&amp;gt;E=mc^2&amp;lt;/&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;math&lt;/ins&gt;&amp;gt;, which states that [[mass]] and [[energy]] are one and the same.&amp;lt;/onlyinclude&amp;gt;&amp;lt;ref name=Knight&amp;gt;R. D. Knight, &quot;Relativity&quot; in &#039;&#039;Physics for Scientists and Engineers: A Strategic Approach,&#039;&#039; 3nd ed. San Francisco, U.S.A.: Pearson Addison-Wesley, 2008, ch.37, sec. 10, pp.1172-1176 &amp;lt;/ref&amp;gt;&amp;lt;ref name=Hawkes&amp;gt;Hawkes et al, &quot;Deformation and Elasticity,&quot; in &#039;&#039;Physics for Scientists and Engineers,&#039;&#039; 1st ed. Toronto: Cengage, 2014, pp. 265-268.&amp;lt;/ref&amp;gt;  This idea was not actually put forth by Einstein, but he was the first to describe an accurate relationship for it in his theory of special relativity, where he first wrote down this famous equation. The &amp;lt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;math&lt;/ins&gt;&amp;gt;c^2&amp;lt;/&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;math&lt;/ins&gt;&amp;gt; term is a tremendously large quantity, so this means that a small amount of mass corresponds to a large amount of energy. This equation is only representative of an object at rest, so this energy is called the &quot;rest energy&quot; of an object. The full equation Einstein wrote down includes the energy of a moving object, but the simplified version is still profound.&amp;lt;ref name=Knight/&amp;gt;  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The implications of such an idea are overwhelming. Mass can be created out of energy, it just takes a lot of energy to do this. In fact, the entire universe was born in the [[Big Bang]] when a whole lot of energy was turned into mass.  &lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The implications of such an idea are overwhelming. Mass can be created out of energy, it just takes a lot of energy to do this. In fact, the entire universe was born in the [[Big Bang]] when a whole lot of energy was turned into mass.  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Jmdonev</name></author>
	</entry>
	<entry>
		<id>https://energyeducation.ca/wiki/index.php?title=Mass-energy_equivalence&amp;diff=1132&amp;oldid=prev</id>
		<title>J.williams: 1 revision imported</title>
		<link rel="alternate" type="text/html" href="https://energyeducation.ca/wiki/index.php?title=Mass-energy_equivalence&amp;diff=1132&amp;oldid=prev"/>
		<updated>2015-08-26T21:31:20Z</updated>

		<summary type="html">&lt;p&gt;1 revision imported&lt;/p&gt;
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				&lt;td colspan=&quot;1&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 21:31, 26 August 2015&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-notice&quot; lang=&quot;en&quot;&gt;&lt;div class=&quot;mw-diff-empty&quot;&gt;(No difference)&lt;/div&gt;
&lt;/td&gt;&lt;/tr&gt;&lt;/table&gt;</summary>
		<author><name>J.williams</name></author>
	</entry>
	<entry>
		<id>https://energyeducation.ca/wiki/index.php?title=Mass-energy_equivalence&amp;diff=1131&amp;oldid=prev</id>
		<title>J.williams at 16:56, 12 August 2015</title>
		<link rel="alternate" type="text/html" href="https://energyeducation.ca/wiki/index.php?title=Mass-energy_equivalence&amp;diff=1131&amp;oldid=prev"/>
		<updated>2015-08-12T16:56:49Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;[[Category:Done 2015-07-24]] &lt;br /&gt;
[[File:sunsun.jpg|300px|thumb|Figure 1. The sun produces its energy by the conversion of mass into energy through the process of nuclear [[fusion]].&amp;lt;ref&amp;gt;Wikimedia Commons [Online], Available: https://upload.wikimedia.org/wikipedia/commons/3/35/The_Sun_in_extreme_ultraviolet.jpg&amp;lt;/ref&amp;gt;]]&lt;br /&gt;
&amp;lt;onlyinclude&amp;gt;&amp;#039;&amp;#039;&amp;#039;Mass-energy equivalence&amp;#039;&amp;#039;&amp;#039; is the famous concept in physics represented mathematically by &amp;lt;m&amp;gt;E=mc^2&amp;lt;/m&amp;gt;, which states that [[mass]] and [[energy]] are one and the same.&amp;lt;/onlyinclude&amp;gt;&amp;lt;ref name=Knight&amp;gt;R. D. Knight, &amp;quot;Relativity&amp;quot; in &amp;#039;&amp;#039;Physics for Scientists and Engineers: A Strategic Approach,&amp;#039;&amp;#039; 3nd ed. San Francisco, U.S.A.: Pearson Addison-Wesley, 2008, ch.37, sec. 10, pp.1172-1176 &amp;lt;/ref&amp;gt;&amp;lt;ref name=Hawkes&amp;gt;Hawkes et al, &amp;quot;Deformation and Elasticity,&amp;quot; in &amp;#039;&amp;#039;Physics for Scientists and Engineers,&amp;#039;&amp;#039; 1st ed. Toronto: Cengage, 2014, pp. 265-268.&amp;lt;/ref&amp;gt;  This idea was not actually put forth by Einstein, but he was the first to describe an accurate relationship for it in his theory of special relativity, where he first wrote down this famous equation. The &amp;lt;m&amp;gt;c^2&amp;lt;/m&amp;gt; term is a tremendously large quantity, so this means that a small amount of mass corresponds to a large amount of energy. This equation is only representative of an object at rest, so this energy is called the &amp;quot;rest energy&amp;quot; of an object. The full equation Einstein wrote down includes the energy of a moving object, but the simplified version is still profound.&amp;lt;ref name=Knight/&amp;gt; &lt;br /&gt;
&lt;br /&gt;
The implications of such an idea are overwhelming. Mass can be created out of energy, it just takes a lot of energy to do this. In fact, the entire universe was born in the [[Big Bang]] when a whole lot of energy was turned into mass. &lt;br /&gt;
&lt;br /&gt;
For example, burning a [[gallon]] of [[gasoline]] (3.78 [[liter]]s) releases about 132 million [[joule]]s of energy, which is enough energy to make 14 ng of mass. This is roughly the mass of a single particle of very finely ground flour. No scale in the world can detect a difference of 14 ng out of the 3 kg of mass of the gasoline.&amp;lt;ref name=Knight/&amp;gt; &lt;br /&gt;
&lt;br /&gt;
This naturally leads to the conclusion that &amp;#039;if the technology existed to just turn that gasoline into pure energy&amp;#039;, the world&amp;#039;s energy problems would go away. Unfortunately, this is forbidden by a deep physical law that says the total number of [[proton]]s and [[neutron]]s must remain the same. Protons can become neutrons, and neutrons can become protons (and both happen with [[beta decay]]). This law is known as baryon conservation and is discussed at [http://hyperphysics.phy-astr.gsu.edu/hbase/astro/wcbar.html hyperphysics] (both protons and neutrons are baryons).&lt;br /&gt;
&lt;br /&gt;
In the gasoline case, a gallon of gasoline weighs about 3 kilograms (~6 pounds). The loss of a nanogram is impossible to detect with any scale, so that&amp;#039;s all theoretical.&lt;br /&gt;
&lt;br /&gt;
The [[strong force]], [[weak force]] and [[electromagnetic force]] work together inside of a nucleus to create stable configurations of protons and neutrons. These nuclear processes make for much stronger [[force]]s than the [[electron]] recombination in the [[combustion]] of [[fossil fuel]]s does. This means that the release of energy from a nuclear reaction creates enough of a mass difference to be measured. Specifically, small amounts of mass are turned into energy from the breaking up ([[fission]]) or combination ([[fusion]]) of the [[nuclei]] of [[atom]]s. Even spontaneous [[radioactive decay]] converts a bit of mass into incredible amounts of energy. &lt;br /&gt;
&lt;br /&gt;
By doing so, the energy from these processes can be used to generate [[electricity]] in [[nuclear power plant]]s, or as [[nuclear weapon]]s, which were first deployed in World War II and have only been tested since then (nuclear weapons have since not been used as a direct attack, just very big threats). Although these reactions cannot convert the entire mass to energy, they still release tremendous amounts of energy. See the page on [[energy density]] for more information.&lt;br /&gt;
&lt;br /&gt;
The [[sun]] uses fusion of [[hydrogen]] into [[helium]] to create sunlight at an astonishing rate. The sun gives off 3.86 x 10&amp;lt;sup&amp;gt;26&amp;lt;/sup&amp;gt; W of [[power]]. That means the sun is losing 4.2 million tonnes of mass every second due to nuclear fusion. &lt;br /&gt;
&lt;br /&gt;
To learn more about mass-energy equivalence, visit [http://hyperphysics.phy-astr.gsu.edu/hbase/relativ/releng.html Hyperphysics]&lt;br /&gt;
&lt;br /&gt;
==References==&lt;br /&gt;
{{reflist}}&lt;br /&gt;
[[Category:Uploaded]]&lt;/div&gt;</summary>
		<author><name>J.williams</name></author>
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