<?xml version="1.0"?>
<feed xmlns="http://www.w3.org/2005/Atom" xml:lang="en">
		<id>https://www.explainxkcd.com/wiki/index.php?action=history&amp;feed=atom&amp;title=2764%3A_Cosmological_Nostalgia_Content</id>
		<title>2764: Cosmological Nostalgia Content - Revision history</title>
		<link rel="self" type="application/atom+xml" href="https://www.explainxkcd.com/wiki/index.php?action=history&amp;feed=atom&amp;title=2764%3A_Cosmological_Nostalgia_Content"/>
		<link rel="alternate" type="text/html" href="https://www.explainxkcd.com/wiki/index.php?title=2764:_Cosmological_Nostalgia_Content&amp;action=history"/>
		<updated>2026-04-10T13:57:35Z</updated>
		<subtitle>Revision history for this page on the wiki</subtitle>
		<generator>MediaWiki 1.30.0</generator>

	<entry>
		<id>https://www.explainxkcd.com/wiki/index.php?title=2764:_Cosmological_Nostalgia_Content&amp;diff=339026&amp;oldid=prev</id>
		<title>172.69.194.184: /* Explanation */ Internalised link format.</title>
		<link rel="alternate" type="text/html" href="https://www.explainxkcd.com/wiki/index.php?title=2764:_Cosmological_Nostalgia_Content&amp;diff=339026&amp;oldid=prev"/>
				<updated>2024-04-07T13:29:54Z</updated>
		
		<summary type="html">&lt;p&gt;‎&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Explanation: &lt;/span&gt; Internalised link format.&lt;/span&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr style=&quot;vertical-align: top;&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;Revision as of 13:29, 7 April 2024&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-l11&quot; &gt;Line 11:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 11:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;==Explanation==&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;==Explanation==&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; 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;The title of this comic is a combination of &amp;quot;{{w|cosmological constant}}&amp;quot; (an astrophysics term related to {{w|dark energy}} and to the accelerated {{w|expansion of the universe}}) and &amp;quot;[https://movementstrategy.com/editorial/nostalgia-social-media/ nostalgia content]&amp;quot; (clickbait marketing aimed at a specific age group referencing pop culture from their youth). The [https://tvtropes.org canonical examples] of nostalgia content are &amp;quot;[https://knowyourmeme.com/memes/only-90s-kids--2 Only 90s Kids Remember...]&amp;quot; and &amp;quot;[https://knowyourmeme.com/memes/feel-old-yet Feel Old yet?]&amp;quot;, and this has also formed the basis for [&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;https&lt;/del&gt;:&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;//www.explainxkcd.com/wiki/index.php/&lt;/del&gt;Category:&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;Comics_to_make_one_feel_old &lt;/del&gt;several XKCD comics]. Some people of relatively advanced years like to make comparisons to others in their age group of where events that they remember fit into history; e.g., &amp;quot;The first moon landing was closer to the end of World War I than to today.&amp;quot; &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; 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;The title of this comic is a combination of &amp;quot;{{w|cosmological constant}}&amp;quot; (an astrophysics term related to {{w|dark energy}} and to the accelerated {{w|expansion of the universe}}) and &amp;quot;[https://movementstrategy.com/editorial/nostalgia-social-media/ nostalgia content]&amp;quot; (clickbait marketing aimed at a specific age group referencing pop culture from their youth). The [https://tvtropes.org canonical examples] of nostalgia content are &amp;quot;[https://knowyourmeme.com/memes/only-90s-kids--2 Only 90s Kids Remember...]&amp;quot; and &amp;quot;[https://knowyourmeme.com/memes/feel-old-yet Feel Old yet?]&amp;quot;, and this has also formed the basis for [&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;[&lt;/ins&gt;:Category:&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;Comics to make one feel old|&lt;/ins&gt;several XKCD comics&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;]&lt;/ins&gt;]. Some people of relatively advanced years like to make comparisons to others in their age group of where events that they remember fit into history; e.g., &amp;quot;The first moon landing was closer to the end of World War I than to today.&amp;quot; &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[File:age by redshift.png|thumb|right|[[Redshift]] indicates the age of the universe for distant astronomical objects as we observe them today, when the universe is 13.78 billion years old.]]&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[File:age by redshift.png|thumb|right|[[Redshift]] indicates the age of the universe for distant astronomical objects as we observe them today, when the universe is 13.78 billion years old.]]&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>172.69.194.184</name></author>	</entry>

	<entry>
		<id>https://www.explainxkcd.com/wiki/index.php?title=2764:_Cosmological_Nostalgia_Content&amp;diff=338979&amp;oldid=prev</id>
		<title>Jkshapiro: /* Explanation */ Add link to category</title>
		<link rel="alternate" type="text/html" href="https://www.explainxkcd.com/wiki/index.php?title=2764:_Cosmological_Nostalgia_Content&amp;diff=338979&amp;oldid=prev"/>
				<updated>2024-04-07T02:05:47Z</updated>
		
		<summary type="html">&lt;p&gt;‎&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Explanation: &lt;/span&gt; Add link to category&lt;/span&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr style=&quot;vertical-align: top;&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;Revision as of 02:05, 7 April 2024&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-l11&quot; &gt;Line 11:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 11:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;==Explanation==&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;==Explanation==&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; 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;The title of this comic is a combination of &amp;quot;{{w|cosmological constant}}&amp;quot; (an astrophysics term related to {{w|dark energy}} and to the accelerated {{w|expansion of the universe}}) and &amp;quot;[https://movementstrategy.com/editorial/nostalgia-social-media/ nostalgia content]&amp;quot; (clickbait marketing aimed at a specific age group referencing pop culture from their youth). The [https://tvtropes.org canonical examples] of nostalgia content are &amp;quot;[https://knowyourmeme.com/memes/only-90s-kids--2 Only 90s Kids Remember...]&amp;quot; and &amp;quot;[https://knowyourmeme.com/memes/feel-old-yet Feel Old yet?]&amp;quot;. Some people of relatively advanced years like to make comparisons to others in their age group of where events that they remember fit into history; e.g., &amp;quot;The first moon landing was closer to the end of World War I than to today.&amp;quot; &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; 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;The title of this comic is a combination of &amp;quot;{{w|cosmological constant}}&amp;quot; (an astrophysics term related to {{w|dark energy}} and to the accelerated {{w|expansion of the universe}}) and &amp;quot;[https://movementstrategy.com/editorial/nostalgia-social-media/ nostalgia content]&amp;quot; (clickbait marketing aimed at a specific age group referencing pop culture from their youth). The [https://tvtropes.org canonical examples] of nostalgia content are &amp;quot;[https://knowyourmeme.com/memes/only-90s-kids--2 Only 90s Kids Remember...]&amp;quot; and &amp;quot;[https://knowyourmeme.com/memes/feel-old-yet Feel Old yet?]&amp;quot;&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;, and this has also formed the basis for [https://www.explainxkcd.com/wiki/index.php/Category:Comics_to_make_one_feel_old several XKCD comics]&lt;/ins&gt;. Some people of relatively advanced years like to make comparisons to others in their age group of where events that they remember fit into history; e.g., &amp;quot;The first moon landing was closer to the end of World War I than to today.&amp;quot; &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[File:age by redshift.png|thumb|right|[[Redshift]] indicates the age of the universe for distant astronomical objects as we observe them today, when the universe is 13.78 billion years old.]]&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[File:age by redshift.png|thumb|right|[[Redshift]] indicates the age of the universe for distant astronomical objects as we observe them today, when the universe is 13.78 billion years old.]]&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Jkshapiro</name></author>	</entry>

	<entry>
		<id>https://www.explainxkcd.com/wiki/index.php?title=2764:_Cosmological_Nostalgia_Content&amp;diff=328994&amp;oldid=prev</id>
		<title>Liv2splain: /* Explanation */ comparison</title>
		<link rel="alternate" type="text/html" href="https://www.explainxkcd.com/wiki/index.php?title=2764:_Cosmological_Nostalgia_Content&amp;diff=328994&amp;oldid=prev"/>
				<updated>2023-11-14T19:55:54Z</updated>
		
		<summary type="html">&lt;p&gt;‎&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Explanation: &lt;/span&gt; comparison&lt;/span&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr style=&quot;vertical-align: top;&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;Revision as of 19:55, 14 November 2023&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-l13&quot; &gt;Line 13:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 13:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The title of this comic is a combination of &amp;quot;{{w|cosmological constant}}&amp;quot; (an astrophysics term related to {{w|dark energy}} and to the accelerated {{w|expansion of the universe}}) and &amp;quot;[https://movementstrategy.com/editorial/nostalgia-social-media/ nostalgia content]&amp;quot; (clickbait marketing aimed at a specific age group referencing pop culture from their youth). The [https://tvtropes.org canonical examples] of nostalgia content are &amp;quot;[https://knowyourmeme.com/memes/only-90s-kids--2 Only 90s Kids Remember...]&amp;quot; and &amp;quot;[https://knowyourmeme.com/memes/feel-old-yet Feel Old yet?]&amp;quot;. Some people of relatively advanced years like to make comparisons to others in their age group of where events that they remember fit into history; e.g., &amp;quot;The first moon landing was closer to the end of World War I than to today.&amp;quot; &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The title of this comic is a combination of &amp;quot;{{w|cosmological constant}}&amp;quot; (an astrophysics term related to {{w|dark energy}} and to the accelerated {{w|expansion of the universe}}) and &amp;quot;[https://movementstrategy.com/editorial/nostalgia-social-media/ nostalgia content]&amp;quot; (clickbait marketing aimed at a specific age group referencing pop culture from their youth). The [https://tvtropes.org canonical examples] of nostalgia content are &amp;quot;[https://knowyourmeme.com/memes/only-90s-kids--2 Only 90s Kids Remember...]&amp;quot; and &amp;quot;[https://knowyourmeme.com/memes/feel-old-yet Feel Old yet?]&amp;quot;. Some people of relatively advanced years like to make comparisons to others in their age group of where events that they remember fit into history; e.g., &amp;quot;The first moon landing was closer to the end of World War I than to today.&amp;quot; &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; 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;[[File:age by redshift.png|thumb|right|[[Redshift]] indicates the age of the universe for distant astronomical objects as we observe them today.]]&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; 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;[[File:age by redshift.png|thumb|right|[[Redshift]] indicates the age of the universe for distant astronomical objects as we observe them today&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;, when the universe is 13.78 billion years old&lt;/ins&gt;.]]&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;In cosmology, &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; is the symbol for {{w|Redshift|redshift}}, the effect whereby photons traveling from an object that is moving away from the observer exhibit an increase in wavelength, resulting in their color shifting towards the red end of the spectrum, and the variable &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; quantifies this amount of shift. Due to the expansion of the universe, objects that are further away from us appear to be moving away from us at a faster velocity, resulting in higher redshift. As light has finite velocity, it {{w|Speed of light#Spaceflight and astronomy|takes a longer time }}for light from faraway objects to arrive at the observer. So the light observed at the present must have been emitted by the faraway object further back in time. In this sense, after assuming a cosmological model, redshift and cosmic time can be put in a one-to-one relation and are often used interchangeably by astronomers. Redshift &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10 would correspond to about 500 million years after the universe was formed, or almost 13 billion years ago[https://www.astro.ucla.edu/~wright/CosmoCalc.html]. Megan is stating that only people that were born at that time (&amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10) can remember when the first stars were still forming. At redshift &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10 the matter filling the universe was mostly constituted of neutral hydrogen gas, referred by Megan as &amp;quot;cold&amp;quot; (it had a temperature of about 300 K) and &amp;quot;dark&amp;quot; (there were no light sources in the universe before the first stars formed. This epoch is indeed called the {{w|Timeline of the early universe#Cosmic Dark Age|cosmic dark ages}}). The ultraviolet light emitted by the first stars started ionizing the hydrogen around them in expanding hot plasma bubbles. This process (called {{w|reionization}}) had probably already begun at &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10, but was really completed only at about &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 6, when the intergalactic hydrogen was completely ionized, as it continues to be at the present day.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;In cosmology, &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; is the symbol for {{w|Redshift|redshift}}, the effect whereby photons traveling from an object that is moving away from the observer exhibit an increase in wavelength, resulting in their color shifting towards the red end of the spectrum, and the variable &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; quantifies this amount of shift. Due to the expansion of the universe, objects that are further away from us appear to be moving away from us at a faster velocity, resulting in higher redshift. As light has finite velocity, it {{w|Speed of light#Spaceflight and astronomy|takes a longer time }}for light from faraway objects to arrive at the observer. So the light observed at the present must have been emitted by the faraway object further back in time. In this sense, after assuming a cosmological model, redshift and cosmic time can be put in a one-to-one relation and are often used interchangeably by astronomers. Redshift &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10 would correspond to about 500 million years after the universe was formed, or almost 13 billion years ago[https://www.astro.ucla.edu/~wright/CosmoCalc.html]. Megan is stating that only people that were born at that time (&amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10) can remember when the first stars were still forming. At redshift &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10 the matter filling the universe was mostly constituted of neutral hydrogen gas, referred by Megan as &amp;quot;cold&amp;quot; (it had a temperature of about 300 K) and &amp;quot;dark&amp;quot; (there were no light sources in the universe before the first stars formed. This epoch is indeed called the {{w|Timeline of the early universe#Cosmic Dark Age|cosmic dark ages}}). The ultraviolet light emitted by the first stars started ionizing the hydrogen around them in expanding hot plasma bubbles. This process (called {{w|reionization}}) had probably already begun at &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10, but was really completed only at about &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 6, when the intergalactic hydrogen was completely ionized, as it continues to be at the present day.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Liv2splain</name></author>	</entry>

	<entry>
		<id>https://www.explainxkcd.com/wiki/index.php?title=2764:_Cosmological_Nostalgia_Content&amp;diff=328835&amp;oldid=prev</id>
		<title>Liv2splain: /* Explanation */ chart</title>
		<link rel="alternate" type="text/html" href="https://www.explainxkcd.com/wiki/index.php?title=2764:_Cosmological_Nostalgia_Content&amp;diff=328835&amp;oldid=prev"/>
				<updated>2023-11-13T11:55:57Z</updated>
		
		<summary type="html">&lt;p&gt;‎&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Explanation: &lt;/span&gt; chart&lt;/span&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr style=&quot;vertical-align: top;&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;Revision as of 11:55, 13 November 2023&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-l12&quot; &gt;Line 12:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 12:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The title of this comic is a combination of &amp;quot;{{w|cosmological constant}}&amp;quot; (an astrophysics term related to {{w|dark energy}} and to the accelerated {{w|expansion of the universe}}) and &amp;quot;[https://movementstrategy.com/editorial/nostalgia-social-media/ nostalgia content]&amp;quot; (clickbait marketing aimed at a specific age group referencing pop culture from their youth). The [https://tvtropes.org canonical examples] of nostalgia content are &amp;quot;[https://knowyourmeme.com/memes/only-90s-kids--2 Only 90s Kids Remember...]&amp;quot; and &amp;quot;[https://knowyourmeme.com/memes/feel-old-yet Feel Old yet?]&amp;quot;. Some people of relatively advanced years like to make comparisons to others in their age group of where events that they remember fit into history; e.g., &amp;quot;The first moon landing was closer to the end of World War I than to today.&amp;quot; &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The title of this comic is a combination of &amp;quot;{{w|cosmological constant}}&amp;quot; (an astrophysics term related to {{w|dark energy}} and to the accelerated {{w|expansion of the universe}}) and &amp;quot;[https://movementstrategy.com/editorial/nostalgia-social-media/ nostalgia content]&amp;quot; (clickbait marketing aimed at a specific age group referencing pop culture from their youth). The [https://tvtropes.org canonical examples] of nostalgia content are &amp;quot;[https://knowyourmeme.com/memes/only-90s-kids--2 Only 90s Kids Remember...]&amp;quot; and &amp;quot;[https://knowyourmeme.com/memes/feel-old-yet Feel Old yet?]&amp;quot;. Some people of relatively advanced years like to make comparisons to others in their age group of where events that they remember fit into history; e.g., &amp;quot;The first moon landing was closer to the end of World War I than to today.&amp;quot; &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; 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;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; 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;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;[[File:age by redshift.png|thumb|right|[[Redshift]] indicates the age of the universe for distant astronomical objects as we observe them today.]]&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;In cosmology, &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; is the symbol for {{w|Redshift|redshift}}, the effect whereby photons traveling from an object that is moving away from the observer exhibit an increase in wavelength, resulting in their color shifting towards the red end of the spectrum, and the variable &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; quantifies this amount of shift. Due to the expansion of the universe, objects that are further away from us appear to be moving away from us at a faster velocity, resulting in higher redshift. As light has finite velocity, it {{w|Speed of light#Spaceflight and astronomy|takes a longer time }}for light from faraway objects to arrive at the observer. So the light observed at the present must have been emitted by the faraway object further back in time. In this sense, after assuming a cosmological model, redshift and cosmic time can be put in a one-to-one relation and are often used interchangeably by astronomers. Redshift &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10 would correspond to about 500 million years after the universe was formed, or almost 13 billion years ago[https://www.astro.ucla.edu/~wright/CosmoCalc.html]. Megan is stating that only people that were born at that time (&amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10) can remember when the first stars were still forming. At redshift &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10 the matter filling the universe was mostly constituted of neutral hydrogen gas, referred by Megan as &amp;quot;cold&amp;quot; (it had a temperature of about 300 K) and &amp;quot;dark&amp;quot; (there were no light sources in the universe before the first stars formed. This epoch is indeed called the {{w|Timeline of the early universe#Cosmic Dark Age|cosmic dark ages}}). The ultraviolet light emitted by the first stars started ionizing the hydrogen around them in expanding hot plasma bubbles. This process (called {{w|reionization}}) had probably already begun at &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10, but was really completed only at about &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 6, when the intergalactic hydrogen was completely ionized, as it continues to be at the present day.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;In cosmology, &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; is the symbol for {{w|Redshift|redshift}}, the effect whereby photons traveling from an object that is moving away from the observer exhibit an increase in wavelength, resulting in their color shifting towards the red end of the spectrum, and the variable &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; quantifies this amount of shift. Due to the expansion of the universe, objects that are further away from us appear to be moving away from us at a faster velocity, resulting in higher redshift. As light has finite velocity, it {{w|Speed of light#Spaceflight and astronomy|takes a longer time }}for light from faraway objects to arrive at the observer. So the light observed at the present must have been emitted by the faraway object further back in time. In this sense, after assuming a cosmological model, redshift and cosmic time can be put in a one-to-one relation and are often used interchangeably by astronomers. Redshift &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10 would correspond to about 500 million years after the universe was formed, or almost 13 billion years ago[https://www.astro.ucla.edu/~wright/CosmoCalc.html]. Megan is stating that only people that were born at that time (&amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10) can remember when the first stars were still forming. At redshift &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10 the matter filling the universe was mostly constituted of neutral hydrogen gas, referred by Megan as &amp;quot;cold&amp;quot; (it had a temperature of about 300 K) and &amp;quot;dark&amp;quot; (there were no light sources in the universe before the first stars formed. This epoch is indeed called the {{w|Timeline of the early universe#Cosmic Dark Age|cosmic dark ages}}). The ultraviolet light emitted by the first stars started ionizing the hydrogen around them in expanding hot plasma bubbles. This process (called {{w|reionization}}) had probably already begun at &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10, but was really completed only at about &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 6, when the intergalactic hydrogen was completely ionized, as it continues to be at the present day.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Liv2splain</name></author>	</entry>

	<entry>
		<id>https://www.explainxkcd.com/wiki/index.php?title=2764:_Cosmological_Nostalgia_Content&amp;diff=323373&amp;oldid=prev</id>
		<title>162.158.95.127: Added missing space</title>
		<link rel="alternate" type="text/html" href="https://www.explainxkcd.com/wiki/index.php?title=2764:_Cosmological_Nostalgia_Content&amp;diff=323373&amp;oldid=prev"/>
				<updated>2023-09-06T14:28:32Z</updated>
		
		<summary type="html">&lt;p&gt;Added missing space&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr style=&quot;vertical-align: top;&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;Revision as of 14:28, 6 September 2023&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-l13&quot; &gt;Line 13:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 13:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The title of this comic is a combination of &amp;quot;{{w|cosmological constant}}&amp;quot; (an astrophysics term related to {{w|dark energy}} and to the accelerated {{w|expansion of the universe}}) and &amp;quot;[https://movementstrategy.com/editorial/nostalgia-social-media/ nostalgia content]&amp;quot; (clickbait marketing aimed at a specific age group referencing pop culture from their youth). The [https://tvtropes.org canonical examples] of nostalgia content are &amp;quot;[https://knowyourmeme.com/memes/only-90s-kids--2 Only 90s Kids Remember...]&amp;quot; and &amp;quot;[https://knowyourmeme.com/memes/feel-old-yet Feel Old yet?]&amp;quot;. Some people of relatively advanced years like to make comparisons to others in their age group of where events that they remember fit into history; e.g., &amp;quot;The first moon landing was closer to the end of World War I than to today.&amp;quot; &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The title of this comic is a combination of &amp;quot;{{w|cosmological constant}}&amp;quot; (an astrophysics term related to {{w|dark energy}} and to the accelerated {{w|expansion of the universe}}) and &amp;quot;[https://movementstrategy.com/editorial/nostalgia-social-media/ nostalgia content]&amp;quot; (clickbait marketing aimed at a specific age group referencing pop culture from their youth). The [https://tvtropes.org canonical examples] of nostalgia content are &amp;quot;[https://knowyourmeme.com/memes/only-90s-kids--2 Only 90s Kids Remember...]&amp;quot; and &amp;quot;[https://knowyourmeme.com/memes/feel-old-yet Feel Old yet?]&amp;quot;. Some people of relatively advanced years like to make comparisons to others in their age group of where events that they remember fit into history; e.g., &amp;quot;The first moon landing was closer to the end of World War I than to today.&amp;quot; &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; 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;In cosmology, &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; is the symbol for {{w|Redshift|redshift}}, the effect whereby photons traveling from an object that is moving away from the observer exhibit an increase in wavelength, resulting in their color shifting towards the red end of the spectrum, and the variable &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; quantifies this amount of shift. Due to the expansion of the universe, objects that are further away from us appear to be moving away from us at a faster velocity, resulting in higher redshift. As light has finite velocity, it {{w|Speed of light#Spaceflight and astronomy|takes a longer time}}for light from faraway objects to arrive at the observer. So the light observed at the present must have been emitted by the faraway object further back in time. In this sense, after assuming a cosmological model, redshift and cosmic time can be put in a one-to-one relation and are often used interchangeably by astronomers. Redshift &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10 would correspond to about 500 million years after the universe was formed, or almost 13 billion years ago[https://www.astro.ucla.edu/~wright/CosmoCalc.html]. Megan is stating that only people that were born at that time (&amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10) can remember when the first stars were still forming. At redshift &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10 the matter filling the universe was mostly constituted of neutral hydrogen gas, referred by Megan as &amp;quot;cold&amp;quot; (it had a temperature of about 300 K) and &amp;quot;dark&amp;quot; (there were no light sources in the universe before the first stars formed. This epoch is indeed called the {{w|Timeline of the early universe#Cosmic Dark Age|cosmic dark ages}}). The ultraviolet light emitted by the first stars started ionizing the hydrogen around them in expanding hot plasma bubbles. This process (called {{w|reionization}}) had probably already begun at &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10, but was really completed only at about &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 6, when the intergalactic hydrogen was completely ionized, as it continues to be at the present day.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; 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;In cosmology, &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; is the symbol for {{w|Redshift|redshift}}, the effect whereby photons traveling from an object that is moving away from the observer exhibit an increase in wavelength, resulting in their color shifting towards the red end of the spectrum, and the variable &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; quantifies this amount of shift. Due to the expansion of the universe, objects that are further away from us appear to be moving away from us at a faster velocity, resulting in higher redshift. As light has finite velocity, it {{w|Speed of light#Spaceflight and astronomy|takes a longer time }}for light from faraway objects to arrive at the observer. So the light observed at the present must have been emitted by the faraway object further back in time. In this sense, after assuming a cosmological model, redshift and cosmic time can be put in a one-to-one relation and are often used interchangeably by astronomers. Redshift &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10 would correspond to about 500 million years after the universe was formed, or almost 13 billion years ago[https://www.astro.ucla.edu/~wright/CosmoCalc.html]. Megan is stating that only people that were born at that time (&amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10) can remember when the first stars were still forming. At redshift &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10 the matter filling the universe was mostly constituted of neutral hydrogen gas, referred by Megan as &amp;quot;cold&amp;quot; (it had a temperature of about 300 K) and &amp;quot;dark&amp;quot; (there were no light sources in the universe before the first stars formed. This epoch is indeed called the {{w|Timeline of the early universe#Cosmic Dark Age|cosmic dark ages}}). The ultraviolet light emitted by the first stars started ionizing the hydrogen around them in expanding hot plasma bubbles. This process (called {{w|reionization}}) had probably already begun at &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10, but was really completed only at about &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 6, when the intergalactic hydrogen was completely ionized, as it continues to be at the present day.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Megan also has a red tint (she is drawn in the color [https://www.color-hex.com/color/462424 #462424], a very dark red; here is a comparison of #462424 and black: &amp;lt;span style=&amp;quot;background-color: #462424&amp;quot;&amp;gt;&amp;amp;emsp;&amp;lt;/span&amp;gt;&amp;amp;thinsp;&amp;lt;span style=&amp;quot;background-color: black&amp;quot;&amp;gt;&amp;amp;emsp;&amp;lt;/span&amp;gt; ), indicating that she is one such &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10 kid, because her image is red-shifted, in the literal sense. The irony is that even if she were actually born 13 billion years ago (which would be absurd,{{Citation needed}}) her image would not appear red-shifted to us now. She would only appear redshifted to a far away observer looking at the young Megan wandering about the primordal cold dark gas.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Megan also has a red tint (she is drawn in the color [https://www.color-hex.com/color/462424 #462424], a very dark red; here is a comparison of #462424 and black: &amp;lt;span style=&amp;quot;background-color: #462424&amp;quot;&amp;gt;&amp;amp;emsp;&amp;lt;/span&amp;gt;&amp;amp;thinsp;&amp;lt;span style=&amp;quot;background-color: black&amp;quot;&amp;gt;&amp;amp;emsp;&amp;lt;/span&amp;gt; ), indicating that she is one such &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10 kid, because her image is red-shifted, in the literal sense. The irony is that even if she were actually born 13 billion years ago (which would be absurd,{{Citation needed}}) her image would not appear red-shifted to us now. She would only appear redshifted to a far away observer looking at the young Megan wandering about the primordal cold dark gas.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>162.158.95.127</name></author>	</entry>

	<entry>
		<id>https://www.explainxkcd.com/wiki/index.php?title=2764:_Cosmological_Nostalgia_Content&amp;diff=315223&amp;oldid=prev</id>
		<title>172.69.22.213: /* Explanation */</title>
		<link rel="alternate" type="text/html" href="https://www.explainxkcd.com/wiki/index.php?title=2764:_Cosmological_Nostalgia_Content&amp;diff=315223&amp;oldid=prev"/>
				<updated>2023-06-09T19:24:54Z</updated>
		
		<summary type="html">&lt;p&gt;‎&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Explanation&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr style=&quot;vertical-align: top;&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;Revision as of 19:24, 9 June 2023&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-l10&quot; &gt;Line 10:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 10:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;==Explanation==&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;==Explanation==&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; 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;&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;{{incomplete|1=Created by a z&amp;amp;#61;90s KID - Needs more explanation of what the click bait in the title text refers to in the context of the Einstein blunder and why that belongs in this nostalgia comic. Do NOT delete this tag too soon.}}&lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The title of this comic is a combination of &amp;quot;{{w|cosmological constant}}&amp;quot; (an astrophysics term related to {{w|dark energy}} and to the accelerated {{w|expansion of the universe}}) and &amp;quot;[https://movementstrategy.com/editorial/nostalgia-social-media/ nostalgia content]&amp;quot; (clickbait marketing aimed at a specific age group referencing pop culture from their youth). The [https://tvtropes.org canonical examples] of nostalgia content are &amp;quot;[https://knowyourmeme.com/memes/only-90s-kids--2 Only 90s Kids Remember...]&amp;quot; and &amp;quot;[https://knowyourmeme.com/memes/feel-old-yet Feel Old yet?]&amp;quot;. Some people of relatively advanced years like to make comparisons to others in their age group of where events that they remember fit into history; e.g., &amp;quot;The first moon landing was closer to the end of World War I than to today.&amp;quot; &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The title of this comic is a combination of &amp;quot;{{w|cosmological constant}}&amp;quot; (an astrophysics term related to {{w|dark energy}} and to the accelerated {{w|expansion of the universe}}) and &amp;quot;[https://movementstrategy.com/editorial/nostalgia-social-media/ nostalgia content]&amp;quot; (clickbait marketing aimed at a specific age group referencing pop culture from their youth). The [https://tvtropes.org canonical examples] of nostalgia content are &amp;quot;[https://knowyourmeme.com/memes/only-90s-kids--2 Only 90s Kids Remember...]&amp;quot; and &amp;quot;[https://knowyourmeme.com/memes/feel-old-yet Feel Old yet?]&amp;quot;. Some people of relatively advanced years like to make comparisons to others in their age group of where events that they remember fit into history; e.g., &amp;quot;The first moon landing was closer to the end of World War I than to today.&amp;quot; &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>172.69.22.213</name></author>	</entry>

	<entry>
		<id>https://www.explainxkcd.com/wiki/index.php?title=2764:_Cosmological_Nostalgia_Content&amp;diff=313277&amp;oldid=prev</id>
		<title>Volatile: Removed multimanteau reference and updated incomplete tag accordingly</title>
		<link rel="alternate" type="text/html" href="https://www.explainxkcd.com/wiki/index.php?title=2764:_Cosmological_Nostalgia_Content&amp;diff=313277&amp;oldid=prev"/>
				<updated>2023-05-16T19:36:37Z</updated>
		
		<summary type="html">&lt;p&gt;Removed multimanteau reference and updated incomplete tag accordingly&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr style=&quot;vertical-align: top;&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;Revision as of 19:36, 16 May 2023&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-l10&quot; &gt;Line 10:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 10:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;==Explanation==&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;==Explanation==&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; 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;{{incomplete|1=Created by a z&amp;amp;#61;90s KID - &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;The entire start of this explanation with the made up word multimanteu that has nothing to do with this comic should be changes maybe just deleted! &lt;/del&gt;Needs more explanation of what the click bait in the title text refers to in the context of the Einstein blunder and why that belongs in this nostalgia comic. Do NOT delete this tag too soon.}}&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; 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;{{incomplete|1=Created by a z&amp;amp;#61;90s KID - Needs more explanation of what the click bait in the title text refers to in the context of the Einstein blunder and why that belongs in this nostalgia comic. Do NOT delete this tag too soon.}}&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; 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;&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;Like many xkcds, &lt;/del&gt;this comic is &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;a figurative {{w|Portmanteau|multimanteau}}, in this case &lt;/del&gt;a combination of &amp;quot;{{w|cosmological constant}}&amp;quot; (an astrophysics term related to {{w|dark energy}} and to the accelerated {{w|expansion of the universe}}) and &amp;quot;[https://movementstrategy.com/editorial/nostalgia-social-media/ nostalgia content]&amp;quot; (clickbait marketing aimed at a specific age group referencing pop culture from their youth). The [https://tvtropes.org canonical examples] of nostalgia content are &amp;quot;[https://knowyourmeme.com/memes/only-90s-kids--2 Only 90s Kids Remember...]&amp;quot; and &amp;quot;[https://knowyourmeme.com/memes/feel-old-yet Feel Old yet?]&amp;quot;. Some people of relatively advanced years like to make comparisons to others in their age group of where events that they remember fit into history; e.g., &amp;quot;The first moon landing was closer to the end of World War I than to today.&amp;quot; &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; 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;&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;The title of &lt;/ins&gt;this comic is a combination of &amp;quot;{{w|cosmological constant}}&amp;quot; (an astrophysics term related to {{w|dark energy}} and to the accelerated {{w|expansion of the universe}}) and &amp;quot;[https://movementstrategy.com/editorial/nostalgia-social-media/ nostalgia content]&amp;quot; (clickbait marketing aimed at a specific age group referencing pop culture from their youth). The [https://tvtropes.org canonical examples] of nostalgia content are &amp;quot;[https://knowyourmeme.com/memes/only-90s-kids--2 Only 90s Kids Remember...]&amp;quot; and &amp;quot;[https://knowyourmeme.com/memes/feel-old-yet Feel Old yet?]&amp;quot;. Some people of relatively advanced years like to make comparisons to others in their age group of where events that they remember fit into history; e.g., &amp;quot;The first moon landing was closer to the end of World War I than to today.&amp;quot; &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;In cosmology, &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; is the symbol for {{w|Redshift|redshift}}, the effect whereby photons traveling from an object that is moving away from the observer exhibit an increase in wavelength, resulting in their color shifting towards the red end of the spectrum, and the variable &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; quantifies this amount of shift. Due to the expansion of the universe, objects that are further away from us appear to be moving away from us at a faster velocity, resulting in higher redshift. As light has finite velocity, it {{w|Speed of light#Spaceflight and astronomy|takes a longer time}}for light from faraway objects to arrive at the observer. So the light observed at the present must have been emitted by the faraway object further back in time. In this sense, after assuming a cosmological model, redshift and cosmic time can be put in a one-to-one relation and are often used interchangeably by astronomers. Redshift &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10 would correspond to about 500 million years after the universe was formed, or almost 13 billion years ago[https://www.astro.ucla.edu/~wright/CosmoCalc.html]. Megan is stating that only people that were born at that time (&amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10) can remember when the first stars were still forming. At redshift &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10 the matter filling the universe was mostly constituted of neutral hydrogen gas, referred by Megan as &amp;quot;cold&amp;quot; (it had a temperature of about 300 K) and &amp;quot;dark&amp;quot; (there were no light sources in the universe before the first stars formed. This epoch is indeed called the {{w|Timeline of the early universe#Cosmic Dark Age|cosmic dark ages}}). The ultraviolet light emitted by the first stars started ionizing the hydrogen around them in expanding hot plasma bubbles. This process (called {{w|reionization}}) had probably already begun at &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10, but was really completed only at about &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 6, when the intergalactic hydrogen was completely ionized, as it continues to be at the present day.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;In cosmology, &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; is the symbol for {{w|Redshift|redshift}}, the effect whereby photons traveling from an object that is moving away from the observer exhibit an increase in wavelength, resulting in their color shifting towards the red end of the spectrum, and the variable &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; quantifies this amount of shift. Due to the expansion of the universe, objects that are further away from us appear to be moving away from us at a faster velocity, resulting in higher redshift. As light has finite velocity, it {{w|Speed of light#Spaceflight and astronomy|takes a longer time}}for light from faraway objects to arrive at the observer. So the light observed at the present must have been emitted by the faraway object further back in time. In this sense, after assuming a cosmological model, redshift and cosmic time can be put in a one-to-one relation and are often used interchangeably by astronomers. Redshift &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10 would correspond to about 500 million years after the universe was formed, or almost 13 billion years ago[https://www.astro.ucla.edu/~wright/CosmoCalc.html]. Megan is stating that only people that were born at that time (&amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10) can remember when the first stars were still forming. At redshift &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10 the matter filling the universe was mostly constituted of neutral hydrogen gas, referred by Megan as &amp;quot;cold&amp;quot; (it had a temperature of about 300 K) and &amp;quot;dark&amp;quot; (there were no light sources in the universe before the first stars formed. This epoch is indeed called the {{w|Timeline of the early universe#Cosmic Dark Age|cosmic dark ages}}). The ultraviolet light emitted by the first stars started ionizing the hydrogen around them in expanding hot plasma bubbles. This process (called {{w|reionization}}) had probably already begun at &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10, but was really completed only at about &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 6, when the intergalactic hydrogen was completely ionized, as it continues to be at the present day.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Volatile</name></author>	</entry>

	<entry>
		<id>https://www.explainxkcd.com/wiki/index.php?title=2764:_Cosmological_Nostalgia_Content&amp;diff=313064&amp;oldid=prev</id>
		<title>141.101.98.101: /* Explanation */ Wikilinks to local template version. Some rephrasing/etc.</title>
		<link rel="alternate" type="text/html" href="https://www.explainxkcd.com/wiki/index.php?title=2764:_Cosmological_Nostalgia_Content&amp;diff=313064&amp;oldid=prev"/>
				<updated>2023-05-13T21:20:32Z</updated>
		
		<summary type="html">&lt;p&gt;‎&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Explanation: &lt;/span&gt; Wikilinks to local template version. Some rephrasing/etc.&lt;/span&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr style=&quot;vertical-align: top;&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;Revision as of 21:20, 13 May 2023&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-l14&quot; &gt;Line 14:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 14:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Like many xkcds, this comic is a figurative {{w|Portmanteau|multimanteau}}, in this case a combination of &amp;quot;{{w|cosmological constant}}&amp;quot; (an astrophysics term related to {{w|dark energy}} and to the accelerated {{w|expansion of the universe}}) and &amp;quot;[https://movementstrategy.com/editorial/nostalgia-social-media/ nostalgia content]&amp;quot; (clickbait marketing aimed at a specific age group referencing pop culture from their youth). The [https://tvtropes.org canonical examples] of nostalgia content are &amp;quot;[https://knowyourmeme.com/memes/only-90s-kids--2 Only 90s Kids Remember...]&amp;quot; and &amp;quot;[https://knowyourmeme.com/memes/feel-old-yet Feel Old yet?]&amp;quot;. Some people of relatively advanced years like to make comparisons to others in their age group of where events that they remember fit into history; e.g., &amp;quot;The first moon landing was closer to the end of World War I than to today.&amp;quot; &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Like many xkcds, this comic is a figurative {{w|Portmanteau|multimanteau}}, in this case a combination of &amp;quot;{{w|cosmological constant}}&amp;quot; (an astrophysics term related to {{w|dark energy}} and to the accelerated {{w|expansion of the universe}}) and &amp;quot;[https://movementstrategy.com/editorial/nostalgia-social-media/ nostalgia content]&amp;quot; (clickbait marketing aimed at a specific age group referencing pop culture from their youth). The [https://tvtropes.org canonical examples] of nostalgia content are &amp;quot;[https://knowyourmeme.com/memes/only-90s-kids--2 Only 90s Kids Remember...]&amp;quot; and &amp;quot;[https://knowyourmeme.com/memes/feel-old-yet Feel Old yet?]&amp;quot;. Some people of relatively advanced years like to make comparisons to others in their age group of where events that they remember fit into history; e.g., &amp;quot;The first moon landing was closer to the end of World War I than to today.&amp;quot; &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; 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;In cosmology, &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; is the symbol for {{w|Redshift|redshift}}&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;: &lt;/del&gt;photons traveling from an object that is moving away from the observer exhibit an increase in wavelength, resulting in &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;its &lt;/del&gt;color shifting towards the red end of the spectrum, and the variable &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; quantifies &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;the &lt;/del&gt;amount of shift. Due to the expansion of the universe, objects that are further away from us appear to be moving away from us at a faster velocity, resulting in higher redshift. As light has finite velocity, it takes a longer time for light from faraway objects to arrive at the observer&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;[https://en.wikipedia.org/wiki/Speed_of_light#Spaceflight_and_astronomy]&lt;/del&gt;. So the light observed at the present must have been emitted by the faraway object further back in time. In this sense, after assuming a cosmological model, redshift and cosmic time can be put in a one-to-one relation and are often used interchangeably by astronomers. Redshift &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10 would correspond to about 500 million years after the universe was formed, or almost 13 billion years ago[https://www.astro.ucla.edu/~wright/CosmoCalc.html]. Megan is stating that only people that were born at that time (&amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10) can remember when the first stars were still forming. At redshift &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10 the matter filling the universe was mostly constituted of neutral hydrogen gas, referred by Megan as &amp;quot;cold&amp;quot; (it had a temperature of about 300 K) and &amp;quot;dark&amp;quot; (there were no light sources in the universe before the first stars formed. This epoch is indeed called the &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;[https://en.wikipedia.org/wiki/Timeline_of_the_early_universe&lt;/del&gt;#&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;Cosmic_Dark_Age &lt;/del&gt;cosmic dark ages&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;]&lt;/del&gt;). The ultraviolet light emitted by the first stars started ionizing the hydrogen around them in expanding hot plasma bubbles. This process (called {{w|reionization}}) had probably already begun at &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10, but was really completed only at about &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 6, when the intergalactic hydrogen was completely ionized, as it continues to be at the present day.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; 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;In cosmology, &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; is the symbol for {{w|Redshift|redshift}}&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;, the effect whereby &lt;/ins&gt;photons traveling from an object that is moving away from the observer exhibit an increase in wavelength, resulting in &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;their &lt;/ins&gt;color shifting towards the red end of the spectrum, and the variable &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; quantifies &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;this &lt;/ins&gt;amount of shift. Due to the expansion of the universe, objects that are further away from us appear to be moving away from us at a faster velocity, resulting in higher redshift. As light has finite velocity, it &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;{{w|Speed of light#Spaceflight and astronomy|&lt;/ins&gt;takes a longer time&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;}}&lt;/ins&gt;for light from faraway objects to arrive at the observer. So the light observed at the present must have been emitted by the faraway object further back in time. In this sense, after assuming a cosmological model, redshift and cosmic time can be put in a one-to-one relation and are often used interchangeably by astronomers. Redshift &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10 would correspond to about 500 million years after the universe was formed, or almost 13 billion years ago[https://www.astro.ucla.edu/~wright/CosmoCalc.html]. Megan is stating that only people that were born at that time (&amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10) can remember when the first stars were still forming. At redshift &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10 the matter filling the universe was mostly constituted of neutral hydrogen gas, referred by Megan as &amp;quot;cold&amp;quot; (it had a temperature of about 300 K) and &amp;quot;dark&amp;quot; (there were no light sources in the universe before the first stars formed. This epoch is indeed called the &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;{{w|Timeline of the early universe&lt;/ins&gt;#&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;Cosmic Dark Age|&lt;/ins&gt;cosmic dark ages&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;}}&lt;/ins&gt;). The ultraviolet light emitted by the first stars started ionizing the hydrogen around them in expanding hot plasma bubbles. This process (called {{w|reionization}}) had probably already begun at &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10, but was really completed only at about &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 6, when the intergalactic hydrogen was completely ionized, as it continues to be at the present day.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; 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;Megan also has a red tint (she is drawn in the color [https://www.color-hex.com/color/462424 #462424], a very dark red; here is a comparison of #462424 and black: &amp;lt;span style=&amp;quot;background-color: #462424&amp;quot;&amp;gt;&amp;amp;emsp;&amp;lt;/span&amp;gt;&amp;amp;thinsp;&amp;lt;span style=&amp;quot;background-color: black&amp;quot;&amp;gt;&amp;amp;emsp;&amp;lt;/span&amp;gt; ), indicating that she is one such &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10 kid, because her image is red-shifted, in the literal sense. The irony is that even if she were actually born 13 billion years ago (which would be absurd{{&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;citation &lt;/del&gt;needed}})&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;, &lt;/del&gt;her image would not appear red-shifted to us now. She would only appear redshifted to a far away observer looking at the young Megan wandering about the primordal cold dark gas.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; 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;Megan also has a red tint (she is drawn in the color [https://www.color-hex.com/color/462424 #462424], a very dark red; here is a comparison of #462424 and black: &amp;lt;span style=&amp;quot;background-color: #462424&amp;quot;&amp;gt;&amp;amp;emsp;&amp;lt;/span&amp;gt;&amp;amp;thinsp;&amp;lt;span style=&amp;quot;background-color: black&amp;quot;&amp;gt;&amp;amp;emsp;&amp;lt;/span&amp;gt; ), indicating that she is one such &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10 kid, because her image is red-shifted, in the literal sense. The irony is that even if she were actually born 13 billion years ago (which would be absurd&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;,&lt;/ins&gt;{{&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;Citation &lt;/ins&gt;needed}}) her image would not appear red-shifted to us now. She would only appear redshifted to a far away observer looking at the young Megan wandering about the primordal cold dark gas.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; 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;White Hat, meanwhile, is referencing the fact that the universe has {{w|Scale factor (cosmology)|three eras}}: radiation dominated, matter dominated&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;, &lt;/del&gt;and dark energy dominated. As the universe expands, the density of radiation and matter decreases due to their dilution, causing the universe, which first started off being dominated by radiation, to then become dominated by matter, then by dark energy (which &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;does &lt;/del&gt;not dilute as the universe expands). &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;Dark &lt;/del&gt;energy dominated era, which is when &amp;quot;dark energy started accelerating the universe's expansion&amp;quot; started around 5 billion years ago &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;while &lt;/del&gt;{{w|Evolution of bacteria|bacteria evolved around 3 billion years ago}}, meaning that they evolved closer to dark energy domination than to today.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; 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;White Hat, meanwhile, is referencing the fact that the universe has {{w|Scale factor (cosmology)|three eras}}: radiation dominated, matter dominated and dark energy dominated. As the universe expands, the density of radiation and matter decreases due to their dilution, causing the universe, which first started off being dominated by radiation, to then become dominated by matter, then by dark energy (which &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;is thought to &lt;/ins&gt;not dilute as the universe expands). &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;The dark &lt;/ins&gt;energy dominated era, which is when &amp;quot;dark energy started accelerating the universe's expansion&amp;quot; started around 5 billion years ago&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;, whilst &lt;/ins&gt;{{w|Evolution of bacteria|bacteria evolved around 3 billion years ago}}, meaning that they evolved closer to dark energy domination than to today.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The title and title text play with the similarity in sound between 'content' and 'constant', segueing between web(page) content and cosmological constant.&amp;#160; &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The title and title text play with the similarity in sound between 'content' and 'constant', segueing between web(page) content and cosmological constant.&amp;#160; &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>141.101.98.101</name></author>	</entry>

	<entry>
		<id>https://www.explainxkcd.com/wiki/index.php?title=2764:_Cosmological_Nostalgia_Content&amp;diff=313044&amp;oldid=prev</id>
		<title>Prallax: expanded explanation of redshift</title>
		<link rel="alternate" type="text/html" href="https://www.explainxkcd.com/wiki/index.php?title=2764:_Cosmological_Nostalgia_Content&amp;diff=313044&amp;oldid=prev"/>
				<updated>2023-05-13T10:24:44Z</updated>
		
		<summary type="html">&lt;p&gt;expanded explanation of redshift&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr style=&quot;vertical-align: top;&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;Revision as of 10:24, 13 May 2023&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-l12&quot; &gt;Line 12:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 12:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;{{incomplete|1=Created by a z&amp;amp;#61;90s KID - The entire start of this explanation with the made up word multimanteu that has nothing to do with this comic should be changes maybe just deleted! Needs more explanation of what the click bait in the title text refers to in the context of the Einstein blunder and why that belongs in this nostalgia comic. Do NOT delete this tag too soon.}}&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;{{incomplete|1=Created by a z&amp;amp;#61;90s KID - The entire start of this explanation with the made up word multimanteu that has nothing to do with this comic should be changes maybe just deleted! Needs more explanation of what the click bait in the title text refers to in the context of the Einstein blunder and why that belongs in this nostalgia comic. Do NOT delete this tag too soon.}}&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; 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;Like many xkcds, this comic is a figurative {{w|Portmanteau|multimanteau}}, in this case a combination of &amp;quot;{{w|cosmological constant}}&amp;quot; (an astrophysics term to &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;quantify &lt;/del&gt;the &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;rate of &lt;/del&gt;expansion of the universe) and &amp;quot;[https://movementstrategy.com/editorial/nostalgia-social-media/ nostalgia content]&amp;quot; (clickbait marketing aimed at a specific age group referencing pop culture from their youth). The [https://tvtropes.org canonical examples] of nostalgia content are &amp;quot;[https://knowyourmeme.com/memes/only-90s-kids--2 Only 90s Kids Remember...]&amp;quot; and &amp;quot;[https://knowyourmeme.com/memes/feel-old-yet Feel Old yet?]&amp;quot;. Some people of relatively advanced years like to make comparisons to others in their age group of where events that they remember fit into history; e.g., &amp;quot;The first moon landing was closer to the end of World War I than to today.&amp;quot; &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; 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;Like many xkcds, this comic is a figurative {{w|Portmanteau|multimanteau}}, in this case a combination of &amp;quot;{{w|cosmological constant}}&amp;quot; (an astrophysics term &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;related to {{w|dark energy}} and &lt;/ins&gt;to the &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;accelerated {{w|&lt;/ins&gt;expansion of the universe&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;}}&lt;/ins&gt;) and &amp;quot;[https://movementstrategy.com/editorial/nostalgia-social-media/ nostalgia content]&amp;quot; (clickbait marketing aimed at a specific age group referencing pop culture from their youth). The [https://tvtropes.org canonical examples] of nostalgia content are &amp;quot;[https://knowyourmeme.com/memes/only-90s-kids--2 Only 90s Kids Remember...]&amp;quot; and &amp;quot;[https://knowyourmeme.com/memes/feel-old-yet Feel Old yet?]&amp;quot;. Some people of relatively advanced years like to make comparisons to others in their age group of where events that they remember fit into history; e.g., &amp;quot;The first moon landing was closer to the end of World War I than to today.&amp;quot; &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; 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;In cosmology, &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; is the symbol for {{w|Redshift|redshift}}&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;, which is the phenomenon where &lt;/del&gt;photons traveling from an object that is moving away from the observer &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;exhibits &lt;/del&gt;an increase in wavelength, resulting in its color shifting towards the red end of the spectrum. Due to the &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;accelerating &lt;/del&gt;expansion of the universe, objects that are further away from us &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;are &lt;/del&gt;moving away from us at a faster velocity, resulting in higher redshift. As light has finite velocity, it takes a longer time for light from faraway objects to arrive at the observer&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;.&lt;/del&gt;[https://en.wikipedia.org/wiki/Speed_of_light#Spaceflight_and_astronomy] So the light observed at the present must have been emitted by the faraway object further back in time. Megan is stating that only people that &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;appear to the observer with high redshift &lt;/del&gt;(&amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10) &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;will have existed sufficiently further back in the past to &lt;/del&gt;remember when the first stars were still forming. Megan also has a red tint (she is drawn in the color [https://www.color-hex.com/color/462424 #462424], a very dark red; here is a comparison of #462424 and black: &amp;lt;span style=&amp;quot;background-color: #462424&amp;quot;&amp;gt;&amp;amp;emsp;&amp;lt;/span&amp;gt;&amp;amp;thinsp;&amp;lt;span style=&amp;quot;background-color: black&amp;quot;&amp;gt;&amp;amp;emsp;&amp;lt;/span&amp;gt; ), indicating that she is one such &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10 kid. &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;This would mean &lt;/del&gt;that she &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;was &lt;/del&gt;born &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;around 500 million years after the universe was formed, or almost &lt;/del&gt;13 billion years ago&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;. However, the James Webb Space Telescope famously discovered fully formed, large, bright galaxies around &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10 &lt;/del&gt;(&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;of &lt;/del&gt;which &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;the only explanations forthcoming so far are &lt;/del&gt;{{&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;w|primordial black hole&lt;/del&gt;}}&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;s[https://iopscience.iop.org/article/10.3847/2041&lt;/del&gt;-&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;8213/ac927f/meta][https://arxiv&lt;/del&gt;.&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;org/abs/2303.09391] or {{w|axion}} miniclusters[https://journals.aps.org/prd/abstract/10.1103/PhysRevD.107.043502]) so &lt;/del&gt;Megan&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;'s nostalgia may be somewhat confabulatory&lt;/del&gt;.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; 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;In cosmology, &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; is the symbol for {{w|Redshift|redshift}}&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;: &lt;/ins&gt;photons traveling from an object that is moving away from the observer &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;exhibit &lt;/ins&gt;an increase in wavelength, resulting in its color shifting towards the red end of the spectrum&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;, and the variable &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; quantifies the amount of shift&lt;/ins&gt;. Due to the expansion of the universe, objects that are further away from us &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;appear to be &lt;/ins&gt;moving away from us at a faster velocity, resulting in higher redshift. As light has finite velocity, it takes a longer time for light from faraway objects to arrive at the observer[https://en.wikipedia.org/wiki/Speed_of_light#Spaceflight_and_astronomy]&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;. &lt;/ins&gt;So the light observed at the present must have been emitted by the faraway object further back in time&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;. In this sense, after assuming a cosmological model, redshift and cosmic time can be put in a one-to-one relation and are often used interchangeably by astronomers. Redshift &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10 would correspond to about 500 million years after the universe was formed, or almost 13 billion years ago[https://www.astro.ucla.edu/~wright/CosmoCalc.html]&lt;/ins&gt;. Megan is stating that only people that &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;were born at that time &lt;/ins&gt;(&amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10) &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;can &lt;/ins&gt;remember when the first stars were still forming. &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;At redshift &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10 the matter filling the universe was mostly constituted of neutral hydrogen gas, referred by Megan as &amp;quot;cold&amp;quot; (it had a temperature of about 300 K) and &amp;quot;dark&amp;quot; (there were no light sources in the universe before the first stars formed. This epoch is indeed called the [https://en.wikipedia.org/wiki/Timeline_of_the_early_universe#Cosmic_Dark_Age cosmic dark ages]). The ultraviolet light emitted by the first stars started ionizing the hydrogen around them in expanding hot plasma bubbles. This process (called {{w|reionization}}) had probably already begun at &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10, but was really completed only at about &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 6, when the intergalactic hydrogen was completely ionized, as it continues to be at the present day.&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; 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;#160;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; 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;Megan also has a red tint (she is drawn in the color [https://www.color-hex.com/color/462424 #462424], a very dark red; here is a comparison of #462424 and black: &amp;lt;span style=&amp;quot;background-color: #462424&amp;quot;&amp;gt;&amp;amp;emsp;&amp;lt;/span&amp;gt;&amp;amp;thinsp;&amp;lt;span style=&amp;quot;background-color: black&amp;quot;&amp;gt;&amp;amp;emsp;&amp;lt;/span&amp;gt; ), indicating that she is one such &amp;lt;i&amp;gt;z&amp;lt;/i&amp;gt; = 10 kid&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;, because her image is red-shifted, in the literal sense&lt;/ins&gt;. &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;The irony is &lt;/ins&gt;that &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;even if &lt;/ins&gt;she &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;were actually &lt;/ins&gt;born 13 billion years ago (which &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;would be absurd&lt;/ins&gt;{{&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;citation needed&lt;/ins&gt;}}&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;), her image would not appear red&lt;/ins&gt;-&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;shifted to us now&lt;/ins&gt;. &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;She would only appear redshifted to a far away observer looking at the young &lt;/ins&gt;Megan &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;wandering about the primordal cold dark gas&lt;/ins&gt;.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;White Hat, meanwhile, is referencing the fact that the universe has {{w|Scale factor (cosmology)|three eras}}: radiation dominated, matter dominated, and dark energy dominated. As the universe expands, the density of radiation and matter decreases due to their dilution, causing the universe, which first started off being dominated by radiation, to then become dominated by matter, then by dark energy (which does not dilute as the universe expands). Dark energy dominated era, which is when &amp;quot;dark energy started accelerating the universe's expansion&amp;quot; started around 5 billion years ago while {{w|Evolution of bacteria|bacteria evolved around 3 billion years ago}}, meaning that they evolved closer to dark energy domination than to today.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;White Hat, meanwhile, is referencing the fact that the universe has {{w|Scale factor (cosmology)|three eras}}: radiation dominated, matter dominated, and dark energy dominated. As the universe expands, the density of radiation and matter decreases due to their dilution, causing the universe, which first started off being dominated by radiation, to then become dominated by matter, then by dark energy (which does not dilute as the universe expands). Dark energy dominated era, which is when &amp;quot;dark energy started accelerating the universe's expansion&amp;quot; started around 5 billion years ago while {{w|Evolution of bacteria|bacteria evolved around 3 billion years ago}}, meaning that they evolved closer to dark energy domination than to today.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Prallax</name></author>	</entry>

	<entry>
		<id>https://www.explainxkcd.com/wiki/index.php?title=2764:_Cosmological_Nostalgia_Content&amp;diff=312835&amp;oldid=prev</id>
		<title>172.68.154.145: /* Explanation */</title>
		<link rel="alternate" type="text/html" href="https://www.explainxkcd.com/wiki/index.php?title=2764:_Cosmological_Nostalgia_Content&amp;diff=312835&amp;oldid=prev"/>
				<updated>2023-05-11T05:51:20Z</updated>
		
		<summary type="html">&lt;p&gt;‎&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Explanation&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr style=&quot;vertical-align: top;&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;Revision as of 05:51, 11 May 2023&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-l20&quot; &gt;Line 20:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 20:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The title and title text play with the similarity in sound between 'content' and 'constant', segueing between web(page) content and cosmological constant.&amp;#160; &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The title and title text play with the similarity in sound between 'content' and 'constant', segueing between web(page) content and cosmological constant.&amp;#160; &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; 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;The title text refers to Einstein's inclusion of the {{w|Cosmological constant|cosmological constant}} to his theory of general relativity in order to attain a static model of the universe, which he later removed, reportedly referring to it as his &amp;quot;biggest blunder&amp;quot;. Cosmological constant has, today, been generally accepted as a part of the current cosmological model, relating to the concept of dark energy.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; 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;The title text refers to Einstein's inclusion of the {{w|Cosmological constant|cosmological constant}} to his theory of general relativity in order to attain a static model of the universe, which he later removed, reportedly referring to it as his &amp;quot;biggest blunder&amp;quot;. Cosmological constant has, today, been generally accepted as a part of the current cosmological model, relating to the concept of dark energy&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;. It is a pun on content and constant. The title text makes the claim that Einstein actually had cosmological content, which he used to clickbait, and he removed it to renounce clickbait&lt;/ins&gt;.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;==Transcript==&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;==Transcript==&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>172.68.154.145</name></author>	</entry>

	</feed>