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	<title>Cosmic background radiation - Revision history</title>
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	<updated>2026-04-25T06:03:30Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
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		<id>https://wikimd.org/index.php?title=Cosmic_background_radiation&amp;diff=6303635&amp;oldid=prev</id>
		<title>Prab: CSV import</title>
		<link rel="alternate" type="text/html" href="https://wikimd.org/index.php?title=Cosmic_background_radiation&amp;diff=6303635&amp;oldid=prev"/>
		<updated>2025-02-16T22:12:17Z</updated>

		<summary type="html">&lt;p&gt;CSV import&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 22:12, 16 February 2025&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-l25&quot;&gt;Line 25:&lt;/td&gt;
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&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[Category:Radiation]]&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[Category:Radiation]]&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;{{Cosmology-stub}}&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;{{Cosmology-stub}}&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
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&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-side-deleted&quot;&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;File:Cobe-cosmic-background-radiation.gif|COBE Cosmic Background Radiation&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
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		<author><name>Prab</name></author>
	</entry>
	<entry>
		<id>https://wikimd.org/index.php?title=Cosmic_background_radiation&amp;diff=5327977&amp;oldid=prev</id>
		<title>Prab: CSV import</title>
		<link rel="alternate" type="text/html" href="https://wikimd.org/index.php?title=Cosmic_background_radiation&amp;diff=5327977&amp;oldid=prev"/>
		<updated>2024-02-28T23:03:11Z</updated>

		<summary type="html">&lt;p&gt;CSV import&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;&amp;#039;&amp;#039;&amp;#039;Cosmic Background Radiation&amp;#039;&amp;#039;&amp;#039; is the residual radiation that fills the observable universe and is a remnant from an early stage of the universe, also known as the [[Big Bang]]. It is isotropic to roughly one part in 100,000 and has a nearly perfect [[Black body|black-body]] spectrum. It has a temperature of 2.72548±0.00057 K. The Cosmic Background Radiation is an important source of data on the early universe because it is the oldest electromagnetic radiation in the universe, dating to the [[Epoch of Recombination|epoch of recombination]].&lt;br /&gt;
&lt;br /&gt;
== Discovery ==&lt;br /&gt;
The Cosmic Background Radiation was first predicted in 1948 by [[Ralph Alpher]] and [[Robert Herman]]. It was first observed inadvertently in 1965 by [[Arno Penzias]] and [[Robert Wilson]] at the [[Bell Telephone Laboratories]] in Murray Hill, New Jersey. The discovery earned them the 1978 [[Nobel Prize in Physics]].&lt;br /&gt;
&lt;br /&gt;
== Characteristics ==&lt;br /&gt;
The Cosmic Background Radiation is almost perfectly uniform and isotropic. It varies by less than 0.003% in all directions. This uniformity is one strong argument for the [[Big Bang theory]], as it is exactly what the theory predicted.&lt;br /&gt;
&lt;br /&gt;
== Significance ==&lt;br /&gt;
The Cosmic Background Radiation is a snapshot of the universe when it was just 380,000 years old. It provides a unique probe of the conditions of the early universe and the physics that governed its evolution.&lt;br /&gt;
&lt;br /&gt;
== See also ==&lt;br /&gt;
* [[Big Bang]]&lt;br /&gt;
* [[Cosmic microwave background polarization]]&lt;br /&gt;
* [[Cosmic neutrino background]]&lt;br /&gt;
* [[Cosmic infrared background]]&lt;br /&gt;
* [[Cosmic X-ray background]]&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
&amp;lt;references /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[Category:Cosmology]]&lt;br /&gt;
[[Category:Physical cosmology]]&lt;br /&gt;
[[Category:Big Bang]]&lt;br /&gt;
[[Category:Radiation]]&lt;br /&gt;
{{Cosmology-stub}}&lt;/div&gt;</summary>
		<author><name>Prab</name></author>
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