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	<title>Tricarbon - Revision history</title>
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	<updated>2026-04-24T22:06:36Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
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		<id>https://wikimd.org/index.php?title=Tricarbon&amp;diff=5624179&amp;oldid=prev</id>
		<title>Prab: CSV import</title>
		<link rel="alternate" type="text/html" href="https://wikimd.org/index.php?title=Tricarbon&amp;diff=5624179&amp;oldid=prev"/>
		<updated>2024-04-18T02:43:00Z</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;[[File:Tricarbon-3D-vdW.png|Tricarbon-3D-vdW|thumb]] &amp;#039;&amp;#039;&amp;#039;Tricarbon&amp;#039;&amp;#039;&amp;#039; ([[chemical formula]]: C₃) is a [[molecule]] composed of three [[carbon]] atoms. It is a linear molecule and is considered a [[cumulene]]. Tricarbon is of interest in the field of [[astrochemistry]] and is observed in the [[interstellar medium]], where it is formed by [[photochemical]] reactions. This molecule is also relevant in the study of [[combustion]] processes and can be found in [[carbon stars]].&lt;br /&gt;
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==Properties==&lt;br /&gt;
Tricarbon is a radical molecule, meaning it has unpaired [[electron]]s, making it highly reactive. Its electronic structure is characterized by a linear arrangement of carbon atoms, indicative of sp hybridization. The molecule exists in several [[isomer]]s, but the linear form is the most stable and common in the interstellar medium.&lt;br /&gt;
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==Formation==&lt;br /&gt;
In the interstellar medium, tricarbon is formed through the photo-dissociation of larger carbon-containing molecules or by the reactions between carbon or carbon monoxide with other carbon species. These processes are influenced by the presence of [[ultraviolet]] (UV) light, which is abundant in space.&lt;br /&gt;
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==Detection==&lt;br /&gt;
Tricarbon has been detected in space using [[spectroscopy]], specifically through its emission lines in the microwave region. Its presence in the interstellar medium provides clues about the chemical processes occurring in space and the formation of complex organic molecules.&lt;br /&gt;
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==Significance==&lt;br /&gt;
The study of tricarbon and other small carbon chains helps scientists understand the chemistry of the early universe and the formation of life-essential molecules like [[amino acids]] and [[nucleotides]]. Tricarbon&amp;#039;s reactivity also makes it a subject of interest in understanding combustion processes and the formation of [[soot]] and other pollutants.&lt;br /&gt;
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==See also==&lt;br /&gt;
* [[Carbon]]&lt;br /&gt;
* [[Astrochemistry]]&lt;br /&gt;
* [[Interstellar medium]]&lt;br /&gt;
* [[Spectroscopy]]&lt;br /&gt;
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[[Category:Chemical compounds]]&lt;br /&gt;
[[Category:Astrochemistry]]&lt;br /&gt;
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{{chemistry-stub}}&lt;/div&gt;</summary>
		<author><name>Prab</name></author>
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