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	<updated>2026-09-14T23:44:00Z</updated>
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		<title>2026年9月13日 (日) 11:23にMiquelElrod3808による</title>
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		<updated>2026-09-13T11:23:40Z</updated>

		<summary type="html">&lt;p&gt;&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;← 古い版&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;2026年9月13日 (日) 20:23時点における版&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l1&quot;&gt;1行目:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;1行目:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;The presence of these weak intermolecular forces &lt;/del&gt;is &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;also revealed by the fact &lt;/del&gt;that, &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;when hydrogen &lt;/del&gt;gas &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;increases from high to reduced pressure &lt;/del&gt;at &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;area temperature, its &lt;/del&gt;temperature level &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;rises, whereas the temperature &lt;/del&gt;of &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;many various &lt;/del&gt;other &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;gases drops&lt;/del&gt;.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;H +3) is &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;located &lt;/del&gt;in the interstellar tool, where it is &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;produced &lt;/del&gt;by ionization of molecular hydrogen from planetary rays This ion has &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;likewise &lt;/del&gt;been observed in the top &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;atmosphere &lt;/del&gt;of Jupiter The ion is long-lived in &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;outer space because of &lt;/del&gt;the low temperature level and thickness. &amp;lt;br&amp;gt;&amp;lt;br&amp;gt;As part of &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;many &lt;/del&gt;carbon &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;compounds&lt;/del&gt;, hydrogen &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;exists &lt;/del&gt;in all animal and veggie &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;cells &lt;/del&gt;and in &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;petroleum&lt;/del&gt;. The Table &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;provides &lt;/del&gt;the &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;crucial &lt;/del&gt;residential properties of molecular hydrogen, &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;H2&lt;/del&gt;. The &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;very low &lt;/del&gt;melting and &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;steaming factors &lt;/del&gt;result from weak forces of &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;destination &lt;/del&gt;in between the molecules.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Amongst atomic kinds, it develops numerous unstable ionized species like a proton &lt;/del&gt;(&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;H+&lt;/del&gt;), a &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;hydride ion (H &lt;/del&gt;−&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;), and &lt;/del&gt;a &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;molecular ion ([https://share.evernote.com/note/92321316-ebff-4aab-066e-c78ece2e7322 h2 chem qa notes]+). Basically pure para-hydrogen can be produced by bringing the mix right into call with charcoal at the temperature level &lt;/del&gt;of &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;liquid hydrogen; this converts all the ortho-hydrogen into para-&lt;/del&gt;hydrogen.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;According to thermodynamic &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;principles&lt;/del&gt;, this &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;suggests &lt;/del&gt;that &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;repulsive &lt;/del&gt;pressures &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;go beyond eye-catching &lt;/del&gt;pressures between hydrogen molecules at &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;space &lt;/del&gt;temperature level-- &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;or else&lt;/del&gt;, the &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;development &lt;/del&gt;would certainly cool the hydrogen. It &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;uses &lt;/del&gt;as an alternative &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;source &lt;/del&gt;of power in the near future (&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;fuel &lt;/del&gt;cells) because of the massive &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;stock &lt;/del&gt;of H2 in the planet's surface water molecules.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Hydrogen&lt;/del&gt;, &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;icon H, molecular formula H2 &lt;/del&gt;is &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;an anemic, odorless, unappetizing, combustible gaseous chemical material in the periodic table. One &lt;/del&gt;of the &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;most essential chemical substance water &lt;/del&gt;(&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;H2O&lt;/del&gt;) &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;is acquired by melting it with oxygen particles&lt;/del&gt;. &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Under regular conditions, &lt;/del&gt;hydrogen &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;gas includes &lt;/del&gt;a &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;set &lt;/del&gt;of &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;atoms or a diatomic particle with a large range &lt;/del&gt;of &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;bonding&lt;/del&gt;.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;In chemistry or chemical scientific research, the hydrogen atom is the only participant of the chemical aspect in which the valence electron is under the straight &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;impact &lt;/del&gt;of the &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;center&lt;/del&gt;. &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;As soon as &lt;/del&gt;stars &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;formed a lot &lt;/del&gt;of the atoms in the intergalactic &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;medium &lt;/del&gt;re-ionized.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Hydrogen is clear to visible light, to infrared light, and to ultraviolet light to wavelengths listed below 1800 Å. Since its molecular weight &lt;/ins&gt;is &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;less than &lt;/ins&gt;that &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;of any other gas&lt;/ins&gt;, &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;its particles have a rate higher than those of any type of other &lt;/ins&gt;gas at &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;a provided &lt;/ins&gt;temperature level &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;and it diffuses faster than any kind &lt;/ins&gt;of other &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;gas&lt;/ins&gt;.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;H +3) is &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;discovered &lt;/ins&gt;in the interstellar tool, where it is &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;generated &lt;/ins&gt;by ionization of molecular hydrogen from planetary rays This ion has &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;actually also &lt;/ins&gt;been observed in the top &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;environment &lt;/ins&gt;of Jupiter The ion is long-lived in &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;celestial spaces due to &lt;/ins&gt;the low temperature level and thickness. &amp;lt;br&amp;gt;&amp;lt;br&amp;gt;As part of &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;innumerable &lt;/ins&gt;carbon &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;substances&lt;/ins&gt;, hydrogen &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;is present &lt;/ins&gt;in all animal and veggie &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;tissue &lt;/ins&gt;and in &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;oil&lt;/ins&gt;. The Table &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;lists &lt;/ins&gt;the &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;important &lt;/ins&gt;residential properties of molecular hydrogen, &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;[https://x.com/JoseWhitl75637/status/2092245130745110805 h2 organic chemistry notes]&lt;/ins&gt;. The &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;exceptionally reduced &lt;/ins&gt;melting and &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;boiling points &lt;/ins&gt;result from weak forces of &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;attraction &lt;/ins&gt;in between the molecules.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;The regular oxidation number or state of hydrogen in chemical substances is +1 yet very electropositive steels &lt;/ins&gt;(&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;alkaline and alkaline earth&lt;/ins&gt;), &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;reveal &lt;/ins&gt;a − &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;1 oxidation state. Electrolysis of water is &lt;/ins&gt;a &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;conceptually easy approach &lt;/ins&gt;of &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;producing &lt;/ins&gt;hydrogen.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;According to thermodynamic &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;concepts&lt;/ins&gt;, this &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;implies &lt;/ins&gt;that &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;undesirable &lt;/ins&gt;pressures &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;exceed appealing &lt;/ins&gt;pressures between hydrogen molecules at &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;area &lt;/ins&gt;temperature level-- &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;otherwise&lt;/ins&gt;, the &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;expansion &lt;/ins&gt;would certainly cool the hydrogen. It &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;utilizes &lt;/ins&gt;as an alternative &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;resource &lt;/ins&gt;of power in the near future (&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;gas &lt;/ins&gt;cells) because of the massive &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;supply &lt;/ins&gt;of H2 in the planet's surface water molecules.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Considering various other truths&lt;/ins&gt;, &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;the digital configuration of hydrogen &lt;/ins&gt;is &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;one electron short &lt;/ins&gt;of the &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;next worthy gas helium &lt;/ins&gt;(&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;He&lt;/ins&gt;). &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Elementary &lt;/ins&gt;hydrogen &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;finds its primary commercial application in the manufacture of ammonia (&lt;/ins&gt;a &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;compound &lt;/ins&gt;of &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;hydrogen and nitrogen, NH3) and in the hydrogenation &lt;/ins&gt;of &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;carbon monoxide gas and organic compounds&lt;/ins&gt;.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;In chemistry or chemical scientific research, the hydrogen atom is the only participant of the chemical aspect in which the valence electron is under the straight &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;influence &lt;/ins&gt;of the &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;nucleus&lt;/ins&gt;. &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Once &lt;/ins&gt;stars &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;developed most &lt;/ins&gt;of the atoms in the intergalactic &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;tool &lt;/ins&gt;re-ionized.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>MiquelElrod3808</name></author>
	</entry>
	<entry>
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		<title>2026年9月11日 (金) 16:11にJordanLegere2による</title>
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		<updated>2026-09-11T16:11:23Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← 古い版&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;2026年9月12日 (土) 01:11時点における版&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l1&quot;&gt;1行目:&lt;/td&gt;
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&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;existence &lt;/del&gt;of these weak intermolecular forces is also &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;disclosed &lt;/del&gt;by the fact that, when hydrogen gas &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;broadens &lt;/del&gt;from high to &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;low &lt;/del&gt;pressure at area temperature &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;level&lt;/del&gt;, its temperature rises, whereas the temperature of many other gases &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;falls&lt;/del&gt;.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;H +3) is &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;discovered &lt;/del&gt;in the interstellar tool, where it is &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;generated &lt;/del&gt;by ionization of molecular hydrogen from planetary rays This ion has likewise been observed in the &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;upper &lt;/del&gt;atmosphere of Jupiter The ion is long-lived in outer space because of the &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;reduced &lt;/del&gt;temperature and &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;density&lt;/del&gt;. &amp;lt;br&amp;gt;&amp;lt;br&amp;gt;As part of &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;countless &lt;/del&gt;carbon compounds, hydrogen exists in all animal and &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;vegetable &lt;/del&gt;cells and in petroleum. The Table &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;details &lt;/del&gt;the &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;essential homes &lt;/del&gt;of molecular hydrogen, H2. The &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;incredibly &lt;/del&gt;low melting and steaming &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;points &lt;/del&gt;result from weak &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;pressures &lt;/del&gt;of &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;attraction &lt;/del&gt;between the &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;particles&lt;/del&gt;.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Among &lt;/del&gt;atomic &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;forms&lt;/del&gt;, it develops &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;various unsteady &lt;/del&gt;ionized &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;types &lt;/del&gt;like a proton (H+), a hydride ion (H −), and a molecular ion (&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;H2&lt;/del&gt;+). &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Essentially &lt;/del&gt;pure para-hydrogen can be &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;generated &lt;/del&gt;by bringing the &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;blend &lt;/del&gt;right into &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;contact &lt;/del&gt;with charcoal at the temperature of &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;fluid &lt;/del&gt;hydrogen; this converts all the ortho-hydrogen &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;right &lt;/del&gt;into para-hydrogen.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;According to thermodynamic principles, this &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;implies &lt;/del&gt;that &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;undesirable &lt;/del&gt;pressures &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;surpass attractive &lt;/del&gt;pressures between hydrogen &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;particles &lt;/del&gt;at &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;room &lt;/del&gt;temperature-- &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;otherwise&lt;/del&gt;, the &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;growth &lt;/del&gt;would cool &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;down &lt;/del&gt;the hydrogen. It uses as an alternative &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;resource &lt;/del&gt;of &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;energy &lt;/del&gt;in the future (&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;gas &lt;/del&gt;cells) &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;as a result &lt;/del&gt;of the &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;big supply &lt;/del&gt;of &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;[https://wefunder.com/feed/374366-o-level-chemistry-homework-help &lt;/del&gt;H2 &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Chemistry Data Booklet] &lt;/del&gt;in the planet's surface water &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;particles&lt;/del&gt;.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Thinking about other facts&lt;/del&gt;, the &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;electronic arrangement of hydrogen is one electron short &lt;/del&gt;of the &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;following honorable gas helium &lt;/del&gt;(&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;He&lt;/del&gt;). &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Elementary &lt;/del&gt;hydrogen &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;locates its primary industrial application in the manufacture &lt;/del&gt;of &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;ammonia (&lt;/del&gt;a &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;compound of hydrogen and nitrogen, NH3) and in the hydrogenation &lt;/del&gt;of &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;carbon monoxide and organic compounds&lt;/del&gt;.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;In chemistry or chemical scientific research, the hydrogen atom is the only &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;member &lt;/del&gt;of the chemical aspect in which the valence electron is under the &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;direct influence &lt;/del&gt;of the &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;nucleus&lt;/del&gt;. As soon as stars &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;created the majority &lt;/del&gt;of the atoms in the intergalactic &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;tool &lt;/del&gt;re-ionized.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;presence &lt;/ins&gt;of these weak intermolecular forces is also &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;revealed &lt;/ins&gt;by the fact that, when hydrogen gas &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;increases &lt;/ins&gt;from high to &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;reduced &lt;/ins&gt;pressure at area temperature, its temperature &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;level &lt;/ins&gt;rises, whereas the temperature of many &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;various &lt;/ins&gt;other gases &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;drops&lt;/ins&gt;.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;H +3) is &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;located &lt;/ins&gt;in the interstellar tool, where it is &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;produced &lt;/ins&gt;by ionization of molecular hydrogen from planetary rays This ion has likewise been observed in the &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;top &lt;/ins&gt;atmosphere of Jupiter The ion is long-lived in outer space because of the &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;low &lt;/ins&gt;temperature &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;level &lt;/ins&gt;and &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;thickness&lt;/ins&gt;. &amp;lt;br&amp;gt;&amp;lt;br&amp;gt;As part of &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;many &lt;/ins&gt;carbon compounds, hydrogen exists in all animal and &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;veggie &lt;/ins&gt;cells and in petroleum. The Table &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;provides &lt;/ins&gt;the &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;crucial residential properties &lt;/ins&gt;of molecular hydrogen, H2. The &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;very &lt;/ins&gt;low melting and steaming &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;factors &lt;/ins&gt;result from weak &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;forces &lt;/ins&gt;of &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;destination in &lt;/ins&gt;between the &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;molecules&lt;/ins&gt;.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Amongst &lt;/ins&gt;atomic &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;kinds&lt;/ins&gt;, it develops &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;numerous unstable &lt;/ins&gt;ionized &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;species &lt;/ins&gt;like a proton (H+), a hydride ion (H −), and a molecular ion (&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;[https://share.evernote.com/note/92321316-ebff-4aab-066e-c78ece2e7322 h2 chem qa notes]&lt;/ins&gt;+). &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Basically &lt;/ins&gt;pure para-hydrogen can be &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;produced &lt;/ins&gt;by bringing the &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;mix &lt;/ins&gt;right into &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;call &lt;/ins&gt;with charcoal at the temperature &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;level &lt;/ins&gt;of &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;liquid &lt;/ins&gt;hydrogen; this converts all the ortho-hydrogen into para-hydrogen.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;According to thermodynamic principles, this &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;suggests &lt;/ins&gt;that &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;repulsive &lt;/ins&gt;pressures &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;go beyond eye-catching &lt;/ins&gt;pressures between hydrogen &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;molecules &lt;/ins&gt;at &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;space &lt;/ins&gt;temperature &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;level&lt;/ins&gt;-- &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;or else&lt;/ins&gt;, the &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;development &lt;/ins&gt;would &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;certainly &lt;/ins&gt;cool the hydrogen. It uses as an alternative &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;source &lt;/ins&gt;of &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;power &lt;/ins&gt;in the &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;near &lt;/ins&gt;future (&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;fuel &lt;/ins&gt;cells) &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;because &lt;/ins&gt;of the &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;massive stock &lt;/ins&gt;of H2 in the planet's surface water &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;molecules&lt;/ins&gt;.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Hydrogen, icon H, molecular formula H2 is an anemic, odorless, unappetizing&lt;/ins&gt;, &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;combustible gaseous chemical material in &lt;/ins&gt;the &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;periodic table. One &lt;/ins&gt;of the &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;most essential chemical substance water &lt;/ins&gt;(&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;H2O&lt;/ins&gt;) &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;is acquired by melting it with oxygen particles&lt;/ins&gt;. &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Under regular conditions, &lt;/ins&gt;hydrogen &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;gas includes a set &lt;/ins&gt;of &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;atoms or a diatomic particle with &lt;/ins&gt;a &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;large range &lt;/ins&gt;of &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;bonding&lt;/ins&gt;.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;In chemistry or chemical scientific research, the hydrogen atom is the only &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;participant &lt;/ins&gt;of the chemical aspect in which the valence electron is under the &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;straight impact &lt;/ins&gt;of the &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;center&lt;/ins&gt;. As soon as stars &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;formed a lot &lt;/ins&gt;of the atoms in the intergalactic &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;medium &lt;/ins&gt;re-ionized.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>JordanLegere2</name></author>
	</entry>
	<entry>
		<id>https://www.xn--3dkvalq0cx455coz1c.com/wiki/index.php?title=Feature_Makes_Use_Of_Information&amp;diff=337053&amp;oldid=prev</id>
		<title>Karri74X446: ページの作成:「The existence of these weak intermolecular forces is also disclosed by the fact that, when hydrogen gas broadens from high to low pressure at area temperature level, its temperature rises, whereas the temperature of many other gases falls.&lt;br&gt;&lt;br&gt;H +3) is discovered in the interstellar tool, where it is generated by ionization of molecular hydrogen from planetary rays This ion has likewise been observed in the upper atmosphere of Jupiter The ion is long-lived in out…」</title>
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		<updated>2026-09-11T04:16:42Z</updated>

		<summary type="html">&lt;p&gt;ページの作成:「The existence of these weak intermolecular forces is also disclosed by the fact that, when hydrogen gas broadens from high to low pressure at area temperature level, its temperature rises, whereas the temperature of many other gases falls.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;H +3) is discovered in the interstellar tool, where it is generated by ionization of molecular hydrogen from planetary rays This ion has likewise been observed in the upper atmosphere of Jupiter The ion is long-lived in out…」&lt;/p&gt;
&lt;p&gt;&lt;b&gt;新規ページ&lt;/b&gt;&lt;/p&gt;&lt;div&gt;The existence of these weak intermolecular forces is also disclosed by the fact that, when hydrogen gas broadens from high to low pressure at area temperature level, its temperature rises, whereas the temperature of many other gases falls.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;H +3) is discovered in the interstellar tool, where it is generated by ionization of molecular hydrogen from planetary rays This ion has likewise been observed in the upper atmosphere of Jupiter The ion is long-lived in outer space because of the reduced temperature and density. &amp;lt;br&amp;gt;&amp;lt;br&amp;gt;As part of countless carbon compounds, hydrogen exists in all animal and vegetable cells and in petroleum. The Table details the essential homes of molecular hydrogen, H2. The incredibly low melting and steaming points result from weak pressures of attraction between the particles.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;Among atomic forms, it develops various unsteady ionized types like a proton (H+), a hydride ion (H −), and a molecular ion (H2+). Essentially pure para-hydrogen can be generated by bringing the blend right into contact with charcoal at the temperature of fluid hydrogen; this converts all the ortho-hydrogen right into para-hydrogen.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;According to thermodynamic principles, this implies that undesirable pressures surpass attractive pressures between hydrogen particles at room temperature-- otherwise, the growth would cool down the hydrogen. It uses as an alternative resource of energy in the future (gas cells) as a result of the big supply of [https://wefunder.com/feed/374366-o-level-chemistry-homework-help H2 Chemistry Data Booklet] in the planet's surface water particles.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;Thinking about other facts, the electronic arrangement of hydrogen is one electron short of the following honorable gas helium (He). Elementary hydrogen locates its primary industrial application in the manufacture of ammonia (a compound of hydrogen and nitrogen, NH3) and in the hydrogenation of carbon monoxide and organic compounds.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;In chemistry or chemical scientific research, the hydrogen atom is the only member of the chemical aspect in which the valence electron is under the direct influence of the nucleus. As soon as stars created the majority of the atoms in the intergalactic tool re-ionized.&lt;/div&gt;</summary>
		<author><name>Karri74X446</name></author>
	</entry>
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