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		<title><![CDATA[io9: Neutron]]></title>
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			<title><![CDATA[io9: Neutron]]></title>
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		<description><![CDATA[io9 posts tagged Neutron]]></description>
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			<title><![CDATA[Neutron star observed creating otherwise impossible form of matter]]></title>
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										<!--  div style="background-color: #B3B3B3; width: 190px; padding: 1px;"><a title="Click here to read Neutron star observed creating otherwise impossible form of matter" href="http://io9.com/astrophysics/" style="background-color:#888888; color:#FFFFFF; font-size:12px;text-align:right; display:block; height:14px; padding:1px 2px; text-decoration:none; text-transform:uppercase; width:156px;"><span style="color: white;" class="hash">#</span><span style="color: white;">astrophysics</span></a></div -->					<div><a title="Click here to read Neutron star observed creating otherwise impossible form of matter" href="http://io9.com/5753303/neutron-star-observed-creating-otherwise-impossible-form-of-matter" class="pp_image">
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				Neutron stars are the unimaginably dense remnants of collapsed giant stars. They get their name because the conditions inside are so fierce that atoms are smashed apart into a soup of protons, electrons, and, yes, neutrons. And now we have the first direct evidence that neutron stars are forming superfluids of neutrons - a totally bizarre state of matter that can't even be created in Earth laboratories.				<a href="http://io9.com/5753303/neutron-star-observed-creating-otherwise-impossible-form-of-matter" title="Click here to read more about Neutron star observed creating otherwise impossible form of matter">More&nbsp;&raquo;</a>
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			<link><![CDATA[http://io9.com/5753303/neutron-star-observed-creating-otherwise-impossible-form-of-matter]]></link>			<guid isPermaLink="false"><![CDATA[io9-5753303]]></guid>
			<category><![CDATA[astrophysics]]></category>
			<category><![CDATA[Astronomy]]></category>
			<category><![CDATA[Matter]]></category>
			<category><![CDATA[neutron]]></category>
			<category><![CDATA[neutron star]]></category>
			<category><![CDATA[Physics]]></category>
			<category><![CDATA[Science]]></category>
			<category><![CDATA[superfluid]]></category>
			<pubDate><![CDATA[Sun, 06 Feb 2011 13:20:00 PST]]></pubDate>
			<dc:creator><![CDATA[Alasdair Wilkins]]></dc:creator>
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			<title><![CDATA[The Ultimate Field Guide to Subatomic Particles]]></title>
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										<!--  div style="background-color: #B3B3B3; width: 190px; padding: 1px;"><a title="Click here to read The Ultimate Field Guide to Subatomic Particles" href="http://io9.com/io9-backgrounder/" style="background-color:#888888; color:#FFFFFF; font-size:12px;text-align:right; display:block; height:14px; padding:1px 2px; text-decoration:none; text-transform:uppercase; width:156px;"><span style="color: white;" class="hash">#</span><span style="color: white;">io9backgrounder</span></a></div -->					<div><a title="Click here to read The Ultimate Field Guide to Subatomic Particles" href="http://io9.com/5639192/the-ultimate-field-guide-to-subatomic-particles" class="pp_image">
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				 Muons, neutrinos, supersymmetric partners, the infamous Higgs boson - with so many different subatomic particles flying about, it's no wonder theoretical physics can be so confusing. That's why we made this (reasonably) simple guide to all the different elementary particles.				<a href="http://io9.com/5639192/the-ultimate-field-guide-to-subatomic-particles" title="Click here to read more about The Ultimate Field Guide to Subatomic Particles">More&nbsp;&raquo;</a>
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			<category><![CDATA[Io9 backgrounder]]></category>
			<category><![CDATA[Electron]]></category>
			<category><![CDATA[Elementary particles]]></category>
			<category><![CDATA[Neutrino]]></category>
			<category><![CDATA[neutron]]></category>
			<category><![CDATA[Particle physics]]></category>
			<category><![CDATA[photon]]></category>
			<category><![CDATA[Physics]]></category>
			<category><![CDATA[Proton]]></category>
			<category><![CDATA[Quantum Mechanics]]></category>
			<category><![CDATA[Science]]></category>
			<category><![CDATA[standard model]]></category>
			<category><![CDATA[Subatomic particles]]></category>
			<category><![CDATA[Top]]></category>
			<pubDate><![CDATA[Thu, 16 Sep 2010 10:44:24 PDT]]></pubDate>
			<dc:creator><![CDATA[Alasdair Wilkins]]></dc:creator>
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			<title><![CDATA[We Can Predict When Stars Will Explode]]></title>
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										<!--  div style="background-color: #B3B3B3; width: 190px; padding: 1px;"><a title="Click here to read We Can Predict When Stars Will Explode" href="http://io9.com/space-porn/" style="background-color:#888888; color:#FFFFFF; font-size:12px;text-align:right; display:block; height:14px; padding:1px 2px; text-decoration:none; text-transform:uppercase; width:156px;"><span style="color: white;" class="hash">#</span><span style="color: white;">spaceporn</span></a></div -->					<div><a title="Click here to read We Can Predict When Stars Will Explode" href="http://io9.com/385853/we-can-predict-when-stars-will-explode" class="pp_image">
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				 Need to get rid of a bunch of space trash, or jumpstart a wormhole? Now you can, at least if you can get near enough to a neutron star when it's heading into explosion mode. Using NASA's Rossi X-ray Timing Explorer (RXTE), some astronomers have made an extraordinary breakthrough: they've discovered how to predict when neutron stars will unleash massive explosions. What this means, in essence, is that stellar explosions can be compared to Old Faithful, the geyser in Yellowstone Park that erupts at precise times. 				<a href="http://io9.com/385853/we-can-predict-when-stars-will-explode" title="Click here to read more about We Can Predict When Stars Will Explode">More&nbsp;&raquo;</a>
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			<category><![CDATA[space porn]]></category>
			<category><![CDATA[astrophysics]]></category>
			<category><![CDATA[Explosions]]></category>
			<category><![CDATA[neutron]]></category>
			<category><![CDATA[Physics]]></category>
			<category><![CDATA[Science]]></category>
			<category><![CDATA[Stars]]></category>
			<pubDate><![CDATA[Wed, 30 Apr 2008 13:21:09 PDT]]></pubDate>
			<dc:creator><![CDATA[Annalee Newitz]]></dc:creator>
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