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	<title>Comments on: Q &amp; BA Episode 2: Journey to the Center of the Sun</title>
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	<link>http://blogs.discovermagazine.com/badastronomy/2007/02/11/q-ba-episode-2-journey-to-the-center-of-the-sun/</link>
	<description>I am an astronomer, writer, and skeptic. I likes reality the way it is, and I aims to keep it that way. My real name is Phil Plait, and I run the Bad Astronomy blog.</description>
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		<title>By: Luke</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/11/q-ba-episode-2-journey-to-the-center-of-the-sun/comment-page-1/#comment-29923</link>
		<dc:creator>Luke</dc:creator>
		<pubDate>Mon, 19 Nov 2007 05:46:25 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/11/q-ba-episode-2-journey-to-the-center-of-the-sun/#comment-29923</guid>
		<description>I am sure you know this, but when speaking about Kelvin you don&#039;t use the term degrees</description>
		<content:encoded><![CDATA[<p>I am sure you know this, but when speaking about Kelvin you don&#8217;t use the term degrees</p>
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		<title>By: Jeremy</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/11/q-ba-episode-2-journey-to-the-center-of-the-sun/comment-page-1/#comment-29922</link>
		<dc:creator>Jeremy</dc:creator>
		<pubDate>Wed, 14 Feb 2007 03:39:36 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/11/q-ba-episode-2-journey-to-the-center-of-the-sun/#comment-29922</guid>
		<description>One minor complaint about this clip.  A couple years ago I heard a seminar about acoustic waves in the sun.  The numbers being thrown around for the speed of sound were actually very slow.  I had to stop the speaker and ask why sound was so slow when everything I had heard about the sun was that it was so incredibly dense.  It turned out that most of the sun is actually very low density (I don&#039;t remember exactly, but I want to say 1/20th of the earth&#039;s atmosphere.)  Big numbers are always cool to throw around, but you run the risk of giving the wrong overall picture if you focus on the extremes.</description>
		<content:encoded><![CDATA[<p>One minor complaint about this clip.  A couple years ago I heard a seminar about acoustic waves in the sun.  The numbers being thrown around for the speed of sound were actually very slow.  I had to stop the speaker and ask why sound was so slow when everything I had heard about the sun was that it was so incredibly dense.  It turned out that most of the sun is actually very low density (I don&#8217;t remember exactly, but I want to say 1/20th of the earth&#8217;s atmosphere.)  Big numbers are always cool to throw around, but you run the risk of giving the wrong overall picture if you focus on the extremes.</p>
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		<title>By: ZB</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/11/q-ba-episode-2-journey-to-the-center-of-the-sun/comment-page-1/#comment-29921</link>
		<dc:creator>ZB</dc:creator>
		<pubDate>Wed, 14 Feb 2007 03:28:23 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/11/q-ba-episode-2-journey-to-the-center-of-the-sun/#comment-29921</guid>
		<description>I was very strongly reminded of Carl Sagan with both of these shows. Yay! I hope you keep them coming.</description>
		<content:encoded><![CDATA[<p>I was very strongly reminded of Carl Sagan with both of these shows. Yay! I hope you keep them coming.</p>
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		<title>By: BC</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/11/q-ba-episode-2-journey-to-the-center-of-the-sun/comment-page-1/#comment-29920</link>
		<dc:creator>BC</dc:creator>
		<pubDate>Tue, 13 Feb 2007 02:54:55 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/11/q-ba-episode-2-journey-to-the-center-of-the-sun/#comment-29920</guid>
		<description>Just in case anyone didn&#039;t figure it out: a Hydrogen nucleus is composed of 1 proton.  A Helium nucleus is 2 protons + 2 neutrons.  Take 4 hydrogen, convert 2 protons to 2 neutrons than add the other 2 protons, ending up with the 2 protons + 2 neutrons in a single helium nucleus.</description>
		<content:encoded><![CDATA[<p>Just in case anyone didn&#8217;t figure it out: a Hydrogen nucleus is composed of 1 proton.  A Helium nucleus is 2 protons + 2 neutrons.  Take 4 hydrogen, convert 2 protons to 2 neutrons than add the other 2 protons, ending up with the 2 protons + 2 neutrons in a single helium nucleus.</p>
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		<title>By: Cameron</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/11/q-ba-episode-2-journey-to-the-center-of-the-sun/comment-page-1/#comment-29919</link>
		<dc:creator>Cameron</dc:creator>
		<pubDate>Tue, 13 Feb 2007 02:04:44 +0000</pubDate>
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		<description>Sticks:
Plasma is a superheated, ionized form of gas. It is kind of a &quot;sub-state&quot; of matter.</description>
		<content:encoded><![CDATA[<p>Sticks:<br />
Plasma is a superheated, ionized form of gas. It is kind of a &#8220;sub-state&#8221; of matter.</p>
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		<title>By: schowster</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/11/q-ba-episode-2-journey-to-the-center-of-the-sun/comment-page-1/#comment-29918</link>
		<dc:creator>schowster</dc:creator>
		<pubDate>Tue, 13 Feb 2007 01:12:00 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/11/q-ba-episode-2-journey-to-the-center-of-the-sun/#comment-29918</guid>
		<description>I had a professor in college who said that when you are explaining differences in temperature scales you leave out the &quot;degrees&quot;.

So the difference between 270 K and 300 K = 30 Kelvin
And the difference between 25 C and 50 C = 25 Celsius

But if we go outside and want to know how warm it is, it would be &quot;298 degrees Kelvin&quot;, or &quot;25 degrees Celsius&quot;.

He knew it wasn&#039;t a consensus among the scientific community, but that&#039;s the way he liked to differentiate and I&#039;ve taken a liking to it.</description>
		<content:encoded><![CDATA[<p>I had a professor in college who said that when you are explaining differences in temperature scales you leave out the &#8220;degrees&#8221;.</p>
<p>So the difference between 270 K and 300 K = 30 Kelvin<br />
And the difference between 25 C and 50 C = 25 Celsius</p>
<p>But if we go outside and want to know how warm it is, it would be &#8220;298 degrees Kelvin&#8221;, or &#8220;25 degrees Celsius&#8221;.</p>
<p>He knew it wasn&#8217;t a consensus among the scientific community, but that&#8217;s the way he liked to differentiate and I&#8217;ve taken a liking to it.</p>
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		<title>By: Bryan D.</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/11/q-ba-episode-2-journey-to-the-center-of-the-sun/comment-page-1/#comment-29917</link>
		<dc:creator>Bryan D.</dc:creator>
		<pubDate>Tue, 13 Feb 2007 00:40:25 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/11/q-ba-episode-2-journey-to-the-center-of-the-sun/#comment-29917</guid>
		<description>I love that face you make you you say &quot;and for the rest of the World&quot; :)

Don&#039;t you like Imperial mesurement?? :)</description>
		<content:encoded><![CDATA[<p>I love that face you make you you say &#8220;and for the rest of the World&#8221; <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_smile.gif' alt=':)' class='wp-smiley' /> </p>
<p>Don&#8217;t you like Imperial mesurement?? <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_smile.gif' alt=':)' class='wp-smiley' /> </p>
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