<?xml version="1.0" encoding="UTF-8"?><rss version="2.0"
	xmlns:content="http://purl.org/rss/1.0/modules/content/"
	xmlns:dc="http://purl.org/dc/elements/1.1/"
	xmlns:atom="http://www.w3.org/2005/Atom"
	xmlns:sy="http://purl.org/rss/1.0/modules/syndication/"
		>
<channel>
	<title>Comments on: Chapter 3 Study Guide Question #6 &#8212; Describe the &#8220;fate&#8221; of most solar energy that reaches the Earth.</title>
	<atom:link href="http://pdsblogs.org/pdsapes810/2009/10/06/chapter-3-study-guide-question-6-describe-the-fate-of-most-solar-energy-that-reaches-the-earth/feed/" rel="self" type="application/rss+xml" />
	<link>http://pdsblogs.org/pdsapes810/2009/10/06/chapter-3-study-guide-question-6-describe-the-fate-of-most-solar-energy-that-reaches-the-earth/</link>
	<description>...just a drop in the ocean...</description>
	<lastBuildDate>Sat, 02 Feb 2013 20:35:11 +0000</lastBuildDate>
	<sy:updatePeriod>hourly</sy:updatePeriod>
	<sy:updateFrequency>1</sy:updateFrequency>
	<generator>http://pdsblogs.org/?v=3.4.1</generator>
	<item>
		<title>By: derrickwillard</title>
		<link>http://pdsblogs.org/pdsapes810/2009/10/06/chapter-3-study-guide-question-6-describe-the-fate-of-most-solar-energy-that-reaches-the-earth/comment-page-1/#comment-69</link>
		<dc:creator>derrickwillard</dc:creator>
		<pubDate>Wed, 07 Oct 2009 02:56:47 +0000</pubDate>
		<guid isPermaLink="false">http://pdsblogs.org/pdsapes810/?p=236#comment-69</guid>
		<description>Great question.  No concern for tomorrow.  The electromagnetic spectrum is disrupted in many ways as it is emitted from the sun.  We&#039;ll deal with the &quot;fate&quot; of all the energy eventually. For now, appreciate that very little reaches the Earth (but just enough for life), and that when it arrives produces rather inefficiently store it in glucose.  Then, most of that is wasted as heat by the fourth trophic level (2nd Law of Thermodynamics)!</description>
		<content:encoded><![CDATA[<p>Great question.  No concern for tomorrow.  The electromagnetic spectrum is disrupted in many ways as it is emitted from the sun.  We&#8217;ll deal with the &#8220;fate&#8221; of all the energy eventually. For now, appreciate that very little reaches the Earth (but just enough for life), and that when it arrives produces rather inefficiently store it in glucose.  Then, most of that is wasted as heat by the fourth trophic level (2nd Law of Thermodynamics)!</p>
]]></content:encoded>
	</item>
</channel>
</rss>
