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	<title>Comments on: disks</title>
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	<description>characterizing planetary systems</description>
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		<title>By: systemic - Lonely Planet Guide to the Hyades</title>
		<link>http://oklo.org/2006/02/09/disks/comment-page-1/#comment-1106</link>
		<dc:creator>systemic - Lonely Planet Guide to the Hyades</dc:creator>
		<pubDate>Fri, 09 Feb 2007 07:43:12 +0000</pubDate>
		<guid isPermaLink="false">http://oklo.org/?p=38#comment-1106</guid>
		<description>[...] For more information, this series: 1, 2, 3, 4 and 5, 6, and 7. of oklo posts that compare and contrast the gravitational instability and core accretion theories for giant planet formation. [...]</description>
		<content:encoded><![CDATA[<p>[...] For more information, this series: 1, 2, 3, 4 and 5, 6, and 7. of oklo posts that compare and contrast the gravitational instability and core accretion theories for giant planet formation. [...]</p>
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		<title>By: systemic - Zoom</title>
		<link>http://oklo.org/2006/02/09/disks/comment-page-1/#comment-174</link>
		<dc:creator>systemic - Zoom</dc:creator>
		<pubDate>Fri, 23 Jun 2006 05:43:59 +0000</pubDate>
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		<description>[...] In this post last February, I wrote about the protostellar disks in Orion that were imaged by the Hubble Space Telescope in the mid-1990s. One of these disks has achieved nearly iconic status (at least among those who give talks on planet formation). The following image shows it viewed edge-on and in silhouette against a background of glowing nebular gas. Only a faint smudge of red hints at the central star embedded within the disk. [...]</description>
		<content:encoded><![CDATA[<p>[...] In this post last February, I wrote about the protostellar disks in Orion that were imaged by the Hubble Space Telescope in the mid-1990s. One of these disks has achieved nearly iconic status (at least among those who give talks on planet formation). The following image shows it viewed edge-on and in silhouette against a background of glowing nebular gas. Only a faint smudge of red hints at the central star embedded within the disk. [...]</p>
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		<title>By: systemic - G.I. No</title>
		<link>http://oklo.org/2006/02/09/disks/comment-page-1/#comment-103</link>
		<dc:creator>systemic - G.I. No</dc:creator>
		<pubDate>Tue, 02 May 2006 02:34:58 +0000</pubDate>
		<guid isPermaLink="false">http://oklo.org/?p=38#comment-103</guid>
		<description>[...] To be fair, there are also some thorny problems associated with core-accretion. In the next few posts of the giant planet formation series [1, 2, 3, 4 and 5] that we&#8217;ve been running, I&#8217;ll describe these in more detail. [...]</description>
		<content:encoded><![CDATA[<p>[...] To be fair, there are also some thorny problems associated with core-accretion. In the next few posts of the giant planet formation series [1, 2, 3, 4 and 5] that we&#8217;ve been running, I&#8217;ll describe these in more detail. [...]</p>
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		<title>By: systemic - Q</title>
		<link>http://oklo.org/2006/02/09/disks/comment-page-1/#comment-68</link>
		<dc:creator>systemic - Q</dc:creator>
		<pubDate>Sat, 15 Apr 2006 21:57:52 +0000</pubDate>
		<guid isPermaLink="false">http://oklo.org/?p=38#comment-68</guid>
		<description>[...] This post continues the oklo.org posts: (1) the black cloud, and (2) disks. [...]</description>
		<content:encoded><![CDATA[<p>[...] This post continues the oklo.org posts: (1) the black cloud, and (2) disks. [...]</p>
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