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	<title>Comments on: i wish i had an evil twin</title>
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	<link>http://oklo.org/2005/12/21/i-wish-i-had-an-evil-twin/</link>
	<description>characterizing planetary systems</description>
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		<title>By: systemic - extrasolar trojans</title>
		<link>http://oklo.org/2005/12/21/i-wish-i-had-an-evil-twin/comment-page-1/#comment-373</link>
		<dc:creator>systemic - extrasolar trojans</dc:creator>
		<pubDate>Wed, 11 Oct 2006 20:44:50 +0000</pubDate>
		<guid isPermaLink="false">http://oklo.org/?p=24#comment-373</guid>
		<description>[...] Last week, during my visit to Harvard CfA, I talked to Eric Ford, who has been exploring the idea searching for trojan companions to extrasolar planets. He pointed out that the discovery of a body in a trojan configuration with a known extrasolar planet would provide an important test of theories of hot Jupiter formation. [...]</description>
		<content:encoded><![CDATA[<p>[...] Last week, during my visit to Harvard CfA, I talked to Eric Ford, who has been exploring the idea searching for trojan companions to extrasolar planets. He pointed out that the discovery of a body in a trojan configuration with a known extrasolar planet would provide an important test of theories of hot Jupiter formation. [...]</p>
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		<title>By: systemic - and inside the second envelope&#8230;</title>
		<link>http://oklo.org/2005/12/21/i-wish-i-had-an-evil-twin/comment-page-1/#comment-363</link>
		<dc:creator>systemic - and inside the second envelope&#8230;</dc:creator>
		<pubDate>Mon, 09 Oct 2006 00:34:46 +0000</pubDate>
		<guid isPermaLink="false">http://oklo.org/?p=24#comment-363</guid>
		<description>[...] [For more about 1:1 resonances, see this post and this post. For a discussion about the audio wave forms that they produce, see this post.] [...]</description>
		<content:encoded><![CDATA[<p>[...] [For more about 1:1 resonances, see this post and this post. For a discussion about the audio wave forms that they produce, see this post.] [...]</p>
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		<title>By: Centauri Dreams &#187; Blog Archive &#187; Systemic: Working with Extrasolar Data</title>
		<link>http://oklo.org/2005/12/21/i-wish-i-had-an-evil-twin/comment-page-1/#comment-19</link>
		<dc:creator>Centauri Dreams &#187; Blog Archive &#187; Systemic: Working with Extrasolar Data</dc:creator>
		<pubDate>Thu, 29 Dec 2005 14:58:26 +0000</pubDate>
		<guid isPermaLink="false">http://oklo.org/?p=24#comment-19</guid>
		<description>[...] Be aware, too, that the Systemic site contains an ongoing weblog laced not only with gorgeous photography but Laughlin&#8217;s insightful posts, the most recent of which discusses, in addition to the Lagrangian points associated with Jupiter and the Sun, the question of whether a stable orbit exists on the opposite side of the Sun from the Earth and in the Sun&#8217;s habitable zone &#8212; a twin of Earth, in other words. The intriguing result is that such an orbit is nonlinearly stable. Laughlin describes the scenario this way: As one planet tries to pass the other one up, it receives a forward gravitational pull. This forward pull gives the planet energy, which causes it to move to a larger-radius orbit, which causes its orbital period to increase, which causes it to begin to lag behind. Likewise, the planet which is about to be passed up receives a backward gravitational pull. This backward pull drains energy from the orbit, causes the semi-major axis to decrease, and causes the period to get shorter. The two planets are thus able to toss a bit of their joint orbital energy back and forth like a hot potato, and orbit in a perfectly stable variety of a 1:1 orbital resonance, known as a horseshoe configuration. The horseshoe orbit is an example of the negative heat capacity of self-gravitating systems, which is one of the most important concepts in astrophysics: If you try to drain heat away from a self gravitating object, it gets hotter. [...]</description>
		<content:encoded><![CDATA[<p>[...] Be aware, too, that the Systemic site contains an ongoing weblog laced not only with gorgeous photography but Laughlin&#8217;s insightful posts, the most recent of which discusses, in addition to the Lagrangian points associated with Jupiter and the Sun, the question of whether a stable orbit exists on the opposite side of the Sun from the Earth and in the Sun&#8217;s habitable zone &#8212; a twin of Earth, in other words. The intriguing result is that such an orbit is nonlinearly stable. Laughlin describes the scenario this way: As one planet tries to pass the other one up, it receives a forward gravitational pull. This forward pull gives the planet energy, which causes it to move to a larger-radius orbit, which causes its orbital period to increase, which causes it to begin to lag behind. Likewise, the planet which is about to be passed up receives a backward gravitational pull. This backward pull drains energy from the orbit, causes the semi-major axis to decrease, and causes the period to get shorter. The two planets are thus able to toss a bit of their joint orbital energy back and forth like a hot potato, and orbit in a perfectly stable variety of a 1:1 orbital resonance, known as a horseshoe configuration. The horseshoe orbit is an example of the negative heat capacity of self-gravitating systems, which is one of the most important concepts in astrophysics: If you try to drain heat away from a self gravitating object, it gets hotter. [...]</p>
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