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	<title>Comments on: Well, Here&#8217;s a Pretty Good Use</title>
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	<link>https://blog.speculist.com/space/well-heres-a-pr.html</link>
	<description>Live to see it.</description>
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		<title>By: Engineer-Poet</title>
		<link>https://blog.speculist.com/space/well-heres-a-pr.html#comment-262</link>
		<dc:creator>Engineer-Poet</dc:creator>
		<pubDate>Fri, 18 Feb 2005 23:15:35 +0000</pubDate>
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		<description><![CDATA[I disagree; such planets WILL be tide-locked.&#160; Here&#039;s my reasoning:

&lt;ol&gt;&lt;li&gt;Tidal effects scale as the inverse cube of distance from the primary.&lt;/li&gt;
&lt;li&gt;You have to get roughly the same total energy flux at your planet.&#160; If you replace a 5700 K primary star with a 2000 K brown dwarf, you&#039;ll have to move roughly 12 times as close (before accounting for the smaller diameter of the dwarf).&lt;/li&gt;
&lt;li&gt;Ergo, the tides increase by a factor of ~1700 due the decreased surface irradiance alone; even if the dwarf was 1/50 solar mass you&#039;d still have 34 times as much tidal effect as Earth sees.&lt;/li&gt;
&lt;li&gt;If the BD is 1/4 solar diameter, cut the orbital distance by another factor of 4 and multiply the tidal effect by a further factor of 64.&lt;/li&gt;&lt;/ol&gt;So no, I can&#039;t see how a planet circling a brown dwarf and capable of holding liquid water anywhere on its surface could fail to be tide-locked, with all the complications for life that this implies.]]></description>
		<content:encoded><![CDATA[<p>I disagree; such planets WILL be tide-locked.&nbsp; Here&#8217;s my reasoning:</p>
<ol>
<li>Tidal effects scale as the inverse cube of distance from the primary.</li>
<li>You have to get roughly the same total energy flux at your planet.&nbsp; If you replace a 5700 K primary star with a 2000 K brown dwarf, you&#8217;ll have to move roughly 12 times as close (before accounting for the smaller diameter of the dwarf).</li>
<li>Ergo, the tides increase by a factor of ~1700 due the decreased surface irradiance alone; even if the dwarf was 1/50 solar mass you&#8217;d still have 34 times as much tidal effect as Earth sees.</li>
<li>If the BD is 1/4 solar diameter, cut the orbital distance by another factor of 4 and multiply the tidal effect by a further factor of 64.</li>
</ol>
<p>So no, I can&#8217;t see how a planet circling a brown dwarf and capable of holding liquid water anywhere on its surface could fail to be tide-locked, with all the complications for life that this implies.</p>
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		<title>By: Stephen Gordon</title>
		<link>https://blog.speculist.com/space/well-heres-a-pr.html#comment-261</link>
		<dc:creator>Stephen Gordon</dc:creator>
		<pubDate>Thu, 10 Feb 2005 12:42:12 +0000</pubDate>
		<guid isPermaLink="false">http://localhost/specblog/?p=213#comment-261</guid>
		<description><![CDATA[AndrewS:

My layman&#039;s guess is no.  And for the same reason the year wouldn&#039;t have to be superfast.

The mass of the brown drawf is so much less than our sun that a planet could be 21 times closer, but still not have locked tides.

Of course the planet itself has to be in a narrow size range.  If its too big it will have locked tides.  If its too small it won&#039;t be able to hold an atmosphere.]]></description>
		<content:encoded><![CDATA[<p>AndrewS:</p>
<p>My layman&#8217;s guess is no.  And for the same reason the year wouldn&#8217;t have to be superfast.</p>
<p>The mass of the brown drawf is so much less than our sun that a planet could be 21 times closer, but still not have locked tides.</p>
<p>Of course the planet itself has to be in a narrow size range.  If its too big it will have locked tides.  If its too small it won&#8217;t be able to hold an atmosphere.</p>
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		<title>By: AndrewS</title>
		<link>https://blog.speculist.com/space/well-heres-a-pr.html#comment-260</link>
		<dc:creator>AndrewS</dc:creator>
		<pubDate>Thu, 10 Feb 2005 09:07:10 +0000</pubDate>
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		<description><![CDATA[Another question for any astrophysicists out there. Would planets in the liquid-water range of brown dwarfs be tidally locked?]]></description>
		<content:encoded><![CDATA[<p>Another question for any astrophysicists out there. Would planets in the liquid-water range of brown dwarfs be tidally locked?</p>
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	<item>
		<title>By: Stephen Gordon</title>
		<link>https://blog.speculist.com/space/well-heres-a-pr.html#comment-259</link>
		<dc:creator>Stephen Gordon</dc:creator>
		<pubDate>Wed, 09 Feb 2005 09:08:49 +0000</pubDate>
		<guid isPermaLink="false">http://localhost/specblog/?p=213#comment-259</guid>
		<description><![CDATA[I&#039;m not sure how much darker it would be.  A brown dwarf doesn&#039;t shine much, but habitable planets would be about 21 times closer to their dwarf than we are to our sun (150 million v. 7 million kilometers).

I&#039;m guessing that planets 21 times closer to their sun would revolve around their star 21 times as fast.  They&#039;d be celebrating New Year every 17 days.  :-)     

Wait, that&#039;s probably not right.  Planets 21 times closer to OUR sun would have to revolve 21 times as fast.  But a brown dwarf has much less mass than our star.  Planets in a brown dwarf habitable zone might have a similar length year to ours.  Somebody help me out with this.  Engineer Poet?

Assuming life could get started in such a place (which assumes that the development of life doesn&#039;t require radiation peculiar to our sort of sun), native life would adapt to that lighting condition.  Maybe they would have huge eyes, or a sonar sense, or eyes adapted to a different spectrum.

Finding earth-like planets around brown dwarves would be easier because brown dwarves are dimmer, but also harder because earth-like planets with liquid water would have to be so close.]]></description>
		<content:encoded><![CDATA[<p>I&#8217;m not sure how much darker it would be.  A brown dwarf doesn&#8217;t shine much, but habitable planets would be about 21 times closer to their dwarf than we are to our sun (150 million v. 7 million kilometers).</p>
<p>I&#8217;m guessing that planets 21 times closer to their sun would revolve around their star 21 times as fast.  They&#8217;d be celebrating New Year every 17 days.  <img src='https://blog.speculist.com/wp-includes/images/smilies/icon_smile.gif' alt=':-)' class='wp-smiley' />      </p>
<p>Wait, that&#8217;s probably not right.  Planets 21 times closer to OUR sun would have to revolve 21 times as fast.  But a brown dwarf has much less mass than our star.  Planets in a brown dwarf habitable zone might have a similar length year to ours.  Somebody help me out with this.  Engineer Poet?</p>
<p>Assuming life could get started in such a place (which assumes that the development of life doesn&#8217;t require radiation peculiar to our sort of sun), native life would adapt to that lighting condition.  Maybe they would have huge eyes, or a sonar sense, or eyes adapted to a different spectrum.</p>
<p>Finding earth-like planets around brown dwarves would be easier because brown dwarves are dimmer, but also harder because earth-like planets with liquid water would have to be so close.</p>
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