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	<title>Comments on: Astronomers Now Looking For Exomoons Around Exoplanets</title>
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	<link>http://www.universetoday.com/2008/12/14/astronomers-now-looking-for-exomoons-around-exoplanets/</link>
	<description>Space and astronomy news</description>
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		<title>By: ROCA</title>
		<link>http://www.universetoday.com/2008/12/14/astronomers-now-looking-for-exomoons-around-exoplanets/comment-page-2/#comment-52081</link>
		<dc:creator>ROCA</dc:creator>
		<pubDate>Mon, 02 Feb 2009 00:00:17 +0000</pubDate>
		<guid isPermaLink="false">http://www.universetoday.com/?p=22299#comment-52081</guid>
		<description>Hi Ian,
I have a huge interest in extrasolar moons as they solve the problem that an exoplanet inside the habitability zone of a red dwarf star has: tidal locking.
In this scenario a gas giant may be tidal locked to the parent star but the exomoon is not. So the exomoon should have a better climate and may be suitable for life.
A tellurian planet inside the habitability zone is always tidal locked and it is a bad handicap for life as we know it.
Of course a red dwarf creates other problems: emission in infrared and terrible solar storms (solar flares) but this is another theme of discussion.
I translated your great article to Portuguese and here is the link:

Astrônomos começam a caça de exoluas orbitando exoplanetas
http://eternosaprendizes.wordpress.com/2009/02/01/astronomos-comecam-a-caca-de-exoluas-orbitando-exoplanetas/
So, let’s find the exomoons!
Tks
ROCA (Brazil)</description>
		<content:encoded><![CDATA[<p>Hi Ian,<br />
I have a huge interest in extrasolar moons as they solve the problem that an exoplanet inside the habitability zone of a red dwarf star has: tidal locking.<br />
In this scenario a gas giant may be tidal locked to the parent star but the exomoon is not. So the exomoon should have a better climate and may be suitable for life.<br />
A tellurian planet inside the habitability zone is always tidal locked and it is a bad handicap for life as we know it.<br />
Of course a red dwarf creates other problems: emission in infrared and terrible solar storms (solar flares) but this is another theme of discussion.<br />
I translated your great article to Portuguese and here is the link:</p>
<p>Astrônomos começam a caça de exoluas orbitando exoplanetas<br />
<a href="http://eternosaprendizes.wordpress.com/2009/02/01/astronomos-comecam-a-caca-de-exoluas-orbitando-exoplanetas/" rel="nofollow">http://eternosaprendizes.wordpress.com/2009/02/01/astronomos-comecam-a-caca-de-exoluas-orbitando-exoplanetas/</a><br />
So, let’s find the exomoons!<br />
Tks<br />
ROCA (Brazil)</p>
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		<title>By: dollhopf</title>
		<link>http://www.universetoday.com/2008/12/14/astronomers-now-looking-for-exomoons-around-exoplanets/comment-page-2/#comment-46671</link>
		<dc:creator>dollhopf</dc:creator>
		<pubDate>Wed, 17 Dec 2008 15:52:14 +0000</pubDate>
		<guid isPermaLink="false">http://www.universetoday.com/?p=22299#comment-46671</guid>
		<description>DJ Barney told me:

&lt;em&gt;&#039;&quot;exocreatures&quot; .. I like it ! That other word has become sort of … xenophobic ?&#039;&lt;/em&gt;

Yes, but I wonder about when the first manned spaceship will be designed to also carry weapons onboard. Will there once be a need to defend against or dominate over other &quot;earthlings&quot; during missions in space? Or will weapon systems once be integrated into space exploration vehicles or armament be foreseen in view of some &quot;strange&quot; (alien) events?</description>
		<content:encoded><![CDATA[<p>DJ Barney told me:</p>
<p><em>&#039;&#034;exocreatures&#034; .. I like it ! That other word has become sort of … xenophobic ?&#039;</em></p>
<p>Yes, but I wonder about when the first manned spaceship will be designed to also carry weapons onboard. Will there once be a need to defend against or dominate over other &#034;earthlings&#034; during missions in space? Or will weapon systems once be integrated into space exploration vehicles or armament be foreseen in view of some &#034;strange&#034; (alien) events?</p>
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		<title>By: Jorge</title>
		<link>http://www.universetoday.com/2008/12/14/astronomers-now-looking-for-exomoons-around-exoplanets/comment-page-2/#comment-46541</link>
		<dc:creator>Jorge</dc:creator>
		<pubDate>Tue, 16 Dec 2008 14:12:13 +0000</pubDate>
		<guid isPermaLink="false">http://www.universetoday.com/?p=22299#comment-46541</guid>
		<description>Ah! NOW it makes perfect sense! Thanks for the explanation and the best of luck for the experiment.</description>
		<content:encoded><![CDATA[<p>Ah! NOW it makes perfect sense! Thanks for the explanation and the best of luck for the experiment.</p>
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		<title>By: David Kipping</title>
		<link>http://www.universetoday.com/2008/12/14/astronomers-now-looking-for-exomoons-around-exoplanets/comment-page-2/#comment-46528</link>
		<dc:creator>David Kipping</dc:creator>
		<pubDate>Tue, 16 Dec 2008 11:47:13 +0000</pubDate>
		<guid isPermaLink="false">http://www.universetoday.com/?p=22299#comment-46528</guid>
		<description>Hello all,

I have noticed some confusion about how the method works so I thought I would briefly summarise the idea.  I&#039;m very happy to see so many interesting discussions on the topic!

The key point to bear in mind is that we are looking at the wobble of the planet, not the the wobble of the star.  Every time a planet transits the star, it affords us information about the position and velocity of the planet.  Even if the moon is too small to show up in the transit lightcurve, its effects on the host planet are not.

Both the position and velocity of the planet will be perturbed by the presence of a moon.  The spatial perturbation causes the planetary transit to occur slightly earlier or slightly later than expected.  The velocity perturbation causes the transit duration to be slightly greater or slightly smaller.  Remarkably, these effects can be minutes in magnitude.

The two effects, called transit time variation (TTV) and transit duration variation (TDV) always exhibit a 90 degrees phase difference.  In other words, we have a quite unique signature.  In addition, the ratio of the two amplitudes allows for a determination of both the moon&#039;s mass and its orbital distance from the host planet.

It&#039;s really fantastic to see so many people interested in exomoons.  Who knows how common these exomoons may be and what potential for habitability they possess!  Ultimately, the only way for us to answer these questions is to start looking!

All the best and continue to ask questions!
David</description>
		<content:encoded><![CDATA[<p>Hello all,</p>
<p>I have noticed some confusion about how the method works so I thought I would briefly summarise the idea.  I&#039;m very happy to see so many interesting discussions on the topic!</p>
<p>The key point to bear in mind is that we are looking at the wobble of the planet, not the the wobble of the star.  Every time a planet transits the star, it affords us information about the position and velocity of the planet.  Even if the moon is too small to show up in the transit lightcurve, its effects on the host planet are not.</p>
<p>Both the position and velocity of the planet will be perturbed by the presence of a moon.  The spatial perturbation causes the planetary transit to occur slightly earlier or slightly later than expected.  The velocity perturbation causes the transit duration to be slightly greater or slightly smaller.  Remarkably, these effects can be minutes in magnitude.</p>
<p>The two effects, called transit time variation (TTV) and transit duration variation (TDV) always exhibit a 90 degrees phase difference.  In other words, we have a quite unique signature.  In addition, the ratio of the two amplitudes allows for a determination of both the moon&#039;s mass and its orbital distance from the host planet.</p>
<p>It&#039;s really fantastic to see so many people interested in exomoons.  Who knows how common these exomoons may be and what potential for habitability they possess!  Ultimately, the only way for us to answer these questions is to start looking!</p>
<p>All the best and continue to ask questions!<br />
David</p>
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		<title>By: Yael Dragwyla</title>
		<link>http://www.universetoday.com/2008/12/14/astronomers-now-looking-for-exomoons-around-exoplanets/comment-page-2/#comment-46492</link>
		<dc:creator>Yael Dragwyla</dc:creator>
		<pubDate>Tue, 16 Dec 2008 05:40:59 +0000</pubDate>
		<guid isPermaLink="false">http://www.universetoday.com/?p=22299#comment-46492</guid>
		<description>dollhopf:  &quot; &#039;maybe every month&#039; I mean OUR month of course. They probably would never have developed a time intervall like a month, which is caused by the observation of our moon.&quot;  From the ever-changing relationship of their primary to their day-star -- i.e., from synod to synod, as the primary and the day-star go from conjunction/New to opposition/Full -- they could easily derive a time-unit based on the average length of a synod.  As for days, that depends on whether they are tidally locked to their primary or not, the length of time it takes them to make one revolution about their primary, and the length of time it takes their primary to orbit their day-star.  But they would have a day of some sort for a time-unit, and could peg their month/synod to that, or vice-versa, whichever was shortest.</description>
		<content:encoded><![CDATA[<p>dollhopf:  &#034; &#039;maybe every month&#039; I mean OUR month of course. They probably would never have developed a time intervall like a month, which is caused by the observation of our moon.&#034;  From the ever-changing relationship of their primary to their day-star &#8212; i.e., from synod to synod, as the primary and the day-star go from conjunction/New to opposition/Full &#8212; they could easily derive a time-unit based on the average length of a synod.  As for days, that depends on whether they are tidally locked to their primary or not, the length of time it takes them to make one revolution about their primary, and the length of time it takes their primary to orbit their day-star.  But they would have a day of some sort for a time-unit, and could peg their month/synod to that, or vice-versa, whichever was shortest.</p>
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		<title>By: Frank Glover</title>
		<link>http://www.universetoday.com/2008/12/14/astronomers-now-looking-for-exomoons-around-exoplanets/comment-page-2/#comment-46458</link>
		<dc:creator>Frank Glover</dc:creator>
		<pubDate>Mon, 15 Dec 2008 22:32:34 +0000</pubDate>
		<guid isPermaLink="false">http://www.universetoday.com/?p=22299#comment-46458</guid>
		<description>&quot;How could they establish a celestial coordinate system so easily? And the seasons on Earth are caused by the change of the inclination during one revolution around the sun. But their seasons would change with every circle around their planet, maybe every month. Thus, what concept of time would they have developed?&quot;

If they watch things long enough, they&#039;ll see patterns and cycles, just as humans did. Perhaps more importantly, such beings might not waste time on the kind of Ptolemaic, planet-centered Universe that western civilization on Earth did...

Beings living on a body directly or indirectly circling one component of a double star might likewise be less inclined to believe the Universe literally revolves around them (unless the companion star was so distant and slow orbiting that it could be mistaken for a background star...)</description>
		<content:encoded><![CDATA[<p>&#034;How could they establish a celestial coordinate system so easily? And the seasons on Earth are caused by the change of the inclination during one revolution around the sun. But their seasons would change with every circle around their planet, maybe every month. Thus, what concept of time would they have developed?&#034;</p>
<p>If they watch things long enough, they&#039;ll see patterns and cycles, just as humans did. Perhaps more importantly, such beings might not waste time on the kind of Ptolemaic, planet-centered Universe that western civilization on Earth did&#8230;</p>
<p>Beings living on a body directly or indirectly circling one component of a double star might likewise be less inclined to believe the Universe literally revolves around them (unless the companion star was so distant and slow orbiting that it could be mistaken for a background star&#8230;)</p>
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		<title>By: DJ Barney</title>
		<link>http://www.universetoday.com/2008/12/14/astronomers-now-looking-for-exomoons-around-exoplanets/comment-page-2/#comment-46444</link>
		<dc:creator>DJ Barney</dc:creator>
		<pubDate>Mon, 15 Dec 2008 21:36:23 +0000</pubDate>
		<guid isPermaLink="false">http://www.universetoday.com/?p=22299#comment-46444</guid>
		<description>dollhopf .... &quot;exocreatures&quot; .. I like it ! That other word has become sort of ... xenophobic ?

I&#039;m scrambling to keep up. Did we get over some kind of &quot;hump&quot; here ? Even if those exoplanets and now exomoons don&#039;t harbour life, the techniques being developed will be invaluable.</description>
		<content:encoded><![CDATA[<p>dollhopf &#8230;. &#034;exocreatures&#034; .. I like it ! That other word has become sort of &#8230; xenophobic ?</p>
<p>I&#039;m scrambling to keep up. Did we get over some kind of &#034;hump&#034; here ? Even if those exoplanets and now exomoons don&#039;t harbour life, the techniques being developed will be invaluable.</p>
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		<title>By: Dark Gnat</title>
		<link>http://www.universetoday.com/2008/12/14/astronomers-now-looking-for-exomoons-around-exoplanets/comment-page-2/#comment-46429</link>
		<dc:creator>Dark Gnat</dc:creator>
		<pubDate>Mon, 15 Dec 2008 18:10:51 +0000</pubDate>
		<guid isPermaLink="false">http://www.universetoday.com/?p=22299#comment-46429</guid>
		<description>Now that some planets have been directly imaged, we could study those images over time to see if the planets themselves wobble.  We wouldn&#039;t have to look at the star to determine of the planet has moon(s).

D. Clayton: 

If the moon is far enough away, and had an inclination relative to the planet, then it would only pass into the planet&#039;s shadow on occasion.  Even if it does regularly pass into the shadow, it be cyclic, and any life forms would have no trouble adapting.</description>
		<content:encoded><![CDATA[<p>Now that some planets have been directly imaged, we could study those images over time to see if the planets themselves wobble.  We wouldn&#039;t have to look at the star to determine of the planet has moon(s).</p>
<p>D. Clayton: </p>
<p>If the moon is far enough away, and had an inclination relative to the planet, then it would only pass into the planet&#039;s shadow on occasion.  Even if it does regularly pass into the shadow, it be cyclic, and any life forms would have no trouble adapting.</p>
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		<title>By: ScepticTim</title>
		<link>http://www.universetoday.com/2008/12/14/astronomers-now-looking-for-exomoons-around-exoplanets/comment-page-2/#comment-46428</link>
		<dc:creator>ScepticTim</dc:creator>
		<pubDate>Mon, 15 Dec 2008 17:48:37 +0000</pubDate>
		<guid isPermaLink="false">http://www.universetoday.com/?p=22299#comment-46428</guid>
		<description>For those interested, I believe the paper that Ian refers to is arXiv:0810.2243v1 [astro-ph] 13 Oct 2008 &quot;Transit Timing Effects due to an Exomoon&quot; David M. Kipping</description>
		<content:encoded><![CDATA[<p>For those interested, I believe the paper that Ian refers to is arXiv:0810.2243v1 [astro-ph] 13 Oct 2008 &#034;Transit Timing Effects due to an Exomoon&#034; David M. Kipping</p>
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		<title>By: law mc</title>
		<link>http://www.universetoday.com/2008/12/14/astronomers-now-looking-for-exomoons-around-exoplanets/comment-page-2/#comment-46426</link>
		<dc:creator>law mc</dc:creator>
		<pubDate>Mon, 15 Dec 2008 16:43:19 +0000</pubDate>
		<guid isPermaLink="false">http://www.universetoday.com/?p=22299#comment-46426</guid>
		<description>would radiation really be that big a problem???

the reason we are so susceptible to it is because we are shielded from it, but what if you were always exposed to it, wouldnt life have found ways to mitigate the problems that arise from it. After all, there are bacteria that are very radiation resistant on earth, so i dont think that idea is very strange at all.</description>
		<content:encoded><![CDATA[<p>would radiation really be that big a problem???</p>
<p>the reason we are so susceptible to it is because we are shielded from it, but what if you were always exposed to it, wouldnt life have found ways to mitigate the problems that arise from it. After all, there are bacteria that are very radiation resistant on earth, so i dont think that idea is very strange at all.</p>
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		<title>By: Jorge</title>
		<link>http://www.universetoday.com/2008/12/14/astronomers-now-looking-for-exomoons-around-exoplanets/comment-page-2/#comment-46420</link>
		<dc:creator>Jorge</dc:creator>
		<pubDate>Mon, 15 Dec 2008 15:37:11 +0000</pubDate>
		<guid isPermaLink="false">http://www.universetoday.com/?p=22299#comment-46420</guid>
		<description>&lt;blockquote&gt;In short, I have no answer to Jorge&#039;s question&lt;/blockquote&gt;

Oh. Too bad. I was really looking forward to learning something new here.

So, either the experiment doesn&#039;t make sense or there&#039;s something here that&#039;s eluding us. Ian, can&#039;t you squeeze something else about this out of your sources?</description>
		<content:encoded><![CDATA[<blockquote><p>In short, I have no answer to Jorge&#039;s question</p></blockquote>
<p>Oh. Too bad. I was really looking forward to learning something new here.</p>
<p>So, either the experiment doesn&#039;t make sense or there&#039;s something here that&#039;s eluding us. Ian, can&#039;t you squeeze something else about this out of your sources?</p>
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		<title>By: dollhopf</title>
		<link>http://www.universetoday.com/2008/12/14/astronomers-now-looking-for-exomoons-around-exoplanets/comment-page-2/#comment-46406</link>
		<dc:creator>dollhopf</dc:creator>
		<pubDate>Mon, 15 Dec 2008 08:35:48 +0000</pubDate>
		<guid isPermaLink="false">http://www.universetoday.com/?p=22299#comment-46406</guid>
		<description>&quot;maybe every month&quot;

I mean OUR month of course. They probably would never have developed  a time intervall like a month, which is caused by the observation of our moon.</description>
		<content:encoded><![CDATA[<p>&#034;maybe every month&#034;</p>
<p>I mean OUR month of course. They probably would never have developed  a time intervall like a month, which is caused by the observation of our moon.</p>
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		<title>By: dollhopf</title>
		<link>http://www.universetoday.com/2008/12/14/astronomers-now-looking-for-exomoons-around-exoplanets/comment-page-2/#comment-46405</link>
		<dc:creator>dollhopf</dc:creator>
		<pubDate>Mon, 15 Dec 2008 08:33:22 +0000</pubDate>
		<guid isPermaLink="false">http://www.universetoday.com/?p=22299#comment-46405</guid>
		<description>I don&#039;t know. Even if the moon that spins around the planet, and which itself spins around the sun togehter with its moon, would furthermore spin around its own axis (and not having one side turned toward the planet all the time like our satellite does).

*#-)*

How could they establish a celestial coordinate system so easily? And the seasons on Earth are caused by the change of the inclination during one revolution around the sun. But their seasons would change with every circle around their planet, maybe every month. Thus, what concept of time would they have developed?</description>
		<content:encoded><![CDATA[<p>I don&#039;t know. Even if the moon that spins around the planet, and which itself spins around the sun togehter with its moon, would furthermore spin around its own axis (and not having one side turned toward the planet all the time like our satellite does).</p>
<p>*#-)*</p>
<p>How could they establish a celestial coordinate system so easily? And the seasons on Earth are caused by the change of the inclination during one revolution around the sun. But their seasons would change with every circle around their planet, maybe every month. Thus, what concept of time would they have developed?</p>
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		<title>By: Nexus</title>
		<link>http://www.universetoday.com/2008/12/14/astronomers-now-looking-for-exomoons-around-exoplanets/comment-page-2/#comment-46402</link>
		<dc:creator>Nexus</dc:creator>
		<pubDate>Mon, 15 Dec 2008 07:30:18 +0000</pubDate>
		<guid isPermaLink="false">http://www.universetoday.com/?p=22299#comment-46402</guid>
		<description>It probably wouldn&#039;t take them as long to work out their world isn&#039;t the center of the universe as it took us.</description>
		<content:encoded><![CDATA[<p>It probably wouldn&#039;t take them as long to work out their world isn&#039;t the center of the universe as it took us.</p>
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		<title>By: dollhopf</title>
		<link>http://www.universetoday.com/2008/12/14/astronomers-now-looking-for-exomoons-around-exoplanets/comment-page-2/#comment-46393</link>
		<dc:creator>dollhopf</dc:creator>
		<pubDate>Mon, 15 Dec 2008 06:04:13 +0000</pubDate>
		<guid isPermaLink="false">http://www.universetoday.com/?p=22299#comment-46393</guid>
		<description>If there were Exocreatures on an Exomoon of a Exoplanet, would it be easier for them to find Kepler&#039;s Laws than it was for our astronomers? Are celestial mechanics more clearly seen, if  one moves around a planet that moves around a star? The imagination makes me dizzy.</description>
		<content:encoded><![CDATA[<p>If there were Exocreatures on an Exomoon of a Exoplanet, would it be easier for them to find Kepler&#039;s Laws than it was for our astronomers? Are celestial mechanics more clearly seen, if  one moves around a planet that moves around a star? The imagination makes me dizzy.</p>
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		<title>By: dollhopf</title>
		<link>http://www.universetoday.com/2008/12/14/astronomers-now-looking-for-exomoons-around-exoplanets/comment-page-2/#comment-46392</link>
		<dc:creator>dollhopf</dc:creator>
		<pubDate>Mon, 15 Dec 2008 05:54:22 +0000</pubDate>
		<guid isPermaLink="false">http://www.universetoday.com/?p=22299#comment-46392</guid>
		<description>&lt;em&gt;As far as Moons, go, my only question centers on its &quot;day.&quot; Since its orbit would constantly take it within its parent planet&#039;s shadow&#039;&lt;/em&gt;

Consider the Moon of the Earth. One could see the Moon in the shadow of the Earth just about hundered times throughout the whole 21st century.</description>
		<content:encoded><![CDATA[<p><em>As far as Moons, go, my only question centers on its &#034;day.&#034; Since its orbit would constantly take it within its parent planet&#039;s shadow&#039;</em></p>
<p>Consider the Moon of the Earth. One could see the Moon in the shadow of the Earth just about hundered times throughout the whole 21st century.</p>
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		<title>By: Darnell Clayton</title>
		<link>http://www.universetoday.com/2008/12/14/astronomers-now-looking-for-exomoons-around-exoplanets/comment-page-2/#comment-46387</link>
		<dc:creator>Darnell Clayton</dc:creator>
		<pubDate>Mon, 15 Dec 2008 04:21:36 +0000</pubDate>
		<guid isPermaLink="false">http://www.universetoday.com/?p=22299#comment-46387</guid>
		<description>As far as Moons, go, my only question centers on its &quot;day.&quot;

Since its orbit would constantly take it within its parent planet&#039;s shadow, wouldn&#039;t this affect life for the worse?

Also, as far as radiation belts go, both Ganymede and Europa orbit within its radiation belts, although the former is known to host a very strong magnetic field (unfortunately it does not block out all of Jupiter&#039;s radiation).

I think Titan would be a better example, of a large moon that orbits just within its parent worlds magnetic field (despite the fact that it lacks one itself).</description>
		<content:encoded><![CDATA[<p>As far as Moons, go, my only question centers on its &#034;day.&#034;</p>
<p>Since its orbit would constantly take it within its parent planet&#039;s shadow, wouldn&#039;t this affect life for the worse?</p>
<p>Also, as far as radiation belts go, both Ganymede and Europa orbit within its radiation belts, although the former is known to host a very strong magnetic field (unfortunately it does not block out all of Jupiter&#039;s radiation).</p>
<p>I think Titan would be a better example, of a large moon that orbits just within its parent worlds magnetic field (despite the fact that it lacks one itself).</p>
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		<title>By: trux</title>
		<link>http://www.universetoday.com/2008/12/14/astronomers-now-looking-for-exomoons-around-exoplanets/comment-page-1/#comment-46371</link>
		<dc:creator>trux</dc:creator>
		<pubDate>Mon, 15 Dec 2008 01:49:15 +0000</pubDate>
		<guid isPermaLink="false">http://www.universetoday.com/?p=22299#comment-46371</guid>
		<description>2 Ilya: I may be wrong, but perhaps the method relies on both measuring the gravitational wobble, and spectrographic analysis of planet transitions. In that case, although the travel of the center of the moon-planet system would be regular, there would be disaccords with the spectral transition measurements, which would then prove the moon presence. It surprises me though that the technology is already so sensitive that it could be detected. In any way, I&#039;d love to read much more details about the methods used.</description>
		<content:encoded><![CDATA[<p>2 Ilya: I may be wrong, but perhaps the method relies on both measuring the gravitational wobble, and spectrographic analysis of planet transitions. In that case, although the travel of the center of the moon-planet system would be regular, there would be disaccords with the spectral transition measurements, which would then prove the moon presence. It surprises me though that the technology is already so sensitive that it could be detected. In any way, I&#039;d love to read much more details about the methods used.</p>
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		<title>By: Ilya</title>
		<link>http://www.universetoday.com/2008/12/14/astronomers-now-looking-for-exomoons-around-exoplanets/comment-page-1/#comment-46368</link>
		<dc:creator>Ilya</dc:creator>
		<pubDate>Mon, 15 Dec 2008 01:08:48 +0000</pubDate>
		<guid isPermaLink="false">http://www.universetoday.com/?p=22299#comment-46368</guid>
		<description>Now that I thought of it, I have to take back what I wrote about center of mass not moving in a simple Keplerian orbit. In short, I have no answer to Jorge&#039;s question. All I can guess is that David Kipping is NOT expecting the star&#039;s wobble to follow planet-moon center of mass, but to follow just the planet. Why, I do not know. And will try to find out.</description>
		<content:encoded><![CDATA[<p>Now that I thought of it, I have to take back what I wrote about center of mass not moving in a simple Keplerian orbit. In short, I have no answer to Jorge&#039;s question. All I can guess is that David Kipping is NOT expecting the star&#039;s wobble to follow planet-moon center of mass, but to follow just the planet. Why, I do not know. And will try to find out.</p>
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		<title>By: Dark Gnat</title>
		<link>http://www.universetoday.com/2008/12/14/astronomers-now-looking-for-exomoons-around-exoplanets/comment-page-1/#comment-46367</link>
		<dc:creator>Dark Gnat</dc:creator>
		<pubDate>Mon, 15 Dec 2008 00:56:32 +0000</pubDate>
		<guid isPermaLink="false">http://www.universetoday.com/?p=22299#comment-46367</guid>
		<description>Even if it does change, it probably wouldn&#039;t be too gret of a change.

Perhaps something like a global winter and summer.  Titan might be a good model.

I think this would be very possible, and a worthy effort!</description>
		<content:encoded><![CDATA[<p>Even if it does change, it probably wouldn&#039;t be too gret of a change.</p>
<p>Perhaps something like a global winter and summer.  Titan might be a good model.</p>
<p>I think this would be very possible, and a worthy effort!</p>
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		<title>By: Some Guy</title>
		<link>http://www.universetoday.com/2008/12/14/astronomers-now-looking-for-exomoons-around-exoplanets/comment-page-1/#comment-46357</link>
		<dc:creator>Some Guy</dc:creator>
		<pubDate>Sun, 14 Dec 2008 23:13:53 +0000</pubDate>
		<guid isPermaLink="false">http://www.universetoday.com/?p=22299#comment-46357</guid>
		<description>ok, no ones brought this up, so i will
any habitable moon that orbits a jupiter like planet beyond its radiation belt will likely have a pretty wide orbit.  SO!  that being said, this wide orbit could vary the moon&#039;s distance from the host star by hundreds of thousands of kilometers within a very short period of time, would that not cause violent tidal swings on the surface, leading to aggressive weather, and putting any life there up against some tough odds?</description>
		<content:encoded><![CDATA[<p>ok, no ones brought this up, so i will<br />
any habitable moon that orbits a jupiter like planet beyond its radiation belt will likely have a pretty wide orbit.  SO!  that being said, this wide orbit could vary the moon&#039;s distance from the host star by hundreds of thousands of kilometers within a very short period of time, would that not cause violent tidal swings on the surface, leading to aggressive weather, and putting any life there up against some tough odds?</p>
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		<title>By: Silver Thread</title>
		<link>http://www.universetoday.com/2008/12/14/astronomers-now-looking-for-exomoons-around-exoplanets/comment-page-1/#comment-46353</link>
		<dc:creator>Silver Thread</dc:creator>
		<pubDate>Sun, 14 Dec 2008 22:32:34 +0000</pubDate>
		<guid isPermaLink="false">http://www.universetoday.com/?p=22299#comment-46353</guid>
		<description>That&#039;s no moon.....</description>
		<content:encoded><![CDATA[<p>That&#039;s no moon&#8230;..</p>
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		<title>By: Jorge</title>
		<link>http://www.universetoday.com/2008/12/14/astronomers-now-looking-for-exomoons-around-exoplanets/comment-page-1/#comment-46346</link>
		<dc:creator>Jorge</dc:creator>
		<pubDate>Sun, 14 Dec 2008 21:28:52 +0000</pubDate>
		<guid isPermaLink="false">http://www.universetoday.com/?p=22299#comment-46346</guid>
		<description>&lt;blockquote&gt;Yes, but that center of mass will not move in complete accordance with Kepler&#039;s Laws. It will periodically speed up and slow down. Which is Kipping&#039;s whole point.&lt;/blockquote&gt;

Hm... still trying to wrap my head around this. So. I can think of only one way for this to happen: if the motion is such that we have to throw in relativity. Right?

If so, surely the variations would be minute?...</description>
		<content:encoded><![CDATA[<blockquote><p>Yes, but that center of mass will not move in complete accordance with Kepler&#039;s Laws. It will periodically speed up and slow down. Which is Kipping&#039;s whole point.</p></blockquote>
<p>Hm&#8230; still trying to wrap my head around this. So. I can think of only one way for this to happen: if the motion is such that we have to throw in relativity. Right?</p>
<p>If so, surely the variations would be minute?&#8230;</p>
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		<title>By: Jason</title>
		<link>http://www.universetoday.com/2008/12/14/astronomers-now-looking-for-exomoons-around-exoplanets/comment-page-1/#comment-46326</link>
		<dc:creator>Jason</dc:creator>
		<pubDate>Sun, 14 Dec 2008 19:42:01 +0000</pubDate>
		<guid isPermaLink="false">http://www.universetoday.com/?p=22299#comment-46326</guid>
		<description>@ Ilya

Yea,  I would guess that the much shorter frequency of wobble induced by an earth sized moon  would be easier to detect than that of a earth sized planet.

The concept of a Titan or Europa like moon in the habitable zone of a star is exciting.</description>
		<content:encoded><![CDATA[<p>@ Ilya</p>
<p>Yea,  I would guess that the much shorter frequency of wobble induced by an earth sized moon  would be easier to detect than that of a earth sized planet.</p>
<p>The concept of a Titan or Europa like moon in the habitable zone of a star is exciting.</p>
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		<title>By: Ilya</title>
		<link>http://www.universetoday.com/2008/12/14/astronomers-now-looking-for-exomoons-around-exoplanets/comment-page-1/#comment-46321</link>
		<dc:creator>Ilya</dc:creator>
		<pubDate>Sun, 14 Dec 2008 18:50:25 +0000</pubDate>
		<guid isPermaLink="false">http://www.universetoday.com/?p=22299#comment-46321</guid>
		<description>&lt;b&gt;It would seem that if we could detect the very slight speeding up and slowing down of a planet moon system, that we could just a easly detect an earth sized planet going around a star. Which is thus far beyond our capibilities.&lt;/b&gt;

Sorry, but your intuition is wrong. An earth sized planet going around a star can not be detected (yet) because the wobble it induces is too small. If a gas giant planet induces a readily detectable wobble, the speed with which it rises and falls is much easier to measure. I have no links handy, but in several known multi-planet systems, planets&#039; gravitational influence on &lt;i&gt;each other&lt;/i&gt; has already been found.</description>
		<content:encoded><![CDATA[<p><b>It would seem that if we could detect the very slight speeding up and slowing down of a planet moon system, that we could just a easly detect an earth sized planet going around a star. Which is thus far beyond our capibilities.</b></p>
<p>Sorry, but your intuition is wrong. An earth sized planet going around a star can not be detected (yet) because the wobble it induces is too small. If a gas giant planet induces a readily detectable wobble, the speed with which it rises and falls is much easier to measure. I have no links handy, but in several known multi-planet systems, planets&#039; gravitational influence on <i>each other</i> has already been found.</p>
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