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	<title>Comments on: More Mercury!</title>
	<atom:link href="http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/feed/" rel="self" type="application/rss+xml" />
	<link>http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/</link>
	<description>I am an astronomer, writer, and skeptic. I likes reality the way it is, and I aims to keep it that way. My real name is Phil Plait, and I run the Bad Astronomy blog.</description>
	<lastBuildDate>Mon, 13 Feb 2012 20:59:37 +0000</lastBuildDate>
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		<title>By: Steve Dutch</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/comment-page-1/#comment-106534</link>
		<dc:creator>Steve Dutch</dc:creator>
		<pubDate>Tue, 29 Jul 2008 02:07:13 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/#comment-106534</guid>
		<description>The near stationary appearance of the sun at Mercury&#039;s perihelion is no accident.  Mercury&#039;s aphelion is 1.5 times its perihelion distance, and since tidal forces are inversely proportional to the cube of distance, the solar tides at perihelion are 3.5 times larger than at aphelion. So Mercury&#039;s rotation is locked to the sun, but locked to the sun at perihelion, since the tidal forces are so much stronger then. We used to think Mercury was locked to the sun like the Moon is locked to the earth, but it&#039;s a more complex kind of lock.</description>
		<content:encoded><![CDATA[<p>The near stationary appearance of the sun at Mercury&#8217;s perihelion is no accident.  Mercury&#8217;s aphelion is 1.5 times its perihelion distance, and since tidal forces are inversely proportional to the cube of distance, the solar tides at perihelion are 3.5 times larger than at aphelion. So Mercury&#8217;s rotation is locked to the sun, but locked to the sun at perihelion, since the tidal forces are so much stronger then. We used to think Mercury was locked to the sun like the Moon is locked to the earth, but it&#8217;s a more complex kind of lock.</p>
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		<title>By: Steve Cooperman</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/comment-page-1/#comment-64195</link>
		<dc:creator>Steve Cooperman</dc:creator>
		<pubDate>Sat, 19 Jan 2008 10:19:24 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/#comment-64195</guid>
		<description>With the pictures of Mercury now coming in, I find it striking (no pun intended) that many of the craters have central rings or craters -- many more than our Moon has.

I haven&#039;t heard any comments about it yet, but they seem similar to the morphology of the craters on Ganymede (one of the moons of Jupiter):
http://img375.imageshack.us/img375/9899/ganmogac4gs.jpg

Here&#039;s a picture of Mercury:
http://messenger.jhuapl.edu/gallery/sciencePhotos/pics/EW0108829708G.4release.jpg

Now, Ganymede is rock and ice, but I&#039;m not implying that Mercury is. But Ganymede may have a large rocky core topped by a rock-ice layer that the craters are in (although way more ice than the inner Galilean moons), and Mercury certainly has a large core (although made of iron). I&#039;m suggesting that the central crater/ring is a seismic &quot;bounce&quot; in some way off the core from the impact.

On the Moon, craters that are small don&#039;t have central peaks. As the craters get larger, they develop central peaks. For even larger craters, you can get double or more complicated central peaks and the largest have central rings. (Mercury has lots of craters with central peaks, too -- I&#039;m just suggesting that Mercury has MORE craters with central craters than it &quot;should have&quot; and wondering about the reason.) But the Moon also has a very small core.

Mercury&#039;s surface is also saturated with craters, like Callisto&#039;s -- another moon of Jupiter:
http://astrored.org/astrofotos/albums/Sistema_Solar/Jupiter/callisto.jpg.html

Look how many craters are there, and most seem to have central craters! Callisto is thought to have an even larger core than Ganymede, but the saturation of large numbers of craters indicates a very OLD surface (nothing&#039;s come by to erase the craters over the age of the Solar System.

This stuff is amazing to me . . .

BTW, for those interested, here&#039;s a website that predicts sizes of craters on the Earth from various impacts:
http://www.lpl.arizona.edu/impacteffects/

   --- Steve &gt;&gt;&gt;&gt;</description>
		<content:encoded><![CDATA[<p>With the pictures of Mercury now coming in, I find it striking (no pun intended) that many of the craters have central rings or craters &#8212; many more than our Moon has.</p>
<p>I haven&#8217;t heard any comments about it yet, but they seem similar to the morphology of the craters on Ganymede (one of the moons of Jupiter):<br />
<a href="http://img375.imageshack.us/img375/9899/ganmogac4gs.jpg" rel="nofollow">http://img375.imageshack.us/img375/9899/ganmogac4gs.jpg</a></p>
<p>Here&#8217;s a picture of Mercury:<br />
<a href="http://messenger.jhuapl.edu/gallery/sciencePhotos/pics/EW0108829708G.4release.jpg" rel="nofollow">http://messenger.jhuapl.edu/gallery/sciencePhotos/pics/EW0108829708G.4release.jpg</a></p>
<p>Now, Ganymede is rock and ice, but I&#8217;m not implying that Mercury is. But Ganymede may have a large rocky core topped by a rock-ice layer that the craters are in (although way more ice than the inner Galilean moons), and Mercury certainly has a large core (although made of iron). I&#8217;m suggesting that the central crater/ring is a seismic &#8220;bounce&#8221; in some way off the core from the impact.</p>
<p>On the Moon, craters that are small don&#8217;t have central peaks. As the craters get larger, they develop central peaks. For even larger craters, you can get double or more complicated central peaks and the largest have central rings. (Mercury has lots of craters with central peaks, too &#8212; I&#8217;m just suggesting that Mercury has MORE craters with central craters than it &#8220;should have&#8221; and wondering about the reason.) But the Moon also has a very small core.</p>
<p>Mercury&#8217;s surface is also saturated with craters, like Callisto&#8217;s &#8212; another moon of Jupiter:<br />
<a href="http://astrored.org/astrofotos/albums/Sistema_Solar/Jupiter/callisto.jpg.html" rel="nofollow">http://astrored.org/astrofotos/albums/Sistema_Solar/Jupiter/callisto.jpg.html</a></p>
<p>Look how many craters are there, and most seem to have central craters! Callisto is thought to have an even larger core than Ganymede, but the saturation of large numbers of craters indicates a very OLD surface (nothing&#8217;s come by to erase the craters over the age of the Solar System.</p>
<p>This stuff is amazing to me . . .</p>
<p>BTW, for those interested, here&#8217;s a website that predicts sizes of craters on the Earth from various impacts:<br />
<a href="http://www.lpl.arizona.edu/impacteffects/" rel="nofollow">http://www.lpl.arizona.edu/impacteffects/</a></p>
<p>   &#8212; Steve &gt;&gt;&gt;&gt;</p>
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		<title>By: Ken B</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/comment-page-1/#comment-64194</link>
		<dc:creator>Ken B</dc:creator>
		<pubDate>Fri, 18 Jan 2008 18:05:52 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/#comment-64194</guid>
		<description>Clearly, it&#039;s Kang (or Kodos) in that image.

    http://www.hvcomputer.com/temp/mercury.html</description>
		<content:encoded><![CDATA[<p>Clearly, it&#8217;s Kang (or Kodos) in that image.</p>
<p>    <a href="http://www.hvcomputer.com/temp/mercury.html" rel="nofollow">http://www.hvcomputer.com/temp/mercury.html</a></p>
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		<title>By: Sally</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/comment-page-1/#comment-64193</link>
		<dc:creator>Sally</dc:creator>
		<pubDate>Thu, 17 Jan 2008 21:57:31 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/#comment-64193</guid>
		<description>Dude, you really should learn about geology.  I think you&#039;d dig it!  :)</description>
		<content:encoded><![CDATA[<p>Dude, you really should learn about geology.  I think you&#8217;d dig it!  <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_smile.gif' alt=':)' class='wp-smiley' /> </p>
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		<title>By: Jack Hagerty</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/comment-page-1/#comment-64192</link>
		<dc:creator>Jack Hagerty</dc:creator>
		<pubDate>Thu, 17 Jan 2008 21:21:39 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/#comment-64192</guid>
		<description>Quiet Desperation says: &quot; &#039;— I’m guessing that in the future, Mercury will be home to a huge metal mining operation.&#039;

In the Transmetropolitan graphic novels, it’s mentioned that Earth is powered by the energy transmitted from Mercury, which has been completely covered by solar panels.&quot;


Don&#039;t forget &quot;Runaround&quot;, one of Asimov&#039;s robot stories.

- Jack</description>
		<content:encoded><![CDATA[<p>Quiet Desperation says: &#8221; &#8216;— I’m guessing that in the future, Mercury will be home to a huge metal mining operation.&#8217;</p>
<p>In the Transmetropolitan graphic novels, it’s mentioned that Earth is powered by the energy transmitted from Mercury, which has been completely covered by solar panels.&#8221;</p>
<p>Don&#8217;t forget &#8220;Runaround&#8221;, one of Asimov&#8217;s robot stories.</p>
<p>- Jack</p>
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		<title>By: Anthony</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/comment-page-1/#comment-64191</link>
		<dc:creator>Anthony</dc:creator>
		<pubDate>Thu, 17 Jan 2008 21:10:31 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/#comment-64191</guid>
		<description>Digging into Mercury, unless at the poles, won&#039;t ever make it cool enough to survive. Underground will simply average out the sunlight, making it hot year-round.</description>
		<content:encoded><![CDATA[<p>Digging into Mercury, unless at the poles, won&#8217;t ever make it cool enough to survive. Underground will simply average out the sunlight, making it hot year-round.</p>
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		<title>By: Sabrina</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/comment-page-1/#comment-64156</link>
		<dc:creator>Sabrina</dc:creator>
		<pubDate>Thu, 17 Jan 2008 16:55:02 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/#comment-64156</guid>
		<description>Connect the dots la la la la Connect the dots la la la la

http://www.moostangproductions.com/temp/other.gif</description>
		<content:encoded><![CDATA[<p>Connect the dots la la la la Connect the dots la la la la</p>
<p><a href="http://www.moostangproductions.com/temp/other.gif" rel="nofollow">http://www.moostangproductions.com/temp/other.gif</a></p>
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		<title>By: Mark Martin</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/comment-page-1/#comment-64155</link>
		<dc:creator>Mark Martin</dc:creator>
		<pubDate>Thu, 17 Jan 2008 16:53:47 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/#comment-64155</guid>
		<description>Jeffersonian,

My guess is that, since MESSENGER is a publicly-funded (non-classified) project, all data are in the public domain. This isn&#039;t to say of course that you wouldn&#039;t have to do some extensive legwork to get hold of the data, especially the non-photographic stuff. For instance, if you want to study the planet&#039;s mass, you&#039;ll need to get all the flight dynamics data, which would consist entirely of reams of numbers telling how the spacecraft&#039;s velocity changed as it grazed Mercury. You also might be asked to pay for the expense of generating a copy of the data. But I&#039;m sure that it&#039;s there for the asking.</description>
		<content:encoded><![CDATA[<p>Jeffersonian,</p>
<p>My guess is that, since MESSENGER is a publicly-funded (non-classified) project, all data are in the public domain. This isn&#8217;t to say of course that you wouldn&#8217;t have to do some extensive legwork to get hold of the data, especially the non-photographic stuff. For instance, if you want to study the planet&#8217;s mass, you&#8217;ll need to get all the flight dynamics data, which would consist entirely of reams of numbers telling how the spacecraft&#8217;s velocity changed as it grazed Mercury. You also might be asked to pay for the expense of generating a copy of the data. But I&#8217;m sure that it&#8217;s there for the asking.</p>
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		<title>By: Sabrina</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/comment-page-1/#comment-64154</link>
		<dc:creator>Sabrina</dc:creator>
		<pubDate>Thu, 17 Jan 2008 16:53:30 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/#comment-64154</guid>
		<description>Connect the dots la la la la Connect the dots la la la la</description>
		<content:encoded><![CDATA[<p>Connect the dots la la la la Connect the dots la la la la</p>
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		<title>By: Tom Marking</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/comment-page-1/#comment-64167</link>
		<dc:creator>Tom Marking</dc:creator>
		<pubDate>Thu, 17 Jan 2008 16:52:13 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/#comment-64167</guid>
		<description>Ken B, Wow!  That animation is way cool.  You can actually see Mercury stop in the sky and go backwards.  I particularly like the surface temperature gauge.  Let me see if I can do a back-of-the-envelope calculation to convince myself that this retrograde motion is correct:

Average distance of Mercury from the sun = 57.9 million kilometers
Orbital period = 87.97 days
Rotation period = 58.65 days
Average orbital velocity = 4.14 million kilometers per day
Average angular velocity of sun due to rotation = 6.14 degrees per day
Average angular velocity of sun due to orbit = 4.09 degrees per day
So on average to compute the time from sunrise to sunrise on Mercury you subtract 4.09 from 6.14 getting 2.05 degrees per day or 360 degrees per 175.6 days.

But, that&#039;s just the average.  The orbit is highly elliptic.
Eccentricity of orbit = 0.206
Perihelion distance = 0.794 * 57.9 million kilometers = 46.0 million kilometers
Perihelion orbital velocity = 1.206 * 4.14 million kilometers per day = 4.99 million kilometers per day
Angular velocity of sun due to orbit at perihelion = 4.99 / 46.0 = 0.108 radians per day = 6.22 degrees per day
So at perihelion the apparent motion of the sun in the sky is 6.14 - 6.22 or -0.08 degrees per day.  That&#039;s a negative number so the sun appears to move backwards (west to east) at a very slow rate of speed, so it will appear almost stationary near perihelion, just like the animation says.

Joshua 10:13 -  &quot;And the sun stood still, and the moon stayed, until the people had avenged themselves upon their enemies. Is not this written in the book of Jasher? So the sun stood still in the midst of heaven, and hasted not to go down about a whole day&quot;

This is a common occurence on Mercury, not a miracle.</description>
		<content:encoded><![CDATA[<p>Ken B, Wow!  That animation is way cool.  You can actually see Mercury stop in the sky and go backwards.  I particularly like the surface temperature gauge.  Let me see if I can do a back-of-the-envelope calculation to convince myself that this retrograde motion is correct:</p>
<p>Average distance of Mercury from the sun = 57.9 million kilometers<br />
Orbital period = 87.97 days<br />
Rotation period = 58.65 days<br />
Average orbital velocity = 4.14 million kilometers per day<br />
Average angular velocity of sun due to rotation = 6.14 degrees per day<br />
Average angular velocity of sun due to orbit = 4.09 degrees per day<br />
So on average to compute the time from sunrise to sunrise on Mercury you subtract 4.09 from 6.14 getting 2.05 degrees per day or 360 degrees per 175.6 days.</p>
<p>But, that&#8217;s just the average.  The orbit is highly elliptic.<br />
Eccentricity of orbit = 0.206<br />
Perihelion distance = 0.794 * 57.9 million kilometers = 46.0 million kilometers<br />
Perihelion orbital velocity = 1.206 * 4.14 million kilometers per day = 4.99 million kilometers per day<br />
Angular velocity of sun due to orbit at perihelion = 4.99 / 46.0 = 0.108 radians per day = 6.22 degrees per day<br />
So at perihelion the apparent motion of the sun in the sky is 6.14 &#8211; 6.22 or -0.08 degrees per day.  That&#8217;s a negative number so the sun appears to move backwards (west to east) at a very slow rate of speed, so it will appear almost stationary near perihelion, just like the animation says.</p>
<p>Joshua 10:13 &#8211;  &#8220;And the sun stood still, and the moon stayed, until the people had avenged themselves upon their enemies. Is not this written in the book of Jasher? So the sun stood still in the midst of heaven, and hasted not to go down about a whole day&#8221;</p>
<p>This is a common occurence on Mercury, not a miracle.</p>
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		<title>By: Crux Australis</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/comment-page-1/#comment-64164</link>
		<dc:creator>Crux Australis</dc:creator>
		<pubDate>Thu, 17 Jan 2008 16:37:27 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/#comment-64164</guid>
		<description>@chris:
I didn&#039;t know there was anyone else here from New Zealand! I&#039;m looking forward to seeing Cloverfield, too. The TV ads look really good.</description>
		<content:encoded><![CDATA[<p>@chris:<br />
I didn&#8217;t know there was anyone else here from New Zealand! I&#8217;m looking forward to seeing Cloverfield, too. The TV ads look really good.</p>
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		<title>By: Kit Peters</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/comment-page-1/#comment-64158</link>
		<dc:creator>Kit Peters</dc:creator>
		<pubDate>Thu, 17 Jan 2008 16:02:48 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/#comment-64158</guid>
		<description>@Barton Paul Levenson:

(On the concept of Mercury being covered in solar panels and the energy being transmitted to Earth)

A) It&#039;s a comic book.  Suspend your disbelief.  :)

B) Suppose, for a second, such a plan were to be considered.  Could you transmit the energy via some sort of tight collimated beam (e.g. a laser or maser)?  I say this not knowing anything about Mercury&#039;s orbit relative to the Earth, but that particular problem is solvable, I think.</description>
		<content:encoded><![CDATA[<p>@Barton Paul Levenson:</p>
<p>(On the concept of Mercury being covered in solar panels and the energy being transmitted to Earth)</p>
<p>A) It&#8217;s a comic book.  Suspend your disbelief.  <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_smile.gif' alt=':)' class='wp-smiley' /> </p>
<p>B) Suppose, for a second, such a plan were to be considered.  Could you transmit the energy via some sort of tight collimated beam (e.g. a laser or maser)?  I say this not knowing anything about Mercury&#8217;s orbit relative to the Earth, but that particular problem is solvable, I think.</p>
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		<title>By: Michelle</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/comment-page-1/#comment-64157</link>
		<dc:creator>Michelle</dc:creator>
		<pubDate>Thu, 17 Jan 2008 15:41:20 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/#comment-64157</guid>
		<description>http://www.badastronomy.com/bad/misc/mccanney/index.html

That guy, Monkey?</description>
		<content:encoded><![CDATA[<p><a href="http://www.badastronomy.com/bad/misc/mccanney/index.html" rel="nofollow">http://www.badastronomy.com/bad/misc/mccanney/index.html</a></p>
<p>That guy, Monkey?</p>
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		<title>By: Monkey</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/comment-page-1/#comment-64190</link>
		<dc:creator>Monkey</dc:creator>
		<pubDate>Thu, 17 Jan 2008 15:26:16 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/#comment-64190</guid>
		<description>off topic -
www.jmccanneyscience.com/

Anyone dipped into this guys work (he seems to be yelling at us in italics...and...using....a lot of .... continuous .... grammar..... techniques.....and offering us NO ANSWERS TO HIS CLAIMS, despite his caps lock syndrome).</description>
		<content:encoded><![CDATA[<p>off topic -<br />
<a href="http://www.jmccanneyscience.com/" rel="nofollow">http://www.jmccanneyscience.com/</a></p>
<p>Anyone dipped into this guys work (he seems to be yelling at us in italics&#8230;and&#8230;using&#8230;.a lot of &#8230;. continuous &#8230;. grammar&#8230;.. techniques&#8230;..and offering us NO ANSWERS TO HIS CLAIMS, despite his caps lock syndrome).</p>
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		<title>By: Ken B</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/comment-page-1/#comment-64189</link>
		<dc:creator>Ken B</dc:creator>
		<pubDate>Thu, 17 Jan 2008 15:16:43 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/#comment-64189</guid>
		<description>Tom Marking:
(What is a day on Mercury?)

I don&#039;t know if this helps or hurts in answering your question:

http://btc.montana.edu/messenger/Interactives/ANIMATIONS/Day_On_Mercury/day_on_mercury_full.htm

Note how, near perihelion, the Sun&#039;s motion appears (&quot;is&quot;?) retrograde in the sky, due to the speed at which Mercury is moving.  (I remember reading this years ago, but this animation makes it quite clear.)

A longer description of the animation is here:

http://www.sciencenetlinks.com/tools.cfm?DocID=72&amp;Grade=6-8</description>
		<content:encoded><![CDATA[<p>Tom Marking:<br />
(What is a day on Mercury?)</p>
<p>I don&#8217;t know if this helps or hurts in answering your question:</p>
<p><a href="http://btc.montana.edu/messenger/Interactives/ANIMATIONS/Day_On_Mercury/day_on_mercury_full.htm" rel="nofollow">http://btc.montana.edu/messenger/Interactives/ANIMATIONS/Day_On_Mercury/day_on_mercury_full.htm</a></p>
<p>Note how, near perihelion, the Sun&#8217;s motion appears (&#8220;is&#8221;?) retrograde in the sky, due to the speed at which Mercury is moving.  (I remember reading this years ago, but this animation makes it quite clear.)</p>
<p>A longer description of the animation is here:</p>
<p><a href="http://www.sciencenetlinks.com/tools.cfm?DocID=72&#038;Grade=6-8" rel="nofollow">http://www.sciencenetlinks.com/tools.cfm?DocID=72&#038;Grade=6-8</a></p>
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		<title>By: JanieBelle</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/comment-page-1/#comment-64188</link>
		<dc:creator>JanieBelle</dc:creator>
		<pubDate>Thu, 17 Jan 2008 15:03:13 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/#comment-64188</guid>
		<description>From Dr. BA&#039;s original post:

&lt;blockquote&gt;I’m not sure what crater it is, or if it was even mapped by Mariner 10 back in ‘74;&lt;/blockquote&gt;

From the page at the Messenger site:

&lt;blockquote&gt;This is one of a set of 68 NAC images showing landscapes near Mercury’s equator on the side of the planet never before imaged by spacecraft.&lt;/blockquote&gt;

So I guess that&#039;s a &quot;no&quot;.

:)</description>
		<content:encoded><![CDATA[<p>From Dr. BA&#8217;s original post:</p>
<blockquote><p>I’m not sure what crater it is, or if it was even mapped by Mariner 10 back in ‘74;</p></blockquote>
<p>From the page at the Messenger site:</p>
<blockquote><p>This is one of a set of 68 NAC images showing landscapes near Mercury’s equator on the side of the planet never before imaged by spacecraft.</p></blockquote>
<p>So I guess that&#8217;s a &#8220;no&#8221;.<br />
 <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_smile.gif' alt=':)' class='wp-smiley' /> </p>
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		<title>By: Ken B</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/comment-page-1/#comment-64187</link>
		<dc:creator>Ken B</dc:creator>
		<pubDate>Thu, 17 Jan 2008 14:51:05 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/#comment-64187</guid>
		<description>So, anyone else notice the portrait of Coco at the bottom-center of the image?

http://images.google.com/imgres?imgurl=http://bp0.blogger.com/_Q55l_ERG5SI/RsIwWHTgkqI/AAAAAAAAAII/Ho4cnsoWxL8/s320/coco1%255B1%255D.jpg&amp;imgrefurl=http://gypsydoodlebug.blogspot.com/2007/08/one-word.html
http://gypsydoodlebug.blogspot.com/2007/08/one-word.html

(Or is that just another Jesus image?)</description>
		<content:encoded><![CDATA[<p>So, anyone else notice the portrait of Coco at the bottom-center of the image?</p>
<p><a href="http://images.google.com/imgres?imgurl=http://bp0.blogger.com/_Q55l_ERG5SI/RsIwWHTgkqI/AAAAAAAAAII/Ho4cnsoWxL8/s320/coco1%255B1%255D.jpg&#038;imgrefurl=http://gypsydoodlebug.blogspot.com/2007/08/one-word.html" rel="nofollow">http://images.google.com/imgres?imgurl=http://bp0.blogger.com/_Q55l_ERG5SI/RsIwWHTgkqI/AAAAAAAAAII/Ho4cnsoWxL8/s320/coco1%255B1%255D.jpg&#038;imgrefurl=http://gypsydoodlebug.blogspot.com/2007/08/one-word.html</a><br />
<a href="http://gypsydoodlebug.blogspot.com/2007/08/one-word.html" rel="nofollow">http://gypsydoodlebug.blogspot.com/2007/08/one-word.html</a></p>
<p>(Or is that just another Jesus image?)</p>
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		<title>By: Qfwfq</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/comment-page-1/#comment-64186</link>
		<dc:creator>Qfwfq</dc:creator>
		<pubDate>Thu, 17 Jan 2008 14:25:58 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/#comment-64186</guid>
		<description>Is it really so moon-like looking? Are those images b/w or is it really so colourless? In Mariner 10 pics I assumed they were b/w, but now, here we go and... more b/w! I expected some little surprise about.</description>
		<content:encoded><![CDATA[<p>Is it really so moon-like looking? Are those images b/w or is it really so colourless? In Mariner 10 pics I assumed they were b/w, but now, here we go and&#8230; more b/w! I expected some little surprise about.</p>
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		<title>By: Tom Marking</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/comment-page-1/#comment-64185</link>
		<dc:creator>Tom Marking</dc:creator>
		<pubDate>Thu, 17 Jan 2008 14:19:55 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/#comment-64185</guid>
		<description>Does NASA or anyone else have any future plans for a Mercury lander?  Or is Mercury considered to be too much like the earth&#039;s moon to bother with such a thing?

Also, what apparent motion of the sun would an observer see located on Mercury?  With an orbital period of 88 days and a rotation period of two thirds of that (i.e., 59 days) I believe that means that the apparent length of the day on Mercury is about 176 days.  But does the sun rise in the east like on Earth or the west?  Also, with an orbital eccentricity of 21 percent I wonder if there are any retrograde motions of the sun in the Mercurian sky.</description>
		<content:encoded><![CDATA[<p>Does NASA or anyone else have any future plans for a Mercury lander?  Or is Mercury considered to be too much like the earth&#8217;s moon to bother with such a thing?</p>
<p>Also, what apparent motion of the sun would an observer see located on Mercury?  With an orbital period of 88 days and a rotation period of two thirds of that (i.e., 59 days) I believe that means that the apparent length of the day on Mercury is about 176 days.  But does the sun rise in the east like on Earth or the west?  Also, with an orbital eccentricity of 21 percent I wonder if there are any retrograde motions of the sun in the Mercurian sky.</p>
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		<title>By: Michelle</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/comment-page-1/#comment-64184</link>
		<dc:creator>Michelle</dc:creator>
		<pubDate>Thu, 17 Jan 2008 14:00:22 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/#comment-64184</guid>
		<description>...Visually uninspiring? Allow me to disagree there. It&#039;s BEAUTIFUL. Absolutely gorgeous.

That full image of Mercury is now my wallpaper.</description>
		<content:encoded><![CDATA[<p>&#8230;Visually uninspiring? Allow me to disagree there. It&#8217;s BEAUTIFUL. Absolutely gorgeous.</p>
<p>That full image of Mercury is now my wallpaper.</p>
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		<title>By: Ian B Gibson</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/comment-page-1/#comment-64183</link>
		<dc:creator>Ian B Gibson</dc:creator>
		<pubDate>Thu, 17 Jan 2008 13:26:46 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/#comment-64183</guid>
		<description>Yep. There&#039;s no doubt that Mercury is visually uninspiring. Kind of like the Sacramento of the solar system. So it&#039;s a harder sell justifying the mission to the public since you&#039;ve got to talk about the usefulness of the data without lots of pretty pictures like you&#039;d get with many other bodies.</description>
		<content:encoded><![CDATA[<p>Yep. There&#8217;s no doubt that Mercury is visually uninspiring. Kind of like the Sacramento of the solar system. So it&#8217;s a harder sell justifying the mission to the public since you&#8217;ve got to talk about the usefulness of the data without lots of pretty pictures like you&#8217;d get with many other bodies.</p>
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		<title>By: Grand Lunar</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/comment-page-1/#comment-64182</link>
		<dc:creator>Grand Lunar</dc:creator>
		<pubDate>Thu, 17 Jan 2008 12:50:43 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/#comment-64182</guid>
		<description>Truly amazing!

Now Mercury seems more like a place then ever before. The iron planet is bound to have surprises in store for us.

An image at THIS range could be confused for the lunar surface. Funny, isn&#039;t it? From a distance, you can distinguish the two, but not up close (least, not without prior knowledge). Sort of oppisite of what you do with people.
Perhaps this could inspire a contest in the future, as more close-ups of Mercury arrive. Show images of Mercury randomly mixed with orbital images of the moon. Then, see how many can tell the two apart. Fun!

I wonder if the company Mercury knows of their namesake&#039;s new fame (okay, it was the god they were named after. But the planet was the inspiration for the name!).</description>
		<content:encoded><![CDATA[<p>Truly amazing!</p>
<p>Now Mercury seems more like a place then ever before. The iron planet is bound to have surprises in store for us.</p>
<p>An image at THIS range could be confused for the lunar surface. Funny, isn&#8217;t it? From a distance, you can distinguish the two, but not up close (least, not without prior knowledge). Sort of oppisite of what you do with people.<br />
Perhaps this could inspire a contest in the future, as more close-ups of Mercury arrive. Show images of Mercury randomly mixed with orbital images of the moon. Then, see how many can tell the two apart. Fun!</p>
<p>I wonder if the company Mercury knows of their namesake&#8217;s new fame (okay, it was the god they were named after. But the planet was the inspiration for the name!).</p>
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		<title>By: Barton Paul Levenson</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/comment-page-1/#comment-64181</link>
		<dc:creator>Barton Paul Levenson</dc:creator>
		<pubDate>Thu, 17 Jan 2008 11:31:21 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/#comment-64181</guid>
		<description>Quiet Desperation writes:

[[&lt;i&gt;In the Transmetropolitan graphic novels, it’s mentioned that Earth is powered by the energy transmitted from Mercury, which has been completely covered by solar panels.&lt;/i&gt;]]

Except that there&#039;s this thing called &quot;the inverse-square law...&quot;</description>
		<content:encoded><![CDATA[<p>Quiet Desperation writes:</p>
<p>[[<i>In the Transmetropolitan graphic novels, it’s mentioned that Earth is powered by the energy transmitted from Mercury, which has been completely covered by solar panels.</i>]]</p>
<p>Except that there&#8217;s this thing called &#8220;the inverse-square law&#8230;&#8221;</p>
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		<title>By: Jeffersonian</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/comment-page-1/#comment-64180</link>
		<dc:creator>Jeffersonian</dc:creator>
		<pubDate>Thu, 17 Jan 2008 08:58:38 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/#comment-64180</guid>
		<description>Since Phil so deftly described how researchers get use of the Hubble, I&#039;m curious about this probe. Is there info/data that non-NASA, interested parties have to apply for or wait in line for, or is the info all inferred from high res photos and, therefore, publicly available? (I clicked around a bit but it&#039;s probably faster to just ask here!).</description>
		<content:encoded><![CDATA[<p>Since Phil so deftly described how researchers get use of the Hubble, I&#8217;m curious about this probe. Is there info/data that non-NASA, interested parties have to apply for or wait in line for, or is the info all inferred from high res photos and, therefore, publicly available? (I clicked around a bit but it&#8217;s probably faster to just ask here!).</p>
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		<title>By: chris</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/comment-page-1/#comment-64179</link>
		<dc:creator>chris</dc:creator>
		<pubDate>Thu, 17 Jan 2008 07:38:27 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/01/16/more-mercury/#comment-64179</guid>
		<description>Totally off-topic, but I just got back from seeing Cloverfield (it opened today here in New Zealand). It is awesome. Intense and awesome.</description>
		<content:encoded><![CDATA[<p>Totally off-topic, but I just got back from seeing Cloverfield (it opened today here in New Zealand). It is awesome. Intense and awesome.</p>
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