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	<title>Comments on: Hubble spies carbon dioxide 600 trillion kilometers away!</title>
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	<link>http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/</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>Tue, 14 Feb 2012 18:23:05 +0000</lastBuildDate>
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		<title>By: hypnoticgenius</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/comment-page-2/#comment-214349</link>
		<dc:creator>hypnoticgenius</dc:creator>
		<pubDate>Sun, 20 Sep 2009 08:44:57 +0000</pubDate>
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		<description>Hi all,

New to the forum, just thought I&#039;d introduce myself :-)</description>
		<content:encoded><![CDATA[<p>Hi all,</p>
<p>New to the forum, just thought I&#8217;d introduce myself <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: StevoR</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/comment-page-2/#comment-140468</link>
		<dc:creator>StevoR</dc:creator>
		<pubDate>Fri, 12 Dec 2008 08:26:43 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/#comment-140468</guid>
		<description>&lt;b&gt;Bill Nettles wrote on Dec 11th, 2008 at 2:42 pm :
&lt;i&gt;  
&quot;.. I have to try to explain the difference between absolute and apparent magnitude to elementary education majors. That makes me hyperventilate, thus contributing to AGW...&quot; &lt;/i&gt;

If it&#039;s any help here&#039;s how I&#039;d explain it in three sentences :

Apparent magnitude is how bright a star * seems * in our sky. 

Absolute Magnitude is how bright a star really is compared with all other stars equally. 

This is done by  putting (in the minds eye) all the stars at the same standard distance of 10 parsces or 32.6 light years. 

I then usually use a couple of example such as our Sun which seems amazingly bright on Earth where its 8 light minutes away at - 27 apparent magnitude but is actually rather faint in absolute magnitude because at 32.6 ly off it shines at a mere  + 4.82 or about as bright as the stars  Alpha Sextans (4.6 app. mag) and Alpha (4.4) &amp; Beta Sagittae. (4.4 also)

In the southern hemisphere the two pointers to the Southern Cross - Alpha Centauri (Rigil Kent or Toliman) and Beta Centauri (Hadar or Agena) areanother good demonstration :  Alpha Centauri is the closest visible star to the Sun at 4.3 light years and seems just a bit brighter than Beta Centauri inour skies. Yet Beta Centauri is about 520 light years away - and thus in reality a far, far brighter star with an absolute magnitude around 
-6 to - 7! 

&#039;Spose its too late now but anyway I hope that helps!  

Thanks &lt;b&gt; Tom Marking &lt;/b&gt; some great examples there &amp; yes I too would love to see more astronomical art featuring those worlds  - and have those exoplanetary systems given halfway reasonable names not just forgettable and unpronouncable catalogue numbers!</description>
		<content:encoded><![CDATA[<p><b>Bill Nettles wrote on Dec 11th, 2008 at 2:42 pm :<br />
<i><br />
&#8220;.. I have to try to explain the difference between absolute and apparent magnitude to elementary education majors. That makes me hyperventilate, thus contributing to AGW&#8230;&#8221; </i></p>
<p>If it&#8217;s any help here&#8217;s how I&#8217;d explain it in three sentences :</p>
<p>Apparent magnitude is how bright a star * seems * in our sky. </p>
<p>Absolute Magnitude is how bright a star really is compared with all other stars equally. </p>
<p>This is done by  putting (in the minds eye) all the stars at the same standard distance of 10 parsces or 32.6 light years. </p>
<p>I then usually use a couple of example such as our Sun which seems amazingly bright on Earth where its 8 light minutes away at &#8211; 27 apparent magnitude but is actually rather faint in absolute magnitude because at 32.6 ly off it shines at a mere  + 4.82 or about as bright as the stars  Alpha Sextans (4.6 app. mag) and Alpha (4.4) &#038; Beta Sagittae. (4.4 also)</p>
<p>In the southern hemisphere the two pointers to the Southern Cross &#8211; Alpha Centauri (Rigil Kent or Toliman) and Beta Centauri (Hadar or Agena) areanother good demonstration :  Alpha Centauri is the closest visible star to the Sun at 4.3 light years and seems just a bit brighter than Beta Centauri inour skies. Yet Beta Centauri is about 520 light years away &#8211; and thus in reality a far, far brighter star with an absolute magnitude around<br />
-6 to &#8211; 7! </p>
<p>&#8216;Spose its too late now but anyway I hope that helps!  </p>
<p>Thanks </b><b> Tom Marking </b> some great examples there &#038; yes I too would love to see more astronomical art featuring those worlds  &#8211; and have those exoplanetary systems given halfway reasonable names not just forgettable and unpronouncable catalogue numbers!</p>
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		<title>By: Bill Nettles</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/comment-page-2/#comment-140355</link>
		<dc:creator>Bill Nettles</dc:creator>
		<pubDate>Thu, 11 Dec 2008 21:42:07 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/#comment-140355</guid>
		<description>Daniel,
I appreciate the encouragement, but I&#039;ve got bigger problems. I have to try to explain the difference between absolute and apparent magnitude to elementary education majors.  That makes me hyperventilate, thus contributing to AGW.  And now &lt;a href=&quot;http://www.nature.com/news/2008/081209/full/456686a.html&quot; rel=&quot;nofollow&quot;&gt;the Carbon market has collapsed.&lt;/a&gt;

Bill</description>
		<content:encoded><![CDATA[<p>Daniel,<br />
I appreciate the encouragement, but I&#8217;ve got bigger problems. I have to try to explain the difference between absolute and apparent magnitude to elementary education majors.  That makes me hyperventilate, thus contributing to AGW.  And now <a href="http://www.nature.com/news/2008/081209/full/456686a.html" rel="nofollow">the Carbon market has collapsed.</a></p>
<p>Bill</p>
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		<title>By: Tom Marking</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/comment-page-2/#comment-140259</link>
		<dc:creator>Tom Marking</dc:creator>
		<pubDate>Thu, 11 Dec 2008 18:02:19 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/#comment-140259</guid>
		<description>@StevoR &quot;The ‘WooS’ was a site I stumbled over when searching for exoplanet info which seemed, heck, still seems pretty good. Yes they are probably being wa-aay overly optimistic when it comes to the chances of life on “Hoth” - but, hey, we can’t really prove that wrong now can we?&quot;

I wonder if the folks at WooS have ever heard of something called the CHZ (Circumstellar Habitable Zone).  Hoth doesn&#039;t seem to be located inside of it.  The following exoplanets are located inside of it for their entire orbit assuming certain values for the albedo and greenhouse temperature increase.  I&#039;d like to see some artistic renditions of some of moons of these planets which have a much better chance of containing life than Hoth does:

HD 10647b:
Semi-major axis = 2.03 AU
Eccentricity = 0.16
Periastrion = 1.71 AU
Apastrion = 2.35 AU
Orbital period = 1,003 days
Mass is greater than 0.93 Jupiter masses
If albedo = 0.15 and greenhouse temperature increase = 80 deg K then
habitable zone goes from 1.49 AU to 2.36 AU

HD 134987	b:
Semi-major axis = 0.82 AU
Eccentricity = 0.224
Periastrion = 0.64 AU
Apastrion = 1.00 AU
Orbital period = 258 days
Mass is greater than 1.61 Jupiter masses
If albedo = 0.84 and greenhouse temperature increase = 79 deg K then
habitable zone goes from 0.638 AU to 1.01 AU

HD 23079b:
Semi-major axis = 1.60 AU
Eccentricity = 0.102
Periastrion = 1.44 AU
Apastrion = 1.76 AU
Orbital period = 730.6 days
Mass is greater than 2.45 Jupiter masses
If albedo = 0.15 and greenhouse temperature increase = 70 deg K then
habitable zone goes from 1.14 AU to 1.77 AU

HD 28185b:
Semi-major axis = 1.03 AU
Eccentricity = 0.070
Periastrion = 0.96 AU
Apastrion = 1.10 AU
Orbital period = 383 days
Mass is greater than 5.72 Jupiter masses
If albedo = 0.37 and greenhouse temperature increase = 40 deg K then
habitable zone goes from 0.776 AU to 1.14 AU

HD 188015	b:
Semi-major axis = 1.20 AU
Eccentricity = 0.137
Periastrion = 1.04 AU
Apastrion = 1.36 AU
Orbital period = 461 days
Mass is greater than 1.50 Jupiter masses
If albedo = 0.26 and greenhouse temperature increase = 40 deg K then
habitable zone goes from 0.923 AU to 1.36 AU

HD 99109b:
Semi-major axis = 1.10 AU
Eccentricity = 0.09
Periastrion = 1.00 AU
Apastrion = 1.20 AU
Orbital period = 439 days
Mass is greater than 0.502 Jupiter masses
If albedo = 0.15 and greenhouse temperature increase = 48 deg K then
habitable zone goes from 0.804 AU to 1.20 AU

HD 108874	b:
Semi-major axis = 1.05 AU
Eccentricity = 0.114
Periastrion = 0.93 AU
Apastrion = 1.17 AU
Orbital period = 394 days
Mass is greater than 1.30 Jupiter masses
If albedo = 0.37 and greenhouse temperature increase = 40 deg K then
habitable zone goes from 0.820 AU to 1.21 AU</description>
		<content:encoded><![CDATA[<p>@StevoR &#8220;The ‘WooS’ was a site I stumbled over when searching for exoplanet info which seemed, heck, still seems pretty good. Yes they are probably being wa-aay overly optimistic when it comes to the chances of life on “Hoth” &#8211; but, hey, we can’t really prove that wrong now can we?&#8221;</p>
<p>I wonder if the folks at WooS have ever heard of something called the CHZ (Circumstellar Habitable Zone).  Hoth doesn&#8217;t seem to be located inside of it.  The following exoplanets are located inside of it for their entire orbit assuming certain values for the albedo and greenhouse temperature increase.  I&#8217;d like to see some artistic renditions of some of moons of these planets which have a much better chance of containing life than Hoth does:</p>
<p>HD 10647b:<br />
Semi-major axis = 2.03 AU<br />
Eccentricity = 0.16<br />
Periastrion = 1.71 AU<br />
Apastrion = 2.35 AU<br />
Orbital period = 1,003 days<br />
Mass is greater than 0.93 Jupiter masses<br />
If albedo = 0.15 and greenhouse temperature increase = 80 deg K then<br />
habitable zone goes from 1.49 AU to 2.36 AU</p>
<p>HD 134987	b:<br />
Semi-major axis = 0.82 AU<br />
Eccentricity = 0.224<br />
Periastrion = 0.64 AU<br />
Apastrion = 1.00 AU<br />
Orbital period = 258 days<br />
Mass is greater than 1.61 Jupiter masses<br />
If albedo = 0.84 and greenhouse temperature increase = 79 deg K then<br />
habitable zone goes from 0.638 AU to 1.01 AU</p>
<p>HD 23079b:<br />
Semi-major axis = 1.60 AU<br />
Eccentricity = 0.102<br />
Periastrion = 1.44 AU<br />
Apastrion = 1.76 AU<br />
Orbital period = 730.6 days<br />
Mass is greater than 2.45 Jupiter masses<br />
If albedo = 0.15 and greenhouse temperature increase = 70 deg K then<br />
habitable zone goes from 1.14 AU to 1.77 AU</p>
<p>HD 28185b:<br />
Semi-major axis = 1.03 AU<br />
Eccentricity = 0.070<br />
Periastrion = 0.96 AU<br />
Apastrion = 1.10 AU<br />
Orbital period = 383 days<br />
Mass is greater than 5.72 Jupiter masses<br />
If albedo = 0.37 and greenhouse temperature increase = 40 deg K then<br />
habitable zone goes from 0.776 AU to 1.14 AU</p>
<p>HD 188015	b:<br />
Semi-major axis = 1.20 AU<br />
Eccentricity = 0.137<br />
Periastrion = 1.04 AU<br />
Apastrion = 1.36 AU<br />
Orbital period = 461 days<br />
Mass is greater than 1.50 Jupiter masses<br />
If albedo = 0.26 and greenhouse temperature increase = 40 deg K then<br />
habitable zone goes from 0.923 AU to 1.36 AU</p>
<p>HD 99109b:<br />
Semi-major axis = 1.10 AU<br />
Eccentricity = 0.09<br />
Periastrion = 1.00 AU<br />
Apastrion = 1.20 AU<br />
Orbital period = 439 days<br />
Mass is greater than 0.502 Jupiter masses<br />
If albedo = 0.15 and greenhouse temperature increase = 48 deg K then<br />
habitable zone goes from 0.804 AU to 1.20 AU</p>
<p>HD 108874	b:<br />
Semi-major axis = 1.05 AU<br />
Eccentricity = 0.114<br />
Periastrion = 0.93 AU<br />
Apastrion = 1.17 AU<br />
Orbital period = 394 days<br />
Mass is greater than 1.30 Jupiter masses<br />
If albedo = 0.37 and greenhouse temperature increase = 40 deg K then<br />
habitable zone goes from 0.820 AU to 1.21 AU</p>
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		<title>By: StevoR-Correcting</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/comment-page-2/#comment-140203</link>
		<dc:creator>StevoR-Correcting</dc:creator>
		<pubDate>Thu, 11 Dec 2008 15:28:40 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/#comment-140203</guid>
		<description>@ &lt;b&gt;Joker &lt;/b&gt;  : 

&quot;Decency&quot; is all the mind of the beholder! ;-)
Its like art that way. 

Correction (sigh) : 

&quot;On Earth we know of extremophiles and bacteria that can endure staggering amounts of heat, cold, radiation, lack of water, the presence of concentrated acids and alkais, etc .. Below our feet it has been suggested a whole region of &#039;deep hot biosphere&#039; exists perhaps including silicon based microbes!&quot; 

&lt;b&gt;Tom Marking&#039;s&lt;/b&gt; quote was meant to be in italics too .. :-( 

When is this editing option coming again? 

Any chance it could speed up &amp; get here! I need it yesterday! ;-)  :-(</description>
		<content:encoded><![CDATA[<p>@ <b>Joker </b>  : </p>
<p>&#8220;Decency&#8221; is all the mind of the beholder! <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_wink.gif' alt=';-)' class='wp-smiley' /><br />
Its like art that way. </p>
<p>Correction (sigh) : </p>
<p>&#8220;On Earth we know of extremophiles and bacteria that can endure staggering amounts of heat, cold, radiation, lack of water, the presence of concentrated acids and alkais, etc .. Below our feet it has been suggested a whole region of &#8216;deep hot biosphere&#8217; exists perhaps including silicon based microbes!&#8221; </p>
<p><b>Tom Marking&#8217;s</b> quote was meant to be in italics too .. <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_sad.gif' alt=':-(' class='wp-smiley' />  </p>
<p>When is this editing option coming again? </p>
<p>Any chance it could speed up &#038; get here! I need it yesterday! <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_wink.gif' alt=';-)' class='wp-smiley' />   <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_sad.gif' alt=':-(' class='wp-smiley' /> </p>
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		<title>By: Plutonium being from Pluto</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/comment-page-1/#comment-140202</link>
		<dc:creator>Plutonium being from Pluto</dc:creator>
		<pubDate>Thu, 11 Dec 2008 15:17:55 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/#comment-140202</guid>
		<description>Actually there&#039;s life on Pluto too! 

Our species lives around Pluto&#039;s core-mantle interface on a thin layer of plutonium that&#039;s found in the Plutonian core. Our mantle is like Euopa&#039;s (&amp; even Eris&#039;es) in having a subterrerean ocean hidden below an icy crust. Charon&#039;s tides keeps our planet nice and geologically active - Nix &amp; hydras&#039; tides not-so much! ;-)  

Its a pretty cool way to live! ;-) 8)

We&#039;ve been around far longer than your youthful species and are &lt;i&gt; (hate to boast but true) &lt;/i&gt; far more advanced than Humanity. When your &#039;New Horizons&#039; probe flies by you&#039;ll see our cities as hollows on the Plutonian surface &amp; then you&#039;ll find us out officially. ;-) 

We&#039;ve actually got a faster than light wormhole device and lots more techno-goodies which we were going to share with humanity to fix things up for ya a litle - getting your spacecraft to all the planets (Pluto most of all!) was our criteria for you proving yourselves worthy of this aid. :-) 

But then you had to go &amp; spoil it all by refusing our world proper planetary status so now you&#039;re going to miss out! We&#039;re kinda patriotic that way! :-P ;-)

Well  you&#039;ll just miss out - at least until you&#039;ve included us on your planets list again and given each of the anti-Pluto IAU members a televised kick up the backside anyway! ;-)</description>
		<content:encoded><![CDATA[<p>Actually there&#8217;s life on Pluto too! </p>
<p>Our species lives around Pluto&#8217;s core-mantle interface on a thin layer of plutonium that&#8217;s found in the Plutonian core. Our mantle is like Euopa&#8217;s (&#038; even Eris&#8217;es) in having a subterrerean ocean hidden below an icy crust. Charon&#8217;s tides keeps our planet nice and geologically active &#8211; Nix &#038; hydras&#8217; tides not-so much! <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_wink.gif' alt=';-)' class='wp-smiley' />   </p>
<p>Its a pretty cool way to live! <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_wink.gif' alt=';-)' class='wp-smiley' />  <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_cool.gif' alt='8)' class='wp-smiley' /> </p>
<p>We&#8217;ve been around far longer than your youthful species and are <i> (hate to boast but true) </i> far more advanced than Humanity. When your &#8216;New Horizons&#8217; probe flies by you&#8217;ll see our cities as hollows on the Plutonian surface &#038; then you&#8217;ll find us out officially. <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_wink.gif' alt=';-)' class='wp-smiley' />  </p>
<p>We&#8217;ve actually got a faster than light wormhole device and lots more techno-goodies which we were going to share with humanity to fix things up for ya a litle &#8211; getting your spacecraft to all the planets (Pluto most of all!) was our criteria for you proving yourselves worthy of this aid. <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_smile.gif' alt=':-)' class='wp-smiley' />  </p>
<p>But then you had to go &#038; spoil it all by refusing our world proper planetary status so now you&#8217;re going to miss out! We&#8217;re kinda patriotic that way! <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_razz.gif' alt=':-P' class='wp-smiley' />  <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_wink.gif' alt=';-)' class='wp-smiley' /> </p>
<p>Well  you&#8217;ll just miss out &#8211; at least until you&#8217;ve included us on your planets list again and given each of the anti-Pluto IAU members a televised kick up the backside anyway! <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_wink.gif' alt=';-)' class='wp-smiley' /> </p>
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		<title>By: StevoR</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/comment-page-1/#comment-140195</link>
		<dc:creator>StevoR</dc:creator>
		<pubDate>Thu, 11 Dec 2008 15:04:29 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/#comment-140195</guid>
		<description>I&#039;ve just  emailed the WooS site author(s?) via their contact link &amp; told them to feel free to visit here. Can&#039;t find anything on there on who they are but then even this still-on-dial-up &amp; not-very-net-savvy web-sufer knows identity can be problematic on the net although they seem legit to me.

Bear in mind too that life has been known or speculated to exist in some pretty astonishing and harsh places. 

On Earth we know of extremophiles and bacteria thatcan endure staggeringamoiunts of heat, cold, radiation, lack of water, presenceof acids and alkais etc .. Below our feet itha sbeen suggested awhole region of deep hotbiosphere exists perhaps including silicon based microbes!  

Elsewhere within our solar system there is possible life on Mars, Europa, Encleadus, Titan, etc .. Arthur C.Clarke has plausibly imagined aerial lifeforms living in the clouds of Jupiter.  Ben Bova has made at least a reasonable speculative case for life existing in his novels on Mars, in the clouds and on the surface of venus, even in the rings of Saturn - see his Sf novels. 

Now I know that&#039;s science fiction where imagination is given more reign but extraopolating to how &#039;Hoth&#039; may be (&amp;how very little wereallyknow for certain about it) I wouldn&#039;t rule out the possibility of &#039;Hoth&#039; having life. Not that I&#039;d put the odds at 100% or anywhere near that but still ..  

 ... I&#039;d love to see us invent an FTL drive and go see! ;-) 
&lt;i&gt;
(Yes, yes, I know that may well NOT be possible either. I love both Sf and science - wish the latter would help accomplish the dreams of the former a bit more rather than squash &#039;em with gosh-durned relativity &amp; so forth.;-) )
 &lt;/i&gt;</description>
		<content:encoded><![CDATA[<p>I&#8217;ve just  emailed the WooS site author(s?) via their contact link &#038; told them to feel free to visit here. Can&#8217;t find anything on there on who they are but then even this still-on-dial-up &#038; not-very-net-savvy web-sufer knows identity can be problematic on the net although they seem legit to me.</p>
<p>Bear in mind too that life has been known or speculated to exist in some pretty astonishing and harsh places. </p>
<p>On Earth we know of extremophiles and bacteria thatcan endure staggeringamoiunts of heat, cold, radiation, lack of water, presenceof acids and alkais etc .. Below our feet itha sbeen suggested awhole region of deep hotbiosphere exists perhaps including silicon based microbes!  </p>
<p>Elsewhere within our solar system there is possible life on Mars, Europa, Encleadus, Titan, etc .. Arthur C.Clarke has plausibly imagined aerial lifeforms living in the clouds of Jupiter.  Ben Bova has made at least a reasonable speculative case for life existing in his novels on Mars, in the clouds and on the surface of venus, even in the rings of Saturn &#8211; see his Sf novels. </p>
<p>Now I know that&#8217;s science fiction where imagination is given more reign but extraopolating to how &#8216;Hoth&#8217; may be (&#038;how very little wereallyknow for certain about it) I wouldn&#8217;t rule out the possibility of &#8216;Hoth&#8217; having life. Not that I&#8217;d put the odds at 100% or anywhere near that but still ..  </p>
<p> &#8230; I&#8217;d love to see us invent an FTL drive and go see! <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_wink.gif' alt=';-)' class='wp-smiley' /><br />
<i><br />
(Yes, yes, I know that may well NOT be possible either. I love both Sf and science &#8211; wish the latter would help accomplish the dreams of the former a bit more rather than squash &#8216;em with gosh-durned relativity &#038; so forth.;-) )<br />
 </i></p>
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		<title>By: StevoR</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/comment-page-1/#comment-140180</link>
		<dc:creator>StevoR</dc:creator>
		<pubDate>Thu, 11 Dec 2008 14:11:41 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/#comment-140180</guid>
		<description>&lt;b&gt; IVAN3MAN &lt;/b&gt; said :

&quot;Also, I see that you have a bad problem with “typos”. I’m sure that you will be relieved to hear that according to the Discover Web Editor, Amos Kenigsberg, we will have a preview/edit facility here on B.A. Blog sometime early next year in January/February.&quot; 

He-elll yes!!! Can&#039;t come soon enough as far as I&#039;m concerned! Great news. :-D 

&lt;b&gt; Tom Marking said on December 10th, 2008 at 12:27 pm : 

&quot;@StevoR “You can go to one of my sources - “Worlds of other Suns” - via clicking my name above - for the named worlds listed earlier. Its an exoplanets website (not mine but a fave of mine) with examples of … er very optimistically but well written info &amp; superbly illustrated exoplanets as named (Hoth Tatooine etc ..) Hopefully interesting for people! Hopefully the link’ll work!”

Concerning the planet Hoth (i.e., OGLE-2005-BLG-390Lb) the URL you provided says the following:

“WoOS gives this planet a 100% probability of harboring it’s own life and ecosystem, a notable first among the discovered Exoplanets. It would be almost impossible for such a world to not have some form of life.” 

Huh? The planet is totally frozen and yet it has a 100% probability of having life? What/who is WoOS and what criteria are being used for this probability? According to Wikipedia the planet’s surface temperature is only 50 degrees Kelvin. This is a slam dunk for life? I don’t think so.&quot; &lt;/i&gt;


Nah, me neither. :-) That&#039;s why I wrote : 

&quot; Its [Worlds of Other Suns) an exoplanets website (not mine but a fave of mine) with examples of &lt;b&gt; … er very optimistically &lt;/b&gt; but well written info &amp; superbly illustrated exoplanets as named (Hoth Tatooine etc ..) 

Mind you, we &lt;b&gt;don&#039;t&lt;/b&gt; actually &lt;i&gt;know &lt;/i&gt; for sure that &#039;Hoth&#039; is frozen either .. Who is to say that it hasn&#039;t got a fair bit of geothermal heat and all sorts of other energy sources keeping it or areas on it warm? (Meteorite impacts? Extreme atmospheric factors like greenhosue gases? Pyromanic alien friends? ;-) )  

The &#039;WooS&#039; was a site I stumbled over when searching for exoplanet info which seemed, heck, still seems pretty good. Yes they are probably being wa-aay overly optimistic when it comes to the chances of life on &quot;Hoth&quot; - but, hey, we can&#039;t really prove that wrong now can we? ;-) 

(ok, ok, I * know * the burden of proof is on those making the extraordinary claims and the chances aren&#039;t 100 % as they suggest and so on but well ..putting that aside I still reckon its a pretty good website &amp; I like their naming ideas -&amp; spaceart - too! ;-) )</description>
		<content:encoded><![CDATA[<p><b> IVAN3MAN </b> said :</p>
<p>&#8220;Also, I see that you have a bad problem with “typos”. I’m sure that you will be relieved to hear that according to the Discover Web Editor, Amos Kenigsberg, we will have a preview/edit facility here on B.A. Blog sometime early next year in January/February.&#8221; </p>
<p>He-elll yes!!! Can&#8217;t come soon enough as far as I&#8217;m concerned! Great news. <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_biggrin.gif' alt=':-D' class='wp-smiley' />  </p>
<p><b> Tom Marking said on December 10th, 2008 at 12:27 pm : </p>
<p>&#8220;@StevoR “You can go to one of my sources &#8211; “Worlds of other Suns” &#8211; via clicking my name above &#8211; for the named worlds listed earlier. Its an exoplanets website (not mine but a fave of mine) with examples of … er very optimistically but well written info &#038; superbly illustrated exoplanets as named (Hoth Tatooine etc ..) Hopefully interesting for people! Hopefully the link’ll work!”</p>
<p>Concerning the planet Hoth (i.e., OGLE-2005-BLG-390Lb) the URL you provided says the following:</p>
<p>“WoOS gives this planet a 100% probability of harboring it’s own life and ecosystem, a notable first among the discovered Exoplanets. It would be almost impossible for such a world to not have some form of life.” </p>
<p>Huh? The planet is totally frozen and yet it has a 100% probability of having life? What/who is WoOS and what criteria are being used for this probability? According to Wikipedia the planet’s surface temperature is only 50 degrees Kelvin. This is a slam dunk for life? I don’t think so.&#8221; </p>
<p>Nah, me neither. <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_smile.gif' alt=':-)' class='wp-smiley' />  That&#8217;s why I wrote : </p>
<p>&#8221; Its [Worlds of Other Suns) an exoplanets website (not mine but a fave of mine) with examples of </b><b> … er very optimistically </b> but well written info &#038; superbly illustrated exoplanets as named (Hoth Tatooine etc ..) </p>
<p>Mind you, we <b>don&#8217;t</b> actually <i>know </i> for sure that &#8216;Hoth&#8217; is frozen either .. Who is to say that it hasn&#8217;t got a fair bit of geothermal heat and all sorts of other energy sources keeping it or areas on it warm? (Meteorite impacts? Extreme atmospheric factors like greenhosue gases? Pyromanic alien friends? <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_wink.gif' alt=';-)' class='wp-smiley' />  )  </p>
<p>The &#8216;WooS&#8217; was a site I stumbled over when searching for exoplanet info which seemed, heck, still seems pretty good. Yes they are probably being wa-aay overly optimistic when it comes to the chances of life on &#8220;Hoth&#8221; &#8211; but, hey, we can&#8217;t really prove that wrong now can we? <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_wink.gif' alt=';-)' class='wp-smiley' />  </p>
<p>(ok, ok, I * know * the burden of proof is on those making the extraordinary claims and the chances aren&#8217;t 100 % as they suggest and so on but well ..putting that aside I still reckon its a pretty good website &#038; I like their naming ideas -&#038; spaceart &#8211; too! <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_wink.gif' alt=';-)' class='wp-smiley' />  )</p>
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		<title>By: Nigel Depledge</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/comment-page-1/#comment-140170</link>
		<dc:creator>Nigel Depledge</dc:creator>
		<pubDate>Thu, 11 Dec 2008 12:35:20 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/#comment-140170</guid>
		<description>Glenn Schneider said:
&lt;blockquote&gt;I’m not a cosmochemsit, don’t claim to be, but when I took Organic Chemestry
I had learned that it was not just CO an CO2 that are not considered organic compounds, but also carbonates, cyanides, and allotroic forms of carbon itself.
Happy to be corrected if need be.&lt;/blockquote&gt;

Glenn, in my understanding, CO, CO2, carbonate and bicarbonate are considered inorganic as you indicate.  Elemental carbon is also considered inorganic, but cyanides depend on the compound.  If the cyanide is clearly ionic in nature, as it is in KCN, it is considered inorganic.  If, however, it forms a functional group within an organic compound (such as acetonitrile), it is quite OK to consider CN to be organic.</description>
		<content:encoded><![CDATA[<p>Glenn Schneider said:</p>
<blockquote><p>I’m not a cosmochemsit, don’t claim to be, but when I took Organic Chemestry<br />
I had learned that it was not just CO an CO2 that are not considered organic compounds, but also carbonates, cyanides, and allotroic forms of carbon itself.<br />
Happy to be corrected if need be.</p></blockquote>
<p>Glenn, in my understanding, CO, CO2, carbonate and bicarbonate are considered inorganic as you indicate.  Elemental carbon is also considered inorganic, but cyanides depend on the compound.  If the cyanide is clearly ionic in nature, as it is in KCN, it is considered inorganic.  If, however, it forms a functional group within an organic compound (such as acetonitrile), it is quite OK to consider CN to be organic.</p>
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		<title>By: Daniel J. Andrews</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/comment-page-1/#comment-140064</link>
		<dc:creator>Daniel J. Andrews</dc:creator>
		<pubDate>Thu, 11 Dec 2008 00:54:36 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/#comment-140064</guid>
		<description>Then you need to read IPCC and Real Climate a little more carefully, Bill. :-) 


[cultural reference]
Phil...I like your use of  &quot;embiggen&quot; underneath the picture.  If anyone complains that it isn&#039;t a real word tell them it is a perfectly &quot;cromulent&quot; word. ;-)
 [/cultural reference]</description>
		<content:encoded><![CDATA[<p>Then you need to read IPCC and Real Climate a little more carefully, Bill. <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_smile.gif' alt=':-)' class='wp-smiley' />  </p>
<p>[cultural reference]<br />
Phil&#8230;I like your use of  &#8220;embiggen&#8221; underneath the picture.  If anyone complains that it isn&#8217;t a real word tell them it is a perfectly &#8220;cromulent&#8221; word. <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_wink.gif' alt=';-)' class='wp-smiley' /><br />
 [/cultural reference]</p>
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		<title>By: Bill Nettles</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/comment-page-1/#comment-140044</link>
		<dc:creator>Bill Nettles</dc:creator>
		<pubDate>Wed, 10 Dec 2008 23:42:03 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/#comment-140044</guid>
		<description>Golly gee, Phil. IPCC and Real Climate had me believing that the only sources of CO2 in the universe were from humans.  Imagine...CO2 occuring without human intervention.

Smile!</description>
		<content:encoded><![CDATA[<p>Golly gee, Phil. IPCC and Real Climate had me believing that the only sources of CO2 in the universe were from humans.  Imagine&#8230;CO2 occuring without human intervention.</p>
<p>Smile!</p>
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		<title>By: Tom Marking</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/comment-page-1/#comment-139942</link>
		<dc:creator>Tom Marking</dc:creator>
		<pubDate>Wed, 10 Dec 2008 19:27:09 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/#comment-139942</guid>
		<description>@StevoR &quot;You can go to one of my sources - “Worlds of other Suns” - via clicking my name above - for the named worlds listed earlier. Its an exoplanets website (not mine but a fave of mine) with examples of … er very optimistically but well written info &amp; superbly illustrated exoplanets as named (Hoth Tatooine etc ..) Hopefully interesting for people! Hopefully the link’ll work!&quot;

Concerning the planet Hoth (i.e., OGLE-2005-BLG-390Lb) the URL you provided says the following:

&quot;WoOS gives this planet a 100% probability of harboring it&#039;s own life and ecosystem, a notable first among the discovered Exoplanets. It would be almost impossible for such a world to not have some form of life.&quot; 

Huh?  The planet is totally frozen and yet it has a 100% probability of having life?  What/who is WoOS and what criteria are being used for this probability?  According to Wikipedia the planet&#039;s surface temperature is only 50 degrees Kelvin.  This is a slam dunk for life?  I don&#039;t think so.</description>
		<content:encoded><![CDATA[<p>@StevoR &#8220;You can go to one of my sources &#8211; “Worlds of other Suns” &#8211; via clicking my name above &#8211; for the named worlds listed earlier. Its an exoplanets website (not mine but a fave of mine) with examples of … er very optimistically but well written info &#038; superbly illustrated exoplanets as named (Hoth Tatooine etc ..) Hopefully interesting for people! Hopefully the link’ll work!&#8221;</p>
<p>Concerning the planet Hoth (i.e., OGLE-2005-BLG-390Lb) the URL you provided says the following:</p>
<p>&#8220;WoOS gives this planet a 100% probability of harboring it&#8217;s own life and ecosystem, a notable first among the discovered Exoplanets. It would be almost impossible for such a world to not have some form of life.&#8221; </p>
<p>Huh?  The planet is totally frozen and yet it has a 100% probability of having life?  What/who is WoOS and what criteria are being used for this probability?  According to Wikipedia the planet&#8217;s surface temperature is only 50 degrees Kelvin.  This is a slam dunk for life?  I don&#8217;t think so.</p>
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		<title>By: Tom Marking</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/comment-page-1/#comment-139932</link>
		<dc:creator>Tom Marking</dc:creator>
		<pubDate>Wed, 10 Dec 2008 19:07:25 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/#comment-139932</guid>
		<description>@Sarafan &quot;I was thinking the same thing… well more specificaly, what keeps the water vapor from dissasociating that close to a star?&quot;

I think steam can exist at the prevailing surface temperature of 1,100 deg K.  If I&#039;m not mistaken don&#039;t some pressurized water nuclear reactors have steam that hot?  I believe you have to go up to temperatures similar to the surface of stars (~3,000 deg K) before you get significant thermal dissociation.

The UV flux might be a different issue.  HD 189733 is a K1-2 main sequence star with a luminosity of 0.264 suns and surface temperature of 4,980 deg K.  That means that out of a total luminosity of 0.264 suns, 0.0135 suns (5.1%) is emitted in the ultraviolet, 0.100 suns (37.9%) is emitted in visible light, and 0.1505 (57.0%) suns is emitted in the infrared.  The UV flux landing on HD 189733 b is quite substantial, 19,200 watts per square meter.  So there should be substantial UV-induced photodissociation of H2O into the hydroxyl molecule OH and hydrogen H.  I wonder if hydroxyl has been detected in the spectrum.  Does anyone know?</description>
		<content:encoded><![CDATA[<p>@Sarafan &#8220;I was thinking the same thing… well more specificaly, what keeps the water vapor from dissasociating that close to a star?&#8221;</p>
<p>I think steam can exist at the prevailing surface temperature of 1,100 deg K.  If I&#8217;m not mistaken don&#8217;t some pressurized water nuclear reactors have steam that hot?  I believe you have to go up to temperatures similar to the surface of stars (~3,000 deg K) before you get significant thermal dissociation.</p>
<p>The UV flux might be a different issue.  HD 189733 is a K1-2 main sequence star with a luminosity of 0.264 suns and surface temperature of 4,980 deg K.  That means that out of a total luminosity of 0.264 suns, 0.0135 suns (5.1%) is emitted in the ultraviolet, 0.100 suns (37.9%) is emitted in visible light, and 0.1505 (57.0%) suns is emitted in the infrared.  The UV flux landing on HD 189733 b is quite substantial, 19,200 watts per square meter.  So there should be substantial UV-induced photodissociation of H2O into the hydroxyl molecule OH and hydrogen H.  I wonder if hydroxyl has been detected in the spectrum.  Does anyone know?</p>
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		<title>By: Tom Marking</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/comment-page-1/#comment-139927</link>
		<dc:creator>Tom Marking</dc:creator>
		<pubDate>Wed, 10 Dec 2008 18:48:22 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/#comment-139927</guid>
		<description>@Ed H &quot;With the planet being that close to its star and still having an atmosphere that hasn’t been completely blasted away by the stellar (guess we can’t say “solar” =) winds, can we assume that this planet must have a strong magnetic field protecting its atmosphere? Or is something else at work here?&quot;

Probably most theories of planet formation would predict a rapid rotation for Jovian sized planets or bigger planets.  However, this particular planet is thought to be tidally locked to its star so that it&#039;s rotation period is 2.2 days - 5 times slower than Jupiter.  So perhaps it&#039;s magnetic field is less than Jupiter&#039;s, say 1 gauss at the equator instead of Jupiter&#039;s value of 4 gauss at the equator.  Nevertheless, there should be a substantial magnetosphere to protect the atmosphere.

On the other hand, Venus has no internally dynamo-generated magnetic field and yet it has an induced magnetosphere caused by the interaction of the planet with the solar wind.  Apparently this weak induced magnetosphere has been sufficient to prevent the loss of Venus&#039; atmosphere into space during the last 4.5 billion years.  So an internal magnetic field is not absolutely necessary to prevent atmospheric loss.</description>
		<content:encoded><![CDATA[<p>@Ed H &#8220;With the planet being that close to its star and still having an atmosphere that hasn’t been completely blasted away by the stellar (guess we can’t say “solar” =) winds, can we assume that this planet must have a strong magnetic field protecting its atmosphere? Or is something else at work here?&#8221;</p>
<p>Probably most theories of planet formation would predict a rapid rotation for Jovian sized planets or bigger planets.  However, this particular planet is thought to be tidally locked to its star so that it&#8217;s rotation period is 2.2 days &#8211; 5 times slower than Jupiter.  So perhaps it&#8217;s magnetic field is less than Jupiter&#8217;s, say 1 gauss at the equator instead of Jupiter&#8217;s value of 4 gauss at the equator.  Nevertheless, there should be a substantial magnetosphere to protect the atmosphere.</p>
<p>On the other hand, Venus has no internally dynamo-generated magnetic field and yet it has an induced magnetosphere caused by the interaction of the planet with the solar wind.  Apparently this weak induced magnetosphere has been sufficient to prevent the loss of Venus&#8217; atmosphere into space during the last 4.5 billion years.  So an internal magnetic field is not absolutely necessary to prevent atmospheric loss.</p>
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		<title>By: Lawny</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/comment-page-1/#comment-139914</link>
		<dc:creator>Lawny</dc:creator>
		<pubDate>Wed, 10 Dec 2008 17:52:56 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/#comment-139914</guid>
		<description>Most interesting is a measurement of CO in the IR in the atmosphere of the planet.  What is the millimeter spectrum of CO in this hot dense planetary atmosphere?  Surely the planet is &#039;darker&#039; over an appropriate bandwidth (larger the deeper the molecule is in the atmosphere I would guess) and the eclipse &#039;deeper&#039;.  I think it would be a plausible target for ALMA at 345 GHz (J=3-2 line of CO).</description>
		<content:encoded><![CDATA[<p>Most interesting is a measurement of CO in the IR in the atmosphere of the planet.  What is the millimeter spectrum of CO in this hot dense planetary atmosphere?  Surely the planet is &#8216;darker&#8217; over an appropriate bandwidth (larger the deeper the molecule is in the atmosphere I would guess) and the eclipse &#8216;deeper&#8217;.  I think it would be a plausible target for ALMA at 345 GHz (J=3-2 line of CO).</p>
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		<title>By: Sir Eccles</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/comment-page-1/#comment-139884</link>
		<dc:creator>Sir Eccles</dc:creator>
		<pubDate>Wed, 10 Dec 2008 14:33:09 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/#comment-139884</guid>
		<description>All this talk of &quot;organic chemistry&quot; reminds me of when I was at university talking to one of the less bright lab technicians.

She asked me why the new organic chemistry building they were constructing next door needed so many fume cupboards if it was all organic...

I can&#039;t recall my response.</description>
		<content:encoded><![CDATA[<p>All this talk of &#8220;organic chemistry&#8221; reminds me of when I was at university talking to one of the less bright lab technicians.</p>
<p>She asked me why the new organic chemistry building they were constructing next door needed so many fume cupboards if it was all organic&#8230;</p>
<p>I can&#8217;t recall my response.</p>
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		<title>By: Torbjörn Larsson, OM</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/comment-page-1/#comment-139868</link>
		<dc:creator>Torbjörn Larsson, OM</dc:creator>
		<pubDate>Wed, 10 Dec 2008 09:56:02 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/#comment-139868</guid>
		<description>No, I didn&#039;t mean to make a tag bug (or rather, dismiss one too many spell check warning so as to not close the blockquote), but I think it nicely made my point. Preview, posthaste, please!</description>
		<content:encoded><![CDATA[<p>No, I didn&#8217;t mean to make a tag bug (or rather, dismiss one too many spell check warning so as to not close the blockquote), but I think it nicely made my point. Preview, posthaste, please!</p>
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		<title>By: Torbjörn Larsson, OM</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/comment-page-1/#comment-139867</link>
		<dc:creator>Torbjörn Larsson, OM</dc:creator>
		<pubDate>Wed, 10 Dec 2008 09:46:37 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/#comment-139867</guid>
		<description>I googled exoplanet oxygen and found that they observed it (and carbon) blowing of a planet atmosphere already 2004. Probably not molecular oxygen, but still: close to have proof of concept of detecting 3-5 potential biosphere indicators. (Water, oxygen/ozone, carbon dioxide/carbon monoxide ratios, methane, &quot;red edge&quot; of multiphoton organic photosynthesis - what else?)

&lt;blockquote&gt;
just to note, this was first reported back on November 23
&lt;/blockquote&gt;

Thanks, I was just about to comment on that.

The web really needs a better way to recognize when corpses of old press releases are paraded from their graves in a 2nd round. [And let&#039;s face it, media isn&#039;t known for actually looking at, even less remembering, what they print in order to get the ad money flowing in.] As it is, it feels like looking at the optical echoecho ofof thethe webweb.

Not that it can&#039;t trigger a good post, of course!

&lt;blockquote&gt;
we will have a preview/edit facility here on B.A. Blog sometime early next year in January/February
&lt;/blockqote&gt;

Ah, a late yule gift then. 

Any chances we may have a sneak preview..., um, &quot;google beta release&quot;, of the preview facility? It doesn&#039;t have to be perfect (edit functionality and/or spel chekkers, for example) to be useful in comparison with what we have now.</description>
		<content:encoded><![CDATA[<p>I googled exoplanet oxygen and found that they observed it (and carbon) blowing of a planet atmosphere already 2004. Probably not molecular oxygen, but still: close to have proof of concept of detecting 3-5 potential biosphere indicators. (Water, oxygen/ozone, carbon dioxide/carbon monoxide ratios, methane, &#8220;red edge&#8221; of multiphoton organic photosynthesis &#8211; what else?)</p>
<blockquote><p>
just to note, this was first reported back on November 23
</p></blockquote>
<p>Thanks, I was just about to comment on that.</p>
<p>The web really needs a better way to recognize when corpses of old press releases are paraded from their graves in a 2nd round. [And let's face it, media isn't known for actually looking at, even less remembering, what they print in order to get the ad money flowing in.] As it is, it feels like looking at the optical echoecho ofof thethe webweb.</p>
<p>Not that it can&#8217;t trigger a good post, of course!</p>
<blockquote><p>
we will have a preview/edit facility here on B.A. Blog sometime early next year in January/February</p>
<p>Ah, a late yule gift then. </p>
<p>Any chances we may have a sneak preview&#8230;, um, &#8220;google beta release&#8221;, of the preview facility? It doesn&#8217;t have to be perfect (edit functionality and/or spel chekkers, for example) to be useful in comparison with what we have now.</p></blockquote>
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		<title>By: IVAN3MAN</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/comment-page-1/#comment-139863</link>
		<dc:creator>IVAN3MAN</dc:creator>
		<pubDate>Wed, 10 Dec 2008 08:29:22 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/#comment-139863</guid>
		<description>StevoR: &quot;Thanks... for the info, link &amp; magnificent location map posted here. Appreciated!&quot;

You&#039;re welcome! If one had a preview/edit facility here, I would have &#039;tweaked&#039; the lettering underneath that image because it did not space out as well as I had expected. 

Also, I see that you have a bad problem with &quot;typos&quot;. I&#039;m sure that you will be relieved to hear that according to the Discover Web Editor, Amos Kenigsberg, we will have a preview/edit facility here on B.A. Blog sometime early next year in January/February. :-)</description>
		<content:encoded><![CDATA[<p>StevoR: &#8220;Thanks&#8230; for the info, link &#038; magnificent location map posted here. Appreciated!&#8221;</p>
<p>You&#8217;re welcome! If one had a preview/edit facility here, I would have &#8216;tweaked&#8217; the lettering underneath that image because it did not space out as well as I had expected. </p>
<p>Also, I see that you have a bad problem with &#8220;typos&#8221;. I&#8217;m sure that you will be relieved to hear that according to the Discover Web Editor, Amos Kenigsberg, we will have a preview/edit facility here on B.A. Blog sometime early next year in January/February. <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: Joker</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/comment-page-1/#comment-139860</link>
		<dc:creator>Joker</dc:creator>
		<pubDate>Wed, 10 Dec 2008 07:19:07 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/#comment-139860</guid>
		<description>&quot;having &lt;b&gt;decent&lt;/b&gt; proper names makes exoplanets more than just a dull, hard to remember, harder to pronounce catalogue number for people!” 

So StevoR, you saying catalogue numbers are &lt;b&gt; *  indecent * &lt;/b&gt; then?;-)

Cool, got meself some new swear words :

Hey, HD 189733b you ya piece of OGLE-o5-390-el B*!&quot; 

Nah, not quite the same is it? ;-)  

Neat news, nowhere near as awesome as imaging Fomalhaut b and that other stars three exoplanets &lt;i&gt; (wha&#039; waz its&#039; number again? Hmm... StevoR may have a point!) &lt;/i&gt; Sorta expect Hot Jupiter gas gainst to have well .. gases even H20 &amp; Co2 .. but still cool to find out &amp; good work. :-)</description>
		<content:encoded><![CDATA[<p>&#8220;having <b>decent</b> proper names makes exoplanets more than just a dull, hard to remember, harder to pronounce catalogue number for people!” </p>
<p>So StevoR, you saying catalogue numbers are <b> *  indecent * </b> then?;-)</p>
<p>Cool, got meself some new swear words :</p>
<p>Hey, HD 189733b you ya piece of OGLE-o5-390-el B*!&#8221; </p>
<p>Nah, not quite the same is it? <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_wink.gif' alt=';-)' class='wp-smiley' />   </p>
<p>Neat news, nowhere near as awesome as imaging Fomalhaut b and that other stars three exoplanets <i> (wha&#8217; waz its&#8217; number again? Hmm&#8230; StevoR may have a point!) </i> Sorta expect Hot Jupiter gas gainst to have well .. gases even H20 &#038; Co2 .. but still cool to find out &#038; good work. <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: StevoR-Correcting</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/comment-page-1/#comment-139859</link>
		<dc:creator>StevoR-Correcting</dc:creator>
		<pubDate>Wed, 10 Dec 2008 07:11:11 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/#comment-139859</guid>
		<description>Than! 
&lt;i&gt;
&quot;.. having decent proper names makes exoplanets more &lt;b&gt; than&lt;/b&gt; just a dull, hard to remember, harder to pronounce catalogue number for people!&quot; &lt;/i&gt;

Sigh. Have I finally got it right?  

Just think, I could do all this in * one * post &amp; not * three * if I could just @$#!#@@# EDIT here! Sigh. :-( 

PS. Yeah, there are other typos, hope y&#039;all get the gist anyhow. Yeah, I know I should check what I type more carefully and prob&#039;ly not type so quickly. Mea culpa. I&#039;m a fallible human being. As they say :

To err is human, to really mess things up requires a computer! ;-)</description>
		<content:encoded><![CDATA[<p>Than!<br />
<i><br />
&#8220;.. having decent proper names makes exoplanets more <b> than</b> just a dull, hard to remember, harder to pronounce catalogue number for people!&#8221; </i></p>
<p>Sigh. Have I finally got it right?  </p>
<p>Just think, I could do all this in * one * post &#038; not * three * if I could just @$#!#@@# EDIT here! Sigh. <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_sad.gif' alt=':-(' class='wp-smiley' />  </p>
<p>PS. Yeah, there are other typos, hope y&#8217;all get the gist anyhow. Yeah, I know I should check what I type more carefully and prob&#8217;ly not type so quickly. Mea culpa. I&#8217;m a fallible human being. As they say :</p>
<p>To err is human, to really mess things up requires a computer! <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_wink.gif' alt=';-)' class='wp-smiley' /> </p>
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		<title>By: StevoR-Correcting</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/comment-page-1/#comment-139857</link>
		<dc:creator>StevoR-Correcting</dc:creator>
		<pubDate>Wed, 10 Dec 2008 06:57:29 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/#comment-139857</guid>
		<description>Aaarrrrgghhh!! Flippin&#039; typos! Yegods, I hate how we can&#039;t edit or even preview our posts here .. Its such a pain. Sigh. :-( 

Anyway what I said was :  

&lt;i&gt; &quot;Now those sort of names beat catalogue designations anyday if y’ask me or, I’d think, most others and instantly give some idea of the exoplanet’s nature or signifcinceor location that inspires,sometimes amuses and makes it less just a number to people - which in turn helps inpromotingand making welcoming astronomy to society. &quot; &lt;/i&gt; 

But what I&#039;d meant to have written (&amp; thought I *had* written until I saw it on screen (Sigh) was : 

Now those sort of names (Bellopheron, Hoth, Tattooine, Balsawood Planet, Polydeuces, etc ..)  beat catalogue designations (like HD 189733b, TrEs-4, OGLE-05-390-Lb even 51Peg b) anyday if y’ask me - or, I’d think, most other reasonable people. Such evocative and instinctively pronouncable names instantly give folks some idea of an exoplanet’s nature, its significance or its location that inspires, sometimes amuses and always &lt;b&gt;makes it more just a dull, hard to remember, harder to pronounce  number to people! &lt;/b&gt; 

Which in turn helps in promoting and making astronomy more welcoming and easier to imagine for broader society. Having such amazing marvellous exoplanets reamining so poorly non-named is doing astronomy in general a dis-service. In My Humble Opinion Naturally (natch)! ;-) 

&lt;i&gt;(Now if only I could correct my first post properly. Sigh. Please Dr Phil Plait, please!) &lt;/i&gt;</description>
		<content:encoded><![CDATA[<p>Aaarrrrgghhh!! Flippin&#8217; typos! Yegods, I hate how we can&#8217;t edit or even preview our posts here .. Its such a pain. Sigh. <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_sad.gif' alt=':-(' class='wp-smiley' />  </p>
<p>Anyway what I said was :  </p>
<p><i> &#8220;Now those sort of names beat catalogue designations anyday if y’ask me or, I’d think, most others and instantly give some idea of the exoplanet’s nature or signifcinceor location that inspires,sometimes amuses and makes it less just a number to people &#8211; which in turn helps inpromotingand making welcoming astronomy to society. &#8221; </i> </p>
<p>But what I&#8217;d meant to have written (&#038; thought I *had* written until I saw it on screen (Sigh) was : </p>
<p>Now those sort of names (Bellopheron, Hoth, Tattooine, Balsawood Planet, Polydeuces, etc ..)  beat catalogue designations (like HD 189733b, TrEs-4, OGLE-05-390-Lb even 51Peg b) anyday if y’ask me &#8211; or, I’d think, most other reasonable people. Such evocative and instinctively pronouncable names instantly give folks some idea of an exoplanet’s nature, its significance or its location that inspires, sometimes amuses and always <b>makes it more just a dull, hard to remember, harder to pronounce  number to people! </b> </p>
<p>Which in turn helps in promoting and making astronomy more welcoming and easier to imagine for broader society. Having such amazing marvellous exoplanets reamining so poorly non-named is doing astronomy in general a dis-service. In My Humble Opinion Naturally (natch)! <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_wink.gif' alt=';-)' class='wp-smiley' />  </p>
<p><i>(Now if only I could correct my first post properly. Sigh. Please Dr Phil Plait, please!) </i></p>
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		<title>By: StevoR-Confirming</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/comment-page-1/#comment-139855</link>
		<dc:creator>StevoR-Confirming</dc:creator>
		<pubDate>Wed, 10 Dec 2008 06:38:15 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/#comment-139855</guid>
		<description>Yes that links working. I also forgot Gliese 581 b wass named by the author of that &quot;Wor;lds of Other Suns&quot; site too - Hades I! It uses its own system and is a bit on the &quot;glass two-thirds full&quot; side of imaginative scientific speculation but I do reckon its well worth a look - or, natch, I wouldn&#039;t have posted it! ;-) :-D</description>
		<content:encoded><![CDATA[<p>Yes that links working. I also forgot Gliese 581 b wass named by the author of that &#8220;Wor;lds of Other Suns&#8221; site too &#8211; Hades I! It uses its own system and is a bit on the &#8220;glass two-thirds full&#8221; side of imaginative scientific speculation but I do reckon its well worth a look &#8211; or, natch, I wouldn&#8217;t have posted it! <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_wink.gif' alt=';-)' class='wp-smiley' />  <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_biggrin.gif' alt=':-D' class='wp-smiley' /> </p>
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		<title>By: Brian</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/comment-page-1/#comment-139854</link>
		<dc:creator>Brian</dc:creator>
		<pubDate>Wed, 10 Dec 2008 06:32:32 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/#comment-139854</guid>
		<description>This. News. Is. So. Cool.

I can&#039;t begin to express how excited I am to see this finally happen. It&#039;s a real milestone.

Here&#039;s to the spectroscopic analysis of many more planetary atmospheres to come!</description>
		<content:encoded><![CDATA[<p>This. News. Is. So. Cool.</p>
<p>I can&#8217;t begin to express how excited I am to see this finally happen. It&#8217;s a real milestone.</p>
<p>Here&#8217;s to the spectroscopic analysis of many more planetary atmospheres to come!</p>
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		<title>By: StevoR</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/comment-page-1/#comment-139853</link>
		<dc:creator>StevoR</dc:creator>
		<pubDate>Wed, 10 Dec 2008 06:27:34 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2008/12/09/hubble-spies-carbon-dioxide-600-trillion-kilometers-away/#comment-139853</guid>
		<description>Thanks &lt;b&gt;Tom Marking &amp; IVAN3MAN &lt;/b&gt; for the info, link &amp; magnificent location map posted here. Appreciated! :-D

You can go to one of my sources - &quot;Worlds of other Suns&quot;  - via clicking my name above - for the named worlds listed earlier. Its an exoplanets website &lt;i&gt;(not mine but a fave of mine)&lt;/i&gt; with examples of  ... er &lt;i&gt;very optimistically &lt;/i&gt; but well written info &amp; superbly illustrated exoplanets as named (Hoth Tatooine etc ..) Hopefully interesting for people!  Hopefully the link&#039;ll work!</description>
		<content:encoded><![CDATA[<p>Thanks <b>Tom Marking &#038; IVAN3MAN </b> for the info, link &#038; magnificent location map posted here. Appreciated! <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_biggrin.gif' alt=':-D' class='wp-smiley' /> </p>
<p>You can go to one of my sources &#8211; &#8220;Worlds of other Suns&#8221;  &#8211; via clicking my name above &#8211; for the named worlds listed earlier. Its an exoplanets website <i>(not mine but a fave of mine)</i> with examples of  &#8230; er <i>very optimistically </i> but well written info &#038; superbly illustrated exoplanets as named (Hoth Tatooine etc ..) Hopefully interesting for people!  Hopefully the link&#8217;ll work!</p>
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