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	<title>Comments on: Another Hubble stunner</title>
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	<link>http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/</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 22:23:20 +0000</lastBuildDate>
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		<title>By: Angel Elf</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/comment-page-1/#comment-339924</link>
		<dc:creator>Angel Elf</dc:creator>
		<pubDate>Wed, 01 Dec 2010 21:30:35 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/#comment-339924</guid>
		<description>What is the name of that beautiful spiral in the lower right hand corner of the image above?</description>
		<content:encoded><![CDATA[<p>What is the name of that beautiful spiral in the lower right hand corner of the image above?</p>
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		<title>By: software</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/comment-page-1/#comment-95713</link>
		<dc:creator>software</dc:creator>
		<pubDate>Thu, 03 Jul 2008 04:14:36 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/#comment-95713</guid>
		<description>Are you sure that your PC not by and other *hit?Are you protected from PC-spy?TAKE A LOOK HERE AND SCAN YOUR PC HERE AT OUR SITE! 
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online</description>
		<content:encoded><![CDATA[<p>Are you sure that your PC not by and other *hit?Are you protected from PC-spy?TAKE A LOOK HERE AND SCAN YOUR PC HERE AT OUR SITE!<br />
>>> [url=http://www.telecentre.org/index.cfm?event=user.detail&#038;id=14601]virus protect[/url] </p>
<p>online</p>
]]></content:encoded>
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		<title>By: ceticismoaberto.com &#187; Blog Archive &#187; Imagem do Universo via Hubble</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/comment-page-1/#comment-29375</link>
		<dc:creator>ceticismoaberto.com &#187; Blog Archive &#187; Imagem do Universo via Hubble</dc:creator>
		<pubDate>Mon, 12 Feb 2007 11:03:53 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/#comment-29375</guid>
		<description>[...] Esta imagem do telesc&#243;pio espacial Hubble da NASA mostra uma cole&#231;&#227;o diversa de gal&#225;xias no agrupamento Abell S0740 a mais de 450 milh&#245;es de anos-luz de dist&#226;ncia na direa&#231;&#227;o da constela&#231;&#227;o de Centauro. A gigante el&#237;ptica ESO 325-G004 figura no centro do agrupamento. A gal&#225;xia &#233; t&#227;o maci&#231;a quanto 100 bilh&#245;es de vezes nosso Sol. O Hubble mostra milhares de agrupamentos estelares globulares orbitando a ESO 325-G004. Agrupamentos globulares s&#227;o grupos compactos de centenas de milhares de estrelas que est&#227;o unidas gravitacionalmente. &#224; dist&#226;ncia da gal&#225;xia, eles parecem pequenos pontos de luz contidos no halo difuso. Outras gal&#225;xias el&#237;pticas t&#234;nues aparecem na imagem. Algumas mostram sinais de uma estrutura em disco ou anel que lhes confere a forma de uma gravata borboleta. V&#225;rias gal&#225;xias espirais tamb&#233;m est&#227;o presentes. A luz estelar destas gal&#225;xias &#233; primariamente contida em um disco e segue os bra&#231;os espirais. Esta imagem foi criada combinando observa&#231;&#245;es cient&#237;ficas do Hubble tomadas em janeiro de 2005 com as observa&#231;&#245;es Hubble Heritage tomadas um ano depois para formar um comspoto de tr&#234;s cores. Os filtors que isolam a luz azul, vermelha e infravermelha foram usadas com a ACS a bordo do Hubble - [release da NASA]. Mais explica&#231;&#245;es, em ingl&#234;s, no Bad Astronomy blog. Infelizmente, a Advanced Camera for Surveys (ACS) usada para capturar a imagem acima e um dos principais instrumentos do Hubble acaba de se tornar inoperante. O telesc&#243;pio espacial Hubble continua firme, contudo, e mal podemos esperar as vis&#245;es numinosas do Universo que seu sucessor dever&#225; revelar. [...]</description>
		<content:encoded><![CDATA[<p>[...] Esta imagem do telesc&oacute;pio espacial Hubble da NASA mostra uma cole&ccedil;&atilde;o diversa de gal&aacute;xias no agrupamento Abell S0740 a mais de 450 milh&otilde;es de anos-luz de dist&acirc;ncia na direa&ccedil;&atilde;o da constela&ccedil;&atilde;o de Centauro. A gigante el&iacute;ptica ESO 325-G004 figura no centro do agrupamento. A gal&aacute;xia &eacute; t&atilde;o maci&ccedil;a quanto 100 bilh&otilde;es de vezes nosso Sol. O Hubble mostra milhares de agrupamentos estelares globulares orbitando a ESO 325-G004. Agrupamentos globulares s&atilde;o grupos compactos de centenas de milhares de estrelas que est&atilde;o unidas gravitacionalmente. &agrave; dist&acirc;ncia da gal&aacute;xia, eles parecem pequenos pontos de luz contidos no halo difuso. Outras gal&aacute;xias el&iacute;pticas t&ecirc;nues aparecem na imagem. Algumas mostram sinais de uma estrutura em disco ou anel que lhes confere a forma de uma gravata borboleta. V&aacute;rias gal&aacute;xias espirais tamb&eacute;m est&atilde;o presentes. A luz estelar destas gal&aacute;xias &eacute; primariamente contida em um disco e segue os bra&ccedil;os espirais. Esta imagem foi criada combinando observa&ccedil;&otilde;es cient&iacute;ficas do Hubble tomadas em janeiro de 2005 com as observa&ccedil;&otilde;es Hubble Heritage tomadas um ano depois para formar um comspoto de tr&ecirc;s cores. Os filtors que isolam a luz azul, vermelha e infravermelha foram usadas com a ACS a bordo do Hubble &#8211; [release da NASA]. Mais explica&ccedil;&otilde;es, em ingl&ecirc;s, no Bad Astronomy blog. Infelizmente, a Advanced Camera for Surveys (ACS) usada para capturar a imagem acima e um dos principais instrumentos do Hubble acaba de se tornar inoperante. O telesc&oacute;pio espacial Hubble continua firme, contudo, e mal podemos esperar as vis&otilde;es numinosas do Universo que seu sucessor dever&aacute; revelar. [...]</p>
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		<title>By: sam slam</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/comment-page-1/#comment-29374</link>
		<dc:creator>sam slam</dc:creator>
		<pubDate>Sun, 11 Feb 2007 22:50:23 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/#comment-29374</guid>
		<description>yay how fun t read</description>
		<content:encoded><![CDATA[<p>yay how fun t read</p>
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		<title>By: Buzz Parsec</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/comment-page-1/#comment-29373</link>
		<dc:creator>Buzz Parsec</dc:creator>
		<pubDate>Sat, 10 Feb 2007 06:13:04 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/#comment-29373</guid>
		<description>Mark -  the web strikes again :-)</description>
		<content:encoded><![CDATA[<p>Mark &#8211;  the web strikes again <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: trinitree88</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/comment-page-1/#comment-29372</link>
		<dc:creator>trinitree88</dc:creator>
		<pubDate>Thu, 08 Feb 2007 20:03:56 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/#comment-29372</guid>
		<description>Is the Abell Cluster one of the clusters that leaves a shadow on the CMB due to the Sunyaev-Zeldovich Effect, or one that doesn&#039;t because the gas and dust in the cluster emits at 2.72 K. We do know that it is closer to us than the surface of last scattering, true? pete</description>
		<content:encoded><![CDATA[<p>Is the Abell Cluster one of the clusters that leaves a shadow on the CMB due to the Sunyaev-Zeldovich Effect, or one that doesn&#8217;t because the gas and dust in the cluster emits at 2.72 K. We do know that it is closer to us than the surface of last scattering, true? pete</p>
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		<title>By: Mark</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/comment-page-1/#comment-29371</link>
		<dc:creator>Mark</dc:creator>
		<pubDate>Thu, 08 Feb 2007 18:28:11 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/#comment-29371</guid>
		<description>Dave and everyone,  Thanks for the answers!</description>
		<content:encoded><![CDATA[<p>Dave and everyone,  Thanks for the answers!</p>
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		<title>By: SF Reader</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/comment-page-1/#comment-29370</link>
		<dc:creator>SF Reader</dc:creator>
		<pubDate>Thu, 08 Feb 2007 16:46:14 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/#comment-29370</guid>
		<description>And the only foreground objects (our galaxy?  our cluster?) are the ones with the diffraction spikes (from the legs supporting  the secondary mirror?).

Just getting the scale straight in my head, so I can explain it all to my 9-year-old!</description>
		<content:encoded><![CDATA[<p>And the only foreground objects (our galaxy?  our cluster?) are the ones with the diffraction spikes (from the legs supporting  the secondary mirror?).</p>
<p>Just getting the scale straight in my head, so I can explain it all to my 9-year-old!</p>
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		<title>By: ioresult</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/comment-page-1/#comment-29369</link>
		<dc:creator>ioresult</dc:creator>
		<pubDate>Thu, 08 Feb 2007 16:05:36 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/#comment-29369</guid>
		<description>Mark: dark matter is only matter that hasn&#039;t been observed directly yet. Neptune was one of the first such examples. It was discovered by its gravitational influence on Uranus in 1846. So before being observed, during a short time when it was known that Neptune existed, it was effectively &quot;dark matter&quot;.

Right now, if I&#039;m not mistaken, about 5% of the universe&#039;s total energy has been observed by its influence on photons. 25% more can be accounted for only by its gravitational influence, so that&#039;s the actual current amount of &quot;dark matter&quot;. 70% is dark energy (the mysterious thing that&#039;s responsible for the expansion&#039;s acceleration).</description>
		<content:encoded><![CDATA[<p>Mark: dark matter is only matter that hasn&#8217;t been observed directly yet. Neptune was one of the first such examples. It was discovered by its gravitational influence on Uranus in 1846. So before being observed, during a short time when it was known that Neptune existed, it was effectively &#8220;dark matter&#8221;.</p>
<p>Right now, if I&#8217;m not mistaken, about 5% of the universe&#8217;s total energy has been observed by its influence on photons. 25% more can be accounted for only by its gravitational influence, so that&#8217;s the actual current amount of &#8220;dark matter&#8221;. 70% is dark energy (the mysterious thing that&#8217;s responsible for the expansion&#8217;s acceleration).</p>
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		<title>By: Dave Kary</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/comment-page-1/#comment-29368</link>
		<dc:creator>Dave Kary</dc:creator>
		<pubDate>Thu, 08 Feb 2007 15:56:16 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/#comment-29368</guid>
		<description>There certainly were indications of a problem all of the way back to the 30&#039;s, but it didn&#039;t really move to the forefront until the 70&#039;s (if I remember right) when Vera Rubin did some detailed studies on the Milky Way and found that the rotation curve is flat, indicating that we weren&#039;t seeing most of the mass of the galaxy (since most of the light comes from the bulge). That&#039;s when &quot;dark matter&quot; became one of the big  problems in astronomy.

I just checked with my wife, (who is a historian of astronomy), and she confirmed that Vera Rubin does have a daughter named Judy, so I&#039;m guessing that&#039;s who Buzz went to school with.</description>
		<content:encoded><![CDATA[<p>There certainly were indications of a problem all of the way back to the 30&#8242;s, but it didn&#8217;t really move to the forefront until the 70&#8242;s (if I remember right) when Vera Rubin did some detailed studies on the Milky Way and found that the rotation curve is flat, indicating that we weren&#8217;t seeing most of the mass of the galaxy (since most of the light comes from the bulge). That&#8217;s when &#8220;dark matter&#8221; became one of the big  problems in astronomy.</p>
<p>I just checked with my wife, (who is a historian of astronomy), and she confirmed that Vera Rubin does have a daughter named Judy, so I&#8217;m guessing that&#8217;s who Buzz went to school with.</p>
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		<title>By: Mark</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/comment-page-1/#comment-29367</link>
		<dc:creator>Mark</dc:creator>
		<pubDate>Thu, 08 Feb 2007 12:51:59 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/#comment-29367</guid>
		<description>Hey Buzz,

Whoa, your class mate&#039;s mom discovered dark matter?  That&#039;s another thing that&#039;s been puzzling me lately... It&#039;s my understanding is that astronomers first realized back in the 30&#039;s that galaxies didn&#039;t have enough mass to behave the way they were behaving.  My impression is that this problem remained in the forefront right up to today.  So my question is, what event constituted the &quot;discovery&quot; of dark matter?</description>
		<content:encoded><![CDATA[<p>Hey Buzz,</p>
<p>Whoa, your class mate&#8217;s mom discovered dark matter?  That&#8217;s another thing that&#8217;s been puzzling me lately&#8230; It&#8217;s my understanding is that astronomers first realized back in the 30&#8242;s that galaxies didn&#8217;t have enough mass to behave the way they were behaving.  My impression is that this problem remained in the forefront right up to today.  So my question is, what event constituted the &#8220;discovery&#8221; of dark matter?</p>
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		<title>By: Buzz Parsec</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/comment-page-1/#comment-29366</link>
		<dc:creator>Buzz Parsec</dc:creator>
		<pubDate>Thu, 08 Feb 2007 07:37:55 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/#comment-29366</guid>
		<description>The talk about dark matter and the missing mass problem reminds me just how incredibly *cool* it was that my astronomy classmate Judy&#039;s mom had just discovered that 90% of the universe had gone missing!</description>
		<content:encoded><![CDATA[<p>The talk about dark matter and the missing mass problem reminds me just how incredibly *cool* it was that my astronomy classmate Judy&#8217;s mom had just discovered that 90% of the universe had gone missing!</p>
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		<title>By: Teapot</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/comment-page-1/#comment-29365</link>
		<dc:creator>Teapot</dc:creator>
		<pubDate>Thu, 08 Feb 2007 06:36:44 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/#comment-29365</guid>
		<description>Hmmm, not that it really makes a difference, but why is APOD&#039;s posting of this photo rotated 90 degrees CW from the BA&#039;s?
http://apod.nasa.gov/apod/ap070208.html</description>
		<content:encoded><![CDATA[<p>Hmmm, not that it really makes a difference, but why is APOD&#8217;s posting of this photo rotated 90 degrees CW from the BA&#8217;s?<br />
<a href="http://apod.nasa.gov/apod/ap070208.html" rel="nofollow">http://apod.nasa.gov/apod/ap070208.html</a></p>
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		<title>By: Mark</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/comment-page-1/#comment-29364</link>
		<dc:creator>Mark</dc:creator>
		<pubDate>Thu, 08 Feb 2007 03:09:21 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/#comment-29364</guid>
		<description>ioresult,  Thanks for the answer!

Is this the primary evidence for the existance of dark matter?</description>
		<content:encoded><![CDATA[<p>ioresult,  Thanks for the answer!</p>
<p>Is this the primary evidence for the existance of dark matter?</p>
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		<title>By: &#187; Links for 08-02-2007 &#187; Velcro City Tourist Board &#187; Blog Archive</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/comment-page-1/#comment-29363</link>
		<dc:creator>&#187; Links for 08-02-2007 &#187; Velcro City Tourist Board &#187; Blog Archive</dc:creator>
		<pubDate>Thu, 08 Feb 2007 02:27:25 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/#comment-29363</guid>
		<description>[...] 2 - Another Hubble stunner &#8220;Astronomers at Space Telescope Science Institute just released a new image, and itâ€™s a beauty.&#8221; New desktop wallpaper here at Velcro City! (tags: S0740 Abell cluster galaxy picture image telescope Hubble space) [...]</description>
		<content:encoded><![CDATA[<p>[...] 2 &#8211; Another Hubble stunner &#8220;Astronomers at Space Telescope Science Institute just released a new image, and itâ€™s a beauty.&#8221; New desktop wallpaper here at Velcro City! (tags: S0740 Abell cluster galaxy picture image telescope Hubble space) [...]</p>
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		<title>By: Dave Kary</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/comment-page-1/#comment-29362</link>
		<dc:creator>Dave Kary</dc:creator>
		<pubDate>Thu, 08 Feb 2007 01:11:59 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/#comment-29362</guid>
		<description>The whole question of &quot;habitability&quot; is a still has way too many variables to get even the right order of magnitude on estimating the likelihood. We certainly know now that among metal-rich stars (which dominate disks of spiral galaxies) like the ones around us, planets are at least 10%, and quite probably more than that.

But beyond that, we still don&#039;t know whether terrestrial planets are common, or how many are on sufficiently circular orbits to give a fairly stable climate, or what the real habitablity range is for those kinds of planets (since atmospheric greenhouse feedback relations can stabilize a temperature over a wide range of distances from the star).

We also don&#039;t know if you need a terrestrial planet? How about a jovian moon? How about the atmosphere of a jovian planet itself? Both of these are at least worth considering as places for life to develop.

Lastly, we don&#039;t know even know if you really need liquid water conditions for life. There are some lovely liquid methane lakes on Titan (see today&#039;s Astronomy Picture of the Day) that look pretty inviting, provided you don&#039;t mind a temperature of 93K.

I think that we will have a much better idea of the likelihood of life elsewhere once we have more thoroughly explored the solar system. If there really isn&#039;t any life in the oceans of Europa or the lakes of Titan, and there really aren&#039;t any fossils in the sedimentary beds on Mars, then maybe we can say that life is rare. On the other hand, if life developed just one more place in our solar system, then I&#039;d bet it is common throughout the universe. After all, if you get it twice in one little solar system, it be easy to get the right conditions.</description>
		<content:encoded><![CDATA[<p>The whole question of &#8220;habitability&#8221; is a still has way too many variables to get even the right order of magnitude on estimating the likelihood. We certainly know now that among metal-rich stars (which dominate disks of spiral galaxies) like the ones around us, planets are at least 10%, and quite probably more than that.</p>
<p>But beyond that, we still don&#8217;t know whether terrestrial planets are common, or how many are on sufficiently circular orbits to give a fairly stable climate, or what the real habitablity range is for those kinds of planets (since atmospheric greenhouse feedback relations can stabilize a temperature over a wide range of distances from the star).</p>
<p>We also don&#8217;t know if you need a terrestrial planet? How about a jovian moon? How about the atmosphere of a jovian planet itself? Both of these are at least worth considering as places for life to develop.</p>
<p>Lastly, we don&#8217;t know even know if you really need liquid water conditions for life. There are some lovely liquid methane lakes on Titan (see today&#8217;s Astronomy Picture of the Day) that look pretty inviting, provided you don&#8217;t mind a temperature of 93K.</p>
<p>I think that we will have a much better idea of the likelihood of life elsewhere once we have more thoroughly explored the solar system. If there really isn&#8217;t any life in the oceans of Europa or the lakes of Titan, and there really aren&#8217;t any fossils in the sedimentary beds on Mars, then maybe we can say that life is rare. On the other hand, if life developed just one more place in our solar system, then I&#8217;d bet it is common throughout the universe. After all, if you get it twice in one little solar system, it be easy to get the right conditions.</p>
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		<title>By: biosparite</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/comment-page-1/#comment-29361</link>
		<dc:creator>biosparite</dc:creator>
		<pubDate>Thu, 08 Feb 2007 00:21:30 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/#comment-29361</guid>
		<description>Ausrick said, &quot;From a statisticians point of view, what Iâ€™ve been reading seems a little more lonelyâ€“that chances of other habitable planets occuring seem to diminish with every new discovery.  The last paper I read had quoted something like there being 202 parameters that need to fall within very specific guidlines to form a habitable planet (another paper only said 120, but I think it was written earlier). &quot;

  Ausrick, before you get too discouraged, remember JBS Haldane&#039;s comment after a lecture on the habitable zone around stars: &quot;But what if they (alien life) look like bloody stones?&quot;</description>
		<content:encoded><![CDATA[<p>Ausrick said, &#8220;From a statisticians point of view, what Iâ€™ve been reading seems a little more lonelyâ€“that chances of other habitable planets occuring seem to diminish with every new discovery.  The last paper I read had quoted something like there being 202 parameters that need to fall within very specific guidlines to form a habitable planet (another paper only said 120, but I think it was written earlier). &#8221;</p>
<p>  Ausrick, before you get too discouraged, remember JBS Haldane&#8217;s comment after a lecture on the habitable zone around stars: &#8220;But what if they (alien life) look like bloody stones?&#8221;</p>
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		<title>By: Troy</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/comment-page-1/#comment-29360</link>
		<dc:creator>Troy</dc:creator>
		<pubDate>Wed, 07 Feb 2007 23:59:36 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/#comment-29360</guid>
		<description>I&#039;m not a deep sky guy, BUT my impression was always that the Milky Way while not a huge galaxy is actually quite large.  Now if you want a small galaxy we have two satellite galaxies called the large and small Magellinic clouds (not generally visible in the Northern hemisphere) those are puny galaxies, but the Milky Way is a big boy.  M31 the galaxy in Andromeda is quite a bit bigger.  And contrary to previous posts; on the level of galaxies the universe can indeed cease its expansion and clump together.   The tendancy is red shift but blue shift is possible, and M31 and the milky way will someday collide forming a huge super galaxy.

Nice picture, it seems Hera&#039;s breast has many heirs.</description>
		<content:encoded><![CDATA[<p>I&#8217;m not a deep sky guy, BUT my impression was always that the Milky Way while not a huge galaxy is actually quite large.  Now if you want a small galaxy we have two satellite galaxies called the large and small Magellinic clouds (not generally visible in the Northern hemisphere) those are puny galaxies, but the Milky Way is a big boy.  M31 the galaxy in Andromeda is quite a bit bigger.  And contrary to previous posts; on the level of galaxies the universe can indeed cease its expansion and clump together.   The tendancy is red shift but blue shift is possible, and M31 and the milky way will someday collide forming a huge super galaxy.</p>
<p>Nice picture, it seems Hera&#8217;s breast has many heirs.</p>
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		<title>By: cope</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/comment-page-1/#comment-29359</link>
		<dc:creator>cope</dc:creator>
		<pubDate>Wed, 07 Feb 2007 23:48:15 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/#comment-29359</guid>
		<description>The galaxy in the lower right...do we know what its distance relative to the more central globular and &quot;disturbed&quot; spiral is?  It is quite a beautiful spiral.

Just curious.</description>
		<content:encoded><![CDATA[<p>The galaxy in the lower right&#8230;do we know what its distance relative to the more central globular and &#8220;disturbed&#8221; spiral is?  It is quite a beautiful spiral.</p>
<p>Just curious.</p>
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		<title>By: skeptigirl</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/comment-page-1/#comment-29358</link>
		<dc:creator>skeptigirl</dc:creator>
		<pubDate>Wed, 07 Feb 2007 20:57:52 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/#comment-29358</guid>
		<description>Kevin Conod Says:
&lt;i&gt;Skeptigirl â€” I do believe you are confusing the expansion of the Universe with local motions of galaxies in clusters.

Also youâ€™re assuming the galaxies are falling inwards, whereas in all likelyhood the galaxies in this cluster are moving too fast to remain in the cluster. Over time one would expect the cluster to fall apart.&lt;/i&gt;

ioresult Says:
&lt;i&gt;Skeptigirl: The universe is pulling away from us at the same speed and acceleration whichever direction we look. According to your idea, that would mean we should be surrounded by black hole matter further than 14 billion light years away in every direction. This canâ€™t be: the gravitational field inside a massive hollow sphere is flat, there is no pull in whatever direction. So even if there were black hole matter all around us, it wouldnâ€™t affect the universeâ€™s expantion. That puts us back at thinking about the cosmological constant, or the quintessence, or dark energy (however you may want to call this thing that ir ripping the universe appart).&lt;/i&gt;

I&#039;m aware of the dif in expansion and movement. I told you it was naive speculation. I suppose I wasn&#039;t taking into account the fact redshifts don&#039;t suggest any gravitational point of attraction. Back to contemplating.... :)</description>
		<content:encoded><![CDATA[<p>Kevin Conod Says:<br />
<i>Skeptigirl â€” I do believe you are confusing the expansion of the Universe with local motions of galaxies in clusters.</p>
<p>Also youâ€™re assuming the galaxies are falling inwards, whereas in all likelyhood the galaxies in this cluster are moving too fast to remain in the cluster. Over time one would expect the cluster to fall apart.</i></p>
<p>ioresult Says:<br />
<i>Skeptigirl: The universe is pulling away from us at the same speed and acceleration whichever direction we look. According to your idea, that would mean we should be surrounded by black hole matter further than 14 billion light years away in every direction. This canâ€™t be: the gravitational field inside a massive hollow sphere is flat, there is no pull in whatever direction. So even if there were black hole matter all around us, it wouldnâ€™t affect the universeâ€™s expantion. That puts us back at thinking about the cosmological constant, or the quintessence, or dark energy (however you may want to call this thing that ir ripping the universe appart).</i></p>
<p>I&#8217;m aware of the dif in expansion and movement. I told you it was naive speculation. I suppose I wasn&#8217;t taking into account the fact redshifts don&#8217;t suggest any gravitational point of attraction. Back to contemplating&#8230;. <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: ioresult</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/comment-page-1/#comment-29357</link>
		<dc:creator>ioresult</dc:creator>
		<pubDate>Wed, 07 Feb 2007 16:56:59 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/#comment-29357</guid>
		<description>Mmh the comment thing doesn&#039;t like web links too much. So I&#039;ll post dirfferently.

Gravity inside a hollow sphere. Do this google search: &quot;gravity inside hollow sphere&quot;. It sould yeld a couple of interesting texts.

About the universeâ€™s quintessence: type &quot;Quintessence (physics)&quot; in wikipedia.</description>
		<content:encoded><![CDATA[<p>Mmh the comment thing doesn&#8217;t like web links too much. So I&#8217;ll post dirfferently.</p>
<p>Gravity inside a hollow sphere. Do this google search: &#8220;gravity inside hollow sphere&#8221;. It sould yeld a couple of interesting texts.</p>
<p>About the universeâ€™s quintessence: type &#8220;Quintessence (physics)&#8221; in wikipedia.</p>
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		<title>By: ioresult</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/comment-page-1/#comment-29356</link>
		<dc:creator>ioresult</dc:creator>
		<pubDate>Wed, 07 Feb 2007 16:48:27 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/#comment-29356</guid>
		<description>Mark and Kevin Conod:
Galaxies in clusters are moving too fast to remain in the cluster if we only take into account the visible matter. Dark matter contributes to the gravitational pull of the whole cluster on itself so the galaxies are really just orbiting around each other.

Skeptigirl:
The universe is pulling away from us at the same speed and acceleration whichever direction we look. According to your idea, that would mean we should be surrounded by black hole matter further than 14 billion light years away in every direction. This can&#039;t be: the gravitational field inside a massive hollow sphere is flat, there is no pull in whatever direction. So even if there were black hole matter all around us, it wouldn&#039;t affect the universe&#039;s expantion. That puts us back at thinking about the cosmological constant, or the quintessence, or dark energy (however you may want to call this thing that ir ripping the universe appart).</description>
		<content:encoded><![CDATA[<p>Mark and Kevin Conod:<br />
Galaxies in clusters are moving too fast to remain in the cluster if we only take into account the visible matter. Dark matter contributes to the gravitational pull of the whole cluster on itself so the galaxies are really just orbiting around each other.</p>
<p>Skeptigirl:<br />
The universe is pulling away from us at the same speed and acceleration whichever direction we look. According to your idea, that would mean we should be surrounded by black hole matter further than 14 billion light years away in every direction. This can&#8217;t be: the gravitational field inside a massive hollow sphere is flat, there is no pull in whatever direction. So even if there were black hole matter all around us, it wouldn&#8217;t affect the universe&#8217;s expantion. That puts us back at thinking about the cosmological constant, or the quintessence, or dark energy (however you may want to call this thing that ir ripping the universe appart).</p>
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		<title>By: Mark</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/comment-page-1/#comment-29355</link>
		<dc:creator>Mark</dc:creator>
		<pubDate>Wed, 07 Feb 2007 16:20:46 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/#comment-29355</guid>
		<description>Kevin Conod:

You said, &quot;whereas in all likelyhood the galaxies in this cluster are moving too fast to remain in the cluster. Over time one would expect the cluster to fall apart.&quot;

If they are moving too fast to remain in the cluster, then that means they aren&#039;t gravitationally bound, doesn&#039;t it?  If they aren&#039;t gravitationally bound, then how did they come to be a cluster in the first place?  Maybe you or Phil could explain this.</description>
		<content:encoded><![CDATA[<p>Kevin Conod:</p>
<p>You said, &#8220;whereas in all likelyhood the galaxies in this cluster are moving too fast to remain in the cluster. Over time one would expect the cluster to fall apart.&#8221;</p>
<p>If they are moving too fast to remain in the cluster, then that means they aren&#8217;t gravitationally bound, doesn&#8217;t it?  If they aren&#8217;t gravitationally bound, then how did they come to be a cluster in the first place?  Maybe you or Phil could explain this.</p>
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		<title>By: Ausrick</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/comment-page-1/#comment-29354</link>
		<dc:creator>Ausrick</dc:creator>
		<pubDate>Wed, 07 Feb 2007 15:30:20 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/#comment-29354</guid>
		<description>You&#039;re right Hearts, The universe seems so huge it makes you wonder by the shear majesty of it what all can be out there!  I love contemplating what could exist... and dangit Einsteinian Reletivity, it seems impossible to go there and find out!

From a statisticians point of view, what I&#039;ve been reading seems a little more lonely--that chances of other habitable planets occuring seem to diminish with every new discovery. :( The last paper I read had quoted something like there being 202 parameters that need to fall within very specific guidlines to form a habitable planet (another paper only said 120, but I think it was written earlier).  It seems that everthing from the metal content of the star to where and when gas giants form and what type of orbit they have seems to have an effect on planetary formation models.  and they quoted the statistical probability of another habitable planet occurring as 1 in 10^140.  I also heard by comparison that there are supposedly only about 10^76 protons in the universe. (this last one is hearsay, I&#039;ve seen it a number of places, but not in a scientific journal and have no idea the context... I&#039;m sure the amount of protons estimated in 1970 would probably be different than the amount estimated today.)

Now I admit, these numbers seem out of whack to me, but to be honest my mind can&#039;t truly conceptualize them anyway... and with every advance or discovery they change as do the models that seem to generate them.  So I see how some one could say they would tend to believe we are alone and I can easily see why someone would say the opposite.

I&#039;m really only qualified to say the universe is awe inspiring and humbling... and I think that galaxy on the lower right side of the picture is pretty :) Oh, and to echo that it makes you think about things like this to begin with... before seeing this picture I was only concerned with where I sat my Mountain Dew. ;)  Thanks Phil!</description>
		<content:encoded><![CDATA[<p>You&#8217;re right Hearts, The universe seems so huge it makes you wonder by the shear majesty of it what all can be out there!  I love contemplating what could exist&#8230; and dangit Einsteinian Reletivity, it seems impossible to go there and find out!</p>
<p>From a statisticians point of view, what I&#8217;ve been reading seems a little more lonely&#8211;that chances of other habitable planets occuring seem to diminish with every new discovery. <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_sad.gif' alt=':(' class='wp-smiley' />  The last paper I read had quoted something like there being 202 parameters that need to fall within very specific guidlines to form a habitable planet (another paper only said 120, but I think it was written earlier).  It seems that everthing from the metal content of the star to where and when gas giants form and what type of orbit they have seems to have an effect on planetary formation models.  and they quoted the statistical probability of another habitable planet occurring as 1 in 10^140.  I also heard by comparison that there are supposedly only about 10^76 protons in the universe. (this last one is hearsay, I&#8217;ve seen it a number of places, but not in a scientific journal and have no idea the context&#8230; I&#8217;m sure the amount of protons estimated in 1970 would probably be different than the amount estimated today.)</p>
<p>Now I admit, these numbers seem out of whack to me, but to be honest my mind can&#8217;t truly conceptualize them anyway&#8230; and with every advance or discovery they change as do the models that seem to generate them.  So I see how some one could say they would tend to believe we are alone and I can easily see why someone would say the opposite.</p>
<p>I&#8217;m really only qualified to say the universe is awe inspiring and humbling&#8230; and I think that galaxy on the lower right side of the picture is pretty <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_smile.gif' alt=':)' class='wp-smiley' />  Oh, and to echo that it makes you think about things like this to begin with&#8230; before seeing this picture I was only concerned with where I sat my Mountain Dew. <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_wink.gif' alt=';)' class='wp-smiley' />   Thanks Phil!</p>
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		<title>By: (HEARTS)</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/comment-page-1/#comment-29353</link>
		<dc:creator>(HEARTS)</dc:creator>
		<pubDate>Wed, 07 Feb 2007 12:15:33 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/02/06/another-hubble-stunner/#comment-29353</guid>
		<description>Alien lifeforms to me seem like a necessity when imagining the number of solar systems out there. We may never find out, but I can only laugh at those who claim that we&#039;re alone.

Fantastic Images!</description>
		<content:encoded><![CDATA[<p>Alien lifeforms to me seem like a necessity when imagining the number of solar systems out there. We may never find out, but I can only laugh at those who claim that we&#8217;re alone.</p>
<p>Fantastic Images!</p>
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