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  <channel>
    <title>Life Sciences</title>
    <link>https://scienceblogs.com/</link>
    <description/>
    <language>en</language>
    
    <item>
  <title>Can scientists detect life without knowing what it looks like?</title>
  <link>https://scienceblogs.com/sb-admin/2025/12/12/can-scientists-detect-life-without-knowing-what-it-looks-151468</link>
  <description>
&lt;span&gt;Astronomers make use of… molecules?&lt;/span&gt;

            &lt;div class="field field--name-body field--type-text-with-summary field--label-hidden field--item"&gt;&lt;p&gt;When I think of molecules, I think of &lt;a href="http://www.yikers.com/video_conan_is_the_molecular_man.html"&gt;Conan O'Brien&lt;/a&gt; doing his skit where he plays Moleculo...&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;/center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/moleculo.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25276" title="moleculo" src="https://scienceblogs.com/files/startswithabang/files/2008/05/moleculo.jpg" alt width="413" height="331" loading="lazy"&gt;&lt;/a&gt;
&lt;p&gt;the molecular man! I don't think of astronomy, and I certainly don't think of the &lt;a href="http://map.gsfc.nasa.gov/universe/bb_tests_cmb.html"&gt;leftover radiation from the big bang&lt;/a&gt; (known as the cosmic microwave background)! But somebody over at the European Southern Observatory put these two together and made &lt;a href="http://www.eso.org/public/outreach/press-rel/pr-2008/pr-13-08.html"&gt;an incredibly tasty science sandwich&lt;/a&gt;.&lt;/p&gt;
&lt;p&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/222470571.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25277" title="222470571" src="https://scienceblogs.com/files/startswithabang/files/2008/05/222470571.jpg" alt width="221" height="98" loading="lazy"&gt;&lt;/a&gt;&lt;/p&gt;
&lt;p&gt;See, we can measure the cosmic microwave background today, because we have photons (particles of light) coming at us in all directions at all locations, with a temperature of 2.725 Kelvin. Theoretical cosmology tells us that when the Universe was younger, it was also smaller. Because the expansion of space stretches the photons in it, causing them to lose energy, it means that photons were hotter when the Universe was younger.&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;/center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/universe_expansion-sml-2.gif"&gt;&lt;img class="aligncenter size-full wp-image-25278" title="universe_expansion-sml-2" src="https://scienceblogs.com/files/startswithabang/files/2008/05/universe_expansion-sml-2.gif" alt width="336" height="336" loading="lazy"&gt;&lt;/a&gt;
&lt;p&gt;But we've never been able to measure that, of course. After all, how can you measure the temperature of something in a place where you aren't? (Hint: read the title of this post.) Use molecules as thermometers! Using a carbon monoxide molecule (CO to you chemists) in a distant galaxy, they were able to measure the temperature of the microwave background when the Universe was only about 3 billion years old! The temperature they measured was 9.15 +/- 0.70 Kelvins; and this compares pretty well with the predicted temperature of 9.315 Kelvin. Not bad! Here's an incomprehensible graph for you to look at while you take it all in:&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/phot-13b-08-preview.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25279" title="PP-53-07" src="https://scienceblogs.com/files/startswithabang/files/2008/05/phot-13b-08-preview.jpg" alt width="490" height="400" loading="lazy"&gt;&lt;/a&gt;&lt;/center&gt;What's nice about this is that, even though it's just what we expected, it rules out or constraints a lot of crazy alternatives (such as theories where the fundamental constants vary), because the temperature of the microwave background evolves according to standard theoretical predictions. Here's a link to &lt;a href="http://www.aanda.org/10.1051/0004-6361:200809727/pdf"&gt;the actual scientific paper&lt;/a&gt;, if you're into that sort of thing.
&lt;p&gt;By the way, while I've got you thinking about astronomy, NASA just announced that their X-ray satellite, Chandra, found a supernova in our own galaxy &lt;a href="http://www.universetoday.com/2008/05/14/the-big-announcement-chandra-vla-find-youngest-supernova-in-our-galaxy/"&gt;that went off in the 1800's&lt;/a&gt;, making it the most recent supernova ever to occur in our galaxy! Why'd it take so long to find? Because the whole damned galaxy was in the way: the explosion happened on the opposite side!&lt;/p&gt;
&lt;/div&gt;
      
&lt;span&gt;&lt;a title="View user profile." href="https://scienceblogs.com/startswithabang" lang about="https://scienceblogs.com/startswithabang" typeof="schema:Person" property="schema:name" datatype&gt;esiegel&lt;/a&gt;&lt;/span&gt;

&lt;span&gt;&lt;time datetime="2008-05-14T04:42:44-04:00" title="Wednesday, May 14, 2008 - 04:42"&gt;Wed, 05/14/2008 - 04:42&lt;/time&gt;
&lt;/span&gt;

  &lt;div class="field field--name-field-blog-tags field--type-entity-reference field--label-inline"&gt;
    &lt;div class="field--label"&gt;Tags&lt;/div&gt;
          &lt;div class="field--items"&gt;
              &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/big-bang" hreflang="en"&gt;Big Bang&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/astronomers" hreflang="en"&gt;astronomers&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/astronomy-0" hreflang="en"&gt;Astronomy&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/background" hreflang="en"&gt;background&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/carbon" hreflang="en"&gt;carbon&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/co" hreflang="en"&gt;CO&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/cosmic" hreflang="en"&gt;cosmic&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/eso" hreflang="en"&gt;ESO&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/european" hreflang="en"&gt;european&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/evolve" hreflang="en"&gt;evolve&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/expanding" hreflang="en"&gt;expanding&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/expansion" hreflang="en"&gt;expansion&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/graph" hreflang="en"&gt;graph&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/kelvin" hreflang="en"&gt;Kelvin&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/kelvins" hreflang="en"&gt;Kelvins&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/man" hreflang="en"&gt;man&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/microwave" hreflang="en"&gt;Microwave&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/molecular" hreflang="en"&gt;molecular&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/molecule" hreflang="en"&gt;molecule&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/moleculo" hreflang="en"&gt;moleculo&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/monoxide" hreflang="en"&gt;monoxide&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/observatories" hreflang="en"&gt;observatories&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/observatory" hreflang="en"&gt;observatory&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/scientific" hreflang="en"&gt;scientific&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/southern" hreflang="en"&gt;southern&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/temp" hreflang="en"&gt;temp&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/temperature" hreflang="en"&gt;temperature&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/theoretical" hreflang="en"&gt;theoretical&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/theory-0" hreflang="en"&gt;Theory&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/thermometer" hreflang="en"&gt;thermometer&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/universe" hreflang="en"&gt;universe&lt;/a&gt;&lt;/div&gt;
              &lt;/div&gt;
      &lt;/div&gt;


&lt;section&gt;
  
  

  
&lt;/section&gt;
&lt;ul class="links inline list-inline"&gt;&lt;li class="comment-forbidden"&gt;&lt;/li&gt;&lt;/ul&gt;</description>
  <pubDate>Fri, 12 Dec 2025 20:42:39 +0000</pubDate>
    <dc:creator>sb admin</dc:creator>
    <guid isPermaLink="false">151468 at https://scienceblogs.com</guid>
    </item>
<item>
  <title>No Secretary Kennedy, The MMR Vaccine Does Not Contain 'Aborted Fetus Debris'</title>
  <link>https://scienceblogs.com/sb-admin/2025/05/02/no-secretary-kennedy-mmr-vaccine-does-not-contain-aborted-fetus-debris-151464</link>
  <description>
&lt;span&gt;Astronomers make use of… molecules?&lt;/span&gt;

            &lt;div class="field field--name-body field--type-text-with-summary field--label-hidden field--item"&gt;&lt;p&gt;When I think of molecules, I think of &lt;a href="http://www.yikers.com/video_conan_is_the_molecular_man.html"&gt;Conan O'Brien&lt;/a&gt; doing his skit where he plays Moleculo...&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;/center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/moleculo.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25276" title="moleculo" src="https://scienceblogs.com/files/startswithabang/files/2008/05/moleculo.jpg" alt width="413" height="331" loading="lazy"&gt;&lt;/a&gt;
&lt;p&gt;the molecular man! I don't think of astronomy, and I certainly don't think of the &lt;a href="http://map.gsfc.nasa.gov/universe/bb_tests_cmb.html"&gt;leftover radiation from the big bang&lt;/a&gt; (known as the cosmic microwave background)! But somebody over at the European Southern Observatory put these two together and made &lt;a href="http://www.eso.org/public/outreach/press-rel/pr-2008/pr-13-08.html"&gt;an incredibly tasty science sandwich&lt;/a&gt;.&lt;/p&gt;
&lt;p&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/222470571.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25277" title="222470571" src="https://scienceblogs.com/files/startswithabang/files/2008/05/222470571.jpg" alt width="221" height="98" loading="lazy"&gt;&lt;/a&gt;&lt;/p&gt;
&lt;p&gt;See, we can measure the cosmic microwave background today, because we have photons (particles of light) coming at us in all directions at all locations, with a temperature of 2.725 Kelvin. Theoretical cosmology tells us that when the Universe was younger, it was also smaller. Because the expansion of space stretches the photons in it, causing them to lose energy, it means that photons were hotter when the Universe was younger.&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;/center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/universe_expansion-sml-2.gif"&gt;&lt;img class="aligncenter size-full wp-image-25278" title="universe_expansion-sml-2" src="https://scienceblogs.com/files/startswithabang/files/2008/05/universe_expansion-sml-2.gif" alt width="336" height="336" loading="lazy"&gt;&lt;/a&gt;
&lt;p&gt;But we've never been able to measure that, of course. After all, how can you measure the temperature of something in a place where you aren't? (Hint: read the title of this post.) Use molecules as thermometers! Using a carbon monoxide molecule (CO to you chemists) in a distant galaxy, they were able to measure the temperature of the microwave background when the Universe was only about 3 billion years old! The temperature they measured was 9.15 +/- 0.70 Kelvins; and this compares pretty well with the predicted temperature of 9.315 Kelvin. Not bad! Here's an incomprehensible graph for you to look at while you take it all in:&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/phot-13b-08-preview.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25279" title="PP-53-07" src="https://scienceblogs.com/files/startswithabang/files/2008/05/phot-13b-08-preview.jpg" alt width="490" height="400" loading="lazy"&gt;&lt;/a&gt;&lt;/center&gt;What's nice about this is that, even though it's just what we expected, it rules out or constraints a lot of crazy alternatives (such as theories where the fundamental constants vary), because the temperature of the microwave background evolves according to standard theoretical predictions. Here's a link to &lt;a href="http://www.aanda.org/10.1051/0004-6361:200809727/pdf"&gt;the actual scientific paper&lt;/a&gt;, if you're into that sort of thing.
&lt;p&gt;By the way, while I've got you thinking about astronomy, NASA just announced that their X-ray satellite, Chandra, found a supernova in our own galaxy &lt;a href="http://www.universetoday.com/2008/05/14/the-big-announcement-chandra-vla-find-youngest-supernova-in-our-galaxy/"&gt;that went off in the 1800's&lt;/a&gt;, making it the most recent supernova ever to occur in our galaxy! Why'd it take so long to find? Because the whole damned galaxy was in the way: the explosion happened on the opposite side!&lt;/p&gt;
&lt;/div&gt;
      
&lt;span&gt;&lt;a title="View user profile." href="https://scienceblogs.com/startswithabang" lang about="https://scienceblogs.com/startswithabang" typeof="schema:Person" property="schema:name" datatype&gt;esiegel&lt;/a&gt;&lt;/span&gt;

&lt;span&gt;&lt;time datetime="2008-05-14T04:42:44-04:00" title="Wednesday, May 14, 2008 - 04:42"&gt;Wed, 05/14/2008 - 04:42&lt;/time&gt;
&lt;/span&gt;

  &lt;div class="field field--name-field-blog-tags field--type-entity-reference field--label-inline"&gt;
    &lt;div class="field--label"&gt;Tags&lt;/div&gt;
          &lt;div class="field--items"&gt;
              &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/big-bang" hreflang="en"&gt;Big Bang&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/astronomers" hreflang="en"&gt;astronomers&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/astronomy-0" hreflang="en"&gt;Astronomy&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/background" hreflang="en"&gt;background&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/carbon" hreflang="en"&gt;carbon&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/co" hreflang="en"&gt;CO&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/cosmic" hreflang="en"&gt;cosmic&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/eso" hreflang="en"&gt;ESO&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/european" hreflang="en"&gt;european&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/evolve" hreflang="en"&gt;evolve&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/expanding" hreflang="en"&gt;expanding&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/expansion" hreflang="en"&gt;expansion&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/graph" hreflang="en"&gt;graph&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/kelvin" hreflang="en"&gt;Kelvin&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/kelvins" hreflang="en"&gt;Kelvins&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/man" hreflang="en"&gt;man&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/microwave" hreflang="en"&gt;Microwave&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/molecular" hreflang="en"&gt;molecular&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/molecule" hreflang="en"&gt;molecule&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/moleculo" hreflang="en"&gt;moleculo&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/monoxide" hreflang="en"&gt;monoxide&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/observatories" hreflang="en"&gt;observatories&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/observatory" hreflang="en"&gt;observatory&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/scientific" hreflang="en"&gt;scientific&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/southern" hreflang="en"&gt;southern&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/temp" hreflang="en"&gt;temp&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/temperature" hreflang="en"&gt;temperature&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/theoretical" hreflang="en"&gt;theoretical&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/theory-0" hreflang="en"&gt;Theory&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/thermometer" hreflang="en"&gt;thermometer&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/universe" hreflang="en"&gt;universe&lt;/a&gt;&lt;/div&gt;
              &lt;/div&gt;
      &lt;/div&gt;


&lt;section&gt;
  
  

  
&lt;/section&gt;
&lt;ul class="links inline list-inline"&gt;&lt;li class="comment-forbidden"&gt;&lt;/li&gt;&lt;/ul&gt;</description>
  <pubDate>Fri, 02 May 2025 19:56:43 +0000</pubDate>
    <dc:creator>sb admin</dc:creator>
    <guid isPermaLink="false">151464 at https://scienceblogs.com</guid>
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<item>
  <title>Curiosity Found New Carbon Molecules On Mars. What Does It Mean For Alien Life?</title>
  <link>https://scienceblogs.com/sb-admin/2025/03/28/curiosity-found-new-carbon-molecules-mars-what-does-it-mean-alien-life-151463</link>
  <description>
&lt;span&gt;Astronomers make use of… molecules?&lt;/span&gt;

            &lt;div class="field field--name-body field--type-text-with-summary field--label-hidden field--item"&gt;&lt;p&gt;When I think of molecules, I think of &lt;a href="http://www.yikers.com/video_conan_is_the_molecular_man.html"&gt;Conan O'Brien&lt;/a&gt; doing his skit where he plays Moleculo...&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;/center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/moleculo.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25276" title="moleculo" src="https://scienceblogs.com/files/startswithabang/files/2008/05/moleculo.jpg" alt width="413" height="331" loading="lazy"&gt;&lt;/a&gt;
&lt;p&gt;the molecular man! I don't think of astronomy, and I certainly don't think of the &lt;a href="http://map.gsfc.nasa.gov/universe/bb_tests_cmb.html"&gt;leftover radiation from the big bang&lt;/a&gt; (known as the cosmic microwave background)! But somebody over at the European Southern Observatory put these two together and made &lt;a href="http://www.eso.org/public/outreach/press-rel/pr-2008/pr-13-08.html"&gt;an incredibly tasty science sandwich&lt;/a&gt;.&lt;/p&gt;
&lt;p&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/222470571.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25277" title="222470571" src="https://scienceblogs.com/files/startswithabang/files/2008/05/222470571.jpg" alt width="221" height="98" loading="lazy"&gt;&lt;/a&gt;&lt;/p&gt;
&lt;p&gt;See, we can measure the cosmic microwave background today, because we have photons (particles of light) coming at us in all directions at all locations, with a temperature of 2.725 Kelvin. Theoretical cosmology tells us that when the Universe was younger, it was also smaller. Because the expansion of space stretches the photons in it, causing them to lose energy, it means that photons were hotter when the Universe was younger.&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;/center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/universe_expansion-sml-2.gif"&gt;&lt;img class="aligncenter size-full wp-image-25278" title="universe_expansion-sml-2" src="https://scienceblogs.com/files/startswithabang/files/2008/05/universe_expansion-sml-2.gif" alt width="336" height="336" loading="lazy"&gt;&lt;/a&gt;
&lt;p&gt;But we've never been able to measure that, of course. After all, how can you measure the temperature of something in a place where you aren't? (Hint: read the title of this post.) Use molecules as thermometers! Using a carbon monoxide molecule (CO to you chemists) in a distant galaxy, they were able to measure the temperature of the microwave background when the Universe was only about 3 billion years old! The temperature they measured was 9.15 +/- 0.70 Kelvins; and this compares pretty well with the predicted temperature of 9.315 Kelvin. Not bad! Here's an incomprehensible graph for you to look at while you take it all in:&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/phot-13b-08-preview.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25279" title="PP-53-07" src="https://scienceblogs.com/files/startswithabang/files/2008/05/phot-13b-08-preview.jpg" alt width="490" height="400" loading="lazy"&gt;&lt;/a&gt;&lt;/center&gt;What's nice about this is that, even though it's just what we expected, it rules out or constraints a lot of crazy alternatives (such as theories where the fundamental constants vary), because the temperature of the microwave background evolves according to standard theoretical predictions. Here's a link to &lt;a href="http://www.aanda.org/10.1051/0004-6361:200809727/pdf"&gt;the actual scientific paper&lt;/a&gt;, if you're into that sort of thing.
&lt;p&gt;By the way, while I've got you thinking about astronomy, NASA just announced that their X-ray satellite, Chandra, found a supernova in our own galaxy &lt;a href="http://www.universetoday.com/2008/05/14/the-big-announcement-chandra-vla-find-youngest-supernova-in-our-galaxy/"&gt;that went off in the 1800's&lt;/a&gt;, making it the most recent supernova ever to occur in our galaxy! Why'd it take so long to find? Because the whole damned galaxy was in the way: the explosion happened on the opposite side!&lt;/p&gt;
&lt;/div&gt;
      
&lt;span&gt;&lt;a title="View user profile." href="https://scienceblogs.com/startswithabang" lang about="https://scienceblogs.com/startswithabang" typeof="schema:Person" property="schema:name" datatype&gt;esiegel&lt;/a&gt;&lt;/span&gt;

&lt;span&gt;&lt;time datetime="2008-05-14T04:42:44-04:00" title="Wednesday, May 14, 2008 - 04:42"&gt;Wed, 05/14/2008 - 04:42&lt;/time&gt;
&lt;/span&gt;

  &lt;div class="field field--name-field-blog-tags field--type-entity-reference field--label-inline"&gt;
    &lt;div class="field--label"&gt;Tags&lt;/div&gt;
          &lt;div class="field--items"&gt;
              &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/big-bang" hreflang="en"&gt;Big Bang&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/astronomers" hreflang="en"&gt;astronomers&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/astronomy-0" hreflang="en"&gt;Astronomy&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/background" hreflang="en"&gt;background&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/carbon" hreflang="en"&gt;carbon&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/co" hreflang="en"&gt;CO&lt;/a&gt;&lt;/div&gt;
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          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/eso" hreflang="en"&gt;ESO&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/european" hreflang="en"&gt;european&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/evolve" hreflang="en"&gt;evolve&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/expanding" hreflang="en"&gt;expanding&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/expansion" hreflang="en"&gt;expansion&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/graph" hreflang="en"&gt;graph&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/kelvin" hreflang="en"&gt;Kelvin&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/kelvins" hreflang="en"&gt;Kelvins&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/man" hreflang="en"&gt;man&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/microwave" hreflang="en"&gt;Microwave&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/molecular" hreflang="en"&gt;molecular&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/molecule" hreflang="en"&gt;molecule&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/moleculo" hreflang="en"&gt;moleculo&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/monoxide" hreflang="en"&gt;monoxide&lt;/a&gt;&lt;/div&gt;
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          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/southern" hreflang="en"&gt;southern&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/temp" hreflang="en"&gt;temp&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/temperature" hreflang="en"&gt;temperature&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/theoretical" hreflang="en"&gt;theoretical&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/theory-0" hreflang="en"&gt;Theory&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/thermometer" hreflang="en"&gt;thermometer&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/universe" hreflang="en"&gt;universe&lt;/a&gt;&lt;/div&gt;
              &lt;/div&gt;
      &lt;/div&gt;


&lt;section&gt;
  
  

  
&lt;/section&gt;
&lt;ul class="links inline list-inline"&gt;&lt;li class="comment-forbidden"&gt;&lt;/li&gt;&lt;/ul&gt;</description>
  <pubDate>Fri, 28 Mar 2025 17:12:55 +0000</pubDate>
    <dc:creator>sb admin</dc:creator>
    <guid isPermaLink="false">151463 at https://scienceblogs.com</guid>
    </item>
<item>
  <title>Genetically Rescued Organism: Toward A Solution For Sudden Oak Death</title>
  <link>https://scienceblogs.com/sb-admin/2021/11/08/genetically-rescued-organism-toward-solution-sudden-oak-death-151458</link>
  <description>
&lt;span&gt;Astronomers make use of… molecules?&lt;/span&gt;

            &lt;div class="field field--name-body field--type-text-with-summary field--label-hidden field--item"&gt;&lt;p&gt;When I think of molecules, I think of &lt;a href="http://www.yikers.com/video_conan_is_the_molecular_man.html"&gt;Conan O'Brien&lt;/a&gt; doing his skit where he plays Moleculo...&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;/center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/moleculo.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25276" title="moleculo" src="https://scienceblogs.com/files/startswithabang/files/2008/05/moleculo.jpg" alt width="413" height="331" loading="lazy"&gt;&lt;/a&gt;
&lt;p&gt;the molecular man! I don't think of astronomy, and I certainly don't think of the &lt;a href="http://map.gsfc.nasa.gov/universe/bb_tests_cmb.html"&gt;leftover radiation from the big bang&lt;/a&gt; (known as the cosmic microwave background)! But somebody over at the European Southern Observatory put these two together and made &lt;a href="http://www.eso.org/public/outreach/press-rel/pr-2008/pr-13-08.html"&gt;an incredibly tasty science sandwich&lt;/a&gt;.&lt;/p&gt;
&lt;p&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/222470571.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25277" title="222470571" src="https://scienceblogs.com/files/startswithabang/files/2008/05/222470571.jpg" alt width="221" height="98" loading="lazy"&gt;&lt;/a&gt;&lt;/p&gt;
&lt;p&gt;See, we can measure the cosmic microwave background today, because we have photons (particles of light) coming at us in all directions at all locations, with a temperature of 2.725 Kelvin. Theoretical cosmology tells us that when the Universe was younger, it was also smaller. Because the expansion of space stretches the photons in it, causing them to lose energy, it means that photons were hotter when the Universe was younger.&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;/center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/universe_expansion-sml-2.gif"&gt;&lt;img class="aligncenter size-full wp-image-25278" title="universe_expansion-sml-2" src="https://scienceblogs.com/files/startswithabang/files/2008/05/universe_expansion-sml-2.gif" alt width="336" height="336" loading="lazy"&gt;&lt;/a&gt;
&lt;p&gt;But we've never been able to measure that, of course. After all, how can you measure the temperature of something in a place where you aren't? (Hint: read the title of this post.) Use molecules as thermometers! Using a carbon monoxide molecule (CO to you chemists) in a distant galaxy, they were able to measure the temperature of the microwave background when the Universe was only about 3 billion years old! The temperature they measured was 9.15 +/- 0.70 Kelvins; and this compares pretty well with the predicted temperature of 9.315 Kelvin. Not bad! Here's an incomprehensible graph for you to look at while you take it all in:&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/phot-13b-08-preview.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25279" title="PP-53-07" src="https://scienceblogs.com/files/startswithabang/files/2008/05/phot-13b-08-preview.jpg" alt width="490" height="400" loading="lazy"&gt;&lt;/a&gt;&lt;/center&gt;What's nice about this is that, even though it's just what we expected, it rules out or constraints a lot of crazy alternatives (such as theories where the fundamental constants vary), because the temperature of the microwave background evolves according to standard theoretical predictions. Here's a link to &lt;a href="http://www.aanda.org/10.1051/0004-6361:200809727/pdf"&gt;the actual scientific paper&lt;/a&gt;, if you're into that sort of thing.
&lt;p&gt;By the way, while I've got you thinking about astronomy, NASA just announced that their X-ray satellite, Chandra, found a supernova in our own galaxy &lt;a href="http://www.universetoday.com/2008/05/14/the-big-announcement-chandra-vla-find-youngest-supernova-in-our-galaxy/"&gt;that went off in the 1800's&lt;/a&gt;, making it the most recent supernova ever to occur in our galaxy! Why'd it take so long to find? Because the whole damned galaxy was in the way: the explosion happened on the opposite side!&lt;/p&gt;
&lt;/div&gt;
      
&lt;span&gt;&lt;a title="View user profile." href="https://scienceblogs.com/startswithabang" lang about="https://scienceblogs.com/startswithabang" typeof="schema:Person" property="schema:name" datatype&gt;esiegel&lt;/a&gt;&lt;/span&gt;

&lt;span&gt;&lt;time datetime="2008-05-14T04:42:44-04:00" title="Wednesday, May 14, 2008 - 04:42"&gt;Wed, 05/14/2008 - 04:42&lt;/time&gt;
&lt;/span&gt;

  &lt;div class="field field--name-field-blog-tags field--type-entity-reference field--label-inline"&gt;
    &lt;div class="field--label"&gt;Tags&lt;/div&gt;
          &lt;div class="field--items"&gt;
              &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/big-bang" hreflang="en"&gt;Big Bang&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/astronomers" hreflang="en"&gt;astronomers&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/astronomy-0" hreflang="en"&gt;Astronomy&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/background" hreflang="en"&gt;background&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/carbon" hreflang="en"&gt;carbon&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/co" hreflang="en"&gt;CO&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/cosmic" hreflang="en"&gt;cosmic&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/eso" hreflang="en"&gt;ESO&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/european" hreflang="en"&gt;european&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/evolve" hreflang="en"&gt;evolve&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/expanding" hreflang="en"&gt;expanding&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/expansion" hreflang="en"&gt;expansion&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/graph" hreflang="en"&gt;graph&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/kelvin" hreflang="en"&gt;Kelvin&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/kelvins" hreflang="en"&gt;Kelvins&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/man" hreflang="en"&gt;man&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/microwave" hreflang="en"&gt;Microwave&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/molecular" hreflang="en"&gt;molecular&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/molecule" hreflang="en"&gt;molecule&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/moleculo" hreflang="en"&gt;moleculo&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/monoxide" hreflang="en"&gt;monoxide&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/observatories" hreflang="en"&gt;observatories&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/observatory" hreflang="en"&gt;observatory&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/scientific" hreflang="en"&gt;scientific&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/southern" hreflang="en"&gt;southern&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/temp" hreflang="en"&gt;temp&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/temperature" hreflang="en"&gt;temperature&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/theoretical" hreflang="en"&gt;theoretical&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/theory-0" hreflang="en"&gt;Theory&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/thermometer" hreflang="en"&gt;thermometer&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/universe" hreflang="en"&gt;universe&lt;/a&gt;&lt;/div&gt;
              &lt;/div&gt;
      &lt;/div&gt;


&lt;section&gt;
  
  

  
&lt;/section&gt;
&lt;ul class="links inline list-inline"&gt;&lt;li class="comment-forbidden"&gt;&lt;/li&gt;&lt;/ul&gt;</description>
  <pubDate>Mon, 08 Nov 2021 22:47:18 +0000</pubDate>
    <dc:creator>sb admin</dc:creator>
    <guid isPermaLink="false">151458 at https://scienceblogs.com</guid>
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  <title>Appreciating van Leeuwenhoek: The Cloth Merchant Who Discovered Microbes</title>
  <link>https://scienceblogs.com/sb-admin/2021/04/06/appreciating-van-leeuwenhoek-cloth-merchant-who-discovered-microbes-151456</link>
  <description>
&lt;span&gt;Astronomers make use of… molecules?&lt;/span&gt;

            &lt;div class="field field--name-body field--type-text-with-summary field--label-hidden field--item"&gt;&lt;p&gt;When I think of molecules, I think of &lt;a href="http://www.yikers.com/video_conan_is_the_molecular_man.html"&gt;Conan O'Brien&lt;/a&gt; doing his skit where he plays Moleculo...&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;/center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/moleculo.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25276" title="moleculo" src="https://scienceblogs.com/files/startswithabang/files/2008/05/moleculo.jpg" alt width="413" height="331" loading="lazy"&gt;&lt;/a&gt;
&lt;p&gt;the molecular man! I don't think of astronomy, and I certainly don't think of the &lt;a href="http://map.gsfc.nasa.gov/universe/bb_tests_cmb.html"&gt;leftover radiation from the big bang&lt;/a&gt; (known as the cosmic microwave background)! But somebody over at the European Southern Observatory put these two together and made &lt;a href="http://www.eso.org/public/outreach/press-rel/pr-2008/pr-13-08.html"&gt;an incredibly tasty science sandwich&lt;/a&gt;.&lt;/p&gt;
&lt;p&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/222470571.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25277" title="222470571" src="https://scienceblogs.com/files/startswithabang/files/2008/05/222470571.jpg" alt width="221" height="98" loading="lazy"&gt;&lt;/a&gt;&lt;/p&gt;
&lt;p&gt;See, we can measure the cosmic microwave background today, because we have photons (particles of light) coming at us in all directions at all locations, with a temperature of 2.725 Kelvin. Theoretical cosmology tells us that when the Universe was younger, it was also smaller. Because the expansion of space stretches the photons in it, causing them to lose energy, it means that photons were hotter when the Universe was younger.&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;/center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/universe_expansion-sml-2.gif"&gt;&lt;img class="aligncenter size-full wp-image-25278" title="universe_expansion-sml-2" src="https://scienceblogs.com/files/startswithabang/files/2008/05/universe_expansion-sml-2.gif" alt width="336" height="336" loading="lazy"&gt;&lt;/a&gt;
&lt;p&gt;But we've never been able to measure that, of course. After all, how can you measure the temperature of something in a place where you aren't? (Hint: read the title of this post.) Use molecules as thermometers! Using a carbon monoxide molecule (CO to you chemists) in a distant galaxy, they were able to measure the temperature of the microwave background when the Universe was only about 3 billion years old! The temperature they measured was 9.15 +/- 0.70 Kelvins; and this compares pretty well with the predicted temperature of 9.315 Kelvin. Not bad! Here's an incomprehensible graph for you to look at while you take it all in:&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/phot-13b-08-preview.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25279" title="PP-53-07" src="https://scienceblogs.com/files/startswithabang/files/2008/05/phot-13b-08-preview.jpg" alt width="490" height="400" loading="lazy"&gt;&lt;/a&gt;&lt;/center&gt;What's nice about this is that, even though it's just what we expected, it rules out or constraints a lot of crazy alternatives (such as theories where the fundamental constants vary), because the temperature of the microwave background evolves according to standard theoretical predictions. Here's a link to &lt;a href="http://www.aanda.org/10.1051/0004-6361:200809727/pdf"&gt;the actual scientific paper&lt;/a&gt;, if you're into that sort of thing.
&lt;p&gt;By the way, while I've got you thinking about astronomy, NASA just announced that their X-ray satellite, Chandra, found a supernova in our own galaxy &lt;a href="http://www.universetoday.com/2008/05/14/the-big-announcement-chandra-vla-find-youngest-supernova-in-our-galaxy/"&gt;that went off in the 1800's&lt;/a&gt;, making it the most recent supernova ever to occur in our galaxy! Why'd it take so long to find? Because the whole damned galaxy was in the way: the explosion happened on the opposite side!&lt;/p&gt;
&lt;/div&gt;
      
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&lt;span&gt;&lt;time datetime="2008-05-14T04:42:44-04:00" title="Wednesday, May 14, 2008 - 04:42"&gt;Wed, 05/14/2008 - 04:42&lt;/time&gt;
&lt;/span&gt;

  &lt;div class="field field--name-field-blog-tags field--type-entity-reference field--label-inline"&gt;
    &lt;div class="field--label"&gt;Tags&lt;/div&gt;
          &lt;div class="field--items"&gt;
              &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/big-bang" hreflang="en"&gt;Big Bang&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/astronomers" hreflang="en"&gt;astronomers&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/astronomy-0" hreflang="en"&gt;Astronomy&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/background" hreflang="en"&gt;background&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/carbon" hreflang="en"&gt;carbon&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/co" hreflang="en"&gt;CO&lt;/a&gt;&lt;/div&gt;
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          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/kelvins" hreflang="en"&gt;Kelvins&lt;/a&gt;&lt;/div&gt;
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          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/moleculo" hreflang="en"&gt;moleculo&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/monoxide" hreflang="en"&gt;monoxide&lt;/a&gt;&lt;/div&gt;
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          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/southern" hreflang="en"&gt;southern&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/temp" hreflang="en"&gt;temp&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/temperature" hreflang="en"&gt;temperature&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/theoretical" hreflang="en"&gt;theoretical&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/theory-0" hreflang="en"&gt;Theory&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/thermometer" hreflang="en"&gt;thermometer&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/universe" hreflang="en"&gt;universe&lt;/a&gt;&lt;/div&gt;
              &lt;/div&gt;
      &lt;/div&gt;


&lt;section&gt;
  
  

  
&lt;/section&gt;
&lt;ul class="links inline list-inline"&gt;&lt;li class="comment-forbidden"&gt;&lt;/li&gt;&lt;/ul&gt;</description>
  <pubDate>Tue, 06 Apr 2021 14:49:13 +0000</pubDate>
    <dc:creator>sb admin</dc:creator>
    <guid isPermaLink="false">151456 at https://scienceblogs.com</guid>
    </item>
<item>
  <title>The Yeast All Around Us</title>
  <link>https://scienceblogs.com/sb-admin/2020/05/11/yeast-all-around-us-151448</link>
  <description>
&lt;span&gt;Astronomers make use of… molecules?&lt;/span&gt;

            &lt;div class="field field--name-body field--type-text-with-summary field--label-hidden field--item"&gt;&lt;p&gt;When I think of molecules, I think of &lt;a href="http://www.yikers.com/video_conan_is_the_molecular_man.html"&gt;Conan O'Brien&lt;/a&gt; doing his skit where he plays Moleculo...&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;/center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/moleculo.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25276" title="moleculo" src="https://scienceblogs.com/files/startswithabang/files/2008/05/moleculo.jpg" alt width="413" height="331" loading="lazy"&gt;&lt;/a&gt;
&lt;p&gt;the molecular man! I don't think of astronomy, and I certainly don't think of the &lt;a href="http://map.gsfc.nasa.gov/universe/bb_tests_cmb.html"&gt;leftover radiation from the big bang&lt;/a&gt; (known as the cosmic microwave background)! But somebody over at the European Southern Observatory put these two together and made &lt;a href="http://www.eso.org/public/outreach/press-rel/pr-2008/pr-13-08.html"&gt;an incredibly tasty science sandwich&lt;/a&gt;.&lt;/p&gt;
&lt;p&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/222470571.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25277" title="222470571" src="https://scienceblogs.com/files/startswithabang/files/2008/05/222470571.jpg" alt width="221" height="98" loading="lazy"&gt;&lt;/a&gt;&lt;/p&gt;
&lt;p&gt;See, we can measure the cosmic microwave background today, because we have photons (particles of light) coming at us in all directions at all locations, with a temperature of 2.725 Kelvin. Theoretical cosmology tells us that when the Universe was younger, it was also smaller. Because the expansion of space stretches the photons in it, causing them to lose energy, it means that photons were hotter when the Universe was younger.&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;/center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/universe_expansion-sml-2.gif"&gt;&lt;img class="aligncenter size-full wp-image-25278" title="universe_expansion-sml-2" src="https://scienceblogs.com/files/startswithabang/files/2008/05/universe_expansion-sml-2.gif" alt width="336" height="336" loading="lazy"&gt;&lt;/a&gt;
&lt;p&gt;But we've never been able to measure that, of course. After all, how can you measure the temperature of something in a place where you aren't? (Hint: read the title of this post.) Use molecules as thermometers! Using a carbon monoxide molecule (CO to you chemists) in a distant galaxy, they were able to measure the temperature of the microwave background when the Universe was only about 3 billion years old! The temperature they measured was 9.15 +/- 0.70 Kelvins; and this compares pretty well with the predicted temperature of 9.315 Kelvin. Not bad! Here's an incomprehensible graph for you to look at while you take it all in:&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/phot-13b-08-preview.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25279" title="PP-53-07" src="https://scienceblogs.com/files/startswithabang/files/2008/05/phot-13b-08-preview.jpg" alt width="490" height="400" loading="lazy"&gt;&lt;/a&gt;&lt;/center&gt;What's nice about this is that, even though it's just what we expected, it rules out or constraints a lot of crazy alternatives (such as theories where the fundamental constants vary), because the temperature of the microwave background evolves according to standard theoretical predictions. Here's a link to &lt;a href="http://www.aanda.org/10.1051/0004-6361:200809727/pdf"&gt;the actual scientific paper&lt;/a&gt;, if you're into that sort of thing.
&lt;p&gt;By the way, while I've got you thinking about astronomy, NASA just announced that their X-ray satellite, Chandra, found a supernova in our own galaxy &lt;a href="http://www.universetoday.com/2008/05/14/the-big-announcement-chandra-vla-find-youngest-supernova-in-our-galaxy/"&gt;that went off in the 1800's&lt;/a&gt;, making it the most recent supernova ever to occur in our galaxy! Why'd it take so long to find? Because the whole damned galaxy was in the way: the explosion happened on the opposite side!&lt;/p&gt;
&lt;/div&gt;
      
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&lt;span&gt;&lt;time datetime="2008-05-14T04:42:44-04:00" title="Wednesday, May 14, 2008 - 04:42"&gt;Wed, 05/14/2008 - 04:42&lt;/time&gt;
&lt;/span&gt;

  &lt;div class="field field--name-field-blog-tags field--type-entity-reference field--label-inline"&gt;
    &lt;div class="field--label"&gt;Tags&lt;/div&gt;
          &lt;div class="field--items"&gt;
              &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/big-bang" hreflang="en"&gt;Big Bang&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/astronomers" hreflang="en"&gt;astronomers&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/astronomy-0" hreflang="en"&gt;Astronomy&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/background" hreflang="en"&gt;background&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/carbon" hreflang="en"&gt;carbon&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/co" hreflang="en"&gt;CO&lt;/a&gt;&lt;/div&gt;
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          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/eso" hreflang="en"&gt;ESO&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/european" hreflang="en"&gt;european&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/evolve" hreflang="en"&gt;evolve&lt;/a&gt;&lt;/div&gt;
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          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/expansion" hreflang="en"&gt;expansion&lt;/a&gt;&lt;/div&gt;
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          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/kelvins" hreflang="en"&gt;Kelvins&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/man" hreflang="en"&gt;man&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/microwave" hreflang="en"&gt;Microwave&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/molecular" hreflang="en"&gt;molecular&lt;/a&gt;&lt;/div&gt;
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          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/moleculo" hreflang="en"&gt;moleculo&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/monoxide" hreflang="en"&gt;monoxide&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/observatories" hreflang="en"&gt;observatories&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/observatory" hreflang="en"&gt;observatory&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/scientific" hreflang="en"&gt;scientific&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/southern" hreflang="en"&gt;southern&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/temp" hreflang="en"&gt;temp&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/temperature" hreflang="en"&gt;temperature&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/theoretical" hreflang="en"&gt;theoretical&lt;/a&gt;&lt;/div&gt;
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          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/thermometer" hreflang="en"&gt;thermometer&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/universe" hreflang="en"&gt;universe&lt;/a&gt;&lt;/div&gt;
              &lt;/div&gt;
      &lt;/div&gt;


&lt;section&gt;
  
  

  
&lt;/section&gt;
&lt;ul class="links inline list-inline"&gt;&lt;li class="comment-forbidden"&gt;&lt;/li&gt;&lt;/ul&gt;</description>
  <pubDate>Mon, 11 May 2020 15:54:57 +0000</pubDate>
    <dc:creator>sb admin</dc:creator>
    <guid isPermaLink="false">151448 at https://scienceblogs.com</guid>
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<item>
  <title>The Biology Of Why Coronavirus Is So Deadly</title>
  <link>https://scienceblogs.com/conversation/2020/04/02/biology-why-coronavirus-so-deadly-151447</link>
  <description>
&lt;span&gt;Astronomers make use of… molecules?&lt;/span&gt;

            &lt;div class="field field--name-body field--type-text-with-summary field--label-hidden field--item"&gt;&lt;p&gt;When I think of molecules, I think of &lt;a href="http://www.yikers.com/video_conan_is_the_molecular_man.html"&gt;Conan O'Brien&lt;/a&gt; doing his skit where he plays Moleculo...&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;/center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/moleculo.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25276" title="moleculo" src="https://scienceblogs.com/files/startswithabang/files/2008/05/moleculo.jpg" alt width="413" height="331" loading="lazy"&gt;&lt;/a&gt;
&lt;p&gt;the molecular man! I don't think of astronomy, and I certainly don't think of the &lt;a href="http://map.gsfc.nasa.gov/universe/bb_tests_cmb.html"&gt;leftover radiation from the big bang&lt;/a&gt; (known as the cosmic microwave background)! But somebody over at the European Southern Observatory put these two together and made &lt;a href="http://www.eso.org/public/outreach/press-rel/pr-2008/pr-13-08.html"&gt;an incredibly tasty science sandwich&lt;/a&gt;.&lt;/p&gt;
&lt;p&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/222470571.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25277" title="222470571" src="https://scienceblogs.com/files/startswithabang/files/2008/05/222470571.jpg" alt width="221" height="98" loading="lazy"&gt;&lt;/a&gt;&lt;/p&gt;
&lt;p&gt;See, we can measure the cosmic microwave background today, because we have photons (particles of light) coming at us in all directions at all locations, with a temperature of 2.725 Kelvin. Theoretical cosmology tells us that when the Universe was younger, it was also smaller. Because the expansion of space stretches the photons in it, causing them to lose energy, it means that photons were hotter when the Universe was younger.&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;/center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/universe_expansion-sml-2.gif"&gt;&lt;img class="aligncenter size-full wp-image-25278" title="universe_expansion-sml-2" src="https://scienceblogs.com/files/startswithabang/files/2008/05/universe_expansion-sml-2.gif" alt width="336" height="336" loading="lazy"&gt;&lt;/a&gt;
&lt;p&gt;But we've never been able to measure that, of course. After all, how can you measure the temperature of something in a place where you aren't? (Hint: read the title of this post.) Use molecules as thermometers! Using a carbon monoxide molecule (CO to you chemists) in a distant galaxy, they were able to measure the temperature of the microwave background when the Universe was only about 3 billion years old! The temperature they measured was 9.15 +/- 0.70 Kelvins; and this compares pretty well with the predicted temperature of 9.315 Kelvin. Not bad! Here's an incomprehensible graph for you to look at while you take it all in:&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/phot-13b-08-preview.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25279" title="PP-53-07" src="https://scienceblogs.com/files/startswithabang/files/2008/05/phot-13b-08-preview.jpg" alt width="490" height="400" loading="lazy"&gt;&lt;/a&gt;&lt;/center&gt;What's nice about this is that, even though it's just what we expected, it rules out or constraints a lot of crazy alternatives (such as theories where the fundamental constants vary), because the temperature of the microwave background evolves according to standard theoretical predictions. Here's a link to &lt;a href="http://www.aanda.org/10.1051/0004-6361:200809727/pdf"&gt;the actual scientific paper&lt;/a&gt;, if you're into that sort of thing.
&lt;p&gt;By the way, while I've got you thinking about astronomy, NASA just announced that their X-ray satellite, Chandra, found a supernova in our own galaxy &lt;a href="http://www.universetoday.com/2008/05/14/the-big-announcement-chandra-vla-find-youngest-supernova-in-our-galaxy/"&gt;that went off in the 1800's&lt;/a&gt;, making it the most recent supernova ever to occur in our galaxy! Why'd it take so long to find? Because the whole damned galaxy was in the way: the explosion happened on the opposite side!&lt;/p&gt;
&lt;/div&gt;
      
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&lt;span&gt;&lt;time datetime="2008-05-14T04:42:44-04:00" title="Wednesday, May 14, 2008 - 04:42"&gt;Wed, 05/14/2008 - 04:42&lt;/time&gt;
&lt;/span&gt;

  &lt;div class="field field--name-field-blog-tags field--type-entity-reference field--label-inline"&gt;
    &lt;div class="field--label"&gt;Tags&lt;/div&gt;
          &lt;div class="field--items"&gt;
              &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/big-bang" hreflang="en"&gt;Big Bang&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/astronomers" hreflang="en"&gt;astronomers&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/astronomy-0" hreflang="en"&gt;Astronomy&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/background" hreflang="en"&gt;background&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/carbon" hreflang="en"&gt;carbon&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/co" hreflang="en"&gt;CO&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/cosmic" hreflang="en"&gt;cosmic&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/eso" hreflang="en"&gt;ESO&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/european" hreflang="en"&gt;european&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/evolve" hreflang="en"&gt;evolve&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/expanding" hreflang="en"&gt;expanding&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/expansion" hreflang="en"&gt;expansion&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/graph" hreflang="en"&gt;graph&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/kelvin" hreflang="en"&gt;Kelvin&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/kelvins" hreflang="en"&gt;Kelvins&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/man" hreflang="en"&gt;man&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/microwave" hreflang="en"&gt;Microwave&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/molecular" hreflang="en"&gt;molecular&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/molecule" hreflang="en"&gt;molecule&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/moleculo" hreflang="en"&gt;moleculo&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/monoxide" hreflang="en"&gt;monoxide&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/observatories" hreflang="en"&gt;observatories&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/observatory" hreflang="en"&gt;observatory&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/scientific" hreflang="en"&gt;scientific&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/southern" hreflang="en"&gt;southern&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/temp" hreflang="en"&gt;temp&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/temperature" hreflang="en"&gt;temperature&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/theoretical" hreflang="en"&gt;theoretical&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/theory-0" hreflang="en"&gt;Theory&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/thermometer" hreflang="en"&gt;thermometer&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/universe" hreflang="en"&gt;universe&lt;/a&gt;&lt;/div&gt;
              &lt;/div&gt;
      &lt;/div&gt;


&lt;section&gt;
  
  

  
&lt;/section&gt;
&lt;ul class="links inline list-inline"&gt;&lt;li class="comment-forbidden"&gt;&lt;/li&gt;&lt;/ul&gt;</description>
  <pubDate>Thu, 02 Apr 2020 18:02:27 +0000</pubDate>
    <dc:creator>The Conversation</dc:creator>
    <guid isPermaLink="false">151447 at https://scienceblogs.com</guid>
    </item>
<item>
  <title>Coronavirus Is Not Passed From Mother to Child Late In Pregnancy</title>
  <link>https://scienceblogs.com/sb-admin/2020/02/12/coronavirus-not-passed-mother-child-late-pregnancy-151442</link>
  <description>
&lt;span&gt;Astronomers make use of… molecules?&lt;/span&gt;

            &lt;div class="field field--name-body field--type-text-with-summary field--label-hidden field--item"&gt;&lt;p&gt;When I think of molecules, I think of &lt;a href="http://www.yikers.com/video_conan_is_the_molecular_man.html"&gt;Conan O'Brien&lt;/a&gt; doing his skit where he plays Moleculo...&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;/center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/moleculo.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25276" title="moleculo" src="https://scienceblogs.com/files/startswithabang/files/2008/05/moleculo.jpg" alt width="413" height="331" loading="lazy"&gt;&lt;/a&gt;
&lt;p&gt;the molecular man! I don't think of astronomy, and I certainly don't think of the &lt;a href="http://map.gsfc.nasa.gov/universe/bb_tests_cmb.html"&gt;leftover radiation from the big bang&lt;/a&gt; (known as the cosmic microwave background)! But somebody over at the European Southern Observatory put these two together and made &lt;a href="http://www.eso.org/public/outreach/press-rel/pr-2008/pr-13-08.html"&gt;an incredibly tasty science sandwich&lt;/a&gt;.&lt;/p&gt;
&lt;p&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/222470571.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25277" title="222470571" src="https://scienceblogs.com/files/startswithabang/files/2008/05/222470571.jpg" alt width="221" height="98" loading="lazy"&gt;&lt;/a&gt;&lt;/p&gt;
&lt;p&gt;See, we can measure the cosmic microwave background today, because we have photons (particles of light) coming at us in all directions at all locations, with a temperature of 2.725 Kelvin. Theoretical cosmology tells us that when the Universe was younger, it was also smaller. Because the expansion of space stretches the photons in it, causing them to lose energy, it means that photons were hotter when the Universe was younger.&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;/center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/universe_expansion-sml-2.gif"&gt;&lt;img class="aligncenter size-full wp-image-25278" title="universe_expansion-sml-2" src="https://scienceblogs.com/files/startswithabang/files/2008/05/universe_expansion-sml-2.gif" alt width="336" height="336" loading="lazy"&gt;&lt;/a&gt;
&lt;p&gt;But we've never been able to measure that, of course. After all, how can you measure the temperature of something in a place where you aren't? (Hint: read the title of this post.) Use molecules as thermometers! Using a carbon monoxide molecule (CO to you chemists) in a distant galaxy, they were able to measure the temperature of the microwave background when the Universe was only about 3 billion years old! The temperature they measured was 9.15 +/- 0.70 Kelvins; and this compares pretty well with the predicted temperature of 9.315 Kelvin. Not bad! Here's an incomprehensible graph for you to look at while you take it all in:&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/phot-13b-08-preview.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25279" title="PP-53-07" src="https://scienceblogs.com/files/startswithabang/files/2008/05/phot-13b-08-preview.jpg" alt width="490" height="400" loading="lazy"&gt;&lt;/a&gt;&lt;/center&gt;What's nice about this is that, even though it's just what we expected, it rules out or constraints a lot of crazy alternatives (such as theories where the fundamental constants vary), because the temperature of the microwave background evolves according to standard theoretical predictions. Here's a link to &lt;a href="http://www.aanda.org/10.1051/0004-6361:200809727/pdf"&gt;the actual scientific paper&lt;/a&gt;, if you're into that sort of thing.
&lt;p&gt;By the way, while I've got you thinking about astronomy, NASA just announced that their X-ray satellite, Chandra, found a supernova in our own galaxy &lt;a href="http://www.universetoday.com/2008/05/14/the-big-announcement-chandra-vla-find-youngest-supernova-in-our-galaxy/"&gt;that went off in the 1800's&lt;/a&gt;, making it the most recent supernova ever to occur in our galaxy! Why'd it take so long to find? Because the whole damned galaxy was in the way: the explosion happened on the opposite side!&lt;/p&gt;
&lt;/div&gt;
      
&lt;span&gt;&lt;a title="View user profile." href="https://scienceblogs.com/startswithabang" lang about="https://scienceblogs.com/startswithabang" typeof="schema:Person" property="schema:name" datatype&gt;esiegel&lt;/a&gt;&lt;/span&gt;

&lt;span&gt;&lt;time datetime="2008-05-14T04:42:44-04:00" title="Wednesday, May 14, 2008 - 04:42"&gt;Wed, 05/14/2008 - 04:42&lt;/time&gt;
&lt;/span&gt;

  &lt;div class="field field--name-field-blog-tags field--type-entity-reference field--label-inline"&gt;
    &lt;div class="field--label"&gt;Tags&lt;/div&gt;
          &lt;div class="field--items"&gt;
              &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/big-bang" hreflang="en"&gt;Big Bang&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/astronomers" hreflang="en"&gt;astronomers&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/astronomy-0" hreflang="en"&gt;Astronomy&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/background" hreflang="en"&gt;background&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/carbon" hreflang="en"&gt;carbon&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/co" hreflang="en"&gt;CO&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/cosmic" hreflang="en"&gt;cosmic&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/eso" hreflang="en"&gt;ESO&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/european" hreflang="en"&gt;european&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/evolve" hreflang="en"&gt;evolve&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/expanding" hreflang="en"&gt;expanding&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/expansion" hreflang="en"&gt;expansion&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/graph" hreflang="en"&gt;graph&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/kelvin" hreflang="en"&gt;Kelvin&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/kelvins" hreflang="en"&gt;Kelvins&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/man" hreflang="en"&gt;man&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/microwave" hreflang="en"&gt;Microwave&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/molecular" hreflang="en"&gt;molecular&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/molecule" hreflang="en"&gt;molecule&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/moleculo" hreflang="en"&gt;moleculo&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/monoxide" hreflang="en"&gt;monoxide&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/observatories" hreflang="en"&gt;observatories&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/observatory" hreflang="en"&gt;observatory&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/scientific" hreflang="en"&gt;scientific&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/southern" hreflang="en"&gt;southern&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/temp" hreflang="en"&gt;temp&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/temperature" hreflang="en"&gt;temperature&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/theoretical" hreflang="en"&gt;theoretical&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/theory-0" hreflang="en"&gt;Theory&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/thermometer" hreflang="en"&gt;thermometer&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/universe" hreflang="en"&gt;universe&lt;/a&gt;&lt;/div&gt;
              &lt;/div&gt;
      &lt;/div&gt;


&lt;section&gt;
  
  

  
&lt;/section&gt;
&lt;ul class="links inline list-inline"&gt;&lt;li class="comment-forbidden"&gt;&lt;/li&gt;&lt;/ul&gt;</description>
  <pubDate>Wed, 12 Feb 2020 18:03:41 +0000</pubDate>
    <dc:creator>sb admin</dc:creator>
    <guid isPermaLink="false">151442 at https://scienceblogs.com</guid>
    </item>
<item>
  <title>CRISPR Immune Cells Not Only Survive, They Thrive After Infusion Into Cancer Patients</title>
  <link>https://scienceblogs.com/sb-admin/2020/02/06/crispr-immune-cells-not-only-survive-they-thrive-after-infusion-cancer-patients</link>
  <description>
&lt;span&gt;Astronomers make use of… molecules?&lt;/span&gt;

            &lt;div class="field field--name-body field--type-text-with-summary field--label-hidden field--item"&gt;&lt;p&gt;When I think of molecules, I think of &lt;a href="http://www.yikers.com/video_conan_is_the_molecular_man.html"&gt;Conan O'Brien&lt;/a&gt; doing his skit where he plays Moleculo...&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;/center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/moleculo.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25276" title="moleculo" src="https://scienceblogs.com/files/startswithabang/files/2008/05/moleculo.jpg" alt width="413" height="331" loading="lazy"&gt;&lt;/a&gt;
&lt;p&gt;the molecular man! I don't think of astronomy, and I certainly don't think of the &lt;a href="http://map.gsfc.nasa.gov/universe/bb_tests_cmb.html"&gt;leftover radiation from the big bang&lt;/a&gt; (known as the cosmic microwave background)! But somebody over at the European Southern Observatory put these two together and made &lt;a href="http://www.eso.org/public/outreach/press-rel/pr-2008/pr-13-08.html"&gt;an incredibly tasty science sandwich&lt;/a&gt;.&lt;/p&gt;
&lt;p&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/222470571.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25277" title="222470571" src="https://scienceblogs.com/files/startswithabang/files/2008/05/222470571.jpg" alt width="221" height="98" loading="lazy"&gt;&lt;/a&gt;&lt;/p&gt;
&lt;p&gt;See, we can measure the cosmic microwave background today, because we have photons (particles of light) coming at us in all directions at all locations, with a temperature of 2.725 Kelvin. Theoretical cosmology tells us that when the Universe was younger, it was also smaller. Because the expansion of space stretches the photons in it, causing them to lose energy, it means that photons were hotter when the Universe was younger.&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;/center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/universe_expansion-sml-2.gif"&gt;&lt;img class="aligncenter size-full wp-image-25278" title="universe_expansion-sml-2" src="https://scienceblogs.com/files/startswithabang/files/2008/05/universe_expansion-sml-2.gif" alt width="336" height="336" loading="lazy"&gt;&lt;/a&gt;
&lt;p&gt;But we've never been able to measure that, of course. After all, how can you measure the temperature of something in a place where you aren't? (Hint: read the title of this post.) Use molecules as thermometers! Using a carbon monoxide molecule (CO to you chemists) in a distant galaxy, they were able to measure the temperature of the microwave background when the Universe was only about 3 billion years old! The temperature they measured was 9.15 +/- 0.70 Kelvins; and this compares pretty well with the predicted temperature of 9.315 Kelvin. Not bad! Here's an incomprehensible graph for you to look at while you take it all in:&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/phot-13b-08-preview.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25279" title="PP-53-07" src="https://scienceblogs.com/files/startswithabang/files/2008/05/phot-13b-08-preview.jpg" alt width="490" height="400" loading="lazy"&gt;&lt;/a&gt;&lt;/center&gt;What's nice about this is that, even though it's just what we expected, it rules out or constraints a lot of crazy alternatives (such as theories where the fundamental constants vary), because the temperature of the microwave background evolves according to standard theoretical predictions. Here's a link to &lt;a href="http://www.aanda.org/10.1051/0004-6361:200809727/pdf"&gt;the actual scientific paper&lt;/a&gt;, if you're into that sort of thing.
&lt;p&gt;By the way, while I've got you thinking about astronomy, NASA just announced that their X-ray satellite, Chandra, found a supernova in our own galaxy &lt;a href="http://www.universetoday.com/2008/05/14/the-big-announcement-chandra-vla-find-youngest-supernova-in-our-galaxy/"&gt;that went off in the 1800's&lt;/a&gt;, making it the most recent supernova ever to occur in our galaxy! Why'd it take so long to find? Because the whole damned galaxy was in the way: the explosion happened on the opposite side!&lt;/p&gt;
&lt;/div&gt;
      
&lt;span&gt;&lt;a title="View user profile." href="https://scienceblogs.com/startswithabang" lang about="https://scienceblogs.com/startswithabang" typeof="schema:Person" property="schema:name" datatype&gt;esiegel&lt;/a&gt;&lt;/span&gt;

&lt;span&gt;&lt;time datetime="2008-05-14T04:42:44-04:00" title="Wednesday, May 14, 2008 - 04:42"&gt;Wed, 05/14/2008 - 04:42&lt;/time&gt;
&lt;/span&gt;

  &lt;div class="field field--name-field-blog-tags field--type-entity-reference field--label-inline"&gt;
    &lt;div class="field--label"&gt;Tags&lt;/div&gt;
          &lt;div class="field--items"&gt;
              &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/big-bang" hreflang="en"&gt;Big Bang&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/astronomers" hreflang="en"&gt;astronomers&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/astronomy-0" hreflang="en"&gt;Astronomy&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/background" hreflang="en"&gt;background&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/carbon" hreflang="en"&gt;carbon&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/co" hreflang="en"&gt;CO&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/cosmic" hreflang="en"&gt;cosmic&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/eso" hreflang="en"&gt;ESO&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/european" hreflang="en"&gt;european&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/evolve" hreflang="en"&gt;evolve&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/expanding" hreflang="en"&gt;expanding&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/expansion" hreflang="en"&gt;expansion&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/graph" hreflang="en"&gt;graph&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/kelvin" hreflang="en"&gt;Kelvin&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/kelvins" hreflang="en"&gt;Kelvins&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/man" hreflang="en"&gt;man&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/microwave" hreflang="en"&gt;Microwave&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/molecular" hreflang="en"&gt;molecular&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/molecule" hreflang="en"&gt;molecule&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/moleculo" hreflang="en"&gt;moleculo&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/monoxide" hreflang="en"&gt;monoxide&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/observatories" hreflang="en"&gt;observatories&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/observatory" hreflang="en"&gt;observatory&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/scientific" hreflang="en"&gt;scientific&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/southern" hreflang="en"&gt;southern&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/temp" hreflang="en"&gt;temp&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/temperature" hreflang="en"&gt;temperature&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/theoretical" hreflang="en"&gt;theoretical&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/theory-0" hreflang="en"&gt;Theory&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/thermometer" hreflang="en"&gt;thermometer&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/universe" hreflang="en"&gt;universe&lt;/a&gt;&lt;/div&gt;
              &lt;/div&gt;
      &lt;/div&gt;


&lt;section&gt;
  
  

  
&lt;/section&gt;
&lt;ul class="links inline list-inline"&gt;&lt;li class="comment-forbidden"&gt;&lt;/li&gt;&lt;/ul&gt;</description>
  <pubDate>Thu, 06 Feb 2020 19:52:53 +0000</pubDate>
    <dc:creator>sb admin</dc:creator>
    <guid isPermaLink="false">151438 at https://scienceblogs.com</guid>
    </item>
<item>
  <title>Don't Teach Your Kids to Attack the Planet</title>
  <link>https://scienceblogs.com/seed/2017/10/17/dont-teach-your-kids-to-attack-the-planet</link>
  <description>
&lt;span&gt;Astronomers make use of… molecules?&lt;/span&gt;

            &lt;div class="field field--name-body field--type-text-with-summary field--label-hidden field--item"&gt;&lt;p&gt;When I think of molecules, I think of &lt;a href="http://www.yikers.com/video_conan_is_the_molecular_man.html"&gt;Conan O'Brien&lt;/a&gt; doing his skit where he plays Moleculo...&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;/center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/moleculo.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25276" title="moleculo" src="https://scienceblogs.com/files/startswithabang/files/2008/05/moleculo.jpg" alt width="413" height="331" loading="lazy"&gt;&lt;/a&gt;
&lt;p&gt;the molecular man! I don't think of astronomy, and I certainly don't think of the &lt;a href="http://map.gsfc.nasa.gov/universe/bb_tests_cmb.html"&gt;leftover radiation from the big bang&lt;/a&gt; (known as the cosmic microwave background)! But somebody over at the European Southern Observatory put these two together and made &lt;a href="http://www.eso.org/public/outreach/press-rel/pr-2008/pr-13-08.html"&gt;an incredibly tasty science sandwich&lt;/a&gt;.&lt;/p&gt;
&lt;p&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/222470571.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25277" title="222470571" src="https://scienceblogs.com/files/startswithabang/files/2008/05/222470571.jpg" alt width="221" height="98" loading="lazy"&gt;&lt;/a&gt;&lt;/p&gt;
&lt;p&gt;See, we can measure the cosmic microwave background today, because we have photons (particles of light) coming at us in all directions at all locations, with a temperature of 2.725 Kelvin. Theoretical cosmology tells us that when the Universe was younger, it was also smaller. Because the expansion of space stretches the photons in it, causing them to lose energy, it means that photons were hotter when the Universe was younger.&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;/center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/universe_expansion-sml-2.gif"&gt;&lt;img class="aligncenter size-full wp-image-25278" title="universe_expansion-sml-2" src="https://scienceblogs.com/files/startswithabang/files/2008/05/universe_expansion-sml-2.gif" alt width="336" height="336" loading="lazy"&gt;&lt;/a&gt;
&lt;p&gt;But we've never been able to measure that, of course. After all, how can you measure the temperature of something in a place where you aren't? (Hint: read the title of this post.) Use molecules as thermometers! Using a carbon monoxide molecule (CO to you chemists) in a distant galaxy, they were able to measure the temperature of the microwave background when the Universe was only about 3 billion years old! The temperature they measured was 9.15 +/- 0.70 Kelvins; and this compares pretty well with the predicted temperature of 9.315 Kelvin. Not bad! Here's an incomprehensible graph for you to look at while you take it all in:&lt;/p&gt;
&lt;p&gt;&lt;/p&gt;&lt;center&gt;&lt;a href="https://scienceblogs.com/files/startswithabang/files/2008/05/phot-13b-08-preview.jpg"&gt;&lt;img class="aligncenter size-full wp-image-25279" title="PP-53-07" src="https://scienceblogs.com/files/startswithabang/files/2008/05/phot-13b-08-preview.jpg" alt width="490" height="400" loading="lazy"&gt;&lt;/a&gt;&lt;/center&gt;What's nice about this is that, even though it's just what we expected, it rules out or constraints a lot of crazy alternatives (such as theories where the fundamental constants vary), because the temperature of the microwave background evolves according to standard theoretical predictions. Here's a link to &lt;a href="http://www.aanda.org/10.1051/0004-6361:200809727/pdf"&gt;the actual scientific paper&lt;/a&gt;, if you're into that sort of thing.
&lt;p&gt;By the way, while I've got you thinking about astronomy, NASA just announced that their X-ray satellite, Chandra, found a supernova in our own galaxy &lt;a href="http://www.universetoday.com/2008/05/14/the-big-announcement-chandra-vla-find-youngest-supernova-in-our-galaxy/"&gt;that went off in the 1800's&lt;/a&gt;, making it the most recent supernova ever to occur in our galaxy! Why'd it take so long to find? Because the whole damned galaxy was in the way: the explosion happened on the opposite side!&lt;/p&gt;
&lt;/div&gt;
      
&lt;span&gt;&lt;a title="View user profile." href="https://scienceblogs.com/startswithabang" lang about="https://scienceblogs.com/startswithabang" typeof="schema:Person" property="schema:name" datatype&gt;esiegel&lt;/a&gt;&lt;/span&gt;

&lt;span&gt;&lt;time datetime="2008-05-14T04:42:44-04:00" title="Wednesday, May 14, 2008 - 04:42"&gt;Wed, 05/14/2008 - 04:42&lt;/time&gt;
&lt;/span&gt;

  &lt;div class="field field--name-field-blog-tags field--type-entity-reference field--label-inline"&gt;
    &lt;div class="field--label"&gt;Tags&lt;/div&gt;
          &lt;div class="field--items"&gt;
              &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/big-bang" hreflang="en"&gt;Big Bang&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/astronomers" hreflang="en"&gt;astronomers&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/astronomy-0" hreflang="en"&gt;Astronomy&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/background" hreflang="en"&gt;background&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/carbon" hreflang="en"&gt;carbon&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/co" hreflang="en"&gt;CO&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/cosmic" hreflang="en"&gt;cosmic&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/eso" hreflang="en"&gt;ESO&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/european" hreflang="en"&gt;european&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/evolve" hreflang="en"&gt;evolve&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/expanding" hreflang="en"&gt;expanding&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/expansion" hreflang="en"&gt;expansion&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/graph" hreflang="en"&gt;graph&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/kelvin" hreflang="en"&gt;Kelvin&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/kelvins" hreflang="en"&gt;Kelvins&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/man" hreflang="en"&gt;man&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/microwave" hreflang="en"&gt;Microwave&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/molecular" hreflang="en"&gt;molecular&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/molecule" hreflang="en"&gt;molecule&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/moleculo" hreflang="en"&gt;moleculo&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/monoxide" hreflang="en"&gt;monoxide&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/observatories" hreflang="en"&gt;observatories&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/observatory" hreflang="en"&gt;observatory&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/scientific" hreflang="en"&gt;scientific&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/southern" hreflang="en"&gt;southern&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/temp" hreflang="en"&gt;temp&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/temperature" hreflang="en"&gt;temperature&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/theoretical" hreflang="en"&gt;theoretical&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/theory-0" hreflang="en"&gt;Theory&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/thermometer" hreflang="en"&gt;thermometer&lt;/a&gt;&lt;/div&gt;
          &lt;div class="field--item"&gt;&lt;a href="https://scienceblogs.com/tag/universe" hreflang="en"&gt;universe&lt;/a&gt;&lt;/div&gt;
              &lt;/div&gt;
      &lt;/div&gt;


&lt;section&gt;
  
  

  
&lt;/section&gt;
&lt;ul class="links inline list-inline"&gt;&lt;li class="comment-forbidden"&gt;&lt;/li&gt;&lt;/ul&gt;</description>
  <pubDate>Tue, 17 Oct 2017 10:43:48 +0000</pubDate>
    <dc:creator>milhayser</dc:creator>
    <guid isPermaLink="false">69288 at https://scienceblogs.com</guid>
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