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<?xml-stylesheet href="/style/rss/rss_feed.xsl" type="text/xsl" media="screen"?><?xml-stylesheet href="/style/rss/rss_feed.css" type="text/css" media="screen" ?><rss version="2.0"><channel><title>Clipmarks | ruralart's clips</title><link>http://clipmarks.com/clipper/ruralart/date/2008/5/4/</link><feedUrl>http://rss.clipmarks.com/clipper/ruralart/date/2008/5/4/</feedUrl><ttl>15</ttl><description>Clip, tag and save information that's important to you. Bookmarks save entire pages...Clipmarks save the specific content that matters to you!</description><language>en-us</language><item><title>Milky Way, the Universe, Galaxies and the development of theories</title><link>http://clipmarks.com/clipmark/D4D6FADF-E976-41C8-A337-528E3B2B4771/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/ruralart/"&gt;ruralart&lt;/a&gt;&lt;br&gt;&lt;b&gt;clipper's remarks:&lt;/b&gt;  A bit on the history of discovery of galaxies and the Milky Way... rather interesting to see how it has evolved. &lt;br&gt;&lt;div border="2" style="margin-top: 10px; border:#000000 1px solid;" width="90%"&gt;&lt;div style="background-color:"&gt;&lt;div align="center" width="100%" style="padding:4px;margin-bottom:4px;background-color:#666666;overflow:hidden;"&gt;&lt;span style="color:#FFFFFF;font-weight:bold;"&gt;Clip Source: &lt;a style="color:#FFFFFF;" href="http://ircamera.as.arizona.edu/NatSci102/NatSci102/lectures/galaxies.htm" title="http://ircamera.as.arizona.edu/NatSci102/NatSci102/lectures/galaxies.htm"&gt;ircamera.as.arizona.edu&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;table background="undefined" bgcolor=""&gt;&lt;tr&gt;&lt;TD width="67%"&gt;&lt;BIG&gt;&lt;BIG&gt;&lt;STRONG&gt;Discovery of Galaxies&lt;/STRONG&gt;&lt;/BIG&gt;&lt;/BIG&gt;&lt;P&gt;&lt;FONT color="#008000"&gt;&lt;EM&gt;&lt;BIG&gt;&lt;BIG&gt;&lt;STRONG&gt;Key points: How it was established that other
    galaxies are island universes of stars; standard candles and distances; the distance
    ladder&lt;/STRONG&gt;&lt;/BIG&gt;&lt;/BIG&gt;&lt;/EM&gt;&lt;/FONT&gt;&lt;/P&gt;
    &lt;P&gt; &lt;/P&gt;
    &lt;P&gt;&lt;BIG&gt;While the Milky Way was considered to be a thin, distorted disk of stars with the
    sun near the center in the early 20th century, other galaxies were confused with gaseous
    nebulae, and were assumed to be part of Milky Way. &lt;/BIG&gt;&lt;/P&gt;
    &lt;P&gt;&lt;FONT size="4" color="#000000"&gt;The best pictures showed other galaxies to have spiral
    arms, but they also appeared smooth and were thought to be a special kind of gaseous
    nebulae, the "spiral nebulae".&lt;/FONT&gt;&lt;/P&gt;
    &lt;P&gt; &lt;/P&gt;
    &lt;P&gt; &lt;/P&gt;
    &lt;P&gt; &lt;/P&gt;
    &lt;P&gt; &lt;/P&gt;&lt;/TD&gt;&lt;/tr&gt;&lt;/table&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://clipmarks.com/image_cache/ruralart/512/BE9AD319-8483-4836-91D0-BED7540EFA3F.gif" alt="picture of spiral galaxy" /&gt;&lt;br /&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;&lt;FONT color="#000000"&gt;&lt;BIG&gt;By the 1920s, a debate was ranging among astronomers about
whether the spiral nebulae were gaseous objects (HII regions) or separate "island
universes" like the Milky Way.&lt;/BIG&gt;&lt;/FONT&gt;&lt;FONT size="5" color="#ff0000"&gt;&lt;STRONG&gt;&lt;SPAN&gt; &lt;/SPAN&gt;&lt;/STRONG&gt;&lt;/FONT&gt;&lt;BIG&gt;Vesto Slipher had obtained &lt;FONT color="#000000"&gt;spectra that showed them to have continuous spectra, not emission lines,
consistent with their being made of stars. &lt;/FONT&gt;&lt;/BIG&gt;&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;BIG&gt;More on the debate at&lt;/BIG&gt;&lt;SPAN&gt; &lt;/SPAN&gt;&lt;A href="http://antwrp.gsfc.nasa.gov/diamond_jubilee/debate_1920.html"&gt;http://antwrp.gsfc.nasa.gov/diamond_jubilee/debate_1920.html&lt;/A&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;br&gt;&lt;div style="margin-bottom: 40px;"&gt;Tags: &lt;a href="http://clipmarks.com/tags/astronomy/" rel="tag"&gt;astronomy&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/galaxies/" rel="tag"&gt;galaxies&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/milky+way/" rel="tag"&gt;milky way&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/history/" rel="tag"&gt;history&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/science/" rel="tag"&gt;science&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/space/" rel="tag"&gt;space&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://ircamera.as.arizona.edu/NatSci102/NatSci102/lectures/galaxies.htm</clipSource><pubDate>Mon, 05 May 2008 02:17:02 GMT</pubDate></item><item><title>Losing the Dark</title><link>http://clipmarks.com/clipmark/D1AECE81-44F6-4BCD-B78D-96CF476F6DFE/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/ruralart/"&gt;ruralart&lt;/a&gt;&lt;br&gt;&lt;b&gt;clipper's remarks:&lt;/b&gt;  Maps showing the loss of dark over the last 50 years or so. &lt;br&gt;&lt;div border="2" style="margin-top: 10px; border:#000000 1px solid;" width="90%"&gt;&lt;div style="background-color:"&gt;&lt;div align="center" width="100%" style="padding:4px;margin-bottom:4px;background-color:#666666;overflow:hidden;"&gt;&lt;span style="color:#FFFFFF;font-weight:bold;"&gt;Clip Source: &lt;a style="color:#FFFFFF;" href="http://www.yosemite.org/naturenotes/NALightPollution.htm" title="http://www.yosemite.org/naturenotes/NALightPollution.htm"&gt;www.yosemite.org&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;STRONG&gt;Growth of Light Pollution in North America&lt;/STRONG&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://clipmarks.com/image_cache/ruralart/512/604BC789-033D-45ED-BA6D-A663B61EEBE3.jpg" alt="" /&gt;&lt;br /&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;FONT size="2" face="Verdana, Arial, Helvetica, sans-serif"&gt;The maps
          show artificial night sky brightness and are based on upward light
          measured by the Defense Meteorological Satellite Program after accounting
          for propagation and scattering of that light in the atmosphere. &lt;/FONT&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;FONT size="2" face="Verdana, Arial, Helvetica, sans-serif"&gt;The night
          sky in all areas here which are not black (but have other colors) is
          considered polluted. Today, two thirds of the USA's population have
          lost naked eye visibility of the Milky Way.&lt;/FONT&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;FONT size="2" face="Verdana, Arial, Helvetica, sans-serif"&gt;The colors
          indicate the artificial night sky brightness as a fraction of the average
          natural night sky brightness.&lt;/FONT&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;br&gt;&lt;div style="margin-bottom: 40px;"&gt;Tags: &lt;a href="http://clipmarks.com/tags/astronomy/" rel="tag"&gt;astronomy&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/night/" rel="tag"&gt;night&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/dark/" rel="tag"&gt;dark&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/sky/" rel="tag"&gt;sky&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/lights/" rel="tag"&gt;lights&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://www.yosemite.org/naturenotes/NALightPollution.htm</clipSource><pubDate>Sun, 04 May 2008 22:35:56 GMT</pubDate></item></channel></rss>