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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 | Galaxies Clips</title><link>http://clipmarks.com/tags/galaxies/</link><feedUrl>http://rss.clipmarks.com/tags/galaxies/</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>High speed crash makes galaxies 'sterile'</title><link>http://clipmarks.com/clipmark/6479CC2E-59FB-4DE8-951C-116E99B91280/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/pokkets/"&gt;pokkets&lt;/a&gt;&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.abc.net.au/science/articles/2008/10/10/2387389.htm?site=science&amp;topic=latest" title="http://www.abc.net.au/science/articles/2008/10/10/2387389.htm?site=science&amp;topic=latest"&gt;www.abc.net.au&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;Larry O'Hanlon&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;P class="first"&gt;A new view of two very well-known galaxies has revealed they are connected by faint, starless filaments of hydrogen gas, which trace back to a very high-speed intergalactic collision.&lt;/P&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/pokkets/512/6E787107-8967-427F-B8C3-8ED7D3BAD753.jpg" alt="M86-NGC4438 complex" /&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;The smash-up between M86 and NGC4438 had not been suspected before, and may explain why M86, which is visible to the naked eye, is unable to give birth to new stars.&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;P&gt;"Stars and gases behave very differently in collisions," says astronomer Professor Jeffrey Kenney of &lt;A target="_blank" href="http://www.yale.edu/"&gt;Yale University&lt;/A&gt; and lead author of a paper in the November 2008 issue of &lt;A target="_blank" href="http://www.journals.uchicago.edu/toc/apj/current"&gt;&lt;EM&gt;Astrophysical Journal Letters&lt;/EM&gt;&lt;/A&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;P&gt;During galactic smash-ups stars rarely collide, since there is so much space between them. But gases do slam into gases. The faster the collision, the higher the temperature the gases reach.&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;P&gt;In the case of M86, its gases are millions of degrees in temperature and radiate x-rays. &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;P&gt;The new evidence of M86's collision may solve that mystery. What's more, the super-hot gas also probably explains why M86 is unable to produce new stars. &lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;br&gt;&lt;div style="margin-bottom: 40px;"&gt;&lt;/div&gt;</description><clipSource>http://www.abc.net.au/science/articles/2008/10/10/2387389.htm?site=science&amp;topic=latest</clipSource><pubDate>Fri, 10 Oct 2008 07:03:34 GMT</pubDate></item><item><title>High-Speed Crash Makes Hot, 'Sterile' Galaxies</title><link>http://clipmarks.com/clipmark/C38C6132-A70F-4617-9547-61560A89089D/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/invictus/"&gt;invictus&lt;/a&gt;&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://dsc.discovery.com/news/2008/10/09/galaxy-virgo-cluster.html" title="http://dsc.discovery.com/news/2008/10/09/galaxy-virgo-cluster.html"&gt;dsc.discovery.com&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://clipmarks.com/image_cache/invictus/512/D3232816-FFA2-42A8-8E78-D0FBE30F8032.jpg" alt="Telling Tendrils" /&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;STRONG&gt;Oct. 9, 2008&lt;/STRONG&gt; -- A new wider view of two very well-known galaxies has revealed a big surprise: They are connected by faint, starless filaments of hydrogen gas which trace back to a very high-speed &lt;A target="_blank" href="http://dsc.discovery.com/news/2008/04/24/galaxy-collision-hubble.html"&gt;intergalactic collision&lt;/A&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;P&gt;The &lt;A target="_blank" href="http://dsc.discovery.com/news/2007/08/08/spitzer_spa.html?category=space"&gt;smash-up between galaxies&lt;/A&gt; M86 and NGC4438 not been suspected before, and may explain why M86, which is visible to the naked eye, is unable to give birth to &lt;A target="_blank" href="http://science.howstuffworks.com/star.htm"&gt;new stars&lt;/A&gt;.&lt;/P&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/space/" rel="tag"&gt;space&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/universe/" rel="tag"&gt;universe&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/science/" rel="tag"&gt;science&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://dsc.discovery.com/news/2008/10/09/galaxy-virgo-cluster.html</clipSource><pubDate>Thu, 09 Oct 2008 20:37:46 GMT</pubDate></item><item><title>Scientists meet for alien summit</title><link>http://clipmarks.com/clipmark/702F837C-BBDE-4ACF-8D7B-D3D45792816E/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/kkcapricorn/"&gt;kkcapricorn&lt;/a&gt;&lt;br&gt;&lt;b&gt;clipper's remarks:&lt;/b&gt;  I hope they share some of their findings and information with the public &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://news.bbc.co.uk/2/hi/uk_news/scotland/edinburgh_and_east/7658797.stm" title="http://news.bbc.co.uk/2/hi/uk_news/scotland/edinburgh_and_east/7658797.stm"&gt;news.bbc.co.uk&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://clipmarks.com/image_cache/kkcapricorn/512/730DDFB3-DA69-4FC4-8144-C5071A24C839.jpg" alt="Exo-planet, which is a planet going around a star other than our Sun (Pic David Hardy)" /&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;DIV class="cap"&gt;An artists impression of the planet going around the star Vega, which the Scuba 2 instrument discovered&lt;/DIV&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;The origins of life in our galaxy and the search for alien life outside our solar system will be at the forefront of discussions by experts in Edinburgh&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; 'Are We Alone?'.
&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;There are now more than 300 planets known beyond our own Solar System.
&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;Known as exo-planets, they are likely to be discovered with the completion of instruments such as Scuba 2, a camera to detect dust from the earliest phases of the formation of galaxies and, in the near future, the James Webb Space Telescope, an orbiting telescope to catch the first light of the universe.
&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;The aim of the workshop is to gather researchers from areas including astrophysics, geophysics and biology to discuss astronomical instruments, both present and future, and laboratory based experiments studying extreme environments.
&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;key speakers in astrobiology, atmospheric physics and astrophysics&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/universe/" rel="tag"&gt;universe&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/alien+life/" rel="tag"&gt;alien life&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/summit/" rel="tag"&gt;summit&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/astrophysics/" rel="tag"&gt;astrophysics&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://news.bbc.co.uk/2/hi/uk_news/scotland/edinburgh_and_east/7658797.stm</clipSource><pubDate>Wed, 08 Oct 2008 20:07:07 GMT</pubDate></item><item><title>Galaxies found to be flowing together</title><link>http://clipmarks.com/clipmark/55B164D7-B64A-45BC-9489-275A112398CB/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/Kelika/"&gt;Kelika&lt;/a&gt;&lt;br&gt;&lt;b&gt;clipper's remarks:&lt;/b&gt;  "He said another interesting idea proposed since the cosmic flow was detected is that instead of a gravitational pull by something beyond the observable universe, the galaxies are being pushed by an absence of mass in the local universe." &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.starbulletin.com/news/20081004_galaxies_found_to_be_flowing_together.html" title="http://www.starbulletin.com/news/20081004_galaxies_found_to_be_flowing_together.html"&gt;www.starbulletin.com&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://clipmarks.com/image_cache/Kelika/512/7D205CA6-989E-4425-83FF-5C8C57439678.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;P class="storytext"&gt;Hundreds of galaxy clusters are flowing toward the same spot in the sky beyond the observable universe, a University of Hawaii astronomer and NASA team members have discovered.&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;P class="storytext"&gt;The clusters, each with hundreds of millions of stars, are moving at more than 1 million mph toward the constellations Centaurus and Vela, said Harald Ebeling, co-author of a paper on the baffling finding in the Astrophysical Journal Letters&lt;I&gt;.&lt;/I&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;P class="storytext"&gt;&lt;I&gt;&lt;/I&gt;"It's pretty bizarre," he said in an interview.&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;P class="storytext"&gt;Ebeling said the "main culprit" behind the phenomenon seems to be the Shapley Concentration, a giant supercluster made up of about 25 galactic clusters about 700 million light-years away which pulls everything toward it.&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;P class="storytext"&gt;But once the clusters reach the Shapley supercluster, he said, they do not subside or reverse -- they defy current cosmic theories and keep on going.&lt;/P&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/space/" rel="tag"&gt;space&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://www.starbulletin.com/news/20081004_galaxies_found_to_be_flowing_together.html</clipSource><pubDate>Sun, 05 Oct 2008 02:44:48 GMT</pubDate></item><item><title>Two Spiral Galaxies Collide</title><link>http://clipmarks.com/clipmark/89ADB44C-CBFC-4C0E-BF32-0210233477B6/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/tabsey/"&gt;tabsey&lt;/a&gt;&lt;br&gt;&lt;b&gt;clipper's remarks:&lt;/b&gt;  There goes the weekender. &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://news.yahoo.com/nphotos/Hubble--Spitzer-Space-Telescopes/ss/events/sc/011305nasahubble/im:/080930/photos_wl_afp/36ba75012e18a1a3d129d453d0d41bb8" title="http://news.yahoo.com/nphotos/Hubble--Spitzer-Space-Telescopes/ss/events/sc/011305nasahubble/im:/080930/photos_wl_afp/36ba75012e18a1a3d129d453d0d41bb8"&gt;news.yahoo.com&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://clipmarks.com/image_cache/tabsey/512/89DCF29B-24BA-475A-BD0C-01DEACA201D6.jpg" alt="A collision between two spiral galaxies in the constellation ..." /&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;H1&gt;Hubble &amp; Spitzer Space Telescopes&lt;/H1&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;/div&gt;</description><clipSource>http://news.yahoo.com/nphotos/Hubble--Spitzer-Space-Telescopes/ss/events/sc/011305nasahubble/im:/080930/photos_wl_afp/36ba75012e18a1a3d129d453d0d41bb8</clipSource><pubDate>Thu, 02 Oct 2008 09:23:02 GMT</pubDate></item><item><title> How A Catholic Priest Gave Us The Primeval Atom Theory</title><link>http://clipmarks.com/clipmark/F5B802A7-F5D5-44B5-9CEF-13285502F24F/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/merrie/"&gt;merrie&lt;/a&gt;&lt;br&gt;&lt;b&gt;clipper's remarks:&lt;/b&gt;  Returning to Belgium in 1925, where he worked at the Catholic University of Leuven as a part-time lecturer, his big break came two years later in 1927 when he proposed his theory of an expanding Universe to explain the movement of the galaxies, published in the Annals of the Scientific Society of Brussels.&lt;br/&gt;&lt;br/&gt;Lemaitre was still pretty hazy about how the process of expansion could have begun. Like many scientists, he was still committed to the idea of a static Universe of unchanging size...&lt;br/&gt;&lt;br/&gt;Einstein, though interested, was largely dismissive, telling Lemaitre that, "Your calculations are good, but your physics is terrible". Einstein was also a little suspicious of the religious implications of these ideas. He declined to describe himself as an atheist (or a theist, or a pantheist) and liked to use the vocabulary of religion, most famously in his misguided rejection of much of quantum physics, "God does not play dice!"&lt;br/&gt;&lt;br/&gt;British physicist, Fred Hoyle coined the Big Bang term &lt;br&gt;&lt;div border="2" style="margin-top: 10px; border:#000000 1px solid;" width="90%"&gt;&lt;div style="background-color:#e5e5e5"&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.americanchronicle.com/articles/47354" title="http://www.americanchronicle.com/articles/47354"&gt;www.americanchronicle.com&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;In addition to discovering these galaxies, Hubble also discovered something significant about them. Just as the pitch of a siren on an emergency vehicle changes as it drives past us - because the length of the sound waves change as they become more distant according to the Doppler effect - so too the light from distant objects can tell us whether they are moving closer or drifting away. &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;Together with Milton L. Humason, Hubble showed that the galaxies were moving further away from us&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;DIV&gt;
But, unknown to either of them, Hubble was actually beaten to the basic idea of Hubble’s Law by a Belgian priest, Fr. Georges Lemaitre. Lemaitre trained as a Jesuit priest, served in the Belgian Army during the remorseless slaughter of World War One, and then became a student of astronomy and mathematics. He studied in Cambridge in England, then in Cambridge, Massachusetts for the Harvard Observatory and finally the Massachusetts Institute of Technology.&lt;/DIV&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/hubble/" rel="tag"&gt;hubble&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/einstein/" rel="tag"&gt;einstein&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/hoyle/" rel="tag"&gt;hoyle&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/fr.+georges+lemaitre/" rel="tag"&gt;fr. georges lemaitre&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/hawkings/" rel="tag"&gt;hawkings&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://www.americanchronicle.com/articles/47354</clipSource><pubDate>Mon, 29 Sep 2008 09:37:13 GMT</pubDate></item><item><title>Giant Red Stars set a new Standard</title><link>http://clipmarks.com/clipmark/43067C98-16DC-4D82-8670-7AADD13B3E90/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/pokkets/"&gt;pokkets&lt;/a&gt;&lt;br&gt;&lt;b&gt;clipper's remarks:&lt;/b&gt;  The most common red giants are the so-called red giant branch stars (RGB stars) whose shells are still fusing hydrogen into helium, while the core is inactive helium.&lt;br/&gt;Prominent bright red giants in the night sky include Aldebaran (Alpha Tauri), Arcturus (Alpha Bootis), and Gamma Crucis (Gacrux), while the even larger Antares (Alpha Scorpii) and Betelgeuse (Alpha Orionis) are red supergiants. &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.abc.net.au/science/articles/2008/09/25/2374351.htm?site=science&amp;topic=latest" title="http://www.abc.net.au/science/articles/2008/09/25/2374351.htm?site=science&amp;topic=latest"&gt;www.abc.net.au&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;A href="http://www.abc.net.au/profiles/content/s2110135.htm?site=science"&gt;Heather Catchpole&lt;/A&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;P class="first"&gt;Australian and US scientists have found that a 'secondary' method of measuring the distance to nearby galaxies is more robust than previously thought. &lt;/P&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/pokkets/512/E47BC3E8-046A-4DA3-9D1A-9BB8E2FB9CB0.jpg" alt="barred 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;Astrophysicists Professor Jeremy Mould from the &lt;A target="_blank" href="http://www.unimelb.edu.au/"&gt;University of Melbourne&lt;/A&gt; and Dr Shoko Sakai from the &lt;A target="_blank" href="http://www.ucla.edu/"&gt;University of California, Los Angeles&lt;/A&gt;, tested the reliability of using stars from the tip of the red giant branch (TRGB) to calculate distance. They found these stars to be just as good, if not better than Cepheids.&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;P&gt;Their research has been accepted for publication in the &lt;A target="_blank" href="http://www.journals.uchicago.edu/toc/apj/current"&gt;&lt;EM&gt;Astrophysical Journal&lt;/EM&gt;&lt;/A&gt;.&lt;/P&gt;&lt;/div&gt;&lt;/div&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://en.wikipedia.org/w/index.php?title=Red_giant&amp;oldid=240175536" title="http://en.wikipedia.org/w/index.php?title=Red_giant&amp;oldid=240175536"&gt;en.wikipedia.org&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://clipmarks.com/image_cache/pokkets/512/5D5DB629-9DEA-4CEB-9752-CFD197352F3D.png" alt="" /&gt;&lt;br /&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/pokkets/512/7C69FF54-1F27-4E1B-8890-99746B6E2CE6.png" alt="The size of the current Sun (now in the main sequence) compared to its estimated size during its red giant phase." /&gt;&lt;br /&gt;&lt;/div&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.abc.net.au/science/articles/2008/09/25/2374351.htm?site=science&amp;topic=latest" title="http://www.abc.net.au/science/articles/2008/09/25/2374351.htm?site=science&amp;topic=latest"&gt;www.abc.net.au&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;Astronomers measure distance in space using various methods depending on how far away the stars are. &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;P&gt;For nearby distances, Cepheid variables - bright stars that expand and contract by 10% - have long been the primary 'standard candles' used. &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;P&gt;"The question has been whether the relationship is more complicated than we think. Things like the composition of the star may make a difference," says Mould.&lt;/P&gt;&lt;/div&gt;&lt;/div&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://en.wikipedia.org/w/index.php?title=Red_giant&amp;oldid=240175536" title="http://en.wikipedia.org/w/index.php?title=Red_giant&amp;oldid=240175536"&gt;en.wikipedia.org&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;include &lt;A title="Aldebaran" href="http://en.wikipedia.org/wiki/Aldebaran"&gt;Aldebaran&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;&lt;/div&gt;</description><clipSource>http://www.abc.net.au/science/articles/2008/09/25/2374351.htm?site=science&amp;topic=latest</clipSource><pubDate>Fri, 26 Sep 2008 06:03:17 GMT</pubDate></item><item><title>Stars Migrate Through Galaxies, Study Suggests </title><link>http://clipmarks.com/clipmark/9D843598-05BB-433C-9CEB-10EFC513F781/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/dannyhurt28/"&gt;dannyhurt28&lt;/a&gt;&lt;br&gt;&lt;b&gt;clipper's remarks:&lt;/b&gt;  About half the stars in our celestial neighborhood may have traveled great distances through the Milky Way, according to a new study, which suggests our sun may be one of them.  &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://news.nationalgeographic.com/news/2008/09/080918-star-migration.html" title="http://news.nationalgeographic.com/news/2008/09/080918-star-migration.html"&gt;news.nationalgeographic.com&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;H1 class="newsTitle"&gt;Stars Migrate Through Galaxies, Study Suggests &lt;/H1&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;P class="intro"&gt;
									
									
About half the &lt;A href="http://science.nationalgeographic.com/science/space/universe/stars-article.html"&gt;stars&lt;/A&gt; in our celestial neighborhood may have traveled great distances through the Milky Way, according to a new study, which suggests our &lt;A href="http://science.nationalgeographic.com/science/space/solar-system/sun-article.html"&gt;sun&lt;/A&gt; may be one of them. 

&lt;/P&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/dannyhurt28/512/0C4D1472-2D63-4DF4-9E80-7DC8ECEDBFC1.jpg" alt="PHOTO: Hurricane Ike Damage" /&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;

People have generally assumed that once a star forms inside a galactic disk, it stays in a more or less fixed orbit around the center of its &lt;A href="http://science.nationalgeographic.com/science/space/universe/galaxies-article.html"&gt;galaxy&lt;/A&gt;, said lead study author Rok Roškar, a graduate student in astronomy at the University of Washington in Seattle. 
								&lt;/P&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/stars+migrate/" rel="tag"&gt;stars migrate&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://news.nationalgeographic.com/news/2008/09/080918-star-migration.html</clipSource><pubDate>Thu, 25 Sep 2008 15:04:23 GMT</pubDate></item><item><title>Is a Dark-Matter Galaxy Orbiting the Milky Way?</title><link>http://clipmarks.com/clipmark/B6941E24-255B-4467-9C3F-03A0CAD2EF97/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/tabsey/"&gt;tabsey&lt;/a&gt;&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.dailygalaxy.com/my_weblog/2008/09/is-a-dark-matte.html" title="http://www.dailygalaxy.com/my_weblog/2008/09/is-a-dark-matte.html"&gt;www.dailygalaxy.com&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://clipmarks.com/image_cache/tabsey/512/188ECD54-83A6-443F-8D39-31A1BB853C2C.gif" alt="M104" /&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;We now know about two dozen of these satellite galaxies.  One of the
most recent is "Segue 1", uncovered by the Sloan Digital Sky Survey
(SDSS), whose extremely low light-to-mass ratio makes it a particularly
significant cosmic find.  Despite having a mass of a million suns it is
nowhere near as luminous as astronomers would expect, with only a
couple of hundred stars visible.  They think "How can so much matter be
so dark?", then they go "Dark matter!" and at this point we like to
believe their monocle flies out and they dash down the street shouting
Eureka.&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;P&gt;
Of course, the actual physics of arriving at this conclusion is a tiny
bit more complicated, but the result is the same: Marla Geha (Yale
professor of astronomy) and colleagues believe that it's a galaxy
composed mainly of dark matter.  A handy thing to have around when
you're trying to study the stuff or even prove that it exists. &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;These mini-galaxies and other
previously unobservable objects offer a wealth of data on galaxy
formation&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;/div&gt;</description><clipSource>http://www.dailygalaxy.com/my_weblog/2008/09/is-a-dark-matte.html</clipSource><pubDate>Thu, 25 Sep 2008 12:33:01 GMT</pubDate></item><item><title>IS THERE INTELLIGENT LIFE- OUT THERE?</title><link>http://clipmarks.com/clipmark/6E5888F1-BDF3-4397-B9CE-AB1BFF783AC6/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/klippety/"&gt;klippety&lt;/a&gt;&lt;br&gt;&lt;b&gt;clipper's remarks:&lt;/b&gt;  'Cause there doesn't seem to be any here. We can only hope....... &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.sciam.com/gallery_directory.cfm?photo_id=E151952B-E214-2082-C35253ACF156A155" title="http://www.sciam.com/gallery_directory.cfm?photo_id=E151952B-E214-2082-C35253ACF156A155"&gt;www.sciam.com&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;H1&gt;Rivers of Stars Found in Milky Way&lt;/H1&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/klippety/512/29487854-D3E2-4B7C-9531-D553ECE29E7C.jpg" alt="Slideshow" /&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;B&gt;RIVERS RUN THROUGH IT: &lt;/B&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;P&gt;Astronomers have discovered nearly a dozen new &lt;A href="http://www.sciam.com/article.cfm?id=our-growing-breathing-gal-2004-01"&gt;stellar rivers&lt;/A&gt;—strings of moving stars—over the disk of the Milky Way. The streams, which seem to represent smaller &lt;A href="http://www.sciam.com/article.cfm?id=what-defines-a-galaxy"&gt;galaxies&lt;/A&gt; torn apart by our own, come from scans of the velocities of about a quarter million stars in our galaxy made for the &lt;A href="http://www.sciam.com/article.cfm?id=reading-the-blueprints-of"&gt;Sloan Digital Sky Survey&lt;/A&gt;. Prior scans had turned up a few narrow rivers such as one extending from the star cluster NGC 5466, 76,000 light-years away, that covers 45 degrees across the northern sky. The 11 new entries form a tangle that's harder to separate. Researchers believe that the streams arose separately when neighboring star clusters known as &lt;A href="http://www.sciam.com/article.cfm?id=big-galaxies-may-have-sto"&gt;dwarf galaxies&lt;/A&gt; were drawn apart like taffy by the Milky Way's larger gravitational field. They say the new findings, &lt;A href="http://www.sdss.org/news/releases/20080816.segue_final.html"&gt;reported&lt;/A&gt; at a conference this week, could be used to improve models of galaxies colliding with and cannibalizing one another.&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;br&gt;&lt;div style="margin-bottom: 40px;"&gt;&lt;/div&gt;</description><clipSource>http://www.sciam.com/gallery_directory.cfm?photo_id=E151952B-E214-2082-C35253ACF156A155</clipSource><pubDate>Thu, 25 Sep 2008 04:46:10 GMT</pubDate></item><item><title>Is a Dark-Matter Galaxy Orbiting the Milky Way?</title><link>http://clipmarks.com/clipmark/C79299A4-6638-45F6-B23D-D2FF7ECF0013/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/spherepet/"&gt;spherepet&lt;/a&gt;&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.dailygalaxy.com/my_weblog/2008/09/is-a-dark-matte.html" title="http://www.dailygalaxy.com/my_weblog/2008/09/is-a-dark-matte.html"&gt;www.dailygalaxy.com&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;H3 class="entry-header"&gt;&lt;A href="http://www.dailygalaxy.com/my_weblog/2008/09/is-a-dark-matte.html"&gt;Is a Dark-Matter Galaxy Orbiting the Milky Way?&lt;/A&gt;&lt;/H3&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;H2 class="date-header"&gt;September 23, 2008&lt;/H2&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/spherepet/512/4F52F0FA-3F7A-4FA6-BA76-43DC2A7F3EA3.gif" alt="M104" /&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;We now know about two dozen of these satellite galaxies.  One of the
most recent is "Segue 1", uncovered by the Sloan Digital Sky Survey
(SDSS), whose extremely low light-to-mass ratio makes it a particularly
significant cosmic find.  Despite having a mass of a million suns it is
nowhere near as luminous as astronomers would expect, with only a
couple of hundred stars visible.  They think "How can so much matter be
so dark?", then they go "Dark matter!"&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;P&gt;
Of course, the actual physics of arriving at this conclusion is a tiny
bit more complicated, but the result is the same: Marla Geha (Yale
professor of astronomy) and colleagues believe that it's a galaxy
composed mainly of dark matter.  A handy thing to have around when
you're trying to study the stuff or even prove that it exists. &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;The SDSS has made many such observations possible, picking out objects
in the sky which have the bad manners not to twinkle&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;despite being little stars&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/galaxy/" rel="tag"&gt;galaxy&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/milkyway/" rel="tag"&gt;milkyway&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://www.dailygalaxy.com/my_weblog/2008/09/is-a-dark-matte.html</clipSource><pubDate>Wed, 24 Sep 2008 22:57:37 GMT</pubDate></item><item><title>Galaxy Clusters Have a Mysterious Motion</title><link>http://clipmarks.com/clipmark/3AA087C8-12D8-400D-A89E-F7B9F5179E9A/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/spherepet/"&gt;spherepet&lt;/a&gt;&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.physorg.com/news141489744.html" title="http://www.physorg.com/news141489744.html"&gt;www.physorg.com&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;H1&gt;Galaxy Clusters Have a Mysterious Motion&lt;/H1&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;A href="http://archive.physorg.com/24/09/2008"&gt;September 24, 2008&lt;/A&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;DIV id="Preview"&gt; 
(PhysOrg.com) -- The stars are in motion, and on a much larger scale than can be explained with current theories, according to astronomers at NASA, the University of Hawaii and UC Davis. The finding could improve our understanding of events in the first moments after the birth of the universe.&lt;BR /&gt;&lt;/DIV&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;DIV&gt;Local flows of galaxies and galaxy clusters are well-known, said Dale Kocevski, a postdoctoral researcher at UC Davis who was part of the team. For instance, our own Milky Way galaxy is moving toward the Andromeda galaxy, and the galaxy group that includes both Andromeda and the Milky Way is moving at about 600 kilometers a second.
&lt;/DIV&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; newly detected motion is over far too large an area to be explained&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;matter -- both stars, dust and gas and the more abundant but invisible "dark matter" -- is distributed in uneven clumps, and gravity pulls galaxy clusters toward those clumps&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;anisotropies&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;catalog of 700 galaxy clusters observed with X-ray astronomy&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/galaxy+clusters/" rel="tag"&gt;galaxy clusters&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/anisotropies/" rel="tag"&gt;anisotropies&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://www.physorg.com/news141489744.html</clipSource><pubDate>Wed, 24 Sep 2008 22:42:55 GMT</pubDate></item><item><title>Mysterious New 'Dark Flow' Discovered in Space</title><link>http://clipmarks.com/clipmark/8EAB1EF7-F4A9-4C76-91EB-AE25ED3BF71B/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/mugofcoffee/"&gt;mugofcoffee&lt;/a&gt;&lt;br&gt;&lt;b&gt;clipper's remarks:&lt;/b&gt;  They discovered that the clusters were moving nearly 2 million mph (3.2 million kph) toward a region in the sky between the constellations of Centaurus and Vela. This motion is different from the outward expansion of the universe (which is accelerated by the force called dark energy). &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.livescience.com/space/080923-dark-flows.html" title="http://www.livescience.com/space/080923-dark-flows.html"&gt;www.livescience.com&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;By &lt;A href="http://www.livescience.com/php/contactus/author.php?r=cm"&gt;Clara Moskowitz&lt;/A&gt;, Staff Writer&lt;/P&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/mugofcoffee/512/295B6A69-CE94-4766-8348-202DC5A9EFCD.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;DIV id="ri_caption"&gt;The galaxy cluster 1E 0657-56 (known as the Bullet Cluster) lies 3.8 billion light-years away. It's one of hundreds that appear to be carried along by a mysterious cosmic flow. Credit: NASA/STScI/Magellan/U.Arizona/D.Clowe et al.&lt;/DIV&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;P class="MsoNormal"&gt;Patches of matter in the universe seem to be moving at very
high speeds and in a uniform direction that can't be explained by any of the
known gravitational forces in the observable universe. Astronomers are calling
the phenomenon "dark flow."&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;P class="MsoNormal"&gt;The stuff that's pulling this matter must be &lt;I&gt;outside&lt;/I&gt;
the observable universe, researchers conclude.&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;discovered the flow by studying some of the
largest structures in the cosmos: &lt;A href="http://www.space.com/php/multimedia/imagedisplay/img_display.php?pic=080923-galaxy-cluster-02.jpg&amp;cap=The+galaxy+cluster+1E+0657-56+(known+as+the+Bullet+Cluster)+lies+3.8+billion+light-years+away.+It%27s+one+of+hundreds+that+appear+to+be+carried+along+by+a+mysterious+cosmic+flow.+Credit:+NASA%2FSTScI%2FMagellan%2FU.Arizona%2FD.Clowe+et+al."&gt;giant
clusters&lt;/A&gt; of galaxies. These clusters are conglomerations of about a
thousand galaxies, as well as very hot gas which emits X-rays. By observing the
interaction of the X-rays with the cosmic microwave background (CMB), which is
leftover radiation from the Big Bang&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;br&gt;&lt;div style="margin-bottom: 40px;"&gt;&lt;/div&gt;</description><clipSource>http://www.livescience.com/space/080923-dark-flows.html</clipSource><pubDate>Tue, 23 Sep 2008 20:58:11 GMT</pubDate></item><item><title>StarCAVE</title><link>http://clipmarks.com/clipmark/27686C99-34BD-4EF3-AFFD-2DE50464A05D/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/balthazarus/"&gt;balthazarus&lt;/a&gt;&lt;br&gt;&lt;b&gt;clipper's remarks:&lt;/b&gt;  Looks like an amazing experience... &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://gizmodo.com/5052552/ucsds-starcave-is-a-real-3d-super+high+def-danger-room" title="http://gizmodo.com/5052552/ucsds-starcave-is-a-real-3d-super+high+def-danger-room"&gt;gizmodo.com&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;A 
href="http://gizmodo.com/5052552/ucsds-starcave-is-a-real-3d-super+high+def-danger-room"&gt;UCSD's 
StarCAVE Is a Real 3D Super-High-Def Danger Room&lt;/A&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/balthazarus/512/08CCBED8-9965-4DFB-BDFF-84B8418163EE.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;UC at San Diego has the closest thing to an X-Men-style Danger Room in its new 
StarCAVE, a small room that entirely surrounds you, hurtling 68 million pixels 
at your eyeballs at near-perfect resolution&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;Pop on polarized glasses and the whole thing goes 3D. Grasping a wireless 
"wand," you can walk through tall buildings, fly over cities, pick apart tiny 
cell structures or embrace entire galaxies. All the while pretending to do 
actual academic research, of course&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/balthazarus/512/6F2F7BF6-6CF1-4820-9EDC-4E8986299CBE.jpg" alt="UCSD StarCAVE - Archaeology" /&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;The room—the third and by far best generation of the "Cave Automated Virtual 
Environment"&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;each panel gets its own serious processing muscle: a quad-core Linux-based PC 
with dual Nvidia GPUs and gigabit ethernet (in some cases 10-gigabit)&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;P&gt;Lest you were worried about an appropriately complementary sound system, fear not. There are three five-speaker arrays hidden behind the panels for all kinds of surround-sound configurations, and there's a subwoofer built into the floor, too.&lt;/P&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/balthazarus/512/BA0779E5-9C4C-4E3D-98AF-0233A23B988D.jpg" alt="UCSD StarCAVE - Structural Engineering" /&gt;&lt;br /&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/balthazarus/512/7008DE2E-30EB-46C1-89C6-DB5FF24EAEF8.jpg" alt="UCSD StarCAVE - Biology 2" /&gt;&lt;br /&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/balthazarus/512/3C436647-2C7F-49D3-965E-5481B6CA6FBB.jpg" alt="UCSD StarCAVE - Biology 1" /&gt;&lt;br /&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/balthazarus/512/CC57D8EB-0897-4A8A-95D2-6E20D84C99CD.jpg" alt="UCSD StarCAVE - Architecture 2" /&gt;&lt;br /&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/technology/" rel="tag"&gt;technology&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/3d/" rel="tag"&gt;3d&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://gizmodo.com/5052552/ucsds-starcave-is-a-real-3d-super+high+def-danger-room</clipSource><pubDate>Mon, 22 Sep 2008 10:23:25 GMT</pubDate></item><item><title>Milky Way ringed by 'missing galaxies'</title><link>http://clipmarks.com/clipmark/8F2390C2-4415-4CEE-98BB-3CBDF09BF6B7/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/invictus/"&gt;invictus&lt;/a&gt;&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.cosmosmagazine.com/news/2201/milky-way-ringed-missing-galaxies" title="http://www.cosmosmagazine.com/news/2201/milky-way-ringed-missing-galaxies"&gt;www.cosmosmagazine.com&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://clipmarks.com/image_cache/invictus/512/4CAB4C08-8772-43ED-B17E-9F17851AC3E7.jpg" alt="Leo II dwarf spheroidal 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;SYDNEY: The Milky Way could be surrounded by up to 2,000 small galaxies, too faint to be seen with current technology, say astrophysicists.&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;P&gt;Their research has implications for understanding how galaxies form and the nature of dark matter – the invisible matter that pervades and surrounds all galaxies, including our own.&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;P&gt;Astronomers know of 24 satellite galaxies of the Milky Way, including the two bright Magellanic Clouds, which on dark nights are visible just to the side of the wide band of the Milky Way.&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;P&gt;But the U.S. researchers, led by astrophysicist Erik Tollerud from the University of California, Irvine, say there are at least 400 and as many as 2,000 more satellite galaxies – we just haven't spotted them yet because they are so faint.&lt;/P&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/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/astronomy/" rel="tag"&gt;astronomy&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/science/" rel="tag"&gt;science&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://www.cosmosmagazine.com/news/2201/milky-way-ringed-missing-galaxies</clipSource><pubDate>Sat, 20 Sep 2008 19:06:46 GMT</pubDate></item></channel></rss>