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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 | tabsey's 'astronomy' clips</title><link>http://clipmarks.com/clipper/tabsey/tag/astronomy/</link><feedUrl>http://rss.clipmarks.com/clipper/tabsey/tag/astronomy/</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>Solar System Dented, Not Round</title><link>http://clipmarks.com/clipmark/B1B1131F-D39F-4BA7-8F4F-600652587442/</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;  The "bottom" of the egg is flattened by a permanent clash of particles, as the outbound solar wind smashes into atomic debris hurtling in from interstellar space, the scientists theorize.&lt;br/&gt;Voyager 2 also crossed the "termination shock" several times within the space of a single day, showing that the boundary is in perpetual flux, like the ebb-and-flow of a tide. &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/2008/07/02/dented-solar-system.html" title="http://dsc.discovery.com/news/2008/07/02/dented-solar-system.html"&gt;dsc.discovery.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;&lt;STRONG&gt;July 2, 2008&lt;/STRONG&gt; -- Millions of textbooks depicting our &lt;A target="_blank" href="http://dsc.discovery.com/news/2007/05/11/solarsystem_spa.html"&gt;solar system&lt;/A&gt; as spherical have got it all wrong, according to studies of data sent back from deep space by NASA's venerable probe, Voyager 2. &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 sun's zone of influence -- called the &lt;A target="_blank" href="http://dsc.discovery.com/news/2008/06/13/ulysses-space-probe.html"&gt;heliosphere&lt;/A&gt; -- turns out to be seriously asymmetrical, not round, they say.&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;Launched in 1977 on a historic trek of the outer planets, Voyager 2 has now crossed the turbulent boundary, known as the "termination shock," where the heliosphere yields to interstellar space.&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;Its twin probe Voyager 1, crossed the same threshold four years earlier at a different spot some one billion miles farther from the sun.&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;This difference proves that the heliosphere is not even close to perfectly round, but is oblong, like an egg, according to the studies, released by the British journal &lt;EM&gt;Nature&lt;/EM&gt; on Wednesday.&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/astronomy/" rel="tag"&gt;astronomy&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/is/" rel="tag"&gt;is&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/for/" rel="tag"&gt;for&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/stars/" rel="tag"&gt;stars&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://dsc.discovery.com/news/2008/07/02/dented-solar-system.html</clipSource><pubDate>Fri, 04 Jul 2008 14:07:16 GMT</pubDate></item><item><title>Strange Ring Found Circling Dead Star</title><link>http://clipmarks.com/clipmark/34B9AAE9-A39F-4F25-9E4D-4D3EB465B19E/</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;  Recommend this article to astronomy tragics. &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://science.nasa.gov/headlines/y2008/29may_magnetar.htm" title="http://science.nasa.gov/headlines/y2008/29may_magnetar.htm"&gt;science.nasa.gov&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;FONT face="Verdana, Arial, Helvetica, sans-serif" size="2"&gt;&lt;STRONG&gt;May 
                    29, 2008:&lt;/STRONG&gt; NASA's Spitzer Space Telescope has found 
                    a bizarre ring of material around the magnetic remains of 
                    a star that blasted itself to smithereens.&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 face="Verdana, Arial, Helvetica, sans-serif" size="2"&gt;The 
                    stellar corpse, called SGR 1900+14, belongs to a class of 
                    objects known as magnetars. These are the cores of massive 
                    stars that blew up in supernova explosions, but unlike most 
                    other dead stars, they have tremendously strong magnetic fields.&lt;/FONT&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/tabsey/512/B574C818-8C8C-4688-972D-45101FC656F0.jpg" alt="see caption" /&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="detailImageDesc"&gt;&lt;FONT face="Verdana, Arial, Helvetica, sans-serif" size="2"&gt;&lt;STRONG&gt;Above:&lt;/STRONG&gt; 
                    A ring around SGR 1900+14 observed by the infrared Spitzer 
                    Space Telescope. [&lt;A href="http://www.nasa.gov/mission_pages/spitzer/multimedia/20080528.html"&gt;more&lt;/A&gt;]&lt;/FONT&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;FONT face="Verdana, Arial, Helvetica, sans-serif" size="2"&gt;&lt;STRONG&gt;Below:&lt;/STRONG&gt; 
                    A selection of rings and spheres in the Milky Way. From left 
                    to right, (1) &lt;A href="http://antwrp.gsfc.nasa.gov/apod/ap050615.html"&gt;light 
                    echoes&lt;/A&gt; from old supernova remnant Cassiopeia A, (2) &lt;A href="http://antwrp.gsfc.nasa.gov/apod/ap020223.html"&gt;a 
                    blast wave&lt;/A&gt; emerging from recent supernova 1987A, and (3) 
                    a planetary nebula named &lt;A href="http://antwrp.gsfc.nasa.gov/apod/ap070803.html"&gt;The 
                    Helix&lt;/A&gt;. The ring around SGR 1900+14 is like none of these 
                    things.&lt;/FONT&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/tabsey/512/C0ABC71E-0961-434B-BD82-7D5EB80AD35A.jpg" alt="see caption" /&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 face="Verdana, Arial, Helvetica, sans-serif" size="2"&gt;A 
                    closer analysis revealed that the ring is most likely a carved-out 
                    cavity in a dust cloud -- a phenomenon that must be somewhat 
                    rare in the universe because it had not been seen before.&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;/div&gt;</description><clipSource>http://science.nasa.gov/headlines/y2008/29may_magnetar.htm</clipSource><pubDate>Thu, 26 Jun 2008 10:40:28 GMT</pubDate></item><item><title>Global Telescope has 10x's the Resolution of the Hubble </title><link>http://clipmarks.com/clipmark/88B2AE40-08C4-4ECC-84B0-3363D1C22BC4/</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/2008/06/global-radio-te.html" title="http://www.dailygalaxy.com/my_weblog/2008/06/global-radio-te.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;P&gt;&lt;A href="http://www.dailygalaxy.com/photos/uncategorized/2008/06/18/allen_radio_telescope_array.jpg"&gt;&lt;IMG height="262" border="0" width="350" src="http://www.dailygalaxy.com/my_weblog/images/2008/06/18/allen_radio_telescope_array.jpg" title="Allen_radio_telescope_array" alt="Allen_radio_telescope_array" /&gt;&lt;/A&gt;
Astronomers at the Arecibo Observatory in Puerto Rico joined a project called
Electronic Very Long Baseline Interferometry (e-VLBI), which can make
temporary radio telescopes that rival the size of the Earth, spanning North America, South America, Europe and Africa.&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 e-VLBI's size gives it 10 times the resolution of the Hubble
Space Telescope, allowing the array to image objects - like the bright
'afterglow' formed when a high-speed jet of matter from a gamma-ray
burst slams into its surroundings, that just look like points to
individual radio telescopes, according to Chris Salter of Arecibo. Now,
with the e-VLBI, the data is sent via fiber optic cables to produce
real-time
images of celestial objects. That allows astronomers to easily plan
follow-up observations for rapidly changing phenomena, such as
supernovae.&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/astronomy/" rel="tag"&gt;astronomy&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/is/" rel="tag"&gt;is&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/out/" rel="tag"&gt;out&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/of/" rel="tag"&gt;of&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/th....................../" rel="tag"&gt;th......................&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://www.dailygalaxy.com/my_weblog/2008/06/global-radio-te.html</clipSource><pubDate>Thu, 19 Jun 2008 13:32:45 GMT</pubDate></item><item><title>Large 'Planet X' May Lurk Beyond Pluto</title><link>http://clipmarks.com/clipmark/04515E59-D425-4737-ADFA-45E0D1729F70/</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;  We have pics of galaxies millions of light years away and yet we are not sure about our solar system (let alone our ocean). &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.space.com/scienceastronomy/080618-planet-x.html" title="http://www.space.com/scienceastronomy/080618-planet-x.html"&gt;www.space.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/B3207DFD-052F-4D74-A345-96C4CD6A8694.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&gt;An icy, unknown world might lurk in the distant reaches of our solar system beyond the orbit of Pluto, according to a new computer model.&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 hidden world -- thought to be much bigger than Pluto based on the model -- could explain unusual features of the Kuiper Belt, a region of space beyond Neptune littered with icy and rocky bodies. Its existence would satisfy the long-held hopes and hypotheses for a "Planet X" envisioned by scientists and sci-fi buffs alike.&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;"Although &lt;A href="http://www.space.com/scienceastronomy/mystery_monday_041122.html"&gt;the search&lt;/A&gt; for a distant planet in the solar system is old, it is far from over," said study team member Patryk Lykawka of Kobe University in Japan.&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 model, created by Lykawka and Kobe University colleague Tadashi Mukai, is detailed in a recent issue of &lt;EM&gt;Astrophysical Journal&lt;/EM&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;If the new world is confirmed, it would not be technically a planet. Under a &lt;A href="http://www.space.com/scienceastronomy/080612-pluto-planet.html"&gt;controversial new definition&lt;/A&gt; adopted by the International Astronomical Union (IAU) last week, it would instead be the largest known "&lt;A href="http://www.space.com/scienceastronomy/080611-plutoid-planets.html"&gt;plutoid&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/astronomy/" rel="tag"&gt;astronomy&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://www.space.com/scienceastronomy/080618-planet-x.html</clipSource><pubDate>Thu, 19 Jun 2008 13:10:31 GMT</pubDate></item><item><title>Black holes have simple feeding habits</title><link>http://clipmarks.com/clipmark/DB0F204A-0F93-478D-89C0-51E48F978FBB/</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;  Not so keen on spinach. &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.eurekalert.org/pub_releases/2008-06/cxc-bhh061808.php" title="http://www.eurekalert.org/pub_releases/2008-06/cxc-bhh061808.php"&gt;www.eurekalert.org&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/BE664F69-FABC-4AAC-9B21-B6E9D8F7D588.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&gt;The biggest black holes may feed just like the smallest ones, according to data from NASA's Chandra X-ray Observatory and ground-based telescopes. This discovery supports the implication of Einstein's relativity theory that black holes of all sizes have similar properties, and will be useful for predicting the properties of a conjectured new class of black holes.&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 conclusion comes from a large observing campaign of the spiral galaxy M81, which is about 12 million light years from Earth.  In the center of M81 is a black hole that is about 70 million times more massive than the Sun, and generates energy and radiation as it pulls gas in the central region of the galaxy inwards at high speed.&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/astronomy/" rel="tag"&gt;astronomy&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://www.eurekalert.org/pub_releases/2008-06/cxc-bhh061808.php</clipSource><pubDate>Thu, 19 Jun 2008 12:38:34 GMT</pubDate></item><item><title>Space Probe Ulysses Reaches End of Odyssey</title><link>http://clipmarks.com/clipmark/F08811EB-660C-46B5-AD73-6A631E3596E8/</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;  Well earned retirement. Off on a voyage, I suppose. &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/2008/06/13/ulysses-space-probe.html" title="http://dsc.discovery.com/news/2008/06/13/ulysses-space-probe.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/tabsey/512/DD9847E3-C8CA-4A1D-B503-EB5CA2888F65.jpg" alt="Ulysses Space Probe" /&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="standardWidgetPadding"&gt;On Its Last Leg&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&gt;&lt;STRONG&gt;June 13, 2008&lt;/STRONG&gt; -- European and American scientists will bid a fond farewell on July 1 to the space probe &lt;A target="_blank" href="http://dsc.discovery.com/news/2008/02/25/ulysses-sun-mission.html"&gt;Ulysses&lt;/A&gt;, which has circled the &lt;A target="_blank" href="http://dsc.discovery.com/news/2007/04/23/sunpics_spa.html"&gt;sun&lt;/A&gt; gathering data for 17 years, almost four times its expected lifetime. &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 first major collaboration between NASA and the European Space Agency (ESA), launched in 1990, "changed forever the way we view the sun and its effect on the surrounding space," David Southwood, ESA's director of science, said in announcing the end of mission.&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;Stuffed with 10 observational instruments, the 814-pound probe is the only satellite to have circled the sun's poles.&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;Its principle objective was to explore the boundaries and impact of the sun's sphere of influence, called the &lt;A target="_blank" href="http://dsc.discovery.com/news/2007/05/11/solarsystem_spa.html?category=space&amp;guid=20070509100030"&gt;heliosphere&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;One of its many findings was that the sun's magnetic fields, thrust outward by solar wind, extends into the solar system in ways that were previously not suspected.&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/astronomy/" rel="tag"&gt;astronomy&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://dsc.discovery.com/news/2008/06/13/ulysses-space-probe.html</clipSource><pubDate>Mon, 16 Jun 2008 17:28:06 GMT</pubDate></item><item><title>NASA finds new type of comet dust mineral</title><link>http://clipmarks.com/clipmark/13669197-3B3C-4AE7-8608-3B9461A00A14/</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.astronomy.com/asy/default.aspx?c=a&amp;id=7067" title="http://www.astronomy.com/asy/default.aspx?c=a&amp;id=7067"&gt;www.astronomy.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/512/1B5155E9-6DC2-40F8-9194-77004C261E8C.jpg" alt="Comet McNaught" /&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;SPAN class="caption"&gt;Brownleeite is believed to have orginated from comet 26P/Grigg-Skjellerup. This image shows Comet McNaught. &lt;EM&gt;Paul Mayo&lt;/EM&gt; [&lt;A href="javascript:alert('This link contains javascript. Please visit the clip source to follow this link.');" target="_self"&gt;View Larger Image&lt;/A&gt;]&lt;/SPAN&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;NASA researchers and scientists from the United States, Germany and Japan have found a new mineral in material that likely came from a comet.&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;The mineral, a manganese silicide named Brownleeite, was discovered within an interplanetary dust particle, or IDP, that appears to have originated from comet 26P/Grigg-Skjellerup. The comet originally was discovered in 1902 and reappears every 5 years. The team that made the discovery is headed by Keiko Nakamura-Messenger, a space scientist at NASA's Johnson Space Center in Houston.&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;"When I saw this mineral for the first time, I immediately knew this was something no one had seen before," says Nakamura-Messenger. "But it took several more months to obtain conclusive data because these mineral grains were only 1/10,000 of an inch in size."&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/astronomy/" rel="tag"&gt;astronomy&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://www.astronomy.com/asy/default.aspx?c=a&amp;id=7067</clipSource><pubDate>Mon, 16 Jun 2008 16:11:27 GMT</pubDate></item><item><title>Ten Amazing Telescopes (2)</title><link>http://clipmarks.com/clipmark/BB7A170B-2F93-4B14-8917-BFF4A587A192/</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://science.howstuffworks.com/ten-amazing-telescopes8.htm" title="http://science.howstuffworks.com/ten-amazing-telescopes8.htm"&gt;science.howstuffworks.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="articlePageTitle"&gt;Telescope Three: Giant Magellan Telescope&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/tabsey/512/E77BA451-C4F1-430B-A04D-9161D46B4CF5.jpg" alt="A spin casting furnace creates a mold to build mirrors for the Giant Magellan Telescope." /&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;SPAN class="caption"&gt;A spin casting furnace creates a mold to build mirrors for the Giant Magellan Telescope.&lt;/SPAN&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://science.howstuffworks.com/ten-amazing-telescopes9.htm" title="http://science.howstuffworks.com/ten-amazing-telescopes9.htm"&gt;science.howstuffworks.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="articlePageTitle"&gt;Telescope Two: Thirty Meter Telescope&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&gt;The name says it all. The Thirty Meter &lt;A href="http://science.howstuffworks.com/telescope.htm"&gt;Telescope's&lt;/A&gt; massive primary mirror has 492 segments, all perfectly aligned to form a 30-meter (98-foot) &lt;A href="http://science.howstuffworks.com/light.htm"&gt;light&lt;/A&gt;-collecting surface. Each segment will be continuously computer-adjusted to maintain the correct alignment to prevent any image distortion. Its adaptive optics correct not only for atmospheric distortion but also for ground winds that can alter observational accuracy.&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/tabsey/512/9A129248-B2BC-4992-9887-AD2EF118CB66.jpg" alt="Intel co-founder Gordon Moore has helped fund the construction of the Thirty Meter Telescope." /&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;SPAN class="caption"&gt;Intel co-founder Gordon Moore has helped fund the construction of the Thirty Meter Telescope.&lt;/SPAN&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://science.howstuffworks.com/ten-amazing-telescopes10.htm" title="http://science.howstuffworks.com/ten-amazing-telescopes10.htm"&gt;science.howstuffworks.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="articlePageTitle"&gt;Telescope One: European Extremely Large Telescope&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/tabsey/512/9996ADDE-6B26-4146-9B70-8A845BFF3139.jpg" alt="An artist's rendering of the European Extremely Large Telescope." /&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;SPAN class="caption"&gt;An artist's rendering of the European Extremely Large Telescope.&lt;/SPAN&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://science.howstuffworks.com/ten-amazing-telescopes8.htm</clipSource><pubDate>Sun, 15 Jun 2008 12:14:50 GMT</pubDate></item><item><title>Ten Amazing Telescopes (1)</title><link>http://clipmarks.com/clipmark/09B23493-2091-4967-8BA3-B2F88C5BC5D4/</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;  And that they are. &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://science.howstuffworks.com/ten-amazing-telescopes1.htm" title="http://science.howstuffworks.com/ten-amazing-telescopes1.htm"&gt;science.howstuffworks.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="articlePageTitle"&gt;Telescope 10: Southern African Large Telescope&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/tabsey/512/7EA7ED61-0545-429C-91E9-97CCCF20093A.jpg" alt="SALT's large mirrors allow it to peer out at distant galactic sights." /&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;SPAN class="caption"&gt;SALT's large mirrors allow it to peer out at distant galactic sights.&lt;/SPAN&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://science.howstuffworks.com/ten-amazing-telescopes2.htm" title="http://science.howstuffworks.com/ten-amazing-telescopes2.htm"&gt;science.howstuffworks.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="articlePageTitle"&gt;Telescope Nine: Keck Observatory&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/tabsey/512/9EAC13DE-323D-4C34-BE8C-C5962793AE9B.jpg" alt="The dome shutters of Keck I and II." /&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;SPAN class="caption"&gt;The dome shutters of Keck I and II top the summit of the dormant volcano Mauna Kea in Hawaii.&lt;/SPAN&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://science.howstuffworks.com/ten-amazing-telescopes3.htm" title="http://science.howstuffworks.com/ten-amazing-telescopes3.htm"&gt;science.howstuffworks.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="articlePageTitle"&gt;Telescope Eight: Great Canary Telescope&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/tabsey/512/D418AE58-0A9D-4DE8-8CAD-CBC7F208E467.jpg" alt="The Great Canary Telescope is located in the Great Canary Islands." /&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;SPAN class="caption"&gt;The Great Canary Telescope is located in the &lt;BR /&gt;Great Canary Islands.&lt;/SPAN&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://science.howstuffworks.com/ten-amazing-telescopes4.htm" title="http://science.howstuffworks.com/ten-amazing-telescopes4.htm"&gt;science.howstuffworks.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="articlePageTitle"&gt;Telescope Seven: Very Large Telescope&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/tabsey/512/1585ACC3-206D-4594-B74A-46D50E969973.jpg" alt="The Very Large Telescope stands on the top of a leveled mountain in northern Chile." /&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;SPAN class="caption"&gt;The Very Large Telescope stands on the top of a leveled mountain in northern Chile. The area's low humidity and rainfall make it perfect for heavenly observation.&lt;/SPAN&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://science.howstuffworks.com/ten-amazing-telescopes5.htm" title="http://science.howstuffworks.com/ten-amazing-telescopes5.htm"&gt;science.howstuffworks.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="articlePageTitle"&gt;Telescope Six: Large Binocular Telescope&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/tabsey/512/2694523A-C463-4E7F-8EC8-76DD80EC193A.jpg" alt="A technician grinds an exceptionally large mirror for the Large Binocular Telescope." /&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;SPAN class="caption"&gt;A technician grinds a large mirror, constructed in a honeycombed fashion. The mirror became part of the LBT.&lt;/SPAN&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://science.howstuffworks.com/ten-amazing-telescopes6.htm" title="http://science.howstuffworks.com/ten-amazing-telescopes6.htm"&gt;science.howstuffworks.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="articlePageTitle"&gt;Telescope Five: Hubble Space Telescope&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/tabsey/512/D9723323-1A0B-47BA-B3DC-103A137ADF44.jpg" alt="The Hubble Space Telescope has provided unparalleled images of space." /&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;SPAN class="caption"&gt;The Hubble Space Telescope has provided unparalleled images of space.&lt;/SPAN&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://science.howstuffworks.com/ten-amazing-telescopes7.htm" title="http://science.howstuffworks.com/ten-amazing-telescopes7.htm"&gt;science.howstuffworks.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="articlePageTitle"&gt;Telescope Four: Chandra X-ray Observatory&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/tabsey/512/A7CA9A8B-381F-4528-B077-BC9E4254FD03.jpg" alt="The Chandra X-ray Observatory created this image of the event horizon of a super-massive black hole." /&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;SPAN class="caption"&gt;The Chandra X-ray Observatory created this image of the event horizon of a super-massive black hole. The exposure lasted two weeks.&lt;/SPAN&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://science.howstuffworks.com/ten-amazing-telescopes1.htm</clipSource><pubDate>Sun, 15 Jun 2008 12:14:45 GMT</pubDate></item><item><title>Cosmic Grim Reaper Seen For First Time</title><link>http://clipmarks.com/clipmark/51A5DDD9-2D7E-46CD-B4DC-BE0E99C7D3BD/</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;  Like, wow, man! &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.space.com/scienceastronomy/080612-star-burst.html" title="http://www.space.com/scienceastronomy/080612-star-burst.html"&gt;www.space.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/512/216BA3A5-81F5-4560-B053-D5D5EE5C8111.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;SPAN&gt;Like a
cosmic Grim Reaper, a blast of ultraviolet light signals the violent death of
the universe's most massive stars. Now astronomers have viewed this heavenly
harbinger for the first time.&lt;/SPAN&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;SPAN&gt;"Astronomers
have been dreaming about seeing the first light from the violent death of a
star for over 30 years," said lead researcher Kevin Schawinksi of the University of Oxford. "Our observations open up an entirely new avenue for studying
the final stages in the lives of massive stars and the physics of
supernovae."&lt;/SPAN&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;SPAN&gt;Schawinksi
and his colleagues detected the ultraviolet signal of a hefty star on the &lt;A href="http://www.space.com/php/multimedia/imagedisplay/img_display.php?pic=080612-star-death-02.jpg&amp;cap=The+red+supergiant+underwent+five+stages+in+the+life+cycle+of+a+star.+The+yellowish+regions+represent+visible+images+taken+with+the+Hubble+Space+Telescope%2C++over+which+are+the+blue+ultraviolet+images+taken+with+GALEX.+Since+GALEX+doesn%27t+have+Hubble%27s+spatial+resolution%2C+the+blue+blobs+show+up+as+blurry+and+larger+than+reality.+Credit:+Kevin+Schawinski+%28Oxford%29%2C+NASA%2FGALEX%2FHST%2C+COSMOS."&gt;verge
of explosion&lt;/A&gt;, which they detail in the June 13 issue of the journal &lt;I&gt;Science&lt;/I&gt;.
&lt;/SPAN&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://www.space.com/scienceastronomy/080612-star-burst.html</clipSource><pubDate>Fri, 13 Jun 2008 13:42:23 GMT</pubDate></item><item><title>Pluto Gets Respect: Dwarf Planets to Be Called 'Plutoids'</title><link>http://clipmarks.com/clipmark/66B2D334-42B6-4625-B867-9F07606D1CB6/</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://dsc.discovery.com/news/2008/06/11/pluto-plutoids.html" title="http://dsc.discovery.com/news/2008/06/11/pluto-plutoids.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/tabsey/512/408CD04B-DF04-44FD-B26D-2E4B5982FBC7.jpg" alt="Who Needs Planets When You've Got Plutoids?" /&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;June 11, 2008&lt;/STRONG&gt; -- Pluto is finally getting its day in the sun, after being &lt;A target="_blank" href="http://dsc.discovery.com/news/2006/08/24/pluto_spa.html"&gt;stripped of planetary status&lt;/A&gt; by astronomers two years ago.&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;From now on all similar distant bodies in the solar system will be called "plutoids." That's the decision by the &lt;A target="_blank" href="http://www.iau.org/"&gt;International Astronomical Union&lt;/A&gt;, which met last week in Oslo, Norway, and announced the decision Wednesday.&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 same group raised a cosmic fuss when it demoted the once-ninth planet to &lt;A target="_blank" href="http://dsc.discovery.com/news/2006/09/14/dwarfplanet_spa.html"&gt;"dwarf" status&lt;/A&gt; in 2006. The new policy allows Pluto to be the standard for a whole new category of dwarf planets.&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;Pluto is one of only two plutoids, the other being Eris. Both are objects that circle the sun and are too small to be considered planets, but big enough to have a level of gravity that keeps them in a near spherical shape. Plutoids also must be farther from the sun than &lt;A target="_blank" href="http://dsc.discovery.com/news/2007/09/21/neptune_spa.html"&gt;Neptune&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/astronomy/" rel="tag"&gt;astronomy&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://dsc.discovery.com/news/2008/06/11/pluto-plutoids.html</clipSource><pubDate>Thu, 12 Jun 2008 13:31:51 GMT</pubDate></item><item><title>Collage of space pictures.</title><link>http://clipmarks.com/clipmark/0440DBBD-8B25-4271-A886-60934B903F14/</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;  The clip may tempt you to visit the site. Very effective. &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://wierdling.longboys.net/images/astronomy/collageFULL.html" title="http://wierdling.longboys.net/images/astronomy/collageFULL.html"&gt;wierdling.longboys.net&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://clipmarks.com/image_cache/tabsey/512/85541DF9-F616-46B1-966E-174C612CA664.jpg" alt="" /&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/collage/" rel="tag"&gt;collage&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/astronomy/" rel="tag"&gt;astronomy&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://wierdling.longboys.net/images/astronomy/collageFULL.html</clipSource><pubDate>Wed, 11 Jun 2008 16:50:29 GMT</pubDate></item><item><title>Mysterious Outburst from the Edge of the Milky Way</title><link>http://clipmarks.com/clipmark/F6F7BF90-F201-4E4B-AFD9-15BEBFD46900/</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;  The outburst may represent a transitory stage in a star's evolution that is rarely seen. The star has some similarities to highly unstable aging stars called eruptive variables, which suddenly and unpredictably increase in brightness. &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/2008/06/mysterious-outb.html" title="http://www.dailygalaxy.com/my_weblog/2008/06/mysterious-outb.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;P&gt;&lt;A href="http://www.dailygalaxy.com/photos/uncategorized/2008/06/10/200880main_rs_image_feature_877_9_3.jpg"&gt;&lt;IMG width="320" height="357" border="0" src="http://www.dailygalaxy.com/my_weblog/images/2008/06/10/200880main_rs_image_feature_877_9_3.jpg" title="200880main_rs_image_feature_877_9_3" alt="200880main_rs_image_feature_877_9_3" /&gt;&lt;/A&gt; This stunning image of swirls of dust surrounding the variable star V838 Monocerotis near the edge of our Milky Way Galaxy, about 20,000 light-years from our sun, was recorded by the Hubble Space Telescope in September 2006. &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 picture spans about 14 light-years. Ever since a sudden outburst was detected in January 2002, this enigmatic star has fascinated astronomers, who expect the expanding echoes to continue to light up the dusty environs of V838 Mon for at least the rest of the current decade. Researchers have now found that V838 Mon is likely a young binary star, but the cause of its extraordinary outburst remains a mystery.&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;V838 Monocerotis did not expel its outer layers. Instead, it grew enormously in size. Its surface temperature dropped to temperatures that were not much hotter than a light bulb. This behavior of ballooning to an enormous size, but not losing its outer layers, is very unusual and completely unlike an ordinary nova explosion.&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/astronomy/" rel="tag"&gt;astronomy&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://www.dailygalaxy.com/my_weblog/2008/06/mysterious-outb.html</clipSource><pubDate>Wed, 11 Jun 2008 14:27:28 GMT</pubDate></item><item><title> Supercomputer sets petaflop pace</title><link>http://clipmarks.com/clipmark/5F4968C4-4841-4ADA-99B9-B448B5421F32/</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;  Those mice must have to run awfully quickly. &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/technology/7443557.stm" title="http://news.bbc.co.uk/2/hi/technology/7443557.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/tabsey/512/5174B8F6-2929-46EC-9528-29BE5542A608.jpg" alt="IBM BlueGene/L" /&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;Currently, BlueGene/L is the most powerful computer in the world &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;B&gt;A supercomputer built with components designed for the Sony PlayStation 3 has set a new computing milestone. &lt;/B&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 IBM machine, codenamed Roadrunner, has been shown to run at "petaflop speeds", the equivalent of one thousand trillion calculations per second. 
&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 benchmark means the computer is twice as nimble as the current world's fastest machine, also built by IBM. 
&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;It will be installed at a US government laboratory later this year where it will monitor the US nuclear stockpile. 
&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;It will also be used for research into astronomy, genomics and climate change. 
&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;"We are getting closer to simulating the real world," Bijan Davari, vice president of next generation computing systems at IBM, told BBC News. 
&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;It would be of particular use for calculating risk in financial markets, he said. 
&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 latency of the calculations is so small that for all practical purposes it is real time." 
&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/computers/" rel="tag"&gt;computers&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://news.bbc.co.uk/2/hi/technology/7443557.stm</clipSource><pubDate>Mon, 09 Jun 2008 15:00:34 GMT</pubDate></item><item><title> Two-Armed Spiral Milky Way</title><link>http://clipmarks.com/clipmark/F197F1AC-0454-454C-90C6-B2A1412D9856/</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;  So it does only have two arms. Donated the others to a black hole, I suppose. &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://antwrp.gsfc.nasa.gov/apod/astropix.html" title="http://antwrp.gsfc.nasa.gov/apod/astropix.html"&gt;antwrp.gsfc.nasa.gov&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;CENTER&gt;
&lt;B&gt; Two-Armed Spiral Milky Way &lt;/B&gt; &lt;BR /&gt;

&lt;B&gt; Illustration Credit: &lt;/B&gt; 

R. Hurt (&lt;A href="http://ssc.spitzer.caltech.edu/"&gt;SSC&lt;/A&gt;), 
&lt;A href="http://www.jpl.nasa.gov/"&gt;JPL-Caltech&lt;/A&gt;, 
&lt;A href="http://www.nasa.gov/home/index.html"&gt;NASA&lt;/A&gt;

&lt;BR /&gt;

&lt;B&gt;Survey Credit: &lt;/B&gt;
&lt;A href="http://www.astro.wisc.edu/sirtf/"&gt;GLIMPSE&lt;/A&gt;

&lt;/CENTER&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/tabsey/512/F1E178CF-6B6B-4B70-AE69-F4673922B74F.jpg" alt="See Explanation.
Moving the cursor over the image will bring up an alternate version.
Clicking on the image will bring up the highest resolution version
available." /&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; Explanation: &lt;/B&gt;

&lt;A href="http://antwrp.gsfc.nasa.gov/apod/ap080104.html"&gt;Gazing out&lt;/A&gt; from within
the Milky Way, our own galaxy's true structure is difficult to discern.

But an
&lt;A href="http://www.spitzer.caltech.edu/Media/releases/ssc2008-10/
release.shtml"&gt;ambitious survey effort&lt;/A&gt; with the
&lt;A href="http://antwrp.gsfc.nasa.gov/apod/ap080605.html"&gt;Spitzer Space Telescope&lt;/A&gt; now
offers convincing evidence
that we live in a large galaxy distinguished by two main
&lt;A href="http://antwrp.gsfc.nasa.gov/apod/ap080517.html"&gt;spiral&lt;/A&gt; arms
(the Scutum-Centaurus and Perseus arms)
emerging from the ends of a large central bar.

In fact, from a vantage point that viewed our galaxy
&lt;A href="http://antwrp.gsfc.nasa.gov/apod/ap040410.html"&gt;face-on&lt;/A&gt;,
astronomers in distant galaxies
would likely see
&lt;A href="http://www.seds.org/messier/more/mw_type.html"&gt;the Milky Way
as&lt;/A&gt; a two-armed &lt;A href="http://antwrp.gsfc.nasa.gov/apod/ap070418.html"&gt;barred spiral&lt;/A&gt;
similar to this
&lt;A href="http://www.spitzer.caltech.edu/Media/releases/ssc2008-10/
visuals.shtml"&gt;artist's illustration&lt;/A&gt;.

Previous investigations have identified
a smaller central barred structure and four spiral arms.

Astronomers still
place the Sun about a third of the way in from
the Milky Way's outer edge, in a minor arm called
the Orion Spur.

To locate the Sun and identify the Milky Way's newly mapped features,
just place your cursor over the image.

&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/astronomy/" rel="tag"&gt;astronomy&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://antwrp.gsfc.nasa.gov/apod/astropix.html</clipSource><pubDate>Fri, 06 Jun 2008 15:43:01 GMT</pubDate></item></channel></rss>