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<?xml-stylesheet type="text/xsl" media="screen" href="/~d/styles/rss2full.xsl"?><?xml-stylesheet type="text/css" media="screen" href="http://feeds.feedburner.com/~d/styles/itemcontent.css"?><rss xmlns:atom="http://www.w3.org/2005/Atom" xmlns:feedburner="http://rssnamespace.org/feedburner/ext/1.0" version="2.0"><channel><title>ESO Top News</title><link>http://www.eso.org/public/news/</link><description>Top News from ESO</description><language>en</language><lastBuildDate>Wed, 16 May 2012 12:00:00 +0200</lastBuildDate><atom10:link xmlns:atom10="http://www.w3.org/2005/Atom" rel="self" type="application/rss+xml" href="http://feeds.feedburner.com/EsoTopNews" /><feedburner:info uri="esotopnews" /><atom10:link xmlns:atom10="http://www.w3.org/2005/Atom" rel="hub" href="http://pubsubhubbub.appspot.com/" /><item><title>A Deeper Look at Centaurus A</title><link>http://feedproxy.google.com/~r/EsoTopNews/~3/OAwNJ_aJfIY/</link><description>The strange galaxy Centaurus A is pictured in a new image from the European Southern Observatory. With a total exposure time of more than 50 hours this is probably the deepest view of this peculiar and spectacular object ever created. The image was produced by the Wide Field Imager of the MPG/ESO 2.2-metre telescope at ESO’s La Silla Observatory in Chile.&lt;img src="http://feeds.feedburner.com/~r/EsoTopNews/~4/OAwNJ_aJfIY" height="1" width="1"/&gt;</description><pubDate>Wed, 16 May 2012 12:00:00 +0200</pubDate><guid isPermaLink="false">http://www.eso.org/public/news/eso1221/</guid><enclosure url="http://www.eso.org/public/archives/images/screen/eso1221a.jpg" length="0" type="image/jpeg" /><feedburner:origLink>http://www.eso.org/public/news/eso1221/</feedburner:origLink></item><item><title>VISTA Views a Vast Ball of Stars</title><link>http://feedproxy.google.com/~r/EsoTopNews/~3/P6hHQZkVCVs/</link><description>A new image of Messier 55 from ESO&amp;#39;s VISTA infrared survey telescope shows tens of thousands of stars crowded together like a swarm of bees. Besides being packed into a relatively small space, these stars are also among the oldest in the Universe. Astronomers study Messier 55 and other ancient objects like it, called globular clusters, to learn how galaxies evolve and stars age.&lt;img src="http://feeds.feedburner.com/~r/EsoTopNews/~4/P6hHQZkVCVs" height="1" width="1"/&gt;</description><pubDate>Wed, 09 May 2012 12:00:00 +0200</pubDate><guid isPermaLink="false">http://www.eso.org/public/news/eso1220/</guid><enclosure url="http://www.eso.org/public/archives/images/screen/eso1220a.jpg" length="0" type="image/jpeg" /><feedburner:origLink>http://www.eso.org/public/news/eso1220/</feedburner:origLink></item><item><title>Sifting through Dust near Orion's Belt</title><link>http://feedproxy.google.com/~r/EsoTopNews/~3/L0PC0rmDt24/</link><description>A new image of the region surrounding the reflection nebula Messier 78, just to the north of Orion’s Belt, shows clouds of cosmic dust threaded through the nebula like a string of pearls. The observations, made with the Atacama Pathfinder Experiment (APEX) telescope[1], use the heat glow of interstellar dust grains to show astronomers where new stars are being formed.&lt;img src="http://feeds.feedburner.com/~r/EsoTopNews/~4/L0PC0rmDt24" height="1" width="1"/&gt;</description><pubDate>Wed, 02 May 2012 12:00:00 +0200</pubDate><guid isPermaLink="false">http://www.eso.org/public/news/eso1219/</guid><enclosure url="http://www.eso.org/public/archives/images/screen/eso1219a.jpg" length="0" type="image/jpeg" /><feedburner:origLink>http://www.eso.org/public/news/eso1219/</feedburner:origLink></item><item><title>A Cluster Within a Cluster</title><link>http://feedproxy.google.com/~r/EsoTopNews/~3/UYwGFkOmauQ/</link><description>The star cluster NGC 6604 is shown in this new image taken by the Wide Field Imager attached to the MPG/ESO 2.2-metre telescope at the La Silla Observatory in Chile. It is often overlooked in favour of its more prominent neighbour, the Eagle Nebula (also known as Messier 16), that lies a mere wingspan away. But the framing of this picture, which places the star cluster in a landscape of surrounding gas and dust clouds, shows what a beautiful object NGC 6604 is in its own right.&lt;img src="http://feeds.feedburner.com/~r/EsoTopNews/~4/UYwGFkOmauQ" height="1" width="1"/&gt;</description><pubDate>Wed, 25 Apr 2012 12:00:00 +0200</pubDate><guid isPermaLink="false">http://www.eso.org/public/news/eso1218/</guid><enclosure url="http://www.eso.org/public/archives/images/screen/eso1218a.jpg" length="0" type="image/jpeg" /><feedburner:origLink>http://www.eso.org/public/news/eso1218/</feedburner:origLink></item><item><title>Serious Blow to Dark Matter Theories?</title><link>http://feedproxy.google.com/~r/EsoTopNews/~3/hH020UW99yI/</link><description>The most accurate study so far of the motions of stars in the Milky Way has found no evidence for dark matter in a large volume around the Sun. According to widely accepted theories, the solar neighbourhood was expected to be filled with dark matter, a mysterious invisible substance that can only be detected indirectly by the gravitational force it exerts. But a new study by a team of astronomers in Chile has found that these theories just do not fit the observational facts. This may mean that attempts to directly detect dark matter particles on Earth are unlikely to be successful.&lt;img src="http://feeds.feedburner.com/~r/EsoTopNews/~4/hH020UW99yI" height="1" width="1"/&gt;</description><pubDate>Wed, 18 Apr 2012 16:00:00 +0200</pubDate><guid isPermaLink="false">http://www.eso.org/public/news/eso1217/</guid><enclosure url="http://www.eso.org/public/archives/images/screen/eso1217a.jpg" length="0" type="image/jpeg" /><feedburner:origLink>http://www.eso.org/public/news/eso1217/</feedburner:origLink></item><item><title>ALMA Reveals Workings of Nearby Planetary System</title><link>http://feedproxy.google.com/~r/EsoTopNews/~3/aCcJtlGKmCo/</link><description>A new observatory still under construction has given astronomers a major breakthrough in understanding a nearby planetary system and provided valuable clues about how such systems form and evolve. Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) have discovered that planets orbiting the star Fomalhaut must be much smaller than originally thought. This is the first published science result from ALMA in its first period of open observations for astronomers worldwide.&lt;img src="http://feeds.feedburner.com/~r/EsoTopNews/~4/aCcJtlGKmCo" height="1" width="1"/&gt;</description><pubDate>Thu, 12 Apr 2012 15:00:00 +0200</pubDate><guid isPermaLink="false">http://www.eso.org/public/news/eso1216/</guid><enclosure url="http://www.eso.org/public/archives/images/screen/eso1216a.jpg" length="0" type="image/jpeg" /><feedburner:origLink>http://www.eso.org/public/news/eso1216/</feedburner:origLink></item><item><title>ESO Expands its Headquarters</title><link>http://feedproxy.google.com/~r/EsoTopNews/~3/jiqhFZgBND0/</link><description>The European Southern Observatory (ESO) has contracted architects Auer+Weber to design an extension to its Headquarters at Garching bei München, Germany. The innovatively styled new office building will help to house the growing number of Garching staff, and be the cradle of the technological innovations needed for ESO’s ambitious projects such as the European Extremely Large Telescope. With construction expected to be completed by the end of 2013, the expanded ESO Headquarters will contribute greatly to the development of the Garching research campus.&lt;img src="http://feeds.feedburner.com/~r/EsoTopNews/~4/jiqhFZgBND0" height="1" width="1"/&gt;</description><pubDate>Wed, 04 Apr 2012 12:00:00 +0200</pubDate><guid isPermaLink="false">http://www.eso.org/public/news/eso1215/</guid><enclosure url="http://www.eso.org/public/archives/images/screen/eso1215a.jpg" length="0" type="image/jpeg" /><feedburner:origLink>http://www.eso.org/public/news/eso1215/</feedburner:origLink></item><item><title>Many Billions of Rocky Planets in the Habitable Zones around Red Dwarfs in the Milky Way</title><link>http://feedproxy.google.com/~r/EsoTopNews/~3/cQWSXceE81U/</link><description>A new result from ESO’s HARPS planet finder shows that rocky planets not much bigger than Earth are very common in the habitable zones around faint red stars. The international team estimates that there are tens of billions of such planets in the Milky Way galaxy alone, and probably about one hundred in the Sun’s immediate neighbourhood. This is the first direct measurement of the frequency of super-Earths around red dwarfs, which account for 80% of the stars in the Milky Way.&lt;img src="http://feeds.feedburner.com/~r/EsoTopNews/~4/cQWSXceE81U" height="1" width="1"/&gt;</description><pubDate>Wed, 28 Mar 2012 12:00:00 +0200</pubDate><guid isPermaLink="false">http://www.eso.org/public/news/eso1214/</guid><enclosure url="http://www.eso.org/public/archives/images/screen/eso1214a.jpg" length="0" type="image/jpeg" /><feedburner:origLink>http://www.eso.org/public/news/eso1214/</feedburner:origLink></item><item><title>VISTA Stares Deep into the Cosmos</title><link>http://feedproxy.google.com/~r/EsoTopNews/~3/aziU1LGfR10/</link><description>ESO&amp;#39;s VISTA telescope has created the widest deep view of the sky ever made using infrared light. This new picture of an unremarkable patch of sky comes from the UltraVISTA survey and reveals more than 200 000 galaxies. It forms just one part of a huge collection of fully processed images from all the VISTA surveys that is now being made available by ESO to astronomers worldwide. UltraVISTA is a treasure trove that is being used to study distant galaxies in the early Universe as well as for many other science projects.&lt;img src="http://feeds.feedburner.com/~r/EsoTopNews/~4/aziU1LGfR10" height="1" width="1"/&gt;</description><pubDate>Wed, 21 Mar 2012 12:00:00 +0100</pubDate><guid isPermaLink="false">http://www.eso.org/public/news/eso1213/</guid><enclosure url="http://www.eso.org/public/archives/images/screen/eso1213a.jpg" length="0" type="image/jpeg" /><feedburner:origLink>http://www.eso.org/public/news/eso1213/</feedburner:origLink></item><item><title>The Feeding Habits of Teenage Galaxies</title><link>http://feedproxy.google.com/~r/EsoTopNews/~3/j6Trnmvo5kM/</link><description>New observations made with ESO’s Very Large Telescope are making a major contribution to understanding the growth of adolescent galaxies. In the biggest survey of its kind astronomers have found that galaxies changed their eating habits during their teenage years - the period from about 3 to 5 billion years after the Big Bang. At the start of this phase smooth gas flow was the preferred snack, but later, galaxies mostly grew by cannibalising other smaller galaxies.&lt;img src="http://feeds.feedburner.com/~r/EsoTopNews/~4/j6Trnmvo5kM" height="1" width="1"/&gt;</description><pubDate>Wed, 14 Mar 2012 12:00:00 +0100</pubDate><guid isPermaLink="false">http://www.eso.org/public/news/eso1212/</guid><enclosure url="http://www.eso.org/public/archives/images/screen/eso1212a.jpg" length="0" type="image/jpeg" /><feedburner:origLink>http://www.eso.org/public/news/eso1212/</feedburner:origLink></item></channel></rss>

