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<feed xmlns:media="http://search.yahoo.com/mrss/" xmlns:gr="http://www.google.com/schemas/reader/atom/" xmlns:idx="urn:atom-extension:indexing" xmlns="http://www.w3.org/2005/Atom" idx:index="no" gr:dir="ltr"><!--
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--><generator uri="http://www.google.com/reader">Google Reader</generator><id>tag:google.com,2005:reader/user/02900617613998287456/label/astro-news</id><link rel="hub" href="http://pubsubhubbub.appspot.com/"/><title>"astro-news" via ioalib in Google Reader</title><gr:continuation>CM-nl4iX-q8C</gr:continuation><link rel="self" href="http://www.google.com/reader/public/atom/user%2F02900617613998287456/label/astro-news"/><author><name>ioalib</name></author><updated>2012-05-19T07:06:39Z</updated><entry gr:crawl-timestamp-msec="1337411199401"><id gr:original-id="http://www.newscientist.com/article/dn21826">tag:google.com,2005:reader/item/3cb943130a4a42a5</id><title type="html">Number of asteroids that pose risk to Earth is doubled</title><published>2012-05-18T14:40:00Z</published><updated>2012-05-18T14:40:00Z</updated><link rel="alternate" href="http://feeds.newscientist.com/c/749/f/10897/s/1f7ae10e/l/0L0Snewscientist0N0Carticle0Cdn218260Enumber0Eof0Easteroids0Ethat0Epose0Erisk0Eto0Eearth0Eis0Edoubled0Bhtml0DDCMP0FOTC0Erss0Gnsref0Fonline0Enews/story01.htm" type="text/html"/><summary xml:base="http://www.newscientist.com/" type="html">The asteroid-tracking NEOWISE mission reveals that twice as many asteroids as previously thought are on low-inclination orbits that could hit our planet&lt;img width="1" height="1" src="http://feeds.newscientist.com/c/749/f/10897/s/1f7ae10e/mf.gif" border="0"&gt;&lt;div&gt;&lt;table border="0"&gt;&lt;tr&gt;&lt;td valign="middle"&gt;&lt;a href="http://share.feedsportal.com/viral/sendEmail.cfm?lang=en&amp;amp;title=Number+of+asteroids+that+pose+risk+to+Earth+is+doubled&amp;amp;link=http%3A%2F%2Fwww.newscientist.com%2Farticle%2Fdn21826-number-of-asteroids-that-pose-risk-to-earth-is-doubled.html%3FDCMP%3DOTC-rss%26nsref%3Donline-news"&gt;&lt;img src="http://res3.feedsportal.com/images/emailthis2.gif" border="0"&gt;&lt;/a&gt;&lt;/td&gt;&lt;td valign="middle"&gt;&lt;a href="http://res.feedsportal.com/viral/bookmark.cfm?title=Number+of+asteroids+that+pose+risk+to+Earth+is+doubled&amp;amp;link=http%3A%2F%2Fwww.newscientist.com%2Farticle%2Fdn21826-number-of-asteroids-that-pose-risk-to-earth-is-doubled.html%3FDCMP%3DOTC-rss%26nsref%3Donline-news"&gt;&lt;img src="http://res3.feedsportal.com/images/bookmark.gif" border="0"&gt;&lt;/a&gt;&lt;/td&gt;&lt;/tr&gt;&lt;/table&gt;&lt;/div&gt;&lt;br&gt;&lt;br&gt;&lt;a href="http://da.feedsportal.com/r/133515952587/u/31/f/10897/c/749/s/1f7ae10e/a2.htm"&gt;&lt;img src="http://da.feedsportal.com/r/133515952587/u/31/f/10897/c/749/s/1f7ae10e/a2.img" border="0"&gt;&lt;/a&gt;&lt;img width="1" height="1" src="http://pi.feedsportal.com/r/133515952587/u/31/f/10897/c/749/s/1f7ae10e/a2t.img" border="0"&gt;</summary><author gr:unknown-author="true"><name>(author unknown)</name></author><source gr:stream-id="feed/http://feeds.newscientist.com/science-news"><id>tag:google.com,2005:reader/feed/http://feeds.newscientist.com/science-news</id><title type="html">New Scientist - Online News</title><link rel="alternate" href="http://www.newscientist.com/" type="text/html"/></source></entry><entry gr:crawl-timestamp-msec="1337411118649"><id gr:original-id="http://science.nasa.gov/science-news/science-at-nasa/2012/18may_venustransit/">tag:google.com,2005:reader/item/721dccac815e693d</id><title type="html">The 2012 Transit of Venus</title><published>2012-05-18T05:24:14Z</published><updated>2012-05-18T05:24:14Z</updated><link rel="alternate" href="http://science.nasa.gov/science-news/science-at-nasa/2012/18may_venustransit/" type="text/html"/><summary xml:base="http://science.nasa.gov/science-news/science-at-nasa/" type="html">It won&amp;#39;t happen again until December 2117: On June 5th, 2012, Venus will transit the face of the sun. The best places to watch are in the south Pacific, but travel is not required. The event is widely visible around the world, including at sunset from the USA.</summary><author gr:unknown-author="true"><name>(author unknown)</name></author><source gr:stream-id="feed/http://science.nasa.gov/rss.xml"><id>tag:google.com,2005:reader/feed/http://science.nasa.gov/rss.xml</id><title type="html">Science@NASA Headline News</title><link rel="alternate" href="http://science.nasa.gov/science-news/science-at-nasa/" type="text/html"/></source></entry><entry gr:crawl-timestamp-msec="1337411065577"><id gr:original-id="http://sci.esa.int/jump.cfm?oid=48658">tag:google.com,2005:reader/item/943dec65c93c149b</id><title type="html">Astrophysics:First Stars IV - From Hayashi to the Future[Mon, 21 May 2012]</title><published>2011-04-18T19:23:00Z</published><updated>2011-04-18T19:23:00Z</updated><link rel="alternate" href="http://sci.esa.int/jump.cfm?oid=48658" type="text/html"/><summary xml:base="http://sci.esa.int/" type="html">In the last decade, great advances have been made in the field of First Stars. So far, three international conferences have been held as a series of First Stars meetings every four years (Garching in 1999, Pennsylvania in 2003, and Santa Fe in 2007).  

The fourth First Stars meeting, &amp;quot;First Stars IV&amp;quot;, is aimed at discussing star formation through cosmic time and the impacts of first stars on galaxy formation, first explosions, cosmic reionization, and formation of massive black holes. This meeting will be held partially as a memorial conference for Professor Hayashi (1920-2010), in honour of his invaluable contributions to the study of star formation and cosmology.</summary><author gr:unknown-author="true"><name>(author unknown)</name></author><source gr:stream-id="feed/http://sci.esa.int/newssyndication/rss/sciweb.xml"><id>tag:google.com,2005:reader/feed/http://sci.esa.int/newssyndication/rss/sciweb.xml</id><title type="html">ESA Science &amp;amp; Technology</title><link rel="alternate" href="http://sci.esa.int" type="text/html"/></source></entry><entry gr:crawl-timestamp-msec="1337329515278"><id gr:original-id="http://sci.esa.int/jump.cfm?oid=49861">tag:google.com,2005:reader/item/cde7cd19859af8f5</id><title type="html">XMM-Newton:XMM-Newton 2012 Science Workshop - Galaxy Clusters as Giant Cosmic Laboratories[Mon, 21 May 2012]</title><published>2012-01-16T23:30:00Z</published><updated>2012-01-16T23:30:00Z</updated><link rel="alternate" href="http://sci.esa.int/jump.cfm?oid=49861" type="text/html"/><summary xml:base="http://sci.esa.int/" type="html">Galaxy clusters are interesting astrophysical laboratories to study large-scale physical processes and important probes to assess the structure and evolution of our Universe. X-ray observations provide the most detailed insight into structure, composition, and evolution of galaxy clusters.</summary><author gr:unknown-author="true"><name>(author unknown)</name></author><source gr:stream-id="feed/http://sci.esa.int/newssyndication/rss/sciweb.xml"><id>tag:google.com,2005:reader/feed/http://sci.esa.int/newssyndication/rss/sciweb.xml</id><title type="html">ESA Science &amp;amp; Technology</title><link rel="alternate" href="http://sci.esa.int" type="text/html"/></source></entry><entry gr:crawl-timestamp-msec="1337329346234"><id gr:original-id="http://www.bbc.co.uk/news/science-environment-18089695">tag:google.com,2005:reader/item/47bacdb1de74c4b0</id><title type="html">'Superflares' from stars counted</title><published>2012-05-17T13:37:09Z</published><updated>2012-05-17T13:37:09Z</updated><link rel="alternate" href="http://www.bbc.co.uk/news/science-environment-18089695#sa-ns_mchannel=rss&amp;ns_source=PublicRSS20-sa" type="text/html"/><summary xml:base="http://www.bbc.co.uk/news/science_and_environment/#sa-ns_mchannel=rss&amp;ns_source=PublicRSS20-sa" type="html">Nasa's Kepler space telescope provides new insight on the colossal explosions that can occur in the atmospheres of some stars.</summary><author gr:unknown-author="true"><name>(author unknown)</name></author><source gr:stream-id="feed/http://newsrss.bbc.co.uk/rss/newsonline_world_edition/science/nature/rss.xml"><id>tag:google.com,2005:reader/feed/http://newsrss.bbc.co.uk/rss/newsonline_world_edition/science/nature/rss.xml</id><title type="html">BBC News - Science &amp;amp; Environment</title><link rel="alternate" href="http://www.bbc.co.uk/news/science_and_environment/#sa-ns_mchannel=rss&amp;ns_source=PublicRSS20-sa" type="text/html"/></source></entry><entry gr:crawl-timestamp-msec="1337243148684"><id gr:original-id="http://dx.doi.org/10.1038/485283b">tag:google.com,2005:reader/item/54a140e02eea8cb1</id><title type="html">Astronomy: Exoplanet signals ring true</title><published>2012-05-16T07:00:00Z</published><updated>2012-05-16T07:00:00Z</updated><link rel="alternate" href="http://feeds.nature.com/~r/nature/rss/current/~3/QY4_-H_KKNA/485283b" type="text/html"/><content xml:base="http://www.nature.com/nature/current_issue/" type="html">&lt;p&gt;
            &lt;b&gt;Astronomy: Exoplanet signals ring true&lt;/b&gt;
         &lt;/p&gt;
         &lt;p&gt;Nature 485, 7398 (2012). &lt;a href="http://dx.doi.org/10.1038/485283b"&gt;doi:10.1038/485283b&lt;/a&gt;
         &lt;/p&gt;
         &lt;p&gt;Most candidate multi-planet systems spotted by the Kepler space telescope probably contain true exoplanets, according to a statistical analysis.Kepler spots potential planets beyond our Solar System by looking for tiny dips in brightness as the planets pass in front of their host stars. The &lt;/p&gt;
				&lt;img src="http://feeds.feedburner.com/~r/nature/rss/current/~4/QY4_-H_KKNA" height="1" width="1"&gt;</content><author gr:unknown-author="true"><name>(author unknown)</name></author><source gr:stream-id="feed/http://www.nature.com/nature/current_issue/rss"><id>tag:google.com,2005:reader/feed/http://www.nature.com/nature/current_issue/rss</id><title type="html">Nature - Issue - nature.com science feeds</title><link rel="alternate" href="http://www.nature.com/nature/current_issue/" type="text/html"/></source></entry><entry gr:crawl-timestamp-msec="1337243138157"><id gr:original-id="http://www.nature.com/doifinder/10.1038/485290a">tag:google.com,2005:reader/item/94707606fecac43c</id><title type="html">Messages from the early Universe</title><published>2012-05-16T07:00:00Z</published><updated>2012-05-16T07:00:00Z</updated><link rel="alternate" href="http://feeds.nature.com/~r/nature/rss/current/~3/Fj_vQG6EtMc/485290a" type="text/html"/><content xml:base="http://www.nature.com/nature/current_issue/" type="html">&lt;p&gt;
            &lt;b&gt;Messages from the early Universe&lt;/b&gt;
         &lt;/p&gt;
         &lt;p&gt;Nature 485, 7398 (2012). &lt;a href="http://www.nature.com/doifinder/10.1038/485290a"&gt;http://www.nature.com/doifinder/10.1038/485290a&lt;/a&gt;
         &lt;/p&gt;
         &lt;p&gt;Author: Eric Hand&lt;/p&gt;
         &lt;p&gt;Bright and brief, &#x3B3;-ray bursts hold clues to cosmic history.&lt;/p&gt;
				&lt;img src="http://feeds.feedburner.com/~r/nature/rss/current/~4/Fj_vQG6EtMc" height="1" width="1"&gt;</content><author><name>Eric Hand</name></author><source gr:stream-id="feed/http://www.nature.com/nature/current_issue/rss"><id>tag:google.com,2005:reader/feed/http://www.nature.com/nature/current_issue/rss</id><title type="html">Nature - Issue - nature.com science feeds</title><link rel="alternate" href="http://www.nature.com/nature/current_issue/" type="text/html"/></source></entry><entry gr:crawl-timestamp-msec="1337243123803"><id gr:original-id="http://dx.doi.org/10.1038/nature11193">tag:google.com,2005:reader/item/32bc6e976e2e09f6</id><title type="html">Planetary science: Martian sand blowing in the wind</title><published>2012-05-09T07:00:00Z</published><updated>2012-05-09T07:00:00Z</updated><link rel="alternate" href="http://feeds.nature.com/~r/nature/rss/current/~3/XmZrkmDDZhc/nature11193" type="text/html"/><content xml:base="http://www.nature.com/nature/current_issue/" type="html">&lt;p&gt;
            &lt;b&gt;Planetary science: Martian sand blowing in the wind&lt;/b&gt;
         &lt;/p&gt;
         &lt;p&gt;Nature 485, 7398 (2012). &lt;a href="http://dx.doi.org/10.1038/nature11193"&gt;doi:10.1038/nature11193&lt;/a&gt;
         &lt;/p&gt;
         &lt;p&gt;Authors: Jasper Kok&lt;/p&gt;
         &lt;p&gt;High-resolution spacecraft images show surprisingly large rates of sand transport on Mars. This finding suggests that the planet's surface is a more active environment than previously thought. See Letter p.339&lt;/p&gt;
				&lt;img src="http://feeds.feedburner.com/~r/nature/rss/current/~4/XmZrkmDDZhc" height="1" width="1"&gt;</content><author><name>Jasper Kok</name></author><source gr:stream-id="feed/http://www.nature.com/nature/current_issue/rss"><id>tag:google.com,2005:reader/feed/http://www.nature.com/nature/current_issue/rss</id><title type="html">Nature - Issue - nature.com science feeds</title><link rel="alternate" href="http://www.nature.com/nature/current_issue/" type="text/html"/></source></entry><entry gr:crawl-timestamp-msec="1337243015677"><id gr:original-id="http://dx.doi.org/10.1038/485282a">tag:google.com,2005:reader/item/127077b183f75a13</id><title type="html">Planetary science: Planet-like asteroid</title><published>2012-05-16T07:00:00Z</published><updated>2012-05-16T07:00:00Z</updated><link rel="alternate" href="http://feeds.nature.com/~r/nature/rss/current/~3/zSfW2oJre5o/485282a" type="text/html"/><content xml:base="http://www.nature.com/nature/current_issue/" type="html">&lt;p&gt;
            &lt;b&gt;Planetary science: Planet-like asteroid&lt;/b&gt;
         &lt;/p&gt;
         &lt;p&gt;Nature 485, 7398 (2012). &lt;a href="http://dx.doi.org/10.1038/485282a"&gt;doi:10.1038/485282a&lt;/a&gt;
         &lt;/p&gt;
         &lt;p&gt;The giant asteroid Vesta resembles a planet more than it does other asteroids, according to Christopher Russell at the University of California, Los Angeles, and his colleagues. In six separate studies, the researchers report their analysis of data from NASA's Dawn spacecraft, which has been &lt;/p&gt;
				&lt;img src="http://feeds.feedburner.com/~r/nature/rss/current/~4/zSfW2oJre5o" height="1" width="1"&gt;</content><author gr:unknown-author="true"><name>(author unknown)</name></author><source gr:stream-id="feed/http://www.nature.com/nature/current_issue/rss"><id>tag:google.com,2005:reader/feed/http://www.nature.com/nature/current_issue/rss</id><title type="html">Nature - Issue - nature.com science feeds</title><link rel="alternate" href="http://www.nature.com/nature/current_issue/" type="text/html"/></source></entry><entry gr:crawl-timestamp-msec="1337242940200"><id gr:original-id="http://dx.doi.org/10.1038/485303a">tag:google.com,2005:reader/item/02cc84f1c6989d91</id><title type="html">Transit of Venus: Last chance to see</title><published>2012-05-16T07:00:00Z</published><updated>2012-05-16T07:00:00Z</updated><link rel="alternate" href="http://feeds.nature.com/~r/nature/rss/current/~3/Hfa_1DgiEiU/485303a" type="text/html"/><content xml:base="http://www.nature.com/nature/current_issue/" type="html">&lt;p&gt;
            &lt;b&gt;Transit of Venus: Last chance to see&lt;/b&gt;
         &lt;/p&gt;
         &lt;p&gt;Nature 485, 7398 (2012). &lt;a href="http://dx.doi.org/10.1038/485303a"&gt;doi:10.1038/485303a&lt;/a&gt;
         &lt;/p&gt;
         &lt;p&gt;Author: Jay M. Pasachoff&lt;/p&gt;
         &lt;p&gt;The June 2012 transit of Venus across the Sun offers an opportunity to check our methods for spotting distant planets crossing far-away stars, says Jay M. Pasachoff.&lt;/p&gt;
				&lt;img src="http://feeds.feedburner.com/~r/nature/rss/current/~4/Hfa_1DgiEiU" height="1" width="1"&gt;</content><author><name>Jay M. Pasachoff</name></author><source gr:stream-id="feed/http://www.nature.com/nature/current_issue/rss"><id>tag:google.com,2005:reader/feed/http://www.nature.com/nature/current_issue/rss</id><title type="html">Nature - Issue - nature.com science feeds</title><link rel="alternate" href="http://www.nature.com/nature/current_issue/" type="text/html"/></source></entry><entry gr:crawl-timestamp-msec="1337242763213"><id gr:original-id="http://www.newscientist.com/article/dn21818">tag:google.com,2005:reader/item/082a547c0738f03f</id><title type="html">Pulsar heavyweight champ challenges Einstein</title><published>2012-05-16T14:32:00Z</published><updated>2012-05-16T14:32:00Z</updated><link rel="alternate" href="http://feeds.newscientist.com/c/749/f/10897/s/1f6ad88c/l/0L0Snewscientist0N0Carticle0Cdn218180Epulsar0Eheavyweight0Echamp0Echallenges0Eeinstein0Bhtml0DDCMP0FOTC0Erss0Gnsref0Fonline0Enews/story01.htm" type="text/html"/><summary xml:base="http://www.newscientist.com/" type="html">A pulsar with twice the sun's mass could challenge Einstein's theory of general relativity: but such a dense object is near impossible, according to his work&lt;img width="1" height="1" src="http://feeds.newscientist.com/c/749/f/10897/s/1f6ad88c/mf.gif" border="0"&gt;&lt;div&gt;&lt;table border="0"&gt;&lt;tr&gt;&lt;td valign="middle"&gt;&lt;a href="http://share.feedsportal.com/viral/sendEmail.cfm?lang=en&amp;amp;title=Pulsar+heavyweight+champ+challenges+Einstein&amp;amp;link=http%3A%2F%2Fwww.newscientist.com%2Farticle%2Fdn21818-pulsar-heavyweight-champ-challenges-einstein.html%3FDCMP%3DOTC-rss%26nsref%3Donline-news"&gt;&lt;img src="http://res3.feedsportal.com/images/emailthis2.gif" border="0"&gt;&lt;/a&gt;&lt;/td&gt;&lt;td valign="middle"&gt;&lt;a href="http://res.feedsportal.com/viral/bookmark.cfm?title=Pulsar+heavyweight+champ+challenges+Einstein&amp;amp;link=http%3A%2F%2Fwww.newscientist.com%2Farticle%2Fdn21818-pulsar-heavyweight-champ-challenges-einstein.html%3FDCMP%3DOTC-rss%26nsref%3Donline-news"&gt;&lt;img src="http://res3.feedsportal.com/images/bookmark.gif" border="0"&gt;&lt;/a&gt;&lt;/td&gt;&lt;/tr&gt;&lt;/table&gt;&lt;/div&gt;&lt;br&gt;&lt;br&gt;&lt;a href="http://da.feedsportal.com/r/133515851153/u/31/f/10897/c/749/s/1f6ad88c/a2.htm"&gt;&lt;img src="http://da.feedsportal.com/r/133515851153/u/31/f/10897/c/749/s/1f6ad88c/a2.img" border="0"&gt;&lt;/a&gt;&lt;img width="1" height="1" src="http://pi.feedsportal.com/r/133515851153/u/31/f/10897/c/749/s/1f6ad88c/a2t.img" border="0"&gt;</summary><author gr:unknown-author="true"><name>(author unknown)</name></author><source gr:stream-id="feed/http://feeds.newscientist.com/science-news"><id>tag:google.com,2005:reader/feed/http://feeds.newscientist.com/science-news</id><title type="html">New Scientist - Online News</title><link rel="alternate" href="http://www.newscientist.com/" type="text/html"/></source></entry><entry gr:crawl-timestamp-msec="1337242337991"><id gr:original-id="http://science.nasa.gov/science-news/science-at-nasa/2012/16may_pha/">tag:google.com,2005:reader/item/e784a4cb59518183</id><title type="html">A New Count of Potentially Hazardous Asteroids</title><published>2012-05-16T22:53:53Z</published><updated>2012-05-16T22:53:53Z</updated><link rel="alternate" href="http://science.nasa.gov/science-news/science-at-nasa/2012/16may_pha/" type="text/html"/><summary xml:base="http://science.nasa.gov/science-news/science-at-nasa/" type="html">NASA has just released a new count of asteroids that come close to the orbit of Earth and could survive entry through our planet&amp;#39;s atmosphere.  The data, gathered by an infrared space telescope named WISE, reveal important new information about the origin and make-up of these potentially hazardous space rocks.</summary><author gr:unknown-author="true"><name>(author unknown)</name></author><source gr:stream-id="feed/http://science.nasa.gov/rss.xml"><id>tag:google.com,2005:reader/feed/http://science.nasa.gov/rss.xml</id><title type="html">Science@NASA Headline News</title><link rel="alternate" href="http://science.nasa.gov/science-news/science-at-nasa/" type="text/html"/></source></entry><entry gr:crawl-timestamp-msec="1337242298895"><id gr:original-id="http://www.nasa.gov/home/hqnews/2012/may/HQ_12-157_NEOWISE_PHAs.html">tag:google.com,2005:reader/item/3b4f13ae88424ece</id><title type="html">NASA Survey Counts Potentially Hazardous Asteroids</title><published>2012-05-16T04:00:00Z</published><updated>2012-05-16T04:00:00Z</updated><link rel="alternate" href="http://www.nasa.gov/home/hqnews/2012/may/HQ_12-157_NEOWISE_PHAs.html" type="text/html"/><summary xml:base="http://www.nasa.gov/audience/formedia/features/index.html" type="html">Observations from NASA's Wide-field Infrared Survey Explorer (WISE) have led to the best assessment yet of our solar system's population of potentially hazardous asteroids.</summary><author gr:unknown-author="true"><name>(author unknown)</name></author><source gr:stream-id="feed/http://www.nasa.gov/rss/breaking_news.rss"><id>tag:google.com,2005:reader/feed/http://www.nasa.gov/rss/breaking_news.rss</id><title type="html">NASA Breaking News</title><link rel="alternate" href="http://www.nasa.gov/audience/formedia/features/index.html" type="text/html"/></source></entry><entry gr:crawl-timestamp-msec="1337242265238"><id gr:original-id="http://www.nasa.gov/home/hqnews/2012/may/HQ_12-155_Galex_to_Caltech.html">tag:google.com,2005:reader/item/458037ebfa748d9e</id><title type="html">NASA Lends Galaxy Evolution Explorer to Caltech</title><published>2012-05-16T04:00:00Z</published><updated>2012-05-16T04:00:00Z</updated><link rel="alternate" href="http://www.nasa.gov/home/hqnews/2012/may/HQ_12-155_Galex_to_Caltech.html" type="text/html"/><summary xml:base="http://www.nasa.gov/audience/formedia/features/index.html" type="html">NASA is lending the Galaxy Evolution Explorer (GALEX) to the California Institute of Technology (Caltech) in Pasadena, where the spacecraft will continue its exploration of the cosmos.</summary><author gr:unknown-author="true"><name>(author unknown)</name></author><source gr:stream-id="feed/http://www.nasa.gov/rss/breaking_news.rss"><id>tag:google.com,2005:reader/feed/http://www.nasa.gov/rss/breaking_news.rss</id><title type="html">NASA Breaking News</title><link rel="alternate" href="http://www.nasa.gov/audience/formedia/features/index.html" type="text/html"/></source></entry><entry gr:crawl-timestamp-msec="1337242190344"><id gr:original-id="http://www.eso.org/public/news/eso1221/">tag:google.com,2005:reader/item/ca3ed85fc89990c7</id><title type="html">A Deeper Look at Centaurus A</title><published>2012-05-16T10:00:00Z</published><updated>2012-05-16T10:00:00Z</updated><link rel="alternate" href="http://feedproxy.google.com/~r/EsoTopNews/~3/OAwNJ_aJfIY/" type="text/html"/><link rel="enclosure" href="http://www.eso.org/public/archives/images/screen/eso1221a.jpg" type="image/jpeg" length="0"/><summary xml:base="http://www.eso.org/public/news/" type="html">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&#x2019;s La Silla Observatory in Chile.&lt;img src="http://feeds.feedburner.com/~r/EsoTopNews/~4/OAwNJ_aJfIY" height="1" width="1"&gt;</summary><author gr:unknown-author="true"><name>(author unknown)</name></author><source gr:stream-id="feed/http://www.eso.org/fcc/news.xml"><id>tag:google.com,2005:reader/feed/http://www.eso.org/fcc/news.xml</id><title type="html">ESO Top News</title><link rel="alternate" href="http://www.eso.org/public/news/" type="text/html"/></source></entry><entry gr:crawl-timestamp-msec="1337242066680"><id gr:original-id="http://sci.esa.int/jump.cfm?oid=50378">tag:google.com,2005:reader/item/19a3fab0b61a4385</id><title type="html">Venus Express:Venus Express unearths new clues to the planet's geological history</title><published>2012-05-16T17:34:00Z</published><updated>2012-05-16T17:34:00Z</updated><link rel="alternate" href="http://sci.esa.int/jump.cfm?oid=50378" type="text/html"/><summary xml:base="http://sci.esa.int/" type="html">ESA&amp;amp;apos;s Venus Express has been used to study the geology in a region near Venus&amp;amp;apos; equator. Using near-infrared observations collected by the Venus Monitoring Camera (VMC), scientists have found evidence that the planet&amp;amp;apos;s rugged highlands are scattered with geochemically more evolved rocks, rather than the basaltic rocks of the volcanic plains. This finding is in agreement with previous studies, which used data from the spacecraft&amp;amp;apos;s Visible and Infrared Thermal Imaging Spectrometer (VIRTIS) to map the planet&amp;amp;apos;s surface in the southern hemisphere.</summary><author gr:unknown-author="true"><name>(author unknown)</name></author><source gr:stream-id="feed/http://sci.esa.int/newssyndication/rss/sciweb.xml"><id>tag:google.com,2005:reader/feed/http://sci.esa.int/newssyndication/rss/sciweb.xml</id><title type="html">ESA Science &amp;amp; Technology</title><link rel="alternate" href="http://sci.esa.int" type="text/html"/></source></entry><entry gr:crawl-timestamp-msec="1337241973562"><id gr:original-id="http://www.bbc.co.uk/news/science-environment-18072625">tag:google.com,2005:reader/item/158f04cb90e1d72f</id><title type="html">Big Picture: The Centaur</title><published>2012-05-16T10:31:07Z</published><updated>2012-05-16T10:31:07Z</updated><link rel="alternate" href="http://www.bbc.co.uk/news/science-environment-18072625#sa-ns_mchannel=rss&amp;ns_source=PublicRSS20-sa" type="text/html"/><summary xml:base="http://www.bbc.co.uk/news/science_and_environment/#sa-ns_mchannel=rss&amp;ns_source=PublicRSS20-sa" type="html">The best-yet view of mysterious galaxy Centaurus A</summary><author gr:unknown-author="true"><name>(author unknown)</name></author><source gr:stream-id="feed/http://newsrss.bbc.co.uk/rss/newsonline_world_edition/science/nature/rss.xml"><id>tag:google.com,2005:reader/feed/http://newsrss.bbc.co.uk/rss/newsonline_world_edition/science/nature/rss.xml</id><title type="html">BBC News - Science &amp;amp; Environment</title><link rel="alternate" href="http://www.bbc.co.uk/news/science_and_environment/#sa-ns_mchannel=rss&amp;ns_source=PublicRSS20-sa" type="text/html"/></source></entry><entry gr:crawl-timestamp-msec="1337070479568"><id gr:original-id="http://www.newscientist.com/blogs/culturelab/2012/05/evening-stars-rare-path-across-the-sun.html">tag:google.com,2005:reader/item/80db5d965d92ec8e</id><title type="html">Evening Star's rare path across the sun</title><published>2012-05-14T09:59:00Z</published><updated>2012-05-14T09:59:00Z</updated><link rel="alternate" href="http://feeds.newscientist.com/c/749/f/10897/s/1f5551ad/l/0L0Snewscientist0N0Cblogs0Cculturelab0C20A120C0A50Cevening0Estars0Erare0Epath0Eacross0Ethe0Esun0Bhtml0DDCMP0FOTC0Erss0Gnsref0Fonline0Enews/story01.htm" type="text/html"/><summary xml:base="http://www.newscientist.com/" type="html">With the last transit of Venus of the 21st century weeks away, authors trace how this rare event sparked international scientific collaboration in 1761&lt;img width="1" height="1" src="http://feeds.newscientist.com/c/749/f/10897/s/1f5551ad/mf.gif" border="0"&gt;&lt;div&gt;&lt;table border="0"&gt;&lt;tr&gt;&lt;td valign="middle"&gt;&lt;a href="http://share.feedsportal.com/viral/sendEmail.cfm?lang=en&amp;amp;title=Evening+Star%27s+rare+path+across+the+sun&amp;amp;link=http%3A%2F%2Fwww.newscientist.com%2Fblogs%2Fculturelab%2F2012%2F05%2Fevening-stars-rare-path-across-the-sun.html%3FDCMP%3DOTC-rss%26nsref%3Donline-news"&gt;&lt;img src="http://res3.feedsportal.com/images/emailthis2.gif" border="0"&gt;&lt;/a&gt;&lt;/td&gt;&lt;td valign="middle"&gt;&lt;a href="http://res.feedsportal.com/viral/bookmark.cfm?title=Evening+Star%27s+rare+path+across+the+sun&amp;amp;link=http%3A%2F%2Fwww.newscientist.com%2Fblogs%2Fculturelab%2F2012%2F05%2Fevening-stars-rare-path-across-the-sun.html%3FDCMP%3DOTC-rss%26nsref%3Donline-news"&gt;&lt;img src="http://res3.feedsportal.com/images/bookmark.gif" border="0"&gt;&lt;/a&gt;&lt;/td&gt;&lt;/tr&gt;&lt;/table&gt;&lt;/div&gt;&lt;br&gt;&lt;br&gt;&lt;a href="http://da.feedsportal.com/r/133515709723/u/31/f/10897/c/749/s/1f5551ad/a2.htm"&gt;&lt;img src="http://da.feedsportal.com/r/133515709723/u/31/f/10897/c/749/s/1f5551ad/a2.img" border="0"&gt;&lt;/a&gt;&lt;img width="1" height="1" src="http://pi.feedsportal.com/r/133515709723/u/31/f/10897/c/749/s/1f5551ad/a2t.img" border="0"&gt;</summary><author gr:unknown-author="true"><name>(author unknown)</name></author><source gr:stream-id="feed/http://feeds.newscientist.com/science-news"><id>tag:google.com,2005:reader/feed/http://feeds.newscientist.com/science-news</id><title type="html">New Scientist - Online News</title><link rel="alternate" href="http://www.newscientist.com/" type="text/html"/></source></entry><entry gr:crawl-timestamp-msec="1337070392217"><id gr:original-id="http://www.newscientist.com/article/dn21809">tag:google.com,2005:reader/item/7d5c7828a1537905</id><title type="html">Dust rings not 'smoking gun' for planets after all</title><published>2012-05-14T17:40:00Z</published><updated>2012-05-14T17:40:00Z</updated><link rel="alternate" href="http://feeds.newscientist.com/c/749/f/10897/s/1f58fb6f/l/0L0Snewscientist0N0Carticle0Cdn2180A90Edust0Erings0Enot0Esmoking0Egun0Efor0Eplanets0Eafter0Eall0Bhtml0DDCMP0FOTC0Erss0Gnsref0Fonline0Enews/story01.htm" type="text/html"/><summary xml:base="http://www.newscientist.com/" type="html">Sharp-edged rings of dust around stars are not necessarily carved by planets, as was thought, but can take shape on their own&lt;img width="1" height="1" src="http://feeds.newscientist.com/c/749/f/10897/s/1f58fb6f/mf.gif" border="0"&gt;&lt;div&gt;&lt;table border="0"&gt;&lt;tr&gt;&lt;td valign="middle"&gt;&lt;a href="http://share.feedsportal.com/viral/sendEmail.cfm?lang=en&amp;amp;title=Dust+rings+not+%27smoking+gun%27+for+planets+after+all&amp;amp;link=http%3A%2F%2Fwww.newscientist.com%2Farticle%2Fdn21809-dust-rings-not-smoking-gun-for-planets-after-all.html%3FDCMP%3DOTC-rss%26nsref%3Donline-news"&gt;&lt;img src="http://res3.feedsportal.com/images/emailthis2.gif" border="0"&gt;&lt;/a&gt;&lt;/td&gt;&lt;td valign="middle"&gt;&lt;a href="http://res.feedsportal.com/viral/bookmark.cfm?title=Dust+rings+not+%27smoking+gun%27+for+planets+after+all&amp;amp;link=http%3A%2F%2Fwww.newscientist.com%2Farticle%2Fdn21809-dust-rings-not-smoking-gun-for-planets-after-all.html%3FDCMP%3DOTC-rss%26nsref%3Donline-news"&gt;&lt;img src="http://res3.feedsportal.com/images/bookmark.gif" border="0"&gt;&lt;/a&gt;&lt;/td&gt;&lt;/tr&gt;&lt;/table&gt;&lt;/div&gt;&lt;br&gt;&lt;br&gt;&lt;a href="http://da.feedsportal.com/r/133515730057/u/31/f/10897/c/749/s/1f58fb6f/a2.htm"&gt;&lt;img src="http://da.feedsportal.com/r/133515730057/u/31/f/10897/c/749/s/1f58fb6f/a2.img" border="0"&gt;&lt;/a&gt;&lt;img width="1" height="1" src="http://pi.feedsportal.com/r/133515730057/u/31/f/10897/c/749/s/1f58fb6f/a2t.img" border="0"&gt;</summary><author gr:unknown-author="true"><name>(author unknown)</name></author><source gr:stream-id="feed/http://feeds.newscientist.com/science-news"><id>tag:google.com,2005:reader/feed/http://feeds.newscientist.com/science-news</id><title type="html">New Scientist - Online News</title><link rel="alternate" href="http://www.newscientist.com/" type="text/html"/></source></entry><entry gr:crawl-timestamp-msec="1336806274474"><id gr:original-id="http://www.newscientist.com/gallery/novaremnants">tag:google.com,2005:reader/item/d56daf968f678c1c</id><title type="html">Ghostly glows mark violent deaths of stars</title><published>2012-05-11T14:06:58Z</published><updated>2012-05-11T14:06:58Z</updated><link rel="alternate" href="http://feeds.newscientist.com/c/749/f/10897/s/1f438b7e/l/0L0Snewscientist0N0Cgallery0Cnovaremnants0DDCMP0FOTC0Erss0Gnsref0Fonline0Enews/story01.htm" type="text/html"/><summary xml:base="http://www.newscientist.com/" type="html">Supernovae leave glowing embers behind &#x2013; see some of the most beautiful remnants of exploding stars in our gallery&lt;img width="1" height="1" src="http://feeds.newscientist.com/c/749/f/10897/s/1f438b7e/mf.gif" border="0"&gt;&lt;div&gt;&lt;table border="0"&gt;&lt;tr&gt;&lt;td valign="middle"&gt;&lt;a href="http://share.feedsportal.com/viral/sendEmail.cfm?lang=en&amp;amp;title=Ghostly+glows+mark+violent+deaths+of+stars&amp;amp;link=http%3A%2F%2Fwww.newscientist.com%2Fgallery%2Fnovaremnants%3FDCMP%3DOTC-rss%26nsref%3Donline-news"&gt;&lt;img src="http://res3.feedsportal.com/images/emailthis2.gif" border="0"&gt;&lt;/a&gt;&lt;/td&gt;&lt;td valign="middle"&gt;&lt;a href="http://res.feedsportal.com/viral/bookmark.cfm?title=Ghostly+glows+mark+violent+deaths+of+stars&amp;amp;link=http%3A%2F%2Fwww.newscientist.com%2Fgallery%2Fnovaremnants%3FDCMP%3DOTC-rss%26nsref%3Donline-news"&gt;&lt;img src="http://res3.feedsportal.com/images/bookmark.gif" border="0"&gt;&lt;/a&gt;&lt;/td&gt;&lt;/tr&gt;&lt;/table&gt;&lt;/div&gt;&lt;br&gt;&lt;br&gt;&lt;a href="http://da.feedsportal.com/r/133515564613/u/31/f/10897/c/749/s/1f438b7e/a2.htm"&gt;&lt;img src="http://da.feedsportal.com/r/133515564613/u/31/f/10897/c/749/s/1f438b7e/a2.img" border="0"&gt;&lt;/a&gt;&lt;img width="1" height="1" src="http://pi.feedsportal.com/r/133515564613/u/31/f/10897/c/749/s/1f438b7e/a2t.img" border="0"&gt;</summary><author gr:unknown-author="true"><name>(author unknown)</name></author><source gr:stream-id="feed/http://feeds.newscientist.com/science-news"><id>tag:google.com,2005:reader/feed/http://feeds.newscientist.com/science-news</id><title type="html">New Scientist - Online News</title><link rel="alternate" href="http://www.newscientist.com/" type="text/html"/></source></entry></feed>

