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<item><guid isPermaLink="false">http://www.zazzle.com/starburst_galaxy_ngc_1569_mousepad-144574115820510574?gl=les_etoiles</guid><pubDate>Wed, 17 Dec 2008 00:21:10 GMT</pubDate><title><![CDATA[Starburst Galaxy NGC 1569]]></title><link>http://www.zazzle.com/starburst_galaxy_ngc_1569_mousepad-144574115820510574?gl=les_etoiles</link><author>les_etoiles</author><description><![CDATA[
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		>Starburst Galaxy NGC 1569</a><br />
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</div>]]></description><media:title><![CDATA[Starburst Galaxy NGC 1569]]></media:title><media:description><![CDATA[&quot;This image taken by NASA's Hubble Space Telescope showcases the brilliant core of one of the most active galaxies in our local neighborhood. The entire core is 5,000 light-years wide.<br /><br />The galaxy, called NGC 1569, sparkles with the light from millions of newly formed young stars. NGC 1569 is pumping out stars at a rate that is 100 times faster than the rate observed in our Milky Way Galaxy. This frenzied pace has been almost continuous for the past 100 million years.<br /><br />A new analysis of NGC 1569 shows that it is one and a half times farther from Earth than astronomers previously thought. The extra distance places the galaxy in the middle of a group of about 10 galaxies centered on the spiral galaxy IC 342. Gravitational interactions among the group's galaxies may be compressing gas in NGC 1569 and igniting the star-birthing frenzy.&quot;<br /><br />(qtd. from Hubblesite.org NewsCenter release <a target="_blank" href="http://hubblesite.org/newscenter/archive/releases/2008/38/" rel="nofollow">STScI-2008-38</a>)<br /><br />Credit: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Aloisi (STScI/ESA)]]></media:description><media:thumbnail url="http://rlv.zcache.com/starburst_galaxy_ngc_1569_mousepad-p144574115820510574td22_125.jpg" /><media:content url="http://rlv.zcache.com/starburst_galaxy_ngc_1569_mousepad-p144574115820510574td22_500.jpg" /><media:keywords>astronomy, deep space, galaxy, galaxies, hubble, hst, hubble telescope, nasa</media:keywords><media:rating scheme="urn:mpaa">g</media:rating></item>
<item><guid isPermaLink="false">http://www.zazzle.com/star_forming_region_ngc_3324_mousepad-144959809365300579?gl=les_etoiles</guid><pubDate>Wed, 17 Dec 2008 00:15:29 GMT</pubDate><title><![CDATA[Star-forming Region NGC 3324]]></title><link>http://www.zazzle.com/star_forming_region_ngc_3324_mousepad-144959809365300579?gl=les_etoiles</link><author>les_etoiles</author><description><![CDATA[
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		>Star-forming Region NGC 3324</a><br />
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</div>]]></description><media:title><![CDATA[Star-forming Region NGC 3324]]></media:title><media:description><![CDATA[&quot;The landmark 10th anniversary of the Hubble Space Telescope's Hubble Heritage Project is being celebrated with a 'landscape' image from the cosmos. Cutting across a nearby star-forming region, called NGC 3324, are the &quot;hills and valleys&quot; of gas and dust displayed in intricate detail. Set amid a backdrop of soft, glowing blue light are wispy tendrils of gas as well as dark trunks of dust that are light-years in height. NGC 3324 is located in the constellation Carina, about 7,200 light-years away from Earth.<br /><br />The Hubble Heritage Project, which began in October 1998, has released nearly 130 images mined from the Hubble data archive as well as a number of observations taken specifically for the project. By releasing a new, previously unseen Hubble image every month, the team's intent was to showcase some of the most attractive images ever taken by the Hubble telescope, and share them with a wide audience. The Heritage team continues to create aesthetic images that present the universe from an artistic perspective.&quot;<br /><br />(qtd. from Hubblesite.org NewsCenter release <a target="_blank" href="http://hubblesite.org/newscenter/archive/releases/2008/34/" rel="nofollow">STScI-2008-34</a>)<br /><br />Credit: NASA, ESA, and The Hubble Heritage Team (STScI/AURA)]]></media:description><media:thumbnail url="http://rlv.zcache.com/star_forming_region_ngc_3324_mousepad-p144959809365300579td22_125.jpg" /><media:content url="http://rlv.zcache.com/star_forming_region_ngc_3324_mousepad-p144959809365300579td22_500.jpg" /><media:keywords>astronomy, deep space, nebula, nebulae, star-forming, region, hubble, hst, hubble telescope, nasa</media:keywords><media:rating scheme="urn:mpaa">g</media:rating></item>
<item><guid isPermaLink="false">http://www.zazzle.com/elliptical_galaxy_ngc_1275_perseus_a_mousepad-144976427623607667?gl=les_etoiles</guid><pubDate>Wed, 17 Dec 2008 00:10:58 GMT</pubDate><title><![CDATA[Elliptical Galaxy NGC 1275 - Perseus A]]></title><link>http://www.zazzle.com/elliptical_galaxy_ngc_1275_perseus_a_mousepad-144976427623607667?gl=les_etoiles</link><author>les_etoiles</author><description><![CDATA[
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</div>]]></description><media:title><![CDATA[Elliptical Galaxy NGC 1275 - Perseus A]]></media:title><media:description><![CDATA[&quot;This Hubble Space Telescope image of galaxy NGC 1275 reveals the fine, thread-like filamentary structures in the gas surrounding the galaxy. The red filaments are composed of cool gas being suspended by a magnetic field, and are surrounded by the 100-million-degree Fahrenheit hot gas in the center of the Perseus galaxy cluster.<br /><br />The filaments are dramatic markers of the feedback process through which energy is transferred from the central massive black hole to the surrounding gas. The filaments originate when cool gas is transported from the center of the galaxy by radio bubbles that rise in the hot interstellar gas.&quot;<br /><br />(qtd. from Hubblesite.org NewsCenter release <a target="_blank" href="http://hubblesite.org/newscenter/archive/releases/2008/28/" rel="nofollow">STScI-2008-28</a>)<br /><br />Credit: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration]]></media:description><media:thumbnail url="http://rlv.zcache.com/elliptical_galaxy_ngc_1275_perseus_a_mousepad-p144976427623607667td22_125.jpg" /><media:content url="http://rlv.zcache.com/elliptical_galaxy_ngc_1275_perseus_a_mousepad-p144976427623607667td22_500.jpg" /><media:keywords>astronomy, deep space, galaxy, galaxies, hubble, hst, hubble telescope, nasa</media:keywords><media:rating scheme="urn:mpaa">g</media:rating></item>
<item><guid isPermaLink="false">http://www.zazzle.com/globular_cluster_ngc_6791_mousepad-144932063938843196?gl=les_etoiles</guid><pubDate>Tue, 16 Dec 2008 23:52:13 GMT</pubDate><title><![CDATA[Globular Cluster NGC 6791]]></title><link>http://www.zazzle.com/globular_cluster_ngc_6791_mousepad-144932063938843196?gl=les_etoiles</link><author>les_etoiles</author><description><![CDATA[
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		>Globular Cluster NGC 6791</a><br />
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</div>]]></description><media:title><![CDATA[Globular Cluster NGC 6791]]></media:title><media:description><![CDATA[&quot;In studying the dimmest burned-out stars in globular star cluster NGC 6791, NASA's Hubble Space Telescope has uncovered a paradox: three different populations of stars exist in an object where all the stars should have formed at the same time out of an interstellar cloud of gas and dust.<br /><br />...Two of the populations are burned-out stars called white dwarfs. One group of these low-wattage stellar remnants (red circles) appears to be 6 billion years old, another (blue circles) appears to be 4 billion years old. The ages are out of sync with those of the cluster's normal stars, which are 8 billion years old.&quot;<br /><br />(qtd. from Hubblesite.org NewsCenter release <a target="_blank" href="http://hubblesite.org/newscenter/releases/2008/25/" rel="nofollow">STScI-2008-25</a>)<br /><br />Credit: NASA, ESA, and L. Bedin (STScI)]]></media:description><media:thumbnail url="http://rlv.zcache.com/globular_cluster_ngc_6791_mousepad-p144932063938843196td22_125.jpg" /><media:content url="http://rlv.zcache.com/globular_cluster_ngc_6791_mousepad-p144932063938843196td22_500.jpg" /><media:keywords>astronomy, deep space, star, star cluster, hubble, hst, hubble telescope, nasa</media:keywords><media:rating scheme="urn:mpaa">g</media:rating></item>
<item><guid isPermaLink="false">http://www.zazzle.com/coma_cluster_abell_1656_mousepad-144514768566997165?gl=les_etoiles</guid><pubDate>Tue, 16 Dec 2008 23:50:51 GMT</pubDate><title><![CDATA[Coma Cluster (Abell 1656)]]></title><link>http://www.zazzle.com/coma_cluster_abell_1656_mousepad-144514768566997165?gl=les_etoiles</link><author>les_etoiles</author><description><![CDATA[
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</div>]]></description><media:title><![CDATA[Coma Cluster (Abell 1656)]]></media:title><media:description><![CDATA[&quot;NASA's Hubble Space Telescope captures the magnificent starry population of the Coma Cluster of galaxies, one of the densest known galaxy collections in the universe. The Hubble's Advanced Camera for Surveys viewed a large portion of the cluster, spanning several million light-years across. The entire cluster contains thousands of galaxies in a spherical shape more than 20 million light-years in diameter.&quot;<br /><br />(qtd. from Hubblesite.org NewsCenter release <a target="_blank" href="http://hubblesite.org/newscenter/releases/2008/24/" rel="nofollow">STScI-2008-24</a>)<br /><br />Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)]]></media:description><media:thumbnail url="http://rlv.zcache.com/coma_cluster_abell_1656_mousepad-p144514768566997165td22_125.jpg" /><media:content url="http://rlv.zcache.com/coma_cluster_abell_1656_mousepad-p144514768566997165td22_500.jpg" /><media:keywords>astronomy, deep space, galaxy, cluster, galaxies, hubble, hst, hubble telescope, nasa</media:keywords><media:rating scheme="urn:mpaa">g</media:rating></item>
<item><guid isPermaLink="false">http://www.zazzle.com/sn_1006_supernova_remnant_mousepad-144452154871293275?gl=les_etoiles</guid><pubDate>Tue, 16 Dec 2008 23:49:49 GMT</pubDate><title><![CDATA[SN 1006 Supernova Remnant]]></title><link>http://www.zazzle.com/sn_1006_supernova_remnant_mousepad-144452154871293275?gl=les_etoiles</link><author>les_etoiles</author><description><![CDATA[
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</div>]]></description><media:title><![CDATA[SN 1006 Supernova Remnant]]></media:title><media:description><![CDATA[&quot;On or around May 1, 1006 A.D., observers from Africa to Europe to the Far East witnessed and recorded the arrival of light from what is now called SN 1006, a tremendous supernova explosion caused by the final death throes of a white dwarf star nearly 7,000 light-years away. The supernova was probably the brightest star ever seen by humans, and surpassed Venus as the brightest object in the night time sky, only to be surpassed by the moon. It was visible even during the day for weeks, and remained visible to the naked eye for at least two and a half years before fading away.<br /><br />It wasn't until the mid-1960s that radio astronomers first detected a nearly circular ring of material at the recorded position of the supernova. The ring was almost 30 arcminutes across, the same angular diameter as the full moon. The size of the remnant implied that the blast wave from the supernova had expanded at nearly 20 million miles per hour over the nearly 1,000 years since the explosion occurred.&quot;<br /><br />(qtd. from Hubblesite.org NewsCenter release <a target="_blank" href="http://hubblesite.org/newscenter/releases/2008/22/" rel="nofollow">STScI-2008-22</a>)<br /><br />Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)]]></media:description><media:thumbnail url="http://rlv.zcache.com/sn_1006_supernova_remnant_mousepad-p144452154871293275td22_125.jpg" /><media:content url="http://rlv.zcache.com/sn_1006_supernova_remnant_mousepad-p144452154871293275td22_500.jpg" /><media:keywords>astronomy, deep space, nebula, nebulae, supernova, remnant, hubble, hst, hubble telescope, nasa</media:keywords><media:rating scheme="urn:mpaa">g</media:rating></item>
<item><guid isPermaLink="false">http://www.zazzle.com/interacting_galaxies_12_mousepad-144875366357731434?gl=les_etoiles</guid><pubDate>Tue, 16 Dec 2008 23:48:33 GMT</pubDate><title><![CDATA[Interacting Galaxies (12)]]></title><link>http://www.zazzle.com/interacting_galaxies_12_mousepad-144875366357731434?gl=les_etoiles</link><author>les_etoiles</author><description><![CDATA[
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		>Interacting Galaxies (12)</a><br />
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</div>]]></description><media:title><![CDATA[Interacting Galaxies (12)]]></media:title><media:description><![CDATA[&quot;Astronomy textbooks typically present galaxies as staid, solitary, and majestic island worlds of glittering stars.<br /><br />But galaxies have a dynamical side. They have close encounters that sometimes end in grand mergers and overflowing sites of new star birth as the colliding galaxies morph into wondrous new shapes.<br /><br />...For all their violence, galactic smash-ups take place at a glacial rate by human standards - timescales on the order of several hundred million years. The images in the Hubble atlas capture snapshots of the various merging galaxies at various stages in their collision.&quot;<br /><br />(qtd. from Hubblesite.org NewsCenter release <a target="_blank" href="http://hubblesite.org/newscenter/releases/2008/16/" rel="nofollow">STScI-2008-16</a>)<br /><br />Credit: NASA, ESA, the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration, and A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University)]]></media:description><media:thumbnail url="http://rlv.zcache.com/interacting_galaxies_12_mousepad-p144875366357731434td22_125.jpg" /><media:content url="http://rlv.zcache.com/interacting_galaxies_12_mousepad-p144875366357731434td22_500.jpg" /><media:keywords>astronomy, deep space, galaxy, galaxies, hubble, hst, hubble telescope, nasa</media:keywords><media:rating scheme="urn:mpaa">g</media:rating></item>
<item><guid isPermaLink="false">http://www.zazzle.com/interacting_galaxies_59_mousepad-144487739639612253?gl=les_etoiles</guid><pubDate>Tue, 16 Dec 2008 23:46:56 GMT</pubDate><title><![CDATA[Interacting Galaxies (59)]]></title><link>http://www.zazzle.com/interacting_galaxies_59_mousepad-144487739639612253?gl=les_etoiles</link><author>les_etoiles</author><description><![CDATA[
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</div>]]></description><media:title><![CDATA[Interacting Galaxies (59)]]></media:title><media:description><![CDATA[&quot;Astronomy textbooks typically present galaxies as staid, solitary, and majestic island worlds of glittering stars. But galaxies have a dynamical side. They have close encounters that sometimes end in grand mergers and overflowing sites of new star birth as the colliding galaxies morph into wondrous new shapes. Today, in celebration of the Hubble Space Telescope's 18th launch anniversary, this poster with 59 views of colliding galaxies constitute the largest collection of Hubble images ever released to the public. This new Hubble atlas dramatically illustrates how galaxy collisions produce a remarkable variety of intricate structures in never-before-seen detail.&quot;<br /><br />(qtd. from Hubblesite.org NewsCenter release <a target="_blank" href="http://hubblesite.org/newscenter/releases/2008/16/" rel="nofollow">STScI-2008-16</a>)<br /><br />Credit: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration]]></media:description><media:thumbnail url="http://rlv.zcache.com/interacting_galaxies_59_mousepad-p144487739639612253td22_125.jpg" /><media:content url="http://rlv.zcache.com/interacting_galaxies_59_mousepad-p144487739639612253td22_500.jpg" /><media:keywords>astronomy, deep space, galaxy, galaxies, hubble, hst, hubble telescope, nasa</media:keywords><media:rating scheme="urn:mpaa">g</media:rating></item>
<item><guid isPermaLink="false">http://www.zazzle.com/core_of_omega_centauri_ngc_2371_mousepad-144593755913318204?gl=les_etoiles</guid><pubDate>Tue, 16 Dec 2008 23:45:31 GMT</pubDate><title><![CDATA[Core of Omega Centauri (NGC 2371)]]></title><link>http://www.zazzle.com/core_of_omega_centauri_ngc_2371_mousepad-144593755913318204?gl=les_etoiles</link><author>les_etoiles</author><description><![CDATA[
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<item><guid isPermaLink="false">http://www.zazzle.com/elliptical_galaxy_ngc_1132_mousepad-144191114097454784?gl=les_etoiles</guid><pubDate>Tue, 16 Dec 2008 23:43:33 GMT</pubDate><title><![CDATA[Elliptical Galaxy NGC 1132]]></title><link>http://www.zazzle.com/elliptical_galaxy_ngc_1132_mousepad-144191114097454784?gl=les_etoiles</link><author>les_etoiles</author><description><![CDATA[
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<item><guid isPermaLink="false">http://www.zazzle.com/dwarf_galaxy_holmberg_ix_mousepad-144978560468311331?gl=les_etoiles</guid><pubDate>Tue, 16 Dec 2008 23:40:52 GMT</pubDate><title><![CDATA[Dwarf Galaxy Holmberg IX]]></title><link>http://www.zazzle.com/dwarf_galaxy_holmberg_ix_mousepad-144978560468311331?gl=les_etoiles</link><author>les_etoiles</author><description><![CDATA[
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<item><guid isPermaLink="false">http://www.zazzle.com/starburst_galaxy_ngc_1569_large_postage-172815239312927319?gl=les_etoiles</guid><pubDate>Tue, 16 Dec 2008 01:59:01 GMT</pubDate><title><![CDATA[Starburst Galaxy NGC 1569 - large]]></title><link>http://www.zazzle.com/starburst_galaxy_ngc_1569_large_postage-172815239312927319?gl=les_etoiles</link><author>les_etoiles</author><description><![CDATA[
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<item><guid isPermaLink="false">http://www.zazzle.com/star_forming_region_ngc_3324_large_postage-172296073285085137?gl=les_etoiles</guid><pubDate>Tue, 16 Dec 2008 01:58:04 GMT</pubDate><title><![CDATA[Star-forming Region NGC 3324 - large]]></title><link>http://www.zazzle.com/star_forming_region_ngc_3324_large_postage-172296073285085137?gl=les_etoiles</link><author>les_etoiles</author><description><![CDATA[
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<item><guid isPermaLink="false">http://www.zazzle.com/star_forming_nebula_near_ngc_2074_large_postage-172849767685746408?gl=les_etoiles</guid><pubDate>Tue, 16 Dec 2008 01:56:18 GMT</pubDate><title><![CDATA[Star-forming Nebula near NGC 2074 - large]]></title><link>http://www.zazzle.com/star_forming_nebula_near_ngc_2074_large_postage-172849767685746408?gl=les_etoiles</link><author>les_etoiles</author><description><![CDATA[
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<item><guid isPermaLink="false">http://www.zazzle.com/elliptical_galaxy_ngc_1275_perseus_a_large_postage-172385656898177018?gl=les_etoiles</guid><pubDate>Tue, 16 Dec 2008 01:53:54 GMT</pubDate><title><![CDATA[Elliptical Galaxy NGC 1275 - Perseus A - large]]></title><link>http://www.zazzle.com/elliptical_galaxy_ngc_1275_perseus_a_large_postage-172385656898177018?gl=les_etoiles</link><author>les_etoiles</author><description><![CDATA[
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