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<rss version="2.0" xmlns:opensearch="http://a9.com/-/spec/opensearch/1.1/" xmlns:media="http://search.yahoo.com/mrss/"><channel><title>Galactica - Astronomy and Space Gifts: Zazzle.com Gallery: Products </title><link>http://feed.zazzle.com/z.2/api/find.aspx?ft=rss&amp;ch=Galactica&amp;ou=/Galactica/rss</link><description></description><language>en-us</language><pubDate>Thu, 26 Nov 2009 00:27:25 GMT</pubDate><ttl>60</ttl><opensearch:totalResults>79</opensearch:totalResults><opensearch:startIndex>1</opensearch:startIndex><opensearch:itemsPerPage>15</opensearch:itemsPerPage><opensearch:Query role="request" searchTerms="" />
<item><guid isPermaLink="false">http://www.zazzle.com/the_heart_of_the_milky_way_galaxy_2009_poster-228097447328597240?gl=Galactica</guid><pubDate>Fri, 13 Nov 2009 16:46:57 GMT</pubDate><title><![CDATA[The Heart of The Milky Way Galaxy 2009]]></title><link>http://www.zazzle.com/the_heart_of_the_milky_way_galaxy_2009_poster-228097447328597240?gl=Galactica</link><author>Galactica</author><description><![CDATA[
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		>The Heart of The Milky Way Galaxy 2009</a><br />
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</div>]]></description><media:title><![CDATA[The Heart of The Milky Way Galaxy 2009]]></media:title><media:description><![CDATA[A never-before-seen view of the turbulent heart of our Milky Way galaxy is being unveiled by NASA on Nov. 10. This event will commemorate the 400 years since Galileo first turned his telescope to the heavens in 1609. In celebration of this International Year of Astronomy, NASA is releasing images of the galactic center region as seen by its Great Observatories to more than 150 planetariums, museums, nature centers, libraries, and schools across the country. The sites will unveil a giant, 6-foot-by-3-foot print of the bustling hub of our galaxy that combines a near-infrared view from the Hubble Space Telescope, an infrared view from the Spitzer Space Telescope, and an X-ray view from the Chandra X-ray Observatory into one multiwavelength picture. Experts from all three observatories carefully assembled the final image from large mosaic photo surveys taken by each telescope. This composite image provides one of the most detailed views ever of our galaxy's mysterious core. Participating institutions also will display a matched trio of Hubble, Spitzer, and Chandra images of the Milky Way's center on a second large panel measuring 3 feet by 4 feet. Each image shows the telescope's different wavelength view of the galactic center region, illustrating not only the unique science each observatory conducts, but also how far astronomy has come since Galileo. The composite image features the spectacle of stellar evolution: from vibrant regions of star birth, to young hot stars, to old cool stars, to seething remnants of stellar death called black holes. This activity occurs against a fiery backdrop in the crowded, hostile environment of the galaxy's core, the center of which is dominated by a supermassive black hole nearly four million times more massive than our Sun. Permeating the region is a diffuse blue haze of X-ray light from gas that has been heated to millions of degrees by outflows from the supermassive black hole as well as by winds from massive stars and by stellar explosions. Infrared light reveals more than a hundred thousand stars along with glowing dust clouds that create complex structures including compact globules, long filaments, and finger-like &quot;pillars of creation,&quot; where newborn stars are just beginning to break out of their dark, dusty cocoons.Courtesy: NASA.]]></media:description><media:thumbnail url="http://rlv.zcache.com/the_heart_of_the_milky_way_galaxy_2009_poster-p228097447328597240td2a_125.jpg" /><media:content url="http://rlv.zcache.com/the_heart_of_the_milky_way_galaxy_2009_poster-p228097447328597240td2a_500.jpg" /><media:keywords>nasa, galaxies, galaxy, space, prints, posters, poster, print, milky way, stars, nebula</media:keywords><media:rating scheme="urn:mpaa">g</media:rating></item>
<item><guid isPermaLink="false">http://www.zazzle.com/the_whirlpool_galaxy_m51_print-228104261153891072?gl=Galactica</guid><pubDate>Mon, 14 Sep 2009 18:47:16 GMT</pubDate><title><![CDATA[The Whirlpool Galaxy M51 Print]]></title><link>http://www.zazzle.com/the_whirlpool_galaxy_m51_print-228104261153891072?gl=Galactica</link><author>Galactica</author><description><![CDATA[
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		>The Whirlpool Galaxy M51 Print</a><br />
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</div>]]></description><media:title><![CDATA[The Whirlpool Galaxy M51 Print]]></media:title><media:description><![CDATA[The graceful, winding arms of the majestic spiral galaxy M51 (NGC 5194) appear like a grand spiral staircase sweeping through space. They are actually long lanes of stars and gas laced with dust. This sharpest-ever image of the Whirlpool Galaxy, taken in January 2005 with the Advanced Camera for Surveys aboard NASA's Hubble Space Telescope, illustrates a spiral galaxy's grand design, from its curving spiral arms, where young stars reside, to its yellowish central core, a home of older stars. The galaxy is nicknamed the Whirlpool because of its swirling structure. The Whirlpool's most striking feature is its two curving arms, a hallmark of so-called grand-design spiral galaxies. Many spiral galaxies possess numerous, loosely shaped arms which make their spiral structure less pronounced. These arms serve an important purpose in spiral galaxies. They are star-formation factories, compressing hydrogen gas and creating clusters of new stars. In the Whirlpool, the assembly line begins with the dark clouds of gas on the inner edge, then moves to bright pink star-forming regions, and ends with the brilliant blue star clusters along the outer edge. Some astronomers believe that the Whirlpool's arms are so prominent because of the effects of a close encounter with NGC 5195, the small, yellowish galaxy at the outermost tip of one of the Whirlpool's arms. At first glance, the compact galaxy appears to be tugging on the arm. Hubble's clear view, however, shows that NGC 5195 is passing behind the Whirlpool. The small galaxy has been gliding past the Whirlpool for hundreds of millions of years. As NGC 5195 drifts by, its gravitational muscle pumps up waves within the Whirlpool's pancake-shaped disk. The waves are like ripples in a pond generated when a rock is thrown in the water. When the waves pass through orbiting gas clouds within the disk, they squeeze the gaseous material along each arm's inner edge. The dark dusty material looks like gathering storm clouds. These dense clouds collapse, creating a wake of star birth, as seen in the bright pink star-forming regions. The largest stars eventually sweep away the dusty cocoons with a torrent of radiation, hurricane-like stellar winds, and shock waves from supernova blasts. Bright blue star clusters emerge from the mayhem, illuminating the Whirlpool's arms like city streetlights. The Whirlpool is one of astronomy's galactic darlings. Located 31 million light-years away in the constellation Canes Venatici (the Hunting Dogs), the Whirlpool's beautiful face-on view and closeness to Earth allow astronomers to study a classic spiral galaxy's structure and star-forming processes. Photograph and description courtesy NASA,]]></media:description><media:thumbnail url="http://rlv.zcache.com/the_whirlpool_galaxy_m51_print-p228104261153891072td2a_125.jpg" /><media:content url="http://rlv.zcache.com/the_whirlpool_galaxy_m51_print-p228104261153891072td2a_500.jpg" /><media:keywords>nasa, astronomy, prints, posters, galaxy, galaxies, stars, star, space, hubble, beautiful, cosmos, science</media:keywords><media:rating scheme="urn:mpaa">g</media:rating></item>
<item><guid isPermaLink="false">http://www.zazzle.com/jupiter_tshirt-235209160014168687?gl=Galactica</guid><pubDate>Fri, 11 Sep 2009 23:20:11 GMT</pubDate><title><![CDATA[Jupiter]]></title><link>http://www.zazzle.com/jupiter_tshirt-235209160014168687?gl=Galactica</link><author>Galactica</author><description><![CDATA[
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<item><guid isPermaLink="false">http://www.zazzle.com/a_ring_of_dark_matter_tshirt-235941282778091654?gl=Galactica</guid><pubDate>Fri, 11 Sep 2009 18:55:17 GMT</pubDate><title><![CDATA[A Ring of Dark Matter]]></title><link>http://www.zazzle.com/a_ring_of_dark_matter_tshirt-235941282778091654?gl=Galactica</link><author>Galactica</author><description><![CDATA[
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</div>]]></description><media:title><![CDATA[A Ring of Dark Matter]]></media:title><media:description><![CDATA[A Ring of Dark Matter T-Shirt. Hubble discovers a ring of dark matter. Source: NASA,]]></media:description><media:thumbnail url="http://rlv.zcache.com/a_ring_of_dark_matter_tshirt-p235941282778091654tr3q_125.jpg" /><media:content url="http://rlv.zcache.com/a_ring_of_dark_matter_tshirt-p235941282778091654tr3q_500.jpg" /><media:keywords>astronomy, space, galaxies, dark matter, tshirt, shirts, blue, beautiful</media:keywords><media:rating scheme="urn:mpaa">g</media:rating></item>
<item><guid isPermaLink="false">http://www.zazzle.com/the_beautiful_pleiades_shirt-235237416283179363?gl=Galactica</guid><pubDate>Fri, 11 Sep 2009 18:46:03 GMT</pubDate><title><![CDATA[The Beautiful Pleiades Shirt]]></title><link>http://www.zazzle.com/the_beautiful_pleiades_shirt-235237416283179363?gl=Galactica</link><author>Galactica</author><description><![CDATA[
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<item><guid isPermaLink="false">http://www.zazzle.com/turbulent_star_birth_region_selection_print-228812515810392219?gl=Galactica</guid><pubDate>Sun, 30 Nov 2008 23:04:14 GMT</pubDate><title><![CDATA[Turbulent Star-Birth Region Selection Print]]></title><link>http://www.zazzle.com/turbulent_star_birth_region_selection_print-228812515810392219?gl=Galactica</link><author>Galactica</author><description><![CDATA[
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		>Turbulent Star-Birth Region Selection Print</a><br />
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</div>]]></description><media:title><![CDATA[Turbulent Star-Birth Region Selection Print]]></media:title><media:description><![CDATA[In commemoration of NASA's Hubble Space Telescope completing its 100,000th orbit in its 18th year of exploration and discovery, scientists at the Space Telescope Science Institute in Baltimore, Md., have aimed Hubble to take a snapshot of a dazzling region of celestial birth and renewal.

Hubble peered into a small portion of the nebula near the star cluster NGC 2074 (upper, left). The region is a firestorm of raw stellar creation, perhaps triggered by a nearby supernova explosion. It lies about 170,000 light-years away near the Tarantula nebula, one of the most active star-forming regions in our Local Group of galaxies.

The three-dimensional-looking image reveals dramatic ridges and valleys of dust, serpent-head &quot;pillars of creation,&quot; and gaseous filaments glowing fiercely under torrential ultraviolet radiation. The region is on the edge of a dark molecular cloud that is an incubator for the birth of new stars.

The high-energy radiation blazing out from clusters of hot young stars already born in NGC 2074 is sculpting the wall of the nebula by slowly eroding it away. Another young cluster may be hidden beneath a circle of brilliant blue gas at center, bottom.

In this approximately 100-light-year-wide fantasy-like landscape, dark towers of dust rise above a glowing wall of gases on the surface of the molecular cloud. The seahorse-shaped pillar at lower, right is approximately 20 light-years long, roughly four times the distance between our Sun and the nearest star, Alpha Centauri.

The region is in the Large Magellanic Cloud (LMC), a satellite of our Milky Way galaxy. It is a fascinating laboratory for observing star-formation regions and their evolution. Dwarf galaxies like the LMC are considered to be the primitive building blocks of larger galaxies.

This representative color image was taken on August 10, 2008, with Hubble's Wide Field Planetary Camera 2. Red shows emission from sulfur atoms, green from glowing hydrogen, and blue from glowing oxygen. Source: NASA]]></media:description><media:thumbnail url="http://rlv.zcache.com/turbulent_star_birth_region_selection_print-p228812515810392219td2a_125.jpg" /><media:content url="http://rlv.zcache.com/turbulent_star_birth_region_selection_print-p228812515810392219td2a_500.jpg" /><media:keywords>hubble, nasa, stars, star, galaxy, galaxies, space, astronomy, nasa, hubble, telescope, beautiful, postcard, postcards, photos, photograph, gift, gifts, nebula</media:keywords><media:rating scheme="urn:mpaa">g</media:rating></item>
<item><guid isPermaLink="false">http://www.zazzle.com/turbulent_star_birth_region_selection_mug-168506109569977954?gl=Galactica</guid><pubDate>Sun, 30 Nov 2008 23:02:06 GMT</pubDate><title><![CDATA[Turbulent Star-Birth Region Selection]]></title><link>http://www.zazzle.com/turbulent_star_birth_region_selection_mug-168506109569977954?gl=Galactica</link><author>Galactica</author><description><![CDATA[
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		>Turbulent Star-Birth Region Selection</a><br />
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</div>]]></description><media:title><![CDATA[Turbulent Star-Birth Region Selection]]></media:title><media:description><![CDATA[In commemoration of NASA's Hubble Space Telescope completing its 100,000th orbit in its 18th year of exploration and discovery, scientists at the Space Telescope Science Institute in Baltimore, Md., have aimed Hubble to take a snapshot of a dazzling region of celestial birth and renewal.

Hubble peered into a small portion of the nebula near the star cluster NGC 2074 (upper, left). The region is a firestorm of raw stellar creation, perhaps triggered by a nearby supernova explosion. It lies about 170,000 light-years away near the Tarantula nebula, one of the most active star-forming regions in our Local Group of galaxies.

The three-dimensional-looking image reveals dramatic ridges and valleys of dust, serpent-head &quot;pillars of creation,&quot; and gaseous filaments glowing fiercely under torrential ultraviolet radiation. The region is on the edge of a dark molecular cloud that is an incubator for the birth of new stars.

The high-energy radiation blazing out from clusters of hot young stars already born in NGC 2074 is sculpting the wall of the nebula by slowly eroding it away. Another young cluster may be hidden beneath a circle of brilliant blue gas at center, bottom.

In this approximately 100-light-year-wide fantasy-like landscape, dark towers of dust rise above a glowing wall of gases on the surface of the molecular cloud. The seahorse-shaped pillar at lower, right is approximately 20 light-years long, roughly four times the distance between our Sun and the nearest star, Alpha Centauri.

The region is in the Large Magellanic Cloud (LMC), a satellite of our Milky Way galaxy. It is a fascinating laboratory for observing star-formation regions and their evolution. Dwarf galaxies like the LMC are considered to be the primitive building blocks of larger galaxies.

This representative color image was taken on August 10, 2008, with Hubble's Wide Field Planetary Camera 2. Red shows emission from sulfur atoms, green from glowing hydrogen, and blue from glowing oxygen. Source: NASA.]]></media:description><media:thumbnail url="http://rlv.zcache.com/turbulent_star_birth_region_selection_mug-p1685061095699779542obaq_125.jpg" /><media:content url="http://rlv.zcache.com/turbulent_star_birth_region_selection_mug-p1685061095699779542obaq_500.jpg" /><media:keywords>hubble, nasa, stars, star, galaxy, galaxies, space, astronomy, nasa, hubble, telescope, beautiful, postcard, postcards, photos, photograph, gift, gifts, nebula</media:keywords><media:rating scheme="urn:mpaa">g</media:rating></item>
<item><guid isPermaLink="false">http://www.zazzle.com/turbulent_star_birth_region_selection_mousepad-144168423267481043?gl=Galactica</guid><pubDate>Sun, 30 Nov 2008 23:02:06 GMT</pubDate><title><![CDATA[Turbulent Star-Birth Region Selection]]></title><link>http://www.zazzle.com/turbulent_star_birth_region_selection_mousepad-144168423267481043?gl=Galactica</link><author>Galactica</author><description><![CDATA[
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</div>]]></description><media:title><![CDATA[Turbulent Star-Birth Region Selection]]></media:title><media:description><![CDATA[In commemoration of NASA's Hubble Space Telescope completing its 100,000th orbit in its 18th year of exploration and discovery, scientists at the Space Telescope Science Institute in Baltimore, Md., have aimed Hubble to take a snapshot of a dazzling region of celestial birth and renewal.

Hubble peered into a small portion of the nebula near the star cluster NGC 2074 (upper, left). The region is a firestorm of raw stellar creation, perhaps triggered by a nearby supernova explosion. It lies about 170,000 light-years away near the Tarantula nebula, one of the most active star-forming regions in our Local Group of galaxies.

The three-dimensional-looking image reveals dramatic ridges and valleys of dust, serpent-head &quot;pillars of creation,&quot; and gaseous filaments glowing fiercely under torrential ultraviolet radiation. The region is on the edge of a dark molecular cloud that is an incubator for the birth of new stars.

The high-energy radiation blazing out from clusters of hot young stars already born in NGC 2074 is sculpting the wall of the nebula by slowly eroding it away. Another young cluster may be hidden beneath a circle of brilliant blue gas at center, bottom.

In this approximately 100-light-year-wide fantasy-like landscape, dark towers of dust rise above a glowing wall of gases on the surface of the molecular cloud. The seahorse-shaped pillar at lower, right is approximately 20 light-years long, roughly four times the distance between our Sun and the nearest star, Alpha Centauri.

The region is in the Large Magellanic Cloud (LMC), a satellite of our Milky Way galaxy. It is a fascinating laboratory for observing star-formation regions and their evolution. Dwarf galaxies like the LMC are considered to be the primitive building blocks of larger galaxies.

This representative color image was taken on August 10, 2008, with Hubble's Wide Field Planetary Camera 2. Red shows emission from sulfur atoms, green from glowing hydrogen, and blue from glowing oxygen. Source: NASA.]]></media:description><media:thumbnail url="http://rlv.zcache.com/turbulent_star_birth_region_selection_mousepad-p144168423267481043td22_125.jpg" /><media:content url="http://rlv.zcache.com/turbulent_star_birth_region_selection_mousepad-p144168423267481043td22_500.jpg" /><media:keywords>hubble, nasa, stars, star, galaxy, galaxies, space, astronomy, nasa, hubble, telescope, beautiful, postcard, postcards, photos, photograph, gift, gifts, nebula</media:keywords><media:rating scheme="urn:mpaa">g</media:rating></item>
<item><guid isPermaLink="false">http://www.zazzle.com/turbulent_star_birth_region_selection_postcard-239185416537268522?gl=Galactica</guid><pubDate>Sun, 30 Nov 2008 23:02:05 GMT</pubDate><title><![CDATA[Turbulent Star-Birth Region Selection]]></title><link>http://www.zazzle.com/turbulent_star_birth_region_selection_postcard-239185416537268522?gl=Galactica</link><author>Galactica</author><description><![CDATA[
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Hubble peered into a small portion of the nebula near the star cluster NGC 2074 (upper, left). The region is a firestorm of raw stellar creation, perhaps triggered by a nearby supernova explosion. It lies about 170,000 light-years away near the Tarantula nebula, one of the most active star-forming regions in our Local Group of galaxies.

The three-dimensional-looking image reveals dramatic ridges and valleys of dust, serpent-head &quot;pillars of creation,&quot; and gaseous filaments glowing fiercely under torrential ultraviolet radiation. The region is on the edge of a dark molecular cloud that is an incubator for the birth of new stars.

The high-energy radiation blazing out from clusters of hot young stars already born in NGC 2074 is sculpting the wall of the nebula by slowly eroding it away. Another young cluster may be hidden beneath a circle of brilliant blue gas at center, bottom.

In this approximately 100-light-year-wide fantasy-like landscape, dark towers of dust rise above a glowing wall of gases on the surface of the molecular cloud. The seahorse-shaped pillar at lower, right is approximately 20 light-years long, roughly four times the distance between our Sun and the nearest star, Alpha Centauri.

The region is in the Large Magellanic Cloud (LMC), a satellite of our Milky Way galaxy. It is a fascinating laboratory for observing star-formation regions and their evolution. Dwarf galaxies like the LMC are considered to be the primitive building blocks of larger galaxies.

This representative color image was taken on August 10, 2008, with Hubble's Wide Field Planetary Camera 2. Red shows emission from sulfur atoms, green from glowing hydrogen, and blue from glowing oxygen. Source: NASA.]]></media:description><media:thumbnail url="http://rlv.zcache.com/turbulent_star_birth_region_selection_postcard-p239185416537268522td81_125.jpg" /><media:content url="http://rlv.zcache.com/turbulent_star_birth_region_selection_postcard-p239185416537268522td81_500.jpg" /><media:keywords>hubble, nasa, stars, star, galaxy, galaxies, space, astronomy, nasa, hubble, telescope, beautiful, postcard, postcards, photos, photograph, gift, gifts, nebula</media:keywords><media:rating scheme="urn:mpaa">g</media:rating></item>
<item><guid isPermaLink="false">http://www.zazzle.com/turbulent_star_birth_region_selection_postcard-239182882453177407?gl=Galactica</guid><pubDate>Sun, 30 Nov 2008 23:02:05 GMT</pubDate><title><![CDATA[Turbulent Star-Birth Region Selection]]></title><link>http://www.zazzle.com/turbulent_star_birth_region_selection_postcard-239182882453177407?gl=Galactica</link><author>Galactica</author><description><![CDATA[
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Hubble peered into a small portion of the nebula near the star cluster NGC 2074 (upper, left). The region is a firestorm of raw stellar creation, perhaps triggered by a nearby supernova explosion. It lies about 170,000 light-years away near the Tarantula nebula, one of the most active star-forming regions in our Local Group of galaxies.

The three-dimensional-looking image reveals dramatic ridges and valleys of dust, serpent-head &quot;pillars of creation,&quot; and gaseous filaments glowing fiercely under torrential ultraviolet radiation. The region is on the edge of a dark molecular cloud that is an incubator for the birth of new stars.

The high-energy radiation blazing out from clusters of hot young stars already born in NGC 2074 is sculpting the wall of the nebula by slowly eroding it away. Another young cluster may be hidden beneath a circle of brilliant blue gas at center, bottom.

In this approximately 100-light-year-wide fantasy-like landscape, dark towers of dust rise above a glowing wall of gases on the surface of the molecular cloud. The seahorse-shaped pillar at lower, right is approximately 20 light-years long, roughly four times the distance between our Sun and the nearest star, Alpha Centauri.

The region is in the Large Magellanic Cloud (LMC), a satellite of our Milky Way galaxy. It is a fascinating laboratory for observing star-formation regions and their evolution. Dwarf galaxies like the LMC are considered to be the primitive building blocks of larger galaxies.

This representative color image was taken on August 10, 2008, with Hubble's Wide Field Planetary Camera 2. Red shows emission from sulfur atoms, green from glowing hydrogen, and blue from glowing oxygen. Source: NASA.]]></media:description><media:thumbnail url="http://rlv.zcache.com/turbulent_star_birth_region_selection_postcard-p239182882453177407trah_125.jpg" /><media:content url="http://rlv.zcache.com/turbulent_star_birth_region_selection_postcard-p239182882453177407trah_500.jpg" /><media:keywords>hubble, nasa, stars, star, galaxy, galaxies, space, astronomy, nasa, hubble, telescope, beautiful, postcard, postcards, photos, photograph, gift, gifts, nebula</media:keywords><media:rating scheme="urn:mpaa">g</media:rating></item>
<item><guid isPermaLink="false">http://www.zazzle.com/turbulent_star_birth_region_selection_postage-172691418978139121?gl=Galactica</guid><pubDate>Sun, 30 Nov 2008 23:02:05 GMT</pubDate><title><![CDATA[Turbulent Star-Birth Region Selection]]></title><link>http://www.zazzle.com/turbulent_star_birth_region_selection_postage-172691418978139121?gl=Galactica</link><author>Galactica</author><description><![CDATA[
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</div>]]></description><media:title><![CDATA[Turbulent Star-Birth Region Selection]]></media:title><media:description><![CDATA[In commemoration of NASA's Hubble Space Telescope completing its 100,000th orbit in its 18th year of exploration and discovery, scientists at the Space Telescope Science Institute in Baltimore, Md., have aimed Hubble to take a snapshot of a dazzling region of celestial birth and renewal.

Hubble peered into a small portion of the nebula near the star cluster NGC 2074 (upper, left). The region is a firestorm of raw stellar creation, perhaps triggered by a nearby supernova explosion. It lies about 170,000 light-years away near the Tarantula nebula, one of the most active star-forming regions in our Local Group of galaxies.

The three-dimensional-looking image reveals dramatic ridges and valleys of dust, serpent-head &quot;pillars of creation,&quot; and gaseous filaments glowing fiercely under torrential ultraviolet radiation. The region is on the edge of a dark molecular cloud that is an incubator for the birth of new stars.

The high-energy radiation blazing out from clusters of hot young stars already born in NGC 2074 is sculpting the wall of the nebula by slowly eroding it away. Another young cluster may be hidden beneath a circle of brilliant blue gas at center, bottom.

In this approximately 100-light-year-wide fantasy-like landscape, dark towers of dust rise above a glowing wall of gases on the surface of the molecular cloud. The seahorse-shaped pillar at lower, right is approximately 20 light-years long, roughly four times the distance between our Sun and the nearest star, Alpha Centauri.

The region is in the Large Magellanic Cloud (LMC), a satellite of our Milky Way galaxy. It is a fascinating laboratory for observing star-formation regions and their evolution. Dwarf galaxies like the LMC are considered to be the primitive building blocks of larger galaxies.

This representative color image was taken on August 10, 2008, with Hubble's Wide Field Planetary Camera 2. Red shows emission from sulfur atoms, green from glowing hydrogen, and blue from glowing oxygen. Source: NASA.]]></media:description><media:thumbnail url="http://rlv.zcache.com/turbulent_star_birth_region_selection_postage-p172691418978139121anrd3_125.jpg" /><media:content url="http://rlv.zcache.com/turbulent_star_birth_region_selection_postage-p172691418978139121anrd3_500.jpg" /><media:keywords>hubble, nasa, stars, star, galaxy, galaxies, space, astronomy, nasa, hubble, telescope, beautiful, postcard, postcards, photos, photograph, gift, gifts, nebula</media:keywords><media:rating scheme="urn:mpaa">g</media:rating></item>
<item><guid isPermaLink="false">http://www.zazzle.com/messier_101_print-228877639092211892?gl=Galactica</guid><pubDate>Thu, 14 Aug 2008 00:27:00 GMT</pubDate><title><![CDATA[Messier 101 Print]]></title><link>http://www.zazzle.com/messier_101_print-228877639092211892?gl=Galactica</link><author>Galactica</author><description><![CDATA[
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		>Messier 101 Print</a><br />
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</div>]]></description><media:title><![CDATA[Messier 101 Print]]></media:title><media:description><![CDATA[Giant galaxies weren’t assembled in a day. Neither was this Hubble Space Telescope image of the face-on spiral galaxy Messier 101 (M101). It is the largest and most detailed photo of a spiral galaxy that has ever been released from Hubble. The galaxy’s portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 in March 1994, September 1994, June 1999, November 2002, and January 2003. The newly composed image also includes elements from images from ground-based photos. Courtesy: NASA]]></media:description><media:thumbnail url="http://rlv.zcache.com/messier_101_print-p228877639092211892td2a_125.jpg" /><media:content url="http://rlv.zcache.com/messier_101_print-p228877639092211892td2a_500.jpg" /><media:keywords>nasa, astronomy, prints, posters, galaxy, galaxies, stars, star, space, hubble, beautiful</media:keywords><media:rating scheme="urn:mpaa">g</media:rating></item>
<item><guid isPermaLink="false">http://www.zazzle.com/messier_101_mousepad-144559245213276773?gl=Galactica</guid><pubDate>Thu, 14 Aug 2008 00:22:16 GMT</pubDate><title><![CDATA[Messier 101]]></title><link>http://www.zazzle.com/messier_101_mousepad-144559245213276773?gl=Galactica</link><author>Galactica</author><description><![CDATA[
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</div>]]></description><media:title><![CDATA[Messier 101]]></media:title><media:description><![CDATA[Giant galaxies weren’t assembled in a day. Neither was this Hubble Space Telescope image of the face-on spiral galaxy Messier 101 (M101). It is the largest and most detailed photo of a spiral galaxy that has ever been released from Hubble. The galaxy’s portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 in March 1994, September 1994, June 1999, November 2002, and January 2003. The newly composed image also includes elements from images from ground-based photos. Courtesy: NASA]]></media:description><media:thumbnail url="http://rlv.zcache.com/messier_101_mousepad-p144559245213276773td22_125.jpg" /><media:content url="http://rlv.zcache.com/messier_101_mousepad-p144559245213276773td22_500.jpg" /><media:keywords>astronomy, space, print, galaxy, galaxies, star, stars, nasa, mousepads, mouse, pad</media:keywords><media:rating scheme="urn:mpaa">g</media:rating></item>
<item><guid isPermaLink="false">http://www.zazzle.com/cassiopeia_shoes-167449193227241049?gl=Galactica</guid><pubDate>Thu, 07 Aug 2008 22:31:29 GMT</pubDate><title><![CDATA[Cassiopeia]]></title><link>http://www.zazzle.com/cassiopeia_shoes-167449193227241049?gl=Galactica</link><author>Galactica</author><description><![CDATA[
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<item><guid isPermaLink="false">http://www.zazzle.com/the_veil_nebula_sgt_2_postage-172347466351156193?gl=Galactica</guid><pubDate>Mon, 04 Feb 2008 07:52:28 GMT</pubDate><title><![CDATA[The Veil Nebula SGT 2]]></title><link>http://www.zazzle.com/the_veil_nebula_sgt_2_postage-172347466351156193?gl=Galactica</link><author>Galactica</author><description><![CDATA[
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