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			<title>RSS @ zorg.ch</title>
			<link>http://www.zorg.ch/</link>
			<description>zorg.ch RSS Feed - Forum, Events, Gallery and more</description>
			<language>de-DE</language>
			<lastBuildDate>Sat, 19 May 2012 16:52:43</lastBuildDate><item>
							<title>GALEX: The Andromeda</title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=14207&parent_id=14207#113653</link>
							<pubDate>Sat, 19 May 2012 00:00:08</pubDate>
							<author>[z]Barbara Harris</author>
							<category><![CDATA[Pic: GALEX: The Andromeda]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=14207&parent_id=14207#113653</guid>
							<description><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1205/AndromedaGalex_2048.jpg'><b>GALEX: The Andromeda Galaxy </b></a><br>
			 <br>Explanation: </b>

A mere 2.5 million light-years away, the Andromeda Galaxy really is
<a href="http://antwrp.gsfc.nasa.gov/apod/ap100109.html">just next door</a> as large galaxies go.

<a href="http://antwrp.gsfc.nasa.gov/apod...]]></description>
							<content:encoded><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1205/AndromedaGalex_2048.jpg'><b>GALEX: The Andromeda Galaxy </b></a><br>
			 <br>Explanation: </b>

A mere 2.5 million light-years away, the Andromeda Galaxy really is
<a href="http://antwrp.gsfc.nasa.gov/apod/ap100109.html">just next door</a> as large galaxies go.

<a href="http://antwrp.gsfc.nasa.gov/apod/ap061228.html">So close, and spanning</a>
some 260,000 light-years, it took 11 different
image fields from the
<a href="http://www.nasa.gov/mission_pages/galex/galex20120516.html">Galaxy Evolution Explorer (GALEX)</a> satellite's
telescope to produce this gorgeous portrait of the spiral galaxy in
ultraviolet light.

While its spiral arms <a href="http://antwrp.gsfc.nasa.gov/apod/ap101027.html">stand out</a>
in visible light images of Andromeda
(also known as M31), the arms look more like rings in
<a href="http://www.nasa.gov/mission_pages/galex/pia15416.html">the
GALEX ultraviolet view</a>, dominated by hot, young, massive stars.

As sites of intense star formation, the rings have been interpreted as
evidence Andromeda collided with its smaller neighboring elliptical
galaxy M32 more than 200 million years ago.

The large <a href="http://arxiv.org/abs/0705.1170">Andromeda galaxy
and our own Milky Way</a> are the dominant members of the
<a href="http://www.atlasoftheuniverse.com/localgr.html">local
galaxy group</a>.

 
 <br><br><a href='http://antwrp.gsfc.nasa.gov/apod/ap120518.html'>Credit &amp; Copyright</a>]]></content:encoded>
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						<item>
							<title>Herschel's Cygnus X </title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=14206&parent_id=14206#113652</link>
							<pubDate>Fri, 18 May 2012 00:00:09</pubDate>
							<author>[z]Barbara Harris</author>
							<category><![CDATA[Pic: Herschel's Cygnus X ]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=14206&parent_id=14206#113652</guid>
							<description><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1205/Herschel_cygnusX_04052012_H.jpg'><b>Herschel's Cygnus X </b></a><br>
			 <br>Explanation: </b>

The Herschel Space Observatory's
<a href="http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=50343">infrared view of Cygnus X</a>
spans some 6x2 degrees across one of the closest, massive star
formin...]]></description>
							<content:encoded><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1205/Herschel_cygnusX_04052012_H.jpg'><b>Herschel's Cygnus X </b></a><br>
			 <br>Explanation: </b>

The Herschel Space Observatory's
<a href="http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=50343">infrared view of Cygnus X</a>
spans some 6x2 degrees across one of the closest, massive star
forming regions in the plane of our Milky Way galaxy.

In fact, the rich stellar nursery already holds the
massive star cluster known as the Cygnus OB2
<a href="http://en.wikipedia.org/wiki/Stellar_association#Stellar_associations">association</a>.

But those stars are more evident by
the region <a href="http://antwrp.gsfc.nasa.gov/apod/ap070726.html">cleared by</a>
their energetic winds and radiation
near the bottom center of this field, and are not detected by
Herschel instruments operating
<a href="http://antwrp.gsfc.nasa.gov/apod/ap110902.html">at long infrared wavelengths</a>.

Herschel does reveal the region's complex filaments of cool gas
and dust that lead
<a  href="http://antwrp.gsfc.nasa.gov/apod/image/1205/Herschel_CygnusX_07052012_Anx600.jpg">to
dense locations</a> where new massive stars are forming.

<a href="http://www.cfa.harvard.edu/cygnusX/whatis.html">Cygnus X
lies</a> some 4500 light-years away toward the heart
of the northern constellation of the Swan.

At that distance this picture would be almost 500 light-years wide.

 
 <br><br><a href='http://antwrp.gsfc.nasa.gov/apod/ap120517.html'>Credit &amp; Copyright</a>]]></content:encoded>
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							<title>Star Formation in th</title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=14205&parent_id=14205#113651</link>
							<pubDate>Thu, 17 May 2012 00:00:10</pubDate>
							<author>[z]Barbara Harris</author>
							<category><![CDATA[Pic: Star Formation in th]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=14205&parent_id=14205#113651</guid>
							<description><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1205/tarantula2_hst_1280.jpg'><b>Star Formation in the Tarantula Nebula </b></a><br>
			 <br>Explanation: </b>
The largest, most violent star forming region known in the whole 
<a href="http://en.wikipedia.org/wiki/Local_Group">Local Group of galaxies</a> 
lies in our neighboring galaxy the 
<a href="http://...]]></description>
							<content:encoded><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1205/tarantula2_hst_1280.jpg'><b>Star Formation in the Tarantula Nebula </b></a><br>
			 <br>Explanation: </b>
The largest, most violent star forming region known in the whole 
<a href="http://en.wikipedia.org/wiki/Local_Group">Local Group of galaxies</a> 
lies in our neighboring galaxy the 
<a href="http://antwrp.gsfc.nasa.gov/apod/ap060510.html">Large Magellanic Cloud</a> (LMC). 

Were the Tarantula Nebula at the distance of the 
<a href="http://antwrp.gsfc.nasa.gov/apod/ap090222.html">Orion Nebula</a> -- a local star forming region -- 
it would take up fully half the sky. 

Also called 
<a href="http://en.wikipedia.org/wiki/30_Doradus">30 Doradus</a>, the red and pink gas indicates a massive 
<a href="http://antwrp.gsfc.nasa.gov/apod/emission_nebulae.html">emission nebula</a>, although 
<a href="http://antwrp.gsfc.nasa.gov/apod/ap091025.html">supernova remnants</a> and 
<a href="http://antwrp.gsfc.nasa.gov/apod/ap120129.html">dark nebula</a> also exist there. 

The bright knot of stars 
<a href="http://www.youtube.com/watch?v=RW35oaEHlHI">left of center</a> 
is called <a href="http://antwrp.gsfc.nasa.gov/apod/ap051211.html">R136</a> and contains many of the most 
massive, hottest, and brightest stars known.  

The 
<a href="http://spacetelescope.org/images/heic1206a/">above image</a> is one of the largest mosaics ever created by 
<a href="http://heritage.stsci.edu/2012/01/index.html">observations</a> of the 
<a href="http://www.stsci.edu/hst/HST_overview">Hubble Space Telescope</a> and has revealed unprecedented details of this enigmatic star forming region. 

<a href="http://heritage.stsci.edu/2012/01/caption.html">The image</a> is being released to celebrate the 
<a href="http://hubblesite.org/newscenter/archive/releases/2012/01/">22nd anniversary</a> of Hubble's launch.

  
 Astronomy Seminar of the Week: </b>
<a href="http://asterisk.apod.com/ampersand/?p=297">The Great Debate, Part I</a> 
 <br><br><a href='http://antwrp.gsfc.nasa.gov/apod/ap120516.html'>Credit &amp; Copyright</a>]]></content:encoded>
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							<title>All the Water on Pla</title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=14204&parent_id=14204#113650</link>
							<pubDate>Wed, 16 May 2012 00:00:10</pubDate>
							<author>[z]Barbara Harris</author>
							<category><![CDATA[Pic: All the Water on Pla]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=14204&parent_id=14204#113650</guid>
							<description><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1205/waterlessearth_woodshole_950.jpg'><b>All the Water on Planet Earth </b></a><br>
			 <br>Explanation: </b>
How much of planet Earth is made of water?

Very little, actually.

Although
<a href="http://www.youtube.com/watch?v=moSBExlLu2M">oceans of water</a> cover about 70 percent of Earth's surface, these...]]></description>
							<content:encoded><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1205/waterlessearth_woodshole_950.jpg'><b>All the Water on Planet Earth </b></a><br>
			 <br>Explanation: </b>
How much of planet Earth is made of water?

Very little, actually.

Although
<a href="http://www.youtube.com/watch?v=moSBExlLu2M">oceans of water</a> cover about 70 percent of Earth's surface, these oceans are
<a href="http://www.cliffshade.com/colorado/images/earth_anatomy.gif">shallow compared</a> to the Earth's radius.

The <a href="http://ga.water.usgs.gov/edu/earthwherewater.html">above illustration</a> shows what would happen if all of
<a href="http://www.whoi.edu/page.do?pid=80696&i=7301">the water</a> on or near the surface of the Earth were bunched up into a <a href="http://news.xinhuanet.com/english2010/photo/2010-04/15/13253168_21n.jpg">ball</a>.

The radius of this ball would be only about 700 kilometers, less than half the radius of the
<a href="http://antwrp.gsfc.nasa.gov/apod/ap091118.html">Earth's Moon</a>, but slightly larger than Saturn's moon
<a href="http://antwrp.gsfc.nasa.gov/apod/ap080513.html">Rhea</a> which, like many moons in our outer Solar System, is mostly water ice.

How even this much
<a href="http://en.wikipedia.org/wiki/Origin_of_water_on_Earth">water came</a> to be on
<a href="http://antwrp.gsfc.nasa.gov/apod/ap100713.html">the Earth</a> and whether any significant amount is
<a href="http://www.ldolphin.org/deepwaters.html">trapped</a> far
<a href="http://news.nationalgeographic.com/news/2002/03/0307_0307_waterworld.html">beneath Earth</a>'s surface remain topics of research.


  
 Poll: </b>
<a href="http://asterisk.apod.com/viewtopic.php?f=10&t=28555">Have you seen today's APOD image before?</a> 
 <br><br><a href='http://antwrp.gsfc.nasa.gov/apod/ap120515.html'>Credit &amp; Copyright</a>]]></content:encoded>
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							<title>Spiral Galaxy NGC 16</title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=14203&parent_id=14203#113649</link>
							<pubDate>Mon, 14 May 2012 00:00:08</pubDate>
							<author>[z]Barbara Harris</author>
							<category><![CDATA[Pic: Spiral Galaxy NGC 16]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=14203&parent_id=14203#113649</guid>
							<description><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1205/ngc1672_hubble_1920.jpg'><b>Spiral Galaxy NGC 1672 from Hubble </b></a><br>
			 <br>Explanation: </b>
Many spiral galaxies have bars across their centers.  

Even our own
<a href="http://antwrp.gsfc.nasa.gov/apod/ap000130.html">Milky Way Galaxy</a> is thought to have a
<a href="http://antwrp.gsfc.nasa.g...]]></description>
							<content:encoded><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1205/ngc1672_hubble_1920.jpg'><b>Spiral Galaxy NGC 1672 from Hubble </b></a><br>
			 <br>Explanation: </b>
Many spiral galaxies have bars across their centers.  

Even our own
<a href="http://antwrp.gsfc.nasa.gov/apod/ap000130.html">Milky Way Galaxy</a> is thought to have a
<a href="http://antwrp.gsfc.nasa.gov/apod/ap050825.html">modest central bar</a>.

Prominently barred spiral galaxy NGC 1672, <a href="http://hubblesite.org/newscenter/archive/releases/2007/15/image/a/">pictured above</a>, was captured in spectacular detail in image taken by the orbiting
<a href="http://en.wikipedia.org/wiki/Hubble_Space_Telescope">Hubble Space Telescope</a>.

Visible are dark filamentary
<a href="http://antwrp.gsfc.nasa.gov/apod/ap060219.html">dust lanes</a>, young
<a href="http://antwrp.gsfc.nasa.gov/apod/open_clusters.html">clusters</a> of bright blue stars, red
<a href="http://antwrp.gsfc.nasa.gov/apod/emission_nebulae.html">emission nebulas</a> of glowing hydrogen gas,
a long bright bar of stars across the center, and a bright
<a href="http://en.wikipedia.org/wiki/Active_galactic_nucleus">active nucleus</a> that likely houses a supermassive
<a href="http://antwrp.gsfc.nasa.gov/htmltest/rjn_bht.html">black hole</a>.  

Light takes about 60 million years to reach us from
<a href="http://heritage.stsci.edu/2007/15/caption.html">NGC 1672</a>, which spans about 75,000
<a href="http://chandra.harvard.edu/photo/cosmic_distance.html">light years</a> across.

<a href="http://www.youtube.com/watch?v=hGuct0CGHiA">NGC 1672</a>, which appears toward the constellation of the Dolphinfish
(<a href="http://www.ianridpath.com/startales/dorado.htm">Dorado</a>), is
<a href="http://adsabs.harvard.edu/abs/2011ApJ...734...33J">being studied</a> to find out how a spiral bar contributes to star formation in a galaxy's central regions.  


  
 Follow APOD: </b> On
<a href="https://www.facebook.com/AstronomyPictureOfTheDay">Facebook</a> or
<a href="https://plus.google.com/u/1/113118420661689340672/">Google+</a> 
 <br><br><a href='http://antwrp.gsfc.nasa.gov/apod/ap120513.html'>Credit &amp; Copyright</a>]]></content:encoded>
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							<title>Comment zu Pic: A Dangerous Sunrise </title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=14191&parent_id=14191#113648</link>
							<pubDate>Sun, 13 May 2012 03:40:54</pubDate>
							<author>IneX</author>
							<category><![CDATA[Pic: A Dangerous Sunrise ]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=14191&parent_id=14191#113648</guid>
							<description><![CDATA[Das isch doch en Screenshot usem Diablo III? ;)]]></description>
							<content:encoded><![CDATA[Das isch doch en Screenshot usem Diablo III? ;)]]></content:encoded>
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							<title>The Hydra Cluster of</title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=14202&parent_id=14202#113647</link>
							<pubDate>Sun, 13 May 2012 00:00:08</pubDate>
							<author>[z]Barbara Harris</author>
							<category><![CDATA[Pic: The Hydra Cluster of]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=14202&parent_id=14202#113647</guid>
							<description><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1205/20120330ACO106042-9-8lau.jpg'><b>The Hydra Cluster of Galaxies </b></a><br>
			 <br>Explanation: </b>

Two stars within our own Milky Way galaxy anchor the foreground
of <a href="http://anguslau.smugmug.com/Nature/Astro/20694276_s3M2pJ#!i=1804842710&k=vGC4NCj">this cosmic snapshot</a>.

Beyond them lie ...]]></description>
							<content:encoded><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1205/20120330ACO106042-9-8lau.jpg'><b>The Hydra Cluster of Galaxies </b></a><br>
			 <br>Explanation: </b>

Two stars within our own Milky Way galaxy anchor the foreground
of <a href="http://anguslau.smugmug.com/Nature/Astro/20694276_s3M2pJ#!i=1804842710&k=vGC4NCj">this cosmic snapshot</a>.

Beyond them lie the galaxies of
<a href="http://www.atlasoftheuniverse.com/superc/hya.html">the
Hydra Cluster</a>.

In fact, while the spiky foreground stars are hundreds of light-years
distant, the Hydra Cluster galaxies are over 100 million light-years
away.

Three large galaxies near the cluster center, two yellow
<a href="http://antwrp.gsfc.nasa.gov/apod/ap060520.html">ellipticals</a>
(NGC 3311, NGC 3309) and one prominent blue spiral (NGC 3312),
are the dominant galaxies, each about 150,000 light-years in diameter.

An intriguing overlapping galaxy pair cataloged as
<a href="http://antwrp.gsfc.nasa.gov/apod/ap110715.html">NGC 3314 is just</a>
above and left of NGC 3312.

Also known as Abell 1060, the Hydra galaxy cluster is one of three large
galaxy clusters within 200 million light-years of the Milky Way.

In the
<a href="http://antwrp.gsfc.nasa.gov/apod/ap110614.html">nearby universe</a>,
galaxies are gravitationally bound into clusters which themselves are
loosely bound
<a href="http://heasarc.nasa.gov/docs/cosmic/nearest_superclusters_info.html">into superclusters</a>
that in turn are seen to align over even larger
<a href="http://antwrp.gsfc.nasa.gov/apod/ap120312.html">scales</a>.

At a distance of 100 million light-years
this picture would be about 1.3 million light-years
<a href="http://chandra.harvard.edu/photo/scale_distance.html">across</a>.

 
 <br><br><a href='http://antwrp.gsfc.nasa.gov/apod/ap120512.html'>Credit &amp; Copyright</a>]]></content:encoded>
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							<title>Sun vs. Super Moon</title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=14201&parent_id=14201#113646</link>
							<pubDate>Sat, 12 May 2012 00:00:08</pubDate>
							<author>[z]Barbara Harris</author>
							<category><![CDATA[Pic: Sun vs. Super Moon]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=14201&parent_id=14201#113646</guid>
							<description><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1205/supermoon-unsupersun_csz.jpg'><b>Sun vs. Super Moon</b></a><br>
			 <br>Explanation: </b>

<a href="http://antwrp.gsfc.nasa.gov/apod/ap120510.html">The Super Moon wins</a>, by just a little, when
<a href="http://antwrp.gsfc.nasa.gov/apod/ap080801.html">its apparent size</a> is
compared to the Sun in thi...]]></description>
							<content:encoded><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1205/supermoon-unsupersun_csz.jpg'><b>Sun vs. Super Moon</b></a><br>
			 <br>Explanation: </b>

<a href="http://antwrp.gsfc.nasa.gov/apod/ap120510.html">The Super Moon wins</a>, by just a little, when
<a href="http://antwrp.gsfc.nasa.gov/apod/ap080801.html">its apparent size</a> is
compared to the Sun in this ingenious composite picture.

To make it, the Full Moon on May 6 was photographed
with the same camera and telescope used to image the Sun
(with a dense solar filter!) on the following day.

Of course, on May 6 the
<a href="http://www.perseus.gr/Astro-Lunar-Scenes-Apo-Perigee-2010.htm">Moon was at perigee</a>,
the closest point to Earth in its eliptical orbit,
making it the largest Full Moon of 2012.

Two weeks later, on May 20, the
<a href="http://apod.nasa.gov/apod/ap041021.html">Moon will be near
apogee</a>, the most distant point in its orbit, so by then it will
be nearly at its smallest apparent size.

It will also be a dark
<a href="http://mplsstartribune.net/wp-content/uploads/2012/02/moon-phases-for-kids1.jpg">New Moon</a> on that date.

And for some the New Moon will be surprisingly easy
to compare to the Sun, because on
<a href="http://eclipse.gsfc.nasa.gov/OH/OH2012.html">May 20 the
first solar eclipse</a> of 2012
will be visible from much of Asia, the Pacific, and North America.

Along a path 240 to 300 kilometers wide, the
<a href="http://www.mreclipse.com/Special/SEprimer.html">eclipse will
be annular</a>.

Near apogee the smaller silhouetted Moon will fit just
<a href="http://antwrp.gsfc.nasa.gov/apod/ap100122.html">inside the bright solar disk</a>.

 
 <br><br><a href='http://antwrp.gsfc.nasa.gov/apod/ap120511.html'>Credit &amp; Copyright</a>]]></content:encoded>
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							<title>Green Flash and Supe</title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=14200&parent_id=14200#113645</link>
							<pubDate>Fri, 11 May 2012 00:00:08</pubDate>
							<author>[z]Barbara Harris</author>
							<category><![CDATA[Pic: Green Flash and Supe]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=14200&parent_id=14200#113645</guid>
							<description><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1205/MoonflashLavederCrop.jpg'><b>Green Flash and Super Moon</b></a><br>
			 <br>Explanation: </b>

It was really not
<a href="http://www.uky.edu/Projects/Chemcomics/html/fl_70_6_mo.html">about superheroes</a> as on May 6 the much touted
Super Moon, the largest <a href="http://antwrp.gsfc.nasa.gov/apod/ap120...]]></description>
							<content:encoded><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1205/MoonflashLavederCrop.jpg'><b>Green Flash and Super Moon</b></a><br>
			 <br>Explanation: </b>

It was really not
<a href="http://www.uky.edu/Projects/Chemcomics/html/fl_70_6_mo.html">about superheroes</a> as on May 6 the much touted
Super Moon, the largest <a href="http://antwrp.gsfc.nasa.gov/apod/ap120505.html">Full Moon of 2012</a>,
rose over this otherwise peaceful harbor.

And no <a href="http://en.wikipedia.org/wiki/List_of_comic_book_supervillain_debuts">supervillains</a>
were present either as boats gently
rocked at their moorings near the checkerboard
La Perdrix lighthouse
<a href="http://maps.google.com/?ie=UTF8&t=h&ll=47.837455,-4.166184
&spn=0.001786,0.003165&z=18">on the coast</a> of Brittany, France.

But the rise of the Super Moon was preceded by a
<a href="http://www.atoptics.co.uk/atoptics/gf1.htm">Green Flash</a>,
captured in the first frame of this
<a href="http://vimeo.com/41670884">timelapse video recorded that night</a>.

The cropped image of the frame, a two second long exposure, shows the
strongly colored flash left of the lighted buoy
near picture center.

While the <a href="http://asterisk.apod.com/viewtopic.php?f=29&t=28458">Super Moon was enjoyed</a>
at locations all around the world,
the circumstances that produced the Green Flash were more restrictive.

Green flashes for both
<a href="http://antwrp.gsfc.nasa.gov/apod/ap110104.html">Sun</a> and <a href="ap050826.html">Moon</a>
are caused by atmospheric
refraction enhanced by long, low, sight lines and strong atmospheric
temperature gradients often
<a href="http://antwrp.gsfc.nasa.gov/apod/ap090620.html">favored by a sea horizon</a>.

 
 <br><br><a href='http://antwrp.gsfc.nasa.gov/apod/ap120510.html'>Credit &amp; Copyright</a>]]></content:encoded>
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							<title>Shuttle Enterprise O</title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=14199&parent_id=14199#113644</link>
							<pubDate>Thu, 10 May 2012 00:00:09</pubDate>
							<author>[z]Barbara Harris</author>
							<category><![CDATA[Pic: Shuttle Enterprise O]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=14199&parent_id=14199#113644</guid>
							<description><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1205/shuttlelibertyempire_nasa_836.jpg'><b>Shuttle Enterprise Over New York </b></a><br>
			 <br>Explanation: </b>
What's that in the background?

Two famous New York City icons stand tall in the 
<a href="http://www.flickr.com/photos/nasahqphoto/7118799989/">above photo</a> 
taken last week.

On the left lo...]]></description>
							<content:encoded><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1205/shuttlelibertyempire_nasa_836.jpg'><b>Shuttle Enterprise Over New York </b></a><br>
			 <br>Explanation: </b>
What's that in the background?

Two famous New York City icons stand tall in the 
<a href="http://www.flickr.com/photos/nasahqphoto/7118799989/">above photo</a> 
taken last week.

On the left looms the 
<a href="http://en.wikipedia.org/wiki/Statue_of_Liberty">Statue of Liberty</a>, 
a universal symbol of freedom, while on the right rises the 
<a href="http://en.wikipedia.org/wiki/Empire_State_Building">Empire State Building</a>, 
now the <a href="http://articles.nydailynews.com/2012-04-30/news/31503081_1_tallest-building-freedom-tower-world-trade-center">second largest building</a> in the city.

What's unique about this once-in-a-lifetime photograph, though, is the third icon that appears to <a href="http://www.youtube.com/watch?v=96NgEpRetvo">Lady Liberty</a>'s left.

High in the air and far in the background 
<a href="http://antwrp.gsfc.nasa.gov/apod/ap070708.html">flies</a> the space shuttle Enterprise -- 
<a href="http://www.drunktiki.com/wp-content/uploads/2011/08/tree-stump-cat-pole-sitter.jpg">perched atop</a> a 747 jet -- 

<a href="http://www.youtube.com/watch?v=9ASL0oS5ksU">on the way</a> to its new home.

New Yorkers and visitors to the 
<a href="http://en.wikipedia.org/wiki/Big_Apple">Big Apple</a> can visit the 
<a href="http://en.wikipedia.org/wiki/Shuttle_enterprise">test space shuttle</a> at the 
<a href="http://www.intrepidmuseum.org/">Intrepid Sea, Air & Space Museum</a> on the West Side of Manhattan starting July 19.


  
 Neptune & Vulcan </b>
<a href="http://asterisk.apod.com/ampersand/?p=295">Astronomy Seminar of the Week</a> 
 <br><br><a href='http://antwrp.gsfc.nasa.gov/apod/ap120509.html'>Credit &amp; Copyright</a>]]></content:encoded>
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							<title>Supermoon Over Paris</title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=14198&parent_id=14198#113643</link>
							<pubDate>Tue, 08 May 2012 00:00:07</pubDate>
							<author>[z]Barbara Harris</author>
							<category><![CDATA[Pic: Supermoon Over Paris]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=14198&parent_id=14198#113643</guid>
							<description><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1205/supermoon_vegastar_707.jpg'><b>Supermoon Over Paris </b></a><br>
			 <br>Explanation: </b>
Did you see that full Moon Saturday night?

Dubbed a
<a href="http://en.wikipedia.org/wiki/Supermoon">supermoon</a>,
the latest fully illuminated moon appeared
slightly larger than usual because it <a href="http:/...]]></description>
							<content:encoded><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1205/supermoon_vegastar_707.jpg'><b>Supermoon Over Paris </b></a><br>
			 <br>Explanation: </b>
Did you see that full Moon Saturday night?

Dubbed a
<a href="http://en.wikipedia.org/wiki/Supermoon">supermoon</a>,
the latest fully illuminated moon appeared
slightly larger than usual because it <a href="http://asterisk.apod.com/viewtopic.php?f=29&t=28458#p174961">occurred</a> unusually near the
closest point in its orbit to Earth.

<a href="http://www.flickr.com/photos/vegastarcarpentier/7146552595/in/photostream/">Pictured above</a>, the supermoon was captured Saturday night rising behind the top of the
<a href="http://www.youtube.com/watch?v=pPOUg26EXiU">Eiffel Tower</a> in
<a href="http://en.wikipedia.org/wiki/Paris">Paris</a>,
<a href="http://en.wikipedia.org/wiki/France">France</a>.

Of course, the angular <a href="http://cosmiclog.msnbc.msn.com/_news/2012/05/05/11557176-how-big-is-that-supermoon-anyway">extent of the moon</a> in comparison to foreground objects can be adjusted just by
<a href="http://www.youtube.com/watch?v=Uo0F1YEYU1U">changing the observer's distance</a> to the foreground object.

When compared to nearby objects the moon may
<a href="http://antwrp.gsfc.nasa.gov/apod/ap040524.html">appear tiny</a>, but when
compared to distant objects -- the moon may
<a href="http://antwrp.gsfc.nasa.gov/apod/ap120310.html">appear huge</a>.

Next month yet another full moon is expected, this one appearing about
<a href="http://www.flickr.com/photos/radicalretinoscopy/7147332123/">one percent smaller</a>.


  
 Browse:  </b>
<a href="http://asterisk.apod.com/viewtopic.php?f=29&t=28458">Supermoon Image Gallery</a> 
 <br><br><a href='http://antwrp.gsfc.nasa.gov/apod/ap120507.html'>Credit &amp; Copyright</a>]]></content:encoded>
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							<title>Comment zu Pic 863</title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=863&parent_id=863#113642</link>
							<pubDate>Mon, 07 May 2012 22:15:43</pubDate>
							<author>IneX</author>
							<category><![CDATA[Pic 863]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=863&parent_id=863#113642</guid>
							<description><![CDATA[is it... die erscht frau anere lanparty?]]></description>
							<content:encoded><![CDATA[is it... die erscht frau anere lanparty?]]></content:encoded>
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							<title>In the Center of the</title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=14197&parent_id=14197#113641</link>
							<pubDate>Mon, 07 May 2012 00:00:08</pubDate>
							<author>[z]Barbara Harris</author>
							<category><![CDATA[Pic: In the Center of the]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=14197&parent_id=14197#113641</guid>
							<description><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1205/omega_hubble_3047.jpg'><b>In the Center of the Omega Nebula </b></a><br>
			 <br>Explanation: </b>
In the depths of the <a href="http://antwrp.gsfc.nasa.gov/apod/ap030202.html">dark clouds</a>
of <a href="http://antwrp.gsfc.nasa.gov/apod/ap030706.html">dust</a> and <a href="ap970430.html">molecular gas<...]]></description>
							<content:encoded><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1205/omega_hubble_3047.jpg'><b>In the Center of the Omega Nebula </b></a><br>
			 <br>Explanation: </b>
In the depths of the <a href="http://antwrp.gsfc.nasa.gov/apod/ap030202.html">dark clouds</a>
of <a href="http://antwrp.gsfc.nasa.gov/apod/ap030706.html">dust</a> and <a href="ap970430.html">molecular gas</a> known as the <a href="ap021210.html">Omega Nebula</a>, stars continue to form.

The <a href="http://hubblesite.org/newscenter/archive/releases/2002/11/image/c/">above image</a> from the <a href="http://antwrp.gsfc.nasa.gov/apod/ap010806.html">Hubble Space Telescope</a>'s <a href="http://acs.pha.jhu.edu/">Advanced Camera for Surveys</a> shows exquisite detail in the
<a href="http://antwrp.gsfc.nasa.gov/apod/ap000919.html">famous star-forming region</a>.

The dark
<a href="http://www.youtube.com/watch?v=95tmYmeHf84">dust</a> filaments that lace the center of <a href="http://www.seds.org/messier/m/m017.html">Omega Nebula</a> were created in the atmospheres of cool <a href="http://www.historyoftheuniverse.com/starold.html">giant stars</a> and in the debris from <a href="http://chandra.harvard.edu/xray_sources/supernovas.html">supernova explosions</a>.

The red and blue hues arise from <a href="http://antwrp.gsfc.nasa.gov/apod/ap020213.html">glowing gas</a> heated by the radiation of massive nearby stars.

The points of light are the <a href="http://antwrp.gsfc.nasa.gov/apod/ap031227.html">young stars</a> themselves, some brighter than 100 Suns.

<a href="http://antwrp.gsfc.nasa.gov/apod/ap030816.html">Dark globules</a> mark even <a href="http://www.ing.iac.es/PR/science/stars.html">younger systems</a>, clouds of gas and dust just now
condensing to form <a href="http://www.ph.surrey.ac.uk/astrophysics/files/how_stars_form.html#starbirth">stars</a> and <a href="http://en.wikipedia.org/wiki/Planets">planets</a>.

The <a href="http://www.astr.ua.edu/gifimages/m17r.html">Omega Nebula</a> lies about 5000 <a href="http://starchild.gsfc.nasa.gov/docs/StarChild/questions/question19.html">light years</a> away toward the <a href="http://www.astro.wisc.edu/~dolan/constellations/extra/constellations.html">constellation</a> of <a href="http://en.wikipedia.org/wiki/Sagittarius_(constellation)">Sagittarius</a>.

The region shown spans about 3000 times the diameter of <a href="http://www.nineplanets.org/overview.html">our Solar System</a>.

  
 Gallery: </b> 
<a href="http://asterisk.apod.com/viewtopic.php?f=29&t=28458">Supermoon 2012</a>
 <br><br><a href='http://antwrp.gsfc.nasa.gov/apod/ap120506.html'>Credit &amp; Copyright</a>]]></content:encoded>
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							<title>Full Moonrise </title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=14196&parent_id=14196#113640</link>
							<pubDate>Sun, 06 May 2012 00:00:08</pubDate>
							<author>[z]Barbara Harris</author>
							<category><![CDATA[Pic: Full Moonrise ]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=14196&parent_id=14196#113640</guid>
							<description><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1205/FullMoonriseArn1250.jpg'><b>Full Moonrise </b></a><br>
			 <br>Explanation: </b>

<a href="http://antwrp.gsfc.nasa.gov/apod/ap081122.html">Rising as</a> the Sun sets,
tonight's Full Moon could be hard to miss.

Remarkably, its exact full
<a href="http://mplsstartribune.net/wp-content/uploads/2012/02/moo...]]></description>
							<content:encoded><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1205/FullMoonriseArn1250.jpg'><b>Full Moonrise </b></a><br>
			 <br>Explanation: </b>

<a href="http://antwrp.gsfc.nasa.gov/apod/ap081122.html">Rising as</a> the Sun sets,
tonight's Full Moon could be hard to miss.

Remarkably, its exact full
<a href="http://mplsstartribune.net/wp-content/uploads/2012/02/moon-phases-for-kids1.jpg">phase</a> (May 6 03:36 UT) will occur less
than two minutes after it reaches perigee,
the closest point to Earth in the Moon's orbit,
making it the largest Full Moon of 2012.

The Full Perigee Moon will <a href="http://antwrp.gsfc.nasa.gov/apod/ap080801.html">appear to be</a>
some 14 percent larger and 30 percent brighter
<a href="http://www.perseus.gr/Astro-Lunar-Scenes-Apo-Perigee-2010.htm">than a Full Moon near apogee</a>,
the most distant point in the elliptical lunar orbit.

In comparison, though, it will appear less than 1 percent larger and
almost as bright as April's Full Moon, captured in
<a href="http://www.astroarn.com/nightscape/h39af2a34#h39af2a34">this
telephoto image</a> rising over suburban Fort Collins, Colorado, USA.

For that <a href="http://antwrp.gsfc.nasa.gov/apod/ap070902.html">lunation</a>,
Full Moon and perigee were about 21 hours apart.

Of course, <a href="http://home.hiwaay.net/~krcool/Astro/moon/moonwords/moonpoems.htm">if you manage to miss</a> May's Full Perigee Moon, make a
note on your calendar.

<a href="http://fourmilab.ch/earthview/pacalc.html">Your next chance</a>
to see a Full Moon close to perigee, will be next year on June 23.

 
 <br><br><a href='http://antwrp.gsfc.nasa.gov/apod/ap120505.html'>Credit &amp; Copyright</a>]]></content:encoded>
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							<title>Fermi Epicycles: The</title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=14195&parent_id=14195#113639</link>
							<pubDate>Sat, 05 May 2012 00:00:10</pubDate>
							<author>[z]Barbara Harris</author>
							<category><![CDATA[Pic: Fermi Epicycles: The]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=14195&parent_id=14195#113639</guid>
							<description><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1205/LatPolar_Vela.jpg'><b>Fermi Epicycles: The Vela Pulsar's Path </b></a><br>
			 <br>Explanation: </b>

<a href="http://www.nasa.gov/mission_pages/GLAST/news/energy-extremes.html">Exploring the cosmos</a> at extreme energies, the
<a href="http://www.nasa.gov/mission_pages/GLAST/main/index.html">Fermi Gamm...]]></description>
							<content:encoded><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1205/LatPolar_Vela.jpg'><b>Fermi Epicycles: The Vela Pulsar's Path </b></a><br>
			 <br>Explanation: </b>

<a href="http://www.nasa.gov/mission_pages/GLAST/news/energy-extremes.html">Exploring the cosmos</a> at extreme energies, the
<a href="http://www.nasa.gov/mission_pages/GLAST/main/index.html">Fermi Gamma-ray Space Telescope</a>
orbits planet Earth every 95 minutes.

<a href="http://www.youtube.com/watch?v=EJfJyI8f7OU">By design</a>,
it rocks to the north and then to the
south on alternate orbits in order to
<a href="http://antwrp.gsfc.nasa.gov/apod/ap100318.html">survey the sky</a>
with its Large Area Telescope (LAT).

The spacecraft also rolls so that
solar panels are kept pointed at the Sun for power,
and the axis of its
<a href="http://en.wikipedia.org/wiki/Precession">orbit precesses</a>
like a top, making a complete rotation once every 54 days.

As a result of these multiple cycles
the paths of <a href="http://antwrp.gsfc.nasa.gov/apod/ap120315.html">gamma-ray sources</a> trace out
complex patterns from the spacecraft's perspective,
like this mesmerising plot of the path of the Vela Pulsar.

Centered on the LAT instrument's field of view, the plot spans 180
degrees and follows Vela's position
from August 2008 through August 2010.

The concentration near the center
shows that Vela was in the sensitive region
of the LAT field during much of that period.

<a href="http://antwrp.gsfc.nasa.gov/apod/ap000609.html">Born in the death explosion</a>
of a massive star within our
Milky Way galaxy,
<a href="http://www.nasa.gov/mission_pages/GLAST/news/pulsar_passel.html">the Vela Pulsar</a>
is a neutron star spinning 11 times a second, seen
as the brightest persistent source in the gamma-ray sky.

 
 <br><br><a href='http://antwrp.gsfc.nasa.gov/apod/ap120504.html'>Credit &amp; Copyright</a>]]></content:encoded>
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