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    <title>Astronomy Picture of the Day RSS Feed</title>
    <link>http://www.acme.com/jef/apod/</link>
    <description>
	<![CDATA[
	<p>
	The
	<a href="http://antwrp.gsfc.nasa.gov/apod/">Astronomy Picture of the Day</a>
	is a wonderful web site that puts up a different astronomy-related
	picture every day.
	However, the site does not have an RSS feed.
	This page fixes that deficiency.
	]]>
    </description>
    <language>en-us</language>
    <lastBuildDate>Wed, 16 May 2012 13:06:01 GMT</lastBuildDate>
    <generator>ACME Labs custom shell script</generator>
    <managingEditor>jef@mail.acme.com</managingEditor>
    <webMaster>webmaster@mail.acme.com</webMaster>
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	<title>Astronomy Picture of the Day RSS Feed</title>
	<link>http://www.acme.com/jef/apod/</link>
    </image>

    <item>
	<title><![CDATA[Star Formation in the Tarantula Nebula </b> <br> ]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap120516.html</link>
	<pubDate>Wed, 16 May 2012 13:06:01 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap120516.html"><img src="http://apod.nasa.gov/apod/image/1205/tarantula2_hst_960.jpg" /></a>
<title>Star Formation in the Tarantula Nebula </b> <br> </title>
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://apod.nasa.gov/apod/ap060510.html">Large Magellanic Cloud</a> (LMC). 

Were the Tarantula Nebula at the distance of the 
<a href="http://apod.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://apod.nasa.gov/apod/emission_nebulae.html">emission nebula</a>, although 
<a href="http://apod.nasa.gov/apod/ap091025.html">supernova remnants</a> and 
<a href="http://apod.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://apod.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.

<p> <center> 
<b> Astronomy Seminar of the Week: </b>
<a href="http://asterisk.apod.com/ampersand/?p=297"
>The Great Debate, Part I</a> <br>
<b> Tomorrow's picture: </b><a href="http://apod.nasa.gov/apod/ap120517.html">Cygnus X</a>

<p> <hr>
<a href="http://apod.nasa.gov/apod/ap120515.html">&lt;</a>
| <a href="http://apod.nasa.gov/apod/archivepix.html">Archive</a>
| <a href="http://apod.nasa.gov/apod/lib/aptree.html">Index</a>
| <a href="http://antwrp.gsfc.nasa.gov/cgi-bin/apod/apod_search">Search</a>
| <a href="http://apod.nasa.gov/apod/calendar/allyears.html">Calendar</a>
| <a href="http://apod.nasa.gov/apod//apod.rss">RSS</a>
| <a href="http://apod.nasa.gov/apod/lib/edlinks.html">Education</a>
| <a href="http://apod.nasa.gov/apod/lib/about_apod.html">About APOD</a>
| <a href=
"http://asterisk.apod.com/discuss_apod.php?date=120516">Discuss</a>
| <a href="http://apod.nasa.gov/apod/ap120517.html">&gt;</a>

<hr><p>
<b> Authors & editors: </b>
<a href="http://www.phy.mtu.edu/faculty/Nemiroff.html">Robert Nemiroff</a>
(<a href="http://www.phy.mtu.edu/">MTU</a>) &
<a href="http://antwrp.gsfc.nasa.gov/htmltest/jbonnell/www/bonnell.html"
>Jerry Bonnell</a> (<a href="http://www.astro.umd.edu/">UMCP</a>)<br>
<b>NASA Official: </b> Phillip Newman
<a href="http://apod.nasa.gov/apod/lib/about_apod.html#srapply">Specific rights apply</a>.<br>
<a href="http://www.nasa.gov/about/highlights/HP_Privacy.html">NASA Web
Privacy Policy and Important Notices</a><br>
<b>A service of:</b>
<a href="http://astrophysics.gsfc.nasa.gov/">ASD</a> at
<a href="http://www.nasa.gov/">NASA</a> /
<a href="http://www.nasa.gov/centers/goddard/">GSFC</a>
<br><b>&</b> <a href="http://www.mtu.edu/">Michigan Tech. U.</a><br>
</center>
</body>
</html>
	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[All the Water on Planet Earth </b> <br> ]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap120515.html</link>
	<pubDate>Tue, 15 May 2012 13:06:01 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap120515.html"><img src="http://apod.nasa.gov/apod/image/1205/waterlessearth_woodshole_960.jpg" /></a>
<title>All the Water on Planet Earth </b> <br> </title>
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 is 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://apod.nasa.gov/apod/ap091118.html">Earth's Moon</a>, but slightly larger than Saturn's moon
<a href="http://apod.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://apod.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.


<p> <center> 
<b> Poll: </b>
<a href="http://asterisk.apod.com/viewtopic.php?f=10&t=28555"
>Have you seen today's APOD image before?</a> <br>
<b> Tomorrow's picture: </b><a href="http://apod.nasa.gov/apod/ap120516.html">open space</a>

<p> <hr>
<a href="http://apod.nasa.gov/apod/ap120514.html">&lt;</a>
| <a href="http://apod.nasa.gov/apod/archivepix.html">Archive</a>
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| <a href="http://apod.nasa.gov/apod//apod.rss">RSS</a>
| <a href="http://apod.nasa.gov/apod/lib/edlinks.html">Education</a>
| <a href="http://apod.nasa.gov/apod/lib/about_apod.html">About APOD</a>
| <a href=
"http://asterisk.apod.com/discuss_apod.php?date=120515">Discuss</a>
| <a href="http://apod.nasa.gov/apod/ap120516.html">&gt;</a>

<hr><p>
<b> Authors & editors: </b>
<a href="http://www.phy.mtu.edu/faculty/Nemiroff.html">Robert Nemiroff</a>
(<a href="http://www.phy.mtu.edu/">MTU</a>) &
<a href="http://antwrp.gsfc.nasa.gov/htmltest/jbonnell/www/bonnell.html"
>Jerry Bonnell</a> (<a href="http://www.astro.umd.edu/">UMCP</a>)<br>
<b>NASA Official: </b> Phillip Newman
<a href="http://apod.nasa.gov/apod/lib/about_apod.html#srapply">Specific rights apply</a>.<br>
<a href="http://www.nasa.gov/about/highlights/HP_Privacy.html">NASA Web
Privacy Policy and Important Notices</a><br>
<b>A service of:</b>
<a href="http://astrophysics.gsfc.nasa.gov/">ASD</a> at
<a href="http://www.nasa.gov/">NASA</a> /
<a href="http://www.nasa.gov/centers/goddard/">GSFC</a>
<br><b>&</b> <a href="http://www.mtu.edu/">Michigan Tech. U.</a><br>
</center>
</body>
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	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[Virtual Flight Over Asteroid Vesta </b> <br> ]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap120514.html</link>
	<pubDate>Mon, 14 May 2012 13:06:01 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap120514.html"><img src="" /></a>
<title>Virtual Flight Over Asteroid Vesta </b> <br> </title>
What would it be like to fly over the asteroid Vesta?

Animators from the 
<a href="http://www.dlr.de/dlr/en/desktopdefault.aspx/tabid-10002/">German Aerospace Center</a> recently took actual images and height data from 
<a href="http://www.nasa.gov/mission_pages/dawn/mission/index.html">NASA's Dawn</a> 
mission currently visiting Vesta to 
<a href="http://dawn.jpl.nasa.gov/feature_stories/secrets_of_vesta_revealed.asp"
>generate</a> such a virtual movie.

The <a href=" http://www.youtube.com/watch?v=YYxPw_T8Vlk">above video</a> begins with a sequence above 
<a href=
" http://planetarynames.wr.usgs.gov/Feature/14911;jsessionid=1701b0012ee300e385522e34ff0b"
>Divalia Fossa</a>, an unusual pair of troughs running parallel over heavily cratered terrain.
Next, the virtual spaceship explores 
<a href="http://en.wikipedia.org/wiki/4_Vesta">Vesta</a>'s 60-km 
<a href="http://www.nasa.gov/mission_pages/dawn/multimedia/pia15491.html">Marcia Crater</a>, showing numerous vivid details.

Last, Dawn images were digitally recast with 
<a href="http://images.teamsugar.com/files/upl1/10/104166/26_2008/greatdanechi.jpg"
>exaggerated height</a> to better reveal 
<a href="http://apod.nasa.gov/apod/ap110802.html">Vesta</a>'s 5-km high mountain <a href="http://photojournal.jpl.nasa.gov/catalog/PIA15386">Aricia Tholus</a>.

Currently, 
<a href="http://en.wikipedia.org/wiki/Dawn_%28spacecraft%29">Dawn</a> is 
<a href="http://dawn.jpl.nasa.gov/mission/status.asp">rising away</a> 
from Vesta after being close enough to obtain the  
<a href="http://dawn.jpl.nasa.gov/mission/Dawn_overview.pdf">most detailed</a> 
surface images and 
<a href="http://apod.nasa.gov/apod/ap030723.html">gravity measurements</a> of the Solar System's second largest asteroid.

In August, 
<a href="http://dawn.jpl.nasa.gov/mission/faqs.asp">Dawn</a> is 
<a href="http://dawn.jpl.nasa.gov/mission/timeline.asp">scheduled</a> 
to blast away from Vesta and head toward 
<a href="http://apod.nasa.gov/apod/ap070622.html">Ceres</a>, the Solar System's largest asteroid.


<p> <center> 
<b> Help Evaluate APOD: </b>
<a href="http://asterisk.apod.com/viewtopic.php?f=28&t=28376&p=174497#p174497"
>Do the pictures (or videos) on APOD make you more interested in reading the text?</a> <br>
<b> Tomorrow's picture: </b><a href="http://apod.nasa.gov/apod/ap120515.html">waterless earth</a>

<p> <hr>
<a href="http://apod.nasa.gov/apod/ap120513.html">&lt;</a>
| <a href="http://apod.nasa.gov/apod/archivepix.html">Archive</a>
| <a href="http://apod.nasa.gov/apod/lib/aptree.html">Index</a>
| <a href="http://antwrp.gsfc.nasa.gov/cgi-bin/apod/apod_search">Search</a>
| <a href="http://apod.nasa.gov/apod/calendar/allyears.html">Calendar</a>
| <a href="http://apod.nasa.gov/apod//apod.rss">RSS</a>
| <a href="http://apod.nasa.gov/apod/lib/edlinks.html">Education</a>
| <a href="http://apod.nasa.gov/apod/lib/about_apod.html">About APOD</a>
| <a href=
"http://asterisk.apod.com/discuss_apod.php?date=120514">Discuss</a>
| <a href="http://apod.nasa.gov/apod/ap120515.html">&gt;</a>

<hr><p>
<b> Authors & editors: </b>
<a href="http://www.phy.mtu.edu/faculty/Nemiroff.html">Robert Nemiroff</a>
(<a href="http://www.phy.mtu.edu/">MTU</a>) &
<a href="http://antwrp.gsfc.nasa.gov/htmltest/jbonnell/www/bonnell.html"
>Jerry Bonnell</a> (<a href="http://www.astro.umd.edu/">UMCP</a>)<br>
<b>NASA Official: </b> Phillip Newman
<a href="http://apod.nasa.gov/apod/lib/about_apod.html#srapply">Specific rights apply</a>.<br>
<a href="http://www.nasa.gov/about/highlights/HP_Privacy.html">NASA Web
Privacy Policy and Important Notices</a><br>
<b>A service of:</b>
<a href="http://astrophysics.gsfc.nasa.gov/">ASD</a> at
<a href="http://www.nasa.gov/">NASA</a> /
<a href="http://www.nasa.gov/centers/goddard/">GSFC</a>
<br><b>&</b> <a href="http://www.mtu.edu/">Michigan Tech. U.</a><br>
</center>
</body>
</html>
	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[Spiral Galaxy NGC 1672 from Hubble </b> <br> ]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap120513.html</link>
	<pubDate>Sun, 13 May 2012 13:06:01 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap120513.html"><img src="http://apod.nasa.gov/apod/image/1205/ngc1672_hubble_960.jpg" /></a>
<title>Spiral Galaxy NGC 1672 from Hubble </b> <br> </title>
Many spiral galaxies have bars across their centers.  

Even our own
<a href="http://apod.nasa.gov/apod/ap000130.html">Milky Way Galaxy</a> is thought to have a
<a href="http://apod.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://apod.nasa.gov/apod/ap060219.html">dust lanes</a>, young
<a href="http://apod.nasa.gov/apod/open_clusters.html">clusters</a> of bright blue stars, red
<a href="http://apod.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.  


<p> <center> 
<b> 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>
<b> Tomorrow's picture: </b><a href="http://apod.nasa.gov/apod/ap120514.html">fly over vesta</a>

<p> <hr>
<a href="http://apod.nasa.gov/apod/ap120512.html">&lt;</a>
| <a href="http://apod.nasa.gov/apod/archivepix.html">Archive</a>
| <a href="http://apod.nasa.gov/apod/lib/aptree.html">Index</a>
| <a href="http://antwrp.gsfc.nasa.gov/cgi-bin/apod/apod_search">Search</a>
| <a href="http://apod.nasa.gov/apod/calendar/allyears.html">Calendar</a>
| <a href="http://apod.nasa.gov/apod//apod.rss">RSS</a>
| <a href="http://apod.nasa.gov/apod/lib/edlinks.html">Education</a>
| <a href="http://apod.nasa.gov/apod/lib/about_apod.html">About APOD</a>
| <a href=
"http://asterisk.apod.com/discuss_apod.php?date=120513">Discuss</a>
| <a href="http://apod.nasa.gov/apod/ap120514.html">&gt;</a>

<hr><p>
<b> Authors & editors: </b>
<a href="http://www.phy.mtu.edu/faculty/Nemiroff.html">Robert Nemiroff</a>
(<a href="http://www.phy.mtu.edu/">MTU</a>) &
<a href="http://antwrp.gsfc.nasa.gov/htmltest/jbonnell/www/bonnell.html"
>Jerry Bonnell</a> (<a href="http://www.astro.umd.edu/">UMCP</a>)<br>
<b>NASA Official: </b> Phillip Newman
<a href="http://apod.nasa.gov/apod/lib/about_apod.html#srapply">Specific rights apply</a>.<br>
<a href="http://www.nasa.gov/about/highlights/HP_Privacy.html">NASA Web
Privacy Policy and Important Notices</a><br>
<b>A service of:</b>
<a href="http://astrophysics.gsfc.nasa.gov/">ASD</a> at
<a href="http://www.nasa.gov/">NASA</a> /
<a href="http://www.nasa.gov/centers/goddard/">GSFC</a>
<br><b>&</b> <a href="http://www.mtu.edu/">Michigan Tech. U.</a><br>
</center>
</body>
</html>
	    ]]>
	</description>
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    <item>
	<title><![CDATA[The Hydra Cluster of Galaxies]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap120512.html</link>
	<pubDate>Sat, 12 May 2012 13:06:03 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap120512.html"><img src="http://apod.nasa.gov/apod/image/1205/20120330ACO106042-9-8lau960.jpg" /></a>
<title>The Hydra Cluster of Galaxies</title>

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://apod.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://apod.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://apod.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://apod.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>.

	    ]]>
	</description>
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    <item>
	<title><![CDATA[Sun vs. Super Moon]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap120511.html</link>
	<pubDate>Fri, 11 May 2012 13:06:02 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap120511.html"><img src="http://apod.nasa.gov/apod/image/1205/supermoon-unsupersun_csz900c.jpg" /></a>
<title>Sun vs. Super Moon</title>

<a href="http://apod.nasa.gov/apod/ap120510.html">The Super Moon wins</a>, by just a little, when
<a href="http://apod.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://apod.nasa.gov/apod/ap100122.html">inside the bright solar disk</a>.

	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[Green Flash and Super Moon]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap120510.html</link>
	<pubDate>Thu, 10 May 2012 13:06:01 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap120510.html"><img src="http://apod.nasa.gov/apod/image/1205/MoonflashLavederCrop900.jpg" /></a>
<title>Green Flash and Super Moon</title>

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

	    ]]>
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    <item>
	<title><![CDATA[Shuttle Enterprise Over New York </b> <br> ]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap120509.html</link>
	<pubDate>Wed, 09 May 2012 13:06:01 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap120509.html"><img src="http://apod.nasa.gov/apod/image/1205/shuttlelibertyempire_nasa_960.jpg" /></a>
<title>Shuttle Enterprise Over New York </b> <br> </title>
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://apod.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.


<p> <center> 
<b> Neptune & Vulcan </b>
<a href="http://asterisk.apod.com/ampersand/?p=295"
>Astronomy Seminar of the Week</a> <br>
<b> Tomorrow's picture: </b><a href="http://apod.nasa.gov/apod/ap120510.html">open space</a>

<p> <hr>
<a href="http://apod.nasa.gov/apod/ap120508.html">&lt;</a>
| <a href="http://apod.nasa.gov/apod/archivepix.html">Archive</a>
| <a href="http://apod.nasa.gov/apod/lib/aptree.html">Index</a>
| <a href="http://antwrp.gsfc.nasa.gov/cgi-bin/apod/apod_search">Search</a>
| <a href="http://apod.nasa.gov/apod/calendar/allyears.html">Calendar</a>
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| <a href="http://apod.nasa.gov/apod/lib/edlinks.html">Education</a>
| <a href="http://apod.nasa.gov/apod/lib/about_apod.html">About APOD</a>
| <a href=
"http://asterisk.apod.com/discuss_apod.php?date=120509">Discuss</a>
| <a href="http://apod.nasa.gov/apod/ap120510.html">&gt;</a>

<hr><p>
<b> Authors & editors: </b>
<a href="http://www.phy.mtu.edu/faculty/Nemiroff.html">Robert Nemiroff</a>
(<a href="http://www.phy.mtu.edu/">MTU</a>) &
<a href="http://antwrp.gsfc.nasa.gov/htmltest/jbonnell/www/bonnell.html"
>Jerry Bonnell</a> (<a href="http://www.astro.umd.edu/">UMCP</a>)<br>
<b>NASA Official: </b> Phillip Newman
<a href="http://apod.nasa.gov/apod/lib/about_apod.html#srapply">Specific rights apply</a>.<br>
<a href="http://www.nasa.gov/about/highlights/HP_Privacy.html">NASA Web
Privacy Policy and Important Notices</a><br>
<b>A service of:</b>
<a href="http://astrophysics.gsfc.nasa.gov/">ASD</a> at
<a href="http://www.nasa.gov/">NASA</a> /
<a href="http://www.nasa.gov/centers/goddard/">GSFC</a>
<br><b>&</b> <a href="http://www.mtu.edu/">Michigan Tech. U.</a><br>
</center>
</body>
</html>
	    ]]>
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    <item>
	<title><![CDATA[The Light of Stars </b> <br> ]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap120508.html</link>
	<pubDate>Tue, 08 May 2012 14:46:17 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap120508.html"><img src="" /></a>
<title>The Light of Stars </b> <br> </title>
What's moving?

Time lapse videos of the sky can be quite spectacular when they last long enough for
<a href="http://apod.nasa.gov/apod/ap110504.html">stars</a>, planets,
<a href="http://apod.nasa.gov/apod/ap110328.html">aurora</a>, and clouds to appear to move in just a few seconds.

<a href="http://vimeo.com/37752523">Pictured above</a>, however, astrovideographer
<a href="http://www.elcielodecanarias.com/sobre%20mi.htm">Daniel Lopez</a> not only treats us to several inspiring time lapse videos of the night sky, but shows us how he used sliders and motorized cranes to move the imaging cameras themselves, creating a thrilling three-dimensional sense of depth.

The video sequences were taken from
<a href="http://www.youtube.com/watch?v=5R1aVKizySY">Tenerife</a> on the
<a href="http://en.wikipedia.org/wiki/Canary_Islands">Canary Islands</a> of Spain over the past two months, and show scenes including sunset shadows approaching
<a href="http://www.iac.es/eno.php?op1=3&lang=en">Observatorio de Tiede</a>, the Milky Way shifting as the sky rotates, bright planets
<a href="http://apod.nasa.gov/apod/ap120318.html">Venus and trailing Jupiter</a> setting, a
<a href="http://apod.nasa.gov/apod/ap110228.html">reddened Moon</a> rising through differing layers of
<a href="http://apod.nasa.gov/apod/ap090223.html">atmospheric refraction</a>, the
<a href="http://apod.nasa.gov/apod/ap111014.html">MAGIC gamma-ray telescopes</a> slewing to observe a new source, and unusual foreground objects including conic
<a href="http://en.wikipedia.org/wiki/Echium_wildpretii">Echium wildpretii</a> plants,  unusual rock formations, and a
<a href="http://jerryandmartha.com/yourdailyart/images/catandbug.jpg"
>spider</a> moving about its web.  

The video concludes by showing the
<a href="http://apod.nasa.gov/apod/ap100404.html">Belt of Venus</a> descending on
<a href="http://en.wikipedia.org/wiki/Teide">Mt. Teide</a> as the morning sun rises.


<p> <center> 
<b> New Mirror: </b> 
<a href="http://apod-id.com/">APOD is now available in Indonesian from Indonesia.</a> <br>
<b> Tomorrow's picture: </b><a href="http://apod.nasa.gov/apod/ap120509.html">flying background</a>

<p> <hr>
<a href="http://apod.nasa.gov/apod/ap120507.html">&lt;</a>
| <a href="http://apod.nasa.gov/apod/archivepix.html">Archive</a>
| <a href="http://apod.nasa.gov/apod/lib/aptree.html">Index</a>
| <a href="http://antwrp.gsfc.nasa.gov/cgi-bin/apod/apod_search">Search</a>
| <a href="http://apod.nasa.gov/apod/calendar/allyears.html">Calendar</a>
| <a href="http://apod.nasa.gov/apod//apod.rss">RSS</a>
| <a href="http://apod.nasa.gov/apod/lib/edlinks.html">Education</a>
| <a href="http://apod.nasa.gov/apod/lib/about_apod.html">About APOD</a>
| <a href=
"http://asterisk.apod.com/discuss_apod.php?date=120508">Discuss</a>
| <a href="http://apod.nasa.gov/apod/ap120509.html">&gt;</a>

<hr><p>
<b> Authors & editors: </b>
<a href="http://www.phy.mtu.edu/faculty/Nemiroff.html">Robert Nemiroff</a>
(<a href="http://www.phy.mtu.edu/">MTU</a>) &
<a href="http://antwrp.gsfc.nasa.gov/htmltest/jbonnell/www/bonnell.html"
>Jerry Bonnell</a> (<a href="http://www.astro.umd.edu/">UMCP</a>)<br>
<b>NASA Official: </b> Phillip Newman
<a href="http://apod.nasa.gov/apod/lib/about_apod.html#srapply">Specific rights apply</a>.<br>
<a href="http://www.nasa.gov/about/highlights/HP_Privacy.html">NASA Web
Privacy Policy and Important Notices</a><br>
<b>A service of:</b>
<a href="http://astrophysics.gsfc.nasa.gov/">ASD</a> at
<a href="http://www.nasa.gov/">NASA</a> /
<a href="http://www.nasa.gov/centers/goddard/">GSFC</a>
<br><b>&</b> <a href="http://www.mtu.edu/">Michigan Tech. U.</a><br>
</center>
</body>
</html>
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    <item>
	<title><![CDATA[Supermoon Over Paris </b> <br> ]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap120507.html</link>
	<pubDate>Mon, 07 May 2012 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap120507.html"><img src="http://apod.nasa.gov/apod/image/1205/supermoon_vegastar_960.jpg" /></a>
<title>Supermoon Over Paris </b> <br> </title>
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://apod.nasa.gov/apod/ap040524.html">appear tiny</a>, but when
compared to distant objects -- the moon may
<a href="http://apod.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>.


<p> <center> 
<b> Browse:  </b>
<a href="http://asterisk.apod.com/viewtopic.php?f=29&t=28458"
>Supermoon Image Gallery</a> <br>
<b> Tomorrow's picture: </b><a href="http://apod.nasa.gov/apod/ap120508.html">on the move</a>

<p> <hr>
<a href="http://apod.nasa.gov/apod/ap120506.html">&lt;</a>
| <a href="http://apod.nasa.gov/apod/archivepix.html">Archive</a>
| <a href="http://apod.nasa.gov/apod/lib/aptree.html">Index</a>
| <a href="http://antwrp.gsfc.nasa.gov/cgi-bin/apod/apod_search">Search</a>
| <a href="http://apod.nasa.gov/apod/calendar/allyears.html">Calendar</a>
| <a href="http://apod.nasa.gov/apod//apod.rss">RSS</a>
| <a href="http://apod.nasa.gov/apod/lib/edlinks.html">Education</a>
| <a href="http://apod.nasa.gov/apod/lib/about_apod.html">About APOD</a>
| <a href=
"http://asterisk.apod.com/discuss_apod.php?date=120507">Discuss</a>
| <a href="http://apod.nasa.gov/apod/ap120508.html">&gt;</a>

<hr><p>
<b> Authors & editors: </b>
<a href="http://www.phy.mtu.edu/faculty/Nemiroff.html">Robert Nemiroff</a>
(<a href="http://www.phy.mtu.edu/">MTU</a>) &
<a href="http://antwrp.gsfc.nasa.gov/htmltest/jbonnell/www/bonnell.html"
>Jerry Bonnell</a> (<a href="http://www.astro.umd.edu/">UMCP</a>)<br>
<b>NASA Official: </b> Phillip Newman
<a href="http://apod.nasa.gov/apod/lib/about_apod.html#srapply">Specific rights apply</a>.<br>
<a href="http://www.nasa.gov/about/highlights/HP_Privacy.html">NASA Web
Privacy Policy and Important Notices</a><br>
<b>A service of:</b>
<a href="http://astrophysics.gsfc.nasa.gov/">ASD</a> at
<a href="http://www.nasa.gov/">NASA</a> /
<a href="http://www.nasa.gov/centers/goddard/">GSFC</a>
<br><b>&</b> <a href="http://www.mtu.edu/">Michigan Tech. U.</a><br>
</center>
</body>
</html>
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    <item>
	<title><![CDATA[In the Center of the Omega Nebula </b> <br> ]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap120506.html</link>
	<pubDate>Sun, 06 May 2012 13:06:01 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap120506.html"><img src="http://apod.nasa.gov/apod/image/1205/omega_hubble_960.jpg" /></a>
<title>In the Center of the Omega Nebula </b> <br> </title>
In the depths of the <a href="http://apod.nasa.gov/apod/ap030202.html">dark clouds</a>
of <a href="http://apod.nasa.gov/apod/ap030706.html">dust</a> and <a href="http://apod.nasa.gov/apod/ap970430.html"
>molecular gas</a> known as the <a href="http://apod.nasa.gov/apod/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://apod.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://apod.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://apod.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://apod.nasa.gov/apod/ap031227.html"
>young stars</a> themselves, some brighter than 100 Suns.

<a href="http://apod.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>.

<p> <center> 
<b> Dark Mysteries: </b>
<a href="http://asterisk.apod.com/ampersand/?p=292"
>Astronomy Seminar of the Week</a> <br> 
<b> Tomorrow's picture: </b><a href="http://apod.nasa.gov/apod/ap120507.html">moving pan</a>

<p> <hr>
<a href="http://apod.nasa.gov/apod/ap120505.html">&lt;</a>
| <a href="http://apod.nasa.gov/apod/archivepix.html">Archive</a>
| <a href="http://apod.nasa.gov/apod/lib/aptree.html">Index</a>
| <a href="http://antwrp.gsfc.nasa.gov/cgi-bin/apod/apod_search">Search</a>
| <a href="http://apod.nasa.gov/apod/calendar/allyears.html">Calendar</a>
| <a href="http://apod.nasa.gov/apod//apod.rss">RSS</a>
| <a href="http://apod.nasa.gov/apod/lib/edlinks.html">Education</a>
| <a href="http://apod.nasa.gov/apod/lib/about_apod.html">About APOD</a>
| <a href=
"http://asterisk.apod.com/discuss_apod.php?date=120506">Discuss</a>
| <a href="http://apod.nasa.gov/apod/ap120507.html">&gt;</a>

<hr><p>
<b> Authors & editors: </b>
<a href="http://www.phy.mtu.edu/faculty/Nemiroff.html">Robert Nemiroff</a>
(<a href="http://www.phy.mtu.edu/">MTU</a>) &
<a href="http://antwrp.gsfc.nasa.gov/htmltest/jbonnell/www/bonnell.html"
>Jerry Bonnell</a> (<a href="http://www.astro.umd.edu/">UMCP</a>)<br>
<b>NASA Official: </b> Phillip Newman
<a href="http://apod.nasa.gov/apod/lib/about_apod.html#srapply">Specific rights apply</a>.<br>
<a href="http://www.nasa.gov/about/highlights/HP_Privacy.html">NASA Web
Privacy Policy and Important Notices</a><br>
<b>A service of:</b>
<a href="http://astrophysics.gsfc.nasa.gov/">ASD</a> at
<a href="http://www.nasa.gov/">NASA</a> /
<a href="http://www.nasa.gov/centers/goddard/">GSFC</a>
<br><b>&</b> <a href="http://www.mtu.edu/">Michigan Tech. U.</a><br>
</center>
</body>
</html>
	    ]]>
	</description>
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    <item>
	<title><![CDATA[Full Moonrise]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap120505.html</link>
	<pubDate>Sat, 05 May 2012 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap120505.html"><img src="http://apod.nasa.gov/apod/image/1205/FullMoonriseArn600.jpg" /></a>
<title>Full Moonrise</title>

<a href="http://apod.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://apod.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://apod.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.

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    </item>

    <item>
	<title><![CDATA[Fermi Epicycles: The Vela Pulsar's Path]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap120504.html</link>
	<pubDate>Fri, 04 May 2012 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap120504.html"><img src="http://apod.nasa.gov/apod/image/1205/LatPolar_Vela900c.jpg" /></a>
<title>Fermi Epicycles: The Vela Pulsar's Path</title>

<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://apod.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://apod.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://apod.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.

	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[M106 Close Up]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap120503.html</link>
	<pubDate>Thu, 03 May 2012 13:06:01 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap120503.html"><img src="http://apod.nasa.gov/apod/image/1205/m106_lumhst_colorablock_red1h600.jpg" /></a>
<title>M106 Close Up</title>

Close to the <a href="http://www.astropix.com/HTML/C_SPRING/
BIGDIP.HTM">Great Bear</a>
(Ursa Major) and surrounded by the stars
of the
<a href="http://en.wikipedia.org/wiki/Canes_Venatici">Hunting Dogs</a>
(Canes Venatici), this celestial wonder was
<a href="http://www.seds.org/messier/Mdes/dm106.html">discovered</a>
in 1781 by the
<a href="http://www.french-metrology.com/en/history/
history-mesurement.asp">metric</a> French astronomer
<a href="http://www.seds.org/messier/xtra/history/
pmechain.html">Pierre Mechain</a>.

Later, it was added to the catalog of his friend and colleague
Charles Messier as
<a href="http://www.seds.org/messier/m/m106.html">M106</a>.

Modern deep telescopic views reveal it to be an
<a href="http://apod.nasa.gov/apod/ap080124.html">island universe</a>:
a spiral galaxy around 30 thousand light-years across located
only about 21 million light-years beyond the stars of the Milky Way.

Along with prominent dust lanes and a bright central core, 
<a href="http://www.astro-photo.nl/photoblog/index.php?showimage=188">this
colorful composite image</a> highlights
youthful blue star clusters and reddish stellar nurseries
that trace <a href="http://apod.nasa.gov/apod/ap070411.html">the galaxy's spiral arms</a>.

The high resolution galaxy portrait is a mosaic of data from Hubble's
sharp ACS camera combined with groundbased color image data.

M106 (aka NGC 4258) is a nearby example of the
<a href="http://apod.nasa.gov/apod/ap981023.html">Seyfert class</a> of active galaxies,
seen <a href="http://coolcosmos.ipac.caltech.edu/cosmic_classroom/
multiwavelength_astronomy/multiwavelength_astronomy/">across
the spectrum</a> from radio to X-rays.

Energetic active galaxies are powered by matter falling into a massive
<a href="http://www.cosmotography.com/images/
supermassive_blackholes_drive_galaxy_evolution_2.html">central black
hole</a>.

	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[Saturn's Moon Helene in Color </b> <br> ]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap120502.html</link>
	<pubDate>Wed, 02 May 2012 13:06:01 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap120502.html"><img src="http://apod.nasa.gov/apod/image/1205/helene2_cassini_960.jpg" /></a>
<title>Saturn's Moon Helene in Color </b> <br> </title>
Although its colors may be subtle, Saturn's moon Helene is an enigma in any light.

The <a href="http://www.planetary.org/blogs/emily-lakdawalla/2012/04201100.html"
>moon was imaged</a> in 
<a href="http://www.nasa.gov/mission_pages/cassini/whycassini/cassini20110620.html"
>unprecedented detail</a> last June as the 
<a href="http://saturn.jpl.nasa.gov/spacecraft/overview/">robotic 
Cassini spacecraft</a> orbiting Saturn 
<a href="http://www.youtube.com/watch?v=HiHSM-_fes4">swooped</a> 
to within a single Earth diameter of the 
<a href="http://en.wikipedia.org/wiki/Helene_%28moon%29">diminutive moon</a>.

Although conventional craters and hills 
<a href="http://apod.nasa.gov/apod/ap110623.html">appear</a>, the 
<a href="http://www.planetary.org/multimedia/space-images/helene-in-color.html"
>above</a>
<a href="http://photojournal.jpl.nasa.gov/catalog/PIA12773">image</a> also 
<a href="http://www.nasa.gov/mission_pages/cassini/whycassini/cassini20100308.html"
>shows</a> terrain that appears unusually smooth and streaked.

<a href="http://www.planetary.org/blogs/emily-lakdawalla/2011/3072.html">Planetary astronomers</a> are inspecting these detailed images of 
<a href="http://en.wikipedia.org/wiki/Helene_%28moon%29">Helene</a> to glean 
<a href="http://www.unmannedspaceflight.com/index.php?showtopic=7293">clues</a> 
about the origin and evolution of the 30-km across floating iceberg.

<a href="http://apod.nasa.gov/apod/ap951010.html">Helene</a> is also unusual because it circles 
Saturn just ahead of the large moon 
<a href="http://apod.nasa.gov/apod/ap070801.html">Dione</a>, making it one of only 
four known Saturnian moons to occupy a gravitational well known as a stable 
<a href="http://en.wikipedia.org/wiki/Lagrange_point">Lagrange point</a>.


<p> <center> 
<b> Dark Mysteries: </b>
<a href="http://asterisk.apod.com/ampersand/?p=292"
>Astronomy Seminar of the Week</a> <br>
<b> Tomorrow's picture: </b><a href="http://apod.nasa.gov/apod/ap120503.html">realm of the nebulae</a>

<p> <hr>
<a href="http://apod.nasa.gov/apod/ap120501.html">&lt;</a>
| <a href="http://apod.nasa.gov/apod/archivepix.html">Archive</a>
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| <a href=
"http://asterisk.apod.com/discuss_apod.php?date=120502">Discuss</a>
| <a href="http://apod.nasa.gov/apod/ap120503.html">&gt;</a>

<hr><p>
<b> Authors & editors: </b>
<a href="http://www.phy.mtu.edu/faculty/Nemiroff.html">Robert Nemiroff</a>
(<a href="http://www.phy.mtu.edu/">MTU</a>) &
<a href="http://antwrp.gsfc.nasa.gov/htmltest/jbonnell/www/bonnell.html"
>Jerry Bonnell</a> (<a href="http://www.astro.umd.edu/">UMCP</a>)<br>
<b>NASA Official: </b> Phillip Newman
<a href="http://apod.nasa.gov/apod/lib/about_apod.html#srapply">Specific rights apply</a>.<br>
<a href="http://www.nasa.gov/about/highlights/HP_Privacy.html">NASA Web
Privacy Policy and Important Notices</a><br>
<b>A service of:</b>
<a href="http://astrophysics.gsfc.nasa.gov/">ASD</a> at
<a href="http://www.nasa.gov/">NASA</a> /
<a href="http://www.nasa.gov/centers/goddard/">GSFC</a>
<br><b>&</b> <a href="http://www.mtu.edu/">Michigan Tech. U.</a><br>
</center>
</body>
</html>
	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[Higgs Boson Explained by Cartoon </b> <br> ]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap120501.html</link>
	<pubDate>Tue, 01 May 2012 13:06:02 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap120501.html"><img src="" /></a>
<title>Higgs Boson Explained by Cartoon </b> <br> </title>
What is all this fuss about the Higgs boson?

The physics community is abuzz that a fundamental particle expected by the largely successful
<a href="http://particleadventure.org/standard-model.html">Standard Model</a> of particle physics may be soon be found by the huge
<a href="http://apod.nasa.gov/apod/ap080225.html">Large Hadron Collider</a> (LHC) at
<a href=
"http://public.web.cern.ch/public/en/About/About-en.html">CERN</a> in Europe.

The term boson refers to a type of fundamental particle with similarities to the photon, while Higgs refers to
<a href="http://en.wikipedia.org/wiki/Peter_Higgs">Peter Higgs</a>, a physicist who among others published research predicting the
<a href="http://en.wikipedia.org/wiki/Higgs_mechanism"
>mechanism</a> through which such a particle might act.

The <a href="http://vimeo.com/41038445">above animated cartoon</a> explains in
<a href="http://en.wikipedia.org/wiki/PHD_Comics">humorous but impressive detail</a> why the
<a href="http://en.wikipedia.org/wiki/Higgs_boson">Higgs boson</a> is expected, and one method that the
<a href="http://www.youtube.com/watch?v=j50ZssEojtM">Large Hadron</> Collider is using to find it.

Although some
<a href=
"http://blogs.discovermagazine.com/cosmicvariance/2011/12/13/first-glimpse-of-the-higgs-boson-guest-post-from-jack-gunion/">rumors hint</a> that preliminary traces of the
<a href="http://www.guardian.co.uk/science/2011/dec/13/higgs-boson-lhc-explained">Higgs boson</a> are already being found, even
<a href=
"http://www.colourbox.com/preview/2305204-692955-one-curious-little-cat-searching-a-billiards-table.jpg">not finding</a> this
<a href="http://asterisk.apod.com/viewforum.php?f=39">unusual</a> particle would open the door to a new
<a href="http://superstringtheory.com/">fundamental understanding</a> of how our universe works.


<p> <center> 
<b> Tomorrow's picture: </b><a href="http://apod.nasa.gov/apod/ap120502.html">open space</a>

<p> <hr>
<a href="http://apod.nasa.gov/apod/ap120430.html">&lt;</a>
| <a href="http://apod.nasa.gov/apod/archivepix.html">Archive</a>
| <a href="http://apod.nasa.gov/apod/lib/aptree.html">Index</a>
| <a href="http://antwrp.gsfc.nasa.gov/cgi-bin/apod/apod_search">Search</a>
| <a href="http://apod.nasa.gov/apod/calendar/allyears.html">Calendar</a>
| <a href="http://apod.nasa.gov/apod//apod.rss">RSS</a>
| <a href="http://apod.nasa.gov/apod/lib/edlinks.html">Education</a>
| <a href="http://apod.nasa.gov/apod/lib/about_apod.html">About APOD</a>
| <a href=
"http://asterisk.apod.com/discuss_apod.php?date=120501">Discuss</a>
| <a href="http://apod.nasa.gov/apod/ap120502.html">&gt;</a>

<hr><p>
<b> Authors & editors: </b>
<a href="http://www.phy.mtu.edu/faculty/Nemiroff.html">Robert Nemiroff</a>
(<a href="http://www.phy.mtu.edu/">MTU</a>) &
<a href="http://antwrp.gsfc.nasa.gov/htmltest/jbonnell/www/bonnell.html"
>Jerry Bonnell</a> (<a href="http://www.astro.umd.edu/">UMCP</a>)<br>
<b>NASA Official: </b> Phillip Newman
<a href="http://apod.nasa.gov/apod/lib/about_apod.html#srapply">Specific rights apply</a>.<br>
<a href="http://www.nasa.gov/about/highlights/HP_Privacy.html">NASA Web
Privacy Policy and Important Notices</a><br>
<b>A service of:</b>
<a href="http://astrophysics.gsfc.nasa.gov/">ASD</a> at
<a href="http://www.nasa.gov/">NASA</a> /
<a href="http://www.nasa.gov/centers/goddard/">GSFC</a>
<br><b>&</b> <a href="http://www.mtu.edu/">Michigan Tech. U.</a><br>
</center>
</body>
</html>
	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[Aurora Over Raufarhofn </b> <br> ]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap120430.html</link>
	<pubDate>Mon, 30 Apr 2012 18:22:04 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap120430.html"><img src="http://apod.nasa.gov/apod/image/1204/arctichenge_vetter_960.jpg" /></a>
<title>Aurora Over Raufarhofn </b> <br> </title>
It was all lined up even without the colorful aurora exploding overhead.

If you follow the apex line of the recently deployed monuments of
<a href="http://sagatrail.is/index.php/en/22arctichenge">Arctic Henge</a> in
<a href="http://en.wikipedia.org/wiki/Raufarhofn">Raufarhofn</a> in northern
<a href="http://en.wikipedia.org/wiki/Iceland">Iceland</a> from this vantage point, you will see that they point due north.

A good way to tell is to follow their apex line to the line connecting the end stars of the
<a href="http://apod.nasa.gov/apod/ap110624.html">Big Dipper, Merak and Dubhe</a>, toward
<a href="http://stars.astro.illinois.edu/sow/polaris.html">Polaris</a>, the bright star near the north
<a href="http://www.youtube.com/watch?v=fD3P_l2sZFI"
>spin axis</a> of the Earth projected onto the sky.  

By design, from this <a href="
http://erasundar.files.wordpress.com/2009/07/cat-peering-into-fishbowl.jpg?w=455&h=322">vantage point</a>, this same apex line will also point directly at the
<a href="http://en.wikipedia.org/wiki/Midnight_sun">midnight sun</a>
at its highest point in the sky just during the
<a href="http://en.wikipedia.org/wiki/Solstice">summer solstice</a> of Earth's northern hemisphere.

In other words, the Sun will not set at
<a href="http://www.heimskautsgerdi.is/">Arctic Henge</a> during the summer solstice in late June, and at its
<a href="http://apod.nasa.gov/apod/ap080922.html">highest point in the sky</a> it will appear just above the aligned vertices of this modern monument.

The above image was taken in late March during a
<a href="http://apod.nasa.gov/apod/ap110517.html">beautiful auroral storm</a>.


<p> <center> 
<b> Tomorrow's picture: </b><a href="http://apod.nasa.gov/apod/ap120501.html">cartoon higgs</a>

<p> <hr>
<a href="http://apod.nasa.gov/apod/ap120429.html">&lt;</a>
| <a href="http://apod.nasa.gov/apod/archivepix.html">Archive</a>
| <a href="http://apod.nasa.gov/apod/lib/aptree.html">Index</a>
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| <a href="http://apod.nasa.gov/apod/calendar/allyears.html">Calendar</a>
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| <a href="http://apod.nasa.gov/apod/lib/edlinks.html">Education</a>
| <a href="http://apod.nasa.gov/apod/lib/about_apod.html">About APOD</a>
| <a href=
"http://asterisk.apod.com/discuss_apod.php?date=120430">Discuss</a>
| <a href="http://apod.nasa.gov/apod/ap120501.html">&gt;</a>

<hr><p>
<b> Authors & editors: </b>
<a href="http://www.phy.mtu.edu/faculty/Nemiroff.html">Robert Nemiroff</a>
(<a href="http://www.phy.mtu.edu/">MTU</a>) &
<a href="http://antwrp.gsfc.nasa.gov/htmltest/jbonnell/www/bonnell.html"
>Jerry Bonnell</a> (<a href="http://www.astro.umd.edu/">UMCP</a>)<br>
<b>NASA Official: </b> Phillip Newman
<a href="http://apod.nasa.gov/apod/lib/about_apod.html#srapply">Specific rights apply</a>.<br>
<a href="http://www.nasa.gov/about/highlights/HP_Privacy.html">NASA Web
Privacy Policy and Important Notices</a><br>
<b>A service of:</b>
<a href="http://astrophysics.gsfc.nasa.gov/">ASD</a> at
<a href="http://www.nasa.gov/">NASA</a> /
<a href="http://www.nasa.gov/centers/goddard/">GSFC</a>
<br><b>&</b> <a href="http://www.mtu.edu/">Michigan Tech. U.</a><br>
</center>
</body>
</html>
	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[A Dangerous Sunrise on Gliese 876d </b> <br> ]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap120429.html</link>
	<pubDate>Sun, 29 Apr 2012 13:06:01 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap120429.html"><img src="http://apod.nasa.gov/apod/image/1204/reddwarf_nielsen_960.jpg" /></a>
<title>A Dangerous Sunrise on Gliese 876d </b> <br> </title>
On planet Gliese 876d, sunrises might be dangerous.

Although nobody really knows what conditions are like on this close-in planet orbiting variable
<a href="http://en.wikipedia.org/wiki/Red_dwarf">red dwarf</a> star
<a href="http://en.wikipedia.org/wiki/Gliese_876">Gliese 876</a>, the
above artistic illustration gives one impression.

With an orbit well inside
<a href="http://www.nineplanets.org/mercury.html">Mercury</a>
and a mass several times that of Earth,
<a href="http://en.wikipedia.org/wiki/Gliese_876_d">Gliese 876d</a> might
<a href="http://www.nature.com/nature/journal/v429/n6994/full/nature02609.html"
>rotate so slowly</a> that dramatic differences exist between night and day.  

<a href="http://exoplanets.org/gl876_web/gl876_graphics.html">Gliese 876d</a>
is imagined above showing significant
<a href="http://apod.nasa.gov/apod/ap051002.html">volcanism</a>, possibly caused by
<a href="http://burro.astr.cwru.edu/Academics/Astr221/Gravity/tides.html"
>gravitational tides</a> flexing and
<a href="http://apod.nasa.gov/apod/ap040502.html">internally heating</a> the planet,
and possibly more volatile during the day.  

The rising
<a href="http://www.youtube.com/watch?v=LRq_SAuQDec"
>red dwarf</a>
star shows expected stellar
<a href="http://apod.nasa.gov/apod/ap060710.html">magnetic activity</a> which includes
<a href="http://apod.nasa.gov/apod/ap060416.html">dramatic</a> and
<a href="http://apod.nasa.gov/apod/ap000403.html">violent prominences</a>.

In the sky above, a hypothetical moon has its
thin atmosphere blown away by the red dwarf's
<a href="http://apod.nasa.gov/apod/ap000318.html">stellar wind</a>.

Gliese 876d excites the
<a href="http://apod.nasa.gov/apod/ap070502.html">imagination</a> partly because it is one of the few
<a href="http://exoplanet.eu/">extrasolar planets</a>
known to be
<a href="http://apod.nasa.gov/apod/ap101001.html">in</a> or
<a href="http://apod.nasa.gov/apod/ap111207.html">near</a> to the
<a href="http://www.pbs.org/lifebeyondearth/alone/habitable.html"
>habitable zone</a> of its parent star.

<p> <center> 
<b> Tomorrow's picture: </b><a href="http://apod.nasa.gov/apod/ap120430.html">apex aurora</a>

<p> <hr>
<a href="http://apod.nasa.gov/apod/ap120428.html">&lt;</a>
| <a href="http://apod.nasa.gov/apod/archivepix.html">Archive</a>
| <a href="http://apod.nasa.gov/apod/lib/aptree.html">Index</a>
| <a href="http://antwrp.gsfc.nasa.gov/cgi-bin/apod/apod_search">Search</a>
| <a href="http://apod.nasa.gov/apod/calendar/allyears.html">Calendar</a>
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| <a href="http://apod.nasa.gov/apod/lib/edlinks.html">Education</a>
| <a href="http://apod.nasa.gov/apod/lib/about_apod.html">About APOD</a>
| <a href=
"http://asterisk.apod.com/discuss_apod.php?date=120429">Discuss</a>
| <a href="http://apod.nasa.gov/apod/ap120430.html">&gt;</a>

<hr><p>
<b> Authors & editors: </b>
<a href="http://www.phy.mtu.edu/faculty/Nemiroff.html">Robert Nemiroff</a>
(<a href="http://www.phy.mtu.edu/">MTU</a>) &
<a href="http://antwrp.gsfc.nasa.gov/htmltest/jbonnell/www/bonnell.html"
>Jerry Bonnell</a> (<a href="http://www.astro.umd.edu/">UMCP</a>)<br>
<b>NASA Official: </b> Phillip Newman
<a href="http://apod.nasa.gov/apod/lib/about_apod.html#srapply">Specific rights apply</a>.<br>
<a href="http://www.nasa.gov/about/highlights/HP_Privacy.html">NASA Web
Privacy Policy and Important Notices</a><br>
<b>A service of:</b>
<a href="http://astrophysics.gsfc.nasa.gov/">ASD</a> at
<a href="http://www.nasa.gov/">NASA</a> /
<a href="http://www.nasa.gov/centers/goddard/">GSFC</a>
<br><b>&</b> <a href="http://www.mtu.edu/">Michigan Tech. U.</a><br>
</center>
</body>
</html>
	    ]]>
	</description>
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    <item>
	<title><![CDATA[Sutter's Mill Meteorite]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap120428.html</link>
	<pubDate>Sat, 28 Apr 2012 13:06:02 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap120428.html"><img src="http://apod.nasa.gov/apod/image/1204/ACD12-0067-001jenniskens900.jpg" /></a>
<title>Sutter's Mill Meteorite</title>

<a href="http://asterisk.apod.com/
viewtopic.php?f=8&t=28345">Last Sunday's bright fireball meteor</a>
falling through skies over
California and Nevada produced sonic booms over a broad area around
7:21 am.

Estimates indicate the meteor was about the size of a minivan.

Astronomer Peter Jenniskens subsequently recovered these fragments of
a crushed 4 gram meteorite, the second find from
<a href="http://www.seti.org/seti-institute/news/meteorite-alert">this
meteor fall</a>, in the parking lot of the Henningsen-Lotus state park,
not far from
<a href="http://en.wikipedia.org/wiki/Sutter%27s_Mill">Sutter's Mill</a>.

This is now known as the Sutter's Mill Meteorite, the location
famous for its association with the California Gold Rush.

The meteorite may well be astronomer's gold too,
thought to be a rare
<a href="http://en.wikipedia.org/wiki/
Carbonaceous_chondrite">CM type carbonaceous chondrite</a>,
a type rich in organic compounds and similar to the
Murchison Meteorite.

To trace the meteor's orbit, details of its breakup, and aid in
locating more fragements, scientists are also searching for video
records.

Security cameras across a wide area could have accidently
captured the fireball event near 7:21 am PDT on April 22;
e.g. California (SF Bay Area, Los Angeles,
near Redding) and Nevada (Reno area, Tonopah), even in southern
parts of Oregon and near Salt Lake City in Utah.

If you have video footage of the event,
<a href="http://www.nasa.gov/centers/ames/news/releases/2012/
M12-41.html">please use the contact information here</a>.

	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[Jupiter and the Moons of Earth]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap120427.html</link>
	<pubDate>Fri, 27 Apr 2012 13:06:01 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap120427.html"><img src="http://apod.nasa.gov/apod/image/1204/MoonJupiterISS_Seip900.jpg" /></a>
<title>Jupiter and the Moons of Earth</title>

<a href="http://apod.nasa.gov/apod/ap050430.html">Planet Earth has many moons</a>.

Its largest artifical moon, the
<a href="http://www.nasa.gov/mission_pages/station/main/
index.html">International Space Station</a>, streaks
through this lovely skyview with clouds in silhouette
against the fading light of
<a href="http://apod.nasa.gov/apod/ap080531.html">a sunset</a>.

Captured from Stuttgart, Germany last Sunday,
the frame also includes Earth's
largest natural satellite 1.5 days after its New Moon phase.

Just below and left of the
<a href="http://apod.nasa.gov/apod/ap020419.html">young crescent</a> is Jupiter, another
<a href="http://earthsky.org/astronomy-essentials/
visible-planets-tonight-mars-jupiter-venus-saturn-mercury">bright
celestial beacon</a> hovering near
the western horizon in early evening skies.

Only <a href="http://www.heavens-above.com/">briefly, as
seen</a> from the photographer's location,
Jupiter and these moons of Earth formed the remarkably close
triple conjunction.

<a href="http://vimeo.com/35740232">Of course, Jupiter</a>
has many moons too.

In fact, close inspection of the photo will reveal tiny pin pricks
of light near the bright planet,
large natural satellites of Jupiter known
<a href="http://apod.nasa.gov/apod/ap091023.html">as Galilean moons</a>.

	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[Morning, Moon, and Mercury]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap120426.html</link>
	<pubDate>Thu, 26 Apr 2012 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap120426.html"><img src="http://apod.nasa.gov/apod/image/1204/MoonMercuryBrisbane_Mudge900.jpg" /></a>
<title>Morning, Moon, and Mercury</title>

Last week
<a href="http://www.fourmilab.ch/images/3planets/elongation.html">Mercury
wandered far</a> to the west of the Sun.

As the solar system's
<a href="http://solarsystem.nasa.gov/planets/
profile.cfm?Object=Mercury">innermost planet</a>
neared its greatest elongation
or greatest angle from the Sun (for this apparition about 27 degrees)
it was joined by an <a href="http://apod.nasa.gov/apod/ap120324.html">old crescent Moon</a>.

The conjunction was an engaging
<a href="http://www.iceinspace.com.au/forum/showthread.php?t=89703">sight
for early morning risers</a>
in the southern hemisphere.

There the pair rose together in predawn skies, climbing
high above the horizon along a steeply inclined
<a href="http://apod.nasa.gov/apod/ap120405.html">ecliptic plane</a>.

This well composed sequence captures the rising Moon and Mercury
above the city lights of
<a href="http://spaceflight.nasa.gov/gallery/images/station/
crew-28/html/iss028e050186.html">Brisbane</a> in Queensland, Australia.

A stack of digital images, it consists of an exposure made
every 3 minutes beginning at 4:15 am local time on
April 19.

Mercury's track is at the far right, separated from
the Moon's path by about 8 degrees.

	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[Meteor Over Crater Lake </b> <br> ]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap120425.html</link>
	<pubDate>Wed, 25 Apr 2012 13:06:02 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap120425.html"><img src="http://apod.nasa.gov/apod/image/1204/lyridcrater_goldpaint_960.jpg" /></a>
<title>Meteor Over Crater Lake </b> <br> </title>
Did you see it? 

One of the more common questions during a meteor shower occurs because the time it takes for a meteor to flash is typically less than the time it takes for a head to turn.

Possibly, though, the glory of seeing 
<a href="http://apod.nasa.gov/apod/ap070812.html">bright meteors</a> shoot across and 
<a href="http://www.amsmeteors.org/meteor-showers/meteor-faq/">knowing that</a> 
they were once small pebbles on another world might make it all worthwhile, even if your 
<a href="http://27.media.tumblr.com/tumblr_lns72yE4mS1qhwmnpo1_500.jpg"
>observing partner(s)</a> could not share in every particular experience.

Peaking over the past few days, a dark moonless sky allowed the 
<a href="http://en.wikipedia.org/wiki/Lyrids">Lyrids meteor shower</a> 
to exhibit as many as 30 visible meteors per hour from some locations.

A <a href="http://apod.nasa.gov/apod/ap090501.html">bright Lyrid meteor</a> streaks above picturesque 
<a href="http://en.wikipedia.org/wiki/Crater_Lake">Crater Lake</a> in 
<a href="http://en.wikipedia.org/wiki/Oregon">Oregon</a>, 
<a href="https://www.cia.gov/library/publications/the-world-factbook/geos/us.html"
>USA</a>, in the 
<a href="http://portfolio.goldpaintphotography.com/p460476961/h111327bd"
>above composite</a> of nine exposures taken last week.

Snow covers the 
<a href="http://www.youtube.com/watch?v=8Eq-xBvLqXs">foreground</a>, 
while the majestic central band of our home galaxy arches well behind the serene lake.

<a href="http://earthsky.org/astronomy-essentials/earthskys-meteor-shower-guide"
>Other meteor showers</a> this year include the 
<a href="http://en.wikipedia.org/wiki/Perseids">Perseids</a> in mid-August and the Leonids in mid-November, both expected to also dodge the 
<a href="http://27.media.tumblr.com/tumblr_lns72yE4mS1qhwmnpo1_500.jpg"
>glare</a> of a bright Moon in 2012.


<p> <center> 
<b> Tomorrow's picture: </b><a href="http://apod.nasa.gov/apod/ap120426.html">open space</a>

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<hr><p>
<b> Authors & editors: </b>
<a href="http://www.phy.mtu.edu/faculty/Nemiroff.html">Robert Nemiroff</a>
(<a href="http://www.phy.mtu.edu/">MTU</a>) &
<a href="http://antwrp.gsfc.nasa.gov/htmltest/jbonnell/www/bonnell.html"
>Jerry Bonnell</a> (<a href="http://www.astro.umd.edu/">UMCP</a>)<br>
<b>NASA Official: </b> Phillip Newman
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<a href="http://www.nasa.gov/centers/goddard/">GSFC</a>
<br><b>&</b> <a href="http://www.mtu.edu/">Michigan Tech. U.</a><br>
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