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		  <channel>
			<title>Pic  @ zorg.ch</title>
			<link>http://www.zorg.ch/forum.php</link>
			<description>Zorg RSS Feed</description>
			<language>de-DE</language>
			<lastBuildDate>Sat, 04 Sep 2010 20:59:25</lastBuildDate><item>
							<title>The Small Cloud of M</title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=13576&parent_id=13576#112751</link>
							<pubDate>Sat, 04 Sep 2010 00:00:07</pubDate>
							<author>[z]Barbara Harris</author>
							<category><![CDATA[Pic: The Small Cloud of M]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=13576&parent_id=13576#112751</guid>
							<description><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1009/SMC_jarzyna.jpg'><b>The Small Cloud of Magellan </b></a><br>
			 <br>Explanation: </b>

Portuguese navigator
<a href="http://www.fordham.edu/halsall/mod/1519magellan.html">Ferdinand Magellan</a> and his crew had plenty
of time to study the southern sky during the
first circumnavigation of planet Earth.
...]]></description>
							<content:encoded><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1009/SMC_jarzyna.jpg'><b>The Small Cloud of Magellan </b></a><br>
			 <br>Explanation: </b>

Portuguese navigator
<a href="http://www.fordham.edu/halsall/mod/1519magellan.html">Ferdinand Magellan</a> and his crew had plenty
of time to study the southern sky during the
first circumnavigation of planet Earth.

As a result, two celestial wonders
easily visible for southern hemisphere skygazers
are known as the Clouds of Magellan.

These cosmic clouds are now understood to be dwarf
irregular galaxies,
<a href="http://www.atlasoftheuniverse.com/sattelit.html">satellites
of our larger spiral</a> Milky Way Galaxy.

The <a href="http://www.seds.org/messier/xtra/ngc/smc.html">Small
Magellanic Cloud</a>
actually spans 15,000 light-years or so
and contains several hundred million stars.

About 210,000 light-years away in the constellation
<a href="http://www.hawastsoc.org/deepsky/tuc/">Tucana</a>,
it is more distant than other known Milky Way
satellite galaxies, including the
<a href="http://www.seds.org/messier/more/cma_dw.html">Canis Major</a>
and
<a href="http://www.seds.org/messier/more/sagdeg.html">Sagittarius
Dwarf</a> galaxies and the
<a href="http://www.seds.org/messier/xtra/ngc/lmc.html">Large
Magellanic Cloud</a>.

<a href="http://www.starrysite.com/index.php?site=galleryitem,218">This
sharp image</a> also includes two foreground globular
star clusters NGC 362 (bottom right) and 47 Tucanae.

Spectacular <a href="http://antwrp.gsfc.nasa.gov/apod/ap080826.html">47 Tuc</a>anae
is a mere 13,000 light-years away and seen here to the left of the
<a href="http://coolcosmos.ipac.caltech.edu/cosmic_classroom/multiwavelength_astronomy/multiwavelength_museum/smc.html">Small Magellanic Cloud</a>.

 

<a href="http://chandra.harvard.edu/mobile/aa.html">Take a short
survey</a> about viewing astronomy images on mobile devices.
 <br><br><a href='http://antwrp.gsfc.nasa.gov/apod/ap100903.html'>Credit &amp; Copyright</a>]]></content:encoded>
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							<title>The Bubble Nebula </title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=13575&parent_id=13575#112750</link>
							<pubDate>Fri, 03 Sep 2010 00:00:04</pubDate>
							<author>[z]Barbara Harris</author>
							<category><![CDATA[Pic: The Bubble Nebula ]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=13575&parent_id=13575#112750</guid>
							<description><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1009/ngc7635_jurasevich_full.jpg'><b>The Bubble Nebula </b></a><br>
			 <br>Explanation: </b>

Blown by the wind from a massive star, this interstellar
apparition has a surprisingly
<a href="http://www.exploratorium.edu/ronh/bubbles/bubbles.html">familiar shape</a>.

Cataloged as NGC 7635, it is also known s...]]></description>
							<content:encoded><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1009/ngc7635_jurasevich_full.jpg'><b>The Bubble Nebula </b></a><br>
			 <br>Explanation: </b>

Blown by the wind from a massive star, this interstellar
apparition has a surprisingly
<a href="http://www.exploratorium.edu/ronh/bubbles/bubbles.html">familiar shape</a>.

Cataloged as NGC 7635, it is also known simply
as <a href="http://heritage.stsci.edu/1998/31/index.html">The
Bubble Nebula</a>.

Although it looks delicate, the 10 light-year diameter
bubble offers evidence of
<a href="http://antwrp.gsfc.nasa.gov/apod/ap080117.html">violent processes</a> at work.

Above and right of the Bubble's center is a hot,
<a href="http://antwrp.gsfc.nasa.gov/apod/ap070726.html">O-type star</a>, several hundred thousand
times more luminous and approximately 45 times more massive
than the Sun.

A fierce stellar wind and intense radiation from that
star has blasted out the
<a href="http://adsabs.harvard.edu/cgi-bin/nph-bib_query?
bibcode=1995A%26A...295..509C">structure of glowing gas</a>
against denser material
<a href="http://antwrp.gsfc.nasa.gov/apod/ap060428.html">in a surrounding</a>
<a href="http://archive.ncsa.uiuc.edu/Cyberia/Bima/GMC.html">molecular
cloud</a>.

The intriguing Bubble Nebula lies a mere
11,000 light-years away toward the boastful constellation
<a href="http://www.hawastsoc.org/deepsky/cas/index.html">Cassiopeia</a>.

A false-color
<a href="http://hubblesite.org/gallery/behind_the_pictures/meaning_of_color/eagle.php">Hubble palette</a> was used to create
this sharp image and
shows emission from sulfur, hydrogen, and oxygen atoms in red,
green, and blue hues. 

<a href="http://www.starimager.com/Image%20Gallery%20Pages/Celestial%20Oddities/ngc%207635%20Bubble%20Nebula_false%20color_1250.html">The image data</a>
was recorded using a small telescope under
clear, steady skies, from Mount Wilson Observatory.

 

 Battle of the APODs (Poll): </b>
<a href="http://bb.nightskylive.net/asterisk/viewtopic.php?f=29&t=20892">Which APOD should be last week's APOW?</a> 
 <br><br><a href='http://antwrp.gsfc.nasa.gov/apod/ap100902.html'>Credit &amp; Copyright</a>]]></content:encoded>
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							<title>Earth and Moon from </title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=13574&parent_id=13574#112748</link>
							<pubDate>Thu, 02 Sep 2010 00:00:05</pubDate>
							<author>[z]Barbara Harris</author>
							<category><![CDATA[Pic: Earth and Moon from ]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=13574&parent_id=13574#112748</guid>
							<description><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1009/earthmoon_messenger_big.png'><b>Earth and Moon from MESSENGER </b></a><br>
			 <br>Explanation: </b>
What does Earth look like from the planet Mercury?

The robotic spacecraft 
<a href="http://messenger.jhuapl.edu/the_mission/index.html">MESSENGER</a> 
found out as it looked toward the 
<a href="http://...]]></description>
							<content:encoded><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1009/earthmoon_messenger_big.png'><b>Earth and Moon from MESSENGER </b></a><br>
			 <br>Explanation: </b>
What does Earth look like from the planet Mercury?

The robotic spacecraft 
<a href="http://messenger.jhuapl.edu/the_mission/index.html">MESSENGER</a> 
found out as it looked toward the 
<a href="http://antwrp.gsfc.nasa.gov/apod/ap070325.html">Earth</a> during its closest approach to the 
<a href="http://en.wikipedia.org/wiki/Sun">Sun</a> about three months ago.  

The <a href="http://antwrp.gsfc.nasa.gov/apod/ap080903.html">Earth and Moon</a> 
are visible as the double spot on the lower left of the 
<a href="http://messenger.jhuapl.edu/gallery/sciencePhotos/image.php?image_id=388">above image</a>.  

Now MESSENGER was not at Mercury when it took the above image, but at a 
<a href="http://www.youtube.com/watch?v=otF2FjpCyZk">location</a> 
from which the view would be similar.  

From Mercury, both the 
<a href="http://antwrp.gsfc.nasa.gov/apod/ap030526.html">Earth</a> and its 
<a href="http://antwrp.gsfc.nasa.gov/apod/ap011015.html">comparatively large moon</a> will always appear as small circles of reflected sunlight and will never show a 
<a href="http://antwrp.gsfc.nasa.gov/apod/ap091213.html">crescent</a> phase.  

MESSENGER has zipped right by 
<a href="http://antwrp.gsfc.nasa.gov/apod/ap080121.html">Mercury</a> three 
<a href="http://antwrp.gsfc.nasa.gov/apod/ap081008.html">times</a> since being 
<a href="http://antwrp.gsfc.nasa.gov/apod/ap040814.html">launched</a> in 2004, and is scheduled to enter orbit around the innermost planet in March of 2011.

 
 New Mirror: </b>
<a href="http://iranapod.com/default.aspx">APOD available in Persian from Iran.</a> 
 <br><br><a href='http://antwrp.gsfc.nasa.gov/apod/ap100901.html'>Credit &amp; Copyright</a>]]></content:encoded>
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							<title>The Annotated Galact</title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=13573&parent_id=13573#112747</link>
							<pubDate>Wed, 01 Sep 2010 00:00:05</pubDate>
							<author>[z]Barbara Harris</author>
							<category><![CDATA[Pic: The Annotated Galact]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=13573&parent_id=13573#112747</guid>
							<description><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1008/gcenter_fernandez_big.jpg'><b>The Annotated Galactic Center </b></a><br>
			 <br>Explanation: </b>
The sky toward the
<a href="http://en.wikipedia.org/wiki/Galactic_center">center of our Galaxy</a> is filled with a wide variety of
<a href="http://antwrp.gsfc.nasa.gov/apod/ap090925.html">celestial wonder...]]></description>
							<content:encoded><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1008/gcenter_fernandez_big.jpg'><b>The Annotated Galactic Center </b></a><br>
			 <br>Explanation: </b>
The sky toward the
<a href="http://en.wikipedia.org/wiki/Galactic_center">center of our Galaxy</a> is filled with a wide variety of
<a href="http://antwrp.gsfc.nasa.gov/apod/ap090925.html">celestial wonders</a>,
many of which are visible from a dark location with common
<a href="http://www.nightskyinfo.com/binoculars/">binoculars</a>.

Constellations near the
<a href="http://www.youtube.com/watch?v=36xZsgZ0oSo">Galactic Center</a> include
<a href="http://www.hawastsoc.org/deepsky/sgr/index.html">Sagittarius</a>,
<a href="http://www.hawastsoc.org/deepsky/lib/index.html">Libra</a>,
<a href="http://www.hawastsoc.org/deepsky/sco/index.html">Scorpius</a>,
<a href="http://www.hawastsoc.org/deepsky/sct/index.html">Scutum</a>, and
<a href="http://www.hawastsoc.org/deepsky/oph/index.html">Ophiuchus</a>.

Nebulas include
<a href="http://en.wikipedia.org/wiki/Charles_Messier">Messier</a> objects
<a href="http://antwrp.gsfc.nasa.gov/apod/ap100805.html">M8</a>,
<a href="http://antwrp.gsfc.nasa.gov/apod/ap090208.html">M16</a>,
<a href="http://antwrp.gsfc.nasa.gov/apod/ap090707.html">M20</a>, as well as the
<a href="http://antwrp.gsfc.nasa.gov/apod/ap020526.html">Pipe</a> and
<a href="http://antwrp.gsfc.nasa.gov/apod/ap100421.html">Cat's Paw</a> nebulas.

Visible
<a href="http://en.wikipedia.org/wiki/Open_cluster">open star clusters</a> include
<a href="http://antwrp.gsfc.nasa.gov/apod/ap990106.html">M6</a>,
<a href="http://antwrp.gsfc.nasa.gov/apod/ap091108.html">M7</a>,
<a href="http://en.wikipedia.org/wiki/Messier_21">M21</a>,
<a href="http://en.wikipedia.org/wiki/Messier_23">M23</a>,
<a href="http://antwrp.gsfc.nasa.gov/apod/ap040921.html">M24</a>, and
<a href="http://antwrp.gsfc.nasa.gov/apod/ap090831.html">M25</a>, while
<a href="http://antwrp.gsfc.nasa.gov/apod/globular_clusters.html">globular star cluster</a>
<a href="http://antwrp.gsfc.nasa.gov/apod/ap010703.html">M22</a> is also visible.

A hole in the dust toward the
<a href="http://antwrp.gsfc.nasa.gov/apod/ap011229.html">Galactic Center</a> reveals a bright region filled with distant stars known as
<a href="http://antwrp.gsfc.nasa.gov/apod/ap071219.html">Baade's Window</a>, which is visible between
<a href="http://antwrp.gsfc.nasa.gov/apod/ap040222.html">M7</a> and
<a href="http://antwrp.gsfc.nasa.gov/apod/ap070804.html">M8</a>.


Moving your cursor over the
<a href="http://www.castillosdesoria.com/astropics/imagen.asp?id=1&seccion=1&id_prod=246">above image</a> the will bring up an un-annotated version.


 
 Poll: </b>
<a href="http://bb.nightskylive.net/asterisk/viewtopic.php?f=29&t=20858">Which images would you select for future APODs?</a> 
 <br><br><a href='http://antwrp.gsfc.nasa.gov/apod/ap100831.html'>Credit &amp; Copyright</a>]]></content:encoded>
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							<title>Comanche Outcrop on </title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=13572&parent_id=13572#112744</link>
							<pubDate>Tue, 31 Aug 2010 00:00:05</pubDate>
							<author>[z]Barbara Harris</author>
							<category><![CDATA[Pic: Comanche Outcrop on ]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=13572&parent_id=13572#112744</guid>
							<description><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1008/comancheoutcrop_spirit_big_annotated.jpg'><b>Comanche Outcrop on Mars Indicates Hospitable Past </b></a><br>
			 <br>Explanation: </b>
Could life once have survived on Mars?

Today, neither
<a href="http://tolweb.org/tree/">animal</a> nor
<a href="http://en.wikipedia.org/wiki/Plant">plant</a> life from
...]]></description>
							<content:encoded><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1008/comancheoutcrop_spirit_big_annotated.jpg'><b>Comanche Outcrop on Mars Indicates Hospitable Past </b></a><br>
			 <br>Explanation: </b>
Could life once have survived on Mars?

Today, neither
<a href="http://tolweb.org/tree/">animal</a> nor
<a href="http://en.wikipedia.org/wiki/Plant">plant</a> life from
<a href="http://antwrp.gsfc.nasa.gov/apod/ap070325.html">Earth</a> could survive for very long on
<a href="http://antwrp.gsfc.nasa.gov/apod/mars.html">Mars</a> because at least one key ingredient -- liquid
<a href="http://antwrp.gsfc.nasa.gov/apod/ap980530.html">water</a> -- is essentially absent on the red planet's rusty surface.

Although evidence from the
<a href="http://marsrovers.jpl.nasa.gov/home/index.html">martian rovers</a> indicates that long ago
<a href="http://antwrp.gsfc.nasa.gov/apod/ap040303.html">Mars might</a> once have had
liquid water on its surface, that water might also have been
<a href="http://www.ehow.com/list_6383560_dangers-acidic-water.html">too acidic</a> for familiar life forms to thrive.  

Recently, however, a newly detailed analysis of an unusual outcropping of rock and soil chanced upon in 2005 by the robotic
<a href="http://antwrp.gsfc.nasa.gov/apod/ap051214.html">Spirit rover</a> has uncovered a clue indicating that not all of Mars was always so acidic.

The mound  in question, dubbed
<a href="http://www.nasa.gov/mission_pages/mer/multimedia/gallery/pia10126-label.html">Comanche</a> Outcrop and visible near the top of the
<a href="http://photojournal.jpl.nasa.gov/catalog/PIA13175">above image</a>, appears to contain unusually
high concentrations of elements such as magnesium iron
<a href="http://en.wikipedia.org/wiki/Carbonate">carbonate</a>.

The <a href="http://photojournal.jpl.nasa.gov/catalog/PIA13175">above image</a> is shown in colors exaggerated to highlight the differences in composition.

Since these
<a href="http://en.wikipedia.org/wiki/Carbonates_on_Mars">carbonates</a>
<a href="http://www.youtube.com/watch?v=uDBWUV6aTQE">dissolve</a> in acid, the persistence of these mounds indicates that water perhaps less
<a href="http://en.wikipedia.org/wiki/Acid">acidic</a> and more
<a href="http://www.astro.wisc.edu/~townsend/static.php?ref=diploma-3">favorable for life</a> might have once flowed across Mars.

More detailed analyses and searches for other signs will surely continue.

 
 Teachers & Students: </b>
<a href="http://bb.nightskylive.net/asterisk/viewforum.php?f=24">Take an online, textbook-free, video class on Introductory Astronomy for free.</a> 
 <br><br><a href='http://antwrp.gsfc.nasa.gov/apod/ap100830.html'>Credit &amp; Copyright</a>]]></content:encoded>
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							<title>The Local Fluff </title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=13571&parent_id=13571#112742</link>
							<pubDate>Mon, 30 Aug 2010 00:00:04</pubDate>
							<author>[z]Barbara Harris</author>
							<category><![CDATA[Pic: The Local Fluff ]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=13571&parent_id=13571#112742</guid>
							<description><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1008/localcloud_frisch_big.gif'><b>The Local Fluff </b></a><br>
			 <br>Explanation: </b>
The stars are not alone.  

In the disk of our
<a href="http://antwrp.gsfc.nasa.gov/apod/milky_way.html">Milky Way Galaxy</a>
about 10 percent of visible matter is in the form of gas, called the
<a href="http://www-ssg....]]></description>
							<content:encoded><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1008/localcloud_frisch_big.gif'><b>The Local Fluff </b></a><br>
			 <br>Explanation: </b>
The stars are not alone.  

In the disk of our
<a href="http://antwrp.gsfc.nasa.gov/apod/milky_way.html">Milky Way Galaxy</a>
about 10 percent of visible matter is in the form of gas, called the
<a href="http://www-ssg.sr.unh.edu/ism/what1.html">interstellar medium</a> (ISM).  

The ISM is
<a href="http://en.wikipedia.org/wiki/Local_Bubble">not uniform</a>,
and shows <a href="http://antwrp.gsfc.nasa.gov/apod/ap990503.html">patchiness</a> even near our
<a href="http://en.wikipedia.org/wiki/Sun">Sun</a>.  

It can be quite difficult to detect the
<a href="http://en.wikipedia.org/wiki/Local_Interstellar_Cloud">local ISM</a> because it is so tenuous and emits so little light.  

This mostly <a href="http://www.webelements.com/webelements/scholar/elements/hydrogen/key.html">hydrogen</a> gas, however, absorbs some very
specific colors that can be detected in the light of the
<a href="http://antwrp.gsfc.nasa.gov/apod/ap010318.html">nearest stars</a>.  

A working map of the local
<a href="http://antwrp.gsfc.nasa.gov/apod/ap980225.html">ISM</a> within 10 light-years
based on recent observations is shown above.  

These observations show that our
<a href="http://antwrp.gsfc.nasa.gov/apod/ap020217.html">Sun is moving</a> through a
<a href="http://en.wikipedia.org/wiki/Local_Interstellar_Cloud">Local Interstellar Cloud</a> as this cloud flows outwards from the
<a href="http://en.wikipedia.org/wiki/Scorpius-Centaurus_Association">Scorpius-Centaurus Association</a> star forming region.  

Our Sun may exit the <a href="http://arxiv.org/abs/0804.3798">Local Interstellar Cloud</a>, also called the Local Fluff,
during the next 10,000 years.  

Much remains unknown about the local
<a href="http://csep10.phys.utk.edu/astr162/lect/milkyway/ism.html">ISM</a>, including details of its distribution,
its origin, and how it affects the
<a href="http://bb.nightskylive.net/asterisk/viewtopic.php?f=24&t=18012">Sun</a> and the
<a href="http://antwrp.gsfc.nasa.gov/apod/earth.html">Earth</a>.


 
 <br><br><a href='http://antwrp.gsfc.nasa.gov/apod/ap100829.html'>Credit &amp; Copyright</a>]]></content:encoded>
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							<title>Hole in the Sun </title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=13570&parent_id=13570#112739</link>
							<pubDate>Sun, 29 Aug 2010 00:00:04</pubDate>
							<author>[z]Barbara Harris</author>
							<category><![CDATA[Pic: Hole in the Sun ]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=13570&parent_id=13570#112739</guid>
							<description><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1008/CoronalHaug2010_sdo.jpg'><b>Hole in the Sun </b></a><br>
			 <br>Explanation: </b>

This ominous, dark shape sprawling across the face of the Sun
is a <a href="http://helios.gsfc.nasa.gov/chole.html">coronal hole</a> --
a low density region extending above
the surface where the solar magnetic field open...]]></description>
							<content:encoded><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1008/CoronalHaug2010_sdo.jpg'><b>Hole in the Sun </b></a><br>
			 <br>Explanation: </b>

This ominous, dark shape sprawling across the face of the Sun
is a <a href="http://helios.gsfc.nasa.gov/chole.html">coronal hole</a> --
a low density region extending above
the surface where the solar magnetic field opens freely into
interplanetary space.

Studied extensively
<a href="http://vestige.lmsal.com/TRACE/POD/Sunscapes.html">from
space</a> since the 1960s in
ultraviolet and
<a href="http://imagine.gsfc.nasa.gov/docs/science/know_l2/sun.html">x-ray light</a>, coronal holes are known to be the source of
the high-speed
<a href="http://www.spaceweathercenter.org/living_with_a_star/06/06.html">solar wind</a>, atoms and electrons
<a href="http://www.astrobio.net/pressrelease/3269/streams-of-the-sun">which flow outward</a> along the open
<a href="http://solar.physics.montana.edu/YPOP/Spotlight/Magnetic/">magnetic field lines</a>.

During periods of low activity,
coronal holes typically cover
regions just above the Sun's poles.

But this extensive coronal hole
dominated the Sun's northern hemisphere earlier this week, captured
here in extreme ultraviolet light by cameras onboard
the <a href="http://sdo.gsfc.nasa.gov/">Solar Dynamics Observatory</a>.

The solar wind streaming from this coronal hole
triggered auroral displays
<a href="http://www.spaceweather.com/submissions/large_image_popup.php?
image_name=Kjetil-Skogli-KSBH10_7826_1282754369.jpg">on planet Earth</a>.

 

 <br><br><a href='http://antwrp.gsfc.nasa.gov/apod/ap100828.html'>Credit &amp; Copyright</a>]]></content:encoded>
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							<title>Brighter Than Mars </title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=13569&parent_id=13569#112736</link>
							<pubDate>Sat, 28 Aug 2010 00:00:07</pubDate>
							<author>[z]Barbara Harris</author>
							<category><![CDATA[Pic: Brighter Than Mars ]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=13569&parent_id=13569#112736</guid>
							<description><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1008/VeMaSpicaDesert_tafreshi.jpg'><b>Brighter Than Mars </b></a><br>
			 <br>Explanation: </b>
 
Even though you may have just read an email
<a href="http://www.snopes.com/science/astronomy/brightmars.asp">claiming</a> Mars will be incredibly bright tonight,
the brightest star on the horizon is not Mars.

F...]]></description>
							<content:encoded><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1008/VeMaSpicaDesert_tafreshi.jpg'><b>Brighter Than Mars </b></a><br>
			 <br>Explanation: </b>
 
Even though you may have just read an email
<a href="http://www.snopes.com/science/astronomy/brightmars.asp">claiming</a> Mars will be incredibly bright tonight,
the brightest star on the horizon is not Mars.

From central Iran on August 24th,
the brightest star in this
<a href="http://www.twanight.org/newTWAN/photos.asp?ID=3002683">twilight
desert skyview</a>
is Venus, aka the Evening Star.

But a bright Mars is in the picture, just above and right
of more <a href="http://www.digitalsky.org.uk/venus/shadow-of-venus.html">brilliant Venus</a>.

Despite claims in the internet's
<a href="http://science.nasa.gov/science-news/science-at-nasa/2010/25aug_marshoax/">annually returning Mars Hoax</a>
that Mars will be as big and bright as the Full Moon,
this celestial scenario is very similar to the western sky you can
see tonight.

Along with Mars, the still beautiful vista includes Spica,
alpha star of the
<a href="http://www.hawastsoc.org/deepsky/vir/index.html">constellation
Virgo</a>, above and left
<a href="http://solarsystem.nasa.gov/planets/profile.cfm?Object=Venus">of Venus</a>.

Farther right of Venus,
<a href="http://solarsystem.nasa.gov/planets/profile.cfm?Object=Saturn">Saturn peeks</a> through the sunset's
fading glow just above the clouds.

Near the opposite horizon, the Full Moon illuminating the
desert is about 400,000 times brighter
<a href="http://beamartian.jpl.nasa.gov/welcome">than Mars</a>.

 
 Note: </b>
<a href="http://twitter.com/apod">APOD tweets are available over Twitter.</a> 

 <br><br><a href='http://antwrp.gsfc.nasa.gov/apod/ap100827.html'>Credit &amp; Copyright</a>]]></content:encoded>
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						<item>
							<title>M27: Not a Comet </title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=13568&parent_id=13568#112735</link>
							<pubDate>Fri, 27 Aug 2010 00:00:04</pubDate>
							<author>[z]Barbara Harris</author>
							<category><![CDATA[Pic: M27: Not a Comet ]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=13568&parent_id=13568#112735</guid>
							<description><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1008/m27_MRussell.jpg'><b>M27: Not a Comet </b></a><br>
			 <br>Explanation: </b>
 
While hunting for comets in the skies above 18th century France,
<a href="http://www.seds.org/messier/xtra/history/biograph.html">astronomer Charles Messier</a>
diligently kept a list of the things
he encountered that were de...]]></description>
							<content:encoded><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1008/m27_MRussell.jpg'><b>M27: Not a Comet </b></a><br>
			 <br>Explanation: </b>
 
While hunting for comets in the skies above 18th century France,
<a href="http://www.seds.org/messier/xtra/history/biograph.html">astronomer Charles Messier</a>
diligently kept a list of the things
he encountered that were definitely not comets.

This is number 27 on his
<a href="http://www.seds.org/messier/xtra/history/m-cat.html">now
famous not-a-comet list</a>.

In fact, 21st century astronomers would identify it as a
<a href="http://www.seds.org/messier/planetar.html">planetary
nebula</a>, but it's not a planet either, even though it may
<a href="http://antwrp.gsfc.nasa.gov/apod/ap030614.html">appear round</a> and
planet-like in a small telescope.

Messier 27 (M27) is an excellent example of a
<a href="http://www.astro.washington.edu/balick/WFPC2/">
gaseous emission nebula</a> created
as a <a href="http://antwrp.gsfc.nasa.gov/apod/ap100221.html">sun-like star runs out</a>
of nuclear fuel in its core.

The nebula forms as the star's outer layers are expelled into
space, with a visible glow generated by atoms excited by the dying
star's intense but invisible
<a href="http://imagine.gsfc.nasa.gov/docs/science/know_l1/emspectrum.html">ultraviolet light</a>.

Known by the popular name of the
<a href="http://www.seds.org/messier/m/m027.html">Dumbbell
Nebula</a>, the beautifully
symmetric interstellar gas cloud is over 2.5 light-years across and
about 1,200 light-years away in the
<a href="http://hawastsoc.org/deepsky/vul/index.html">constellation
Vulpecula</a>.

This <a href="http://www.telescopes.cc/m27.htm">impressive color
composite</a> highlights details within
the well-studied central region and fainter, seldom imaged
features in the nebula's <a href="http://antwrp.gsfc.nasa.gov/apod/ap100509.html">outer halo</a>.

It includes narrowband images recorded using
filters sensitive to emission from oxygen atoms, shown in
blue-green hues, and hydrogen atoms in red.

 
 Poll: </b>
<a href="http://bb.nightskylive.net/asterisk/viewtopic.php?f=29&t=20794">Which of last week's APODs should be the APOW?</a> 

 <br><br><a href='http://antwrp.gsfc.nasa.gov/apod/ap100826.html'>Credit &amp; Copyright</a>]]></content:encoded>
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							<title>Galaxy Cluster Abell</title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=13566&parent_id=13566#112732</link>
							<pubDate>Wed, 25 Aug 2010 00:00:05</pubDate>
							<author>[z]Barbara Harris</author>
							<category><![CDATA[Pic: Galaxy Cluster Abell]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=13566&parent_id=13566#112732</guid>
							<description><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1008/abell1689_hst_big.jpg'><b>Galaxy Cluster Abell 1689 Magnifies the Dark Universe </b></a><br>
			 <br>Explanation: </b>
What's the matter with this cluster of galaxies?

To find out what forms matter takes in the
<a href="http://antwrp.gsfc.nasa.gov/apod/ap040627.html">Abell 1689 cluster</a> requires not...]]></description>
							<content:encoded><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1008/abell1689_hst_big.jpg'><b>Galaxy Cluster Abell 1689 Magnifies the Dark Universe </b></a><br>
			 <br>Explanation: </b>
What's the matter with this cluster of galaxies?

To find out what forms matter takes in the
<a href="http://antwrp.gsfc.nasa.gov/apod/ap040627.html">Abell 1689 cluster</a> requires not only deep images from telescopes like the
<a href="http://hubblesite.org/the_telescope/hubble_essentials/">Hubble Space Telescope</a>, but detailed 
<a href="http://bb.nightskylive.net/asterisk/viewforum.php?f=35">computer modeling</a> as well.

To start, almost every fuzzy yellow patch in the
<a href="http://hubblesite.org/newscenter/archive/releases/2010/26/image/a/">above image</a> is an entire galaxy.

A close inspection, however, shows that many background galaxies are strangely magnified and distorted into
<a href="http://antwrp.gsfc.nasa.gov/apod/ap090921.html">long curving arcs</a> by the
<a href="http://en.wikipedia.org/wiki/Gravitational_lens">gravitational lens</a> deflections of the cluster.  

Computer analyses of the
<a href="http://www.youtube.com/watch?v=2-My9CChyBw">placement</a> and smoothness of these arcs indicate that in addition to the matter in the galaxies you can see, the cluster must also contain a significant amount of
<a href="http://chandra.harvard.edu/xray_astro/dark_matter/index5.html">dark matter</a> such as the model digitally superposed in 
<a href="http://en.wikipedia.org/wiki/Purple">purple</a>.  

Now <a href="http://en.wikipedia.org/wiki/Abell_1689">Abell 1689</a> remains enigmatic because the arcs are so numerous and diverse that no single 
<a href="http://astro.berkeley.edu/~mwhite/darkmatter/dm.html">dark matter</a> model has emerged that can 
<a href="http://adsabs.harvard.edu/abs/2010arXiv1008.2758L">explain them all</a> and still remain consistent with dark matter models needed to constrain their motion.  

Still, the detailed information available from 
<a href="http://antwrp.gsfc.nasa.gov/apod/clusters_of_galaxies.html">clusters of galaxies</a> like Abell 1689 gives hope that one day full solutions will be found that will not only fully reveal the 
<a href="http://antwrp.gsfc.nasa.gov/apod/ap080917.html">dark matter in clusters</a>, 
but also reveal the amounts of 
<a href="http://en.wikipedia.org/wiki/Dark_energy">dark energy</a> 
in the 
<a href="http://adsabs.harvard.edu/abs/2008AmJPh..76..265N">universe</a> 
needed to lie along the line of sight to the 
<a href="http://antwrp.gsfc.nasa.gov/apod/ap040217.html">distant arcs</a>.

 
 Students and Teachers: </b>
<a href="http://bb.nightskylive.net/asterisk/viewforum.php?f=24">Free video online Astro 101 course</a> 
 <br><br><a href='http://antwrp.gsfc.nasa.gov/apod/ap100824.html'>Credit &amp; Copyright</a>]]></content:encoded>
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							<title>A Milky Way Shadow a</title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=13565&parent_id=13565#112731</link>
							<pubDate>Tue, 24 Aug 2010 00:00:05</pubDate>
							<author>[z]Barbara Harris</author>
							<category><![CDATA[Pic: A Milky Way Shadow a]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=13565&parent_id=13565#112731</guid>
							<description><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1008/mwshadow_cherney_big.jpg'><b>A Milky Way Shadow at Loch Ard Gorge </b></a><br>
			 <br>Explanation: </b>
Have you ever seen the Milky Way's glow create shadows?

To do so, conditions need to be just right.

First and foremost, the sky must be relatively clear of clouds so that the
<a href="http://antwrp...]]></description>
							<content:encoded><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1008/mwshadow_cherney_big.jpg'><b>A Milky Way Shadow at Loch Ard Gorge </b></a><br>
			 <br>Explanation: </b>
Have you ever seen the Milky Way's glow create shadows?

To do so, conditions need to be just right.

First and foremost, the sky must be relatively clear of clouds so that the
<a href="http://antwrp.gsfc.nasa.gov/apod/ap070930.html">long band</a> of the
<a href="http://cass.ucsd.edu/public/tutorial/MW.html">Milky Way's central disk</a> can be seen.

The surroundings must be very near to completely dark, with no bright
<a href="http://antwrp.gsfc.nasa.gov/apod/ap010827.html">artificial lights visible</a> anywhere.  

Next, the
<a href="http://antwrp.gsfc.nasa.gov/apod/ap051113.html">Moon</a> cannot be anywhere above the horizon,
or its glow will dominate the landscape.

Last, the <a href="http://antwrp.gsfc.nasa.gov/apod/ap090415.html">shadows</a>
can best be caught on <a href="http://antwrp.gsfc.nasa.gov/apod/ap060915.html">long camera exposures</a>.  

In the <a href="http://www.terrastro.com/galleries/milky-way-shadow/">above image</a> taken in
<a href="http://en.wikipedia.org/wiki/Port_Campbell_National_Park">Port Campbell National Park</a>,
<a href="http://en.wikipedia.org/wiki/Victoria,_Australia">Victoria</a>,
<a href="http://en.wikipedia.org/wiki/Australia">Australia</a>,
seven 15-second images of the ground and
de-<a href="http://antwrp.gsfc.nasa.gov/apod/ap010110.html">rotated sky</a> were digitally added to bring up the needed light and detail.  

In the foreground lies
<a href="http://en.wikipedia.org/wiki/Loch_Ard_Gorge">Loch Ard Gorge</a>, named after a
ship that tragically ran aground in
<a href="http://en.wikipedia.org/wiki/1878">1878</a>.

The two rocks pictured are the remnants of a collapsed arch and are named Tom and Eva after the only two people who survived that
<a href="http://en.wikipedia.org/wiki/Loch_Ard_(ship)">Loch Ard ship</a> wreck.

A close inspection of the
<a href="http://www.youtube.com/watch?v=QgNtzFtm-m8">water just before the rocks</a> will show reflections and 
shadows in light thrown by our
<a href="http://bb.nightskylive.net/asterisk/viewtopic.php?f=24&t=18006">Milky Way galaxy</a>.

Low clouds are visible moving through the serene scene in
<a href="http://vimeo.com/14054461">this movie</a>.

 
 Keep looking up: </b>
<a href="http://bb.nightskylive.net/asterisk/viewtopic.php?f=31&t=20718">Jack Horkheimer: 1938-2010.  Do you remember watching Jack?</a> 
 <br><br><a href='http://antwrp.gsfc.nasa.gov/apod/ap100823.html'>Credit &amp; Copyright</a>]]></content:encoded>
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						<item>
							<title>Hoag's Object: A Str</title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=13564&parent_id=13564#112730</link>
							<pubDate>Mon, 23 Aug 2010 00:00:04</pubDate>
							<author>[z]Barbara Harris</author>
							<category><![CDATA[Pic: Hoag's Object: A Str]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=13564&parent_id=13564#112730</guid>
							<description><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1008/hoag_hst_big.jpg'><b>Hoag's Object: A Strange Ring Galaxy </b></a><br>
			 <br>Explanation: </b>
Is this one galaxy or two?  

This question came to light in 1950 when astronomer
<a href="http://en.wikipedia.org/wiki/Arthur_Allen_Hoag">Art Hoag</a>
chanced upon this unusual
<a href="http://bb.nightskyli...]]></description>
							<content:encoded><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1008/hoag_hst_big.jpg'><b>Hoag's Object: A Strange Ring Galaxy </b></a><br>
			 <br>Explanation: </b>
Is this one galaxy or two?  

This question came to light in 1950 when astronomer
<a href="http://en.wikipedia.org/wiki/Arthur_Allen_Hoag">Art Hoag</a>
chanced upon this unusual
<a href="http://bb.nightskylive.net/asterisk/viewtopic.php?f=24&t=18005">extragalactic object</a>.  

On the outside is a
<a href="http://antwrp.gsfc.nasa.gov/apod/ap051022.html">ring</a> dominated by bright blue stars,
while near the center lies a ball of much redder stars
that are likely much older.  

Between the two is a
<a href="http://antwrp.gsfc.nasa.gov/apod/ap040702.html">gap</a> that appears almost completely dark.  

How <a href="http://adsabs.harvard.edu/abs/1990ApJ...348..448W">Hoag's Object</a>
formed remains unknown, although similar objects
have now been
<a href="http://mergers.galaxyzoo.org/">identified and collectively labeled</a>
as a form of
<a href="http://antwrp.gsfc.nasa.gov/apod/ap010612.html">ring galaxy</a>.  

Genesis hypotheses include a
<a href="http://nedwww.ipac.caltech.edu/level5/Struck/frames.html">galaxy collision</a>
billions of years ago and the gravitational affect of a
<a href="http://antwrp.gsfc.nasa.gov/apod/ap080622.html">central bar</a> that has
<a href="http://adsabs.harvard.edu/doi/10.1007/s10569-010-9289-z">since vanished</a>.


The <a href="http://heritage.stsci.edu/2002/21/caption.html">above</a>
<a href="http://hubblesite.org/gallery/album/galaxy/pr2002021a/">photo</a> taken by the
<a href="http://antwrp.gsfc.nasa.gov/apod/ap010806.html">Hubble Space Telescope</a>
in July 2001 reveals unprecedented details of Hoag's Object and may yield a
<a href="http://nedwww.ipac.caltech.edu/level5/Rings/Rings17_2.html">better understanding</a>.  


Hoag's Object spans about 100,000
<a href="http://chandra.harvard.edu/photo/cosmic_distance.html">light years</a> and lies about 600 million <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 the Snake
(<a href="http://en.wikipedia.org/wiki/Serpens_(constellation)">Serpens</a>).  

Coincidentally, visible in the gap
(at about one o'clock) is yet another
<a href="http://antwrp.gsfc.nasa.gov/apod/ap040426.html">ring galaxy</a> that likely lies
<a href="http://antwrp.gsfc.nasa.gov/apod/ap020901.html">far in the distance</a>.

 
 <br><br><a href='http://antwrp.gsfc.nasa.gov/apod/ap100822.html'>Credit &amp; Copyright</a>]]></content:encoded>
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						<item>
							<title>Perseid Storm </title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=13563&parent_id=13563#112729</link>
							<pubDate>Sun, 22 Aug 2010 00:00:05</pubDate>
							<author>[z]Barbara Harris</author>
							<category><![CDATA[Pic: Perseid Storm ]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=13563&parent_id=13563#112729</guid>
							<description><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1008/PerseidStorm_arn.jpg'><b>Perseid Storm </b></a><br>
			 <br>Explanation: </b>
 
Storms on the distant horizon and comet dust raining through the
heavens above are combined in this alluring
<a href="http://barn.zenfolio.com/p1068266116">nightscape</a>.

The scene <a href="http://www.cloudynights.com/ubbt...]]></description>
							<content:encoded><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1008/PerseidStorm_arn.jpg'><b>Perseid Storm </b></a><br>
			 <br>Explanation: </b>
 
Storms on the distant horizon and comet dust raining through the
heavens above are combined in this alluring
<a href="http://barn.zenfolio.com/p1068266116">nightscape</a>.

The scene <a href="http://www.cloudynights.com/ubbthreads/showflat.php/Number/3985299">was recorded</a>
in the early hours of August 13 from
the Keota Star Party site on the
<a href="http://www.fs.fed.us/r2/recreation/map/colorado/index.shtml">Pawnee National Grasslands</a>
of northeastern Colorado, USA.

Looking east across the prairie,
<a href="http://barn.zenfolio.com/p1068266116/h3e4cb2d#h3e4cb2d">the
composite</a> of 8 consecutive
exposures each 30 seconds long captures the flash of
<a href="http://antwrp.gsfc.nasa.gov/apod/ap100720.html">lightning</a> and a bright Perseid
<a href="http://antwrp.gsfc.nasa.gov/apod/ap100812.html">meteor</a>.

On the right, even the clouds can't block the light from brilliant
<a href="http://solarsystem.nasa.gov/planets/profile.cfm?Object=Jupiter">planet Jupiter</a>, whose mythological
<a href="http://www.pantheon.org/articles/j/jupiter.html">namesake</a>
knew how to handle both lightning bolts and meteors.

Of course, this meteor's streak points back toward the
<a href="http://antwrp.gsfc.nasa.gov/apod/ap100814.html">shower's radiant</a>
in the heroic constellation Perseus,
sharing a starry background that includes the
<a href="http://antwrp.gsfc.nasa.gov/apod/ap071122.html">Pleiades</a> star
cluster poised above the storm clouds.

Just above the bright meteor lies the faint
<a href="http://www.seds.org/messier/m/m031.html">Andromeda Galaxy</a>.

 

 <br><br><a href='http://antwrp.gsfc.nasa.gov/apod/ap100821.html'>Credit &amp; Copyright</a>]]></content:encoded>
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						<item>
							<title>NGC 1365: Majestic I</title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=13562&parent_id=13562#112728</link>
							<pubDate>Sat, 21 Aug 2010 00:00:04</pubDate>
							<author>[z]Barbara Harris</author>
							<category><![CDATA[Pic: NGC 1365: Majestic I]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=13562&parent_id=13562#112728</guid>
							<description><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1008/NGC1365_pugh.jpg'><b>NGC 1365: Majestic Island Universe </b></a><br>
			 <br>Explanation: </b>
 
Barred <a href="http://www.seds.org/messier/spir.html">spiral galaxy</a>
NGC 1365 is truly a majestic
<a href="http://antwrp.gsfc.nasa.gov/apod/ap100109.html">island universe</a> some 200,000
light-years acr...]]></description>
							<content:encoded><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1008/NGC1365_pugh.jpg'><b>NGC 1365: Majestic Island Universe </b></a><br>
			 <br>Explanation: </b>
 
Barred <a href="http://www.seds.org/messier/spir.html">spiral galaxy</a>
NGC 1365 is truly a majestic
<a href="http://antwrp.gsfc.nasa.gov/apod/ap100109.html">island universe</a> some 200,000
light-years across.

Located a mere 60 million light-years away toward the
chemical constellation
<a href="http://www.hawastsoc.org/deepsky/for/index.html">Fornax</a>,
NGC 1365 is a dominant member of the well-studied
<a href="http://heritage.stsci.edu/2005/09/supplemental.html">Fornax
galaxy cluster</a>.

This impressively
<a href="http://www.martinpughastrophotography.id.au/Galaxies/NGC1365.htm">sharp color image</a> shows intense
star forming regions at the ends of the bar and along the
spiral arms, and details of dust lanes cutting
across the galaxy's bright core.

At the core lies a supermassive black hole.

Astronomers think
<a href="http://arxiv.org/abs/0907.2602">NGC 1365's</a>
prominent bar plays a crucial role in the
<a href="http://hubblesite.org/newscenter/archive/releases/1999/34/">galaxy's evolution</a>, drawing gas and dust into a
star-forming maelstrom and ultimately feeding material into the
<a href="http://hubblesite.org/newscenter/archive/releases/2000/22">central black hole</a>.

 

 <br><br><a href='http://antwrp.gsfc.nasa.gov/apod/ap100820.html'>Credit &amp; Copyright</a>]]></content:encoded>
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						<item>
							<title>Pelican Nebula Close</title>
							<link>http://www.zorg.ch/gallery.php?show=pic&picID=13561&parent_id=13561#112727</link>
							<pubDate>Fri, 20 Aug 2010 00:00:05</pubDate>
							<author>[z]Barbara Harris</author>
							<category><![CDATA[Pic: Pelican Nebula Close]]></category>
							<guid isPermaLink="false">http://www.zorg.ch/gallery.php?show=pic&picID=13561&parent_id=13561#112727</guid>
							<description><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1008/PelicanIC5067_hallas.jpg'><b>Pelican Nebula Close-up</b></a><br>
			 <br>Explanation: </b>
 
The prominent ridge of emission featured in
<a href="http://astrophoto.com/Pelican.htm">this intensely
colorful skyscape</a> is designated <a href="http://antwrp.gsfc.nasa.gov/apod/ap061227.html">IC 5067</a>.

P...]]></description>
							<content:encoded><![CDATA[<a href='http://antwrp.gsfc.nasa.gov/apod/image/1008/PelicanIC5067_hallas.jpg'><b>Pelican Nebula Close-up</b></a><br>
			 <br>Explanation: </b>
 
The prominent ridge of emission featured in
<a href="http://astrophoto.com/Pelican.htm">this intensely
colorful skyscape</a> is designated <a href="http://antwrp.gsfc.nasa.gov/apod/ap061227.html">IC 5067</a>.

Part of a larger
<a href="http://www.noao.edu/image_gallery/emission_nebulae.html">emission
nebula</a> with a distinctive shape, popularly called
<a href="http://antwrp.gsfc.nasa.gov/apod/ap061130.html">The Pelican Nebula</a>, the ridge spans about
10 light-years and follows the
curve of the cosmic pelican's head and neck.

Fantastic, dark shapes inhabiting the view
are clouds of cool gas and dust
<a href="http://www.noao.edu/outreach/press/pr03/pr0308.html">sculpted by</a>
energetic radiation from hot, massive stars.

But stars are also forming within the dark shapes.

In fact, twin jets emerging from the tip of the central,
<a href="http://astrophoto.com/PelCU.jpg">dark tendril</a>
are the telltale signs of an embedded protostar cataloged as
<a href="http://en.wikipedia.org/wiki/Herbig-Haro_objects">Herbig-Haro</a>
555.

The Pelican Nebula itself, also known as IC 5070,
is about 2,000 light-years away.

<a href="http://antwrp.gsfc.nasa.gov/apod/ap070702.html">To find</a> it, look northeast of bright
<a href="http://antwrp.gsfc.nasa.gov/apod/ap070920.html">star Deneb</a> in the
high flying constellation Cygnus.

 
 Rare chance: </b>
<a href="http://bb.nightskylive.net/asterisk/viewtopic.php?f=31&t=20532">Ask APOD editor Jerry T. Bonnell questions about APOD.</a>

 <br><br><a href='http://antwrp.gsfc.nasa.gov/apod/ap100819.html'>Credit &amp; Copyright</a>]]></content:encoded>
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