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<channel>

    <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>Fri, 03 Jul 2009 13:06:00 GMT</lastBuildDate>
    <generator>ACME Labs custom shell script</generator>
    <managingEditor>jef@mail.acme.com</managingEditor>
    <webMaster>webmaster@mail.acme.com</webMaster>
    <image>
	<url>http://www.acme.com/jef/apod/apod.GIF</url>
	<title>Astronomy Picture of the Day RSS Feed</title>
	<link>http://www.acme.com/jef/apod/</link>
    </image>

    <item>
	<title><![CDATA[Perihelion and Aphelion]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap090703.html</link>
	<pubDate>Fri, 03 Jul 2009 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap090703.html"><img src="http://antwrp.gsfc.nasa.gov/apod/image/0907/PerihelionAphelion_cervignon800.jpg" /></a>
<title>Perihelion and Aphelion</title>

This year Aphelion, the point in Earth's
<a href="http://www.windows.ucar.edu/tour/link=/physical_science/
physics/mechanics/orbit/ellipse.html&edu=high">elliptical orbit</a>
when it is farthest from the Sun, occurs tomorrow, July 4th.

Of course, that doesn't
<a href="http://csep10.phys.utk.edu/astr161/lect/time/
seasons.html">affect the seasons</a> on
<a href="http://eol.jsc.nasa.gov/">our fair planet</a>.

Those are determined by the tilt of Earth's axis of rotation and not
Earth's distance from the Sun, so July is still winter in the south
and summer in northern hemisphere.

But it does mean that on July 4th the Sun will be at its smallest
apparent size.

This composite neatly compares two pictures of the Sun taken with the
same telescope and camera
<a href="http://aa.usno.navy.mil/data/docs/EarthSeasons.php">on the
dates of</a> Perihelion (closest approach) and Aphelion in 2008.

The image labels include Earth's distance in kilometers
from the Sun on the two dates.

Otherwise difficult
<a href="http://www.sungazer.net/">to notice</a>, the change in the Sun's
apparent diameter between
<a href="http://www.windows.ucar.edu/tour/link=/physical_science/
physics/mechanics/orbit/perihelion_aphelion.html&edu=high">Perihelion
and Aphelion</a> is clear.

The difference amounts to a little over 3 percent.

	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[Lyman Alpha Blob]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap090702.html</link>
	<pubDate>Thu, 02 Jul 2009 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap090702.html"><img src="http://antwrp.gsfc.nasa.gov/apod/image/0907/labs900_multiCXC.jpg" /></a>
<title>Lyman Alpha Blob</title>

Dubbed a Lyman-alpha blob, an enormous cloud of hydrogen gas spans
several hundred thousand light-years in
<a href="http://chandra.harvard.edu/photo/2009/labs/">this remarkable
image</a> (left), a composite of
<a href="http://coolcosmos.ipac.caltech.edu/cosmic_classroom/
multiwavelength_astronomy/multiwavelength_astronomy/">x-ray, optical,
and infrared</a> data
from space and ground based observatories.

The gigantic, amoeba-like structure is seen as it was when
<a href="http://antwrp.gsfc.nasa.gov/apod/ap060323.html">the universe was</a> a
<a href="http://www.astro.ucla.edu/~wright/CosmoCalc.html">mere</a> 2 billion
years old (about 12 billion
<a href="http://map.gsfc.nasa.gov/universe/uni_age.html">years ago</a>).

Lyman-alpha blobs are so called because they strongly emit
radiation due to the
<a href="http://en.wikipedia.org/wiki/Lyman_series">Lyman-alpha emission</a>
line of hydrogen gas.

Normally, Lyman-alpha emission is in the ultraviolet part of
the spectrum, but Lyman-apha blobs are so distant, their light is
redshifted to (longer) optical
<a href="http://hyperphysics.phy-astr.gsu.edu/hbase/
ems1.html">wavelengths</a>.

X-ray data (blue)
<a href="http://arxiv.org/abs/0904.0452">indicates</a> the presence of a
<a href="http://chandra.harvard.edu/xray_sources/
blackholes_sm.html">supermassive black hole</a>
feeding at the center of an active galaxy embedded in the blob.

Illustrated close up in the right hand panel, radiation and outflows
from the active galaxy are thought to be a source for energizing
and heating the blob's hydrogen gas.

In fact, Lyman-alpha blobs could represent an early phase in
galaxy formation where the heating is so great it begins
to limit further rapid growth of
<a href="http://chandra.harvard.edu/xray_sources/quasars.html">active
galaxies</a> and their supermassive black holes.

	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[Three Galaxies in Draco]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap090701.html</link>
	<pubDate>Wed, 01 Jul 2009 13:06:01 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap090701.html"><img src="http://antwrp.gsfc.nasa.gov/apod/image/0907/NGC5982_benintende.jpg" /></a>
<title>Three Galaxies in Draco</title>

This intriguing trio of galaxies is sometimes
called the Draco Group, located in the northern
constellation of (you guessed it)
<a href="http://www.hawastsoc.org/deepsky/dra/index.html">Draco</a>.

From left to right are
<a href="http://antwrp.gsfc.nasa.gov/apod/ap010510.html">edge-on spiral</a> NGC 5981,
<a href="http://antwrp.gsfc.nasa.gov/apod/ap060520.html">elliptical galaxy</a> NGC 5982, and
<a href="http://antwrp.gsfc.nasa.gov/apod/ap040410.html">face-on spiral</a> NGC 5985 --
all within this single telescopic
field of view spanning a little more than
half the width of the full moon.

While the group is far too small to be a
<a href="http://www.seds.org/messier/gal_clus.html">galaxy cluster</a>
and has not been
<a href="http://www.astro.ubc.ca/people/hickson/hcg/">cataloged</a>
compact group, these galaxies all do lie roughly
100 million light-years from planet Earth.

On close examination with <a href="http://imagine.gsfc.nasa.gov/docs/
science/how_l1/spectral.html">spectrographs</a>, the bright core of the
striking face-on spiral NGC 5985 shows
prominent emission in specific wavelengths of light, prompting
astronomers to classify it as a
<a href="http://www.seds.org/~spider/spider/ScholarX/
seyferts.html">Seyfert</a>, a type of active galaxy.

Not as well known as other tight
<a href="http://antwrp.gsfc.nasa.gov/apod/ap090313.html">groupings of galaxies</a>,
the contrast in visual appearance
makes this triplet an attractive subject for
astrophotographers.

This <a href="http://www.astrogb.com/ngc5982.htm">impressively
deep exposure</a> of the region also reveals faint
and even more distant
<a href="http://www.noao.edu/outreach/aop/observers/
bggalaxies.html">background galaxies</a>.

	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[The North America and Pelican Nebulae]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap090630.html</link>
	<pubDate>Tue, 30 Jun 2009 13:06:02 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap090630.html"><img src="http://antwrp.gsfc.nasa.gov/apod/image/0906/northpelican_russell.jpg" /></a>
<title>The North America and Pelican Nebulae</title>
Here are some familiar shapes in unfamiliar locations.  

This 
<a href="http://antwrp.gsfc.nasa.gov/apod/emission_nebulae.html">emission nebula</a> on the left
is famous partly because it resembles Earth's continent of 
<a href="http://en.wikipedia.org/wiki/North_America">North America</a>. 

To the right of the 
<a href="http://en.wikipedia.org/wiki/North_America_Nebula"
>North America Nebula</a>, cataloged as NGC 7000, 
is a less luminous nebula that resembles a 
<a href="http://en.wikipedia.org/wiki/Pelican">pelican</a> dubbed the
<a href="http://antwrp.gsfc.nasa.gov/apod/ap020829.html">Pelican Nebula</a>. 

The two emission
<a href="http://en.wikipedia.org/wiki/Nebula">nebula</a> 
measure about 50 light-years across, are located about 1,500 
<a href=
"http://starchild.gsfc.nasa.gov/docs/StarChild/questions/question19.html"
>light-years</a> away, and are separated by a 
<a href="http://antwrp.gsfc.nasa.gov/apod/dark_nebulae.html">dark absorption</a> cloud. 

This spectacular image captures the nebulas, bright 
<a href="http://antwrp.gsfc.nasa.gov/apod/ap000703.html">ionization fronts</a>, and fine details of the dark dust.

The <a href="http://www.youtube.com/watch?v=LtKUuAM3zDY">nebulae can be seen</a> with binoculars from a dark location. 

Look for a 
<a href="http://antwrp.gsfc.nasa.gov/apod/ap971009.html">small nebular patch</a> 
north-east of bright star
<a href="http://www.astro.wisc.edu/~dolan/constellations/hr/7924.html"
>Deneb</a> in the constellation of <a href="
http://www.astro.wisc.edu/~dolan/constellations/constellations/Cygnus.html"
>Cygnus</a>. 

It is still unknown which star or stars 
ionize the red-glowing 
<a href="http://periodic.lanl.gov/elements/1.html"
>hydrogen</a> gas. 


	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[Kaguya Spacecraft Crashes into the Moon]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap090629.html</link>
	<pubDate>Mon, 29 Jun 2009 13:06:01 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap090629.html"><img src="" /></a>
<title>Kaguya Spacecraft Crashes into the Moon</title>
Japan's Kaguya spacecraft crashed into the Moon last week, as planned.

Officially named the
<a href="http://en.wikipedia.org/wiki/Selenology">Selenological</a>
and Engineering Explorer (SELENE)</a>, the spacecraft was given the nickname Kaguya after the princess in the Japanese folklore story 
<a href="http://en.wikipedia.org/wiki/Tale_of_the_Bamboo_Cutter"
>The Tale of the Bamboo Cutter</a>.

<a href="http://www.jaxa.jp/press/2009/06/20090619_kaguya_hdtv_e.html"
>Pictured above</a> is a movie taken by Kaguya during the last orbit of its 
twenty-month lunar mission.

A <a href="http://antwrp.gsfc.nasa.gov/apod/ap031109.html">desolate</a>, hilly, and cratered terrain passes underneath as the spacecraft barely clears a few peaks.  

At <a href="http://www.jaxa.jp/press/2009/06/20090619_kaguya_hdtv_e.html"
>the movie</a>'s end, the spacecraft disappears into darkness 
<a href="http://www.jaxa.jp/press/2009/06/20090611_kaguya_e.html"
>near GILL crater</a>.

Robotic <a href="http://www.jaxa.jp/projects/sat/selene/index_e.html"
>SELENE</a> carried thirteen scientific instruments and two 
<a href="http://en.wikipedia.org/wiki/HDTV">HDTV</a> cameras.

The <a href="http://en.wikipedia.org/wiki/Pun">groundbreaking</a> mission took data on lunar topology and composition that are being used to better understand the origin and history of Earth's 
<a href="http://en.wikipedia.org/wiki/Moon">unique and ancient companion</a>.

Data and images from 
<a href="http://en.wikipedia.org/wiki/SELENE">Kayuga</a> 
and the recently launched 
<a href="http://lro.gsfc.nasa.gov/">Lunar Reconnaissance Orbiter</a> 
could be used to choose good locations to land future 
<a href="http://antwrp.gsfc.nasa.gov/apod/ap051217.html">Moon-exploring astronauts</a>.  


	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[Fresh Tiger Stripes on Saturn's Enceladus]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap090628.html</link>
	<pubDate>Sun, 28 Jun 2009 13:06:03 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap090628.html"><img src="http://antwrp.gsfc.nasa.gov/apod/image/0906/enceladusstripes_cassini.jpg" /></a>
<title>Fresh Tiger Stripes on Saturn's Enceladus</title>
Do underground oceans vent through the tiger stripes on Saturn's moon Enceladus?  

Long features dubbed tiger stripes are known to be
<a href="http://antwrp.gsfc.nasa.gov/apod/ap071013.html">spewing ice</a> from the moon's icy interior into space,
creating a cloud of fine ice particles over the moon's South Pole
and creating Saturn's mysterious <a href=
"ap070327.html">E-ring</a>.  

Evidence for this has come from the
<a href="http://saturn.jpl.nasa.gov/mission/presentposition/"
>robot Cassini spacecraft</a> now orbiting
<a href="http://en.wikipedia.org/wiki/Saturn">Saturn</a>.  

<a href="http://photojournal.jpl.nasa.gov/catalog/PIA06254">Pictured above</a>,
a high resolution image of Enceladus is shown from a close flyby.  

The unusual surface features dubbed
<a href="http://en.wikipedia.org/wiki/Tiger"
>tiger</a> stripes are visible on in false-color blue.  

Why
<a href="http://antwrp.gsfc.nasa.gov/cgi-bin/apod/apod_search?enceladus"
>Enceladus</a> is active remains a mystery, as the neighboring moon
<a href="http://antwrp.gsfc.nasa.gov/apod/ap090517.html">Mimas</a>,
approximately the same size, appears
<a href="http://www.davidpbrown.co.uk/jokes/monty-python-parrot.html"
>quite dead</a>.

Most recently, an
<a href="http://saturn.jpl.nasa.gov/news/newsreleases/newsrelease20090624/"
>analysis of dust</a> captured by
<a href="http://www.youtube.com/watch?v=0BzXC4qfV44"
>Cassini found evidence</a> for sodium as expected in a deep salty ocean.  

Conversely however, recent Earth-based observations of ice ejected by Enceladus into Saturn's E-Ring showed no
<a href="http://www.universetoday.com/2009/06/24/does-enceladus-harbor-a-liquid-ocean-reasonable-minds-disagree/">evidence</a> of the expected 
<a href="http://en.wikipedia.org/wiki/Sodium">sodium</a>.  

Such research is particularly interesting since such an ocean would be a candidate to
<a href="http://www1.nasa.gov/mission_pages/cassini/media/enceladus-f20080326.html">contain life</a>. 


	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[Saharan Starry Night]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap090627.html</link>
	<pubDate>Sat, 27 Jun 2009 13:06:01 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap090627.html"><img src="http://antwrp.gsfc.nasa.gov/apod/image/0906/Tassili-Lines_tafreshi.jpg" /></a>
<title>Saharan Starry Night</title>

This panoramic image of a starry night looks across
a dry, desolate landscape.

<a href="http://antwrp.gsfc.nasa.gov/apod/image/0906/Tassili_tafreshi.jpg">The magnificent view</a>
was recorded from
<a href="http://whc.unesco.org/en/list/179">Tassili National Park</a>, in
the heart of the Sahara desert in southern Algeria.

Rising above <a href="http://www.dreamview.net/dv/new/
photos.asp?id=101903&cat=Nature">eroded sandstone cliffs</a>,
the celestial menagerie of constellations includes
<a href="http://www.windows.ucar.edu/tour/link=/mythology/
draco_dragon.html&edu=high">Draco</a> the Dragon,
<a href="http://www.windows.ucar.edu/tour/link=/mythology/
cygnus.html&edu=high">Cygnus</a> the Swan,
<a href="http://www.windows.ucar.edu/tour/link=/the_universe/
Constellations/summer/aquila.html&edu=high">Aquila</a> the Eagle, and
<a href="http://www.windows.ucar.edu/tour/link=/mythology/
scorpius.html">Scorpius</a> the Scorpion.

Ruling planet Jupiter shines through
clouds very close to the horizon near picture center, while
star clouds of the Milky Way arc
<a href="http://antwrp.gsfc.nasa.gov/apod/ap070711.html">through Sagittarius</a>
above the rocks at the far right.

Bright blue stars <a href="http://antwrp.gsfc.nasa.gov/apod/ap070920.html">Deneb</a>, in Cygnus, and
<a href="http://www.astro.illinois.edu/~jkaler/sow/altair.html">Altair</a>,
in Aquila, also
shine in the starry night along with Scorpius' bright yellowish star
<a href="http://antwrp.gsfc.nasa.gov/apod/ap080603.html">Antares</a>, the rival of Mars.

Prehistoric skygazers surely witnessed a similar sky.

In addition to dramatic sandstone formations,
<a href="http://en.wikipedia.org/wiki/Tassili_n%27Ajjer">the Tassili
region</a> is noted for
<a href="http://www.metmuseum.org/toah/hd/tass/hd_tass.htm">rock art</a>
and archaeological sites dating to
<a href="http://en.wikipedia.org/wiki/Neolithic">Neolithic times</a>
when the local climate was wetter.

	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[Solstice to Solstice Solargraph]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap090626.html</link>
	<pubDate>Fri, 26 Jun 2009 13:06:01 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap090626.html"><img src="http://antwrp.gsfc.nasa.gov/apod/image/0906/solsolargraph_zapior850.jpg" /></a>
<title>Solstice to Solstice Solargraph</title>

This six month long exposure compresses the
<a href="http://www.moma.org/collection/
browse_results.php?object_id=79018">time</a>
from solstice to solstice
(~ December 21, 2008 to June 20, 2009) into a single
point of view.

Dubbed a solargraph, the
<a href="http://www.asu.cas.cz/~sos/staff/maciek/puszki.htm">unconventional
picture</a> was recorded with a pinhole camera
<a href="http://www.pinholephotography.org/
Solargraph%20instructions.htm">made from</a> an aluminum  can lined
with a piece of photographic paper.

Fixed to a
<a href="http://www.solargraphy.com/index.php?
option=com_content&task=view&id=16&Itemid=18">single spot</a>
for the entire exposure, the simple camera continuously
records the Sun's daily path as a glowing trail
burned into the photosensitive paper.

Breaks and gaps in the trails are caused by cloud cover.

In this case, the spot was chosen to look out
from inside a
<a href="http://www.asu.cas.cz/_data/k40l_1232294978.jpg">radio telescope</a>
at the
<a href="http://www.asu.cas.cz/history">Ondrejov Observatory</a>
in the Czech Republic.

At the end of the exposure, the paper was removed from the
can and immediately scanned digitally.

Contrasts and colors were then enhanced and added to the
digital image.

Of course, in December, the Sun trails
<a href="http://antwrp.gsfc.nasa.gov/apod/ap071222.html">begin lower</a> down
at the northern hemisphere's winter solstice.

The trails <a href="http://antwrp.gsfc.nasa.gov/apod/ap081221.html">climb higher</a> in the sky as the
June 21st summer solstice approaches.

	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[Sarychev Peak Volcano in Stereo]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap090625.html</link>
	<pubDate>Thu, 25 Jun 2009 13:06:01 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap090625.html"><img src="http://antwrp.gsfc.nasa.gov/apod/image/0906/ISS020-E-9050_52ana_public800.jpg" /></a>
<title>Sarychev Peak Volcano in Stereo</title>

From 400 kilometers
<a href="http://spaceflight.nasa.gov/realdata/tracking/index.html">above
planet Earth</a>, the Expedition 20 Crew
onboard the International Space Station
(<a href="http://antwrp.gsfc.nasa.gov/apod/ap090406.html">ISS</a>) was able to witness a
remarkable event from a remarkable vantage point --
the June 12 eruption of the
<a href="http://www.volcano.si.edu/world/
volcano.cfm?vnum=0900-24=">Sarychev Peak Volcano</a>.

The active volcano is located in Russia's
<a href="http://en.wikipedia.org/wiki/Kuril_Islands">Kuril Island chain</a>,
stretching to the northeast of Japan.

Emphasizing the orbital perspective, this stunning color
<a href="http://www.tridi.be/">stereo view</a>
was made by combining two
<a href="http://earthobservatory.nasa.gov/NaturalHazards/
view.php?id=38985">images from the ISS</a> and is
intended to be viewed with
<a href="http://mpfwww.jpl.nasa.gov/MPF/mpf/glasses.html">red/blue
glasses</a> (red for the left eye).

Punching upwards into the atmosphere at an early stage of the eruption,
the volcanic plume features a brown column of ash topped with a smooth,
bubble-like, white cloud that is likely water condensation.

Below, a cloud of denser grey ash slides down the volcanic slope.

About 1.5 kilometers of the island coastline is visible at ground
level.

The evolving
<a href="http://earthobservatory.nasa.gov/NaturalHazards/
event.php?id=38937">ash plume</a> posed no danger to the Expedition 20 crew,
but commercial airline flights were diverted away
from the region to minimize the danger of engine failures from ash intake. 

	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[Noctilucent Clouds Over Germany]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap090624.html</link>
	<pubDate>Wed, 24 Jun 2009 13:06:01 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap090624.html"><img src="http://antwrp.gsfc.nasa.gov/apod/image/0906/noctilucent_rollwagen.jpg" /></a>
<title>Noctilucent Clouds Over Germany</title>
Sometimes it's night on the ground but day in the air.
 
As the Earth rotates to eclipse the Sun,
<a href="http://antwrp.gsfc.nasa.gov/apod/ap070713.html">sunset</a> rises up from the ground.
 
Therefore, at sunset on the ground,
sunlight still shines on <a href="
http://ww2010.atmos.uiuc.edu/(Gh)/guides/mtr/cld/home.rxml"
>clouds</a> above.  
 
Under usual circumstances, a
<a href="http://antwrp.gsfc.nasa.gov/apod/ap980526.html">pretty sunset</a>
might be visible, but unusual
<a href="http://en.wikipedia.org/wiki/Noctilucent_clouds"
>noctilucent clouds</a> float so high up they
can be seen well after dark.  
 
Pictured above last week, a network of
<a href="http://www.youtube.com/watch?v=pslcQXWQz3k">noctilucent
clouds</a> cast an eerie white glow after dusk, beyond a local field near
<a href="http://en.wikipedia.org/wiki/Potsdam">Potsdam</a>,
<a href="http://en.wikipedia.org/wiki/Germany">Germany</a>.
 
Although
<a href="http://www.spaceweather.com/nlcs/gallery2009_page1.htm"
>noctilucent clouds</a> are thought to be composed of
small ice-coated particles,
<a href="http://www.nlcnet.co.uk/"
>much remains unknown</a> about them.
 
Satellites launched to help study these clouds includes Sweden's
<a href="http://en.wikipedia.org/wiki/Odin_%28satellite%29">Odin</a> and NASA's
<a href="http://en.wikipedia.org/wiki/Aeronomy_of_Ice_in_the_Mesosphere"
>AIM</a>.

<a href="http://www.nrl.navy.mil/pressRelease.php?Y=2003&R=35-03r"
>Recent evidence</a> indicates that at least some
<a href="http://www.youtube.com/watch?v=-xF2vSKINK0"
>noctilucent clouds</a> result from freezing water exhaust from
<a href="http://antwrp.gsfc.nasa.gov/apod/ap021023.html">Space Shuttle</a>s.

	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[Molecular Cloud Barnard 68]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap090623.html</link>
	<pubDate>Tue, 23 Jun 2009 13:06:02 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap090623.html"><img src="http://antwrp.gsfc.nasa.gov/apod/image/0906/barnard68v2_vlt.jpg" /></a>
<title>Molecular Cloud Barnard 68</title>
Where did all the stars go?  

What used to be considered a hole in the sky
is now known to astronomers as a dark <a href=
"http://en.wikipedia.org/wiki/Molecular_cloud"
>molecular cloud</a>.  

Here, a high concentration of
<a href="http://antwrp.gsfc.nasa.gov/apod/ap030706.html">dust</a> and
<a href="http://antwrp.gsfc.nasa.gov/apod/ap970430.html">molecular gas</a>
absorb practically all the visible light
emitted from background stars.
  
The eerily dark surroundings help make the interiors of
<a href="http://www.youtube.com/watch?v=YbdwTwB8jtc"
>molecular clouds</a> some of the coldest
and most isolated places in the universe.  

One of the most notable of these
<a href="http://antwrp.gsfc.nasa.gov/apod/dark_nebulae.html">dark absorption nebulae</a>
is a cloud toward the constellation
<a href="http://www.seds.org/Maps/Stars_en/Fig/ophiuchus.html"
>Ophiuchus</a> known as
<a href="http://en.wikipedia.org/wiki/Barnard_68">Barnard 68</a>,
<a href="http://www.eso.org/gallery/v/ESOPIA/Stars/phot-02a-01.tif.html"
>pictured above</a>.  

That no stars are visible in the center indicates that
<a href="http://en.wikipedia.org/wiki/Edward_Emerson_Barnard">Barnard</a>
68 is relatively nearby, with measurements placing it about
500 light-years away and half a <a href="
http://starchild.gsfc.nasa.gov/docs/StarChild/questions/question19.html"
>light-year</a> across.  

It is not known exactly how
<a href="http://archive.ncsa.uiuc.edu/Cyberia/Bima/GMC.html"
>molecular clouds</a> like
<a href="http://curious.astro.cornell.edu/question.php?number=597"
>Barnard 68</a> form, but it is known that these clouds are themselves
<a href="http://antwrp.gsfc.nasa.gov/apod/ap070218.html">likely places</a>
for <a href="http://zebu.uoregon.edu/~js/ast122/lectures/lec14.html"
>new stars to form</a>.

In fact, <a href="http://adsabs.harvard.edu/abs/2009ApJ...695.1308B"
>Barnard 68</a> itself has
<a href="http://www.universetoday.com/2009/06/09/astronomers-predict-birth-of-a-new-star/">recently been found</a> likely to collapse and form a new star system.

It is possible to
<a href="http://www.eso.org/outreach/press-rel/pr-1999/phot-29-99.html"
>look right through</a> the cloud in <a href="
http://coolcosmos.ipac.caltech.edu/cosmic_classroom/ir_tutorial/discovery.html"
>infrared</a> light.


	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[Atlas 5 Rocket Launches to the Moon]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap090622.html</link>
	<pubDate>Mon, 22 Jun 2009 13:06:01 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap090622.html"><img src="http://antwrp.gsfc.nasa.gov/apod/image/0906/lrolaunch_nasa.jpg" /></a>
<title>Atlas 5 Rocket Launches to the Moon</title>
This rocket is headed for the Moon.

<a href="http://www.nasa.gov/images/content/361142main_atlasliftoff3000.jpg"
>Pictured above</a>, a huge
<a href="http://en.wikipedia.org/wiki/Atlas_V">Altas V</a> rocket
<a href="http://www.youtube.com/watch?v=j-5t4de6jjI">roared off the
launch pad</a> last week to start NASA's  
<a href="http://www.filmsite.org/voya.html">first missions to Earth's</a>
<a href="http://www.youtube.com/watch?v=xbGd_240ynk">Moon</a> in 10 years.

The <a href="http://antwrp.gsfc.nasa.gov/apod/ap020916.html">rocket</a> is carrying two robotic spacecraft.  

The <a href="http://lro.gsfc.nasa.gov/">Lunar Reconnaissance Orbiter</a>
(<a href="http://en.wikipedia.org/wiki/Lunar_Reconnaissance_Orbiter">LRO</a>)
is scheduled to orbit and better map the Moon, search for buried and hidden ice, and return many high resolution images.  

Some images will be below one-meter in resolution and include images of historic
<a href="http://antwrp.gsfc.nasa.gov/apod/ap070720.html">Apollo landing site</a>s.  

Exploratory data and images should allow a more informed choice of possible future astronaut landing sites.

The <a href="http://lcross.arc.nasa.gov/">Lunar CRater Observation and Sensing Satellite</a> (LCROSS) is scheduled to
<a href="http://twitter.com/LCROSS_NASA">monitor</a> the controlled
<a hreff="ap050705.html">impact</a> of the rocket's
upper stage into a permanently shadowed crater near the
<a href="http://antwrp.gsfc.nasa.gov/apod/ap980306.html">Moon's south pole</a>.    

This impact, which should occur in about three months, might be visible on Earth through <a href="http://antwrp.gsfc.nasa.gov/apod/ap050413.html">small telescopes</a>.

	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[Sunrise over the Parthenon]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap090621.html</link>
	<pubDate>Sun, 21 Jun 2009 13:06:02 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap090621.html"><img src="http://antwrp.gsfc.nasa.gov/apod/image/0906/parthenon_ayiomamitis.jpg" /></a>
<title>Sunrise over the Parthenon</title>
Today, the sun will stay in the sky longer than any other day of the year, as seen from the northern hemisphere of Earth.

Named the Summer Solstice, today's
<a href="http://antwrp.gsfc.nasa.gov/apod/ap080922.html">maximum daylight</a> is indicative of the high amount of sunlight this time of year that is primarily responsible for the heat of the
<a href="http://en.wikipedia.org/wiki/Summer">summer season</a>.  

At the <a href="http://antwrp.gsfc.nasa.gov/apod/ap040919.html">north pole</a> and for all places above the
<a href="http://en.wikipedia.org/wiki/Arctic_Circle">arctic circle</a>,
there will be no night -- the entire day today will be lit by sunlight.  

The situation is reversed in Earth's southern hemisphere, where today has the least sunlight of any day.

Today's <a href="http://en.wikipedia.org/wiki/Solstice"
>solstice</a> is commemorated above by a
<a href="http://www.perseus.gr/Astro-Solar-Scenes-Parthenon-04.htm"
>well-planned picture</a> of our five billion year old Sun rising behind the 2,500 year old
<a href="http://en.wikipedia.org/wiki/Parthenon">Parthenon</a> in
<a href="http://en.wikipedia.org/wiki/Greece">Greece</a>.

Trees and birds occupy the foreground, while a modern
<a href="http://cic.nist.gov/vrml/equip.html">crane</a>
is shown restoring parts of this historic symbol of a cultural
<a href="http://www.historyworld.net/wrldhis/PlainTextHistories.asp?historyid=ab25"
>civilization</a>.


	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[Seaside Moon Mirage]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap090620.html</link>
	<pubDate>Sat, 20 Jun 2009 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap090620.html"><img src="http://antwrp.gsfc.nasa.gov/apod/image/0906/Navires013_audrin900.jpg" /></a>
<title>Seaside Moon Mirage</title>

This surprising view of the Full Moon
<a href="http://stardate.org/nightsky/moon/">rising on</a>
June 7 was captured
with a telephoto lens from a seaside balcony near Nice, France.

The <a href="http://antwrp.gsfc.nasa.gov/apod/ap050922.html">orange Moon's</a>
dark markings and odd shape put the photographer
in mind of an alien creature's face staring down at the passing ship.

Of course, the Moon's distorted appearance is due to the unusual bending
(<a href="http://interactagram.com/physics/optics/
refraction/">refraction</a>) of light rays
creating multiple images or
<a href="http://en.wikipedia.org/wiki/
Mirage_of_astronomical_objects">mirages</a>, similar to
<a href="http://www.atoptics.co.uk/atoptics/sunmir.htm">sunset and
sunrise mirages</a>.

The effects are most pronounced when
<a href="http://www.atoptics.co.uk/atoptics/mirtemp.htm">temperature
layers</a> in the atmosphere produce sharp changes in air density and
refractive index.

Acting over long sight-lines to the rising and setting Sun or Moon,
the refraction significantly alters the
<a href="http://www.atoptics.co.uk/atoptics/gfmmform.htm">path of
light rays</a> creating merged, distorted images.

Such mirages are also associated with the
<a href="http://antwrp.gsfc.nasa.gov/apod/ap040321.html">Green Flash</a>.

	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[Dunhuang Star Atlas]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap090619.html</link>
	<pubDate>Fri, 19 Jun 2009 13:06:01 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap090619.html"><img src="http://antwrp.gsfc.nasa.gov/apod/image/0906/dunhuang_npole_c800.jpg" /></a>
<title>Dunhuang Star Atlas</title>

This ancient Chinese map of planet Earth's northern sky is part
of the Dunhuang Star Atlas, one of the most impressive
documents in the <a href="http://en.wikipedia.org/wiki/
Timeline_of_Chinese_astronomy">history of astronomy</a>.

The oldest complete star atlas known, it dates to the years 649 to
684, discovered at the
<a href="http://antwrp.gsfc.nasa.gov/apod/ap080831.html">Silk Road</a> town of Dunhuang in 1907.

<a href="http://arxiv.org/abs/0906.3034">A recent analysis</a>
that examines the accuracy and projections
used to make it notes the atlas marks positions of over
1,300 stars and outlines 257 Chinese
<a href="http://www.lcsd.gov.hk/CE/Museum/Space/Research/StarName/
e_research_chinengstarzone.htm">star groups or asterisms</a>.

The star positions in the hand drawn atlas were found to be
accurate to within a few degrees.

In this example showing the north polar region, a very
recognizable <a href="http://antwrp.gsfc.nasa.gov/apod/ap070108.html">Big Dipper</a>, part of the modern
constellation Ursa Major, lies along the bottom of the chart.

An additional 12 charts depict equatorial regions in 30 degree
sections and also include a grouping resembling the modern
constellation <a href="http://antwrp.gsfc.nasa.gov/apod/ap030207.html">Orion</a>.

The <a href="http://www.nature.com/nature/journal/v459/n7248/full/
459778a.html">atlas is on display</a>
at the British Library in London to celebrate the
<a href="http://www.iya2009.org/">International Year of Astronomy</a>.

	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[NGC 6240: Merging Galaxies]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap090618.html</link>
	<pubDate>Thu, 18 Jun 2009 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap090618.html"><img src="http://antwrp.gsfc.nasa.gov/apod/image/0906/ngc6240_spitzerhubble_c800.jpg" /></a>
<title>NGC 6240: Merging Galaxies</title>

NGC 6240 offers a rare glimpse of a cosmic catastrophe in its
final throes.

The titanic galaxy-galaxy
<a href="http://burro.case.edu/JavaLab/GalCrashWeb/main.html">collision</a>
is located a mere 400 million light-years away in the constellation
<a href="http://www.hawastsoc.org/deepsky/oph/index.html">Ophiuchus</a>.

One of the brightest sources in the
<a href="http://coolcosmos.ipac.caltech.edu/cosmic_classroom/
ir_tutorial/index.html">infrared sky</a>, the merging galaxies
spew distorted <a href="http://antwrp.gsfc.nasa.gov/apod/ap060108.html">tidal tails</a>
of stars, gas, and dust and undergo frantic bursts of star
formation. 

The <a href="http://antwrp.gsfc.nasa.gov/apod/ap021128.html">two supermassive</a>
black holes in the original galactic cores
will also coalesce into a single, even more massive black hole. 

<a href="http://hubblesite.org/newscenter/archive/releases/2008/16/
image/ae/">Soon, only</a> one large galaxy will remain.

<a href="http://www.spitzer.caltech.edu/Media/releases/ssc2009-06/
release.shtml">This dramatic image</a> of the scene is a
multiwavelength composite;
red colors trace infrared emission from dust recorded by the
<a href="http://www.spitzer.caltech.edu/Media/releases/ssc2009-12/
release.shtml">Spitzer Space Telescope</a>, with Hubble visible light
images of stars and gas in green and blue hues.

The view spans over 300,000 light-years at the estimated distance
<a href="http://arxiv.org/abs/0807.4549">of NGC 6240</a>.

	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[M13: A Great Globular Cluster of Stars]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap090617.html</link>
	<pubDate>Wed, 17 Jun 2009 13:06:01 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap090617.html"><img src="http://antwrp.gsfc.nasa.gov/apod/image/0906/m13_russell.jpg" /></a>
<title>M13: A Great Globular Cluster of Stars</title>
<a href="http://www.seds.org/messier/m/m013.html">M13</a>
is one of the most prominent and best known
<a href="http://antwrp.gsfc.nasa.gov/apod/globular_clusters.html">globular clusters</a>.  

Visible with binoculars in the constellation of <a href=
"http://en.wikipedia.org/wiki/Hercules_(constellation)"
>Hercules</a>, M13 is frequently one of the first objects found by
<a href="http://antwrp.gsfc.nasa.gov/apod/ap040808.html">curious sky gazers</a> seeking
<a href="http://www.astropics.co.uk/m13.htm"
>celestials wonders</a>
<a href="http://en.wikipedia.org/wiki/Man_Plus">beyond
normal human</a> vision.  

<a href="http://www.concentric.net/~Richmann/m13w.htm"
>M13</a> is a colossal home to over 100,000 stars, spans over 150
<a href="http://www.howstuffworks.com/question94.htm"
>light years</a> across,
lies over 20,000 light years distant,
and is over 12 billion years old.  

At the 1974 dedication of
<a href="http://www.naic.edu/">Arecibo Observatory</a>, a
<a href="http://antwrp.gsfc.nasa.gov/apod/ap000123.html">radio message</a>
about Earth was sent in the direction of
<a href="http://www.windows.umich.edu/cgi-bin/tour_def/the_universe/Globulars.html">M13</a>.  

The reason for the low abundance of unusual
<a href="http://antwrp.gsfc.nasa.gov/apod/ap971104.html">blue straggler stars</a>
in M13 is <a href="http://adsabs.harvard.edu/abs/1997ApJ...484L.145F"
>remains unknown</a>. 

	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[Moonrise Over Turkey]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap090616.html</link>
	<pubDate>Tue, 16 Jun 2009 13:06:01 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap090616.html"><img src="http://antwrp.gsfc.nasa.gov/apod/image/0906/moonrise_sisman.jpg" /></a>
<title>Moonrise Over Turkey</title>
Is the Moon larger when near the horizon?  

No -- as shown above, the 
<a href="http://en.wikipedia.org/wiki/Moon">Moon</a> 
appears to be very nearly the same size no matter 
its location on the sky.  

Oddly, the cause or causes for the common 
<a href="http://en.wikipedia.org/wiki/Moon_illusion"
>Moon Illusion</a> are still being debated.

Two leading explanations both hinge on the 
<a href="http://www.badastronomy.com/bad/misc/moonbig.html"
>illusion</a> that foreground objects make a 
<a href="http://antwrp.gsfc.nasa.gov/apod/ap010219.html">horizon Moon</a> 
seem farther in the distance.  

The historically <a href="http://unmuseum.mus.pa.us/exmoon.htm"
>most popular explanation</a> then holds that the 
mind interprets more distant objects as wider, while a 
<a href="http://facstaff.uww.edu/mccreadd/"
>more recent explanation</a> adds that the distance illusion 
may actually make the <a href="http://www.youtube.com/watch?v=AsKeu4wm3XI"
>eye focus</a> differently.  

Either way, the 
<a href="http://antwrp.gsfc.nasa.gov/apod/ap071025.html">angular diameter of the Moon</a> is 
always about 0.5 degrees.  

In the above time-lapse sequence of the 
<a href="http://antwrp.gsfc.nasa.gov/apod/ap031011.html">Moon</a> taken in 2007, 
with one exposure taken to bring up the foreground of 
<a href="http://en.wikipedia.org/wiki/Izmit">Izmit</a> Bay in 
<a href="http://en.wikipedia.org/wiki/Turkey">Turkey</a>.
 
On the occasion of our 14th <a href=
"http://antwrp.gsfc.nasa.gov/apod/archivepix.html">anniversary</a>, the 
<a href="http://antwrp.gsfc.nasa.gov/apod/image/0906/astronomybeat_apod.pdf">APOD editors</a> thank all of our contributors and <a href="http://antwrp.gsfc.nasa.gov/apod/lib/about_apod.html"
>mirror site operators</a> whose volunteer efforts help 
bring the wonders of 
<a href="http://www.astronomy2009.org/">astronomy</a> to millions of people around the world.

Additional thanks also go to our 
<a href="http://www.bulutsu.org/ggg/">Turkish mirror site</a> operators for submitting the above mouseover image.

	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[Streaming Dark Nebulas near B44]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap090615.html</link>
	<pubDate>Mon, 15 Jun 2009 13:06:01 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap090615.html"><img src="http://antwrp.gsfc.nasa.gov/apod/image/0906/b44_davis.jpg" /></a>
<title>Streaming Dark Nebulas near B44</title>
Dark dust lit by the bright yellow star Antares highlight this photogenic starscape of the southern sky.

A <a href="http://antwrp.gsfc.nasa.gov/apod/ap070911.html">wider angle image</a> shows the
<a href="http://antwrp.gsfc.nasa.gov/apod/ap070930.html">central band</a> of our
<a href="http://en.wikipedia.org/wiki/Milky_Way_galaxy">Milky Way Galaxy</a> connected to
<a href="http://en.wikipedia.org/wiki/Antares">Antares</a> by streams of
dust knows as the
<a href="http://antwrp.gsfc.nasa.gov/apod/ap080603.html">Dark River</a>.  

At the <a href="http://antwrp.gsfc.nasa.gov/apod/ap070903.html">head of the Dark River</a> the
<a href="http://nedwww.ipac.caltech.edu/level5/Mathis/Mathis1.html"
>dust</a> appears in dense knots.  

One of the densest knots is
<a href="http://cosmonut.org/Rho%20Ophiuchus.htm"
>B44</a>, pictured near the bottom of the above image.

Off to the left of the
<a href="http://www.tvdavisastropics.com/astroimages-1_00007f.htm">above
image</a> lies Antares, a star so bright that the
<a href="http://server1.sky-map.org/starview?object_type=3&object_id=236"
>pictured dust</a> reflects its light, giving it a distinct yellow hue.  

<a href="http://www.youtube.com/watch?v=SQtcjz7Q9Cg">Light</a> from the blue star on the image left creates a surrounding blue
<a href="http://antwrp.gsfc.nasa.gov/apod/reflection_nebulae.html">reflection nebula</a>
named <a href="http://www.capella-observatory.com/ImageHTMLs/DiffuseNebula/IC4605.htm">IC 4605</a>.  

B44 and IC 4605 lies about 500 <a href=
"http://starchild.gsfc.nasa.gov/docs/StarChild/questions/question19.html"
>light years</a> distant toward the
<a href="http://en.wikipedia.org/wiki/Constellation">constellation</a> of the
<a href="http://en.wikipedia.org/wiki/Scorpion">Scorpion</a>.

	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[Stars at the Galactic Center]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap090614.html</link>
	<pubDate>Sun, 14 Jun 2009 13:06:01 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap090614.html"><img src="http://antwrp.gsfc.nasa.gov/apod/image/0906/mwcenter_spitzer.jpg" /></a>
<title>Stars at the Galactic Center</title>
<a href="http://antwrp.gsfc.nasa.gov/apod/ap040411.html">The center</a>
of our Milky Way Galaxy
<a href="http://antwrp.gsfc.nasa.gov/apod/ap051004.html">is hidden</a>
from the prying eyes of optical telescopes by clouds of
obscuring dust and gas.

But in <a href="http://www.spitzer.caltech.edu/Media/releases/
ssc2006-02/ssc2006-02a.shtml">this stunning vista</a>,
the Spitzer Space Telescope's
<a href="http://coolcosmos.ipac.caltech.edu/cosmic_classroom/
ir_tutorial/importance.html">infrared</a> cameras, penetrate
much of the
<a href="http://www.youtube.com/watch?v=Z_SOytjGxlM"
>dust revealing</a> the stars of the crowded
<a href="http://en.wikipedia.org/wiki/Galactic_center">galactic center</a>
region.

A mosaic of many smaller snapshots, the detailed,
<a href="http://www.spitzer.caltech.edu/Media/releases/
ssc2006-02/release.shtml">false-color image shows</a>
older, cool stars in bluish hues.

Reddish glowing dust clouds are associated with
young, hot stars in stellar nurseries.

The very center of the Milky Way was only
<a href="http://www.spitzer.caltech.edu/Media/releases/ssc2009-13/release.shtml"
>recently found capable</a> of forming
<a href="http://www.universetoday.com/2009/06/10/astronomers-announce-first-newborn-stars-at-milky-ways-core/">newborn stars</a>.

The <a href="http://antwrp.gsfc.nasa.gov/apod/ap051023.html">galactic center</a>
lies some 26,000 light-years away, toward the constellation
<a href="http://hawastsoc.org/deepsky/sgr/index.html">Sagittarius</a>.

At that distance, this picture spans about 900 light-years.

	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[The Milky Road]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap090613.html</link>
	<pubDate>Sat, 13 Jun 2009 13:06:01 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap090613.html"><img src="http://antwrp.gsfc.nasa.gov/apod/image/0906/milkyroadMan_landolfi.jpg" /></a>
<title>The Milky Road</title>

Inspired by the night skies of planet Earth
in the <a href="http://www.iya2009.org/">International
Year of Astronomy</a>,
photographer Larry Landolfi created this
<a href="http://www.landolfiphoto.com/Site_2/SURREAL_FUN_.html">tantalizing
fantasy</a> view.

The <a href="http://www.landolfiphoto.com/Site_2/
-Composited_Astrophotos-.html">composited image</a>
suggests a luminous Milky Way is the heavenly extension of a country road.

Of course, the
<a href="http://en.wikipedia.org/wiki/
List_of_names_for_the_Milky_Way">name</a> for our galaxy, the
<a href="http://seds.org/messier/more/mw.html">Milky Way</a>
(in Latin, Via Lactea), does refer to its appearance
as a milky band or path in the sky.

In fact, the word galaxy itself derives from the Greek for milk.

Visible on
<a href="http://antwrp.gsfc.nasa.gov/apod/ap040923.html">moonless nights</a>
from <a href="http://antwrp.gsfc.nasa.gov/apod/ap070508.html">dark sky</a> areas,
though not so bright or colorful as in this image, the glowing
<a href="http://science.nasa.gov/headlines/y2001/
ast01nov_1.htm">celestial
band</a> is due to the collective light of myriad stars along the
plane of our galaxy, too faint to be distinguished individually.

The diffuse starlight is cut by dark swaths of
obscuring galactic dust clouds.

Four hundred years ago, Galileo turned his
telescope on the Milky Way and announced it to be

"... a congeries of
<a href="http://www.100hoursofastronomy.org/component/content/
article/55-rfienberg/230-qoh-my-god-its-full-of-starsq">innumerable
stars</a> ..."

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	</description>
    </item>

    <item>
	<title><![CDATA[SNR 0104: An Unusual Suspect]]></title>
	<link>http://antwrp.gsfc.nasa.gov/apod/ap090612.html</link>
	<pubDate>Fri, 12 Jun 2009 13:06:01 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://antwrp.gsfc.nasa.gov/apod/ap090612.html"><img src="http://antwrp.gsfc.nasa.gov/apod/image/0906/snr0104_comp.jpg" /></a>
<title>SNR 0104: An Unusual Suspect</title>

SNR 0104 is a supernova remnant with an unusual shape.

Found 190,000 light-years away in our neighboring galaxy
the <a href="http://antwrp.gsfc.nasa.gov/apod/ap071001.html">Small Magellanic Cloud</a>,
SNR 0104 is suspected of being the expanding debris cloud from a
<a href="http://en.wikipedia.org/wiki/Type_Ia_supernova">Type 1a
supernova</a> - the catastrophic thermonuclear explosion of
a white dwarf star.

For example, like Type 1a supernova remnants within
our galaxy, investigations show that it contains
large amounts of iron.

But unlike other Type 1a remnants, including the well-studied
<a href="http://antwrp.gsfc.nasa.gov/apod/ap090317.html">Tycho</a>,
<a href="http://antwrp.gsfc.nasa.gov/apod/ap070116.html">Kepler</a>, and
<a href="http://antwrp.gsfc.nasa.gov/apod/ap080704.html">SN 1006</a>, SNR 0104 is
definitely not spherical.

In fact, the remnant's shape suggests this supernova explosion
was very asymmetric and produced strong jets.

<a href="http://chandra.harvard.edu/photo/2009/snr0104/">This intriguing
composite image</a> combines
<a href="http://chandra.harvard.edu/about/">Chandra Observatory</a>
x-ray data of the remnant, shown in purple hues, with
<a href="http://www.spitzer.caltech.edu/Media/releases/ssc2009-10/
release.shtml">Spitzer Space Telescope</a> infrared
data covering the wider region, mapped to red and green colors.

It indicates that the supernova explosion
took place in the complicated and dense environment of a
<a href="http://antwrp.gsfc.nasa.gov/apod/ap080829.html">star-forming region</a>.

So, an alternative explanation is that the expanding debris cloud
is sweeping up clumpy interstellar material, accounting
for the odd shape of SNR 0104.

The broad, <a href="http://coolcosmos.ipac.caltech.edu/cosmic_classroom/
multiwavelength_astronomy/multiwavelength_astronomy/">multiwavelength</a>
view spans about 1,800 light-years at the
estimated distance of SNR 0104.

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	</description>
    </item>

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