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		<title>APOD@coRank: Featured</title>
		<link>http://apod.corank.com/tech/all/fp/</link>
		<description>APOD@coRank: Featured</description>
<image><title>coRank.com</title><link>http://apod.corank.com/tech/all/fp/</link><url>http://www.corank.com/pics/coRank2.gif</url></image>
	<item>
			<dc:creator>APOD</dc:creator>
			<title>SNR 0104: An Unusual Suspect</title>
			<link>http://apod.corank.com/tech/story/ap090612.html</link>
			<description><![CDATA[



SNR 0104 is a supernova remnant with an unusual shape.

Found 190,000 light-years away in our neighboring galaxy
the  Small Magellanic Cloud ,
SNR 0104 is suspected of being the expanding debris cloud from a
 Type 1a
supernova  - 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
 Tycho ,
 Kepler , and
 SN 1006 , SNR 0104 is
definitely not spherical.

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

 This intriguing
composite image  combines
 Chandra Observatory 
x-ray data of the remnant, shown in purple hues, with
 Spitzer Space Telescope  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
 star-forming region .

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,  multiwavelength 
view spans about 1,800 light-years at the
estimated distance of SNR 0104.

  
<p/>
<div style="font-size:90%;font-weight:bold">
<a href="http://apod.corank.com/tech/story/ap090612.html">Read more...</a> |
<a href="http://apod.corank.com/tech/story/ap090612.html">Original picture</a> |

Votes so far: <span style="color:#080">20</span> / <span style="color:#800">1</span>

</div>

			]]></description>
			<guid isPermaLink="true">http://apod.corank.com/tech/story/ap090612.html</guid>
			<pubDate>Thu, 26 Nov 2009 15:29:33 GMT</pubDate>
		</item>
	<item>
			<dc:creator>APOD</dc:creator>
			<title>The Milky Road</title>
			<link>http://apod.corank.com/tech/story/ap090613.html</link>
			<description><![CDATA[



Inspired by the night skies of planet Earth
in the  International
Year of Astronomy ,
photographer Larry Landolfi created this
 tantalizing
fantasy  view.

The  composited image 
suggests a luminous Milky Way is the heavenly extension of a country road.

Of course, the
 name  for our galaxy, the
 Milky Way 
(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
 moonless nights 
from  dark sky  areas,
though not so bright or colorful as in this image, the glowing
 celestial
band  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
 innumerable
stars  ..."

  
<p/>
<div style="font-size:90%;font-weight:bold">
<a href="http://apod.corank.com/tech/story/ap090613.html">Read more...</a> |
<a href="http://apod.corank.com/tech/story/ap090613.html">Original picture</a> |

Votes so far: <span style="color:#080">11</span> / <span style="color:#800">1</span>

</div>

			]]></description>
			<guid isPermaLink="true">http://apod.corank.com/tech/story/ap090613.html</guid>
			<pubDate>Thu, 26 Nov 2009 15:29:33 GMT</pubDate>
		</item>
	<item>
			<dc:creator>APOD</dc:creator>
			<title>SNR 0104: An Unusual Suspect</title>
			<link>http://apod.corank.com/tech/story/ap090612.html</link>
			<description><![CDATA[



SNR 0104 is a supernova remnant with an unusual shape.

Found 190,000 light-years away in our neighboring galaxy
the  Small Magellanic Cloud ,
SNR 0104 is suspected of being the expanding debris cloud from a
 Type 1a
supernova  - 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
 Tycho ,
 Kepler , and
 SN 1006 , SNR 0104 is
definitely not spherical.

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

 This intriguing
composite image  combines
 Chandra Observatory 
x-ray data of the remnant, shown in purple hues, with
 Spitzer Space Telescope  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
 star-forming region .

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,  multiwavelength 
view spans about 1,800 light-years at the
estimated distance of SNR 0104.

  
<p/>
<div style="font-size:90%;font-weight:bold">
<a href="http://apod.corank.com/tech/story/ap090612.html">Read more...</a> |
<a href="http://apod.corank.com/tech/story/ap090612.html">Original picture</a> |

Votes so far: <span style="color:#080">20</span> / <span style="color:#800">1</span>

</div>

			]]></description>
			<guid isPermaLink="true">http://apod.corank.com/tech/story/ap090612.html</guid>
			<pubDate>Thu, 26 Nov 2009 15:29:33 GMT</pubDate>
		</item>
	<item>
			<dc:creator>APOD</dc:creator>
			<title>Pyrenees Paraselene</title>
			<link>http://apod.corank.com/tech/story/ap090611.html</link>
			<description><![CDATA[



A sea of clouds laps at rugged moutain peaks
of the French Pyrenees in this serene view from
 Pic du Midi  Observatory.

The time exposure was recorded on June 4, with
the constellations Sagittarius and
Scorpius shining in the  starry night .

At the top right lies a faint, but colorful
 moondog
or paraselene .

Analogous to a  sundog or parhelion ,
the paraselene
 is produced by 
moonlight shining through
thin,  hexagonal-shaped  ice crystals in high
 cirrus clouds .

As determined by the ice crystal geometry, a bright
 gibbous Moon  illuminates the scene from beyond the
picture's right edge, 22 degrees from the lovely paraselene.

  
<p/>
<div style="font-size:90%;font-weight:bold">
<a href="http://apod.corank.com/tech/story/ap090611.html">Read more...</a> |
<a href="http://apod.corank.com/tech/story/ap090611.html">Original picture</a> |

Votes so far: <span style="color:#080">26</span> / <span style="color:#800">4</span>

</div>

			]]></description>
			<guid isPermaLink="true">http://apod.corank.com/tech/story/ap090611.html</guid>
			<pubDate>Thu, 26 Nov 2009 15:29:33 GMT</pubDate>
		</item>
	<item>
			<dc:creator>APOD</dc:creator>
			<title>Markarian's Chain of Galaxies</title>
			<link>http://apod.corank.com/tech/story/ap090609.html</link>
			<description><![CDATA[


Across the heart of the
 Virgo Cluster of Galaxies 
lies a striking string of galaxies known as Markarian's Chain.  

The chain,
 pictured above , is highlighted on the upper right with
two large but featureless
 lenticular  galaxies,
 M84  and
 M86 .

Prominent to their lower left is a pair of interacting galaxies known as
 The Eyes .

The home  Virgo Cluster  is the nearest
 cluster of galaxies , contains over 2000 galaxies,
and has a noticeable gravitational pull on the galaxies of the
 Local Group of Galaxies  surrounding our
 Milky Way Galaxy .  

The  center  of the
 Virgo Cluster  is located about 70 million
 light years  away toward the  constellation  of  Virgo .  

At least seven galaxies in
 the chain   
 appear to move coherently ,
although others appear to be superposed by chance.  


  
<p/>
<div style="font-size:90%;font-weight:bold">
<a href="http://apod.corank.com/tech/story/ap090609.html">Read more...</a> |
<a href="http://apod.corank.com/tech/story/ap090609.html">Original picture</a> |

Votes so far: <span style="color:#080">45</span> / <span style="color:#800">3</span>

</div>

			]]></description>
			<guid isPermaLink="true">http://apod.corank.com/tech/story/ap090609.html</guid>
			<pubDate>Thu, 26 Nov 2009 15:29:33 GMT</pubDate>
		</item>
	<item>
			<dc:creator>APOD</dc:creator>
			<title>A Dusty Iris Nebula</title>
			<link>http://apod.corank.com/tech/story/ap090610.html</link>
			<description><![CDATA[



These clouds of interstellar dust and gas have blossomed
1,300 light-years away in the fertile
star fields of the  constellation Cepheus .

Sometimes called the Iris Nebula and dutifully
cataloged as
 NGC 7023 ,
this is not the only nebula in the
sky to evoke the imagery  of flowers .

Surrounding it, obscuring clouds of dust and cold molecular
gas are also present and can suggest other
 convoluted  and
 fantastic  shapes.

Within the Iris, dusty nebular material surrounds a hot,
young star.

The dominant color of the brighter reflection nebula is blue,
 characteristic
of dust  grains reflecting starlight.

Central filaments of the cosmic dust glow with a faint
reddish photoluminesence as some dust grains
 effectively
convert  the star's invisible
 ultraviolet 
radiation to visible red light.

Infrared  observations 
indicate that this nebula may contain
complex carbon molecules known as
 PAHs .

At the estimated distance of the Iris Nebula
 this
remarkable wide field view  is over 30 light-years across.

  
<p/>
<div style="font-size:90%;font-weight:bold">
<a href="http://apod.corank.com/tech/story/ap090610.html">Read more...</a> |
<a href="http://apod.corank.com/tech/story/ap090610.html">Original picture</a> |

Votes so far: <span style="color:#080">38</span> / <span style="color:#800">1</span>

</div>

			]]></description>
			<guid isPermaLink="true">http://apod.corank.com/tech/story/ap090610.html</guid>
			<pubDate>Thu, 26 Nov 2009 15:29:33 GMT</pubDate>
		</item>
	<item>
			<dc:creator>APOD</dc:creator>
			<title>Markarian's Chain of Galaxies</title>
			<link>http://apod.corank.com/tech/story/ap090609.html</link>
			<description><![CDATA[


Across the heart of the
 Virgo Cluster of Galaxies 
lies a striking string of galaxies known as Markarian's Chain.  

The chain,
 pictured above , is highlighted on the upper right with
two large but featureless
 lenticular  galaxies,
 M84  and
 M86 .

Prominent to their lower left is a pair of interacting galaxies known as
 The Eyes .

The home  Virgo Cluster  is the nearest
 cluster of galaxies , contains over 2000 galaxies,
and has a noticeable gravitational pull on the galaxies of the
 Local Group of Galaxies  surrounding our
 Milky Way Galaxy .  

The  center  of the
 Virgo Cluster  is located about 70 million
 light years  away toward the  constellation  of  Virgo .  

At least seven galaxies in
 the chain   
 appear to move coherently ,
although others appear to be superposed by chance.  


  
<p/>
<div style="font-size:90%;font-weight:bold">
<a href="http://apod.corank.com/tech/story/ap090609.html">Read more...</a> |
<a href="http://apod.corank.com/tech/story/ap090609.html">Original picture</a> |

Votes so far: <span style="color:#080">45</span> / <span style="color:#800">3</span>

</div>

			]]></description>
			<guid isPermaLink="true">http://apod.corank.com/tech/story/ap090609.html</guid>
			<pubDate>Thu, 26 Nov 2009 15:29:33 GMT</pubDate>
		</item>
	<item>
			<dc:creator>APOD</dc:creator>
			<title>Asteroid Eros Reconstructed</title>
			<link>http://apod.corank.com/tech/story/ap090607.html</link>
			<description><![CDATA[


Orbiting the
 Sun  between
 Mars  and
 Earth , asteroid 433 Eros was visited by the
 robot spacecraft NEAR-Shoemaker  in 2000 February.  


High-resolution surface 
 images  
and measurements made by  NEAR 's Laser Rangefinder
( NLR )
have been 
 combined  into the
 above visualization  based on the derived
 3D model  of the
 tumbling space rock .

NEAR allowed scientists to discover that
 Eros  is a single solid body,
that its composition is nearly uniform,
and that it formed during the early years of our
 Solar System .  

Mysteries remain, however, including why some
rocks on the surface have disintegrated.  

On 2001 February 12, the NEAR mission drew to a
dramatic close as it was
 crash landed  onto the
 asteroid's surface ,
 surviving well enough  to return an
analysis of the
 composition  of the surface
 regolith .

In December of 2002, NASA made an unsuccessful
 attempt
to communicate  with the spacecraft after it spent 22 months
resting on the asteroid's surface.

NEAR will likely remain on the
 asteroid 
for billions of years as a monument to
human ingenuity at the turn of the
 third millennium .

  
<p/>
<div style="font-size:90%;font-weight:bold">
<a href="http://apod.corank.com/tech/story/ap090607.html">Read more...</a> |
<a href="http://apod.corank.com/tech/story/ap090607.html">Original picture</a> |

Votes so far: <span style="color:#080">53</span> / <span style="color:#800">4</span>

</div>

			]]></description>
			<guid isPermaLink="true">http://apod.corank.com/tech/story/ap090607.html</guid>
			<pubDate>Thu, 26 Nov 2009 15:29:33 GMT</pubDate>
		</item>
	<item>
			<dc:creator>APOD</dc:creator>
			<title>Possible Jet Blown Shells Near Microquasar Cygnus X-1</title>
			<link>http://apod.corank.com/tech/story/ap090608.html</link>
			<description><![CDATA[


What happens to matter that falls toward an energetic black hole?

In the case of
 Cygnus X-1 ,
perhaps little of that matter actually makes it in.

Infalling gas may first collide not only with itself  but with an
 accretion disk 
of  swirling material  surrounding the
 black hole .

The result may be a
 microquasar  that glows across the
 electromagnetic spectrum  and produces powerful
 jets  that expel much of the
infalling matter back into the cosmos at near light speed
before it can even
 approach the black 
hole's
 event horizon .

Confirmation that black hole jets may create expanding shells has come recently from the  discovery of shells  surrounding  Cygnus X-1 .

Pictured above on the upper right is one such shell quite possibly created by the jet of microquasar and black hole candidate
 Cygnus X-1 .  

Rolling your cursor over the image will bring up an annotated version.

The physical processes that create the
 black hole jets  is a topic that continues to be researched.


  
<p/>
<div style="font-size:90%;font-weight:bold">
<a href="http://apod.corank.com/tech/story/ap090608.html">Read more...</a> |
<a href="http://apod.corank.com/tech/story/ap090608.html">Original picture</a> |

Votes so far: <span style="color:#080">55</span> / <span style="color:#800">2</span>

</div>

			]]></description>
			<guid isPermaLink="true">http://apod.corank.com/tech/story/ap090608.html</guid>
			<pubDate>Thu, 26 Nov 2009 15:29:33 GMT</pubDate>
		</item>
	<item>
			<dc:creator>APOD</dc:creator>
			<title>Asteroid Eros Reconstructed</title>
			<link>http://apod.corank.com/tech/story/ap090607.html</link>
			<description><![CDATA[


Orbiting the
 Sun  between
 Mars  and
 Earth , asteroid 433 Eros was visited by the
 robot spacecraft NEAR-Shoemaker  in 2000 February.  


High-resolution surface 
 images  
and measurements made by  NEAR 's Laser Rangefinder
( NLR )
have been 
 combined  into the
 above visualization  based on the derived
 3D model  of the
 tumbling space rock .

NEAR allowed scientists to discover that
 Eros  is a single solid body,
that its composition is nearly uniform,
and that it formed during the early years of our
 Solar System .  

Mysteries remain, however, including why some
rocks on the surface have disintegrated.  

On 2001 February 12, the NEAR mission drew to a
dramatic close as it was
 crash landed  onto the
 asteroid's surface ,
 surviving well enough  to return an
analysis of the
 composition  of the surface
 regolith .

In December of 2002, NASA made an unsuccessful
 attempt
to communicate  with the spacecraft after it spent 22 months
resting on the asteroid's surface.

NEAR will likely remain on the
 asteroid 
for billions of years as a monument to
human ingenuity at the turn of the
 third millennium .

  
<p/>
<div style="font-size:90%;font-weight:bold">
<a href="http://apod.corank.com/tech/story/ap090607.html">Read more...</a> |
<a href="http://apod.corank.com/tech/story/ap090607.html">Original picture</a> |

Votes so far: <span style="color:#080">53</span> / <span style="color:#800">4</span>

</div>

			]]></description>
			<guid isPermaLink="true">http://apod.corank.com/tech/story/ap090607.html</guid>
			<pubDate>Thu, 26 Nov 2009 15:29:33 GMT</pubDate>
		</item>
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