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	<channel>
		<title>APOD@coRank: Upcoming stories</title>
		<link>http://apod.corank.com/tech/all/upcoming/</link>
		<description>APOD@coRank: Upcoming stories</description>
<image><title>coRank.com</title><link>http://apod.corank.com/tech/all/upcoming/</link><url>http://www.corank.com/pics/coRank2.gif</url></image>
	<item>
			<dc:creator>APOD</dc:creator>
			<title>Stickney Crater</title>
			<link>http://apod.corank.com/tech/story/ap091107.html</link>
			<description><![CDATA[



Stickney Crater, the largest crater on the martian moon Phobos,
is named for
 Chloe
Angeline Stickney  Hall,
mathematician and wife of astronomer Asaph Hall.

Asaph Hall discovered both the
 Red Planet's moons  in 1877.

Over 9 kilometers across, Stickney is nearly half the
 diameter
of Phobos itself , so large that the
impact that blasted out the crater likely came close
to shattering the tiny moon.

This  stunning,
enhanced-color image  of Stickney and surroundings
was recorded by the HiRISE camera onboard the
Mars Reconnaissance Orbiter as it passed within some
six thousand kilometers
 of Phobos  in March of 2008.

Even though the surface gravity of
 asteroid-like
Phobos 
is less than 1/1000th Earth's gravity, streaks suggest loose
material has slid down inside the crater walls over time.

Light bluish regions near the crater's rim could indicate
a relatively freshly exposed surface.

The origin of the
 curious grooves  along the surface is
mysterious but may be related to the crater-forming impact.

  
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			<guid isPermaLink="true">http://apod.corank.com/tech/story/ap091107.html</guid>
			<pubDate>Sat, 07 Nov 2009 11:18:02 GMT</pubDate>
		</item>
	<item>
			<dc:creator>APOD</dc:creator>
			<title>Ring Nebula Deep Field</title>
			<link>http://apod.corank.com/tech/story/ap091106.html</link>
			<description><![CDATA[



A familiar sight to sky enthusiasts with even a small telescope,
the  Ring
Nebula (M57)  is
some 2,000 light-years away in the musical
 constellation
Lyra .

The  central ring  is about one light-year across,
but  this remarkably deep exposure  -
a collaborative effort combining data from three different telescopes -
 explores 
the looping filaments
of glowing gas extending much farther from the nebula's
 central star .

Of course, in this
 well-studied
example  of a
 planetary nebula ,
the glowing material does not come from planets.

Instead,
the  gaseous shroud  represents outer layers
expelled from a dying, sun-like star.

This remarkable composite image includes narrowband image data
recording the Ring's atomic hydrogen emission (shown as violet)
in visible light and molecular hydrogen emission (shown as red)
at near infrared wavelengths.

The much  more distant  spiral
galaxy IC 1296 is also visible at the upper right.

  
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			<pubDate>Sat, 07 Nov 2009 11:18:02 GMT</pubDate>
		</item>
	<item>
			<dc:creator>APOD</dc:creator>
			<title>Halloween's Moon</title>
			<link>http://apod.corank.com/tech/story/ap091105.html</link>
			<description><![CDATA[



Illuminating the landscape  all through the
night  of November 2nd,
this week's bright Full Moon was
known in the northern hemisphere as a
 Hunter's Moon .

But this
 dramatic  view of the shining lunar orb, from
Sobreda, Portugal, was captured just a few nights earlier,
 on Halloween .

In the spirit of
 the season , the image plays a
little trick.

The picture is actually two digital photos - one short and one
long exposure.

They were combined to bring out the details of the
 bright lunar surface  and the
fainter features in the dark, surrounding clouds,
in a single image.

Of course, you may recognize some of the
 spookier shapes 
in the clouds as having visited your neighborhood
last week, along with Halloween's
 Moon .

  
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			<guid isPermaLink="true">http://apod.corank.com/tech/story/ap091105.html</guid>
			<pubDate>Sat, 07 Nov 2009 11:18:02 GMT</pubDate>
		</item>
	<item>
			<dc:creator>APOD</dc:creator>
			<title>Blue Sun Bristling</title>
			<link>http://apod.corank.com/tech/story/ap091104.html</link>
			<description><![CDATA[


Our Sun may look like all soft and fluffy, but it's not.  

 Our Sun  is an
extremely large ball of
 bubbling hot gas , mostly
 hydrogen  gas.  

The  above picture  of our Sun was taken last month in a
specific red color of light emitted by hydrogen gas called
 Hydrogen-alpha 
and then color inverted to appear blue.  

In this light, details of the Sun's
 chromosphere  are particularly visible,  highlighting  numerous thin tubes of
magnetically-confined hot gas known as
 spicules  rising from the Sun like
 bristles  from a shag carpet.

Our Sun glows because it is hot, but it is
 not on fire .  

 Fire  is the rapid acquisition of oxygen,
and there is very little
 oxygen  on the Sun.  

The energy source of our Sun is the nuclear
 fusion  of hydrogen into
 helium  deep within its core.  

No  sunspots  or
 large active regions  were visible on the Sun this day, although some  solar prominences 
are visible around the edges.  


  
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			<pubDate>Sat, 07 Nov 2009 11:18:02 GMT</pubDate>
		</item>
	<item>
			<dc:creator>APOD</dc:creator>
			<title>Seven Sisters Versus California</title>
			<link>http://apod.corank.com/tech/story/ap091103.html</link>
			<description><![CDATA[


On the upper right, dressed in blue, is the
 Pleiades .  

Also known as the
 Seven
Sisters  and
 M45 ,
 the Pleiades 
is one of the brightest and
 most easily visible 
 open clusters 
on the sky.

 The Pleiades 
contains over 3,000 stars, is about 400 light years away, and only 13 light
years across.

 Surrounding the stars  is a spectacular blue
 reflection nebula  made of fine
 dust .  

 A
common legend  is that one of the brighter stars
faded since the cluster was named.

On the lower left, shining in red, is the
 California Nebula .  

Named for its shape, the
 California 
Nebula is much dimmer and hence harder to see
than  the Pleiades .  

Also known as  NGC 1499 , this mass of red glowing
hydrogen gas is about 1,500  light years  away.

Although about 250 full moons could fit
 between them , the above wide angle, deep field image composite has captured
 them   
 both .  



  
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			<guid isPermaLink="true">http://apod.corank.com/tech/story/ap091103.html</guid>
			<pubDate>Sat, 07 Nov 2009 11:18:02 GMT</pubDate>
		</item>
	<item>
			<dc:creator>APOD</dc:creator>
			<title>Ares 1-X Rocket Lifts Off</title>
			<link>http://apod.corank.com/tech/story/ap091102.html</link>
			<description><![CDATA[


Last week, NASA test fired a new rocket.

The  Ares 1 -X was the
first non- shuttle rocket  launched from
 Kennedy Space Center  since the
 Saturn  launched humans to Earth
orbit and the Moon in the 1960s and 1970s.

 NASA  is testing Ares as a
prelude to replacing the aging space shuttle fleet.

The tremendous thrust of the
 Ares 1-X  can bring the massive rocket from a standing start to a
vertical speed of over 100 kilometers per hour in under eight seconds.  

The test  rocket launched  last week was longer than a
football field and covered with over 700 sensors to record data that will enable engineers to refine details of future Ares rockets.  

Pictured above, the
 Ares 1-X blasts into space  while the top part of the rocket becomes engulfed in a
 shock collar  of water droplets likely created by the sudden drop of air pressure.


  
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			<pubDate>Sat, 07 Nov 2009 11:18:02 GMT</pubDate>
		</item>
	<item>
			<dc:creator>APOD</dc:creator>
			<title>The Average Color of the Universe</title>
			<link>http://apod.corank.com/tech/story/ap091101.html</link>
			<description><![CDATA[


What color is the universe?  

More precisely, if the
 entire sky  was smeared out,
what color would the final mix be?  

This  whimsical question  came up when trying to determine
what stars are commonplace in nearby galaxies.

The answer,
 depicted above ,
is a  conditionally perceived shade  of
 beige .  

To determine this, astronomers computationally averaged
the light emitted by one of the largest sample of
 galaxies 
yet analyzed: the 200,000
 galaxies  of the
 2dF survey .  

The resulting
 cosmic
spectrum  has some emission in all parts of the
 electromagnetic spectrum , but a single perceived composite color.  

 This color  has become much less blue over the past 10 billion years,
indicating that redder stars are becoming more prevalent.  

In a  contest  to better name the color, notable entries
included skyvory, univeige, and the winner:
 cosmic latte .


  
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			<guid isPermaLink="true">http://apod.corank.com/tech/story/ap091101.html</guid>
			<pubDate>Sat, 07 Nov 2009 11:18:02 GMT</pubDate>
		</item>
	<item>
			<dc:creator>APOD</dc:creator>
			<title>VdB 152: Reflection Nebula in Cepheus</title>
			<link>http://apod.corank.com/tech/story/ap091031.html</link>
			<description><![CDATA[



Described as a "dusty curtain" or "ghostly apparition",
mysterious reflection nebula VdB 152 really is very faint.

Far from your neighborhood on this
 Halloween Night ,
the cosmic phantom is nearly 1,400 light-years away.

Also cataloged as Ced 201, it lies along the northern Milky Way
in the  royal  constellation Cepheus.

Near the edge of a large molecular cloud,
pockets of interstellar dust in the region block light from
background stars or scatter light from the embedded bright star
giving parts of
 the nebula 
a characteristic blue  color .

Ultraviolet light from the star is also
 thought 
to cause a dim reddish
 luminescence 
in the nebular dust.

Though stars do form in
 molecular clouds , this star
seems to have only accidentally wandered
into the area, as its measured velocity through
space is very different from the cloud's velocity.

This  deep telescopic image 
of the region spans about 7 light-years.

  
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			<pubDate>Sat, 07 Nov 2009 11:18:02 GMT</pubDate>
		</item>
	<item>
			<dc:creator>APOD</dc:creator>
			<title>The Bubble and M52</title>
			<link>http://apod.corank.com/tech/story/ap091030.html</link>
			<description><![CDATA[



To the eye,
 this cosmic composition 
nicely balances the
Bubble Nebula at the upper right with open star cluster M52.

The pair would be lopsided on other scales, though.

Embedded in a complex of
 interstellar dust
and gas  and blown by the winds from a single, massive
 O-type star , the
 Bubble Nebula  (aka NGC 7635) is a
mere 10 light-years wide.  

On the other hand,
 M52 is  a rich open
cluster of around a thousand stars.

The cluster is about 25 light-years across.

Seen toward the northern boundary
 of Cassiopeia , distance estimates
for the Bubble Nebula and associated cloud complex are around
11,000 light-years, while
 star cluster M52 
lies nearly 5,000 light-years away.

  
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			<pubDate>Sat, 07 Nov 2009 11:18:02 GMT</pubDate>
		</item>
	<item>
			<dc:creator>APOD</dc:creator>
			<title>Zodiacal Light Over Laguna Verde</title>
			<link>http://apod.corank.com/tech/story/ap091029.html</link>
			<description><![CDATA[


An unusual triangle of light is visible this time of year just before dawn, in the northern hemisphere.

 Once considered a false dawn , this triangle of light is actually
 Zodiacal Light , light reflected from
 interplanetary dust particles .  

The  bright reflecting triangle  is clearly visible on the right of the above image
taken from Laguna Verde near
 Valpara
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			<pubDate>Sat, 07 Nov 2009 11:18:02 GMT</pubDate>
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