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	<title>Astronomy Blog &#187; Astrinomy Photo</title>
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		<title>International Year of Astronomy (NASA, Chandra, two/ten/09)</title>
		<link>http://www.astronomyinfoblog.com/archives/international-year-of-astronomy-nasa-chandra-twoten09/</link>
		<comments>http://www.astronomyinfoblog.com/archives/international-year-of-astronomy-nasa-chandra-twoten09/#comments</comments>
		<pubDate>Sun, 30 Jan 2011 06:11:45 +0000</pubDate>
		<dc:creator>admin</dc:creator>
				<category><![CDATA[Astrinomy Photo]]></category>
		<category><![CDATA[2/10/09]]></category>
		<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Chandra]]></category>
		<category><![CDATA[International]]></category>
		<category><![CDATA[NASA]]></category>
		<category><![CDATA[Year]]></category>

		<guid isPermaLink="false">http://www.astronomyinfoblog.com/archives/international-year-of-astronomy-nasa-chandra-twoten09/</guid>
		<description><![CDATA[A few great Astronomy images I observed: Astronomy&#32&#97&#110d Astrophysics Advisory Committee Meeting 22-23 Fe&#98&#32&#50011 Astronomy and Astrophysics Advisory Committee &#77&#101&#101ting 22-23 Feb 2011 International Yr of Astronomy &#40&#78&#65SA, Chandra, 2/ten/09) Picture by NASA&#8217;s Marshall Space Flight &#67&#101&#110ter Messier 101 (M101) is a experience-on spiral g&#97&#108&#97xy about 22 million light a long time absent in th&#101&#32&#99onstellation [...]]]></description>
			<content:encoded><![CDATA[<p>A few great Astronomy images I observed:</p>
<p><strong>Astronomy&#32&#97&#110d Astrophysics Advisory Co<s></s>mmittee Meeting 22-23 Fe&#98&#32&#50011</strong><br />
Astronomy and Astrophysics Advisory Committee &#77&#101&#101<s></s>ting 22-23 Feb 2011</p>
<p><strong>International Yr of Astronomy &#40&#78&#65SA, Chandra, 2/ten/09)</strong><br />
<img alt="Astronomy" src="http://farm4.static.flickr.com/3337/3269451739_cfc71914d2.jpg" width="400"/><br/><br />
<i>Pic<input id="tracker" type="hidden" />ture by NASA&#8217;s Marshall Space Flight &#67&#101&#110ter</i><br />
Messier 101 (M101) is a experience-on spiral g&#97&#108&#97x<input type="hidden" />y about 22 million light a long time absent in th&#101&#32&#99onstellation Ursa Key. It is<input id="apps" type="hidden" /> related to the Milky &#87&#97&#121 galaxy in several approaches, but is more substan&#116&#105&#97l.<input id="tracker" type="hidden" /> The new &quot;Great Observatories&quot; composite picture of M101 was distributed to ov&#101&#114&#32one hundred planetariums, mus<input id="apps" type="hidden" />eums, nature centers,&#32&#97&#110d colleges across the nation in conjunction with G&#97&#108&#105leo&#8217;s birthday on<s></s> February 15. The year 2009 marks the 400th ann&#105&#118&#101rsary of Galileo&#8217;s telescope and has been de<input id="phpint" type="hidden" />signated the Global &#89&#101&#97r of Astronomy to celebrate this historic annivers&#97&#114&#121. </p>
<p>T<input id="counter" type="hidden" />his picture of the spiral galaxy Messier 101 (&#77&#49&#481) is a composite of informatio<s></s>n from NASA&#8217;s Chandra X-ray Obser&#118&#97&#116ory, the Hubble Area Telescope, and the Spitzer Ar&#101&#97&#32Teles<input id="tracker" type="hidden" />cope. The colors correspond to the following &#119&#97&#118elengths: The X-rays detected by<s></s> Chandra are color&#101&#100&#32blue. Sources of X-rays involve million-diploma ga&#115&#111&#108ine, t<input id="counter" type="hidden" />he debris from exploded stars, and material &#122&#111&#111ming close to black holes and neu<input id="tracker" type="hidden" />tron stars. The r&#101&#100&#32shade exhibits Spitzer&#8217;s watch in infrared light. It highlights &#116&#104&#101 warmth<input id="tracker" type="hidden" /> emitted by dust lanes in the galaxy where &#98&#121&#32stars can kind. Lastly, the yellow<input id="tracker" type="hidden" /> coloring is vis&#105&#98&#108e light information from Hubble. Most of this ligh&#116&#32&#97rrives f<input id="stats" type="hidden" />rom stars, and they trace the very same sp&#105&#114&#97l framework as the dust lanes. </p>
<p>Ima<input id="counter" type="hidden" />ge credit:<br />
X-ra&#121&#58&#32NASA/CXC/JHU/K.Kuntz et al.; Optical: NASA/ESA/STScI/JHU/K. &#75&#117&#110tz et al; IR: NASA/<input id="tracker" type="hidden" />JPL-Caltech/STScI/K. Gordon </p>
<p>Find out mor&#101&#58<br />&#10<a href="http://www.nasa.gov/mission_pages/chandra/news/H-09-026.html" rel="nofollow">www.nasa.gov/mission_pages/chandra/i<input id="counter" type="hidden" />nformation/H-0&#57&#45&#4826.html</a></p>
<p>p.s. You can see all of our Chandra pictur&#101&#115&#32in the Cha<input id="apps" type="hidden" />ndra Group in Flickr at: <a href="http://www.flickr.com/groups/chandranasa/">www.flickr.com/&#103&#114&#111ups/chandranasa/</a>  We&#8217;d appreciate to have you as a <input id="apps" type="hidden" />member!</p>
<p><strong>Astro&#110&#111&#109y For Novices</strong><br />
<img alt="Astronomy" src="http://farm2.static.flickr.com/1293/1160110085_d4026d1271.jpg" width="400"/><br/><br />
<i>Picture by AndyRob</i><br />
<a href="http://astronomy-for-beginners.blogspot.com/">Astronomy For No&#118&#105&#99es</a></p>
<p>A blog p<input id="counter" type="hidden" />age to indulge two biggest interests &#8211; amateur astron&#111&#109&#121 and the internet.</p>
<p><b>Comet Facts</b></p>
<p>Fact1: <input id="apps" type="hidden" />A comet is a&#32&#99&#111nglomerate of particles bound collectively by ice &#40&#110&#111t automatica<s></s>lly H2O h2o ice, it could be dry ice (&#67&#79&#50), for illustration)</p>
<p>Fact2: When a come<input id="tracker" type="hidden" />t methods t&#104&#101&#32sun the ice melts and releases the particles from &#116&#104&#101 primary syst<input id="counter" type="hidden" />em.</p>
<p>Fact3: The tail of a comet often &#112&#111&#105nts away from the sun.</p>
<p>As the photograph<input id="tracker" type="hidden" /> beneath s&#104&#111&#119s, there are in actuality two tails, both curved, &#97&#110&#100 they are 30 M<input id="stats" type="hidden" />ILLION kilometres very long. That&#8217;s a whole lot of&#32&#103&#114eat particles. The concept is that the so<input id="stats" type="hidden" />lar wind &#105&#115&#32accountable for the blue fuel and gravity by yours&#101&#108&#102 for the bigger<input id="counter" type="hidden" /> particles.</p>
<p>Far more fascinating co&#115&#109&#111logical details will unfold at <a href="http://astronomy-for-beginners.blogspot.com/">Astronomy F<input type="hidden" />or Newco&#109&#101&#114s</a></p>
<p><strong>Mullard Radio Astronomy Observatory</strong><br />
<img alt="Astronomy" src="http://farm5.static.flickr.com/4007/4550186343_28d00db203.jpg" width="400"/><br/><br />
<i>Image by Jo&#110&#97&#116han Herbert</i><br />
This<input id="tracker" type="hidden" /> is the Mullard Radio Astronomy Ob&#115&#101&#114vatory, this was captured at sunset and the<input id="counter" type="hidden" />n photm&#97&#116&#114ix was made use of to provide out the specifics of&#32&#116&#104e highlights and <input id="phpint" type="hidden" />then pushed as a result of a b\w &#102&#105&#108ter to get the b\w impact.  This is my initi<input id="phpint" type="hidden" />ally a&#116&#116&#101mpt at a b/w photo.</p>
<p><a href="http://www.flickr.com/photos/flcherb/4550186343/sizes/l/">See Substantial </a></p>
<p><a href="http://bighugelabs.com/onblack.php?id=4550186343&amp;size=large" rel="nofollow">View On Black</a></p>

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		<title>Newly Found Solar System</title>
		<link>http://www.astronomyinfoblog.com/archives/newly-found-solar-system/</link>
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		<pubDate>Fri, 27 Aug 2010 00:56:59 +0000</pubDate>
		<dc:creator>admin</dc:creator>
				<category><![CDATA[Astrinomy Photo]]></category>
		<category><![CDATA[newly]]></category>
		<category><![CDATA[solar system]]></category>

		<guid isPermaLink="false">http://www.astronomyinfoblog.com/?p=248</guid>
		<description><![CDATA[This is cool stuff, astronomers making use of the&#32&#69&#83O HARPS instrument have discovered a planetary pro&#103&#114&#97m with no less than 5 planets and possibly a coupl&#101&#32&#109uch more all-around a Sun-like star. The superstar&#32&#105&#115 known as HD10180 and is positioned 127 light-year&#115&#32&#97way from the constellation Hydrus. Here’s the pr&#101&#115&#115 release from the ESO: “We have found [...]]]></description>
			<content:encoded><![CDATA[<p><img src="http://tomsastroblog.com/images/hd10180_eso.jpg" alt="solar" /><br />
This is cool stuff, astronomers making use of the&#32&#69&#83O HARPS instrument have di<input id="counter" type="hidden" />scovered a planetary pro&#103&#114&#97m with no less than 5 planets and possibly a coupl&#101&#32&#109<input id="stats" type="hidden" />uch more all-around a Sun-like star. The superstar&#32&#105&#115 known as HD10180 and is po<input type="hidden" />sitioned 127 light-year&#115&#32&#97way from the constellation Hydrus.</p>
<p>Here’s the pr&#101&#115&#115 <input id="stats" type="hidden" />release from the ESO:</p>
<p>“We have found what is mo&#115&#116&#32likely the program with the <input id="tracker" type="hidden" />most planets yet found&#44&#226&#128 claims Christophe Lovis, lead author on the pape&#114&#32&#114ep<input id="tracker" type="hidden" />orting the end result. “This remarkable discov&#101&#114&#121 also highlights the reality <input id="counter" type="hidden" />that we are now enter&#105&#110&#103 a new era in exoplanet investigation: the study o&#102&#32&#99omp<input type="hidden" />licated planetary methods and not just of perso&#110&#32&#112lanets. Studies of planetary m<input id="apps" type="hidden" />otions in the new me&#116&#104&#111d reveal intricate gravitational interactions amon&#103&#32&#116he p<input id="phpint" type="hidden" />lanets and give us insights into the long-term&#32&#101&#118olution on the method.”</p>
<p>The t<input id="tracker" type="hidden" />eam of astronomers &#117&#116&#105lized the HARPS spectrograph, attached to ESO’s &#116&#104&#114ee.6-<s></s>metre telescope at La Silla, Chile, for a six&#45&#121&#101ar-long analyze in the Sun-like <input type="hidden" />take the leading r&#111&#108&#101 HD 10180, situated 127 light-years away within th&#101&#32&#115outher<input type="hidden" />n constellation of Hydrus (the Male Water Sn&#97&#107&#101).<br /> HARPS is an instrument with un<input id="apps" type="hidden" />rivalled measurem&#101&#110&#116 stability and great precision and may be the worl&#100&#226&#128s most<input id="phpint" type="hidden" /> successful exoplanet hunter.</p>
<p>Thanks toward&#115&#32&#116he 190 person HARPS measurements, <input id="stats" type="hidden" />the astronomers &#100&#101&#116ected the tiny back and forth motions of the take &#116&#104&#101 leading<input id="tracker" type="hidden" /> role caused from the complicated gravitat&#105&#111&#110al attractions from 5 or far more p<input id="tracker" type="hidden" />lanets. The fiv&#101&#32&#115trongest signals correspond to planets with Neptun&#101&#45&#108ike masse<input id="phpint" type="hidden" />s — involving 13 and 25 Earth masses &#148&#32&#119hich orbit the superstar with period<input id="apps" type="hidden" />s ranging from&#32&#97&#98out 6 to 600 days. These planets are found involvi&#110&#103&#32.06 and 1.<input id="phpint" type="hidden" />4 times the Earth–Sun distance from th&#101&#105&#114 central take the leading role.</p>
<p>“We<s></s> also have fi&#110&#101&#32factors to believe that two other planets are pres&#101&#110&#116,” says L<input type="hidden" />ovis. One can be a Saturn-like planet (&#116&#104&#97t has a minimum mass of 65 Earth masse<input id="phpint" type="hidden" />s) orbiting &#105&#110&#322200 days. The other could be the least substantia&#108&#32&#101xoplanet eve<input id="tracker" type="hidden" />r identified, with a mass of about 1.4&#32&#116&#105mes that from the Earth. It&#8217;s really close to its hos<input id="stats" type="hidden" />t take the &#108&#101&#97ding role, at just 2 percent of the Earth–Sun di&#115&#116&#97nce. A single<input type="hidden" /> “year” on this planet would last&#32&#111&#110ly 1.18 Earth-days.</p>
<p>“This object cause<input id="stats" type="hidden" />s a wobble&#32&#111&#102 its star of only about 3 km/hour— slower than w&#97&#108&#107ing speed — <s></s>and this motion is really difficult &#116&#111&#32measure,” says group member Damien Ség<input id="stats" type="hidden" />ransan. I&#102&#32&#99onfirmed, this object could well be an additional &#101&#120&#97mple of the hot<input id="apps" type="hidden" /> rocky planet, comparable to Corot-&#55&#98&#32(a href=”http://www.eso.org/public/news/<input id="stats" type="hidden" />eso0933/&#226&#128&#157>eso0933).</p>
<p>The newly found out method of planets a&#108&#108&#32around HD 10180 <input id="counter" type="hidden" />is distinctive in various respects&#46&#32&#49st of all, with no less than five Neptune-l<input id="apps" type="hidden" />ike pla&#110&#101&#116s lying within a range equivalent for the orbit of&#32&#77&#97rs, this method i<input id="apps" type="hidden" />s much more populated than our So&#108&#97&#114 Technique in its inner region, and has many<input id="apps" type="hidden" /> addit&#105&#111&#110al huge planets there. Furthermore, the program al&#109&#111&#115t certainly has no<s></s> Jupiter-like gas giant. In addi&#116&#105&#111n, all the planets appear to have virtually c<input id="phpint" type="hidden" />ircul&#97&#114&#32orbits.</p>
<p>So far, astronomers know of fifteen method&#115&#32&#119ith a minimum of 3 <input type="hidden" />planets. The last record-holder&#32&#119&#97s 55 Cancri, which contains five planets, two <input id="tracker" type="hidden" />of t&#104&#101&#109 getting giant planets. “Systems of low-mass pla&#110&#101&#116s like the one parti<input id="phpint" type="hidden" />cular all-around HD 10180 appe&#97&#114&#32to be really frequent, but their formation hist<s></s>ory&#32&#114&#101mains a puzzle,” says Lovis.</p>
<p>Applying the new di&#115&#99&#111very too as informati<input id="phpint" type="hidden" />on for other planetary system&#115&#44&#32the astronomers found an equivalent with the Tit<input id="tracker" type="hidden" />iu&#115&#226&#128Bode law that exists in our Solar System: the dis&#116&#97&#110ces on the planets fro<input id="tracker" type="hidden" />m their take the leading rol&#101&#32&#97ppear to follow a frequent pattern. “This could<input id="apps" type="hidden" /> &#112&#111&#115sibly be a signature with the formation course of &#97&#99&#116ion of these planetary <input id="tracker" type="hidden" />systems,” states team mem&#98&#101&#114 Michel Mayor.</p>
<p>An additional critical result uncov<input id="counter" type="hidden" />&#101&#114&#101d from the astronomers whilst studying these devic&#101&#115&#32is that there can be a r<input id="tracker" type="hidden" />elationship among the mass&#32&#111&#102 a planetary program and the mass and chemical con&#116<s></s>&#101&#110t of its host movie star. All extremely substantia&#108&#32&#112lanetary techniques are o<input id="stats" type="hidden" />bserved all-around huge a&#110&#100&#32metal-rich stars, even though the four lowest-mass&#32&#115<input type="hidden" />&#121stems are found approximately lower-mass and metal&#45&#112&#111or stars. Such properties <input id="counter" type="hidden" />confirm present theoreti&#99&#97&#108 models.</p>
<p>The discovery is announced nowadays in th&#101&#32&#105<s></s>nternational colloquium “Detection and dynamics &#111&#102&#32transiting exoplanets”, i<input type="hidden" />n the Observatoire de H&#97&#117&#116e-Provence, France.</p>

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		<title>Lost to the Galaxy</title>
		<link>http://www.astronomyinfoblog.com/archives/lost-to-the-galaxy/</link>
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		<pubDate>Thu, 12 Aug 2010 02:57:28 +0000</pubDate>
		<dc:creator>admin</dc:creator>
				<category><![CDATA[Astrinomy Photo]]></category>
		<category><![CDATA[Astronomy Report]]></category>
		<category><![CDATA[Galaxy]]></category>
		<category><![CDATA[yard]]></category>

		<guid isPermaLink="false">http://www.astronomyinfoblog.com/?p=194</guid>
		<description><![CDATA[We use the exact same process when we sling our s&#112&#97&#99ecraft close to planets to give them a speed-boost&#46&#32&#73t works Really well. How frequent is such an event&#32&#119&#101 really don&#8217;t know. We’ve observed 16 so far. The original com&#112&#97&#110ion planets from the stars may well be on their wa&#121&#32&#111ut on the galaxy, also, but because [...]]]></description>
			<content:encoded><![CDATA[<p><img src="http://tomsastroblog.com/images/2010/08/Chandra-image-of-Sgr-A.jpg" alt="Galaxy" /><br />
We use the exact same process when we sling our s&#112&#97&#99ecraft close to planets to<input id="tracker" type="hidden" /> give them a speed-boost&#46&#32&#73t works Really well.</p>
<p>How frequent is such an event&#32&#119&#101<input id="apps" type="hidden" /> really don&#8217;t know. We’ve observed 16 so far. The original com&#112&#97&#110ion planets from the stars <s></s>may well be on their wa&#121&#32&#111ut on the galaxy, also, but because they are not s&#104&#105&#110y<input id="stats" type="hidden" /> we never see them. They aren’t nonetheless cir&#99&#108&#105ng their star, that is for s<input id="apps" type="hidden" />pecific. They all may &#112&#101&#114haps eventually be captured, but it won’t be in &#116&#104&#105s <input id="counter" type="hidden" />galaxy. They’re outta here.</p>
<p>Theorized in 1988 &#97&#110&#100 found out in 2005, not a lot<input id="tracker" type="hidden" /> yet is identified ab&#111&#117&#116 HVS. So far, the theory runs that there may well &#98&#101&#32as <input type="hidden" />several as 1,000 of them inside Milky Way Galax&#121&#46&#32Thinking about you can find 10<input id="tracker" type="hidden" />0 billion stars insi&#100&#101&#32Milky Way, that’s not a entire great deal. Still&#44&#32&#116hey <input id="stats" type="hidden" />confident aren’t hanging close to waiting fo&#114&#32&#117s to take their picture. We cou<s></s>ld possibly be acqu&#105&#114&#105ng new ones all of the time.<br />
<img src="http://tomsastroblog.com/images/2010/08/IsolatedNeutronStar.jpg" alt="HST-WFPC2" /><br />
Some scientists beli&#101&#118&#101 our <input id="apps" type="hidden" />HVS could possibly be stars our galaxy origin&#97&#108&#108y captured from an orbiting dwar<input id="tracker" type="hidden" />f galaxy which got&#32&#97&#115 well close. Some neutron stars are inferred to be&#32&#97&#116 high <input id="stats" type="hidden" />velocity, but that is the result of an asymm&#101&#116&#114ical supernova. Not just did it s<input id="phpint" type="hidden" />upernova, it supe&#114&#110&#111vaed messily. An example of that will be the neutr&#111&#110&#32star RX<input id="tracker" type="hidden" /> J0822-4300, which moves at .5% of light ra&#116&#101&#44 or about 1500 km/s. That speed do<input type="hidden" />esn’t grab you&#63&#32&#84he 125X1400mm shell fired out of a tank travels at&#32&#97&#98out 1700<input id="tracker" type="hidden" /> m/s. Or about 6120 km/h. Hmmm, which is k&#105&#108&#111meters per second vs kilometers per<input id="stats" type="hidden" /> hour. These pu&#112&#112&#105es are not wasting time.</p>
<p>The first HVS discovered &#105&#115&#32SDSS J090<input id="tracker" type="hidden" />744.99 024506.8. Its “other” name is &#116&#104&#101 Outcast Star. I never know which is<input id="phpint" type="hidden" /> worse. 1 fact&#111&#114&#32is for certain; you can find a great deal of strange, strang&#101&#32&#105ssues in t<input type="hidden" />he universe. Some of them in our own bac&#107&#32&#121ard.</p>

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		<title>The Antennae from the Great Observatories</title>
		<link>http://www.astronomyinfoblog.com/archives/the-antennae-from-the-great-observatories/</link>
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		<pubDate>Sat, 07 Aug 2010 18:02:23 +0000</pubDate>
		<dc:creator>admin</dc:creator>
				<category><![CDATA[Astrinomy Photo]]></category>
		<category><![CDATA[Astronomy Report]]></category>
		<category><![CDATA[Antennae]]></category>
		<category><![CDATA[Great Observatories]]></category>

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		<description><![CDATA[Here’s a Chandra release from the Antennae Gala&#120&#105&#101s. The compilation of the colliding galaxies can b&#101&#32&#97 collaborative effort by Chandra, Hubble and the S&#112&#105&#116zer Room telescopes. I’ve included the press rel&#101&#97&#115e below, but there is also a video on the Chandra &#119&#101&#98site and you&#8217;ll be able to access much more and larger images in&#99&#108&#117ding desktops [...]]]></description>
			<content:encoded><![CDATA[<p><img src="http://tomsastroblog.com/images/chandra080610.jpg" alt="Antennae" /><br />
Here’s a Chandra release from the Antennae Gala&#120&#105&#101s. The compilation of the <input id="stats" type="hidden" />colliding galaxies can b&#101&#32&#97 collaborative effort by Chandra, Hubble and the S&#112&#105&#116<input id="phpint" type="hidden" />zer Room telescopes. I’ve included the press rel&#101&#97&#115e below, but there is also <input id="tracker" type="hidden" />a video on the Chandra &#119&#101&#98site and you&#8217;ll be able to access much more and larger images in&#99&#108&#117d<input id="apps" type="hidden" />ing desktops so be certain to have a look.</p>
<p>The Ch&#97&#110&#100ra press release:</p>
<p>A stunning<input id="counter" type="hidden" /> new image of two coll&#105&#100&#105ng galaxies has been released by NASA’s Good Obs&#101&#114&#118at<input id="counter" type="hidden" />ories. The Antennae galaxies, located about 62 m&#105&#108&#108ion light years from Earth, a<input id="tracker" type="hidden" />re shown in this comp&#111&#115&#105te graphic from the Chandra X-ray Observatory (blu&#101&#41&#44 th<input type="hidden" />e Hubble Space Telescope (gold), along with the&#32&#83&#112itzer Space Telescope (red).</p>
<p>T<input id="stats" type="hidden" />he collision, which &#98&#101&#103an more than 100 million years ago and is still oc&#99&#117&#114ring<input id="tracker" type="hidden" />, has triggered the formation of millions of s&#116&#97&#114s in clouds of dusts and gas in<input id="tracker" type="hidden" />side the galaxies. &#84&#104&#101 most massive of these young stars have already sp&#101&#100&#32via t<input id="stats" type="hidden" />heir evolution in a few million many years an&#100&#32&#101xploded as supernovas.</p>
<p>The X-ray<input id="counter" type="hidden" /> picture from Chan&#100&#114&#97 shows massive clouds of hot, interstellar gas tha&#116&#32&#104ave be<input id="phpint" type="hidden" />en injected with rich deposits of elements f&#114&#111&#109 supernova explosions. This enric<input id="counter" type="hidden" />hed gas, which in&#99&#108&#117des elements such as oxygen, iron, magnesium and s&#105&#108&#105con, wi<input id="tracker" type="hidden" />ll be incorporated into new generations of &#115&#116&#97rs and planets. The bright, point-<input type="hidden" />like sources in &#116&#104&#101 graphic are produced by material falling onto bla&#99&#107&#32holes an<input id="counter" type="hidden" />d neutron stars that happen to be remnants&#32&#111&#110 the massive stars. Some of these b<s></s>lack holes may &#104&#97&#118e masses that happen to be nearly one hundred time&#115&#32&#116hat from <input id="stats" type="hidden" />the Sun.</p>
<p>The Spitzer data show infrared l&#105&#103&#104t from warm dust clouds that have be<input id="tracker" type="hidden" />en heated by n&#101&#119&#98orn stars, with the brightest clouds lying in the &#111&#118&#101rlap regio<input id="tracker" type="hidden" />n between the two galaxies. The Hubble i&#110&#102&#111rmation reveal old stars in red, fila<input id="apps" type="hidden" />ments of dust&#32&#105&#110 brown and star-forming regions in yellow and whit&#101&#46&#32Numerous in<input type="hidden" /> the fainter objects within the optical&#32&#103&#114aphic are clusters containing thousand<input id="apps" type="hidden" />s of stars.</p>
<p>&#84&#104&#101 Antennae galaxies take their name from the long a&#110&#116&#101nna-like “<input id="counter" type="hidden" />arms,” seen in wide-angle views in t&#104&#101&#32system. These functions were produced b<input id="counter" type="hidden" />y tidal for&#99&#101&#115 generated from the collision.</p>
<p>Credits: X-ray: NAS&#65&#47&#67XC/SAO/J.DePa<s></s>squale; IR: NASA/JPL-Caltech; Optical: NASA/STScI</p>

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		<title>Images Show Oil&#8217;s Invasion Along Louisiana Coast</title>
		<link>http://www.astronomyinfoblog.com/archives/images-show-oils-invasion-along-louisiana-coast/</link>
		<comments>http://www.astronomyinfoblog.com/archives/images-show-oils-invasion-along-louisiana-coast/#comments</comments>
		<pubDate>Fri, 06 Aug 2010 14:37:29 +0000</pubDate>
		<dc:creator>admin</dc:creator>
				<category><![CDATA[Astrinomy Photo]]></category>
		<category><![CDATA[Astronomy Report]]></category>
		<category><![CDATA[Coast]]></category>
		<category><![CDATA[Images]]></category>
		<category><![CDATA[NASA]]></category>
		<category><![CDATA[Oil's Invasion]]></category>

		<guid isPermaLink="false">http://www.astronomyinfoblog.com/?p=174</guid>
		<description><![CDATA[These images, acquired on May perhaps 24, 2010 by&#32&#116&#104e Multi-angle Imaging SpectroRadiometer (MISR) ins&#116&#114&#117ment aboard NASA&#8217;s Terra spacecraft, show the encroachment of oi&#108&#32&#102rom the former Deepwater Horizon rig into Louisian&#97&#8217;s wildlife h&#97&#98&#105tats. The source with the spill is located off the&#32&#115&#111utheastern (bottom suitable) edge from the images.&#10&#68&#97rk filaments of oil are observed approaching the s&#104&#111&#114es [...]]]></description>
			<content:encoded><![CDATA[<p><img src="http://www.nasa.gov/images/content/460536main_pia13174-combo_946-710.jpg" alt="Oil" /><br />
These images, acquired on May perhaps 24, 2010 by&#32&#116&#104e Multi-angle Imaging Spec<input id="stats" type="hidden" />troRadiometer (MISR) ins&#116&#114&#117ment aboard NASA&#8217;s Terra spacecraft, show the encroachment of oi&#108&#32&#102<input id="tracker" type="hidden" />rom the former Deepwater Horizon rig into Louisian&#97&#8217;s wildlife h&#97&#98&#105tats. The source with the s<input id="stats" type="hidden" />pill is located off the&#32&#115&#111utheastern (bottom suitable) edge from the images.</p>&#10<p>&#68&#97r<input id="counter" type="hidden" />k filaments of oil are observed approaching the s&#104&#111&#114es of Blind Bay and Redfish <input type="hidden" />Bay at the eastern edg&#101&#32&#111n the Mississippi River delta, and also nearing Ga&#114&#100&#101n <input id="counter" type="hidden" />Island Bay and East Bay farther towards south. T&#104&#101&#115e areas are house to several <input id="phpint" type="hidden" />varieties of fish. To&#32&#116&#104e north, the arc-shaped pattern of land and runoff&#32&#105&#115 as<input type="hidden" />sociated with the Chandeleur Islands, which are&#32&#112&#97rt of the Breton National Wild<input id="tracker" type="hidden" />life Refuge. This re&#102&#117&#103e is the second oldest inside the United States an&#100&#32&#99an b<input id="phpint" type="hidden" />e a habitat for dozens of seabird, shorebird a&#110&#100&#32waterfowl species. Oil is repor<input id="tracker" type="hidden" />ted to have reached&#32&#116&#104e islands on May possibly 6. Eighteen days later, &#116&#104&#105s ima<input id="counter" type="hidden" />ge shows filaments of oil crossing the island&#32&#98&#97rrier &#8212; which had been heavily eroded by Hurri<input id="apps" type="hidden" />cane Katrina in 20&#48&#53&#32&#8212; and entering the Breton and Chandeleur Sounds.</p>
<p>The left-hand i&#109&#97&#103e cont<input id="apps" type="hidden" />ains information from MISR&#8217;s vertical-viewing camera. It i&#115&#32&#115hown in near-true color, except t<input id="tracker" type="hidden" />hat data in the i&#110&#115&#116rument&#8217;s near-infrared band, where vegetation appears bright, ha&#118&#101&#32been bl<input id="tracker" type="hidden" />ended using the instrument&#8217;s green band to enhance the ap&#112&#101&#97rance of vegetation.</p>
<p>The Mississip<input type="hidden" />pi River delta i&#115&#32&#108ocated below the picture center. The slick is obse&#114&#118&#101d approa<input id="phpint" type="hidden" />ching the delta from the lower suitable, a&#110&#100&#32filaments of oil are also apparent <s></s>farther for the&#32&#110&#111rth (towards the top). The oil is made visible by &#115&#117&#110 reflecti<input id="phpint" type="hidden" />ng off the sea surface at the same angle &#102&#114&#111m which the instrument is viewing it<input id="apps" type="hidden" />, a phenomenon&#32&#107&#110own as sunglint. Oil makes the surface look bright&#101&#114&#32under thes<input id="phpint" type="hidden" />e viewing conditions than it would if no&#32&#111&#105l were present. Even so, other factor<input id="apps" type="hidden" />s can also ca&#117&#115&#101 enhanced glint, for example reduced surface wind &#115&#112&#101ed. To sepa<input id="apps" type="hidden" />rate glint patterns caused by oil from &#116&#104&#101se other factors, additional informati<input id="counter" type="hidden" />on from MISR&#8217;s cameras is &#101&#109&#112loyed inside the right-hand image.</p>
<p>Previous MISR i&#109&#97&#103ery in the s<input id="stats" type="hidden" />pill shows that the contrast of the oi&#108&#32&#97gainst the surroundings is enhanced by <input id="phpint" type="hidden" />using a com&#98&#105&#110ation of vertical views and oblique-angle views. T&#104&#101&#32right-hand pa<input id="stats" type="hidden" />nel was constructed by combining data&#32&#102&#114om various MISR channels. In this false-<input id="counter" type="hidden" />color view&#44&#32&#111il appears in shades of inky blue to black; silt-laden water&#32&#97&#115 a result of r<input id="phpint" type="hidden" />unoff in the Mississippi River shows&#32&#117&#112 as orange, red and violet; and land and clouds app<input id="phpint" type="hidden" />ear in sh&#97&#100&#101s of cyan.</p>

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		<title>Clouds like a Dragon!</title>
		<link>http://www.astronomyinfoblog.com/archives/clouds-like-a-dragon/</link>
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		<pubDate>Fri, 06 Aug 2010 14:34:05 +0000</pubDate>
		<dc:creator>admin</dc:creator>
				<category><![CDATA[Astrinomy Photo]]></category>
		<category><![CDATA[Astronomy Report]]></category>
		<category><![CDATA[Clouds]]></category>
		<category><![CDATA[Dragon]]></category>

		<guid isPermaLink="false">http://www.astronomyinfoblog.com/?p=172</guid>
		<description><![CDATA[A dragon in the clouds. Click for a larger versio&#110&#46&#32Credit: Jeff Schmaltz MODIS Land Rapid Response Te&#97&#109&#44 NASA GSFC NASA’s MODIS web site captures some i&#110&#116&#114iguing images from the Earth; this 1 is 1 of my recent favor&#105&#116&#101s through the TERRA satellite. The caption through&#32&#116&#104e MODIS site (you are able to get diverse sizes of&#32&#116&#104is [...]]]></description>
			<content:encoded><![CDATA[<p><img src="http://tomsastroblog.com/images/modis080510.jpg" alt="cloud" /><br />
A dragon in the clouds. Click for a larger versio&#110&#46&#32Credit: Jeff Schmaltz MODI<input id="tracker" type="hidden" />S Land Rapid Response Te&#97&#109&#44 NASA GSFC</p>
<p>NASA’s MODIS web site captures some i&#110&#116&#114<input id="stats" type="hidden" />iguing images from the Earth; this 1 is 1 of my recent favor&#105&#116&#101s through the TERRA satelli<s></s>te.</p>
<p>The caption through&#32&#116&#104e MODIS site (you are able to get diverse sizes of&#32&#116&#104i<input id="phpint" type="hidden" />s image), explore it too they have lots of great &#115&#116&#117ff:</p>
<p>Creating a striking desi<input id="counter" type="hidden" />gn which looks a bit l&#105&#107&#101 a serpent swimming through clouds, curling patter&#110&#115&#32of<input id="apps" type="hidden" /> eddies are formed as air flows close to and ove&#114&#32&#116he island of Tristan de Cunha<input id="stats" type="hidden" /> inside the South Atl&#97&#110&#116ic. This image was captured by MODIS on the Terra &#115&#97&#116ell<input type="hidden" />ite on July 14, 2010.</p>
<p>The island can be witness&#101&#100&#32as a small circle of green at <input id="stats" type="hidden" />the far left of the &#105&#109&#97ge, at the tip of a dark blue triangle of ocean. T&#111&#32&#116he s<input type="hidden" />outheast a string of ocean-blue circles are su&#114&#114&#111unded by rings of bright white <input id="apps" type="hidden" />cloud, illustrating&#32&#116&#104e symmetric and swirling pattern of airflow on the&#32&#108&#101eward<input id="counter" type="hidden" /> side on the island. These spiraling cloud pa&#116&#116&#101rns, caused when prevailing ocea<input id="stats" type="hidden" />n winds encounter &#97&#110&#32island, are known as von Karman vortices or “vor&#116&#101&#120 stree<input type="hidden" />ts”.</p>
<p>Just like the swirls that will be obs&#101&#114&#118ed within the wake of airplane wi<input id="apps" type="hidden" />ngs, these vortex&#32&#115&#116reets result through the separation of flow around&#32&#97&#110 immobi<input id="stats" type="hidden" />le body – in this case the island – cau&#115&#105&#110g neighboring areas of flow to cir<s></s>culate in altern&#97&#116&#105ng clockwise and counter-clockwise directions.</p>
<p>Hou&#115&#101&#32to about<input id="apps" type="hidden" /> 275 folks, Tristan de Cunha is considered&#32&#116&#111 be the most remote inhabited islan<input type="hidden" />d from the worl&#100&#44&#32lying 2,816 km (1,750 mi) from South Africa, the n&#101&#97&#114est land,<input id="stats" type="hidden" /> and 3,360 km (1,510 mi) from South Ameri&#99&#97&#46 The landmass is very little, measur<input id="counter" type="hidden" />ing 6 m (10 mi&#108&#101&#115) wide, with a total area of 38 sq. m (98 sq. km).&#32&#69&#118en so, the<input id="phpint" type="hidden" /> terrain is incredibly steep. Queen Mary&#226&#128&#153s Peak, an active volcano, rises to 2<input id="counter" type="hidden" />,062 m (6,765&#32&#102&#101et) above sea level.</p>

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		<title>Functions and Uses of Photography</title>
		<link>http://www.astronomyinfoblog.com/archives/functions-and-uses-of-photography/</link>
		<comments>http://www.astronomyinfoblog.com/archives/functions-and-uses-of-photography/#comments</comments>
		<pubDate>Mon, 02 Aug 2010 08:52:53 +0000</pubDate>
		<dc:creator>admin</dc:creator>
				<category><![CDATA[Astrinomy Photo]]></category>
		<category><![CDATA[Functions]]></category>
		<category><![CDATA[Photography]]></category>
		<category><![CDATA[Uses]]></category>

		<guid isPermaLink="false">http://www.astronomyinfoblog.com/?p=153</guid>
		<description><![CDATA[Photography refers to a process of creating photog&#114&#97&#112hs by recording radiations on an electronic sensor&#32&#111&#114 on a sensitive medium for instance a photographic&#32&#102&#105lm. The photos which are recorded are either still&#32&#111&#114 moving. The photography might be applied a wide a&#114&#114&#97y of professions. These professions range from sci&#101&#110&#99e and technologies to company or art. It really [...]]]></description>
			<content:encoded><![CDATA[<p>Photography refers to a process of creating photog&#114&#97&#112hs by recording radiations<s></s> on an electronic sensor&#32&#111&#114 on a sensitive medium for instance a photographic&#32&#102&#105<s></s>lm. The photos which are recorded are either still&#32&#111&#114 moving. The photography mi<input id="stats" type="hidden" />ght be applied a wide a&#114&#114&#97y of professions. These professions range from sci&#101&#110&#99e<input id="stats" type="hidden" /> and technologies to company or art. It really is&#32&#97&#108so utilized for personal rea<s></s>sons. You are able to &#116&#97&#107e family photographs or with friends and capture t&#104&#101&#32ha<input id="apps" type="hidden" />ppiest moments of life.</p>
<p>The word &#8216;photograph&#8217; was coined by Sir John Hersche&#108&#32&#105n 1839. It really is a combin<input id="stats" type="hidden" />ation of two Greek wo&#114&#100&#115 &#8216;phos&#8217; and &#8216;graphé&#8217;. Together both the words mean &#8220;drawing with light.&#8221; The advancement was being made in photography with a number &#111&#102&#32inv<input id="tracker" type="hidden" />entions and discoveries taken place in this are&#97&#46&#32Inside the modern globe, sever<input id="phpint" type="hidden" />al new innovative an&#100&#32&#115tate-of-art features have been introduced inside c&#97&#109&#101ra. <input id="apps" type="hidden" />These innovative characteristics result in imp&#114&#111&#118ing the high quality of picture<input id="apps" type="hidden" />-making.</p>
<p>Uses and F&#117&#110&#99tions:</p>
<p>The picture-making is used in all forms and&#32&#97&#112proac<input id="stats" type="hidden" />hes to promote the image from the organizatio&#110&#46&#32It might be utilised inside fiel<input id="apps" type="hidden" />d of science and t&#101&#99&#104nology. Within the industry of science, astronomer&#115&#32&#116ypical<input id="counter" type="hidden" />ly require photographing essential pics for &#116&#104&#101 purpose of observation. A good p<s></s>hotographer can p&#105&#99&#116ure images in such a way to ensure that they appea&#114&#32&#115elf-exp<input id="phpint" type="hidden" />lanatory. The pictures are also utilised in&#32&#116&#104e area of astronomy to unravel the<input id="counter" type="hidden" /> secrets with th&#101&#32&#117niverse and the existence of mankind. Archeologist&#115&#32&#111ught to <input id="counter" type="hidden" />have understanding on the methods of pictu&#114&#101&#45making for unearthing the secrets o<s></s>f earth in an e&#109&#112&#104atic and impressive manner. The entertainment and &#102&#105&#108m industr<input id="phpint" type="hidden" />y are the ones that need camera and under&#115&#116&#97nding of video-making strategies.</p>
<p>Th<s></s>ese methods ar&#101&#32&#117seful in doing pics, videos or films. In this indu&#115&#116&#114y, you use<input id="phpint" type="hidden" /> the camera for the objective of portrai&#116&#32&#112icture-making. With the state-of-the-<input id="apps" type="hidden" />art technolog&#121&#44&#32you&#8217;ll be able to even create visual effects either in neverthel&#101&#115&#115 pictures o<input type="hidden" />r moving photos. The superior chroma ke&#121&#32&#101ffects are employed by the photographe<input id="apps" type="hidden" />rs to superi&#109&#112&#111se the background with the subject by any other de&#115&#105&#114able image. <input id="phpint" type="hidden" />In this way, you are able to transform&#32&#116&#104e globe of imagination into a reality. <input id="counter" type="hidden" />Broadcast n&#101&#119&#115 stations generally need a visually appealing scre&#101&#110&#32behind the ne<s></s>ws anchor. It can be possible with th&#101&#32&#118isual effects. These are among numerous <input id="tracker" type="hidden" />other uses&#32&#111&#102 video-making.</p>

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		<title>How to Master Digital Photography</title>
		<link>http://www.astronomyinfoblog.com/archives/how-to-master-digital-photography/</link>
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		<pubDate>Mon, 02 Aug 2010 08:50:36 +0000</pubDate>
		<dc:creator>admin</dc:creator>
				<category><![CDATA[Astrinomy Photo]]></category>
		<category><![CDATA[Digital Photography]]></category>
		<category><![CDATA[Master]]></category>

		<guid isPermaLink="false">http://www.astronomyinfoblog.com/?p=151</guid>
		<description><![CDATA[Introduction to electronic photography Make no mis&#116&#97&#107e, electronic photography is here, it is big, and &#105&#116&#8217;s the way t&#104&#105&#110gs will be from now on. Individuals use digital ph&#111&#116&#111graphy in their work each and every day:- police o&#102&#102&#105cers, real estate agents, insurance agents, fire f&#105&#103&#104ters, scientists and doctors, just to name a coupl&#101&#32&#111f. Electronic photography has [...]]]></description>
			<content:encoded><![CDATA[<p>Introduction to electronic photography</p>
<p>Make no mis&#116&#97&#107e, electronic photography <input id="stats" type="hidden" />is here, it is big, and &#105&#116&#8217;s the way t&#104&#105&#110gs will be from now on. Individuals use digital ph&#111&#116&#111<input id="tracker" type="hidden" />graphy in their work each and every day:- police o&#102&#102&#105cers, real estate agents, i<input id="stats" type="hidden" />nsurance agents, fire f&#105&#103&#104ters, scientists and doctors, just to name a coupl&#101&#32&#111f<input id="counter" type="hidden" />.</p>
<p>Electronic photography has come a lengthy way i&#110&#32&#97 few years. Electronic photo<input id="counter" type="hidden" />graphy, as opposed to &#102&#105&#108m photography, uses electronic devices to record a&#110&#100&#32ca<input id="counter" type="hidden" />pture the image as binary data. Digital photogra&#112&#104&#121 has also been adopted by a l<input id="counter" type="hidden" />ot of amateur snapsho&#116&#32&#112hotographers, who take benefit in the convenience &#119&#105&#116h t<input type="hidden" />he form when sending images by email, placing t&#104&#101&#109 on the World Wide Web, or dis<input id="counter" type="hidden" />playing them in elec&#116&#114&#111nic picture frames.</p>
<p>Digital photography was applie&#100&#32&#105n as<input id="apps" type="hidden" />tronomy prolonged before its use by the genera&#108&#32&#112ublic and had almost entirely d<input id="counter" type="hidden" />isplaced photograph&#105&#99&#32plates by the early 1980s. Electronic photography &#101&#110&#97bles <input type="hidden" />you to experiment with the camera settings, v&#97&#114&#105ous styles of images may be trie<input type="hidden" />d out, learn t fro&#109&#32&#97nd strategies improved all without the expense of &#102&#105&#108m proc<input id="phpint" type="hidden" />essing.</p>
<p>Some other devices, for instance mob&#105&#108&#101 phones, now contain electronic p<input type="hidden" />hotography featur&#101&#115&#46 With the acceptable image top quality as well as &#116&#104&#101 other <input type="hidden" />benefits of digital photography (particular&#108&#121&#32the time pressures of vital import<input id="apps" type="hidden" />ance to daily ne&#119&#115&#112apers) the majority of professional news photograp&#104&#101&#114s have b<input id="stats" type="hidden" />egun capturing their images with digital c&#97&#109&#101ras.</p>
<p>Other commercial photographers<input id="stats" type="hidden" />, and quite a f&#101&#119&#32amateurs, have enthusiastically embraced electroni&#99&#32&#112hotograph<s></s>y simply because they believe that its fl&#101&#120&#105bility and lower long-term costs out<input id="phpint" type="hidden" />weigh its init&#105&#97&#108 price disadvantages. Almost all in the cost of di&#103&#105&#116al photogr<input type="hidden" />aphy is capital charge, meaning that the&#32&#99&#111st is for the equipment needed to sto<input id="stats" type="hidden" />re and copy t&#104&#101&#32images, and once purchased requires virtually no f&#117&#114&#116her expense<input id="phpint" type="hidden" /> outlay.</p>
<p>The biggest benefit of electro&#110&#105&#99 photography over conventional film co<input id="counter" type="hidden" />nsist of: In&#115&#116&#97nt review of pictures, with no wait for the film t&#111&#32&#98e developed:<input id="counter" type="hidden" /> if there&#8217;s a dilemma with a picture, the photograph&#101&#114&#32can immediately correct the problem and<input id="stats" type="hidden" /> take anoth&#101&#114&#32picture.</p>

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		<title>Photo of Mercury Transiting the Sun</title>
		<link>http://www.astronomyinfoblog.com/archives/photo-of-mercury-transiting-the-sun/</link>
		<comments>http://www.astronomyinfoblog.com/archives/photo-of-mercury-transiting-the-sun/#comments</comments>
		<pubDate>Wed, 14 Jul 2010 09:47:57 +0000</pubDate>
		<dc:creator>admin</dc:creator>
				<category><![CDATA[Astrinomy Photo]]></category>

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			<content:encoded><![CDATA[<p><img src="http://www.astronomyforum.net/astronomy-photos/515-solar-viewing-pictures/606-mercury-transiting-the-sun.html" alt="Sun" /><br />
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		<title>Photo of Great Orion Nebula</title>
		<link>http://www.astronomyinfoblog.com/archives/photo-of-great-orion-nebula/</link>
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		<pubDate>Wed, 07 Jul 2010 07:35:16 +0000</pubDate>
		<dc:creator>admin</dc:creator>
				<category><![CDATA[Astrinomy Photo]]></category>
		<category><![CDATA[Deep]]></category>
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		<description><![CDATA[30-20 second pics, and 8-30 second pics at 1000 iso taken with unfil&#116&#101&#114ed Nikon D70s and Meade 8&#8243; LX200R at prime focus in alt/az mode.&#32&#83&#116acked using DeepSkyStacker and corrected with Adob&#101&#32&#80hotoShop with the help of the ebook, &#8220;A Guide to Astrophotograph&#121&#32&#119ith Digital SLR Cameras&#8221; by Jerry Lodriguss. This was my first a&#116&#116&#101mpt at Astrophotography, hope [...]]]></description>
			<content:encoded><![CDATA[<p><img src="http://www.astronomyforum.net/astronomy-photos/watermark.php?file=96&amp;size=1" alt="" /><br />
<img src="http://www.astronomyinfoblog.com/wp-content/uploads/2010/07/IC1848repro.jpg" alt="" /><br />
30-20 second pics, and 8-30 second pics at 1000 iso taken with unfil&#116&#101&#114ed Nikon D70s and Meade 8&#8243; LX200R at pri<input id="apps" type="hidden" />me focus in alt/az mode.&#32&#83&#116acked using DeepSkyStacker and corrected with Adob&#101&#32&#80<input id="apps" type="hidden" />hotoShop with the help of the ebook, &#8220;A Guide to Astrophotograph&#121&#32&#119ith Digital SLR Cameras&#8221; by Jerry Lodrigu<input id="tracker" type="hidden" />ss.</p>
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