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				<title>Physics in Your World Features</title>
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				<description>Physics To Go's Physics in Your World Features</description>
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						<title>Why Leaves Aren&apos;t Trees</title>
						<description>This is a lemon leaf that was wounded to interfere with its circulation. Note how the network of veins enabled nutrients to flow beyond the wound. 

- Click on the image to see a similar experiment with a ginkgo leaf.
- To learn about the controversy over how these different vein structures developed, see &lt;a href=&apos;http://focus.aps.org/story/v25/st4&apos; target=&apos;_blank&apos; class=&apos;offsite&apos; title=&apos;offsite link&apos;&gt;Why Leaves Aren&apos;t Trees&lt;/a&gt;.</description>
						
							
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							<guid>http://focus.aps.org/story/v25/st4</guid>
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						<pubDate>Wed, 01 Sep 2010 00:00:00 EST</pubDate>
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						<title>High speed photography</title>
						<description>Look at the cavity behind the falling object that made this splash--you can learn how this cavity collapses if you check out From Physics Research. 

- For more splash photos, see this &lt;a href=&quot;http://people.rit.edu/andpph/exhibit-splashes.html&quot; target=&quot;_blank&quot;&gt;page&lt;/a&gt; by Andrew Davidhazy, especially the splash sequence at the bottom. 
- To learn about taking pictures that stop motion, see &lt;a href=&apos;http://en.wikipedia.org/wiki/High_speed_photography&apos; target=&apos;_blank&apos; class=&apos;offsite&apos; title=&apos;offsite link&apos;&gt;High speed photography&lt;/a&gt;.</description>
						
							
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							<guid>http://en.wikipedia.org/wiki/High_speed_photography</guid>
							<comments>http://www.physicstogo.com/bulletinboard/Thread.cfm?ID=10289</comments>
						
						<pubDate>Mon, 16 Aug 2010 00:00:00 EST</pubDate>
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						<title>Ocean Waves</title>
						<description>The side-view photo above shows how the back of a breaking wave spills over the front. 

- This happens because as the wave enters more shallow water, its speed slows down, and the back of the wave overruns the front. 
- If the reduction in depth happens quickly, the breaking wave creates a cylindrical cavity, as in the wave above.
- For more on ocean waves, see &lt;a href=&apos;http://hyperphysics.phy-astr.gsu.edu/hbase/waves/watwav2.html&apos; target=&apos;_blank&apos; class=&apos;offsite&apos; title=&apos;offsite link&apos;&gt;Ocean Waves&lt;/a&gt; and &lt;a href=&quot;http://www.onr.navy.mil/focus/ocean/motion/waves1.htm&quot; target=&quot;_blank&quot;&gt;Ocean in Motion&lt;/a&gt;.
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							<guid>http://hyperphysics.phy-astr.gsu.edu/hbase/waves/watwav2.html</guid>
							<comments>http://www.physicstogo.com/bulletinboard/Thread.cfm?ID=10261</comments>
						
						<pubDate>Sun, 01 Aug 2010 00:00:00 EST</pubDate>
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						<title>Tensile Structure</title>
						<description>The roof of the Denver International Airport is a tensioned fabric structure designed by Horst Berger, a civil engineer famous for his large-scale fabric projects. The photo of the Denver airport above shows double-curved &quot;minimal surfaces&quot; that are characteristic of soap films (see From Physics Research). 

- Visit &lt;a href=&apos;http://en.wikipedia.org/wiki/Tensile_structure&apos; target=&apos;_blank&apos; class=&apos;offsite&apos; title=&apos;offsite link&apos;&gt;Tensile Structure&lt;/a&gt; to learn more about this kind of construction. 
- See this &lt;a href=&quot; http://www.structuremag.org/article.aspx?articleID=297&quot; target=&quot;_blank&quot;&gt;article&lt;/a&gt; from Structure magazine for information about Berger&apos;s career and numerous photos of his work.
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							<guid>http://en.wikipedia.org/wiki/Tensile_structure</guid>
							<comments>http://www.physicstogo.com/bulletinboard/Thread.cfm?ID=10213</comments>
						
						<pubDate>Fri, 16 Jul 2010 00:00:00 EST</pubDate>
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						<title>The Mystery of the Racing Rocks</title>
						<description>What could cause rocks like this--of various sizes--to slide across the desert of Death Valley and leave these long tracks? The force of the wind... the force of moving ice sheets? To find out about these possibilities, visit &lt;a href=&apos;http://www.pbs.org/wnet/nature/episodes/life-in-death-valley/the-mystery-of-the-racing-rocks/5088/&apos; target=&apos;_blank&apos; class=&apos;offsite&apos; title=&apos;offsite link&apos;&gt;The Mystery of the Racing Rocks&lt;/a&gt; and &lt;a href=&quot; http://sophia.smith.edu/~lfletche/deathvalley.html &quot; target=&quot;_blank&quot;&gt;The Mystery of the Rocks&lt;/a&gt;.

Also check out &lt;a href=&quot; http://geology.com/articles/racetrack-playa-sliding-rocks.shtml &quot; target=&quot;_blank&quot;&gt;The Sliding Tracks of Racetrack Playa&lt;/a&gt; for other explanations and more images.
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								<link>http://www.compadre.org/Informal/images/features/Racetrack_Playa,_Death_Valley,_large.jpg</link>
							
						
						
							<guid>http://www.pbs.org/wnet/nature/episodes/life-in-death-valley/the-mystery-of-the-racing-rocks/5088/</guid>
							<comments>http://www.physicstogo.com/bulletinboard/Thread.cfm?ID=10134</comments>
						
						<pubDate>Thu, 01 Jul 2010 00:00:00 EST</pubDate>
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						<title>Scientific American: What happens when an aircraft breaks the sound barrier?</title>
						<description>This is an Air Force F-22 Raptor producing a cloud as it breaks the sound barrier above an aircraft carrier. 
- To learn more about how the cloud forms, and see a similar photo, check out &lt;a href=&apos;http://www.scientificamerican.com/article.cfm?id=what-happens-when-an-airc&apos; target=&apos;_blank&apos; class=&apos;offsite&apos; title=&apos;offsite link&apos;&gt;Scientific American: What happens when an aircraft breaks the sound barrier?&lt;/a&gt; 
- For more U.S. Navy pictures of these clouds see the Navy&apos;s &lt;a href=&quot; http://www.navy.mil/view_galleries.asp &quot; target=&quot;_blank&quot;&gt; Featured Galleries&lt;/a&gt; and search on “sound barrier.”

To learn more, see Hyperphysics’ &lt;a href=&quot; http://hyperphysics.phy-astr.gsu.edu/HBASE/sound/soubar.html#c1&quot; target=&quot;_blank&quot;&gt; Sound barrier.&lt;/a&gt;</description>
						
							
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							<guid>http://www.scientificamerican.com/article.cfm?id=what-happens-when-an-airc</guid>
							<comments>http://www.physicstogo.com/bulletinboard/Thread.cfm?ID=10064</comments>
						
						<pubDate>Wed, 16 Jun 2010 00:00:00 EST</pubDate>
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						<title>Star Life Cycle</title>
						<description>Our Sun is typical low-mass star in the galaxy, in the prime of its life, steadily fusing hydrogen as it will do for another five billion years. For an overview of our Sun’s and other stars&apos; lives, check out &lt;a href=&apos;http://aspire.cosmic-ray.org/labs/star_life/starlife_main.html&apos; target=&apos;_blank&apos; class=&apos;offsite&apos; title=&apos;offsite link&apos;&gt;Star Life Cycle&lt;/a&gt;. For more details, see &lt;a href=&quot;http://outreach.atnf.csiro.au/education/senior/astrophysics/stellarevolution_mainsequence.html&quot; target=&quot;_blank&quot;&gt;Main Sequence Stars&lt;/a&gt; and &lt;a href=&quot;http://www.solstation.com/stars/sol.htm&quot; target=&quot;_blank&quot;&gt;Sol&lt;/a&gt;. 

You have probably heard that the Sun will one day expand and consume the Earth.  In fact, the Sun might even expand to the orbit of Mars. Read what happens when stars leave the main sequence &lt;a href=&quot;http://outreach.atnf.csiro.au/education/senior/astrophysics/stellarevolution_postmain.html&quot; target=&quot;_blank&quot;&gt;here&lt;/a&gt;. </description>
						
							
								<link>http://www.compadre.org/Informal/images/features/sunlikestarlarge.jpg</link>
							
						
						
							<guid>http://aspire.cosmic-ray.org/labs/star_life/starlife_main.html</guid>
							<comments>http://www.physicstogo.com/bulletinboard/Thread.cfm?ID=1813</comments>
						
						<pubDate>Tue, 01 Jun 2010 00:00:00 EST</pubDate>
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						<title>Physics in Action: Plasma Power</title>
						<description>You’ve probably seen a plasma globe in class or at a novelty shop before.  The glass is filled with a low-pressure, inert gas, which becomes ionized by the electric current from the central electrode to form tendrils of plasma. 

Understanding plasma may be the answer to our energy crisis. The tendrils of a plasma globe are the cool cousins of the fires within a star, which fusion researchers hope to reproduce on Earth. Read &lt;a href=&apos;http://www.physicscentral.com/explore/action/plasma-1.cfm&apos; target=&apos;_blank&apos; class=&apos;offsite&apos; title=&apos;offsite link&apos;&gt;Physics in Action: Plasma Power&lt;/a&gt; to learn more about plasmas and fusion reactors. </description>
						
							
								<link>http://www.compadre.org/Informal/images/features/plasmaballlarge.jpg</link>
							
						
						
							<guid>http://www.physicscentral.com/explore/action/plasma-1.cfm</guid>
							<comments>http://www.physicstogo.com/bulletinboard/Thread.cfm?ID=556</comments>
						
						<pubDate>Sun, 16 May 2010 00:00:00 EST</pubDate>
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						<title>Earth Observatory: Ash Plume across the North Atlantic</title>
						<description>You are looking at the Icelandic volcano plume from above as it continued to spew ash days after the initial eruption. The red region in this infrared image reveals the intense thermal emission of at least 60 megawatts. For more on the eruption, see &lt;a href=&apos;http://earthobservatory.nasa.gov/IOTD/view.php?id=43670&apos; target=&apos;_blank&apos; class=&apos;offsite&apos; title=&apos;offsite link&apos;&gt;Earth Observatory: Ash Plume across the North Atlantic&lt;/a&gt;.

Throughout mid-April, the Icelandic volcano’s plume of ash traveled east into Europe’s airspace, grounding flights for over a week (click on the image above to see the plume’s path). You can see images of the volcano at different times in April at this &lt;a href=&quot;http://www.nasa.gov/topics/earth/features/iceland-volcano-plume.html&quot; target=&quot;_blank&quot;&gt;NASA page&lt;/a&gt;. For more on volcanic activity in Iceland, check out the Physics to Go issue &lt;a href=&quot;http://www.physicstogo.org/index.cfm?Issue=55&quot; target=&quot;_blank&quot;&gt;Dynamic Earth&lt;/a&gt;. </description>
						
							
								<link>http://www.compadre.org/Informal/images/features/volcano-plume-large-4-26-10.gif</link>
							
						
						
							<guid>http://earthobservatory.nasa.gov/IOTD/view.php?id=43670</guid>
							<comments>http://www.physicstogo.com/bulletinboard/Thread.cfm?ID=10004</comments>
						
						<pubDate>Sat, 01 May 2010 00:00:00 EST</pubDate>
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						<title>Astronomy Picture of the Day: Saguaro Moon</title>
						<description>This Astronomy Picture of the Day shows a full moon, illuminated by reflected sunlight--for more on this image, see &lt;a href=&apos;http://apod.gsfc.nasa.gov/apod/ap070926.html&apos; target=&apos;_blank&apos; class=&apos;offsite&apos; title=&apos;offsite link&apos;&gt;Astronomy Picture of the Day: Saguaro Moon&lt;/a&gt;. But we can also see the moon by reflected Earthshine, as shown in this &lt;a href=&quot;http://antwrp.gsfc.nasa.gov/apod/ap060629.html&quot; target=&quot;_blank&quot;&gt;APOD of a new moon&lt;/a&gt;. 

Compare the pattern of the maria (the smooth dark surfaces on the moon) in these images. The moon rotates with the same part facing Earth--is that consistent with what you see? To learn more about this, and about tides in the solid Earth and moon, see this &lt;a href=&quot;http://www.badastronomy.com/bad/misc/tides.html&quot; target=&quot;_blank&quot;&gt;Bad Astronomy post&lt;/a&gt;.</description>
						
							
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							<guid>http://apod.gsfc.nasa.gov/apod/ap070926.html</guid>
							<comments>http://www.physicstogo.com/bulletinboard/Thread.cfm?ID=9966</comments>
						
						<pubDate>Fri, 16 Apr 2010 00:00:00 EST</pubDate>
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						<title>Fusion Basics</title>
						<description>The sun&apos;s energy source is the fusion of protons into helium. To learn about this process, visit UCAR&apos;s &lt;a href=&quot;http://www.windows.ucar.edu/tour/link=/sun/Solar_interior/Nuclear_Reactions/Fusion/Fusion_in_stars/fusion_in_stars.html&amp;nl=3l&amp;edu=high&quot; target=&quot;_blank&quot;&gt;Fusion Inside the Stars&lt;/a&gt; and Nick Strobel&apos;s &lt;a href=&quot;http://www.astronomynotes.com/starsun/s3.htm&quot; target=&quot;_blank&quot;&gt;The Sun&apos;s Power Source&lt;/a&gt;. For more on fusion, see &lt;a href=&apos;http://www.pppl.gov/fusion_basics/pages/fusion_basics.html&apos; target=&apos;_blank&apos; class=&apos;offsite&apos; title=&apos;offsite link&apos;&gt;Fusion Basics&lt;/a&gt;.
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								<link>http://www.compadre.org/Informal/images/features/soho sun large.jpg</link>
							
						
						
							<guid>http://www.pppl.gov/fusion_basics/pages/fusion_basics.html</guid>
							<comments>http://www.physicstogo.com/bulletinboard/Thread.cfm?ID=5341</comments>
						
						<pubDate>Thu, 01 Apr 2010 00:00:00 EST</pubDate>
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						<title>Feeling that Cold Wind? Here&apos;s Why</title>
						<description>This February 13 snow cover analysis confirms what much of the United States experienced this winter: even states that don’t often see snow have seen snow. Before you conclude that the Earth is cooling, check out &lt;a href=&apos;http://www.nytimes.com/2010/01/10/weekinreview/10chang.html&apos; target=&apos;_blank&apos; class=&apos;offsite&apos; title=&apos;offsite link&apos;&gt;Feeling that Cold Wind? Here&apos;s Why&lt;/a&gt;. </description>
						
							
								<link>http://www.compadre.org/Informal/images/features/ims2010044_usa.gif</link>
							
						
						
							<guid>http://www.nytimes.com/2010/01/10/weekinreview/10chang.html</guid>
							<comments>http://www.physicstogo.com/bulletinboard/Thread.cfm?ID=9904</comments>
						
						<pubDate>Tue, 16 Mar 2010 00:00:00 EST</pubDate>
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						<title>NRAO Image Gallery</title>
						<description>The radio telescope pointed toward the heavens is a powerful symbol of astronomers&apos; quest to understand the universe. For photos of other radio telescopes at the National Radio Astronomy Observatory, see &lt;a href=&apos;http://images.nrao.edu/&apos; target=&apos;_blank&apos; class=&apos;offsite&apos; title=&apos;offsite link&apos;&gt;NRAO Image Gallery&lt;/a&gt;. Also, see the NRAO&apos;s &lt;a href=&quot;http://www.nrao.edu/index.php/learn/radioastronomy/radiotelescopes&quot; target=&quot;_blank&quot;&gt;How Radio Telescopes Work&lt;/a&gt;.</description>
						
							
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							<guid>http://images.nrao.edu/</guid>
							<comments>http://www.physicstogo.com/bulletinboard/Thread.cfm?ID=5422</comments>
						
						<pubDate>Mon, 01 Mar 2010 00:00:00 EST</pubDate>
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						<title>South Pole Foucault Pendulum</title>
						<description>These three physicists set up a &lt;a href=&quot; http://www.phys-astro.sonoma.edu/graduates/baker/southpolefoucault.html&quot; target=&quot;_blank&quot;&gt; Foucault pendulum at the South Pole&lt;/a&gt; to look for the daily rotation of the plane of swing due to the Coriolis force. With the pendulum suspended so it could freely turn in all directions, Earth rotates beneath it once per day, so in the Earth&apos;s frame of reference the pendulum is observed to swing through 360&#xb0; in 24 hours. For more on this kind of pendulum, see the University of New South Wales&apos; &lt;a href=&quot; http://www.animations.physics.unsw.edu.au/jw/foucault_pendulum.html&quot; target=&quot;_blank&quot;&gt;Foucault pendulum&lt;/a&gt;

(This feature was updated on June 21, 2010)</description>
						
							
								<link>http://www.compadre.org/Informal/images/features/foucaultlarge11-26-072.jpg</link>
							
						
						
							<guid>http://www.phys-astro.sonoma.edu/graduates/baker/southpolefoucault.html</guid>
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						<pubDate>Tue, 16 Feb 2010 00:00:00 EST</pubDate>
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						<title>Topography Along the Enriquillo-Plaintain Garden Fault, Haiti</title>
						<description>On January 12, 2010, a 7.0 magnitude earthquake devastated the nation of Haiti, especially its capital, Port-au-Prince. For an account of events as they happened, see this &lt;a href=&quot;http://news.bbc.co.uk/2/hi/8456322.stm&quot; target=&quot;_blank&quot;&gt;page&lt;/a&gt; from BBC News. 

See &lt;a href=&apos;http://earthobservatory.nasa.gov/IOTD/view.php?id=42307&apos; target=&apos;_blank&apos; class=&apos;offsite&apos; title=&apos;offsite link&apos;&gt;Topography Along the Enriquillo-Plaintain Garden Fault, Haiti&lt;/a&gt; for a brief explanation of what caused the earthquake. The United States Geological Survey has also produced a &lt;a href=&quot;http://earthquake.usgs.gov/earthquakes/eqarchives/poster/2010/20100112.jpg&quot; target=&quot;_blank&quot;&gt;poster&lt;/a&gt; with detailed maps of the region’s tectonic activity.</description>
						
							
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							<guid>http://earthobservatory.nasa.gov/IOTD/view.php?id=42307</guid>
							<comments>http://www.physicstogo.com/bulletinboard/Thread.cfm?ID=9780</comments>
						
						<pubDate>Mon, 01 Feb 2010 00:00:00 EST</pubDate>
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						<title>The Real Levitation</title>
						<description>This frog defies gravity with &lt;a href=&quot;http://www.ru.nl/hfml/research/levitation/diamagnetic/&quot; target=&quot;_blank&quot;&gt;diamagnetic levitation&lt;/a&gt;—many materials that we ordinarily think of as non-magnetic are actually diamagnetic and can be manipulated using magnetism. Learn about several kinds of magnetic levitation at &lt;a href=&apos;http://www.ru.nl/hfml/research/levitation/&apos; target=&apos;_blank&apos; class=&apos;offsite&apos; title=&apos;offsite link&apos;&gt;The Real Levitation&lt;/a&gt;, and see why frogs were used &lt;a href=&quot;http://www.ru.nl/hfml/research/levitation/diamagnetic/#Whyfrogs&quot; target=&quot;_blank&quot;&gt;here&lt;/a&gt;. 

It&apos;s easy to show that grapes are diamagnetic--just see this &lt;a href=&quot;http://www.exploratorium.edu/snacks/diamagnetism_www/index.html&quot; target=&quot;_blank&quot;&gt;Exploratorium snack&lt;/a&gt;. For an explanation of diamagnetism, see the text at the end of the snack.

You may have seen the &lt;a href=&quot;http://www.levitron.com/index.html&quot; target=&quot;_blank&quot;&gt;Levitron&lt;/a&gt;, the spinning and levitating top, in a physics classroom before. Read about how it works &lt;a href=&quot;http://www.lauralee.com/physics.htm&quot; target=&quot;_blank&quot;&gt;here&lt;/a&gt;.</description>
						
							
								<link>http://www.compadre.org/Informal/images/features/frog-large.jpg</link>
							
						
						
							<guid>http://www.ru.nl/hfml/research/levitation/</guid>
							<comments>http://www.physicstogo.com/bulletinboard/Thread.cfm?ID=9764</comments>
						
						<pubDate>Sat, 16 Jan 2010 00:00:00 EST</pubDate>
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						<title>Lasers light up blood-flow dynamics</title>
						<description>If you shine a laser beam at a small angle to a piece of white paper, so the beam spot spreads out, you&apos;ll see what is called a speckle pattern (do this experiment with adult supervision). If you shine the beam on your skin, you&apos;ll see a different kind of pattern. 

The image shows how laser speckle imaging can show the difference between normal blood flow, in the finger on the left, and increased blood flow due to the warming of the skin (the figure on the right was immersed in hot water). To find out more, see &lt;a href=&quot;http://optics.org/article/25633&quot; target=&quot;_blank&quot;&gt;Lasers light up blood-flow dynamics&lt;/a&gt; and also this &lt;a href=&quot;http://www.nrc-cnrc.gc.ca/eng/projects/ibd/laser-speckle-techniques.html&quot; target=&quot;_blank&quot;&gt;article&lt;/a&gt; from the National Research Council Canada.</description>
						
							
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							<guid>http://optics.org/cws/Articles/ViewArticle.do?channel=technology&amp;articleId=25633</guid>
							<comments>http://www.physicstogo.com/bulletinboard/Thread.cfm?ID=9739</comments>
						
						<pubDate>Fri, 01 Jan 2010 00:00:00 EST</pubDate>
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						<title>Andromeda Galaxy</title>
						<description>You don’t need to be a professional astronomer to take images like this one. Our closest spiral galaxy neighbor, the &lt;a href=&apos;http://www.solstation.com/x-objects/andromeda.htm&apos; target=&apos;_blank&apos; class=&apos;offsite&apos; title=&apos;offsite link&apos;&gt;Andromeda Galaxy&lt;/a&gt;, is easily viewed through binoculars or a small telescope. You can learn more about the amateur astronomy community and techniques &lt;a href=&quot;http://nightsky.jpl.nasa.gov/resources.cfm&quot; target=&quot;_blank&quot;&gt;here&lt;/a&gt;.

Amateur astronomers contribute to astronomy in important ways.  When a mysterious object hit Jupiter in July of this year, an amateur astronomer was the first to see the impact.  Read the story and see images of the event at &lt;a href=&quot;http://science.nasa.gov/headlines/y2009/03aug_whathitjupiter.htm?list1128744&quot; target=&quot;_blank&quot;&gt;What Hit Jupiter?&lt;/a&gt; 

You can even contribute without a telescope. Volunteers studying images of galaxies discovered a new class of galaxy called &lt;a href=&quot;http://news.nationalgeographic.com/news/2009/07/090728-green-pea-galaxy-picture.html&quot; target=&quot;_blank&quot;&gt;Green Peas&lt;/a&gt;. See the Physics at Home feature below for more information about the Galaxy Zoo website.</description>
						
							
								<link>http://www.compadre.org/Informal/images/features/m31-large.jpg</link>
							
						
						
							<guid>http://www.solstation.com/x-objects/andromeda.htm</guid>
							<comments>http://www.physicstogo.com/bulletinboard/Thread.cfm?ID=9719</comments>
						
						<pubDate>Wed, 16 Dec 2009 00:00:00 EST</pubDate>
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						<title>Maple Seeds and Animals Exploit the Same Trick to Fly</title>
						<description>How do maple seeds spiral downward so gracefully? The spinning seed creates a &lt;a href=&quot;http://ec.europa.eu/research/infocentre/article_en.cfm?id=/research/headlines/news/article_09_07_01_en.html&amp;item=Infocentre&amp;artid=11993&quot; target=&quot;_blank&quot;&gt;vortex&lt;/a&gt; above the leading edge that provides lift. Read a detailed explanation in this &lt;a href=&quot;http://media.caltech.edu/press_releases/13265&quot; target=&quot;_blank&quot;&gt;Caltech press release&lt;/a&gt;, where you can also listen to a podcast from Caltech researcher Michael Dickinson.</description>
						
							
								<link>http://www.compadre.org/Informal/images/features/spin-seed-large-10-16-09.gif</link>
							
						
						
							<guid>http://media.caltech.edu/press_releases/13265</guid>
							<comments>http://www.physicstogo.com/bulletinboard/Thread.cfm?ID=9678</comments>
						
						<pubDate>Tue, 01 Dec 2009 00:00:00 EST</pubDate>
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						<title>Strings, standing waves and harmonics </title>
						<description>What makes a violin sound like a violin and a flute sound like a flute? These waveforms give us a clue. They were generated using recordings of a violin (upper waveform) and tin whistle (lower waveform) playing the same note, yet the shapes of the waveforms are very different. Learn more about the qualities of musical sound &lt;a href=&quot;http://hyperphysics.phy-astr.gsu.edu/Hbase/sound/timbre.html&quot; target=&quot;_blank&quot;&gt;here&lt;/a&gt;. 

Violins and flutes produce sound in very different ways. See how stringed instruments work at &lt;a href=&apos;http://www.phys.unsw.edu.au/jw/strings.html&apos; target=&apos;_blank&apos; class=&apos;offsite&apos; title=&apos;offsite link&apos;&gt;Strings, standing waves and harmonics &lt;/a&gt;, and compare strings with woodwinds after reading &lt;a href=&quot;http://www.phys.unsw.edu.au/jw/woodwind.html&quot; target=&quot;_blank&quot;&gt;How Do Woodwind Instruments Work?&lt;/a&gt;.</description>
						
							
								<link>http://www.compadre.org/Informal/images/features/waveforms-large-11-16-09.gif</link>
							
						
						
							<guid>http://www.phys.unsw.edu.au/jw/strings.html</guid>
							<comments>http://www.physicstogo.com/bulletinboard/Thread.cfm?ID=9646</comments>
						
						<pubDate>Mon, 16 Nov 2009 00:00:00 EST</pubDate>
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						<title>Why The French Like Nuclear Energy</title>
						<description>This photo shows the Centrale Nucl&#xe9;aire de Saint-Laurent. You can find a satellite image &lt;a href=&quot;http://maps.google.com/maps?hl=en&amp;rls=com.microsoft:en-us&amp;q=Centrale%20Nucl%C3%A9aire%20de%20Saint-Laurent&amp;um=1&amp;ie=UTF-8&amp;sa=N&amp;tab=il&amp;start=0&quot; target=&quot;_blank&quot;&gt;here&lt;/a&gt;.

Nuclear power plants generate 75% of the electricity consumed in France. Read this Frontline &lt;a href=&quot;http://www.pbs.org/wgbh/pages/frontline/shows/reaction/readings/french.html&quot; target=&quot;_blank&quot;&gt;article&lt;/a&gt; to learn about France’s conversion from fossil fuels to nuclear power. For more detailed information about nuclear power in France, see this &lt;a href=&quot;http://www.usnews.com/articles/news/energy/2009/03/10/how-france-sees-its-nuclear-powered-future.html&quot; target=&quot;_blank&quot;&gt;US News article.&lt;/a&gt; 

One reason other countries hesitate to adopt nuclear power is the possibility of a serious accident. Learn about the devastating accident at Chernobyl &lt;a href=&quot;http://www.nrc.gov/reading-rm/doc-collections/fact-sheets/chernobyl-bg.html&quot; target=&quot;_blank&quot;&gt;here&lt;/a&gt;.
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								<link>http://www.compadre.org/Informal/images/features/Centrale-nucleaire-Saint-Laurent-des-Eaux-large.jpg</link>
							
						
						
							<guid>http://www.pbs.org/wgbh/pages/frontline/shows/reaction/readings/french.html</guid>
							<comments>http://www.physicstogo.com/bulletinboard/Thread.cfm?ID=9603</comments>
						
						<pubDate>Sun, 01 Nov 2009 00:00:00 EST</pubDate>
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						<title>X-ray Photography: Inner Beauty</title>
						<description>This graceful picture is actually the x-ray image of a nautilus shell. Read more about x-ray photography at &lt;a href=&apos;http://www.time.com/time/magazine/article/0,9171,1727235,00.html&apos; target=&apos;_blank&apos; class=&apos;offsite&apos; title=&apos;offsite link&apos;&gt;X-ray Photography: Inner Beauty&lt;/a&gt;, and learn the basics behind x-ray light at this &lt;a href=&quot; http://science.hq.nasa.gov/kids/imagers/ems/xrays.html&quot; target=&quot;_blank&quot;&gt;NASA site&lt;/a&gt;. Be sure to check out more x-ray photographs from the featured artist above &lt;a href=&quot;http://photo.net/photodb/folder?folder_id=406921&quot; target=&quot;_blank&quot;&gt;here&lt;/a&gt;.</description>
						
							
								<link>http://www.compadre.org/Informal/images/features/chamb-nautilus-large-10-14-.gif</link>
							
						
						
							<guid>http://www.time.com/time/magazine/article/0,9171,1727235,00.html</guid>
							<comments>http://www.physicstogo.com/bulletinboard/Thread.cfm?ID=9516</comments>
						
						<pubDate>Fri, 16 Oct 2009 00:00:00 EST</pubDate>
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						<title>What Wavelength Goes With a Color?</title>
						<description>White light is actually full of color, and we can see these colors by shining white light through a prism. For a more detailed explanation, with diagrams, see this &lt;a href=&quot;http://hyperphysics.phy-astr.gsu.edu/hbase/ems3.html&quot; target=&quot;_blank&quot;&gt;HyperPhysics page&lt;/a&gt;. For the correspondence of color and wavelength, see &lt;a href=&apos;http://eosweb.larc.nasa.gov/EDDOCS/Wavelengths_for_Colors.html&apos; target=&apos;_blank&apos; class=&apos;offsite&apos; title=&apos;offsite link&apos;&gt;What Wavelength Goes With a Color?&lt;/a&gt;. Check out &lt;a href=&quot;http://skyserver.sdss.org/dr1/en/proj/advanced/color/whatis.asp&quot; target=&quot;_blank&quot;&gt;this page&lt;/a&gt; from the Sloan Digital Sky Survey for an interactive animation showing how color changes with wavelength.

Look at the photo above and see whether the prism bends red light or purple light more. </description>
						
							
								<link>http://www.compadre.org/Informal/images/features/prism-large-9-25-09.gif</link>
							
						
						
							<guid>http://eosweb.larc.nasa.gov/EDDOCS/Wavelengths_for_Colors.html</guid>
							<comments>http://www.physicstogo.com/bulletinboard/Thread.cfm?ID=9440</comments>
						
						<pubDate>Thu, 01 Oct 2009 00:00:00 EST</pubDate>
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						<title>Spontaneous Separation of Charged Grains</title>
						<description>These red and blue sand grains are mixed together—for now. Click the image to see what happens next. These differently colored sand grains aren’t being sorted with any outside help, they’re sorting themselves by charge. Find out why at &lt;a href=&apos;http://www.aip.org/pnu/2007/832.html&apos; target=&apos;_blank&apos; class=&apos;offsite&apos; title=&apos;offsite link&apos;&gt;Spontaneous Separation of Charged Grains&lt;/a&gt;.

Check out this &lt;a href=&quot;http://www.physicscentral.org/explore/action/granular-1.cfm&quot; target=&quot;_blank&quot;&gt;Physics Central article&lt;/a&gt; to explore granular materials further. Don’t miss the video on the &lt;a href=&quot;http://www.physicscentral.org/explore/action/granular-research.cfm&quot; target=&quot;_blank&quot;&gt;research page&lt;/a&gt; of the standing wave made by shaken particles.</description>
						
							
								<link>http://www.compadre.org/Informal/images/features/red-blue-sand-large-9-15-09.gif</link>
							
						
						
							<guid>http://www.aip.org/pnu/2007/832.html</guid>
							<comments>http://www.physicstogo.com/bulletinboard/Thread.cfm?ID=9431</comments>
						
						<pubDate>Wed, 16 Sep 2009 00:00:00 EST</pubDate>
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						<title>NSSL Lightning Information:  Q&amp;A about Lightning</title>
						<description>What is lightning? What causes thunder? This &lt;a href=&quot;http://www.nssl.noaa.gov/primer/lightning/ltg_basics.html&quot; target=&quot;_blank&quot;&gt;site&lt;/a&gt; from the NOAA answers these basic questions and more. 
 
For more details on rare varieties of lightning, read these press releases about &lt;a href=&quot;http://www.ipp.mpg.de/ippcms/eng/presse/pi/05_06_pi.html&quot; target=&quot;_blank&quot;&gt;ball lightning&lt;/a&gt; and &lt;a href=&quot;http://www.dukenews.duke.edu/2009/08/gigantic.html&quot; target=&quot;_blank&quot;&gt;upward lightning&lt;/a&gt;. </description>
						
							
								<link>http://www.compadre.org/Informal/images/features/NASA-lightning-8-26-09-larg.jpg</link>
							
						
						
							<guid>http://www.nssl.noaa.gov/primer/lightning/ltg_basics.html</guid>
							<comments>http://www.physicstogo.com/bulletinboard/Thread.cfm?ID=4244</comments>
						
						<pubDate>Tue, 01 Sep 2009 00:00:00 EST</pubDate>
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