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	<title>Uncertain Principles &#187; Aaron Bergman</title>
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	<link>http://scienceblogs.com/principles</link>
	<description>Physics, Politics, Pop Culture</description>
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		<title>Sayonara</title>
		<link>http://scienceblogs.com/principles/2007/09/09/sayonara/</link>
		<comments>http://scienceblogs.com/principles/2007/09/09/sayonara/#comments</comments>
		<pubDate>Sun, 09 Sep 2007 11:49:34 +0000</pubDate>
		<dc:creator>Aaron Bergman</dc:creator>
				<category><![CDATA[Aaron]]></category>
		<category><![CDATA[Guest Bloggers]]></category>

		<guid isPermaLink="false">http://scienceblogs.com/principles/2007/09/09/sayonara/</guid>
		<description><![CDATA[Well, Chad&#8217;s back, and I guess that means that this guest-blogging stint has come to an end (free! I&#8217;m free!). I want to thank Chad again for the opportunity to play in his sandbox for a few weeks. I didn&#8217;t get the chance to write every post I had planned. Real life &#8212; or at&#8230;]]></description>
				<content:encoded><![CDATA[<p>Well, Chad&#8217;s back, and I guess that means that this guest-blogging stint has come to an end (free! I&#8217;m free!). I want to thank Chad again for the opportunity to play in his sandbox for a few weeks. I didn&#8217;t get the chance to write every post I had planned. Real life &#8212; or at least the closest academic imitation thereof &#8212; does sometimes get in the way of blogging. Anyways, having seen it from the other side now, this blogging stuff isn&#8217;t easy. I don&#8217;t know how Chad manages to come up with two or more things to say every day, but I guess that&#8217;s why he&#8217;s the blogger and I&#8217;m the guest-blogger. So, I hope you all appreciate Chad for all the hard work he puts in daily to give us the opportunity to avoid work.</p>
<p>As for my time here, I didn&#8217;t have to resort to a guess-the-lyrics post, Lee Smolin or, thankfully, politics. By that measure, I consider it a success. I enjoyed it, and I hope you enjoyed it, too. Maybe we can all do it again some time.</p>
<p>Later.</p>
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		<title>The Loss of Night</title>
		<link>http://scienceblogs.com/principles/2007/09/08/the-loss-of-night/</link>
		<comments>http://scienceblogs.com/principles/2007/09/08/the-loss-of-night/#comments</comments>
		<pubDate>Sat, 08 Sep 2007 18:40:34 +0000</pubDate>
		<dc:creator>Aaron Bergman</dc:creator>
				<category><![CDATA[Aaron]]></category>
		<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Guest Bloggers]]></category>

		<guid isPermaLink="false">http://scienceblogs.com/principles/2007/09/08/the-loss-of-night/</guid>
		<description><![CDATA[I remember the last time I saw the milky way. I was at my aunt&#8217;s house in the foothills of the Sierras, and late at night the dense river of stars emerges. But that is still not the true milky way, or so I hear. And, in more urban areas, the detritus of our incandescent&#8230;]]></description>
				<content:encoded><![CDATA[<p>I remember the last time I saw the milky way. I was at my aunt&#8217;s house in the foothills of the Sierras, and late at night the dense river of stars emerges. But that is still not the true milky way, or so I hear. And, in more urban areas, the detritus of our incandescent society reduces the night sky to an inchoate glow. This <a href = "http://www.newyorker.com/reporting/2007/08/20/070820fa_fact_owen?printable=true">article</a> in the New Yorker talks about the poorly designed night time illumination that has resulted in our current situation, and what can be and is being done about it.</p>
<p>(via <a href = "http://science.slashdot.org/science/07/09/08/1635219.shtml">Slashdot</a>)</p>
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		<title>The Job Hunt</title>
		<link>http://scienceblogs.com/principles/2007/09/06/the-job-hunt/</link>
		<comments>http://scienceblogs.com/principles/2007/09/06/the-job-hunt/#comments</comments>
		<pubDate>Thu, 06 Sep 2007 16:01:37 +0000</pubDate>
		<dc:creator>Aaron Bergman</dc:creator>
				<category><![CDATA[Aaron]]></category>
		<category><![CDATA[Academia]]></category>
		<category><![CDATA[Guest Bloggers]]></category>
		<category><![CDATA[Technology]]></category>

		<guid isPermaLink="false">http://scienceblogs.com/principles/2007/09/06/the-job-hunt/</guid>
		<description><![CDATA[Now that I&#8217;m back in College Station, it&#8217;s time to start getting applications ready for the great job search. I don&#8217;t know how it is in other fields, but in math/physics, this generally involves three to four letters of recommendation, a CV, a research statement, sometimes a teaching statement and maybe an annotated bibliography. In&#8230;]]></description>
				<content:encoded><![CDATA[<p>Now that I&#8217;m back in College Station, it&#8217;s time to start getting applications ready for the great job search. I don&#8217;t know how it is in other fields, but in math/physics, this generally involves three to four letters of recommendation, a CV, a research statement, sometimes a teaching statement and maybe an annotated bibliography. In high energy physics, we have the <a href = "http://particle.physics.ucdavis.edu/rumor/doku.php">Theoretical Particle Physics Job Rumor Mill</a> run by the now nonymous John Terning. In addition to listing offers and educated guesses at short lists, it also serves as a nice clearinghouse of positions. <a href = "http://www.slac.stanford.edu/spires/jobs/">SPIRES</a>, the <a href = "http://careers.aps.org/search.cfm">APS</a>, <a href = "http://www.physicstoday.org/jobs/">Physics Today</a> and I&#8217;m sure many others offer job listings, too.</p>
<p>This is one situation where the math world definitely has the physics world beat, however. The <a href = "http://www.ams.org/">AMS</a> runs a site called <a href = "http://www.mathjobs.org/jobs">MathJobs</a> which is completely brilliant. There&#8217;s a searchable database of jobs which I&#8217;ve configured to send me newly listed relevant offers daily. You can upload all the relevant documentation, and it will automatically send an e-mail to your recommenders so that they can upload their letters. The application then becomes a simple matter of ensuring that the relevant files are available and clicking away. It&#8217;s easy, efficient, and it saves countless manila envelopes.</p>
<p>I don&#8217;t know if any other academic fields do this right now, but I bet they all will in a few years. I hear rumors high energy physics postdocs may implement such a system in the nearish future.</p>
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		<title>Flying Things</title>
		<link>http://scienceblogs.com/principles/2007/09/05/flying-things/</link>
		<comments>http://scienceblogs.com/principles/2007/09/05/flying-things/#comments</comments>
		<pubDate>Wed, 05 Sep 2007 17:05:12 +0000</pubDate>
		<dc:creator>Aaron Bergman</dc:creator>
				<category><![CDATA[Aaron]]></category>
		<category><![CDATA[Experiment]]></category>
		<category><![CDATA[Guest Bloggers]]></category>
		<category><![CDATA[Physics]]></category>

		<guid isPermaLink="false">http://scienceblogs.com/principles/2007/09/05/flying-things/</guid>
		<description><![CDATA[Steinn reports that the NRC has made its recommendations for NASA&#8217;s Beyond Einstein program. The winners appear to be LISA, a gravity wave observatory, and JDEM, a competition of dark energy focussed satellites. Steinn has lots of links to the various projects. The executive summary of the report is availabe here (pdf). I know next&#8230;]]></description>
				<content:encoded><![CDATA[<p>Steinn <a href = "http://scienceblogs.com/catdynamics/2007/09/beyond_einstein_verdict_1.php">reports</a> that the NRC has made its recommendations for NASA&#8217;s <a href = "http://universe.nasa.gov/">Beyond Einstein</a> program. The winners appear to be <a href = "http://lisa.nasa.gov/">LISA</a>, a gravity wave observatory, and <a href = "http://universe.nasa.gov/program/probes/jdem.html">JDEM</a>, a competition of dark energy focussed satellites. Steinn has lots of links to the various projects. The executive summary of the report is availabe <a href = "http://books.nap.edu/execsumm_pdf/12006.pdf">here</a> (pdf).</p>
<p>I know next to nothing about these things, but from afar it always seemed like LISA was one of those neat ideas that was never actually going to happen. The basic idea is to put three satellites in orbit around the sun and bounce lasers around to measure gravitational waves. To keep things stable, as I understand it, the lasers would be inside the satellites, but not actually attached to them. Not cheap, but it could possibly open up an entirely new spectrum with which to do astronomy. But, as I said, I know nothing of the politics or technical details, so hopefully some astronomer/astrophysicist can write something up.</p>
<p><b>Update</b>: Sean <a href = "http://cosmicvariance.com/2007/09/05/national-academy-dark-energy-first-maybe-lisa-second/">weighs in</a>.</p>
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		<title>New Toys</title>
		<link>http://scienceblogs.com/principles/2007/09/05/new-toys/</link>
		<comments>http://scienceblogs.com/principles/2007/09/05/new-toys/#comments</comments>
		<pubDate>Wed, 05 Sep 2007 14:22:37 +0000</pubDate>
		<dc:creator>Aaron Bergman</dc:creator>
				<category><![CDATA[Aaron]]></category>
		<category><![CDATA[Guest Bloggers]]></category>
		<category><![CDATA[Technology]]></category>

		<guid isPermaLink="false">http://scienceblogs.com/principles/2007/09/05/new-toys/</guid>
		<description><![CDATA[Well, I&#8217;m back in Texas and just in time for Steve Jobs to introduce new toys I can&#8217;t afford. At the risk of turning Chad&#8217;s blog into an Apple advertisement, every time I pass an Apple store, it takes significant willpower to not walk out of there with a new iPhone. I find it endlessly&#8230;]]></description>
				<content:encoded><![CDATA[<p>Well, I&#8217;m back in Texas and just in time for Steve Jobs to introduce new toys I can&#8217;t afford. At the risk of turning Chad&#8217;s blog into an Apple advertisement, every time I pass an Apple store, it takes significant willpower to not walk out of there with a new iPhone. I find it endlessly amusing to load up my papers on the demo models &#8212; yes, I am easily amused. A certain theorist was showing his off at Aspen, too. Well, you don&#8217;t want a phone with your iPod? You can now get an iPod touch, WiFi included. 8 and 16 gigs. iPod Nano? Smaller with really tiny video. Old school iPods? 160 gigs now. And if you did happen to spend 600 bucks on your iPhone, sucks to be you. 400 now.</p>
<p>It&#8217;s getting a lot harder to convince myself to wait for iPhone 2.0.</p>
<p>Here&#8217;s coverage from <a href = "http://arstechnica.com/news.ars/post/20070905-apple-unveils-new-ipod-touch-fat-ipod-nano-at-special-event.html">ArsTechnica</a> and <a href = "http://www.macworld.com/news/2007/09/04/livecoverage/index.php">MacWorld</a>.</p>
<p><b>Update</b>: And the <a href = "http://www.apple.com">Apple website</a> has now been updated, too.</p>
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		<title>Happy Labor Day</title>
		<link>http://scienceblogs.com/principles/2007/09/03/happy-labor-day/</link>
		<comments>http://scienceblogs.com/principles/2007/09/03/happy-labor-day/#comments</comments>
		<pubDate>Mon, 03 Sep 2007 12:15:46 +0000</pubDate>
		<dc:creator>Aaron Bergman</dc:creator>
				<category><![CDATA[Aaron]]></category>
		<category><![CDATA[Guest Bloggers]]></category>

		<guid isPermaLink="false">http://scienceblogs.com/principles/2007/09/03/happy-labor-day/</guid>
		<description><![CDATA[Happy Labor Day to everyone. I&#8217;ll be traveling back to Texas, so no blog for me for a day or so.]]></description>
				<content:encoded><![CDATA[<p>Happy Labor Day to everyone. I&#8217;ll be traveling back to Texas, so no blog for me for a day or so. </p>
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		<title>Are You Ready for Some Football?</title>
		<link>http://scienceblogs.com/principles/2007/09/02/are-you-ready-for-some-footbal/</link>
		<comments>http://scienceblogs.com/principles/2007/09/02/are-you-ready-for-some-footbal/#comments</comments>
		<pubDate>Sun, 02 Sep 2007 11:33:36 +0000</pubDate>
		<dc:creator>Aaron Bergman</dc:creator>
				<category><![CDATA[Aaron]]></category>
		<category><![CDATA[Football]]></category>
		<category><![CDATA[Guest Bloggers]]></category>
		<category><![CDATA[Sports]]></category>

		<guid isPermaLink="false">http://scienceblogs.com/principles/2007/09/02/are-you-ready-for-some-footbal/</guid>
		<description><![CDATA[Because my team, the Forty Niners, aren&#8217;t. Neither apparently is Michigan. On the other hand, my co-guest blogger is surely happy.]]></description>
				<content:encoded><![CDATA[<p>Because my team, the <a href = "http://www.sfgate.com/cgi-bin/article.cgi?f=/c/a/2007/08/26/SP3ORPPAV.DTL">Forty</a> <a href = "http://www.sfgate.com/cgi-bin/article.cgi?f=/c/a/2007/08/31/SPP8RSDBO.DTL">Niners</a>, aren&#8217;t. Neither apparently is <a href = "http://sports.espn.go.com/espn/columns/story?columnist=forde_pat&#038;id=3001214&#038;sportCat=ncf">Michigan</a>. On the other hand, my co-guest blogger is surely <a href = "http://sfgate.com/cgi-bin/article.cgi?f=/c/a/2007/09/02/SP3DRU2J4.DTL">happy</a>.</p>
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		<title>Hugo Winners</title>
		<link>http://scienceblogs.com/principles/2007/09/01/hugo-winners/</link>
		<comments>http://scienceblogs.com/principles/2007/09/01/hugo-winners/#comments</comments>
		<pubDate>Sat, 01 Sep 2007 13:50:46 +0000</pubDate>
		<dc:creator>Aaron Bergman</dc:creator>
				<category><![CDATA[Aaron]]></category>
		<category><![CDATA[Guest Bloggers]]></category>
		<category><![CDATA[SF]]></category>

		<guid isPermaLink="false">http://scienceblogs.com/principles/2007/09/01/hugo-winners/</guid>
		<description><![CDATA[The Principles proprietor is currently at WorldCon where the Hugo awards are given out. This year&#8217;s winners are available (among many other places, I&#8217;m sure) at Patrick and Teresa Nielsen Hayden&#8217;s blog. I wasn&#8217;t a huge fan of Rainbows End myself. I did like &#8220;The Girl in the Fireplace&#8221;, a Doctor Who episode. The writer,&#8230;]]></description>
				<content:encoded><![CDATA[<p>The Principles proprietor is currently at WorldCon where the Hugo awards are given out. This year&#8217;s winners are available (among many other places, I&#8217;m sure) at Patrick and Teresa Nielsen Hayden&#8217;s <a href = "http://nielsenhayden.com/makinglight/archives/009335.html#009335">blog</a>. I wasn&#8217;t a huge fan of <i>Rainbows End</i> myself. I did like &#8220;The Girl in the Fireplace&#8221;, a Doctor Who episode. The writer, Steven Moffat, also wrote &#8220;Blink&#8221;, this season&#8217;s best episode.</p>
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		<title>Arithmetic and Music</title>
		<link>http://scienceblogs.com/principles/2007/09/01/arithmetic-and-music/</link>
		<comments>http://scienceblogs.com/principles/2007/09/01/arithmetic-and-music/#comments</comments>
		<pubDate>Sat, 01 Sep 2007 11:20:15 +0000</pubDate>
		<dc:creator>Aaron Bergman</dc:creator>
				<category><![CDATA[Aaron]]></category>
		<category><![CDATA[Guest Bloggers]]></category>
		<category><![CDATA[Music]]></category>

		<guid isPermaLink="false">http://scienceblogs.com/principles/2007/09/01/arithmetic-and-music/</guid>
		<description><![CDATA[Taking a break from all this physics, I thought I&#8217;d talk a little about music and some related mathematical coincidences. One of the fundamental concepts of music is that of consonance and dissonance. Consonant things sound nice when played together and dissonant things do not. For example, if you play two Cs together on a&#8230;]]></description>
				<content:encoded><![CDATA[<p>Taking a break from all this physics, I thought I&#8217;d talk a little about music and some related mathematical coincidences. One of the fundamental concepts of music is that of consonance and dissonance. Consonant things sound nice when played together and dissonant things do not. For example, if you play two Cs together on a piano (or your instrument of choice), it&#8217;s a pleasing sound, but playing a C and an F# together sound unpleasant.</p>
<p>It could have been the case that what we find pleasing and displeasing on this simple level could be purely random, but our tastes align with a very elementary mathematical fact. Ratios of frequencies that involve small numbers in the denominator sound good. Take a 2:1 ratio, for example. That is an octave. The A above middle C on a piano is usually tuned to around 440 Hz. An octave above that is 880 Hz, and an octave below that is 220 Hz.<br />
<span id="more-1699"></span><br />
Sticking with ones in the denominator, we next have a 3:1 ratio. This would be somewhere between one octave and two octaves. To keep things in the same octave, we can go down an octave from 3:1 and examine the ratio of 3:2. From the A on the piano, that is a frequency of 660 Hz. This interval is called a perfect fifth. When a singer sings a fifth, for example, they will usually sing a perfect fifth. I think that violinists and other fretless instruments also play perfect fifths, too, but I don&#8217;t remember. You will not find any key on a modern piano with the frequency of 660 Hz, however.</p>
<p>If we keep sticking to ratios between 1:1 and 2:1, the next smallest denominator is 4:3. This is a perfect fourth. If you pick a note and go a perfect fourth above it and follow that with a perfect fifth, you find that you are at a ratio of 3:2 * 4:3 = 2:1, an octave. Intervals which obey this relation are called complementary intervals. The octave, the perfect fourth and the perfect fifth are generally the most pleasent sounding intervals. Beyond this, there are ratios such as 5:3, a major sixth, 5:4, a major third, filling out much of the usual musical scale. Such a scale is called just intonation.</p>
<p>But where does the scale come from? Why stop at some particular point? Since the fourth and the fifth are complementary, we can pick one and focus on the fifth. What happens if we keep going up by fifths? We get a sequence of ratios that look like 3^n : 2^n. A funny thing happens when n=12. We can compute</p>
<p>(3/2)^12 = 129.75</p>
<p>This is remarkably close to 2^7. If we go up twelve fifths, we almost end up at seven octaves. Two fifths, for example, gives a ratio of 9:4. Going down and octave from there gives us 9:8 which is a major second. Going up again gives us 27:16 which has a pretty big denominator. However, 27/16 = 1.69 which is pretty close to 5/3=1.67 or a major sixth. Up a fifth and down an octave from there is 81/64 = 1.27 which isn&#8217;t all that close to the major third, but up a fifth from 5:3 (as opposed to 27:16) hits it on the nose. </p>
<p>This coincidence, that 129.75 is almost 128 tells us that we should think about a 12 note scale. We pick a note, called the tonic, on which to start the scale. If we choose C and go up  and down by fifths, we get</p>
<p>Gb &#8211; Db &#8211; Ab &#8211; Eb &#8211; Bb &#8211; F &#8211; C &#8211; G &#8211; D &#8211; A &#8211; E &#8211; B &#8211; F#</p>
<p>The notes Gb and F# are declared to be the same even though they differ by the factor of 3^12/2^19 = 1.014. This is called Pythagorean tuning, and the above sequence of notes (with the ends connected) is called the circle of fifths. Be construction, we get our fifths and fourths perfect. The major second and minor seventh are also hit on the nose. Others, like the major third (a pretty important interval) aren&#8217;t so great. </p>
<p>You can start fudging to get closer to just intonation. Just put the notes you want back to their nice ratios. But there&#8217;s no reason to only look at intervals starting at the tonic. As you fudge, the other fifths won&#8217;t sound so good anymore. The particularly bad intervals in various tunings are called &#8220;wolves&#8221;. If you change keys, you hit these intervals a lot. Back when, music in different keys actually sounded different.</p>
<p>There&#8217;s a conservation of trouble here. That 129.75 will always show up somewhere. The modern perspective is to put it everywhere. There are twelve notes in the scale, and we want the octave to be 2:1. Thus, we make each half-step (twelve half-steps form an octave) have a ratio of 2^(1/12):1. This is called equitempered tuning. The octave is still there, but all the other intervals have been fudged. For example, a fifth is now a ratio of 1.498:1 as opposed to 1.5:1. A fourth is  1.335:1 as opposed to 4:3. And all the fifths and fourths are equally close to the perfect interval. How about the major third that the Pythagorean tuning had trouble with? 1.26:1 as opposed to 1.25:1. Major sixth? 1:68:1 as opposed to 1.67:1. Not so bad, all things considered.</p>
<p>Intervals are cool and all that, but music is a lot more than that. At this point, we&#8217;ve made ourselves a chromatic scale:</p>
<p>C &#8211; C# &#8211; D &#8211; D# &#8211; E &#8211; F &#8211; F# &#8211; G &#8211; G# &#8211; A &#8211; A# &#8211; B &#8211; C</p>
<p>but almost no music is played in this scale. Instead, some subset of notes is chosen. The major diatonic scale starting on C, for example, is</p>
<p>C &#8211; D &#8211; E &#8211; F &#8211; G &#8211; A &#8211; B &#8211; C</p>
<p>and the natural minor scale is</p>
<p>C &#8211; D &#8211; Eb &#8211; F &#8211; G &#8211; Ab &#8211; Bb &#8211; C</p>
<p>There are other scales, too, but let&#8217;s stick with these. One explanation for them is that this sequence of notes appears in the circle of fifths. Starting at F, for example, one finds the major scale and starting at Eb gives the minor scale. I don&#8217;t find this particularly satisfying, so I&#8217;m going to talk about another &#8220;explanation&#8221; which I found on the internet (I forget the page, unfortunately).</p>
<p>Before getting to that, we need to talk about chords. We like small denominators, and the smallest denominator one can have is one. Thus, it helps to look at the sequence of ratios:</p>
<p>2:1 3:1 4:1 5:1 &#8230;</p>
<p>The first is the octave. The rest I will transpose to be less than one octave. The second becomes 3:2 which is the fifth. The third is another octave, and the fourth is 5:4, or the major third. These three notes form the major triad. We can keep going. 6:1 is the fifth again. 7:1 goes to 7/4 = 1.75. This is somewhere between a minor and major seventh. Depending on this choice, we get a dominant seventh chord or a major seventh chord. After this the chords get pretty busy, but the next new note is 9/8, the major second. This is a 9-chord. 11/8=1.375 is reasonably close to the perfect fourth, 4/3, which would make an 11-chord, but at this point we&#8217;re pretty dissonant.</p>
<p>The three most important notes in a scale are the tonic, the perfect fourth and the perfect fifth. If we add in the major triads on these notes, we get exactly the major scale. This is secretly the circle of fifths in disguise, really, but I think it makes the role of the tonic much more clear.</p>
<p>What about the minor triad, then, where the major third is replaced by a minor third? I don&#8217;t know if there&#8217;s a pat answer for that one. But, if you wanted to introduce some more dissonance in the major triad, the third would be the place to do it. If you take the minor triads on the tonic, fourth and fifth, you get the natural minor scale. The other minor scales are modifications that get you that nice major seventh note to lead into the tonic.</p>
<p>One last scale worth mentioning is the pentatonic scale. If you take five consecutive notes in the circle of fifths, you get the major pentatonic. It consists of the tonic, major second, major third, perfect fifth and major sixth. In C, that is</p>
<p>C &#8211; D &#8211; E &#8211; G &#8211; A &#8211; C</p>
<p>We can make a minor pentatonic by analogy to the major and minor diatonic scales. The natural minor in A has the same notes as the major scale in C. In general, the minor scale with the same notes as a given major scale (starting a minor third below the tonic of the major scale) is called the relative minor. So, we can define the minor pentatonic scale in C to be the same as the major pentatonic scale in Eb. Thus, we have</p>
<p>C &#8211; Eb &#8211; F &#8211; G &#8211; Bb &#8211; C</p>
<p>The pentatonic scale is great because you can play almost anything in it, and it won&#8217;t sound so bad. Much of pop music improvisation is done in this scale, in fact. It&#8217;s also the case that the black notes on a piano exactly form a pentatonic scale. This actually isn&#8217;t a coincidence given the discussion of the circle of fifths. There are twelve notes in the circle of fifths, forming the chromatic scale. If we take seven consecutive ones, we get the major diatonic scale which, in C, is the white notes on the piano. We have five notes left over, then, the black notes forming a nice pentatonic scale. So go nuts on the black notes.</p>
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		<title>Sky, Full of Stars</title>
		<link>http://scienceblogs.com/principles/2007/08/31/sky-full-of-stars/</link>
		<comments>http://scienceblogs.com/principles/2007/08/31/sky-full-of-stars/#comments</comments>
		<pubDate>Fri, 31 Aug 2007 09:39:44 +0000</pubDate>
		<dc:creator>Aaron Bergman</dc:creator>
				<category><![CDATA[Aaron]]></category>
		<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Guest Bloggers]]></category>
		<category><![CDATA[Science]]></category>

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		<description><![CDATA[If you&#8217;re on the west coast tonight and are willing to stay up late or wake up early, you have the chance to see the Aurigid meteor shower. This shower is fairly unique because it arises from a comet with a period of around 900 years. Some people have even claimed that there&#8217;s a chance&#8230;]]></description>
				<content:encoded><![CDATA[<p>If you&#8217;re on the west coast tonight and are willing to stay up late or wake up early, you have the chance to see the <a href = "http://aurigids.seti.org/">Aurigid</a> meteor shower. This shower is fairly unique because it arises from a comet with a period of around 900 years. Some people have even claimed that there&#8217;s a chance this could be <a href = "http://www.imcce.fr/page.php?nav=en/ephemerides/phenomenes/meteor/DATABASE/Alpha-Aurigids/2007/index.php">spectacular</a>, but these predictions are often wrong. After the disappointing Perseids, I&#8217;d love to be able to stay up for this one, but I&#8217;m still on the east coast. Ah well. Maybe <a href = "http://www.earthsky.org/article/2007-meteors">some other shower</a>.</p>
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