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	<title>Comments on: Common Sense for Uncommon Physics</title>
	<atom:link href="http://blogs.discovermagazine.com/cosmicvariance/2009/04/26/common-sense-for-uncommon-physics/feed/" rel="self" type="application/rss+xml" />
	<link>http://blogs.discovermagazine.com/cosmicvariance/2009/04/26/common-sense-for-uncommon-physics/</link>
	<description>Random samplings from a universe of ideas.</description>
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		<title>By: Paul Murray</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/04/26/common-sense-for-uncommon-physics/comment-page-1/#comment-74829</link>
		<dc:creator>Paul Murray</dc:creator>
		<pubDate>Wed, 13 May 2009 05:16:31 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2009/04/26/common-sense-for-uncommon-physics/#comment-74829</guid>
		<description>3db is approximately double.

1 bit of information at room temperature is about 1/55th of an electron volt. At liquid nitrogen temperature, its about 1/200th .

To cycle through all values of a 128-bit key at liquid nitrogen temperatures will need about 10^19.6 J, about 2.5 seconds of the total amout of solar radiation hitting the earth.

Roughly. Of course, you&#039;ll need one mother of a heatsink to keep that comfy liquid nitrogen temperature. And that&#039;s simply to cycle through the values. If you want to do some computations as well, that&#039;ll cost you more.</description>
		<content:encoded><![CDATA[<p>3db is approximately double.</p>
<p>1 bit of information at room temperature is about 1/55th of an electron volt. At liquid nitrogen temperature, its about 1/200th .</p>
<p>To cycle through all values of a 128-bit key at liquid nitrogen temperatures will need about 10^19.6 J, about 2.5 seconds of the total amout of solar radiation hitting the earth.</p>
<p>Roughly. Of course, you&#8217;ll need one mother of a heatsink to keep that comfy liquid nitrogen temperature. And that&#8217;s simply to cycle through the values. If you want to do some computations as well, that&#8217;ll cost you more.</p>
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		<title>By: philip</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/04/26/common-sense-for-uncommon-physics/comment-page-1/#comment-73944</link>
		<dc:creator>philip</dc:creator>
		<pubDate>Mon, 04 May 2009 03:29:41 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2009/04/26/common-sense-for-uncommon-physics/#comment-73944</guid>
		<description>A billion seconds is about 30 years.</description>
		<content:encoded><![CDATA[<p>A billion seconds is about 30 years.</p>
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		<title>By: Jonathan Thornburg</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/04/26/common-sense-for-uncommon-physics/comment-page-1/#comment-73928</link>
		<dc:creator>Jonathan Thornburg</dc:creator>
		<pubDate>Sun, 03 May 2009 19:22:21 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2009/04/26/common-sense-for-uncommon-physics/#comment-73928</guid>
		<description>(a) kT = 1 electron volt at a temperature of just over 10^4 Kelvin
(b) 1g (acceleration) * 1 year = approximately the speed of light
(c) 2^10 = 1024 = approximately 10^3 (useful for quicly converting powers of 2 to powers of 10)
(d) another astronomy one: 1 arcsecond = 1/206265 radians,
      or equivalently, 1 parsec = 206265 AU
 (e) and one more astronomy one, 1AU (= radius of Earth&#039;s orbit around sun)
      = 149 million km (but astronomers tend to write things like 10^13 cm,
     which always makes me stop and convert to meters then kilometers than AU)</description>
		<content:encoded><![CDATA[<p>(a) kT = 1 electron volt at a temperature of just over 10^4 Kelvin<br />
(b) 1g (acceleration) * 1 year = approximately the speed of light<br />
(c) 2^10 = 1024 = approximately 10^3 (useful for quicly converting powers of 2 to powers of 10)<br />
(d) another astronomy one: 1 arcsecond = 1/206265 radians,<br />
      or equivalently, 1 parsec = 206265 AU<br />
 (e) and one more astronomy one, 1AU (= radius of Earth&#8217;s orbit around sun)<br />
      = 149 million km (but astronomers tend to write things like 10^13 cm,<br />
     which always makes me stop and convert to meters then kilometers than AU)</p>
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		<title>By: Heather</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/04/26/common-sense-for-uncommon-physics/comment-page-1/#comment-73927</link>
		<dc:creator>Heather</dc:creator>
		<pubDate>Sun, 03 May 2009 19:20:59 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2009/04/26/common-sense-for-uncommon-physics/#comment-73927</guid>
		<description>A barn is 10 fm by 10 fm.

An erg is about 600 GeV and the Planck mass is of order 10 nanograms.

The local density of dark matter is about one WIMP [of 100 GeV] per coffee cup [300 mL].</description>
		<content:encoded><![CDATA[<p>A barn is 10 fm by 10 fm.</p>
<p>An erg is about 600 GeV and the Planck mass is of order 10 nanograms.</p>
<p>The local density of dark matter is about one WIMP [of 100 GeV] per coffee cup [300 mL].</p>
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		<title>By: Gavin Flower</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/04/26/common-sense-for-uncommon-physics/comment-page-1/#comment-73471</link>
		<dc:creator>Gavin Flower</dc:creator>
		<pubDate>Thu, 30 Apr 2009 01:41:26 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2009/04/26/common-sense-for-uncommon-physics/#comment-73471</guid>
		<description>oops!

&quot;36 Km per hour = 20 metres per second&quot;

should be

&quot;36 Km per hour = 10 metres per second&quot;


does no one check these approximations???     :-)</description>
		<content:encoded><![CDATA[<p>oops!</p>
<p>&#8220;36 Km per hour = 20 metres per second&#8221;</p>
<p>should be</p>
<p>&#8220;36 Km per hour = 10 metres per second&#8221;</p>
<p>does no one check these approximations???     <img src='http://blogs.discovermagazine.com/cosmicvariance/wp-includes/images/smilies/icon_smile.gif' alt=':-)' class='wp-smiley' /> </p>
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		<title>By: melior</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/04/26/common-sense-for-uncommon-physics/comment-page-1/#comment-73439</link>
		<dc:creator>melior</dc:creator>
		<pubDate>Wed, 29 Apr 2009 19:53:31 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2009/04/26/common-sense-for-uncommon-physics/#comment-73439</guid>
		<description>60 miles an hour is also a mile a minute, or 88 ft/second.</description>
		<content:encoded><![CDATA[<p>60 miles an hour is also a mile a minute, or 88 ft/second.</p>
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		<title>By: rob</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/04/26/common-sense-for-uncommon-physics/comment-page-1/#comment-73427</link>
		<dc:creator>rob</dc:creator>
		<pubDate>Wed, 29 Apr 2009 18:17:06 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2009/04/26/common-sense-for-uncommon-physics/#comment-73427</guid>
		<description>i like hc~1234 ev nm 

a megaparsec-barn is about the volume of your fingertip.

pi squared is ~10 (or as mentioned above, g)</description>
		<content:encoded><![CDATA[<p>i like hc~1234 ev nm </p>
<p>a megaparsec-barn is about the volume of your fingertip.</p>
<p>pi squared is ~10 (or as mentioned above, g)</p>
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		<title>By: Peter Erwin</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/04/26/common-sense-for-uncommon-physics/comment-page-1/#comment-73395</link>
		<dc:creator>Peter Erwin</dc:creator>
		<pubDate>Wed, 29 Apr 2009 11:51:13 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2009/04/26/common-sense-for-uncommon-physics/#comment-73395</guid>
		<description>Another shortcut from astronomy: 1 km/sec is roughly 1 parsec/million years. (Useful because typical motions of stars are measured in km/sec and distances are measured in parsecs.)

Example: how long does it take the Sun to make one complete Galactic orbit, given that its orbit is roughly circular with a radius of 8 kiloparsecs (kpc) and a velocity of about 200 km/s? Circumference of orbit = 2 pi x 8 kpc = 50,000 parsecs; divide this by 200 and you get 250, so the answer is &quot;about 250 million years&quot;.</description>
		<content:encoded><![CDATA[<p>Another shortcut from astronomy: 1 km/sec is roughly 1 parsec/million years. (Useful because typical motions of stars are measured in km/sec and distances are measured in parsecs.)</p>
<p>Example: how long does it take the Sun to make one complete Galactic orbit, given that its orbit is roughly circular with a radius of 8 kiloparsecs (kpc) and a velocity of about 200 km/s? Circumference of orbit = 2 pi x 8 kpc = 50,000 parsecs; divide this by 200 and you get 250, so the answer is &#8220;about 250 million years&#8221;.</p>
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		<title>By: citrine</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/04/26/common-sense-for-uncommon-physics/comment-page-1/#comment-73347</link>
		<dc:creator>citrine</dc:creator>
		<pubDate>Wed, 29 Apr 2009 01:11:31 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2009/04/26/common-sense-for-uncommon-physics/#comment-73347</guid>
		<description>The weight of an average apple is about 1 Newton.</description>
		<content:encoded><![CDATA[<p>The weight of an average apple is about 1 Newton.</p>
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		<title>By: just another astronomer</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/04/26/common-sense-for-uncommon-physics/comment-page-1/#comment-73330</link>
		<dc:creator>just another astronomer</dc:creator>
		<pubDate>Tue, 28 Apr 2009 22:35:36 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2009/04/26/common-sense-for-uncommon-physics/#comment-73330</guid>
		<description>Here are two rules of thumb that I&#039;ve used in the last week or so (though not, I hasten to add, for anything very important):

-- Most chemical reactions yield about an eV per bond, so typically a few eV per molecule.  This is useful for calculating the energy density of all kinds of things (like, say, gasoline), particularly if you remember that 1 eV is about 1.6x10^-19 Joules, and that a mole is about 6x10^23 whatevers.  A mole of carbon weighs about 12 grams.

-- Less generally useful, but interesting: the flux of solar radiation at Earth&#039;s distance is about 1400 Watts per square meter.  Fifteen lightbulbs.</description>
		<content:encoded><![CDATA[<p>Here are two rules of thumb that I&#8217;ve used in the last week or so (though not, I hasten to add, for anything very important):</p>
<p>&#8211; Most chemical reactions yield about an eV per bond, so typically a few eV per molecule.  This is useful for calculating the energy density of all kinds of things (like, say, gasoline), particularly if you remember that 1 eV is about 1.6&#215;10^-19 Joules, and that a mole is about 6&#215;10^23 whatevers.  A mole of carbon weighs about 12 grams.</p>
<p>&#8211; Less generally useful, but interesting: the flux of solar radiation at Earth&#8217;s distance is about 1400 Watts per square meter.  Fifteen lightbulbs.</p>
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