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	<id>https://prancer.physics.louisville.edu/astrowiki/index.php?action=history&amp;feed=atom&amp;title=The_Earth_Rotates</id>
	<title>The Earth Rotates - Revision history</title>
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	<updated>2026-05-13T11:00:37Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
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	<entry>
		<id>https://prancer.physics.louisville.edu/astrowiki/index.php?title=The_Earth_Rotates&amp;diff=360&amp;oldid=prev</id>
		<title>WikiSysop: /* Movies */</title>
		<link rel="alternate" type="text/html" href="https://prancer.physics.louisville.edu/astrowiki/index.php?title=The_Earth_Rotates&amp;diff=360&amp;oldid=prev"/>
		<updated>2012-01-08T00:01:11Z</updated>

		<summary type="html">&lt;p&gt;&lt;span class=&quot;autocomment&quot;&gt;Movies&lt;/span&gt;&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 00:01, 8 January 2012&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l147&quot;&gt;Line 147:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 147:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;available now on YouTube:&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;available now on YouTube:&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[http://www.youtube.com/watch?v=S2id35aQH0s Close-up view over 5 minutes on January 27, 2010 &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;| &lt;/del&gt;center &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;]&lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;&amp;lt;center&amp;gt;&lt;/ins&gt;[http://www.youtube.com/watch?v=S2id35aQH0s Close-up view over 5 minutes on January 27, 2010&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;]&amp;lt;/&lt;/ins&gt;center&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;&amp;gt;&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;#039;&amp;#039;4. How long does it take for this pendulum to complete one full swing?&amp;#039;&amp;#039;&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;#039;&amp;#039;4. How long does it take for this pendulum to complete one full swing?&amp;#039;&amp;#039;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>WikiSysop</name></author>
	</entry>
	<entry>
		<id>https://prancer.physics.louisville.edu/astrowiki/index.php?title=The_Earth_Rotates&amp;diff=27&amp;oldid=prev</id>
		<title>WikiSysop at 03:14, 12 September 2011</title>
		<link rel="alternate" type="text/html" href="https://prancer.physics.louisville.edu/astrowiki/index.php?title=The_Earth_Rotates&amp;diff=27&amp;oldid=prev"/>
		<updated>2011-09-12T03:14:44Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;== Discover the Rotation of the Earth ==&lt;br /&gt;
&lt;br /&gt;
In 1851 Leon Foucault (1819-1868) was made famous when he devised an experiment with a pendulum that&lt;br /&gt;
demonstrated the rotation of the Earth. Inside the dome of the Pantheon of Paris, Foucault suspended&lt;br /&gt;
an iron ball about 1 foot in diameter from a wire 67 meters (220 feet) long. The ball could easily&lt;br /&gt;
swing back and forth more than 4 meters (12 feet). He built a circular ring on which he placed a&lt;br /&gt;
ridge of sand just under the swinging ball. A pin attached to the ball would scrape sand away each&lt;br /&gt;
time the ball passed by.The ball was drawn to the side and held in place by a cord until itwas&lt;br /&gt;
absolutely still. The cord was burned to start the pendulum swinging in a perfect plane. Swing after&lt;br /&gt;
swing the plane of the pendulum turned slowly because the floor of the Pantheon was moving under the&lt;br /&gt;
pendulum. We know this device today as the Foucault pendulum. Almost every major science museum has one on&lt;br /&gt;
display. For this experiment you&amp;#039;ll use photographs and videos of a Foucault pendulum if you do not&lt;br /&gt;
have one nearby to visit.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== The Earth&amp;#039;s Rotation ==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
While our clocks are set by an average 24 hour day for the passage of the Sun from noon to noon, the&lt;br /&gt;
Earth rotates on its axis in 23 hours 56 minutes and 4.1 seconds with respect to the rest of the&lt;br /&gt;
universe. From our perspective here on the Earth, it appears that the entire universe circles us in&lt;br /&gt;
this time. It is possible to do some rather simple experiments that demonstrate that it is really&lt;br /&gt;
the rotation of the Earth that makes this daily motion occur.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:paschen_rug_20050117_sm.jpg | 600px | center]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Our solar heated cat knows to return to his favorite rug at noon every day.&lt;br /&gt;
He must move from time to time to stay in the light.&lt;br /&gt;
&lt;br /&gt;
== A Primer on the Foucault Pendulum ==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
It is said that Foucault&amp;#039;s discovery was based on an observation he made in a machine shop. If a&lt;br /&gt;
long metal rod is clamped at one end and given a whack at the other, it will vibrate back and forth&lt;br /&gt;
in a plane. The rod will oscillate rapidly back and forth, and although the motion dies down after a&lt;br /&gt;
while, it remains confined to a plane in space, even if the rod is rotated. This is not an&lt;br /&gt;
experiment you can repeat easily, but there is a demonstration you can do for yourself.&lt;br /&gt;
Find a piece of string about a meter long (a meter is 40 inches). Tie one end of it to a weight of&lt;br /&gt;
some sort -- most anything small and heavy will do -- to make a pendulum. Hold the other end of the&lt;br /&gt;
string and start the pendulum swinging back and forth in a plane.&lt;br /&gt;
As best you can manage, hold your hand in one spot in space while the pendulum swings. Walk around&lt;br /&gt;
the pendulum, letting the string freely swing from your hand.&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;1. What happens to the plane of swing of the pendulum when you walk around your support for the&lt;br /&gt;
&amp;quot;fixed&amp;quot; end?&amp;#039;&amp;#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Answer to this with what you actually saw. The apparent behavior will be influenced by how you hold&lt;br /&gt;
the string, but in the perfect experiment you would not influence the swinging pendulum by your own&lt;br /&gt;
motion. When Leon Foucault saw this, he thought that it might provide a way to detect the rotation of the&lt;br /&gt;
Earth.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;2. Why do you think this happens?&amp;#039;&amp;#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Imagine that you could locate a pendulum at the north pole of the Earth, pull the weight to one&lt;br /&gt;
side, and start it swinging. Like the demonstration, it would swing in a fixed plane. Even as the&lt;br /&gt;
Earth rotated on its axis, the pendulum would continue to swing in the original plane that it was&lt;br /&gt;
started in. An observer watching from the rotating Earth, though, would see the plane of vibration&lt;br /&gt;
of the pendulum apparently swing around. In 23 hours 56 minutes at the north pole the plane would&lt;br /&gt;
sweep out one full turn.&lt;br /&gt;
&lt;br /&gt;
The plane of swing is fixed as we watch from our perspective, locked in with distant stars and&lt;br /&gt;
galaxies. The continents on the Earth rotate under the pendulum making the pendulum appear to move&lt;br /&gt;
around an observer at the Earth&amp;#039;s pole.&lt;br /&gt;
The sense of the Earth&amp;#039;s rotation can be determined by watching the pendulum. It&amp;#039;s easiest to see&lt;br /&gt;
from space, looking down a pole. Imagine now that you are watching the pendulum from Earth.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;3. In which sense would the plane of oscillation of a pendulum seem to rotate if you were watching&lt;br /&gt;
it from the north pole of the Earth? What about from the south pole? (Hint: Seen from above the&lt;br /&gt;
north pole the Earth would seem to rotate counter clockwise.&amp;#039;&amp;#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
There&amp;#039;s a helpful website about a Foucault Pendulum in the southern hemisphere that you can visit at&lt;br /&gt;
the School of Physics of the University of New South Wales, Australia.&lt;br /&gt;
&lt;br /&gt;
http://www.animations.physics.unsw.edu.au/jw/foucault_pendulum.html&lt;br /&gt;
&lt;br /&gt;
Actually what we have said only applies to a pendulum at one of the poles. At the equator there&lt;br /&gt;
wouldn&amp;#039;t be any effect of this sort. There, the rotation of the Earth simply carries the top of the&lt;br /&gt;
pendulum around; from space, the surface of the Earth will not seem to rotate under the pendulum.&lt;br /&gt;
Consequently, the size of this effect varies with latitude, from a rotation in 23 hours 56 minutes&lt;br /&gt;
at the poles to 32 hours in Paris to an infinitely long time at the equator.&lt;br /&gt;
&lt;br /&gt;
Consider a pendulum at a mid-northern latitude, and think about it swinging in a north-south plane.&lt;br /&gt;
As it moves toward the north, it starts out also moving to the east because if the rotation of the&lt;br /&gt;
Earth. The closer to a pole a point on Earth is, the lower its speed; the closer to the equator the&lt;br /&gt;
faster it goes. A point on the equator travels around the Earth once a day at 1674 km/hr (1040&lt;br /&gt;
mi/hr). That swinging pendulum starts out moving east faster than the surface of the earth at the&lt;br /&gt;
north end of its swing, and slower than the surface at the south end. The Earth overtakes it at the&lt;br /&gt;
south, and falls behind it at the north. If you are on Earth, it seems to you that the pendulum&amp;#039;s&lt;br /&gt;
swing is slowly drifting around.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== A Real Foucault Pendulum ==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Typical demonstrations of the Foucault Pendulum have a very heavy ``bob&amp;#039;&amp;#039;, the weight at one end, and&lt;br /&gt;
are very long. The time it takes for a pendulum to complete a swing depends only on the length of&lt;br /&gt;
the pendulum, not on how heavy the bob is or on big the swing is. A long pendulum is quite slow&lt;br /&gt;
compared to the one that you experimented with here.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
&lt;br /&gt;
[[File:foucault_pendulum_lower_sm.jpg | center ]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
From the lower level of Grawmeyer Hall at the Unversity of Louisville you can watch the Foucault&lt;br /&gt;
pendulum in motion.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:foucault_pendulum_upward_sm.jpg | center]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
If you look upward you will see the skylight at the top of the dome supporting the pendulum.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:foucault_pendulum_back_sm.jpg | center]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
The pendulum swings away from the camera.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:foucault_pendulum_forth_sm.jpg | center]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
The pendulum swings toward the camera.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
As the pendulum swings back and forth it passes over the compass ``rose&amp;#039;&amp;#039; on the floor and the marks&lt;br /&gt;
on the ring that are 1 degree apart. The time it takes to complete one full swing is called the&lt;br /&gt;
``period&amp;#039;&amp;#039; of the pendulum. It takes many cycles of the pendulum for the slow rotation of the Earth to&lt;br /&gt;
be apparent.&lt;br /&gt;
&lt;br /&gt;
== Movies ==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
We have made a few movies of the pendulum that you should be able view on your computer. Here is one&lt;br /&gt;
available now on YouTube:&lt;br /&gt;
&lt;br /&gt;
[http://www.youtube.com/watch?v=S2id35aQH0s Close-up view over 5 minutes on January 27, 2010 | center ]&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;4. How long does it take for this pendulum to complete one full swing?&amp;#039;&amp;#039;&lt;br /&gt;
&lt;br /&gt;
There is a small magnet that is actuated on each swing to give enough impulse to the pendulum to&lt;br /&gt;
keep it going. The magnet does not affect the period of the pendulum or the plane of its swing, but&lt;br /&gt;
does insure that it keeps running 24 hours a day.&lt;br /&gt;
&lt;br /&gt;
Now let&amp;#039;s look at the rotation of the Earth by watching the pendulum change its apparent plane of&lt;br /&gt;
swing. Notice that n this video the pendulum is swinging in a slightly different direction at the&lt;br /&gt;
end from where it was at the beginning. Since the video plays in real time, you can measure the rate at which this change is occuring. The&lt;br /&gt;
marks on the ring are 1 degree apart.&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;5. Over the course of this video, how many degrees did the plane of the pendulum&amp;#039;s swing change by?&amp;#039;&amp;#039;&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;6. Based on this, about how long would it take for the pendulum to change its plane by 1 degree?&amp;#039;&amp;#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Since there are 360 degrees in a circle, and you now know how long it takes to go 1 degree, you can&lt;br /&gt;
calculate how long it would take to go a full turn by multiplying by 360.&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;7. How many hours does it take this pendulum to complete a rotation?&amp;#039;&amp;#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
You can check your answer by looking at photos taken several minutes apart.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:foucault_20100127_140128_sm.jpg | 600 px | center]]&lt;br /&gt;
&lt;br /&gt;
Foucault pendulum swing on January 27, 2010 at 14:01:28 EST&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:foucault_20100127_144130_02_sm.jpg | 600 px | center ]]&lt;br /&gt;
&lt;br /&gt;
Foucault pendulum swing on January 27, 2010 at 14:43:23 EST&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;8. Note how much time elapsed between these two pictures, and how far the pendulum precessed.&lt;br /&gt;
Since each mark is one degree, how many degrees per minute is this? Does it agree with your&lt;br /&gt;
observation from the movie clip?&amp;#039;&amp;#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
It is a easier just to notice which way the pendulum is rotating. The sequence of videos will tell&lt;br /&gt;
you this from the point of view of the camera. Imagine, instead, that you are looking up on the&lt;br /&gt;
pendulum from the floor.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;9. Is the direction of rotation clockwise or counterclockwise as seen from the bottom looking up?&amp;#039;&amp;#039;&lt;br /&gt;
&lt;br /&gt;
Just for the sake of stimulating a brainstorm, imagine that you are at the north pole of the Earth,&lt;br /&gt;
looking straight up toward the north celestial pole in the night sky. You would see stars apparently&lt;br /&gt;
circling overhead daily. Now imagine that the pendulum is there too, swinging back and forth&lt;br /&gt;
overhead.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;10. Compare the rotation of the plane of the pendulum&amp;#039;s motion with the apparent rotation of the&lt;br /&gt;
stars seen from the north pole.&amp;#039;&amp;#039;&lt;/div&gt;</summary>
		<author><name>WikiSysop</name></author>
	</entry>
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