Foucault pendulum
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- This article is about the physics experiment and implement. For the novel by Italian philosopher Umberto Eco, see Foucault's Pendulum.
A Foucault pendulum, or Foucault's pendulum, named after the French physicist Léon Foucault, was conceived as an experiment to demonstrate the rotation of the Earth; its action is a result of the Coriolis effect. It is a tall pendulum free to oscillate in any vertical plane and ideally should include some sort of motor so that it can run continuously rather than have its motion damped by air resistance. The first Foucault pendulum exhibited to the public was in February 1851 in the Meridian Room of the Paris Observatory, although Vincenzo Viviani had already experimented with a similar device in 1661. A few weeks later, Foucault made his most famous pendulum when he suspended a 28-kg bob with a 67-metre wire from the dome of the Panthéon in Paris. In 1851 it was well known that the Earth moved: experimental evidence included the aberration of starlight, stellar parallax, and the Earth's measured polar flattening and equatorial bulge. However Foucault's pendulum was the first dynamical proof of the rotation in an easy-to-see experiment, and it created a justified sensation in both the learned and everyday worlds.
At either the North Pole or South Pole, the plane of oscillation of a pendulum remains pointing in the same direction with respect to the fixed stars, while the Earth rotates underneath it, taking one sidereal day to complete a rotation. When a Foucault pendulum is suspended somewhere on the equator, then the plane of oscillation of the Foucault pendulum is at all times co-rotating with the rotation of the Earth. What happens at other latitudes is an intermediate between these two effects.
At the equator the equilibrium position of the pendulum is in a direction that is perpendicular to the Earth's axis of rotation. Because of that, the plane of oscillation is co-rotating with the Earth. Away from the equator the co-rotating with the Earth is diminished. Between the poles and the equator the plane of oscillation is rotating both with respect to the stars and with respect to the Earth. The direction of the plane of oscillation of a pendulum with respect to the Earth rotates with an angular speed proportional to the sine of its latitude; thus one at 45° rotates once every 1.4 days and one at 30° every 2 days.
n = degrees per day
φ = Latitude
Many people found the sine factor difficult to understand, which prompted Foucault to conceive the gyroscope in 1852. The gyroscope's spinning rotor tracks the stars directly. Its axis of rotation turns once per day whatever the latitude, unaffected by any sine factor.
A Foucault pendulum is tricky to set up because imprecise construction can cause additional veering which masks the terrestrial effect. The initial launch of the pendulum is critical; the traditional way to do this, without imparting any unwanted sideways motion, is to use a flame to burn through a thread which is temporarily holding the bob in its starting position. Air resistance damps the oscillation, so Foucault pendulums in museums usually either incorporate an electromagnetic or other drive to keep the bob swinging or are restarted regularly and in fact may have a launching ceremony as an added show.
The Foucault pendulum that hangs in the rotunda of the Lexington Public Library in Lexington, Kentucky in the United States is the largest ceiling clock in the world.[citation needed]
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[edit] The dynamics of the Foucault pendulum
The diagram shows the precession of the plane of swing of a Foucault pendulum as a function of latitude. The horizontal axis is the latitude: from 90 degrees latitude (at the north or south pole) to 0 degrees latitude (at the equator). The vertical axis shows the rate of precession in degrees per hour; positive numbers indicate precession in the direction which the fixed stars appear to rotate (clockwise in the northern hemisphere, and counterclockwise in the southern hemisphere).
The red line shows the precession with respect to the Earth of a Foucault pendulum. At the pole the pendulum precesses (with respect to the Earth) through an entire circle in one sidereal day.
For example: A Foucault pendulum located on the southern hemisphere at 30 degrees latitude will take two days to precess through an entire circle with respect to the Earth, precessing counterclockwise with respect to the Earth at a rate of 7.5 degrees per hour.
[edit] Foucault pendula in the world
- Further information: List of Foucault pendula
There is an abundance of Foucault pendula in the world, mainly at universities, science museums and planetariums. The experiment has even been carried out at the South Pole [1].
[edit] See also
- Foucault Pendulum connections
- Foucault Pendulum drive systems
- Foucault Pendulum vector diagrams
[edit] External links
- Lansey, Jonathan "Bowling Ball Foucault's Pendulum Experiment".
- "South Pole Foucault Pendulum". Winter, 2001.
- Wolfe, Joe, "A derivation of the precession of the Foucault pendulum".
- "The Foucault Pendulum", derivation of the precession in polar coordinates.
- "Webcam Kirchhoff-Institut für Physik, Universität Heidelberg".
- Tobin, William "The Life and Science of Léon Foucault".
- Dooley, J. W. "Non-Rigorous derivation of its precession".
- "The Foucault Pendulum" with film clip and animations.
- "Foucault pendulum video" Foucault pendulum at the Musée des arts et métiers, Paris, France) (video clip)
- "Science Design's Small Portable Foucault Pendulum" A company selling a Foucault Pendulum for the classroom.
[edit] References
- Durran, D. R., 1993: Is the Coriolis force really responsible for the inertial oscillation?, Bull. Amer. Meteor. Soc., 74, 2179–2184; Corrigenda. Bulletin of the American Meteorological Society, 75, 261
- Persson, A.
- How do we Understand the Coriolis Force? Bulletin of the American Meteorological Society 79, 1998, 1373-1385.
- The Coriolis Effect: Four centuries of conflict between common sense and mathematics, Part I: A history to 1885 History of Meteorology 2 (2005)
- Norman A. Phillips
- An Explication of the Coriolis Effect, Bulletin of the American Meteorological Society: Vol. 81, No. 2, 2000, pp. 299–303.
- What Makes the Foucault Pendulum Move among the Stars? Science and Education, Volume 13, Number 7, November 2004, pp. 653-661(9)
- Classical dynamics of particles and systems, 4ed, Marion Thornton (ISBN 0-03-097302-3 ), P.398-401.