Kater's pendulum
A Kater's pendulum is a reversible free swinging
Description
A pendulum can be used to measure the acceleration of gravity g because for narrow swings its period of swing T depends only on g and its length L:[2]
So by measuring the length L and period T of a pendulum, g can be calculated.
The Kater's pendulum consists of a rigid metal bar with two pivot points, one near each end of the bar. It can be suspended from either pivot and swung. It also has either an adjustable weight that can be moved up and down the bar, or one adjustable pivot, to adjust the periods of swing. In use, it is swung from one pivot, and the period timed, and then turned upside down and swung from the other pivot, and the period timed. The movable weight (or pivot) is adjusted until the two periods are equal. At this point the period T is equal to the period of an 'ideal' simple pendulum of length equal to the distance between the pivots. From the period and the measured distance L between the pivots, the acceleration of gravity can be calculated with great precision from the equation (1) above.
The acceleration due to gravity by Kater's pendulum is given by[3]
where T1 and T2 are the time periods of oscillations when it is suspended from K1 and K2 respectively and ℓ1 and ℓ2 are the distances of knife edges K1 and K2 from the center of gravity respectively.
History
Gravity measurement with pendulums
![](http://upload.wikimedia.org/wikipedia/commons/thumb/2/28/PenduloCaminos.jpg/220px-PenduloCaminos.jpg)
The first person to discover that gravity varied over the Earth's surface was French scientist
Pendulums were so universally used to measure gravity that, in Kater's time, the local strength of gravity was usually expressed not by the value of the acceleration g now used, but by the length at that location of the seconds pendulum, a pendulum with a period of two seconds, so each swing takes one second. It can be seen from equation (1) that for a seconds pendulum, the length is simply proportional to g:
Inaccuracy of gravimeter pendulums
In Kater's time, the period T of pendulums could be measured very precisely by timing them with precision clocks set by the passage of stars overhead. Prior to Kater's discovery, the accuracy of g measurements was limited by the difficulty of measuring the other factor L, the length of the pendulum, accurately. L in equation (1) above was the length of an ideal mathematical 'simple pendulum' consisting of a point mass swinging on the end of a massless cord. However the 'length' of a real pendulum, a swinging rigid body, known in mechanics as a
To get around this problem, most early gravity researchers, such as
Kater's solution
However, in Horologium Oscillatorium, Huygens had also proved that the pivot point and the center of oscillation were interchangeable. That is, if any pendulum is suspended upside down from its center of oscillation, it has the same period of swing, and the new center of oscillation is the old pivot point. The distance between these two conjugate points was equal to the length of a simple pendulum with the same period.
As part of a committee appointed by the Royal Society in 1816 to reform British measures, Kater had been contracted by the House of Commons to determine accurately the length of the seconds pendulum in London.[6] He realized Huygens' principle could be used to find the center of oscillation, and so the length L, of a rigid (compound) pendulum. If a pendulum were hung upside down from a second pivot point that could be adjusted up and down on the pendulum's rod, and the second pivot were adjusted until the pendulum had the same period as it did when swinging right side up from the first pivot, the second pivot would be at the center of oscillation, and the distance between the two pivot points would be L.
Kater was not the first to have this idea.
![](http://upload.wikimedia.org/wikipedia/commons/thumb/e/ea/Kater_pendulum.png/400px-Kater_pendulum.png)
(a) opposing knife edge pivots from which pendulum is suspended
(b) fine adjustment weight moved by adjusting screw
(c) coarse adjustment weight clamped to rod by setscrew
(d) bob
(e) pointers for reading
The pendulum
Kater built a pendulum consisting of a brass rod about 2 meters long, 1+1⁄2 inches wide and one-eighth inch thick, with a weight (d) on one end.[1][9] For a low friction pivot he used a pair of short triangular 'knife' blades attached to the rod. In use the pendulum was hung from a bracket on the wall, supported by the edges of the knife blades resting on flat agate plates. The pendulum had two of these knife blade pivots (a), facing one another, about a meter (40 in) apart, so that a swing of the pendulum took approximately one second when hung from each pivot.
Kater found that making one of the pivots adjustable caused inaccuracies, making it hard to keep the axis of both pivots precisely parallel. Instead he permanently attached the knife blades to the rod, and adjusted the periods of the pendulum by a small movable weight (b,c) on the pendulum shaft. Since gravity only varies by a maximum of 0.5% over the Earth, and in most locations much less than that, the weight only had to be adjusted slightly. Moving the weight toward one of the pivots decreased the period when hung from that pivot, and increased the period when hung from the other pivot. This also had the advantage that the precision measurement of the separation between the pivots only had to be made once.
Experimental procedure
To use, the pendulum was hung from a bracket on a wall, with the knife blade pivots supported on two small horizontal agate plates, in front of a precision pendulum clock to time the period. It was swung first from one pivot, and the oscillations timed, then turned upside down and swung from the other pivot, and the oscillations timed again. The small weight (b) was adjusted with the adjusting screw, and the process repeated until the pendulum had the same period when swung from each pivot. By putting the measured period T, and the measured distance between the pivot blades L, into the period equation (1), g could be calculated very accurately.
Kater performed 12 trials.[1] He measured the period of his pendulum very accurately using the clock pendulum by the method of coincidences; timing the interval between the coincidences when the two pendulums were swinging in synchronism. He measured the distance between the pivot blades with a microscope comparator, to an accuracy of 10−4 in. (2.5 μm). As with other pendulum gravity measurements, he had to apply small corrections to the result for a number of variable factors:
- the finite width of the pendulum's swing, which increased the period
- temperature, which caused the length of the rod to vary due to thermal expansion
- atmospheric pressure, which reduced the effective mass of the pendulum by the buoyancy of the displaced air, increasing the period
- altitude, which reduced the gravitational force with distance from the center of the Earth. Gravity measurements are always referenced to sea level.
He gave his result as the length of the
In 1824, the British Parliament made Kater's measurement of the seconds pendulum the official backup standard of length for defining the
Use
![](http://upload.wikimedia.org/wikipedia/commons/thumb/8/80/Repsold.jpg/220px-Repsold.jpg)
The large increase in gravity measurement accuracy made possible by Kater's pendulum established
Reversible pendulums remained the standard method used for absolute gravity measurements until they were superseded by free-fall
Repsold–Bessel pendulum
![](http://upload.wikimedia.org/wikipedia/commons/thumb/6/64/Repsold_pendulum.png/80px-Repsold_pendulum.png)
Repeatedly timing each period of a Kater pendulum, and adjusting the weights until they were equal, was time-consuming and error-prone.
Here and are the distances of the two pivots from the pendulum's center of gravity. The distance between the pivots, , can be measured with great accuracy. and , and thus their difference , cannot be measured with comparable accuracy. They are found by balancing the pendulum on a knife edge to find its center of gravity, and measuring the distances of each of the pivots from the center of gravity. However, because is so much smaller than , the second term on the right in the above equation is small compared to the first, so doesn't have to be determined with high accuracy, and the balancing procedure described above is sufficient to give accurate results.
Therefore, the pendulum doesn't have to be adjustable at all, it can simply be a rod with two pivots. As long as each pivot is close to the
In addition, Bessel showed that if the pendulum was made with a symmetrical shape, but internally weighted on one end, the error caused by effects of air resistance would cancel out. Also, another error caused by the finite diameter of the pivot knife edges could be made to cancel out by interchanging the knife edges.
Bessel didn't construct such a pendulum, but in 1864 Adolf Repsold, under contract to the Swiss Geodetic Commission, developed a symmetric pendulum 56 cm long with interchangeable pivot blades, with a period of about 3⁄4 second. The Repsold pendulum was used extensively by the Swiss and Russian Geodetic agencies, and in the
International Association of Geodesy
The 1875 Conference of the
The determination of gravity by the reversible pendulum was subject to two types of error. On the one hand the resistance of the air and on the other hand the movements that the oscillations of the pendulum imparted to its plane of suspension. These movements were particularly important with the apparatus designed by the Repsold brothers on the indications of Bessel, because the pendulum had a large mass in order to counteract the effect of the viscosity of the air. While Emile Plantamour was carrying out a series of experiments with this device, Adolph Hirsch found a way to demonstrate the movements of the pendulum's suspension plane by an ingenious process of optical amplification. Isaac-Charles Élisée Cellérier, a mathematician from Geneva and Charles Sanders Peirce would independently develop a correction formula that allowed the use of the observations made with this type of gravimeter.[18][19]
President of the Permanent Commission of the European Arc Measurement from 1874 to 1886, Carlos Ibáñez Ibáñez de Ibero became the first president of the International Geodetic Association (1887–1891) after the death of Johann Jacob Baeyer. Under Ibáñez's presidency, the International Geodetic Association acquired a global dimension with the accession of the United States, Mexico, Chile, Argentina and Japan. As a result of the work of the International Geodetic Association, in 1901, Friedrich Robert Helmert found, mainly by gravimetry, parameters of the ellipsoid remarkably close to reality.[20][21][22][23]
References
- ^ a b c Kater, Henry (1818). "An account of experiments for determining the length of the pendulum vibrating seconds in the latitude of London". Phil. Trans. R. Soc. 104 (33). London: 109. Retrieved 2008-11-25.
- ^ Nave, C. R. (2005). "Simple Pendulum". Hyperphysics. Dept. of Physics and Astronomy, Georgia State Univ. Retrieved 2009-02-20.
- ^ "Kater's Pendulum". Virtual Amrita Laboratories. Amrita Vishwa Vidyapeetham. 2011. Retrieved 2019-01-26.
- ^ Poynting, John Henry; Joseph John Thompson (1907). A Textbook of Physics, 4th Ed. London: Charles Griffin & Co. p. 20.
- ^ Victor F., Lenzen; Robert P. Multauf (1964). "Paper 44: Development of gravity pendulums in the 19th century". United States National Museum Bulletin 240: Contributions from the Museum of History and Technology reprinted in Bulletin of the Smithsonian Institution. Washington: Smithsonian Institution Press. p. 307. Retrieved 2009-01-28.
- ISBN 0-87169-186-8.
- ^ Lenzen & Multauf 1964, p. 315
- ^ Poynting & Thompson 1907, p. 12
- ^ Elias Loomis (1864). Elements of Natural Philosophy, 4th Ed. New York: Harper & Brothers. p. 109.
- ^ An Act for ascertaining and establishing Uniformity of Weights and Measures, British Parliament, 17 June 1824, reprinted in Raithby, John (1824). The Statutes of the United Kingdom of Great Britain and Ireland, Volume 27. London: Andrew Strahan. p. 759. The wording of the Act indicates that the pendulum definition is to be used to restore the yard if the prototype is destroyed.
- ^ Trautwine, John Cresson (1907). The Civil Engineer's Pocket-book, 18th Ed. Wiley. p. 216.
- ^ Rutter, Henry (1866). The Metric System of Weights and Measures Compared with British Standard Weights and Measures in a Complete Set of Comparative Tables. Effingham Wilson. pp. xvii.
pendulum.
- ISBN 9780871691866.
- ISBN 3-11-017072-8.
- ^ Poynting & Thompson 1907, p. 15
- ^ Zuerich, ETH-Bibliothek. "Bulletin de la Société des Sciences Naturelles de Neuchâtel". E-Periodica (in French). p. 256. Retrieved 2021-10-25.
- ^ "Report from Charles S. Peirce on his second European trip for the Anual Report of the Superintendent of the U. S. Coast Survey, New York, 18.05.1877". www.unav.es. Retrieved 2021-10-25.
- ^ texte, Académie des sciences (France) Auteur du (January 1880). "Comptes rendus hebdomadaires des séances de l'Académie des sciences / publiés... par MM. les secrétaires perpétuels". Gallica (in French). pp. 1463–1466. Retrieved 2021-10-25.
- ^ Ibáñez e Ibáñez de Ibero, Carlos (1881). Discursos leidos ante la Real Academia de Ciencias Exactas Fisicas y Naturales en la recepcion pública de Don Joaquin Barraquer y Rovira (in Spanish). Madrid: Imprenta de la Viuda e Hijo de D.E. Aguado. pp. 70–73.
- OCLC 36747385.
- ISBN 978-3-319-30895-1.
- S2CID 120943411.
- S2CID 119447198.
External links
- The Accurate Measurement of g using Kater's pendulum, U. of Sheffield Has derivation of equations
- Kater, Henry (June 1818) An Account of the Experiments for determining the length of the pendulum vibrating seconds in the latitude of London, The Edinburgh Review, Vol. 30, p.407 Has detailed account of experiment, description of pendulum, value determined, interest of French scientists