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Pendulum
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=== 1656: The pendulum clock === {{multiple image | align = left | direction = horizontal | footer = The first pendulum clock | image1 = Huygens first pendulum clock - front view.png | width1 = 120 | image2 = Huygens first pendulum clock.png | width2 = 112 }}{{Main|Pendulum clock}} In 1656 the Dutch scientist [[Christiaan Huygens]] built the first [[pendulum clock]].<ref>although there are unsubstantiated references to prior pendulum clocks made by others: {{cite book | last=Usher | first=Abbott Payson | title=A History of Mechanical Inventions | year=1988 | publisher=Courier Dover | pages= 310–311 | isbn=978-0-486-25593-4 | url=https://books.google.com/books?id=xuDDqqa8FlwC&pg=PA312 }}</ref> This was a great improvement over existing mechanical clocks; their best accuracy was improved from around 15 minutes deviation a day to around 15 seconds a day.<ref>{{cite book | last = Eidson | first = John C. | title = Measurement, Control, and Communication using IEEE 1588 | publisher = Burkhausen | year = 2006 | page = 11 | url = https://books.google.com/books?id=jmfkJYdEANEC&q=%22accuracy+of+clocks%22&pg=PA11 | isbn = 978-1-84628-250-8 }}</ref> Pendulums spread over Europe as existing clocks were [[retrofitted]] with them.<ref>Milham 1945, p.145</ref> The English scientist [[Robert Hooke]] studied the [[conical pendulum]] around 1666, consisting of a pendulum that is free to swing in two dimensions, with the bob rotating in a circle or ellipse.<ref name="OConnor2002">{{cite web | last = O'Connor | first = J.J. | author2 = E.F. Robertson | title = Robert Hooke | website = Biographies, MacTutor History of Mathematics Archive | publisher = School of Mathematics and Statistics, Univ. of St. Andrews, Scotland | date = August 2002 | url = http://www-groups.dcs.st-and.ac.uk/~history/Biographies/Hooke.html | access-date = 2009-02-21 | archive-date = 2009-03-03 | archive-url = https://web.archive.org/web/20090303081753/http://www-groups.dcs.st-and.ac.uk/~history/Biographies/Hooke.html | url-status = dead }}</ref> He used the motions of this device as a model to analyze the [[orbital motion]]s of the [[planet]]s.<ref>{{cite conference | first = Michael | last = Nauenberg | title = Robert Hooke's seminal contribution to orbital dynamics | book-title = Robert Hooke: Tercentennial Studies | pages = 17–19 | publisher = Ashgate Publishing | year = 2006 | isbn = 0-7546-5365-X }}</ref> Hooke suggested to [[Isaac Newton]] in 1679 that the components of orbital motion consisted of inertial motion along a tangent direction plus an attractive motion in the radial direction. This played a part in Newton's formulation of the [[law of universal gravitation]].<ref>{{cite journal | last=Nauenberg | first=Michael | title=Hooke and Newton: Divining Planetary Motions | journal=Physics Today | year=2004 | volume=57 | issue=2 | page=13 | url=http://scitation.aip.org/journals/doc/PHTOAD-ft/vol_57/iss_2/13_1.shtml | access-date=2007-05-30 | doi=10.1063/1.1688052 |bibcode = 2004PhT....57b..13N | doi-access=free | url-access=subscription }}</ref><ref>{{cite web |author=The KGM Group, Inc. |year=2004 |url=http://www.sciencemaster.com/space/item/helio_4.php |title=Heliocentric Models |publisher=Science Master |access-date=2007-05-30 |url-status=dead |archive-url=https://web.archive.org/web/20070713175810/http://www.sciencemaster.com/space/item/helio_4.php |archive-date=2007-07-13 }}</ref> Robert Hooke was also responsible for suggesting as early as 1666 that the pendulum could be used to measure the force of gravity.<ref name="OConnor2002" /> During his expedition to [[Cayenne]], [[French Guiana]] in 1671, [[Jean Richer]] found that a [[pendulum clock]] was {{frac|2|1|2}} minutes per day slower at Cayenne than at Paris. From this he deduced that the force of gravity was lower at Cayenne.<ref>{{cite conference | first = Victor F. | last = Lenzen |author2=Robert P. Multauf | title = Paper 44: Development of gravity pendulums in the 19th century | book-title = United States National Museum Bulletin 240: Contributions from the Museum of History and Technology reprinted in Bulletin of the Smithsonian Institution | pages = 307 | publisher = Smithsonian Institution Press | year = 1964 | location = Washington | url = https://books.google.com/books?id=A1IqAAAAMAAJ&pg=RA2-PA307 | access-date = 2009-01-28}}</ref><ref>{{cite book | last=Richer | first=Jean | year=1679 | title=Observations astronomiques et physiques faites en l'isle de Caïenne | publisher=Mémoires de l'Académie Royale des Sciences | bibcode=1679oaep.book.....R }} cited in [https://books.google.com/books?id=A1IqAAAAMAAJ&pg=RA2-PA307 Lenzen & Multauf, 1964], p.307</ref> In 1687, [[Isaac Newton]] in ''[[Philosophiæ Naturalis Principia Mathematica|Principia Mathematica]]'' showed that this was because the Earth was not a true sphere but slightly [[Oblate spheroid|oblate]] (flattened at the poles) from the effect of [[centrifugal force]] due to its rotation, causing gravity to increase with [[latitude]].<ref>[https://books.google.com/books?id=A1IqAAAAMAAJ&pg=RA2-PA307 Lenzen & Multauf, 1964], p.307</ref> Portable pendulums began to be taken on voyages to distant lands, as precision [[gravimeter]]s to measure the [[Gravity of Earth|acceleration of gravity]] at different points on Earth, eventually resulting in accurate models of the [[Figure of the Earth|shape of the Earth]].<ref>{{cite book | last = Poynting | first = John Henry |author2=Joseph John Thompson | title = A Textbook of Physics, 4th Ed | publisher = Charles Griffin & Co. | year = 1907 | location = London | pages = [https://archive.org/details/bub_gb_TL4KAAAAIAAJ/page/n30 20]–22 | url = https://archive.org/details/bub_gb_TL4KAAAAIAAJ }}</ref>
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