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CLAIRAULT (or CLAIRAUT), See also: born on the 13th or 7th of May 1713, at See also: Paris, where his See also: father was a teacher of See also: mathematics
.
Under his father's tuition he made such rapid progress in mathematical studies that in his thirteenth See also: year he read before the French See also: Academy an account of the properties of four curves which he had then discovered
.
When only sixteen he finished a See also: treatise, Recherches sur See also: les courbes a See also: double courbure, which, on its publication in 1731, procured his See also: admission into the Academy of Sciences, although even then he was below the legal age
.
In 1736, together with See also: Pierre See also: Louis Maupertuis, he took
See also: part in the expedition to See also: Lapland, which was undertaken for the purpose of estimating a degree of the meridian, and on his return he published his treatise Theorie de la figure de la terre (1743)
.
In this See also: work he promulgated the theorem, known as " Clairault's theorem," which connects the gravity at points on the See also: surface of a rotating See also: ellipsoid with the See also: compression and the centrifugal force at the equator (see See also: EARTH, FIGURE OF THE)
.
He obtainedan ingenious approximate solution of the problem of the three bodies; in 1750 he gained the prize of the St See also: Petersburg Academy for his essay Theorie de la lune; and in 1759 he calculated the perihelion of See also: Halley's See also: comet
.
He also detected singular solutions in See also: differential equations of the first See also: order, and of the second and higher degrees
.
Clairault died at Paris, on the 17th of May 1765
.
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