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MYSTERIES OF THE EQUILATERAL TRIANGLE - HIKARI Ltd

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Biographical Vignettes 163<br />

infinity. He also studied the integration of differential equations and fluid mechanics<br />

where he introduced the Lagrangian function. In 1764, he submitted<br />

a prize essay to the French Academy of Sciences on the libration of the moon<br />

containing an explanation as to why the same face is always turned towards<br />

Earth which utilized the Principle of Virtual Work and the idea of generalized<br />

equations of motion. In 1766, Lagrange succeeded Euler as the Director of<br />

Mathematics at the Berlin Academy where he stayed until 1787. During the<br />

intervening 20 years, he published a steady stream of top quality papers and<br />

regularly won the prize from the Académie des Sciences in Paris. These papers<br />

covered astronomy, stability of the solar system, mechanics, dynamics, fluid<br />

mechanics, probability and the foundation of calculus. His work on number<br />

theory in Berlin included the Four Squares Theorem and Wilson’s Theorem<br />

(n is prime if and only if (n − 1)! + 1 is divisible by n). He also made a<br />

fundamental investigation of why equations of degree up to 4 can be solved<br />

by radicals and studied permutations of their roots which was a first step in<br />

the development of group theory. However, his greatest achievement in Berlin<br />

was the preparation of his monumental work Traité de mécanique analytique<br />

(1788) which presented from a unified perspective the various principles of mechanics,<br />

demonstrating their connections and mutual dependence. This work<br />

transformed mechanics into a branch of mathematical analysis. In 1787, he<br />

left Berlin to accept a non-teaching post at the Académie des Sciences in Paris<br />

where he stayed for the rest of his career. He was a member of the committee to<br />

standardize weights and measures that recommended the adoption of the metric<br />

system and served on the Bureau des Longitudes which was charged with<br />

the improvement of navigation, the standardization of time-keeping, geodesy<br />

and astronomical observation. His move to Paris signalled a marked decline<br />

in his mathematical productivity with his single notable achievement being<br />

his work on polynomial interpolation. See Property 39 for a description of<br />

his contribution to the Polygonal Number Theorem and Applications 7&8 for<br />

a summary of his research on the Three-Body Problem. He died and was<br />

buried in the Panthéon in Paris, aged 77, before he could finish a thorough<br />

revision of Mécanique analytique. Source material for Lagrange is available in<br />

[23, 42, 297].<br />

Vignette 20 (Johann Karl Friedrich Gauss: 1777-1855).<br />

Karl Friedrich Gauss, Princeps mathematicorum, was born to poor workingclass<br />

parents in Braunschweig in the Electorate of Brunswick-Lüneburg of the<br />

Holy Roman Empire now part of Lower Saxony, Germany [36, 90, 160]. He<br />

was a child prodigy, correcting his father’s financial calculations at age 3 and<br />

discovering the sum of an arithmetic series in primary school. His intellectual<br />

abilities attracted the attention and financial support of the Duke of Braunschweig,<br />

who sent him to the Collegium Carolinum (now Technische Univer-

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