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Lenses and Waves

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96 CHAPTER 3<br />

During the final weeks of 1659, Huygens took up <strong>and</strong> solved a problem<br />

that Mersenne had discussed 12 years earlier in Reflexiones physico-mathematicae<br />

(1647). The problem was to determine the distance traversed by a body in its<br />

first second of free fall, which amounts to determining half the value of the<br />

constant of gravitational acceleration. After having tried Mersenne’s<br />

experimental approach, Huygens ab<strong>and</strong>oned it in favor of a theoretical<br />

consideration of gravitational acceleration. He began a study of circular<br />

motion which in his view was closely connected to gravity: “The weight of a<br />

body is the same as the conatus of matter, equal to it <strong>and</strong> moved very swiftly,<br />

to recede from a center.” 189 Circular motion had been discussed by both<br />

Descartes <strong>and</strong> Galileo, but only in qualitative <strong>and</strong> fairly rough terms. 190<br />

Huygens set out to analyze circular motion mathematically. He derived an<br />

expression for the tension on a chord exerted by a body moving in a circle,<br />

by equating it with the tension exerted by the weight of the body. 191 He then<br />

considered the situation in which a body revolves on a chord in such a way<br />

that a stable situation is created <strong>and</strong> centrifugal <strong>and</strong> gravitational tension are<br />

counterbalanced. With the conical pendulum thus procured <strong>and</strong> reversing his<br />

calculations, Huygens found an improved value for gravitational acceleration<br />

<strong>and</strong> dismissed Mersenne’s original experiment. 192 Analyzing the experiment<br />

mathematically <strong>and</strong> comparing the time of vertical fall to the time of fall<br />

along an arc, he derived a theory of pendulum motion eventually resulting in<br />

the discovery of the isochronity of the cycloid. 193<br />

The aim of Huygens’ studies of curvilinear fall <strong>and</strong> circular motion was to<br />

render these motions with the same exactness Galileo had achieved with free<br />

fall. 194 In the case of curvilinear fall this meant to solve the tricky<br />

mathematical problem of relating the times with which curved <strong>and</strong> straight<br />

paths are traversed. In the case of circular motion, he quantitatively<br />

compared centrifugal <strong>and</strong> gravitational acceleration. Huygens’ success came<br />

from his proficiency in using infinitesimal analysis <strong>and</strong> his control of<br />

geometrical reasoning. 195 He conceptualized the forces he was studying in a<br />

way that could be geometrically represented, which in his view meant to treat<br />

free fall <strong>and</strong> centrifugal force in terms of velocities. 196 He considered, for<br />

example, gravity as mere weight, <strong>and</strong> acceleration as continuous alteration of<br />

inertial motion. 197 In other words, rather than mathematizing these<br />

189<br />

Yoder, Unrolling time, 16-17.<br />

190<br />

Yoder, Unrolling time, 33-34.<br />

191<br />

Yoder, Unrolling time, 19-23. This expression for centrifugal tendency amounts to the modern formula:<br />

F = mv2/r. 192<br />

Yoder, Unrolling time, 27-32.<br />

193<br />

Yoder, Unrolling time, 48-59.<br />

194<br />

The first draft of De vi centrifuga opened with a quotation of Horace: “Freely I stepped into the void, the<br />

first”, above his discovery of the isochronicity of the cycloid he wrote: “Great matters not investigated by<br />

the men of genius among our forefathers; Yoder, Unrolling time, 42 <strong>and</strong> 61.<br />

195<br />

Yoder, Unrolling time, 62-64.<br />

196<br />

The same goes for his earlier study of impact, to be discussed in section 4.2.2.<br />

197 Westfall, Force, 160-165.

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