Lenses and Waves
Lenses and Waves
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.