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Lenses and Waves

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Chapter 3<br />

1655-1672 - 'De Aberratione'<br />

Huygens' practical optics <strong>and</strong> the aspirations of dioptrical theory<br />

In the decade following Tractatus, Huygens was at home were his<br />

mathematical virtuosity grew to full stature. These are the years of his most<br />

renowned achievements: the invention – in 1656 – improvement <strong>and</strong><br />

employment of the pendulum clock <strong>and</strong> the theory of pendulum that were<br />

the basis of his master piece Horologium Oscillatorium (1673); the discovery in<br />

1655 of a satellite of Saturn <strong>and</strong> the identification of its ring. Through his<br />

correspondence <strong>and</strong> publications Huygens increasingly gained recognition<br />

among Europe’s scholars. He traveled abroad, first to Paris in 1655 to meet<br />

the leading French mathematicians, then to Paris <strong>and</strong> London in 1660-1, <strong>and</strong><br />

again in 1663-4, the last time being elected fellow of the Royal Society. There<br />

were squabbles as well, in Italy in particular, over the priority of the<br />

pendulum clock with Florentine sympathizers of the late Galileo <strong>and</strong> with<br />

the Roman telescope maker Divini over the superiority of his telescopes.<br />

Probably as a result of the clock dispute, he did not obtain a position at the<br />

court of prince Leopold, but in 1666 Huygens realized his learned assets. At<br />

the instigation of Colbert he came to Paris to help organize an ‘académie des<br />

sciences’, thus confirming his status as Europe’s leading mathematician. Life<br />

in Paris, with it competitive milieu, was no unqualified pleasure. Huygens<br />

correspondence shows symptoms of homesickness, he particularly missed<br />

his brother Constantijn, <strong>and</strong> in 1670 he was was smitten with ‘melancholie’<br />

for the first time. In these years he also experienced the first major setback in<br />

his science: a design for a perfect telescope proved useless. The design was<br />

the outcome of Huygens’ practical activities in telescopy of the late 1650s<br />

<strong>and</strong> his subsequent theoretical reflections thereupon of the 1660s. These are<br />

the subject of this chapter.<br />

When Huygens’ interest in dioptrics was sparked late 1652, it was both its<br />

theoretical <strong>and</strong> practical aspects. He immediately began inquiring about the<br />

art of lens making, but he engaged in practical dioptrics only after he put<br />

aside the manuscript of Tractatus. Around 1655, he <strong>and</strong> his brother<br />

Constantijn acquired the art of lens making <strong>and</strong> started building telescopes. 1<br />

The practice bore fruit almost immediately. In 1656, Christiaan published a<br />

pamphlet De saturni luna observatio nova on the discovery of a satellite around<br />

Saturn. It was the first new celestial body in the solar system to be<br />

1 Editor’s comment, OC15, 10. See also Anne van Helden, “Lens production”, 70.

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