Lenses and Waves
Lenses and Waves
Lenses and Waves
Create successful ePaper yourself
Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.
64 CHAPTER 3<br />
that the power of a telescope could better be determined by calculation than<br />
using the ordinary ways of comparison. He referred to a theorem in<br />
“Dioptricis nostris”: the magnification is equal to the proportion of the focal<br />
distances of objective <strong>and</strong> ocular. 49<br />
Figure 24 Huygens’ eyepiece. (see also the diagram in Figure 25)<br />
The year 1662 marks a turn in Huygens’ dioptrics. He invented something<br />
new <strong>and</strong> then turned to dioptrical theory again. The invention was a<br />
particular configuration of three lenses in a compound ocular (Figure 24).<br />
Nowadays called ‘Huygens’ eyepiece’, it had considerable advantages over<br />
earlier solutions: it produced a large field of view <strong>and</strong> images that suffered<br />
relatively little from aberrations. 50 Huygens had developed the eyepiece after<br />
his trip to Paris <strong>and</strong> London in 1660-1, where he had talked much on<br />
telescopes <strong>and</strong> related matters. In Paris he had seen the artisan Menard <strong>and</strong><br />
the ingeneer Pierre Petit, who had the best collection of telescopes in Paris.<br />
In London he saw telescopes with compound eyepieces made by the<br />
telescope makers Paul Neile <strong>and</strong> Richard Reeve. 51<br />
In 1662, Huygens made his first telescopes with field lenses. Later that<br />
year, he found out what configuration of lenses produced bright images <strong>and</strong><br />
a wide field. On 5 October he wrote to his brother Lodewijk in Paris:<br />
“As for oculars, you will see that I have found something new that causes that<br />
distinctness in daytime telescopes [i.e. terrestrial], <strong>and</strong> the same thing in the very long<br />
ones, while giving them at the same time a wide opening.” 52<br />
Huygens’ design quickly became known <strong>and</strong> was adopted widely. How<br />
Huygens had found the precise configuration is unknown, yet everything<br />
points at it being a matter of trial-<strong>and</strong>-error inspired by the examples he had<br />
seen. 53<br />
After the invention, however, Huygens did something others like Wiesel<br />
<strong>and</strong> Reeve did not do. He set out to underst<strong>and</strong> how it worked by analyzing<br />
the dioptrical properties of his eyepiece. Huygens described its configuration<br />
in a proposition inserted in the third part of Tractatus. 54<br />
49<br />
OC15, 230-233.<br />
50<br />
Van Helden, “Compound eyepieces”, 33; Van Helden, “Huygens <strong>and</strong> the astronomers”, 158.<br />
51<br />
OC22, 568-576.<br />
52<br />
OC4, 242-3: “car pour les oculaires vous voyez bien que j’y ay trouvè quelque chose de nouveau, qui<br />
cause cette nettetè dans les lunettes du jour, et de mesme dans les plus longues, leur donnant en mesme<br />
temps une gr<strong>and</strong>e ouverture.”<br />
53<br />
Van Helden, “Compound eyepieces”, 33.<br />
54<br />
OC13, 252-259. The text in Oeuvres Complètes is probably from 1666. The notes contain some previous<br />
phrasing, probably from 1662. OC13, 252n1