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Lenses and Waves

Lenses and Waves

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80 CHAPTER 3<br />

A new design<br />

We could have passed over this episode with Nul<strong>and</strong>t, if its conclusion had<br />

not coincided with the next phase in Huygens’ study of spherical aberration.<br />

On that same 1st of February, he gloriously<br />

wrote down “A composite lens emulating a<br />

hyperbolic lens. EUPHKA” 123 He had found a<br />

new solution to the problem of neutralizing<br />

spherical aberration that made his earlier one<br />

superfluous. It consisted of a combination of<br />

two lenses that would replace one objective<br />

lens. This composite lens could therefore be<br />

used in telescopes for astronomical<br />

observation, whereas the earlier solution was<br />

useful for terrestrial telescopes only. On<br />

February 22, he asked his brother Lodewijk to<br />

tell Constantijn<br />

“… that I ab<strong>and</strong>on the little ocular I had asked<br />

from him, because I have found something better<br />

<strong>and</strong> more substantial in these matters, that I would<br />

like to try out myself.” 124<br />

Huygens’ idea was as follows (Figure 33).<br />

The bi-concave lens VBC <strong>and</strong> the plano-convex<br />

lens KSTG have the same focus E, with respect<br />

to diverging rays MV coming from M, <strong>and</strong><br />

parallel rays QK, respectively. In addition, the<br />

spherical aberration EN produced by each lens<br />

is the same for these rays. An arbitrary ray QK,<br />

parallel to the axis ASM, is refracted by lens KST<br />

towards point N, a little off its focus E. Lens<br />

VBC, in its turn, refracts a ray MV towards the<br />

same point N, at the same distance from its<br />

focus E. Ray CN is therefore refracted towards<br />

M. As a result, the composite lens brings all<br />

parallel rays QK to a perfect focus M <strong>and</strong> “…<br />

will emulate a hyperbolical or elliptical lens<br />

perfectly.” 125 The system acts as a converging<br />

lens <strong>and</strong> can therefore replace the objective of<br />

any telescope. In his proof, Huygens worked<br />

Figure 33 The invention of 1669<br />

123<br />

OC13, 408. “Lens composita hyperbolicae aemula. EUPHKA 1 Febr. 1669.”<br />

124<br />

OC6, 377. “Vous pourrez luy dire que je le quite pour ce qui est du petit oculaire que je luy avois<br />

dem<strong>and</strong>è, ayant trouvè quelque chose meilleur et de plus considerable en cette matiere, dont j’ay envie de<br />

faire moy mesme l’essay.”<br />

125<br />

OC13, 413. “…[lens] compositae ex duabus VBC, KST, quae Hyperbolicae aut Ellipticae perfectionem<br />

aemulabitur.”

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