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Lenses and Waves

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60 CHAPTER 3<br />

The inversion of the picture a Keplerian telescope produced could be<br />

overcome by adding a third lens. Given the quality of the earliest lenses it<br />

was not advisable to ‘multiply’ glasses, but by the 1640s multi-lens telescopes<br />

were beginning to become acceptable. With the increase of length <strong>and</strong><br />

magnification, however, the field of a Keplerian telescope also became<br />

narrow. For example, the 23-foot telescope that Huygens used in his<br />

observations of Saturn had a field of only 17'. It could not display the entire<br />

Moon at once. The limited field of view could be overcome by adding a field<br />

lens. The Augsburg telescope maker Johann Wiesel was probably the first to<br />

make telescopes with such compound oculars. 32 In a letter of 17 December<br />

1649, Wiesel described a four-lens telescope. It had an eyepiece consisting of<br />

two plano-convex lenses fitted in a small tube. The eyepiece tube was<br />

inserted in a composition of tubes which held an objective lens at the far side<br />

<strong>and</strong> a plano-convex ocular which acted as a field lens. Wiesel added:<br />

“Sir you may bee assured this is y. e first starrie tubus wch I have made of this manner &<br />

so good yt it goes farre beyond all others wherof my selfe also doe not little rejoyce.” 33<br />

The fame of Wiesel’s telescopes spread quickly <strong>and</strong> throughout Europe<br />

telescope makers tried to equal them. On a visit to his relative Edelheer in<br />

Antwerpen on New Year’s eve 1652, Huygens saw a Wiesel telescope <strong>and</strong><br />

was very impressed. It was a four-lens telescope, probably comparable to one<br />

Wiesel described in 1649. Towards the end of 1654 Huygens acquired two<br />

letters written by Wiesel - one to his cousin Vogelaer - describing the<br />

construction <strong>and</strong> use of several optical instruments. 34 In the first letter a sixlens<br />

telescope was described, which could be used for both terrestrial <strong>and</strong><br />

celestial purposes. Wiesel was an artisan, a very good one with an unmatched<br />

underst<strong>and</strong>ing of lenses <strong>and</strong> their configurations. His was another kind of<br />

underst<strong>and</strong>ing than the dioptrical theory Huygens developed in 1653. This<br />

kind of experiential knowledge Huygens acquired the following years in his<br />

practical dioptrics. Then, some ten years later, in an artisanal manner<br />

Huygens made his own compound eyepiece with excellent dioptrical<br />

properties.<br />

Experiential knowledge<br />

Telescope makers had a great deal of knowledge of dioptrics, as witnessed by<br />

the fruits of their labor that are preserved. Like the process of production,<br />

the thinking behind these products is more difficult to retrieve. It is barely<br />

documented as craftsmen in general were reluctant to reveal the secrets of<br />

their trade. There is reason to believe that their knowledge of dioptrics was<br />

of a different kind than that of mathematicians. That much we can infer<br />

from what little material that has been preserved. Lens makers knew very<br />

32<br />

Van Helden, “Compound”, 27-29; Keil, “Technology transfer”, 272-273. They are first mentioned in<br />

Rheita’s Oculus Enoch et Eliae (1645), who referred his readers to Wiesel. For the relationship between<br />

Rheita <strong>and</strong> Wiesel see Keill, Augustanus Opticus, 66-77.<br />

33<br />

Van Helden, “Compound eyepieces”, 34. The entire letter is reproduced on 34-35.<br />

34<br />

OC1, 308-311.

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