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Lenses and Waves

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1655-1672 - DE ABERRATIONE 61<br />

well how to grind lenses to suitable proportions <strong>and</strong><br />

configure appropriately. The nature of this knowledge<br />

<strong>and</strong> to what extent they understood the dioptrical<br />

properties of lenses will be discussed now. Note that<br />

this is a discussion of very limited scope, determined<br />

by the considerations <strong>and</strong> activities of Huygens, that<br />

passes over the a wealth of historical knowledge that<br />

can be, <strong>and</strong> has been, gathered regarding the telescope<br />

making trade. 35<br />

A booklet on spectacles written in 1623 gives an<br />

indication of the underst<strong>and</strong>ing their manufacturers<br />

had of glasses. Uso de los antojos was written by the<br />

Andalusian licentiate Daza de Valdez. It explained<br />

how to choose glasses of appropriate strength for a<br />

patient. Daza described a procedure to determine the<br />

‘grado’ of a given lens (Figure 23). 36 He drew two solid<br />

circles X <strong>and</strong> Q of unequal diameter on a sheet of<br />

paper as well as a specific scale at one of the circles. A<br />

glass was then positioned on the scale in such a way<br />

that both circles were seen equally large. The position<br />

of the lens on the scale gave its ‘grado’. 37 Daza did not<br />

explain the method, he only described how it was<br />

employed. It was a practical procedure that did not require any<br />

underst<strong>and</strong>ing of its effect on rays.<br />

A manuscript written around 1670 in Rome by a certain Giovanni<br />

Bolantio contains a similar kind of procedural knowledge. It discussed the<br />

manufacture of telescopes <strong>and</strong> probably recorded the daily routine in some<br />

workshop. 38 It contains two tables listing the ocular <strong>and</strong> objective lenses<br />

needed to make a telescope of a specific strength, characterized by its length.<br />

The lenses are characterized by the doubled radius of the pattern in which<br />

they were ground. 39 Figure 23 Daza’s scale<br />

With these tables at h<strong>and</strong>, the workman could choose the<br />

patterns needed to make a telescope on order. Bolantio did not explain<br />

whether he had constructed the tables himself nor how they were made.<br />

Some dioptrical rules are implicit in them. For example, the length of a<br />

35<br />

See for example the recent, formidable study on Wiesel by Inge Keill which may serve as a guide to<br />

themes <strong>and</strong> literature: Keil, Augustanus Opticus.<br />

36<br />

Daza, Uso de los antojos, 137-140. It appears that this classification in terms of ‘degrees’ was, at that time,<br />

replacing an older one in terms of the common age of someone bearing spectacles of a particular<br />

strength. The ‘grados’ Daza employs seem to be identical with the ‘punti’ Garzoni mentions in his<br />

discussion of the craft in La piazza universale (1585). See also: Pflugk, “Beiträge”, 50-55.<br />

37<br />

Daza did not explain how the scale on the paper was established. Von Rohr has given an alluring<br />

suggestion as to how such a scale might be construed. Spectacle makers knew that multiple lenses of a<br />

given strength could be substituted by a stronger one to reach the same effect. Thus the first position on<br />

the scale was determined by a weak lens <strong>and</strong> the other positions determined by the amount of equal lenses<br />

which had to be put in those positions. Von Rohr, “Versuch”, 4.<br />

38<br />

Bedini & Bennet, “Treatise”.<br />

39<br />

Bedini & Bennet, “Treatise”, 120-121.

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