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2000 HSS/PSA Program 1 - History of Science Society

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Yaakov Zik University <strong>of</strong> Haifa, Israel<br />

<strong>HSS</strong> Abstracts<br />

Beyond the Naked Eye<br />

Historians <strong>of</strong> science commonly describe Kepler as the father <strong>of</strong> modern<br />

geometrical optics. Kepler clarified the foundation <strong>of</strong> optics and solved a series<br />

<strong>of</strong> problems that had confounded his predecessors: the problem <strong>of</strong> vision, the<br />

camera obscura and the geometrical theory <strong>of</strong> the telescope. Kepler’s books<br />

on optics, Ad Vitellionem Paralipomena (1604), which is solidly based upon a<br />

medieval foundation and Dioptrice (1611) which is considered to be the first<br />

treatise in modern geometrical optics, are the mile stones <strong>of</strong> his optical work.<br />

However, careful analysis <strong>of</strong> related texts and events, will clearly show that<br />

something in the above description is missing. In 1604, while Kepler was<br />

working on the Paralipomena, he disparaged the telescope most vigorously.<br />

The first time Kepler understood the potential <strong>of</strong> this instrument as a scientific<br />

device was after he had read about Galileo’s discoveries, published in the<br />

Sidereus Nuncius (March 1610). Kepler wrote the Conversation with Galileo’s<br />

Sidereal Messenger (an answer to the Sidereus Nuncius) in April 1610 and<br />

from the way he described the construction <strong>of</strong> the telescope, it was clear that<br />

he had not understood the importance <strong>of</strong> the focal length ratio and how the<br />

magnification was determined. By the end <strong>of</strong> August 1610 he got a telescope,<br />

made by Galileo, with which he was able to see Jupiter and its satellites. In<br />

late September 1610 Kepler completed his Dioptrice (which was published in<br />

the beginning <strong>of</strong> 1611). The chronological course <strong>of</strong> events strongly suggests<br />

that Kepler’s reading <strong>of</strong> Sidereus Nuncius was not enough for him to understand<br />

the optical principles <strong>of</strong> the telescope. Only after examining and employing a<br />

telescope made by Galileo, was Kepler able to exploit the technical details<br />

and to learn how it works. It appears that the whole story deserves a reexamination.<br />

On the one hand it seems that Galileo must have known something<br />

about the science <strong>of</strong> optics and that we have underestimated his knowledge at<br />

our peril. On the other hand Kepler needed the knowledge that Galileo had<br />

attained, as reflected by his inability to construct the telescope, much more<br />

than what historians <strong>of</strong> sciences have been willing to accept. In this paper I<br />

shall argue that there are more key figures in this story and that its various<br />

aspects have not been properly appreciated up to this very day. Moreover,<br />

most <strong>of</strong> the theoretical aspects regarding the phenomena <strong>of</strong> light, vision, and<br />

lens properties necessary for the construction <strong>of</strong> the telescope (with the<br />

exception <strong>of</strong> the law <strong>of</strong> refraction which is in any event not essential to our<br />

case), had been at hand even before the time when Kepler addressed himself<br />

seriously to optics. I shall claim that over and above the actual building <strong>of</strong> the<br />

telescope it was Galileo who put all the theoretical pieces together. In my<br />

paper, I shall present a few aspects <strong>of</strong> the claim that in Galileo one finds a<br />

fusion <strong>of</strong> practical and theoretical knowledge which is crucial for the<br />

construction <strong>of</strong> an instrument that is also a bearer <strong>of</strong> theory.<br />

H<br />

S<br />

S<br />

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