2000 HSS/PSA Program 1 - History of Science Society
2000 HSS/PSA Program 1 - History of Science Society
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 />
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