The retinal image and the theory of lenses (Ad Vitellionem paralipomena)

1604 Light and sky theory

An optical book of 1604 in which vision is explained entirely as optics, and the eye is described as an instrument that can be calculated. Conceived as a supplement to Witelo's Perspectiva, its author, Johannes Kepler, shows that the pupil gathers the light radiating from every point of the object onto the crystalline lens, which refracts it and paints on the retina a real, reversed and inverted image that Kepler calls a pictura. How this picture turns into visual sensation he left to others.

The same book gives the first correct mathematics of the camera obscura, the behaviour of light in media and the rules for constructing images; with them one can also calculate the lenses of spectacles, which by then had been worn for three centuries.

Kepler completed the theory of lenses in another, later work. From there also comes the two-convex-lens design of the telescope, which is still called Keplerian.

Why this date

exact: Ad Vitellionem paralipomena, quibus astronomiae pars optica traditur, Frankfurt, 1604 (MacTutor; Smith 2022). The theory of the retinal image is set out in chapter 5. The plan as a supplement to Witelo took shape earlier: according to the DSB (Gingerich), by 1602 that task had already taken second place to the broader programme of Astronomiae pars optica. The theory of lenses and of the telescope was completed later, in the Dioptrice (Prague, 1611), written within six months of Galileo's Sidereus nuncius (1610); the axis value is 1604, the year of first publication.

What it grew from

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