Charles Taylor

Summary

Charles Taylor 1911 Encyclopædia Britannica (1911)

Kepler dearly loves analogies, his most trusty teachers, acquainted with all the secrets of nature, “omnium naturae arcanorum conscios.” And they are to be especially regarded in geometry as, by the use of “however absurd expressions,” classing extreme limiting forms with an infinity of intermediate cases, and placing the whole essence of a thing clearly before the eyes.
Here, then, we find formulated by Kepler the doctrine of the concurrence of parallels at a single point at infinity and the principle of continuity (under the name analogy) in relation to the infinitely great.
Source: Wikisource

Charles Taylor 1911 Encyclopædia Britannica (1911)

Any point P of the parabola, in which the second focus is missing or infinitely distant, is equidistant from the focus B and the line through D which we call the directrix, this taking the place of either circle when its centre C is at infinity, and every line CP being then parallel to the axis. Thus Briggs, and we know not how many “savans géomètres” who have left no record, had already taken up the new doctrine in geometry in its author’s lifetime.
Source: Wikisource

Charles Taylor 1911 Encyclopædia Britannica (1911)

Boscovich’s first principle was that of Kepler, by whose quantumvis absurdis locutionibus the boldest applications of it are covered, as when we say with Poncelet that all concentric circles in a plane touch one another in two imaginary fixed points at infinity. In G. K. Ch. von Staudt’s Geometrie der Lage and Beiträge zur G. der L. (Nürnberg, 1847, 1856–1860) the geometry of position, including the extension of the field of pure geometry to the infinite and the imaginary, is presented as an independent science, “welche des Messens nicht bedarf.” (See Geometry: Projective.)
Source: Wikisource

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