A List
of Kepler's Firsts
First to
correctly explain planetary motion, thereby, becoming founder of celestial
mechanics and the first "natural
laws" in the modern sense; being universal, verifiable, precise.
In his
book Astronomia Pars Optica, for which he earned the title of founder of modern
optics he was the:
First to
investigate the formation of pictures with a pin hole camera;
First to
explain the process of vision by refraction within the eye;
First to
formulate eyeglass designing for nearsightedness and farsightedness;
First to
explain the use of both eyes for depth perception.
In his
book Dioptrice (a term coined by Kepler and still used today) he was
the:
First to
describe: real, virtual, upright and inverted images and magnification;
First to
explain the principles of how a telescope works;
First to
discover and describe the properties of total internal reflection.
In
addition:
His book Stereometrica Doliorum formed the basis of integral calculus.
First to
explain that the tides are caused by the Moon (Galileo reproved him for this).
Tried to
use stellar parallax caused by the Earth's orbit to measure the distance to
the stars; the same principle as depth
perception. Today this branch of research is called astrometry.
First to
suggest that the Sun rotates about its axis in Astronomia Nova
First to
derive the birth year of Christ, that is now universally accepted.
First to
derive logarithms purely based on mathematics, independent of Napier's tables
published in 1614.
He coined
the word "satellite" in his pamphlet Narratio de Observatis a se quatuor Iovis sattelitibus erronibus
Kepler's
Laws of Planetary Motion Kepler was
assigned the task by Tycho Brahe to analyze the observations that Tycho had made of Mars. Of all the planets, the
predicted position of Mars had the largest errors and therefore posed the greatest problem. Tycho's data were
the best available before the invention of the telescope and the accuracy was good enough for Kepler to show that Mars'
orbit would precisely fit an ellipse. In
1605 he announced The First Law:
Planets
move in ellipses with the Sun at one focus.
The figure
below illustrates two orbits with the same semi-major axis, focus and orbital
period: one a circle with an eccentricity
of 0.0; the other an ellipse with an eccentricity of 0.8.