27 Dec. 1571 in Weil der Stadt - 15 Nov. 1630 in Regensburg
Kepler showed that a planet moves round the Sun in an elliptical orbit which has the Sun in one of its two foci. He also showed that a line joining the planet to the Sun sweeps out equal areas in equal times as the planet describes its orbit. Both these laws were first formulated for the planet Mars, and published in Astronomia Nova (1609). The calculations for the Area Law involved a numerical technique that (with hindsight) resembles integral calculus.
Kepler's third law - that the squares of the periods of planets are proportional to the cubes of the mean radii of their orbits - appeared in Harmonice mundi (1619).
Kepler proved that sight was by the reception of light rays in the eye (1604), and
wrote on the optics of the telescope, introducing the design using two convex lenses
(1611). He also wrote on the new star of 1604 (now called "Kepler's supernova")
(1606), and sent Galileo an enthusiastic endorsement of his
telescopic discoveries (in an open letter published in 1610). Kepler's Epitome
astronomiae copernicanae (1618 to 1621) became a widely used textbook.
His Rudolphine Tables (1627), based on Tycho's observations and Kepler's laws, proved to be accurate over a long time scale. Their success did much to gain general acceptance for heliocentric astronomy.
Kepler also did important work on polyhedra and on logarithms.
Article by: J. V. Field, London, 26 March 1995.
Portrait: current portrait displayed "seems to be a 20th Century sentimentalised portrait - authentic ones are in Kepler's Complete Works (1938), and in Vistas in Astronomy vol.18 (1975)" (J V Field)
Zusätzliche Informationen über Orbits and Gravitation: https://mathshistory.st-andrews.ac.uk/HistTopics/Orbits/