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Johannes Kepler

(1571-1630)


Kepler's life and education:

Johannes Kepler was born in Weil der Stadt in Swabia, 

in southwest Germany. He moved to nearby Leonberg with 

his parents in 1576. His father was a mercenary soldier who 

is believed to have died in the war in the Netherlands.His 

mother was the daughter of an innkeeper; both of his 

grandfathers were mayors. Kepler started his education at a

local school and then attended a nearby seminary. From 

there, he went on to enroll at the University of Tubingen.


There he was taught by one of the leading astronomers Michael 

Maestlin. He introduced him to the new, heliocentric 

cosmological system of Copernicus. The curriculum was geoentric

astronomy: the theory in which all seven planets (Moon, 

Mercury, Venus, Sun, Mars, Jupiter, and Saturn) moved around 

the Earth. However, Kepler did not like this very much. In his 

earliest published work, Mysterium Cosmographicum (1596), he 

considered the actual paths of the planets, not the circles used 

to construct them. In Kepler's writings, he tended to lay his 

opinions on the line. This tendency to openness led the authorities

at Tubingen to doubt his religious orthodoxy. This may explain

why Maestiln persuaded Kepler to give up his plan for ordination 

and, instead, teach mathematics at Graz. Kepler was 

excommunicated in 1612 and never succeeded in getting the ban

lifted. 

Marriage and Death:

Kepler married twice throughout his lifetime. The first seemed to be

for love, however, his wife Barbara died in 1612.They had three 

children; only one Ludwig lived for longer than seven years.The 

second, however, was out of necessity; he needed a wife to watch 

over the children. Her name was Susanna Reuttinger, and they had 

seven children but 3 died at a young age. Kepler eventually died in 

Regensburg, after a short illness. He was buried in the local church, 

but the tomb was destroyed during the Thirty Years' War and 

nothing remains.

Kepler's Writings:

The Harmony of the World, planned in 1599 as a development

of his Mystery of the Cosmos, contains Kepler's Third Law. The 

mathematics in this work contains the first sustematic proof that

there is only thirteen convex uniform polyhera (the Archimedean 

solids. Two non-convex regular polyhedra are also first accounted 

in this writing. IIn 1604 Astronomia pars Optica ("The Optical Part 

of Astronomy") appeared, in which he treated atmospheic refraction 

but also treated lenses and gave the modern explanation of the 

workings of the eye. His first two laws appear in his book 

Astronomia Nova ("New Astronomy"), finished in 1609. Another 

writing by Kepler De Vero Anno quo Aeternus Dei Filius 

Humanam Naturam in Utero Benedictae Virginis Mariae 

Assumpsit (Concerning the True Year in which the Son of 

God assumed a Human Nature in the Uterus of the Blessed Virgin 

Mary") stated Kepler's idea that the Christian calender was in error

by 5 years. He stated that Jesus was actually born in 4 b.c., a 

conclusion that is now universally accepted. He also published 

other writings including Epitome Astronomiae Copernicanae 

("Epitome of Copernican Astronomy") which eventually became

known as the most influential intorduction to heliocentric astronomy.

Before Kepler:

<Ptolemy

The discovery of retrograde motion in the orbit of mars 

was a serious challenge to the standard geocentric cosmology. 

Ptolemy created a theory of all the planets orbitting around the 

earth in the same directoin, with the earth being the center of the 

universe.

View Ptolemy's Theory

Trivia:

As a child, Kepler helped at 
his grandparents' inn by 
serving customers. 

Kepler married his second
wife only to have someone
to look after his children.

Kepler's Laws:

1. The paths of the planets are
ellipses with the center of the
sun at one focus. View Kepler's 
First Law!

2. An imaginary line from the
sun to a planet sweeps out 
equal areas in equal time 
intervals. Thus, planets move
faster when closest to the sun
and slowest when farthest 
the sun. View Kepler's Second 
Law!

3. The ratios of the squares of
the periods of any two planets
revolving about the sun is 
equal to the ratio of the cubes
of their average distances from
 
 


^Kepler's First Law^
 
 
 
 
 
 


^Kepler's Second Law^
 
 
 
 
 
 


^Kepler's Third Law^

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