He felt that Ptolemy's model was to complicated
In his time data was still based on observation with the naked eye
He adopted Ptolemy's idea that planetary paths should be perfect circles
Like Ptolemy he used a "wheels-on-wheels" system
The heliocentric model of Copernicus is generally seen as the first step in the development of modern models of the solar system
He then tried other types of paths and found that ellipses fit best
Kelper formulated 3 principals which today are known as Kelper's laws
1st law states that planetary orbits are ellipses with the sun at one focus
2nd law states that planets move faster in their orbits when closer to the sun
3rd law relates the distance of a planet from the sun to the time it takes to go once around its orbit
He made scientific improvements to the newly invented telescope
He observed the moons Io, Europa, Callisto, & Ganymede orbiting Jupiter- today these moons are known as the Galilean Satellites
His observations showed that Earth was not the only object that could be orbited-this gave support to the heliocentric model
He also observed that Venus went through phases like the Earth- because where the sun hits Venus