2nd year of post-compulsory secondary education
Gravitational fields
José Luis San Emeterio
 GRAVF 
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Kepler's laws

After the victory of the heliocentric theory, a new prejudice had to be defeated.

Both Copernicus and Galileo assumed that the orbits of the planets had to be circular, because circles are "perfect" shapes.

Kepler was able to defeat this prejudice of "circular perfection" by using the data he obtained from his own observations and those of his master, Tycho Brahe, the last defender of the geocentric theory.

Click on Next to see a visual where you will be able to learn about his discoveries.
Historical background
Freely falling bodies
Two theories of the universe
Kepler's laws
Conclusions
The force of gravity
Newton's law
The superposition of forces
Angular momentum and central force
Conclusions
Field intensity
The concept of field intensity
Variations according to position
Conclusions
Energy in the gravitational field
Gravitational potential energy
Equipotential surfaces and lines of force
Conclusions
Some consequences of the theory
Explanation of the tides
The movement of artificial satellites
Coherence of galaxies
Conclusions
Evaluation