Keplers 1st Law
Orbit of a planet is an ellipse, with sun at one focus
Keplers 2nd law
A line segment joint a plant and the sun sweeps out equal areas during intervals of equal time.
(because it moves faster when closer to the sun)
Keplers 3rd law
The square of the orbital period is proportional to the cube of the average distance r from the sun
GF & EF
Similarity
Field strength ∝ 1/sep^2
Difference
GF linked to m, EF linked to Q
GF always attractive, EF attractive or repulsive