Newtons universal law of gravitation
“Every single point mass attracts every other point mass with a force that is directly proportional to the product of their masses and inversely proportional to the square of their separation.”
Point mass
A mass which doesn’t take up any space (infinitely small).
Gravitational Field
A region of space where a mass experiences a force because of its mass
Gravitational field strength
The force per unit mass experienced by a small point mass placed at that point
Field strength on a point mass in between two larger objects
The field strength at that point is the sum of the individual field strengths
Orbital motion
The motion of one body around another, it has a curved path
Keplers first law
Planets move on ellipses with the sun at one of the foci of the ellipse
Perihelion
The point at which a planet in elliptical orbit will be closest to the sun
Aphelion
The point at which a planet in elliptical orbit will be furthest away from the sun
Keplers second law
The line joining a planet and the sun sweeps equal areas in equal times
Formula showing planets move faster at the perihelion
Vp/Va=SA/SP
Keplers Third law
The square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit.