A universal attraction between any 2 masses
F = -GMm/r²
G = gravitational constant
A line that indicates the direction of the gravitational force that would act on a test mass in a field
A mass small enough to not affect the shape of a gravitational field with its own gravity
The gravitational force per unit mass
g = F/m
g = -GM/r²
The closest point to the sun in orbit
The furthest point from the sun
The orbit of every planet is an elipse with the sun at one of the foci
A line segment joining a planet & the sun sweeps out equal areas during intervals of time
The square of the orbital period of a planet is directly proportional to the cube of its average distance from the sun
- 1 day/ 24hours
They travel in the same direction as the earth rotation(along the equatorial plane)
An object that orbits another object
- Telecommunications(e.g. TV broadcasts)
- Surveying(e.g. weather)
v = √GM/r
The work done per unit mass to move an object to that point from infinity
V = -GM/r
The work done per unit mass to remove an object from a field
The work done to move a mass to a point in a field from infinity
E = -GMm/r
v = √2GM/r