Unit 4: Planetary Motion

KE = 1/2(mass x velocity^2)

PE = mass x 9.8 m/s^2 x height

Force = mass x acceleration

E = distance between foci/major axis

Momentum = mass x velocity

p = mv

Force of Gravity = (G x m1 x m2)/d^2

G = 6.673 x 10^-11 N m^2/kg^2

1. Law of Ellipses

2. Law of Equal Areas

3. Law of Harmonies

The path of the planets about the Sun is elliptical in shape

Center of Sun is one focus

Eccentricity = distance between foci/width of ellipse

Closer foci = more circular

Describes the speed at which any given planet will move while orbiting the sun

A planet moves fastest when closer to the sun (perihelion) and slowest when farthest from sun (aphelion)

Triangles are equal throughout orbit but some wider and shorter and some skinnier and taller

Compares the orbital period and radius of orbit (distance from sun) of a planet to those of other planets.

Comparison of planet/satellite speeds

Period^2 = Distance from Sun^3

1. Law of Inertia

2. F = ma

3. Law of action and reaction

An object at rest remains at rest and an object in motion maintains its velocity unless it experiences an unbalanced force

Inertia: the tendency of an object at rest to remain at rest or continue moving with a constant velocity.

Force = mass x acceleration Measured in Newtons

Acceleration = change in velocity (speed or direction)

Balanced: force = 0

For every action force, there is an equal and opposite reaction force

Forces are equal and opposite but not balanced because two different objects are involved

Some forces are from contact and others are from action-at-a-distance interactions (like gravitational)

The force of gravitational attraction is directly dependent upon the masses of both objects and inversely proportional to the square of the distance that separates their centers.

Mass increases = force of gravity increases

Greater separation distance = weaker gravity

Apophis orbit is very circular

Orbit speeds up when closer to the sun (higher gravity)

Will remain in this motion unless acted on by unbalanced force (it was and path is changed)

Any force that pulls or pushes an object towards the center of the circle

For objects moving a a circular motion, there is a net force acting towards the center

An object moving in circles requires there to be an unbalanced force (like gravity)

The motion of an object in a circle at a constant speed

As objects move in circles, they constantly change direction, therefore accelerating

Centripetal force is occurring

Stored energy or energy held in readiness

Elastic: energy stored in any type of stretched or compressed material

Gravitational: stored energy that depends on height and mass. Affected more by height

PE = Mass x 9.8 m/s^2 x height

Energy that an object has because it’s in motion

Depends on mass and velocity (affected more by velocity)

Small increase in velocity = large increase in energy

Energy cannot be created or destroyed but can be transferred

Energy Conversions: energy transfers or changes form to another type of energy

Total energy in the system stays the same

Total momentum is maintained in a collision