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These physical laws are the foundation to understanding the motion of satellites and planets.


Physical Laws

Law of conservation of energy states that in a conservative field total mechanical energy is constant. Total mechanical energy is the sum of potential and kinetic energy of an object.

Newton's Laws

1. A body remains at rest or in motion with constant velocity unless acted on by a force.

2. The time rate of change of a body's momentum equals the net applied force. Momentum is the product of body mass and velocity.

3. For every action there is an equal and opposite reaction.

Law of conservation of momentum, an implication of Newton's Third Law, states that the momentum of a system is always conserved. If the applied net force is zero, then linear momentum is conserved; if the torque is zero, then angular momentum is conserved.

Kepler's Laws

1. The orbit of a planet is the shape of an ellipse with the Sun at one of the two foci.

2. The line from a planet to the Sun sweeps out equal areas in equal times.

3. The square of an orbit's period is proportional to the cube of its semimajor axis.

 

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