The equations of motion describe the mathematical relationship between the motion of an object and the forces acting on it.

They are fundamental in physics and engineering, providing a framework to analyse how objects move under various conditions.
1. Newton’s Second Law (General Form)
This is the foundation of the equations of motion:
Where:
Net force acting on an object (N)
Mass of the object (kg)
Acceleration of the object (m/s^2)
It states that the acceleration of an object is directly proportional to the net force acting on it and inversely proportional to its mass.
2. Kinematic Equations (Constant Acceleration)
These equations are used to describe the motion of an object under constant acceleration, such as free-fall or uniform acceleration. They relate displacement (), velocity (
), acceleration (
), and time (
).
a. First Equation
Where:
Final velocity (m/s)
Initial velocity (m/s)
Acceleration (m/s^2)
Time (s)
b. Second Equation
Where:
Displacement (m)
c. Third Equation
d. Fourth Equation (Average Velocity)
3. Rotational Motion (Angular Equivalents)
For rotational systems, the equations of motion have analogues in terms of angular quantities:
Where:
Torque (Nm)
Moment of inertia (kg·m^2)
Angular acceleration (rad/s^2)
The kinematic equations also have rotational counterparts:
Angular displacement (rad)
Angular velocity (rad/s)
Angular acceleration (rad/s^2)
Time (s)
For example:
4. Lagrangian and Hamiltonian Mechanics
For advanced systems, especially in multiple dimensions, motion is described using energy principles:
- Lagrangian Mechanics: Based on the Lagrangian function,
, where
kinetic energy and
potential energy.
- Hamiltonian Mechanics: Based on the total energy of the system,
.
These approaches use generalised coordinates and provide powerful tools for analysing complex systems.
Applications
- Predicting the trajectory of projectiles
- Designing mechanisms in mechanical engineering
- Studying planetary orbits and satellite motions
- Analysing the dynamics of rotating machinery