Relativistic Velocity Addition Calculator
Adding Velocities in Special Relativity
In classical (Newtonian) physics, if you are on a train moving at velocity u and you throw a ball forward at velocity v' relative to the train, an observer on the ground would see the ball moving at u + v'. However, this simple addition breaks down at speeds approaching the speed of light (c).
Einstein's Special Theory of Relativity provides a different formula for adding velocities. This formula ensures that the resultant velocity never exceeds the speed of light, which is a fundamental postulate of the theory.
How to use this calculator:
- Enter Velocity u: This is the velocity of a moving reference frame S' (e.g., a spaceship) relative to a stationary frame S (e.g., Earth).
- Enter Velocity v': This is the velocity of an object (e.g., a probe, or light pulse) relative to the moving frame S' (the spaceship).
- Velocities can be positive (in the chosen direction) or negative (opposite direction).
- Click "Calculate Resultant Velocity".
- The result will be v: the velocity of the object as observed from the stationary frame S (Earth).
Theory & Formula
The relativistic formula for adding velocities along the same line (collinear velocities) is:
Where:
- v: The resultant velocity of the object as measured in the stationary frame S. This is what we are calculating.
- u: The velocity of the moving frame S' relative to the stationary frame S. (Your first input)
- v': The velocity of the object as measured in the moving frame S'. (Your second input)
- c: The speed of light in a vacuum (approximately 299,792,458 m/s).
Key Implications:
- If u and v' are much smaller than c, the denominator (1 + uv'/c2) is very close to 1, and the formula approximates the classical v = u + v'.
- If either u or v' is c (e.g., adding the velocity of light), the resultant velocity v will also be c. This means the speed of light is constant for all inertial observers, regardless of the motion of the source.
- It is impossible to accelerate an object with mass to the speed of light, and this formula inherently prevents the resultant velocity from exceeding c if u < c and v' < c.
Calculator Inputs
Calculation Results
Resultant Velocity (v) (Object relative to Frame S, e.g., Probe relative to Earth):
m/s
c (fraction of speed of light)