Relativistic Kinetic Energy Calculator

Enter an object's mass and velocity to calculate its relativistic kinetic energy — the true kinetic energy at speeds approaching the speed of light. You get the relativistic KE, the Lorentz factor (γ), the classical KE for comparison, and the relativistic momentum. The formula used is K = mc²(γ − 1), where γ = 1/√(1 − v²/c²).

kg

Mass of the object in kilograms

c

Enter velocity as a fraction of the speed of light (0 to < 1). E.g. 0.9 means 90% of c.

Results

Relativistic Kinetic Energy

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Lorentz Factor (γ)

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Classical Kinetic Energy (½mv²)

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Relativistic Momentum

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Velocity

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Relativistic / Classical KE Ratio

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Relativistic vs Classical Kinetic Energy

Frequently Asked Questions

What is relativistic kinetic energy?

Relativistic kinetic energy is the energy an object possesses due to its motion, calculated using Einstein's special theory of relativity. Unlike classical kinetic energy (½mv²), it accounts for the fact that mass effectively increases as an object approaches the speed of light. The formula is K = mc²(γ − 1), where γ is the Lorentz factor.

What is the relativistic formula for kinetic energy?

The relativistic kinetic energy formula is K = mc²(γ − 1), where m is the rest mass, c is the speed of light (~2.998 × 10⁸ m/s), and γ (the Lorentz factor) = 1/√(1 − v²/c²). This reduces to the classical formula ½mv² at low speeds, confirming it as a generalization of Newtonian mechanics.

What happens to relativistic kinetic energy at low velocities?

At velocities much less than the speed of light (v ≪ c), the relativistic formula converges to the classical kinetic energy expression ½mv². The Lorentz factor γ approaches 1, so the relativistic and classical values become nearly identical. As a rule of thumb, classical KE is a good approximation when v < 1% of c.

Can relativistic kinetic energy be negative?

No. Relativistic kinetic energy is always zero or positive. Since the Lorentz factor γ is always ≥ 1 for any real velocity (0 ≤ v < c), the quantity (γ − 1) is always ≥ 0. A kinetic energy of zero means the object is at rest.

Can an object reach the speed of light?

No object with mass can reach or exceed the speed of light. As velocity approaches c, the Lorentz factor γ approaches infinity, meaning the energy required to accelerate the object also approaches infinity. This is why only massless particles, like photons, can travel at exactly c.

How do I calculate the relativistic kinetic energy of an electron at 0.990c?

An electron has a rest mass of about 9.109 × 10⁻³¹ kg. At v = 0.990c, the Lorentz factor γ = 1/√(1 − 0.990²) ≈ 7.089. The relativistic KE = mc²(γ − 1) ≈ 9.109×10⁻³¹ × (3×10⁸)² × (7.089 − 1) ≈ 4.99 × 10⁻¹³ J. Enter these values into the calculator above to verify.

What is the Lorentz factor and why does it matter?

The Lorentz factor γ = 1/√(1 − v²/c²) is a dimensionless quantity central to special relativity. It quantifies how much time dilation, length contraction, and mass-energy increase occur at a given velocity. At v = 0, γ = 1 (no relativistic effects). At v = 0.99c, γ ≈ 7.09, meaning relativistic effects are dramatic.

How is relativistic momentum related to relativistic kinetic energy?

Relativistic momentum is p = γmv, and it is related to total energy via the energy-momentum relation: E² = (pc)² + (mc²)². The kinetic energy is then K = E − mc² = √((pc)² + (mc²)²) − mc². This calculator also outputs relativistic momentum so you can explore both quantities simultaneously.

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