Physics Laws & Theorems
Intermediate

Mass–Energy Equivalence

Mass and energy are equivalent and interconvertible.

Formula

E=mc2E = mc^2

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Variables

mMass
cSpeed of light

Example

The Sun converts about 4 million tonnes of mass into energy every second.

How it works

Mass–energy equivalence says that a body with mass has a huge amount of energy stored in it simply by virtue of existing, because mass is a concentrated form of energy. The factor c^2 is enormous, so even a tiny loss of mass can produce a very large release of energy; this is why nuclear reactions and particle–antiparticle annihilation can be so powerful. It comes from special relativity, which shows that mass and energy are not separate categories but different forms of the same physical quantity.

When to use it

Use this formula when you need to find how much energy is released from a known change in mass, or the equivalent mass of a given amount of energy. It is especially relevant in nuclear physics, particle physics, astrophysics, and any problem involving extremely high-energy processes.

Worked example, step by step

A nuclear reaction converts 0.50 g of mass into energy. Find the energy released. Step 1: Convert the mass to kilograms: m = 0.50 g = 0.00050 kg = 5.0 × 10^-4 kg Step 2: Use c = 3.0 × 10^8 m/s Step 3: Substitute into E = mc^2 E = (5.0 × 10^-4)(3.0 × 10^8)^2 Step 4: Square the speed of light (3.0 × 10^8)^2 = 9.0 × 10^16 Step 5: Multiply E = (5.0 × 10^-4)(9.0 × 10^16) = 4.5 × 10^13 J Final answer: 4.5 × 10^13 joules of energy are released.

Common mistakes to avoid

  • Forgetting to convert grams to kilograms before calculating
  • Using c instead of c^2
  • Thinking the formula applies to ordinary chemical reactions in the same way it does to nuclear reactions

Did You Know?

The Sun converts about 4 million tons of mass into energy every second via E = mc².

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Reviewed & maintained by the FormulaWon editorial teamLast reviewed September 2026