Audited 31 Jul 2026·Last updated 28 Oct 2026·3 citations·Tier 2·0 uses

Electron Speed Calculator

Find how fast an electron moves from its kinetic energy in electron volts, using the exact relativistic formula valid from a fraction of an eV to the TeV range.

Electron Speed Calculator

eV
Relativistic electron speed
5,930,099.2476
The speed of a free electron with the kinetic energy entered, in meters per second, from the exact relativistic relation.
Model scope
Single free electron kinetic-energy conversion; fields, potential losses, binding energy, scattering, radiation, and velocity direction are outside it.

Background.

Push an electron through 100 volts and it leaves at nearly 6,000 kilometers a second — about 2% of the speed of light — from a voltage you could build on a bench. Electrons are so light that modest energies make them very fast, and that is why the speed has to be worked out with special relativity rather than the schoolbook ½mv².

The deciding number is the electron's rest energy, mₑc², about 511,000 eV. Compared with that, 100 eV is tiny, and the classical formula is only 0.015% off. The error grows quickly: about 0.1% near 700 eV, 1% near 7,000 eV, and 3.6% at 25,000 eV, roughly the voltage that drove a colour television tube. At 511,000 eV the classical formula claims 1.41 times the speed of light, while the true answer is 86.6% of it. Beyond that, extra energy barely moves the speed: a 1 GeV electron travels at 99.999987% of c, and its energy goes into momentum instead.

The calculator therefore uses the exact relations at every energy, from 10⁻¹⁰ eV up to 10¹⁴ eV, so there is no need to decide whether an energy is small enough to treat classically. For an electron that starts at rest and is accelerated through U volts, the kinetic energy in electron volts is simply U, which makes a gun or tube voltage the usual input.

The result describes one free electron carrying exactly the energy you enter. How it got that energy, what it loses along the way, any binding to an atom, scattering, radiation and the direction it travels are all outside the calculation, as the scope note beside the result says.

What is electron speed calculator?

An electron's speed follows from its kinetic energy through the Lorentz factor γ, the ratio of its total energy to its rest energy. Kinetic energy K adds to the rest energy mₑc², so γ = 1 + K ÷ mₑc², and speed follows from γ = 1 ÷ √(1 − v² ÷ c²), rearranged to v = c√(1 − 1 ÷ γ²). The electron volt is the energy one electron gains crossing a potential difference of one volt, exactly 1.602176634 × 10⁻¹⁹ joules. With mₑ = 9.1093837139 × 10⁻³¹ kg from the 2022 CODATA values, the rest energy is 510,998.95 eV.

How to use this calculator.

  1. Enter the kinetic energy in electron volts. For an electron accelerated from rest through a voltage, that is the voltage itself: 100 V gives 100 eV, 25 kV gives 25,000 eV.
  2. Read the speed in meters per second. Dividing by 299,792,458 gives the fraction of light speed, often the more telling figure.
  3. Above about a tenth of light speed, the relativistic result differs noticeably from ½mv², so use it rather than a classical estimate for related calculations.
  4. For momentum or de Broglie wavelength, use p = γmₑv with the same γ, not mₑv; a separate de Broglie calculator handles the wavelength.
  5. The rest energy is fixed for the electron. For a proton or ion, substitute that particle's rest energy in the same formulas instead.

The formula.

γ = 1 + K/(m_ec²); v = c sqrt(1 - 1/γ²)

Special relativity gives a moving particle total energy E = γmₑc², of which mₑc² is present even at rest, so the kinetic energy is K = (γ − 1)mₑc². Solving for γ gives γ = 1 + K ÷ mₑc². The calculator converts K from electron volts to joules with the exact elementary charge, divides by mₑc² computed from the CODATA 2022 electron mass and the exact speed of light, and then applies v = c√(1 − 1 ÷ γ²), the inverse of the Lorentz factor's definition. For small K, expanding the square root gives back ½mₑv² = K, so the classical formula is the low-energy limit of this one rather than a different law. For large K, 1 ÷ γ² shrinks toward zero and v approaches c without reaching it. The result carries 12 significant figures; above roughly 3 × 10¹¹ eV the difference from c falls below that precision, and the display reads exactly 299,792,458 m/s even though the electron is still slower than light.

A worked example.

Example

An electron is accelerated from rest through 100 V, so it carries 100 eV of kinetic energy. The Lorentz factor is γ = 1 + 100 ÷ 510,998.95 = 1.0001957. Squaring and inverting, 1 ÷ γ² = 0.9996087, so 1 − 1 ÷ γ² = 0.00039128, whose square root is 0.019781. Multiplying by c gives v = 0.019781 × 299,792,458 = 5,930,099.2476 m/s, about 5,930 km/s or 1.98% of the speed of light. The classical formula √(2K ÷ mₑ) would have given 5,930,969.58 m/s, only 0.015% higher, which shows how well ½mv² still works at this energy.

kinetic Energy Ev100

Frequently asked questions.

At what energy does an electron need relativity?
There is no sharp switch, only a growing error in the classical formula: about 0.1% near 700 eV, 1% near 7 keV, 3.6% at 25 keV and 14% at 100 keV. Compare the energy with the 511 keV rest energy; once it is more than a percent or so of that, relativistic treatment is needed.
Why does the result show exactly the speed of light at very high energies?
Only because of display precision. Above roughly 3 × 10¹¹ eV the electron's shortfall from c is smaller than the 12 significant figures the result carries. A 1 GeV electron, for comparison, is still visibly short at 299,792,418.899 m/s — about 39 m/s slower than light.
How fast were the electrons in the Davisson–Germer experiment?
Davisson and Germer's famous diffraction peak used 54 eV electrons scattered off nickel. Entering 54 gives 4,358,009.3528 m/s, about 1.45% of light speed, and a de Broglie wavelength of about 0.167 nm — similar to the spacing between atoms in a crystal, which is why diffraction appeared.
What does relativity change in an electron microscope?
Mainly the wavelength, which sets resolution. At 100 keV the electron has γ = 1.1957 and moves at 54.8% of light speed; its relativistic wavelength is 3.70 pm, against 3.88 pm from a classical calculation. Microscopes running at 100 to 300 kV must be designed with the relativistic value.
Can I use this for protons or ions?
Not directly, because the electron's rest energy is built in. A proton is about 1,836 times heavier, so at 100 eV it moves at only about 138 km/s and stays well described by classical mechanics to far higher energies. The same two formulas apply with the proton's rest energy substituted.
Does this give the speed of an electron inside an atom?
No — bound electrons are outside the model. In hydrogen's ground state the electron's average kinetic energy is about 13.6 eV, and entering 13.6 returns roughly c ÷ 137, the speed Bohr's model assigned, but quantum mechanics gives a bound electron a spread of speeds rather than a single orbit speed.

How this page was produced

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Quanta Calculator
Primary sources
3 cited below
Method
γ = 1 + K/(m_ec²); v = c sqrt(1 - 1/γ²)
Published
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