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Lorentz Force Calculator

The force on a charged particle moving through a magnetic field — and the radius and period of the circle it is bent into, which is how mass spectrometers, cyclotrons and the aurora all work.

A charge moving across a magnetic field feels a force qvB at right angles to both its velocity and the field.

Results update as you type
Results
Force (N)
8.0109e-14
Radius of the circular path (m)
Period of one orbit (s)
Cyclotron frequency (Hz)
Centripetal acceleration (m/s²)
Kinetic energy (eV)
Radius an electron would have at the same speed (m)
Reading
Reviewed September 2026. Physics is the same everywhere: SI units in, with imperial equivalents in the results.
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About lorentz force

How the lorentz force calculator works

A charge moving across a magnetic field feels a force qvB at right angles to both its velocity and the field. Because the force is always perpendicular to the motion it does no work: the particle keeps its speed and curves into a circle of radius mv/qB.

The period of that circle, 2πm/qB, does not depend on speed at all. That single fact is what makes a cyclotron possible.

Formula: F = q v B sin θ; r = m v / (q B); T = 2π m / (q B)

Worked examples

InputsForce (N)Note
A proton at 1,000 km/s in 0.5 T8.0109e-14a 2 cm circle
A stronger field3.2044e-13a quarter of the radius
Along the field0no force at all

Frequently asked questions

What is the Lorentz force?

The force on a charge from electric and magnetic fields. This page takes the magnetic part, qv × B, which is what bends a moving charge into a curve.

Why does the particle not speed up?

Because the force is always at right angles to the velocity, so it does no work. It changes direction only, which is why the path is a circle.

Why does the period not depend on speed?

A faster particle makes a bigger circle, and the two effects cancel exactly. The cyclotron exploits that: the same frequency accelerates the particle on every turn.

How does a mass spectrometer use this?

Ions of the same speed and charge curve by a radius proportional to their mass. Heavier ions land further along the detector.

What about the aurora?

Charged particles from the sun spiral along the Earth's field lines — the helix case here — and strike the atmosphere near the poles where the lines come down.

Where these figures come from

Last checked: September 2026. Constants are the CODATA 2018 values; formulas are the standard textbook forms.