Circular Motion of Charged Particles

When a charged particle moves through a uniform magnetic field with its velocity directed perpendicular to the field lines, it experiences a continuous magnetic force that is always perpendicular to its motion. This perpendicular force does no work on the particle — it cannot change the particle's speed — but it constantly redirects the particle's velocity, causing it to travel in a perfect circle. This phenomenon is called circular motion of a charged particle in a magnetic field, and it underlies technologies from particle accelerators to mass spectrometers. The key insight is that the magnetic force acts as the centripetal force for the circular orbit. The radius of this circular path depends on the particle's mass, charge, speed, and the strength of the magnetic field. Heavier or faster particles curve less; stronger fields or larger charges cause tighter curves. By measuring the radius of curvature in a known magnetic field, physicists can determine a particle's charge-to-mass ratio — a technique that was central to the discovery of the electron. Understanding this concept requires combining knowledge of the magnetic force law (the Lorentz force), Newton's second law, and centripetal acceleration. Mastery of circular motion in magnetic fields is essential for topics such as cyclotrons, the Hall effect, and the behavior of plasma in fusion reactors. The mathematics is clean and elegant, making this one of the most satisfying applications of classical electromagnetism at the high school level.

Key takeaways
  • The Magnetic Force on a Moving Charge
  • Setting the Magnetic Force Equal to the Centripetal Force
  • Period and Frequency of Circular Motion
  • Direction of Circular Motion

The Magnetic Force on a Moving Charge

The force on a charge qq moving with velocity v⃗\vec{v} in a magnetic field B⃗\vec{B} is given by the Lorentz force law: F⃗=qv⃗×B⃗\vec{F} = q\vec{v} \times \vec{B}. The magnitude is F=qvBsin⁡θF = qvB\sin\theta. When the velocity is perpendicular to the field (θ=90°\theta = 90°), this simplifies to F=qvBF = qvB. This force is always perpendicular to v⃗\vec{v}, so it cannot do work (recall W=F⃗⋅d⃗W = \vec{F} \cdot \vec{d}, and a perpendicular force has zero component along displacement). The particle's speed stays constant, but its direction changes continuously.

Setting the Magnetic Force Equal to the Centripetal Force

For any object moving in a circle of radius rr at speed vv, Newton's second law requires a centripetal force Fc=mv2rF_c = \frac{mv^2}{r} directed toward the center. Since the magnetic force provides exactly this centripetal force, we set them equal: qvB = \frac{mv^2}{r}. Solving for rr, we divide both sides by vv (since v≠0v \neq 0) and rearrange to get r=mvqBr = \frac{mv}{qB}. This is the fundamental equation for the radius of a charged particle's circular orbit in a magnetic field.

Period and Frequency of Circular Motion

The time for one complete revolution is the period TT. Since the particle travels a circumference 2πr2\pi r at constant speed vv, we have T=2πrvT = \frac{2\pi r}{v}. Substituting r=mvqBr = \frac{mv}{qB} gives T = \frac{2\pi m}{qB}. Remarkably, the period is independent of the particle's speed! Faster particles travel larger circles but complete orbits in the same time. The cyclotron frequency (number of orbits per second) is f=1T=qB2πmf = \frac{1}{T} = \frac{qB}{2\pi m}. This speed-independence is the principle behind the cyclotron particle accelerator.

Direction of Circular Motion

The direction of the circular orbit depends on the sign of the charge and the direction of B⃗\vec{B}. Using the right-hand rule for v⃗×B⃗\vec{v} \times \vec{B}: point fingers in the direction of v⃗\vec{v}, curl them toward B⃗\vec{B}, and the thumb points in the direction of the force on a positive charge. A negative charge (like an electron) experiences the opposite force direction and curves the other way. If B⃗\vec{B} points into the page and v⃗\vec{v} points to the right, a proton curves upward initially and orbits counterclockwise; an electron orbits clockwise.

The Key Equation

r=mvqBr = \frac{mv}{qB}
  • r — Orbital radius (metres (m)): The radius of the circular path traced by the particle in the magnetic field.
  • m — Mass of particle (kilograms (kg)): The inertial mass of the charged particle; larger mass means larger radius.
  • v — Speed of particle (metres per second (m/s)): The constant speed of the particle; the magnetic force cannot change this value.
  • q — Charge of particle (coulombs (C)): The magnitude of the particle's electric charge; larger charge means smaller radius.
  • B — Magnetic field strength (tesla (T)): The magnitude of the uniform magnetic field; stronger fields produce tighter orbits.

Worked Example

Problem. A proton (mass mp=1.67×10−27m_p = 1.67 \times 10^{-27} kg, charge q=1.60×10−19q = 1.60 \times 10^{-19} C) travels at 3.0×1063.0 \times 10^6 m/s perpendicular to a uniform magnetic field of strength B=0.25B = 0.25 T. (a) Calculate the radius of its circular orbit. (b) Calculate the period of the orbit.

r≈0.125 m,T≈2.62×10−7 sr \approx 0.125 \text{ m}, \quad T \approx 2.62 \times 10^{-7} \text{ s}

Answer. The proton orbits with radius approximately 12.5 cm and completes one full orbit in approximately 262 nanoseconds.

Figure
Diagram
Circular Motion of a Proton in a Magnetic FieldMagnetic field B directed into the page (shown by × symbols)××××××××××××××××××××××××××××××××××××××××rp⁺vFp⁺vFp⁺vFCentre■Velocity (v) — tangent to circle■Magnetic Force (F) — toward centre— —Circular orbit× B field into page
Origins · 1 minJ. J. Thomson and how this was discovered
JJ
J. J. Thomson
1856–1940 · British

Joseph John Thomson discovered the electron in 1897 by studying cathode rays bent by electric and magnetic fields. By measuring the radius of curvature of the electron beam in a known magnetic field and applying the equation r=mvqBr = \frac{mv}{qB}, he determined the charge-to-mass ratio eme\frac{e}{m_e} of the electron — the first subatomic particle ever identified. This experiment is a direct application of charged particle circular motion. Thomson won the Nobel Prize in Physics in 1906 for discovering the electron, and his son George Paget Thomson won the same prize in 1937 — for demonstrating that electrons behave as waves. Father proved the particle; son proved the wave!

  • The Lorentz Force Law — The magnetic component of the Lorentz force, F⃗=qv⃗×B⃗\vec{F} = q\vec{v} \times \vec{B}, is the fundamental force that causes circular motion in a magnetic field. Understanding vector cross products and the right-hand rule is essential prerequisite knowledge.
  • Centripetal Acceleration and Force — The derivation of orbital radius sets the magnetic force equal to the centripetal force Fc=mv2rF_c = \frac{mv^2}{r}. A solid understanding of circular motion mechanics is required to follow and apply this derivation correctly.
  • The Mass Spectrometer — Mass spectrometers use circular motion in magnetic fields to separate ions by mass. By measuring orbital radii, scientists determine atomic masses with extreme precision — a direct technological application of r=mvqBr = \frac{mv}{qB}.
  • The Cyclotron Particle Accelerator — The cyclotron exploits the fact that the orbital period T=2πmqBT = \frac{2\pi m}{qB} is independent of speed, allowing particles to be accelerated in synchrony with an alternating electric field as they spiral outward in a magnetic field.