A Hall effect thruster is a form of electric propulsion used on satellites and deep-space probes. Xenon gas is fed into an annular ceramic channel where a hot cathode supplies electrons that ionize the propellant. A radial magnetic field traps those electrons, forcing them into a circulating "Hall current" instead of drifting straight to the anode. That trapped electron cloud sets up a strong axial electric field, which accelerates the much heavier xenon ions out of the channel at high speed to produce thrust.
Hall thrusters get their name from the Hall effect discovered by Edwin Hall in 1879 — the same underlying E×B drift physics used here to trap electrons was originally observed as a sideways voltage across a current-carrying conductor in a magnetic field.
A cutaway of a Hall effect thruster's annular discharge channel, where ionized xenon spirals under a radial magnetic field and accelerates axially under the induced electric field to form a glowing exhaust plume.
Electrons trapped by the radial magnetic field circulate as a Hall current, building the axial electric field that accelerates heavier xenon ions straight out of the channel — the crossed-field mechanism behind real electric propulsion.
Adjust magnetic field strength, propellant flow, and discharge voltage to see how ion spiral rate, exhaust velocity, and simulated thrust respond. Toggle the field-line overlay and channel cutaway to see inside.
Hall thrusters have propelled missions like ESA's SMART-1 to the Moon and are used for station-keeping on hundreds of communications satellites, running for thousands of hours on only a few kilograms of xenon.