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Inside the fusion drive

Zoom from the whole ship to one nucleus and watch 0.39% of the fuel's mass leave as motion.

See it in the tour: chapter long passage, shot 0.7.

The deep zoom in the tour has four rungs. This page walks them in order and then does the arithmetic the last one only shows.

Step 1: the ship

Two drums at the left, a cluster of tanks and orange radiator strips along the truss, the round shield at the right and a violet plume streaming away.
The whole ship under power. Two drums at the left, a cluster of tanks and orange radiator strips along the truss, the round shield at the right and a violet plume streaming away.

The Long Passage is 650 m long and 122 m across design. Her engine sits at the stern, far from the people. It pushes with 63.7 kN, an exhaust speed of 200 km/s and 10.6 GW of fusion power challenge. Everything else on the truss, the shield, the radiators, the tanks, exists to serve or to hide that one machine.

Step 2: the magnetic nozzle

A magnetic field holds the plasma column off the walls.
Deep zoom: the magnetic nozzle. A magnetic field holds the plasma column off the walls.

At the scale of ten metres the engine is a ring of three superconducting coils, 13 m in radius design. No solid wall could touch the plasma inside. A charged particle cannot cross a magnetic field line, it spirals along it physics. So the field is the container, and the same field, opening toward the stern, is the nozzle challenge.

Step 3: the plasma

Deuterium and helium-3 nuclei at fusion temperature.
Deep zoom: inside the plasma. Deuterium and helium-3 nuclei at fusion temperature.

At ten centimetres the column is a gas of bare nuclei, deuterium and helium-3, at hundreds of millions of kelvin physics. Both carry positive charge and repel each other. Only the fastest pairs get close enough for the short-range nuclear force to win. Most meetings change nothing, and the nuclei spiral on until the next one physics.

Step 4: the nuclei

Two nuclei fuse and the products weigh a little less than the reactants, the difference leaving as energy.
Deep zoom: mass becomes energy. Two nuclei fuse and the products weigh a little less than the reactants, the difference leaving as energy.

The last rung is drawn at 10⁻¹⁵ m. A deuteron and a helion merge and two things leave: a helium-4 nucleus and a proton illustrative. The picture is a diagram, not a photograph. The arithmetic behind it is not.

The mass defect, worked

1 Weigh2 Convert3 ShareFuel D + ³He2.014102 + 3.016029 = 5.030131 uProducts ⁴He + p4.002603 + 1.007825 = 5.010428 uMissing: 0.019703 u (0.39%)E = Δm × c²0.019703 u × 931.494 MeV/u1 u of mass is 931.494 MeVfrom the atomic mass unit and c= 18.35 MeVEqual and opposite momentum:the light proton takes the largershare of the energyproton 4.003 / 5.01080% to the proton⁴He 3.69 MeVproton 14.66 MeVWhere the 18.35 MeV goesBoth products carry charge, so the magnetic nozzle can steer both. A neutron would carry its share straight out of the field.Atomic masses from AME, as in the DZ3 script. Non-relativistic split with the fuel at rest.
Weigh the fuel and the products, convert the missing 0.019703 u to 18.35 MeV, and momentum hands 80% of it to the proton and the rest to the helium-4 nucleus. physics illustrative
  1. Weigh the fuel. Deuterium is 2.014102 u and helium-3 is 3.016029 u, 5.030131 u together physics.
  2. Weigh the products. Helium-4 is 4.002603 u and a proton, as a hydrogen atom, is 1.007825 u, 5.010428 u together physics.
  3. Subtract. The products weigh 0.019703 u less, 0.39% of the fuel physics.
  4. Convert. One atomic mass unit is 931.494 MeV, so the missing mass is 18.35 MeV physics.
  5. Share. The fuel starts nearly at rest, so the two products leave with equal and opposite momentum. The light proton moves fast and takes about 80% of the energy, 14.7 MeV. The helium nucleus takes the other 3.7 MeV physics.

Both products are charged, so the magnetic nozzle can steer both. That is the whole case for this fuel. A neutron would take its share straight through the coils, which is the subject of Shadow shields and neutrons.

What one kilogram buys

Per kilogram of fuel the reaction gives 3.5 × 10¹⁴ J physics. A crossing burns about 371 kg challenge. Compare that with chemistry on Energy per kilogram, and see where the fuel comes from in Helium-3 from Saturn and Deuterium from ice.

Key numbers

QuantityValueBasis
Fuel mass, D + ³He5.030131 uphysics
Product mass, ⁴He + p5.010428 uphysics
Mass lost0.019703 u, 0.39%physics
Energy released18.35 MeVphysics
Proton / helium-4 share14.7 MeV / 3.7 MeVphysics
Nozzle coils3, 13 m radiusdesign
Thrust / exhaust speed63.7 kN / 200 km/schallenge
Fusion power10.6 GWchallenge

Sources