Fission vs Fusion — Two Ways to Release Nuclear Energy

Nuclear Fission

A heavy nucleus (like uranium-235) splits into lighter nuclei when struck by a neutron, releasing energy plus more neutrons that can sustain a chain reaction. One U-235 fission releases about 200 MeV.

E=Δmc2E = \Delta m c^2

Unit: mega-electronvolt (MeV)

Example: Today's nuclear power plants fission uranium-235: each split releases neutrons that split further nuclei, and the heat makes steam for turbines.

Nuclear Fusion

Light nuclei (like deuterium and tritium) combine into a heavier nucleus, releasing energy. The Sun does this — fusing ~600 million tonnes of hydrogen every second. A D–T fusion releases about 17.6 MeV.

E=Δmc2E = \Delta m c^2

Unit: mega-electronvolt (MeV)

Example: Experimental reactors like ITER heat hydrogen isotopes past 100 million °C, trying to make fusion release more energy than it consumes.

Key differences

AspectNuclear FissionNuclear Fusion
What happensHeavy nucleus splits into lighter onesLight nuclei merge into a heavier one
FuelUranium-235, plutonium-239 (rare, mined)Hydrogen isotopes (abundant in seawater)
ConditionsRoom temperature; needs neutron moderation and control rodsOver 100 million °C plasma confined by magnets or lasers
WasteLong-lived radioactive fission productsMostly helium; reactor parts become mildly radioactive
Energy per reaction~200 MeV per U-235 split~17.6 MeV per D–T fusion (but far more reactions per kg of fuel)
StatusCommercial power since the 1950sStill experimental — net energy gain only just demonstrated
Why students confuse them

Both are 'nuclear energy' but they are opposites on the binding-energy curve: fission climbs down from the heavy end, fusion climbs up from the light end, and iron sits at the peak where neither releases energy.