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Always isotopes of hydrogen combine to make helium.

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U-235 and Pu-239 only. No other isotopes are fissionable

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bombardment

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spontaneous
natural decay
decay
alpha decay, beta decay, etc.

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Laser inertial confinement (National Ignition Facility)

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Beta decay
Positron decay

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Magnetic confinement (ITER)

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Fusion is how all stars produce their energy

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Mass number and atomic number must be balanced on both sides of the equation

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Reactions require high temperature to give the positively charged nuclei the energy they require to overcome their mutual repulsion 

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Reactions require high temperature to give the positively charged nuclei the energy they require to overcome their mutual repulsion 

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Atomic Numbers and mass numbers still must be balanced on each side of the equation!

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slow moving neutrons hit the the nucleus to split it

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Physics - Nuclear Fission reaction explained - Physics

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Results in two separate elements and remaining neutrons.

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Results in two separate elements and remaining neutrons.

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example: hydrogen with a mass # of 2 and an atomic # of 1 + hydrogen with a mass # of 2 and an atomic # of 1 yields helium with a mass # of 4 and an atomic # of 2

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example: hydrogen with a mass # of 2 and an atomic # of 1 + hydrogen with a mass # of 2 and an atomic # of 1 yields helium with a mass # of 4 and an atomic # of 2

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Occurs as a result of unstable neutron to proton ratios

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Forcing an element to change into another by bombarding it with high energy particles

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Man can force one element to change into another by bombarding it with high energy particles.

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The combination of lighter particles into heavier particles:

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The combination of lighter particles into heavier particles:

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Includes alpha,beta, and positron decay types

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The splitting of the nucleus of an atom. The larger particle(s)  split into smaller particles.

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The splitting of the nucleus of an atom. The larger particle(s)  split into smaller particles.