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okay as you can see in todayamp;#39;s video weamp;#39;re gonna go over nuclear fusion and mass defect and binding energy when we combine a hydrogen two which is known as a deuterium and a hydrogen three atom which is known as a tritium and when we do that weamp;#39;re going to get a helium four and a neutron and this is new clear fusion and this is what occurs in the Sun this is where the Sun gets its energy from from the combination for example of deuterium and tritium are combined and theyamp;#39;re gonna form a helium nucleus and theyamp;#39;re gonna release energy and a neutron and we are going to use the average atomic masses of those things to determine the energy that is released from that reaction so hereamp;#39;s the reaction again we have hydrogen two hydrogen three deuterium and tritium we react those two together we can combine those two in nuclear fusion and when we do that we get a helium four and a neutron now this basically just becomes a problem involving conserv