Mass defect is a fundamental concept in nuclear physics. It refers to the difference between the sum of the masses of a system's individual protons and neutrons and the actual mass of the nucleus.
When protons and neutrons come together to form a nucleus, some of their mass is converted into energy, which binds them together. This phenomenon is a result of binding energy, which stabilizes the nucleus. The difference in mass is the mass defect.
- To calculate the mass defect, first identify the number of protons and neutrons in the nucleus.
- Next, find their individual masses. For protons, this is approximately 1.007276 amu, and for neutrons, it's about 1.008665 amu.
- Sum these masses and subtract the nuclear mass from this sum. This gives you the mass defect in atomic mass units (amu).
Understanding mass defect helps explain why the binding energy exists and how much energy would be required to break a nucleus apart, making it a crucial part of nuclear science.