In this section, we delve into the atomic mass unit (u), defined as one twelfth of the mass of a carbon-12 atom, giving a practical unit for measuring the minute masses of atoms. The section emphasizes that an atom's mass is far smaller than a kilogram, necessitating the use of atomic mass units for convenience. Atomic masses are close to integer multiples of the hydrogen atom mass, though exceptions exist, such as chlorine. Moreover, the section introduces isotopes, explaining how elements can exist in multiple forms with varying masses due to differing neutron counts; this affects the average atomic mass of elements. The discovery of neutrons clarified the composition of the nucleus, revealing that it consists of protons and neutrons, which are collectively referred to as nucleons. The mass defect phenomenon is also discussed, demonstrating that the nucleus's mass is less than the sum of its constituent particles, leading to the concept of binding energy, which is the energy required to separate the nucleons. Understanding these components is central to the broader topics of nuclear physics, including stability and nuclear reactions.