In this section, we will look at the early ideas about the atom, beginning with Democritus, who first proposed that all matter is made of tiny, indivisible particles called atoms. We will then discuss Dalton’s Atomic Theory, which provided a scientific foundation by describing atoms as solid, indivisible spheres and explaining how they combine to form compounds. Finally, we will examine the limitations of Dalton’s model, which could not explain phenomena such as subatomic particles, isotopes, or the internal structure of the atom.
In this section, we will explore the discovery of subatomic particles, beginning with J. J. Thomson’s identification of the electron through the cathode ray experiment, which proved that atoms contain negatively charged particles. We will then discuss Goldstein’s discovery of the proton using canal rays, showing the presence of positively charged particles in atoms. Chadwick’s work will be highlighted for revealing the neutron, a neutral particle found in the nucleus. The section also includes the determination of the electron’s charge-to-mass ratio (e/m), an important milestone in understanding the structure of matter.
In this section, we will discuss Thomson’s Atomic Model, often called the plum pudding model, which described the atom as a positively charged sphere with electrons embedded like “plums” inside it. This model successfully explained the overall neutrality of matter and the presence of electrons, but it had major limitations. It could not account for the scattering of alpha particles or the existence of a concentrated nucleus, leading to its replacement by later atomic models.
In this section, we will examine Rutherford’s Atomic Model, beginning with the famous alpha scattering or gold foil experiment, which showed that most alpha particles passed through the foil while a few were deflected. From this, Rutherford concluded that atoms contain a small, dense, positively charged nucleus and are mostly empty space. His nuclear model described electrons orbiting this central nucleus. However, the model had limitations: it could not explain the stability of atoms or the discrete line spectra observed in atomic emissions, paving the way for more advanced models.
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