AtomsClass 12 Physics Notes

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Introduction to Atomic Models

By the late 19th century, scientists knew that atoms contained negatively charged particles called electrons, which were identical across all elements. Since atoms are electrically neutral overall, they must also contain a positive charge to balance the negative charge of the electrons. The main question was: how are these positive and negative charges arranged inside an atom?

Thomson's Model of the Atom

In 1898, J. J. Thomson proposed the first model of the atom, often called the plum pudding model.

  • He suggested that an atom is a sphere of uniformly distributed positive charge.
  • The negatively charged electrons are embedded within this sphere, much like seeds in a watermelon or plums in a pudding.
Example
Imagine a watermelon. The red, fleshy part represents the sphere of positive charge, and the black seeds scattered throughout it represent the electrons. The whole watermelon is the atom.

This model, however, was later proven incorrect by further experiments.

Atomic Spectra

When we look at the light emitted by different substances, we see different types of spectra.

  • Continuous Spectrum: Solids, liquids, and dense gases emit electromagnetic radiation with a continuous range of all wavelengths, like a rainbow. This is due to the complex interactions between neighbouring atoms.
  • Line Spectrum (Discrete Spectrum): In contrast, rarefied (low-density) gases, when heated or electrically excited, emit light at only a few specific, discrete wavelengths. This appears as a series of bright lines on a dark background and is called an emission line spectrum. Since the atoms in these gases are far apart, the light is emitted by individual atoms.

Each element has its own unique, characteristic line spectrum, which acts like a "fingerprint." This suggested a deep connection between an atom's internal structure and the light it emits.

Rutherford's Model of the Atom

Building on Thomson's work, Ernst Rutherford conducted a famous experiment that completely changed our understanding of the atom. In 1911, his associates Hans Geiger and Ernst Marsden performed the alpha-particle scattering experiment. This led to the Rutherford's planetary model of atom, also known as the nuclear model.

According to this model:

  • The entire positive charge and almost all the mass of the atom are concentrated in a very small, dense core called the nucleus.
  • The electrons revolve around this nucleus in orbits, similar to how planets revolve around the sun.

While a major step forward, Rutherford's model also had problems. It couldn't explain why atoms only emit light at discrete wavelengths. According to classical physics, an orbiting electron should continuously lose energy and spiral into the nucleus, making the atom unstable.