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Q.Write two shortcomings of Rutherford's nuclear model and explain how Bohr's model of hydrogen atom overcame these shortcomings. OR Explain nuclear fusion and fission with the help of one example each.
Madhya Pradesh MpbseMP Board Higher Secondary 2024Subjective· 4mImportance★★★★★
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Start your 14-day free trial to unlock the full solution →Rutherford's model failed on atomic stability and line spectra; Bohr fixed both with quantized non-radiating orbits. Fission splits a heavy nucleus; fusion combines light nuclei — both release energy.
Two shortcomings of Rutherford's nuclear model:
- Instability of the atom: according to classical electromagnetic theory, an accelerating (orbiting) charged particle must continuously radiate energy. Since the electron revolves around the nucleus (a form of acceleration), it should continuously lose energy, causing its orbital radius to shrink, and it should spiral into the nucleus within a fraction of a second — meaning atoms should be highly unstable. This contradicts the observed stability of atoms.
- No explanation for line spectra: since the electron's radius (and hence energy) would change continuously as it spirals inward under Rutherford's model, it would emit a continuous spectrum of radiation, not the observed sharp, discrete spectral lines characteristic of each element.
How Bohr's model overcame these:
Niels Bohr introduced quantum postulates on top of Rutherford's nuclear model:
- Electrons revolve only in certain stationary (stable, non-radiating) orbits, for which the angular momentum is quantized: , n = 1, 2, 3, ... While in a stationary orbit, the electron does not radiate energy — this directly resolves the stability problem.
- Radiation (a photon) is emitted or absorbed only when an electron jumps from one stationary orbit to another, with the photon's energy equal to the energy difference between the two orbits: . Since only specific orbits (and hence specific energy differences) are allowed, only specific frequencies of radiation are emitted, which explains the observed discrete line spectra.
OR — Nuclear fission and fusion:
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