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Question
niels bohr modified rutherfords nuclear atom model to explain how light interacted with the electrons in an atom to produce spectral lines. his model included electrons orbiting the nucleus at specific energy levels. electrons absorb energy from various sources (electricity) when they move from lower energy levels (ground state) to higher energy levels (excited states). energy is released as electrons return to their lower energy levels. model 3 - bohr model of a hydrogen atom a. ( n = 6 \to n = 2 ) b. ( n = 5 \to n = 2 ) c. ( n = 4 \to n = 2 ) d. ( n = 3 \to n = 2 ) 15. is light absorbed or released in the electron transitions above? explain. 16. a. which of the electron transitions involves the most energy? b. explain why this transition involves the most energy based on your understanding of the attractive forces between the electrons and protons in the atom.
- Question 15: When electrons move from higher to lower energy levels (as in all the transitions shown \(n = 6\to n = 2\), \(n=5\to n = 2\), \(n = 4\to n=2\), \(n=3\to n = 2\)), energy is released in the form of light. This is because the electron is losing energy as it moves to a more stable (lower - energy) state.
- Question 16a: The energy of a photon released during an electron transition is given by \(E=h
u=\frac{hc}{\lambda}\), and also related to the energy difference between two energy levels \(\Delta E=E_{final}-E_{initial}\). The greater the difference in energy levels (\(\Delta n\)), the greater the energy change. For transition \(A\) (\(n = 6\to n = 2\)), \(\Delta n=6 - 2=4\); for \(B\) (\(n = 5\to n = 2\)), \(\Delta n=5 - 2 = 3\); for \(C\) (\(n = 4\to n=2\)), \(\Delta n=4 - 2=2\); for \(D\) (\(n=3\to n = 2\)), \(\Delta n=3 - 2=1\). So transition \(A\) involves the most energy.
- Question 16b: The force of attraction \(F=\frac{kq_1q_2}{r^{2}}\) (Coulomb's law, where \(q_1\) is the charge of the proton, \(q_2\) is the charge of the electron, and \(r\) is the distance between them). Electrons in higher energy levels (\(n\) values) are on average farther from the nucleus. When an electron moves from \(n = 6\) to \(n = 2\) (transition \(A\)), it has to overcome a larger change in the electrostatic potential energy (due to the change in distance \(r\) from the nucleus). The energy change \(\Delta E\) is related to the work done against (or by) the electrostatic force. A larger \(\Delta n\) (change in energy level) corresponds to a larger change in the potential energy of the electron - proton system, and thus a larger energy of the emitted photon.
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- Light is released. When electrons move from higher (\(n = 6,5,4,3\)) to lower (\(n = 2\)) energy levels, they lose energy, which is emitted as light.
- a. Transition \(A\) (\(n = 6\to n = 2\)) involves the most energy.
b. Electrons in higher \(n\) (e.g., \(n = 6\)) are farther from the nucleus. The change in the electrostatic potential energy (due to the change in distance from the nucleus) is larger for \(n = 6\to n = 2\) compared to other transitions (\(n = 5\to n = 2\), \(n = 4\to n=2\), \(n=3\to n = 2\)), so more energy is released.