Correct answer Carries: 4.
Wrong Answer Carries: -1.
What characterizes the emission line spectrum of a hydrogen atom?
The emission line spectrum consists of bright lines on a dark background, corresponding to specific wavelengths emitted during electron transitions.
In Bohr’s model, what defines the stationary orbits of an electron?
Bohr’s second postulate defines stationary orbits as those where the angular momentum is an integral multiple of \( h/2\pi \).
In Bohr’s model, what is the state of a hydrogen atom when its electron is in the \( n = \infty \) orbit?
At \( n = \infty \), the energy is zero, meaning the electron is ionized and no longer bound to the nucleus.
What does the de Broglie hypothesis suggest about the electron in Bohr’s model?
De Broglie suggests that electrons exhibit wave-like behavior, forming standing waves in orbits where the circumference is an integer multiple of the wavelength.
In the Bohr model, how many de Broglie wavelengths fit into the circumference of the \( n = 6 \) orbit?
\( 2\pi r_n = n\lambda \).
For \( n = 6 \), number of wavelengths = 6.
Which of the following statements is incorrect about Rutherford’s nuclear model?
Rutherford’s model does not explain atomic stability, as it predicts electrons would emit radiation and collapse into the nucleus, not maintain stable orbits.
An electron in a hydrogen atom transitions from \( n = 3 \) to \( n = 1 \). What is the energy of the emitted photon? (Use \( E_n = -\frac{13.6}{n^2} \, \text{eV} \))
\( E_3 = -\frac{13.6}{3^2} = -1.51 \, \text{eV} \), \( E_1 = -13.6 \, \text{eV} \).
\( \Delta E = E_3 - E_1 = -1.51 - (-13.6) = 12.09 \, \text{eV} \).
What is the total energy of an electron in the \( n = 4 \) state of a hydrogen atom? (Use \( E_n = -\frac{13.6}{n^2} \, \text{eV} \))
\( E_4 = -\frac{13.6}{4^2} = -\frac{13.6}{16} = -0.85 \, \text{eV} \).
What is the wavelength of the photon emitted when an electron drops from \( n = 2 \) to \( n = 1 \) in a hydrogen atom? (Use \( h = 6.6 \times 10^{-34} \, \text{J·s} \), \( c = 3 \times 10^8 \, \text{m/s} \), 1 eV = \( 1.6 \times 10^{-19} \, \text{J} \))
\( \Delta E = 10.2 \, \text{eV} = 1.632 \times 10^{-18} \, \text{J} \).
\( \lambda = \frac{hc}{\Delta E} = \frac{6.6 \times 10^{-34} \times 3 \times 10^8}{1.632 \times 10^{-18}} \approx 1.21 \times 10^{-7} \, \text{m} \).
What is the energy difference between the \( n = 5 \) and \( n = 3 \) states in a hydrogen atom? (Use \( E_n = -\frac{13.6}{n^2} \, \text{eV} \))
\( E_5 = -0.544 \, \text{eV} \), \( E_3 = -1.51 \, \text{eV} \).
\( \Delta E = -0.544 - (-1.51) = 0.966 \, \text{eV} \approx 0.97 \, \text{eV} \).
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