Bohr Model of the Atom
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Questions and Answers

What does the variable 'n' represent in the equation $E_n = -2.18 \times 10^{-18} J (\frac{1}{n^2})$?

  • The energy of the electron
  • The number of electrons
  • The ionization energy
  • The principal quantum number (correct)
  • How does the energy of an electron change as 'n' increases in the Bohr model?

  • The energy increases
  • The energy becomes more positive (correct)
  • The energy remains constant
  • The energy decreases
  • What is true about the wavelength of light emitted during an electronic transition in a one-electron atom?

  • It remains constant regardless of the transition
  • It is inversely proportional to the energy change (correct)
  • It is irrelevant in electronic transitions
  • It is directly proportional to the energy change
  • If an electron transitions from n=3 to n=2, what happens to its energy?

    <p>It decreases as it moves to a lower energy level (B)</p> Signup and view all the answers

    In the equation $E_n = -2.18 \times 10^{-18} J (\frac{1}{n^2})$, what does the negative sign signify?

    <p>The energy is a bound state (A)</p> Signup and view all the answers

    Study Notes

    Bohr Model

    • The Bohr model describes the electron's orbit around the nucleus of an atom.

    • Electrons orbit the nucleus in specific, stable energy levels (quantized).

    • Energy levels are indexed by the principal quantum number, n (n=1, 2, 3...).

    • As n increases, the electron's energy and distance from the nucleus increase.

    • The electron's energy is quantized and calculated using the equation:

      𝐸n=−2.18×10−18J(1𝑛2) where n is the principal quantum number.

    Electron Energy Calculation

    • Electron energy depends directly on the principal quantum number (n).
    • As n increases, the electron energy becomes less negative, and moves away from the nucleus (higher energy state).
    • When n=1, the electron is in its lowest energy state (ground state).
    • The ground state energy of the atom is a negative value.

    Electronic Transitions

    • Electrons can jump between energy levels by absorbing or emitting photons (light) of specific energy.
    • The energy difference between energy levels corresponds to the energy of the absorbed or emitted photon.
    • The Δ𝐸 represents the energy change during the transition: Δ𝐸 = 𝐸final - 𝐸initial

    Energy Change Calculation

    • The energy change during a transition between two energy levels (ninitial and nfinal) is calculated using: Δ𝐸 = 𝐸nfinal - 𝐸ninitial = −2.18×10−18 J [(1/nfinal2) − (1/ninitial2)]

    Wavelength Calculation

    • If the energy change (Δ𝐸) of a transition is known, the wavelength of the emitted or absorbed photon can be calculated using the equation:

      Δ𝐸 = h𝑐/𝜆

      where:

      • Δ𝐸 is the energy change
      • h is Planck's constant (6.626 x 10-34 J•s)
      • 𝑐 is the speed of light (3.00 x 108 m/s)
      • 𝜆 is the wavelength.

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    Description

    This quiz explores the Bohr model, focusing on electron orbits around the atomic nucleus, quantized energy levels, and the relationship between principal quantum numbers and electron energy. Test your understanding of electronic transitions and energy calculations.

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