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Quantum Theory and the Atom Bohr’s Model of the Atom

Bohr’s Model · Bohr’s Explanation of Hydrogen’s Line Spectrum According to Bohr, when the electron is in the ground state, also called the ground state or n = 1 orbit, the

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  • Quantum Theory and the Atom

    Bohr’s Model of the Atom

  • Atomic Emission SpectrumWhen atoms of different elements emit

    electromagnetic waves of light, they emit only a certain set of frequencies of light that we call the

    element’s atomic emission spectrum.

  • Identifying ElementsEach element’s atomic emission spectrum is unique and can be used to identify various elements within

    compounds or even within stars.

  • Non-Continuous LinesNotice that the emission lines are individual lines, not a

    continuous spectrum like in a rainbow.

    Non-Continuous Continuous

  • Niels BohrIn 1913, Niels Bohr built upon Planck’s and Einstein's

    concepts of quantized energy to explain the discontinuous nature of Hydrogen’s atomic emission

    spectrum by proposing a quantum model for the Hydrogen atom.

    Ephotons = hv

  • Energy States of HydrogenBohr proposed that hydrogen’s electron orbits the nucleus in circular orbits related to the amount of

    energy that the electron contains.

    When an atom gains energy, it is said to be in an excited state.

    The lowest energy state is called its ground state

    Nucleus

    Ground State

    Excited State

    Bohr called the orbitsenergy states

  • Multiple Excited States

    Ground State

    1st Excited State

    Although hydrogen has only one electron, it is capable of having many different excited states.

    2nd Excited State 3rd Excited

    State

    4th Excited State

  • Energy States of HydrogenBohr assigned a quantum number, n, to each orbit and calculated the orbit’s radius. The smaller orbits were

    closer to the nucleus.

    Bohr’s Description of the Hydrogen Atom

    Bohr Atomic Orbit Quantum Number Orbit Radius (nm) Energy Level Relative Energy

    First n = 1 0.0529 1 E1

    Second n = 2 0.212 2 E2 = 4E1

    Third n = 3 0.476 3 E3 = 9E1

    Fourth n = 4 0.846 4 E4 = 16E1

    Fifth n = 5 1.32 5 E5 = 25E1

    Sixth n = 6 1.90 6 E6 = 36E1

    Seventh n = 7 2.59 7 E7 = 49E1

  • Bohr’s Explanation of Hydrogen’s Line SpectrumAccording to Bohr, when the electron is in the ground state, also called the ground state or n = 1 orbit, the

    atom does not radiate energy.

    When energy is added from an outside source, the electron

    moves to a higher energy orbit, such as n=2.

    This raises the atom to an excited state.

  • Bohr’s Explanation of Hydrogen’s Line SpectrumWhen the atom is in an excited state, the electron

    can drop from a higher energy orbit down to a lower energy orbit.

    As the electron drops down, the atom emits a photon of energy.

  • Bohr’s Explanation of Hydrogen’s Line SpectrumThe energy of the released photon is equal to the

    difference between the energy levels associated with the two orbits.

    ∆E = Ehigher energy level – Elower energy level = Ephoton = hv

  • Bohr’s Explanation of Hydrogen’s Line SpectrumBecause only certain atomic energies are possible,

    only certain frequencies of electromagnetic radiation can be emitted.

    ∆E = Ehigher energy level – Elower energy level = Ephoton = hv

    Hydrogen’s Atomic Emission Spectrum

    Wavelength = Wave Speed Frequency

  • Hydrogen’s Spectral LinesThe hydrogen atom not only emits photons in the

    visible portion of the electromagnetic spectrum, but also in the infrared and ultraviolet portions.

    Balmer Series

    Lyman Series Paschen Series

  • Balmer SeriesThe photon emissions in the visible light range, known as

    the Balmer Series, occur when electrons drop from higher energy levels into the 2nd energy level.

    Balmer Series

  • Paschen SeriesThe photon emissions in the infrared range, known as the Paschen Series, occur when electrons drop from

    higher energy levels into the 3rd energy level.

    Paschen Series

  • Lyman SeriesThe photon emissions in the ultraviolet range, known as

    the Lyman Series, occur when electrons drop from higher energy levels into the 1st energy level.

    Lyman Series

  • Reference Table

    Nanometer = billionth meter = 10-9

    0.000 000 001

    434 nm = 0.000 000 434 m

    4.34 x 10-7 m

  • Bohr Model of AtomsWhile hydrogen has only one electron and thus one

    ground state energy level, atoms with multiple electrons will have many energy levels when the electrons are at

    ground state.

  • Each energy level can hold a certain amount of electrons.

    Always work from the nucleus outwards.

    Work clockwise, NSEW, before pairing.

    X 1 2 3

    4

    Nucleus

    1 1st Energy level

    2 2nd Energy level

    3 3rd Energy level

    4

    4th Energy level

    X

    Bohr Model of Atoms

  • X 2 3 4

    The 1st Energy Level can Hold Up To 2 Electrons

    Bohr Model of Atoms

  • The 2nd Energy Level Can Hold Up To 8 Electrons

    X 1

    23

    4

    Bohr Model of Atoms

  • The 3rd Energy Level Can Hold Up To 18 Electrons

    X 1

    23

    4

    Bohr Model of Atoms

  • The 4th Energy Level Can Hold Up To 32 Electrons

    X 1

    23

    4

    Bohr Model of Atoms

  • Valence ElectronsDuring chemical reactions, only the outer electrons are involved.

    Therefore, these outer electrons are given a special name and are

    called valence electrons.

    Sodium has 1

    valence electronMagnesium has 2

    valence electrons

  • Periodic Patterns

    Groups

    Valence Electrons

    Periods

    Energy Levels