bohr’s model of the atom 1913. scientists noticed that the laws of classical physics that applied...

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Bohr’s Model of the Atom 1913

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Page 1: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Bohr’s Model of the Atom1913

Page 2: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain the behaviour of electrons giving rise to:

Planck’s Quantum Theory The new experimental field of “Spectroscopy”

demonstrated that atoms absorb and release bundles of energy.

Bohr used both quantum theory and spectroscopy in formulating his model of the atom.

Bohr’s model

Page 3: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Bohr’s model of the Atom

Atoms and their electrons can only exist in certain specific Energy States.

When moving within these allowed energy states (stationary states) the electron does NOT emit (release) energy.

Page 4: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Bohr’s model of the Atom

For the Hydrogen atom:

En = -R /n2

R = 2.18 x 10-18 J/atomE1 = -R /12 = - 21.8 x 10-19 J/atom

E2 = -R /22 = - 5.44 x 10-19 J/atom

E3 = -R /32 = - 2.42 x 10-19 J/atom

Page 5: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Fixed Energy Levels

n = Principal Quantum number; indicates the orbit.

Page 6: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Energy Levels in a Hydrogen atom

Page 7: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Why is there a negative sign in En?

Bohr defined the point of zero potential energy as the point when the electron was infinitely removed from the atom.

Page 8: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Why is there a negative sign in En?

When an electron moves closer to the nucleus, it feels an increasing attraction and the potential energy of the electron (and atom) decreases

Page 9: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Why is there a negative sign in En?

When a free electron (at infinity) “falls” into E1 (n=1) ,

2.18 x 10-18 J ( or 13.6 ev) is released.

Page 10: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Why is there a negative sign in En?

For the Hydrogen atom:

E1 = -R /1E2 = -R /4 E3 = -R /9 Note that because of the

negative sign, E1 is the lowest in energy

(instead of the highest)

Page 11: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Electron Jumps Between Energy Levels

2. Each Energy level corresponds to an orbit.

3. The electron can travel in an orbit without radiating energy

4. An electron may only change its energy by jumping from one allowed level to another.

Page 12: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Electron Transitions-Excitation

Energy Conversion:

Radiant energy (EM radiation) Potential energy (of electron)

Electron jumps up a level

Page 13: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Electron Transitions

Excitation Relaxation

Electron moves To a higher E level

Energy is Absorbed

Form of Energy Heat, light, electrical

Electromagnetic radiation

Page 14: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Electron Transitions-Relaxation

Energy Conversion:

Potential energy (of electron) Radiant energy (EM radiation)

Electron jumps down a level

Page 15: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Electron Transitions

Excitation Relaxation

Electron moves To a higher E level

To a lower E level

Energy is Absorbed Released

Form of Energy Heat, light, electrical

Electromagnetic radiation

Page 16: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Energy of an atom or electron is “quantized”

Atoms can only absorb or release the amount of energy necessary to move from one allowed energy level to another.

Page 17: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Excitation - Energy Absorbed

n=1

n=2

n=4

n=3

n=5n=6

Page 18: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Excitation - Energy Absorbed

n=1

n=2

n=4

n=3

n=5n=6

Absorbance of Energy(Excitation)

Page 19: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Relaxation - Energy Released

n=1

n=2

n=4

n=3

n=5n=6

Absorbance of Energy(Excitation)

Emission of Energy(Relaxation)

Page 20: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Relaxation - Energy Released

n=1

n=2

n=4

n=3

n=5n=6

Absorbance of Energy(Excitation)

Emission of Energy(Relaxation)

E2 to E6 E6 to E2

Page 21: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Relaxation - Energy Released

n=1

n=2

n=4

n=3

n=5n=6

Absorbance of Energy(Excitation)

Emission of Energy(Relaxation)

E2 to E6 E6 to E2

BOTH TRANSITIONS INVOLVE THE SAME AMOUNT OF ENERGY. THUS INVOLVE THE SAME FREQUENCY OF EM RADIATION

Page 22: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

What is observed during these transitions?

Page 23: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Background information:

•Electromagnetic energy (aka light energy) is often released and absorbed by chemical systems.

•The part of this radiation that we see is called the visible spectrum

Page 24: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Background information:

•Planck’s equation: E = hfStates that the greater the frequency of the radiation, the greater the energy of the photons.

Page 25: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

What happens to white light as it passes through a prism or diffraction grating (basis of spectroscopic

instruments)?

It is dispersed/separated according to the different colours (wavelengths, frequencies)

Continuous spectrum

Page 26: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

What happens to a sample of hydrogen gas (in a discharge tube) when an electric current is run

through it?

Electrical energy is absorbed and excites the electrons

Relaxation follows

H2 emits a purplish light is emitted.

Separating the light by a prism or diffraction grating produces…

Page 27: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Hydrogen Emission Spectrum

Each coloured line is produced by a specific relaxation transition.

Why do we only see 4 lines if many more transitions are possible?

Page 28: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Hydrogen Emission Spectrum

Only the 4 transitions in the BALMER SERIES involve EM radiation in the VISIBLE range

Page 29: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Spectroscopy

Analysis of the way matter absorbs or releases radiant energy

Examples: IR-spectra, atomic emission spectra, NMR (nuclear magnetic resonance), absorption spectra

Page 30: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Spectroscopy is used to:

a) identify elements or compoundsAtomic Spectra: Fingerprints of Elements

Page 31: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Spectroscopy is used to:

b) obtain information about bonding and structures of compounds

IR spectrum

Page 32: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Spectroscopy is used to:

c) Quantitatively determine the concentrations of substances present.

Page 33: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Two main types of atomic spectra:Emission and Absorption Spectra

“Bright-line Spectra” is atomic emission spectra in the visible range.

Page 34: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Absorption vs. Emission Spectra of H2

Note that the spectral lines are on the same wavelength.

Page 35: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Advantages/Uses of Spectroscopy

a) can definitively distinguish between substances with very similar physical and chemical properties.

eg. Members of the alkali metals family

K Na

Page 36: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Advantages/Uses of Spectroscopy

b) Sample is distant Eg. Applications in Astronomy

Astronomers have made the first direct detection and chemical analysis of an atmosphere of a planet that exists outside our solar system.

Page 37: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Spectrum of the hot gases in a nearby star-forming region, the Omega Nebula

(M17)

Page 38: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

Advantages/Uses of Spectroscopy

b) Sample quantity is limited eg. in Forensics “Crystal meth”

Page 39: Bohr’s Model of the Atom 1913. Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain

The End