Chapter 13Electrons in Atoms

Section 13.1Models of the Atom

OBJECTIVES: Summarize the development of

atomic theory.

Section 13.1Models of the Atom

OBJECTIVES: Explain the significance of

quantized energies of electrons as they relate to the quantum mechanical model of the atom.

J. J. Thomson’s Model

Discovered electrons Negative electron

floating around “Plum-Pudding”

model

Ernest Rutherford’s Model Discovered dense

positive piece at the center of the atom- nucleus

“Nuclear model”

Niels Bohr’s Model Move like planets around the sun. In circular orbits at different levels. Amounts of energy separate one

level from another. “Planetary model”

Bohr’s planetary model electron cannot exist between energy

levels, just like you can’t stand between rungs on ladder

Quantum of energy required to move to the next highest level

The Quantum Mechanical Model

Since the energy of an atom is never “in between” there must be a quantum leap in energy.

Erwin Schrodinger Mathematical solution

Has energy levels for electrons.

Orbits are not circular. It can only tell us the

probability of finding an electron a certain distance from the nucleus.

The Quantum Mechanical Model

The atom is found inside a blurry “electron cloud”

An area where there is a chance of finding an electron.

Think of fan blades

The Quantum Mechanical Model

Atomic Orbitals Principal Quantum Number (n) = the

energy level of the electron. Within each energy level, the complex

math of Schrodinger’s equation describes several shapes.

Atomic orbitals - regions where there is a high probability of finding an electron.

Sublevels

Summary

s

p

d

f

# of shapes

Max electrons

Starts at energy level

1 2 1

3 6 2

5 10 3

7 14 4

By Energy Level First Energy Level only s orbital only 2 electrons 1s2

Second Energy Level

s and p orbitals are available

2 in s, 6 in p 2s22p6

8 total electrons

By Energy Level Third energy level s, p, and d

orbitals 2 in s, 6 in p, and

10 in d 3s23p63d10

18 total electrons

Fourth energy level

s,p,d, and f orbitals

2 in s, 6 in p, 10 in d, ahd 14 in f

4s24p64d104f14

32 total electrons

Section 13.2Electron Arrangement in Atoms

OBJECTIVES: Apply the aufbau principle, the

Pauli exclusion principle, and Hund’s rule in writing the electron configurations of elements.

Section 13.2Electron Arrangement in Atoms

OBJECTIVES: Explain why the electron

configurations for some elements differ from those assigned using the aufbau principle.

Incr

easi

ng e

nerg

y

1s

2s

3s

4s

5s6s

7s

2p

3p

4p

5p

6p

3d

4d

5d

7p 6d

4f

5f

Aufbau diagram - page 367

Electron Configurations Aufbau principle- electrons enter the

lowest energy first. This causes difficulties because of the

overlap of orbitals of different energies. Pauli Exclusion Principle- at most 2

electrons per orbital - different spins

Electron Configuration Hund’s Rule- When electrons

occupy orbitals of equal energy they don’t pair up until they have to.

Phosphorus (15 electrons)

The first two electrons go into the 1s orbital

Notice the opposite spins

only 13 more to go...

Incr

easi

ng e

nerg

y

1s

2s

3s

4s

5s6s

7s

2p

3p

4p

5p

6p

3d

4d

5d

7p 6d

4f

5f

The next electrons go into the 2s orbital

only 11 more...Incr

easi

ng e

nerg

y

1s

2s

3s

4s

5s6s

7s

2p

3p

4p

5p

6p

3d

4d

5d

7p 6d

4f

5f

• The next electrons go into the 2p orbital

• only 5 more...Incr

easi

ng e

nerg

y

1s

2s

3s

4s

5s6s

7s

2p

3p

4p

5p

6p

3d

4d

5d

7p 6d

4f

5f

• The next electrons go into the 3s orbital

• only 3 more...Incr

easi

ng e

nerg

y

1s

2s

3s

4s

5s6s

7s

2p

3p

4p

5p

6p

3d

4d

5d

7p 6d

4f

5f

Incr

easi

ng e

nerg

y

1s

2s

3s

4s

5s6s

7s

2p

3p

4p

5p

6p

3d

4d

5d

7p 6d

4f

5f

• The last three electrons go into the 3p orbitals.

• They each go into separate shapes

• 3 unpaired electrons

• = 1s22s22p63s23p3

The easy way to remember

1s2s 2p3s 3p 3d4s 4p 4d 4f

5s 5p 5d 5f6s 6p 6d 6f7s 7p 7d 7f

• 1s2

• 2 electrons

Fill from the bottom up following the arrows

1s2s 2p3s 3p 3d4s 4p 4d 4f

5s 5p 5d 5f6s 6p 6d 6f7s 7p 7d 7f

• 1s2 2s2

• 4 electrons

Fill from the bottom up following the arrows

1s2s 2p3s 3p 3d4s 4p 4d 4f

5s 5p 5d 5f6s 6p 6d 6f7s 7p 7d 7f

• 1s2 2s2 2p6 3s2

• 12 electrons

Fill from the bottom up following the arrows

1s2s 2p3s 3p 3d4s 4p 4d 4f

5s 5p 5d 5f6s 6p 6d 6f7s 7p 7d 7f

• 1s2 2s2 2p6 3s2

3p6 4s2

• 20 electrons

Fill from the bottom up following the arrows

1s2s 2p3s 3p 3d4s 4p 4d 4f

5s 5p 5d 5f6s 6p 6d 6f7s 7p 7d 7f

• 1s2 2s2 2p6 3s2

3p6 4s2 3d10 4p6

5s2

• 38 electrons

Fill from the bottom up following the arrows

1s2s 2p3s 3p 3d4s 4p 4d 4f

5s 5p 5d 5f6s 6p 6d 6f7s 7p 7d 7f

• 1s2 2s2 2p6 3s2

3p6 4s2 3d10 4p6

5s2 4d10 5p6 6s2

• 56 electrons

Fill from the bottom up following the arrows

1s2s 2p3s 3p 3d4s 4p 4d 4f

5s 5p 5d 5f6s 6p 6d 6f7s 7p 7d 7f

• 1s2 2s2 2p6 3s2

3p6 4s2 3d10 4p6

5s2 4d10 5p6 6s2

4f14 5d10 6p6 7s2

• 88 electrons

Fill from the bottom up following the arrows

1s2s 2p3s 3p 3d4s 4p 4d 4f

5s 5p 5d 5f6s 6p 6d 6f7s 7p 7d 7f

• 1s2 2s2 2p6 3s2

3p6 4s2 3d10 4p6

5s2 4d10 5p6 6s2

4f14 5d10 6p6 7s2

5f14 6d10 7p6 • 108 electrons

Section 13.3Physics and the Quantum

Mechanical Model OBJECTIVES:

Calculate the wavelength, frequency, or energy of light, given two of these values.

Section 13.3Physics and the Quantum

Mechanical Model OBJECTIVES:

Explain the origin of the atomic emission spectrum of an element.

Light The study of light led to the

development of the quantum mechanical model.

Light is a kind of electromagnetic radiation.

Electromagnetic radiation includes many kinds of waves

All move at 3.00 x 108 m/s = c

Parts of a wave

Wavelength

AmplitudeOrigin

Crest

Trough

Parts of Wave - p.372 Origin - the base line of the energy. Crest - high point on a wave Trough - Low point on a wave Amplitude - distance from origin to crest Wavelength - distance from crest to

crest Wavelength is abbreviated by the Greek

letter lambda =

Frequency The number of waves that pass a

given point per second. Units: cycles/sec or hertz (hz or sec-1) Abbreviated by Greek letter nu =

c =

Frequency and wavelength Are inversely related As one goes up the other goes down. Different frequencies of light are

different colors of light. There is a wide variety of frequencies The whole range is called a spectrum,

Fig. 13.10, page 373

Radiowaves

Microwaves

Infrared .

Ultra-violet

X-Rays

GammaRays

Low energy

High energy

Low Frequency

High Frequency

Long Wavelength

Short WavelengthVisible Light

Energy and frequency E = h x E is the energy of the photon is the frequency h is Planck’s constant h = 6.6262 x 10 -34 Joules x sec. joule is the metric unit of Energy

Examples What is the wavelength of blue light

with a frequency of 8.3 x 1015 hz? What is the frequency of red light

with a wavelength of 4.2 x 10-5 m? What is the energy of a photon of

each of the above?