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Title: Chp 4: Electron Arrangement Slide 1


1
Unit 2 Electrons and Periodic Behavior
Cartoon courtesy of NearingZero.net
2
  • Chapter 4 Exam Review
  • Know
  • the equation c ??
  • All electromagnetic radiation (light, uv,
    infared, xray, gamma ray, radio) has the same
    speed speed of light
  • Because c is constant, wavelength and frequency
    are inversely proportional
  • As it travels through space, em radiation
    exhibits wavelike behavior

3
  • Chapter 4 Exam Review
  • The distance between two peaks on a wave is its
    wavelength
  • What is the photoelectric effect? Why cant
    certain kinds of light eject photons?
  • A quantum of em radiation is called a photon.
  • Who proposed that hot objects emit radiation in
    amounts called quanta? (Max Planck)

4
  • Chapter 4 Exam Review
  • The energy of a photon is related to its
    frequency
  • A line spectrum is produced when an electron
    moves from one energy level to a lower energy
    level
  • Hydrogen (and other atoms) produce the same line
    spectrum because it releases photons of only
    certain energies.

5
  • Chapter 4 Exam Review
  • What is an electron cloud?
  • What does the Heisenberg Uncertainty Principle
    state?
  • What is an orbital?
  • Know the four quantum number names and
    descriptions

6
  • s orbital spherical shape
  • p orbital dumbell shaped
  • How many electrons can an orbital hold?
  • How many orbitals are in each sublevel
    (s, p, d, and f)?
  • How many electrons can each sublevel hold?
  • How many sublevels are in each period?

7
  • Know the principles
  • Pauli Exclusion Principle
  • Aufbau Principle
  • Hunds Rule
  • Know orbital filling order (1s, 2s, 2p, etc)
  • Full s and p sublevels full octet noble gas
  • Know how to do electron configurations

8
In order to understand current atomic theory we
must first understand the properties of light
Light behaves both as a wave and as a particle
9
Wave-Particle Duality
JJ Thomson won the Nobel prize for describing the
electron as a particle.
His son, George Thomson won the Nobel prize for
describing the wave-like nature of the electron.
The electron is a particle!
The electron is an energy wave!
Dont you get sassy with me, Boy!
Oh, go fly a kite, you old geezer!
10
The Particle-like Electron
The photoelectric effect. Incoming EM radiation
on the left ejects electrons, depicted as flying
off to the right, from a substance. Only one
photon (a packet of light energy) can eject one
electron. Therefore, light acts like particles
(Einstein, 1905) because of the photons
quantized energy nature. This differed from
the description of EM radiation by Maxwell (1865)
which showed the infinite divisibility of EM
energy in physical systems.
11
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12
Section 4.1
Light is a form of Electromagnetic Radiation It
exhibits wavelike behavior as it travel through
space Kinds of em radiation x-rays, ultraviolet
light, infared light, microwaves, radio
waves Together, all of the types of em radiation
form the electromagnetic spectrum
13
Electromagnetic radiation propagates through
space as a wave moving at the speed of light.
c ??
C speed of light, a constant (3.00 x 108 m/s)
? frequency, in units of hertz (hz, sec-1)
? wavelength, in meters
14
The energy (E ) of electromagnetic radiation is
directly proportional to the frequency (?) of the
radiation.
E h?
E Energy, in units of Joules (kgm2/s2)
h Plancks constant (6.626 x 10-34 Js)
? frequency, in units of hertz (hz, sec-1)
15
Spectroscopic analysis of the visible spectrum
produces all of the colors in a continuous
spectrum
16
Longer Wavelength, Lower Energy
17
Types of electromagnetic radiation
18
Wavelength Table
Long Wavelength Low Frequency Low ENERGY
Short Wavelength High Frequency High ENERGY
19
Higher Frequency and Energy
20
Wavelength (?) the distance between
corresponding points on adjacent waves. Frequency
(?) the number of waves that pass a given point
in a specific time, usually one second C
?? Max Planck proposed that hot objects emit
energy in small, specific amounts called quanta
(1900). Quantum the minimum quantity of energy
that can be lost or gained by an atom
21
E hv Albert Einstein (1905) EM radiation has
a dual wave-particle nature Photon a particle
of electromagnetic radiation that has zero mass
and carries a quantum of energy
22
Ground State the lowest energy state of an
atom Excited state a state at which an atom has
a higher potential energy than in its ground
state Continuous spectrum the emission of a
continuous range of frequencies of
electromagnetic radiation Line emission
spectrum a series of specific light frequencies
emitted from excited atoms of a specific element
23
  • Electron absorbs
  • energy from the flame
  • goes to a higher energy
  • state.

2. Electron goes back down to lower energy state
and releases the energy it absorbed as light.
24
lithium
sodium
potassium
copper
16.11
25
Bohrs Model of the Atom (1913)
  • e- can only have specific (quantized) energy
    values
  • light is emitted as e- moves from one energy
    level to a lower energy level

n (principal quantum number) 1,2,3,
RH (Rydberg constant) 2.18 x 10-18J
7.3
26
The Wave-like Electron
The electron propagates through space as an
energy wave. To understand the atom, one must
understand the behavior of electromagnetic waves.
Louis deBroglie
27
Heisenberg Uncertainty Principle
It is impossible to determine simultaneously both
the position and velocity of an electron or any
other particle
28
Schrodinger Wave Equation
Published in 1926, used the hypothesis that
electrons have a dual wave-particle nature
Together with the Heisenberg Uncertainty
Principle, it laid the foundation for modern
quantum theory Quantum Theory describes
mathematically the wave properties of electrons
and other very small particles
29
The Bohr Model of the Atom
I pictured electrons orbiting the nucleus much
like planets orbiting the sun.
But I was wrong! Theyre more like bees around a
hive.
WRONG!!!
Neils Bohr
30
Wave function equations only give the probability
of finding an electron at any given place around
the nucleus They do not travel around the nucleus
in neat orbits. Instead they exist in
orbitals Orbital A three-dimensional region
around the nucleus that indicates the probable
location of an electron.
31
Quantum Numbers
Each electron in an atom has a unique set of 4
quantum numbers which describe it.
  • Principal quantum number
  • Angular momentum quantum number
  • Magnetic quantum number
  • Spin quantum number

32
Think of the 4 quantum numbers as describing
where your seat is in the Superdome 1. Level 2.
Gate 3. Row 4. Seat
33
Pauli Exclusion Principle
No two electrons in an atom can have the same
four quantum numbers.
And, no two fans in the Superdome should have the
same 4 seat numbers!
Wolfgang Pauli
34
Principal Quantum Number
Generally symbolized by n, it denotes the shell
(energy level) in which the electron is located.
Number of electrons that can fit in a shell
2n2
35
Angular Momentum Quantum Number
The angular momentum quantum number, generally
symbolized by l, denotes the orbital (subshell)
in which the electron is located.
36
Magnetic Quantum Number
The magnetic quantum number, generally symbolized
by m, denotes the orientation of the electrons
orbital with respect to the three axes in space.
37
Spin Quantum Number
Spin quantum number denotes the behavior
(direction of spin) of an electron within a
magnetic field.
Possibilities for electron spin
38
Assigning the Numbers
  • The three quantum numbers (n, l, and m) are
    integers.
  • The principal quantum number (n) cannot be zero.
  • n must be 1, 2, 3, etc.
  • The angular momentum quantum number (l) can be
    any integer between 0 and n - 1.
  • For n 3, l can be either 0, 1, or 2.
  • The magnetic quantum number (m) can be any
    integer between -l and l.
  • For l 2, m can be either -2, -1, 0, 1, or 2.

39
Principle, angular momentum, and magnetic quantum
numbers n, l, and ml
40
An orbital is a region within an atom where
thereis a probability of finding an electron.
This is a probability diagram for the s orbital
in the first energy level
Orbital shapes are defined as the surface that
contains 90 of the total electron probability.
41
Sizes of s orbitals
Orbitals of the same shape (s, for instance) grow
larger as n increases
Nodes are regions of low probability within an
orbital.
42
s orbital shape
The s orbital has a spherical shape centered
around the origin of the three axes in space.
43
P orbital shape
There are three dumbbell-shaped p orbitals in
each energy level above n 1, each assigned to
its own axis (x, y and z) in space.
44
d orbital shapes
Things get a bit more complicated with the five d
orbitals that are found in the d sublevels
beginning with n 3. To remember the shapes,
think of double dumbells
and a dumbell with a donut!
45
Shape of the f orbitals
46
  • Max Planck proposed the idea of quanta, small
    specific amounts of energy.
  • The electron cloud is the region outside of the
    nucleus where an electron can most probably be
    found.
  • The Pauli exclusion principle states that no two
    electrons in the same atom can have the same four
    quantum numbers
  • Hunds rule says that orbitals of equal energy are
    each occupied by one electron of the same spin
    before any is occupied by a second

47
  • Louis deBroglie believed that electrons could
    have a dual wave-particle nature
  • The magnetic quantum number indicates the
    position of an orbital about the three axes in
    space.
  • The photoelectric effect is the emission of
    electrons from metals that have absorbed photons.
  • The wave model of light did not explain the
    photoelectric effect. Only the particle model
    could.
  • The energy of a photon, or quantum, is related to
    its frequency.
  • Both the Heisenberg uncertainty principle and the
    Schrodinger equation led to the concept of atomic
    orbitals

48
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49
Quantum Numbers (4) Specify the properties of
atomic orbitals and the properties of electrons
in orbitals Principal Quantum Number
(n) Indicates the main energy level occupied by
the electron Values are 1, 2, 3 etc
50
Angular Momentum Quantum Number (l) Indicates the
shape of the orbital (values 0, 1, 2, or
3) (letter designation s, p, d, or f)
51
Magnetic Quantum Number (m) Indicates the
orientation of an orbital around the nucleus
(values depend on orbital) for an s orbital, m
0 for a p orbital, m px, py, or pz (5 d
orientations, 7 f orientations)
52
Spin Quantum Number Electrons can be thought of
as spinning on an internal axis. values are
either 1/2 or -1/2, which indicate the two
fundamental spin states of an electron
53
Orbital filling table
54
Principal Quantum Number
Generally symbolized by n, it denotes the shell
(energy level) in which the electron is located.
Number of electrons that can fit in a shell
2n2
55
Angular Momentum Quantum Number
The angular momentum quantum number, generally
symbolized by l, denotes the orbital (subshell)
56
Magnetic Quantum Number
The magnetic quantum number, generally symbolized
by m, denotes the orientation
57
s orbital shape
The s orbital has a spherical shape centered
around the origin of the three axes in space.
58
Sizes of s orbitals
Orbitals of the same shape (s, for instance) grow
larger as n increases
Nodes are regions of low probability within an
orbital.
59
P orbital shape
There are three dumbbell-shaped p orbitals in
each energy level above n 1, each assigned to
its own axis (x, y and z) in space.
60
d orbital shapes
Things get a bit more complicated with the five d
orbitals that are found in the d sublevels
beginning with n 3. To remember the shapes,
think of double dumbells
and a dumbell with a donut!
61
Shape of f orbitals
62
Quantum Numbers
Each electron in an atom has a unique set of 4
quantum numbers which describe it.
  • Principal quantum number
  • Angular momentum quantum number
  • Magnetic quantum number
  • Spin quantum number

63
Angular Momentum Quantum Number
The angular momentum quantum number, generally
symbolized by l, denotes the orbital (subshell)
64
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65
Orbital Subshells
Subshell of orbitals e- in each
total e- s 1 2 2
p 3 2
6 d 5
2 10 f
7 2
14
66
Pauli Exclusion Principle
  • A maximum of two electrons can occupy each
    orbital. Each electron must have different spin
    quantum numbers

67
Aufbau Principle
Electrons in an atom will occupy the
lowest-energy orbitals available (aufbau
building up)
68
Hunds Rule
The most stable arrangement of electrons is that
with the most unpaired electrons all with the
same spin
69
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70
Orbital Filling Order
71
Orbital filling table
72
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73
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74
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75
Writing Electron Configurations
  • Determine the number of electrons and atom has
  • Fill orbitals in order of increasing energy

76
Orbital Diagrams
Orbital Diagrams are models of electron
arrangements showing configuration, subshell,
aufbau, hunds, and pauli H ? 1S
77
Orbital Diagrams
He ?? 1S Li ?? ?
1s 2s
78
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79
Practice Problems
1. Write the electron configuration and orbital
diagram for B
80
Practice Problems
  • Write the electron configuration and orbital
    diagram for B
  • 1s2 2s2 2p1

81
Practice Problems
  • Write the electron configuration and orbital
    diagram for P

82
Practice Problems
  • Write the electron configuration and orbital
    diagram for P
  • 1s2 2s2 2p6 3s2 3p3

83
Practice Problems
  • Write the electron configuration and orbital
    diagram for Sc

84
Practice Problems
  • Write the electron configuration and orbital
    diagram for Sc
  • 1s2 2s2 2p6 3s2 3p6 4s2 3d1

85
Practice Problems
  • Write the electron configuration and orbital
    diagram for Pr

86
Practice Problems
  • Write the electron configuration and orbital
    diagram for Pr
  • 1s2 2s2 2p6 3s2 3p6 4s2 3d10 4p6 5s2 4d10 5p6 6s2
    4f3

87
2.7 PT and Electron Configuration
The First 20 elements
1s
  • H 1s1
  • He 1s2
  • Li 1s2 2s1
  • Be 1s2 2s2
  • B 1s2 2s2 2p1
  • C 1s2 2s2 2p2
  • N 1s2 2s2 2p3
  • O 1s2 2s2 2p4
  • F 1s2 2s2 2p5
  • Ne 1s2 2s22p6
  • Na 1s2 2s2 2p6 3s23s1
  • Mg 1s2 2s2 2p6 3s2 3s2
  • Al 1s2 2s2 2p6 3s2 3p1
  • Si 1s2 2s2 2p6 3s2 3p2
  • P 1s2 2s2 2p6 3 s 2 3p1
  • S 1s2 2s2 2p6 3s2 3p4
  • Cl 1s2 2s2 2p6 3s2 3p5
  • Ar 1s2 2s2 2p6 3s2 3p6

2s
2p
3s
3p
88
Orbital filling table
89
Electronic Structure of Atoms
The First 10 elements
1s
  • H 1s1
  • He 1s2
  • Li 1s2 2s1
  • Be 1s2 2s2
  • B 1s2 2s2 2p1
  • C 1s2 2s2 2p2
  • N 1s2 2s2 2p3
  • O 1s2 2s2 2p4
  • F 1s2 2s2 2p5
  • Ne 1s2 2s2 2p6

2s
2p
90
Hund's Rule
The most stable arrangement of electrons is that
with the maximum number of unpaired electrons,
all with the same spin quantum number
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