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AP Chem Notes chapters 7 8 9
ReadDo Problems for Chapters 7 8 9Chapter 7 Atomic Structure and Periodicity
Electromagnetic Radiation Radiant energy that exhibits wavelength-like behavior and travels
through space at the speed of light in a vacuum
Label the parts of the graph below wavelength amplitude node
Waves have 3 primary characteristics 1 Wavelength (λ) distance between two peaks in a wave2 Frequency (ν) number of waves per second that pass a given point in space3
Speed (c) speed of light is 29979 x 108 meterssecond (ms)
Wavelength and frequency can be inter-converted
c = λν
ν = frequency (s-1 1s Hz cycs or wavess ) 1 hertz (Hz) = 1s
λ = wavelength (m) c = speed of light (ms)
Max Planck (1858-1947)
An object can gain or lose energy by absorbing or emitting radiant energy in QUANTA
Transfer of energy is quantized and can only occur in discrete units called quanta
∆ E=hν=hcλ
ΔE = change in energy (J)h = Planckrsquos constant 6626 x 10-34 J s ν = frequency (s-1) λ = wavelength (m)
Photoelectric EffectAlbert Einstein (1879-1955)
Experiment demonstrates the particle nature of light Einstein called light particles ldquophotonsrdquo
Classical theory said that E of ejected electron should increase with increase in light intensityhellip but
No e- observed until light of a certain minimum E is used Number of e- ejected depends on light intensity
Energy has mass E = mc2
E = energy m = mass c = speed of light
Classical physics viewed light as a form of energy so it predicted that a metal would eventually collect enough energy to eject an electron regardless of the wavelength of the light
The emission of electrons from a metal when light shines on the metal
For a given metal no electrons were emitted if the frequency of light was below a ldquothresholdrdquo value regardless of how long the light was shining on the metal
Ephoton = hcλ
mphoton = hλc
Hence the dual nature of light or wave-particle duality
Line Spectra of excited atomsExcited atoms emit light of only certain wavelengthsThe wavelengths of emitted light depend on the element Observe spectrum tubes with diffraction gratings (spectroscopes)
Visible lines in H atom spectrum are called the BALMER series
Continuous spectrum Contains all the wavelengths of light
Line (discrete) spectrum Contains only some of the wavelengths of light
Niels Bohr (1885-1962) Bohrrsquos greatest contribution to science was in building a simple model of the atom It was based on an understanding of the SHARP LINE SPECTRA of excited atoms
One view of atomic structure in early 20th century was that an electron (e-) traveled about the nucleus in an orbit (Bohrrsquos Atomic Model)
+Electronorbit
1 Any orbit should be possible and so is any energy2 But a charged particle moving in an electric field should emit energy
End result should be destruction
Bohr said classical view is wrong Need a new theory mdash now called QUANTUM or WAVE MECHANICS e- can only exist in certain discrete orbits mdash called stationary states e- is restricted to QUANTIZED energy states Energy of state = - Cn2 where C is a constant amp where n = quantum no = 1 2 3 4
Bohr Model The e- in a hydrogen atom moves around the nucleus only in certain allowed circular
orbits
E = energy of the levels in the H-atomz = nuclear charge (for H z = 1)n = an integer
E becomes more negative as the electron moves closer to the nucleus
Ground State The lowest possible energy state for an atom (n = 1)
Shielding Effect Higher energy electrons are in outer shells and are easier to remove because they are more shielded from the positive nucleus by inner shell electrons
Energy Changes in the Hydrogen AtomΔE = Efinal state ndash Einitial state
λ= hcΔE
Failure of Bohr ModelFailure of Bohr Model The Bohr Model of the atom paved the way for the Quantum Mechanical Theory
but current theory is in no way derived from the Bohr Model of the atom The Bohr Model of the Atom was fundamentally incorrect--electrons do not move in
circular orbits about the nucleus
Umhellipso what is quantum mechanics
Louis deBroglie (1892-1987)
de Broglie (1924) proposed that all moving objects have wave properties
λ = hm v
λ = wavelength (m)h = Planckrsquos constant 6626 x 10-34 J s = kg m2 s-1 m = mass (kg)v = velocity (ms) ndash do not confuse with nu (frequency) or c (speed of light) ndash do not confuse with nu (frequency) or c (speed of light)
See Sample Exercise 73 on page 298
Baseball (0100 kg) at 35 ms
λ = 19 x 10-34 m
e- with velocity = 10 x 107 ms
λ = 727 x 10-11 m
Erwin Schrodinger 1887-1961
Schrodinger applied idea of e- behaving as a wave to the problem of electrons in atomsWave Equation Based on the wave properties of the atom
Ĥ ψ = E ψψ = wave function Ĥ = mathematical operatorE = total energy of the atomA specific wave function is often called an orbital Electrons move in orbitals not Bohr orbits
Werner Heisenberg 1901-1976
Heisenberg Uncertainty Principle Problem of defining nature of electrons in atoms solved by Werner Heisenberg Cannot simultaneously define the position and momentum (p = mbullv) of an electron We define e- energy exactly but accept the limitation that we do not know exact
position
x = positionmv = momentum (p)h = Planckrsquos constant
The more accurately we know a particlersquos position the less accurately we can know its momentum
Probability Distribution square of the wave function (ψ2) probability of finding an electron at a given position Radial probability distribution is the probability distribution in each spherical shell
Quantum Numbers describe the location of the eQuantum Numbers describe the location of the e--
symbol
name possible values what it tells about electron
cloud
n principal quantum number
1-7 size(energy level)
langular momentum(sublevel) quantum
numberl =0 to n-1 shape
l = 0 (s sublevel) l = 1 (p sublevel) l = 2 (d sublevel) l = 3 (f sublevel)
ml magnetic quantum number m
l = l to -l 3D orientation
in space
ms spin quantum number plusmn 12
spin states of electron
Pauli Exclusion Principle In a given atom no two electrons can have the same set of four quantum numbers
(n l ml ms) Therefore an orbital can hold only two electrons and they must have opposite spins
Shapes of Electron Orbitals
The following are graphical representations of the shapes of the orbitals within atoms Remember these shapes do not exist but are mainly three-dimensional probabilities of locating the electron Also remember a maximum of two electrons can occupy any of the following shapes
How many different kinds of orbitals does each energy level have n =
the number of the energy level
n2 = the number of orbitals in an energy level 2n2 = the number of electrons in an energy level
s-orbital (spherical)The following picture shows the relative sizes of 1s 2s and 3s orbitals
p-orbital (dumbbell)
3 orbitals px py pz - The three p orbitals lie 90deg apart in space
When l = 1 there is a PLANAR NODE thru the nucleus When n = 2 then l = 0 and 1Therefore in n = 2 shell there are 2 types of orbitals mdash 2 subshells For l = 0 m
l = 0 this is a s subshell
For l = 1 ml = -1 0 +1 this is a p subshell with 3 orbitals
d-orbital (double dumbbell and dumbbelldonut)5 orbitalsWhen n = 3 what are the values of l
l = 0 1 2 and so there are 3 subshells in the shell
For l = 0 ml = 0 ---gt s subshell with single orbital
For l = 1 ml = -1 0 +1 ---gt p subshell with 3 orbitals
For l = 2 ml = -2 -1 0 +1 +2---gt d subshell with 5 orbitals
s orbitals have no planar node (l = 0) and so are spherical
p orbitals have l = 1 and have 1 planar node and so are ldquodumbbellrdquo shaped
This means d orbitals (with l = 2) have 2 planar nodes
f-orbital (quadruple dumbbell and dumbbelldouble donut)7 orbitalsWhen n = 4 When n = 4 l = 0 1 2 3 so there are 4 subshells in the shell = 0 1 2 3 so there are 4 subshells in the shell
For For l = 0 = 0 ml = 0 ---gt s subshell with single orbital = 0 ---gt s subshell with single orbital
For For l = 1 = 1 ml = -1 0 +1 ---gt p subshell with 3 orbitals = -1 0 +1 ---gt p subshell with 3 orbitals
For For l = 2 = 2 ml = -2 -1 0 +1 +2 = -2 -1 0 +1 +2 ---gt d subshell with 5 orbitals ---gt d subshell with 5 orbitals
For For l = 3 = 3 ml = -3 -2 -1 0 +1 +2 +3 = -3 -2 -1 0 +1 +2 +3 ---gt f subshell with 7 orbitals ---gt f subshell with 7 orbitals
Aufbau principleAs protons are added one by one to the nucleus to build up the elements electrons
are similarly added to these hydrogen-like orbitals
electron filling order (aufbau)
Hundrsquos Rule The lowest energy configuration for an atom is the one having the maximum number of unpaired electrons allowed by the Pauli principle in a particular set of degenerate (same energy) orbitals
Valence electrons electrons in the outermost principle quantum level of an atomThe inner electron are called core electrons
atom valence electronsCa 2N 5Br 7Arrangement of Electrons in Atoms
Shells (energy levels) = ndarr
Sublevels = ldarr
Orbitals = ml
Assigning electrons to atomsAssigning electrons to atomsElectrons generally assigned to orbitals of successively higher energyFor H atoms - Cn2 E depends only on nFor many-electron atoms energy depends on both n and l
Effective Nuclear Charge Zeff
Zeff is the nuclear charge experienced by the outermost electrons Explains why E(2s) lt E(2p)
Zeff increases across a period owing to incomplete shielding by inner electrons
Estimate Zeff by --gt [ Z - (no inner electrons) ]
Charge felt by 2s e- in Li Zeff = 3 - 2 = 1Be Zeff = 4 - 2 = 2B Zeff = 5 - 2 = 3and so on
Writing Atomic Electron Configurations
Orbital Notation Each electron is represented by a half-arrow
When electrons share an orbital opposite spins are represented by half-arrows going in opposite directions
Examples Write the orbital notation for the following atoms
N (7 e-) ____ ____ ____ ____ ____
1s 2s 2p
P ( ___ e-)
Electron Configuration Notation Write the energy level and orbital (in increasing energy) Write the number of electrons in the sublevel with a superscript
Examples Write the electron configuration notation for the following atoms
N
P
Tc
Electron Configuration Notation (Noble Gas Shorthand) Start with the noble gas ldquocloset without going overrdquo in brackets Continue normal electron configuration
Examples Write the electron configuration notation for the PREVIOUS atoms (use the noble gas shorthand)
Lewis Dot Diagrams
Valence electrons (e- in the outermost energy level) are the only electrons that are lost or gained in ordinary chemical reactions
Lewis Dot Diagrams only include electrons in valence (highest energy level) Write the letter and dots around the outside (2 on each side maximum of 8)
Examples Draw the Lewis Dot Diagram for
N Ca Cl
Ion configurations To form cations from elements remove 1 or more e- from subshell of highest n [or highest (n + l)]
P [Ne] 3s2 3p3 - 3e- ---gt P3+ [Ne] 3s2 3p0
For transition metals remove ns electrons and then (n - 1) electronsFe [Ar] 4s2 3d5
loses 2 electrons ---gt Fe2+ [Ar] 4s0 3d6
loses 3 electrons ---gt Fe3+
[Ar] 4s0 3d5
Information Contained on the Periodic Table1 Each group member has the same valence electron configuration
(these electrons primarily determine an atomrsquos chemistry)
2 The electron configuration of any representative element (see order)
3 Certain groups have special names (alkali metals halogens etc)02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
4 Metals and nonmetals are characterized by their chemical and physical properties
Periodic Trends overall change in physical property through row or group on the periodic
table These are general trends (there are exceptions)
Trend 1 Atomic Radius
Trend 2 Ionic Radius
Cations (positive ions) generally are smaller than their respective atoms
Anions (negative ions) generally are larger than their respective atoms
Trend 3 ndash Ionization Energy (IE)
Trend 4 ndash Electronegativity (en)
Redox Reactions Why do metals lose electrons in their reactions
Why does Mg form Mg2+ ions and not Mg3+Why do nonmetals take on electrons
Electron Affinity A few elements GAIN electrons to form anions
Electron affinity is the energy involved when an anion loses an electron A -(g) rarr A(g) + e- EA = ΔE
EA = 141 kJΔE is ENDOthermic because O has an affinity for an e-
O [He] - ion
[He] O atom
EA = 0 kJΔE is zero for N-
due to electron-electron repulsions
Trend 5 Electron AffinityAffinity for electron increases across a period (EA becomes more negative)
Reason
Affinity decreases down a group (EA becomes less negative)
Reason
[He] N- ion
[He] N atom
Atom EAF +328 kJCl+349 kJBr+325 kJI +295 kJ
1 2 3 4 5 6 7S1
S2
S3
S4
0
50
100
150
200
250
300
350
Elec
tron
affi
nity
(kJm
ol)
Group
Period
02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
Increasing Periodic Trends
electronegativity ionization energy ionic radii electron affinityatomic radii
ionic amp atomic radii
ionization energyelectron affinity amp electronegativity
Transfer of energy is quantized and can only occur in discrete units called quanta
∆ E=hν=hcλ
ΔE = change in energy (J)h = Planckrsquos constant 6626 x 10-34 J s ν = frequency (s-1) λ = wavelength (m)
Photoelectric EffectAlbert Einstein (1879-1955)
Experiment demonstrates the particle nature of light Einstein called light particles ldquophotonsrdquo
Classical theory said that E of ejected electron should increase with increase in light intensityhellip but
No e- observed until light of a certain minimum E is used Number of e- ejected depends on light intensity
Energy has mass E = mc2
E = energy m = mass c = speed of light
Classical physics viewed light as a form of energy so it predicted that a metal would eventually collect enough energy to eject an electron regardless of the wavelength of the light
The emission of electrons from a metal when light shines on the metal
For a given metal no electrons were emitted if the frequency of light was below a ldquothresholdrdquo value regardless of how long the light was shining on the metal
Ephoton = hcλ
mphoton = hλc
Hence the dual nature of light or wave-particle duality
Line Spectra of excited atomsExcited atoms emit light of only certain wavelengthsThe wavelengths of emitted light depend on the element Observe spectrum tubes with diffraction gratings (spectroscopes)
Visible lines in H atom spectrum are called the BALMER series
Continuous spectrum Contains all the wavelengths of light
Line (discrete) spectrum Contains only some of the wavelengths of light
Niels Bohr (1885-1962) Bohrrsquos greatest contribution to science was in building a simple model of the atom It was based on an understanding of the SHARP LINE SPECTRA of excited atoms
One view of atomic structure in early 20th century was that an electron (e-) traveled about the nucleus in an orbit (Bohrrsquos Atomic Model)
+Electronorbit
1 Any orbit should be possible and so is any energy2 But a charged particle moving in an electric field should emit energy
End result should be destruction
Bohr said classical view is wrong Need a new theory mdash now called QUANTUM or WAVE MECHANICS e- can only exist in certain discrete orbits mdash called stationary states e- is restricted to QUANTIZED energy states Energy of state = - Cn2 where C is a constant amp where n = quantum no = 1 2 3 4
Bohr Model The e- in a hydrogen atom moves around the nucleus only in certain allowed circular
orbits
E = energy of the levels in the H-atomz = nuclear charge (for H z = 1)n = an integer
E becomes more negative as the electron moves closer to the nucleus
Ground State The lowest possible energy state for an atom (n = 1)
Shielding Effect Higher energy electrons are in outer shells and are easier to remove because they are more shielded from the positive nucleus by inner shell electrons
Energy Changes in the Hydrogen AtomΔE = Efinal state ndash Einitial state
λ= hcΔE
Failure of Bohr ModelFailure of Bohr Model The Bohr Model of the atom paved the way for the Quantum Mechanical Theory
but current theory is in no way derived from the Bohr Model of the atom The Bohr Model of the Atom was fundamentally incorrect--electrons do not move in
circular orbits about the nucleus
Umhellipso what is quantum mechanics
Louis deBroglie (1892-1987)
de Broglie (1924) proposed that all moving objects have wave properties
λ = hm v
λ = wavelength (m)h = Planckrsquos constant 6626 x 10-34 J s = kg m2 s-1 m = mass (kg)v = velocity (ms) ndash do not confuse with nu (frequency) or c (speed of light) ndash do not confuse with nu (frequency) or c (speed of light)
See Sample Exercise 73 on page 298
Baseball (0100 kg) at 35 ms
λ = 19 x 10-34 m
e- with velocity = 10 x 107 ms
λ = 727 x 10-11 m
Erwin Schrodinger 1887-1961
Schrodinger applied idea of e- behaving as a wave to the problem of electrons in atomsWave Equation Based on the wave properties of the atom
Ĥ ψ = E ψψ = wave function Ĥ = mathematical operatorE = total energy of the atomA specific wave function is often called an orbital Electrons move in orbitals not Bohr orbits
Werner Heisenberg 1901-1976
Heisenberg Uncertainty Principle Problem of defining nature of electrons in atoms solved by Werner Heisenberg Cannot simultaneously define the position and momentum (p = mbullv) of an electron We define e- energy exactly but accept the limitation that we do not know exact
position
x = positionmv = momentum (p)h = Planckrsquos constant
The more accurately we know a particlersquos position the less accurately we can know its momentum
Probability Distribution square of the wave function (ψ2) probability of finding an electron at a given position Radial probability distribution is the probability distribution in each spherical shell
Quantum Numbers describe the location of the eQuantum Numbers describe the location of the e--
symbol
name possible values what it tells about electron
cloud
n principal quantum number
1-7 size(energy level)
langular momentum(sublevel) quantum
numberl =0 to n-1 shape
l = 0 (s sublevel) l = 1 (p sublevel) l = 2 (d sublevel) l = 3 (f sublevel)
ml magnetic quantum number m
l = l to -l 3D orientation
in space
ms spin quantum number plusmn 12
spin states of electron
Pauli Exclusion Principle In a given atom no two electrons can have the same set of four quantum numbers
(n l ml ms) Therefore an orbital can hold only two electrons and they must have opposite spins
Shapes of Electron Orbitals
The following are graphical representations of the shapes of the orbitals within atoms Remember these shapes do not exist but are mainly three-dimensional probabilities of locating the electron Also remember a maximum of two electrons can occupy any of the following shapes
How many different kinds of orbitals does each energy level have n =
the number of the energy level
n2 = the number of orbitals in an energy level 2n2 = the number of electrons in an energy level
s-orbital (spherical)The following picture shows the relative sizes of 1s 2s and 3s orbitals
p-orbital (dumbbell)
3 orbitals px py pz - The three p orbitals lie 90deg apart in space
When l = 1 there is a PLANAR NODE thru the nucleus When n = 2 then l = 0 and 1Therefore in n = 2 shell there are 2 types of orbitals mdash 2 subshells For l = 0 m
l = 0 this is a s subshell
For l = 1 ml = -1 0 +1 this is a p subshell with 3 orbitals
d-orbital (double dumbbell and dumbbelldonut)5 orbitalsWhen n = 3 what are the values of l
l = 0 1 2 and so there are 3 subshells in the shell
For l = 0 ml = 0 ---gt s subshell with single orbital
For l = 1 ml = -1 0 +1 ---gt p subshell with 3 orbitals
For l = 2 ml = -2 -1 0 +1 +2---gt d subshell with 5 orbitals
s orbitals have no planar node (l = 0) and so are spherical
p orbitals have l = 1 and have 1 planar node and so are ldquodumbbellrdquo shaped
This means d orbitals (with l = 2) have 2 planar nodes
f-orbital (quadruple dumbbell and dumbbelldouble donut)7 orbitalsWhen n = 4 When n = 4 l = 0 1 2 3 so there are 4 subshells in the shell = 0 1 2 3 so there are 4 subshells in the shell
For For l = 0 = 0 ml = 0 ---gt s subshell with single orbital = 0 ---gt s subshell with single orbital
For For l = 1 = 1 ml = -1 0 +1 ---gt p subshell with 3 orbitals = -1 0 +1 ---gt p subshell with 3 orbitals
For For l = 2 = 2 ml = -2 -1 0 +1 +2 = -2 -1 0 +1 +2 ---gt d subshell with 5 orbitals ---gt d subshell with 5 orbitals
For For l = 3 = 3 ml = -3 -2 -1 0 +1 +2 +3 = -3 -2 -1 0 +1 +2 +3 ---gt f subshell with 7 orbitals ---gt f subshell with 7 orbitals
Aufbau principleAs protons are added one by one to the nucleus to build up the elements electrons
are similarly added to these hydrogen-like orbitals
electron filling order (aufbau)
Hundrsquos Rule The lowest energy configuration for an atom is the one having the maximum number of unpaired electrons allowed by the Pauli principle in a particular set of degenerate (same energy) orbitals
Valence electrons electrons in the outermost principle quantum level of an atomThe inner electron are called core electrons
atom valence electronsCa 2N 5Br 7Arrangement of Electrons in Atoms
Shells (energy levels) = ndarr
Sublevels = ldarr
Orbitals = ml
Assigning electrons to atomsAssigning electrons to atomsElectrons generally assigned to orbitals of successively higher energyFor H atoms - Cn2 E depends only on nFor many-electron atoms energy depends on both n and l
Effective Nuclear Charge Zeff
Zeff is the nuclear charge experienced by the outermost electrons Explains why E(2s) lt E(2p)
Zeff increases across a period owing to incomplete shielding by inner electrons
Estimate Zeff by --gt [ Z - (no inner electrons) ]
Charge felt by 2s e- in Li Zeff = 3 - 2 = 1Be Zeff = 4 - 2 = 2B Zeff = 5 - 2 = 3and so on
Writing Atomic Electron Configurations
Orbital Notation Each electron is represented by a half-arrow
When electrons share an orbital opposite spins are represented by half-arrows going in opposite directions
Examples Write the orbital notation for the following atoms
N (7 e-) ____ ____ ____ ____ ____
1s 2s 2p
P ( ___ e-)
Electron Configuration Notation Write the energy level and orbital (in increasing energy) Write the number of electrons in the sublevel with a superscript
Examples Write the electron configuration notation for the following atoms
N
P
Tc
Electron Configuration Notation (Noble Gas Shorthand) Start with the noble gas ldquocloset without going overrdquo in brackets Continue normal electron configuration
Examples Write the electron configuration notation for the PREVIOUS atoms (use the noble gas shorthand)
Lewis Dot Diagrams
Valence electrons (e- in the outermost energy level) are the only electrons that are lost or gained in ordinary chemical reactions
Lewis Dot Diagrams only include electrons in valence (highest energy level) Write the letter and dots around the outside (2 on each side maximum of 8)
Examples Draw the Lewis Dot Diagram for
N Ca Cl
Ion configurations To form cations from elements remove 1 or more e- from subshell of highest n [or highest (n + l)]
P [Ne] 3s2 3p3 - 3e- ---gt P3+ [Ne] 3s2 3p0
For transition metals remove ns electrons and then (n - 1) electronsFe [Ar] 4s2 3d5
loses 2 electrons ---gt Fe2+ [Ar] 4s0 3d6
loses 3 electrons ---gt Fe3+
[Ar] 4s0 3d5
Information Contained on the Periodic Table1 Each group member has the same valence electron configuration
(these electrons primarily determine an atomrsquos chemistry)
2 The electron configuration of any representative element (see order)
3 Certain groups have special names (alkali metals halogens etc)02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
4 Metals and nonmetals are characterized by their chemical and physical properties
Periodic Trends overall change in physical property through row or group on the periodic
table These are general trends (there are exceptions)
Trend 1 Atomic Radius
Trend 2 Ionic Radius
Cations (positive ions) generally are smaller than their respective atoms
Anions (negative ions) generally are larger than their respective atoms
Trend 3 ndash Ionization Energy (IE)
Trend 4 ndash Electronegativity (en)
Redox Reactions Why do metals lose electrons in their reactions
Why does Mg form Mg2+ ions and not Mg3+Why do nonmetals take on electrons
Electron Affinity A few elements GAIN electrons to form anions
Electron affinity is the energy involved when an anion loses an electron A -(g) rarr A(g) + e- EA = ΔE
EA = 141 kJΔE is ENDOthermic because O has an affinity for an e-
O [He] - ion
[He] O atom
EA = 0 kJΔE is zero for N-
due to electron-electron repulsions
Trend 5 Electron AffinityAffinity for electron increases across a period (EA becomes more negative)
Reason
Affinity decreases down a group (EA becomes less negative)
Reason
[He] N- ion
[He] N atom
Atom EAF +328 kJCl+349 kJBr+325 kJI +295 kJ
1 2 3 4 5 6 7S1
S2
S3
S4
0
50
100
150
200
250
300
350
Elec
tron
affi
nity
(kJm
ol)
Group
Period
02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
Increasing Periodic Trends
electronegativity ionization energy ionic radii electron affinityatomic radii
ionic amp atomic radii
ionization energyelectron affinity amp electronegativity
Ephoton = hcλ
mphoton = hλc
Hence the dual nature of light or wave-particle duality
Line Spectra of excited atomsExcited atoms emit light of only certain wavelengthsThe wavelengths of emitted light depend on the element Observe spectrum tubes with diffraction gratings (spectroscopes)
Visible lines in H atom spectrum are called the BALMER series
Continuous spectrum Contains all the wavelengths of light
Line (discrete) spectrum Contains only some of the wavelengths of light
Niels Bohr (1885-1962) Bohrrsquos greatest contribution to science was in building a simple model of the atom It was based on an understanding of the SHARP LINE SPECTRA of excited atoms
One view of atomic structure in early 20th century was that an electron (e-) traveled about the nucleus in an orbit (Bohrrsquos Atomic Model)
+Electronorbit
1 Any orbit should be possible and so is any energy2 But a charged particle moving in an electric field should emit energy
End result should be destruction
Bohr said classical view is wrong Need a new theory mdash now called QUANTUM or WAVE MECHANICS e- can only exist in certain discrete orbits mdash called stationary states e- is restricted to QUANTIZED energy states Energy of state = - Cn2 where C is a constant amp where n = quantum no = 1 2 3 4
Bohr Model The e- in a hydrogen atom moves around the nucleus only in certain allowed circular
orbits
E = energy of the levels in the H-atomz = nuclear charge (for H z = 1)n = an integer
E becomes more negative as the electron moves closer to the nucleus
Ground State The lowest possible energy state for an atom (n = 1)
Shielding Effect Higher energy electrons are in outer shells and are easier to remove because they are more shielded from the positive nucleus by inner shell electrons
Energy Changes in the Hydrogen AtomΔE = Efinal state ndash Einitial state
λ= hcΔE
Failure of Bohr ModelFailure of Bohr Model The Bohr Model of the atom paved the way for the Quantum Mechanical Theory
but current theory is in no way derived from the Bohr Model of the atom The Bohr Model of the Atom was fundamentally incorrect--electrons do not move in
circular orbits about the nucleus
Umhellipso what is quantum mechanics
Louis deBroglie (1892-1987)
de Broglie (1924) proposed that all moving objects have wave properties
λ = hm v
λ = wavelength (m)h = Planckrsquos constant 6626 x 10-34 J s = kg m2 s-1 m = mass (kg)v = velocity (ms) ndash do not confuse with nu (frequency) or c (speed of light) ndash do not confuse with nu (frequency) or c (speed of light)
See Sample Exercise 73 on page 298
Baseball (0100 kg) at 35 ms
λ = 19 x 10-34 m
e- with velocity = 10 x 107 ms
λ = 727 x 10-11 m
Erwin Schrodinger 1887-1961
Schrodinger applied idea of e- behaving as a wave to the problem of electrons in atomsWave Equation Based on the wave properties of the atom
Ĥ ψ = E ψψ = wave function Ĥ = mathematical operatorE = total energy of the atomA specific wave function is often called an orbital Electrons move in orbitals not Bohr orbits
Werner Heisenberg 1901-1976
Heisenberg Uncertainty Principle Problem of defining nature of electrons in atoms solved by Werner Heisenberg Cannot simultaneously define the position and momentum (p = mbullv) of an electron We define e- energy exactly but accept the limitation that we do not know exact
position
x = positionmv = momentum (p)h = Planckrsquos constant
The more accurately we know a particlersquos position the less accurately we can know its momentum
Probability Distribution square of the wave function (ψ2) probability of finding an electron at a given position Radial probability distribution is the probability distribution in each spherical shell
Quantum Numbers describe the location of the eQuantum Numbers describe the location of the e--
symbol
name possible values what it tells about electron
cloud
n principal quantum number
1-7 size(energy level)
langular momentum(sublevel) quantum
numberl =0 to n-1 shape
l = 0 (s sublevel) l = 1 (p sublevel) l = 2 (d sublevel) l = 3 (f sublevel)
ml magnetic quantum number m
l = l to -l 3D orientation
in space
ms spin quantum number plusmn 12
spin states of electron
Pauli Exclusion Principle In a given atom no two electrons can have the same set of four quantum numbers
(n l ml ms) Therefore an orbital can hold only two electrons and they must have opposite spins
Shapes of Electron Orbitals
The following are graphical representations of the shapes of the orbitals within atoms Remember these shapes do not exist but are mainly three-dimensional probabilities of locating the electron Also remember a maximum of two electrons can occupy any of the following shapes
How many different kinds of orbitals does each energy level have n =
the number of the energy level
n2 = the number of orbitals in an energy level 2n2 = the number of electrons in an energy level
s-orbital (spherical)The following picture shows the relative sizes of 1s 2s and 3s orbitals
p-orbital (dumbbell)
3 orbitals px py pz - The three p orbitals lie 90deg apart in space
When l = 1 there is a PLANAR NODE thru the nucleus When n = 2 then l = 0 and 1Therefore in n = 2 shell there are 2 types of orbitals mdash 2 subshells For l = 0 m
l = 0 this is a s subshell
For l = 1 ml = -1 0 +1 this is a p subshell with 3 orbitals
d-orbital (double dumbbell and dumbbelldonut)5 orbitalsWhen n = 3 what are the values of l
l = 0 1 2 and so there are 3 subshells in the shell
For l = 0 ml = 0 ---gt s subshell with single orbital
For l = 1 ml = -1 0 +1 ---gt p subshell with 3 orbitals
For l = 2 ml = -2 -1 0 +1 +2---gt d subshell with 5 orbitals
s orbitals have no planar node (l = 0) and so are spherical
p orbitals have l = 1 and have 1 planar node and so are ldquodumbbellrdquo shaped
This means d orbitals (with l = 2) have 2 planar nodes
f-orbital (quadruple dumbbell and dumbbelldouble donut)7 orbitalsWhen n = 4 When n = 4 l = 0 1 2 3 so there are 4 subshells in the shell = 0 1 2 3 so there are 4 subshells in the shell
For For l = 0 = 0 ml = 0 ---gt s subshell with single orbital = 0 ---gt s subshell with single orbital
For For l = 1 = 1 ml = -1 0 +1 ---gt p subshell with 3 orbitals = -1 0 +1 ---gt p subshell with 3 orbitals
For For l = 2 = 2 ml = -2 -1 0 +1 +2 = -2 -1 0 +1 +2 ---gt d subshell with 5 orbitals ---gt d subshell with 5 orbitals
For For l = 3 = 3 ml = -3 -2 -1 0 +1 +2 +3 = -3 -2 -1 0 +1 +2 +3 ---gt f subshell with 7 orbitals ---gt f subshell with 7 orbitals
Aufbau principleAs protons are added one by one to the nucleus to build up the elements electrons
are similarly added to these hydrogen-like orbitals
electron filling order (aufbau)
Hundrsquos Rule The lowest energy configuration for an atom is the one having the maximum number of unpaired electrons allowed by the Pauli principle in a particular set of degenerate (same energy) orbitals
Valence electrons electrons in the outermost principle quantum level of an atomThe inner electron are called core electrons
atom valence electronsCa 2N 5Br 7Arrangement of Electrons in Atoms
Shells (energy levels) = ndarr
Sublevels = ldarr
Orbitals = ml
Assigning electrons to atomsAssigning electrons to atomsElectrons generally assigned to orbitals of successively higher energyFor H atoms - Cn2 E depends only on nFor many-electron atoms energy depends on both n and l
Effective Nuclear Charge Zeff
Zeff is the nuclear charge experienced by the outermost electrons Explains why E(2s) lt E(2p)
Zeff increases across a period owing to incomplete shielding by inner electrons
Estimate Zeff by --gt [ Z - (no inner electrons) ]
Charge felt by 2s e- in Li Zeff = 3 - 2 = 1Be Zeff = 4 - 2 = 2B Zeff = 5 - 2 = 3and so on
Writing Atomic Electron Configurations
Orbital Notation Each electron is represented by a half-arrow
When electrons share an orbital opposite spins are represented by half-arrows going in opposite directions
Examples Write the orbital notation for the following atoms
N (7 e-) ____ ____ ____ ____ ____
1s 2s 2p
P ( ___ e-)
Electron Configuration Notation Write the energy level and orbital (in increasing energy) Write the number of electrons in the sublevel with a superscript
Examples Write the electron configuration notation for the following atoms
N
P
Tc
Electron Configuration Notation (Noble Gas Shorthand) Start with the noble gas ldquocloset without going overrdquo in brackets Continue normal electron configuration
Examples Write the electron configuration notation for the PREVIOUS atoms (use the noble gas shorthand)
Lewis Dot Diagrams
Valence electrons (e- in the outermost energy level) are the only electrons that are lost or gained in ordinary chemical reactions
Lewis Dot Diagrams only include electrons in valence (highest energy level) Write the letter and dots around the outside (2 on each side maximum of 8)
Examples Draw the Lewis Dot Diagram for
N Ca Cl
Ion configurations To form cations from elements remove 1 or more e- from subshell of highest n [or highest (n + l)]
P [Ne] 3s2 3p3 - 3e- ---gt P3+ [Ne] 3s2 3p0
For transition metals remove ns electrons and then (n - 1) electronsFe [Ar] 4s2 3d5
loses 2 electrons ---gt Fe2+ [Ar] 4s0 3d6
loses 3 electrons ---gt Fe3+
[Ar] 4s0 3d5
Information Contained on the Periodic Table1 Each group member has the same valence electron configuration
(these electrons primarily determine an atomrsquos chemistry)
2 The electron configuration of any representative element (see order)
3 Certain groups have special names (alkali metals halogens etc)02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
4 Metals and nonmetals are characterized by their chemical and physical properties
Periodic Trends overall change in physical property through row or group on the periodic
table These are general trends (there are exceptions)
Trend 1 Atomic Radius
Trend 2 Ionic Radius
Cations (positive ions) generally are smaller than their respective atoms
Anions (negative ions) generally are larger than their respective atoms
Trend 3 ndash Ionization Energy (IE)
Trend 4 ndash Electronegativity (en)
Redox Reactions Why do metals lose electrons in their reactions
Why does Mg form Mg2+ ions and not Mg3+Why do nonmetals take on electrons
Electron Affinity A few elements GAIN electrons to form anions
Electron affinity is the energy involved when an anion loses an electron A -(g) rarr A(g) + e- EA = ΔE
EA = 141 kJΔE is ENDOthermic because O has an affinity for an e-
O [He] - ion
[He] O atom
EA = 0 kJΔE is zero for N-
due to electron-electron repulsions
Trend 5 Electron AffinityAffinity for electron increases across a period (EA becomes more negative)
Reason
Affinity decreases down a group (EA becomes less negative)
Reason
[He] N- ion
[He] N atom
Atom EAF +328 kJCl+349 kJBr+325 kJI +295 kJ
1 2 3 4 5 6 7S1
S2
S3
S4
0
50
100
150
200
250
300
350
Elec
tron
affi
nity
(kJm
ol)
Group
Period
02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
Increasing Periodic Trends
electronegativity ionization energy ionic radii electron affinityatomic radii
ionic amp atomic radii
ionization energyelectron affinity amp electronegativity
Niels Bohr (1885-1962) Bohrrsquos greatest contribution to science was in building a simple model of the atom It was based on an understanding of the SHARP LINE SPECTRA of excited atoms
One view of atomic structure in early 20th century was that an electron (e-) traveled about the nucleus in an orbit (Bohrrsquos Atomic Model)
+Electronorbit
1 Any orbit should be possible and so is any energy2 But a charged particle moving in an electric field should emit energy
End result should be destruction
Bohr said classical view is wrong Need a new theory mdash now called QUANTUM or WAVE MECHANICS e- can only exist in certain discrete orbits mdash called stationary states e- is restricted to QUANTIZED energy states Energy of state = - Cn2 where C is a constant amp where n = quantum no = 1 2 3 4
Bohr Model The e- in a hydrogen atom moves around the nucleus only in certain allowed circular
orbits
E = energy of the levels in the H-atomz = nuclear charge (for H z = 1)n = an integer
E becomes more negative as the electron moves closer to the nucleus
Ground State The lowest possible energy state for an atom (n = 1)
Shielding Effect Higher energy electrons are in outer shells and are easier to remove because they are more shielded from the positive nucleus by inner shell electrons
Energy Changes in the Hydrogen AtomΔE = Efinal state ndash Einitial state
λ= hcΔE
Failure of Bohr ModelFailure of Bohr Model The Bohr Model of the atom paved the way for the Quantum Mechanical Theory
but current theory is in no way derived from the Bohr Model of the atom The Bohr Model of the Atom was fundamentally incorrect--electrons do not move in
circular orbits about the nucleus
Umhellipso what is quantum mechanics
Louis deBroglie (1892-1987)
de Broglie (1924) proposed that all moving objects have wave properties
λ = hm v
λ = wavelength (m)h = Planckrsquos constant 6626 x 10-34 J s = kg m2 s-1 m = mass (kg)v = velocity (ms) ndash do not confuse with nu (frequency) or c (speed of light) ndash do not confuse with nu (frequency) or c (speed of light)
See Sample Exercise 73 on page 298
Baseball (0100 kg) at 35 ms
λ = 19 x 10-34 m
e- with velocity = 10 x 107 ms
λ = 727 x 10-11 m
Erwin Schrodinger 1887-1961
Schrodinger applied idea of e- behaving as a wave to the problem of electrons in atomsWave Equation Based on the wave properties of the atom
Ĥ ψ = E ψψ = wave function Ĥ = mathematical operatorE = total energy of the atomA specific wave function is often called an orbital Electrons move in orbitals not Bohr orbits
Werner Heisenberg 1901-1976
Heisenberg Uncertainty Principle Problem of defining nature of electrons in atoms solved by Werner Heisenberg Cannot simultaneously define the position and momentum (p = mbullv) of an electron We define e- energy exactly but accept the limitation that we do not know exact
position
x = positionmv = momentum (p)h = Planckrsquos constant
The more accurately we know a particlersquos position the less accurately we can know its momentum
Probability Distribution square of the wave function (ψ2) probability of finding an electron at a given position Radial probability distribution is the probability distribution in each spherical shell
Quantum Numbers describe the location of the eQuantum Numbers describe the location of the e--
symbol
name possible values what it tells about electron
cloud
n principal quantum number
1-7 size(energy level)
langular momentum(sublevel) quantum
numberl =0 to n-1 shape
l = 0 (s sublevel) l = 1 (p sublevel) l = 2 (d sublevel) l = 3 (f sublevel)
ml magnetic quantum number m
l = l to -l 3D orientation
in space
ms spin quantum number plusmn 12
spin states of electron
Pauli Exclusion Principle In a given atom no two electrons can have the same set of four quantum numbers
(n l ml ms) Therefore an orbital can hold only two electrons and they must have opposite spins
Shapes of Electron Orbitals
The following are graphical representations of the shapes of the orbitals within atoms Remember these shapes do not exist but are mainly three-dimensional probabilities of locating the electron Also remember a maximum of two electrons can occupy any of the following shapes
How many different kinds of orbitals does each energy level have n =
the number of the energy level
n2 = the number of orbitals in an energy level 2n2 = the number of electrons in an energy level
s-orbital (spherical)The following picture shows the relative sizes of 1s 2s and 3s orbitals
p-orbital (dumbbell)
3 orbitals px py pz - The three p orbitals lie 90deg apart in space
When l = 1 there is a PLANAR NODE thru the nucleus When n = 2 then l = 0 and 1Therefore in n = 2 shell there are 2 types of orbitals mdash 2 subshells For l = 0 m
l = 0 this is a s subshell
For l = 1 ml = -1 0 +1 this is a p subshell with 3 orbitals
d-orbital (double dumbbell and dumbbelldonut)5 orbitalsWhen n = 3 what are the values of l
l = 0 1 2 and so there are 3 subshells in the shell
For l = 0 ml = 0 ---gt s subshell with single orbital
For l = 1 ml = -1 0 +1 ---gt p subshell with 3 orbitals
For l = 2 ml = -2 -1 0 +1 +2---gt d subshell with 5 orbitals
s orbitals have no planar node (l = 0) and so are spherical
p orbitals have l = 1 and have 1 planar node and so are ldquodumbbellrdquo shaped
This means d orbitals (with l = 2) have 2 planar nodes
f-orbital (quadruple dumbbell and dumbbelldouble donut)7 orbitalsWhen n = 4 When n = 4 l = 0 1 2 3 so there are 4 subshells in the shell = 0 1 2 3 so there are 4 subshells in the shell
For For l = 0 = 0 ml = 0 ---gt s subshell with single orbital = 0 ---gt s subshell with single orbital
For For l = 1 = 1 ml = -1 0 +1 ---gt p subshell with 3 orbitals = -1 0 +1 ---gt p subshell with 3 orbitals
For For l = 2 = 2 ml = -2 -1 0 +1 +2 = -2 -1 0 +1 +2 ---gt d subshell with 5 orbitals ---gt d subshell with 5 orbitals
For For l = 3 = 3 ml = -3 -2 -1 0 +1 +2 +3 = -3 -2 -1 0 +1 +2 +3 ---gt f subshell with 7 orbitals ---gt f subshell with 7 orbitals
Aufbau principleAs protons are added one by one to the nucleus to build up the elements electrons
are similarly added to these hydrogen-like orbitals
electron filling order (aufbau)
Hundrsquos Rule The lowest energy configuration for an atom is the one having the maximum number of unpaired electrons allowed by the Pauli principle in a particular set of degenerate (same energy) orbitals
Valence electrons electrons in the outermost principle quantum level of an atomThe inner electron are called core electrons
atom valence electronsCa 2N 5Br 7Arrangement of Electrons in Atoms
Shells (energy levels) = ndarr
Sublevels = ldarr
Orbitals = ml
Assigning electrons to atomsAssigning electrons to atomsElectrons generally assigned to orbitals of successively higher energyFor H atoms - Cn2 E depends only on nFor many-electron atoms energy depends on both n and l
Effective Nuclear Charge Zeff
Zeff is the nuclear charge experienced by the outermost electrons Explains why E(2s) lt E(2p)
Zeff increases across a period owing to incomplete shielding by inner electrons
Estimate Zeff by --gt [ Z - (no inner electrons) ]
Charge felt by 2s e- in Li Zeff = 3 - 2 = 1Be Zeff = 4 - 2 = 2B Zeff = 5 - 2 = 3and so on
Writing Atomic Electron Configurations
Orbital Notation Each electron is represented by a half-arrow
When electrons share an orbital opposite spins are represented by half-arrows going in opposite directions
Examples Write the orbital notation for the following atoms
N (7 e-) ____ ____ ____ ____ ____
1s 2s 2p
P ( ___ e-)
Electron Configuration Notation Write the energy level and orbital (in increasing energy) Write the number of electrons in the sublevel with a superscript
Examples Write the electron configuration notation for the following atoms
N
P
Tc
Electron Configuration Notation (Noble Gas Shorthand) Start with the noble gas ldquocloset without going overrdquo in brackets Continue normal electron configuration
Examples Write the electron configuration notation for the PREVIOUS atoms (use the noble gas shorthand)
Lewis Dot Diagrams
Valence electrons (e- in the outermost energy level) are the only electrons that are lost or gained in ordinary chemical reactions
Lewis Dot Diagrams only include electrons in valence (highest energy level) Write the letter and dots around the outside (2 on each side maximum of 8)
Examples Draw the Lewis Dot Diagram for
N Ca Cl
Ion configurations To form cations from elements remove 1 or more e- from subshell of highest n [or highest (n + l)]
P [Ne] 3s2 3p3 - 3e- ---gt P3+ [Ne] 3s2 3p0
For transition metals remove ns electrons and then (n - 1) electronsFe [Ar] 4s2 3d5
loses 2 electrons ---gt Fe2+ [Ar] 4s0 3d6
loses 3 electrons ---gt Fe3+
[Ar] 4s0 3d5
Information Contained on the Periodic Table1 Each group member has the same valence electron configuration
(these electrons primarily determine an atomrsquos chemistry)
2 The electron configuration of any representative element (see order)
3 Certain groups have special names (alkali metals halogens etc)02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
4 Metals and nonmetals are characterized by their chemical and physical properties
Periodic Trends overall change in physical property through row or group on the periodic
table These are general trends (there are exceptions)
Trend 1 Atomic Radius
Trend 2 Ionic Radius
Cations (positive ions) generally are smaller than their respective atoms
Anions (negative ions) generally are larger than their respective atoms
Trend 3 ndash Ionization Energy (IE)
Trend 4 ndash Electronegativity (en)
Redox Reactions Why do metals lose electrons in their reactions
Why does Mg form Mg2+ ions and not Mg3+Why do nonmetals take on electrons
Electron Affinity A few elements GAIN electrons to form anions
Electron affinity is the energy involved when an anion loses an electron A -(g) rarr A(g) + e- EA = ΔE
EA = 141 kJΔE is ENDOthermic because O has an affinity for an e-
O [He] - ion
[He] O atom
EA = 0 kJΔE is zero for N-
due to electron-electron repulsions
Trend 5 Electron AffinityAffinity for electron increases across a period (EA becomes more negative)
Reason
Affinity decreases down a group (EA becomes less negative)
Reason
[He] N- ion
[He] N atom
Atom EAF +328 kJCl+349 kJBr+325 kJI +295 kJ
1 2 3 4 5 6 7S1
S2
S3
S4
0
50
100
150
200
250
300
350
Elec
tron
affi
nity
(kJm
ol)
Group
Period
02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
Increasing Periodic Trends
electronegativity ionization energy ionic radii electron affinityatomic radii
ionic amp atomic radii
ionization energyelectron affinity amp electronegativity
Umhellipso what is quantum mechanics
Louis deBroglie (1892-1987)
de Broglie (1924) proposed that all moving objects have wave properties
λ = hm v
λ = wavelength (m)h = Planckrsquos constant 6626 x 10-34 J s = kg m2 s-1 m = mass (kg)v = velocity (ms) ndash do not confuse with nu (frequency) or c (speed of light) ndash do not confuse with nu (frequency) or c (speed of light)
See Sample Exercise 73 on page 298
Baseball (0100 kg) at 35 ms
λ = 19 x 10-34 m
e- with velocity = 10 x 107 ms
λ = 727 x 10-11 m
Erwin Schrodinger 1887-1961
Schrodinger applied idea of e- behaving as a wave to the problem of electrons in atomsWave Equation Based on the wave properties of the atom
Ĥ ψ = E ψψ = wave function Ĥ = mathematical operatorE = total energy of the atomA specific wave function is often called an orbital Electrons move in orbitals not Bohr orbits
Werner Heisenberg 1901-1976
Heisenberg Uncertainty Principle Problem of defining nature of electrons in atoms solved by Werner Heisenberg Cannot simultaneously define the position and momentum (p = mbullv) of an electron We define e- energy exactly but accept the limitation that we do not know exact
position
x = positionmv = momentum (p)h = Planckrsquos constant
The more accurately we know a particlersquos position the less accurately we can know its momentum
Probability Distribution square of the wave function (ψ2) probability of finding an electron at a given position Radial probability distribution is the probability distribution in each spherical shell
Quantum Numbers describe the location of the eQuantum Numbers describe the location of the e--
symbol
name possible values what it tells about electron
cloud
n principal quantum number
1-7 size(energy level)
langular momentum(sublevel) quantum
numberl =0 to n-1 shape
l = 0 (s sublevel) l = 1 (p sublevel) l = 2 (d sublevel) l = 3 (f sublevel)
ml magnetic quantum number m
l = l to -l 3D orientation
in space
ms spin quantum number plusmn 12
spin states of electron
Pauli Exclusion Principle In a given atom no two electrons can have the same set of four quantum numbers
(n l ml ms) Therefore an orbital can hold only two electrons and they must have opposite spins
Shapes of Electron Orbitals
The following are graphical representations of the shapes of the orbitals within atoms Remember these shapes do not exist but are mainly three-dimensional probabilities of locating the electron Also remember a maximum of two electrons can occupy any of the following shapes
How many different kinds of orbitals does each energy level have n =
the number of the energy level
n2 = the number of orbitals in an energy level 2n2 = the number of electrons in an energy level
s-orbital (spherical)The following picture shows the relative sizes of 1s 2s and 3s orbitals
p-orbital (dumbbell)
3 orbitals px py pz - The three p orbitals lie 90deg apart in space
When l = 1 there is a PLANAR NODE thru the nucleus When n = 2 then l = 0 and 1Therefore in n = 2 shell there are 2 types of orbitals mdash 2 subshells For l = 0 m
l = 0 this is a s subshell
For l = 1 ml = -1 0 +1 this is a p subshell with 3 orbitals
d-orbital (double dumbbell and dumbbelldonut)5 orbitalsWhen n = 3 what are the values of l
l = 0 1 2 and so there are 3 subshells in the shell
For l = 0 ml = 0 ---gt s subshell with single orbital
For l = 1 ml = -1 0 +1 ---gt p subshell with 3 orbitals
For l = 2 ml = -2 -1 0 +1 +2---gt d subshell with 5 orbitals
s orbitals have no planar node (l = 0) and so are spherical
p orbitals have l = 1 and have 1 planar node and so are ldquodumbbellrdquo shaped
This means d orbitals (with l = 2) have 2 planar nodes
f-orbital (quadruple dumbbell and dumbbelldouble donut)7 orbitalsWhen n = 4 When n = 4 l = 0 1 2 3 so there are 4 subshells in the shell = 0 1 2 3 so there are 4 subshells in the shell
For For l = 0 = 0 ml = 0 ---gt s subshell with single orbital = 0 ---gt s subshell with single orbital
For For l = 1 = 1 ml = -1 0 +1 ---gt p subshell with 3 orbitals = -1 0 +1 ---gt p subshell with 3 orbitals
For For l = 2 = 2 ml = -2 -1 0 +1 +2 = -2 -1 0 +1 +2 ---gt d subshell with 5 orbitals ---gt d subshell with 5 orbitals
For For l = 3 = 3 ml = -3 -2 -1 0 +1 +2 +3 = -3 -2 -1 0 +1 +2 +3 ---gt f subshell with 7 orbitals ---gt f subshell with 7 orbitals
Aufbau principleAs protons are added one by one to the nucleus to build up the elements electrons
are similarly added to these hydrogen-like orbitals
electron filling order (aufbau)
Hundrsquos Rule The lowest energy configuration for an atom is the one having the maximum number of unpaired electrons allowed by the Pauli principle in a particular set of degenerate (same energy) orbitals
Valence electrons electrons in the outermost principle quantum level of an atomThe inner electron are called core electrons
atom valence electronsCa 2N 5Br 7Arrangement of Electrons in Atoms
Shells (energy levels) = ndarr
Sublevels = ldarr
Orbitals = ml
Assigning electrons to atomsAssigning electrons to atomsElectrons generally assigned to orbitals of successively higher energyFor H atoms - Cn2 E depends only on nFor many-electron atoms energy depends on both n and l
Effective Nuclear Charge Zeff
Zeff is the nuclear charge experienced by the outermost electrons Explains why E(2s) lt E(2p)
Zeff increases across a period owing to incomplete shielding by inner electrons
Estimate Zeff by --gt [ Z - (no inner electrons) ]
Charge felt by 2s e- in Li Zeff = 3 - 2 = 1Be Zeff = 4 - 2 = 2B Zeff = 5 - 2 = 3and so on
Writing Atomic Electron Configurations
Orbital Notation Each electron is represented by a half-arrow
When electrons share an orbital opposite spins are represented by half-arrows going in opposite directions
Examples Write the orbital notation for the following atoms
N (7 e-) ____ ____ ____ ____ ____
1s 2s 2p
P ( ___ e-)
Electron Configuration Notation Write the energy level and orbital (in increasing energy) Write the number of electrons in the sublevel with a superscript
Examples Write the electron configuration notation for the following atoms
N
P
Tc
Electron Configuration Notation (Noble Gas Shorthand) Start with the noble gas ldquocloset without going overrdquo in brackets Continue normal electron configuration
Examples Write the electron configuration notation for the PREVIOUS atoms (use the noble gas shorthand)
Lewis Dot Diagrams
Valence electrons (e- in the outermost energy level) are the only electrons that are lost or gained in ordinary chemical reactions
Lewis Dot Diagrams only include electrons in valence (highest energy level) Write the letter and dots around the outside (2 on each side maximum of 8)
Examples Draw the Lewis Dot Diagram for
N Ca Cl
Ion configurations To form cations from elements remove 1 or more e- from subshell of highest n [or highest (n + l)]
P [Ne] 3s2 3p3 - 3e- ---gt P3+ [Ne] 3s2 3p0
For transition metals remove ns electrons and then (n - 1) electronsFe [Ar] 4s2 3d5
loses 2 electrons ---gt Fe2+ [Ar] 4s0 3d6
loses 3 electrons ---gt Fe3+
[Ar] 4s0 3d5
Information Contained on the Periodic Table1 Each group member has the same valence electron configuration
(these electrons primarily determine an atomrsquos chemistry)
2 The electron configuration of any representative element (see order)
3 Certain groups have special names (alkali metals halogens etc)02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
4 Metals and nonmetals are characterized by their chemical and physical properties
Periodic Trends overall change in physical property through row or group on the periodic
table These are general trends (there are exceptions)
Trend 1 Atomic Radius
Trend 2 Ionic Radius
Cations (positive ions) generally are smaller than their respective atoms
Anions (negative ions) generally are larger than their respective atoms
Trend 3 ndash Ionization Energy (IE)
Trend 4 ndash Electronegativity (en)
Redox Reactions Why do metals lose electrons in their reactions
Why does Mg form Mg2+ ions and not Mg3+Why do nonmetals take on electrons
Electron Affinity A few elements GAIN electrons to form anions
Electron affinity is the energy involved when an anion loses an electron A -(g) rarr A(g) + e- EA = ΔE
EA = 141 kJΔE is ENDOthermic because O has an affinity for an e-
O [He] - ion
[He] O atom
EA = 0 kJΔE is zero for N-
due to electron-electron repulsions
Trend 5 Electron AffinityAffinity for electron increases across a period (EA becomes more negative)
Reason
Affinity decreases down a group (EA becomes less negative)
Reason
[He] N- ion
[He] N atom
Atom EAF +328 kJCl+349 kJBr+325 kJI +295 kJ
1 2 3 4 5 6 7S1
S2
S3
S4
0
50
100
150
200
250
300
350
Elec
tron
affi
nity
(kJm
ol)
Group
Period
02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
Increasing Periodic Trends
electronegativity ionization energy ionic radii electron affinityatomic radii
ionic amp atomic radii
ionization energyelectron affinity amp electronegativity
Schrodinger applied idea of e- behaving as a wave to the problem of electrons in atomsWave Equation Based on the wave properties of the atom
Ĥ ψ = E ψψ = wave function Ĥ = mathematical operatorE = total energy of the atomA specific wave function is often called an orbital Electrons move in orbitals not Bohr orbits
Werner Heisenberg 1901-1976
Heisenberg Uncertainty Principle Problem of defining nature of electrons in atoms solved by Werner Heisenberg Cannot simultaneously define the position and momentum (p = mbullv) of an electron We define e- energy exactly but accept the limitation that we do not know exact
position
x = positionmv = momentum (p)h = Planckrsquos constant
The more accurately we know a particlersquos position the less accurately we can know its momentum
Probability Distribution square of the wave function (ψ2) probability of finding an electron at a given position Radial probability distribution is the probability distribution in each spherical shell
Quantum Numbers describe the location of the eQuantum Numbers describe the location of the e--
symbol
name possible values what it tells about electron
cloud
n principal quantum number
1-7 size(energy level)
langular momentum(sublevel) quantum
numberl =0 to n-1 shape
l = 0 (s sublevel) l = 1 (p sublevel) l = 2 (d sublevel) l = 3 (f sublevel)
ml magnetic quantum number m
l = l to -l 3D orientation
in space
ms spin quantum number plusmn 12
spin states of electron
Pauli Exclusion Principle In a given atom no two electrons can have the same set of four quantum numbers
(n l ml ms) Therefore an orbital can hold only two electrons and they must have opposite spins
Shapes of Electron Orbitals
The following are graphical representations of the shapes of the orbitals within atoms Remember these shapes do not exist but are mainly three-dimensional probabilities of locating the electron Also remember a maximum of two electrons can occupy any of the following shapes
How many different kinds of orbitals does each energy level have n =
the number of the energy level
n2 = the number of orbitals in an energy level 2n2 = the number of electrons in an energy level
s-orbital (spherical)The following picture shows the relative sizes of 1s 2s and 3s orbitals
p-orbital (dumbbell)
3 orbitals px py pz - The three p orbitals lie 90deg apart in space
When l = 1 there is a PLANAR NODE thru the nucleus When n = 2 then l = 0 and 1Therefore in n = 2 shell there are 2 types of orbitals mdash 2 subshells For l = 0 m
l = 0 this is a s subshell
For l = 1 ml = -1 0 +1 this is a p subshell with 3 orbitals
d-orbital (double dumbbell and dumbbelldonut)5 orbitalsWhen n = 3 what are the values of l
l = 0 1 2 and so there are 3 subshells in the shell
For l = 0 ml = 0 ---gt s subshell with single orbital
For l = 1 ml = -1 0 +1 ---gt p subshell with 3 orbitals
For l = 2 ml = -2 -1 0 +1 +2---gt d subshell with 5 orbitals
s orbitals have no planar node (l = 0) and so are spherical
p orbitals have l = 1 and have 1 planar node and so are ldquodumbbellrdquo shaped
This means d orbitals (with l = 2) have 2 planar nodes
f-orbital (quadruple dumbbell and dumbbelldouble donut)7 orbitalsWhen n = 4 When n = 4 l = 0 1 2 3 so there are 4 subshells in the shell = 0 1 2 3 so there are 4 subshells in the shell
For For l = 0 = 0 ml = 0 ---gt s subshell with single orbital = 0 ---gt s subshell with single orbital
For For l = 1 = 1 ml = -1 0 +1 ---gt p subshell with 3 orbitals = -1 0 +1 ---gt p subshell with 3 orbitals
For For l = 2 = 2 ml = -2 -1 0 +1 +2 = -2 -1 0 +1 +2 ---gt d subshell with 5 orbitals ---gt d subshell with 5 orbitals
For For l = 3 = 3 ml = -3 -2 -1 0 +1 +2 +3 = -3 -2 -1 0 +1 +2 +3 ---gt f subshell with 7 orbitals ---gt f subshell with 7 orbitals
Aufbau principleAs protons are added one by one to the nucleus to build up the elements electrons
are similarly added to these hydrogen-like orbitals
electron filling order (aufbau)
Hundrsquos Rule The lowest energy configuration for an atom is the one having the maximum number of unpaired electrons allowed by the Pauli principle in a particular set of degenerate (same energy) orbitals
Valence electrons electrons in the outermost principle quantum level of an atomThe inner electron are called core electrons
atom valence electronsCa 2N 5Br 7Arrangement of Electrons in Atoms
Shells (energy levels) = ndarr
Sublevels = ldarr
Orbitals = ml
Assigning electrons to atomsAssigning electrons to atomsElectrons generally assigned to orbitals of successively higher energyFor H atoms - Cn2 E depends only on nFor many-electron atoms energy depends on both n and l
Effective Nuclear Charge Zeff
Zeff is the nuclear charge experienced by the outermost electrons Explains why E(2s) lt E(2p)
Zeff increases across a period owing to incomplete shielding by inner electrons
Estimate Zeff by --gt [ Z - (no inner electrons) ]
Charge felt by 2s e- in Li Zeff = 3 - 2 = 1Be Zeff = 4 - 2 = 2B Zeff = 5 - 2 = 3and so on
Writing Atomic Electron Configurations
Orbital Notation Each electron is represented by a half-arrow
When electrons share an orbital opposite spins are represented by half-arrows going in opposite directions
Examples Write the orbital notation for the following atoms
N (7 e-) ____ ____ ____ ____ ____
1s 2s 2p
P ( ___ e-)
Electron Configuration Notation Write the energy level and orbital (in increasing energy) Write the number of electrons in the sublevel with a superscript
Examples Write the electron configuration notation for the following atoms
N
P
Tc
Electron Configuration Notation (Noble Gas Shorthand) Start with the noble gas ldquocloset without going overrdquo in brackets Continue normal electron configuration
Examples Write the electron configuration notation for the PREVIOUS atoms (use the noble gas shorthand)
Lewis Dot Diagrams
Valence electrons (e- in the outermost energy level) are the only electrons that are lost or gained in ordinary chemical reactions
Lewis Dot Diagrams only include electrons in valence (highest energy level) Write the letter and dots around the outside (2 on each side maximum of 8)
Examples Draw the Lewis Dot Diagram for
N Ca Cl
Ion configurations To form cations from elements remove 1 or more e- from subshell of highest n [or highest (n + l)]
P [Ne] 3s2 3p3 - 3e- ---gt P3+ [Ne] 3s2 3p0
For transition metals remove ns electrons and then (n - 1) electronsFe [Ar] 4s2 3d5
loses 2 electrons ---gt Fe2+ [Ar] 4s0 3d6
loses 3 electrons ---gt Fe3+
[Ar] 4s0 3d5
Information Contained on the Periodic Table1 Each group member has the same valence electron configuration
(these electrons primarily determine an atomrsquos chemistry)
2 The electron configuration of any representative element (see order)
3 Certain groups have special names (alkali metals halogens etc)02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
4 Metals and nonmetals are characterized by their chemical and physical properties
Periodic Trends overall change in physical property through row or group on the periodic
table These are general trends (there are exceptions)
Trend 1 Atomic Radius
Trend 2 Ionic Radius
Cations (positive ions) generally are smaller than their respective atoms
Anions (negative ions) generally are larger than their respective atoms
Trend 3 ndash Ionization Energy (IE)
Trend 4 ndash Electronegativity (en)
Redox Reactions Why do metals lose electrons in their reactions
Why does Mg form Mg2+ ions and not Mg3+Why do nonmetals take on electrons
Electron Affinity A few elements GAIN electrons to form anions
Electron affinity is the energy involved when an anion loses an electron A -(g) rarr A(g) + e- EA = ΔE
EA = 141 kJΔE is ENDOthermic because O has an affinity for an e-
O [He] - ion
[He] O atom
EA = 0 kJΔE is zero for N-
due to electron-electron repulsions
Trend 5 Electron AffinityAffinity for electron increases across a period (EA becomes more negative)
Reason
Affinity decreases down a group (EA becomes less negative)
Reason
[He] N- ion
[He] N atom
Atom EAF +328 kJCl+349 kJBr+325 kJI +295 kJ
1 2 3 4 5 6 7S1
S2
S3
S4
0
50
100
150
200
250
300
350
Elec
tron
affi
nity
(kJm
ol)
Group
Period
02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
Increasing Periodic Trends
electronegativity ionization energy ionic radii electron affinityatomic radii
ionic amp atomic radii
ionization energyelectron affinity amp electronegativity
ml magnetic quantum number m
l = l to -l 3D orientation
in space
ms spin quantum number plusmn 12
spin states of electron
Pauli Exclusion Principle In a given atom no two electrons can have the same set of four quantum numbers
(n l ml ms) Therefore an orbital can hold only two electrons and they must have opposite spins
Shapes of Electron Orbitals
The following are graphical representations of the shapes of the orbitals within atoms Remember these shapes do not exist but are mainly three-dimensional probabilities of locating the electron Also remember a maximum of two electrons can occupy any of the following shapes
How many different kinds of orbitals does each energy level have n =
the number of the energy level
n2 = the number of orbitals in an energy level 2n2 = the number of electrons in an energy level
s-orbital (spherical)The following picture shows the relative sizes of 1s 2s and 3s orbitals
p-orbital (dumbbell)
3 orbitals px py pz - The three p orbitals lie 90deg apart in space
When l = 1 there is a PLANAR NODE thru the nucleus When n = 2 then l = 0 and 1Therefore in n = 2 shell there are 2 types of orbitals mdash 2 subshells For l = 0 m
l = 0 this is a s subshell
For l = 1 ml = -1 0 +1 this is a p subshell with 3 orbitals
d-orbital (double dumbbell and dumbbelldonut)5 orbitalsWhen n = 3 what are the values of l
l = 0 1 2 and so there are 3 subshells in the shell
For l = 0 ml = 0 ---gt s subshell with single orbital
For l = 1 ml = -1 0 +1 ---gt p subshell with 3 orbitals
For l = 2 ml = -2 -1 0 +1 +2---gt d subshell with 5 orbitals
s orbitals have no planar node (l = 0) and so are spherical
p orbitals have l = 1 and have 1 planar node and so are ldquodumbbellrdquo shaped
This means d orbitals (with l = 2) have 2 planar nodes
f-orbital (quadruple dumbbell and dumbbelldouble donut)7 orbitalsWhen n = 4 When n = 4 l = 0 1 2 3 so there are 4 subshells in the shell = 0 1 2 3 so there are 4 subshells in the shell
For For l = 0 = 0 ml = 0 ---gt s subshell with single orbital = 0 ---gt s subshell with single orbital
For For l = 1 = 1 ml = -1 0 +1 ---gt p subshell with 3 orbitals = -1 0 +1 ---gt p subshell with 3 orbitals
For For l = 2 = 2 ml = -2 -1 0 +1 +2 = -2 -1 0 +1 +2 ---gt d subshell with 5 orbitals ---gt d subshell with 5 orbitals
For For l = 3 = 3 ml = -3 -2 -1 0 +1 +2 +3 = -3 -2 -1 0 +1 +2 +3 ---gt f subshell with 7 orbitals ---gt f subshell with 7 orbitals
Aufbau principleAs protons are added one by one to the nucleus to build up the elements electrons
are similarly added to these hydrogen-like orbitals
electron filling order (aufbau)
Hundrsquos Rule The lowest energy configuration for an atom is the one having the maximum number of unpaired electrons allowed by the Pauli principle in a particular set of degenerate (same energy) orbitals
Valence electrons electrons in the outermost principle quantum level of an atomThe inner electron are called core electrons
atom valence electronsCa 2N 5Br 7Arrangement of Electrons in Atoms
Shells (energy levels) = ndarr
Sublevels = ldarr
Orbitals = ml
Assigning electrons to atomsAssigning electrons to atomsElectrons generally assigned to orbitals of successively higher energyFor H atoms - Cn2 E depends only on nFor many-electron atoms energy depends on both n and l
Effective Nuclear Charge Zeff
Zeff is the nuclear charge experienced by the outermost electrons Explains why E(2s) lt E(2p)
Zeff increases across a period owing to incomplete shielding by inner electrons
Estimate Zeff by --gt [ Z - (no inner electrons) ]
Charge felt by 2s e- in Li Zeff = 3 - 2 = 1Be Zeff = 4 - 2 = 2B Zeff = 5 - 2 = 3and so on
Writing Atomic Electron Configurations
Orbital Notation Each electron is represented by a half-arrow
When electrons share an orbital opposite spins are represented by half-arrows going in opposite directions
Examples Write the orbital notation for the following atoms
N (7 e-) ____ ____ ____ ____ ____
1s 2s 2p
P ( ___ e-)
Electron Configuration Notation Write the energy level and orbital (in increasing energy) Write the number of electrons in the sublevel with a superscript
Examples Write the electron configuration notation for the following atoms
N
P
Tc
Electron Configuration Notation (Noble Gas Shorthand) Start with the noble gas ldquocloset without going overrdquo in brackets Continue normal electron configuration
Examples Write the electron configuration notation for the PREVIOUS atoms (use the noble gas shorthand)
Lewis Dot Diagrams
Valence electrons (e- in the outermost energy level) are the only electrons that are lost or gained in ordinary chemical reactions
Lewis Dot Diagrams only include electrons in valence (highest energy level) Write the letter and dots around the outside (2 on each side maximum of 8)
Examples Draw the Lewis Dot Diagram for
N Ca Cl
Ion configurations To form cations from elements remove 1 or more e- from subshell of highest n [or highest (n + l)]
P [Ne] 3s2 3p3 - 3e- ---gt P3+ [Ne] 3s2 3p0
For transition metals remove ns electrons and then (n - 1) electronsFe [Ar] 4s2 3d5
loses 2 electrons ---gt Fe2+ [Ar] 4s0 3d6
loses 3 electrons ---gt Fe3+
[Ar] 4s0 3d5
Information Contained on the Periodic Table1 Each group member has the same valence electron configuration
(these electrons primarily determine an atomrsquos chemistry)
2 The electron configuration of any representative element (see order)
3 Certain groups have special names (alkali metals halogens etc)02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
4 Metals and nonmetals are characterized by their chemical and physical properties
Periodic Trends overall change in physical property through row or group on the periodic
table These are general trends (there are exceptions)
Trend 1 Atomic Radius
Trend 2 Ionic Radius
Cations (positive ions) generally are smaller than their respective atoms
Anions (negative ions) generally are larger than their respective atoms
Trend 3 ndash Ionization Energy (IE)
Trend 4 ndash Electronegativity (en)
Redox Reactions Why do metals lose electrons in their reactions
Why does Mg form Mg2+ ions and not Mg3+Why do nonmetals take on electrons
Electron Affinity A few elements GAIN electrons to form anions
Electron affinity is the energy involved when an anion loses an electron A -(g) rarr A(g) + e- EA = ΔE
EA = 141 kJΔE is ENDOthermic because O has an affinity for an e-
O [He] - ion
[He] O atom
EA = 0 kJΔE is zero for N-
due to electron-electron repulsions
Trend 5 Electron AffinityAffinity for electron increases across a period (EA becomes more negative)
Reason
Affinity decreases down a group (EA becomes less negative)
Reason
[He] N- ion
[He] N atom
Atom EAF +328 kJCl+349 kJBr+325 kJI +295 kJ
1 2 3 4 5 6 7S1
S2
S3
S4
0
50
100
150
200
250
300
350
Elec
tron
affi
nity
(kJm
ol)
Group
Period
02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
Increasing Periodic Trends
electronegativity ionization energy ionic radii electron affinityatomic radii
ionic amp atomic radii
ionization energyelectron affinity amp electronegativity
p-orbital (dumbbell)
3 orbitals px py pz - The three p orbitals lie 90deg apart in space
When l = 1 there is a PLANAR NODE thru the nucleus When n = 2 then l = 0 and 1Therefore in n = 2 shell there are 2 types of orbitals mdash 2 subshells For l = 0 m
l = 0 this is a s subshell
For l = 1 ml = -1 0 +1 this is a p subshell with 3 orbitals
d-orbital (double dumbbell and dumbbelldonut)5 orbitalsWhen n = 3 what are the values of l
l = 0 1 2 and so there are 3 subshells in the shell
For l = 0 ml = 0 ---gt s subshell with single orbital
For l = 1 ml = -1 0 +1 ---gt p subshell with 3 orbitals
For l = 2 ml = -2 -1 0 +1 +2---gt d subshell with 5 orbitals
s orbitals have no planar node (l = 0) and so are spherical
p orbitals have l = 1 and have 1 planar node and so are ldquodumbbellrdquo shaped
This means d orbitals (with l = 2) have 2 planar nodes
f-orbital (quadruple dumbbell and dumbbelldouble donut)7 orbitalsWhen n = 4 When n = 4 l = 0 1 2 3 so there are 4 subshells in the shell = 0 1 2 3 so there are 4 subshells in the shell
For For l = 0 = 0 ml = 0 ---gt s subshell with single orbital = 0 ---gt s subshell with single orbital
For For l = 1 = 1 ml = -1 0 +1 ---gt p subshell with 3 orbitals = -1 0 +1 ---gt p subshell with 3 orbitals
For For l = 2 = 2 ml = -2 -1 0 +1 +2 = -2 -1 0 +1 +2 ---gt d subshell with 5 orbitals ---gt d subshell with 5 orbitals
For For l = 3 = 3 ml = -3 -2 -1 0 +1 +2 +3 = -3 -2 -1 0 +1 +2 +3 ---gt f subshell with 7 orbitals ---gt f subshell with 7 orbitals
Aufbau principleAs protons are added one by one to the nucleus to build up the elements electrons
are similarly added to these hydrogen-like orbitals
electron filling order (aufbau)
Hundrsquos Rule The lowest energy configuration for an atom is the one having the maximum number of unpaired electrons allowed by the Pauli principle in a particular set of degenerate (same energy) orbitals
Valence electrons electrons in the outermost principle quantum level of an atomThe inner electron are called core electrons
atom valence electronsCa 2N 5Br 7Arrangement of Electrons in Atoms
Shells (energy levels) = ndarr
Sublevels = ldarr
Orbitals = ml
Assigning electrons to atomsAssigning electrons to atomsElectrons generally assigned to orbitals of successively higher energyFor H atoms - Cn2 E depends only on nFor many-electron atoms energy depends on both n and l
Effective Nuclear Charge Zeff
Zeff is the nuclear charge experienced by the outermost electrons Explains why E(2s) lt E(2p)
Zeff increases across a period owing to incomplete shielding by inner electrons
Estimate Zeff by --gt [ Z - (no inner electrons) ]
Charge felt by 2s e- in Li Zeff = 3 - 2 = 1Be Zeff = 4 - 2 = 2B Zeff = 5 - 2 = 3and so on
Writing Atomic Electron Configurations
Orbital Notation Each electron is represented by a half-arrow
When electrons share an orbital opposite spins are represented by half-arrows going in opposite directions
Examples Write the orbital notation for the following atoms
N (7 e-) ____ ____ ____ ____ ____
1s 2s 2p
P ( ___ e-)
Electron Configuration Notation Write the energy level and orbital (in increasing energy) Write the number of electrons in the sublevel with a superscript
Examples Write the electron configuration notation for the following atoms
N
P
Tc
Electron Configuration Notation (Noble Gas Shorthand) Start with the noble gas ldquocloset without going overrdquo in brackets Continue normal electron configuration
Examples Write the electron configuration notation for the PREVIOUS atoms (use the noble gas shorthand)
Lewis Dot Diagrams
Valence electrons (e- in the outermost energy level) are the only electrons that are lost or gained in ordinary chemical reactions
Lewis Dot Diagrams only include electrons in valence (highest energy level) Write the letter and dots around the outside (2 on each side maximum of 8)
Examples Draw the Lewis Dot Diagram for
N Ca Cl
Ion configurations To form cations from elements remove 1 or more e- from subshell of highest n [or highest (n + l)]
P [Ne] 3s2 3p3 - 3e- ---gt P3+ [Ne] 3s2 3p0
For transition metals remove ns electrons and then (n - 1) electronsFe [Ar] 4s2 3d5
loses 2 electrons ---gt Fe2+ [Ar] 4s0 3d6
loses 3 electrons ---gt Fe3+
[Ar] 4s0 3d5
Information Contained on the Periodic Table1 Each group member has the same valence electron configuration
(these electrons primarily determine an atomrsquos chemistry)
2 The electron configuration of any representative element (see order)
3 Certain groups have special names (alkali metals halogens etc)02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
4 Metals and nonmetals are characterized by their chemical and physical properties
Periodic Trends overall change in physical property through row or group on the periodic
table These are general trends (there are exceptions)
Trend 1 Atomic Radius
Trend 2 Ionic Radius
Cations (positive ions) generally are smaller than their respective atoms
Anions (negative ions) generally are larger than their respective atoms
Trend 3 ndash Ionization Energy (IE)
Trend 4 ndash Electronegativity (en)
Redox Reactions Why do metals lose electrons in their reactions
Why does Mg form Mg2+ ions and not Mg3+Why do nonmetals take on electrons
Electron Affinity A few elements GAIN electrons to form anions
Electron affinity is the energy involved when an anion loses an electron A -(g) rarr A(g) + e- EA = ΔE
EA = 141 kJΔE is ENDOthermic because O has an affinity for an e-
O [He] - ion
[He] O atom
EA = 0 kJΔE is zero for N-
due to electron-electron repulsions
Trend 5 Electron AffinityAffinity for electron increases across a period (EA becomes more negative)
Reason
Affinity decreases down a group (EA becomes less negative)
Reason
[He] N- ion
[He] N atom
Atom EAF +328 kJCl+349 kJBr+325 kJI +295 kJ
1 2 3 4 5 6 7S1
S2
S3
S4
0
50
100
150
200
250
300
350
Elec
tron
affi
nity
(kJm
ol)
Group
Period
02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
Increasing Periodic Trends
electronegativity ionization energy ionic radii electron affinityatomic radii
ionic amp atomic radii
ionization energyelectron affinity amp electronegativity
s orbitals have no planar node (l = 0) and so are spherical
p orbitals have l = 1 and have 1 planar node and so are ldquodumbbellrdquo shaped
This means d orbitals (with l = 2) have 2 planar nodes
f-orbital (quadruple dumbbell and dumbbelldouble donut)7 orbitalsWhen n = 4 When n = 4 l = 0 1 2 3 so there are 4 subshells in the shell = 0 1 2 3 so there are 4 subshells in the shell
For For l = 0 = 0 ml = 0 ---gt s subshell with single orbital = 0 ---gt s subshell with single orbital
For For l = 1 = 1 ml = -1 0 +1 ---gt p subshell with 3 orbitals = -1 0 +1 ---gt p subshell with 3 orbitals
For For l = 2 = 2 ml = -2 -1 0 +1 +2 = -2 -1 0 +1 +2 ---gt d subshell with 5 orbitals ---gt d subshell with 5 orbitals
For For l = 3 = 3 ml = -3 -2 -1 0 +1 +2 +3 = -3 -2 -1 0 +1 +2 +3 ---gt f subshell with 7 orbitals ---gt f subshell with 7 orbitals
Aufbau principleAs protons are added one by one to the nucleus to build up the elements electrons
are similarly added to these hydrogen-like orbitals
electron filling order (aufbau)
Hundrsquos Rule The lowest energy configuration for an atom is the one having the maximum number of unpaired electrons allowed by the Pauli principle in a particular set of degenerate (same energy) orbitals
Valence electrons electrons in the outermost principle quantum level of an atomThe inner electron are called core electrons
atom valence electronsCa 2N 5Br 7Arrangement of Electrons in Atoms
Shells (energy levels) = ndarr
Sublevels = ldarr
Orbitals = ml
Assigning electrons to atomsAssigning electrons to atomsElectrons generally assigned to orbitals of successively higher energyFor H atoms - Cn2 E depends only on nFor many-electron atoms energy depends on both n and l
Effective Nuclear Charge Zeff
Zeff is the nuclear charge experienced by the outermost electrons Explains why E(2s) lt E(2p)
Zeff increases across a period owing to incomplete shielding by inner electrons
Estimate Zeff by --gt [ Z - (no inner electrons) ]
Charge felt by 2s e- in Li Zeff = 3 - 2 = 1Be Zeff = 4 - 2 = 2B Zeff = 5 - 2 = 3and so on
Writing Atomic Electron Configurations
Orbital Notation Each electron is represented by a half-arrow
When electrons share an orbital opposite spins are represented by half-arrows going in opposite directions
Examples Write the orbital notation for the following atoms
N (7 e-) ____ ____ ____ ____ ____
1s 2s 2p
P ( ___ e-)
Electron Configuration Notation Write the energy level and orbital (in increasing energy) Write the number of electrons in the sublevel with a superscript
Examples Write the electron configuration notation for the following atoms
N
P
Tc
Electron Configuration Notation (Noble Gas Shorthand) Start with the noble gas ldquocloset without going overrdquo in brackets Continue normal electron configuration
Examples Write the electron configuration notation for the PREVIOUS atoms (use the noble gas shorthand)
Lewis Dot Diagrams
Valence electrons (e- in the outermost energy level) are the only electrons that are lost or gained in ordinary chemical reactions
Lewis Dot Diagrams only include electrons in valence (highest energy level) Write the letter and dots around the outside (2 on each side maximum of 8)
Examples Draw the Lewis Dot Diagram for
N Ca Cl
Ion configurations To form cations from elements remove 1 or more e- from subshell of highest n [or highest (n + l)]
P [Ne] 3s2 3p3 - 3e- ---gt P3+ [Ne] 3s2 3p0
For transition metals remove ns electrons and then (n - 1) electronsFe [Ar] 4s2 3d5
loses 2 electrons ---gt Fe2+ [Ar] 4s0 3d6
loses 3 electrons ---gt Fe3+
[Ar] 4s0 3d5
Information Contained on the Periodic Table1 Each group member has the same valence electron configuration
(these electrons primarily determine an atomrsquos chemistry)
2 The electron configuration of any representative element (see order)
3 Certain groups have special names (alkali metals halogens etc)02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
4 Metals and nonmetals are characterized by their chemical and physical properties
Periodic Trends overall change in physical property through row or group on the periodic
table These are general trends (there are exceptions)
Trend 1 Atomic Radius
Trend 2 Ionic Radius
Cations (positive ions) generally are smaller than their respective atoms
Anions (negative ions) generally are larger than their respective atoms
Trend 3 ndash Ionization Energy (IE)
Trend 4 ndash Electronegativity (en)
Redox Reactions Why do metals lose electrons in their reactions
Why does Mg form Mg2+ ions and not Mg3+Why do nonmetals take on electrons
Electron Affinity A few elements GAIN electrons to form anions
Electron affinity is the energy involved when an anion loses an electron A -(g) rarr A(g) + e- EA = ΔE
EA = 141 kJΔE is ENDOthermic because O has an affinity for an e-
O [He] - ion
[He] O atom
EA = 0 kJΔE is zero for N-
due to electron-electron repulsions
Trend 5 Electron AffinityAffinity for electron increases across a period (EA becomes more negative)
Reason
Affinity decreases down a group (EA becomes less negative)
Reason
[He] N- ion
[He] N atom
Atom EAF +328 kJCl+349 kJBr+325 kJI +295 kJ
1 2 3 4 5 6 7S1
S2
S3
S4
0
50
100
150
200
250
300
350
Elec
tron
affi
nity
(kJm
ol)
Group
Period
02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
Increasing Periodic Trends
electronegativity ionization energy ionic radii electron affinityatomic radii
ionic amp atomic radii
ionization energyelectron affinity amp electronegativity
Aufbau principleAs protons are added one by one to the nucleus to build up the elements electrons
are similarly added to these hydrogen-like orbitals
electron filling order (aufbau)
Hundrsquos Rule The lowest energy configuration for an atom is the one having the maximum number of unpaired electrons allowed by the Pauli principle in a particular set of degenerate (same energy) orbitals
Valence electrons electrons in the outermost principle quantum level of an atomThe inner electron are called core electrons
atom valence electronsCa 2N 5Br 7Arrangement of Electrons in Atoms
Shells (energy levels) = ndarr
Sublevels = ldarr
Orbitals = ml
Assigning electrons to atomsAssigning electrons to atomsElectrons generally assigned to orbitals of successively higher energyFor H atoms - Cn2 E depends only on nFor many-electron atoms energy depends on both n and l
Effective Nuclear Charge Zeff
Zeff is the nuclear charge experienced by the outermost electrons Explains why E(2s) lt E(2p)
Zeff increases across a period owing to incomplete shielding by inner electrons
Estimate Zeff by --gt [ Z - (no inner electrons) ]
Charge felt by 2s e- in Li Zeff = 3 - 2 = 1Be Zeff = 4 - 2 = 2B Zeff = 5 - 2 = 3and so on
Writing Atomic Electron Configurations
Orbital Notation Each electron is represented by a half-arrow
When electrons share an orbital opposite spins are represented by half-arrows going in opposite directions
Examples Write the orbital notation for the following atoms
N (7 e-) ____ ____ ____ ____ ____
1s 2s 2p
P ( ___ e-)
Electron Configuration Notation Write the energy level and orbital (in increasing energy) Write the number of electrons in the sublevel with a superscript
Examples Write the electron configuration notation for the following atoms
N
P
Tc
Electron Configuration Notation (Noble Gas Shorthand) Start with the noble gas ldquocloset without going overrdquo in brackets Continue normal electron configuration
Examples Write the electron configuration notation for the PREVIOUS atoms (use the noble gas shorthand)
Lewis Dot Diagrams
Valence electrons (e- in the outermost energy level) are the only electrons that are lost or gained in ordinary chemical reactions
Lewis Dot Diagrams only include electrons in valence (highest energy level) Write the letter and dots around the outside (2 on each side maximum of 8)
Examples Draw the Lewis Dot Diagram for
N Ca Cl
Ion configurations To form cations from elements remove 1 or more e- from subshell of highest n [or highest (n + l)]
P [Ne] 3s2 3p3 - 3e- ---gt P3+ [Ne] 3s2 3p0
For transition metals remove ns electrons and then (n - 1) electronsFe [Ar] 4s2 3d5
loses 2 electrons ---gt Fe2+ [Ar] 4s0 3d6
loses 3 electrons ---gt Fe3+
[Ar] 4s0 3d5
Information Contained on the Periodic Table1 Each group member has the same valence electron configuration
(these electrons primarily determine an atomrsquos chemistry)
2 The electron configuration of any representative element (see order)
3 Certain groups have special names (alkali metals halogens etc)02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
4 Metals and nonmetals are characterized by their chemical and physical properties
Periodic Trends overall change in physical property through row or group on the periodic
table These are general trends (there are exceptions)
Trend 1 Atomic Radius
Trend 2 Ionic Radius
Cations (positive ions) generally are smaller than their respective atoms
Anions (negative ions) generally are larger than their respective atoms
Trend 3 ndash Ionization Energy (IE)
Trend 4 ndash Electronegativity (en)
Redox Reactions Why do metals lose electrons in their reactions
Why does Mg form Mg2+ ions and not Mg3+Why do nonmetals take on electrons
Electron Affinity A few elements GAIN electrons to form anions
Electron affinity is the energy involved when an anion loses an electron A -(g) rarr A(g) + e- EA = ΔE
EA = 141 kJΔE is ENDOthermic because O has an affinity for an e-
O [He] - ion
[He] O atom
EA = 0 kJΔE is zero for N-
due to electron-electron repulsions
Trend 5 Electron AffinityAffinity for electron increases across a period (EA becomes more negative)
Reason
Affinity decreases down a group (EA becomes less negative)
Reason
[He] N- ion
[He] N atom
Atom EAF +328 kJCl+349 kJBr+325 kJI +295 kJ
1 2 3 4 5 6 7S1
S2
S3
S4
0
50
100
150
200
250
300
350
Elec
tron
affi
nity
(kJm
ol)
Group
Period
02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
Increasing Periodic Trends
electronegativity ionization energy ionic radii electron affinityatomic radii
ionic amp atomic radii
ionization energyelectron affinity amp electronegativity
Hundrsquos Rule The lowest energy configuration for an atom is the one having the maximum number of unpaired electrons allowed by the Pauli principle in a particular set of degenerate (same energy) orbitals
Valence electrons electrons in the outermost principle quantum level of an atomThe inner electron are called core electrons
atom valence electronsCa 2N 5Br 7Arrangement of Electrons in Atoms
Shells (energy levels) = ndarr
Sublevels = ldarr
Orbitals = ml
Assigning electrons to atomsAssigning electrons to atomsElectrons generally assigned to orbitals of successively higher energyFor H atoms - Cn2 E depends only on nFor many-electron atoms energy depends on both n and l
Effective Nuclear Charge Zeff
Zeff is the nuclear charge experienced by the outermost electrons Explains why E(2s) lt E(2p)
Zeff increases across a period owing to incomplete shielding by inner electrons
Estimate Zeff by --gt [ Z - (no inner electrons) ]
Charge felt by 2s e- in Li Zeff = 3 - 2 = 1Be Zeff = 4 - 2 = 2B Zeff = 5 - 2 = 3and so on
Writing Atomic Electron Configurations
Orbital Notation Each electron is represented by a half-arrow
When electrons share an orbital opposite spins are represented by half-arrows going in opposite directions
Examples Write the orbital notation for the following atoms
N (7 e-) ____ ____ ____ ____ ____
1s 2s 2p
P ( ___ e-)
Electron Configuration Notation Write the energy level and orbital (in increasing energy) Write the number of electrons in the sublevel with a superscript
Examples Write the electron configuration notation for the following atoms
N
P
Tc
Electron Configuration Notation (Noble Gas Shorthand) Start with the noble gas ldquocloset without going overrdquo in brackets Continue normal electron configuration
Examples Write the electron configuration notation for the PREVIOUS atoms (use the noble gas shorthand)
Lewis Dot Diagrams
Valence electrons (e- in the outermost energy level) are the only electrons that are lost or gained in ordinary chemical reactions
Lewis Dot Diagrams only include electrons in valence (highest energy level) Write the letter and dots around the outside (2 on each side maximum of 8)
Examples Draw the Lewis Dot Diagram for
N Ca Cl
Ion configurations To form cations from elements remove 1 or more e- from subshell of highest n [or highest (n + l)]
P [Ne] 3s2 3p3 - 3e- ---gt P3+ [Ne] 3s2 3p0
For transition metals remove ns electrons and then (n - 1) electronsFe [Ar] 4s2 3d5
loses 2 electrons ---gt Fe2+ [Ar] 4s0 3d6
loses 3 electrons ---gt Fe3+
[Ar] 4s0 3d5
Information Contained on the Periodic Table1 Each group member has the same valence electron configuration
(these electrons primarily determine an atomrsquos chemistry)
2 The electron configuration of any representative element (see order)
3 Certain groups have special names (alkali metals halogens etc)02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
4 Metals and nonmetals are characterized by their chemical and physical properties
Periodic Trends overall change in physical property through row or group on the periodic
table These are general trends (there are exceptions)
Trend 1 Atomic Radius
Trend 2 Ionic Radius
Cations (positive ions) generally are smaller than their respective atoms
Anions (negative ions) generally are larger than their respective atoms
Trend 3 ndash Ionization Energy (IE)
Trend 4 ndash Electronegativity (en)
Redox Reactions Why do metals lose electrons in their reactions
Why does Mg form Mg2+ ions and not Mg3+Why do nonmetals take on electrons
Electron Affinity A few elements GAIN electrons to form anions
Electron affinity is the energy involved when an anion loses an electron A -(g) rarr A(g) + e- EA = ΔE
EA = 141 kJΔE is ENDOthermic because O has an affinity for an e-
O [He] - ion
[He] O atom
EA = 0 kJΔE is zero for N-
due to electron-electron repulsions
Trend 5 Electron AffinityAffinity for electron increases across a period (EA becomes more negative)
Reason
Affinity decreases down a group (EA becomes less negative)
Reason
[He] N- ion
[He] N atom
Atom EAF +328 kJCl+349 kJBr+325 kJI +295 kJ
1 2 3 4 5 6 7S1
S2
S3
S4
0
50
100
150
200
250
300
350
Elec
tron
affi
nity
(kJm
ol)
Group
Period
02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
Increasing Periodic Trends
electronegativity ionization energy ionic radii electron affinityatomic radii
ionic amp atomic radii
ionization energyelectron affinity amp electronegativity
Orbitals = ml
Assigning electrons to atomsAssigning electrons to atomsElectrons generally assigned to orbitals of successively higher energyFor H atoms - Cn2 E depends only on nFor many-electron atoms energy depends on both n and l
Effective Nuclear Charge Zeff
Zeff is the nuclear charge experienced by the outermost electrons Explains why E(2s) lt E(2p)
Zeff increases across a period owing to incomplete shielding by inner electrons
Estimate Zeff by --gt [ Z - (no inner electrons) ]
Charge felt by 2s e- in Li Zeff = 3 - 2 = 1Be Zeff = 4 - 2 = 2B Zeff = 5 - 2 = 3and so on
Writing Atomic Electron Configurations
Orbital Notation Each electron is represented by a half-arrow
When electrons share an orbital opposite spins are represented by half-arrows going in opposite directions
Examples Write the orbital notation for the following atoms
N (7 e-) ____ ____ ____ ____ ____
1s 2s 2p
P ( ___ e-)
Electron Configuration Notation Write the energy level and orbital (in increasing energy) Write the number of electrons in the sublevel with a superscript
Examples Write the electron configuration notation for the following atoms
N
P
Tc
Electron Configuration Notation (Noble Gas Shorthand) Start with the noble gas ldquocloset without going overrdquo in brackets Continue normal electron configuration
Examples Write the electron configuration notation for the PREVIOUS atoms (use the noble gas shorthand)
Lewis Dot Diagrams
Valence electrons (e- in the outermost energy level) are the only electrons that are lost or gained in ordinary chemical reactions
Lewis Dot Diagrams only include electrons in valence (highest energy level) Write the letter and dots around the outside (2 on each side maximum of 8)
Examples Draw the Lewis Dot Diagram for
N Ca Cl
Ion configurations To form cations from elements remove 1 or more e- from subshell of highest n [or highest (n + l)]
P [Ne] 3s2 3p3 - 3e- ---gt P3+ [Ne] 3s2 3p0
For transition metals remove ns electrons and then (n - 1) electronsFe [Ar] 4s2 3d5
loses 2 electrons ---gt Fe2+ [Ar] 4s0 3d6
loses 3 electrons ---gt Fe3+
[Ar] 4s0 3d5
Information Contained on the Periodic Table1 Each group member has the same valence electron configuration
(these electrons primarily determine an atomrsquos chemistry)
2 The electron configuration of any representative element (see order)
3 Certain groups have special names (alkali metals halogens etc)02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
4 Metals and nonmetals are characterized by their chemical and physical properties
Periodic Trends overall change in physical property through row or group on the periodic
table These are general trends (there are exceptions)
Trend 1 Atomic Radius
Trend 2 Ionic Radius
Cations (positive ions) generally are smaller than their respective atoms
Anions (negative ions) generally are larger than their respective atoms
Trend 3 ndash Ionization Energy (IE)
Trend 4 ndash Electronegativity (en)
Redox Reactions Why do metals lose electrons in their reactions
Why does Mg form Mg2+ ions and not Mg3+Why do nonmetals take on electrons
Electron Affinity A few elements GAIN electrons to form anions
Electron affinity is the energy involved when an anion loses an electron A -(g) rarr A(g) + e- EA = ΔE
EA = 141 kJΔE is ENDOthermic because O has an affinity for an e-
O [He] - ion
[He] O atom
EA = 0 kJΔE is zero for N-
due to electron-electron repulsions
Trend 5 Electron AffinityAffinity for electron increases across a period (EA becomes more negative)
Reason
Affinity decreases down a group (EA becomes less negative)
Reason
[He] N- ion
[He] N atom
Atom EAF +328 kJCl+349 kJBr+325 kJI +295 kJ
1 2 3 4 5 6 7S1
S2
S3
S4
0
50
100
150
200
250
300
350
Elec
tron
affi
nity
(kJm
ol)
Group
Period
02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
Increasing Periodic Trends
electronegativity ionization energy ionic radii electron affinityatomic radii
ionic amp atomic radii
ionization energyelectron affinity amp electronegativity
Tc
Electron Configuration Notation (Noble Gas Shorthand) Start with the noble gas ldquocloset without going overrdquo in brackets Continue normal electron configuration
Examples Write the electron configuration notation for the PREVIOUS atoms (use the noble gas shorthand)
Lewis Dot Diagrams
Valence electrons (e- in the outermost energy level) are the only electrons that are lost or gained in ordinary chemical reactions
Lewis Dot Diagrams only include electrons in valence (highest energy level) Write the letter and dots around the outside (2 on each side maximum of 8)
Examples Draw the Lewis Dot Diagram for
N Ca Cl
Ion configurations To form cations from elements remove 1 or more e- from subshell of highest n [or highest (n + l)]
P [Ne] 3s2 3p3 - 3e- ---gt P3+ [Ne] 3s2 3p0
For transition metals remove ns electrons and then (n - 1) electronsFe [Ar] 4s2 3d5
loses 2 electrons ---gt Fe2+ [Ar] 4s0 3d6
loses 3 electrons ---gt Fe3+
[Ar] 4s0 3d5
Information Contained on the Periodic Table1 Each group member has the same valence electron configuration
(these electrons primarily determine an atomrsquos chemistry)
2 The electron configuration of any representative element (see order)
3 Certain groups have special names (alkali metals halogens etc)02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
4 Metals and nonmetals are characterized by their chemical and physical properties
Periodic Trends overall change in physical property through row or group on the periodic
table These are general trends (there are exceptions)
Trend 1 Atomic Radius
Trend 2 Ionic Radius
Cations (positive ions) generally are smaller than their respective atoms
Anions (negative ions) generally are larger than their respective atoms
Trend 3 ndash Ionization Energy (IE)
Trend 4 ndash Electronegativity (en)
Redox Reactions Why do metals lose electrons in their reactions
Why does Mg form Mg2+ ions and not Mg3+Why do nonmetals take on electrons
Electron Affinity A few elements GAIN electrons to form anions
Electron affinity is the energy involved when an anion loses an electron A -(g) rarr A(g) + e- EA = ΔE
EA = 141 kJΔE is ENDOthermic because O has an affinity for an e-
O [He] - ion
[He] O atom
EA = 0 kJΔE is zero for N-
due to electron-electron repulsions
Trend 5 Electron AffinityAffinity for electron increases across a period (EA becomes more negative)
Reason
Affinity decreases down a group (EA becomes less negative)
Reason
[He] N- ion
[He] N atom
Atom EAF +328 kJCl+349 kJBr+325 kJI +295 kJ
1 2 3 4 5 6 7S1
S2
S3
S4
0
50
100
150
200
250
300
350
Elec
tron
affi
nity
(kJm
ol)
Group
Period
02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
Increasing Periodic Trends
electronegativity ionization energy ionic radii electron affinityatomic radii
ionic amp atomic radii
ionization energyelectron affinity amp electronegativity
loses 3 electrons ---gt Fe3+
[Ar] 4s0 3d5
Information Contained on the Periodic Table1 Each group member has the same valence electron configuration
(these electrons primarily determine an atomrsquos chemistry)
2 The electron configuration of any representative element (see order)
3 Certain groups have special names (alkali metals halogens etc)02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
4 Metals and nonmetals are characterized by their chemical and physical properties
Periodic Trends overall change in physical property through row or group on the periodic
table These are general trends (there are exceptions)
Trend 1 Atomic Radius
Trend 2 Ionic Radius
Cations (positive ions) generally are smaller than their respective atoms
Anions (negative ions) generally are larger than their respective atoms
Trend 3 ndash Ionization Energy (IE)
Trend 4 ndash Electronegativity (en)
Redox Reactions Why do metals lose electrons in their reactions
Why does Mg form Mg2+ ions and not Mg3+Why do nonmetals take on electrons
Electron Affinity A few elements GAIN electrons to form anions
Electron affinity is the energy involved when an anion loses an electron A -(g) rarr A(g) + e- EA = ΔE
EA = 141 kJΔE is ENDOthermic because O has an affinity for an e-
O [He] - ion
[He] O atom
EA = 0 kJΔE is zero for N-
due to electron-electron repulsions
Trend 5 Electron AffinityAffinity for electron increases across a period (EA becomes more negative)
Reason
Affinity decreases down a group (EA becomes less negative)
Reason
[He] N- ion
[He] N atom
Atom EAF +328 kJCl+349 kJBr+325 kJI +295 kJ
1 2 3 4 5 6 7S1
S2
S3
S4
0
50
100
150
200
250
300
350
Elec
tron
affi
nity
(kJm
ol)
Group
Period
02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
Increasing Periodic Trends
electronegativity ionization energy ionic radii electron affinityatomic radii
ionic amp atomic radii
ionization energyelectron affinity amp electronegativity
Trend 4 ndash Electronegativity (en)
Redox Reactions Why do metals lose electrons in their reactions
Why does Mg form Mg2+ ions and not Mg3+Why do nonmetals take on electrons
Electron Affinity A few elements GAIN electrons to form anions
Electron affinity is the energy involved when an anion loses an electron A -(g) rarr A(g) + e- EA = ΔE
EA = 141 kJΔE is ENDOthermic because O has an affinity for an e-
O [He] - ion
[He] O atom
EA = 0 kJΔE is zero for N-
due to electron-electron repulsions
Trend 5 Electron AffinityAffinity for electron increases across a period (EA becomes more negative)
Reason
Affinity decreases down a group (EA becomes less negative)
Reason
[He] N- ion
[He] N atom
Atom EAF +328 kJCl+349 kJBr+325 kJI +295 kJ
1 2 3 4 5 6 7S1
S2
S3
S4
0
50
100
150
200
250
300
350
Elec
tron
affi
nity
(kJm
ol)
Group
Period
02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
Increasing Periodic Trends
electronegativity ionization energy ionic radii electron affinityatomic radii
ionic amp atomic radii
ionization energyelectron affinity amp electronegativity
EA = 0 kJΔE is zero for N-
due to electron-electron repulsions
Trend 5 Electron AffinityAffinity for electron increases across a period (EA becomes more negative)
Reason
Affinity decreases down a group (EA becomes less negative)
Reason
[He] N- ion
[He] N atom
Atom EAF +328 kJCl+349 kJBr+325 kJI +295 kJ
1 2 3 4 5 6 7S1
S2
S3
S4
0
50
100
150
200
250
300
350
Elec
tron
affi
nity
(kJm
ol)
Group
Period
02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
Increasing Periodic Trends
electronegativity ionization energy ionic radii electron affinityatomic radii
ionic amp atomic radii
ionization energyelectron affinity amp electronegativity
Atom EAF +328 kJCl+349 kJBr+325 kJI +295 kJ
1 2 3 4 5 6 7S1
S2
S3
S4
0
50
100
150
200
250
300
350
Elec
tron
affi
nity
(kJm
ol)
Group
Period
02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
Increasing Periodic Trends
electronegativity ionization energy ionic radii electron affinityatomic radii
ionic amp atomic radii
ionization energyelectron affinity amp electronegativity
02_29
1H
3Li
11Na
19K
37Rb
55Cs
87Fr
4Be
12Mg
20Ca
38Sr
56Ba
88Ra
21Sc
39Y
57La
89Acdagger
22Ti
40Zr
72Hf
104Unq
23V
41Nb
73Ta
105Unp
24Cr
42Mo
74W
106Unh
25Mn
43Tc
75Re
107Uns
26Fe
44Ru
76Os
108Uno
27Co
45Rh
77Ir
109Une
110Uun
111Uuu
28Ni
46Pd
78Pt
29Cu
47Ag
79Au
30Zn
3 4 5 6 7 8 9 10 11 12
48Cd
80Hg
31Ga
49In
81Tl
5B
13Al
32Ge
50Sn
82Pb
6C
14Si
33As
51Sb
83Bi
7N
15P
34Se
52Te
84Po
8O
16S
9F
17Cl
35Br
53I
85At
10Ne
18Ar
36Kr
54Xe
86Rn
2He
58Ce
90Th
59Pr
91Pa
60Nd
92U
61Pm
93Np
62Sm
94Pu
63Eu
95Am
64Gd
96Cm
65Tb
97Bk
66Dy
98Cf
67Ho
99Es
68Er
100Fm
69Tm
101Md
70Yb
102No
71Lu
103Lr
1A
2A
Transition metals
3A 4A 5A 6A 7A
8A1
2 13 14 15 16 17
18
Alk
ali m
etal
s
Alkalineearth metals Halogens
Noblegases
Lanthanides
dagger Actinides
Increasing Periodic Trends
electronegativity ionization energy ionic radii electron affinityatomic radii
ionic amp atomic radii
ionization energyelectron affinity amp electronegativity