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Chemistry Unit 2

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Title: Chemistry Unit 2


1
ChemistryUnit 2
  • Chapters 4-6
  • Atomic Properties and Bonding

2
First Things First
  • Lab reports
  • Give back homework
  • Tests

3
The Modern Atom
  • Bohr Model
  • Atoms made of 3 particles

4
Light
  • Originally thought to be a wave
  • Discovered to also behave like a particle
  • A packet of energy called a quantum is wavelike
  • A photon contains a quantum and behaves like a
    particle

5
Wave-Particle Duality
  • Developed by Einstein
  • Light behaves both as a wave and a particle
  • Quanta act like waves and are a unit of energy
  • Photons act as particles and are made of quanta
  • Photons have 0 mass and are pure energy

6
Electromagnetic Radiation
  • Energy that acts as a wave
  • Energy linked to wavelength and frequency of the
    light

7
Electromagnetic Radiation
  • All waves move at 3.00 x 108 m/s in a vacuum
  • Wavelength (?) is the distance between
    corresponding points on a wave
  • Frequency (?) is the number of waves per second
    that pass by a point

8
Energy of Waves
  • High frequency and low wavelength are high energy
  • Low frequency and high wavelength are low energy

9
Electromagnetic Spectrum
10
Electromagnetic Spectrum
11
Visible Light
  • Only certain range detectible to human eyes
  • 400-700 nm or 5 x 1014 1 x 1015 Hz
  • Violet is the highest energy, red the lowest

12
Ultraviolet and Infrared
  • Ultraviolet (UV) means more than violet, higher
    energy and frequency, shorter wavelength
  • This is why UV rays are damaging
  • Infrared (IR) is less than red, lower energy and
    frequency, longer wavelength
  • This is why IR remotes dont do damage

13
Electromagnetic Spectrum
  • Be able to rank from high to low by wavelength,
    frequency, or energy
  • Pg 98

14
Relations of Wavelength and Frequency
  • The speed of light (m/s) is equal to the
    wavelength (m) times the frequency (1/s)
  • c ??
  • Which is where a physics joke comes from.

15
The Photoelectric Effect
  • Explains part of the particle nature of light
  • When light shines on some metals they emit
    electrons

16
The Energy of Light
  • Quantum also happens to be energy gained or lost
    by electrons as they move closer or further from
    the nucleus, emitted as photons
  • Energy (J) equals Plancks Constant (Js) times
    the frequency (1/s)
  • E h?

17
Plancks Constant
  • Developed by Max Planck
  • Relates the energy to the frequency
  • 6.626 x 10-34 Js

18
Line-Emission Spectra
  • Energy added to gas atoms and electrons emit
    light waves
  • Electrons promoted from the ground state to an
    excited state
  • Ground state is the lowest energy level
  • Excited state is any higher energy state

19
Line-Emission Spectra
  • Each element has a unique set of lines

20
Line-Emission Spectra
  • Lyman Series
  • UV
  • Balmer Series
  • Visible, most commonly used
  • Paschen Series
  • IR

21
Quantum Theory
  • When electrons lose energy they emit it as
    photons
  • Studies the behavior of atoms and their energies
    in relation to photons and quanta of energy

22
Niels Bohr
  • Proposed set orbitals for electrons
  • These were based on the line-emission spectrum of
    different elements
  • Photons emitted have specific energies based on
    how much energy is lost in falling to a lower
    energy level

23
Energy Levels
  • Electrons can gain or lose energy and move up or
    down in energy states
  • Each element has its own set of allowed energy
    levels
  • Biggest difference in energy levels Lyman
  • Moderate difference in energy levels Balmer
  • Small difference in energy levels Paschen

24
Energy Levels
25
Energy Levels
26
Wave-Particle Duality (Again)
  • 1924 Louis de Broglie realized electrons also
    acted like a wave as well as a particle
  • Waves confined to a set space have only certain
    frequencies, much like electrons do
  • de Broglie pointed out that electrons acted like
    waves confined to the space around an atom

27
de Broglie Waves
  • All matter can behave as a wave
  • Wavelength of a particle determined by the mass
    and speed of the particle
  • ? h/mv

28
Detecting de Broglie Waves
  • Electrons detected by photons, but act similarly
    to photons (wave-particle duality)
  • Any attempt to find where an electron is changes
    where it is
  • A solution proposed by Werner Heisenberg

29
Heisenberg Uncertainty Principle
  • It is impossible to determine both the position
    and velocity of a particle.
  • Also stated Observing a system disturbs it in
    such a way that any data collected cannot be
    certain.

30
Schrödingers Equation
  • Erwin Schrödinger developed an equation to
    mathematically show electrons act as wave
  • Solutions prove that only certain energies are
    allowed
  • Gives probability regions, called orbitals, where
    electrons can be
  • Probability regions are where electrons are 95
    likely to be

31
Solutions to Schrödingers Equation
  • Gives 4 quantum numbers
  • Principal quantum number n
  • Angular momentum quantum number l
  • Magnetic quantum number m
  • Spin quantum number

32
Principal Quantum Number
  • n gt 0
  • Gives the energy level of the electron
  • As n increases so does energy and distance from
    the nucleus
  • Electrons allowed per level is 2n2 up to 32

33
Principle Quantum Number
34
Angular Momentum Quantum Number
  • 0 l n-1 3
  • Gives the sublevel
  • All sublevels but n1 have multiple orbitals

35
Angular Momentum Quantum Number
36
s Sublevel Orbitals
  • Spherical
  • Holds 2 electrons

37
p Sublevel Orbitals
  • 3 orbitals
  • Named by which axis they lay along
  • Holds 6 electrons total

38
d Sublevel Orbitals
  • 5 orbitals
  • Named for orientation
  • Holds 10 electrons total

39
f Sublevel Orbitals
  • 7 orbitals
  • Dont worry about what they look like or are
    named
  • Holds 14 electrons total

40
f Sublevel Orbitals
41
Orbitals
  • s is lowest energy, then p, d, and f

42
Magnetic Quantum Number
  • -l m l
  • Gives orientation of the orbitals
  • Gives number of allowed orbitals
  • 2l 1

43
Spin Quantum Number
  • Only 2 possible values, relating to the two
    magnetic poles
  • 1/2 or -1/2
  • Each orbital can have 2 electrons and they must
    have opposite spins

44
Game
  • Pick a partner and sit together
  • You can use your book and planner, just not other
    teams papers
  • If you dont have a calculator get one from the
    bench
  • The team with the highest ratio of right/time
    gets an ECP

45
Game
  • Go over answers

46
Electron Configurations
47
Electron Configurations
  • Shows how electrons are arranged
  • Gives energy level, sublevel, and how many
    electrons

48
3 Rules to Placing Electrons
  • Aufbau Principle
  • Pauli Exclusion Principle
  • Hunds Rule

49
Aufbau Principle
  • Naturally, electrons are found in the lowest
    energy levels possible

50
Aufbau Principle
51
Pauli Exclusion Principle
  • Each electron has to have a unique set of quantum
    numbers
  • AKA Electrons must be paired by opposite spins.

52
Pauli Exclusion Principle
  • 1/2 and -1/2 spin are paired
  • Each orbital holds 2 electrons

53
Pauli Exclusion Principle
54
Hunds Rule
  • Electrons being placed in sublevel orbitals of
    equal energy will be placed unpaired first.
  • All unpaired electrons must have the same spin.

55
Hunds Rule
56
Practice
  • Following Hunds Rule, how many unpaired
    electrons are allowed in each sublevel?

57
Orbital Notation
  • Shows electrons as up or down arrows,
    representing 1/2 and -1/2 spin states
  • Orbitals as lines (sometimes boxes) labeled with
    energy level and sublevel

58
Practice
  • Using the diagram, and what you know about
    orbitals, and show atoms with 3, 7, and 18
    electrons

59
Electron Configuration Notation
  • Uses energy level diagram and orbital notation to
    write out the electron configuration in the form
    nlx
  • n is principle quantum number (energy level), l
    is the sublevel (letter) derived from the angular
    momentum number, and x is the number of electrons
    in that sublevel

60
Refresher
  • How many electrons are allowed in each sublevel?
  • s
  • p
  • d
  • f

61
Example
  • H is 1s1
  • He is 1s2
  • C is 1s2 2s2 2p2
  • Kr is 1s2 2s2 2p6 3s2 3p6 4s2 3d10 4p6

62
Why does the d Block Start at 3?
  • 3d is higher energy than 4s, but less than 4p
  • s and p are always the same as the period, d is
    one less, f is 2 less

63
Writing Electron Configuration Notation
  • Work up from atomic 1
  • Electrons shown in notation always equals the
    atomic number of the element for neutral atoms
  • Use the periodic table as your guide

64
Writing Electron Configuration Notation
  • Start at 1 and move across a period

65
Noble Gas Notation
  • Written as previous noble gas in brackets and
    then the electron configuration not included in
    the noble gas
  • C is He 2s2 2p2

66
Practice
  • Write the following in noble gas notation
  • Germanium
  • Strontium
  • Tin

67
The Periodic Table
68
The Periodic Table
  • Periodic means repeating in a pattern
  • The Periodic Table of the Elements arranges
    elements by increasing mass and of protons

69
The Periodic Table
  • 2 groupings
  • Groups Vertical columns, elements in groups
    have similar properties
  • Periods Horizontal rows, show similar electron
    configurations and energy levels

70
Famous Dead Guys
  • Dmitri Mendeleev
  • Russian 1834-1907
  • Arranged the 63 known elements by mass on a
    periodic table and in groups by properties

71
Mendeleev
  • Based on properties of the groups he could
    predict the masses and properties of undiscovered
    elements
  • Arranged in order of mass, and noticed a pattern.

72
The Periodic Table
73
Group 1
  • Alkali Metals
  • 1 electron in the s sublevel
  • Malleable, ductile, good conductors, very soft
    metals, very reactive, explosive in water, cesium
    and francium are some of the most reactive
    elements, never found free in nature

74
Group 2
  • Alkaline Earth Metals
  • 2 electrons in the s sublevel
  • Malleable, ductile, good conductors, very
    reactive, but less than alkali metals, never
    found free in nature

75
Groups 3-12
  • Transition Metals
  • Central block of metals
  • 2 electrons in the s sublevel and 1-10 in the d
    sublevel
  • Malleable, ductile, good conductors, some can
    produce magnetic fields, have unusual electron
    shells

76
Group 13-15 Metals
  • Very dense solids
  • Bottom left corner of the p block
  • Only 7
  • Aluminum, Gallium, Indium, Tin, Thallium, Lead,
    and Bismuth

77
Group 13-16 Metalloids
  • Found on the line between metals and nonmetals
  • What is a metalloid?
  • Only 7
  • Boron, Silicon, Germanium, Arsenic, Antimony,
    Tellurium, Polonium

78
Group 14-16 Nonmetals
  • Upper right of 14-16
  • Nonmetals
  • Only 6
  • Carbon, Nitrogen, Oxygen, Phosphorus, Sulfur, and
    Selenium

79
Group 17
  • Halogens
  • Only group to have solids, liquids, and gases
  • Have 2 electrons in the s sublevel, some have d
    sublevel, all have 5 electrons in the p sublevel
  • Nonmetals, insulators, form salts

80
Group 18
  • Noble Gases
  • Inert (dont react)
  • The most stable elements
  • Full outer electron shell (valence shell)

81
Lanthanides and Actinides
  • 2 periods at the bottom of the chart
  • Also called Rare Earth Metals
  • Have the f sublevel
  • Most are synthetic
  • Most are radioactive
  • Very heavy and unstable

82
The Modern Periodic Table
  • There were a few places where Mendeleevs table
    didnt quite work
  • This was fixed by Henry Moseley in 1911

83
Famous Dead Guy
  • Henry Moseley
  • English 1911
  • Working in Rutherfords lab
  • Developed the Periodic Law
  • Studied spectra of elements
  • Found that the elements should be arranged by
    protons, not mass

84
Periodic Law
  • The physical and chemical properties of the
    elements are functions of their protons and
    electrons, not mass.

85
Periodicity and Electron Configurations
86
Periodicity and Electron Configurations
  • According to the Periodic Law the properties and
    periodicity are a function of the protons and
    electrons of an atom

87
Atom Radii
  • Defined by ½ the distance between the nuclei of
    identical atoms bonded together
  • Radii get smaller across a period and larger down
    a group
  • Smallest radii are at the upper right, largest at
    the lower left

88
Atomic Radii
89
Practice
  • Which in each group has the larger radius
  • Ba or Mn
  • In or Sn
  • O or S

90
Ionization Energy
  • The energy required to remove an electron from an
    atom
  • The stronger the electron is held to the atom the
    higher the ionization energy
  • Only deals with loss of an electron
  • Increases across the period and decrease down the
    group

91
Electronegativity
  • Developed by Linus Pauling
  • Measures the ability for an atom in a compound to
    attract electrons from another atom in the
    compound
  • AKA Measures how badly they want another electron

92
Electronegativity
  • High electronegativities mean they will more
    readily take an electron, lower means less likely
  • Electronegativities near or below 2 means they
    will readily give up electrons

93
Electronegativity
  • Tend to increase across a period and decrease
    down a group
  • Upper right of the p block will very easily take
    electrons
  • Lower left of s block easily lose electrons

94
Valence Electrons
  • Electrons in the outer electron shell
  • Highest energy level electrons
  • Interact in chemical reactions and compounds
  • Up to 8 in main block elements
  • The s and p blocks
  • Called an octet
  • Group patterns emerge

95
Practice
  • How many valence electrons?
  • H
  • Ca
  • Al
  • Te
  • Kr
  • Mo

96
d and f Block Properties
97
d and f Block Properties
  • All transition metals have similar properties
  • Almost like theyre all part of the same group
  • Can lose or gain several different numbers of
    electrons

98
d and f Block Properties
  • Similar properties because they all have the same
    number of valence electrons
  • Remember d block energy level is 1 less than
    period

99
d and f Block Properties
  • The d block
  • Radii decrease across a period, but less than
    main block
  • The f block
  • Radii fluctuate across a period
  • Caused by filling orbital 2 energy levels less
    than valence

100
d and f Block Properties
  • Ionization energies increase across period
  • Ionization energies increase down the groups,
    unlike main block elements

101
d and f Block Properties
  • Electronegativities are weak, prefer to give up
    electrons
  • Follow same trends as main block elements

102
Ions
103
Ions
  • Charged atoms
  • Caused by adding or removing electrons
  • Cation positive ion
  • Lost electron(s)
  • Anion negative ion
  • Gained electron(s)

104
Ions
  • Atoms gain or lose electrons to be more like
    noble gases
  • Will usually only lose valence electrons
  • Charge equal to number of electrons gained or lost

105
Practice
  • Will these form cations or anions?
  • Li
  • Ba
  • Sb
  • F
  • W

106
Practice
  • What is the charge on these ions when they are
    like noble gases?
  • Mg
  • O
  • P
  • Fr

107
Ionic Radii
  • Cations smaller than their neutral version
  • More protons than electrons, held tighter
  • Anions larger than their neutral version
  • More electrons than protons, held less tightly
  • Increase down a group

108
Ionic Radii
109
Practice
  • What is the smallest ion?
  • Are these ions smaller or larger than their atom?
  • Li
  • O2-
  • I-
  • Pd2

110
Chapter 5 Review Worksheet
111
Bonding
112
Bonding
  • The periodic table is like a parts list or a
    buffet
  • Atoms mix together to make compounds
  • Chemical bonds are the attraction of atoms and
    interactions of valence electrons

113
Why bonding?
  • Atoms are most stable when they have full octets
  • Either share or take electrons

114
Ionic Bonding
  • One atom steals the electrons of another
  • Attraction between anions and cations
  • Large difference in electronegativies
  • ?EN gt 1.7
  • Usually s block and nonmetal

115
Ionic Bonding
  • Na has EN of 0.9
  • Cl has EN of 3.0
  • ?EN of 2.1
  • ?EN ENanion Encation
  • Use table on page 161

116
Covalent Bonding
  • Sharing electrons
  • Small difference in EN
  • ?EN lt 1.2

117
Covalent Bonding
  • Cl2
  • ?EN 0
  • HCl
  • H has EN of 2.1
  • Cl has EN of 3.0
  • ?EN of 0.9

118
Polar Covalent Bonding
  • Unequal sharing
  • Moderate difference between atoms
  • 1.2 lt ?EN lt 1.7

119
Polar Covalent Bonding
  • LiI
  • Li has EN of 1.0
  • I has EN of 2.5
  • ?EN of 1.5

120
Metallic Bonding
  • Lots of cations (metals that have lost electrons)
    all have electrons flying around between them
  • Occurs only between 2 or more metals
  • These arrangements make metals malleable,
    ductile, and good conductors
  • Malleable ability to be hammered into sheets
  • Ductile ability to be drawn into wires

121
Bonding Visuals
122
Bonding Visuals
123
Bonding Visuals
124
Practice
  • What type of bonds are these?
  • NaAt
  • FrBr
  • MgCl2
  • AgBr2
  • HgO
  • ZnCu

125
Displaying Bonds
126
The Octet Rule
  • Atoms are most stable when they have a full octet
  • Outer electron shell (energy level) is filled

127
Practice
  • Draw the orbital notation of these atoms and show
    that they are more stable with overlapping
    orbitals
  • HCl
  • H2O
  • NaCl
  • MgF2

128
Exceptions to the Octet Rule
  • Hydrogen and helium only need 2 valence electrons
  • Boron likes 6
  • Expanded valence atoms can have more than 8
    valence electrons when bonded with very
    electronegative elements

129
Electron Dot Diagrams
  • Shows valence electrons as dots surrounding the
    elements symbol
  • Use 2 dots per side, for up to 8 total

130
Practice
  • H
  • Sr
  • Bi
  • O
  • Ar
  • B

131
Lewis Structures
  • Show molecules as electron dot structures with
    shared electrons shown between them
  • Unshared electrons are called lone pairs
  • 2 shared electrons can be shown with a dash
  • 1 dash (2 electrons) is a single bond
  • 2 dashes (4 electrons) is a double bond
  • 3 dashes (6 electrons) is a triple bond

132
Drawing Lewis Structures
  • Find how many electrons each atom wants to gain
    or lose
  • Draw each atom separately
  • Combine them and show shared electrons as dashes

133
Example
134
Practice
  • Draw the following as Lewis Structures
  • O2
  • CH4
  • C2H5OH
  • N2

135
Resonance Structures
  • Compounds with multiple Lewis Structures
  • Reality is a combination of structures
  • Resonance adds to stability

136
Example
  • Ozone
  • O3

137
Practice
  • C4H6
  • C5H8
  • C6H6

138
Structural Formula
  • Doesnt show dots for lone pairs, only dashes for
    bonds
  • Carbons with all 8 electrons shared dont have to
    be shown, just as points

139
Practice
  • HCl
  • H2O
  • CO2
  • C6H6

140
Ionic Bonding
141
Ionic Bonding
  • Ionic bonds are bonds where the difference in
    electronegativities is great enough that one atom
    steals the electron from another

142
Crystals
  • Many ionic compounds for crystals
  • A 3D structure of cations and anions held together

143
Formula Units
  • Shows the simplest ratio of cations and anions
  • Since they form crystals the real structure is
    usually a multiple of this
  • NaCl is a 11 ratio, but is found in large
    crystals

144
Why Crystals
  • The regular arrangement of the ions in a crystal
    have the lowest energy
  • This makes them more stable
  • The structure of the crystal (where the ions fit
    in) is called a crystal lattice

145
Lattice Energy
  • The energy released when ions as a gas form an
    ordered crystal
  • Negative energy is a release of energy, this is
    favorable
  • The more negative the value the more stable the
    crystal

146
Forming Ionic Bonds
  • Ionic compounds are shown as ions in Lewis
    Structures
  • Final structures must be stable

147
Example
148
Ionic Properties
149
Ionic Properties
  • Atoms held together by attraction of positive and
    negative charges
  • Molecules barely held together

150
Ionic Properties
  • Hardness of the compound, melting point, and
    boiling point all depend on how well the formula
    units are held together
  • Stronger attractions harder, higher bp and mp

151
Ionic Properties
  • Most are solids at room temperature
  • Strong attraction between formula units
  • In solutions (liquids, usually water) they
    dissociate
  • Dissociate means falls apart
  • Cations and anions found seperately

152
Visual
153
Polyatomic Ions
154
Polyatomic Ions
  • Cations or anions made of multiple atoms
  • A group of covalently bonded atoms with a net
    charge

155
Polyatomic Ions
156
3D Chemistry
157
VSEPR Theory
  • Valence Shell Electron-Pair Repulsion Theory
  • The repulsion of the electrons to each other
    makes the bonds between atoms desirable to be as
    far apart as possible.

158
VSEPR Theory
  • Lone pairs need to be accounted for as well
  • Geometry can be determined based on the number of
    atoms and lone pairs bonded to the central atom
    (stearic ) and the number of lone pairs

159
(No Transcript)
160
Example
  • Draw the Lewis Structure for water (H2O)
  • According to VSEPR Theory how do we get the
    electrons farthest apart?
  • Hint Think 3-Dimensionally
  • 4 bonds, 2 lone pairs
  • Bent Structure

161
Practice
  • NH3
  • CO2
  • NaAt
  • PCl3
  • HCP
  • CH4

162
Bond Hybridization
163
Hybridization
  • Geometry determined by hybridization of the bond
  • A hybrid bond is a combination of orbitals to
    create a new orbital

164
Example
  • Draw methanes (CH4) orbital notation
  • 2s and 2p merge to form a 2sp3
  • An sp3 sublevel has 4 orbitals, as many as there
    were before, just at a single energy

165
Hybridization
166
Intermolecular Forces
167
Intermolecular Forces
  • Forces between compounds, not within
  • Forces within a compound are intramolecular

168
Dipole-Dipole
  • Strongest force between polar molecules
  • Uneven distribution of charges
  • Polar covalent bonding

169
Hydrogen Bonding
  • A specific type of dipole-dipole force
  • Only occurs in H-O, H-F, and H-N bonds
  • Hydrogens are attracted to the lone pairs of
    another molecule

170
London Dispersion Force
  • Attraction due to momentary dipole created by the
    natural movements of electrons
  • Very weak, occurs in all atoms and compounds

171
End of Unit 1
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