Chapter 3 Flashcards

1
Q

________
13.8 Billion years ago – singularity
________ – rapid expansion of Universe

A

Big Bang

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

Following the Big Bang
- 1 ________ after – no atoms, only leptons (electrons) and quarks
- 1 ________ after – protons and neutrons
- Few ________ after – H+ D+ He2+ Li3+ (density of air)
- For _______ years temp dropped as the Universe expanded – no further fusion occurred
- Then, electrons combined with nuclei to give atoms
- After _______ years, matter began to clump together and stars were formed (we’ll get to that)

A

Picosecond, microsecond, minutes, 380K, a billion

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
3
Q

Everything in the Universe is …

A

Moving away from us with increasing speed

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

If an object emitting light is moving away from us, which direction will the wavelength of light be shifted?
1. To longer wavelengths
2. To shorter wavelengths
3. Toward the red end of the spectrum
4. Toward the blue end of the spectrum
5. It will not be shifted
A. 1 and 3
B. 1 and 4
C. 2 and 3
D. 2 and 4
E. 5 only

A

A.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

Spectra of elements are more ______ shifted the farther away they are.

A

Red

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
6
Q

We can extrapolate backwards in time and, at some point in the past, we see all the matter and energy in the universe concentrated at one point (________).

A

singularity

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
7
Q

_____________
- Universe is expanding (red shift)
- Computer Models
- CMBR (cosmic microwave background radiation)
- 1.9 mm (microwave) radiation – relic of early Universe when electrons and protons were “recombining” into hydrogen atoms

A

Evidence of the Big Bang

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

_____________
- Involve rearrangements (sharing, donating or accepting) of valence electrons.
- The identity of the element undergoing a chemical reaction does not change (EVER).

A

Chemical Reactions

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

_____________
- Involve nucleus (not electrons).
- Often result in change in element (since element is defined by the number of protons).

A

Nuclear Reactions

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

A
Fe
B
A:
B:

A

A: Mass number
B: Atomic number

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
11
Q

Which element has an atomic number of 19?
A. F
B. K
C. Na
D. Br

A

B.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
12
Q

How many protons and neutrons does 12^(N) have?
A. 6p, 6n
B. 7p, 5n
C. 5p, 7n
D. 7p, 7n

A

B.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

Isotopes have the same # of _______ and a different # of _______.

A

Protons, neutrons

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
14
Q

Which is an isotope of 12^(C)?
A. 13^C
B. 12^(N)
C. 12^(Mg)

A

A.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
15
Q

(Types of Nuclear Reactions)
- ________ (adding two nuclei together)
- ________ (breaking a nucleus apart)
- ________ (emitting particles, α, β, γ etc)

A

Fusion, fission, radioactive decay

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
16
Q

At very high temperatures ________ can occur.

A

Nuclear fusion

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
17
Q

At very high temperatures, electrons on atoms are stripped away (they have so much energy that they can overcome the attraction to the nucleus) resulting in a …

A

Plasma

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
18
Q

As two nuclei move toward each other (but are still separated by distances greater than the size of the nucleus) what force affects them?
A. Electrostatic
B. Gravity
C. Strong nuclear
D. Weak nuclear

A

A.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
19
Q

As two nuclei move toward each other (but are still separated by distances greater than the size of the nucleus) what happens to the potential energy of the system?
A. Increases
B. Decreases
C. Stays the same

A

A.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
20
Q

If there is enough kinetic energy in the system (eg by heating it), the nuclei can get really close together. At that point the _________ comes into play.

A

Strong nuclear force

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
21
Q

To for atoms to get really close, a great deal of energy is required to overcome the _________ between the nuclei.

A

Electrostatic repulsion

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
22
Q

As two nuclei move very close together (at distances less than the size of the nucleus), the strong nuclear force comes into effect. What happens to the potential energy of the system?
A. Increases
B. Decreases
C. Stays the same

A

B.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
23
Q

Nuclear reactions are accompanied by changes in …

A

Mass

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
24
Q

The mass of the individual nucleons is greater than the mass of the …

A

Nucleus

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
25
What happened to the mass of the nucleons that was lost when they combined to form a nucleus? What is it quantified as?
It was converted to binding energy, E=mc^2
26
E = mc^2 E = (mass in kg) × (3.00 × 10^8 m/s)^2 E = kg·m^2·s^-2 1 J = 1 kg·m^2·s^-2
Mass loss converted to binding energy
27
The energy released from nuclear reactions is ________ than from chemical reactions.
Much greater
28
Each deuterium atom is formed from 1 proton, 1 neutron, and 1 electron. How much energy is released by the formation of 1 deuterium (D) atom? Useful Info: E = mc^2 Mass defect: 0.00238 amu 1 amu = 1.6606 × 10^–27 kg c = 3.00 × 10^8 m/s 1 J = 1 kg·m^2·s^-2
3.56 x 10^-13 (kg x m^2 x s^2)
29
Each deuterium atom is formed from 1 proton, 1 neutron, and 1 electron (3.56 x 10^-13 J). How much energy is released by the formation of 1 mole of deuterium (D) atoms?
2.14 x 10^8 kJ/mol
30
It takes a lot of _______ to start a fusion reaction.
Energy
31
Slide 49 and 50
32
___________ is the fragmentation of heavy nuclei to form lighter, more stable ones + energy.
Nuclear Fission
33
Nuclear fission chain reactions can be used for ____________ (or __________).
Nuclear energy generation, nuclear bombs
34
__________ is the mass of the isotope required for the chain reaction to become self-sustaining.
Critical mass
35
___________ Nucleus emits or captures particles or energy in the form of electromagnetic radiation.
Radioactivity
36
____________ - Alpha particle emission - Beta particle emission - Electron emission - Positron emission - Electron capture - γ electromagnetic radiation
Common types of radioactivity
37
Do isolated atoms or molecules exist in a state (solid, liquid or gas)? A. Yes B. No
B
38
Do isolated atoms or molecules have melting points or boiling points? A. Yes B. No
B
39
States of matter, boiling points, and melting points are …
Emergent properties
40
When atoms interact to form larger collections, they have …
Emergent properties
41
__________ belong to a collection, but not the individual components.
Emergent properties
42
If a solid reacts with a gas, what state of matter will the product be? A. Solid B. Liquid C. Gas D. Part solid, part gas E. We cannot tell from the information given
E
43
The properties of any substance depend on the ________________ that exist within that substance.
Arrangement of atoms
44
The _________ of a substance depend on the bonding/interactions within that substance.
Properties
45
________ and ________ have similar causes (electrostatic attraction of the electrons of one atom to the nucleus of another).
LDF, covalent bonds
46
_____________ The magnitude of the attraction and how the electrons are arranged in the new species (which is formed by the interaction).
The difference between LDF and covalent bonds
47
Why do bonds form between atoms? A. Because atoms want to share electrons. B. Because atoms need to have a full octet. C. Because valence electrons are attracted to the nuclei of other atoms. D. Because the potential energy is at a minimum.
C
48
__________ electrons from one atom become attracted to the other nucleus.
Valence
49
_________ is most stable distance between the atoms - ie lowest potential energy.
Bond length
50
When bonds form energy is …
Released into the surroundings
51
Bonding Theories: Just like we have different atomic theories – we also have models of bonding. 1. 2.
Molecular Orbital Theory, Valence Bond Theory
52
Recall that electrons are ______ and can therefore combine constructively and destructively.
Waves
53
In _____ Theory, n atomic orbitals combine to give n molecular orbitals.
MO
54
Molecular Orbital (MO) Theory When atomic orbitals combine constructively, _____________ form.
Bonding molecular orbitals
55
Bonding MOs are ________ energy than the atomic orbitals.
Lower
56
Molecular Orbital (MO) Theory Electrons in bonding orbitals make the species ...
More stable
57
Molecular Orbital (MO) Theory When atomic orbitals combine destructively, _____________ form.
Antibonding molecular orbitals
58
Antibonding orbitals are ________ energy than the atomic orbitals.
Higher
59
Electrons in antibonding orbitals make the species _________.
Less stable
60
Atomic orbitals can also combine destructively to form a molecular orbital of ...
Higher energy
61
Atomic orbitals can combine constructively (recall electrons can be considered as waves) to form a molecular orbital of ______ energy.
Lower
62
Both bonding and antibonding orbitals are in the same place in space – just at different ...
Energies
63
A bond will form if…
There are two electrons in a bonding molecular orbital
64
If there are also two electrons in an antibonding orbital, this cancels out the stabilization from two electrons in bonding orbital and, therefore ...
No bond forms
65
To break the bond, enough energy has to be added to ...
Raise an electron to the anti-bonding orbital
66
If we combine 2 atoms with 9 atomic orbitals each, how many molecular orbitals will result? A. 2 B. 4 C. 9 D. 18
D
67
When two O atoms interact, how many molecular orbitals are generated by the atomic orbitals in the core and valence shells? (Hint: Write the electron configuration for O.) A. 2 B. 4 C. 6 D. 10
A
68
How many bonds form between two O atoms? A. 0 B. 1 C. 2 D. 3 E. 4
C
69
As the number of MOs increases, the energy gap between them ...
Decreases
70
Bonding in Metals As the number of MOs increases, they form bands of MOs of ...
Almost continuous energy
71
Bonding in Metals Electrons can ________ between MOs.
Move freely
72
Bonding in Metals Electrons can ________ over whole system.
Move freely
73
Properties of Metals _______________ will promote an electron to a higher energy level.
Absorption of a photon
74
Properties of Metals The metal interacts with _________, so the metal appears white or colorless (silvery).
Light of many wavelengths
75
Why are metals shiny? A. Because electrons are ejected from the metal when light shines on it. B. Because photons of light are reflected off the metal. C. Because photons of many wavelengths are absorbed and then re-emitted. D. Because visible light is diffracted by the metal.
C.
76
Because atoms can move with respect to one another, metals are ...
Malleable and ductile
77
Because electrons can move around freely, metals ...
Conduct electricity
78
Band Theory In materials that are insulators (eg diamond), there is a ___________ between the valence and conduction band.
Large energy gap
79
Band Theory In semi-conductors (eg Si, Ge) there is a _________ between the bands, these materials are often used for solar cells and in computer equipment.
Small gap
80
Band Theory In metals, the valence band (bonding MO’s) _________ with the conduction band (antibonding MO’s).
Overlaps
81
Melting to Boiling Do these processes absorb or release energy? A. Absorb B. Release
A
82
Melting to Boiling Where does the energy come from? A. The system B. The surroundings
B
83
Melting to Boiling Where are the attractions that are being overcome? A. Within particles B. Between particles
B
84
Freezing and Condensing Do these processes absorb or release energy? A. Absorb B. Release
B
85
Freezing and Condensing Where does the energy go? A. The system B. The surroundings
B
86
Freezing and Condensing Where are the attractions that are being formed? A. Within particles B. Between particles
B
87
When a substance ______, some of the interactions between the particles must be overcome so that they can move relative to each other.
Melts
88
When a substance _______, all the interactions between the particles must be overcome.
Boils
89
The magnitude of the melting point and boiling point provides an estimate of the strength of the __________ between particles.
Attractive interactions
90
What kinds of interactions must be overcome between particles in order to melt: H2, He, Li, C ? A. LDF B. Covalent C. Metallic D. LDF and Covalent
A, A, C, B
91
_____________ - Strong (require a lot of energy to break - Caused by attraction of electrons from one atom to nucleus of another atom - Hard to predict bond strength - Present only when atomic orbitals interact constructively - Present within molecules and networks
Covalent bond
92
______________ - Relatively weak - Caused by fluctuating charge distribution - Increase (predictably) with size of electron cloud - Present between all molecular species
London Dispersion Force
93
Each carbon atom forms 4 bonds to 4 identical carbon atoms. The bonds arrange them- selves towards the corners of a 4-sided figure. We call this geometry _________.
Tetrahedral
94
_______________ - Atomic orbitals combine to form an equal number of molecular orbitals. - Each orbital can contain up to two electrons. - Electrons in bonding orbitals stabilize the system. - Electrons in anti-bonding orbital make it less stable. - Electrons are delocalized.
Molecular Orbital
95
_______________ - Atomic orbitals overlap to form a bond. - The greater the overlap, the stronger the bond. - Each bond made up of two electrons. - Electrons are localized in the bond.
Valence Bond
96
What is the electron configuration of carbon? A. [He] 2s^2 2p^2 B. [Ne] 2s^2 2p^2 C. 1s2 1p^2 D. [He] 2s^2 4p^2
A
97
How many atomic orbitals (on one carbon) must combine to make 4 hybrid orbitals? A. 1 B. 2 C. 3 D. 4
D
98
Atomic orbitals “________” (mix up) to form bonding orbitals that then combine with orbitals from other atom to form a bond.
Hybridize
99
When the hybrid orbitals combine there is a _______ between the bonding and antibonding molecular orbitals.
Large gap
100
Hybridized atomic orbitals (sp3) overlap to give ...
Strong directed bonds
101
These bonds are called “sigma bonds”. Sigma bonds form when atomic orbitals overlap ...
End-to-end
102
Diamond Properties _____________ 3D network of strong bonds, you would have to break bonds to melt.
High mp/bp and/or hard
103
Diamond Properties _____________ Electrons are localized in bonds between atoms – not free to roam. There is a large “band gap” between the bonding and antibonding orbitals.
Does not conduct electricity
104
Diamond Properties _____________ Light passes through or is reflected. To absorb light an electron must be promoted to a higher energy level. There is a large “band gap” between the bonding and antibonding orbitals.
Translucent
105
__________ overlap of atomic orbitals gives π bond.
Side-to-side
106
107
The _________ p-orbitals overlap to form pi-bonds. Since the overlap occurs across the entire sheet of atoms, “__________” pi molecular orbitals form over the sheet.
Unhybridized, delocalized
108
Graphite Properties __________ – because electrons can move freely over the entire sheet within its delocalized pi MOs.
Conducts electricity
109
Graphite Properties __________ – because it can absorb and emit photons of many wavelengths (just like metals).
Shiny
110
Graphite Properties _________ – sheets can slide over each other – only “held together” by ...
Slippery, LDFs