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Standard temperature and pressure
0 °C (273 K) and 1 atm
the molar volume at STP for an ideal gas is 1 mol gas = 22.4 L
Boyle’s Law
P1V1=P2V2
how the volume of a gas changes if the pressure is doubled
Charles’ Law
V1/T1 = V2/T2
predict what happens to the volume of a balloon if it's heated or
cooled
Gay-Lussac’s Law
P1/T1 = P2/T2
what happens to the pressure of a sealed container if it is
heated
Avogadro’s Law
V1/n1 = V2/n2
how volume changes as the amount (moles) of a gas changes
Combined gas law
When more than 1 variable is changed, how does that affect
the final values, which variable has a greater effect
Ideal gas law
PV= nRT
An ideal gas is a hypothetical substance that follows these rules perfectly
Molecules have negligible volume compared to the container's volume
There are no attractive or repulsive forces between the molecules
Collisions are perfectly elastic, meaning no energy is lost
Relationship between Density and Temperature: a gas sample is heated in a
flexible container (at constant pressure) Volume increases and density
decreases
d ∝ 1/𝑇
Relationship between Density and Pressure in a sealed container that cannot
expand an increase of pressure on a gas increases the density
d ∝ P
Relationship between Density and Molar Mass: At the same temperature and
pressure, the gas that has a higher molar mass would have the higher density
d ∝ 𝑀
Explain the principle behind effusion/diffusion and how it relates to gas density
and molar mass
Effusion and diffusion occur due to the random motion of gas particles
Rate ∝ 1 / √(molar mass) → lighter gases spread or escape faster
Higher molar mass or density = slower movement, lower molar mass or density = faster movement.
Partial pressures
the total pressure of a mixture of gases is the sum of their individual partial pressures
Grahams’ Law
the rate of diffusion or effusion of a gas is inversely proportional to the square root of its molar mass
What is the relationship between frequency and wavelength?
inverse
What is the relationship between frequency and energy?
direct
How can frequency be converted to wavelength
divide the speed of light by the frequency
How can frequency be converted to energy
multiply frequency by Planck’s constant (6.63 × 10 ^-34)
Bohr model of the Hydrogen atom and Energy of electron transitions
triangle E = - 2.28 x 10-18 (1/nf^2 – 1/ni^2)
Electrons orbit a nucleus in specific, allowed paths called
energy levels or orbits
Energy levels are quantized according to the equation
E = - 2.28 x 10-18 (1/n2)
Electrons can jump between these levels by absorbing or emitting
specific amounts of energy as photons
The emission spectra of elements like hydrogen result from
transitions from higher energy orbits to lower energy ones
A negative value indicates the photon being emitted while the positive value
indicates
the photon being absorbed
The further apart the orbits are
the larger the energy
Quantum numbers
a set of four numerical values that describe the unique location and properties of an electron in an atom
they specify the electron’s energy level, shape of its orbital, orientation in space, and spin direction
Atomic orbitals
regions around the nucleus of an atom where there is a high probability of finding an electron
characterized by the first three quantum numbers (𝑛, 𝑙 and
𝑚𝑙)
Principal Quantum Number (n)
This number indicates the electron's main energy level,
or shell, and can be any positive integer (1,2,3, . ..)
As 𝑛 increases, the electron's average
distance from the nucleus and its energy increases
Angular Momentum Quantum Number (𝑙)
This number describes the shape of an atomic orbital and specifies the subshell
𝑙=0 corresponds to an s orbital (spherical)
𝑙=1 corresponds to a p orbital (dumbbell-shaped)
𝑙=2 corresponds to a d orbital (cloverleaf-shaped)
Magnetic Quantum Number (𝑚𝑙)
This number describes the orientation of the orbital in
space
Its possible values range from −𝑙 to +𝑙, including zero
For a given subshell, there are 2𝑙 + 1 possible orientations corresponding to the odd integers (1, 3, 5, 7)
Spin Quantum Number (𝑚𝑠)
This number describes the intrinsic angular momentum, or
"spin," of an electron
There are only two possible values for 𝑚𝑠: + ½ or – ½ (“up” or
“down” arrows)
Electron configuration
shows the arrangement of electrons in an atom’s orbitals
tells you which orbitals are occupied and how many electrons are in each
How to write an electron configuration
Find the atomic number of the element.
This equals the number of electrons in a neutral atom.
Use the Aufbau order (1s → 2s → 2p → 3s → 3p → 4s → 3d → 4p → 5s → 4d → 5p → 6s → 4f → 5d → 6p → 7s → 5f → 6d → 7p) to assign electrons to orbitals.
Write the configuration by listing the orbitals in order with their electron counts as superscripts.
Example: 1s² 2s² 2p⁶ 3s²
Check your total number of electrons — it should equal the atomic number
Aufbau Principle
Electrons fill the lowest energy orbitals first before moving to
higher energy ones
(1s → 2s → 2p → 3s → 3p → 4s → 3d → 4p → 5s → 4d → 5p → 6s → 4f → 5d → 6p → 7s → 5f → 6d → 7p)
Pauli Exclusion Principle
No two electrons in an atom can have the same set of
four quantum numbers
This means each orbital can hold a maximum of two
electrons, and they must have opposite spins
Hund’s Rule
Within a subshell, electrons will occupy each orbital individually
before any orbital gets a second electron
For example, in a p subshell, one electron will go into each of the three p orbitals before a second electron is added to any of them
Valence electrons
the outermost electrons of an atom
they are responsible for an element's chemical properties and reactivity
they are the electrons that are gained, lost, or shared during chemical reactions and used to create chemical bonds
How to determine how many valence electrons an atom or ion has
Atom
Find the element on the periodic table.
Look at its group number (column number).
Use the group number to find valence electrons:
Group | Elements | Valence Electrons |
|---|---|---|
1 (IA) | H, Li, Na, K... | 1 |
2 (IIA) | Be, Mg, Ca... | 2 |
13 (IIIA) | B, Al, Ga... | 3 |
14 (IVA) | C, Si, Ge... | 4 |
15 (VA) | N, P, As... | 5 |
16 (VIA) | O, S, Se... | 6 |
17 (VIIA) | F, Cl, Br... | 7 |
18 (VIIIA) | He, Ne, Ar... | 8 (except He has 2) |
Confirm by writing the electron configuration and identifying electrons in the outermost shell (highest n value).
Example:
Oxygen: 1s² 2s² 2p⁴ → highest n = 2 → 2 + 4 = 6 valence electrons
Sodium: 1s² 2s² 2p⁶ 3s¹ → highest n = 3 → 1 valence electron
Ion
Start with the neutral atom’s valence electrons.
Add or remove electrons depending on the ion’s charge:
For cations (positive ions): subtract electrons.
Example: Na → 1 valence e⁻ → Na⁺ → 0 valence electrons (empty outer shell; next lower shell is full).
For anions (negative ions): add electrons.
Example: Cl → 7 valence e⁻ → Cl⁻ → 8 valence electrons (stable octet).
How to determine how many valence electrons there are in an atom
from electron configuration or position on the periodic table
Periodic Table
Find the element’s group number (the column it’s in).
Use the group number to determine valence electrons for main group elements (Groups 1–2 and 13–18).
Group | Example Elements | Valence Electrons |
|---|---|---|
1 (IA) | H, Li, Na, K | 1 |
2 (IIA) | Be, Mg, Ca | 2 |
13 (IIIA) | B, Al, Ga | 3 |
14 (IVA) | C, Si, Ge | 4 |
15 (VA) | N, P, As | 5 |
16 (VIA) | O, S, Se | 6 |
17 (VIIA) | F, Cl, Br | 7 |
18 (VIIIA) | He, Ne, Ar | 8 (He has 2) |
Electron configuration
Write or look up the atom’s electron configuration.
Identify the highest principal energy level (n) — this is the outermost shell.
Count all the electrons in orbitals with that same n value — those are the valence electrons
Atoms form ions to achieve
a stable electron configuration
Metals typically have few valence electrons and lose them to become stable. This
results in a positive charge because
the atom now has more protons (positive) than
electrons (negative)
the resulting positive ion is called a cation
Nonmetals have larger numbers of valence electrons (e.g., 6 or 7) and tend
to gain electrons. Gaining negatively charged electrons results in a negative ion which is called an
anion
Trends in metallic character
Metals are defined as elements that readily lose their electrons to make cations
Metallic character decreases from left to right across a period and increases
from top to bottom down a group on the periodic table. This is because as you move across a period, the number of protons increases, pulling electrons closer and making them harder to lose
As you move down a group, the atomic radius increases, placing outer electrons further from the nucleus, and shielding by inner electrons makes them easier to lose
Trends in radius size across a period or down a group
Across a period (left to right) atomic radius decreases
As you move across a period, the number of protons in the nucleus increases, creating a stronger positive charge
Down a group (top to bottom) atomic radius increases
Cations
positive ions
smaller than their parent atoms because they have lost
their valence shell
Anions
negative ions
larger than their parent atoms due to increased electron-electron repulsion
Ionization energy
refers to the amount of energy needed to remove an electron from an atom
across a period (left to right) ionization energy increases
down a group (top to bottom) ionization energy decreases
Electron affinity
the energy emitted when an atom takes in an electron
across a period (left to right) electron affinity becomes more negative
down a group (top to bottom) electron affinity becomes less negative
Electronegativity
the ability of an atom to attract shared electrons in a chemical bond
atoms with high electronegativity (like nonmetals) pull electrons more strongly
across a period (left to right) electronegativity increases
down a group (top to bottom) electronegativity decreases
Where are the most electronegative elements found
the top right of the periodic table
Where are the least electronegative elements found
the bottom left of the periodic table
How to determine bond polarity
subtract the electronegativities of the 2 atoms in a bond to
determine if the bond is polar ( If the electronegativity difference < 0.4 is nonpolar, > 0.4
is polar – if it has a metal, it is ionic)
Covalent bonds
the sharing of electron pairs between atoms
it is created when a valence orbital from an element containing 1 electron overlaps with the valence orbital of another element also containing 1 electron
Lewis structures
diagrams that show how valence electrons are arranged in a molecule
bonds between atoms shown as lines and non-bonding electrons shown as dots
a single line is a single bond (2 electrons), a double line is a double bond (4
electrons), and a triple line is a triple bond (6 electrons)
Formal charge
the hypothetical charge an atom would have if bonding electrons were split equally between atoms and the molecule's total charge was distributed equally
the number of valence electrons for a particular atom minus the number of
assigned electrons determines the formal charge on the atom
Resonance
a way to describe the positions of electrons in certain molecules or
ions where a single Lewis structure is not enough to represent the true
bonding
this lowers the energy of the molecule, making it more stable than one particular structure
to identify molecules with resonance look for a multiple bond next to an atom
that is capable of taking part of that multiple bond, usually on that has a lone
pair of electrons
VSEPR theory
a model used to predict the 3D shape of a molecule
To use VSEPR, draw a Lewis structure, count the total number of electron group: bonds (single bonds, double bonds, triple bonds are all 1 bond) and lone pairs around the central atom, and determine the geometry that positions these groups at maximum distance from each other