CHEMISTRY/ORGANIC CHEMISTRY FINAL REVIEW Flashcards
Atomic number
Z - number of protons found in an atom of that element
Mass number
A - sum of the protons and neutrons in the atom’s nucleus
-varies in isotopes
Planck relation
E = hf
Energy is related to frequency times Planck’s constant
Principal quantum number, maximum number of electrons per number
n - indicates the electron’s shell
Maximum number of electrons within a shell = 2n^2
Azimuthal quantum number, range of possible values
l - shape and number of subshells
range of possible values: 0 to n-1
- only one subshell in first principal energy level (0)
- two in second principal energy level
- three in third principal quantum level
indicated as a letter (s,p,d,f)
Maximum number of electrons within a subshell = 4l + 2 (s2,p6,d10,f14)
Magnetic quantum number, range of possible values
ml - specifies the electrons orbital
range of possible values: -l to l
orbitals in s are spheral, p are dumbbell
Spin quantum number
ms - designated +½ or -½
Electron configuration determination and description
2p4 indicates that there are four electrons in the second (p) subshell of the second principal energy level
Read the periodic table to determine electron configuration
-lowest s is 1s, lowest p is 2p, lowest d is 3d, lowest f is 4f
Hund’s rule and implications, special elements
finding a seat on a crowded bus, electrons find their own orbital
half-filled and fully filled orbitals have more stability
chromium and copper groups are therefore exceptions to electron configuration, moving an electron from s to d
chromium = 4s13d5
copper = 4s13d10
paramagnetic vs diamagnetic
paramagnetic materials have unpaired electrons and are weakly attracted to the magnetic field
diamagnetic materials have only paired electrons and will be slightly repelled to the magnetic field
A elements and B elements
A elements are representative elements and include groups 1A through 8A (everything but transition elements and bottom of periodic table)
B elements are nonrepresentative elements and include the transition elements and lanthanide and actinide series
Effective nuclear charge trend and equation
indicates the electrostatic attraction between the valence shell electrons and the nucleus
increases from right to left, as one moves down a group principal quantum number increases and Zeff is more or less constant
Zeff = Z(atomic number) - S(non-valence electrons)
Atomic and ionic radii definition and trend
atomic radius decreases from left to right and from bottom to top
ionic radii of metals near the metalloid line is dramatically smaller than that of other metals
Ionization energy definition and trend
energy required to remove an electron from a gaseous species
-removing an electron is an endothermic process
increases from left to right and from bottom to top
groups 1 and 2 are called active metals for their low ionization energy
Electron affinity definition and trend
the energy dissipated by a gaseous species when it gains an electron, opposite of ionization energy
increases from left to right and from bottom to top
noble gases have extremely small electron affinities however
Electronegativity definition and trend
the attractive force generated in a chemical bond
increases from left to right and from bottom to top
Alkali metals
largest atomic radii, react readily with nonmetals to lose an electron
Alkaline earth metals
two electrons in valence shell
Chalcogens
Oxygen group not as reactive as halogens but crucial in biology
Halogens
desperate to complete their octets
Noble gases
inert
Transition metals
low electron affinities, ionization energies, and electronegativities have different possible oxidation states
Exceptions to the octet rule and examples
Incomplete octet hydrogen, helium, and lithium (2), beryllium (4), boron (6)
Expanded octet
-Any element in period 3 and greater can hold more than 8 electrons, including phosphorus (10), sulfur (12), chlorine (14), and others
Odd numbers of electrons Ex: NO has eleven valence electrons
Coordinate covalent bond
If both of the shared electrons are contributed by only one of the two atoms, that is a coordinate covalent bond
once it is formed it is indistinguishable from any other covalent bond
Ionic bonds in solid state
In solid state, the ionic constituents of the compound form a crystalline lattice of repeating positive and negative ions
Formal charge calculation
Valence shell - dots - dashes
Lewis structures steps
Draw out backbone with the least electronegative atom in the center
Count all the valence electrons
Complete the octets of all atoms bonded to the central atom, using the remaining valence electrons left to be assigned
Place any extra electrons on the central atom
VSEPR Theory Arrange the electron pairs around the central atom so that they are as far apart as possible
Electronic geometry
Spatial arrangement of all pairs of electrons
Molecular geometry
spatial arrangement of only the bonding pairs of electrons
determined by coordinate number -number of atoms that surround and are bonded to a central atom
Hydrogen bonds
Even hydrogen bonds have only about 10 percent the strength of a covalent bond
Nitrogen, Oxygen, or fluorine bonded to hydrogen
Moles calculation
Moles = mass of sample/ molar mass
Gram equivalent weight
the amount of a compound, measured in grams, that produces one equivalent of the particle of interest
Gram equivalent weight = molar mass/n where n is the number of particles of interest produced or consumed
Ex: gram equivalent weight of H2Co3 is half of its molar mass with interest towards h+ ions
Useful for acid-base chemistry
Normality
equivalents/L (where molarity is moles per liter)
most commonly used for hydrogen ions concentration
Ex: A 1N solution of acid would be like HCL, and 2N would be like H2So4
Molarity
Normality/n or moles per liter
Empirical formula
gives the simplest whole-number ratio
Combustion reaction
involves a fuel (usually hydrocarbon) and a oxidant (normally oxygen), forming carbon dioxide and water
Neutralization reactions
a specific type of double-displacement reaction: acid + base = water + salt
Cations and Ions naming (metals, less charge, more charge, monatomic, less oxygen, more oxygen)
For metals the charge is indicated by a Roman numeral in parentheses
- ous: less charge, -ic: greater charge
- ide: monatomic anions
Hypo- indicates less oxygen, per- indicates more oxygen
Formula and Charge:
Acetate, Cyanide Permanagante, Chromate, Dichromate, Borate, Ammonium, Thiocyanate
When is a solute considered a strong electrolyte?
A solute is considered a strong electrolyte if it dissociates completely into its constituent ions
Arrhenius equation takeaways
k = Ae^(-Ea/RT) k is the rate constant, A is the frequency factor, Ea is the activation energy of the reaction, R is the ideal gas constant, and T is the temperature in kelvins
Transition state energy
Transition state/activation complex has greater energy than both the reactants and the products and is denoted by the symbol ‡
Homogenous catalysis
the catalyst is in the same phase as the reactants
heterogeneous catalysis
the catalyst is in a distinct phase
Determination of rate law
For the general reaction aA + bB -> cC + dD, rate = k[A]^x[B]^y The values of x and y are almost never the same as the stoichiometric coefficients, the orders of a reaction must be determined experimentally
Mixed-order/broken-order reactions
refer to either non-integer orders (fractions) or to reactions with varying rate orders
fractions are specifically described as broken-order
law of mass action (determining Keq from concentration)
For a generic reversible reaction aA + bB ⇔ cC + dD, if the system is at equilibrium constant temperature
Keq = [C]^c[D]^d / [A]^a[B]^b
products over reactants
Keq = (x)^2/1-x
- if x amount of A has reacted and x amount of B and C have been produced, and 1 is the starting concentration
- can be rounded so the denominator is simply the starting concentration (in this case 1)
Types of systems and energy/matter exchange
Isolated System cannot exchange energy or matter with surroundings
Closed System can exchange energy but not matter with surroundings
Open System can exchange energy or matter with surrounds
First law of thermodynamics
Change in internal energy can only occur through heat or work
ΔU = Q - W
Isothermal processes
Constant temperature, Internal energy is constant
ΔU = 0
Adiabatic processes
no heat exchanged between the system and environment
ΔU = - W
Isobaric processes
constant pressure does not alter the first law, but appears as a flat line on a P-V graph
Isovolumetric (Isochoric) processes
constant volume
ΔU = Q
State functions
describe the system in an equilibrium state without respect to process
Pressure, density, temperature, volume, enthalpy, internal energy, Gibbs free energy, entropy
Standard conditions vs standard temperature and pressure
Standard conditions: 298K 1atm and 1 M concentrations
Standard temperature and pressure (STP): 273K and 1 atm
Phase diagrams- critical point
the temperature and pressure above which there is no distinction between the phases
-supercritical fluid
Enthalpy, Change in Enthalpy equation
equivalent to heat under constant pressure (an assumption the MCAT usually makes)
ΔHrxn = Hproducts - Hreactants
Equation for heat change, specific heat of water
q = mcΔT
specific heat of water = 1cal/g*K
definition of heat capacity
the product mc, mass times specific heat
Bomb calorimeter
constant-volume calorimetry
Because W = PΔV, no work is done in an isovolumetric process, and (ΔU = Q)
Also an adiabatic process, no heat is exchanged between the calorimeter and the rest of the universe, but it is exchanged between the steel decomposition vessel and the surrounding water
Equation for heat required for phase change
q=mL
m is mass and L is latent heat
Entropy, second law of thermodynamics
time’s arrow, entropy always increases if not hindered from doing so
Entropy equation (heat and temperature)
ΔS = Qrev/T
change in entropy = heat gained or lost in a reversible process/ Temperature in Kelvin
Gibbs free energy equation
ΔG = ΔH - TΔS get higher test scores
Free energy change equations with K
ΔGrxn = -RTlnK deriving the standard free energy change for a reaction
ΔGrxn = -RTlnQ/K deriving the free energy change for a reaction not at equilibrium K is equilibrium constant
atm to mmHG to torr to kPA
1 atm = 760mmHG = 760 torr = 100kPA
when to use STP or standard state conditions
STP is generally used for gas law calculations; standard state conditions are used when measuring standard enthalpy, entropy, free energy changes, and electrochemical cell voltage
ideal gas law
PV=nRT
density equation, density gas equation
p (density) = mass/Volume = PM/RT
density = pressure*molar mass / R*Temperature
R = 0.0821 liter·atm/mol·K
R = 8.3145 J/mol·K
constant relationships of gas exchange
PV/T is constant, PV is constant, V/T is constant, n/V is constant and equals k (moles/volume is constant)
-these can all be derived from the PV=nRT equation
Molar mass of gas calculation
M = (Density@STP) * 22.4L/mol
Molar Mass can be calculated as the product of the gases density at STP and the STP volume of one mole of gas
Partial Pressures equations
Pt = Pa + Pb + Pc
Partial pressure of gas is related to its mole fraction
Partial pressure = moles of gas A / total moles of gas
The relationship between concentration and pressure is constant
Kinetic molecular theory assumptions
explains the behavior of gases
Assumptions
1 Particles have negligible volume
2 There is no intermolecular attractions or repulsions
3 Particles are in continuous, random motion, undergoing collisions with other particles and the container walls
4 Collisions between any two gas particles are elastic, with conservation of both momentum and kinetic energy
5 The average kinetic energy of gas particles is proportional to the absolute temperature of the gas, and is the same for all gases at a given temperature, irrespective of chemical identity or atomic mass
two Average molecular speed of gas equation
KE = 1/2mv^2 = 3/2kBT proportional to 3/2 the absolute temperature of the gas and Boltzmann constant
uRMS = sqr(3RT/M) M is molar mass
Diffusion calculation from molar mass
Graham’s law: under isothermal and isobaric conditions, the rate at which two gases diffuse are inversely proportional to the square roots of their molar masses
r1/r2 = sqr(M2/M1) r is the diffusion rate, M is the molar mass