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93 Cards in this Set

  • Front
  • Back

Coulomb's Law

The electrostatic force between two charges separated by a distance is FΩ(QeQn)/r^2

Effective Nuclear Charge

Qneff ~ Qn - (# of shielding electrons)

Qe

-1

Qn

Charge of the elements nucleus

Atomic Radius Trend

Increases as you down and left.

Explanation of Atomic Radius Trend

Valence shell decreases/stays the same.


Core increases/stays the same


Qneff decreases/stays the same



Qneff decrease had bigger affect than valence shell decrease(left)


When Qneff stays so does valence, core increases size(top to bottom)

Ionization Energy

The energy required to remove the outermost (highest energy) electron from an atom in the gaseous state

Ionization Energy Trend

Increases moving right and up.

Ionization Energy Trend Explanation

Atomic Radius decreases


Qneff increases(right)/constant(up)

Third Ionization Energy

Very large increase in IE because the atom is smaller (r smaller) and Qneff is larger

Electron Affinity

The energy change when an electron is added to an atom in the gaseous state.

Negative Electron Affinity

The ion is more stable than the atom.

Positive Electron Affinity

The ion is unstable and doesn't form spontaneously.

Negative Electron Affinity Tend

An electron is added into a partially filled subshell.

Positive Electron Affinity Trend

An electron is added to an element that has filed subshells.

Anion Atomic Size

Larger than there atoms

Cation Atomic Size

Smaller than there atom.

Ionic Bond

One or more electrons is permanently transferred from one atom to another.

Lattice Energy

The energy reqired to create a mole of ionic solid from its constituent ions in the gas phase. Inferred from the force of attraction

Force of Attraction

FΩ(Q1Q2)/r^2

Comparing Lattice Energies

The size affects r, the charge affects Q1,Q2

Properties of Ionic Materials

Very high melting points


Hard but brittle


Conducts electricity: never in solid, always in aqueous solution

Covalent Charge

When 2 nonmetal atoms share electrons.

Isoelectric

Has the same number of electrons

Electronegativity

The ability of an atom to attract the electrons in a chemical bond.

Electronegativity Trend

Increases right and up, same reasons as ionization energy.

Rules for Drawing Electron Dot Formulas

1. Calculate the total number of valence electrons


2. Draw the skeleton structure


3. Distribute the remaining v.e. amongst the outer atoms to complete there octets


4. Place any remaining v.e. on the central atom

Delocalized Bonding

The electrons in the double bond are spread over two bonds

Resonance Form

Each possible lewis structure connected by double-headed arrows.


Same atoms arranged in the same way but with double or triple bonds in different places.

Bond Order

Indicates the extent of multiple bonding.


Single bond: bond order=1


Triple bond: bond order= 3

Polyatomic Ion

Molecule with a charge

Formal Charge

(Original # of valence electrons) - ( # of electrons in lone pairs) - (# of bonds)

Linear

2 electron groups

Trigonal Planar

3 electron groups

Tetrahedral

4 electron groups

Trigonal Bipyramidal

5 electron groups

Octahedral

6 electron groups

AX2E

Bent

A3E

Trigonal Pyramidal

AX2E2

Bent

AX3E2

T shaped

AX4E

See saw

AX2E3

Linear

AX5E

Square pyramidal

AX4E2

Square planar

Hybridization

The blending of occupied atomic orbitals to make the same number of hybrid orbitals

Valence Bond Theory Steps

1. Draw the lewis structure


2. Calculate the formal charge on the atom toy are interested in


3. Draw ground state orbital diagram


4. Promote electrons


5. Keep one p-orbital unhybridized for each pi-bond attached


6. Hybridizevall remaining occupied orbitals in the valence shell

Rotational Isomers

Molecules with the same atoms, but in different arrangements.

Phase Diagram

Shows the phase (state) of a substance as a function of pressure and temperature.

Triple Point

The point at which all three phases are in equilibrium (all present in the same place at the same time)

Critical Point

The end of the gas-liquid phase transition line

Supercritical Fluid

No distinction between liquid and gas.

Attractive Forces

Holding together particles that are weakly attached. Not much energy is required to separate particles. They break apart and reattach often under normal conditions.

Bond

Ionic and covalent attractions between atoms or ions.

Chemical Bonds

Ionic and covalent bonds

Intermolecular Forces

Attractive forces between molecules.

Temporary Dipoles

Form due to random motion of 'electron clouds'

London Dispersion Forces

The attraction between partial charges (temporary dipole and an induced dipole)

Dipole-Dipole Forces

Attraction between permanent dipoles.

H-Bonds

The strong electrostatic attraction between a very Ω+ H-atom and a 'concentrated' lone pair of electrons (Ω-) on an O, N, or F-atom.

Dipole-Induced Dipole Forces

A polar molecule (permanent dipole) can induce a temporary dipolein a nonpolar atom/molecule.

Ion-Induced Dipole Forces

An ion induces a temporary dipole in a nonpolar atom/molecule.

Ion-Dipole Forces

Attractive force between an ion and a molecule with a permanent dipole.

Vapor Pressure

The pressure of the gaseous vapor above a liquid.

Boiling

When the vapor pressure is equal to the atmospheric pressure.

Surface Tension

The energy used to create new surface area (J/m^2). The energy needed to seperate the molecules.

Capillary

When a liquid rises up into a narrow space. Occurs when there is a stronger attraction between liquid molecules and the sides of the glad tube than between the lewis molecules themselves.

Viscosity

How 'thick' or 'sticky' a liquid is.

Solution

Solute dissolved in a solvent.

Molarity

(Moles of solute)/(liters of solution)

Molality

(Moles of solute)/(kg of solution)

Mass percent

(Mass solute)/((mass solute)+(mass solvent)) × 100%

Volume Percent

(Volume of solute)/(volume of solution) × 100%

Mole Fraction

(Moles of A)/(total moles in mixture)

^Hsolvent

The heat required to seperate the solvent molecules so that the solute can be added - endothermic

^Hsolute

The heat required to separate the solute molecules so that they can be dispersed evenly throughout the solvent - endothermic

^Hmix

The heat produced by the attraction between the solvent and solute molecules/ions (bond formation) - exothermic

^Hsolution

The overall enthalpy change when a solute is dissolved in a solvent - tge solute molecules are separated and dispersed homogeneously throughout the solvent.

Exothermic

Enthalpy decreases

Endothermic

Enthalpy increases

Gibbs Free Energy

Thermodynamic potential

Entropy

The something else that turns H until G includes a measure of how disordered the system is.

Why Endothermic Reactions Happen

The product (the solution) is more disordered than the reactants (the solid and the solvent) - The system's entropy increases. Increase in entropy makes a system a little more stable. This added stability can compensate for the loss of stability that accompanies an endothermic process.

Polar Solvent

A liquid composed of polar molecule.

Nonpolar Solvent

A liquid composed of nonpolar molecules.

Henry's Law

Gas solubility = kH × Pgas


((gas solubility 1)/(gas solubility2)) = ((P1)/(P2))

Solubility

The maximum amount of solute that can be dissolved in a solvent.

Colligative Properties of a Solution

Vapor pressure lowering


Freezing point depression


Boiling point elevation


Osmotic pressure

Van't Hoff Factor

The number of moles of particles produced by 1 mole of solute.

Van't Hoff Factor Equation

i = (moles of particles in solution)/(moles of solute in solution)

Raoult's Law

When a solute, B, is added to a solvent, A, the vapor pressure of the solvent can be found using the mole fraction of the solvent, XA, in the solution;


PA=P°A×XA


PA - the new vapor pressure of the solvent in the solution


P°A - the vapor pressure of the pure solvent.

Freezing Point Depression

^Tf=i×Kf×cm


^Tf - the difference between the freezing point of the pure solvent and that of the mixture.


i - van't Hoff factor


cm - molal concentration of the solute (mol/kg)

Boiling Point Elevation

^Tf=i×Kb×cm


Kb - the boiling poit elevation constant.