C200_ General Chemistry equation Sheet

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119 Terms

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Dilutions

M1V1=M2V2 or C1V1=C2V2

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colligative properties

properties that depend on the concentration of solute particles but not on their identity

* Examples of these include boiling point depression, freezing point depression, osmotic pressure and vapor pressure

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Amphoteric

Compounds that can react as both an acid and a base, depending on the reaction conditions

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Percent error

(A-T)/T x 100

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absorbance and beer lambert law

ecl (e=molar extinction coefficient; c=samples concentration; l= path length

*if you know the absorbance of a solution, you can determine its concentration

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1 mol = how many atoms

6.023x10^23

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combustion reaction

(hydrocarbon or alcohol) + 02 --> co2 to H20

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Emprical Formula

most reduced form of a molecular formula

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Energy of a photon equation

Planck's constant x speed of light / frequency (HC/F)

*H=6.63x10^-34

*c=3.0x10^8

f= photons frequency

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quantum numbers

n (principle number), l(azimuthal), ml(magnetic), ms (spin)

*n= shell (distance from the nucleus)

*l= subshell (type of orbital)

-l=0 (s); 1(p); 2(d); 3(f)

*Ml=(-1....1) (determined by the l value )

ms= 1/2 & -1/2

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paramagnetic vs diamagnetic

unpaired electrons attracted to magnets

dia: all paired and slightly repelled by magnets

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relationship between energy, frequency and wave length

high energy = high frequency = low wave length

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ionic bond properties

(metal + nonmetal)

generally have high melting & boiling points, tend to be hard, brittle solids; tend to conduct electricity only when melted or dissolved in water----not in solid state

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covalent bond properties

(between two nonmetals)

sharing of electrons between with elements with similar electronegativity.

* high melting and boiling poiints, hard and do no conduct electricity

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molecular bonds

(2 or more non metals) low melting points and do not conduct electricity

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Ion size

more electrons = bigger size (anion) -

less electrons = smaller size (cation +)

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isoelectronic series

comparing elements with the same number of electrons.

The compound with the smallest amount of protons will be the largest in size

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ionization energy

The amount of energy required to remove an electron from an atom

trend: like electronegativity but includes noble gasses

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electronegativity

how thirst an atom is for electrons

up and to the right excluding noble gasses

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electron affinity

the energy given off when an atoms gains an elecctron (exothermic reaction)

*Cl has highest electro negativity

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temperature c to k

k= c+ 273

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Volume

1cm^3=1ml =1cc

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pressure

force/area (1atm = 760 torr or mmhg)

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Ideal gases behave

most ideally under low pressures and high temperatures

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at STP 1 mole of any gas =

22.4 L

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boyles law (gas law)

V is inversely related to pressure. ( V= 1/p)

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Charles law (gas law)

V and temperature are related

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Avagadro's Law

V=N

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Combined Gas Law

P1V1/n1T1 = P2V2/n2T2

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Ideal gas law

PV=nRT

R=.0821

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At STP

P=1atm and T =273k

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Density

P(MM)/RT = m/v

r=.0821 L*ATM/ mol k

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Dalton's Law of Partial Pressures

Total pressure of a gas is equal to the sum of the partial pressure of the component gases

Ptotal= Pa + Pb...

In terms of gas A : Pa=Xa P total

Xa= mol fraction of gas A

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Graham's law of effusion

Effusion refers to the movement of gas particles through a small hole. Graham's Law states that the effusion rate of a gas is inversely proportional to the square root of the mass of its particles.

r1/r2 = √(M2/M1) M=mola

r mass

r=rate of effusion

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intramolecular forces vs Intermolecular forces

Intramolecular forces are the forces that hold atoms together within a molecule.

Intermolecular forces are forces that exist between molecules.

<p>Intramolecular forces are the forces that hold atoms together within a molecule.</p><p>Intermolecular forces are forces that exist between molecules.</p>
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intermolecular forces

are forces that exist between molecules.

1). hydrogen bonding (strongest)

2) dipole dipole

3) dispersion forces (london disp/ van der wall) (weakest)

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hydrogen bonding

Hydrogen atom bonded to either an O, N, or F

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Dipole-Diople Forces

NON METAL molecules with polar bond causing the molecule to have a partial negative and positive charge

They line up in a complementary to each other and have big electronegativity differences between the two

<p>NON METAL molecules with polar bond causing the molecule to have a partial negative and positive charge</p><p>They line up in a complementary to each other and have big electronegativity differences between the two</p>
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dispersion force

no significant difference in electronegativity

Dispersion forces are in all molecules and are responsible for molecules boiling points

<p>no significant difference in electronegativity</p><p>Dispersion forces are in all molecules and are responsible for molecules boiling points</p>
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intermolecular forces and boiling points

responsible for boiling points. stronger the intermolecular forces leads to :

1) higher boiling point

2)high heat of vaporization

3) higher viscosity

4) higher surface tension

5) LOWER vapor pressure

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Intramolecular forces

forces are the forces that hold atoms together within a molecule.

Metallic bonds, Ionic bonds, Polar covalent bonds, covalent bonds,

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Phase changes

Freezing: crystalization

melting : fusion

Sublimation; fusion and vaporization : consumer heat therefore are endothermic reactions with a positive +ΔH and +ΔS (entropy, increasing disorder)

Deposition; condensation; crystallization are exothermic -ΔH because they release heat and have a -ΔS (because more order is being established)

<p>Freezing: crystalization</p><p>melting : fusion</p><p>Sublimation; fusion and vaporization : consumer heat therefore are endothermic reactions with a positive +ΔH and +ΔS (entropy, increasing disorder)</p><p>Deposition; condensation; crystallization are exothermic -ΔH because they release heat and have a -ΔS (because more order is being established)</p>
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Boiling point and vapor pressure

boiling point is when the vapor pressure = external pressure.

high boiling point = low vapor pressure

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Phase Diagram - triple point

unique for each substance, point where all three phases are in equilibrium

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Phase diagram - critical point

Point where liquid and gas are no longer distinguishable

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Molarity (M)

moles of solute/liters of solution

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Molality (m)

moles of solute/kg of solvent

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Solubility of ionic compounds in water rules

most group one metal cations NO3-; clo4-;c2h302- and nh4+ salts are soluble

most ag2+; pb2+; s2-: oh-; hg2 (2+); co3 2-; po4 2- are insoluble

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Solubility of solids and gasses (henrys law)

Pa=Kh(A)

pa= partial pressure of gas a

Kh= henerys law constant; changes with each problem

A= concentration of gas a

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Freezing point depression

ΔTf= -iKfm

i= vant hoff factor

Kf= freexing point depression constant

m= molality

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Boiling point elevation

ΔTb=- iKbm

i= vant hoff factor

Kb= boiling point depression constant

m= molality

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Vapor pressure depression

Psoln=X solv P solv

Psoln= new VP of solution

x solv = mol fraction of solvent (percent of solvent in new solution)

P solv = VP of pure solvent

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Osmotic pressure

pi=iMRT

i= vant hoff

M= molarity

r= .0821

T= temp

Pi= (n/v)RT

(n/v) = M

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chemical kinetics

the study of how fast a reaction occurs or the reaction rate

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Thermodynamics

tells us whether a reaction will occur but not how fast or slow it will occur

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General Rate rate

rate= k (A)^m (B)^n

k= rate constant

m&n: determined experimentally

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Rate constant units

Zeroth order: M/s (m^1 x s^-1)

First order: 1/s ( x s^-1)

Second order: 1/ M *S (m^-1 x s^-1)

Third order: 1/ M^2 *s (m^-2 x s^-1)

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Integrated rate law units (Graphs)

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Collison theory and arrhenius equation

K = Ae ^-Ea/RT

ea= activation energy

A= frequency factor

r= 8.314 J/mol k

k=rate constant

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Equilibrium constant expressions

Kc & Kp = Products/ reactants

Keq= kForward/ kreverse

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Keq Rules

K>1 = products are favored at equilibrium

k<1= reactant are favored at equilibrium

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solubility product constant (Ksp)

Ksp= products / reactants

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pH & pOH

pH = -log (H+)

pOH= -LOG (oh-)

ph +poh = 14

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(h+) & (oh-)

(H+)= 10^-PH

(OH-)= 10^-POH

(H+)(OH-)= 1*10^-14

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Weak acids

HA + H2O <----> h30+ + A-

ka= (h30+)(A-)/ (HA)

*ka= acid dissociation constant

(H+) = SR(ka)(HA)

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Weak base

A- + H2O <----> HA + OH-

kB= (HA)(OH-)/ (A-)

*kB= BASE dissociation constant

(OH-) = SR(kB)(A-)

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pKa and pKb

pKa=-log(ka)

pKb=-log(kb)

pka+pkb = 14

Kw=ka x kb =1

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Ka and Kb strength

larger Ka = smaller pka = stronger acid

larger kb= smaller pka = stronger base

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Arrhenius acid

h+ donor in water

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arrhenius base

OH- donor in water

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Bronsted-Lowry acid

h+ donor

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Bronsted-Lowry base

H+ acceptor

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lewis acid

electron pair acceptor

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lewis base

electron pair donor

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conjugate acid-base pair

acid --> base (remove hydrogen and the charge decreases by one_

base---> acid (adds 1 hydrogen and increases the charge by 1)

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Trends in acid strength

the more oxygen atoms means the more acidic it is due to resonance.

if the number of oxygens is the same the the more electronegative heteroatom = more acidic

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Neutralization reactions and normality

*reactions that occur between acids and base; which always makes h20 and a salt

NaMaVa=NbMbVb

Na= number of hydrogen groups the acid can donate

Nb= number of oh groups the base can donate

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Buffers and henderson hasselbalch

buffer= is a solution that resists ph change. it is made from a weak conjugate acid/ conjugate base pair

ph= pka +log (A-)/(HA)

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Enthalpy

the amount of heat energy a substance contains

HA + H2O <----> h30+ + A-

ΔH > 0 -endothermic

ΔH < 0 exothermic

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Enthalpy of formation (ΔHf)

Δhf = nΔH(products) - nΔH(reactants)

n= coefficient from the balanced reaction

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first law of thermodynamics (law of conservation of energy)

ΔE= q + w

q= heat

w=work

ΔE= change in internal energy

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pressure-volume work

w= -p Δ V

ΔV= change in volume

p= external pressure

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calorimetry thermal energy

q= -Ccalorimetry ΔT

Cal= specific heat of calorimeter

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heat curves and thermal energy

q=mc ΔT or q=mc ΔH(fusion or vaporization)

m=mass

c= specific heat

ΔT= change in heat (final - initial )

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entropy formula

a measure of how disordered something is

ΔS= Sum(n)Sproducts- Sum(n) S reactants

Sgas> Sliquid> Ssolid

saq> Ssolid

Srxn> 0: when there is an increase in the number of moles of gas

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Bond Disociation Energy

ΔH= Sum ΔH (products) - S ΔH (reactants)

=Sum ΔHbroken - Sum ΔH formed

making bonds = exothermic (ΔH-)

breaking bonds= endothermic (ΔH+)

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Gibbs free energy equation

a measure of spontaneity

ΔG^0 = ΔH - TΔS

ΔG^0= standard conditions

ΔH= enthalpy

ΔS= entropy

T= temperature in kelvins

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Gibs free energy equation (Keq standard and nonstandard conditons)

ΔG= ΔG^0 + R(T)(Ln Q)

ΔG^0= -RTLnKeq

ΔG^0= standard conditions

Keq= equilibrium constant

Q= reaction quotient

R= 8.314 J/mol k

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standard cell potential (E°cell) (reduction potentials)

E^o cell = E^o reduction + E^o oxidation

E^o = E^o cathode + E^o anode

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Gibs free energy (ΔG) rules

ΔG= - (spontaeous)

ΔG= + (nonspontaenous)

ΔG= 0 at equilibrium

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Gibs free energy relation with enthalapy (ΔH) and entropy (ΔS)

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Relating Gibbs Free Energy and K

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Redox reactions

Reactions that involve the transfer of electrons from one element to another.

Reduction-oxidation reaction

(OIL RIG)

-3------> 3 (OXIDATION)

3+-------> 3 (REDUCTION)

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Reducing agent (reductant) in redox reactions

is the element that GIVE UP e- (gets oxidized) is the REDUCING AGENT

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Oxidizing agent (oxidant) in redox reactions

is the reactant that gets reduced

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Balancing redox reactions

Break the reactions into (1/2) reactions

1 should be the oxidation reaction and the other should be the reduction equation

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anode

is the site of oxidation

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cathode

is the site of reduction

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Balancing Redox Reactions (under acidic conditions)

1). identify what is being oxidized and what is being reduced

2). seperate the oxidation reaction from the reduction reaction (1/2) reactions

3). balance all the atoms the ARE NOT HYDROGENS OR OXYGENS

4). balance the oxygens by adding H2o to which side needs it

5). balance the hydrogens by adding h+ to the side the needs it

6). add e- wherever necessary to balance the charge on each side of the equation

7). as needed, add integer to your half reactions to make the number of moles of e- equal in each of your half reactions.

8). the final balanced number of e-s is the number of overall electrons per mole that get transferred in this particular redox reaction

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Balancing Redox reactions (under basic conditions)

1). identify what is being oxidized and what is being reduced

2). seperate the oxidation reaction from the reduction reaction (1/2) reactions

3). balance all the atoms the ARE NOT HYDROGENS OR OXYGENS

4). balance the oxygens by adding H2o to which side needs it

5). balance the hydrogens by adding h+ to the side the needs it

6). add the same number of OH- to both side of the equation that you added to your half reactions.

- combine the h+ and oh- on the same side of the equation to form H2o. and eliminate excess h20

7). add e- wherever necessary to balance the charge on each side of the equation

8). as needed, add integers to your half reactions to make the number of moles of e- equal in each of your half reaction.

9) the final balanced number of e-s is the number of overall electrons per mole that get transferred in this particular redox reaction