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mole ratio
ratio of coefficients in balanced equation
theoretical yield
maximum amount of product that can be produced, answer when you have grams + grams
actual yield
the amount produced in the lab
percent yield
measure of how efficient a chemical reaction is, actual yield/theoretical yield x 100
energy
the ability do work or produce heat
thermodynamics
study of energy
potential energy
held within chemical bonds
kinetic energy
exhibited by moving particles
endothermic
energy absorbed, ex. ice cube melting
exothermic
energy is released, ex. fire burning
the first Law of Thermodynamics
energy is neither created nor destroyed
system
the part of the universe observed
surroundings
everything else in the universe
heat
a flow of energy due to a temp difference
q
heat energy in J
m
mass in grams
C
specific heat capacity in J/g °C
ΔT
change is temperature, Tf - Ti
temperature
measure random motions of components of a substance
enthalpy
a measure of energy of a system, ΔH
electromagnetic energy
energy that travels as waves through space at a speed of light in a vacuum
wavelength
distance between two consecutive wave peaks, lil wave thing
frequency
number of wave peaks that pass a point per given time period, V
speed
how fast a given peak travels, C
wavelength unit
meters
frequency unit
hertz
speed unit
3.00 × 108 m/s
orbital
3D region where there is high probability of finding an electron
principle energy level
discreet energy level of an atom
sublevel
part of principle energy level that corresponds to an electron orbital, indicated by a letter
number of electrons an orbital can hold
2
labeling orbitals
number of principle energy level
letter of sublevel
level 1
1s, one orbital
level 2
2s and 2p, 3 orbitals
level 3
3s, 3p, 3d, 5 orbitals
electron configuration
shows the arrangement of electrons in an atom
noble gas abbreviation
use noble gas on row directly above your element
put noble gas in brackets
continue configuration left - right same row as element
pauli exlcusion principle
orbitals can hold up to two electrons, those electrons must have opposite spins
valence electrons
electrons in the outermost principal energy level of an atom, the ones involved in making bonds
core electrons
inner electrons
nuclear attractive force
stronger when electrons are closer
atomic size (radius)
distance between the nucleus and the edge of the electron cloud
atomic size trend
decreases across a row, increases down a group
ionization energy
the amount of energy required to remove an electron
ionization energy trend
opposite of atomic size, increases across a row and decreases down a group
energy is released by . . .
emitting light
these are carried by . . .
photons
quantized
energy of an atom can only exist in specific, discrete units
ground state
lowest possible energy state
excited state
atom exposed to energy source, excited to higher energy level
the Bohr model
only works for hydrogen atom, electrons do not orbit nucleus
the wave mechanical model
electrons in orbitals, not orbits, gives probability of where electrons could be
octet rule
atoms form bonds that give them 8 valence electrons
electronegativity
the ability of an atom to attract electrons while in a compound
bond polarity
the difference between the EN values of the atoms in a bond
below 0.4
nonpolar
0.4 - 1.7
polar
above 1.7
ionic
lone pair
unshared pair of electrons
duet rule
followed by hydrogen, most stable when surrounded by 2 electrons
what atoms go in the center?
first atom, carbon
what atoms don’t go in center?
hydrogen, halogens
steps for Lewis Structures
calculate total # of valence electrons
connect each atom with line
subtract those values from total
distribute remaining # to satisfy rules
resonance
when more than 1 valid Lewis Structure exists for a bond
for ions . . .
add an electron for each negative or subtract for each positive, add brackets with charge
VESPR model
electron pairs want to be as far from each other as possible
double bonds treated as one repulsive unit
2 atoms are linear
pressure
force of all gas particle and wall collisions
vacuum
absence of pressure
pressure units
pascal (Pa), mmHg, torr, atm, psi
atmospheric pressure
caused by weight of air in atmosphere, measured by barometer
barometer
air pushes down on mercury, the more pressure there is, the higher the mercury rises in the tube
Boyle’s Law
pressure + volume have indirect relationship, P1V1 = P2V2
Charle’s Law
volume + temperature have a direct relationship, V1/T1 = V2/T2
Avogadro’s Law
volume + moles have a direct relationship, V1/n1 = V2/n2 ALSO 22.4 L = 1 mole
The Ideal Gas Law
PV = nRT
Dalton’s Law of Partial Pressures
total pressure of a mixture of gases is equal to sum of their pressures
characteristics of gases
no fixed volume
low density
mixtures are homogeneous
kinetic molecular theory
movement of particles in matter, attempts to explain ideal gas behavior
intramolecular forces
between atoms, chemical bonds
intermolecular forces
between molecules, keeps solids + liquids together
London Dispersion
nonpolar bonds, C + h, noble gases
Dipole-Dipole
polar bonds, ionic bonds
Hydrogen bonding
N, O, F
polarizability
ability of electron cloud to be unevenly distributed
number of atoms
stronger intermolecular forces, more attraction sites
relationship between atomic size/boiling point
larger atomic size causes higher boiling point
shape of molecule
more linear structure means more attraction sites
crystaline
regular microscopic arrangement
amorphous
disordered microscopic structure
ionic solids
made of ions, stable, high melting points
molecular solids
held together by weak intermolecular forces, lower melting points
metallic solids
held together by metallic bonds, “electron sea” model
alloids
homogeneous mixture of metals
solution
homogeneous mixture
solvent
dissolves other substances
solute
the substance being dissolved
soluble
able to dissolve in a particular solvent
insoluble
unable to dissolve in a particular solvent
miscible
liquids that dissolve in each other
immiscible
liquids that are insoluble in each other