1/40
Looks like no tags are added yet.
Name | Mastery | Learn | Test | Matching | Spaced | Call with Kai | Chat |
|---|
No analytics yet
Send a link to your students to track their progress
Solids
Fixed shape regardless of container
Particlesâre closed together and held rigidly in place
Movement of solid particles - vibration, stretching, and rotation
Liquid
Adopts the shape of a container to the extent of its volume
Forms an upper surface
Particles're close together but are free to move around each other
Gases
Adopts container shape and fills it
Particles're far apart and move randomly
High kinetic energy
Compelling and predictable properties common to all
Gas Property 1
Gas volume changes significantly with pressure
Solid and liquid volumes aren't greatly affected by pressure
Pressure and volume are inversely proportional
Gas Property 2
Gases expand when heated (due to high energy) and shrink when cooled
The volume change is 50 to 100 times greater for gases than for liquids and solids
Gas Property 3
Gases move freely / spread out and occupy all the space they can
Gas Property 4
Gases have relatively low densities
Even in large containers, the amt of gas particles're relatively iow
Gas Property 5
Gases form a solution in any proportions
They're freely miscible with each other
Kinetic Molecular Theory of Gases
Applies specifically to an ideal gas
5 postulates
Ideal gas
DNE
Imaginary gas whose behavior perfectly fits all assumptions of the KMT
Postulate 1
Gases consist of very large numbers of tiny spherical particles thatâre far apart from each other compared to their size (lots of empty space)
Postulate 2
Gas particles are in constant rapid motion in random directions
Explains why gases move quickly
Postulate 3
Collisions between gas particles and container walls are elastic collisions
Elastic Collisions
Particles bounce off each other and don't lose energy when they collide
Colliding energy is conserved (remains the same)
Postulate 4
There are no forces of attraction or repulsion between gas particles
Postulate 5
The avg kinetic energy of gas particles is dependent upon the temp of the gas
Hotter = faster, cooler = slower: directly proportional
Pressure
Amt of force applied for each unit of area
Amt of force applied by the gas molecules against the walls of its container
P = f/a - force/area
Atmospheric pressure
Arises from the force exerted by atmospheric gases on the Earth's surface
Decreases with altitude (higher location = lower pressure)
Currently, the atmosphere is applying 14.7 lb/s² or 14.7 psi to the Earth's surface
Our body has 1 atm
1 atm is equal to
1.01325 Ă 10âľ Pa
101.325 kPa
760 mmhg
760 torr
14.7 lb/s² or 14.7 psi
1.01325 Bar
Boyle's Law
P1V1 = P2V2
Pressure and volume are inversely proportional
Proposed by Robert Boyle in 1662
The volume of a gas at constant temp varies inversely with the pressure exerted on it
Less space (decreased volume) â more chances for gas and container wall collision â increased pressure
Charles' Law
V1/T1 = V2/T2
Proposed by Jacques Charles in 1780
The volume occupied by a fixed amt of gas is directly proportional to its absolute temp at constant pressure
Increased temp â increased KE â increase in space between gas particles â volume increase
The temperature should always be in Kelvin
Avogadro's Law
V1/n1 = V2/n2
Proposed by Amadeo Avogadro in 1880
The volume of a gas is directly proportional to the amt of gas at constant temp and pressure
Gases occupy all the space they occupy â volume increase â more gases need to occupy all available spaces
Avogadro's hypothesis
At a given pressure and temp, = volumes of all gases contain = number of moles/particles
At standard pressure and temp (STP, 0°C/273K and 1atm), the volume of 1 mole of any gas will occupy the same volume of 22.4L
1 mole = 22.4L (molar volume)
Ideal Gas Law
PV = nRT
For a specific amt of gas, the product of pressure and volume is directly proportional to the absolute temp
All gases have the same # of gas molecules when under equal volume, temp, and pressure
Universal Gas Constant (R)
Determined by using values at STP (273K, 22.4L, 1mol, 1atm)
PV/nT
= 0.08205 L*Atm / k*Mol
Diffusion
Gradual movement/mixing of diff gases by random molecular motion and collision in response to the diff concentration
Effusion
Gas escapes from a container through a hole of diameter considerably smaller than the free mean path of the molecules
Graham's Law of Effusion
The ratio of the rates of effusion for 2 gases is equal to the square root of the inverse ratio of the gasesâ molar masses
Rate of effusion is inversely proportional to the square root of its molar mass
The time of effusion is directly proportional to the square root of its molar mass
relationship that closely approximates the rate of effusion
Light gases diffuse and effuse much more rapidly than heavier gases
Graham's Law of Effusion formulas
Tip: make gas A the lighter gas
RateA/RateB = â(M.M.B/M.M.A)
tA/tB = (M.M.A/M.M.B)
DALTONâS LAW OF PARTIAL PRESSURE
total pressure in a mixture is the sum of the partial pressures(exerted by an indiv gas) of the component gases.
higher partial pressure = more amt of gas molecules
partial pressure isnât affected by types of gas (ex: 2molecs N + 2molecs O = 4molecs O2)
partial pressure is proportional to mole fraction
History of the Atomic Model
John Dalton
JJ Thomson (Plum Pudding Model)
Ernest Rutherford (Nuclear Model, Gold Foil Experiment)
Bohr Model - electron orbits, disproved due to Heisenbergâs Uncertainty Principle
Schrodinger (Quantum Mechanical Model Electron Cloud or Planetary Model) - orbitals; probable but uncertain positions of electrons
Quantum Mechanical Model
elements with only a few electrons still have many orbitals
Electron Configuration
shorthand way of determining the probable location of the electrons of an atom
nl#
nl#
n - energy lvl where the electrons are found
l - subshell where the electrons are found
# - # of electrons found in the energy lvl/subshell
atomic orbital
specified by 3 quantum #s
PRINCIPAL QUANTUM NUMBER (n)
Describes the size of the orbital
Indicates relative size of the orbital & relative distance of the electron from the nucleus.
symbolizes/corresponds to the atomâs energy level or shell occupied by the electron/atomic nucleus.
larger value = greater the distance from the nucleus and greater size of an atom
Integral value(+): 1, 2 , 3 ,4 , 5, 6, 7, ...
electronâs distance from the nucleus is directly proportional to the energy of the electron n is also a measure of the orbital
nearest energy lvl to the nucleus is K (followed by L,M,N)(?)
ANGULAR MOMENTUM QUANTUM NUMBER (l)
Describes the shape of the orbital
= to an integer from 0 to (n â 1)
indicates the sub energy levels of the atom and the relative shape and characteristics of the orbital
corresponds to the subshell or sublvl occupied by the electron
MAGNETIC QUANTUM NUMBER (ml)
prescribes the three-dimensional orientation of the orbital in the space around the nucleus
value is -(l) to +(l), amt of possible ml = number of orientations
indicates the spacial orientation of the orbital
MAGNETIC SPIN QUANTUM NUMBER (ms)
Direction where the electron is spinning.
Determine if atom can produce a magnetic field
only possible values are +½ and -½ (because each orbital can only have at most one of each spin direction)
#
maximum number of electrons the l can hold