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kinematics
study of motion and the values used to describe it
distance
total path taken
displacement
the direct distance between starting and ending points
scalar
has magnitude only
vectors
has magnitude and direction
speed
change of distance over time
velocity
change in distance over time with direction
instantaneous speed
can be calculated from finding the slope on a distance time graph
acceleration
change of velocity over time
acceleration is the slope
velocity time graph
area under a velocity time graph
displacement
area under a acceleration time graph
change in velocity
area under a force time graph
impulse
trajectory
path in air
kinematic equations only apply
acceleration is constant
area under speed time graph
distance
why does gravity not affect horizontal motion
horizontal and vertical motion are completely independent of each other
what speed do objects hit the ground with
the same speed it was released with
fluids
gases and liquids
air resistance comes from what
an objects kinetic energy transferring into the fluid
terminal velocity
when the speed of a falling object does not increase
inertia
resistance to change in motion
newtons first law
an object remains stationary or moves at constant velocity until acted upon by an external force
Newton’s second law
Force = mass x acceleration
Newtons
applied force needed to accelerate 1 kg of mass at the rate of 1 m/s
Newton’s third law
every action has an equal and opposite reaction
translational equilibrium
an object when it is either at rest or moving at constant velocity
non-contact forces
when forces are acting between objects that dont touch
contact forces
forces we observe when objects are touching in some way
extension
change in length from the springs intial length
Hooke’s Law
F = K(change in x)
K
spring constant
combinging springs in series
(1/kt)= (1/k1)+ (1/k2)
combining springs in parallel
kt = k1 + k2
total spring extension in series
(2mg)/k
density
mass/volume
pressure
normal force/area
buoyancy force
density x gravity x volume
height of a floating object
depends on densities of object and fluid
archimedes’ principle
upwards buoyancy is equal to the weight of the fluid displaced by said object
ratio for coefficient of friction
friction/normal force
Stokes Law for drag
6π(viscosity)(speed)(radius)
momentum
mass x velocity
collision
any interaction where momentum is transferred or shared between moving objects
impulse
force x change in time
principle of conservation of linear momentum
momentum is always constant when no resultant external force acts on the system
if an initially stationary system separates abruptly, what’s the final momentum
final momentum is zero because they are opposite in direction.
kinetic energy using momentum
Ke = (p²/2m)

what happens if the densities are equal
it floats
pressure units
N/m²
1 N
1 kg/m²
range
horizontal velocity x time
centripetal force
(mv²)/r
magnetic force
Qvb = F
Q - charge
v - velocuty
b - mangetic field
angular velocity from linear velocity
𝜔=𝑣/𝑟
angular velocity from angular displacement
𝜔 = theta/ time
angular velocity from time period
𝜔 = 2π/T
angular velocity from frequency
𝜔 = 2πf
circumference
2πr
Keplers 1st law
planets’ orbits are eliptical ovals not perfect circles
Keplers 2nd law
orbits of planets sweep equal areas in equal amounts of time
Keplers 3rd law
planets orbital period squared is proportional to average distance cubed
gravitational force
((G)(m1)(m2))/r²
when objects in a collision stick together
add masses
a perfectly elastic collision forms
a right angle
elastic potential energy
(1/2)kx
heat formula
Q=mct
specific temperature (C)
amount of energy needed to change temperature of a given object w mass
units for specific temperature
J/((kg)(k))
Heat equation for phase changes
Q=mL
energy being proportional to mass means what
larger objects w slow kinetic particles have more energy than small objects w high kinetic particles
specific heat of water
4185
specific heat of ice
2100
specific heat of vapor
2010
latent heat of fusion
334000
latent heat of vaporization
2.26×10^6
ideal gas law with moles
PV=nRT
ideal gas law with particles
PV = NKBT
R
gas constant - 8.31
KB
botzman constant - 1.38 ×10^-23
n
moles
N
number of particles
Internal energy
U = (3/2)nRT = (3/2)NKBT
root mean velocity square
((3KBT)/m)^1/2
Volume in a piston problem
Area (change in length)