Circular Motion & Gravitation (topic 6) Flashcards
Linear speed equation
v = 2πr / T
where,
v = linear speed (ms^-1)
r = radius (m)
T = period (sec)
Angular speed equation
ω = 2π / T OR ω = 2πf
where,
ω = angular speed (rad sec^-1)
T = period (sec)
f = frequency (Hz or sec^-1)
Relation between linear speed and angular speed
v = ωr
where,
v = linear speed (ms^-1)
ω = angular speed (rad sec^-1)
r = radius (m)
Centripetal acceleration equation
a = v^2 / r
where,
a = acceleration (ms^-2)
v = linear speed (ms^-1)
r = radius (m)
Centripetal force equation
F = mv^2 / r OR F = mω^2r
where,
F = force (N)
m = mass (kg)
v = linear speed (ms^-1)
r = radius (m)
ω = angular speed (rad sec^-1)
Field strength equation
F = G Mm / r^2
where,
F = force of attraction between two masses (N)
G = gravitational constant
M, m = mass (kg)
r = distance between center of both masses (m)
Gravitational field strength
g = F / M OR g = G M/r^2
where,
g = gravitational field strength (N kg^-1)
F = force (N)
M = mass (kg)
Orbital speed equation
V = √(GM / r)
where,
V = linear speed
G = gravitational constant
M = mass
r = orbital radius
Kepler’s 3rd law
T^2 = 4π^2 / GM * r^3
Where,
T = time
G = constant
M = mass
r = radius
Force exerted on mass by rod
- Is non zero
- Changes magnitude throughout rotation
- Is not always directed towards the center
- Is a minimum at the top