MECHANICS
- Galilean Equations of Motion under
Constant Acceleration
(No s)
(No v)
(No t)
where a = constant acceleration
u
= initial velocity
v
= final velocity
s
= displacement
and t = time taken.
Note: For a projectile at maximum height the speed is zero.

where p is momentum, m is mass and v
is velocity.
- Conservation of Momentum

where a pair of masses
and
have velocities
and
respectively.
After they interact they have velocities
and
respectively.
or 
where F is force, p is momentum and t is time
or F is average
force, m is mass, v is final velocity and u is
initial velocity.
- Newton’s Second Law.

where F is force, m is mass and a
is acceleration.

where W is the weight of an object of mass
m and g is the acceleration due to gravity.
and

where x is the horizontal component and y is the vertical
component of a vector v which is at angle of
to the horizontal.

where P is pressure, F is force and
A is area.

where
is
the density of a body with mass m and volume V.

where P is the pressure in a fluid,
is
the density of the fluid, g is the acceleration due to gravity and h
is the depth at which the pressure is being taken.
- Boyle’s Law

where P is the pressure of an ideal gas and V is its volume.

where F is the gravitational force between
a mass
and
a mass
separated
by a distance of d metres and where G is the universal
gravitational constant.

where g is the acceleration due to gravity
at a distance d from a planet of mass M.
G is the universal gravitational constant.

where M is the moment of a force F
applied at a distance d from a given point.

where T is the torque (moment) of a couple, i.e. a pair of force
each of magnitude F, having opposing directions and separated by a
distance d.

where W is the work done when a force F
moves a body a distance s in the direction of the force.

where
is
the kinetic energy of a body of mass m and velocity v.

where
is the potential energy required to
move a mass m a vertical distance h and g is the
acceleration due to gravity.

where P is the average power when W is the work done in a
time t.


where
is
the angle in radians corresponding to an arc length l in a circle
of radius length r.

where
is the average angular speed when a
body in circular motion traces an angle of
radians in t seconds.

where v is the tangential velocity of an
object moving in a circle of radius length r with a constant
angular speed
.
or 
where a is the centripetal acceleration of a body moving in a
circle of radius length r with a constant angular velocity
and
a tangential velocity v.
or

where F is the centripetal force required to keep a body of mass m
moving in a circle of radius r. The body moves with a constant
angular velocity
and
a tangential velocity v.

where v is the speed of a satellite in a
circular orbit of radius R around a planet of mass M. G
is the universal constant of gravitation.

where T is the period of a satellite moving at a constant velocity v
in a circular orbit of radius R.
- Kepler’s Third Law

where T is the period of a a circular orbit of radius R around a planet of
mass M. G is the universal constant of gravitation.

where R is the radius of a circular orbit
of period T around a planet of mass M. G is the
universal constant of gravitation.
Note: for a geostationary or parking orbit T = one day = 86, 400
seconds. The height, h, of such an orbit is given by
, where r is the radius of the
planet..
- Hooke’s Law

where F is the force required to give a
spring a displacement s and k is a constant of
proportionality. (Note: the spring must not be extended by beyond its
elastic limit.)

where a is the acceleration of a body
moving in simple harmonic motion when it has a displacement s from
its equilibrium position. The constant of proportionality is given by
.

where T is the period of a body moving in
simple harmonic motion with a constant of proportionality
.

where T is the period of a simple pendulum
of length l and g is the acceleration due to gravity.