Object motion is represented with vectors.
Velocity is a vector:
Vector direction is direction of movement
Vector magnitude is speed of movement
Velocity vector corresponds to amount object will move in one unit of time.
Displacement = Velocity * time
If an object starts at position P0,
with velocity V,
after t time units, its position P(t) is:
P(t) = P0 + V * t
Note: choice of units is arbitrary, as long as things are consistent.
e.g. use meters for distance, seconds for time, and meters/second for velocity.
Don't try to combine meters/second with miles/hour, for instance.
The previous formula only works if the object moves with a constant velocity.
In many cases, objects' velocities change over time.
In such a case, velocity is a function that we integrate.
Displacement = Velocity dt
In complex motion, there isn't an analytical solution (i.e. a simple formula).
Euler integration approximates an integral by step-wise addition.
At each time step, we move the object in a straight line using the current velocity:
dt = t1 - t0 P(t1) = P(t0) + V * dt
Velocity is the integral of acceleration:
Applying Euler integration again gives:
dt = t1 - t0 Acc = computeAcceleration() Vel = Vel + Acc * dt Pos = Pos + Vel * dt
Gravity near the Earth's surface produces a constant acceleration of 9.8 m/sec2
In this case:
Acc = Vector([0, -9.8, 0])
Newton's 2nd Law of Motion:
Which can be rewritten as
If an object has mass M, and force F is applied to it,
its motion can be calculated via Euler integration:
Acc = F / M Vel += Acc * dt Pos += Vel * dt
Note that F, Acc, Vel, and Pos are all vectors. M is a scalar.
F = (G * M1 * M2) / d2
For a complete simulation, we need to calculate the force on each object every frame.
When multiple forces are applied, their vectors are added.
Drag (slow moving objects):
F = Cdrag * V
Drag (fast moving objects):
F = Cdrag * V2
F = ρliquid * g * Volume