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            A driver makes a turn.

The inertial force prevents them from moving forward and cracking their skull.

This inertial force is fictitious, It seems real, but only because the observerā€™s frame of reference is rotating or accelerating

  1. The force of gravity is negligible

  2. The force of tension will head to the center

  3. The only time this system is undergoing UCM is when the force to keep the system up is enough to counteract the force of gravity

  4. The force of gravity would be 0

Top-Down View

Side(Rear) View

a

Acceleration points to center

v

a

Acceleration points to center

a

n

F

g

F

The x-component

nx

F

contributes to acceleration

The y-component

ny

F

counteracts

g

F

Velocity is tangent to the curve

v

If a car wants to make a turn, there is a certain velocity (lets call it v ) that a car needs to be at to successfully make the turn with UCM.

In these cases of UCM, friction does not need to act.

However, if the car moves quicker or slower than , Friction will have to act to assist in the turn.

ideal

v

ideal

ideal

v

assist

Friction

quicker or slower

needs to be at

If v > v

ideal

Centripetal Force is greater

greater

If youā€™re going faster, you will need to turn quicker to make the turn

Friction acts down the slope. It assists acceleration

If v < v

ideal

Centripetal Force is smaller

smaller

If youā€™re going slower, you will need to turn slower to make the turn

Friction acts up the slope. It combats acceleration

Friction

Friction

On a banked curve, an object does not need Friction to make a turn. This is because the curve is already on an incline

Instead, what allows the object to turn is the Normal Force

n

F

F

This is because the object is actually accelerating into the ground

accelerating into the ground

Net

F

=

nx

F

=

n

F

Īø

  • sin

Īø

Īø

nX

F

v > v

ideal

F

g

F

n

F

f

Īø

Īø

F

fy

F

fx

F

ny

F

nx

Horizontal:

F

net

=

F

fx

F

nx

ma =

F * Ī¼ * cosĪø

n

F * sinĪø

n

Īø

mv

F * Ī¼ * cosĪø

n

F * sinĪø

n

r

2

=

Vertical:

F

ny

=

F

g

F

fy

F * cosĪø

n

=

mg

F * Ī¼ * sinĪø

n

mg

=

F * Ī¼ * sinĪø

n

F * cosĪø

n

Lets divide the 2 equations

mv

r

2

mg

=

F * Ī¼ * cosĪø

n

F * sinĪø

n

F * Ī¼ * sinĪø

n

F * cosĪø

n

v

rg

2

=

Ī¼cosĪø + sinĪø

cosĪø - Ī¼sinĪø

v > v

ideal

F

g

F

f

Īø

F

fy

F

fx

Īø

Horizontal:

F

Net

=

F

nx

F

fx

mv

r

2

=

F * sinĪø

n

F * Ī¼ * cosĪø

n

Vertical:

F

ny

F

fy

=

F

g

F * cosĪø

n

F * Ī¼ * sinĪø

n

F

n

Īø

F

ny

F

nx

=

mg

Divide the 2

mv

r

2

mg

=

F * sinĪø

n

F * Ī¼ * cosĪø

n

F * cosĪø

n

F * Ī¼ * sinĪø

n

v

rg

2

=

sinĪø - Ī¼cosĪø

cosĪø + Ī¼sinĪø