The centripetal force is the product of mass and centripetal acceleration, so $F_c = m \dfrac{v^2}{r}$.
Lesson 4 treated uniform circular motion on a flat road, where friction supplied the horizontal inward force. This lesson changes the geometry so the normal force itself can contribute that inward component. The prerequisite ideas are centripetal force, resolution of forces into perpendicular components, and Newton's second law. Lesson 6 then keeps the same centripetal structure but replaces the contact-force setting with gravitation.
The app surface keeps these relationships visible without turning the lesson into a dashboard. The main reading panel remains dense and printable, while the tutoring workflow lives in its own dedicated pane.
- Derive the ideal banking relation $ \tan\theta = \dfrac{v^2}{rg} $ from force components.
- Predict the direction of friction when the vehicle moves above or below the design speed.
- Transfer the same force geometry to a conical pendulum, including the radius relation $r = L\sin\theta$.
- Evaluate competing designs using quantitative evidence rather than descriptive commentary.
- Method Force diagram first, resolved equations second, algebraic reduction third.
- Units Convert km h$^{-1}$ to m s$^{-1}$ before substitution and retain units in prose.
- Reasoning Turn each numerical result into a physical claim about friction demand or robustness.
- Writing Finish with a judgement sentence that names the decisive evidence and the practical qualification.