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The Timpson Lyceum · University Physics I (2025)

Motion in Two or Three Dimensions – Lecture 3 (University Physics I)

Overview

This lecture extends one-dimensional kinematics to two- and three-dimensional motion, using vectors and the trick of splitting motion into independent components. It covers two headline applications: projectile motion (an object moving under gravity alone, which always traces a downward parabola) and uniform circular motion (motion around a circle at constant speed). Along the way it builds the angular language — radians, angular velocity, period, frequency — and derives centripetal acceleration. The recurring theme: a hard 2-D problem becomes two easy 1-D problems once you resolve it into perpendicular components.

Key Concepts

Projectiles. A projectile is an object on which the only force is gravity (air resistance ignored). Its motion stays in a single vertical plane, so it is a 2-D problem with ax=0a_x = 0 and ay=−ga_y = -g (g=9.8 m/s2g = 9.8\ \text{m/s}^2). Resolve the launch velocity by angle: v0x=v0cos⁡θv_{0x} = v_0\cos\theta and v0y=v0sin⁡θv_{0y} = v_0\sin\theta. The horizontal and vertical motions are then completely independent — constant velocity across, free fall up/down — and (taking the launch point as the origin):

x=(v0cos⁡θ) ty=(v0sin⁡θ) t−12gt2vx=v0cos⁡θvy=v0sin⁡θ−gt\begin{aligned} x &= (v_0\cos\theta)\,t \\ y &= (v_0\sin\theta)\,t - \tfrac{1}{2} g t^{2} \\ v_x &= v_0\cos\theta \\ v_y &= v_0\sin\theta - g t \end{aligned}

Trajectory and its two key results. Eliminating tt between the xx and yy equations gives yy as a quadratic in xx — the path is always a downward-opening parabola. At the peak the vertical velocity is zero (vy=0v_y = 0); using that and the symmetry of the parabola yields the maximum height HH and the horizontal range DD:

H=v02sin⁡2θ2gD=v02sin⁡2θg\begin{aligned} H &= \frac{v_0^{2}\sin^{2}\theta}{2g} \\ D &= \frac{v_0^{2}\sin 2\theta}{g} \end{aligned}

These pass the intuition check: more launch speed → higher and farther; more gravity → lower and shorter; height is greatest at θ=90∘\theta = 90^\circ (straight up), and range is greatest at θ=45∘\theta = 45^\circ (since sin⁡2θ\sin 2\theta peaks there).

The monkey-and-hunter problem. Aim a projectile directly at a target that drops the instant you fire. You always hit it — regardless of distance, launch angle, or launch speed — because the projectile and the target fall by the same 12gt2\tfrac{1}{2} g t^{2} in the same time, so gravity removes exactly the same amount from both. (The only caveat: the projectile must reach the target before hitting the ground.)

Radians and angular quantities. An angle in radians is arc length over radius, so it is dimensionless; the arc length for angle θ\theta is s=rθs = r\theta. Define angular displacement Δθ\Delta\theta, angular speed ω=Δθ/Δt\omega = \Delta\theta/\Delta t (rad/s), and angular acceleration α=Δω/Δt\alpha = \Delta\omega/\Delta t — the exact rotational analogues of xx, vv, aa. They connect to the linear quantities through the radius:

s=rθv=ωrarad=ω2r=v2r\begin{aligned} s &= r\theta \\ v &= \omega r \\ a_{\text{rad}} &= \omega^{2} r = \frac{v^{2}}{r} \end{aligned}

Period and frequency. The period TT is the time for one full revolution and the frequency ff is revolutions per second; they are reciprocals, with ff measured in hertz (s−1\text{s}^{-1}):

T=2πω,f=1TT = \frac{2\pi}{\omega}, \qquad f = \frac{1}{T}

Uniform circular motion. "Uniform" means α=0\alpha = 0, so ω\omega — and therefore the speed ∣v⃗∣=ωr|\vec v| = \omega r — is constant. The velocity is not constant, though: its direction is always changing. That changing direction is an acceleration directed radially inward (centripetal), arad=v2/ra_{\text{rad}} = v^{2}/r. Faster spin or a tighter circle means more centripetal acceleration.

Worked Example

A projectile launched at v0=20 m/sv_0 = 20\ \text{m/s}, angle θ=30∘\theta = 30^\circ above horizontal. Find its maximum height and horizontal range (g=9.8 m/s2g = 9.8\ \text{m/s}^2).

  1. Maximum height — apply the height result, then substitute:
H=v02sin⁡2θ2g=(20)2 sin⁡230∘2(9.8)≈5.1 m\begin{aligned} H &= \frac{v_0^{2}\sin^{2}\theta}{2g} \\ &= \frac{(20)^2\,\sin^{2}30^\circ}{2(9.8)} \approx 5.1\ \text{m} \end{aligned}
  1. Range — apply the range result, then substitute:
D=v02sin⁡2θg=(20)2 sin⁡60∘9.8≈35.3 m\begin{aligned} D &= \frac{v_0^{2}\sin 2\theta}{g} \\ &= \frac{(20)^2\,\sin 60^\circ}{9.8} \approx 35.3\ \text{m} \end{aligned}
  1. As a check, both grow with v0v_0 and shrink with gg, as expected; and had the launch angle been 45∘45^\circ, the range would have been at its maximum.

Summary