Projectile Motion
Why a thrown ball traces a perfect parabola — and how to predict exactly where it lands.
The idea that makes projectiles easy
Watch a basketball sail toward the hoop. It feels like one smooth, curved motion — and it is. But here's the insight that makes projectiles simple: the horizontal and vertical motions do not affect each other.
Horizontally, nothing pushes the ball (we ignore air resistance), so it keeps a constant speed. Vertically, gravity pulls it down, speeding its fall and slowing its rise — exactly as if you had simply dropped it. Run both at once and the curve you get is a parabola.
Writing it as equations
Split the launch speed \(v_0\) at angle \(\theta\) into components, then apply constant-velocity motion horizontally and constant-acceleration motion (\(g \approx 9.8\,\text{m/s}^2\) downward) vertically:
The results worth knowing (and re-deriving)
From those two position equations you can pull out three headline quantities. None of them is worth memorizing blindly — each falls out of \(x(t)\) and \(y(t)\) in a line or two of algebra. Play with the simulation above and confirm each one for yourself:
- Use the range formula: \(R = \dfrac{v_0^2 \sin 2\theta}{g}\).
- Here \(v_0 = 20\), \(\theta = 30°\) so \(2\theta = 60°\), and \(\sin 60° \approx 0.866\).
- \(R = \dfrac{20^2 \times 0.866}{9.8} = \dfrac{400 \times 0.866}{9.8} = \dfrac{346.4}{9.8}\).
- Resolve the launch velocity: \(v_{0x} = 20\cos30° = 17.3\,\text{m/s}\) and \(v_{0y} = 20\sin30° = 10\,\text{m/s}\).
- The ball lands when \(y = 0\): \(v_{0y}t - \tfrac{1}{2}gt^2 = 0 \Rightarrow t\,(10 - 4.9\,t) = 0\).
- Discard \(t = 0\) (the launch): \(t = 10 / 4.9 = 2.04\,\text{s}\) — the time of flight.
- Range is just horizontal speed × time: \(x = v_{0x}\,t = 17.3 \times 2.04\).
Where you meet this in the real world
- Sport: the arc of a basketball, a golf drive, a long jump.
- Engineering: water from a fountain or fire hose, ballistics, the safe landing zone under a ski jump.
- Space: an orbit is really just a projectile falling so fast it keeps missing the Earth — the bridge to the Astrophysics module.
Check your understanding
- Horizontal and vertical motion are independent — solve each axis on its own.
- Position: x = v₀cosθ·t and y = v₀sinθ·t − ½gt². Combine them and y-vs-x is a parabola.
- On level ground: range R = v₀²sin2θ/g, max height H = v₀²sin²θ/2g, flight time t = 2v₀sinθ/g.
- Range is greatest at 45°; complementary angles (like 30° & 60°) share the same range.