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Reading a Whole Flight from One Launch

Irodov 1.29DifficultyDifficulty 3 of 5UniquenessUniqueness 3 of 5

Problem Irodov 1.29

A body is launched from ground level with initial speed v0v_0 at an angle α\alpha above the horizontal, under constant gravitational acceleration gg and negligible air drag. Find:

  1. the total time of flight τ\tau, until the body returns to launch height

  2. the maximum height hh and the horizontal range ll, and the angle α\alpha at which h=lh=l

  3. the trajectory equation y(x)y(x), with xx horizontal and yy vertical displacement from the launch point

  4. the radius of curvature of the trajectory at the launch point and at the highest point

The trajectory from launch to landing. v_0 leaves at angle α; the dashed droppers mark the peak height h and the range l.

The trajectory from launch to landing. v0\vect v_0 leaves at angle α\alpha; the dashed droppers mark the peak height hh and the range ll.

Given
  • v0v_0
  • α\alpha
  • gg
Find
(a) τ\tau, (b) hh, ll, and the α\alpha where h=lh=l, (c) y(x)y(x), (d) R1R_1 at launch, R2R_2 at the peak

Solution

Step 1Set up the components

With xx horizontal and yy vertical from the launch point, the horizontal velocity stays constant while gravity acts only along yy; both coordinates follow from one integration of constant acceleration.

x(t)=v0cos⁡α t,y(t)=v0sin⁡α t−g2t2(1)x(t)=v_0\cos\alpha\,t, \qquad y(t)=v_0\sin\alpha\,t-\frac{g}{2}t^2 \tag{1}
Step 2Flight time from the landing condition

The flight ends when yy returns to zero; factoring out tt isolates the nonzero root.

0=v0sin⁡α τ−g2τ20=τ(v0sin⁡α−g2τ)\begin{align*}0 &= v_0\sin\alpha\,\tau-\frac{g}{2}\tau^2 \\ 0 &= \tau\left(v_0\sin\alpha-\frac{g}{2}\tau\right)\end{align*}

τ=0\tau=0 is the launch instant; the landing is the other root.

τ=2v0sin⁡αg\tau = \dfrac{2v_0\sin\alpha}{g}
(2)
Step 3Peak height and range

The peak occurs at t=τ/2t=\tau/2, where y(t)y(t) is largest; the range is xx evaluated at the full flight time (2).

h=y ⁣(τ2)=v0sin⁡α⋅v0sin⁡αg−g2(v0sin⁡αg)2=v02sin⁡2αg−v02sin⁡2α2gl=x(τ)=v0cos⁡α⋅2v0sin⁡αg=2v02sin⁡αcos⁡αg\begin{align*}h &= y\!\left(\frac{\tau}{2}\right) \\ &= v_0\sin\alpha\cdot\frac{v_0\sin\alpha}{g}-\frac{g}{2}\left(\frac{v_0\sin\alpha}{g}\right)^2 \\ &= \frac{v_0^2\sin^2\alpha}{g}-\frac{v_0^2\sin^2\alpha}{2g} \\ l &= x(\tau) \\ &= v_0\cos\alpha\cdot\frac{2v_0\sin\alpha}{g} \\ &= \frac{2v_0^2\sin\alpha\cos\alpha}{g}\end{align*}

Collecting the two terms of hh over the common denominator 2g2g, and folding ll’s product of a sine and a cosine into the double angle sin⁡2α=2sin⁡αcos⁡α\sin2\alpha=2\sin\alpha\cos\alpha,

h=v02sin⁡2α2g,l=v02sin⁡2αgh=\dfrac{v_0^2\sin^2\alpha}{2g},\qquad l=\dfrac{v_0^2\sin2\alpha}{g}
(3)

Setting h=lh=l gives the angle at which the peak height equals the range.

v02sin⁡2α2g=v02sin⁡2αgsin⁡2α=2sin⁡2α=4sin⁡αcos⁡αsin⁡2αsin⁡αcos⁡α=4sin⁡αcos⁡αsin⁡αcos⁡αtan⁡α=4\begin{align*}\frac{v_0^2\sin^2\alpha}{2g} &= \frac{v_0^2\sin2\alpha}{g} \\ \sin^2\alpha &= 2\sin2\alpha \\ &= 4\sin\alpha\cos\alpha \\ \frac{\sin^2\alpha}{\sin\alpha\cos\alpha} &= \frac{4\sin\alpha\cos\alpha}{\sin\alpha\cos\alpha} \\ \tan\alpha &= 4\end{align*}
α=arctan⁡4≈76∘\alpha = \arctan4 \approx 76^\circ
(4)
Step 4Eliminate tt for the trajectory

Solving the horizontal law of (1) for tt and substituting it into the vertical law gives the path as a function of xx alone.

t=xv0cos⁡αy=v0sin⁡α⋅xv0cos⁡α−g2(xv0cos⁡α)2\begin{align*}t&=\frac{x}{v_0\cos\alpha} \\ y &= v_0\sin\alpha\cdot\frac{x}{v_0\cos\alpha}-\frac{g}{2}\left(\frac{x}{v_0\cos\alpha}\right)^2\end{align*}
y=xtan⁡α−g2v02cos⁡2αx2y = x\tan\alpha-\dfrac{g}{2v_0^2\cos^2\alpha}x^2
(5)
Step 5Curvature radius from the normal component of gravity

The curvature radius of any path satisfies the general relation below, where wnw_n is the component of acceleration perpendicular to the velocity; only gravity acts here, so wnw_n is gg resolved against the local flight direction.

R=v2wn(6)R = \frac{v^2}{w_n} \tag{6}

At launch the velocity makes angle α\alpha with the horizontal, so the component of g\vect g normal to v0\vect v_0 is gcos⁡αg\cos\alpha while v=v0v=v_0; at the peak the velocity is purely horizontal, so all of g\vect g is normal to it and v=v0cos⁡αv=v_0\cos\alpha.

wn(0)=gcos⁡α,v(0)=v0wn(τ/2)=g,v(τ/2)=v0cos⁡α\begin{align*}w_n(0) &= g\cos\alpha, & v(0) &= v_0 \\ w_n(\tau/2) &= g, & v(\tau/2) &= v_0\cos\alpha\end{align*}
R1=v02gcos⁡α,R2=v02cos⁡2αgR_1=\dfrac{v_0^2}{g\cos\alpha},\qquad R_2=\dfrac{v_0^2\cos^2\alpha}{g}
(7)
Check

At α=90∘\alpha=90^\circ (straight up), R1→∞R_1\to\infty: gravity is then purely tangential at launch, decelerating the body along a straight line with no curvature, exactly as (6) predicts. Also R2/R1=cos⁡3α≤1R_2/R_1=\cos^3\alpha\le1 always, consistent with the peak being the tightest turn on this trajectory.

Remark

R1R_1 and R2R_2 never need the flight time, the height or the range: the curvature radius depends only on the local velocity and the local normal acceleration, which is why the same R=v2/wnR=v^2/w_n reasoning carries over unchanged to circular motion, banked curves, or any other path once the normal acceleration is identified.