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Physics · Ch 3 — Motion in a Plane

Projectile Motion

3.9

Projectile Motion

Projectile Motion

When an object is thrown or projected into the air and continues in flight under the influence of gravity alone, it is called a projectile. A cricket ball, a football, a baseball, or even a stone thrown from a cliff — all are projectiles once they leave the thrower's hand and are acted upon only by gravity (we neglect air resistance throughout this discussion).

The key insight, first stated by Galileo in 1632, is that projectile motion is the combination of two independent motions happening simultaneously: a horizontal motion with constant velocity (no acceleration) and a vertical motion with constant acceleration due to gravity. These two components do not interfere with each other.

We set up our coordinate system with the x-axis horizontal and the y-axis vertical. The projectile is launched from the origin with an initial speed v0v_0 at an angle θ0\theta_0 measured from the positive x-axis. The acceleration is purely vertical and downward:

ax=0,ay=−ga_x = 0, \quad a_y = -g

The components of the initial velocity are:

v0x=v0cos⁡θ0,v0y=v0sin⁡θ0v_{0x} = v_0 \cos\theta_0, \quad v_{0y} = v_0 \sin\theta_0

Important

The independence of horizontal and vertical motions means we can treat the x-motion and y-motion as two separate one-dimensional problems. This is the central idea that makes analysing projectiles straightforward.


Position and Velocity at Any Time

Starting from the general equations for motion with constant acceleration (Eq. 3.34b from the previous section), and taking the initial position as the origin (x0=0,y0=0x_0 = 0, y_0 = 0), we get:

x=v0xt=(v0cos⁡θ0)tx = v_{0x} t = (v_0 \cos\theta_0) t

y=v0yt+12ayt2=(v0sin⁡θ0)t−12gt2y = v_{0y} t + \frac{1}{2} a_y t^2 = (v_0 \sin\theta_0) t - \frac{1}{2} g t^2

The velocity components at any time tt follow from the constant-acceleration velocity equations:

vx=v0x=v0cos⁡θ0v_x = v_{0x} = v_0 \cos\theta_0

vy=v0y+ayt=v0sin⁡θ0−gtv_y = v_{0y} + a_y t = v_0 \sin\theta_0 - g t

Notice that vxv_x never changes — the horizontal component of velocity remains constant throughout the flight. Only the vertical component changes, exactly as it would for an object in free fall.


Equation of the Path (Trajectory)

To find the shape of the path, we eliminate time tt between the expressions for xx and yy. From x=(v0cos⁡θ0)tx = (v_0 \cos\theta_0) t, we have:

t=xv0cos⁡θ0t = \frac{x}{v_0 \cos\theta_0}

Substitute this into y=(v0sin⁡θ0)t−12gt2y = (v_0 \sin\theta_0) t - \frac{1}{2} g t^2:

y=(v0sin⁡θ0)(xv0cos⁡θ0)−12g(xv0cos⁡θ0)2y = (v_0 \sin\theta_0) \left( \frac{x}{v_0 \cos\theta_0} \right) - \frac{1}{2} g \left( \frac{x}{v_0 \cos\theta_0} \right)^2

y=xtan⁡θ0−g2v02cos⁡2θ0x2y = x \tan\theta_0 - \frac{g}{2 v_0^2 \cos^2\theta_0} x^2

Since gg, θ0\theta_0, and v0v_0 are constants, this is of the form y=ax+bx2y = ax + bx^2, where a=tan⁡θ0a = \tan\theta_0 and b=−g2v02cos⁡2θ0b = -\frac{g}{2 v_0^2 \cos^2\theta_0}. This is the equation of a parabola. The path of a projectile is therefore a parabola.

Note

The negative sign on the x2x^2 term tells us the parabola opens downward — the projectile rises, reaches a peak, and then falls back to the ground.


Time of Maximum Height

At the highest point of the trajectory, the vertical velocity becomes zero for an instant. Let tmt_m be the time to reach maximum height. Setting vy=0v_y = 0:

v0sin⁡θ0−gtm=0v_0 \sin\theta_0 - g t_m = 0

tm=v0sin⁡θ0gt_m = \frac{v_0 \sin\theta_0}{g}


Time of Flight

The total time the projectile remains in the air, TfT_f, is found by setting y=0y = 0 (the projectile returns to its launch level):

0=(v0sin⁡θ0)Tf−12gTf20 = (v_0 \sin\theta_0) T_f - \frac{1}{2} g T_f^2

Factor out TfT_f:

Tf(v0sin⁡θ0−12gTf)=0T_f \left( v_0 \sin\theta_0 - \frac{1}{2} g T_f \right) = 0

The solution Tf=0T_f = 0 corresponds to the launch instant. The other solution gives:

Tf=2v0sin⁡θ0gT_f = \frac{2 v_0 \sin\theta_0}{g}

Notice that Tf=2tmT_f = 2 t_m — the time to go up equals the time to come down, as expected from the symmetry of the parabola.


Maximum Height

The maximum height hmh_m is the y-coordinate at time t=tmt = t_m. Substitute tm=v0sin⁡θ0gt_m = \frac{v_0 \sin\theta_0}{g} into the equation for yy:

hm=(v0sin⁡θ0)(v0sin⁡θ0g)−12g(v0sin⁡θ0g)2h_m = (v_0 \sin\theta_0) \left( \frac{v_0 \sin\theta_0}{g} \right) - \frac{1}{2} g \left( \frac{v_0 \sin\theta_0}{g} \right)^2

hm=v02sin⁡2θ0g−v02sin⁡2θ02gh_m = \frac{v_0^2 \sin^2\theta_0}{g} - \frac{v_0^2 \sin^2\theta_0}{2g}

hm=v02sin⁡2θ02gh_m = \frac{v_0^2 \sin^2\theta_0}{2g}

hm=v02sin⁡2θ02gh_m = \frac{v_0^2 \sin^2\theta_0}{2g}


Horizontal Range

The horizontal range RR is the distance travelled along the x-direction during the total time of flight TfT_f:

R=v0xTf=(v0cos⁡θ0)(2v0sin⁡θ0g)R = v_{0x} T_f = (v_0 \cos\theta_0) \left( \frac{2 v_0 \sin\theta_0}{g} \right)

Using the trigonometric identity 2sin⁡θ0cos⁡θ0=sin⁡2θ02 \sin\theta_0 \cos\theta_0 = \sin 2\theta_0:

R=v02sin⁡2θ0gR = \frac{v_0^2 \sin 2\theta_0}{g}

R=v02sin⁡2θ0gR = \frac{v_0^2 \sin 2\theta_0}{g}

Maximum Range

For a fixed launch speed v0v_0, the range is maximum when sin⁡2θ0\sin 2\theta_0 is maximum, i.e., when sin⁡2θ0=1\sin 2\theta_0 = 1. This occurs when 2θ0=90∘2\theta_0 = 90^\circ, or:

θ0=45∘\theta_0 = 45^\circ

The maximum possible horizontal range is therefore:

Rm=v02gR_m = \frac{v_0^2}{g} …

Figure 3.16Motion of an object projected with velocity vo at angle θo.
Fig. 3.16 — Motion of an object projected with velocity vo at angle θo.

Drawn by us to help you understand the concept clearly, and verified to make sure it's accurate. For exams, practice from your NCERT textbook's own diagram.

The figure is the standard launch diagram for projectile motion. It shows an xx–yy coordinate system with the origin OO at the point of projection. From OO, a curved parabolic path rises to a maximum height and then falls back to the xx-axis. The initial velocity vector v0\mathbf{v}_0 is drawn as an arrow from OO at an angle θ0\theta_0 above the positive xx-axis. Two perpendicular dashed arrows from the tail of v0\mathbf{v}_0 show its rectangular components: a horizontal component v0cos⁡θ0v_0\cos\theta_0 along the xx-axis and a vertical component v0sin⁡θ0v_0\sin\theta_0 along the yy-axis. A single downward arrow labelled a=−g j^\mathbf{a} = -g\,\hat{\mathbf{j}} is placed near the path, indicating that the only acceleration is constant gravity acting vertically downward.

The physical idea is that the motion separates cleanly into two independent parts. Horizontally, there is no acceleration, so the xx-component of velocity stays constant at v0cos⁡θ0v_0\cos\theta_0. Vertically, the acceleration is constant at −g-g, so the yy-component of velocity changes uniformly from its initial value v0sin⁡θ0v_0\sin\theta_0 to zero at the peak, then to negative values on the descent. The parabolic shape of the trajectory is the result of combining this uniform horizontal motion with uniformly accelerated vertical motion.

From this figure the textbook develops the core equations of projectile motion. The position at any time tt is given by

x(t)=(v0cos⁡θ0) t,y(t)=(v0sin⁡θ0) t−12gt2.x(t) = (v_0\cos\theta_0)\,t, \qquad y(t) = (v_0\sin\theta_0)\,t - \frac{1}{2}gt^2.

The velocity components are

vx=v0cos⁡θ0,vy=v0sin⁡θ0−gt.v_x = v_0\cos\theta_0, \qquad v_y = v_0\sin\theta_0 - gt.

The time of flight TT (when y=0y=0 again) is T=2v0sin⁡θ0gT = \frac{2v_0\sin\theta_0}{g}, the maximum height HH (when vy=0v_y=0) is H=v02sin⁡2θ02gH = \frac{v_0^2\sin^2\theta_0}{2g}, and the horizontal range RR is R=v02sin⁡2θ0gR = \frac{v_0^2\sin 2\theta_0}{g}. …

Figure 3.17The path of a projectile is a parabola.
Fig. 3.17 — The path of a projectile is a parabola.

Drawn by us to help you understand the concept clearly, and verified to make sure it's accurate. For exams, practice from your NCERT textbook's own diagram.

Fig. 3.17 is a single plot of the projectile’s path — the familiar curved arc — drawn on a standard xx–yy coordinate grid. The horizontal axis is labelled xx (range) and the vertical axis yy (height). The curve itself is a smooth, symmetric parabola that starts at the origin (0,0)(0,0), rises to a maximum height, then falls back to the xx-axis at the landing point.

The key visual elements are the velocity vectors drawn at three distinct moments: at launch, at the highest point, and just before landing. At the launch point, the initial velocity v0\mathbf{v}_0 is shown as an arrow making an angle θ0\theta_0 with the horizontal. This arrow is resolved into two perpendicular components: a horizontal component v0xi^v_{0x}\hat{\mathbf{i}} (pointing right along the xx-axis) and a vertical component v0yj^v_{0y}\hat{\mathbf{j}} (pointing upward). The figure makes clear that the horizontal component stays constant throughout the flight — the arrow for v0xv_{0x} is drawn with the same length at every stage.

At the apex of the parabola, the vertical velocity arrow disappears: only the horizontal component v0xi^v_{0x}\hat{\mathbf{i}} remains, because vy=0v_y = 0 at the highest point. On the descent, the vertical component reappears but now points downward, labelled −v0yj^-v_{0y}\hat{\mathbf{j}}. Just before landing, the velocity vector is again at an angle −θ0-\theta_0 below the horizontal — the same magnitude as the launch velocity but with the vertical component reversed.

Note

The symmetry of the figure is deliberate: the launch and landing velocities are mirror images across the horizontal axis. This reflects the fact that, in the absence of air resistance, the time to rise equals the time to fall, and the speed at any height is the same on the way up and on the way down.

The physical idea the figure teaches is that projectile motion is the superposition of two independent motions: uniform motion along xx (no acceleration) and uniformly accelerated motion along yy (acceleration =−g= -g). The parabolic shape emerges because yy is a quadratic function of xx.

The textbook develops the following central formulas from this figure. The initial velocity components are:

v0x=v0cos⁡θ0,v0y=v0sin⁡θ0.v_{0x} = v_0 \cos\theta_0, \qquad v_{0y} = v_0 \sin\theta_0.

At any time tt, the position coordinates are:

x=v0xt,y=v0yt−12gt2.x = v_{0x} t, \qquad y = v_{0y} t - \frac{1}{2} g t^2.

Eliminating tt gives the equation of the trajectory:

y=(tan⁡θ0) x−g2v02cos⁡2θ0 x2,y = (\tan\theta_0)\, x - \frac{g}{2 v_0^2 \cos^2\theta_0}\, x^2,

which is of the form y=ax−bx2y = ax - bx^2 — a parabola. Here gg is the acceleration due to gravity (9.8 m/s29.8\ \text{m/s}^2), v0v_0 is the initial speed, and θ0\theta_0 is the launch angle measured from the horizontal.

Watch out

A common mistake is to think the horizontal velocity changes. The figure’s constant-length v0xv_{0x} arrows are a visual reminder: vxv_x stays v0cos⁡θ0v_0\cos\theta_0 throughout the entire flight. Only the vertical component changes, and it does so at a constant rate gg. …