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How do objects move when launched or turned by a force?

Analyse projectile motion and uniform circular motion using vectors and Newton's laws.

How to analyse projectiles by separating horizontal and vertical motion, and how a centripetal force keeps objects in uniform circular motion.

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What this dot point is asking

This dot point combines the kinematics of straight-line motion with Newton's laws to handle two of the most common exam scenarios: a launched projectile and an object turning in a circle.

Projectile motion

A projectile is any object moving only under gravity after launch, with air resistance ignored. The key idea is that the horizontal and vertical components of motion are completely independent and share only the time of flight.

Horizontally there is no force, so velocity is constant:

x=uxtx = u_x t

where ux=ucosθu_x = u\cos\theta is the horizontal launch component.

Vertically the only acceleration is gravity, g=9.8 m s2g = 9.8\ \text{m s}^{-2} downward, so the constant-acceleration equations apply:

vy=uygty=uyt12gt2v_y = u_y - g t \qquad y = u_y t - \tfrac{1}{2} g t^2

with uy=usinθu_y = u\sin\theta. At the highest point vy=0v_y = 0, which lets you find the time to the top and the maximum height. The trajectory is a parabola, and for level ground the path is symmetric: the launch speed equals the landing speed, and the launch angle equals the landing angle below the horizontal.

To find the resultant velocity at any instant, combine the components:

v=vx2+vy2tanϕ=vyvx.v = \sqrt{v_x^2 + v_y^2} \qquad \tan\phi = \frac{v_y}{v_x}.

Uniform circular motion

An object moving in a circle at constant speed is still accelerating because its velocity direction changes continually. This acceleration points toward the centre and is the centripetal acceleration:

ac=v2ra_c = \frac{v^2}{r}

By Newton's second law a net force must produce it, the centripetal force:

Fc=mv2rF_c = \frac{m v^2}{r}

This is not a new kind of force. It is whatever real force (tension, friction, gravity, the normal force, or a magnetic force) happens to point toward the centre. If you know the period TT for one revolution, the speed is the circumference divided by the period:

v=2πrT.v = \frac{2\pi r}{T}.

The centripetal force does no work on the object because it is always perpendicular to the velocity, which is why the speed stays constant even though the object accelerates.

Conical pendulums and banked turns

A favourite TCE scenario is an object swung in a horizontal circle on a string at an angle, or a vehicle on a banked or flat curve. The method is always the same: draw the forces, resolve into vertical and horizontal, set the vertical components to balance (no vertical acceleration) and the net horizontal force equal to mv2r\dfrac{mv^2}{r}. For a string at angle θ\theta from the vertical, dividing the horizontal equation by the vertical gives tanθ=v2rg\tan\theta = \dfrac{v^2}{rg}, which neatly eliminates the tension and the mass.

The link between the two halves of this dot point is the role of gravity. A projectile near the surface follows a parabola because gravity is effectively constant and vertical; a satellite follows a circle (or ellipse) because gravity always points toward the central mass and supplies the centripetal force. Newton's famous cannonball thought-experiment connects them: fire a projectile fast enough and its parabolic fall curves around the whole planet, becoming an orbit.

When you analyse circular motion in the exam, first identify which real force provides the centripetal force, then set that force equal to mv2r\dfrac{mv^2}{r} and solve. For a car on a flat curve it is friction; for a satellite it is gravity; for a charge in a magnetic field it is the magnetic force. Keeping the source force separate from the centripetal requirement is the clearest way to avoid confusion.

Exam-style practice questions

Practice questions written in the style of TASC exam questions on this dot point, with worked answer explainers. The year tag is the paper they imitate, not the source.

TCE 20244 marksA parent swings a child of mass 25 kg25\ \text{kg} in a horizontal circle by the arms, radius 1.3 m1.3\ \text{m}, with the arms held at 2020^\circ above the horizontal. Calculate the magnitude of the force on the child's arms and the tangential speed of the child.
Show worked answer →

Two forces act on the child: weight mgmg (down) and the arm force TT along the arms (2020^\circ above the horizontal). The vertical component of TT balances weight; the horizontal component provides the centripetal force.

Vertical: Tsin20=mgT\sin 20^\circ = mg, so T=mgsin20=(25)(9.81)0.342=717 NT = \dfrac{mg}{\sin 20^\circ} = \dfrac{(25)(9.81)}{0.342} = 717\ \text{N}.

Horizontal (centripetal): Tcos20=mv2rT\cos 20^\circ = \dfrac{mv^2}{r}, so mv2r=(717)(0.940)=674 N\dfrac{mv^2}{r} = (717)(0.940) = 674\ \text{N}, giving v2=(674)(1.3)25=35.0v^2 = \dfrac{(674)(1.3)}{25} = 35.0 and v=5.92 m s1v = 5.92\ \text{m s}^{-1}.

The tangential speed is about 5.9 m s15.9\ \text{m s}^{-1} and the arm force about 717 N717\ \text{N}. Markers want the vertical balance to find TT, then the horizontal component as the centripetal force.

TCE 20243 marksA cricket six has a range of 120 m120\ \text{m}, struck at 4040^\circ from ground level and landing at ground level. Using ucos40=120tu\cos 40^\circ = \dfrac{120}{t} and usin40=4.91tu\sin 40^\circ = 4.91t, calculate the initial speed uu of the ball.
Show worked answer →

Treat the projectile as independent horizontal and vertical motion. The two relations come from the range (horizontal) and the time of flight (the ball returns to the same height after time tt when usin40=12gt=4.91tu\sin 40^\circ = \tfrac12 gt = 4.91t).

From the first: t=120ucos40t = \dfrac{120}{u\cos 40^\circ}. Substitute into the second:

usin40=(4.91)(120)ucos40,u\sin 40^\circ = \frac{(4.91)(120)}{u\cos 40^\circ},

so u2sin40cos40=(4.91)(120)=589.2u^2 \sin 40^\circ \cos 40^\circ = (4.91)(120) = 589.2.
u2=589.2sin40cos40=589.20.4924=1196.6,u=34.6 m s1.u^2 = \frac{589.2}{\sin 40^\circ \cos 40^\circ} = \frac{589.2}{0.4924} = 1196.6, \quad u = 34.6\ \text{m s}^{-1}.

The ball leaves the bat at about 35 m s135\ \text{m s}^{-1}. Markers want elimination of tt between the two equations.

TCE 20193 marksA golf ball is hit at 140 km h1140\ \text{km h}^{-1} at 4040^\circ to the horizontal on flat ground (g=9.81 m s2g = 9.81\ \text{m s}^{-2}). Calculate the time the ball is above the ground, ignoring air resistance.
Show worked answer →

Convert the speed: 140 km h1=1403.6=38.9 m s1140\ \text{km h}^{-1} = \dfrac{140}{3.6} = 38.9\ \text{m s}^{-1}.

Vertical launch component: uy=38.9sin40=(38.9)(0.643)=25.0 m s1u_y = 38.9\sin 40^\circ = (38.9)(0.643) = 25.0\ \text{m s}^{-1} upwards.

Time to the top (where vy=0v_y = 0): tup=uyg=25.09.81=2.55 st_\text{up} = \dfrac{u_y}{g} = \dfrac{25.0}{9.81} = 2.55\ \text{s}.
Total flight =2tup=5.10 s= 2 t_\text{up} = 5.10\ \text{s}.

The ball is in the air for about 5.1 s5.1\ \text{s}. Markers want the vertical component, the time to apex, then doubling for the full symmetric flight.

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