Forces and Motion

Newton’s Laws of Motion

First Law (Law of Inertia)

An object remains at rest or continues to move with uniform velocity unless acted upon by a net External force.

\sum \vec{F} = \vec{0} \implies \vec{v} = \mathrm{constant}

Inertia is the resistance of an object to changes in its state of motion. It is quantified by the Object’s mass: a larger mass implies greater inertia.

Second Law

The net force acting on an object equals the rate of change of its momentum:

\vec{F}_{\mathrm{net}} = \frac{d\vec{p}}{dt} = \frac{d(m\vec{v})}{dt}

For constant mass this reduces to:

\vec{F}_{\mathrm{net}} = m\vec{a}

The SI unit of force is the newton (N), where $1 \mathrm{ N} = 1 \mathrm{ kg}\cdot\mathrm{m/s}^2$ .

Third Law

If body A exerts a force on body B. Then body B exerts an equal and opposite force on body A:

\vec{F}_{AB} = -\vec{F}_{BA}

Action-reaction pairs always act on different bodies. They are equal in magnitude, opposite in Direction, and of the same type (both gravitational, both contact, etc.).

Worked Example 1

A block of mass $8 \mathrm{ kg}$ is pushed across a rough horizontal surface by a horizontal force of $50 \mathrm{ N}$ . The coefficient of kinetic friction is $0.3$ . Find the acceleration.

Solution

Normal reaction: $N = mg = 8 \times 9.81 = 78.48 \mathrm{ N}$

Friction: $f_k = \mu_k N = 0.3 \times 78.48 = 23.54 \mathrm{ N}$

a = \frac{F_{\mathrm{net}}}{m} = \frac{50 - 23.54}{8} = \frac{26.46}{8} = 3.31 \mathrm{ m/s}^2

Worked Example 2

Two blocks, $m_1 = 3 \mathrm{ kg}$ and $m_2 = 5 \mathrm{ kg}$ Are placed on a smooth horizontal Table and connected by a light inextensible string. A horizontal force of $24 \mathrm{ N}$ is applied To $m_2$ Pulling the system to the right. Find the acceleration and the tension in the string.

Solution

The two blocks move together with the same acceleration:

a = \frac{F}{m_1 + m_2} = \frac{24}{3 + 5} = \frac{24}{8} = 3.0 \mathrm{ m/s}^2

For block $m_1$ alone, the only horizontal force is the tension $T$ :

T = m_1 a = 3 \times 3.0 = 9.0 \mathrm{ N}

Worked Example 3

A lift (elevator) of mass $800 \mathrm{ kg}$ carries 3 passengers of total mass $210 \mathrm{ kg}$ . The lift accelerates upward at $1.5 \mathrm{ m/s}^2$ for the first 3 seconds. Find the tension in the cable during this acceleration and the distance travelled.

Solution

Total mass: $m = 800 + 210 = 1010 \mathrm{ kg}$

Applying Newton’s second law upward: $T - mg = ma$

T = m(g + a) = 1010(9.81 + 1.5) = 1010 \times 11.31 = 11423 \mathrm{ N}

Distance: $s = ut + \frac{1}{2}at^2 = 0 + \frac{1}{2}(1.5)(9) = 6.75 \mathrm{ m}$

Friction

Static and Kinetic Friction

Type	Symbol	Condition	Magnitude
Static	$f_s$	No relative motion	$0 \leqslant f_s \leqslant \mu_s N$
Kinetic	$f_k$	Surfaces sliding	$f_k = \mu_k N$

The coefficient of static friction $\mu_s$ is always greater than or equal to the coefficient of Kinetic friction $\mu_k$ :

\mu_s \geqslant \mu_k

Static friction adjusts its magnitude to match the applied force, up to a maximum of $\mu_s N$ . Once the applied force exceeds this maximum, the object begins to slide, and kinetic friction takes over.

Inclined Planes

For an object on an inclined plane at angle $\theta$ to the horizontal:

Component of weight parallel to the plane: $mg\sin\theta$
Component of weight perpendicular to the plane: $mg\cos\theta$
Normal reaction: $N = mg\cos\theta$
Friction (if sliding): $f = \mu mg\cos\theta$

The object slides down the plane when $mg\sin\theta \gt \mu_s mg\cos\theta$ I.e.:

\tan\theta \gt \mu_s

Worked Example 3

A $5 \mathrm{ kg}$ block rests on a rough plane inclined at $35^\circ$ . The block is on the verge of Sliding. Find the coefficient of static friction.

Solution

At the point of sliding, $mg\sin\theta = \mu_s mg\cos\theta$ :

\mu_s = \tan 35^\circ = 0.700

Worked Example 4

A $10 \mathrm{ kg}$ block sits on a rough horizontal surface with $\mu_s = 0.4$ and $\mu_k = 0.3$ . A force of $30 \mathrm{ N}$ is applied at $30^\circ$ above the horizontal. Does the Block move? If so, find its acceleration.

Solution

Resolve the applied force:

F_x = 30\cos 30^\circ = 25.98 \mathrm{ N}, \quad F_y = 30\sin 30^\circ = 15.0 \mathrm{ N}

Normal reaction: $N = mg - F_y = 10 \times 9.81 - 15.0 = 98.1 - 15.0 = 83.1 \mathrm{ N}$

Maximum static friction: $f_{s,\max} = \mu_s N = 0.4 \times 83.1 = 33.2 \mathrm{ N}$

Since $F_x = 25.98 \mathrm{ N} \lt 33.2 \mathrm{ N}$ The block does not move.

Momentum and Impulse

Linear Momentum

\vec{p} = m\vec{v}

Momentum is a vector quantity with SI unit $\mathrm{ kg\, m/s}$ .

Conservation of Momentum

For a system of objects with no external net force:

\sum \vec{p}_{\mathrm{initial}} = \sum \vec{p}_{\mathrm{final}}

m_1 \vec{u}_1 + m_2 \vec{u}_2 = m_1 \vec{v}_1 + m_2 \vec{v}_2

Impulse

\vec{J} = \vec{F}\,\Delta t = \Delta \vec{p}

Impulse equals the change in momentum. It is also the area under a force-time graph. The SI unit is $\mathrm{ N\, s}$ .

Collisions

Type	Momentum	Kinetic Energy
Elastic	Conserved	Conserved
Inelastic	Conserved	Not conserved
Perfectly inelastic	Conserved	Maximum loss (objects stick)

Worked Example 5

A $0.2 \mathrm{ kg}$ ball travelling at $15 \mathrm{ m/s}$ strikes a wall and rebounds at $10 \mathrm{ m/s}$ along the same line. Contact time is $0.02 \mathrm{ s}$ . Find the average force.

Solution

Taking the initial direction as positive:

\Delta p = m(v - u) = 0.2(-10 - 15) = 0.2(-25) = -5.0 \mathrm{ kg\, m/s}

F = \frac{\Delta p}{\Delta t} = \frac{-5.0}{0.02} = -250 \mathrm{ N}

The magnitude of the average force is $250 \mathrm{ N}$ Directed away from the wall.

Worked Example 6

A $3 \mathrm{ kg}$ trolley moving at $4 \mathrm{ m/s}$ collides with a stationary $5 \mathrm{ kg}$ Trolley and they stick together. Find the velocity after the collision and the kinetic energy lost.

Solution

By conservation of momentum:

m_1 u_1 + m_2 u_2 = (m_1 + m_2)v

3 \times 4 + 5 \times 0 = (3 + 5)v \implies 12 = 8v \implies v = 1.5 \mathrm{ m/s}

Initial KE: $E_{k,i} = \frac{1}{2}(3)(4^2) = 24.0 \mathrm{ J}$

Final KE: $E_{k,f} = \frac{1}{2}(8)(1.5^2) = 9.0 \mathrm{ J}$

Energy lost: $\Delta E_k = 24.0 - 9.0 = 15.0 \mathrm{ J}$

Worked Example 7

A $0.05 \mathrm{ kg}$ bullet travelling at $400 \mathrm{ m/s}$ embeds itself in a $2 \mathrm{ kg}$ wooden block at rest on a smooth surface. Find the velocity of the block Immediately after impact.

Solution

By conservation of momentum (perfectly inelastic collision):

m_1 u_1 + m_2 u_2 = (m_1 + m_2)v

0.05 \times 400 + 2 \times 0 = (0.05 + 2)v

20 = 2.05v \implies v = 9.76 \mathrm{ m/s}

Projectile Motion

Analysis by Components

For a projectile launched with speed $u$ at angle $\theta$ above the horizontal:

Quantity	Horizontal	Vertical
Acceleration	$0$	$-g$
Velocity	$u_x = u\cos\theta$ (constant)	$u_y = u\sin\theta - gt$
Displacement	$x = u\cos\theta\cdot t$	$y = u\sin\theta\cdot t - \frac{1}{2}gt^2$

Key Results

Time of flight (landing at same height):

T = \frac{2u\sin\theta}{g}

Maximum height:

H = \frac{u^2\sin^2\theta}{2g}

Horizontal range:

R = \frac{u^2\sin 2\theta}{g}

Maximum range occurs at $\theta = 45^\circ$ Giving $R_{\max} = u^2/g$ .

Complementary angles ( $\theta$ and $90^\circ - \theta$ ) produce the same range.

Explore how launch angle and initial speed affect the trajectory.

Worked Example 7

A ball is thrown from ground level with speed $20 \mathrm{ m/s}$ at $50^\circ$ above the horizontal. Find the range and maximum height.

Solution

R = \frac{20^2 \sin 100^\circ}{9.81} = \frac{400 \times 0.9848}{9.81} = 40.2 \mathrm{ m}

H = \frac{20^2 \sin^2 50^\circ}{2 \times 9.81} = \frac{400 \times 0.5868}{19.62} = 11.97 \mathrm{ m}

Circular Motion

Angular Quantities

Quantity	Symbol	SI Unit	Relation
Angular displacement	$\theta$	rad	$\theta = s/r$
Angular velocity	$\omega$	rad/s	$\omega = d\theta/dt$
Period	$T$	s	$T = 2\pi/\omega$
Frequency	$f$	Hz	$f = 1/T = \omega/(2\pi)$

Linear-angular relation: $v = r\omega$ , $a = r\alpha$

Centripetal Acceleration and Force

An object moving at constant speed $v$ in a circle of radius $r$ has centripetal acceleration:

a_c = \frac{v^2}{r} = \omega^2 r = \frac{4\pi^2 r}{T^2}

Directed towards the centre of the circle. The required centripetal force is:

F_c = \frac{mv^2}{r} = m\omega^2 r

Vertical Circular Motion

For an object on a string in vertical circular motion, speed varies because gravity does work. At the top of the circle:

T + mg = \frac{mv_{\mathrm{top}}^2}{r}

At the bottom:

T - mg = \frac{mv_{\mathrm{bottom}}^2}{r}

For the object to complete the full circle, the string must remain taut at the top ( $T \geqslant 0$ ):

v_{\mathrm{top}} \geqslant \sqrt{gr}

Worked Example 8

A car of mass $1200 \mathrm{ kg}$ travels around a flat curve of radius $60 \mathrm{ m}$ at $15 \mathrm{ m/s}$ . Find the minimum coefficient of friction required.

Solution

F_c = \frac{mv^2}{r} = \frac{1200 \times 15^2}{60} = \frac{1200 \times 225}{60} = 4500 \mathrm{ N}

The centripetal force is provided by friction: $F_c = \mu_s mg$

\mu_s = \frac{F_c}{mg} = \frac{4500}{1200 \times 9.81} = \frac{4500}{11772} = 0.382

Worked Example 9

A $0.5 \mathrm{ kg}$ ball is attached to a string of length $0.8 \mathrm{ m}$ and whirled in a Vertical circle. Find the minimum speed at the lowest point for the ball to complete the full circle.

Solution

For the ball to complete the full circle, the speed at the top must satisfy $v_{\mathrm{top}} \geqslant \sqrt{gr}$ .

Using energy conservation between the bottom and top:

\frac{1}{2}mv_{\mathrm{bottom}}^2 = \frac{1}{2}mv_{\mathrm{top}}^2 + mg(2r)

Setting $v_{\mathrm{top}} = \sqrt{gr}$ :

\frac{1}{2}mv_{\mathrm{bottom}}^2 = \frac{1}{2}m(gr) + 2mgr = \frac{5}{2}mgr

v_{\mathrm{bottom}} = \sqrt{5gr} = \sqrt{5 \times 9.81 \times 0.8} = \sqrt{39.24} = 6.26 \mathrm{ m/s}

Gravitation

Newton’s Law of Universal Gravitation

F = \frac{Gm_1 m_2}{r^2}

Where $G = 6.67 \times 10^{-11} \mathrm{ N\, m}^2\,\mathrm{ kg}^{-2}$ .

Gravitational Field Strength

g = \frac{F}{m} = \frac{GM}{r^2}

Near the Earth’s surface, $g \approx 9.81 \mathrm{ N/kg}$ (equivalent to $\mathrm{ m/s}^2$ ).

Gravitational Potential Energy

For two masses separated by distance $r$ :

E_p = -\frac{GMm}{r}

The negative sign reflects the convention that $E_p = 0$ at infinite separation. Work must be done against gravity to increase the separation.

Orbital Motion

For a satellite of mass $m$ orbiting a central body of mass $M$ at radius $r$ :

\frac{GMm}{r^2} = \frac{mv^2}{r} \implies v = \sqrt{\frac{GM}{r}}

T = \frac{2\pi r}{v} = 2\pi\sqrt{\frac{r^3}{GM}}

This is Kepler’s third law: $T^2 \propto r^3$ .

Visualise how orbital speed and period depend on the distance from the central body.

Worked Example 10

Find the orbital speed of a satellite orbiting the Earth at a height of $400 \mathrm{ km}$ . (Earth Radius $R_E = 6.37 \times 10^6 \mathrm{ m}$ Earth mass $M_E = 5.97 \times 10^{24} \mathrm{ kg}$ )

Solution

r = R_E + 400 \times 10^3 = 6.77 \times 10^6 \mathrm{ m}

v = \sqrt{\frac{GM_E}{r}} = \sqrt{\frac{6.67 \times 10^{-11} \times 5.97 \times 10^{24}}{6.77 \times 10^6}} = \sqrt{5.88 \times 10^7} = 7668 \mathrm{ m/s}

Common Pitfalls

Confusing action-reaction pairs with balanced forces. Newton’s third law pairs act on different objects; balanced forces act on the same object.
Forgetting that friction opposes relative motion, not necessarily the direction of the applied force.
Using $\mu_s N$ for kinetic friction or $\mu_k N$ for static friction. They are different.
In projectile motion, treating horizontal and vertical components as coupled. They share only the common variable $t$ .
Adding centripetal force as an extra force on a free body diagram. Centripetal force is the name given to the net inward force, not an additional force.

Summary Table

Topic	Key Formula	Key Concept
Newton’s Second Law	$F = ma$	Net force causes acceleration
Static friction	$f_s \leqslant \mu_s N$	Adjusts to match applied force
Kinetic friction	$f_k = \mu_k N$	Constant during sliding
Momentum	$p = mv$	Vector quantity
Impulse	$J = F\Delta t = \Delta p$	Area under F-t graph
Projectile range	$R = u^2\sin 2\theta/g$	Maximum at $45^\circ$
Centripetal force	$F_c = mv^2/r$	Net force towards centre
Gravitation	$F = Gm_1 m_2/r^2$	Inverse square law
Orbital speed	$v = \sqrt{GM/r}$	Balances gravity

Problem Set

Problem 1. A $6 \mathrm{ kg}$ block on a smooth horizontal table is connected by a light Inextensible string over a smooth pulley to a $4 \mathrm{ kg}$ block hanging freely. Find the Acceleration of the system and the tension in the string.

Solution

For the $4 \mathrm{ kg}$ block (taking downward as positive): $4g - T = 4a$

For the $6 \mathrm{ kg}$ block: $T = 6a$

Adding: $4g = 10a \implies a = \frac{4 \times 9.81}{10} = 3.92 \mathrm{ m/s}^2$

T = 6 \times 3.92 = 23.5 \mathrm{ N}

If you get this wrong, revise: Newton’s Laws of Motion / Second Law

Problem 2. A $3 \mathrm{ kg}$ block is placed on a rough inclined plane at $30^\circ$ . The coefficient of static friction is $0.35$ . Does the block slide? If it does, find the Acceleration ( $\mu_k = 0.25$ ).

Solution

Check: $\tan 30^\circ = 0.577 \gt \mu_s = 0.35$ So the block slides.

a = g(\sin\theta - \mu_k\cos\theta) = 9.81(0.5 - 0.25 \times 0.866) = 9.81(0.5 - 0.217) = 9.81 \times 0.283 = 2.78 \mathrm{ m/s}^2

If you get this wrong, revise: Friction / Inclined Planes

Problem 3. A $2 \mathrm{ kg}$ object moving at $6 \mathrm{ m/s}$ collides elastically with a $4 \mathrm{ kg}$ object at rest. Find the velocities after collision.

Solution

Conservation of momentum: $2(6) + 4(0) = 2v_1 + 4v_2 \implies 12 = 2v_1 + 4v_2 \quad (1)$

Conservation of KE: $\frac{1}{2}(2)(36) = \frac{1}{2}(2)v_1^2 + \frac{1}{2}(4)v_2^2 \implies 36 = v_1^2 + 2v_2^2 \quad (2)$

From (1): $v_1 = 6 - 2v_2$ . Substituting into (2):

36 = (6 - 2v_2)^2 + 2v_2^2 = 36 - 24v_2 + 4v_2^2 + 2v_2^2 = 36 - 24v_2 + 6v_2^2

6v_2^2 - 24v_2 = 0 \implies 6v_2(v_2 - 4) = 0

$v_2 = 0$ (original) or $v_2 = 4 \mathrm{ m/s}$ . Therefore $v_1 = 6 - 8 = -2 \mathrm{ m/s}$ .

The $2 \mathrm{ kg}$ object rebounds at $2 \mathrm{ m/s}$ ; the $4 \mathrm{ kg}$ object moves forward at $4 \mathrm{ m/s}$ .

If you get this wrong, revise: Momentum and Impulse / Collisions

Problem 4. A $150 \mathrm{ g}$ cricket ball is hit by a bat. The force-time graph is a Triangle with peak force $600 \mathrm{ N}$ and contact time $0.005 \mathrm{ s}$ . Find the Impulse and the speed of the ball after impact (initially at rest).

Solution

Impulse = area under F-t graph $= \frac{1}{2} \times 600 \times 0.005 = 1.5 \mathrm{ N\, s}$

J = \Delta p = mv \implies v = \frac{J}{m} = \frac{1.5}{0.150} = 10.0 \mathrm{ m/s}

If you get this wrong, revise: Momentum and Impulse / Impulse

Problem 5. A projectile is launched at $25 \mathrm{ m/s}$ from the edge of a cliff $80 \mathrm{ m}$ high at $40^\circ$ above the horizontal. Find the horizontal distance from the Cliff edge where it lands.

Solution

Vertical: $y = u_y t + \frac{1}{2}at^2$ Where $u_y = 25\sin 40^\circ = 16.07 \mathrm{ m/s}$

-80 = 16.07t - 4.905t^2 \implies 4.905t^2 - 16.07t - 80 = 0

t = \frac{16.07 \pm \sqrt{258.2 + 1569.6}}{9.81} = \frac{16.07 \pm \sqrt{1827.8}}{9.81} = \frac{16.07 + 42.76}{9.81} = 5.99 \mathrm{ s}

Horizontal distance: $d = u_x t = 25\cos 40^\circ \times 5.99 = 19.15 \times 5.99 = 114.7 \mathrm{ m}$

If you get this wrong, revise: Projectile Motion / Analysis by Components

Problem 6. A stone is tied to a string of length $1.2 \mathrm{ m}$ and whirled in a horizontal Circle. The string breaks when the tension reaches $50 \mathrm{ N}$ . The stone has mass $0.4 \mathrm{ kg}$ . Find the maximum speed before the string breaks.

Solution

The tension provides the centripetal force: $T = \frac{mv^2}{r}$

v = \sqrt{\frac{Tr}{m}} = \sqrt{\frac{50 \times 1.2}{0.4}} = \sqrt{150} = 12.2 \mathrm{ m/s}

If you get this wrong, revise: Circular Motion / Centripetal Acceleration and Force

Problem 7. A satellite orbits the Earth at a height of $600 \mathrm{ km}$ . Find the orbital Period and the gravitational field strength at that altitude.

Solution

r = 6.37 \times 10^6 + 600 \times 10^3 = 6.97 \times 10^6 \mathrm{ m}

g = \frac{GM_E}{r^2} = \frac{6.67 \times 10^{-11} \times 5.97 \times 10^{24}}{(6.97 \times 10^6)^2} = \frac{3.98 \times 10^{14}}{4.86 \times 10^{13}} = 8.19 \mathrm{ N/kg}

T = 2\pi\sqrt{\frac{r^3}{GM_E}} = 2\pi\sqrt{\frac{(6.97 \times 10^6)^3}{6.67 \times 10^{-11} \times 5.97 \times 10^{24}}} = 2\pi\sqrt{\frac{3.385 \times 10^{20}}{3.982 \times 10^{14}}} = 2\pi\sqrt{850300} = 2\pi \times 922.1 = 5794 \mathrm{ s} = 96.6 \mathrm{ minutes}

If you get this wrong, revise: Gravitation / Orbital Motion

Problem 8. A $4 \mathrm{ kg}$ block slides down a rough incline of length $6 \mathrm{ m}$ at $30^\circ$ to the horizontal. The coefficient of kinetic friction is $0.25$ . Find the speed at the Bottom if the block starts from rest.

Solution

Net force down the plane: $F = mg\sin 30^\circ - \mu_k mg\cos 30^\circ$

F = 4 \times 9.81 \times 0.5 - 0.25 \times 4 \times 9.81 \times 0.866 = 19.62 - 8.50 = 11.12 \mathrm{ N}

a = \frac{F}{m} = \frac{11.12}{4} = 2.78 \mathrm{ m/s}^2

v = \sqrt{2as} = \sqrt{2 \times 2.78 \times 6} = \sqrt{33.36} = 5.78 \mathrm{ m/s}

If you get this wrong, revise: Friction / Inclined Planes and Newton’s Second Law

Problem 9. A $1.5 \mathrm{ kg}$ ball on a string of length $0.5 \mathrm{ m}$ is swung in a Vertical circle. At the lowest point, the tension is $45 \mathrm{ N}$ . Find the speed at the Lowest point and the speed at the highest point.

Solution

At the lowest point: $T - mg = \frac{mv^2}{r}$

45 - 1.5 \times 9.81 = \frac{1.5 v_{\mathrm{bottom}}^2}{0.5} \implies 45 - 14.7 = 3 v_{\mathrm{bottom}}^2

v_{\mathrm{bottom}}^2 = \frac{30.3}{3} = 10.1 \implies v_{\mathrm{bottom}} = 3.18 \mathrm{ m/s}

Energy conservation between bottom and top:

\frac{1}{2}mv_{\mathrm{bottom}}^2 = \frac{1}{2}mv_{\mathrm{top}}^2 + mg(2r)

10.1 = v_{\mathrm{top}}^2 + 2 \times 9.81 \times 1.0 = v_{\mathrm{top}}^2 + 19.62

v_{\mathrm{top}}^2 = -9.52

The result is negative, meaning the ball does not reach the top of the circle. The speed is Insufficient.

If you get this wrong, revise: Circular Motion / Vertical Circular Motion

Problem 10. Two astronauts of masses $80 \mathrm{ kg}$ and $60 \mathrm{ kg}$ are initially at Rest in deep space, connected by a light rope. They push off each other and the $80 \mathrm{ kg}$ Astronaut moves away at $0.5 \mathrm{ m/s}$ . Find the velocity of the $60 \mathrm{ kg}$ astronaut and the distance between them after 5 seconds.

Solution

By conservation of momentum (initially at rest, total momentum = 0):

80 \times 0.5 + 60 \times v_2 = 0 \implies v_2 = -\frac{40}{60} = -0.667 \mathrm{ m/s}

The $60 \mathrm{ kg}$ astronaut moves at $0.667 \mathrm{ m/s}$ in the opposite direction.

Relative speed $= 0.5 + 0.667 = 1.167 \mathrm{ m/s}$

\mathrm{Distance\ after\ 5\ s} = 1.167 \times 5 = 5.83 \mathrm{ m}

If you get this wrong, revise: Momentum and Impulse / Conservation of Momentum

For the A-Level treatment of this topic, see Dynamics.

Diagnostic Test Ready to test your understanding of Forces and Motion? The contains the hardest questions

within the DSE specification for this topic, each with a full worked solution.

Unit tests probe edge cases and common misconceptions. Integration tests combine Forces and Motion with other physics topics to test synthesis under exam conditions.

Derivations

Derivation: Centripetal Acceleration

Consider an object moving at constant speed $v$ in a circle of radius $r$ . In a small time $\Delta t$ It moves from point A to point B, subtending a small angle $\Delta\theta$ at the Centre.

The change in velocity is directed towards the centre (radially inward). For small angles:

\Delta v \approx v \cdot \Delta\theta = v \cdot \frac{v\Delta t}{r} = \frac{v^2 \Delta t}{r}

The centripetal acceleration is:

a_c = \frac{\Delta v}{\Delta t} = \frac{v^2}{r}

In terms of angular velocity ( $v = r\omega$ ):

a_c = \frac{(r\omega)^2}{r} = r\omega^2 = \frac{4\pi^2 r}{T^2}

This acceleration is always directed towards the centre of the circle and is perpendicular to the Velocity (which is tangential). Since the force is perpendicular to the velocity, the magnetic Force does no work and the speed remains constant.

Derivation: Escape Velocity

For an object to escape from the surface of a planet of mass $M$ and radius $R$ Its total energy (kinetic + gravitational potential) at infinity must be at least zero.

At the surface: $E_{\mathrm{total}} = \frac{1}{2}mv_e^2 - \frac{GMm}{R}$

At infinity: $E_{\mathrm{total}} = 0$ (just barely escaping)

\frac{1}{2}mv_e^2 = \frac{GMm}{R}

v_e = \sqrt{\frac{2GM}{R}}

Derivation: Orbital Speed and Period

For a satellite in circular orbit at radius $r$ around a central body of mass $M$ The Gravitational force provides the centripetal force:

\frac{GMm}{r^2} = \frac{mv^2}{r}

v = \sqrt{\frac{GM}{r}}

The orbital period is:

T = \frac{2\pi r}{v} = \frac{2\pi r}{\sqrt{GM/r}} = 2\pi\sqrt{\frac{r^3}{GM}}

Squaring both sides: $T^2 = \frac{4\pi^2}{GM}r^3$ Which is Kepler’s third law ( $T^2 \propto r^3$ ).

Derivation: Range of a Projectile

For a projectile launched from ground level with speed $u$ at angle $\theta$ :

Horizontal: $x = u\cos\theta \cdot t$

Vertical at landing ( $y = 0$ ): $0 = u\sin\theta \cdot t - \frac{1}{2}gt^2 \implies t = \frac{2u\sin\theta}{g}$

Substituting: $R = u\cos\theta \cdot \frac{2u\sin\theta}{g} = \frac{u^2 \cdot 2\sin\theta\cos\theta}{g} = \frac{u^2\sin 2\theta}{g}$

Maximum range when $\sin 2\theta = 1$ I.e., $\theta = 45^\circ$ : $R_{\max} = u^2/g$ .

Experimental Methods

Determining Acceleration Due to Gravity Using a Free-Fall Apparatus

Apparatus: An electromagnetic release mechanism, a metal ball, a trapdoor, an electronic Timer, and a metre rule.

Procedure:

Measure the height $h$ from the bottom of the ball to the trapdoor.
Release the ball electromagnetically; the timer starts.
The ball hits the trapdoor, stopping the timer. Record the time $t$ .
Repeat for several heights.
Plot $h$ (y-axis) versus $t^2$ (x-axis).
From $h = \frac{1}{2}gt^2$ : gradient $= g/2$ So $g = 2 \times \mathrm{gradient}$ .

Sources of error:

Reaction time of the timer mechanism (minimised by using electronic timing).
Air resistance on the ball (use a dense, small ball to minimise).
Measurement of height $h$ (measure from the bottom of the ball, not the centre).

Improvements: Repeat each measurement multiple times and average. Use a heavier ball to reduce Air resistance effects.

Verifying Newton’s Second Law Using a Trolley on a Ramp

Apparatus: A trolley on a horizontal track, light gates, a set of slotted masses, a string Over a pulley, and a data logger.

Procedure:

Attach a string to the trolley, passing over a pulley at the edge of the track, with a hanging mass $m$ providing the accelerating force.
Measure the acceleration $a$ of the trolley using the light gates for different values of the total mass ( $m + M$ Where $M$ is the trolley mass) while keeping the accelerating force $mg$ constant.
Plot $a$ (y-axis) versus $1/(m + M)$ (x-axis). A straight line through the origin confirms $a \propto 1/(\mathrm{total\ mass})$ .
Alternatively, keep the total mass constant and vary the hanging mass. Plot $a$ versus $F = mg$ . A straight line through the origin confirms $a \propto F$ .

Precautions:

Compensate for friction by tilting the track slightly so the trolley moves at constant speed with no hanging mass.
Ensure the string is parallel to the track.
Use a light string and low-friction pulley.

Measuring the Coefficient of Friction on an Inclined Plane

Apparatus: An inclined plane, a block, a protractor, and a set of masses.

Procedure:

Place the block on the inclined plane and gradually increase the angle.
Record the angle $\theta_c$ at which the block just begins to slide.
At this critical angle: $\tan\theta_c = \mu_s$ .
Repeat several times and average.
For the coefficient of kinetic friction, measure the acceleration $a$ of the block sliding down the plane: $a = g(\sin\theta - \mu_k\cos\theta)$ So $\mu_k = \tan\theta - a/(g\cos\theta)$ .

Data Analysis and Uncertainty

Uncertainty in Acceleration Calculations

When determining $g$ from $h = \frac{1}{2}gt^2$ :

g = \frac{2h}{t^2}

\frac{\Delta g}{g} = \sqrt{\left(\frac{\Delta h}{h}\right)^2 + \left(2\frac{\Delta t}{t}\right)^2}

The time measurement dominates the uncertainty due to the factor of 2.

Example: $h = (1.00 \pm 0.01) \mathrm{ m}$ , $t = (0.450 \pm 0.005) \mathrm{ s}$ :

g = \frac{2 \times 1.00}{(0.450)^2} = \frac{2.00}{0.2025} = 9.88 \mathrm{ m/s}^2

\frac{\Delta g}{g} = \sqrt{(0.01)^2 + (2 \times 0.0111)^2} = \sqrt{0.0001 + 0.000493} = \sqrt{0.000593} = 0.0244 = 2.4\%

\Delta g = 0.024 \times 9.88 = 0.24 \mathrm{ m/s}^2

g = (9.9 \pm 0.2) \mathrm{ m/s}^2

Linearising Projectile Motion Data

To verify $R = u^2\sin 2\theta / g$ at constant launch speed:

Plot $R$ (y-axis) versus $\sin 2\theta$ (x-axis).
A straight line through the origin confirms the relationship.
The gradient equals $u^2/g$ .

Additional Worked Examples

Worked Example 11

A $3.0 \mathrm{ kg}$ block is pushed against a spring of spring constant $300 \mathrm{ N/m}$ Compressing it by $0.10 \mathrm{ m}$ . The block is released and moves across a rough horizontal Surface with $\mu_k = 0.2$ . How far does the block travel before coming to rest?

Solution

Energy stored in spring: $E_p = \frac{1}{2}(300)(0.10)^2 = 1.5 \mathrm{ J}$

This energy is dissipated by friction: $E_p = f_k \times d = \mu_k mg \times d$

1.5 = 0.2 \times 3.0 \times 9.81 \times d = 5.886d

d = \frac{1.5}{5.886} = 0.255 \mathrm{ m}

Worked Example 12

A ball is thrown from the top of a building $45 \mathrm{ m}$ high with initial velocity $20 \mathrm{ m/s}$ at $30^\circ$ above the horizontal. Find: (a) the time taken to reach the ground, (b) the horizontal distance from the base of the building where it lands, (c) the speed and direction of the ball just before impact.

Solution

$u_x = 20\cos 30^\circ = 17.32 \mathrm{ m/s}$ , $u_y = 20\sin 30^\circ = 10.0 \mathrm{ m/s}$

(a) Vertical motion (taking upward as positive, $h = -45 \mathrm{ m}$ ):

-45 = 10.0t - \frac{1}{2}(9.81)t^2 \implies 4.905t^2 - 10.0t - 45 = 0

t = \frac{10.0 \pm \sqrt{100 + 882.9}}{9.81} = \frac{10.0 \pm \sqrt{982.9}}{9.81} = \frac{10.0 + 31.35}{9.81} = 4.21 \mathrm{ s}

(b) Horizontal distance: $d = u_x t = 17.32 \times 4.21 = 72.9 \mathrm{ m}$

Horizontal velocity at impact: $v_x = 17.32 \mathrm{ m/s}$ (constant)

v = \sqrt{v_x^2 + v_y^2} = \sqrt{17.32^2 + 31.3^2} = \sqrt{300 + 980} = \sqrt{1280} = 35.8 \mathrm{ m/s}

Angle below horizontal: $\alpha = \tan^{-1}\left(\frac{31.3}{17.32}\right) = \tan^{-1}(1.807) = 61.0^\circ$ below horizontal

Worked Example 13

A satellite of mass $500 \mathrm{ kg}$ is in a circular orbit $300 \mathrm{ km}$ above the Earth’s surface. Calculate: (a) the orbital speed, (b) the orbital period, (c) the gravitational potential energy, (d) the kinetic energy, (e) the total energy.

(Earth mass $= 5.97 \times 10^{24} \mathrm{ kg}$ Earth radius $= 6.37 \times 10^6 \mathrm{ m}$ )

Solution

r = 6.37 \times 10^6 + 300 \times 10^3 = 6.67 \times 10^6 \mathrm{ m}

(a) $v = \sqrt{\frac{GM}{r}} = \sqrt{\frac{6.67 \times 10^{-11} \times 5.97 \times 10^{24}}{6.67 \times 10^6}} = \sqrt{5.97 \times 10^7} = 7727 \mathrm{ m/s}$

(b) $T = \frac{2\pi r}{v} = \frac{2\pi \times 6.67 \times 10^6}{7727} = \frac{4.19 \times 10^7}{7727} = 5421 \mathrm{ s} = 90.4 \mathrm{ minutes}$

(c) $E_p = -\frac{GMm}{r} = -\frac{6.67 \times 10^{-11} \times 5.97 \times 10^{24} \times 500}{6.67 \times 10^6} = -\frac{1.99 \times 10^{17}}{6.67 \times 10^6} = -2.98 \times 10^{10} \mathrm{ J}$

(d) $E_k = \frac{1}{2}mv^2 = \frac{1}{2}(500)(7727)^2 = 250 \times 5.97 \times 10^7 = 1.49 \times 10^{10} \mathrm{ J}$

(e) $E_{\mathrm{total}} = E_k + E_p = 1.49 \times 10^{10} + (-2.98 \times 10^{10}) = -1.49 \times 10^{10} \mathrm{ J}$

Note: For a circular orbit, $E_{\mathrm{total}} = -E_k = \frac{1}{2}E_p$ .

Exam-Style Questions

Question 1 (DSE Structured)

A student investigates the motion of a trolley down an inclined plane. The plane is inclined at $20^\circ$ to the horizontal. The trolley is released from rest and its acceleration is measured Using light gates at different distances from the starting point.

Distance from start (m)	Speed (m/s)
0.20	1.10
0.40	1.58
0.60	1.95
0.80	2.25
1.00	2.52

(a) Plot a graph of $v^2$ (y-axis) against distance $s$ (x-axis). Determine the acceleration From the gradient.

(b) Calculate the theoretical acceleration for a frictionless incline and compare it with the Experimental value. Hence determine the coefficient of kinetic friction.

(d) Suggest two improvements to this experiment to reduce random errors.

Solution

(a)

$s$ (m)	$v^2$ (m $^2$ /s $^2$ )
0.20	$1.10^2 = 1.21$
0.40	$1.58^2 = 2.50$
0.60	$1.95^2 = 3.80$
0.80	$2.25^2 = 5.06$
1.00	$2.52^2 = 6.35$

From $v^2 = u^2 + 2as$ with $u = 0$ : $v^2 = 2as$ .

Gradient $= \Delta v^2 / \Delta s \approx (6.35 - 1.21)/(1.00 - 0.20) = 5.14/0.80 = 6.42 \mathrm{ m/s}^2$

Since gradient $= 2a$ : $a = 6.42/2 = 3.21 \mathrm{ m/s}^2$

(b) Theoretical (frictionless): $a = g\sin 20^\circ = 9.81 \times 0.342 = 3.36 \mathrm{ m/s}^2$

Experimental: $a = 3.21 \mathrm{ m/s}^2$

The difference is due to friction: $a_{\mathrm{exp}} = g\sin\theta - \mu_k g\cos\theta$

3.21 = 3.36 - \mu_k \times 9.81 \times \cos 20^\circ = 3.36 - 9.22\mu_k

\mu_k = \frac{3.36 - 3.21}{9.22} = \frac{0.15}{9.22} = 0.016

(c) From the kinematic equation $v^2 = u^2 + 2as$ Plotting $v^2$ against $s$ (with $u = 0$ ) Gives a straight line through the origin with gradient $2a$ . A plot of $v$ against $s$ would be A curve ( $v = \sqrt{2as}$ ), which is harder to analyse.

(d) Two improvements:

Repeat each measurement several times and use the average to reduce random errors.
Use a data logger with higher time resolution (smaller uncertainty in timing).

Question 2 (DSE Structured)

Two objects, A ( $2.0 \mathrm{ kg}$ ) and B ( $3.0 \mathrm{ kg}$ ), are connected by a light Inextensible string over a smooth pulley. Object A rests on a rough horizontal table ( $\mu_k = 0.3$ ) and object B hangs freely.

(a) Draw free body diagrams for both objects.

(b) Calculate the acceleration of the system and the tension in the string.

(d) If the string is cut just as B reaches the floor (having fallen $0.80 \mathrm{ m}$ ), how Far does A slide before stopping?

Solution

(a) Object A: Weight $2g$ down, normal reaction $N$ up, tension $T$ right, friction $f$ left. Object B: Weight $3g$ down, tension $T$ up.

(b) For B (taking down as positive): $3g - T = 3a \quad (1)$

For A (taking right as positive): $T - f = 2a$ Where $f = \mu_k N = \mu_k \times 2g = 0.3 \times 2g = 0.6g$

T - 0.6g = 2a \quad (2)

Adding (1) and (2): $3g - 0.6g = 5a \implies 2.4g = 5a$

a = \frac{2.4 \times 9.81}{5} = \frac{23.54}{5} = 4.71 \mathrm{ m/s}^2

From (2): $T = 2a + 0.6g = 2(4.71) + 0.6(9.81) = 9.42 + 5.89 = 15.3 \mathrm{ N}$

v = \sqrt{7.54} = 2.75 \mathrm{ m/s}

(d) After the string is cut, A slides with initial speed $2.75 \mathrm{ m/s}$ and decelerates due To friction only:

a = -\frac{f}{m} = -\frac{\mu_k mg}{m} = -\mu_k g = -0.3 \times 9.81 = -2.94 \mathrm{ m/s}^2

v^2 = u^2 + 2as \implies 0 = (2.75)^2 + 2(-2.94)s

s = \frac{7.56}{5.89} = 1.28 \mathrm{ m}

A slides $1.28 \mathrm{ m}$ before stopping.

Question 3 (DSE Structured)

(a) State the conditions for an object to be in equilibrium.

(b) A uniform beam of weight $80 \mathrm{ N}$ and length $4.0 \mathrm{ m}$ is hinged at one End (point P) and supported by a cable attached to the other end (point Q). The cable makes an Angle of $30^\circ$ with the beam. A $150 \mathrm{ N}$ weight hangs from a point $1.5 \mathrm{ m}$ From P.

(i) Calculate the tension in the cable. (ii) Calculate the magnitude and direction of the force exerted by the hinge on the beam.

Solution

(a) For an object to be in equilibrium:

The net force on the object must be zero ( $\sum \vec{F} = 0$ ).
The net moment (torque) about any point must be zero ( $\sum \tau = 0$ ).

(b) (i) Take moments about P (eliminates the hinge force):

Clockwise moments = $80 \times 2.0 + 150 \times 1.5 = 160 + 225 = 385 \mathrm{ N\, m}$

(Weight of beam acts at centre, $2.0 \mathrm{ m}$ from P.)

Anticlockwise moment = $T\sin 30^\circ \times 4.0 = T \times 0.5 \times 4.0 = 2.0T$

2.0T = 385 \implies T = 192.5 \mathrm{ N}

(ii) Resolving forces on the beam:

Vertical: $H_y + T\sin 30^\circ = 80 + 150$

H_y + 192.5 \times 0.5 = 230 \implies H_y + 96.25 = 230 \implies H_y = 133.75 \mathrm{ N}

(upward)

Horizontal: $H_x = T\cos 30^\circ = 192.5 \times 0.866 = 166.7 \mathrm{ N}$ (away from the wall)

H = \sqrt{H_x^2 + H_y^2} = \sqrt{166.7^2 + 133.75^2} = \sqrt{27789 + 17889} = \sqrt{45678} = 213.7 \mathrm{ N}

Angle above horizontal: $\alpha = \tan^{-1}(133.75/166.7) = \tan^{-1}(0.803) = 38.7^\circ$

Question 4 (DSE Structured)

A $500 \mathrm{ g}$ ball is attached to a string of length $0.80 \mathrm{ m}$ and swung in a Vertical circle.

(a) The ball has speed $6.0 \mathrm{ m/s}$ at the lowest point. Calculate the tension in the String at this point.

(b) Calculate the speed of the ball at the highest point.

(d) Calculate the minimum speed at the lowest point for the ball to complete the full circle.

(e) Explain why the ball cannot complete the full circle if the string is replaced by a light Rod (consider what happens at the top).

Solution

(a) At the lowest point: $T_{\mathrm{bottom}} - mg = \frac{mv_{\mathrm{bottom}}^2}{r}$

T_{\mathrm{bottom}} = mg + \frac{mv_{\mathrm{bottom}}^2}{r} = 0.5 \times 9.81 + \frac{0.5 \times 36}{0.80} = 4.905 + 22.5 = 27.4 \mathrm{ N}

(b) Energy conservation between lowest and highest points (height difference $= 2r = 1.6 \mathrm{ m}$ ):

\frac{1}{2}mv_{\mathrm{bottom}}^2 = \frac{1}{2}mv_{\mathrm{top}}^2 + mg(2r)

\frac{1}{2}(0.5)(36) = \frac{1}{2}(0.5)v_{\mathrm{top}}^2 + 0.5 \times 9.81 \times 1.6

9.0 = 0.25v_{\mathrm{top}}^2 + 7.85

v_{\mathrm{top}}^2 = \frac{9.0 - 7.85}{0.25} = \frac{1.15}{0.25} = 4.6

v_{\mathrm{top}} = \sqrt{4.6} = 2.14 \mathrm{ m/s}

T_{\mathrm{top}} = \frac{mv_{\mathrm{top}}^2}{r} - mg = \frac{0.5 \times 4.6}{0.80} - 4.905 = 2.875 - 4.905 = -2.03 \mathrm{ N}

Since the tension is negative, the string goes slack before the ball reaches the top. The ball Does not complete the full circle.

(d) For the ball to just complete the circle: $T_{\mathrm{top}} = 0$ at the top, so $v_{\mathrm{top}} = \sqrt{gr} = \sqrt{9.81 \times 0.80} = \sqrt{7.848} = 2.80 \mathrm{ m/s}$

\frac{1}{2}mv_{\mathrm{bottom}}^2 = \frac{1}{2}m(gr) + mg(2r) = \frac{1}{2}mgr + 2mgr = \frac{5}{2}mgr

v_{\mathrm{bottom}} = \sqrt{5gr} = \sqrt{5 \times 9.81 \times 0.80} = \sqrt{39.24} = 6.26 \mathrm{ m/s}

(e) With a light rod, the rod can push as well as pull. At the top, even if $v_{\mathrm{top}} < \sqrt{gr}$ The rod can exert a push (compression) to provide the additional centripetal force. The ball will Still complete the circle as long as it reaches the top with any speed (the rod supports it).

With a string, the string can only pull (tension $\geq 0$ ). If the speed at the top is too low, The string goes slack and the ball falls.

Question 5 (DSE Structured)

A spacecraft of mass $1000 \mathrm{ kg}$ is travelling towards the Moon. The Moon has mass $7.35 \times 10^{22} \mathrm{ kg}$ and radius $1.74 \times 10^6 \mathrm{ m}$ .

(a) Calculate the gravitational field strength on the surface of the Moon.

(b) The spacecraft is at a height of $500 \mathrm{ km}$ above the Moon’s surface. Calculate the Gravitational force on the spacecraft.

(d) Explain why the Moon has no atmosphere, referring to escape velocity and molecular speeds.

Solution

(a) $g_{\mathrm{Moon}} = \frac{GM}{R^2} = \frac{6.67 \times 10^{-11} \times 7.35 \times 10^{22}}{(1.74 \times 10^6)^2}$

g_{\mathrm{Moon}} = \frac{4.90 \times 10^{12}}{3.03 \times 10^{12}} = 1.62 \mathrm{ N/kg}

(b) $r = 1.74 \times 10^6 + 500 \times 10^3 = 2.24 \times 10^6 \mathrm{ m}$

F = \frac{GMm}{r^2} = \frac{6.67 \times 10^{-11} \times 7.35 \times 10^{22} \times 1000}{(2.24 \times 10^6)^2} = \frac{4.90 \times 10^{15}}{5.02 \times 10^{12}} = 976 \mathrm{ N}

(c) $v_e = \sqrt{\frac{2GM}{R}} = \sqrt{\frac{2 \times 6.67 \times 10^{-11} \times 7.35 \times 10^{22}}{1.74 \times 10^6}} = \sqrt{\frac{9.80 \times 10^{12}}{1.74 \times 10^6}} = \sqrt{5.63 \times 10^6} = 2370 \mathrm{ m/s}$

(d) The Moon’s escape velocity ( $2370 \mathrm{ m/s}$ ) is relatively low. Gas molecules in the Upper atmosphere have a range of speeds described by the Maxwell-Boltzmann distribution. A Significant fraction of molecules (especially lighter ones like hydrogen and helium) have speeds Exceeding the escape velocity. Over geological time, these molecules escape into space, and the Moon cannot retain an atmosphere. The Earth’s much higher escape velocity ( $11200 \mathrm{ m/s}$ ) Means very few molecules have sufficient speed to escape.

Extended Problems

Extended Problem 1: Banked Curve with Friction

A road curve of radius $80 \mathrm{ m}$ is banked at $15^\circ$ . The coefficient of static Friction between tyres and road is $0.40$ .

(a) Calculate the maximum speed at which a car can negotiate the curve without sliding up the Bank.

(b) Calculate the minimum speed at which the car can negotiate the curve without sliding down The bank.

Solution

(a) At maximum speed, friction acts down the bank. Taking components:

Horizontally: $N\sin\theta + f\cos\theta = \frac{mv_{\max}^2}{r}$

Vertically: $N\cos\theta - f\sin\theta = mg$

Dividing the horizontal by the vertical equation:

\frac{\sin\theta + \mu_s\cos\theta}{\cos\theta - \mu_s\sin\theta} = \frac{v_{\max}^2}{rg}

v_{\max}^2 = rg\frac{\sin 15^\circ + 0.40\cos 15^\circ}{\cos 15^\circ - 0.40\sin 15^\circ} = 80 \times 9.81 \times \frac{0.259 + 0.386}{0.966 - 0.104} = 784.8 \times \frac{0.645}{0.862} = 587

v_{\max} = \sqrt{587} = 24.2 \mathrm{ m/s}

(b) At minimum speed, friction acts up the bank:

v_{\min}^2 = rg\frac{\sin\theta - \mu_s\cos\theta}{\cos\theta + \mu_s\sin\theta} = 80 \times 9.81 \times \frac{0.259 - 0.386}{0.966 + 0.104} = 784.8 \times \frac{-0.127}{1.070}

Since the numerator is negative, $v_{\min}^2 < 0$ Meaning the car will not slide down the bank At any speed (the banking alone provides enough centripetal force for stationary or very slow Speeds). The minimum speed is effectively $0$ .

Extended Problem 2: Satellite Orbit Transfer

A satellite of mass $500 \mathrm{ kg}$ is in a circular orbit of radius $7.0 \times 10^6 \mathrm{ m}$ Around the Earth. The satellite needs to transfer to a higher circular orbit of radius $7.5 \times 10^6 \mathrm{ m}$ .

(a) Calculate the orbital speed in the lower orbit.

(b) Calculate the orbital speed in the higher orbit.

(Earth mass $= 5.97 \times 10^{24} \mathrm{ kg}$ )

Solution

(a) $v_1 = \sqrt{\frac{GM}{r_1}} = \sqrt{\frac{6.67 \times 10^{-11} \times 5.97 \times 10^{24}}{7.0 \times 10^6}} = \sqrt{5.69 \times 10^7} = 7544 \mathrm{ m/s}$

(b) $v_2 = \sqrt{\frac{GM}{r_2}} = \sqrt{\frac{6.67 \times 10^{-11} \times 5.97 \times 10^{24}}{7.5 \times 10^6}} = \sqrt{5.31 \times 10^7} = 7287 \mathrm{ m/s}$

E_1 = -\frac{6.67 \times 10^{-11} \times 5.97 \times 10^{24} \times 500}{2 \times 7.0 \times 10^6} = -\frac{1.99 \times 10^{17}}{1.4 \times 10^7} = -1.42 \times 10^{10} \mathrm{ J}

E_2 = -\frac{1.99 \times 10^{17}}{1.5 \times 10^7} = -1.33 \times 10^{10} \mathrm{ J}

Energy required: $\Delta E = E_2 - E_1 = -1.33 \times 10^{10} - (-1.42 \times 10^{10}) = 9.0 \times 10^8 \mathrm{ J}$

Worked Examples

Example 1: Connected bodies

Problem. A $5 \mathrm{ kg}$ block on a smooth horizontal table is connected by a string over a pulley to a $3 \mathrm{ kg}$ block hanging freely. Find the acceleration and tension.

Solution. For the $3 \mathrm{ kg}$ block: $3g - T = 3a$ . For the $5 \mathrm{ kg}$ block: $T = 5a$ .

Adding: $3g = 8a \implies a = \frac{3 \times 9.81}{8} = 3.68 \mathrm{ m/s^2}$ .

$T = 5(3.68) = 18.4 \mathrm{ N}$ .

$\blacksquare$

Example 2: Projectile off a cliff

Problem. A ball is thrown horizontally at $15 \mathrm{ m/s}$ from a cliff $60 \mathrm{ m}$ high. Find the horizontal distance and velocity at impact.

Solution. Vertical: $h = \frac{1}{2}gt^2 \implies t = \sqrt{\frac{2h}{g}} = \sqrt{\frac{120}{9.81}} = 3.50 \mathrm{ s}$ .

Horizontal: $d = v_x t = 15 \times 3.50 = 52.5 \mathrm{ m}$ .

$v_y = gt = 34.3 \mathrm{ m/s}$ . $v = \sqrt{15^2 + 34.3^2} = 37.4 \mathrm{ m/s}$ .

$\blacksquare$

Summary

Newton’s three laws: inertia ( $\sum F = 0 \Rightarrow v = \text{const}$ ), $F = ma$ , and action-reaction (equal and opposite, on different bodies).
Free body diagrams are essential: include all forces acting ON the body, not BY the body.
Projectile motion: resolve into horizontal (constant velocity) and vertical (constant acceleration) components.
Conservation of momentum: $m_1 u_1 + m_2 u_2 = m_1 v_1 + m_2 v_2$ (always conserved in collisions).
Kinetic energy is conserved only in elastic collisions; use the coefficient of restitution for inelastic cases.

Cross-References

Topic	Site	Link
[Kinematics (Physics)]	A-Level	View
[Kinematics (Physics)]	IB	View
[Kinematics (Physics)]	DSE	View

Intuition

Physics reveals that nature follows mathematical laws at every scale. Matter is made of atoms, forces arise from field interactions, and energy is conserved in every transformation. The power of physics lies in its predictive ability - from calculating projectile trajectories to designing particle accelerators. Understanding these principles helps us technology, predict natural phenomena, and appreciate the universe’s underlying order.

References

Halliday, D., Resnick, R. & Walker, J. (2013). Fundamentals of Physics (10th ed.). John Wiley & Sons.
Feynman, R. P., Leighton, R. B. & Sands, M. (2011). The Feynman Lectures on Physics, Vol. I: The New Millennium Edition, Mechanics, Radiation, and Heat. Basic Books.
Kleppner, D. & Kolenkow, R. J. (2013). An Introduction to Mechanics (2nd ed.). Cambridge University Press.
Beer, F. P., Johnston, E. R., Cornwell, R. D. & Self, B. (2019). Vector Mechanics for Engineers: Statics and Dynamics (12th ed.). McGraw-Hill Education.
Giancoli, D. C. (2013). Physics: Principles with Applications (7th ed.). Pearson.

Mark this page as reviewed

Forces and Motion

Newton’s Laws of Motion

First Law (Law of Inertia)

Second Law

Third Law

Worked Example 1

Worked Example 2

Worked Example 3

Friction

Static and Kinetic Friction

Inclined Planes

Worked Example 3

Worked Example 4

Momentum and Impulse

Linear Momentum

Conservation of Momentum

Impulse

Collisions

Worked Example 5

Worked Example 6

Worked Example 7

Projectile Motion

Analysis by Components

Key Results

Worked Example 7

Circular Motion

Angular Quantities

Centripetal Acceleration and Force

Vertical Circular Motion

Worked Example 8

Worked Example 9

Gravitation

Newton’s Law of Universal Gravitation

Gravitational Field Strength

Gravitational Potential Energy

Orbital Motion

Worked Example 10

Common Pitfalls

Summary Table

Problem Set

Intuition

See Also

References