Hey Tara! Welcome to your Topic 1 study guide. This topic is the foundation of ALL of physics, and I promise you it is not as scary as it looks. We will take it step by step, with examples from everyday life in Bangalore that you already understand. Every time you see a formula, I will show you exactly how to use it with worked examples. You have got this!
Measuring Length and Volume
Using a Ruler
A ruler is the simplest instrument you use every day. It measures length - the distance from one point to another. Here is how to use it properly:
- Place the ruler right next to the object - do not hold it above or at an angle. Place it flat on the surface so there is no gap between the ruler and the object.
- Read to the nearest millimetre (mm) - a standard ruler is marked in cm and mm. The small divisions are 1 mm each. So if a pencil ends between 15.2 cm and 15.3 cm, estimate which mm line it is closest to.
- Avoid parallax error - your eye must be directly above the marking you are reading, not looking at an angle. If you look from the side, you will read the wrong value.
- Use the markings, not the end of the ruler - some rulers have a worn or chipped end. It is better to measure from, say, the 1.0 cm mark to the end of the object, then subtract 1.0 cm from your reading.
Indian example: Imagine you are measuring the length of your NCERT Physics textbook. You place the ruler alongside it. The book starts at 0.0 cm and ends at 24.8 cm. The length of the book is 24.8 cm, or 248 mm, or 0.248 m.
Always state your measurement with the correct unit. A number without a unit is meaningless in physics. "24.8" means nothing. "24.8 cm" is a proper measurement.
Using a Measuring Cylinder
A measuring cylinder measures the volume of a liquid. You have seen your amma measure water for cooking - a measuring cylinder is the same idea, but more precise.
- Place the cylinder on a flat, level surface - do not hold it in your hand; it will tilt and give a wrong reading.
- Pour in the liquid gently to avoid splashing.
- Read at the meniscus - this is the key part! Water curves upward at the edges of the glass (because water molecules are attracted to glass). The bottom of this curve is the meniscus. Always read the volume at the bottom of the meniscus, not at the edges where the water climbs up.
- Keep your eye level with the liquid surface - if you look from above, the reading will be too high; from below, too low. Bend down so your eye is at the same height as the liquid.
Indian example: Suppose you want to measure the volume of water that fits in a stainless steel tumbler (the kind you drink water from at home). You pour the water from the tumbler into a measuring cylinder. The bottom of the meniscus sits at the 250 cm³ mark. So the tumbler holds 250 cm³ (which is the same as 250 mL) of water.
Measuring Volume of an Irregular Object (Displacement Method)
What if you need to find the volume of a small stone or a metal idol? You cannot use a ruler because the shape is irregular. Instead, you use the displacement method:
- Fill a measuring cylinder partway with water. Record the initial volume (say, 50 cm³).
- Gently lower the object into the water using a thread (do not drop it - that causes splashing!).
- The water level rises. Record the new volume (say, 62 cm³).
- Volume of the object = new volume - initial volume = 62 - 50 = 12 cm³.
Indian example: You want to find the volume of a small brass Ganesha idol. You lower it into a measuring cylinder. The water rises from 40 cm³ to 53 cm³. The volume of the idol is 53 - 40 = 13 cm³.
The object must be completely submerged (fully underwater) for the displacement method to work. If there are air bubbles stuck to the object, tap the cylinder gently to release them before reading.
Measuring Time Intervals
Time is something we measure constantly in everyday life. In physics, we need to be precise about it.
Instruments for Measuring Time
- Analogue clocks - the regular clocks with hour, minute, and second hands. Good for longer time intervals (hours, minutes) but not precise for short intervals.
- Digital stopwatches - these measure to the nearest 0.01 s (one hundredth of a second). You press start when the event begins and stop when it ends.
- Digital timers with sensors - these use light gates or pressure pads to start and stop automatically. They are more accurate because there is no human reaction time error.
Indian example: Think about Sports Day at your school. When the PE teacher times the 100 m race, they use a stopwatch. They press start when they see the starting gun fire (not when they hear it - light travels faster than sound!). They press stop when the runner crosses the finish line.
Another example: Timing how long your pressure cooker whistles. If it whistles 3 times in 4 minutes, each whistle interval is about 80 seconds. But if you wanted to measure this precisely, you would use a digital stopwatch.
Human reaction time is about 0.2 to 0.5 seconds. This means every time you start or stop a stopwatch by hand, your measurement could be off by up to 0.5 s. This is why we use the "multiples" method for short time intervals (see next section).
Measuring Small Distances and Short Times by Averaging
Here is a brilliant trick that scientists use: if a single measurement is too small to measure accurately, measure MANY of them together and divide.
Why Do We Measure Multiples?
Let us say you want to measure the thickness of a single page of your textbook. If you try to measure one page with a ruler, you might get "about 0.1 mm" - but that is very imprecise. The ruler is not fine enough.
Instead:
- Measure the thickness of 100 pages together: say, 8.4 mm.
- Divide by 100: thickness of one page = 8.4 / 100 = 0.084 mm.
Now you have a much more precise answer!
The Pendulum: A Classic Example
A pendulum is a weight hanging from a string that swings back and forth. One complete back-and-forth swing is called one oscillation. The time for one complete oscillation is called the period (T).
A single swing might take about 1 second. If you time just one swing with a stopwatch, your reaction time error (about 0.3 s) is a huge fraction of the measurement - that is a 30% error! Terrible!
Instead, you time 20 swings. If 20 swings take 18.4 s, then one swing takes 18.4 / 20 = 0.92 s. Now your reaction time error of 0.3 s is only 0.3/18.4 = 1.6% of the total time. Much better!
When counting oscillations, start your count from zero, not one! When you release the pendulum and start the stopwatch, the pendulum is at position 0. When it comes back to the same position going in the same direction, that is oscillation 1.
Also, always start timing from the middle (equilibrium) position of the swing, not from the highest point. The pendulum moves fastest at the middle, so it is easier to judge the exact moment it passes through.
Scalars and Vectors
This is one of those ideas in physics that sounds complicated but is actually really simple once you get it.
What is a Scalar?
A scalar is a quantity that has only magnitude (size). That is it. Just a number with a unit.
For example: "The temperature in Bangalore today is 28 degrees Celsius." You do not need to say in which direction the temperature is 28 degrees - that would not make sense! Temperature is just a number.
What is a Vector?
A vector is a quantity that has both magnitude AND direction. You need to state which way it is pointing for it to make full sense.
For example: "The auto-rickshaw is travelling at 30 km/h towards Majestic." The "towards Majestic" part is the direction. Without it, you only know how fast the auto is going, not where it is going.
The Cricket Analogy
Think about Jasprit Bumrah bowling in a cricket match:
- Speed of the ball: 145 km/h - this is a scalar. It tells you how fast the ball is moving, but not in which direction.
- Velocity of the ball: 145 km/h towards the off stump - this is a vector. It tells you both the speed AND the direction. The batsman cares about the direction!
The Scalar Quantities You Must Know
| Scalar Quantity | What It Measures | Example |
|---|---|---|
| Distance | How far something has travelled (total path) | The walk from your classroom to the canteen is 200 m |
| Speed | How fast something is going | An auto-rickshaw going at 40 km/h |
| Time | Duration of an event | The school assembly lasted 30 minutes |
| Mass | Amount of matter in an object | A bag of rice has a mass of 5 kg |
| Energy | Ability to do work | A cup of chai gives you about 300 kJ of energy |
| Temperature | How hot or cold something is | Bangalore in April: 34 degrees C |
Remember the scalars with: "D-S-T-M-E-T" = "Dosas Served To Me Every Tuesday"
Distance, Speed, Time, Mass, Energy, Temperature - all scalars!
The Vector Quantities You Must Know
| Vector Quantity | Why It Needs Direction | Example |
|---|---|---|
| Force | A push or pull acts in a specific direction | You push a door with 10 N to the right |
| Weight | Force of gravity always acts downwards | Your weight is 500 N downwards |
| Velocity | Speed in a specific direction | A train moving at 80 km/h northwards |
| Acceleration | Rate of change of velocity has a direction | The bus accelerates at 2 m/s² forwards |
| Momentum | Mass x velocity, so it inherits direction from velocity | A cricket ball has momentum towards the boundary |
| Electric field strength | Force per unit charge acts in a direction | Electric field points from positive to negative |
| Gravitational field strength | Force per unit mass, acts towards centre of Earth | g = 9.8 N/kg directed downward |
Remember the vectors with: "F-W-V-A-M-E-G" = "Five Wickets! Virat And MS Earn Glory"
Force, Weight, Velocity, Acceleration, Momentum, Electric field strength, Gravitational field strength - all vectors!
A very common exam question asks: "What is the difference between speed and velocity?" The answer: Speed is a scalar (magnitude only); velocity is a vector (magnitude AND direction). Similarly for distance (scalar) vs displacement (vector).
Adding Vectors at Right Angles (Resultant)
When two vectors act at right angles (90 degrees) to each other, we can find the single vector that has the same overall effect. This single vector is called the resultant.
Think about it this way: if you walk 3 km east and then 4 km north, you have not ended up 7 km from where you started. You have ended up at a diagonal distance that is less than 7 km. The resultant is that diagonal.
River current speed = 3 m/s (this is sideways, at 90 degrees to the boat's intended direction)
Wind speed = 50 km/h eastward (perpendicular to north)
When finding the resultant of two perpendicular vectors, you will ALWAYS need: (1) Pythagoras for the magnitude, (2) tan⁻¹ for the angle. Always draw a diagram first - it helps you see which side is opposite and which is adjacent for the angle.
Remember: the resultant of two perpendicular vectors is ALWAYS less than their arithmetic sum. If forces are 3 N and 4 N, the resultant is 5 N, not 7 N!
1 m = 1000 mm, so 3450 mm ÷ 1000 = 3.450 m = 3.45 m
Step 2: Compare.
Arch height = 3.50 m. Bus height = 3.45 m.
3.45 m < 3.50 m, so yes, the bus fits — with 0.05 m (5 cm) to spare.
Step 3: Choose the instrument.
The arch is about 3.5 m tall — far too large for a ruler (30 cm) or even a metre ruler. The driver should use a measuring tape (e.g., a 5 m steel tape). It can measure large lengths accurately to the nearest mm, it’s portable, and it’s flexible enough to reach the top of the arch.
When you read a measuring cylinder, your eye must be level with the bottom of the meniscus. The chai wallah does this.
His taller helper looks down at the cylinder. From above, the line of sight crosses the scale at a lower reading than the true value — this is why he reads 46 mL instead of 48 mL.
This mistake is called a parallax error. It happens whenever you read a scale from the wrong angle.
Ruler: precision ≈ ±1 mm. Can measure up to 30 cm or 100 cm. But ±1 mm is far too imprecise — she needs ±0.1 mm. ❌
Micrometer screw gauge: precision = ±0.01 mm (excellent!). But its maximum opening is typically only about 25 mm. The tile is 5 cm = 50 mm — it won’t fit! ❌
Vernier caliper: precision = ±0.1 mm. Can measure objects up to about 150 mm. The tile (50 mm) fits easily, and the precision matches exactly what she needs. ✅
Answer: Vernier caliper. It gives ±0.1 mm precision and can accommodate a 50 mm tile.
Sum = 14.2 + 13.8 + 14.1 + 13.9 + 14.5 = 70.5 s
Average = 70.5 ÷ 5 = 14.1 s
Step 2: Calculate the percentage error.
Percentage error = (error ÷ measured value) × 100%
= (0.3 ÷ 14.1) × 100%
= 2.1%
Step 3: Is this significant?
A 2.1% error is relatively small but not negligible. For a school PE lesson, it’s acceptable. For an Olympic sprint (where races are decided by 0.01 s), this error would be huge!
Average speed = distance ÷ time = 100 ÷ 14.1 = 7.1 m/s (about 25.5 km/h).
Method 1 — Measuring cylinder (if the blade fits):
1. Fill a measuring cylinder with water and record the initial volume, V₁.
2. Carefully lower the blade into the water (it must be fully submerged).
3. Record the new volume, V₂.
4. Volume of blade = V₂ − V₁.
Method 2 — Displacement (Eureka) can (if the blade is too large for a measuring cylinder):
1. Fill the displacement can until water flows out of the spout. Wait until dripping stops.
2. Place a measuring cylinder under the spout.
3. Gently lower the blade into the can until fully submerged.
4. Collect all displaced water in the measuring cylinder.
5. The volume of displaced water = volume of the blade.
Key readings: initial water level (V₁) and final water level (V₂), OR the volume of displaced water collected.
Speed
Speed is one of the first things you learn in physics, and you already understand it intuitively. When your parents say "the auto is going too fast," they are talking about speed.
Definition
Speed is the distance travelled per unit time. In simple terms, it tells you how much distance an object covers in each second (or each hour, or any unit of time).
You can rearrange this formula into three forms. Remember the triangle trick: write s at the top, v and t at the bottom. Cover the one you want to find:
- v = s / t (cover v: s over t)
- s = v x t (cover s: v times t)
- t = s / v (cover t: s over v)
Unit consistency is crucial! If speed is in m/s, distance must be in metres and time in seconds. If speed is in km/h, distance must be in km and time in hours. Do NOT mix units!
To convert km/h to m/s: divide by 3.6 (because 1 km/h = 1000m / 3600s = 1/3.6 m/s).
To convert m/s to km/h: multiply by 3.6.
v = s / t = 6 km / 0.25 h = 24 km/h
v = s / t = 6000 m / 900 s = 6.67 m/s
OR simply: 24 km/h / 3.6 = 6.67 m/s
Time = 5 min = 5 x 60 = 300 s
Velocity
You have already seen this in Section 1.1 when we talked about scalars and vectors. Now let us make it formal.
Definition
Velocity is speed in a given direction. It is a vector quantity.
The difference between speed and velocity:
- Speed = 50 km/h (scalar - just tells you how fast)
- Velocity = 50 km/h due north (vector - tells you how fast AND which way)
Why does direction matter? Imagine a car driving around a circular roundabout at a constant speed of 30 km/h. Its speed never changes, but its velocity is constantly changing because the direction is constantly changing! This is an important concept for understanding acceleration later.
Cricket analogy: When a batsman hits the ball, the ball comes towards the bat at, say, 140 km/h. After the shot, the ball goes away at maybe 120 km/h. The speed did not change much, but the velocity changed dramatically because the direction completely reversed!
Average Speed
This is a very important concept. Average speed takes into account the whole journey, including the fast bits, the slow bits, and even stops.
When a question asks for "average speed," you MUST include all time - including time spent stationary. The total distance is the distance actually travelled along the path, not the straight-line displacement. This catches many students out!
Distance-Time Graphs
Graphs are one of the most powerful tools in physics. They tell a story about how an object moves, and once you learn to read them, you can extract all kinds of useful information.
What does a distance-time graph show?
The horizontal axis (x-axis) shows time. The vertical axis (y-axis) shows distance from the starting point. As time increases (you move right), the distance changes depending on how the object is moving.
| Graph Shape | What It Means | Example |
|---|---|---|
| Horizontal line | Object is stationary (at rest) - distance is not changing | An auto-rickshaw waiting at a red light |
| Straight line going up | Object moving at constant speed - distance increases steadily | A train cruising at 100 km/h on a straight track |
| Curve getting steeper | Object is accelerating - covering more distance each second | A bus pulling away from a stop |
| Curve getting flatter | Object is decelerating - covering less distance each second | A bus approaching a stop and slowing down |
| Steeper straight line | Faster constant speed (steeper = faster) | Comparing a cycle vs a car on the same road |
Calculating Speed from a Distance-Time Graph
Here is the key idea: the speed of an object is the gradient (slope) of the distance-time graph.
If the line is straight, the gradient (and therefore speed) is constant. If the line is curved, the gradient is changing, meaning the speed is changing.
At t = 6 s, distance = 90 m
Speed-Time Graphs
Now let us move to speed-time graphs. These are even more useful than distance-time graphs because they can tell you about acceleration AND distance.
| Graph Shape | What It Means | Example |
|---|---|---|
| Horizontal line | Constant speed - speed is not changing | A Namma Metro train cruising between stations |
| Straight line going up | Constant acceleration - speed increasing at a steady rate | A car accelerating smoothly from a traffic light |
| Straight line going down | Constant deceleration - speed decreasing steadily | An auto-rickshaw braking to a stop |
| Curve getting steeper (upward) | Increasing acceleration | A motorcycle whose engine gets more powerful at higher revs |
| Curve getting flatter (upward) | Decreasing acceleration | A car approaching its top speed |
| Line at zero | Object is stationary | A parked scooter |
Distance from a Speed-Time Graph
Here is the second powerful thing about speed-time graphs: the area under the graph equals the distance travelled.
Why? Because distance = speed x time. And "speed x time" is exactly what area means when the x-axis is time and the y-axis is speed!
A very common mistake is confusing the two graph types. Remember:
Distance-time graph: gradient = speed
Speed-time graph: gradient = acceleration, area = distance
Never say "area under a distance-time graph" or "gradient of a speed-time graph gives speed" - that is wrong!
Acceleration of Free Fall (g)
When you drop something, it speeds up as it falls. Gravity pulls it downward, making it go faster and faster. This acceleration due to gravity is given the symbol g.
Indian example: Imagine a coconut falls from a tree. The moment it detaches from the tree, it is at rest (speed = 0 m/s). After 1 second of falling, it is going at about 10 m/s. After 2 seconds, about 20 m/s. Gravity does not care how heavy the coconut is - a heavy coconut and a small coconut both accelerate at the same rate (ignoring air resistance). This was famously demonstrated by Galileo!
Important: The value of g is the same for ALL objects, regardless of their mass (as long as we ignore air resistance). A cricket ball and a marble, if dropped from the same height at the same time, will hit the ground at the same time.
On your IGCSE exam, g = 9.8 m/s² will usually be given in the question or on the data sheet. Some questions say "take g = 10 m/s²" for simpler calculations. Always use the value given in the question!
Acceleration
Definition
Acceleration is the rate of change of velocity. In simpler terms, it tells you how quickly the speed is changing.
The unit m/s² means "metres per second, per second." If a = 2 m/s², it means the object's speed increases by 2 m/s every second. So after 1 second, it is 2 m/s faster; after 2 seconds, 4 m/s faster; and so on.
Acceleration from a Speed-Time Graph
Just like speed is the gradient of a distance-time graph, acceleration is the gradient of a speed-time graph.
At t = 6 s, speed = 15 m/s
Constant vs Changing Acceleration
On a speed-time graph:
- Straight line = constant acceleration (the gradient is the same everywhere)
- Curved line = changing acceleration (the gradient changes from point to point)
If the curve gets steeper, the acceleration is increasing. If it gets flatter, the acceleration is decreasing.
Deceleration (Negative Acceleration)
Deceleration is simply acceleration in the opposite direction to the motion. It means the object is slowing down. In calculations, deceleration shows up as a negative value of acceleration.
There is nothing special about deceleration - it is just acceleration with a minus sign. The formulas work exactly the same way.
When a question says "deceleration of 5 m/s²," it means the object is slowing down by 5 m/s every second. In the formula, use a = -5 m/s² (with the negative sign). The negative sign is important because it indicates the direction opposite to motion.
If a question asks "what is the deceleration?" and your calculated acceleration is -3 m/s², the deceleration is 3 m/s² (positive number, because deceleration is the magnitude of the negative acceleration).
Falling Objects: Air Resistance and Terminal Velocity
This is one of the most interesting topics in motion. Let us think about what happens when you drop something from a great height.
Falling Without Air Resistance (in a vacuum)
In a vacuum (like on the Moon, where there is no air), ALL objects fall with the same acceleration of g = 9.8 m/s², regardless of their mass or shape. A feather and a hammer would hit the ground at the same time! (This was actually demonstrated on the Moon by astronaut David Scott in 1971.)
Falling With Air Resistance (in the real world)
In the real world, air resistance (also called drag) plays a big role. Here is what happens when you drop a coconut from a tall coconut tree:
- At the moment of release: The coconut is not moving, so there is no air resistance (drag only acts on moving objects). The only force is weight (gravity) acting downward. The coconut accelerates at g = 9.8 m/s².
- As it falls faster: Air resistance increases because the coconut is moving faster through the air. Now there are two forces: weight downward and air resistance upward. The net (resultant) force downward decreases, so the acceleration decreases (but the coconut is still speeding up, just more slowly).
- Eventually: The air resistance grows until it equals the weight. Now the net force is zero. With no net force, there is no acceleration. The coconut falls at a constant speed. This constant speed is called the terminal velocity.
Why a coconut and a leaf fall differently
If you drop a coconut and a leaf from the same height, the coconut hits the ground first. Why?
- The coconut is heavy (large weight) and compact (small air resistance relative to its weight). Air resistance takes a long time to match its weight, so it reaches a high terminal velocity and hits the ground quickly.
- The leaf is light (small weight) and has a large flat surface area (large air resistance relative to its weight). Air resistance matches its tiny weight almost immediately, so it reaches a low terminal velocity quickly and drifts down slowly.
Falling in a Liquid
The same principle applies when an object falls through a liquid (like a marble dropped in a tall jar of oil). The liquid provides much more resistance (drag) than air, so:
- Terminal velocity is reached much sooner
- Terminal velocity is much lower than in air
When drawing or describing a speed-time graph for a falling object reaching terminal velocity:
1. The graph starts with a steep gradient (high acceleration near g).
2. The gradient decreases (curve gets flatter) as air resistance increases.
3. The graph becomes horizontal (zero gradient) at terminal velocity.
The curve must be smooth - no sudden kinks or straight-line segments! And it must never go beyond the terminal velocity (it cannot overshoot).
Ratio = falcon speed ÷ metro speed = 390 ÷ 80 = 4.875 times faster
(Nearly 5 times faster!)
Step 2: Convert 390 km/h to m/s.
To convert km/h → m/s, divide by 3.6 (because 1 km = 1000 m and 1 h = 3600 s, so the factor is 1000 ÷ 3600 = 1 ÷ 3.6).
390 ÷ 3.6 = 108.3 m/s (to 1 d.p.)
That’s about 108 metres every second — roughly the length of a football pitch!
Total distance = 21 + 21 = 42 km
Step 2: Find total time (convert everything to hours).
First half: 2 h
Rest: 3 min = 3 ÷ 60 = 0.05 h
Second half: 2 h 15 min = 2.25 h
Total time = 2 + 0.05 + 2.25 = 4.30 h
Step 3: Calculate average speed.
Average speed = total distance ÷ total time
= 42 ÷ 4.30
= 9.77 km/h (or about 9.8 km/h)
In m/s: 9.77 ÷ 3.6 = 2.71 m/s
a = (v − u) ÷ t
v = 7600 m/s, u = 0, t = 20 min = 20 × 60 = 1200 s
a = (7600 − 0) ÷ 1200 = 6.33 m/s²
Namma Metro:
First convert 80 km/h to m/s: 80 ÷ 3.6 = 22.2 m/s
a = (v − u) ÷ t
v = 22.2 m/s, u = 0, t = 30 s
a = (22.2 − 0) ÷ 30 = 0.74 m/s²
The rocket has the greater acceleration — about 8.6 times greater than the Metro train.
u = 0 (starts from rest), a = g = 10 m/s², s = 20 m
Part 1: Find the final velocity (v).
v² = u² + 2as
v² = 0² + 2 × 10 × 20
v² = 400
v = √400 = 20 m/s
That’s 72 km/h — as fast as a car on a city road!
Part 2: Find the time (t).
Use v = u + at
20 = 0 + 10 × t
t = 20 ÷ 10 = 2.0 s
The coconut takes just 2 seconds to fall 20 metres.
When an object falls, it accelerates due to gravity. As it speeds up, air resistance increases (air resistance depends on speed, shape, and surface area).
Terminal velocity is reached when: air resistance = weight. At this point, the resultant force is zero and the object stops accelerating.
Parcel A (light, large carton):
• Low weight (small gravitational force)
• Large surface area (high air resistance, even at low speeds)
• Air resistance matches its small weight at a LOW speed
• Reaches terminal velocity quickly
• Terminal velocity is LOW
Parcel B (small, dense metal part):
• High weight (large gravitational force)
• Small surface area (lower air resistance at the same speed)
• Must reach a much HIGHER speed before air resistance matches its weight
• Takes longer to reach terminal velocity
• Terminal velocity is HIGH
Tara, have you ever wondered why astronauts float around inside the International Space Station, yet they still look the same size? Their mass has not changed one bit — but their weight has almost disappeared! Mass and weight sound like the same thing, but they are very different ideas in physics. Understanding this difference is one of the most important things in your IGCSE course, and examiners love to test it. Let us break it down step by step.
What is Mass?
Mass is a measure of the quantity of matter in an object at rest relative to the observer. In simpler words, mass tells you how much "stuff" is inside something.
Think about it this way: a 5 kg bag of Sona Masoori rice from Big Bazaar contains a certain amount of rice grains. Whether you carry that bag in Bangalore, take it on a train to Chennai, or even fly it to the Moon, the bag still contains the exact same rice grains. The mass stays at 5 kg no matter where you go in the universe.
Key facts about mass:
- Mass is measured in kilograms (kg)
- Mass is a scalar quantity (it has magnitude only, no direction)
- Mass does not change with location — your mass is the same in Bangalore, on the Moon, or floating in deep space
- Mass is measured using a beam balance (or electronic balance)
- Mass tells you how much an object resists being accelerated (this is called inertia)
"Mass stays, weight strays." Your mass is loyal — it never changes wherever you travel. Your weight is a wanderer — it changes depending on which planet or moon you are on!
What is Weight?
Weight is the gravitational force acting on an object that has mass. It is the force with which a planet, moon, or star pulls an object towards its centre.
Right now, the Earth is pulling you downwards towards its centre. That pull is your weight. If you stood on the Moon, the Moon would pull you much less strongly (because the Moon is smaller and less massive than the Earth), so your weight would be much less.
Key facts about weight:
- Weight is measured in newtons (N) — because weight is a force!
- Weight is a vector quantity (it has both magnitude and direction — always directed towards the centre of the planet)
- Weight changes depending on where you are — it is different on the Earth, Moon, and Jupiter
- Weight is measured using a spring balance (also called a newton meter or force meter)
- Weight depends on two things: the object's mass and the gravitational field strength at that location
Mass vs Weight — The Big Comparison
| Property | Mass | Weight |
|---|---|---|
| What is it? | Amount of matter in an object | Gravitational force on an object |
| Unit | Kilogram (kg) | Newton (N) |
| Type of quantity | Scalar (magnitude only) | Vector (magnitude + direction) |
| Changes with location? | No — same everywhere | Yes — depends on gravitational field strength |
| Measured with | Beam balance / electronic balance | Spring balance (newton meter) |
| Direction | None (scalar) | Always towards the centre of the planet |
| In zero gravity (deep space) | Still the same | Becomes zero |
A very common exam mistake: writing "mass is measured in newtons" or "weight is measured in kilograms." Remember — mass in kg, weight in N. The examiner will give zero marks if you swap the units. Also, never say weight is "the amount of gravity" — always say it is the gravitational force on an object.
Gravitational Field Strength (g)
Gravitational field strength is defined as the force per unit mass. It tells you how strong gravity is at a particular location. On the surface of the Earth, g = 9.8 N/kg. This means every kilogram of mass experiences a gravitational force of 9.8 N.
The equation linking weight, mass, and gravitational field strength is:
You can rearrange this equation to find any of the three quantities:
- g = W / m — to find gravitational field strength
- m = W / g — to find mass
Here are the values of g you need to know:
| Location | g (N/kg) | What it means |
|---|---|---|
| Earth | 9.8 (use 10 if the exam says so) | Every 1 kg has a weight of 9.8 N |
| Moon | 1.6 | About 1/6 of Earth — you would feel very light! |
| Jupiter | 24.8 (approximately 25) | About 2.5 times Earth — you would feel very heavy! |
| Deep space (far from any planet) | ≈ 0 | Weightless — you float! |
Important: The gravitational field strength g is numerically equal to the acceleration of free fall. So g = 9.8 N/kg is the same as g = 9.8 m/s². The units are different because they describe different things (force per unit mass vs acceleration), but the number is the same. When a coconut falls from a tree in your backyard, it accelerates at 9.8 m/s² due to gravity!
Some exam questions use g = 10 N/kg (or 10 m/s²) to make calculations easier. Always check the question — if it says "take g = 10 N/kg," use 10. If it says nothing, use 9.8 N/kg. Read the question carefully!
Worked Examples
(b) On the Moon: W = 50 × 1.6 = 80 N
(c) On Jupiter: W = 50 × 24.8 = 1240 N
Think of the formula triangle: put W on top, and m and g on the bottom side by side. Cover the quantity you want to find:
• Cover W → you see m × g (multiply)
• Cover m → you see W / g (divide)
• Cover g → you see W / m (divide)
Just like the dosa batter triangle — you need all three ingredients to work together!
Comparing Weights and Masses Using a Balance
There are two main types of balances you need to know about:
1. Beam Balance (for comparing masses): A beam balance works by comparing an unknown mass against a set of known masses. You place the object on one pan and add known masses to the other pan until the beam is level. When the beam is balanced, the unknown mass equals the sum of the known masses. A beam balance gives the same reading everywhere — on Earth, on the Moon, or on Jupiter — because both pans are affected equally by gravity.
2. Spring Balance / Newton Meter (for measuring weight): A spring balance works by stretching a spring. The heavier the object, the more the spring stretches. The scale is calibrated in newtons (N). A spring balance gives different readings on different planets because the weight of the object changes when g changes.
Here is an important scenario to understand: Imagine you use a beam balance to measure 1 kg of mangoes at a fruit stall in KR Market. If you take that beam balance and those mangoes to the Moon, the balance will still show 1 kg, because both the mangoes and the 1 kg weight are pulled less by the Moon's gravity — they are still equal. But if you use a spring balance, the mangoes would show only about 1.6 N on the Moon instead of 9.8 N on Earth!
If a question asks "how would the reading change on the Moon?" — the answer depends on the instrument. A spring balance reading would decrease (because weight decreases). A beam balance reading stays the same (because both sides are affected equally by the weaker gravity).
Weight as the Effect of a Gravitational Field on a Mass
Every object that has mass creates a gravitational field around itself. A gravitational field is an invisible region of space where a mass experiences a force. The bigger the mass, the stronger the field.
Think of it like this: the Earth is like a giant magnet for mass. It creates an invisible "zone of pull" all around it. Any object with mass that enters this zone gets pulled towards the Earth's centre. That pull is what we call weight.
The concept works like this:
- The Earth has mass, so it creates a gravitational field around it
- When an object (like a cricket ball) is placed in this field, the field exerts a force on the ball
- This force is the ball's weight
- The strength of this field is called gravitational field strength (g)
- Closer to the Earth's surface, the field is stronger; farther away, it weakens
Imagine you are standing at Lalbagh Botanical Garden. The Earth's gravitational field is pulling you downwards with a certain force. Now imagine you are on top of Mount Everest — you are farther from the Earth's centre, so the field is very slightly weaker, and your weight is very slightly less. But the change is tiny because even Everest's height is small compared to the Earth's radius.
Gravitational field strength g is defined as:
This tells us that g is the force acting on each kilogram of mass. On Earth, g ≈ 9.8 N/kg, meaning every kilogram experiences a pull of 9.8 newtons.
W = m × g = 70 × 1.6 = 112 N
Step 2: What does the scale display?
On Earth, the scale is calibrated so that a weight of 700 N (70 × 10) displays “70 kg.” It divides the force by 10 to show “kg.”
On the Moon, the spring compresses with only 112 N of force. The scale divides by 10 and displays: 112 ÷ 10 = 11.2 kg.
This is WRONG — her mass is still 70 kg! The scale gives a false reading because it was calibrated for Earth’s gravity.
Step 3: Has her mass changed?
No. Mass is a property of matter — she has the same number of atoms whether she’s on Earth, the Moon, or floating in deep space. Her mass is always 70 kg.
Step 4: Pushing the 200 kg module on the Moon.
The module weighs less on the Moon (200 × 1.6 = 320 N vs 200 × 10 = 2000 N on Earth), so it’s easier to lift. But to push it horizontally on a frictionless surface, you still need to overcome its inertia, which depends on mass (200 kg), not weight. The resistance to getting it moving is exactly the same. In practice, if there’s friction, the lower weight means less friction, so it would be somewhat easier to slide.
The beam balance compares the tomatoes on one side with standard 2 kg masses on the other. On Mars, BOTH sides experience the same reduced gravity. The tomatoes pull down with 2 × 3.7 = 7.4 N and the standard masses pull down with 2 × 3.7 = 7.4 N. They still balance! Reading: 2 kg — CORRECT.
Spring balance on Mars:
On Earth, 2 kg of tomatoes weigh 2 × 10 = 20 N, and the scale shows “2 kg.”
On Mars, the same tomatoes weigh 2 × 3.7 = 7.4 N. The spring stretches much less. The scale (calibrated for Earth) divides by 10 and shows: 7.4 ÷ 10 = 0.74 kg — WRONG.
The tomatoes still have a mass of 2 kg, but the spring balance thinks they’re lighter because gravity is weaker.
W = m × g = 0.16 × 10 = 1.6 N throughout the entire flight.
Whether the ball is going up, at its highest point, or coming down, g is still 10 N/kg near Earth’s surface. The ball only rises a few metres — g doesn’t measurably change over such a small height.
What DOES change?
• Velocity changes — the ball slows down as it rises (gravity decelerates it) and speeds up as it falls (gravity accelerates it).
• Direction changes — the ball follows a curved path.
• Kinetic energy converts to gravitational potential energy and back.
But mass, weight, and gravitational field strength all stay the same.
W = m × g, so m = W ÷ g = 500 ÷ 10 = 50 kg
Step 2: Find her weight on Jupiter.
W = m × g = 50 × 25 = 1250 N
Step 3: Could she stand up?
On Jupiter, she would feel like she’s carrying an extra 75 kg on her back (total effective “felt mass” of 125 kg in Earth terms). Her muscles are used to supporting 500 N — now they must support 1250 N, which is 2.5 times her Earth weight. Standing would be extremely difficult. Walking would be nearly impossible. Even breathing would be much harder because her rib cage would feel 2.5 times heavier.
Yes! At 408 km altitude, g ≈ 8.7 N/kg. If the astronaut has a mass of 70 kg, her weight is 70 × 8.7 = 609 N. She definitely has weight.
So why does she float?
The ISS is in free fall around the Earth. It’s falling towards Earth constantly, but it’s moving sideways so fast (~28,000 km/h) that it keeps missing! The astronaut, the ISS, and everything inside are all falling at exactly the same rate.
Think of it this way: imagine you’re in a lift and the cable snaps. You and the lift both fall at the same rate. You’d float inside the lift — not because gravity disappeared, but because the floor is falling away beneath you just as fast as you’re falling. There’s no contact force pushing up on you, so you feel weightless.
This is apparent weightlessness, not true weightlessness.
Tara, have you ever wondered why a small gold earring feels so heavy in your hand, but a big slab of thermocol (polystyrene) feels super light, even though the thermocol is much bigger? The answer is density! Gold packs a huge amount of mass into a tiny volume, while thermocol has very little mass spread out over a large volume. Density is one of the most useful ideas in physics, and it helps explain everything from why oil floats on water in your kitchen to why massive ships made of steel can float on the ocean.
What is Density?
Density is defined as mass per unit volume. It tells you how much mass is packed into each unit of volume. If a material has a high density, it means a lot of mass is squeezed into a small space. If a material has a low density, the mass is spread out over a large space.
You can rearrange this equation to find mass or volume:
- m = ρ × V — to find mass when you know density and volume
- V = m / ρ — to find volume when you know mass and density
The Greek letter ρ (pronounced "rho") is used for density. It is not the letter "p"!
Use the density triangle: put m on top, and ρ and V on the bottom. Cover what you want to find:
• Cover m → ρ × V
• Cover ρ → m / V
• Cover V → m / ρ
Think of it as: "Mangoes Rest on Vines" — M on top, R (ρ) and V on the bottom!
Common Density Values
| Material | Density (kg/m³) | Density (g/cm³) | Everyday Example |
|---|---|---|---|
| Air (at sea level) | 1.2 | 0.0012 | The air you breathe |
| Cork | 240 | 0.24 | Bulletin board material |
| Wood (teak) | 650 | 0.65 | Furniture from your home |
| Coconut oil | 920 | 0.92 | Used for cooking in South India |
| Water | 1 000 | 1.00 | Your drinking water |
| Aluminium | 2 700 | 2.70 | Pressure cooker, idli plates |
| Iron / Steel | 7 800 | 7.80 | Dosa tawa, iron kadai |
| Gold | 19 300 | 19.30 | Gold jewellery from Tanishq |
Unit consistency is critical! If mass is in kg, volume must be in m³ to get density in kg/m³. If mass is in g, volume must be in cm³ to get density in g/cm³. A common mistake is mixing units. Remember: 1 m³ = 1 000 000 cm³ (that is 100 × 100 × 100). Also, the density of water is exactly 1 g/cm³ or 1000 kg/m³ — a very useful reference to remember!
Worked Examples
How to Determine Density Experimentally
The IGCSE exam loves to ask about the practical methods for finding density. There are three scenarios you need to know, Tara. Let us go through each one carefully.
1. Density of a Regularly Shaped Solid (e.g., a metal cuboid)
If the solid has a regular shape (cube, cuboid, cylinder, sphere), you can calculate its volume using measurements and a formula.
Method:
- Measure the mass of the solid using an electronic balance (in grams)
- Measure the dimensions using a ruler or vernier calliper:
- For a cuboid: measure length (l), width (w), and height (h). Volume = l × w × h
- For a cylinder: measure radius (r) and height (h). Volume = πr²h
- For a sphere: measure radius (r). Volume = (4/3)πr³
- Calculate density: ρ = m / V
Example: To find the density of an aluminium idli plate, you could measure its mass on a balance (say 180 g), measure its dimensions with a ruler and calculate the volume (say 72 cm³), then divide: ρ = 180 / 72 = 2.5 g/cm³.
2. Density of an Irregularly Shaped Solid that Sinks in Water (e.g., a stone idol)
If the solid has an irregular shape (like a stone Ganesha idol, a pebble, or a metal key), you cannot calculate its volume from measurements. Instead, you use the displacement method.
Method:
- Measure the mass of the object using an electronic balance
- Fill a measuring cylinder partially with water and record the initial water level (V₁)
- Gently lower the object into the water using a thin string (so it does not splash). The water level rises.
- Record the new water level (V₂)
- Volume of the object = V₂ − V₁ (this is the volume of water displaced)
- Calculate density: ρ = m / (V₂ − V₁)
Why does this work? When you submerge the object, it pushes aside (displaces) a volume of water exactly equal to its own volume. The rise in water level tells you the volume of the object. This is the same idea that Archimedes discovered in his bathtub — and shouted "Eureka!"
When describing the displacement method in an exam, always mention: (1) use a measuring cylinder, (2) record the initial water level, (3) gently lower the object (to avoid splashing), (4) record the new water level, (5) subtract to find volume. If the object is too large for a measuring cylinder, you can use a displacement can (eureka can) instead — the overflow water is collected and its volume measured.
3. Density of a Liquid
Method:
- Place an empty measuring cylinder on an electronic balance and record its mass (m₁). Alternatively, you can "tare" (zero) the balance with the empty cylinder on it.
- Pour a known volume of the liquid into the measuring cylinder. Read the volume (V) at the bottom of the meniscus at eye level.
- Record the new mass of the cylinder + liquid (m₂)
- Mass of the liquid = m₂ − m₁
- Calculate density: ρ = (m₂ − m₁) / V
Example: To find the density of coconut oil, you could measure an empty measuring cylinder (50 g), pour 100 cm³ of coconut oil into it, and weigh again (142 g). Mass of oil = 142 − 50 = 92 g. Density = 92 / 100 = 0.92 g/cm³.
When reading the volume of a liquid in a measuring cylinder, always read from the bottom of the meniscus (the curved surface of the liquid). Your eye should be at the same level as the meniscus to avoid parallax error. This is a favourite question topic!
Floating and Sinking
Here is the golden rule for floating and sinking, Tara:
- If the object's density is less than the liquid's density → the object floats
- If the object's density is greater than the liquid's density → the object sinks
- If the object's density is equal to the liquid's density → the object stays wherever you place it (neutral buoyancy)
Real-life examples:
- A coconut floats in water because its overall density (including the air inside) is less than 1 g/cm³
- An iron kadai sinks in water because iron has a density of 7.8 g/cm³, which is much greater than water's 1.0 g/cm³
- Coconut oil floats on water because its density (0.92 g/cm³) is less than water (1.0 g/cm³) — you can see this when a drop of coconut oil sits on top of water in a glass
- A wooden log floats in a river because wood (like teak at 0.65 g/cm³) is less dense than water
"Less dense, goes up — More dense, goes down." Think of it like a crowded BMTC bus: if you are lighter (less dense), you get pushed upward by the crowd. If you are heavier (more dense), you sink to the bottom. The lighter material always floats on top of the denser material!
Liquids Floating on Liquids
The same floating and sinking rule applies to liquids! If you carefully pour different liquids into a tall glass, they will arrange themselves in layers based on density. The least dense liquid floats on top, and the most dense liquid sinks to the bottom.
Example from your kitchen: If you pour honey, water, and coconut oil into a glass, they will form three layers:
- Top layer: Coconut oil (ρ = 0.92 g/cm³) — least dense, floats
- Middle layer: Water (ρ = 1.00 g/cm³)
- Bottom layer: Honey (ρ ≈ 1.42 g/cm³) — most dense, sinks
This also explains why when you mix oil and water, the oil always rises to the top — no matter how much you shake the mixture, the oil floats because it is less dense. You can see this in your amma's kitchen when she makes tadka (tempering)!
Next: Water (1.00 g/cm³)
Next: Mustard oil (0.91 g/cm³)
Top: Kerosene (0.82 g/cm³)
This is more dense than kerosene (0.82) — so it sinks through kerosene.
But it is less dense than mustard oil (0.91) — so it floats on mustard oil.
Human body density ≈ 1010 kg/m³. Since 1010 > 1000, the body is denser than freshwater — so you sink (or barely float if you fill your lungs with air, which lowers your average density).
In the Dead Sea (ρ = 1240 kg/m³):
Human body density ≈ 1010 kg/m³. Since 1010 < 1240, the body is less dense than the Dead Sea water — so you float easily. In fact, you float so high that a large portion of your body sticks out above the surface!
How high do you float?
The fraction submerged = body density ÷ liquid density = 1010 ÷ 1240 ≈ 0.81. So about 81% of your body is underwater and 19% sticks out — that’s why people can sit up and read a newspaper in the Dead Sea!
Mass = 50 g = 0.050 kg
Volume = 4.5 cm³ = 4.5 × 10⁻⁶ m³ (since 1 cm³ = 1 × 10⁻⁶ m³)
Step 2: Calculate density.
ρ = m ÷ V = 0.050 ÷ (4.5 × 10⁻⁶) = 11,111 kg/m³
Or more simply in g/cm³: 50 ÷ 4.5 = 11.1 g/cm³
Step 3: Compare to gold.
Gold: 19,300 kg/m³ (19.3 g/cm³)
This chain: 11,111 kg/m³ (11.1 g/cm³)
It is NOT real gold! The density is far too low.
Step 4: What could it be?
Lead has a density of about 11,340 kg/m³ (11.3 g/cm³) — very close to our calculated value. The chain is likely made of lead (possibly gold-plated to look real).
Mass of cold air = ρ × V = 1.225 × 2800 = 3430 kg
Step 2: Find the buoyancy force (weight of displaced cold air).
Buoyancy = m × g = 3430 × 10 = 34,300 N
Step 3: Find the weight of the hot air inside.
Mass of hot air = 1.097 × 2800 = 3071.6 kg
Weight of hot air = 3071.6 × 10 = 30,716 N
Step 4: Find the net upward force.
Net force = Buoyancy − Weight of hot air = 34,300 − 30,716 = 3584 N
Step 5: Maximum payload.
This 3584 N of net lift must support the basket, burner, envelope fabric, AND passengers.
Maximum payload mass = 3584 ÷ 10 = 358.4 kg
That’s enough for about 4–5 people plus equipment.
A solid ball is 100% steel. Its density is 7800 kg/m³, which is much greater than water (1000 kg/m³). Since object density > liquid density, it sinks.
Why does a steel ship float?
A ship is a hollow shell of steel filled with air. Air has a density of only about 1.2 kg/m³. The average density of the ship (steel + air + cargo + everything inside) is calculated using the total mass divided by the total volume of the hull. This average density works out to be less than 1000 kg/m³, so the ship floats.
Volume of water displaced:
For the ship to float, the weight of water displaced must equal the weight of the ship.
Mass of ship = 50,000 tonnes = 50,000,000 kg
Mass of water displaced = 50,000,000 kg
Volume = mass ÷ density = 50,000,000 ÷ 1000 = 50,000 m³
1. Honey (1400 kg/m³) — bottom
2. Water (1000 kg/m³)
3. Vegetable oil (920 kg/m³)
4. Rubbing alcohol (790 kg/m³) — top
Now for each solid object:
Grape (1100 kg/m³): Denser than water (1000) but less dense than honey (1400). It sinks through alcohol, oil, and water, but floats on honey. It settles at the water–honey boundary.
Cherry tomato (950 kg/m³): Denser than oil (920) but less dense than water (1000). It sinks through alcohol and oil, but floats on water. It settles at the oil–water boundary.
Cork (120 kg/m³): Less dense than all four liquids (even rubbing alcohol at 790). It floats right on top of the rubbing alcohol at the very surface.
Forces are everywhere in your life, Tara! Every time a BMTC bus brakes, every time a cricket ball is hit for a six, every time you open a door or sit on a see-saw, forces are at work. In this section, you will learn what forces do, how to calculate them, and how objects stay balanced. Let us start!
1.5.1 Effects of Forces
What Can Forces Do?
A force is a push or a pull that acts on an object. Forces are measured in newtons (N). You cannot see a force directly, but you can always see what it does. A force can cause three effects on an object:
- Change the speed of an object — speed it up or slow it down. When a BMTC bus driver presses the accelerator, the engine force speeds the bus up. When the driver hits the brakes, friction slows it down.
- Change the direction of an object — even if the speed stays the same. When a cricket batsman hits the ball, the bat pushes the ball in a completely new direction. The ball was coming towards the batsman but now flies away towards the boundary.
- Change the shape of an object — squash it, stretch it, bend it, or twist it. When you sit on a sofa cushion at home, your weight force compresses the cushion and changes its shape. When you stretch a rubber band, the pulling force changes its shape.
When the exam asks "describe the effects of a force," always mention all three: change in speed, change in direction, and change in shape. If you write just one, you lose marks!
Types of Forces
There are many different types of forces. You need to know each one and be able to identify them in diagrams and real-life situations. Let us go through them one by one:
| Force | What It Is | Indian Example | Contact or Non-Contact? |
|---|---|---|---|
| Friction | A force that opposes (resists) motion between two surfaces that are touching and sliding past each other | The brake pads on a BMTC bus grip the wheel — friction between the pads and the wheel slows the bus down | Contact |
| Air Resistance (Drag) | Friction between an object and the air it moves through. It opposes the direction of motion through air. | When you stick your hand out of a moving auto-rickshaw, you feel the air pushing your hand back — that is air resistance | Contact |
| Tension | The pulling force in a stretched rope, wire, cable, or string | During tug of war at your school sports day, both teams pull the rope. The rope is under tension. | Contact |
| Normal Contact Force | The support force that a surface pushes back with when an object sits on it. It acts perpendicular (at 90°) to the surface. | Your physics textbook sits on your desk. The desk pushes up on the book with a normal contact force, preventing it from falling through. | Contact |
| Upthrust | The upward force that a liquid or gas exerts on an object submerged (or partially submerged) in it | When you float in a swimming pool, the water pushes you upward. That upward push is upthrust. | Contact |
| Weight (Gravitational Force) | The force of gravity pulling an object towards the centre of the Earth. Weight = mass × gravitational field strength (W = mg). | A 1 kg bag of rice weighs about 10 N on Earth, because the Earth pulls it downward with a gravitational force | Non-contact |
| Electric Force | The force between electrically charged objects. Like charges repel, opposite charges attract. | After rubbing a plastic comb on your hair, the comb can pick up small pieces of paper — that is the electric force | Non-contact |
| Magnetic Force | The force between magnets or between a magnet and a magnetic material (iron, cobalt, nickel) | Fridge magnets stick to the steel fridge door without touching — magnetic force pulls them | Non-contact |
| Nuclear Force | The strong force that holds protons and neutrons together inside the nucleus of an atom. It only acts over extremely tiny distances. | The reason the Sun shines and nuclear power plants work — nuclear forces hold the nuclei of atoms together | Non-contact |
Contact Forces vs Non-Contact Forces
The forces in the table above fall into two categories:
- Contact forces require the objects to be physically touching. Friction, air resistance, tension, normal contact force, and upthrust are all contact forces. The objects must be in physical contact for these forces to act.
- Non-contact forces can act across a distance, even through empty space. Gravitational, electric, magnetic, and nuclear forces are non-contact forces. They do not need the objects to be touching.
To remember the non-contact forces, think: G.E.M.N. — Gravitational, Electric, Magnetic, Nuclear. Everything else is a contact force.
Weight is NOT the same as mass! Mass is the amount of matter in an object (measured in kg). Weight is the gravitational force pulling that mass down (measured in N). A 50 kg person has a weight of about 500 N on Earth.
More everyday Indian examples of each force type:
- Friction: When you rub your hands together on a cold Bangalore winter morning to warm them up, friction between your palms generates heat. When a BMTC bus brakes suddenly, friction between the tyres and the road is what actually stops the bus.
- Air resistance: When you cycle to school, you feel the wind pushing against your face. The faster you pedal, the stronger the air resistance becomes. This is why professional cyclists crouch low — to reduce air resistance.
- Tension: When your mother hangs wet clothes on a clothesline, the weight of the wet clothes pulls the line down. The line stretches slightly and the pulling force inside the rope is tension. The heavier the clothes, the greater the tension in the line.
- Normal contact force: Right now, the chair you are sitting on pushes you upward with a normal contact force. If it did not, you would fall straight through the chair! This force is always perpendicular (at 90°) to the surface.
- Upthrust: If you have ever tried to push a beach ball underwater in a swimming pool, you felt the water pushing it back up very strongly. That upward push from the water is upthrust. It is also what keeps boats floating.
Free-Body Diagrams
A free-body diagram shows all the forces acting on a single object, drawn as arrows. Each arrow starts from the object and points in the direction the force acts. The length of the arrow shows the size (magnitude) of the force — a longer arrow means a bigger force.
Here is an example: a book sitting on a desk. There are exactly two forces acting on it:
Rules for drawing free-body diagrams:
- Draw the object as a simple box or dot.
- Draw each force as an arrow starting from the object.
- Label every arrow with the name of the force and, if known, its value in newtons.
- Make the arrow length proportional to the force size — bigger forces get longer arrows.
- Only include forces acting on the object, not forces the object exerts on other things.
Here is a more complex example: a Namma Metro train accelerating along the track.
Resultant Force
When more than one force acts on an object, we can combine them into a single force called the resultant force. The resultant force is the overall (net) effect of all the individual forces acting on the object.
Forces in the same direction: add them together.
Forces in opposite directions: subtract the smaller from the larger. The resultant force points in the direction of the larger force.
Think of resultant force like a tug of war: if one side pulls harder, that side wins. The resultant is the difference, and it acts in the direction of the stronger side.
Resultant Force and Acceleration
If the resultant force on an object is not zero, the object will accelerate (change its velocity). The acceleration happens in the direction of the resultant force.
- If the resultant force is in the direction of motion, the object speeds up.
- If the resultant force is opposite to the direction of motion, the object slows down (decelerates).
- If the resultant force is at an angle to the direction of motion, the object changes direction.
This is described by Newton's Second Law, which gives us one of the most important equations in all of physics:
This equation tells us: the bigger the resultant force, the bigger the acceleration. And the bigger the mass, the smaller the acceleration (heavier objects are harder to speed up).
You can rearrange this equation three ways:
- F = m × a — to find the force
- a = F / m — to find the acceleration
- m = F / a — to find the mass
The F in F = ma is the resultant force, not just any single force! If you are given multiple forces, you must find the resultant first, then use F = ma. Also, make sure mass is in kg and acceleration is in m/s² before you calculate.
1.5.2 Turning Effect of Forces
What Is a Moment?
Have you ever tried to open a heavy door? You probably pushed near the handle, far from the hinges. If you tried pushing near the hinges instead, you would need a much bigger force — the door barely moves! This is because of the turning effect of a force, which we call the moment of the force.
The moment of a force is a measure of its ability to make an object rotate (turn) about a point called the pivot (or fulcrum). The moment depends on two things:
- The size of the force — a bigger force creates a bigger turning effect.
- The perpendicular distance from the pivot to the line of action of the force — the farther from the pivot, the bigger the turning effect.
Important: The distance must be the perpendicular (at right angles) distance from the pivot to the line along which the force acts. If the force is applied at an angle, only the perpendicular component counts.
The Principle of Moments
The principle of moments states:
For a body in equilibrium (balanced), the sum of the clockwise moments about any point equals the sum of the anticlockwise moments about that same point.
In simpler words: if a see-saw is balanced, the turning effect pushing it clockwise equals the turning effect pushing it anticlockwise. They cancel each other out exactly.
Child B creates a clockwise moment: 500 × d
d = 800 / 500 = 1.6 m
1 N weight is at 30 cm, so distance = 50 − 30 = 20 cm = 0.20 m (left side, anticlockwise)
W is at 80 cm, so distance = 80 − 50 = 30 cm = 0.30 m (right side, clockwise)
W × 0.30 = (2 × 0.30) + (1 × 0.20)
W × 0.30 = 0.60 + 0.20 = 0.80
Tara pushes at the other end: 3.0 − 0.5 = 2.5 m from pivot (creates anticlockwise moment).
F × 2.5 = 300
Always convert distances to metres before calculating moments! If you are given 30 cm, convert it to 0.30 m. Moments must be in Nm (newton-metres), not N×cm.
Moments with Forces in More Than One Direction
Sometimes forces do not all act vertically. In these cases, you must use the perpendicular distance from the pivot to the line of action of the force.
The line of action is an imaginary line extending along the direction of the force. The perpendicular distance is the shortest distance from the pivot to this line, measured at right angles (90°).
For example, if you push a door at an angle instead of straight on, the effective moment is reduced because the perpendicular distance from the hinge to the line of push is shorter.
The 30 N horizontal force acts at the end of the beam. Since the beam is horizontal and this force is horizontal, its line of action passes through all points at the same height. The perpendicular distance from the pivot to this horizontal line is 0 m (the force acts along the beam direction, but since the force is horizontal and the beam is horizontal, the perpendicular distance is actually the vertical distance, which is 0 m — so this force creates no moment about the pivot if the pivot and the point of application are at the same height).
Moment of 30 N force = 30 × 0 = 0 Nm (since perpendicular distance from pivot is zero for this horizontal force acting along the line of the beam)
Perpendicular distance = 1.5 m
Clockwise moment = 200 × 1.5 = 300 Nm
Anticlockwise moment = 300 × 1.2 = 360 Nm
1.5.3 Conditions for Equilibrium
What Does Equilibrium Mean?
An object is in equilibrium when it is completely balanced — it is not accelerating and it is not rotating. Think of a book sitting still on your study desk, or a balanced see-saw with nobody going up or down.
For an object to be in equilibrium, two conditions must be met at the same time:
- The resultant force must be zero. All the forces cancel each other out — the total force in every direction adds up to zero. This means the object will not start moving or speed up.
- The resultant moment about any point must be zero. All the clockwise moments equal all the anticlockwise moments. This means the object will not start rotating.
Both conditions must be true at the same time! If the forces balance but the moments do not, the object will spin. If the moments balance but the forces do not, the object will move. For true equilibrium, you need both.
Centre of Gravity
The centre of gravity of an object is the single point where all of its weight appears to act. You can think of it as the "balance point" of the object.
- For a regular, uniform object (like a ruler, a brick, or a ball), the centre of gravity is at the geometric centre.
- For an irregular object (like an oddly shaped piece of cardboard), the centre of gravity might not be at an obvious point — you need to find it experimentally.
- The centre of gravity does not have to be inside the object! For example, the centre of gravity of a ring-shaped bangle is at the centre of the ring, where there is no material.
Finding the Centre of Gravity of an Irregular Shape (Plumb Line Method)
Here is a simple experiment to find the centre of gravity of a thin, flat, irregular piece of card:
- Make a small hole near one edge of the card.
- Hang the card from a pin through the hole so it can swing freely.
- Hang a plumb line (a string with a small weight, like a heavy nut) from the same pin. Wait for it to stop swinging.
- Draw a line on the card along the plumb line string. The centre of gravity lies somewhere on this line.
- Repeat from a different hole — make another hole in a different edge, hang the card again, and draw a second line along the plumb line.
- The centre of gravity is at the point where the two lines cross (intersect). You can do it a third time to check — all three lines should meet at the same point.
Think of balancing a cardboard cutout on your fingertip. The one point where it balances perfectly — that is the centre of gravity! The plumb line method just finds this point using gravity itself.
Centre of Gravity and Stability
The position of the centre of gravity affects how stable an object is — that is, how easily it topples over.
Three rules of stability:
- A lower centre of gravity makes an object more stable. This is why a BMTC bus (heavy engine low down) is more stable than an auto-rickshaw (higher centre of gravity). The bus is harder to tip over.
- A wider base makes an object more stable. A pyramid shape is very stable because it has a wide base. A tall, thin object like a cricket stump is easy to knock over because it has a narrow base.
- An object topples when its centre of gravity moves beyond the edge of its base. As long as a vertical line from the centre of gravity falls within the base, the object is stable. The moment the line falls outside the base, the object tips over.
Real-life Indian examples:
- A BMTC bus has a low centre of gravity (heavy engine underneath) and a wide wheelbase — very stable, rarely tips over.
- An auto-rickshaw is narrower and has a higher centre of gravity — it can feel tippy when turning sharp corners in Bangalore traffic!
- A matka (clay water pot) is round at the bottom and must be placed on a ring stand. Without the stand, it rolls and topples because its centre of gravity is above a tiny contact point.
- Stacking steel tiffin boxes — when you stack too many, the centre of gravity rises and eventually the stack topples. If you put the heaviest box at the bottom, the centre of gravity stays lower and the stack is more stable.
- During Dasara/Dussehra celebrations, tall Ravan effigies are very unstable because they have a high centre of gravity. They need thick, heavy bases and guy ropes to stay upright.
Explaining Stability Using Centre of Gravity and Pivot Point
When you tilt an object, you are effectively rotating it about the edge of its base (which becomes the pivot point). Here is what happens:
- When you start tilting, the centre of gravity rises slightly. The weight of the object still acts downward through the centre of gravity.
- As long as the vertical line from the centre of gravity falls within the base, the weight creates a restoring moment that pushes the object back to its upright position. The object is stable.
- If you tilt it far enough that the vertical line from the centre of gravity falls beyond the edge of the base (beyond the pivot point), the weight now creates a toppling moment that tips the object further over. The object is unstable and will fall.
Why is a low centre of gravity more stable? Because you need to tilt the object through a larger angle before the centre of gravity passes over the edge of the base. With a higher centre of gravity, even a small tilt can move the line of weight outside the base.
Why is a wider base more stable? Because the edge of the base is farther from the centre, so the centre of gravity needs to move a greater horizontal distance to get beyond the base edge. A wider base gives more room.
Indian example: Imagine a loaded bullock cart. If the load is stacked very high, the centre of gravity is high and the cart might topple on a sloping road. If the load is kept low and spread wide, the cart is much more stable. This is exactly why Indian truck drivers are told to distribute heavy loads low and evenly!
When answering stability questions in the exam, always mention three things: (1) the position of the centre of gravity, (2) the width of the base, and (3) whether the vertical line from the CG falls within or outside the base. This structure gets you full marks.
Remember "Low and Wide = Stable Pride": a low centre of gravity and a wide base make an object stable and hard to topple. Think of a pyramid — it has been standing for thousands of years!
Key Formulas Summary for 1.5
| Formula | What It Calculates | Units |
|---|---|---|
| Resultant = sum of forces (with direction) | The overall net force on an object | Newtons (N) |
| F = m × a [Supplement] | Resultant force from mass and acceleration | N = kg × m/s² |
| Moment = F × d | Turning effect of a force about a pivot | Nm = N × m |
| Clockwise moments = Anticlockwise moments | Condition for rotational equilibrium (balance) | Nm = Nm |
Unit conversions to remember: Always convert cm to m before using in moment calculations (divide by 100). Always convert g to kg before using in F = ma (divide by 1000). Forgetting unit conversions is the most common reason students lose marks in forces questions!
Constant speed means the resultant force is zero.
So: driving force = friction force
Friction force = 8000 N
Part 2: Find the resultant force when the engine force increases.
The friction force doesn’t change suddenly — it stays at 8000 N.
Resultant force = driving force − friction force
Resultant force = 10,000 − 8000 = 2000 N (forward)
Part 3: Find the acceleration.
F = ma, so a = F ÷ m
a = 2000 ÷ 12,000 = 0.167 m/s² (to 3 s.f.)
Clockwise moment (load) = Anticlockwise moment (worker)
600 × 0.4 = F × 1.2
240 = 1.2F
F = 240 ÷ 1.2 = 200 N
Part 2: Load moved closer (0.3 m from pivot).
600 × 0.3 = F × 1.2
180 = 1.2F
F = 180 ÷ 1.2 = 150 N
The required force decreases from 200 N to 150 N when the load is moved closer to the pivot.
2 kg → 4 cm (extension per 2 kg = 4 cm)
4 kg → 8 cm (extension per 2 kg = 4 cm) ✅
6 kg → 12 cm (extension per 2 kg = 4 cm) ✅
8 kg → 16 cm (extension per 2 kg = 4 cm) ✅
10 kg → 22 cm (extension per 2 kg = 6 cm) ❌
The spring obeys Hooke’s Law up to 8 kg (up to a force of 8 × 10 = 80 N).
Step 2: Find the spring constant (using data within Hooke’s Law range).
Convert units: at 2 kg, F = 2 × 10 = 20 N, extension = 4 cm = 0.04 m
k = F ÷ x = 20 ÷ 0.04 = 500 N/m
Step 3: What happened at 10 kg?
The spring extended more than expected (22 cm instead of the predicted 20 cm). This means the spring has passed its limit of proportionality — the spring is being permanently deformed and will not return to its original length.
Support A is at position 0 m. Support B is at position 4 m.
Plank weight (200 N) acts at centre = 2 m from A.
Painter (700 N) stands at 1 m from A.
Step 2: Take moments about support A (to find force at B).
Clockwise moments = Anticlockwise moments
(Weight of plank × distance from A) + (Weight of painter × distance from A) = FB × 4
(200 × 2) + (700 × 1) = FB × 4
400 + 700 = 4FB
1100 = 4FB
FB = 1100 ÷ 4 = 275 N
Step 3: Find force at A using equilibrium.
Total upward forces = Total downward forces
FA + FB = 200 + 700
FA + 275 = 900
FA = 900 − 275 = 625 N
The forces act in opposite directions, so we subtract.
Resultant force = 2500 − 2400 = 100 N to the left (towards Team A)
Step 2: Find the acceleration.
F = ma, so a = F ÷ m
a = 100 ÷ 5 = 20 m/s² to the left
Hey Tara! This entire section on momentum is Supplement (Extended) content, which means it appears on your Paper 4 exam. Momentum is one of the most satisfying topics in physics because once you understand it, you can predict what happens in collisions — from cricket balls hitting bats to cars crashing on Bangalore roads. Let us dive in!
What is Momentum?
Imagine two things coming towards you: a cricket ball bowled by Jasprit Bumrah at 140 km/h, and a heavy BMTC bus moving slowly at 5 km/h. Both feel dangerous, right? That is because both have a lot of momentum. Momentum depends on two things: how heavy something is (mass) and how fast it is moving (velocity).
Momentum is a measure of how hard it is to stop a moving object. A heavier object or a faster object has more momentum. Think of it as the "unstoppability" of an object.
Key point: Momentum is a vector quantity — it has both size and direction. If an object moves to the right, its momentum is positive. If it moves to the left, its momentum is negative. This becomes very important in collision problems!
"Please Move the Van" — p = m × v. The letter p stands for momentum (because m was already taken by mass!).
Impulse
When a force acts on an object for some time, it changes the object's momentum. This change is called impulse. Think about a cricket batsman — the longer the bat stays in contact with the ball (bigger Δt), and the harder the batsman hits (bigger F), the more the ball's momentum changes.
Why do we care about impulse? It explains why catching a cricket ball hurts less if you pull your hands back! By increasing the time (Δt) over which you stop the ball, you reduce the force (F) on your hands. Same change in momentum, but spread over more time = less force = less pain!
Impulse is the SAME as change in momentum. The units kg m/s and N s are equivalent. In exams, you might see either one — they mean the same thing!
Conservation of Momentum
This is one of the most powerful ideas in all of physics! Here is the rule:
In any collision (or explosion), the total momentum before = total momentum after, as long as no external forces act on the system.
Think about playing carrom. When the striker hits a coin, the striker slows down (loses momentum) and the coin speeds up (gains momentum). The total momentum of striker + coin stays the same! Momentum is simply transferred from one object to the other.
"Momentum is like money — it cannot be created or destroyed, only transferred!" In a collision, one object gives momentum to the other, just like paying money from one pocket to another. The total stays the same.
Types of Collisions
| Property | Elastic Collision | Inelastic Collision |
|---|---|---|
| Momentum conserved? | Yes | Yes |
| Kinetic energy conserved? | Yes | No (some converted to heat/sound) |
| Objects after collision | Bounce apart | May stick together |
| Example | Carrom striker hitting coin | Two cars crashing and sticking together |
0.005v₂ = 0.015
v₂ = 0.015 ÷ 0.005 = 3 m/s
p(after) = 1,600 × v
v = 4,000 ÷ 1,600 = 2.5 m/s
Remaining rocket mass = 0.5 − 0.05 = 0.45 kg
p(rocket) = 0.45 × v
0.45v = 5
v = 5 ÷ 0.45 = 11.1 m/s upwards
Force and Rate of Change of Momentum
Newton's Second Law can also be written using momentum. The resultant force on an object equals the rate of change of its momentum:
This is actually the original way Newton wrote his second law! F = ma is a special case of this when mass stays constant.
Real-world application: This is why cars have crumple zones and airbags. In a crash, Δp (change in momentum) is fixed — the car goes from moving to stopped. By making the crumple zone collapse slowly (increasing Δt), the force F on passengers is reduced. Same idea as catching a cricket ball with soft hands!
The formula F = Δp/Δt and the impulse formula FΔt = Δp are the SAME equation, just rearranged. In exams, choose whichever version is easier for the question you are given.
Common exam question: "Explain why airbags/crumple zones/helmets reduce injury." Answer: They increase the time over which momentum changes (Δt increases), so the force on the person decreases (F = Δp/Δt). Always mention: same change in momentum, longer time, smaller force.
Momentum of train = m × v = 50,000 × 20 = 1,000,000 kg m/s
Momentum of wagon = 30,000 × 0 = 0 kg m/s (stationary)
Total momentum before = 1,000,000 + 0 = 1,000,000 kg m/s
Step 2: After the collision, they move together.
Combined mass = 50,000 + 30,000 = 80,000 kg
Total momentum after = combined mass × v
1,000,000 = 80,000 × v
Step 3: Solve for v.
v = 1,000,000 ÷ 80,000 = 12.5 m/s
Let’s say “away from the bat” (the direction the ball leaves) is positive.
So: initial velocity u = −40 m/s (towards the bat = negative)
Final velocity v = +50 m/s (away from the bat = positive)
Step 2: Calculate the change in momentum.
Δp = m × v − m × u = m(v − u)
Δp = 0.16 × (50 − (−40))
Δp = 0.16 × 90 = 14.4 kg m/s
Step 3: Calculate the average force.
F = Δp ÷ Δt = 14.4 ÷ 0.005 = 2880 N
Step 2: Total momentum after must also = 0.
Mass of remaining rocket = 0.2 − 0.05 = 0.15 kg
Momentum of gas (downward) = 0.05 × 80 = 4 kg m/s (downward)
Momentum of rocket (upward) = 0.15 × v (upward)
Step 3: Set total momentum = 0.
0.15v (up) − 4 (down) = 0
0.15v = 4
v = 4 ÷ 0.15 = 26.7 m/s upward
Why does it keep accelerating?
The rocket continues to burn fuel and expel gas. Each burst of gas provides another “push” (impulse). As fuel burns away, the rocket gets lighter, so the same force produces an even greater acceleration (F = ma — smaller m means bigger a).
Δp = m × v − m × u = 1200 × 0 − 1200 × 15 = −18,000 kg m/s
The magnitude of the change = 18,000 kg m/s
Step 2: Rigid car (stops in 0.05 s).
F = Δp ÷ Δt = 18,000 ÷ 0.05 = 360,000 N
Step 3: Car with crumple zones (stops in 0.3 s).
F = Δp ÷ Δt = 18,000 ÷ 0.3 = 60,000 N
The crumple zone reduces the force by a factor of 6!
360,000 ÷ 60,000 = 6 times less force on the passengers.
p(before) = (400 × 10) + (350 × 0) = 4000 + 0 = 4000 kg m/s
Step 2: Total momentum after (must equal 4000 kg m/s).
p(after) = (400 × 3) + (350 × v)
4000 = 1200 + 350v
350v = 2800
v = 2800 ÷ 350 = 8 m/s
Step 3: Check kinetic energy.
KE before = ½ × 400 × 10² = ½ × 400 × 100 = 20,000 J
KE after = (½ × 400 × 3²) + (½ × 350 × 8²)
KE after = (½ × 400 × 9) + (½ × 350 × 64)
KE after = 1800 + 11,200 = 13,000 J
KE before (20,000 J) ≠ KE after (13,000 J)
Kinetic energy is NOT conserved — 7000 J was converted to heat, sound, and deformation. This is an inelastic collision.
1.7.1 Energy Stores
Energy is the ability to do work. It cannot be seen directly, but we can see its effects — things moving, heating up, glowing, or growing. Energy comes in many forms, which physicists call energy stores. Think of energy stores like different kinds of bank accounts — the money (energy) is stored differently but it's all still money!
The IGCSE syllabus lists exactly 8 energy stores. Learn them all! Questions often ask you to identify which energy store is involved in a situation. Remember: energy is always stored somewhere and transferred from one store to another.
The 8 Energy Stores
| Energy Store | What It Means | Indian Examples | Symbol / Formula |
|---|---|---|---|
| Kinetic | Energy stored in moving objects — anything that moves has kinetic energy. The faster it moves or the more mass it has, the more kinetic energy it stores. | Namma Metro train moving through Bangalore; a cricket ball bowled by Jasprit Bumrah; a BMTC bus on MG Road; you running to catch an auto-rickshaw | Ek = ½mv² |
| Gravitational Potential | Energy stored in an object because of its height above the ground. The higher up it is, the more it has. It's "potential" because it has the potential to fall. | Water stored behind the Tehri Dam in Uttarakhand; a coconut at the top of a palm tree in Kerala; a book on a shelf; water in an overhead tank on a rooftop in Koramangala | ΔEp = mgΔh |
| Chemical | Energy stored in chemical bonds between atoms. Released during chemical reactions (burning, digestion, battery discharge). | LPG cylinder used for cooking; food like dosas and idlis (which give you energy to study!); a car battery; coal from Jharkhand; petrol in a two-wheeler; a torch battery | — |
| Elastic (Strain) | Energy stored in a stretched or compressed object. When you stretch or squash something elastic, it stores energy that it releases when it returns to its original shape. | A stretched rubber catapult (gulel) used by children; the compressed spring inside a ballpoint pen; a stretched rubber band; the bent bow in archery at the Olympics | — |
| Nuclear | Energy stored in the nucleus (centre) of atoms. Released during nuclear fission (splitting heavy atoms) or nuclear fusion (joining light atoms). This is an enormous amount of energy from a tiny amount of matter. | Uranium fuel rods at the Kudankulam Nuclear Power Plant in Tamil Nadu; the Sun (which uses nuclear fusion); nuclear fuel at Tarapur Atomic Power Station | E = mc² |
| Thermal | Energy stored in the random movement of particles inside a substance. The hotter something is, the more thermal energy it stores. Also called internal energy or heat energy. | A hot cup of chai; a hot tawa (griddle) after making rotis; the hot engine of a motorcycle; hot water in a geyser; the surface of a road on a hot Bangalore afternoon | — |
| Electrostatic | Energy stored in separated electric charges. When positive and negative charges are separated, they have the potential to come together, releasing energy. | Electric charges stored in storm clouds before a lightning strike over the Western Ghats; a charged capacitor in a circuit; static electricity when you rub a balloon on your hair | — |
| Magnetic | Energy stored in a magnetic field. Two magnets that repel or attract each other store magnetic energy in the space between them. | A fridge magnet holding a child's drawing; an electromagnet in the Namma Metro's electric motor; the magnetic field in a loudspeaker; MRI machines in hospitals like Manipal Hospital | — |
Remember the 8 energy stores with: "King George Can Eat Nuclear Toast Every Morning"
Kinetic | Gravitational potential | Chemical | Elastic | Nuclear | Thermal | Electrostatic | Magnetic
Conservation of Energy
This is one of the most important principles in all of physics. Here it is:
Let's see this with some Indian examples of energy transfers:
| Situation | Energy Transfer | Energy "Lost" To |
|---|---|---|
| Burning wood in a chulha (wood stove) | Chemical → Thermal + Light | Thermal energy in surroundings (smoke, heated air) |
| Namma Metro accelerating from a station | Electrical → Kinetic + Thermal (friction) | Thermal energy in rails and brake pads |
| Coconut falling from a palm tree | Gravitational potential → Kinetic | Thermal + Sound when it hits the ground |
| Charging your phone | Electrical → Chemical (stored in battery) | Thermal energy (phone gets warm while charging) |
| Water flowing from Tehri Dam to turbines | Gravitational potential → Kinetic → Electrical | Thermal (friction in turbines and generators) |
| Lighting a diya (oil lamp) during Diwali | Chemical → Thermal + Light | Thermal energy in surrounding air |
In exams, when you write an energy transfer, always go from the source store to the destination store using an arrow (→). For example: "Chemical energy in petrol → Kinetic energy of car + Thermal energy (wasted)". Always mention wasted thermal energy — it shows the examiner you understand conservation of energy!
Kinetic Energy Formula
We can calculate exactly how much kinetic energy a moving object has using this formula:
Think of it as: "Half a Mass of Velocity squared". The ½ is because kinetic energy is derived from the work-energy theorem using calculus — but for your exam, just remember the formula! Notice that speed (v) is squared, which means speed has a BIG effect on kinetic energy.
Speed of bus: v = 15 m/s
Find: Kinetic energy Ek = ?
Ek = ½ × 8000 × 225
Ek = 4000 × 225
Ek = 900,000 J
Speed 1: v1 = 40 m/s
Speed 2: v2 = 20 m/s
Find: Ek at each speed
Ek = ½ × 0.16 × 1600
Ek = 0.08 × 1600 = 128 J
Ek = ½ × 0.16 × 400
Ek = 0.08 × 400 = 32 J
Even though speed only doubled (×2), the kinetic energy quadrupled (×4). This is because v is squared in the formula!
Gravitational Potential Energy Formula
When an object is raised to a height, it gains gravitational potential energy (GPE). This is the energy stored due to its position in the Earth's gravitational field. If it falls, this energy converts to kinetic energy.
In IGCSE Physics, always use g = 10 N/kg (or 10 m/s²) unless the question tells you otherwise. Some questions might give g = 9.8 N/kg — use whatever the question provides. Also remember: Δh is the vertical height gained, not the distance along a slope!
g = 10 N/kg
Height gained: Δh = 600 m
Find: ΔEp = ?
ΔEp = 60 × 6000
ΔEp = 360,000 J
By conservation of energy: Ep lost = Ek gained
So the coconut gains 180 J of kinetic energy.
180 = 0.75 × v²
v² = 180 ÷ 0.75 = 240
v = √240 ≈ 15.5 m/s
1.7.2 Work Done
In everyday life, "work" means any effort you make. But in physics, work has a very specific meaning: work is done only when a force causes an object to move in the direction of that force. If you push against a wall all day and it doesn't move — you've done zero work in physics terms (even though you're exhausted!).
The Work Formula
The distance must be in the direction of the force! If you carry a heavy bag horizontally, the vertical weight force does no work (because the bag moves horizontally, not vertically). If you carry it upstairs, the vertical component of displacement matters. This trips up many students — always check the direction!
Distance: d = 150 m (horizontal — same direction as force)
Find: W = ?
W = 30,000 J
The distance in the direction of this force: d = 6 m (vertical height only)
Note: the horizontal distance walked along the corridor does NOT count!
W = F × d = 80 × 400 = 32,000 J
1.7.3 Energy Resources
The world needs energy for everything — electricity, transport, heating, cooking, industry. We get this energy from various energy resources. These fall into two main categories: renewable (won't run out, naturally replenished) and non-renewable (limited supply, will eventually run out).
The Sun: The Ultimate Source
Here's something remarkable: almost all of Earth's energy resources ultimately come from the Sun! Think about it:
| Energy Resource | Connection to the Sun |
|---|---|
| Fossil fuels (coal, oil, gas) | Ancient plants and animals used sunlight for photosynthesis millions of years ago. Their remains became fossil fuels — so fossil fuels are really stored ancient sunlight! |
| Biofuels (wood, biogas, ethanol) | Plants grow using sunlight (photosynthesis). Burning them releases that solar energy. |
| Wind energy | The Sun heats the Earth unevenly, causing air to move (wind). So wind energy = solar energy! |
| Hydroelectric (water) | The Sun evaporates water from oceans; it falls as rain on mountains; rivers flow downhill to reservoirs. The Sun drives the water cycle! |
| Solar (photovoltaic/thermal) | Direct use of sunlight. |
| Tidal | Caused mainly by the Moon's gravity (not the Sun!) — one exception to the Sun-rule. |
| Geothermal | Heat from inside the Earth (radioactive decay in the Earth's core) — another exception. |
| Nuclear fission | Uranium was formed in ancient star explosions — not from our Sun, but from stars! Another exception. |
The three energy resources NOT from the Sun are: Tidal (Moon's gravity), Geothermal (Earth's internal heat), and Nuclear (energy from atomic nuclei). All others — fossil fuels, wind, hydro, solar, biofuels — trace back to the Sun. This is a very common exam question!
Renewable vs Non-Renewable Energy Resources
Non-renewable resources took millions of years to form and are being used faster than they are replaced. Once gone, they're gone forever. Renewable resources are naturally replenished and will not run out on a human timescale.
| Energy Resource | Type | How it works | Indian Example | Advantages | Disadvantages |
|---|---|---|---|---|---|
| Coal / Oil / Gas (Fossil Fuels) | Non-renewable | Burnt to boil water → steam drives turbines → electricity generated | Coal from Jharkhand's Jharia coalfields; NTPC Ramagundam power plant in Telangana | Reliable, available 24/7; high energy density; cheap and existing infrastructure | Produces CO₂, main cause of climate change; limited supply; causes air pollution; oil spills damage ecosystems |
| Biofuels (Wood, Biogas) | Renewable | Organic matter burnt or decomposed (biogas) → heat or electricity | Biogas plants in rural Gujarat; chulha (wood stoves) in villages; biogas from cow dung (gobar gas) | Carbon-neutral (CO₂ released = CO₂ absorbed during growth); uses waste materials; helps rural communities | Can contribute to deforestation; burning releases particulates causing health problems; needs large land area |
| Hydroelectric | Renewable | Water stored at height falls through turbines → electricity | Tehri Dam (Uttarakhand); Sharavathi Hydroelectric Project (Karnataka); Bhakra-Nangal Dam (Punjab/Himachal) | No greenhouse gas emissions during operation; very reliable; can store energy (pump water uphill); long lifespan | Destroys ecosystems; displaces communities (Tehri dam displaced 100,000 people); depends on rainfall; expensive to build |
| Tidal | Renewable | Tidal movement of sea water drives turbines | Potential in Gulf of Kutch (Gujarat) and Sundarbans; India exploring tidal energy in coastal regions | Predictable and reliable; no fuel cost; no greenhouse gas emissions | Very expensive to build; limited locations (need large tidal range); affects coastal ecosystems; no large operational plants in India yet |
| Geothermal | Renewable | Heat from Earth's interior heats water → steam drives turbines | Puga Valley (Ladakh) has geothermal potential; hot springs at Manikaran (Himachal Pradesh) | Available 24/7 regardless of weather; low operating costs; small land footprint; no greenhouse gas emissions | Limited to geologically active areas; can release sulfur gases; expensive drilling; potential for local earthquakes |
| Nuclear Fission | Non-renewable (uranium is limited) | Uranium atoms split in a controlled chain reaction → huge heat → steam → turbines → electricity | Kudankulam Nuclear Power Plant (Tamil Nadu) — India's largest nuclear plant; Tarapur Atomic Power Station (Maharashtra) | No CO₂ during operation; very high energy density (small amount of fuel = huge energy); reliable 24/7; low fuel costs | Radioactive waste that remains dangerous for thousands of years; risk of accidents (Chernobyl, Fukushima); very expensive to build; uranium mining is hazardous; nuclear weapons proliferation risk |
| Solar | Renewable | Photovoltaic (PV) cells convert sunlight directly to electricity; solar thermal uses sunlight to heat water | Bhadla Solar Park (Rajasthan) — one of the world's largest; rooftop solar panels across Bangalore; PM KUSUM scheme for farmers | No greenhouse gas emissions; free fuel (sunlight); low maintenance; scalable from a phone charger to a power station; rapidly falling costs | Only works in daylight; much less effective in cloudy/rainy weather; batteries needed for storage (expensive); large land area for utility-scale power |
| Wind | Renewable | Moving air rotates wind turbine blades → generator → electricity | Muppandal Wind Farm (Tamil Nadu) — one of Asia's largest; Jaisalmer Wind Farm (Rajasthan); Karnataka has growing wind capacity | No greenhouse gas emissions; no fuel cost; can share land with agriculture; rapidly becoming cheapest electricity source | Intermittent (only when wind blows); visual impact; noise; affects birds and bats; needs backup power for calm days; best wind often in remote areas (transmission costs) |
For non-renewable: "Coal Needs No Renewal" — Coal, oil, Natural gas, Nuclear are non-renewable.
Everything else — Solar, Wind, Hydro, Tidal, Geothermal, Biofuel — is renewable!
1.7.4 Efficiency
Nothing is perfect. Whenever energy is transferred from one store to another, some energy is always wasted — usually as thermal energy (heat). This wasted energy is transferred to the surroundings, where it becomes spread out and is no longer useful. Efficiency tells us how good a device is at converting energy into the form we actually want.
For example, an ordinary incandescent light bulb converts only about 5% of the electrical energy into light — the other 95% becomes heat! That's why LED bulbs (which are about 80% efficient) have largely replaced them.
Efficiency can be expressed as a decimal (0 to 1) or a percentage (0% to 100%). If the question asks for percentage, multiply by 100. If it asks for the ratio/decimal, don't multiply. Also remember: you can NEVER have efficiency greater than 100% — that would violate conservation of energy, which is impossible!
Sankey Diagrams
A Sankey diagram is a visual way to show energy transfers in a device. The key features are:
- A thick arrow enters from the left showing the total energy input
- The arrow splits: a thick arrow continues straight ahead showing useful energy output
- Thinner arrows bend downward showing wasted energy (usually thermal)
- The width of each arrow is proportional to the amount of energy it represents
- The total widths of all output arrows must equal the width of the input arrow (conservation of energy!)
Example — Ceiling Fan: A ceiling fan in an Indian home receives 75 J of electrical energy. 60 J is transferred usefully as kinetic energy (moving air). 15 J is wasted as thermal energy (friction in the motor and bearings) and some sound. In a Sankey diagram: a wide arrow (75 J) enters, a moderately wide arrow (60 J) goes straight (kinetic energy of moving air), and a thin arrow (15 J) curves down (thermal + sound).
Useful energy output: 60 J (kinetic energy of air)
Wasted energy: 80 - 60 = 20 J (thermal + sound)
Find: efficiency = ?
Efficiency = (60 ÷ 80) × 100%
Useful energy output: 3500 J (heat in water)
Efficiency = 0.70 × 100% = 70%
Wasted energy = 5000 − 3500 = 1500 J
This 1500 J is lost to the surroundings as thermal radiation, conduction, and convection from the heater's surface.
The incandescent bulb wastes 95 J as thermal energy (that's why it gets so hot!)
The LED wastes only 2 J — it stays cool and uses far less electricity for the same brightness.
Efficiency Using Power
Efficiency can also be calculated using power instead of energy. Since power = energy ÷ time, and both input and output are measured over the same time, the time cancels out:
Useful power output: 42,000 W (mechanical)
Efficiency = 0.84 × 100% = 84%
This 8,000 W of power is dissipated as thermal energy in the motor windings and friction — which is why metro trains have cooling systems.
Useful power output: 150 kW = 150,000 W
(Or you can keep both in kW — the units cancel in the ratio anyway!)
1.7.5 Power
We've talked about energy and work, but they don't tell us how fast the work is done. That's what power measures. A strong person might do the same work as a weak person, but a powerful person does it much faster.
Power is defined as work done per unit time, or equivalently, the rate of energy transfer.
Power is how fast energy is transferred. A 100 W bulb transfers 100 joules every second. A 1000 W electric kettle transfers 1000 joules every second — that's why it boils water faster! The unit Watt (W) is named after Scottish inventor James Watt, who improved the steam engine.
Always convert time to seconds before using P = W/t! If time is given in minutes, multiply by 60. If in hours, multiply by 3600. This is one of the most common mistakes — using minutes instead of seconds.
Time taken: t = 8 s
Find: P = ?
Time taken: t = 3 minutes = 3 × 60 = 180 s (convert to seconds!)
t = 10 s
(Kudankulam Unit 1 actually produces about 1000 MW — this example is simplified!)
Power = Force × Velocity (P = Fv)
There's another very useful formula for power when an object moves at constant velocity with a constant force applied to it. This is derived from combining P = W/t with W = Fd:
Use P = Fv when the question gives you force and speed but NOT time or distance directly. This formula is especially useful for vehicles! If a car moves at constant speed, the driving force equals the drag force (they're in equilibrium), so F is the driving force = drag force.
Speed: v = 12 m/s (constant speed means force = drag)
Find: P = ?
W = P × t = 300 × 600 = 180,000 J
(Check: distance = speed × time = 5 × 600 = 3000 m ✓)
Solar power per m² = 1000 W
Panel area = 2 m²
Total solar power input = 1000 × 2 = 2000 W
Step 2: Apply efficiency to find electrical power output.
Efficiency = 20% = 0.20
Useful electrical power = 0.20 × 2000 = 400 W
Step 3: Find energy produced per panel per day.
Assume about 6 hours of good sunshine per day (realistic for Karnataka).
Energy per panel per day = 400 W × 6 h = 2400 Wh = 2.4 kWh
Step 4: Find the number of panels needed.
Home uses 5 kWh per day.
Number of panels = 5 ÷ 2.4 ≈ 2.1 panels
Since you can’t have a fraction of a panel, you need 3 panels (round up to be safe).
W = mgh = 50 × 10 × 20 = 10,000 J (10 kJ)
Step 2: Convert time to seconds.
t = 2 minutes = 2 × 60 = 120 s
Step 3: Calculate useful power output.
P = W ÷ t = 10,000 ÷ 120 = 83.3 W
Step 4: Find total chemical energy used.
Body efficiency = 25% = 0.25
Efficiency = useful energy output ÷ total energy input
So total energy input = useful energy output ÷ efficiency
Total chemical energy = 10,000 ÷ 0.25 = 40,000 J (40 kJ)
That means 30,000 J was “wasted” as thermal energy (which is why Tara feels hot and sweaty at the top!).
GPE = mgh = 500 × 10 × 30 = 150,000 J
Step 2: Find the theoretical speed at the bottom (no friction).
All GPE converts to KE: mgh = ½mv²
The mass cancels! gh = ½v²
v² = 2gh = 2 × 10 × 30 = 600
v = √600 ≈ 24.5 m/s
Step 3: Calculate actual KE at the bottom.
Actual speed = 20 m/s
Actual KE = ½ × 500 × 20² = ½ × 500 × 400 = 100,000 J
Step 4: Calculate efficiency.
Efficiency = useful energy output ÷ total energy input × 100%
Efficiency = 100,000 ÷ 150,000 × 100% = 66.7%
Step 5: Where did the lost energy go?
Energy “lost” = 150,000 − 100,000 = 50,000 J
This was dissipated as thermal energy (friction between wheels and track, air resistance) and sound energy (the screaming doesn’t count — that’s the passengers!).
W = mgh = 2000 × 10 × 15 = 300,000 J (300 kJ)
Step 2: Calculate useful power.
P = W ÷ t = 300,000 ÷ 30 = 10,000 W (10 kW)
Step 3: Calculate efficiency.
Motor rated power (total input power) = 15 kW = 15,000 W
Total energy input in 30 s = 15,000 × 30 = 450,000 J (450 kJ)
Efficiency = useful output ÷ total input × 100%
Efficiency = 300,000 ÷ 450,000 × 100% = 66.7%
Step 4: Sankey diagram.
Think of it as a flow diagram with arrows whose width shows the amount of energy:
• Input arrow (left): 450 kJ of electrical energy (full width)
• Useful output arrow (right, going straight): 300 kJ of gravitational PE (2/3 width)
• Wasted arrow (going down): 150 kJ of thermal energy + sound (1/3 width)
The input arrow width = the sum of the output arrows. Energy is conserved!
At constant speed, driving force = friction force = 40 N
P = Fv = 40 × 6 = 240 W
Step 2: Find useful power from the e-bike motor.
Motor total power = 250 W
Efficiency = 80% = 0.80
Useful power = 0.80 × 250 = 200 W
Step 3: Find maximum speed of the e-bike.
At maximum constant speed, all useful power is used to overcome friction:
P = Fv, so v = P ÷ F
v = 200 ÷ 40 = 5 m/s
(That’s 18 km/h — a comfortable cruising speed!)
What is Pressure?
Imagine you are lying on a bed. Now imagine someone pokes you with one finger versus laying their whole palm flat on your shoulder. Which hurts more? The single finger, right! Even though the person pushes with the same force, the finger concentrates all that force onto a tiny area. That concentration of force is exactly what pressure is!
Here is the formal definition that you need to know for your exam:
Pressure is defined as the force acting per unit area. The force must act perpendicular (at right angles) to the surface.
The unit of pressure is the pascal (Pa). One pascal equals one newton per square metre:
The most common mistake is leaving the area in cm² instead of converting to m². Always convert before using the formula!
1 cm² = 0.0001 m² = 1 × 10⁻⁴ m²
(Because 1 cm = 0.01 m, so 1 cm² = 0.01 × 0.01 = 0.0001 m²)
Think of it like sharing a pizza! If 3 friends share a pizza, each gets a decent slice (low pressure on the pizza box). If 1 person takes the whole pizza and puts all their weight on a tiny spot — that spot feels a LOT of pressure. Same force, smaller area = more pressure.
Rearranging the Formula
You need to be able to find any one of the three quantities if you know the other two. Here are all three forms:
Worked Examples: p = F / A
Number of feet = 4
Area of each foot = 0.2 m²
Total contact area = 4 × 0.2 = 0.8 m²
p = 50,000 Pa
Area = 0.0001 m²
p = 600 ÷ 0.0001
p = 6,000,000 Pa = 6 MPa
Area = 0.015 m²
p = 600 ÷ 0.015
p = 40,000 Pa = 40 kPa
Wide strap: 60 cm² = 60 × 0.0001 = 0.006 m²
Pressure in Everyday Life
Once you understand pressure, you will start noticing it everywhere! Here are some brilliant examples from daily life in India and around the world:
| Situation | Area | Pressure | Effect / Why? |
|---|---|---|---|
| Sharp knife blade | Tiny (very thin edge) | Very HIGH | Cuts through food easily — same hand force, tiny area |
| Drawing pin (thumb tack) | Tiny point | Very HIGH | Pushes into a wall or notice board easily |
| Elephant feet | Very large (wide, flat feet) | LOW | Weight spread over large area — doesn't sink into soft ground |
| High heels | Tiny heel tip | Extremely HIGH | More pressure than an elephant! Damages soft floors |
| Snowshoes / Skis | Very large | LOW | Spreads body weight across snow — you don't sink! |
| Wide tractor tyres | Large | LOW | Spreads tractor's weight on soft farm soil in Karnataka |
| Camel's flat wide feet | Large and flat | LOW | Doesn't sink into desert sand — nature's snowshoe! |
| Bed of nails (fakir) | Hundreds of nail tips together = large area | LOW per nail | Weight spread across 500+ nails means pressure per nail is tiny |
| Wide building foundation | Very large base | LOW | Heavy building spreads weight over large area — doesn't sink into ground |
In "explain" questions about pressure, always mention TWO things:
1. What happens to the area (increases or decreases)
2. The effect on pressure (so pressure increases/decreases)
Example: "Wide tractor tyres increase the contact area, which reduces the pressure on soft soil, so the tractor does not sink."
How Pressure Varies with Force and Area
From the formula p = F / A, we can see two clear relationships:
- Force increases → Pressure increases: Push a drawing pin harder → more pressure → goes deeper into the wall. Same area, more force = more pressure.
- Area decreases → Pressure increases: A sharp knife cuts better than a blunt one. Same force but smaller area = much more pressure at the cutting edge.
More examples from India:
- Pressure cooker: The sealed lid traps steam. As heat builds up, the pressure inside rises — the high pressure raises the boiling point of water above 100°C, so rice and dal cook faster. (The cooker whistles when the safety valve releases excess pressure!)
- Drinking through a straw: You reduce the air pressure inside the straw by sucking. The higher air pressure outside then pushes the drink up into your mouth.
- Why surgeons use thin, sharp scalpels: The tiny blade area concentrates force to give enormous pressure — the blade cuts through skin easily with minimal force applied.
- Why it hurts to kneel on a hard floor: Your body weight concentrated on the small area of your knees creates high pressure on the hard floor — and the floor pushes back with equal pressure on your knees.
Pressure in Liquids: p = ρgh
Have you ever dived to the bottom of a swimming pool and felt your ears hurt? Or noticed that the walls of a dam are much thicker at the bottom than at the top? Both of these observations are about how pressure in a liquid increases with depth.
Think about it this way: if you are at a depth of 2 metres underwater, you have a column of water 2 metres tall sitting above you, pushing down on you. The deeper you go, the more water sits above you, and the greater the pressure.
This formula gives the pressure due to the liquid column only (pressure difference). To find the total absolute pressure at depth h, you would also add atmospheric pressure (about 100,000 Pa). However, in most IGCSE questions, you are asked to find the pressure difference caused by the liquid, so p = ρgh is what you use.
Remember "Roh-gah" — ρ (rho) × g × h. Or think: Dense Gravity Height — density, gravity, how high (deep) the column is. The denser the liquid, the stronger gravity, the deeper you are — all three increase pressure.
Key facts about liquid pressure:
- Pressure depends only on depth, not on the shape or total volume of the container
- At the same depth, a wide tank and a narrow tube have the same pressure
- Pressure increases with depth (more liquid above = more weight pushing down)
- Pressure increases with density (denser liquids push harder — mercury is 13.6 times denser than water, so it creates 13.6 times the pressure at the same depth)
Density of common liquids to know:
| Liquid | Density (kg/m³) |
|---|---|
| Fresh water | 1000 |
| Sea water | 1025 |
| Mercury | 13,600 |
| Mango juice (approximately) | ~1050 |
Worked Examples: p = ρgh
g = 10 N/kg
h = 2 m (depth at bottom)
p = 20,000 Pa = 20 kPa
g = 10 N/kg
h = 260 m
p = 1000 × 10 × 260
p = 2,600,000 Pa = 2.6 MPa
g = 10 N/kg
h = 0.15 m
p = 1050 × 10 × 0.15
p = 1575 Pa
Pressure in a Fluid Acts Equally in All Directions
Here is something fascinating: at any single point inside a fluid (a liquid or gas), the pressure acts equally in all directions — up, down, sideways, diagonally — all the same!
At point P inside the fluid, pressure pushes equally in every direction
Why does this matter? Here are brilliant examples:
- Round balloons: When you blow air into a balloon, the air pressure inside acts equally outward in all directions — that is why the balloon becomes roughly spherical (round). If pressure were stronger in one direction, the balloon would be lopsided!
- Toothpaste tube: Poke a hole anywhere in the tube and toothpaste squirts out. The pressure inside the paste is equal in every direction, so it escapes from wherever there is an opening.
- A diver underwater: Pressure acts on the diver from all sides equally — not just from above. This is why deep-sea pressure can crush submarine hulls — it pushes in from every direction at once.
- Hydraulic systems (Pascal's Principle): Because pressure in a fluid acts equally in all directions, when you apply pressure at one point, it transmits equally throughout the fluid. This is how car brakes, JCB excavators, and hydraulic lifts in car service centres work!
- A drinking straw: When you suck on a straw, you reduce pressure at the top. The atmospheric pressure acting equally in all directions on the surface of the liquid pushes the drink up the straw.
If asked to explain why pressure acts in all directions, say: "In a fluid, the molecules are free to move. They collide with any surface, regardless of orientation. So the fluid exerts a force on surfaces facing in any direction — the pressure is the same at a given depth in all directions."
Quick Summary
| Formula | What it finds | Syllabus level |
|---|---|---|
| p = F / A | Pressure (Pa) from force (N) and area (m²) | Core |
| F = p × A | Force (N) from pressure (Pa) and area (m²) | Core |
| A = F / p | Area (m²) from force (N) and pressure (Pa) | Core |
| p = ρgh | Pressure difference (Pa) due to liquid depth | Supplement |
Convert area to m²: 5 cm² = 5 × 10−⁴ m² = 0.0005 m²
Pressure = F ÷ A = 100 ÷ 0.0005 = 200,000 Pa
Step 2: This same pressure acts on the large piston.
Convert area: 200 cm² = 200 × 10−⁴ m² = 0.02 m²
Force on large piston = p × A = 200,000 × 0.02 = 4000 N
Step 3: Can it lift the Maruti car?
Weight of car = mg = 1500 × 10 = 15,000 N
The jack produces only 4000 N, so no — one push of 100 N is not enough. The mechanic would need to push with at least 375 N, or pump multiple times (which is exactly how real hydraulic jacks work!).
Step 4: The trade-off.
The force is multiplied by 40 (the ratio of the areas: 200 ÷ 5 = 40). But the large piston moves 40 times less distance than the small piston. Energy is conserved: small force × large distance = large force × small distance.
Water boils when its vapour pressure equals the atmospheric pressure pushing down on its surface. At sea level, atmospheric pressure is high (101,325 Pa), so water needs to reach 100°C before its vapour pressure is strong enough to overcome that.
At the summit (80,000 Pa), atmospheric pressure is lower, so water’s vapour pressure can match it at only about 93°C. The water molecules don’t need as much energy to escape into the gas phase.
Why the chip bag puffs up:
The chip bag was sealed at Bangalore (around 920 m, approximately 91,000 Pa). The air inside the bag was at that pressure. As Tara climbs to 1930 m, the outside atmospheric pressure drops to 80,000 Pa.
The air inside the bag is still at the original higher pressure. Since the inside pressure is now greater than the outside pressure, the air inside pushes outward, causing the bag to puff up and expand.
p = ρgh = 1025 × 10 × 200 = 2,050,000 Pa (2050 kPa)
Step 2: Find the total pressure.
Total pressure = water pressure + atmospheric pressure
Total pressure = 2,050,000 + 101,325 = 2,151,325 Pa ≈ 2151 kPa
That’s about 21 times atmospheric pressure!
Step 3: Calculate the area of the circular hatch.
Diameter = 0.8 m, so radius = 0.4 m
Area = πr² = π × 0.4² = π × 0.16 ≈ 0.503 m²
Step 4: Calculate the force on the hatch.
F = p × A = 2,151,325 × 0.503 ≈ 1,082,000 N
That’s over 1 million newtons — equivalent to the weight of about 108 tonnes pressing on one hatch!
Weight = mg = 5000 × 10 = 50,000 N
Total foot area = 4 × 0.08 = 0.32 m²
Pressure = F ÷ A = 50,000 ÷ 0.32 = 156,250 Pa ≈ 156 kPa
Step 2: Calculate the stiletto heel pressure.
Weight = mg = 55 × 10 = 550 N
Assume she stands on one heel (worst case): area = 0.00005 m²
Pressure = F ÷ A = 550 ÷ 0.00005 = 11,000,000 Pa = 11,000 kPa
Step 3: Compare!
Stiletto: 11,000 kPa vs Elephant: 156 kPa
The stiletto exerts about 70 times more pressure than the elephant!
Pressure increases with depth (p = ρgh). At the bottom of the dam, the water pressure is at its maximum because there are 40 m of water above. At the top, there is almost no water above, so the pressure is very low. The dam wall must be thicker at the bottom to withstand this greater pressure without cracking.
Step 2: Calculate the pressure at the bottom.
p = ρgh = 1000 × 10 × 40 = 400,000 Pa (400 kPa)
That’s about 4 times atmospheric pressure.
Step 3: Calculate the force through the crack.
Crack area = width × height = 0.1 × 0.01 = 0.001 m²
Force = p × A = 400,000 × 0.001 = 400 N
That’s like the weight of a 40 kg child pushing through a tiny crack — enough to widen it rapidly and potentially cause a catastrophic failure!