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Complete Content Guide for Physics Paper 1 Exam

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✨Zara✨

29/11/2025

Physics

All of physics paper 1 content

409

29 Nov 2025

9 pages

Complete Content Guide for Physics Paper 1 Exam

user profile picture

✨Zara✨

@zara_miah19

Physics can seem intimidating, but it's actually about understanding the... Show more

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1 / 9
PADER

VECTORS SCALARS
CONTACT FORCE: when objects physically touching.
NON-CONTACT FORCE when not touching.
>
magnetism.
17 electrostatic f

Forces and Vectors

Ever wondered why a magnet can move a paperclip without touching it? That's the difference between contact forces (like pushing a door) and non-contact forces (like magnetism, gravity, and electrostatic force).

Understanding scalars and vectors is crucial for your exams. A scalar only has size (magnitude) - like distance or temperature. A vector has both size and direction - like displacement or force. When you're walking to school, the distance you travel is scalar, but your displacement straightlinedistancefromstarttofinishstraight-line distance from start to finish is vector.

The resultant force is simply adding up all the forces acting on an object. If forces are balanced resultant=0resultant = 0, there's no acceleration - this is Newton's first law. Think of a book sitting on a table - gravity pulls down, the table pushes up, so it stays put.

Weight is the force gravity exerts on an object: W = mg. On Earth, every 1kg weighs about 10N, but on the moon, you'd weigh much less because g = 1.6 N/kg there!

Quick Tip: Remember that mass stays the same everywhere, but weight changes depending on the planet's gravity!

PADER

VECTORS SCALARS
CONTACT FORCE: when objects physically touching.
NON-CONTACT FORCE when not touching.
>
magnetism.
17 electrostatic f

Motion Graphs and Analysis

Your walking speed is about 1.5 m/s, running is 3 m/s, and cycling reaches 6 m/s - these real-world examples help you judge if your calculations make sense!

Distance-time graphs are straightforward: the gradient gives you speed. A steep line means fast movement, a flat line means you're stationary. For displacement-time graphs, the gradient gives velocity (which includes direction).

Speed-time graphs are where things get interesting. The gradient gives you acceleration - how quickly you're speeding up or slowing down. A horizontal line means constant speed, an upward slope means accelerating, and a downward slope means decelerating.

The key equations are simple: v = d/t for speed and a = v/t for acceleration. These form the foundation for understanding motion in physics.

Exam Success: Practice sketching these graphs - they're exam favourites and once you master the gradient rules, you'll ace motion questions!

PADER

VECTORS SCALARS
CONTACT FORCE: when objects physically touching.
NON-CONTACT FORCE when not touching.
>
magnetism.
17 electrostatic f

Newton's Laws and Motion Equations

Newton's equations of motion might look scary, but they're incredibly useful. You've got four main equations, but honestly, v² = u² + 2as is the one you'll use most - it connects initial velocity (u), final velocity (v), acceleration (a), and distance (s).

Here's the magic: if something starts from rest, u = 0. If something stops, v = 0. If gravity is the only force, a = 9.8 m/s² or10m/s2tomakecalculationseasieror 10 m/s² to make calculations easier.

Newton's first law is about inertia - objects resist changes to their motion. Newton's second law gives us F = ma, connecting force, mass, and acceleration. This is probably the most important equation in mechanics.

Newton's third law states that every action has an equal and opposite reaction. When you walk, you push backwards on the ground, and it pushes forwards on you - that's what moves you forward!

Study Hack: For motion equations, always write down what you know and what you need to find - then pick the right equation!

PADER

VECTORS SCALARS
CONTACT FORCE: when objects physically touching.
NON-CONTACT FORCE when not touching.
>
magnetism.
17 electrostatic f

Stopping Distances and Energy Stores

Stopping distance = thinking distance + braking distance. Your thinking distance depends on your reaction time (affected by distractions, alcohol, tiredness), while braking distance depends on your car's condition and the road.

Here's the crucial bit: if you double your speed, your kinetic energy quadruples because KE = ½mv². This means braking distance increases dramatically with speed - why speed limits save lives.

Energy stores are everywhere around you. Moving objects have kinetic energy, objects at height have gravitational potential energy (GPE = mgh), and stretched springs have elastic potential energy (E = ½ke²).

Your hot cup of tea has thermal energy (ΔE = mcΔT), your phone battery stores chemical potential energy, and nuclear power stations use nuclear energy. Energy is always conserved - it never disappears, just changes form.

Real-world Connection: Understanding energy stores explains everything from why you feel the 'drop' on rollercoasters to how your phone battery works!

PADER

VECTORS SCALARS
CONTACT FORCE: when objects physically touching.
NON-CONTACT FORCE when not touching.
>
magnetism.
17 electrostatic f

Energy Transfers and Conservation

When objects interact in a closed system, energy transforms from one store to another. Drop a ball and GPE converts to KE - this is energy transfer in action!

Here's a brilliant shortcut for falling objects: v = √(2gh). This comes from equating GPE at the top with KE at the bottom. If your calculated speed seems too low, energy has been lost to air resistance or friction.

The rollercoaster example shows this perfectly: a 400kg cart dropping 30m reaches 24.5 m/s at the bottom. You can solve this by setting mgh = ½mv² and rearranging, or use the shortcut formula.

Energy conservation is fundamental - energy cannot be created or destroyed, only transferred. In real situations, some energy always transfers to thermal energy through friction and air resistance.

Exam Tip: Energy problems often involve equating different energy stores - master this technique and you'll solve most energy questions easily!

PADER

VECTORS SCALARS
CONTACT FORCE: when objects physically touching.
NON-CONTACT FORCE when not touching.
>
magnetism.
17 electrostatic f

Waves and the Electromagnetic Spectrum

Waves transfer energy without transferring matter - think of stadium waves where people move up and down but the wave travels around the stadium. There are two types: longitudinal waves (like sound) where oscillations are parallel to energy transfer, and transverse waves (like light) where oscillations are perpendicular.

The wave equation v = fλ connects wave speed, frequency, and wavelength. This applies to everything from sound waves to radio waves to light.

The electromagnetic spectrum covers all EM waves: radio waves (phones, WiFi), microwaves (cooking), infrared (heat), visible light, UV (tanning), X-rays (medical scans), and gamma rays (medical treatments). They all travel at the speed of light in a vacuum.

Higher energy waves like UV, X-rays, and gamma rays are ionising radiation - they can knock electrons out of atoms, which is why they're dangerous but also useful in medicine.

Memory Aid: Remember the EM spectrum with "Radio Mice In Visible UV X-ray Galaxies" - from lowest to highest energy!

PADER

VECTORS SCALARS
CONTACT FORCE: when objects physically touching.
NON-CONTACT FORCE when not touching.
>
magnetism.
17 electrostatic f

Refraction and Wave Behaviour

When waves enter a new material, they change speed and direction - this is refraction. You see this when a straw looks bent in a glass of water or when light creates rainbows through a prism.

The key rule: when waves slow down, they bend towards the normal (the perpendicular line). When they speed up, they bend away from the normal. This happens because wavelength changes but frequency stays constant.

Most materials slow down light compared to air, so light usually bends towards the normal when entering materials like glass or water. This is why lenses can focus light and why objects underwater appear closer than they really are.

Understanding refraction explains how your eyes work, why glasses correct vision, and how optical fibres carry internet signals around the world.

Visual Learning: Try putting a pencil in water and observe how it appears bent - this demonstrates refraction perfectly!

PADER

VECTORS SCALARS
CONTACT FORCE: when objects physically touching.
NON-CONTACT FORCE when not touching.
>
magnetism.
17 electrostatic f

Nuclear Decay and Radiation

Unstable atomic nuclei become more stable by nuclear decay, emitting radiation in the process. There are three main types you need to know.

Alpha decay occurs in large nuclei that eject a helium nucleus 2protons+2neutrons2 protons + 2 neutrons. The example shows americium-241 becoming neptunium-237 plus an alpha particle. Beta decay happens when a neutron turns into a proton plus an electron - the high-energy electron is beta radiation.

Alpha particles are heavy and highly ionising but easily stopped by paper. Beta particles are lighter, moderately ionising, and stopped by thin metal. Both can be deflected by magnetic fields because they're charged.

Each type of radiation has different properties affecting their danger level and uses. Alpha is most dangerous if ingested, beta can penetrate skin, while gamma (coming next) is the most penetrating.

Safety First: Understanding radiation helps you appreciate both its dangers and its vital medical applications in treatments and imaging!

PADER

VECTORS SCALARS
CONTACT FORCE: when objects physically touching.
NON-CONTACT FORCE when not touching.
>
magnetism.
17 electrostatic f

Radioactivity and Half-Life

Gamma radiation consists of high-energy electromagnetic waves with no mass or charge. They're weakly ionising but highly penetrating - only stopped by thick lead or concrete. Unlike alpha and beta, magnetic fields don't deflect gamma rays.

Half-life is the time for radioactive activity to halve. In the example, activity drops from 96 Bq to 12 Bq in 12 months. Count the halvings: 96→48→24→12 thats3halflivesthat's 3 half-lives, so each half-life is 4 months.

Radioactivity measures how quickly nuclei decay in a sample. We detect this using Geiger-Müller tubes that count radiation particles. The activity decreases predictably following the half-life pattern.

Understanding half-life is crucial for medical treatments, carbon dating, and nuclear waste management. Each radioactive isotope has its own unique half-life, from fractions of seconds to millions of years.

Calculation Tip: For half-life problems, keep halving the original amount until you reach the final value, then count how many steps it took!



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The app is very easy to use and well designed. I have found everything I was looking for so far and have been able to learn a lot from the presentations! I will definitely use the app for a class assignment! And of course it also helps a lot as an inspiration.

Stefan S

iOS user

This app is really great. There are so many study notes and help [...]. My problem subject is French, for example, and the app has so many options for help. Thanks to this app, I have improved my French. I would recommend it to anyone.

Samantha Klich

Android user

Wow, I am really amazed. I just tried the app because I've seen it advertised many times and was absolutely stunned. This app is THE HELP you want for school and above all, it offers so many things, such as workouts and fact sheets, which have been VERY helpful to me personally.

Anna

iOS user

Best app on earth! no words because it’s too good

Thomas R

iOS user

Just amazing. Let's me revise 10x better, this app is a quick 10/10. I highly recommend it to anyone. I can watch and search for notes. I can save them in the subject folder. I can revise it any time when I come back. If you haven't tried this app, you're really missing out.

Basil

Android user

This app has made me feel so much more confident in my exam prep, not only through boosting my own self confidence through the features that allow you to connect with others and feel less alone, but also through the way the app itself is centred around making you feel better. It is easy to navigate, fun to use, and helpful to anyone struggling in absolutely any way.

David K

iOS user

The app's just great! All I have to do is enter the topic in the search bar and I get the response real fast. I don't have to watch 10 YouTube videos to understand something, so I'm saving my time. Highly recommended!

Sudenaz Ocak

Android user

In school I was really bad at maths but thanks to the app, I am doing better now. I am so grateful that you made the app.

Greenlight Bonnie

Android user

very reliable app to help and grow your ideas of Maths, English and other related topics in your works. please use this app if your struggling in areas, this app is key for that. wish I'd of done a review before. and it's also free so don't worry about that.

Rohan U

Android user

I know a lot of apps use fake accounts to boost their reviews but this app deserves it all. Originally I was getting 4 in my English exams and this time I got a grade 7. I didn’t even know about this app three days until the exam and it has helped A LOT. Please actually trust me and use it as I’m sure you too will see developments.

Xander S

iOS user

THE QUIZES AND FLASHCARDS ARE SO USEFUL AND I LOVE THE SCHOOLGPT. IT ALSO IS LITREALLY LIKE CHATGPT BUT SMARTER!! HELPED ME WITH MY MASCARA PROBLEMS TOO!! AS WELL AS MY REAL SUBJECTS ! DUHHH 😍😁😲🤑💗✨🎀😮

Elisha

iOS user

This apps acc the goat. I find revision so boring but this app makes it so easy to organize it all and then you can ask the freeeee ai to test yourself so good and you can easily upload your own stuff. highly recommend as someone taking mocks now

Paul T

iOS user

 

Physics

409

29 Nov 2025

9 pages

Complete Content Guide for Physics Paper 1 Exam

user profile picture

✨Zara✨

@zara_miah19

Physics can seem intimidating, but it's actually about understanding the world around you - from why your phone works to how rollercoasters give you that thrilling drop! This summary covers the essential physics concepts you need to know, including forces,... Show more

PADER

VECTORS SCALARS
CONTACT FORCE: when objects physically touching.
NON-CONTACT FORCE when not touching.
>
magnetism.
17 electrostatic f

Sign up to see the contentIt's free!

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Forces and Vectors

Ever wondered why a magnet can move a paperclip without touching it? That's the difference between contact forces (like pushing a door) and non-contact forces (like magnetism, gravity, and electrostatic force).

Understanding scalars and vectors is crucial for your exams. A scalar only has size (magnitude) - like distance or temperature. A vector has both size and direction - like displacement or force. When you're walking to school, the distance you travel is scalar, but your displacement straightlinedistancefromstarttofinishstraight-line distance from start to finish is vector.

The resultant force is simply adding up all the forces acting on an object. If forces are balanced resultant=0resultant = 0, there's no acceleration - this is Newton's first law. Think of a book sitting on a table - gravity pulls down, the table pushes up, so it stays put.

Weight is the force gravity exerts on an object: W = mg. On Earth, every 1kg weighs about 10N, but on the moon, you'd weigh much less because g = 1.6 N/kg there!

Quick Tip: Remember that mass stays the same everywhere, but weight changes depending on the planet's gravity!

PADER

VECTORS SCALARS
CONTACT FORCE: when objects physically touching.
NON-CONTACT FORCE when not touching.
>
magnetism.
17 electrostatic f

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Motion Graphs and Analysis

Your walking speed is about 1.5 m/s, running is 3 m/s, and cycling reaches 6 m/s - these real-world examples help you judge if your calculations make sense!

Distance-time graphs are straightforward: the gradient gives you speed. A steep line means fast movement, a flat line means you're stationary. For displacement-time graphs, the gradient gives velocity (which includes direction).

Speed-time graphs are where things get interesting. The gradient gives you acceleration - how quickly you're speeding up or slowing down. A horizontal line means constant speed, an upward slope means accelerating, and a downward slope means decelerating.

The key equations are simple: v = d/t for speed and a = v/t for acceleration. These form the foundation for understanding motion in physics.

Exam Success: Practice sketching these graphs - they're exam favourites and once you master the gradient rules, you'll ace motion questions!

PADER

VECTORS SCALARS
CONTACT FORCE: when objects physically touching.
NON-CONTACT FORCE when not touching.
>
magnetism.
17 electrostatic f

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Newton's Laws and Motion Equations

Newton's equations of motion might look scary, but they're incredibly useful. You've got four main equations, but honestly, v² = u² + 2as is the one you'll use most - it connects initial velocity (u), final velocity (v), acceleration (a), and distance (s).

Here's the magic: if something starts from rest, u = 0. If something stops, v = 0. If gravity is the only force, a = 9.8 m/s² or10m/s2tomakecalculationseasieror 10 m/s² to make calculations easier.

Newton's first law is about inertia - objects resist changes to their motion. Newton's second law gives us F = ma, connecting force, mass, and acceleration. This is probably the most important equation in mechanics.

Newton's third law states that every action has an equal and opposite reaction. When you walk, you push backwards on the ground, and it pushes forwards on you - that's what moves you forward!

Study Hack: For motion equations, always write down what you know and what you need to find - then pick the right equation!

PADER

VECTORS SCALARS
CONTACT FORCE: when objects physically touching.
NON-CONTACT FORCE when not touching.
>
magnetism.
17 electrostatic f

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Stopping Distances and Energy Stores

Stopping distance = thinking distance + braking distance. Your thinking distance depends on your reaction time (affected by distractions, alcohol, tiredness), while braking distance depends on your car's condition and the road.

Here's the crucial bit: if you double your speed, your kinetic energy quadruples because KE = ½mv². This means braking distance increases dramatically with speed - why speed limits save lives.

Energy stores are everywhere around you. Moving objects have kinetic energy, objects at height have gravitational potential energy (GPE = mgh), and stretched springs have elastic potential energy (E = ½ke²).

Your hot cup of tea has thermal energy (ΔE = mcΔT), your phone battery stores chemical potential energy, and nuclear power stations use nuclear energy. Energy is always conserved - it never disappears, just changes form.

Real-world Connection: Understanding energy stores explains everything from why you feel the 'drop' on rollercoasters to how your phone battery works!

PADER

VECTORS SCALARS
CONTACT FORCE: when objects physically touching.
NON-CONTACT FORCE when not touching.
>
magnetism.
17 electrostatic f

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Energy Transfers and Conservation

When objects interact in a closed system, energy transforms from one store to another. Drop a ball and GPE converts to KE - this is energy transfer in action!

Here's a brilliant shortcut for falling objects: v = √(2gh). This comes from equating GPE at the top with KE at the bottom. If your calculated speed seems too low, energy has been lost to air resistance or friction.

The rollercoaster example shows this perfectly: a 400kg cart dropping 30m reaches 24.5 m/s at the bottom. You can solve this by setting mgh = ½mv² and rearranging, or use the shortcut formula.

Energy conservation is fundamental - energy cannot be created or destroyed, only transferred. In real situations, some energy always transfers to thermal energy through friction and air resistance.

Exam Tip: Energy problems often involve equating different energy stores - master this technique and you'll solve most energy questions easily!

PADER

VECTORS SCALARS
CONTACT FORCE: when objects physically touching.
NON-CONTACT FORCE when not touching.
>
magnetism.
17 electrostatic f

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Waves and the Electromagnetic Spectrum

Waves transfer energy without transferring matter - think of stadium waves where people move up and down but the wave travels around the stadium. There are two types: longitudinal waves (like sound) where oscillations are parallel to energy transfer, and transverse waves (like light) where oscillations are perpendicular.

The wave equation v = fλ connects wave speed, frequency, and wavelength. This applies to everything from sound waves to radio waves to light.

The electromagnetic spectrum covers all EM waves: radio waves (phones, WiFi), microwaves (cooking), infrared (heat), visible light, UV (tanning), X-rays (medical scans), and gamma rays (medical treatments). They all travel at the speed of light in a vacuum.

Higher energy waves like UV, X-rays, and gamma rays are ionising radiation - they can knock electrons out of atoms, which is why they're dangerous but also useful in medicine.

Memory Aid: Remember the EM spectrum with "Radio Mice In Visible UV X-ray Galaxies" - from lowest to highest energy!

PADER

VECTORS SCALARS
CONTACT FORCE: when objects physically touching.
NON-CONTACT FORCE when not touching.
>
magnetism.
17 electrostatic f

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Refraction and Wave Behaviour

When waves enter a new material, they change speed and direction - this is refraction. You see this when a straw looks bent in a glass of water or when light creates rainbows through a prism.

The key rule: when waves slow down, they bend towards the normal (the perpendicular line). When they speed up, they bend away from the normal. This happens because wavelength changes but frequency stays constant.

Most materials slow down light compared to air, so light usually bends towards the normal when entering materials like glass or water. This is why lenses can focus light and why objects underwater appear closer than they really are.

Understanding refraction explains how your eyes work, why glasses correct vision, and how optical fibres carry internet signals around the world.

Visual Learning: Try putting a pencil in water and observe how it appears bent - this demonstrates refraction perfectly!

PADER

VECTORS SCALARS
CONTACT FORCE: when objects physically touching.
NON-CONTACT FORCE when not touching.
>
magnetism.
17 electrostatic f

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Nuclear Decay and Radiation

Unstable atomic nuclei become more stable by nuclear decay, emitting radiation in the process. There are three main types you need to know.

Alpha decay occurs in large nuclei that eject a helium nucleus 2protons+2neutrons2 protons + 2 neutrons. The example shows americium-241 becoming neptunium-237 plus an alpha particle. Beta decay happens when a neutron turns into a proton plus an electron - the high-energy electron is beta radiation.

Alpha particles are heavy and highly ionising but easily stopped by paper. Beta particles are lighter, moderately ionising, and stopped by thin metal. Both can be deflected by magnetic fields because they're charged.

Each type of radiation has different properties affecting their danger level and uses. Alpha is most dangerous if ingested, beta can penetrate skin, while gamma (coming next) is the most penetrating.

Safety First: Understanding radiation helps you appreciate both its dangers and its vital medical applications in treatments and imaging!

PADER

VECTORS SCALARS
CONTACT FORCE: when objects physically touching.
NON-CONTACT FORCE when not touching.
>
magnetism.
17 electrostatic f

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Radioactivity and Half-Life

Gamma radiation consists of high-energy electromagnetic waves with no mass or charge. They're weakly ionising but highly penetrating - only stopped by thick lead or concrete. Unlike alpha and beta, magnetic fields don't deflect gamma rays.

Half-life is the time for radioactive activity to halve. In the example, activity drops from 96 Bq to 12 Bq in 12 months. Count the halvings: 96→48→24→12 thats3halflivesthat's 3 half-lives, so each half-life is 4 months.

Radioactivity measures how quickly nuclei decay in a sample. We detect this using Geiger-Müller tubes that count radiation particles. The activity decreases predictably following the half-life pattern.

Understanding half-life is crucial for medical treatments, carbon dating, and nuclear waste management. Each radioactive isotope has its own unique half-life, from fractions of seconds to millions of years.

Calculation Tip: For half-life problems, keep halving the original amount until you reach the final value, then count how many steps it took!

We thought you’d never ask...

What is the Knowunity AI companion?

Our AI Companion is a student-focused AI tool that offers more than just answers. Built on millions of Knowunity resources, it provides relevant information, personalised study plans, quizzes, and content directly in the chat, adapting to your individual learning journey.

Where can I download the Knowunity app?

You can download the app from Google Play Store and Apple App Store.

Is Knowunity really free of charge?

That's right! Enjoy free access to study content, connect with fellow students, and get instant help – all at your fingertips.

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The app is very easy to use and well designed. I have found everything I was looking for so far and have been able to learn a lot from the presentations! I will definitely use the app for a class assignment! And of course it also helps a lot as an inspiration.

Stefan S

iOS user

This app is really great. There are so many study notes and help [...]. My problem subject is French, for example, and the app has so many options for help. Thanks to this app, I have improved my French. I would recommend it to anyone.

Samantha Klich

Android user

Wow, I am really amazed. I just tried the app because I've seen it advertised many times and was absolutely stunned. This app is THE HELP you want for school and above all, it offers so many things, such as workouts and fact sheets, which have been VERY helpful to me personally.

Anna

iOS user

Best app on earth! no words because it’s too good

Thomas R

iOS user

Just amazing. Let's me revise 10x better, this app is a quick 10/10. I highly recommend it to anyone. I can watch and search for notes. I can save them in the subject folder. I can revise it any time when I come back. If you haven't tried this app, you're really missing out.

Basil

Android user

This app has made me feel so much more confident in my exam prep, not only through boosting my own self confidence through the features that allow you to connect with others and feel less alone, but also through the way the app itself is centred around making you feel better. It is easy to navigate, fun to use, and helpful to anyone struggling in absolutely any way.

David K

iOS user

The app's just great! All I have to do is enter the topic in the search bar and I get the response real fast. I don't have to watch 10 YouTube videos to understand something, so I'm saving my time. Highly recommended!

Sudenaz Ocak

Android user

In school I was really bad at maths but thanks to the app, I am doing better now. I am so grateful that you made the app.

Greenlight Bonnie

Android user

very reliable app to help and grow your ideas of Maths, English and other related topics in your works. please use this app if your struggling in areas, this app is key for that. wish I'd of done a review before. and it's also free so don't worry about that.

Rohan U

Android user

I know a lot of apps use fake accounts to boost their reviews but this app deserves it all. Originally I was getting 4 in my English exams and this time I got a grade 7. I didn’t even know about this app three days until the exam and it has helped A LOT. Please actually trust me and use it as I’m sure you too will see developments.

Xander S

iOS user

THE QUIZES AND FLASHCARDS ARE SO USEFUL AND I LOVE THE SCHOOLGPT. IT ALSO IS LITREALLY LIKE CHATGPT BUT SMARTER!! HELPED ME WITH MY MASCARA PROBLEMS TOO!! AS WELL AS MY REAL SUBJECTS ! DUHHH 😍😁😲🤑💗✨🎀😮

Elisha

iOS user

This apps acc the goat. I find revision so boring but this app makes it so easy to organize it all and then you can ask the freeeee ai to test yourself so good and you can easily upload your own stuff. highly recommend as someone taking mocks now

Paul T

iOS user

The app is very easy to use and well designed. I have found everything I was looking for so far and have been able to learn a lot from the presentations! I will definitely use the app for a class assignment! And of course it also helps a lot as an inspiration.

Stefan S

iOS user

This app is really great. There are so many study notes and help [...]. My problem subject is French, for example, and the app has so many options for help. Thanks to this app, I have improved my French. I would recommend it to anyone.

Samantha Klich

Android user

Wow, I am really amazed. I just tried the app because I've seen it advertised many times and was absolutely stunned. This app is THE HELP you want for school and above all, it offers so many things, such as workouts and fact sheets, which have been VERY helpful to me personally.

Anna

iOS user

Best app on earth! no words because it’s too good

Thomas R

iOS user

Just amazing. Let's me revise 10x better, this app is a quick 10/10. I highly recommend it to anyone. I can watch and search for notes. I can save them in the subject folder. I can revise it any time when I come back. If you haven't tried this app, you're really missing out.

Basil

Android user

This app has made me feel so much more confident in my exam prep, not only through boosting my own self confidence through the features that allow you to connect with others and feel less alone, but also through the way the app itself is centred around making you feel better. It is easy to navigate, fun to use, and helpful to anyone struggling in absolutely any way.

David K

iOS user

The app's just great! All I have to do is enter the topic in the search bar and I get the response real fast. I don't have to watch 10 YouTube videos to understand something, so I'm saving my time. Highly recommended!

Sudenaz Ocak

Android user

In school I was really bad at maths but thanks to the app, I am doing better now. I am so grateful that you made the app.

Greenlight Bonnie

Android user

very reliable app to help and grow your ideas of Maths, English and other related topics in your works. please use this app if your struggling in areas, this app is key for that. wish I'd of done a review before. and it's also free so don't worry about that.

Rohan U

Android user

I know a lot of apps use fake accounts to boost their reviews but this app deserves it all. Originally I was getting 4 in my English exams and this time I got a grade 7. I didn’t even know about this app three days until the exam and it has helped A LOT. Please actually trust me and use it as I’m sure you too will see developments.

Xander S

iOS user

THE QUIZES AND FLASHCARDS ARE SO USEFUL AND I LOVE THE SCHOOLGPT. IT ALSO IS LITREALLY LIKE CHATGPT BUT SMARTER!! HELPED ME WITH MY MASCARA PROBLEMS TOO!! AS WELL AS MY REAL SUBJECTS ! DUHHH 😍😁😲🤑💗✨🎀😮

Elisha

iOS user

This apps acc the goat. I find revision so boring but this app makes it so easy to organize it all and then you can ask the freeeee ai to test yourself so good and you can easily upload your own stuff. highly recommend as someone taking mocks now

Paul T

iOS user