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PhysicsPhysics73 views·Updated May 19, 2026·4 pages

Dynamics: Understanding Motion and Forces

user profile picture
Libby@libby_w

Physics dynamics might seem intimidating, but it's actually about understanding... Show more

1
of 4
Dynamics

Speed
speed = distance=
time S
ms meters per
second m
Average speed is over a long period of
time.
Instantaneous speed is over a v

Speed and Motion

Speed is simply how fast something travels, calculated by dividing distance by time measuredinmetrespersecond,m/smeasured in metres per second, m/s. You'll encounter two types: average speed over longer journeys and instantaneous speed at any given moment.

Speed-time graphs tell brilliant stories about motion. A horizontal line shows constant speed, whilst an upward slope indicates acceleration (speeding up) and a downward slope shows deceleration (slowing down). The steeper the line, the greater the change in speed.

Quick Tip: The area under a speed-time graph gives you the total distance travelled - super useful for exam questions!

Understanding these basics sets you up perfectly for tackling more complex motion problems. Speed graphs are your visual tool for making sense of any moving object.

2
of 4
Dynamics

Speed
speed = distance=
time S
ms meters per
second m
Average speed is over a long period of
time.
Instantaneous speed is over a v

Acceleration Calculations

Acceleration measures how quickly speed changes, calculated using: acceleration = finalvelocityinitialvelocityfinal velocity - initial velocity ÷ time. The units are metres per second squared m/s2m/s², which might look odd but makes perfect sense.

The key equation v = u + at becomes your best friend in physics. Here, v is final velocity, u is initial velocity, a is acceleration, and t is time. You can rearrange this formula to find any missing variable.

In acceleration experiments, you'll use light gates to measure precise timings. The card's width divided by the time gives you velocity at each gate, then you apply the acceleration formula using the time between gates.

Exam Success: Remember that the gradient of a speed-time graph directly gives you the acceleration - no calculation needed!

3
of 4
Dynamics

Speed
speed = distance=
time S
ms meters per
second m
Average speed is over a long period of
time.
Instantaneous speed is over a v

Newton's Three Laws

Newton's First Law explains that objects hate changing what they're doing. Things at rest stay put, and moving objects keep moving, unless an unbalanced force acts on them. Balanced forces mean no change in motion.

Newton's Second Law gives us the famous equation: Force = mass × acceleration F=maF = ma. This tells you exactly how much force you need to accelerate any object. Heavier objects need more force to achieve the same acceleration.

Newton's Third Law states that every action creates an equal and opposite reaction. When you push against a wall, it pushes back with exactly the same force. This isn't just theory - it's why rockets work and why walking is possible.

Real-World Connection: These laws explain everything from why you wear seatbelts to how athletes push off starting blocks!

4
of 4
Dynamics

Speed
speed = distance=
time S
ms meters per
second m
Average speed is over a long period of
time.
Instantaneous speed is over a v

Weight, Mass and Terminal Velocity

Don't confuse mass (amount of matter, measured in kg) with weight (force due to gravity, measured in Newtons). Weight equals mass times gravitational field strength W=mgW = mg, where Earth's gravity pulls at roughly 10 N/kg.

Terminal velocity happens when falling objects reach maximum speed. Initially, weight pulls down whilst air resistance pushes up. As speed increases, air resistance grows stronger until both forces balance perfectly.

At terminal velocity, acceleration becomes zero because the forces are balanced. This explains why parachutists don't just keep getting faster and faster - they reach a steady falling speed.

Key Insight: Terminal velocity depends on the object's shape and size - that's why feathers fall slower than stones in air!

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Where can I download the Knowunity app?

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PhysicsPhysics73 views·Updated May 19, 2026·4 pages

Dynamics: Understanding Motion and Forces

user profile picture
Libby@libby_w

Physics dynamics might seem intimidating, but it's actually about understanding how things move around you every day. From cars accelerating down the street to objects falling through the air, Newton's laws explain the motion you see everywhere.

1
of 4
Dynamics

Speed
speed = distance=
time S
ms meters per
second m
Average speed is over a long period of
time.
Instantaneous speed is over a v

Sign up to see the content. It's free!

  • Access to all documents
  • Improve your grades
  • Join milions of students

Speed and Motion

Speed is simply how fast something travels, calculated by dividing distance by time measuredinmetrespersecond,m/smeasured in metres per second, m/s. You'll encounter two types: average speed over longer journeys and instantaneous speed at any given moment.

Speed-time graphs tell brilliant stories about motion. A horizontal line shows constant speed, whilst an upward slope indicates acceleration (speeding up) and a downward slope shows deceleration (slowing down). The steeper the line, the greater the change in speed.

Quick Tip: The area under a speed-time graph gives you the total distance travelled - super useful for exam questions!

Understanding these basics sets you up perfectly for tackling more complex motion problems. Speed graphs are your visual tool for making sense of any moving object.

2
of 4
Dynamics

Speed
speed = distance=
time S
ms meters per
second m
Average speed is over a long period of
time.
Instantaneous speed is over a v

Sign up to see the content. It's free!

  • Access to all documents
  • Improve your grades
  • Join milions of students

Acceleration Calculations

Acceleration measures how quickly speed changes, calculated using: acceleration = finalvelocityinitialvelocityfinal velocity - initial velocity ÷ time. The units are metres per second squared m/s2m/s², which might look odd but makes perfect sense.

The key equation v = u + at becomes your best friend in physics. Here, v is final velocity, u is initial velocity, a is acceleration, and t is time. You can rearrange this formula to find any missing variable.

In acceleration experiments, you'll use light gates to measure precise timings. The card's width divided by the time gives you velocity at each gate, then you apply the acceleration formula using the time between gates.

Exam Success: Remember that the gradient of a speed-time graph directly gives you the acceleration - no calculation needed!

3
of 4
Dynamics

Speed
speed = distance=
time S
ms meters per
second m
Average speed is over a long period of
time.
Instantaneous speed is over a v

Sign up to see the content. It's free!

  • Access to all documents
  • Improve your grades
  • Join milions of students

Newton's Three Laws

Newton's First Law explains that objects hate changing what they're doing. Things at rest stay put, and moving objects keep moving, unless an unbalanced force acts on them. Balanced forces mean no change in motion.

Newton's Second Law gives us the famous equation: Force = mass × acceleration F=maF = ma. This tells you exactly how much force you need to accelerate any object. Heavier objects need more force to achieve the same acceleration.

Newton's Third Law states that every action creates an equal and opposite reaction. When you push against a wall, it pushes back with exactly the same force. This isn't just theory - it's why rockets work and why walking is possible.

Real-World Connection: These laws explain everything from why you wear seatbelts to how athletes push off starting blocks!

4
of 4
Dynamics

Speed
speed = distance=
time S
ms meters per
second m
Average speed is over a long period of
time.
Instantaneous speed is over a v

Sign up to see the content. It's free!

  • Access to all documents
  • Improve your grades
  • Join milions of students

Weight, Mass and Terminal Velocity

Don't confuse mass (amount of matter, measured in kg) with weight (force due to gravity, measured in Newtons). Weight equals mass times gravitational field strength W=mgW = mg, where Earth's gravity pulls at roughly 10 N/kg.

Terminal velocity happens when falling objects reach maximum speed. Initially, weight pulls down whilst air resistance pushes up. As speed increases, air resistance grows stronger until both forces balance perfectly.

At terminal velocity, acceleration becomes zero because the forces are balanced. This explains why parachutists don't just keep getting faster and faster - they reach a steady falling speed.

Key Insight: Terminal velocity depends on the object's shape and size - that's why feathers fall slower than stones in air!

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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PhysicsPhysics

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Explore key concepts in Forces and Motion, including Hooke's Law, velocity, acceleration, and the principles of moments. This summary covers essential topics such as the relationship between force and extension, terminal velocity, and the impact of safety devices in physics. Ideal for AQA Physics Unit 5 revision.

108,973864
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physics paper 1 notes

notes for all of physics paper q

103,79773
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Master key concepts for AQA Combined Physics Paper 2, including electromagnetic waves, mechanics, forces, and motion. This comprehensive summary covers essential topics like wave properties, Newton's laws, and the motor effect, ensuring you're well-prepared for your exam.

1115,758934
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Pl-Energy topic to revise for GCSE

101,0972
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1011,216477
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94131
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125,337122
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quick key active recall of physics equations you need to learn for the GCSEs. many questions use to equations in one question in the paper therefore knowing all is beneficial. here the quiz teaches you about the units and the formula for the equations.

116543
PhysicsPhysics

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Explore the fundamentals of energy flow diagrams, including energy stores, pathways, and transfers. This summary covers key concepts such as heating, electrical transfer, and the eight energy stores, providing a clear understanding of how energy is measured and transformed in various systems. Ideal for students studying energy principles in physics.

92,564247

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Key Romeo and Juliet themes and analysed quotes

106,578195
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Explore the complex themes of guilt and ambition in Shakespeare's 'Macbeth'. This analysis covers key characters, including Macbeth and Lady Macbeth, their moral dilemmas, and the tragic consequences of their ambition. Ideal for students studying character motivations, thematic elements, and the psychological impact of power. Includes insights on the natural order, manipulation, and the descent into madness.

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Students love us — and so will you.

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4.7/5Google Play

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 SiOS 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 KlichAndroid 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.

AnnaiOS user