1. Kinematics

Equations Of Motion

Uses kinematic equations to solve motion problems in one dimension.

Equations of Motion

Welcome, students! In this lesson, we’re diving deep into the fascinating world of equations of motion. By the end, you’ll understand how to describe the motion of objects using kinematic equations. Our goal is to master the key formulas that allow you to solve real-world problems involving speed, acceleration, and displacement. Ready to become a motion master? Let’s get started! 🚀

Understanding Motion: The Basics

Before we jump into equations, let’s clarify some key concepts. Motion is all about how objects change position over time. To describe motion, we use quantities like:

  • Displacement ($s$): The change in position of an object. It’s a vector, meaning it has both magnitude and direction.
  • Velocity ($v$): The rate of change of displacement. It’s also a vector, so it includes both speed and direction.
  • Acceleration ($a$): The rate of change of velocity. If velocity changes, that’s acceleration (even if it’s slowing down, which we call deceleration).
  • Time ($t$): How long the motion takes.

These form the foundation of the equations of motion. The good news? There are only a few core equations to remember, and they’re incredibly powerful.

Real-World Example: Car Acceleration

Imagine you’re in a car. You press the accelerator, and the car speeds up from rest to 20 m/s in 5 seconds. How do we describe that motion? That’s exactly what kinematic equations help us solve.

The Four Key Equations of Motion

The equations of motion are known as the kinematic equations. They apply when acceleration is constant (doesn’t change over time). These four equations relate displacement, initial velocity, final velocity, acceleration, and time.

Here they are:

  1. $v = u + at$
  2. $s = ut + \frac{1}{2}at^2$
  3. $v^2 = u^2 + 2as$
  4. $s = \frac{(u + v)}{2}t$

Let’s break them down one by one (don’t worry, we’ll practice using them soon!).

Equation 1: $v = u + at$

This is the velocity-time equation. It tells you how the velocity of an object changes over time if you know its initial velocity ($u$), its acceleration ($a$), and the time interval ($t$).

  • $v$ = final velocity (m/s)
  • $u$ = initial velocity (m/s)
  • $a$ = acceleration (m/s²)
  • $t$ = time (s)

📌 Example: You’re on a bike moving at 2 m/s. You speed up with a steady acceleration of 1.5 m/s² for 4 seconds. What’s your final velocity?

Let’s plug into the equation:

$v = u + at = 2 + (1.5 \times 4) = 2 + 6 = 8 \text{ m/s}$

So, after 4 seconds, your final velocity is 8 m/s.

Equation 2: $s = ut + \frac{1}{2}at^2$

This is the displacement-time equation. It helps you find how far an object travels while accelerating over time.

  • $s$ = displacement (m)
  • $u$ = initial velocity (m/s)
  • $a$ = acceleration (m/s²)
  • $t$ = time (s)

📌 Example: A car starts from rest ($u = 0$) and accelerates at 3 m/s² for 6 seconds. How far does it travel?

$s = ut + \frac{1}{2}at^2 = 0 \times 6 + \frac{1}{2} \times 3 \times 6^2 = 0 + \frac{1}{2} \times 3 \times 36 = 54 \text{ m}$

The car travels 54 meters in 6 seconds.

Equation 3: $v^2 = u^2 + 2as$

This is the velocity-displacement equation. It relates velocity and displacement without involving time. It’s super useful when you don’t know how long something takes but you know how far it’s gone.

  • $v$ = final velocity (m/s)
  • $u$ = initial velocity (m/s)
  • $a$ = acceleration (m/s²)
  • $s$ = displacement (m)

📌 Example: A ball is thrown upwards with an initial velocity of 15 m/s. How high does it go before it stops momentarily (i.e., $v = 0$)?

We know $u = 15 \text{ m/s}$, $v = 0 \text{ m/s}$, and the acceleration due to gravity is $a = -9.8 \text{ m/s}^2$. (We use negative because gravity is pulling down, opposite to the direction of motion.)

Let’s solve for $s$:

$0^2 = 15^2 + 2(-9.8)s$

$0 = 225 - 19.6s$

$19.6s = 225$

$s = \frac{225}{19.6} = 11.48 \text{ m}$

So, the ball reaches a maximum height of about 11.48 meters before falling back down.

Equation 4: $s = \frac{(u + v)}{2}t$

This is the average velocity equation. It’s useful when you know the initial and final velocities and want to find the displacement over a certain time.

  • $s$ = displacement (m)
  • $u$ = initial velocity (m/s)
  • $v$ = final velocity (m/s)
  • $t$ = time (s)

📌 Example: A train slows down from 30 m/s to 10 m/s over 20 seconds. How far does it travel during this time?

$s = \frac{(u + v)}{2}t = \frac{(30 + 10)}{2} \times 20 = 20 \times 20 = 400 \text{ m}$

The train covers 400 meters while slowing down.

Applying the Equations: Step-by-Step

Now that we know the equations, how do we apply them to solve problems? Let’s go through a step-by-step process.

Step 1: Identify What’s Given

First, read the problem carefully and write down what you know. Look for the values of $u$, $v$, $a$, $s$, and $t$. Some might be missing—that’s okay!

Step 2: Choose the Right Equation

Next, pick the equation that includes what you know and what you need to find. For example, if you know $u$, $a$, and $t$, and want $v$, use $v = u + at$.

Step 3: Solve for the Unknown

Plug in the values and solve for the unknown. Make sure to pay attention to units (meters, seconds, etc.).

Step 4: Check Your Answer

Finally, check if your answer makes sense. Does it fit the situation described? For example, a negative displacement might mean the object moved in the opposite direction.

Worked Example: Rocket Launch 🚀

Let’s put this all together with a full example.

A rocket starts from rest and accelerates straight up at 20 m/s² for 10 seconds. How high does it go in that time, and what’s its final velocity?

Step 1: Identify what we know:

  • $u = 0 \text{ m/s}$ (it starts from rest)
  • $a = 20 \text{ m/s}^2$
  • $t = 10 \text{ s}$

Step 2: We want to find the height ($s$) and the final velocity ($v$).

First, let’s find the height using $s = ut + \frac{1}{2}at^2$:

$s = 0 \times 10 + \frac{1}{2} \times 20 \times 10^2 = 0 + 10 \times 100 = 1000 \text{ m}$

So, the rocket climbs 1000 meters in 10 seconds.

Step 3: Now, let’s find the final velocity using $v = u + at$:

$v = 0 + 20 \times 10 = 200 \text{ m/s}$

The rocket’s final velocity after 10 seconds is 200 m/s.

Step 4: Check if it makes sense. A rocket accelerating at 20 m/s² for 10 seconds covers 1000 meters and reaches 200 m/s—these values seem reasonable for a powerful rocket launch.

Real-World Applications of Equations of Motion

Let’s see where these equations pop up in the real world.

Sports: Sprinting

When athletes sprint, they accelerate quickly from rest. Coaches use equations of motion to calculate how fast an athlete should be at various points in the race. For example, if a sprinter accelerates at 4 m/s² for 3 seconds, how far will they have traveled?

$s = ut + \frac{1}{2}at^2 = 0 + \frac{1}{2} \times 4 \times 3^2 = 18 \text{ m}$

So, the sprinter covers 18 meters in 3 seconds.

Roller Coasters

Roller coasters are a perfect example of motion under acceleration. Engineers use these equations to design the thrilling ups and downs. For instance, if a roller coaster car accelerates down a slope at 9 m/s² for 5 seconds, its final velocity can be found using $v = u + at$.

If it starts from rest:

$v = 0 + 9 \times 5 = 45 \text{ m/s}$

That’s 45 m/s (or 162 km/h) after 5 seconds of acceleration!

Free Fall

One of the most famous applications is free fall. When objects fall freely under gravity (ignoring air resistance), they accelerate at approximately $9.8 \text{ m/s}^2$. We use the same equations to find out how long it takes for something to hit the ground, or how fast it’s going when it hits.

For example, if a stone is dropped from a height of 50 meters, how long does it take to hit the ground?

We use $s = \frac{1}{2}at^2$ and set $u = 0$:

$50 = \frac{1}{2} \times 9.8 \times t^2$

$50 = 4.9t^2$

$t^2 = \frac{50}{4.9} \approx 10.2$

$t = \sqrt{10.2} \approx 3.19 \text{ s}$

So, it takes about 3.19 seconds for the stone to fall.

Common Mistakes and How to Avoid Them

Even with practice, there are a few common pitfalls when using these equations. Let’s highlight them so you can avoid them.

1. Mixing Up Units

Always check that your units are consistent. For example, if velocity is in m/s, make sure time is in seconds and distance is in meters. Mixing units can lead to incorrect answers.

2. Using the Wrong Equation

Make sure you’re choosing the equation that fits the known and unknown quantities. If time isn’t mentioned, use $v^2 = u^2 + 2as$. If acceleration isn’t constant, these equations won’t apply.

3. Forgetting Direction (Signs)

Remember that velocity and acceleration are vectors—they can be positive or negative depending on direction. For example, if an object is slowing down, acceleration might be negative. Always be consistent with signs.

4. Not Checking for Realism

After solving, think: Does the answer make sense? If you get a time of 0.001 seconds for a car to reach 100 km/h, something’s probably off. Re-check your steps.

Conclusion

In this lesson, we’ve explored the powerful equations of motion that help us describe how objects move under constant acceleration. We learned how to use the four key kinematic equations to solve problems involving displacement, velocity, acceleration, and time. We also saw how these equations apply in real-life scenarios, from sports to roller coasters.

By mastering these equations, you’re not just solving physics problems—you’re unlocking the secrets of how things move in the world around you. Keep practicing, students, and soon you’ll be solving motion problems like a pro! 🌟

Study Notes

  • Displacement ($s$): Change in position (m).
  • Initial velocity ($u$): Velocity at the start (m/s).
  • Final velocity ($v$): Velocity at the end (m/s).
  • Acceleration ($a$): Rate of change of velocity (m/s²).
  • Time ($t$): Duration of motion (s).

Key Equations of Motion (for constant acceleration):

  1. Velocity-Time Equation:

$v = u + at$

  1. Displacement-Time Equation:

$s = ut + \frac{1}{2}at^2$

  1. Velocity-Displacement Equation:

$v^2 = u^2 + 2as$

  1. Average Velocity Equation:

$s = \frac{(u + v)}{2}t$

Gravity (Free Fall):

  • Acceleration due to gravity on Earth: $a = 9.8 \text{ m/s}^2$ (downward).
  • For objects dropped from rest, $u = 0$.

Common Mistakes to Avoid:

  • Check units: Use meters, seconds, and m/s consistently.
  • Pay attention to signs: Positive or negative depending on direction.
  • Always verify if the answer makes sense in real-world terms.

Happy solving, students! 🚀

Practice Quiz

5 questions to test your understanding

Equations Of Motion — GCSE Physics | A-Warded