IB PHYSICS • SPACE, TIME AND MOTION

Understand Kinematics — Understand A.1 Kinematics

Describe and predict how objects move using displacement, velocity, and acceleration without worrying about forces.

Historical Context & Motivation

Humans have always been fascinated by motion — from tracking the paths of planets across the night sky to timing the fall of a stone from a cliff. For centuries, ancient Greek philosophers like Aristotle believed that heavier objects fall faster than lighter ones and that a force was needed to keep anything moving. These ideas went essentially unchallenged for nearly two thousand years. It was not until the Renaissance that scientists began to rigorously test these assumptions, giving birth to kinematics — the branch of physics that describes motion using quantities like position, velocity, and acceleration, without asking why things move.

~350 BCE
Aristotle's Physics
Aristotle taught that objects have a natural resting place and that heavier objects fall faster. His qualitative approach dominated Western thought for nearly two millennia.
1604
Galileo's Inclined Plane
Galileo Galilei rolled balls down inclined planes, carefully timing them with water clocks. He showed that all objects accelerate uniformly under gravity, regardless of mass — directly contradicting Aristotle.
1687
Newton's Principia
Isaac Newton published his three laws of motion and the law of universal gravitation, building on Galileo's kinematics to create a complete framework linking motion to forces (dynamics).
1905
Einstein's Special Relativity
Albert Einstein showed that time and space are relative at speeds near the speed of light, extending kinematics beyond the everyday realm explored by Galileo and Newton.

The central question kinematics addresses is deceptively simple: How can we precisely describe where an object is, how fast it is going, and how its speed is changing — all as functions of time? Answering this question gives us the language we need before we can tackle the deeper question of why objects move, which is the domain of dynamics and forces.

Core Principles & Definitions

Kinematics revolves around a handful of fundamental quantities that describe motion. Before diving into equations, it is essential to understand what each quantity means and how it differs from everyday language. In physics, words like "speed" and "velocity" have distinct, precise definitions. Mastering these definitions is the first step toward solving any kinematics problem.

1

Displacement (s or Δx)

The change in position of an object, measured from start to finish in a straight line. Displacement is a vector — it has both magnitude and direction. Walking 5 m east and then 5 m west gives zero displacement, even though you walked 10 m total.
2

Velocity (v)

The rate of change of displacement with respect to time. Velocity is a vector, so it includes direction. A car moving at 60 km/h north has a different velocity than one moving at 60 km/h south, even though their speeds are identical.
3

Speed vs. Velocity

Speed is a scalar — it tells you how fast an object is moving without specifying direction. Speed equals the magnitude of velocity. Average speed = total distance ÷ total time, while average velocity = displacement ÷ total time.
4

Acceleration (a)

The rate of change of velocity with respect to time. Acceleration is also a vector. An object can accelerate by speeding up, slowing down, or changing direction — even if its speed stays constant (like a car turning a corner).
5

Uniform vs. Non-uniform Motion

Uniform motion means constant velocity (zero acceleration). Uniformly accelerated motion means acceleration is constant (like free fall near Earth's surface, where a ≈ 9.8 m s⁻²). Non-uniform acceleration varies with time.
KEY TAKEAWAY
Think of kinematics like the commentary on a car's GPS. The GPS tells you where you are (position), how fast you're going and in what direction (velocity), and whether you're speeding up or slowing down (acceleration). It doesn't care about the engine, the fuel, or the road surface — it only describes the motion itself. That separation of description from cause is exactly what kinematics does.

Motion Graphs — The Visual Language of Kinematics

One of the most powerful tools in kinematics is the motion graph. Graphs of displacement versus time, velocity versus time, and acceleration versus time let you see patterns that equations alone can hide. In the IB syllabus, you need to interpret and sketch all three types of graph and understand how they relate to each other.

For uniformly accelerated motion, the displacement–time graph is a parabola, the velocity–time graph is a straight line, and the acceleration–time graph is a horizontal line. The slope of one graph gives the value plotted on the next, while the area under one graph gives the change in the quantity plotted on the previous graph.

The diagram above captures the single most important idea for interpreting motion graphs. The slope of the displacement–time graph at any instant gives the instantaneous velocity. Similarly, the slope of the velocity–time graph gives the instantaneous acceleration. Going the other direction, the area under the acceleration–time curve equals the change in velocity, and the area under the velocity–time curve equals the displacement. These relationships work for any motion — uniform, uniformly accelerated, or even non-uniform — making motion graphs incredibly versatile.

The SUVAT Equations

When acceleration is constant (uniform acceleration), the motion can be fully described by a set of equations often called the SUVAT equations — named after the five variables they connect: s (displacement), u (initial velocity), v (final velocity), a (acceleration), and t (time). Each equation omits one of these five variables, so you choose the equation that fits the information you are given.

EQUATION 1 — NO s
v = u + at
Final velocity equals initial velocity plus the product of acceleration and time. This equation defines constant acceleration directly.
EQUATION 2 — NO v
s = ut + ½at²
Displacement equals the initial velocity multiplied by time, plus half the acceleration multiplied by the square of time. This is derived from the area under the v–t graph.
EQUATION 3 — NO t
v² = u² + 2as
The square of the final velocity equals the square of the initial velocity plus twice the product of acceleration and displacement. Useful when time is not given or required.
EQUATION 4 — NO a
s = ½(u + v)t
Displacement equals the average of the initial and final velocities, multiplied by time. This is simply the area of a trapezoid under the v–t graph.
💡 IB Exam Tip
These equations are provided in the IB Physics data booklet, so you don't need to memorise them. Focus instead on recognising which variable is missing from the problem, then pick the equation that omits that same variable. Also remember: these equations only work for constant acceleration. If acceleration changes, you need to use graphs or calculus-based methods.

Free Fall and Projectile Motion

A crucial special case of uniformly accelerated motion is free fall — motion under the influence of gravity alone, with air resistance neglected. Near the Earth's surface, the acceleration due to gravity is approximately g = 9.8 m s⁻² directed downward. All the SUVAT equations apply with a = g (or a = −g if you choose upward as positive). When an object is launched at an angle, the motion becomes two-dimensional — this is projectile motion.

The key insight for projectile motion is that the horizontal and vertical components of motion are independent of each other. Horizontally, there is no acceleration (ignoring air resistance), so the horizontal velocity remains constant. Vertically, the only acceleration is g downward. By treating each direction separately using SUVAT, you can predict the full trajectory of a projectile.

A projectile launched at angle θ follows a parabolic path. The horizontal component of velocity (uₓ = u cos θ) stays constant throughout the flight. The vertical component (uᵧ = u sin θ) decreases on the way up, reaches zero at the peak, and increases on the way down due to gravitational acceleration g.
Projectile motion equations separated by component
QuantityHorizontal (x)Vertical (y)
Acceleration0 (no horizontal force)g = 9.8 m s⁻² downward
Initial velocityuₓ = u cos θuᵧ = u sin θ
Velocity at time tvₓ = uₓ (constant)vᵧ = uᵧ − gt
Displacementx = uₓty = uᵧt − ½gt²

Worked Example — Projectile Launched Horizontally

A ball is kicked horizontally off the edge of a cliff with a speed of 15 m s⁻¹. The cliff is 45 m high. Assuming air resistance is negligible and g = 9.8 m s⁻², find (a) the time it takes the ball to reach the ground and (b) the horizontal distance from the base of the cliff where it lands.

Horizontal Projectile from a Cliff
1
Step 1 — Identify Given Values and Choose DirectionsTake downward as positive for the vertical direction, and horizontal in the direction of the kick as positive. The ball is launched horizontally, so the initial vertical velocity is zero. Given: uₓ = 15 m s⁻¹, uᵧ = 0, vertical displacement sᵧ = 45 m (downward), a = g = 9.8 m s⁻².
2
Step 2 — Find the Time of Flight (vertical analysis)Use sᵧ = uᵧt + ½gt². Since uᵧ = 0, this simplifies to sᵧ = ½gt². Rearranging for t gives t = √(2sᵧ / g).
t = √(2 × 45 / 9.8) = √(90 / 9.8) = √9.184 ≈ 3.03 s
3
Step 3 — Find the Horizontal DistanceHorizontally, there is no acceleration, so x = uₓ × t. Substitute the known values.
x = 15 × 3.03 ≈ 45.5 m
4
Step 4 — Verify and State Final AnswersThe answers are reasonable: a 45 m cliff gives about 3 seconds of fall time, during which the ball travels roughly 45 m horizontally. The ball lands approximately 45.5 m from the base of the cliff after a flight time of about 3.0 s.
(a) t ≈ 3.0 s (b) x ≈ 45 m (2 s.f.)

Strengths & Limitations — Graphs versus Equations

In IB Physics, you are expected to solve kinematics problems both algebraically (using SUVAT equations) and graphically. Each approach has advantages and limitations, and the best physicists know when to use each one.

Comparing algebraic and graphical approaches to kinematics
CriterionSUVAT EquationsMotion Graphs
Applicable when...Acceleration is constant throughout the motionAny type of motion — uniform, uniformly accelerated, or non-uniform
PrecisionExact numerical answers from algebraValues read from graphs are approximate, limited by scale
Qualitative insightLess intuitive — requires interpretation of numbersExcellent — you can see changes in speed, direction, and acceleration at a glance
Best for...Precise calculations with known constant accelerationDescribing and analysing real-world motion data, which is rarely perfectly uniform
Common IB tasksNumerical problems; Paper 1 and Paper 2 calculationsSketch and interpret graphs; extract slopes and areas; Paper 1 and Paper 2
KEY TAKEAWAY
SUVAT equations and motion graphs are two lenses for viewing the same reality. Imagine you're a detective investigating a car crash. The equations are like witness statements — precise and specific but only useful if you know the right questions to ask. The graphs are like security camera footage — they show you the whole story at once, even details you didn't think to ask about. A good physicist uses both tools together to build a complete picture of motion.

Connection to Advanced Theory

The SUVAT framework is powerful, but it is only the starting point. In real life, acceleration is rarely constant. Air resistance, for example, causes acceleration to decrease as an object speeds up, eventually reaching terminal velocity where the net force — and therefore the acceleration — becomes zero. Handling these situations requires either graphical methods (which you have already learned) or calculus-based kinematics, which is explored at university level.

How A.1 Kinematics connects to more advanced physics
FeatureA.1 Kinematics (this topic)Advanced / University-Level
AccelerationConstant (uniform)Can vary with time, position, or velocity
Math toolsAlgebra and trigonometryCalculus (derivatives and integrals)
Dimensions1D and 2D (projectiles)3D motion, curvilinear coordinates, polar/spherical
Air resistanceNeglected (ideal case)Modeled as drag force (often velocity-dependent)
RelativityNot considered (Galilean relativity)Special relativity for speeds near c

Even within the IB course, kinematics connects forward to topics like circular motion (where acceleration constantly changes direction) and simple harmonic motion (where acceleration is proportional to displacement). The skills you build here — breaking motion into components, reading graphs, and selecting equations — will be the foundation for every subsequent mechanics topic.

Practice Problems

PROBLEM 1CONCEPTUAL
A car drives around a circular track at a constant speed of 20 m s⁻¹. Is the car accelerating? Explain your reasoning using the definitions of velocity and acceleration.
PROBLEM 2BASIC CALCULATION
A cyclist accelerates uniformly from rest to 12 m s⁻¹ in 8.0 s. Calculate (a) the acceleration and (b) the distance covered during this time.
PROBLEM 3INTERMEDIATE
A stone is thrown vertically upward with an initial speed of 20 m s⁻¹ from the edge of a bridge that is 25 m above a river. Taking g = 9.8 m s⁻² and upward as positive, find the speed of the stone just before it hits the water.
PROBLEM 4APPLIED
A football is kicked from ground level at 25 m s⁻¹ at an angle of 35° above the horizontal. Ignoring air resistance, calculate (a) the maximum height reached and (b) the total horizontal range. Use g = 9.8 m s⁻².
PROBLEM 5CRITICAL THINKING
A velocity–time graph for a car shows the following: from t = 0 to t = 4 s the velocity increases linearly from 0 to 16 m s⁻¹; from t = 4 s to t = 10 s the velocity is constant at 16 m s⁻¹; from t = 10 s to t = 14 s the velocity decreases linearly from 16 m s⁻¹ to 0. (a) Sketch the corresponding acceleration–time and displacement–time graphs. (b) Calculate the total displacement.

Lesson Summary

Kinematics is the study of motion without considering forces. It is built on four core quantities: displacement (change in position, a vector), velocity (rate of change of displacement, a vector), acceleration (rate of change of velocity, a vector), and time (a scalar). When acceleration is constant, the four SUVAT equations — v = u + at, s = ut + ½at², v² = u² + 2as, and s = ½(u + v)t — relate these quantities algebraically.

Motion graphs (s–t, v–t, a–t) provide a complementary visual approach: the slope of one graph gives the value on the next, while the area under one graph gives the change in the quantity on the previous graph. In projectile motion, the horizontal and vertical components of motion are treated independently: constant velocity horizontally and uniform acceleration (g ≈ 9.8 m s⁻²) vertically. Mastering these tools — equations, graphs, and vector decomposition — gives you the complete language needed to describe and predict motion in IB Physics.

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