Historical Context & Motivation
For thousands of years, humans have tried to describe and predict how things move. 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 largely unchallenged for nearly two millennia.
It was not until the Renaissance that careful experiments began to replace pure philosophy. Kinematics — the branch of mechanics that describes motion without worrying about its causes — was born from this revolution. The word itself comes from the Greek kinēma, meaning "movement." Today, kinematics provides the foundational language for everything from engineering to space exploration.
The central question kinematics answers is deceptively simple: If I know where something is and how fast it is moving right now, where will it be in the future? Answering that question precisely requires a clear set of definitions, sign conventions, and equations — all of which you will master in this lesson.
Core Principles & Definitions
Before solving any kinematics problem, you need to be fluent in the key quantities and how they relate. In IB Physics, kinematics in Topic A.1 deals with motion in one and two dimensions under uniform acceleration (constant acceleration). The following grid outlines the core concepts you must internalize.
Displacement (s)
Velocity (v)
Acceleration (a)
Time (t)
Sign Convention
Visualising Motion: Position–Time & Velocity–Time Graphs
Graphs are one of the most powerful tools in kinematics. In the IB Physics course, you are expected to extract quantitative information from position–time (s–t) and velocity–time (v–t) graphs. The diagram below shows both graph types side by side for an object that accelerates uniformly from rest.
There are two critical relationships to remember here. On a position–time graph, the gradient (slope) of the curve at any instant gives the instantaneous velocity. On a velocity–time graph, the gradient gives the acceleration, and the area between the line and the time axis equals the displacement. Mastering graph interpretation is essential for IB Paper 1 and Paper 2 questions.
The SUVAT Equations
When acceleration is constant (uniform), four kinematic equations — often called the SUVAT equations — connect displacement (s), initial velocity (u), final velocity (v), acceleration (a), and time (t). Each equation omits one of the five variables, so you choose the equation that matches the variables you know and the variable you need to find.
For problems involving free fall, replace a with g (acceleration due to gravity, approximately 9.81 m s⁻² downward near Earth's surface). Remember to set your sign convention — if you choose upward as positive, then g = −9.81 m s⁻².
Projectile Motion: Combining Two Dimensions
One of the most important applications of kinematics is projectile motion — the motion of an object launched into the air and subject only to gravity (ignoring air resistance). The key insight is that horizontal and vertical motions are independent of each other. Horizontally, there is no acceleration, so the object moves at constant velocity. Vertically, the object accelerates downward at g = 9.81 m s⁻². By treating these two directions separately and linking them through time, you can solve any projectile problem.
| Direction | Acceleration | Key Equations |
|---|---|---|
| Horizontal (x) | 0 (no horizontal acceleration) | x = vx × t, where vx = v₀ cos θ |
| Vertical (y) | −g = −9.81 m s⁻² (downward) | vy = v₀ sin θ − gt; y = v₀ sin θ × t − ½gt² |
To resolve the initial velocity into components, use trigonometry: v₀ₓ = v₀ cos θ and v₀ᵧ = v₀ sin θ, where θ is the angle of launch measured from the horizontal. Time links both components: the projectile lands when vertical displacement returns to zero (for level ground), and horizontal range follows from that same time.
Worked Example: Ball Thrown from a Cliff
A student throws a ball horizontally at 12 m s⁻¹ from the top of a 45 m high cliff. Determine (a) the time to reach the ground, (b) the horizontal distance from the base of the cliff where the ball lands, and (c) the speed of the ball just before impact. Take g = 9.81 m s⁻².
Strengths & Limitations of the SUVAT Model
The SUVAT equations are incredibly powerful, but like any model in physics they come with assumptions. Understanding when these equations work — and when they break down — is just as important as knowing how to use them.
| Strengths | Limitations |
|---|---|
| Give exact solutions quickly when acceleration is constant. | Cannot be used when acceleration changes over time (e.g., drag force increasing with speed). |
| Apply to both horizontal and vertical motion independently in projectile problems. | Projectile equations ignore air resistance, which is significant for light or fast-moving objects. |
| Only require algebra — no calculus needed at the IB level. | For variable acceleration, calculus-based methods (integration of a(t)) are required instead. |
| Widely applicable: free fall, vehicles braking, balls thrown, rockets during burns at constant thrust. | Do not account for relativistic effects at speeds approaching the speed of light. |
Connection to Advanced Dynamics
Kinematics describes how things move; the next step is understanding why they move. This is the domain of dynamics (IB Topic A.2), which introduces Newton's laws and forces. Kinematics gives you the vocabulary; dynamics explains the underlying causes. Here is how the two relate.
| Feature | Kinematics (A.1) | Dynamics (A.2+) |
|---|---|---|
| Central question | Where will the object be and how fast will it move? | What forces cause the observed acceleration? |
| Key quantities | s, u, v, a, t | Force (F), mass (m), momentum (p) |
| Core equation | v = u + at | F = ma (Newton's second law) |
| Acceleration | Given or measured | Calculated from net force and mass |
| Advanced extensions | Relative motion, reference frames | Circular motion, energy, momentum conservation |
In the IB course, you will also encounter situations where acceleration is not constant — for example, an object falling with air resistance where drag increases with speed. In such cases, you cannot use the SUVAT equations directly. Instead, you will use graphical methods (finding areas and slopes on v–t or a–t graphs) or, in the Higher Level course, numerical and calculus-based approaches. Mastering the constant-acceleration case now gives you the foundation for tackling these more complex scenarios later.
Practice Problems
Lesson Summary
Kinematics is the study of motion without reference to forces. The five key variables — displacement (s), initial velocity (u), final velocity (v), acceleration (a), and time (t) — are connected by four SUVAT equations that apply whenever acceleration is constant. Choose the equation that matches the variables you have by identifying which variable is missing from the problem.
For projectile motion, split the problem into independent horizontal and vertical components, linked by time. Horizontal motion has zero acceleration; vertical motion has acceleration g = 9.81 m s⁻². Use position–time and velocity–time graphs to extract velocity (from slopes) and displacement (from areas). Always establish a clear sign convention before substituting values. These tools form the foundation for all subsequent mechanics in the IB Physics course.