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Kinematics Physics

- Astrophysics
- Absolute Magnitude
- Astronomical Objects
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- Angular Work and Power
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- Non-Flow Processes
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- Rotational Kinetic Energy
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- Thermodynamics and Engines
- Torque and Angular Acceleration
- Fields in Physics
- Alternating Currents
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- Energy Stored by a Capacitor
- Escape Velocity
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- Newton’s Laws
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- Planetary Orbits
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- Absolute Pressure and Gauge Pressure
- Application of Bernoulli's Equation
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- Force
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- Conservation of Momentum
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- Force and Motion
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- Moment Physics
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- Pressure
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- Safety First
- Time Speed and Distance
- Velocity and Acceleration
- Work Done
- Fundamentals of Physics
- Further Mechanics and Thermal Physics
- Bottle Rocket
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- Geometrical and Physical Optics
- Kinematics Physics
- Air Resistance
- Angular Kinematic Equations
- Average Velocity and Acceleration
- Displacement, Time and Average Velocity
- Frame of Reference
- Free Falling Object
- Kinematic Equations
- Motion in One Dimension
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- Rotational Motion
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- Linear Momentum
- Magnetism
- Ampere force
- Earth's Magnetic Field
- Fleming's Left Hand Rule
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- Magnetic Flux
- Magnetic Materials
- Monopole vs Dipole
- RL Circuit
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- Mechanics and Materials
- Acceleration Due to Gravity
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- Graphs of Motion
- Linear Motion
- Materials
- Materials Energy
- Moments
- Momentum
- Power and Efficiency
- Projectile Motion
- Scalar and Vector
- Terminal Velocity
- Vector Problems
- Work and Energy
- Young's Modulus
- Medical Physics
- Absorption of X-Rays
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- Physics of Vision
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- Modern Physics
- Bohr Model of the Atom
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- Oscillations
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- Energy in Simple Harmonic Motion
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- Phase Angle
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- Restoring Force
- Simple Pendulum
- Spring-Block Oscillator
- Torsional Pendulum
- Velocity
- Particle Model of Matter
- Physical Quantities and Units
- Converting Units
- Physical Quantities
- SI Prefixes
- Standard Form Physics
- Units Physics
- Use of SI Units
- Physics of Motion
- Acceleration
- Angular Acceleration
- Angular Displacement
- Angular Velocity
- Centrifugal Force
- Centripetal Force
- Displacement
- Equilibrium
- Forces of Nature Physics
- Galileo's Leaning Tower of Pisa Experiment
- Inclined Plane
- Inertia
- Mass in Physics
- Speed Physics
- Static Equilibrium
- Radiation
- Antiparticles
- Antiquark
- Atomic Model
- Classification of Particles
- Collisions of Electrons with Atoms
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- Electromagnetic Radiation and Quantum Phenomena
- Isotopes
- Neutron Number
- Particles
- Photons
- Protons
- Quark Physics
- Specific Charge
- The Photoelectric Effect
- Wave-Particle Duality
- Rotational Dynamics
- Angular Impulse
- Angular Kinematics
- Angular Motion and Linear Motion
- Connecting Linear and Rotational Motion
- Orbital Trajectory
- Rotational Equilibrium
- Rotational Inertia
- Satellite Orbits
- Third Law of Kepler
- Scientific Method Physics
- Data Collection
- Data Representation
- Drawing Conclusions
- Equations in Physics
- Uncertainties and Evaluations
- Space Physics
- Thermodynamics
- Heat Radiation
- Thermal Conductivity
- Thermal Efficiency
- Thermodynamic Diagram
- Thermodynamic Force
- Thermodynamic and Kinetic Control
- Torque and Rotational Motion
- Centripetal Acceleration and Centripetal Force
- Conservation of Angular Momentum
- Force and Torque
- Muscle Torque
- Newton's Second Law in Angular Form
- Simple Machines
- Unbalanced Torque
- Translational Dynamics
- Centripetal Force and Velocity
- Critical Speed
- Free Fall and Terminal Velocity
- Gravitational Acceleration
- Gravitational Force
- Kinetic Friction
- Object in Equilibrium
- Orbital Period
- Resistive Force
- Spring Force
- Static Friction
- Turning Points in Physics
- Cathode Rays
- Discovery of the Electron
- Einstein's Theory of Special Relativity
- Electromagnetic Waves
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- Electron Specific Charge
- Length Contraction
- Michelson-Morley Experiment
- Millikan's Experiment
- Newton's and Huygens' Theories of Light
- Photoelectricity
- Relativistic Mass and Energy
- Special Relativity
- Thermionic Electron Emission
- Time Dilation
- Wave Particle Duality of Light
- Waves Physics
- Acoustics
- Applications of Ultrasound
- Applications of Waves
- Diffraction
- Diffraction Gratings
- Doppler Effect in Light
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- Properties of Waves
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- Total Internal Reflection in Optical Fibre
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- Ultrasound
- Wave Characteristics
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- X-rays
- Work Energy and Power
- Conservative Forces and Potential Energy
- Dissipative Force
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- Energy in Pendulum
- Force and Potential Energy
- Force vs. Position Graph
- Orbiting Objects
- Potential Energy Graphs and Motion
- Spring Potential Energy
- Total Mechanical Energy
- Translational Kinetic Energy
- Work Energy Theorem
- Work and Kinetic Energy

Planetary orbits, bike riding, track running, flying bees, and falling apples — we’re always on the move, and so is the world and universe we live in. In this article, we’ll introduce one of the foundational branches of classical physics: kinematics. In this article, we’ll go over the definition of kinematics in physics, some of the basic concepts that make up this subfield, and the physics equations you’ll need to know in order to start solving kinematics problems. We’ll also introduce a few of the core types of kinematics problems that you’ll be encountering. Let’s get started!

Studying motion is unavoidable: physical movement is an inherent part of life. We are constantly observing, experiencing, causing, and stopping motion. Before we examine the sources and drivers of more complex movement, we want to understand motion as it’s happening: where an object is heading, how fast it’s moving, and how long it lasts. This simplified lens we start out with is the study of kinematics in physics.

**Kinematics** is the study of the motion of objects without reference to the forces that caused the motion.

Our study of kinematics is an important starting point for understanding the moving and interacting world around us. Because mathematics is the language of physics, we’ll need a set of mathematical tools to describe and analyze all sorts of physical phenomena in our universe. Let’s dive into some basic concepts of kinematics next: the key variables of kinematic motion and the kinematics equations behind these.

Before we introduce the key kinematics equations, let’s briefly go through the background information and various parameters you need to know first.

In kinematics, we can divide physical quantities into two categories: scalars and vectors.

A **scalar** is a physical quantity with only a magnitude.

In other words, a scalar is simply a numerical measurement with a size. This can be a plain old positive number or a number with a unit that doesn’t include a direction. Some common examples of scalars that you regularly interact with are:

The mass (but not weight!) of a ball, textbook, yourself, or some other object.

The volume of coffee, tea, or water contained in your favorite mug.

The amount of time passed between two classes at school, or how long you slept last night.

So, a scalar value seems pretty straightforward — how about a vector?

A **vector** is a physical quantity with both a magnitude and direction.

When we say that a vector has direction, we mean that the **direction of the quantity matters**. That means the coordinate system we use is important, because the direction of a vector, including most variables of kinematic motion, will change signs depending on whether the direction of motion is positive or negative. Now, let’s look at a few simple examples of vector quantities in daily life.

The amount of force you use to push open a door.

The downward acceleration of an apple falling from a tree branch due to gravity.

How fast you ride a bike east starting from your home.

You’ll encounter several conventions for denoting vector quantities throughout your physics studies. A vector can be written as a variable with a right arrow above, such as the force vector \(\overrightarrow{F}\) or a bolded symbol, such as \(\mathbf{F}\). Make sure you’re comfortable working with multiple types of symbols, including no denotation for vector quantities!

Mathematically solving kinematics problems in physics will involve understanding, calculating, and measuring several physical quantities. Let’s go through the definition of each variable next.

Before we know how fast an object is moving, we have to know *where* something is first. We use the position variable to describe where an object resides in physical space.

The **position** of an object is its physical location in space relative to an origin or other reference point in a defined coordinate system.

For simple linear motion, we use a one-dimensional axis, such as the \(x\), \(y\), or \(z\)-axis. For motion along the horizontal axis, we denote a position measurement using the symbol \(x\), the initial position using \(x_0\) or \(x_i\), and the final position using \(x_1\) or \(x_f\). We measure position in units of length, with the most common unit choice being in meters, represented by the symbol \(\mathrm{m}\).

If we instead want to compare how much an object’s final position differs from its initial position in space, we can measure the displacement after an object has undergone some type of linear motion.

**Displacement** is a measurement of a change in position, or how far an object has moved from a reference point, calculated by the formula:

\begin{align*} \Delta x=x_f-x_i \end{align*}

We measure the displacement \(\Delta x\), sometimes denoted as \(s\), using the same units as position. Sometimes, we only want to know how much ground an object has covered altogether instead, such as the total number of miles a car has driven during a road trip. This is where the distance variable comes in handy.

**Distance** is a measurement of the total movement an object has traveled without reference to the direction of motion.

In other words, we sum up the absolute value of the length of each segment along a path to find the total distance \(d\) covered. Both displacement and distance are also measured in units of length.

The most important distinction to remember between these quantities is that position and displacement are vectors, while distance is a scalar.

Consider a horizontal axis spanning a driveway of \(\mathrm{10\, m}\), with the origin defined at \(5\,\mathrm{m}\) You walk in the positive \(x\)-direction from the car to your mailbox at the end of the driveway, where you then turn around to walk to your front door. Determine your initial and final positions, displacement, and total distance walked.

In this case, your initial position \(x_i\) is the same as the car at \(x=5\, \mathrm{m}\) in the positive \(x\)-direction. Traveling to the mailbox from the car covers \(5\,\mathrm{m}\), and traveling towards the door covers the whole length of the driveway of \(10\,\mathrm{m}\) in the opposite direction. Your displacement is:

\begin{align*} \Delta x=\mathrm{5\,m-10\,m=-5\,m} \end{align*}

\(x_f=-5\,\mathrm{m}\) is also our final position, measured along the negative \(x\)-axis from the car to the house. Finally, the total distance covered ignores the direction of motion:

\begin{align*} \Delta x=\mathrm{5\,m+\left |-10\,m \right |=15\,m} \end{align*}

You walked \(15\,\mathrm{m}\) total.

Since displacement calculations take direction into account, these measurements can be positive, negative, or zero. However, distance can only be positive if any motion has occurred.

An important and deceptively simple variable that we rely on for both day-to-day structure and many physics problems is time, particularly elapsed time.

**Elapsed time** is a measurement of how long an event takes, or the amount of time taken for observable changes to happen.

We measure a time interval \(\Delta t\) as the difference between the final timestamp and initial timestamp, or:

\begin{align*} \Delta t=t_f-t_i \end{align*}

We record time typically in units of seconds, denoted by the symbol \(\mathrm{s}\) in physics problems. Time may seem very straightforward on the surface, but as you journey deeper into your physics studies, you’ll find that defining this parameter is a bit more difficult than before! Don’t worry — for now, all you need to know is how to identify and calculate how much time has passed in a problem according to a standard clock or stopwatch.

We often talk about how “fast” something is moving, like how fast a car is driving or how quickly you’re walking. In kinematics, the concept of how fast an object is moving refers to how its position is changing through time, along with the direction it’s headed.

**Velocity** is the rate of change of displacement over time, or:

\begin{align*} \mathrm{Velocity=\frac{Displacement}{\Delta Time}} \end{align*}

In other words, the velocity variable \(v\) describes how much an object changes its position for each unit of time that passes. We measure velocity in units of length per time, with the most common unit being in meters per second, denoted by the symbol \(\mathrm{\frac{m}{s}}\). For example, this means that an object with a velocity of \(10\,\mathrm{\frac{m}{s}}\) moves \(\mathrm{10\, m}\) every second that passes.

Speed is a similar variable, but instead calculated using the total distance covered during some period of elapsed time.

**Speed** is the rate an object covers distance, or:

\begin{align*} \mathrm{Speed=\frac{Distance}{Time}} \end{align*}

We measure the speed \(s\) using the same units as velocity. In everyday conversation, we often use the terms velocity and speed interchangeably, whereas in physics the distinction matters. Just like displacement, velocity is a vector quantity with direction and magnitude, while speed is a scalar quantity with only size. A careless mistake between the two can result in the wrong calculation, so be sure to pay attention and recognize the difference between the two!

When driving a car, before we reach a constant speed to cruise at, we have to increase our velocity from zero. Changes in the velocity result in a nonzero value of acceleration.

**Acceleration** is the rate of change of velocity over time, or:

\begin{align*} \mathrm{Acceleration=\frac{\Delta Velocity}{\Delta Time}} \end{align*}

In other words, acceleration describes how quickly the velocity changes, including its direction, with time. For example, a constant, positive acceleration of \(indicates a steadily increasing velocity for each unit of time that passes.

We use units of length per squared time for acceleration, with the most common unit being in meters per second squared, denoted by the symbol \(\mathrm{\frac{m}{s^2}}\). Like displacement and velocity, acceleration measurements can be positive, zero, or negative since acceleration is a vector quantity.

You likely already have enough physical intuition to guess that motion can’t simply occur from nothing — you have to push your furniture to change its position when redecorating or apply a brake to stop a car. A core component of motion is the interaction between objects: forces.

A **force **is an interaction, such as a push or pull between two objects, that influences the motion of a system.

Forces are vector quantities, which means the direction of the interaction is important. Force measurement can be positive, negative, or zero. A force is usually measured in units of Newtons, denoted by the symbol \(\mathrm{N}\), which is defined as:

\begin{align*} \mathrm{1\, N=1\,\frac{kg\cdot m}{s^2}}\end{align*}

According to our definition of kinematics, we don’t need to account for any pushing or pulling interactions that might’ve kick-started motion. For now, all we need to pay attention to is the motion as it’s happening: how fast a car is traveling, how far a ball has rolled, how much an apple is accelerating downward. However, it’s beneficial to keep forces such as gravity in the back of your mind as you analyze kinematics problems. Kinematics is just a stepping stone to building our understanding of the world before we dive into more difficult concepts and systems!

The kinematics equations, also known as equations of motion, are a set of four key formulas we can use to find the position, velocity, acceleration, or time elapsed for the motion of an object. Let’s walk through each of the four kinematic equations and how to use them.

The first kinematic equation allows us to solve for the final velocity given an initial velocity, acceleration, and time period:

\begin{align*} v=v_0+a \Delta t \end{align*}

where \(v_0\) is the initial velocity, \(a\) is the acceleration, and \(\Delta t\) is the time elapsed. The next kinematic equation lets us find the position of an object given its initial position, initial and final velocities, and elapsed time:

\begin{align*} x=x_0+(\frac{v+v_0}{2}) \Delta t,\, \mathrm{or} \\ \Delta x=(\frac{v+v_0}{2}) \Delta t \end{align*}

where \(x_0\) is the initial position in the \(x\)-direction. We can substitute \(x\) for \(y\) or \(z\) for motion in any other direction. Notice how we’ve written this equation in two different ways — since the displacement \(\Delta x\) is equal to \(x-x_0\), we can move our initial position variable to the left side of the equation and rewrite the left side as the displacement variable. This handy trick also applies to our third kinematic equation, the equation for the position given the initial position, initial velocity, acceleration, and elapsed time:

\begin{align*} x=x_0+v_0t+\frac{1}{2}a\Delta t^2,\, \mathrm{or} \\ \Delta x=v_0t+\frac{1}{2}a\Delta t^2 \end{align*}

Again, we can always substitute the position variables with whichever variable we need in a given problem. Our final kinematic equation allows us to find the velocity of an object with only the initial velocity, acceleration, and displacement:

\begin{align*} v^2=v_0^2+2a\Delta x \end{align*}

All four of the kinematic equations assume that the **acceleration value is constant**, or unchanging, during the time period we observed the motion. This value could be the acceleration due to gravity on the surface of Earth, another planet or body, or any other value for acceleration in another direction.

Choosing which kinematic equation to use might seem confusing at first. The best method to determine which formula you need is by listing the information you’ve been given in a problem by variable. Sometimes, the value of a variable may be implied in the context, such as zero initial velocity when dropping an object. If you think you haven’t been given enough details to solve a problem, read it again, and draw a diagram too!

Though kinematics in physics broadly includes motion without regard to causal forces, there are several types of recurring kinematics problems you’ll encounter as you begin your studies of mechanics. Let’s briefly introduce a few of these types of kinematic motion: free fall, projectile motion, and rotational kinematics.

Free fall is a type of one-dimensional vertical motion where objects accelerate only under the influence of gravity. On Earth, the acceleration due to gravity is a constant value we represent with the symbol \(\mathrm{g}\):

\begin{align*} \mathrm{g=9.81\, \frac{m}{s^2}} \end{align*}

In the case of free fall, we don’t consider the effects of air resistance, friction, or any initially applied forces that don’t fit in with the definition of free-falling motion. An object undergoing free fall motion will descend a distance of \(\Delta y\), sometimes called \(\mathrm{h_0}\), from its initial position to the ground. To get a better understanding of how free fall motion works, let’s walk through a brief example.

Your calculator falls off your desk from a height of \(\mathrm{0.7\, m}\) and lands on the floor below. Since you’ve been studying free fall, you want to calculate the average velocity of your calculator during its fall. Choose one of the four kinematic equations and solve for the average velocity.

First, let’s organize the information we’ve been given:

- The displacement is the change in position from the desk to the floor, \(\mathrm{0.7\, m}\).
- The calculator begins at rest just as it begins to fall, so the initial velocity is \(v_i=0\,\mathrm{\frac{m}{s}}\).
- The calculator is falling only under the influence of gravity, so \(a=\mathrm{g=9.8\, \frac{m}{s^2}}\).
- For simplicity, we can define the down direction of motion to be the positive y-axis.
- We don’t have the duration of time for the fall, so we can’t use an equation that depends on time.

Given the variables we do and do not have, the best kinematic equation to use is the equation for velocity without knowing the duration of time, or:

\begin{align*} v^2=v_0^2+2a \Delta y \end{align*}

To make our math even simpler, we should first take the square root of both sides to isolate the velocity variable on the left:

\begin{align*} v=\sqrt{v_0^2+2a \Delta y} \end{align*}

Finally, let’s plug in our known values and solve:

\begin{align*} v=\sqrt{\mathrm{0\, \frac{m}{s}+(2\cdot 9.8\, \frac{m}{s^2}\cdot 0.7\, m)}} \\ v=\sqrt{\mathrm{13.72\, \frac{m^2}{s^2}}} \\ v=\mathrm{3.7\, \frac{m}{s}} \end{align*}

The average velocity of the calculator is \(3.7\,\mathrm{\frac{m}{s}}\).

Though most free fall problems take place on Earth, it’s important to note that acceleration due to gravity on different planets or smaller bodies in space will have different numeric values. For example, acceleration due to gravity is considerably smaller on the moon and significantly greater on Jupiter than what we’re used to on Earth. So, it isn’t a true constant — it’s only “constant” enough for simplifying physics problems on our home planet!

Projectile motion is the two-dimensional, usually parabolic motion of an object that has been launched into the air. For parabolic motion, an object’s position, velocity, and acceleration can be split into horizontal and vertical **components**, using \(x\) and \(y\) subscripts respectively. After splitting a variable of motion into individual components, we can analyze how fast the object moves or accelerates in each direction, as well as predict the position of the object at different points in time.

All objects experiencing projectile motion exhibit symmetric motion and have a max range and height — as the classic saying goes, “what goes up must come down”!

Rotational motion, also known as rotational kinematics, is an extension of the study of linear kinematics to the motion of orbiting or spinning objects.

**Rotational motion** is the circular or revolving motion of a body about a fixed point or rigid axis of rotation.

Examples of rotational motion exist all around us: take the planetary orbits revolving around the Sun, the inner movement of cogs in a watch, and the rotation of a bicycle wheel. The equations of motion for rotational kinematics are analogous to the equations of motion for linear motion. Let’s look at the variables we use to describe rotational motion.

Variable | Linear Motion | |

Position and Displacement | \(x\) | \(\theta\) (Greek theta) |

Velocity | \(v\) | \(\omega\) (Greek omega) |

Acceleration | \(a\) | \(\alpha\) (Greek alpha) |

Kinematics and classical mechanics as a whole are extensive branches of physics that may feel daunting at first. But don’t worry — we’ll be going into much more detail for all the new variables and equations in the next few articles!

Kinematics is the study of the motion of objects without reference to the causal forces involved.

Linear motion is the motion of an object in one dimension, or in one direction across coordinate space.

Displacement is the change measured between a final and initial position.

Velocity is the change in an object’s position per unit of time.

Acceleration is the rate of change in velocity per unit of time.

Free fall is a type of linear, vertical motion, with a constant acceleration resulting from gravity on Earth.

Projectile motion is the two-dimensional motion of an object launched from some angle, subject to gravity.

Rotational motion is the study of the revolving motion of a body or system and is analogous to linear motion.

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