Acceleration calculator is a tool that helps you to find out **how fast the speed of an object is changing**. It works in three different ways, based on:

- difference between velocities at two distinct points in time,
- distance traveled during acceleration,
- the mass of an accelerating object and the force that acts on it.

If you're asking yourself what is acceleration, what is the acceleration formula or what are the units of acceleration, keep reading, and you'll learn how to find acceleration. Acceleration is strictly related to the motion of an object, and every moving object possesses specific energy. If you need to estimate it, visit our other calculators where you can find the kinetic energy formula, and it's angular version - the rotational kinetic energy formula.

To keep things clear, we also prepared some acceleration examples that are common in physics. You can find there:

- centripetal acceleration and tangential acceleration,
- angular acceleration,
- acceleration of gravity,
- particle accelerator.

Acceleration always occurs whenever there is a non-zero net force acting on an object. You can feel it in an elevator when you become a little heavier (accelerating) or lighter (decelerating), or when you're riding down a steep slope on your sled in the snow. What's more, from the general theory of relativity we know that the entire Universe is not only expanding, but it is even an accelerated expansion! That means that the distance between two points is constantly becoming greater and greater, but we can't feel that on an everyday basis because every scale in the world expands too.

## What is acceleration? - acceleration definition

Acceleration is the rate of change of an objects speed; in other words, it's how fast velocity changes. According to Newton's second law, acceleration is directly proportional to the summation of all forces that act on an object and inversely proportional to its mass. It's all common sense - if several different forces are pushing an object, you need to work out what they add up to (they may be working in different directions), and then divide the resulting net force by your object's mass.

This acceleration definition says that acceleration and force are, in fact, the same thing. When the force changes, acceleration changes too, but the magnitude of its change depends on the mass of an object. This is not true in a situation when the mass also changes, e.g., in rocket thrust, where burnt propellants exit from the rocket's nozzle. If you've ever wondered what the physics behind space travel are, look at this Tsiolkovsky rocket equation.

We can measure acceleration experienced by an object directly with an **accelerometer**. If you hang an object on the accelerometer, it will show a non-zero value. Why is that? Well, it's because of gravitational forces that acts on every particle that has mass. And where is a net force, there is an acceleration. An accelerometer at rest thus measures the acceleration of gravity, which on the Earth surface is about **32.17 ft/s² (9.81 m/s²)**. In other words, this is the acceleration due to gravity that any object gains in free fall when in a vacuum.

Speaking of vacuums, have you ever watched Star Wars or another movie that takes place in space? The epic battles of spaceships, the sounds of blasters, engines and explosions. Well, it's a lie. Space is a vacuum, and no sound can be heard there (sound waves requires matter to propagate). Those battles should be soundless! In space, no one can hear you scream. To check the speed of sound in air or water, try our speed of sound calculator. It even takes temperature into account!

## How to find acceleration? - acceleration calculator

The acceleration calculator on this site considers only a situation in which an object has a uniform (constant) acceleration. In that case, the acceleration equation is by definition the ratio of the change in velocity over a particular time. However, here you can find out how to find acceleration in two more ways. Let's see how to use our calculator (you can find acceleration equations in the section after):

- Depending on what data you have, you may calculate acceleration in three different ways. First at all,
**select an appropriate window**(#1, #2 or #3), **[if you choose #1]**- Enter the initial`v_i`

and final`v_f`

speeds of the object, and how much time`Δt`

it took for the speed to change.**[if you choose #2]**- Enter initial speed`v_i`

, distance traveled`Δd`

and time`Δt`

passed during acceleration. Here, you don't need to know the final speed.**[if you choose #3]**- Enter mass`m`

of the object and the net force`F`

acting on this object. This is an entirely different set of variables that arises from the Newton's second law of motion (another definition of acceleration).**Read the resulting acceleration**from the last field. You can also perform calculations in the other way if you know what is acceleration, for example, to estimate distance`Δd`

. Just provide the rest of the parameters in this window.

Knowing what is acceleration is essential for analyzing the motion of objects. For example, you can find what the momentum change is over a certain time with this formula for momentum. This is on of the physical quantities we use in our car crash calculator where we explain and visualize the importance of seat belts using numbers, and determine at what speed can you die in a car crash. Speeding and alcohol content in the blood are the top causes of car accidents. Please, drive carefully!

## Acceleration formula - three acceleration equations

In the 17th century, **Sir Isaac Newton**, one of the most influential scientists of all time, published his famous book *Principia*. In it, he formulated the law of universal gravitation which states that any two objects with mass will attract each other with a force exponentially dependent on distance between these objects (specifically, it is inversely proportional to the distance squared). The heavier the objects are, the greater is gravitational force. It explains, for example, why planets orbit around the very dense Sun.

In *Principia*, Newton also includes three laws of motion which are central to understanding the physics of our world. The acceleration calculator is based on three various acceleration equations, where the third is derived from Newton's work:

`a = (v_f - v_i) / Δt`

,`a = 2 * (Δd - v_i * Δt) / Δt²`

,`a = F / m`

,

where:

`a`

is the acceleration,`v_i`

and`v_f`

are respectively the initial and final velocities,`Δt`

is the acceleration time,`Δd`

is the distance traveled during acceleration,`F`

is the net force acting on an object that accelerates,`m`

is the mass of this object.

Now you know how to calculate acceleration! In the next paragraph, we discuss the units of acceleration (SI and Imperial). Have you already seen our conversion calculators? They might save you a lot of time when dealing with various units. In the case of distance, you may be interested in the length converter which includes a length conversion table. If you want to switch between different units of mass, here's our weight converter. Both calculators allow you to perform calculations quickly with any set of units you want. Give them a try!

## Acceleration units

If you already know how to calculate acceleration let's focus on the units of acceleration. You can derive them from the equations we listed above. All you need to know is that speed is expressed in feet per second (imperial/US system) or in meters per second (SI system) and time in seconds. Therefore, if you divide speed by time (as we do in the first acceleration formula), you'll get acceleration unit `ft/s²`

or `m/s²`

depending on which system you use.

Alternatively, you can use the third equation. In this case, you need to divide force (poundals in US and newtons in SI) by mass (pounds in US and kilograms in SI) obtaining `pdl/lb`

or `N/kg`

. They both represent the same thing, as poundal is `pdl = lb * ft/s²`

and the newton is `N = kg * m/s²`

. When you substitute it and reduce the units, you'll get `(lb * ft/s²) / lb = ft/s²`

or `(kg * m/s²) / kg = m/s²`

.

There is also a third option that is, in fact, widely used. You can express acceleration by **standard acceleration**, due to gravity near the surface of the Earth which is defined as `g = 31.17405 ft/s² = 9.80665 m/s²`

. For example, if you say that an elevator is moving upwards with the acceleration of `0.2g`

, it means that it accelerates with about `6.2 ft/s²`

or `2 m/s²`

(i.e., `0.2*g`

). We rounded the above expressions to two significant figures with the significant figures rules that you can find in our math category.

## Acceleration examples

**Centripetal acceleration and tangential acceleration**

Acceleration is generally a vector, so you can always decompose it into components. Usually, we have two parts that are perpendicular to each other: the centripetal and the **tangential**. Centripetal acceleration **changes the direction of the velocity**, and therefore the shape of the track, but doesn't affect the value of the velocity. On the other hand, tangential acceleration is always perpendicular to the trajectory of motion. It **changes the value of velocity** only, and not its direction.

In a circular motion (the leftmost picture below) where an object moves around the circumference of a circle, there is only the centripetal component. An object will keep its speed at a constant value; think of the Earth that has centripetal acceleration due to the gravity of the Sun (in fact its speed changes a bit during a year - see orbital velocity calculator and orbital period calculator for more information).

When both components are present, the object's trajectory looks like the right picture. What happens if there is only tangential acceleration? Then linear motion occurs. This is similar to when you press down on the gas pedal in a car on a straight part of the freeway. And if you're a driver, our gas calculator might be of interest to you as well; it estimates the cost of car travel. You provide your fuel economy, distance and gas price and you'll quickly get the cost of the trip. There's even an option to split it with a few people, as traveling together is fun and beneficial! A group of talkative friends in your car will, e.g., prevent you from falling asleep.

**Angular acceleration**

Angular acceleration plays a vital role in the description of rotational motion. However, don't confuse it with the previously mentioned centripetal or tangential accelerations. This physical quantity corresponds to the rate of change of angular velocity. In other words, it tells you how fast an object's rotations accelerates - object spins faster and faster (or slower and slower if angular acceleration is less than zero).

Did you know that we can find an analogy between this and Newton's law of dynamics in rotational motion? In his second law, if you can switch acceleration with angular acceleration, force with torque and mass with moment of inertia, you'll end up with the angular acceleration equation. You might notice that some physical laws, like this one, are universal, which makes them really important in physics.

**Gravitational acceleration**

We mentioned acceleration due to gravity a few times earlier. It arises from the gravitational force that exists between every two objects that have mass (note that the gravity equation isn't dependent on an objects volume - only mass is essential here). It may sound weird at first, but according to the third Newton's law of motion, **you act with the same force on the Earth as the Earth acts on you**. However, the mass of the Earth is much bigger than a human mass (~10²² times bigger), so our impact on the Earth is pretty much zero. It's analogous to all the bacteria (~10¹⁸ times lighter than a human) living on your hand; you can't even notice them! On the other hand, we can feel the influence of our planet, and that's acceleration due to gravity.

Standard gravity is by definition 31.17405 ft/s² (9.80665 m/s²), so if a human weighs 220 lb (about 100 kg) he is subjected to the gravitational force of about 7000 pdl (1000 N). Let's enter this value to window #3 of our calculator along with the mass of the Earth (1.317 × 10²⁵ lbs or 5.972 × 10²⁴ kg in scientific notation). What is the calculated acceleration? It is **so small** that our calculator considers it to be **zero**. We mean nothing compared to the planet!

**Particle accelerator**

After talking about huge objects in space, let's move to the microscopic world of particles. Although we can't see them with our eyes, we have harnessed high energy particles, like electrons and protons, and use them regularly in particle accelerators; common in physics, chemistry, and medicine. We use them to kill cancer cells while sparing the surrounding healthy tissue or investigate a materials structure at the atomic scale. Recently, cancer is one of the diseases of affluence that probably result from the increasing wealth in society. Even poor nutrition can increase the risk of cancer! With this daily protein calculator you can check how much protein do you need a day and, if also want to get fit, our macro calculator is here to help you.

You probably know about the Large Hadron Collider (CERN), the most powerful particle accelerator in the world. It allows us to take a step further to understand how the universe works and develop technologies that may have many essential applications in the future. However, to achieve such high energies, we have to accelerate particles to the speeds that are close to the speed of light. Briefly, we can do it using magnetic or electric fields. To see how fast particles accelerate when compared to standard gravity, check out our acceleration in the electric field calculator, where we explained how to calculate the acceleration of charged particles.

The world of microscopic particles is ruled by statistical physics, which focuses specifically on the concept of probability. We've got many calculators related to this topic. Take a look at the probability calculator to learn how to find probability or try the permutation calculator to determine the number of ways in which you can order a certain amount of elements. Physicists use permutation to predict theoretical material properties that can be then observed in everyday life. For example, you can find out what is the average velocity of gas particles.

## FAQ

### Is acceleration a vector?

**Yes**, acceleration is a vector as **it has both magnitude and direction**. The magnitude is how quickly the object is accelerating, while the direction is if the acceleration is in the direction that the object is moving, or against it. This is acceleration and deceleration respectively.

### How does mass affect acceleration?

If the force the object is being pushed with stays the same, the **acceleration will decrease as the mass increases**. This is because F/m = a, so as the mass increases the fraction becomes smaller and smaller.

### Can acceleration be negative?

**Yes**, acceleration can be negative, **which is known as deceleration**. Two objects that have equal but opposite acceleration will be accelerating by the same amount, just in two opposite directions.

### How do you find average acceleration?

- Work out the
**change in velocity**for you given time. -
Calculate the
**change in time**for the period you are considering. - Divide the change in velocity by the change in time.
- The result is the average acceleration for that period.

### How do I find the magnitude of acceleration?

- Convert the
**magnitude of the force**into Newtons. -
Change the
**mass**of the object to kilograms. -
Multiply both values by together to find the acceleration in m/s
^{2}.

### What is the difference between velocity and acceleration?

**Velocity is the speed with which an object is moving** in a particular direction, while **acceleration is how the speed of that object changes** with time. Both have a magnitude and a direction, but their units are m/s and m/s^{2} respectively.

### How do you find angular acceleration?

- Find the
**initial and final angular velocity**in radians/s. -
Subtract the final angular velocity from the initial angular velocity to get the
**change in angular velocity**. -
Find the
**initial and final time**for the period being considered. -
Subtract the final time from the initial time to get the
**change in time**. -
Divide the change in angular velocity by the change in time to get the angular acceleration in radians/s
^{2}.