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Newton's laws of motion

What a force is, how mass is measured, and the three laws that connect forces to motion.

You need this first

Full reading path (4 pages)
  1. Vectors (8.01)
  2. Position and velocity in one dimension (8.01)
  3. Acceleration in one dimension (8.01)
  4. Motion in two dimensions and projectiles (8.01)
On this page · 8 sections
  1. What is a force?
  2. Measuring mass
  3. The first law: inertia
  4. The second law: force changes momentum
  5. The third law: forces come in pairs
  6. Try it
  7. Where Newton's laws stop working
  8. Summary

The previous lessons described how things move. Newton's laws explain why: they connect motion to the forces that act on a body. Isaac Newton published them in 1687 in the Principia, building on Galileo's work on falling bodies and inertia.

What is a force?#

In everyday language a force is a push or a pull. Physics needs something we can measure. The MIT notes define force operationally, through the acceleration it produces on a chosen standard body of mass msm_s:

Force, defined with a standard body
F⃗≡ms a⃗\vec F \equiv m_s\,\vec a
In words

vector F is defined as m sub s vector a

Source: 8.01SC Course Notes, Chapter 7: Newton's Laws of Motion, Sections 7.1–7.4, Sec. 7.1, Eq. (7.1.1)

A force has a size and a direction, the direction of the acceleration it causes. Experiments then show something that is not obvious: when two forces act together, the accelerations add as vectors, so the forces add as vectors too. That is why we can find the net force on a body by vector addition.

Measuring mass#

Apply the same force to the standard body and to an unknown body. The unknown body's inertial mass follows from the ratio of the accelerations:

Mass from equal forces
min=ms asainm_\text{in} = m_s\,\frac{a_s}{a_\text{in}}
In words

m sub in equals m sub s a sub s over a sub in

Source: 8.01SC Course Notes, Chapter 7: Newton's Laws of Motion, Sections 7.1–7.4, Sec. 7.1.1, Eq. (1.9) as printed

A body that accelerates half as much under the same push has twice the mass. Mass is a measure of inertia, of how hard it is to change a body's motion.

The first law: inertia#

With no net force acting on it, a body stays at rest or keeps moving in a straight line at constant speed.

Before Galileo, it seemed natural that moving things need a push to keep going, because on Earth friction always slows them down. The first law says the opposite. Motion at constant velocity needs no cause; only changes in velocity do. Any change in speed or direction means a net force is acting.

The first law also tells us which reference frames to use. A frame in which it holds is called an inertial frame. Sitting in a train moving smoothly at constant velocity, no experiment inside the carriage can tell you whether you are moving or the station is. Both frames are inertial. A train that is braking or turning is not: objects in it start to move with no force pushing them.

MIT's segments 4.3 and 4.4 make this precise. If one frame moves at constant velocity relative to another, both measure the same acceleration for any object, so F⃗=ma⃗\vec F = m\vec a holds equally in both: every frame moving at constant velocity relative to an inertial frame is itself inertial. If a frame accelerates with A⃗\vec A, objects in it seem to feel an extra fictitious force −mA⃗-m\vec A, the push back into your seat when a car speeds up. No real body exerts that force; it only appears because the frame is accelerating.

The second law: force changes momentum#

Newton described motion through the momentum p⃗=mv⃗\vec p = m\vec v. A force acting for a short time Δt\Delta t changes the momentum by Δp⃗=F⃗ Δt\Delta\vec p = \vec F\,\Delta t, the impulse. In the limit of a very short time:

Newton's second law
F⃗=dp⃗dtand, for constant mass,F⃗=m dv⃗dt=m a⃗\vec F = \frac{d\vec p}{dt} \qquad\text{and, for constant mass,}\qquad \vec F = m\,\frac{d\vec v}{dt} = m\,\vec a
In words

vector F equals d vector p over dt and, for constant mass, vector F equals m d vector v over dt equals m vector a

Source: 8.01SC Course Notes, Chapter 7: Newton's Laws of Motion, Sections 7.1–7.4, Sec. 7.3, Eqs. (7.3.1)–(7.3.5)

Here F⃗\vec F is the total force, the vector sum of every force on the body. This equation is more than a definition, because each kind of force (gravity, springs, electric forces) has its own force law found by experiment. Put a force law into F⃗=ma⃗\vec F = m\vec a and you can predict motion.

Worked example

Two forces on a puck

A 2.02.0 kg puck rests on frictionless ice. Two people pull on it with horizontal ropes: F⃗1=(6.0 N) i^\vec F_1 = (6.0\ \text{N})\,\hat i and F⃗2=(−2.0 N) i^+(4.0 N) j^\vec F_2 = (-2.0\ \text{N})\,\hat i + (4.0\ \text{N})\,\hat j. Find its acceleration and its velocity after 3.03.0 s.

Add the forces as vectors

F⃗net=(6.0−2.0) i^+(0+4.0) j^=(4.0 i^+4.0 j^)\vec F_\text{net} = (6.0 - 2.0)\,\hat i + (0 + 4.0)\,\hat j = (4.0\,\hat i + 4.0\,\hat j) N. (Gravity and the ice's upward push cancel, so they are left out.)

Apply the second law

a⃗=F⃗net/m=(2.0 i^+2.0 j^) m/s2\vec a = \vec F_\text{net}/m = (2.0\,\hat i + 2.0\,\hat j)\ \text{m/s}^2, with magnitude 2.83 m/s22.83\ \text{m/s}^2, pointing at 45∘45^\circ between the +x+x and +y+y axes.

Velocity after 3.0 s

The acceleration is constant and the puck starts at rest, so v⃗=a⃗ t=(6.0 i^+6.0 j^) m/s\vec v = \vec a\,t = (6.0\,\hat i + 6.0\,\hat j)\ \text{m/s}, a speed of 8.5 m/s8.5\ \text{m/s}.

The third law: forces come in pairs#

Newton's third law
F⃗1,2=−F⃗2,1\vec F_{1,2} = -\vec F_{2,1}
In words

vector F sub 1,2 equals minus vector F sub 2,1

Source: 8.01SC Course Notes, Chapter 7: Newton's Laws of Motion, Sections 7.1–7.4, Sec. 7.4, Eq. (7.4.1)

Here F⃗1,2\vec F_{1,2} means the force on body 2 due to body 1. Every force is one half of an interaction: if you push on a wall, the wall pushes back on you just as hard. The two forces act on different bodies, so they never cancel each other out in one body's equation of motion.

Try it#

Push a crate, add friction, and watch the net force, the acceleration and the speed change.

Forces and Motion: Basics. Simulation by PhET Interactive Simulations, University of Colorado Boulder, licensed under CC BY-NC 4.0 (https://phet.colorado.edu). Open full screen

Where Newton's laws stop working#

The MIT notes stress that Newtonian mechanics is a model with limits. At speeds approaching the speed of light it is replaced by special relativity. For electrons in atoms it is replaced by quantum mechanics. And for the structure of the universe on the largest scales, it is replaced by general relativity. Those are exactly the subjects of later years on this site.

Summary#

  • A force is defined by the acceleration it produces; forces add as vectors.
  • Mass measures inertia: under the same force, min/ms=as/ainm_\text{in}/m_s = a_s/a_\text{in}.
  • First law: no net force means constant velocity (and defines inertial frames).
  • Second law: F⃗=dp⃗/dt=ma⃗\vec F = d\vec p/dt = m\vec a, with F⃗\vec F the total force.
  • Third law: F⃗1,2=−F⃗2,1\vec F_{1,2} = -\vec F_{2,1}; the pair acts on two different bodies.

Symbols on this page

Show the 5 symbols used here
Δ\Delta capital delta
A change or difference in a quantity, e.g. Δx = x₂ − x₁. Say it: “capital delta”.
∘\circ degree
Degrees of angle (as in 45°). Say it: “degrees”.
≡\equiv identical to
Is defined as (or is identically equal to). Say it: “is defined as”.
v⃗\vec v vector arrow
A vector: a quantity with a size and a direction. Say it: “vector”.
ı^\hat\imath hat
A unit vector: a vector of length 1 that only gives a direction (î, r̂). Say it: “hat”.

Tap or click a symbol in a formula to see the same explanation. All symbols: symbols and notation.

Where this leads

In cosmology

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Check your understanding

  1. A hockey puck slides across frictionless ice at constant velocity. What is the net force on it?
  2. The same force gives object A an acceleration of 6 m/s26\ \text{m/s}^2 and object B an acceleration of 2 m/s22\ \text{m/s}^2. How do their masses compare?
  3. A small car collides with a heavy truck. During the collision, the force of the car on the truck is…
  4. Two forces act on a 2.0 kg2.0\ \text{kg} object: F⃗1=(6 N)i^\vec F_1 = (6\ \text{N})\hat i and F⃗2=(−2 N)i^+(4 N)j^\vec F_2 = (-2\ \text{N})\hat i + (4\ \text{N})\hat j. What is its acceleration?
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Flashcards

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Credits and license

This page is a rewritten explanation based on MIT 8.01SC Lesson 4: Newton's Laws of Motion (4.1–4.4) from MIT 8.01SC Classical Mechanics (Fall 2016), taught by Prof. Deepto Chakrabarty, Dr. Peter Dourmashkin, Dr. Michelle Tomasik, Prof. Anna Frebel and Prof. Vladan Vuletic, published on MIT OpenCourseWare under CC BY-NC-SA 4.0.

MIT readings used: 8.01SC Course Notes, Chapter 7: Newton's Laws of Motion (Sections 7.1–7.4).

The 8.01SC course notes, Chapter 7, are © Peter Dourmashkin 2012 and published by MIT OpenCourseWare under CC BY-NC-SA 4.0.

MIT and the instructors do not endorse this site. All diagrams and plots on this page are generated by this site. This page is licensed CC BY-NC-SA 4.0: you may share and adapt it for non-commercial use with attribution, under the same license.