Mechanics of particles and systems Foundations of particle mechanics Fact
Newton's laws of motion
Builds on Classical mechanicsInertial frame of referenceMomentum
Statement
Consider point particles described in an inertial frame of reference, in the setting of classical mechanics. Write for the mass of a particle, for its position at time , and for its momentum.
- First law: a particle on which the net force is zero moves with constant velocity.
- Second law: if is the net force on a particle at time , then ; for constant mass this reads .
- Third law: if is the force that particle exerts on particle , then .
Remarks
The three laws are the axioms of Newtonian mechanics, not theorems; they are confirmed by experiment within their range of validity. The first law singles out the inertial frames, and the second law then gives the equations of motion, a system of second-order differential equations. The third law, together with the second, gives conservation of the total momentum of an isolated system. The strong form of the third law adds that is parallel to ; it gives conservation of angular momentum as well. Example: a ball of mass near the ground feels the force , so the second law gives . The ball then moves on a parabola, or on a vertical line if it is thrown straight up or down. In a rotating frame the second law fails unless fictitious forces are added, which is why the frame must be inertial.
Going deeper
For a student
The second law turns a mechanical problem into an initial value problem for an ordinary differential equation. Under mild conditions on the forces, the positions and velocities at one time determine the motion. From the three laws one derives the conservation laws of momentum, angular momentum and, for conservative forces, energy. Lagrangian and Hamiltonian mechanics reformulate the same laws in coordinates adapted to constraints and symmetries.
Reading path
To understand this page from the ground up, read these 9 pages in order. The foundations come first.
Show the path as a graph
- no evidence level
- Derivative concept
- Euclidean space object
- Euclidean vector concept
- Ordinary differential equation concept
- Velocity concept
- Classical mechanics concept
- Momentum concept
- Inertial frame of reference concept
- Newton's laws of motion statement
Where this leads
122 pages build on this one.
- Emden–Chandrasekhar equation
- Newton's law of universal gravitation
- Physical oceanography
- Chandrasekhar's white dwarf equation
- Dedekind ellipsoid
- Hydrostatic equilibrium
- Tidal force
- Molecular dynamics
- Magnetic braking
- Coriolis force
- Virial theorem
- Tests of general relativity
- Milankovitch cycles
- Stellar structure
- Thermal wind
- Modified Newtonian dynamics
- Kelvin–Helmholtz mechanism
- Atmospheric dynamics
- Hohmann transfer orbit
- Central configuration
- Schwarzschild criterion for convection
- Virial mass
- von Zeipel theorem
- Norton's dome
- Jacobi integral
- Galaxy rotation curve
- Celestial mechanics
- Weak gravitational lensing
- Kepler's equation
- Bi-elliptic transfer
- Ekman spiral
- Mass–luminosity relation
- Accretion disk
- Conservation of energy
- Einstein–Infeld–Hoffmann equations
- Lens equation
- Taylor's constraint
- Two-body problem
- Ledoux criterion
- Impulse
- Orbital mechanics
- Bonnor–Ebert mass
- Tolman–Oppenheimer–Volkoff limit
- Post-Newtonian expansion
- Adams–Williamson equation
- Tisserand's parameter
- Polytrope
- Projectile motion
- Gravitational microlensing
- Painlevé paradox
- Tsiolkovsky rocket equation
- Hayashi track
- Stellar pulsation
- Euler's three-body problem
- Conservation of angular momentum
- Parker solar wind model
- Hadley cell and Held–Hou model
- Impulse
- Elsasser number
- Clohessy–Wiltshire equations
- Escape velocity
- Chandrasekhar limit
- Tidal acceleration
- Gravitational deflection of light
- Fictitious force
- Maclaurin spheroid
- Jacobi integral
- Kepler's laws of planetary motion
- Dynamical friction
- Mixing length theory
- Kepler's equation
- Kepler orbit
- Foucault pendulum
- Euler force
- Hill sphere
- Spherical astronomy
- Roche limit
- Coriolis force
- Stommel's model of western intensification
- Baroclinic instability
- Mechanical similarity
- Schönberg–Chandrasekhar limit
- Geopotential
- N-body simulation
- Celestial mechanics
- Vogt–Russell theorem
- Eddington luminosity
- Hill sphere
- Barnes–Hut simulation
- Vis-viva equation
- Euler's laws of motion
- Work–energy theorem
- Stellar dynamics
- Rigid body dynamics
- Conservation of momentum
- Variable-mass system
- Parker instability
- Cauchy momentum equation
- F-plane
- Einstein radius
- Sitnikov problem
- Sverdrup balance
- Mechanical similarity
- Free-fall time
- Jacobi ellipsoid
- Lagrange points
- Two-body relaxation time
- Munk's wind-driven circulation model
- Parker spiral
- Centrifugal force
- Atwood machine
- Beta plane
- Newtonian limit
- Strong gravitational lensing
- Einstein ring
- Cauchy's stress theorem
- Circular restricted three-body problem
- Gradient wind
- Bullen parameter
- Roche lobe
- Laplace tidal equations
- Fictitious force
Further reading
About this page
| Tag | KNBP19FG6K |
|---|---|
| URI | m2://KNBP19FG6K |
| Kind | statement, fact |
| Writing | W0 stub |
| MSC | 70A05, 70F10 |
| Status | This copy of the site has no build data. Run m2 status KNBP19FG6K. |
| About | Classical mechanics, Inertial frame of reference |
| Uses | Classical mechanics, Inertial frame of reference, Momentum |
| Same as | |
| Changed | 3 November 2026 |
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What links here
Used by
- Newton's law of universal gravitation
- Molecular dynamics
- Virial theorem
- Norton's dome
- Conservation of energy
- Impulse
- Orbital mechanics
- Projectile motion
- Painlevé paradox
- Conservation of angular momentum
- Impulse
- Fictitious force
- Mechanical similarity
- Euler's laws of motion
- Work–energy theorem
- Rigid body dynamics
- Conservation of momentum
- Variable-mass system
- Mechanical similarity
- Atwood machine
- Fictitious force