# Newton's laws of motion <!-- MICROSIMGEN:BEGIN v1.7 — generated by g08_place_microsims.py; three.js first (§15); do not hand-edit inside --> ## Microsims — p5.js ### Newton's laws of motion (p5.js) <div class="microsim-player"> <iframe src="https://editor.p5js.org/sciencenibber/full/ONl3-NO3g" width="100%" height="480" frameborder="0" loading="lazy" sandbox="allow-scripts allow-same-origin" title="Newton's laws of motion — p5.js microsim"></iframe> </div> *Newton's three laws animated; apply a force to a mass and watch inertia, F = m·a acceleration, and the equal-and-opposite reaction play out live.* **Open in the editor:** [&#9654; fork this sketch](https://editor.p5js.org/sciencenibber/sketches/ONl3-NO3g) · library `p5js` ### Related microsims Live sims on neighbouring articles — 1 of them inside this article's own Wikipedia link tree: - [[Force]] *(in tree)* *Sim hosted off-article; the article owns the reference, not the runtime (WIKI_RULES §10.4). Placed by `g08_place_microsims.py`.* <!-- MICROSIMGEN:END --> ## Microsim > *Microsim pending. The pipeline is currently authoring and saving a sketch in the [p5.js Web Editor](https://editor.p5js.org). Once saved, this section will hold the editor URL, a 100-word description of what the sketch demonstrates, and the full source code.* **Editor URL:** `<paste editor URL after save>` **Description (100 words):** _<filled in at finalize>_ ```js // sketch.js will be inlined here once finalized ``` ## Links (Wikipedia order) <!-- injected from _registry/childlinks/Newton's_laws_of_motion.json (2026-07-30T02:09:12Z) --> `Abraham_de_Moivre` · `Absolute_space_and_time` · `Acceleration` · `Acceleration_(special_relativity)` · `Action_at_a_distance` · `Aether_theories` · `Albert_of_Saxony_(philosopher)` · `Alchemy` · `Alexis_Clairaut` · `American_Journal_of_Physics` · `An_Historical_Account_of_Two_Notable_Corruptions_of_Scripture` · `Analytical_mechanics` · `Andrew_M._Gleason` · `Andrew_Wiles` · `Angular_acceleration` · `Angular_displacement` · [[Angular_frequency]] · `Angular_momentum` · `Angular_velocity` · `Anneliese_Maier` · `Anthony_French` · `Anthony_Zee` · `Appell's_equation_of_motion` · 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`The_Princeton_Companion_to_Mathematics` · `The_World_(book)` · `Theory_of_impetus` · `Theory_of_relativity` · `Thermal_energy` · `Thought_experiment` · `Three-body_problem` · `Tide` · `Time` · `Timeline_of_classical_mechanics` · `Timothy_Gowers` · `Tom_M._Apostol` · `Torque` · `Traité_de_mécanique_céleste` · `Trinity_College,_Cambridge` · `Truncated_Newton_method` · `Two-body_problem` · `Variable-mass_system` · `Vector_(mathematics_and_physics)` · [[Velocity]] · `Vibration` · `Virtual_work` · `Vis_viva` · [[Viscosity]] · `William_Clarke_(apothecary)` · `William_G._McCallum` · `William_Jones_(mathematician)` · `William_R._Newman` · `William_Rowan_Hamilton` · `William_Stukeley` · `William_Whiston` · `Woolsthorpe_Manor` · `Work_(physics)` · `Wren_Library` · `XMM-Newton` · `Yvonne_Choquet-Bruhat` · `Émilie_du_Châtelet` ## From the Real GENERATIVE library ![Newton's Laws of Motion](https://upload.wikimedia.org/wikipedia/commons/thumb/6/6f/Stylised_atom_with_three_Bohr_model_orbits_and_stylised_nucleus.svg/14px-Stylised_atom_with_three_Bohr_model_orbits_and_stylised_nucleus.svg.png) *Newton's Laws of Motion — placed from the Real G.E.N.E.R.A.T.I.V.E. course library (Engineering room). Source: Wikimedia Commons (via Wikipedia article media). [Details & license](https://commons.wikimedia.org/wiki/File:Stylised_atom_with_three_Bohr_model_orbits_and_stylised_nucleus.svg).* ![Animated: Newton's Laws of Motion](https://upload.wikimedia.org/wikipedia/commons/a/ae/Binary_system_orbit_q%3D3_e%3D0.gif) *Animated: Newton's Laws of Motion — placed from the Real G.E.N.E.R.A.T.I.V.E. course library (Engineering room). Source: Wikimedia Commons (via Wikipedia article media). [Details & license](https://commons.wikimedia.org/wiki/File:Binary_system_orbit_q%3D3_e%3D0.gif).* > Newton's laws of motion are three physical laws that describe the relationship between the motion of an object and the forces acting on it. These laws, which provide the basis for Newtonian mechanics, can be paraphrased as follows: ([Wikipedia](https://en.wikipedia.org/wiki/Newton%27s_Laws_of_Motion)) <!-- REAL-GENERATIVE-MEDIA:END --> ## Media (PD/CC) <!-- MEDIA-DEPLOY:Newton's_laws_of_motion/Binary_system_orbit_q=3_e=0.gif --> !Gif Library/Newtonian mechanics/Binary system orbit q=3 e=0.gif *Binary_system_orbit_q=3_e=0.gif · Philip D. Hall · CC BY-SA 4.0 · [source](https://commons.wikimedia.org/wiki/File:Binary_system_orbit_q%3D3_e%3D0.gif)* <!-- /MEDIA-DEPLOY --> <!-- SIGN-SYSTEMS:START --> **Semiotic universals** (the notations and alphabet letters this article speaks — each opens its canonical card): kanji radicals · force · energy · momentum · conservation. Index: the glyph gallery · SEMIOTICS PORTAL. <!-- SIGN-SYSTEMS:END --> > **Room:** [[Energy]] · **Status:** ⏳ awaiting microsim · ← back to MAIN ## Overview Newton's laws of motion are the three foundational propositions that govern the dynamics of classical bodies under forces. Stated by [[Isaac_Newton|Isaac Newton]] in his 1687 Philosophiae Naturalis Principia Mathematica, they remain the conceptual backbone of mechanics for any [[System|system]] whose speeds are small compared with light and whose action is large compared with Planck's constant. The First Law (inertia) asserts that a body persists in its state of rest or uniform motion in a straight line unless compelled to change by a net external [[Force|force]]; the law makes inertial frames the privileged setting for the other two and pins down what "force" must mean. The Second Law packages the relationship between force and motion: the time rate of change of momentum equals the applied force, F = dp/dt, which for constant mass collapses to the celebrated F = m*a. The Third Law states that whenever one body exerts a force on a second, the second exerts an equal and opposite force on the first; pairwise this guarantees conservation of total linear momentum for any [[Isolated_system|isolated system]]. Together the three laws are equivalent to a complete prescription for the trajectories of point particles and, by integration over rigid distributions, of extended bodies. ## See also - Room hub: [[Energy]] - p5.js Editor conventions: P5 JS EDITOR - Wiki root: MAIN --- *Scaffolded by `generative-microsim` from row 0 of the Energy sheet on 2026-04-30T09:28:35Z.* <!-- REAL-GENERATIVE-MEDIA:START --> <!-- CRAFT-LINK:START g12 --> *Built to the [[WT!P5_js_Microsim_Master_Class|p5.js Master Class]].* <!-- CRAFT-LINK:END --> <!-- SPINEPATH:BEGIN g20 — shortest chain of Wikipedia links between local articles to a Compendium Main article; do not hand-edit inside --> *Connected to the Apex Spine:* Newton's laws of motion → [[Fluid_dynamics|Fluid dynamics]] — [[WT!Thury_Hydrodynamics_Compendium|Compendium]] section 1, *Fluid dynamics*. <!-- SPINEPATH:END --> <!-- MATTERSIM:BEGIN g33 — Matter & Energy Cluster microsim (framework build, specs/sims/Newton's_laws_of_motion.json); do not hand-edit inside --> **Microsim — three.js (Wikitube framework):** *Newton's laws of motion* <div class="wt-sim" data-src="https://wikitube-3d-microsims.netlify.app/matter/Newton's_laws_of_motion.html" data-title="Newton's laws of motion"></div> *Built from `MICROSIM_GUIDE/specs/sims/Newton's_laws_of_motion.json`; part of the [[PORTAL_Matter|Matter portal]] spine (section sims and See-also variants).* <!-- MATTERSIM:END --> ## Wikipedia : Wikitube **Strict pair:** [Wikipedia](https://en.wikipedia.org/wiki/Newton's_laws_of_motion) : [Wikitube](https://en.wikitube.io/wiki/Newton's_laws_of_motion) ## Previous hub tags Tree parents: [[Dynamical_system]] · [[Systems_theory]]. Legacy hubs: `GENERATIVE`. --- *Sources: 1 legacy note. Minted wave 1, 2026-07-30 (v1.6 order).*