{"id":588,"date":"2026-07-17T11:20:14","date_gmt":"2026-07-17T11:20:14","guid":{"rendered":"https:\/\/physicsfundamentalsinfo.com\/blog\/?p=588"},"modified":"2026-08-24T13:04:03","modified_gmt":"2026-08-24T13:04:03","slug":"physics-formulas","status":"publish","type":"post","link":"https:\/\/physicsfundamentalsinfo.com\/blog\/mechanics\/physics-formulas\/","title":{"rendered":"Physics Formulas: The Complete Cheat Sheet"},"content":{"rendered":"\n<div class=\"pf-citation\"><div class=\"eyebrow\">Definition<\/div><p>\nPhysics formulas are compact equations that state exactly how measurable physical quantities depend on one another, such as force equals mass times acceleration. Each symbol stands for a quantity with its own SI unit, so a formula is both a calculation rule and a statement about how the physical world behaves.\n<\/p><\/div>\n\n<p>Open any physics textbook to the inside back cover and you meet a wall of equations. Dozens of them, packed shoulder to shoulder, with no hint about which ones matter or how they connect. It reads like a list to be memorised. It isn&#8217;t.<\/p>\n\n<p>Here is what actually happens in an exam hall. You know the physics cold \u2014 and then you stall, because you cannot recall whether it was v<sup>2<\/sup> = u<sup>2<\/sup> + 2as or v<sup>2<\/sup> = u<sup>2<\/sup> + 2at, and you have ninety seconds to choose. That moment is what this page is built for.<\/p>\n\n<h2>What Are Physics Formulas?<\/h2>\n\n<p>A physics formula is a compact statement that one physical quantity is fixed by other physical quantities in an exact, testable way. Not a rule of thumb. Not an approximation someone found convenient. A claim about reality that experiment can break.<\/p>\n\n<p>Take Q = mc\u0394T. It says the heat you must pour into something is set by three things and nothing else: how much of it there is, what it is made of, and how far you want its temperature to move. Change any one of those and the answer moves with it, in a way you can predict before you touch the apparatus.<\/p>\n\n<p>That is the part most formula sheets throw away. They give you the equation and leave out what each letter <em>is<\/em> \u2014 which is precisely the information you need to use it.<\/p>\n\n<figure class=\"pf-figure\" style=\"margin:1.6em 0;\"><img src=\"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-content\/uploads\/2026\/08\/physics-formulas-labelling-every-part-formula-q.webp\" width=\"1400\" height=\"754\" alt=\"Physics formulas - Diagram labelling every part of the physics formula Q equals m c delta T, showing each symbol as a quantity with its SI unit, and a unit check confirming joules on both sides\" loading=\"lazy\" decoding=\"async\" style=\"width:100%;height:auto;max-width:700px;display:block;margin:0 auto;\" \/><\/figure>\n\n<p style=\"text-align:center;font-size:13px;font-style:italic;color:#1F2E47;margin-top:-14px;\">Every physics formula has this same anatomy: a subject, quantities, and units that must cancel correctly on both sides.<\/p>\n\n<h3>Every Symbol Is a Quantity, and Every Quantity Has a Unit<\/h3>\n\n<p>The unit line at the bottom of that diagram is not decoration \u2014 it is a free correctness check. Kilograms times joules-per-kilogram-per-kelvin times kelvin leaves joules. The kilograms cancel, the kelvins cancel, and joules survive on both sides.<\/p>\n\n<p>If your units do not cancel down to the units of the answer, the formula is wrong or you have written it down wrong. No exceptions. This works because since 20 May 2019 the entire <a href=\"https:\/\/www.bipm.org\/en\/measurement-units\" target=\"_blank\" rel=\"noopener\">International System of Units<\/a> has been defined by seven fixed constants of nature, so every unit in every formula on this page traces back to the same seven numbers.<\/p>\n\n<h2>The 10 Groups That Organise Every Physics Formula<\/h2>\n\n<p>Introductory physics is not one subject with a hundred formulas. It is ten small subjects with about ten formulas each \u2014 and that reframing is the single most useful thing on this page.<\/p>\n\n<p>Each group answers one question, and each has one signature formula that the rest of the group hangs off. Learn the signature and you have a hook to hang the others on.<\/p>\n\n<figure class=\"pf-figure\" style=\"margin:1.6em 0;\"><img src=\"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-content\/uploads\/2026\/08\/physics-formulas-map-ten-groups-each-signature.webp\" width=\"1400\" height=\"964\" alt=\"Map of the ten groups of physics formulas, each with its signature formula: kinematics, forces, energy, momentum, gravitation, fluids, thermodynamics, waves, electricity and modern physics\" loading=\"lazy\" decoding=\"async\" style=\"width:100%;height:auto;max-width:700px;display:block;margin:0 auto;\" \/><\/figure>\n\n<p style=\"text-align:center;font-size:13px;font-style:italic;color:#1F2E47;margin-top:-14px;\">The ten groups of physics formulas and the signature equation of each.<\/p>\n\n<div class=\"pf-table-scroll\" style=\"display:block;width:100%;max-width:100%;overflow-x:auto;-webkit-overflow-scrolling:touch;margin:1.5em 0;\">\n<table style=\"width:100%;border-collapse:collapse;\">\n<thead>\n<tr style=\"background:#0A1628;color:#FAF6EE;\">\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">#<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Group<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">The question it answers<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Signature formula<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Core SI units<\/th>\n<\/tr>\n<\/thead>\n<tbody>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">1<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><strong>Kinematics<\/strong><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">How is it moving?<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">v = u + at<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">m, s, m\/s, m\/s<sup>2<\/sup><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">2<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><strong>Forces<\/strong><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Why did the motion change?<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">F = ma<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">N, kg, m\/s<sup>2<\/sup><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">3<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><strong>Work, energy &amp; power<\/strong><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">What did it cost, and how fast?<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">KE = \u00bdmv<sup>2<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">J, W<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">4<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><strong>Momentum<\/strong><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">What survives a collision?<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">p = mv<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">kg\u00b7m\/s, N\u00b7s<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">5<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><strong>Circular motion &amp; gravitation<\/strong><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">What holds it on a curve?<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">F = GMm\/r<sup>2<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">N, m, rad\/s<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">6<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><strong>Fluids<\/strong><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Will it float, and how hard does it push?<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">P = F\/A<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Pa, kg\/m<sup>3<\/sup><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">7<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><strong>Thermodynamics<\/strong><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Where did the heat go?<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Q = mc\u0394T<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">J, K, Pa<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">8<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><strong>Waves, sound &amp; optics<\/strong><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">How does it travel and repeat?<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">v = f\u03bb<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Hz, m, m\/s<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">9<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><strong>Electricity &amp; magnetism<\/strong><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">What is charge doing?<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">V = IR<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">V, A, \u03a9, T<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">10<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><strong>Modern physics<\/strong><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">What happens when it is very fast or very small?<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">E = mc<sup>2<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">J, eV, Hz<\/td><\/tr>\n<\/tbody>\n<\/table>\n<\/div>\n\n<p>Everything below is grouped in that order. If you would rather put numbers in than read equations, every formula here also has a matching tool in our <a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/\">library of 97 physics calculators<\/a>, which solves each one for any variable you like.<\/p>\n\n<h2>Mechanics Formulas: Motion, Forces, Energy and Momentum<\/h2>\n\n<p>Mechanics is roughly half of any introductory course, and groups 1 to 5 all live here. Start with motion described, then move to motion explained.<\/p>\n\n<h3>Kinematics: Constant Acceleration (SUVAT)<\/h3>\n\n<p>These five formulas describe any object whose acceleration does not change. They are not five separate facts \u2014 they are one fact viewed from five angles, which is why you can always get from any three known quantities to the other two.<\/p>\n\n<div class=\"pf-formula\">v = u + at<\/div>\n\n<div class=\"pf-table-scroll\" style=\"display:block;width:100%;max-width:100%;overflow-x:auto;-webkit-overflow-scrolling:touch;margin:1.5em 0;\">\n<table style=\"width:100%;border-collapse:collapse;\">\n<thead>\n<tr style=\"background:#0A1628;color:#FAF6EE;\">\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Formula<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Gives you<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Use it when<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Calculator<\/th>\n<\/tr>\n<\/thead>\n<tbody>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">v = u + at<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Final velocity<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">You know the time, not the distance<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/suvat\">SUVAT<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">s = ut + \u00bdat<sup>2<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Displacement<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">You know the time and the start speed<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/suvat\">SUVAT<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">s = \u00bd(u + v)t<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Displacement<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">You know both speeds, not the acceleration<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/suvat\">SUVAT<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">v<sup>2<\/sup> = u<sup>2<\/sup> + 2as<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Final velocity<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><strong>Time is not mentioned<\/strong> \u2014 the most useful one<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/suvat\">SUVAT<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">s = vt \u2212 \u00bdat<sup>2<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Displacement<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">You know the end speed, not the start<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/suvat\">SUVAT<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">v<sub>av<\/sub> = \u0394s \/ \u0394t<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Average velocity<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Acceleration is not constant<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/velocity\">Velocity<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">a = \u0394v \/ \u0394t<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Average acceleration<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Acceleration is not constant<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/acceleration\">Acceleration<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">R = v<sub>0<\/sub><sup>2<\/sup> sin(2\u03b8) \/ g<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Projectile range<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Level ground, no air resistance<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/projectile-motion\">Projectile Motion<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">H = v<sub>0<\/sub><sup>2<\/sup> sin<sup>2<\/sup>\u03b8 \/ (2g)<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Projectile peak height<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Level ground, no air resistance<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/projectile-motion\">Projectile Motion<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">T = 2v<sub>0<\/sub> sin\u03b8 \/ g<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Projectile flight time<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Level ground, no air resistance<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/projectile-motion\">Projectile Motion<\/a><\/td><\/tr>\n<\/tbody>\n<\/table>\n<\/div>\n\n<ul>\n<li><strong>s<\/strong> = displacement \u2014 metres (m)<\/li>\n<li><strong>u<\/strong> = initial velocity \u2014 metres per second (m\/s)<\/li>\n<li><strong>v<\/strong> = final velocity \u2014 metres per second (m\/s)<\/li>\n<li><strong>a<\/strong> = acceleration \u2014 metres per second squared (m\/s<sup>2<\/sup>)<\/li>\n<li><strong>t<\/strong> = time \u2014 seconds (s)<\/li>\n<li><strong>v<sub>0<\/sub><\/strong> = launch speed \u2014 metres per second (m\/s)<\/li>\n<li><strong>\u03b8<\/strong> = launch angle above the horizontal \u2014 degrees or radians<\/li>\n<li><strong>g<\/strong> = acceleration due to gravity \u2014 9.81 m\/s<sup>2<\/sup> near Earth&#8217;s surface<\/li>\n<\/ul>\n\n<p>The full derivation of all five, and why the fourth is the one examiners love, is in our guide to the <a href=\"https:\/\/physicsfundamentalsinfo.com\/blog\/kinematics\/suvat-equations\/\">SUVAT equations<\/a>. To skip the algebra entirely, give any three values to the <a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/suvat\">SUVAT calculator<\/a> and it returns the other two.<\/p>\n\n<h3>Forces and Newton&#8217;s Laws<\/h3>\n\n<p>Kinematics tells you what happened. Forces tell you why. The bridge between them is a single equation that Newton published in 1687 and that has not needed correcting since \u2014 except at speeds near light.<\/p>\n\n<div class=\"pf-formula\">F = ma<\/div>\n\n<div class=\"pf-table-scroll\" style=\"display:block;width:100%;max-width:100%;overflow-x:auto;-webkit-overflow-scrolling:touch;margin:1.5em 0;\">\n<table style=\"width:100%;border-collapse:collapse;\">\n<thead>\n<tr style=\"background:#0A1628;color:#FAF6EE;\">\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Formula<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Gives you<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Watch out for<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Calculator<\/th>\n<\/tr>\n<\/thead>\n<tbody>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">\u03a3F = ma<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Acceleration from the <em>net<\/em> force<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">\u03a3F is the total, not one single force<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/newtons-second-law\">Newton&#8217;s 2nd Law<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">W = mg<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Weight (a force)<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Weight is in newtons; mass is in kilograms<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/weight-on-other-planets\">Weight Calculator<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">f = \u03bcN<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Friction force<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">N is the normal force, not always mg<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/friction\">Friction<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">F = kx<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Spring force (Hooke\u2019s law)<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">x is the <em>extension<\/em>, not the total length<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/hookes-law\">Hooke\u2019s Law<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">F = \u0394p \/ \u0394t<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Force as rate of momentum change<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Newton\u2019s actual second law; works if mass changes<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/impulse\">Impulse<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">F<sub>AB<\/sub> = \u2212F<sub>BA<\/sub><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Newton\u2019s third law<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">The pair acts on <em>different<\/em> bodies<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">\u2014<\/td><\/tr>\n<\/tbody>\n<\/table>\n<\/div>\n\n<ul>\n<li><strong>F, \u03a3F<\/strong> = force and net force \u2014 newtons (N), where 1 N = 1 kg\u00b7m\/s<sup>2<\/sup><\/li>\n<li><strong>m<\/strong> = mass \u2014 kilograms (kg)<\/li>\n<li><strong>a<\/strong> = acceleration \u2014 metres per second squared (m\/s<sup>2<\/sup>)<\/li>\n<li><strong>W<\/strong> = weight \u2014 newtons (N)<\/li>\n<li><strong>f<\/strong> = friction force \u2014 newtons (N)<\/li>\n<li><strong>\u03bc<\/strong> = coefficient of friction \u2014 dimensionless (no unit)<\/li>\n<li><strong>N<\/strong> = normal force \u2014 newtons (N)<\/li>\n<li><strong>k<\/strong> = spring constant \u2014 newtons per metre (N\/m)<\/li>\n<li><strong>x<\/strong> = extension from natural length \u2014 metres (m)<\/li>\n<li><strong>p<\/strong> = momentum \u2014 kilogram metres per second (kg\u00b7m\/s)<\/li>\n<\/ul>\n\n<p>Three laws underpin that whole table, and they are worth reading as a set rather than three slogans \u2014 our explainer on <a href=\"https:\/\/physicsfundamentalsinfo.com\/blog\/mechanics\/newtons-laws-of-motion\/\">Newton&#8217;s laws of motion<\/a> covers what each one actually claims.<\/p>\n\n<h3>Work, Energy and Power<\/h3>\n\n<p>Energy is the accountant of physics. It never lies and it never vanishes \u2014 it only changes form, and every formula in this group is a statement about where it went.<\/p>\n\n<div class=\"pf-formula\">KE = \u00bdmv<sup>2<\/sup><\/div>\n\n<div class=\"pf-table-scroll\" style=\"display:block;width:100%;max-width:100%;overflow-x:auto;-webkit-overflow-scrolling:touch;margin:1.5em 0;\">\n<table style=\"width:100%;border-collapse:collapse;\">\n<thead>\n<tr style=\"background:#0A1628;color:#FAF6EE;\">\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Formula<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Gives you<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Note<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Calculator<\/th>\n<\/tr>\n<\/thead>\n<tbody>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">W = Fd cos \u03b8<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Work done by a force<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">\u03b8 = 90\u00b0 means zero work, however tired you feel<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/work-power\">Work &amp; Power<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">KE = \u00bdmv<sup>2<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Kinetic energy<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Double the speed, quadruple the energy<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/kinetic-energy\">Kinetic Energy<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">PE = mgh<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Gravitational potential energy<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Only <em>differences<\/em> in h matter<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/gravitational-potential-energy\">Gravitational PE<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">E<sub>elastic<\/sub> = \u00bdkx<sup>2<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Energy stored in a spring<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Area under a force-extension graph<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/spring-constant\">Spring Constant<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">W<sub>net<\/sub> = \u0394KE<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Work-energy theorem<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Often faster than F = ma<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/kinetic-energy\">Kinetic Energy<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">P = W \/ t<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Power<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">1 W = 1 J\/s<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/power\">Power<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">P = Fv<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Power at constant speed<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">The engine version of P = W\/t<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/power\">Power<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">\u03b7 = (useful \/ total) \u00d7 100%<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Efficiency<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Never above 100%, ever<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/work-power\">Work &amp; Power<\/a><\/td><\/tr>\n<\/tbody>\n<\/table>\n<\/div>\n\n<ul>\n<li><strong>W<\/strong> = work done \u2014 joules (J), where 1 J = 1 N\u00b7m<\/li>\n<li><strong>F<\/strong> = force \u2014 newtons (N)<\/li>\n<li><strong>d<\/strong> = distance moved in the direction of the force \u2014 metres (m)<\/li>\n<li><strong>\u03b8<\/strong> = angle between force and displacement \u2014 degrees or radians<\/li>\n<li><strong>KE, PE<\/strong> = kinetic and potential energy \u2014 joules (J)<\/li>\n<li><strong>h<\/strong> = height change \u2014 metres (m)<\/li>\n<li><strong>P<\/strong> = power \u2014 watts (W)<\/li>\n<li><strong>\u03b7<\/strong> = efficiency \u2014 a percentage or a fraction<\/li>\n<\/ul>\n\n<h3>Momentum, Circular Motion and Gravitation<\/h3>\n\n<p>Momentum is what a collision preserves. Circular motion and gravitation are what happens when a force refuses to point along the direction of travel.<\/p>\n\n<div class=\"pf-table-scroll\" style=\"display:block;width:100%;max-width:100%;overflow-x:auto;-webkit-overflow-scrolling:touch;margin:1.5em 0;\">\n<table style=\"width:100%;border-collapse:collapse;\">\n<thead>\n<tr style=\"background:#0A1628;color:#FAF6EE;\">\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Formula<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Gives you<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Note<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Calculator<\/th>\n<\/tr>\n<\/thead>\n<tbody>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">p = mv<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Momentum<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">A vector \u2014 direction counts<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/momentum\">Momentum<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">J = F\u0394t = \u0394p<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Impulse<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Why airbags work: stretch \u0394t, shrink F<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/impulse\">Impulse<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">m<sub>1<\/sub>u<sub>1<\/sub> + m<sub>2<\/sub>u<sub>2<\/sub> = m<sub>1<\/sub>v<sub>1<\/sub> + m<sub>2<\/sub>v<sub>2<\/sub><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Conservation of momentum<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Holds in every collision, elastic or not<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/collision\">Collision<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">a<sub>c<\/sub> = v<sup>2<\/sup> \/ r<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Centripetal acceleration<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Points inward, always<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/circular-motion\">Circular Motion<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">F<sub>c<\/sub> = mv<sup>2<\/sup> \/ r<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Centripetal force<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Not a new force \u2014 a job some force is doing<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/centripetal-force\">Centripetal Force<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">\u03c9 = 2\u03c0f = 2\u03c0 \/ T<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Angular velocity<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Radians per second<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/angular-velocity\">Angular Velocity<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">v = \u03c9r<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Linear speed on a circle<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Outer edge moves faster<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/circular-motion\">Circular Motion<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">F = GMm \/ r<sup>2<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Gravitational force<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">r is centre-to-centre, not surface-to-surface<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/gravitational-force\">Gravitational Force<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">g = GM \/ r<sup>2<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Gravitational field strength<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Why g differs on the Moon<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/gravitational-force\">Gravitational Force<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">v<sub>esc<\/sub> = sqrt(2GM \/ r)<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Escape velocity<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Independent of the escaping mass<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/escape-velocity\">Escape Velocity<\/a><\/td><\/tr>\n<\/tbody>\n<\/table>\n<\/div>\n\n<ul>\n<li><strong>p<\/strong> = momentum \u2014 kilogram metres per second (kg\u00b7m\/s)<\/li>\n<li><strong>J<\/strong> = impulse \u2014 newton seconds (N\u00b7s), identical to kg\u00b7m\/s<\/li>\n<li><strong>u, v<\/strong> = velocity before and after \u2014 metres per second (m\/s)<\/li>\n<li><strong>a<sub>c<\/sub>, F<sub>c<\/sub><\/strong> = centripetal acceleration (m\/s<sup>2<\/sup>) and force (N)<\/li>\n<li><strong>r<\/strong> = radius or separation \u2014 metres (m)<\/li>\n<li><strong>\u03c9<\/strong> = angular velocity \u2014 radians per second (rad\/s)<\/li>\n<li><strong>T<\/strong> = period \u2014 seconds (s); <strong>f<\/strong> = frequency \u2014 hertz (Hz)<\/li>\n<li><strong>G<\/strong> = gravitational constant \u2014 6.674 \u00d7 10<sup>-11<\/sup> N\u00b7m<sup>2<\/sup>\/kg<sup>2<\/sup><\/li>\n<li><strong>M, m<\/strong> = the two masses \u2014 kilograms (kg)<\/li>\n<\/ul>\n\n<h2>Fluids and Thermodynamics Formulas<\/h2>\n\n<p>Both groups deal with the same awkward fact: you cannot track every particle, so you track averages instead. Pressure is an average push; temperature is an average kinetic energy.<\/p>\n\n<h3>Fluids<\/h3>\n\n<div class=\"pf-formula\">P = F \/ A<\/div>\n\n<div class=\"pf-table-scroll\" style=\"display:block;width:100%;max-width:100%;overflow-x:auto;-webkit-overflow-scrolling:touch;margin:1.5em 0;\">\n<table style=\"width:100%;border-collapse:collapse;\">\n<thead>\n<tr style=\"background:#0A1628;color:#FAF6EE;\">\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Formula<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Gives you<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Note<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Calculator<\/th>\n<\/tr>\n<\/thead>\n<tbody>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">\u03c1 = m \/ V<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Density<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Water is 1000 kg\/m<sup>3<\/sup> \u2014 a useful anchor<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/density\">Density<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">P = F \/ A<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Pressure<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">1 Pa = 1 N\/m<sup>2<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/pressure\">Pressure<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">P = \u03c1gh<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Pressure at depth h<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Depends on depth, never on container shape<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/pressure\">Pressure<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">F<sub>1<\/sub>\/A<sub>1<\/sub> = F<sub>2<\/sub>\/A<sub>2<\/sub><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Pascal&#8217;s law (hydraulics)<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Force gain is paid for in distance<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/pascals-law\">Pascal&#8217;s Law<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">F<sub>b<\/sub> = \u03c1Vg<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Buoyant force (Archimedes)<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">\u03c1 is the <em>fluid&#8217;s<\/em> density; V is displaced volume<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/buoyancy\">Buoyancy<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">A<sub>1<\/sub>v<sub>1<\/sub> = A<sub>2<\/sub>v<sub>2<\/sub><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Continuity (flow rate)<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Narrow pipe, faster flow<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/bernoulli-equation\">Bernoulli Equation<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">P + \u00bd\u03c1v<sup>2<\/sup> + \u03c1gh = constant<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Bernoulli&#8217;s equation<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Energy conservation for a streamline<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/bernoulli-equation\">Bernoulli Equation<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">F<sub>d<\/sub> = \u00bd\u03c1v<sup>2<\/sup>C<sub>d<\/sub>A<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Drag force<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Grows with the <em>square<\/em> of speed<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/drag-force\">Drag Force<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">v<sub>t<\/sub> = sqrt(2mg \/ (\u03c1C<sub>d<\/sub>A))<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Terminal velocity<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">When drag finally balances weight<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/terminal-velocity\">Terminal Velocity<\/a><\/td><\/tr>\n<\/tbody>\n<\/table>\n<\/div>\n\n<ul>\n<li><strong>\u03c1<\/strong> = density \u2014 kilograms per cubic metre (kg\/m<sup>3<\/sup>)<\/li>\n<li><strong>P<\/strong> = pressure \u2014 pascals (Pa)<\/li>\n<li><strong>A<\/strong> = area \u2014 square metres (m<sup>2<\/sup>)<\/li>\n<li><strong>V<\/strong> = volume \u2014 cubic metres (m<sup>3<\/sup>)<\/li>\n<li><strong>h<\/strong> = depth or height \u2014 metres (m)<\/li>\n<li><strong>F<sub>b<\/sub><\/strong> = buoyant force \u2014 newtons (N)<\/li>\n<li><strong>C<sub>d<\/sub><\/strong> = drag coefficient \u2014 dimensionless<\/li>\n<li><strong>v<sub>t<\/sub><\/strong> = terminal velocity \u2014 metres per second (m\/s)<\/li>\n<\/ul>\n\n<h3>Thermodynamics and Gas Laws<\/h3>\n\n<div class=\"pf-formula\">Q = mc\u0394T<\/div>\n\n<div class=\"pf-table-scroll\" style=\"display:block;width:100%;max-width:100%;overflow-x:auto;-webkit-overflow-scrolling:touch;margin:1.5em 0;\">\n<table style=\"width:100%;border-collapse:collapse;\">\n<thead>\n<tr style=\"background:#0A1628;color:#FAF6EE;\">\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Formula<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Gives you<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Note<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Calculator<\/th>\n<\/tr>\n<\/thead>\n<tbody>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Q = mc\u0394T<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Heat to change temperature<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Only while it stays in one phase<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/specific-heat\">Specific Heat<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Q = mL<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Heat to change phase<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Temperature does <em>not<\/em> move during this<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/latent-heat\">Latent Heat<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">\u0394L = \u03b1L<sub>0<\/sub>\u0394T<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Thermal expansion<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Why bridges have gaps<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/thermal-expansion\">Thermal Expansion<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">PV = nRT<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Ideal gas law<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">T <strong>must<\/strong> be in kelvin<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/ideal-gas-law\">Ideal Gas Law<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">P<sub>1<\/sub>V<sub>1<\/sub> = P<sub>2<\/sub>V<sub>2<\/sub><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Boyle&#8217;s law<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Constant temperature<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/boyles-law\">Boyle&#8217;s Law<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">V<sub>1<\/sub>\/T<sub>1<\/sub> = V<sub>2<\/sub>\/T<sub>2<\/sub><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Charles&#8217;s law<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Constant pressure<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/charles-law\">Charles&#8217;s Law<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">P<sub>1<\/sub>\/T<sub>1<\/sub> = P<sub>2<\/sub>\/T<sub>2<\/sub><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Gay-Lussac&#8217;s law<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Constant volume<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/gay-lussac-law\">Gay-Lussac&#8217;s Law<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">\u0394U = Q \u2212 W<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">First law of thermodynamics<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Energy conservation, heat included<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">\u2014<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">\u03b7 = 1 \u2212 T<sub>c<\/sub>\/T<sub>h<\/sub><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Carnot efficiency<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">The ceiling no engine can beat<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/carnot-efficiency\">Carnot Efficiency<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Q\/t = kA\u0394T \/ d<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Conduction rate (Fourier)<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Thicker insulation, slower loss<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/thermal-conduction\">Thermal Conduction<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">P = \u03c3A\u03b5T<sup>4<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Radiated power (Stefan-Boltzmann)<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">The fourth power bites hard<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/stefan-boltzmann\">Stefan-Boltzmann<\/a><\/td><\/tr>\n<\/tbody>\n<\/table>\n<\/div>\n\n<ul>\n<li><strong>Q<\/strong> = heat energy \u2014 joules (J)<\/li>\n<li><strong>c<\/strong> = specific heat capacity \u2014 J\/(kg\u00b7K)<\/li>\n<li><strong>L<\/strong> = specific latent heat \u2014 joules per kilogram (J\/kg)<\/li>\n<li><strong>\u0394T<\/strong> = temperature change \u2014 kelvin (K)<\/li>\n<li><strong>\u03b1<\/strong> = linear expansion coefficient \u2014 per kelvin (K<sup>-1<\/sup>)<\/li>\n<li><strong>n<\/strong> = amount of substance \u2014 moles (mol)<\/li>\n<li><strong>R<\/strong> = molar gas constant \u2014 8.314 J\/(mol\u00b7K)<\/li>\n<li><strong>\u0394U<\/strong> = internal energy change \u2014 joules (J)<\/li>\n<li><strong>k<\/strong> = thermal conductivity \u2014 W\/(m\u00b7K)<\/li>\n<li><strong>\u03c3<\/strong> = Stefan-Boltzmann constant \u2014 5.670 \u00d7 10<sup>-8<\/sup> W\/(m<sup>2<\/sup>\u00b7K<sup>4<\/sup>)<\/li>\n<li><strong>\u03b5<\/strong> = emissivity \u2014 dimensionless, between 0 and 1<\/li>\n<\/ul>\n\n<p>A common slip is treating \u0394T in celsius as if it were the T in PV = nRT. A <em>change<\/em> of 10 \u00b0C equals a change of 10 K, so \u0394T is safe either way \u2014 but an absolute T of 10 \u00b0C is 283.15 K, and the gas laws will punish you for the difference. The reasoning behind all four laws is in our guide to the <a href=\"https:\/\/physicsfundamentalsinfo.com\/blog\/thermodynamics\/laws-of-thermodynamics\/\">laws of thermodynamics<\/a>.<\/p>\n\n<h2>Waves, Sound and Optics Formulas<\/h2>\n\n<p>One formula runs this entire group, and it is almost embarrassingly simple: a wave&#8217;s speed is how often it wiggles times how long each wiggle is.<\/p>\n\n<div class=\"pf-formula\">v = f\u03bb<\/div>\n\n<div class=\"pf-table-scroll\" style=\"display:block;width:100%;max-width:100%;overflow-x:auto;-webkit-overflow-scrolling:touch;margin:1.5em 0;\">\n<table style=\"width:100%;border-collapse:collapse;\">\n<thead>\n<tr style=\"background:#0A1628;color:#FAF6EE;\">\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Formula<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Gives you<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Note<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Calculator<\/th>\n<\/tr>\n<\/thead>\n<tbody>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">v = f\u03bb<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Wave speed<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">True for every wave, from sound to gamma rays<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/wave-speed\">Wave Speed<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">f = 1 \/ T<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Frequency from period<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">1 Hz = one cycle per second<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/wave-speed\">Wave Speed<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">n<sub>1<\/sub> sin \u03b8<sub>1<\/sub> = n<sub>2<\/sub> sin \u03b8<sub>2<\/sub><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Snell\u2019s law of refraction<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Angles measured from the <em>normal<\/em><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/snells-law\">Snell&#8217;s Law<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">n = c \/ v<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Refractive index<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Always 1 or greater in a medium<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/refractive-index\">Refractive Index<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">sin \u03b8<sub>c<\/sub> = n<sub>2<\/sub> \/ n<sub>1<\/sub><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Critical angle<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Only when n<sub>1<\/sub> is greater than n<sub>2<\/sub><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/snells-law\">Snell&#8217;s Law<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">1\/f = 1\/d<sub>o<\/sub> + 1\/d<sub>i<\/sub><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Thin lens and mirror equation<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Sign conventions matter enormously<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/lens-mirror\">Lens &amp; Mirror<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">m = \u2212d<sub>i<\/sub> \/ d<sub>o<\/sub><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Magnification<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Negative means inverted<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/lens-mirror\">Lens &amp; Mirror<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">d sin \u03b8 = n\u03bb<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Diffraction grating maxima<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">n is the order, an integer<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/diffraction-grating\">Diffraction Grating<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">I = I<sub>0<\/sub> cos<sup>2<\/sup>\u03b8<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Malus&#8217;s law (polarisation)<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Cross the filters and it goes dark<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/malus-law\">Malus&#8217;s Law<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">T = 2\u03c0 sqrt(L \/ g)<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Pendulum period<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Mass cancels; small angles only<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/pendulum-period\">Pendulum Period<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">T = 2\u03c0 sqrt(m \/ k)<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Mass-spring period<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Here mass does <em>not<\/em> cancel<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/simple-harmonic-motion\">SHM<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">L = 10 log<sub>10<\/sub>(I \/ I<sub>0<\/sub>)<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Sound level in decibels<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">A logarithmic scale, so +10 dB is 10\u00d7 the intensity<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/decibel\">Decibel<\/a><\/td><\/tr>\n<\/tbody>\n<\/table>\n<\/div>\n\n<ul>\n<li><strong>v<\/strong> = wave speed \u2014 metres per second (m\/s)<\/li>\n<li><strong>f<\/strong> = frequency \u2014 hertz (Hz)<\/li>\n<li><strong>\u03bb<\/strong> = wavelength \u2014 metres (m)<\/li>\n<li><strong>T<\/strong> = period \u2014 seconds (s)<\/li>\n<li><strong>n<\/strong> = refractive index \u2014 dimensionless<\/li>\n<li><strong>\u03b8<\/strong> = angle from the normal \u2014 degrees or radians<\/li>\n<li><strong>d<sub>o<\/sub>, d<sub>i<\/sub><\/strong> = object and image distance \u2014 metres (m)<\/li>\n<li><strong>d<\/strong> = grating slit spacing \u2014 metres (m)<\/li>\n<li><strong>I, I<sub>0<\/sub><\/strong> = intensity \u2014 watts per square metre (W\/m<sup>2<\/sup>)<\/li>\n<li><strong>L<\/strong> = pendulum length \u2014 metres (m); sound level \u2014 decibels (dB)<\/li>\n<\/ul>\n\n<p>Notice that <em>L<\/em> carries two meanings inside this one table \u2014 a pendulum&#8217;s length, and a sound level in decibels. <em>n<\/em> is worse still: refractive index in one row, diffraction order in another, moles back in thermodynamics, and turns per metre in the section below.<\/p>\n\n<p>Symbols are recycled across physics, and the only reliable guide is context \u2014 which is exactly why every table on this page names its symbols rather than assuming you remember. Our explainer on the <a href=\"https:\/\/physicsfundamentalsinfo.com\/blog\/waves\/frequency-formula\/\">frequency formula<\/a> unpacks the f and T relationship properly.<\/p>\n\n<h2>Electricity and Magnetism Formulas<\/h2>\n\n<p>This is the largest group, and the one students most often try to brute-force. Resist that. Almost all of it grows from two ideas: charge flowing, and charge creating fields.<\/p>\n\n<div class=\"pf-formula\">V = IR<\/div>\n\n<div class=\"pf-table-scroll\" style=\"display:block;width:100%;max-width:100%;overflow-x:auto;-webkit-overflow-scrolling:touch;margin:1.5em 0;\">\n<table style=\"width:100%;border-collapse:collapse;\">\n<thead>\n<tr style=\"background:#0A1628;color:#FAF6EE;\">\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Formula<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Gives you<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Note<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Calculator<\/th>\n<\/tr>\n<\/thead>\n<tbody>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Q = It<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Charge from current<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">1 A = 1 C\/s<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/electric-current\">Electric Current<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">V = IR<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Ohm&#8217;s law<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Only for ohmic conductors at fixed temperature<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/ohms-law\">Ohm&#8217;s Law<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">P = IV = I<sup>2<\/sup>R = V<sup>2<\/sup>\/R<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Electrical power, three ways<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Pick whichever two quantities you know<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/ohms-law\">Ohm&#8217;s Law<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">R = \u03c1L \/ A<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Resistance of a wire<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">\u03c1 here is resistivity, not density<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/resistivity\">Resistivity<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">R<sub>total<\/sub> = R<sub>1<\/sub> + R<sub>2<\/sub> + \u2026<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Series resistance<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Always larger than the biggest one<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/resistor\">Resistor<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">1\/R<sub>total<\/sub> = 1\/R<sub>1<\/sub> + 1\/R<sub>2<\/sub> + \u2026<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Parallel resistance<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Always smaller than the smallest one<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/resistor\">Resistor<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">V = W \/ Q<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Potential difference<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Energy per unit charge<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/potential-difference\">Potential Difference<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">F = kq<sub>1<\/sub>q<sub>2<\/sub> \/ r<sup>2<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Coulomb&#8217;s law<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Same inverse-square shape as gravity<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/coulombs-law\">Coulomb&#8217;s Law<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">E = F \/ q = kQ \/ r<sup>2<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Electric field strength<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Volts per metre, or newtons per coulomb<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/electric-field\">Electric Field<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">C = Q \/ V<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Capacitance<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Charge stored per volt<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/capacitance\">Capacitance<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">E = \u00bdCV<sup>2<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Energy in a capacitor<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Same \u00bd shape as \u00bdmv<sup>2<\/sup> and \u00bdkx<sup>2<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/capacitance\">Capacitance<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">F = qvB sin \u03b8<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Force on a moving charge<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Zero if it moves along the field<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/magnetic-force\">Magnetic Force<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">F = BIL sin \u03b8<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Force on a current-carrying wire<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">How every electric motor turns<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/magnetic-force\">Magnetic Force<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">B = \u03bc<sub>0<\/sub>nI<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Field inside a solenoid<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">n is turns per metre, not total turns<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/magnetic-field\">Magnetic Field<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">\u03b5 = \u2212N \u0394\u03a6 \/ \u0394t<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Faraday&#8217;s law of induction<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">The minus sign is Lenz&#8217;s law<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/faradays-law\">Faraday&#8217;s Law<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">V<sub>s<\/sub>\/V<sub>p<\/sub> = N<sub>s<\/sub>\/N<sub>p<\/sub><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Transformer ratio<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Ideal transformer only<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/faradays-law\">Faraday&#8217;s Law<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">\u03c4 = RC<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">RC time constant<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Ohms times farads gives seconds<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/rc-time-constant\">RC Time Constant<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">V<sub>rms<\/sub> = V<sub>0<\/sub> \/ sqrt(2)<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">RMS from peak voltage<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Mains figures are always RMS<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/rms-voltage\">RMS Voltage<\/a><\/td><\/tr>\n<\/tbody>\n<\/table>\n<\/div>\n\n<ul>\n<li><strong>Q, q<\/strong> = charge \u2014 coulombs (C)<\/li>\n<li><strong>I<\/strong> = current \u2014 amperes (A)<\/li>\n<li><strong>V<\/strong> = potential difference \u2014 volts (V)<\/li>\n<li><strong>R<\/strong> = resistance \u2014 ohms (\u03a9)<\/li>\n<li><strong>\u03c1<\/strong> = resistivity \u2014 ohm metres (\u03a9\u00b7m)<\/li>\n<li><strong>P<\/strong> = power \u2014 watts (W)<\/li>\n<li><strong>E<\/strong> = electric field strength \u2014 volts per metre (V\/m)<\/li>\n<li><strong>C<\/strong> = capacitance \u2014 farads (F)<\/li>\n<li><strong>B<\/strong> = magnetic flux density \u2014 teslas (T)<\/li>\n<li><strong>\u03a6<\/strong> = magnetic flux \u2014 webers (Wb)<\/li>\n<li><strong>\u03b5<\/strong> = induced emf \u2014 volts (V)<\/li>\n<li><strong>N<\/strong> = number of turns \u2014 dimensionless<\/li>\n<li><strong>\u03c4<\/strong> = time constant \u2014 seconds (s)<\/li>\n<li><strong>k<\/strong> = Coulomb constant \u2014 8.99 \u00d7 10<sup>9<\/sup> N\u00b7m<sup>2<\/sup>\/C<sup>2<\/sup><\/li>\n<li><strong>\u03bc<sub>0<\/sub><\/strong> = vacuum magnetic permeability \u2014 1.2566 \u00d7 10<sup>-6<\/sup> N\/A<sup>2<\/sup><\/li>\n<\/ul>\n\n<p>The trap in this group is <em>\u03c1<\/em>. In the fluids table it meant density; here it means resistivity. Different quantity, different unit, same Greek letter. For the full picture of the group&#8217;s cornerstone see our <a href=\"https:\/\/physicsfundamentalsinfo.com\/blog\/electromagnetism\/ohms-law\/\">Ohm&#8217;s law explainer<\/a>, or put your own numbers into the <a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/ohms-law\">Ohm&#8217;s Law calculator<\/a> to check a circuit in one step.<\/p>\n\n<h2>Modern Physics Formulas<\/h2>\n\n<p>These are the formulas that took over when classical physics ran out of road \u2014 at speeds approaching light, and at scales where matter stops behaving like a tiny billiard ball.<\/p>\n\n<div class=\"pf-formula\">E = mc<sup>2<\/sup><\/div>\n\n<div class=\"pf-table-scroll\" style=\"display:block;width:100%;max-width:100%;overflow-x:auto;-webkit-overflow-scrolling:touch;margin:1.5em 0;\">\n<table style=\"width:100%;border-collapse:collapse;\">\n<thead>\n<tr style=\"background:#0A1628;color:#FAF6EE;\">\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Formula<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Gives you<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Note<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Calculator<\/th>\n<\/tr>\n<\/thead>\n<tbody>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">E = mc<sup>2<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Rest energy of a mass<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Mass is a form of energy, not a source of it<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/e-mc2\">E = mc<sup>2<\/sup><\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">E = hf = hc \/ \u03bb<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Photon energy<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Colour sets the energy, brightness sets the count<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/photon-energy\">Photon Energy<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">KE<sub>max<\/sub> = hf \u2212 \u03c6<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Photoelectric equation<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Below the threshold, nothing happens at all<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/photoelectric-effect\">Photoelectric Effect<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">\u03bb = h \/ (mv)<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">De Broglie wavelength<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Everything has one; yours is absurdly small<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/de-broglie-wavelength\">De Broglie Wavelength<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">\u03b3 = 1 \/ sqrt(1 \u2212 v<sup>2<\/sup>\/c<sup>2<\/sup>)<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Lorentz factor<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Essentially 1 until you approach c<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/lorentz-factor\">Lorentz Factor<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">t = \u03b3t<sub>0<\/sub><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Time dilation<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">t<sub>0<\/sub> is the proper time<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/time-dilation\">Time Dilation<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">L = L<sub>0<\/sub> \/ \u03b3<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Length contraction<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Only along the direction of motion<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/lorentz-factor\">Lorentz Factor<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">p = \u03b3mv<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Relativistic momentum<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Reduces to p = mv at everyday speeds<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/momentum\">Momentum<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">N = N<sub>0<\/sub>(\u00bd)<sup>(t \/ t\u00bd)<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Radioactive decay<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Halving is independent of how much you started with<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/half-life\">Half-Life<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">\u03bb = ln2 \/ t\u00bd<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Decay constant<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">\u03bb here is <em>not<\/em> wavelength<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/half-life\">Half-Life<\/a><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">A = \u03bbN<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Activity<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Measured in becquerels (Bq)<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/half-life\">Half-Life<\/a><\/td><\/tr>\n<\/tbody>\n<\/table>\n<\/div>\n\n<ul>\n<li><strong>E<\/strong> = energy \u2014 joules (J), often quoted in electronvolts (eV)<\/li>\n<li><strong>m<\/strong> = mass \u2014 kilograms (kg)<\/li>\n<li><strong>c<\/strong> = speed of light in vacuum \u2014 299,792,458 m\/s exactly<\/li>\n<li><strong>h<\/strong> = Planck constant \u2014 6.626 \u00d7 10<sup>-34<\/sup> J\u00b7s<\/li>\n<li><strong>f<\/strong> = photon frequency \u2014 hertz (Hz)<\/li>\n<li><strong>\u03c6<\/strong> = work function \u2014 joules (J) or electronvolts (eV)<\/li>\n<li><strong>\u03b3<\/strong> = Lorentz factor \u2014 dimensionless<\/li>\n<li><strong>t<sub>0<\/sub>, L<sub>0<\/sub><\/strong> = proper time (s) and proper length (m)<\/li>\n<li><strong>N, N<sub>0<\/sub><\/strong> = number of undecayed nuclei \u2014 dimensionless<\/li>\n<li><strong>t\u00bd<\/strong> = half-life \u2014 seconds (s)<\/li>\n<li><strong>\u03bb<\/strong> = decay constant \u2014 per second (s<sup>-1<\/sup>) <em>in this table only<\/em><\/li>\n<li><strong>A<\/strong> = activity \u2014 becquerels (Bq)<\/li>\n<\/ul>\n\n<p>That last group is where symbol collisions get genuinely dangerous: \u03bb is a wavelength in the optics table and a decay constant here. Our guide to <a href=\"https:\/\/physicsfundamentalsinfo.com\/blog\/modern-physics\/special-relativity\/\">special relativity<\/a> works through where \u03b3 comes from, and the <a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/e-mc2\">E = mc<sup>2<\/sup> calculator<\/a> will show you just how much energy hides inside a gram of anything.<\/p>\n\n<h2>Physical Constants Every Formula Assumes<\/h2>\n\n<p>A formula is only half a tool without its constants. These are the numbers that appear inside the equations above, and the ones worth having on the same sheet.<\/p>\n\n<div class=\"pf-table-scroll\" style=\"display:block;width:100%;max-width:100%;overflow-x:auto;-webkit-overflow-scrolling:touch;margin:1.5em 0;\">\n<table style=\"width:100%;border-collapse:collapse;\">\n<thead>\n<tr style=\"background:#0A1628;color:#FAF6EE;\">\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Constant<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Symbol<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Value<\/th>\n<th style=\"padding:10px;text-align:left;border:1px solid #D9CFB8;\">Unit<\/th>\n<\/tr>\n<\/thead>\n<tbody>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Speed of light in vacuum<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">c<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">299,792,458 <strong>(exact)<\/strong><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">m\/s<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Standard gravity<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">g<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">9.80665 (use 9.81)<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">m\/s<sup>2<\/sup><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Gravitational constant<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">G<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">6.67430 \u00d7 10<sup>-11<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">N\u00b7m<sup>2<\/sup>\/kg<sup>2<\/sup><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Planck constant<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">h<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">6.62607015 \u00d7 10<sup>-34<\/sup> <strong>(exact)<\/strong><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">J\u00b7s<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Elementary charge<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">e<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">1.602176634 \u00d7 10<sup>-19<\/sup> <strong>(exact)<\/strong><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">C<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Boltzmann constant<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">k<sub>B<\/sub><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">1.380649 \u00d7 10<sup>-23<\/sup> <strong>(exact)<\/strong><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">J\/K<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Avogadro constant<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">N<sub>A<\/sub><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">6.02214076 \u00d7 10<sup>23<\/sup> <strong>(exact)<\/strong><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">mol<sup>-1<\/sup><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Molar gas constant<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">R<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">8.314462618<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">J\/(mol\u00b7K)<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Coulomb constant<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">k<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">8.9875518 \u00d7 10<sup>9<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">N\u00b7m<sup>2<\/sup>\/C<sup>2<\/sup><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Vacuum electric permittivity<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">\u03b5<sub>0<\/sub><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">8.8541878188 \u00d7 10<sup>-12<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">F\/m<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Vacuum magnetic permeability<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">\u03bc<sub>0<\/sub><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">1.25663706127 \u00d7 10<sup>-6<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">N\/A<sup>2<\/sup><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Stefan-Boltzmann constant<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">\u03c3<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">5.670374419 \u00d7 10<sup>-8<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">W\/(m<sup>2<\/sup>\u00b7K<sup>4<\/sup>)<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Electron mass<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">m<sub>e<\/sub><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">9.1093837139 \u00d7 10<sup>-31<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">kg<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Proton mass<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">m<sub>p<\/sub><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">1.67262192595 \u00d7 10<sup>-27<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">kg<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Atomic mass constant<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">u<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">1.66053906892 \u00d7 10<sup>-27<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">kg<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Electronvolt<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">eV<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">1.602176634 \u00d7 10<sup>-19<\/sup> <strong>(exact)<\/strong><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">J<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Speed of sound in air (20 \u00b0C)<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">v<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">343<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">m\/s<\/td><\/tr>\n<\/tbody>\n<\/table>\n<\/div>\n\n<p>Values follow the CODATA 2022 set; the full list, with uncertainties, lives in the <a href=\"https:\/\/physics.nist.gov\/cuu\/Constants\/index.html\" target=\"_blank\" rel=\"noopener\">NIST fundamental constants database<\/a>. For exam work, three or four significant figures is almost always enough.<\/p>\n\n<p>Here is a sanity check worth trying once. Take \u03b5<sub>0<\/sub> and \u03bc<sub>0<\/sub> from that table and compute 1 divided by the square root of their product. You get 299,792,458 m\/s \u2014 the speed of light, falling out of two electrical constants. That is not a coincidence; it is Maxwell&#8217;s discovery that light <em>is<\/em> an electromagnetic wave.<\/p>\n\n<h2>How Do You Rearrange a Physics Formula?<\/h2>\n\n<p>You rearrange a physics formula by doing the same operation to both sides until the quantity you want is alone \u2014 divide to undo a multiplication, subtract to undo an addition, take a square root to undo a square.<\/p>\n\n<p>That is the whole method. It is also the single biggest source of lost marks in physics, because students learn a shortcut instead \u2014 and the shortcut has a blind spot.<\/p>\n\n<figure class=\"pf-figure\" style=\"margin:1.6em 0;\"><img src=\"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-content\/uploads\/2026\/08\/physics-formulas-two-panels-comparing-formula-triangle.webp\" width=\"1400\" height=\"684\" alt=\"Physics formulas - Two panels comparing the formula triangle, which works for three-symbol products such as v equals f lambda, with algebra, which is required for formulas containing squares or sums such as v squared equals u squared plus 2as\" loading=\"lazy\" decoding=\"async\" style=\"width:100%;height:auto;max-width:700px;display:block;margin:0 auto;\" \/><\/figure>\n\n<p style=\"text-align:center;font-size:13px;font-style:italic;color:#1F2E47;margin-top:-14px;\">Formula triangles only handle three-symbol products. Everything else needs the algebra.<\/p>\n\n<p>Formula triangles are not wrong \u2014 they are just narrow. They handle exactly one shape: one quantity equals two others multiplied together.<\/p>\n\n<p>F = ma fits. V = IR fits. v = f\u03bb fits. Roughly a third of this page fits.<\/p>\n\n<p>The other two thirds do not, and a student who has only ever used triangles will stall the first time a square or a plus sign appears. Learn the algebra; keep the triangle as a shortcut you can justify.<\/p>\n\n<p>The lab below lets you drill exactly that. Pick a relationship, choose which variable to solve for, and watch the rearranged equation and the answer update together.<\/p>\n\n<div class=\"pf-sim-slot\"><div class=\"pf-sim-slot-header\"><span class=\"icon-dot\"><\/span><span class=\"label\">Physics Formula Rearranger Lab<\/span><\/div><div class=\"pf-sim-slot-body\"><style>.pf-sim-frame{width:100%;border:none;height:600px}@media(max-width:760px){.pf-sim-frame{height:1000px}}<\/style><iframe src=\"\/labs\/physics-formulas.html?embed=1\" class=\"pf-sim-frame\" loading=\"lazy\"><\/iframe><\/div><\/div>\n\n<h2>Which Physics Formulas Should You Memorise First?<\/h2>\n\n<p>Memorise the six that everything else is built from: F = ma, KE = \u00bdmv<sup>2<\/sup>, p = mv, v = f\u03bb, V = IR and Q = mc\u0394T. Learn those cold and you can reconstruct or recognise most of the rest.<\/p>\n\n<p>Six of the ten signatures on the map above do the heaviest lifting, and those are they. Once F = ma is automatic, W = Fd is one step away, and P = W\/t is one step after that.<\/p>\n\n<h3>The Order That Works<\/h3>\n\n<ol>\n<li><strong>The six signatures above.<\/strong> Non-negotiable. These are the hooks.<\/li>\n<li><strong>The five SUVAT equations.<\/strong> High yield, and they appear in disguise everywhere.<\/li>\n<li><strong>The energy family:<\/strong> W = Fd, PE = mgh, P = W\/t, W<sub>net<\/sub> = \u0394KE.<\/li>\n<li><strong>The inverse-square pair:<\/strong> F = GMm\/r<sup>2<\/sup> and F = kq<sub>1<\/sub>q<sub>2<\/sub>\/r<sup>2<\/sup>. Identical shape, so learn them together.<\/li>\n<li><strong>Your syllabus&#8217;s data sheet.<\/strong> Find out what is given to you \u2014 and stop memorising that.<\/li>\n<\/ol>\n\n<p>That last point saves more time than any mnemonic. Most exam boards hand you a formula sheet. Spend an hour finding out precisely which formulas are on yours, and you have just deleted half your memorisation workload.<\/p>\n\n<p>One more habit worth building: check magnitudes. If you calculate a car&#8217;s kinetic energy and get 3 joules, something is wrong \u2014 a moving car carries hundreds of thousands. Physicists develop a feel for what answers should look like, and that instinct catches errors no formula sheet ever will.<\/p>\n\n<h2>Common Misconceptions About Physics Formulas<\/h2>\n\n<h3>&#8220;You have to memorise all of them&#8221;<\/h3>\n\n<p>You do not. Professional physicists look formulas up constantly \u2014 what they carry in their heads is which formula <em>exists<\/em> and roughly what shape it has. Recognition beats recall. Knowing that a v<sup>2<\/sup> term means energy is somewhere in the problem is worth more than reciting the equation perfectly.<\/p>\n\n<h3>&#8220;Physical constants are measured, so they might change&#8221;<\/h3>\n\n<p>Several of them cannot change, because they are now definitions rather than measurements. Since 20 May 2019, c, h, e, k<sub>B<\/sub> and N<sub>A<\/sub> have exact fixed values, and the kilogram, kelvin, ampere and mole were <a href=\"https:\/\/www.nist.gov\/si-redefinition\" target=\"_blank\" rel=\"noopener\">redefined in terms of constants of nature<\/a>.<\/p>\n\n<p>The traffic even ran the other way. \u03bc<sub>0<\/sub> used to be exactly 4\u03c0 \u00d7 10<sup>-7<\/sup> N\/A<sup>2<\/sup> by definition; it is now a measured quantity, and it sits about 1 part in 10 billion away from that old value.<\/p>\n\n<h3>&#8220;A formula and a law are the same thing&#8221;<\/h3>\n\n<p>A law is a claim about nature; a formula is one way of writing it down. Newton&#8217;s second law is the claim that force sets the rate of change of momentum. F = ma is a formula expressing it \u2014 and only when mass is constant, which is why F = \u0394p\/\u0394t is the more honest version.<\/p>\n\n<h3>&#8220;If the numbers go in, the answer comes out&#8221;<\/h3>\n\n<p>Every formula has a domain, and outside it the arithmetic still works while the physics does not. T = 2\u03c0 sqrt(L\/g) fails for a pendulum swung hard. V = IR fails for a filament lamp as it heats. Ohm&#8217;s law is not a law of nature at all \u2014 it is a description of how <em>some<\/em> materials behave, some of the time.<\/p>\n\n<h2>Worked Problems<\/h2>\n\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 1<\/div><div class=\"pf-problem-question\">A net force of 3000 N accelerates a car at 2.5 m\/s^2. What is the car&#039;s mass?<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n<p><strong>Solution:<\/strong><\/p>\n<p>Step 1: Newton&#8217;s second law relates these three quantities: F = ma<\/p>\n<p>Step 2: Rearrange for mass by dividing both sides by a: m = F \/ a<\/p>\n<p>Step 3: Substitute with units: m = 3000 N \/ 2.5 m\/s<sup>2<\/sup> = 1200 kg<\/p>\n<p><strong>Answer: 1200 kg (2 s.f.)<\/strong><\/p>\n<\/div><\/details><\/div>\n\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 2<\/div><div class=\"pf-problem-question\">A 500 g ball is thrown at 12 m\/s. What is its kinetic energy?<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n<p><strong>Solution:<\/strong><\/p>\n<p>Step 1: Use KE = \u00bdmv<sup>2<\/sup><\/p>\n<p>Step 2: Convert the mass to SI units first \u2014 this is where marks are lost: 500 g = 0.500 kg<\/p>\n<p>Step 3: Substitute: KE = \u00bd \u00d7 0.500 kg \u00d7 (12 m\/s)<sup>2<\/sup> = \u00bd \u00d7 0.500 \u00d7 144 = 36 J<\/p>\n<p><strong>Answer: 36 J<\/strong><\/p>\n<p>Leaving the mass in grams would have given 36,000 J \u2014 a ball with the energy of a rifle round.<\/p>\n<\/div><\/details><\/div>\n\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 3<\/div><div class=\"pf-problem-question\">A car braking uniformly slows from 28 m\/s to rest in 40 m. What is its acceleration?<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n<p><strong>Solution:<\/strong><\/p>\n<p>Step 1: Time is not given and not asked for, so use the SUVAT equation without t: v<sup>2<\/sup> = u<sup>2<\/sup> + 2as<\/p>\n<p>Step 2: Rearrange for a: a = (v<sup>2<\/sup> \u2212 u<sup>2<\/sup>) \/ (2s)<\/p>\n<p>Step 3: Substitute: a = (0<sup>2<\/sup> \u2212 28<sup>2<\/sup>) \/ (2 \u00d7 40) = \u2212784 \/ 80 = \u22129.8 m\/s<sup>2<\/sup><\/p>\n<p><strong>Answer: \u22129.8 m\/s<sup>2<\/sup> (the minus sign means deceleration)<\/strong><\/p>\n<\/div><\/details><\/div>\n\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 4<\/div><div class=\"pf-problem-question\">A 2.0 kW kettle heats 2.0 kg of water from 20 \u00b0C to 100 \u00b0C. Specific heat capacity of water = 4180 J\/(kg\u00b7K). How much energy is needed, and how long does it take?<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n<p><strong>Solution:<\/strong><\/p>\n<p>Step 1: Heat needed uses Q = mc\u0394T, and \u0394T = 100 \u2212 20 = 80 \u00b0C = 80 K<\/p>\n<p>Step 2: Substitute: Q = 2.0 kg \u00d7 4180 J\/(kg\u00b7K) \u00d7 80 K = 668,800 J<\/p>\n<p>Step 3: Time comes from P = W \/ t, rearranged to t = Q \/ P<\/p>\n<p>Step 4: Substitute: t = 668,800 J \/ 2000 W = 334 s<\/p>\n<p><strong>Answer: 6.7 \u00d7 10<sup>5<\/sup> J, taking about 330 s (5.6 minutes)<\/strong><\/p>\n<\/div><\/details><\/div>\n\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 5<\/div><div class=\"pf-problem-question\">A 60 W lamp runs on a 230 V supply. Find its resistance and the current through it.<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n<p><strong>Solution:<\/strong><\/p>\n<p>Step 1: You know P and V but not I, so use the power form containing only those: P = V<sup>2<\/sup> \/ R<\/p>\n<p>Step 2: Rearrange for R: R = V<sup>2<\/sup> \/ P<\/p>\n<p>Step 3: Substitute: R = (230 V)<sup>2<\/sup> \/ 60 W = 52,900 \/ 60 = 881.7 \u03a9<\/p>\n<p>Step 4: For current use P = IV, so I = P \/ V = 60 \/ 230 = 0.26 A<\/p>\n<p><strong>Answer: R = 8.8 \u00d7 10<sup>2<\/sup> \u03a9 and I = 0.26 A<\/strong><\/p>\n<p>Check: I<sup>2<\/sup>R = 0.26<sup>2<\/sup> \u00d7 882 = 60 W. It closes.<\/p>\n<\/div><\/details><\/div>\n\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 6<\/div><div class=\"pf-problem-question\">A radio station transmits at 98.5 MHz. What is the wavelength of the broadcast?<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n<p><strong>Solution:<\/strong><\/p>\n<p>Step 1: Radio waves are electromagnetic, so they travel at c and obey v = f\u03bb, giving c = f\u03bb<\/p>\n<p>Step 2: Rearrange for wavelength: \u03bb = c \/ f<\/p>\n<p>Step 3: Convert the frequency: 98.5 MHz = 98.5 \u00d7 10<sup>6<\/sup> Hz<\/p>\n<p>Step 4: Substitute: \u03bb = 299,792,458 m\/s \/ 98.5 \u00d7 10<sup>6<\/sup> Hz = 3.044 m<\/p>\n<p><strong>Answer: 3.04 m (3 s.f.)<\/strong><\/p>\n<\/div><\/details><\/div>\n\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 7<\/div><div class=\"pf-problem-question\">Light of wavelength 400 nm falls on sodium, work function 2.28 eV. What is the maximum kinetic energy of the emitted electrons? Take h = 6.626 x 10^-34 J s, c = 2.998 x 10^8 m\/s and 1 eV = 1.602 x 10^-19 J.<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n<p><strong>Solution:<\/strong><\/p>\n<p>Step 1: Photon energy comes from E = hc \/ \u03bb<\/p>\n<p>Step 2: Substitute, converting 400 nm to 400 \u00d7 10<sup>-9<\/sup> m:<br>E = (6.626 \u00d7 10<sup>-34<\/sup> J\u00b7s \u00d7 2.998 \u00d7 10<sup>8<\/sup> m\/s) \/ (400 \u00d7 10<sup>-9<\/sup> m) = 4.966 \u00d7 10<sup>-19<\/sup> J<\/p>\n<p>Step 3: Convert to electronvolts to match the work function:<br>E = 4.966 \u00d7 10<sup>-19<\/sup> \/ 1.602 \u00d7 10<sup>-19<\/sup> = 3.10 eV<\/p>\n<p>Step 4: Apply the photoelectric equation KE(max) = hf \u2212 \u03c6:<br>KE(max) = 3.10 eV \u2212 2.28 eV = 0.82 eV<\/p>\n<p><strong>Answer: 0.82 eV, which is 1.3 \u00d7 10<sup>-19<\/sup> J<\/strong><\/p>\n<\/div><\/details><\/div>\n\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 8<\/div><div class=\"pf-problem-question\">A baseball is thrown vertically upward at 40 m\/s. Ignoring air resistance, how high does it rise? Its mass is 0.145 kg.<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n<p><strong>Solution:<\/strong><\/p>\n<p>Step 1: Use conservation of energy \u2014 all kinetic energy becomes potential energy at the top: \u00bdmv<sup>2<\/sup> = mgh<\/p>\n<p>Step 2: Mass appears on both sides, so it cancels: \u00bdv<sup>2<\/sup> = gh<\/p>\n<p>Step 3: Rearrange for h: h = v<sup>2<\/sup> \/ (2g)<\/p>\n<p>Step 4: Substitute: h = (40 m\/s)<sup>2<\/sup> \/ (2 \u00d7 9.81 m\/s<sup>2<\/sup>) = 1600 \/ 19.62 = 81.5 m<\/p>\n<p><strong>Answer: about 82 m (2 s.f.)<\/strong><\/p>\n<p>The 0.145 kg was never needed \u2014 a deliberate distractor. Heavy and light objects rise to the same height at the same launch speed.<\/p>\n<\/div><\/details><\/div>\n\n<h2>Frequently Asked Questions<\/h2>\n\n<details class=\"pf-faq-item\"><summary>What are the most important physics formulas?<\/summary><div class=\"pf-faq-item-answer\">\nThe six most important physics formulas are F = ma, KE = \u00bdmv<sup>2<\/sup>, p = mv, v = f\u03bb, V = IR and Q = mc\u0394T. Each one is the signature equation of a whole branch, and most other formulas in that branch can be derived from it or recognised through it. Learn these six before anything else.\n<\/div><\/details>\n\n<details class=\"pf-faq-item\"><summary>How do I know which physics formula to use in a problem?<\/summary><div class=\"pf-faq-item-answer\">\nMatch the formula to the quantities the question actually gives you. List what you know with units, list what is asked, then find the formula containing exactly those symbols. If a question mentions distance but never time, that alone tells you to use v<sup>2<\/sup> = u<sup>2<\/sup> + 2as rather than v = u + at.\n<\/div><\/details>\n\n<details class=\"pf-faq-item\"><summary>Do I need to memorise physics formulas for exams?<\/summary><div class=\"pf-faq-item-answer\">\nUsually not all of them. Most exam boards provide a data or formula sheet, so the first thing to do is find out exactly which formulas yours supplies. Memorise the handful that are not given, and spend the time you save practising how to select and rearrange formulas instead.\n<\/div><\/details>\n\n<details class=\"pf-faq-item\"><summary>What is the difference between a physics formula and a physics law?<\/summary><div class=\"pf-faq-item-answer\">\nA law is a claim about how nature behaves; a formula is one mathematical way of writing that claim. Newton&#8217;s second law states that force equals the rate of change of momentum. F = ma is a formula expressing that law, valid only when mass stays constant.\n<\/div><\/details>\n\n<details class=\"pf-faq-item\"><summary>Why do physics formulas use Greek letters?<\/summary><div class=\"pf-faq-item-answer\">\nGreek letters extend the alphabet, because physics has far more quantities than the 26 Latin letters can cover. They also carry convention: \u0394 signals a change, \u03c1 usually means density, \u03bb usually means wavelength, and \u03c9 means angular velocity. The same letter can still mean different things in different topics, so always check the context.\n<\/div><\/details>\n\n<details class=\"pf-faq-item\"><summary>How many physics formulas are there?<\/summary><div class=\"pf-faq-item-answer\">\nAn introductory physics course covers roughly 100 formulas, and this page lists them grouped into ten branches. Advanced physics has no fixed count, since new relationships are derived constantly. The useful number is much smaller: about six signature formulas generate or connect most of the rest.\n<\/div><\/details>\n\n<details class=\"pf-faq-item\"><summary>Is there a complete physics formulas list for GCSE and A-Level?<\/summary><div class=\"pf-faq-item-answer\">\nYes \u2014 this page is a complete physics formulas list covering every branch you meet at GCSE and A-Level, from motion and forces to electricity, waves, thermodynamics and modern physics. Each formula is grouped by topic, defined with its symbols and SI units, and linked to a calculator so you can check your working instantly.\n<\/div><\/details>\n\n<details class=\"pf-faq-item\"><summary>How many calculators does this physics formulas list link to?<\/summary><div class=\"pf-faq-item-answer\">\nThis list links to 97 individual calculators \u2014 one for every formula that can be rearranged to solve for a different variable. Each calculator is free and handles all the rearranging and unit-checking for you, so you can focus on the physics rather than the algebra.\n<\/div><\/details>\n","protected":false},"excerpt":{"rendered":"<p>A complete physics formula cheat sheet: every core equation grouped into ten branches, with each symbol and its SI unit defined, plus worked examples and the constants that go with them.<\/p>\n","protected":false},"author":1,"featured_media":589,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[2],"tags":[],"class_list":["post-588","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-mechanics"],"_links":{"self":[{"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/posts\/588","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/comments?post=588"}],"version-history":[{"count":7,"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/posts\/588\/revisions"}],"predecessor-version":[{"id":1574,"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/posts\/588\/revisions\/1574"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/media\/589"}],"wp:attachment":[{"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/media?parent=588"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/categories?post=588"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/tags?post=588"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}