Tools in This Collection
Work-Energy Theorem Calculator
Work done by force over distance with energy conservation
Torque Calculator
Calculate torque from force and lever arm distance
Friction Calculator
Static and kinetic friction force with material table
Snell's Law Calculator
Refraction angle from indices and critical angle check
Circuit Calculator
Series and parallel resistor, capacitor, inductor calculator
Fluid Pressure Calculator
Pressure at depth using Pascal's law
Bernoulli Equation Calculator
Fluid dynamics pressure, velocity, and height solver
Gravitational Force Calculator
Newton's law of universal gravitation solver
Specific Heat Calculator
Q=mcΔT solver with material database
Electromagnetic Spectrum Reference
Interactive EM spectrum with wavelength and energy
Projectile Motion Visualizer
Animated trajectory with adjustable angle and velocity
Electric Circuit Visualizer
Interactive circuit builder with voltage and current display
Rotational Motion Calculator
Angular velocity, acceleration, and moment of inertia
Spring Constant Calculator
Hooke's law solver with elastic potential energy
Terminal Velocity Calculator
Calculate terminal velocity for falling objects
Carnot Efficiency Calculator
Theoretical maximum efficiency from reservoir temperatures
Magnetic Field Calculator
B-field from wire, solenoid, and loop configurations
Time Dilation Calculator
Time dilation and length contraction at relativistic speeds
Physics Formulas Cheatsheet
Searchable formula reference for all major physics topics
Decibel Calculator
Add and subtract decibel levels and intensity
Guides & Articles
Physics Calculators for Students and Engineers
Physics problems span an enormous range — from classical Newtonian mechanics to relativistic time dilation and electromagnetic field calculations. This collection covers the most searched physics calculator topics: work and energy, torque, friction, fluid dynamics, optics, thermodynamics, and electromagnetism. All tools support both SI and imperial units and run entirely in your browser.
Mechanics: Work, Force, and Rotation
Work-energy calculations are central to mechanics at every level. The work-energy theorem states that the net work done on an object equals its change in kinetic energy: W_net = ΔKE = ½mv₂² − ½mv₁². For a force applied at angle θ over distance d, W = F × d × cos θ. A 50 N force applied at 30° over 10 m does W = 50 × 10 × cos(30°) = 433 J. The Work-Energy Theorem Calculator solves for any variable and shows the energy conservation breakdown.
Torque problems involve force applied at a lever arm: τ = r × F × sin θ, where r is the distance from the pivot and θ is the angle between the force vector and lever arm. A 100 N force applied perpendicular to a 0.5 m wrench handle produces 50 N·m of torque. The Torque Calculator outputs in both N·m and ft·lb. For rotational systems, the Rotational Motion Calculator handles angular velocity (ω), angular acceleration (α), moment of inertia (I), and torque with shape presets for common objects (disk, ring, rod, sphere).
Friction and Springs
Friction force depends on the coefficient of friction and normal force: f = μN. For a 10 kg block on a surface with μ_k = 0.3, the kinetic friction force is f = 0.3 × (10 × 9.8) = 29.4 N. Static friction uses μ_s (higher than kinetic) and represents the maximum force before the object begins sliding. The Friction Calculator includes a material lookup table for common surface pairs. Hooke's law for springs (F = kx) connects spring constant k, displacement x, and force. The Spring Constant Calculator solves for k, F, x, or elastic potential energy (PE = ½kx²) and connects to the simple harmonic motion period T = 2π√(m/k).
Fluid Dynamics and Thermodynamics
Pascal's law states that pressure applied to an enclosed fluid is transmitted equally throughout: P = ρgh for pressure at depth h in a fluid of density ρ. At 10 m depth in water (ρ = 1000 kg/m³), gauge pressure = 1000 × 9.8 × 10 = 98,000 Pa ≈ 0.97 atm. The Fluid Pressure Calculator solves for gauge and absolute pressure with density and depth inputs.
Bernoulli's principle relates pressure, velocity, and height for ideal fluid flow: P₁ + ½ρv₁² + ρgh₁ = P₂ + ½ρv₂² + ρgh₂. This explains why airplane wings generate lift (faster airflow over the top surface lowers pressure) and why water speeds up through a narrow pipe. The Bernoulli Equation Calculator solves for any of the six variables given the other five.
Specific heat calculations use Q = mcΔT, where m is mass, c is specific heat capacity, and ΔT is temperature change. Water's specific heat (4,186 J/kg·K) means heating 1 kg of water from 20°C to 100°C requires 4,186 × 1 × 80 = 334,880 J. The Specific Heat Calculator includes a material database and supports calorimetry problems with mixed materials. For heat engine efficiency, the Carnot Efficiency Calculator gives the theoretical maximum efficiency η = 1 − T_cold/T_hot.
Optics and Waves
Snell's law governs refraction at the boundary between two media: n₁ sin θ₁ = n₂ sin θ₂. Light entering water (n = 1.33) from air (n = 1.00) at 45° refracts to sin θ₂ = sin(45°)/1.33 = 0.532, giving θ₂ = 32.1°. When n₁ > n₂ and the angle exceeds the critical angle θ_c = arcsin(n₂/n₁), total internal reflection occurs — the principle behind fiber optic cables. The Snell's Law Calculator solves for any angle or refractive index and checks for total internal reflection. The Electromagnetic Spectrum Reference provides an interactive visualization of the full EM spectrum from radio waves to gamma rays with wavelength, frequency, energy, and typical sources for each region.
Electromagnetism
Magnetic fields from current-carrying conductors vary by geometry. For a long straight wire: B = μ₀I/(2πr). For a solenoid with n turns per meter: B = μ₀nI. For a circular loop of radius r: B = μ₀I/(2r) at the center. The Magnetic Field Calculator handles all three geometries with SI and customary unit support. For circuit analysis, the Circuit Calculator computes equivalent resistance, total capacitance, and equivalent inductance for series and parallel combinations, along with voltage divider ratios. The Electric Circuit Visualizer provides an interactive canvas-based circuit builder showing current and voltage at each element.
Special Topics
Terminal velocity occurs when drag force equals gravitational force: v_t = √(2mg/ρAC_d), where ρ is air density, A is cross-sectional area, and C_d is drag coefficient. A skydiver (m = 80 kg, A = 0.5 m², C_d = 1.0) has terminal velocity v_t = √(2×80×9.8/(1.225×0.5×1.0)) ≈ 50 m/s (180 km/h). The Terminal Velocity Calculator handles any combination of these inputs. For special relativity, the Time Dilation Calculator shows how time slows and length contracts at relativistic speeds: t' = t/√(1−v²/c²). At 80% the speed of light, γ = 1/√(1−0.64) = 1.67, so 1 year on the rocket is 1.67 years on Earth. The Physics Formulas Cheatsheet provides a printable, searchable reference covering all major topics.
Frequently Asked Questions
How do I calculate work done by a force?
Work is calculated as W = F × d × cos θ, where F is the magnitude of the force, d is the displacement, and θ is the angle between the force vector and the direction of motion. If the force is parallel to the motion (θ = 0°), W = Fd. If perpendicular (θ = 90°), no work is done. Work is measured in joules (J) — one joule equals one newton times one meter. The work-energy theorem states the net work done equals the change in kinetic energy.
What is the difference between static and kinetic friction?
Static friction acts on a stationary object and prevents it from sliding. It can vary from zero up to a maximum value of f_s = μ_s × N, where μ_s is the static friction coefficient and N is the normal force. Kinetic friction acts on a sliding object and has a constant value f_k = μ_k × N, where μ_k < μ_s. This is why it takes more force to start an object sliding than to keep it sliding. Friction coefficients depend on both materials in contact.
How does Snell's law work for light refraction?
Snell's law n₁ sin θ₁ = n₂ sin θ₂ describes how light bends when crossing between media with different refractive indices. When light moves from a less dense medium (smaller n) to a denser medium (larger n), it bends toward the normal (smaller angle). When moving from denser to less dense, it bends away from the normal. At the critical angle θ_c = arcsin(n₂/n₁), the refracted ray runs along the surface. Beyond the critical angle, total internal reflection occurs — no light passes through.
How do I calculate the magnetic field around a current-carrying wire?
For a long straight wire, the magnetic field at distance r from the wire is B = μ₀I/(2πr), where μ₀ = 4π × 10⁻⁷ T·m/A is the permeability of free space. The field forms concentric circles around the wire, with direction given by the right-hand rule (thumb in direction of current, fingers curl in direction of B). A wire carrying 10 A creates a field of B = (4π × 10⁻⁷ × 10)/(2π × 0.01) = 0.2 mT at 1 cm distance.
What is terminal velocity and how is it calculated?
Terminal velocity is the constant speed reached when the drag force equals the gravitational force on a falling object. The formula is v_t = √(2mg / ρAC_d), where m is mass, g is gravitational acceleration (9.8 m/s²), ρ is air density (1.225 kg/m³ at sea level), A is the cross-sectional area, and C_d is the drag coefficient. For a typical skydiver in a spread-eagle position, terminal velocity is about 53 m/s (190 km/h). In a head-down position with smaller cross-section, it can reach 90 m/s (320 km/h).