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Physics Guide

A comprehensive guide to physics: motion, projectile trajectories, Newton's laws of force, kinetic and potential energy, wave speed, Ohm's law electricity, density, and horsepower. Learn the core ideas with worked examples and links to dedicated calculators.

Introduction

Physics is the science of how the universe behaves — how things move, why they fall, how energy flows, and how electricity powers everything from a phone to a city. You encounter physics every time you brake a car, swing a bat, charge a battery, or hear music through a wall. It is not reserved for laboratory coats; it is the operating manual for the physical world.

This guide walks through the core ideas of classical physics in plain language: motion and projectile paths, the forces described by Newton's laws, the kinetic and potential energy stored in moving and elevated objects, the speed of waves, the flow of current described by Ohm's law, the density of matter, and the horsepower that measures mechanical power. Each section pairs intuition with a worked numerical example and links to a dedicated calculator you can use to verify your hand calculations.

The goal is to build physical intuition first and equations second. When a formula feels abstract, plug your own numbers into the linked tool and watch the quantities resolve.

Physics also unifies ideas that look separate. The same conservation-of-energy principle that explains a falling ball also governs a roller coaster, a hydroelectric dam, and the fuel burned in a jet engine. The same wave equation that describes a guitar string describes light, radio, and the seismic waves that shake the ground. Learning the fundamentals here gives you a lens for nearly every technology you touch, and a way to estimate answers in daily life without reaching for a device.

Motion & Projectile Motion

Motion is described by three quantities: position (where something is), velocity (how fast and in what direction it moves), and acceleration (how quickly velocity changes). The simplest model assumes constant acceleration, which leads to the kinematic equations. For an object starting at rest and accelerating at a for time t, the distance traveled is d = ½at², and its final speed is v = at.

Projectile motion is the classic application: an object launched into the air follows a curved, parabolic path because gravity pulls it downward while its horizontal speed stays constant (ignoring air resistance). The horizontal and vertical motions are independent — a ball dropped and a ball thrown sideways from the same height hit the ground at the same instant.

v_yv_xv
A projectile's velocity has independent horizontal (v_x) and vertical (v_y) components; the launch angle sets how they split.

The Projectile Motion Calculator takes a launch speed, angle, and initial height and returns the time of flight, maximum height, and horizontal range. A worked example: a ball thrown at 20 m/s at a 45° angle from the ground. The horizontal and vertical components are each 20 · cos(45°) ≈ 14.1 m/s. Time to peak is v_y / g = 14.1 / 9.81 ≈ 1.44 s, so total flight is about 2.88 s, and the range is v_x · t ≈ 14.1 · 2.88 ≈ 40.6 m. The 45° angle maximizes range for a given speed on level ground.

Real projectiles are also slowed by air drag, which shortens the range and lowers the peak — a reminder that ideal models are approximations, not the whole story.

Forces & Newton's Laws

A force is a push or a pull, measured in newtons (N). Isaac Newton distilled motion into three laws. The first says an object at rest stays at rest, and an object in motion stays in motion at constant velocity, unless acted on by a net force — this is inertia. The second law is the backbone of mechanics:

F=maF = m \cdot a

Force equals mass times acceleration. To accelerate a 1,200 kg car at 2 m/s², the engine must supply F = 1200 · 2 = 2,400 N. The third law states that every action has an equal and opposite reaction: a rocket pushes exhaust downward, and the exhaust pushes the rocket upward.

When an object moves in a circle, it constantly changes direction, so it constantly accelerates toward the center. That inward acceleration requires a centripetal (center-seeking) force:

Fc=mv2rF_c = \frac{m v^2}{r}

The Force Calculator applies F = ma directly, while the Centripetal Force Calculator computes the inward pull needed to hold a mass m moving at speed v around a radius r. For a 1,000 kg car taking a 50 m curve at 20 m/s, F_c = 1000 · 20² / 50 = 8,000 N — a substantial force supplied by tire friction. Take the curve too fast and friction is exceeded, and the car slides outward.

aFm
Newton's second law: a net force F applied to a mass m produces acceleration a in the same direction as the force.

Kinetic & Potential Energy

Energy is the capacity to do work, measured in joules (J). An object in motion carries kinetic energy:

KE=12mv2KE = \frac{1}{2} m v^2

Notice the squared velocity: doubling speed quadruples kinetic energy, which is why high-speed collisions are so destructive. A 1,500 kg car at 30 m/s has KE = 0.5 · 1500 · 30² = 675,000 J.

An object raised against gravity stores gravitational potential energy:

PE=mghPE = m g h

A 10 kg box lifted 2 m gains PE = 10 · 9.81 · 2 ≈ 196 J. This energy is released as kinetic energy if the box falls: by the time it reaches the floor, its potential energy has converted into motion (minus losses to air resistance).

The Kinetic & Potential Energy Calculator computes both quantities from mass, speed, and height. A key idea is conservation of energy: in a closed system, total energy stays constant, only shifting between forms. A pendulum trades potential energy at the top of its swing for kinetic energy at the bottom, the sum remaining fixed.

Numerical example: a 2 kg ball dropped from 5 m starts with PE = 2 · 9.81 · 5 ≈ 98 J and zero kinetic energy. Just before impact, all of it has become kinetic energy, so ½mv² = 98, giving v = √(2·98/2) ≈ 9.9 m/s — exactly what free-fall kinematics predicts.

Waves & Wave Speed

A wave transfers energy through a medium without transporting the medium itself — sound through air, ripples across water, light through space. Every wave has a frequency f (how many cycles pass per second, in hertz) and a wavelength λ (the distance between successive crests). These set the wave's speed:

v=fλv = f \cdot \lambda

For sound in air at room temperature, v ≈ 343 m/s. If a note has frequency 686 Hz, its wavelength is λ = v/f = 343/686 = 0.5 m. Higher frequency means shorter wavelength, which is why a squeak (high pitch) has a tighter wave than a rumble (low pitch).

The Wave Speed Calculator returns any one of v, f, or λ given the other two. The relationship explains why you see lightning before you hear thunder: light travels at about 300,000,000 m/s while sound crawls at 343 m/s, so the delay between flash and boom tells you the storm's distance (roughly 3 seconds per kilometer).

Different media carry waves at different speeds. Sound moves faster in water and steel than in air because their particles are more tightly coupled; light slows in glass or water, which is what bends a straw in a glass of water.

Electricity & Ohm's Law

Electricity is the flow of electric charge (electrons) through a conductor. Three quantities govern a simple circuit: voltage V (electrical pressure, in volts), current I (flow rate of charge, in amperes), and resistance R (opposition to flow, in ohms). Ohm's law ties them together:

V=IRV = I \cdot R

Raise the voltage and current rises; raise the resistance and current falls. If a 12 V battery drives a 4 Ω resistor, the current is I = V/R = 12/4 = 3 A.

The Ohms Law Calculator solves for any one of the three variables from the other two. Real circuits, however, are rarely a single resistor. Components are wired in series (current is the same, resistances add) or in parallel (voltage is the same, reciprocal resistances add). The Resistor Calculator handles equivalent resistance for these combinations and decodes color-band resistor markings common on circuit boards.

Wires themselves have resistance, so voltage drops along a long run — a problem in power delivery and audio cabling. The Voltage Drop Calculator estimates that loss from wire length, gauge, current, and material, helping you choose a thick enough conductor. The Electricity Calculator bundles related electrical conversions and power computations in one place.

Numerical example: a 9 V battery feeds two 6 Ω resistors in series, total R = 12 Ω, so I = 9/12 = 0.75 A. Each resistor drops V = IR = 0.75 · 6 = 4.5 V, and the two drops sum back to the 9 V supply — a consistency check that always holds in series.

Density & Matter

Density is how much mass is packed into a given volume, ρ = m/V, in kilograms per cubic meter (or grams per cubic centimeter). It decides whether objects float: a substance less dense than water (≈ 1,000 kg/m³) rises, a denser one sinks. Wood (≈ 600 kg/m³) floats; iron (≈ 7,870 kg/m³) sinks.

The Density Calculator computes density, mass, or volume from any two of the three. Worked example: a gold bar (density ≈ 19,300 kg/m³) with volume 0.0001 m³ has mass m = ρV = 19,300 · 0.0001 = 1.93 kg. Density also drives buoyancy — Archimedes' principle says a floating object displaces a weight of fluid equal to its own weight, which is how ships of steel (dense) float by enclosing large volumes of air.

Temperature changes density: most substances expand when heated, lowering their density, which is why warm air rises and drives weather and convection in oceans and pots.

Power & Horsepower

Power is the rate of doing work, measured in watts (W), where 1 W = 1 J/s. Lifting a 100 J weight in 1 second takes 100 W; taking 10 seconds takes only 10 W, the same total energy spread over more time. Mechanical power is also force times speed, P = F · v.

Horsepower (hp) is a traditional unit: 1 hp ≈ 746 W, originally defined by James Watt to compare steam engines to draft horses. The Horsepower Calculator converts between hp, watts, and other units. The Engine Horsepower Calculator estimates an engine's output from torque and rotational speed, since Power = Torque · AngularSpeed, or in familiar units hp = (Torque · RPM) / 5252.

Numerical example: an engine producing 300 N·m of torque at 4,000 RPM delivers hp = 300 · 4000 / 5252 ≈ 228 hp. Double the RPM at the same torque and you double the horsepower — until the engine's breathing or fueling limits torque at high speed.

Power also matters for efficiency. A more powerful engine is not automatically less efficient; it simply has more reserve. What drains fuel is running an engine far from its optimal load, which is why steady highway cruising sips less than stop-and-go city driving even at higher speeds. The same idea applies to electric motors and household appliances, where matching the tool to the task saves energy.

Practical Tips for Learning Physics

  1. Draw a free-body diagram. For any force problem, sketch the object and every force arrow (gravity down, normal up, friction opposing motion). Visualizing forces prevents sign errors.
  2. Keep units attached. Treat 9.81 m/s² as a quantity, not a number. If your final answer's units are wrong, the equation was misapplied.
  3. Check with the linked calculators. Solve by hand, then confirm with the relevant tool. A mismatch usually means a sign or unit slip, not a flaw in the calculator.
  4. Separate the axes. In projectile motion, horizontal and vertical are independent. Solve each with its own rules, then recombine.
  5. Watch for squared terms. Kinetic energy scales with and centripetal force with ; small speed changes produce large effects.
  6. Respect idealizations. Frictionless ramps, massless pulleys, and no air resistance are teaching tools. Real-world results differ, often importantly.

Limitations & Caveats

  • Constant-acceleration equations assume a is fixed. They fail for rockets burning fuel or objects with drag, where acceleration changes continuously.
  • Projectile formulas ignore air resistance. At high speeds or light masses, drag dominates and the real range is far shorter than the parabola predicts.
  • Ohm's law is not universal. It holds for ohmic (resistor-like) materials at stable temperature. Diodes, transistors, and incandescent bulbs are non-linear; their current does not scale linearly with voltage.
  • Density varies with temperature and pressure. A single number is a snapshot at given conditions, not an immutable constant for a substance.
  • Horsepower figures depend on measurement method. Crank, wheel, and brake horsepower differ; conversions assume ideal conditions.
  • Energy is conserved, but not always useful. Some input energy always becomes waste heat, so real efficiency is below 100%.

Frequently Asked Questions

What is the difference between speed and velocity?
Speed is how fast something moves (a scalar, no direction). Velocity includes direction (a vector), so 60 km/h north differs from 60 km/h south, and an object moving in a circle at constant speed has a changing velocity because its direction changes.
Why does a 45° launch angle give maximum range?
The range formula depends on sin(2θ), which peaks at 1 when 2θ = 90°, so θ = 45°. On level ground with no air resistance, this splits launch speed evenly between horizontal and vertical motion for the longest flat-flight distance.
What does Newton's third law really mean?
For every force one object exerts, it feels an equal and opposite force from the other. When you push a wall, the wall pushes back with equal force; the reason you move and the wall does not is the difference in mass and what each is anchored to.
Why is kinetic energy proportional to velocity squared?
It follows from integrating force over distance. Because work is force times distance and acceleration ties force to velocity, the energy needed to reach a speed v comes out as ½mv². The v² term is why stopping distance grows with the square of speed.
What is the difference between kinetic and potential energy?
Kinetic energy is energy of motion, possessed by anything moving. Potential energy is stored energy of position or configuration — gravitational (height), elastic (stretched spring), or chemical. They convert into each other, keeping total energy constant in a closed system.
How do I remember v = fλ?
Wave speed is distance per time. Wavelength λ is the distance of one cycle and frequency f is cycles per second, so λ times f gives distance per second — the speed. Units confirm it: meters times 1/seconds equals meters/second.
What is Ohm's law used for in real circuits?
It lets you compute the missing value among voltage, current, and resistance, size current-limiting resistors, predict how bright a bulb will be, and troubleshoot why a circuit draws too much or too little current.
Why do objects float or sink based on density?
An object floats if it is less dense than the fluid it displaces. Buoyant force equals the weight of displaced fluid (Archimedes' principle); if the object's density is lower, that upward force exceeds the object's weight and it rises.
What is the difference between horsepower and watts?
Both measure power (energy per time). One mechanical horsepower is about 746 watts. Horsepower is traditional in engines and motors; watts are the SI unit used in electrical and scientific contexts, and conversions between them are exact by definition.
Why does air resistance matter so much for projectiles?
Drag grows roughly with the square of speed and opposes motion, so fast or light objects lose horizontal and vertical energy quickly. A cannonball and a ping-pong ball launched identically behave nothing alike because drag dominates the lighter one.
Is Ohm's law always true?
No. It applies to ohmic materials whose resistance stays constant with voltage and temperature. Many components — LEDs, diodes, batteries, and hot filaments — are non-ohmic, so current is not proportional to voltage across them.
How is wave speed different from the speed of the medium?
The wave travels through the medium, but the medium's particles mostly oscillate in place. In a stadium wave, the pattern moves around the stands while each person only stands and sits; the wave speed is not the speed of any individual person.
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