Physics

From falling apples to black holes. 10 topics covering the laws that govern everything.

10 topics

Topics in Physics

Physics - From Newton to Quantum

You Never Actually Touch Anything

You are sitting in a chair right now. You can feel it. Your weight pressing into the seat, the backrest against your spine. Feels pretty solid. But you are not actually touching the chair. The atoms in your body and the atoms in the chair never make contact. What you feel is electromagnetic repulsion: the negatively charged electron clouds around your atoms pushing against the negatively charged electron clouds around the chair's atoms. At the atomic level, there is a gap. Always. You have never touched anything in your entire life, and you never will. Physics says so.

That fact alone captures what physics is. Not a collection of formulas to memorize for an exam. Not an abstract branch of science that only matters in laboratories. Physics is the study of why things happen, from the smallest particles inside an atom to the largest structures in the universe. It explains why a ball curves when you throw it, why your coffee gets cold, why the sky is blue, why magnets stick to fridges, why the sun shines, and why you don't fall through your chair. Every other science, chemistry, biology, geology, astronomy, is really applied physics with extra context.

This subject covers Newtonian mechanics (the physics of everyday motion), thermodynamics (heat, energy, and entropy), electricity and magnetism (the force behind every device you own), waves and optics (light, sound, and everything in between), and modern physics (the weird stuff that turns out to be how reality actually works). Ten topics. One coherent picture of how the universe operates.

299,792,458 m/s
Speed of light in a vacuum. Nothing with mass can reach it. Ever.
1080
Estimated number of atoms in the observable universe
-273.15°C
Absolute zero. The temperature where all molecular motion stops.
9.8 m/s²
Earth's gravitational acceleration. The reason everything falls.

Classical Mechanics: The Physics You Can See

Drop a ball. It falls. Push a shopping cart. It moves. Hit the brakes in your car. You lurch forward. These are all examples of Newtonian mechanics, and they trace back to three laws that Isaac Newton published in 1687. Three laws. That's it. From those three statements, you can predict the motion of baseballs, rockets, roller coasters, planets, and everything else that isn't absurdly small or absurdly fast.

Newton's first law says objects resist changes in motion. A hockey puck on ice keeps sliding until friction slows it down. You fly forward in a car crash because your body wants to keep moving even after the car stops. This is inertia, and it is the reason seatbelts exist. Newton's second law says force equals mass times acceleration (F = ma). Push something harder, it accelerates more. Push something heavier, it accelerates less. Simple arithmetic, but from it you get the physics of bridges, airplanes, and Olympic sprinters. Newton's third law says every action has an equal and opposite reaction. A rocket pushes exhaust downward; the exhaust pushes the rocket upward. You stand on the floor; the floor pushes back up on you with exactly the same force.

The mechanics of everyday life extend into circular and rotational motion, which explains why figure skaters spin faster when they pull their arms in, why you feel pushed outward on a merry-go-round, and how washing machines extract water from clothes. And it connects to gravitation, the reason apples fall, moons orbit, and tides rise and fall. Classical mechanics is the foundation. You build everything else on top of it.

What makes classical mechanics so satisfying is its predictability. If you know where something is, how fast it's moving, and what forces act on it, you can calculate exactly where it will be at any future moment. Engineers use this to design bridges that hold thousands of tons of traffic. NASA uses it to land rovers on Mars with pinpoint accuracy after a seven-month journey through space. The mathematics behind it is algebra and calculus, tools that translate physical intuition into precise numbers.

Thermodynamics: Why Your Coffee Gets Cold and the Universe Winds Down

Pour a hot cup of coffee and leave it on your desk. Come back in an hour. It's room temperature. You already knew that would happen, but thermodynamics explains why, and the explanation has consequences far bigger than lukewarm coffee.

Heat flows from hot objects to cold objects. Always. Never the other way around, not spontaneously. Your coffee loses heat to the surrounding air because the coffee molecules are vibrating faster (higher temperature) than the air molecules. Energy transfers from the faster-vibrating system to the slower one until they equalize. This is the second law of thermodynamics at work, and it is arguably the most important law in all of physics.

The second law introduces entropy, a measure of disorder in a system. Entropy always increases in an isolated system. A neat room gets messy. A sandcastle erodes. An ice cube melts. Energy spreads out and becomes less concentrated, less useful. You can locally decrease entropy (clean your room, build a sandcastle, freeze water), but only by increasing entropy somewhere else by an even greater amount. The total disorder of the universe always goes up. This is why perpetual motion machines are impossible. This is why every engine wastes some energy as heat. This is, physicists believe, why time has a direction at all.

The Arrow of Time

Almost every law of physics works the same forwards and backwards in time. Drop a ball and film it; play the video in reverse; the reverse looks physically plausible. But the second law of thermodynamics doesn't work in reverse. Scrambled eggs never unscramble. Shattered glass never reassembles. Entropy gives time a direction. Without it, the universe would have no past or future, just a sequence of equally valid states. The reason you remember yesterday but not tomorrow may ultimately be thermodynamic.

Thermodynamics also governs every engine and refrigerator ever built. A car engine converts chemical energy (gasoline) into heat, then into mechanical motion, with unavoidable waste heat escaping. A refrigerator moves heat from inside (cold space) to outside (warm room), but only by pumping in electrical energy. The study of energy and power formalizes these relationships: how energy transforms from one type to another, how efficiently, and where the losses go. This connects directly to chemistry (chemical energy, reaction heat) and to engineering (designing systems that waste less).

Electricity and Magnetism: The Force Behind Modern Civilization

Take away electricity and magnetism, and modern life doesn't just become inconvenient. It ceases to exist. No phones, no lights, no computers, no internet, no medical imaging, no electric motors, no power grid. The entire technological infrastructure of human civilization runs on the electromagnetic force, and the physics behind it is one of the most elegant structures in all of science.

Electric charge comes in two types: positive and negative. Like charges repel; opposite charges attract. Moving charges (current) create magnetic fields. Changing magnetic fields create electric fields. That last fact is the one that changed the world. In 1831, Michael Faraday showed that moving a magnet near a wire induces an electric current. That's electromagnetic induction, and it is how every power plant on Earth generates electricity, from coal plants to nuclear reactors to wind turbines. A turbine spins a magnet inside coils of wire, and current flows. The engineering varies. The physics is always the same.

In the 1860s, James Clerk Maxwell unified electricity and magnetism into a single framework with four equations. Those four equations predicted that oscillating electric and magnetic fields would propagate through space as waves, at a speed Maxwell calculated to be 3 x 108 meters per second. That number matched the measured speed of light. Light, Maxwell realized, is an electromagnetic wave. So are radio waves, microwaves, X-rays, and gamma rays. Every form of electromagnetic radiation, from the Wi-Fi signal crossing your room right now to the gamma rays from a distant supernova, follows Maxwell's equations.

The electromagnetic force is also responsible for essentially every chemical bond. The atoms in your body stick together because of electromagnetic attraction between protons and electrons. Chemical reactions are electromagnetic rearrangements. When you think about it, chemistry is really the study of electromagnetic interactions between atoms. Physics just gets there first.

1687
Newton publishes the Principia

Three laws of motion and universal gravitation. Mechanics becomes predictive science.

1831
Faraday discovers electromagnetic induction

Moving magnets create electric current. Foundation for generators and the entire power grid.

1865
Maxwell's equations unify electricity, magnetism, and light

Four equations predict electromagnetic waves and identify light as one. Radio communication follows.

1905
Einstein publishes special relativity and the photoelectric effect

Time dilation, mass-energy equivalence (E = mc²), and the quantum nature of light. Physics splits in two directions.

1915
General relativity: gravity is curved spacetime

Mass bends the fabric of space and time. Explains Mercury's orbit, predicts black holes, and redefines gravity.

1926
Quantum mechanics formalized

Schrödinger, Heisenberg, and others build the math of the quantum world. Particles become probability waves.

1964
Higgs mechanism proposed

Explains why particles have mass. Confirmed in 2012 at CERN with the discovery of the Higgs boson.

2015
LIGO detects gravitational waves

Ripples in spacetime from colliding black holes, confirmed a century after Einstein predicted them.

Waves and Optics: How Information Travels

Why is the sky blue? Because sunlight enters the atmosphere and shorter wavelengths (blue light) scatter more than longer wavelengths (red light) when they hit air molecules. That's Rayleigh scattering, and it's a direct consequence of wave physics. The same wave principles explain why you hear your neighbor's bass through the wall but not their conversation (low frequencies diffract around obstacles better than high ones), why rainbows form (refraction separates white light into its component wavelengths), and why noise-canceling headphones work (destructive interference cancels unwanted sound waves).

Waves are one of physics' great unifying concepts. Sound waves, water waves, light waves, seismic waves, and radio waves all share the same core behavior: they carry energy without carrying matter. A sound wave moves through air, but the air molecules themselves just vibrate back and forth. An ocean wave moves across the surface, but the water mostly stays in place. Understanding frequency, wavelength, amplitude, interference, diffraction, and resonance gives you a toolkit that applies everywhere.

Optics, the study of light specifically, has shaped technology at every turn. Lenses focus light in cameras, microscopes, telescopes, and your own eyes. Fiber optic cables carry internet data as pulses of light across oceans. Lasers produce coherent light for surgery, manufacturing, barcode scanners, and the disc drives that were everywhere before streaming took over. The physics of how light reflects, refracts, diffracts, and interferes is the physics behind nearly every imaging and communication technology humans have built.

And then there's the electromagnetic spectrum. Visible light is just one narrow band of electromagnetic radiation. Below it in frequency: infrared (heat lamps, TV remotes), microwaves (your kitchen, Wi-Fi, cell signals), and radio waves (FM, TV broadcast, Bluetooth). Above it: ultraviolet (sunburn), X-rays (medical imaging), and gamma rays (nuclear reactions, cancer treatment). All of these are the same phenomenon, electromagnetic waves, at different frequencies. Your phone receives microwaves from a cell tower, displays visible light on its screen, and connects to your earbuds via radio waves. All wave physics. All the same equations.

Modern Physics: Where Reality Gets Strange

Classical physics, everything covered so far, works brilliantly for objects you can see and speeds you can experience. But at the start of the twentieth century, physicists discovered that the rules break down at two extremes: the very small (atoms and subatomic particles) and the very fast (speeds approaching light). Modern physics is what replaced the broken rules.

Classical Physics

Objects have definite positions and velocities at all times. Energy is continuous. Space and time are absolute and separate. Gravity is a force pulling objects together. Works perfectly for everyday objects at everyday speeds. Breaks down at atomic scales and near light speed.

Modern Physics

Particles exist as probability distributions until measured. Energy comes in discrete packets (quanta). Space and time are woven together and bend in the presence of mass. Gravity is the curvature of spacetime itself. Required for atoms, nuclei, light-speed phenomena, and extreme gravity.

Einstein's special relativity (1905) showed that time slows down for objects moving close to the speed of light, that lengths contract in the direction of motion, and that mass and energy are two forms of the same thing (E = mc²). This is not theoretical speculation. GPS satellites move fast enough relative to the ground that their clocks tick measurably slower due to special relativity (and faster due to general relativity's gravitational time dilation). Without correcting for both effects, GPS would drift by about 10 kilometers per day. Your navigation app depends on Einstein being right.

General relativity (1915) went further: gravity is not a force in the Newtonian sense. Massive objects curve the fabric of spacetime, and other objects follow that curvature. The Earth orbits the Sun not because the Sun pulls on it, but because the Sun's mass warps the space around it, and the Earth follows the straightest possible path through that curved space. This framework predicts black holes (regions where spacetime curves so extremely that nothing, not even light, can escape), gravitational waves (ripples in spacetime caused by accelerating masses), and the expansion of the universe itself.

Quantum mechanics is the other pillar of modern physics, governing the subatomic world. Electrons don't orbit the nucleus like tiny planets. They exist as probability clouds. You cannot simultaneously know a particle's exact position and exact momentum (Heisenberg's uncertainty principle). Light behaves as both a wave and a particle. These are not limitations of our instruments. They are fundamental features of reality. The technology that runs on quantum mechanics includes semiconductors (every computer chip), lasers, MRI machines, and LED displays. Quantum mechanics is not abstract. It is the physics inside your phone. For a deeper look at where this leads, the connection from quantum mechanics to quantum computing is one of the most fascinating threads in modern technology.

The Overlooked Middle: Fluids, Materials, and Gravity

Three topics in physics often get less attention than they deserve, even though they govern enormous parts of the physical world.

Fluid mechanics describes how liquids and gases behave. It explains why airplanes fly (pressure differences created by air flowing over curved wings), why blood flows through arteries the way it does, why weather systems form, and why a curveball curves. The same equations govern water flowing through pipes, oil being extracted from reservoirs, and the aerodynamics of Formula 1 cars. Any engineer working with moving fluids, which includes aerospace, civil, biomedical, chemical, and mechanical engineering, needs fluid mechanics.

Materials and their properties connect physics to the real world of building things. Why is steel strong but heavy? Why is glass transparent? Why do rubber bands stretch but metal bars don't? The answers lie in atomic structure, molecular bonds, and the way forces propagate through crystalline and amorphous materials. Material science sits at the intersection of physics and chemistry, and it drives innovation in everything from smartphone screens (Gorilla Glass bends without breaking because of ion-exchange strengthening) to aircraft bodies (carbon fiber composites are stronger than steel at a fraction of the weight).

Gravitation connects the physics of falling apples to the physics of orbiting galaxies. Newton described gravity as a force proportional to mass and inversely proportional to distance squared. Einstein redescribed it as the curvature of spacetime. Both descriptions make accurate predictions in their respective domains. Gravitation explains tides, satellite orbits, the trajectories of space probes, and the large-scale structure of the cosmos. It's also the one fundamental force that physicists still can't fully reconcile with quantum mechanics, making it one of the biggest open problems in all of science.

How the 10 Topics Connect

Physics is not a collection of separate topics that happen to share a name. The ten topics in this subject form a connected structure, where each one feeds into and draws from the others.

Newtonian Mechanics
Circular & Rotational Motion
Gravitation
Energy & Power
Thermodynamics
Fluid Mechanics
Electricity & Magnetism
Waves & Optics
Modern Physics

Newtonian mechanics provides the foundation: forces, acceleration, momentum. From there, circular and rotational motion extends those ideas to spinning and orbiting objects, which leads naturally into gravitation (the force responsible for most orbital motion). Meanwhile, energy and power introduces the conservation laws that underpin thermodynamics, which in turn informs fluid mechanics (pressure, temperature, and energy transfer in fluids). Electricity and magnetism generates the electromagnetic waves studied in waves and optics, and both of these topics find their deeper explanations in modern physics. Materials and properties draws from all three streams: mechanics (stress, strain), thermodynamics (thermal expansion), and electromagnetism (conductivity, magnetism).

The point is that learning one topic in physics does not just add knowledge. It deepens your understanding of every other topic. Forces explain energy. Energy explains heat. Heat explains engines. Engines run on electromagnetism. Electromagnetism is light. Light is quantum. The chain doesn't end.

Where Physics Meets Everything Else

Physics is the foundation that other sciences and engineering fields build on. This is not a claim of superiority. It's a structural fact about how knowledge layers.

Chemistry is electromagnetic interactions between atoms. Chemical bonding, reaction rates, molecular structures: all governed by quantum mechanics and electromagnetism. Physical chemistry is one of the largest subfields in chemistry, and it's essentially applied physics. If you understand thermodynamics and quantum mechanics, half of chemistry clicks into place immediately.

Engineering is applied physics with constraints. Civil engineers use mechanics and materials science to design structures. Electrical engineers use circuit theory and electromagnetism. Mechanical engineers use thermodynamics and fluid mechanics. Aerospace engineers combine all of the above. The physics comes first; the engineering adds real-world constraints like cost, manufacturing, and safety margins.

Computer science intersects with physics in multiple ways. At the hardware level, every computer chip runs on semiconductor physics (quantum mechanics of electron behavior in silicon). At the cutting edge, quantum computing is literally building computers that run on quantum mechanical principles. Physics simulations are among the most computationally demanding tasks in computer science, driving advances in algorithms and hardware alike.

Astronomy is physics pointed at the sky. Every tool astronomers use, telescopes (optics), radio dishes (electromagnetic waves), spectroscopy (quantum mechanics), gravitational wave detectors (general relativity), is a physics instrument. Astrophysics is not a separate subject. It is physics applied to the cosmos.

Even fields far from the lab have physics roots. Economics uses thermodynamic concepts like equilibrium and entropy as analogies (and sometimes as direct models). Biology depends on biophysics for understanding protein folding, nerve impulses, blood flow, and vision. Music is acoustics. Sports science is biomechanics. Architecture is structural physics. Mathematics provides the language, but physics provides the meaning.

Why Physics Feels Hard (and Why It's Worth It)

Physics has a reputation for being difficult. Some of that reputation is earned. It requires comfort with abstraction, fluency in mathematics, and a willingness to abandon common-sense intuitions when experiments demand it. The quantum world does not care about your intuitions. Neither does relativity. You have to follow the math and the evidence, even when they lead somewhere your brain resists.

But a lot of physics' difficulty is artificial, created by bad teaching and worse textbooks. Physics taught as a list of formulas to plug numbers into is brutal and pointless. Physics taught as a sequence of questions (why does this happen? what predicts it? how do we test that prediction?) is one of the most intellectually rewarding subjects that exists. The formulas matter, but they're the output of understanding, not the input.

A Counterintuitive Truth

Heavy objects and light objects fall at the same rate. Galileo demonstrated this around 1590 (the Tower of Pisa story is probably a legend, but the physics is real). In a vacuum, a bowling ball and a feather hit the ground at the same time. Apollo 15 astronaut David Scott confirmed this on the Moon in 1971 with a hammer and a falcon feather on live television. Gravity accelerates all objects equally regardless of mass. Your intuition that heavier things fall faster comes from air resistance, not from gravity. Remove the air, and the distinction vanishes.

The payoff for learning physics is a different way of seeing the world. You start noticing forces everywhere. You watch a car take a turn and think about centripetal acceleration. You see a sunset and think about photon wavelengths scattering through atmosphere. You hold your phone and think about the billions of electrons flowing through transistors smaller than a virus. Physics doesn't make the world less beautiful. It adds another layer of beauty that most people never get to see.

Physics is the operating system of reality. Every other science runs on top of it. These ten topics give you the core framework: how objects move, how heat flows, how electricity works, how waves carry information, how matter behaves under stress, and how the universe operates at scales too small or too fast for classical rules. You don't need to become a physicist to benefit from thinking like one. The habit of asking "why does this happen?" and insisting on a testable answer is the most transferable skill physics teaches. Start with Newtonian mechanics if you want to build from the ground up, or jump to modern physics if the strange stuff drew you here. Either way, you are learning the language the universe is written in.