From protons to the universe: what physics is, how scientists work, how we measure things and read graphs, with diagrams, animations and worked examples.
Why does a ball fall when you let it go? Why is the sky blue? How does a phone know where you are? How can an invisible force hold the Moon in orbit? Physics is the science that tries to answer questions like these, from the smallest particles inside an atom to the largest structures in the universe. The word comes from the Greek physis, meaning nature. Physicists look for the simple rules that lie behind the complicated things we see, test those rules with careful experiments, and write them in the language of mathematics. This opening article explains what physics is, how scientists work, how we measure things, and how to read graphs and handle numbers. It also serves as a map to the rest of the EDUSAMBAM physics series.
Physics is the study of matter, energy, and the forces and interactions between them. It asks what things are made of, how they move, how energy is stored and transferred, and what rules govern everything from falling apples to galaxies. Because physics looks for basic principles, it underlies other sciences. Chemistry depends on the physics of atoms and electrons; biology on the physics of molecules, fluids and electrical signals; geology on heat flow and forces inside the Earth; and engineering on all of them.
Physics has three characteristic features:
Physics is not only for scientists. It explains the technology around you and builds skills that every career needs: logical thinking, careful measurement and problem solving.
| Branch | What it studies | Read more on EDUSAMBAM |
|---|---|---|
| Mechanics | Motion, forces, energy, momentum, machines, fluids | Motion, Force and Newton's laws, Work, power and machines, Pressure and buoyancy |
| Thermal physics | Heat, temperature, states of matter, gases | Heat and temperature, Matter and its states |
| Waves and optics | Sound, light and other waves; mirrors and lenses | Waves, Sound, Light |
| Electricity and magnetism | Charge, current, circuits, magnets, induction | Electricity and magnetism |
| Energy and its uses | Forms, conservation, resources, efficiency | Energy |
| Astronomy and cosmology | Planets, stars, galaxies, the universe | Gravity and space |
| Atomic, nuclear and particle physics | Atoms, radioactivity, nuclear energy, fundamental particles | Atomic and nuclear physics |
| Modern physics | Relativity and quantum mechanics | Introduced in the timeline and frontiers below |
Physics is a human story that spans many cultures and centuries. Here are a few landmarks.
| When | Who and what |
|---|---|
| c. 1011–1021 | Ibn al-Haytham (Alhazen) writes the Book of Optics. He shows that we see because light enters the eye, and he insists on testing ideas with controlled experiments, a major step towards the modern scientific method. |
| c. 1025 | Al-Biruni estimates the Earth's radius by measuring the height of a mountain and the angle of the horizon, obtaining a value remarkably close to the modern one. |
| 1609–1610 | Galileo Galilei uses the telescope to observe the Moon's mountains and Jupiter's moons, and carries out careful studies of falling bodies and motion. |
| 1687 | Isaac Newton publishes the Principia, setting out the laws of motion and universal gravitation. |
| 1831 | Michael Faraday discovers electromagnetic induction, leading to generators and transformers. |
| 1865 | James Clerk Maxwell shows that light is an electromagnetic wave. |
| 1898–1911 | Marie Curie studies radioactivity and wins Nobel Prizes in Physics (1903) and Chemistry (1911). |
| 1900–1926 | Max Planck introduces the quantum idea; Einstein explains the photoelectric effect (1905); Rutherford discovers the atomic nucleus (1911); Bohr proposes his atomic model (1913); Heisenberg and Schrödinger develop quantum mechanics (1925–26). |
| 1905, 1915 | Albert Einstein publishes special relativity (1905) and general relativity (1915), including E = mc². |
| 1938–1939 | Lise Meitner and Otto Frisch explain nuclear fission, building on experiments by Otto Hahn and Fritz Strassmann. |
| 1979 | Abdus Salam, born in what is now Pakistan, shares the Nobel Prize in Physics with Sheldon Glashow and Steven Weinberg for the theory that unifies the electromagnetic and weak forces. |
| 2012 | Experiments at CERN announce the discovery of the Higgs boson. |
| 2015 | The LIGO detectors observe gravitational waves from two merging black holes, a century after Einstein predicted them. |
Notice that discoveries build on each other: Faraday's experiments helped Maxwell, Maxwell's equations led to relativity, and so on. Scientists everywhere, from every culture, contribute to this shared body of knowledge.
There is no single fixed recipe, but most scientific investigations follow a cycle like the one below.
You want to find out whether a longer pendulum swings more slowly.
Independent variable: the length of the string (e.g. 20, 40, 60, 80, 100 cm).
Dependent variable: the time for one swing (the period), found by timing 20 swings and dividing by 20 to reduce the effect of reaction time.
Control variables: the mass of the bob, the starting angle (small, about 10°), the same stopwatch, the same location.
Repeat each length three times and take the mean. Plot period against length, or period squared against length, which gives a straight line for small angles.
A measurement has two parts: a number and a unit. "5" means nothing; "5 m" or "5 s" does. To share results across the world, scientists use the International System of Units (SI). It has seven base units:
| Quantity | Unit | Symbol | Defined using |
|---|---|---|---|
| Length | metre | m | the speed of light, c = 299 792 458 m/s |
| Mass | kilogram | kg | the Planck constant, h = 6.626 070 15 × 10⁻³⁴ J·s |
| Time | second | s | the caesium-133 atomic frequency, 9 192 631 770 Hz |
| Electric current | ampere | A | the elementary charge, e = 1.602 176 634 × 10⁻¹⁹ C |
| Temperature | kelvin | K | the Boltzmann constant, k = 1.380 649 × 10⁻²³ J/K |
| Amount of substance | mole | mol | the Avogadro constant, 6.022 140 76 × 10²³ per mole |
| Luminous intensity | candela | cd | a fixed luminous efficacy of light |
Since 2019 all seven units have been defined using fixed values of fundamental constants of nature. Before then the kilogram was the mass of a platinum-iridium cylinder kept near Paris; now, nothing physical needs to be kept. Other quantities have derived units built from the base units:
| Quantity | Unit | In base units |
|---|---|---|
| Force | newton (N) | kg·m/s² |
| Energy, work | joule (J) | N·m = kg·m²/s² |
| Power | watt (W) | J/s |
| Pressure | pascal (Pa) | N/m² |
| Frequency | hertz (Hz) | 1/s |
| Charge | coulomb (C) | A·s |
| Voltage | volt (V) | J/C |
| Resistance | ohm (Ω) | V/A |
To avoid very long numbers, we use prefixes that multiply units by powers of ten:
| Prefix | Symbol | Factor | Prefix | Symbol | Factor |
|---|---|---|---|---|---|
| nano | n | 10⁻⁹ | kilo | k | 10³ |
| micro | µ | 10⁻⁶ | mega | M | 10⁶ |
| milli | m | 10⁻³ | giga | G | 10⁹ |
| centi | c | 10⁻² | tera | T | 10¹² |
Standard form writes a number as A × 10ⁿ, where 1 ≤ A < 10. For example, the speed of light is 3.00 × 10⁸ m/s and the mass of an electron is about 9.11 × 10⁻³¹ kg.
Convert (a) 72 km/h to m/s, (b) 1.5 g/cm³ to kg/m³, (c) 250 mm² to m².
(a) 72 km/h = 72 × 1000 m ÷ 3600 s = 20 m/s (divide km/h by 3.6).
(b) 1.5 g/cm³ = 1.5 × 10⁻³ kg ÷ 10⁻⁶ m³ = 1500 kg/m³ (multiply g/cm³ by 1000).
(c) 1 mm = 10⁻³ m, so 1 mm² = 10⁻⁶ m². 250 mm² = 250 × 10⁻⁶ = 2.5 × 10⁻⁴ m².
Remember to square (or cube) the conversion factor for area and volume.
An important tool is dimensional checking. Both sides of an equation must have the same units. For example, in v = fλ, hertz × metres = (1/s) × m = m/s, which is the unit of speed ✓. If the units do not match, the equation (or your algebra) is wrong.
Scalars and vectors. A scalar has size only (mass, time, speed, energy); a vector has size and direction (displacement, velocity, force, acceleration). Two forces of 3 N and 4 N acting at right angles do not give 7 N but 5 N, found with Pythagoras' theorem, because direction matters.
Physics covers an astonishing range of sizes, more than 40 orders of magnitude. An order of magnitude is a factor of ten. Using powers of ten helps us estimate and compare.
An atom is about 10⁻¹⁰ m across. How many atoms would fit end to end across a human hair of width 10⁻⁴ m?
Number = 10⁻⁴ ÷ 10⁻¹⁰ = 10⁶ = about one million atoms.
| Instrument | Measures | Typical precision |
|---|---|---|
| Metre rule | Length | 1 mm |
| Vernier calipers | Small lengths, diameters | 0.1 mm (or 0.05 mm) |
| Micrometer screw gauge | Very small thicknesses, wire diameters | 0.01 mm |
| Measuring cylinder | Volume of liquids | 1 mL or 0.5 mL |
| Balance | Mass | 0.01 g to 1 g |
| Stopwatch | Time (human reaction time adds about 0.2 s) | 0.01 s (digital) |
| Thermometer | Temperature | 1 °C or 0.1 °C |
| Newton meter | Force | 0.1 N to 1 N |
| Ammeter and voltmeter | Current and voltage | depends on the scale |
(a) A micrometer shows 5.5 mm on the sleeve and 23 divisions on the thimble (each 0.01 mm). With the jaws closed it reads +0.02 mm. Find the true diameter.
Reading = 5.5 + 23 × 0.01 = 5.73 mm. True value = 5.73 − 0.02 = 5.71 mm.
(b) A vernier caliper shows the zero of the vernier scale just after 12 mm on the main scale, and the 6th vernier division lines up with a main-scale mark. Each vernier division adds 0.1 mm.
Reading = 12 + 6 × 0.1 = 12.6 mm.
No measurement is perfect. Two ideas describe how good it is:
Five measurements of a length are 20.1, 20.3, 20.2, 20.0 and 20.4 cm. Find the mean, the uncertainty and the percentage uncertainty.
Step 1. Mean = (20.1 + 20.3 + 20.2 + 20.0 + 20.4) ÷ 5 = 101.0 ÷ 5 = 20.2 cm.
Step 2. Range = 20.4 − 20.0 = 0.4 cm, so the uncertainty is about half the range: ± 0.2 cm.
Step 3. Percentage uncertainty = 0.2 ÷ 20.2 × 100% ≈ 1.0%.
Result: length = (20.2 ± 0.2) cm.
Significant figures. Your final answer should not suggest more accuracy than the data justify. For multiplication and division, give the answer to the same number of significant figures as the least precise value used. For example, 5.0 × 3.21 = 16.05, which is quoted as 16 (2 significant figures). Do not round intermediate steps; round only at the end.
Graphs reveal the relationship between two quantities. Plot the independent variable on the horizontal axis, label axes with quantity and unit, choose a scale that uses most of the paper, mark each point clearly, and draw a smooth line of best fit (it need not pass through every point but should have roughly equal points on either side).
For a straight-line graph y = mx + c, the gradient m = (change in y) ÷ (change in x) and the intercept c is where the line crosses the y-axis. Gradients often have a physical meaning: on a distance–time graph the gradient is speed, on a velocity–time graph it is acceleration, on a force–extension graph it is the spring constant.
A spring is stretched with forces of 2.0, 4.0, 6.0 and 8.0 N, producing extensions of 1.0, 2.0, 3.0 and 4.0 cm. Find the spring constant.
Step 1. The graph of force against extension is a straight line through the origin. Gradient = (8.0 − 2.0) ÷ (4.0 − 1.0) = 6.0 ÷ 3.0 = 2.0 N/cm.
Step 2. Convert: 2.0 N/cm = 2.0 ÷ 0.01 = 200 N/m. So k = 200 N/m.
Learn to understand, not just memorise: ask "why does this make sense?" for each formula. Use real-life examples, practise many problems of different types, and learn from errors rather than hiding them.
Physics is not finished. Some of the biggest open questions are:
The next great discoveries might come from someone who is learning the basics today.
Try each question before opening the answer.
Metre (m), kilogram (kg) and second (s).
3.5 km = 3500 m. 450 mL = 0.45 L.
4.5 × 10⁻⁵ m.
Mean = 7.65 ÷ 5 = 1.53 m. Range = 0.02, half-range = 0.01 m, so percentage uncertainty = 0.01 ÷ 1.53 × 100% ≈ 0.7%.
A systematic (zero) error of +2 °C. Subtract it: true reading = 57 − 2 = 55 °C.
Independent: the mass added. Dependent: the length (or extension) of the spring. Control: for example the same spring, or the same ruler, or the same temperature.
The force is directly proportional to the extension (Hooke's law), and the gradient is the spring constant.
m/s = m/s + (m/s²)(s) = m/s + m/s ✓. All terms have units of speed.
Activities for this opening topic: have students measure the same object with a ruler, vernier calipers and a micrometer and compare precision; measure the thickness of a page from a stack; time 20 swings of a pendulum to explore a fair test; ask groups to design an experiment on a simple question (for example, "does the size of a paper parachute affect fall time?"), identify the variables, and critique each other's designs; make a powers-of-ten poster comparing sizes; discuss a scientist from your own region and their contribution. Emphasise units and sensible estimates in every calculation. Numerical values are rounded; please check that they match the data booklet used by your examination board.
This article is original EDUSAMBAM writing. Definitions, constants and historical facts were checked against the sources below. Diagrams are original and were not copied from any source.
Note on the numbers: historical dates are the commonly accepted ones; for some early scientists they are approximate. Please check numerical values against your own syllabus or exam board specification before relying on them.
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