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Edexcel GCSE Physics

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Notes for Pearson Edexcel GCSE Physics (1PH0, the March 2024 issue of the specification), in folders that follow its topics, with the eight core practicals in the topics they belong to. Higher-tier content is marked where it sits, and each equation has a worked example. Delete any note your tier does not need once the notes are yours.

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Có gì bên trong

  • Key concepts and skills
    • Units, prefixes and standard form6 KB
    • Working scientifically8 KB
  • Motion and forces
    • Scalars, vectors and describing motion5 KB
    • Acceleration and velocity-time graphs6 KB
    • Newton's laws, weight and circular motion9 KB
    • Momentum and collisions6 KB
    • Stopping distances and reaction times6 KB
  • Energy
    • Energy stores and conservation6 KB
    • Dissipation, insulation and efficiency6 KB
    • Work done and power5 KB
    • Energy resources6 KB
  • Waves
    • Wave properties and measuring wave speed8 KB
    • Sound, ultrasound and infrasound6 KB
  • Light and the electromagnetic spectrum
    • Reflection, refraction and total internal reflection8 KB
    • Colour, filters and lenses6 KB
    • The electromagnetic spectrum6 KB
    • Thermal radiation and the Earth's temperature7 KB
  • Radioactivity
    • Atoms, isotopes and the development of the atomic model6 KB
    • Radioactive decay and nuclear equations6 KB
    • Activity and half-life5 KB
    • Background radiation, detection, uses and dangers9 KB
    • Nuclear fission and fusion7 KB
  • Astronomy
    • Gravity, the Solar System and orbits5 KB
    • The origin of the Universe5 KB
    • Stars and observing the Universe5 KB
  • Forces and their effects
    • Forces, vectors and free-body diagrams7 KB
    • Moments, levers and gears5 KB
    • Springs and elastic distortion6 KB
    • Pressure in fluids and upthrust7 KB
  • Electricity and circuits
    • Circuits, current and potential difference5 KB
    • Resistance, series and parallel circuits6 KB
    • Resistors, lamps, diodes, LDRs and thermistors7 KB
    • Energy and power in circuits5 KB
    • Mains electricity and safety5 KB
    • Static electricity and electric fields7 KB
  • Magnetism and electromagnetic induction
    • Magnets and magnetic fields6 KB
    • The motor effect and electric motors5 KB
    • Electromagnetic induction, generators and microphones5 KB
    • Transformers and the National Grid5 KB
  • Particle model
    • Density and states of matter6 KB
    • Specific heat capacity and latent heat7 KB
    • Gas pressure, temperature and volume6 KB

Ghi chú đầu tiên

Key concepts and skills / Units, prefixes and standard form

SI units

Every physical quantity is measured in a unit, and physics uses the International System (SI) so that a value means the same thing everywhere. Six base units are needed at GCSE, and every other unit in the course is built from them.

QuantityUnitSymbol
lengthmetrem
masskilogramkg
timeseconds
electric currentampereA
temperaturekelvinK
amount of substancemolemol

Some combinations of base units are used so often that they have their own name. These are the derived units the course uses.

QuantityUnitSymbolIn base units or other units
energyjouleJN m\mathrm{N\,m}
electric chargecoulombCA s\mathrm{A\,s}
potential differencevoltVJ/C\mathrm{J/C}
resistanceohmΩ\OmegaV/A\mathrm{V/A}
forcenewtonNkg m/s2\mathrm{kg\,m/s^2}
pressurepascalPaN/m2\mathrm{N/m^2}
frequencyhertzHzone wave per second, s−1\mathrm{s^{-1}}
magnetic flux densityteslaTN/(A m)\mathrm{N/(A\,m)}
powerwattWJ/s\mathrm{J/s}

Temperature differences are often given in degrees Celsius, and a change of 1 °C is the same size as a change of 1 K. Units such as m/s\mathrm{m/s} and kg/m3\mathrm{kg/m^3} are compound units, made by dividing one unit by another, and the way they are written tells you how the quantity is built: speed is distance per unit time, and density is mass per unit volume.

A calculation gives a number and a unit together. An answer of 12 with no unit says nothing, and a wrong unit usually means a step has gone wrong, so it is worth checking that the unit of the answer is the one the quantity should have.

Multiples and sub-multiples

Values that are very large or very small are written with a prefix in front of the unit. The prefixes needed are these.

PrefixSymbolMeaningPower of ten
gigaGone thousand million10910^{9}
megaMone million10610^{6}
kilokone thousand10310^{3}
centicone hundredth10−210^{-2}
millimone thousandth10−310^{-3}
microμ\muone millionth10−610^{-6}
nanonone thousand-millionth10−910^{-9}

To convert to the base unit, multiply by the power of ten. A frequency of 2.5 GHz is 2.5×1092.5 \times 10^{9} Hz, and a current of 470 mA is 470×10−3=0.47470 \times 10^{-3} = 0.47 A. To go the other way, divide by the power of ten. An energy of 3,600,000 J is 3 600 000÷106=3.63\,600\,000 \div 10^{6} = 3.6 MJ.

Two conversions cause most of the slips. Areas and volumes use the prefix twice or three times, so a square centimetre is (10−2)2=10−4(10^{-2})^2 = 10^{-4} square metres, and 1 cm3\mathrm{cm^3} is 10−6 m310^{-6}\ \mathrm{m^3}. A block of volume 250 cm3250\ \mathrm{cm^3} is therefore 250×10−6=2.5×10−4 m3250 \times 10^{-6} = 2.5 \times 10^{-4}\ \mathrm{m^3}. The other is time, which is not counted in tens: there are 60 seconds in a minute and 60×60=360060 \times 60 = 3600 seconds in an hour.

Converting between units

Convert by multiplying or dividing by the ratio between the two units, and let the units guide the arrangement so that the one you want to remove cancels.

A vehicle travels at 72 km/h72\ \mathrm{km/h}. There are 1000 m in 1 km and 3600 s in 1 h, so

72 km/h=72×1000 m3600 s=20 m/s 72\ \mathrm{km/h} = \frac{72 \times 1000\ \mathrm{m}}{3600\ \mathrm{s}} = 20\ \mathrm{m/s}

The same method turns hours into seconds. A lesson that lasts 1.5 hours is 1.5×3600=54001.5 \times 3600 = 5400 s, and a 45 minute drive is 45×60=270045 \times 60 = 2700 s. Equations in physics are written for SI units, so a quantity given in kilometres, grams, minutes or millijoules should be converted before it goes into an equation, and the answer then comes out in the SI unit.

The same care applies to rates. A rate compares two quantities, and it can be worked out by proportional reasoning. If a machine transfers 900 J in 15 s, then it transfers 900÷15=60900 \div 15 = 60 J each second, which is 60 W. Ratios are written with no unit when the two quantities have the same unit, as with the efficiency of a device or the magnification of a lens.

Significant figures and standard form

The significant figures of a number are the digits that carry information, counted from the first non-zero digit. So 3,450 has three significant figures if the final zero only shows the place of the digit, 0.0072 has two, and 0.4050 has four. To round to a number of significant figures, look at the digit after the last one you keep. If it is 5 or more, round up.

In a calculation, give the answer to the same number of significant figures as the least precise value used, or one more than that when it is a step on the way to a longer calculation. Rounding a value in the middle of a calculation and using the rounded value causes a small error in the answer, so keep the full calculator value until the end and round once.

Standard form writes a number as A×10nA \times 10^{n}, where AA is at least 1 and less than 10, and nn is a whole number. It is used for very large and very small numbers, since a physicist reads the size of a number from its power of ten.

Ordinary numberStandard form
300,000,0003×1083 \times 10^{8}
0.000 000 55×10−75 \times 10^{-7}
46,0004.6×1044.6 \times 10^{4}
0.00323.2×10−33.2 \times 10^{-3}

Multiplying and dividing in standard form uses the rules of powers. Multiply the numbers, add the powers, and put the answer back into standard form.

(3.0×108)×(2.0×10−3)=6.0×105 (3.0 \times 10^{8}) \times (2.0 \times 10^{-3}) = 6.0 \times 10^{5}
4.8×1061.2×10−2=4.0×108 \frac{4.8 \times 10^{6}}{1.2 \times 10^{-2}} = 4.0 \times 10^{8}

If the number part comes out as 10 or more, or below 1, change the power to fix it. For example (5×104)×(4×103)=20×107=2×108(5 \times 10^{4}) \times (4 \times 10^{3}) = 20 \times 10^{7} = 2 \times 10^{8}.

Orders of magnitude

To estimate, round each value to the nearest power of ten and compare. An atom has a diameter of the order of 10−1010^{-10} m, and a nucleus is of the order of 10−1510^{-15} m across, so the nucleus is about 10510^{5} times smaller than the atom. Answers found this way are given with the approximation symbol ≈\approx or ∼\sim, and the aim is to check that a calculated value is sensible before trusting it: a person walking at 30 m/s, or a car with a mass of 1.2 kg, cannot be right.

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