3.1 Measurements and their errors — revision question pack

3 specification points · notes, questions, answers and worked methods

Checked against AQA 7408 section 3.1. Review basis: the qualification registry sourced from the AQA A-level Physics (7408) specification; registry verification recorded 11 July 2026.

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3.1.1 · Use of SI units and their prefixes

Explanation

  • The required base quantities and SI units are mass in kilograms, length in metres, time in seconds, amount of substance in moles, temperature in kelvin and electric current in amperes; candela is excluded.
  • Derived units combine base units, for example N=kg m s2\text{N}=\text{kg m s}^{-2}.
  • Prefixes required are T\text{T}, G\text{G}, M\text{M}, k\text{k}, c\text{c}, m\text{m}, μ\mu, n\text{n}, p\text{p} and f\text{f}, used with standard form.
  • Conversions also include units of the same quantity, such as joules and electronvolts or kilowatt-hours.
  • Base-quantity definitions and dimensional analysis are not required.
Common SI prefixes step through powers of one thousand around the base unit.

Worked example

Convert an area of 0.36mm20.36\,\text{mm}^2 to square metres.

  1. 1.1mm=103m1\,\text{mm}=10^{-3}\,\text{m}.
  2. 2.Square the whole conversion: 1mm2=106m21\,\text{mm}^2=10^{-6}\,\text{m}^2.
  3. 3.0.36×106=3.6×1070.36\times10^{-6}=3.6\times10^{-7}.

Answer: The area is 3.6 × 10⁻⁷ m².

Common mistakes

  • Don't square a measurement and fail to square its prefix conversion.
  • Don't use grams rather than kilograms as the SI base unit of mass.
  • Don't write a numerical conversion without retaining the physical unit.

Exam tip

Convert every quantity to a consistent unit system before substitution and show each prefix multiplier.

Tier 1 · Easy

  1. Convert 4.7μm4.7\,\mu\text{m} into metres.

    [1 mark]

    Total for this question: 1

  2. Convert 3.2pF3.2\,\text{pF} into farads.

    [1 mark]

    Total for this question: 1

Tier 2 · Standard

  1. A heater transfers 2.4kW h2.4\,\text{kW h} of energy. Calculate this energy in joules. Use 1kW h=3.60×106J1\,\text{kW h}=3.60\times10^6\,\text{J}.

    [2 marks]

    Total for this question: 2

  2. A spring exerts a force of 6.4mN6.4\,\text{mN}. Give this force in SI base units.

    [2 marks]

    Total for this question: 2

  3. The pressure changes by 18Pa18\,\text{Pa} across a 2.5mm2.5\,\text{mm} filter layer. Calculate the pressure gradient in SI base units.

    [3 marks]

    Total for this question: 3

Tier 3 · Hard

  1. A pulse transfers charge 5.4nC5.4\,\text{nC} through a sensor of area 0.36mm20.36\,\text{mm}^2 in 12μs12\,\mu\text{s}. Calculate the mean current density in A m2\text{A m}^{-2}.

    [4 marks]

    Total for this question: 4

  2. A metal has density 7.9g cm37.9\,\text{g cm}^{-3}. Calculate the mass in kilograms of a cube of this metal with side 2.5cm2.5\,\text{cm}.

    [4 marks]

    Total for this question: 4

  3. A detector deposits 2.8GeV2.8\,\text{GeV} of energy uniformly in a volume of 4.5×1017m34.5\times10^{-17}\,\text{m}^3. Calculate the energy per unit volume in SI base units. Use 1eV=1.60×1019J1\,\text{eV}=1.60\times10^{-19}\,\text{J}.

    [4 marks]

    Total for this question: 4

  4. A laser pulse transfers 38mJ38\,\text{mJ} in 0.75ns0.75\,\text{ns} through a circular spot of diameter 42μm42\,\mu\text{m}. Calculate the mean intensity in W m2\text{W m}^{-2} and give its unit in SI base units.

    [5 marks]

    Total for this question: 5

  5. A sensor crystal contains 4.6pC4.6\,\text{pC} of charge per cubic millimetre. Calculate the charge density in C m3\text{C m}^{-3} and SI base units. Calculate the charge in a crystal volume of 0.38cm30.38\,\text{cm}^3.

    [4 marks]

    Total for this question: 4

3.1.2 · Limitation of physical measurements

Explanation

  • Random errors cause scatter and are reduced by repeats and averaging; systematic errors shift results consistently and require correction or removal. Accuracy means closeness to the true value, precision concerns spread, resolution is the smallest detectable change, repeatability keeps method and operator fixed, and reproducibility changes them.
  • Uncertainty may be absolute, fractional or percentage. For addition and subtraction, combine absolute uncertainties; for multiplication and division, combine percentage uncertainties; for a power xnx^n, multiply percentage uncertainty by n|n|.
  • Graph points may carry error bars.
  • Steepest and shallowest acceptable lines give gradient uncertainty, with corresponding intercept limits.
  • Report value and absolute uncertainty to compatible decimal places and significant figures.
Error bars constrain the steepest and shallowest acceptable straight lines.

Worked example

A rectangle measures (4.20±0.05)cm(4.20\pm0.05)\,\text{cm} by (2.10±0.03)cm(2.10\pm0.03)\,\text{cm}. Find its area and uncertainty.

  1. 1.A=4.20(2.10)=8.82cm2A=4.20(2.10)=8.82\,\text{cm}^2.
  2. 2.Percentage uncertainty is 100(0.05/4.20+0.03/2.10)=2.62%100(0.05/4.20+0.03/2.10)=2.62\%.
  3. 3.Absolute uncertainty is 0.0262(8.82)=0.23cm20.0262(8.82)=0.23\,\text{cm}^2.

Answer: The area is (8.8 ± 0.2) cm².

Common mistakes

  • Don't add absolute uncertainties for a multiplication calculation.
  • Don't call a tightly clustered but offset set of readings accurate.
  • Don't quote the measured value to more decimal places than its absolute uncertainty.

Exam tip

State whether each operation needs absolute or percentage uncertainty before combining terms.

Tier 1 · Easy

  1. A diameter is measured as (82.0±0.5)mm(82.0\pm0.5)\,\text{mm}. Calculate its percentage uncertainty.

    [2 marks]

    Total for this question: 2

  2. Repeated measurements of a time are 14.214.2, 14.614.6, 14.314.3 and 14.8s14.8\,\text{s}. Determine the absolute uncertainty using half the range.

    [2 marks]

    Total for this question: 2

Tier 2 · Standard

  1. The sides of a rectangular card are (4.20±0.05)cm(4.20\pm0.05)\,\text{cm} and (2.10±0.03)cm(2.10\pm0.03)\,\text{cm}. Determine its area and absolute uncertainty.

    [3 marks]

    Total for this question: 3

  2. A balance reads 0.15g0.15\,\text{g} when its pan is empty. Identify this error, state its effect on every reading and describe one correction.

    [3 marks]

    Total for this question: 3

  3. A calibrated source has a true temperature of 20.0C20.0\,^\circ\text{C}. Sensor A gives repeated readings 19.819.8, 20.020.0 and 20.2C20.2\,^\circ\text{C}; sensor B gives 21.0C21.0\,^\circ\text{C} each time. Determine which sensor is more precise, which is more accurate, and explain why averaging more readings from sensor B will not correct its error.

    [3 marks]

    Total for this question: 3

Tier 3 · Hard

  1. A pendulum has length (0.842±0.002)m(0.842\pm0.002)\,\text{m}. The time for 2020 oscillations is (36.4±0.2)s(36.4\pm0.2)\,\text{s}. Use g=4π2L/T2g=4\pi^2L/T^2 to calculate gg with its absolute uncertainty.

    [5 marks]

    Total for this question: 5

  2. A graph has best-fit gradient 2.46V A12.46\,\text{V A}^{-1}. The steepest and shallowest acceptable gradients are 2.58V A12.58\,\text{V A}^{-1} and 2.31V A12.31\,\text{V A}^{-1}. Using the larger deviation from the best-fit gradient, determine the gradient with its absolute and percentage uncertainty.

    [4 marks]

    Total for this question: 4

  3. A straight-line graph is described by y=mx+cy=mx+c, where m=(4.80±0.12)V s1m=(4.80\pm0.12)\,\text{V s}^{-1} and c=(1.20±0.06)Vc=(1.20\pm0.06)\,\text{V}. Determine the xx-intercept with its absolute uncertainty, giving the uncertainty to 11 significant figure.

    [4 marks]

    Total for this question: 4

  4. An object distance is (0.420±0.003)m(0.420\pm0.003)\,\text{m} and the corresponding image distance is (0.680±0.004)m(0.680\pm0.004)\,\text{m}. Use f=uvu+vf=\dfrac{uv}{u+v} to determine the focal length with its absolute uncertainty.

    [5 marks]

    Total for this question: 5

  5. A graph has best-fit gradient 1.841.84. The steepest and shallowest acceptable gradients are 1.931.93 and 1.701.70. A constant is calculated from K=4π2/m2K=4\pi^2/m^2, where mm is the gradient. Using the larger gradient deviation, determine KK with its absolute uncertainty. Deduce whether a reference value of 13.813.8 is consistent with the result.

    [5 marks]

    Total for this question: 5

3.1.3 · Estimation of physical quantities

Explanation

  • An order of magnitude is the nearest power of ten. A sound estimate chooses plausible approximate inputs, states assumptions such as representative size, density or operating fraction, and uses relevant physics to derive the requested quantity.
  • Intermediate values usually need only one significant figure.
  • The final numerical estimate is then compared with neighbouring powers of ten: the boundary between 10n10^n and 10n+110^{n+1} is 10×10n3.2×10n\sqrt{10}\times10^n\approx3.2\times10^n.
  • Units and dimensions provide an essential reasonableness check.
  • Estimation is not guessing a remembered number; the awarded reasoning comes from transparent assumptions, a valid physical relationship and a final answer rounded to the nearest order of magnitude.
The nearest-order boundary lies at approximately 3.2 times the lower power of ten.

Worked example

Estimate the order of magnitude of the mass of air in an 8m×6m×3m8\,\text{m}\times6\,\text{m}\times3\,\text{m} room, using air density 1kg m31\,\text{kg m}^{-3}.

  1. 1.Volume is approximately 8(6)(3)=1.4×102m38(6)(3)=1.4\times10^2\,\text{m}^3.
  2. 2.m=ρV1(1.4×102)=1.4×102kgm=\rho V\approx1(1.4\times10^2)=1.4\times10^2\,\text{kg}.
  3. 3.This is nearer 10210^2 than 10310^3.

Answer: The mass has order of magnitude 102kg10^2\,\text{kg}.

Common mistakes

  • Don't report a multi-significant-figure value instead of a power-of-ten order of magnitude.
  • Don't use an assumed value without stating or justifying it.
  • Don't round every coefficient above one to the next power of ten.

Exam tip

Show the assumption, physics relationship and numerical estimate before stating the nearest power of ten.

Tier 1 · Easy

  1. Estimate the order of magnitude of the mass of air in a room measuring 8m×6m×3m8\,\text{m}\times6\,\text{m}\times3\,\text{m}. Take the density of air as 1kg m31\,\text{kg m}^{-3}.

    [1 mark]

    Total for this question: 1

  2. State the nearest power-of-ten order of magnitude of a time interval of 2.6×107s2.6\times10^{-7}\,\text{s}.

    [1 mark]

    Total for this question: 1

Tier 2 · Standard

  1. Estimate the order of magnitude of the number of water molecules in 250cm3250\,\text{cm}^3 of water. Use density 1.0g cm31.0\,\text{g cm}^{-3}, molar mass 18g mol118\,\text{g mol}^{-1} and NA=6.0×1023mol1N_A=6.0\times10^{23}\,\text{mol}^{-1}.

    [3 marks]

    Total for this question: 3

  2. A 5kg5\,\text{kg} bag contains rice grains of average mass 25mg25\,\text{mg}. Estimate how many grains it contains to the nearest order of magnitude.

    [3 marks]

    Total for this question: 3

  3. A storm drops 12mm12\,\text{mm} of rain uniformly over a city of area 25km225\,\text{km}^2. Take the density of water as 1.0×103kg m31.0\times10^3\,\text{kg m}^{-3}. Estimate the mass of rain to the nearest power of ten.

    [4 marks]

    Total for this question: 4

Tier 3 · Hard

  1. Estimate the order of magnitude of the total electrical power drawn by domestic kettles in a country of population 6.8×1076.8\times10^7. Assume 2.52.5 people per household, a 3kW3\,\text{kW} kettle in each household, and that 4%4\% of kettles are operating at one time.

    [5 marks]

    Total for this question: 5

  2. Estimate the order of magnitude of the electrical energy used in one school day by 6060 rooms, each with eight 12W12\,\text{W} lamps operating for 7h7\,\text{h}.

    [5 marks]

    Total for this question: 5

  3. Estimate the number of molecules in Earth's atmosphere to the nearest power of ten. Model Earth as a sphere of radius 6.4×106m6.4\times10^6\,\text{m} with uniform surface pressure 1.0×105Pa1.0\times10^5\,\text{Pa}. Use g=9.81N kg1g=9.81\,\text{N kg}^{-1}, mean atmospheric molar mass 2.9×102kg mol12.9\times10^{-2}\,\text{kg mol}^{-1} and NA=6.02×1023mol1N_A=6.02\times10^{23}\,\text{mol}^{-1}.

    [6 marks]

    Total for this question: 6

  4. Estimate the order of magnitude of the number of electrons passing through a charger during one year. Assume its current is 1.4A1.4\,\text{A} for 2.0h2.0\,\text{h} each day and that the charge magnitude of one electron is 1.60×1019C1.60\times10^{-19}\,\text{C}.

    [5 marks]

    Total for this question: 5

  5. Estimate the order of magnitude of the force that radiation would exert on a planet if all incident radiation were absorbed. Treat the planet as a disc of radius 5.8×106m5.8\times10^6\,\text{m}, take the incident intensity as 7.1×102W m27.1\times10^2\,\text{W m}^{-2} and use F=P/cF=P/c with c=3.00×108m s1c=3.00\times10^8\,\text{m s}^{-1}.

    [5 marks]

    Total for this question: 5

Answer key

Answers begin on a new printed page so the question pack can be completed without the solutions alongside it.

3.1.1 · Use of SI units and their prefixes

Tier 1 · Easy

Mark scheme for 3.1.1 Tier 1 · Easy
QuestionAnswersAdditional comments/GuidelinesMark
01.1
  • 4.7×106m4.7\times10^{-6}\,\text{m}
The prefix μ\mu means 10610^{-6}, so 4.7μm=4.7×106m4.7\,\mu\text{m}=4.7\times10^{-6}\,\text{m}.1
02.1
  • 3.2×1012F3.2\times10^{-12}\,\text{F}
The prefix p\text{p} represents 101210^{-12}, so 3.2pF=3.2×1012F3.2\,\text{pF}=3.2\times10^{-12}\,\text{F}.1

Tier 2 · Standard

Mark scheme for 3.1.1 Tier 2 · Standard
QuestionAnswersAdditional comments/GuidelinesMark
01.1
  • 8.6×106J8.6\times10^6\,\text{J}
Multiply by the stated conversion factor: E=2.4×3.60×106=8.64×106JE=2.4\times3.60\times10^6=8.64\times10^6\,\text{J}. The input 2.42.4 has two significant figures, so E=8.6×106JE=8.6\times10^6\,\text{J}.2
02.1
  • 6.4×103kg m s26.4\times10^{-3}\,\text{kg m s}^{-2}
The prefix m\text{m} means 10310^{-3} and 1N=1kg m s21\,\text{N}=1\,\text{kg m s}^{-2}. Therefore 6.4mN=6.4×103kg m s26.4\,\text{mN}=6.4\times10^{-3}\,\text{kg m s}^{-2}.2
03.1
  • 7.2×103kg m2 s27.2\times10^3\,\text{kg m}^{-2}\text{ s}^{-2}
Convert the distance: 2.5mm=2.5×103m2.5\,\text{mm}=2.5\times10^{-3}\,\text{m}. The gradient is 18/(2.5×103)=7.2×103Pa m118/(2.5\times10^{-3})=7.2\times10^3\,\text{Pa m}^{-1}. Since Pa=kg m1 s2\text{Pa}=\text{kg m}^{-1}\text{ s}^{-2}, the base units are kg m2 s2\text{kg m}^{-2}\text{ s}^{-2}.3

Tier 3 · Hard

Mark scheme for 3.1.1 Tier 3 · Hard
QuestionAnswersAdditional comments/GuidelinesMark
01.1
  • 1.3×103A m21.3\times10^3\,\text{A m}^{-2}
Convert every quantity to SI units: Q=5.4×109CQ=5.4\times10^{-9}\,\text{C}, A=0.36×106=3.6×107m2A=0.36\times10^{-6}=3.6\times10^{-7}\,\text{m}^2 and t=12×106st=12\times10^{-6}\,\text{s}. The current is I=Q/t=(5.4×109)/(12×106)=4.5×104AI=Q/t=(5.4\times10^{-9})/(12\times10^{-6})=4.5\times10^{-4}\,\text{A}. Hence the current density is J=I/A=(4.5×104)/(3.6×107)=1.25×103A m2J=I/A=(4.5\times10^{-4})/(3.6\times10^{-7})=1.25\times10^3\,\text{A m}^{-2}, which to two significant figures is 1.3×103A m21.3\times10^3\,\text{A m}^{-2}.4
02.1
  • 0.12kg0.12\,\text{kg}
The density is 7.9×103kg m37.9\times10^3\,\text{kg m}^{-3} and the side is 2.5×102m2.5\times10^{-2}\,\text{m}. The volume is (2.5×102)3=1.5625×105m3(2.5\times10^{-2})^3=1.5625\times10^{-5}\,\text{m}^3. Hence m=ρV=(7.9×103)(1.5625×105)=0.1234375kgm=\rho V=(7.9\times10^3)(1.5625\times10^{-5})=0.1234375\,\text{kg}, which is 0.12kg0.12\,\text{kg} to two significant figures.4
03.1
  • 1.0×107kg m1 s21.0\times10^7\,\text{kg m}^{-1}\text{ s}^{-2}
The energy is 2.8×109×1.60×1019=4.48×1010J2.8\times10^9\times1.60\times10^{-19}=4.48\times10^{-10}\,\text{J}. Hence the energy per unit volume is (4.48×1010)/(4.5×1017)=9.96×106J m3=1.0×107J m3(4.48\times10^{-10})/(4.5\times10^{-17})=9.96\times10^6\,\text{J m}^{-3}=1.0\times10^7\,\text{J m}^{-3} to two significant figures. Since J=kg m2 s2\text{J}=\text{kg m}^2\text{ s}^{-2}, J m3=kg m1 s2\text{J m}^{-3}=\text{kg m}^{-1}\text{ s}^{-2}.4
04.1
  • 3.7×1016W m2=3.7×1016kg s33.7\times10^{16}\,\text{W m}^{-2}=3.7\times10^{16}\,\text{kg s}^{-3}
Convert the data: E=38×103JE=38\times10^{-3}\,\text{J}, t=0.75×109st=0.75\times10^{-9}\,\text{s} and r=21×106mr=21\times10^{-6}\,\text{m}. The mean power is P=E/t=(38×103)/(0.75×109)=5.0667×107WP=E/t=(38\times10^{-3})/(0.75\times10^{-9})=5.0667\times10^7\,\text{W}. The spot area is A=πr2=π(21×106)2=1.3854×109m2A=\pi r^2=\pi(21\times10^{-6})^2=1.3854\times10^{-9}\,\text{m}^2. Hence I=P/A=(5.0667×107)/(1.3854×109)=3.6571×1016W m2I=P/A=(5.0667\times10^7)/(1.3854\times10^{-9})=3.6571\times10^{16}\,\text{W m}^{-2}, or 3.7×1016W m23.7\times10^{16}\,\text{W m}^{-2} to two significant figures. Since W=kg m2 s3\text{W}=\text{kg m}^2\text{ s}^{-3}, W m2=kg s3\text{W m}^{-2}=\text{kg s}^{-3}.5
05.1
  • 4.6×103C m3=4.6×103A s m34.6\times10^{-3}\,\text{C m}^{-3}=4.6\times10^{-3}\,\text{A s m}^{-3}
  • 1.7×109C1.7\times10^{-9}\,\text{C}
One cubic millimetre is (103m)3=109m3(10^{-3}\,\text{m})^3=10^{-9}\,\text{m}^3, while 4.6pC=4.6×1012C4.6\,\text{pC}=4.6\times10^{-12}\,\text{C}. The charge density is therefore (4.6×1012)/(109)=4.6×103C m3(4.6\times10^{-12})/(10^{-9})=4.6\times10^{-3}\,\text{C m}^{-3}. Since C=A s\text{C}=\text{A s}, its SI base units are A s m3\text{A s m}^{-3}. The volume is 0.38cm3=0.38×106=3.8×107m30.38\,\text{cm}^3=0.38\times10^{-6}=3.8\times10^{-7}\,\text{m}^3, so the charge is (4.6×103)(3.8×107)=1.748×109C(4.6\times10^{-3})(3.8\times10^{-7})=1.748\times10^{-9}\,\text{C}, or 1.7×109C1.7\times10^{-9}\,\text{C} to two significant figures.4

3.1.2 · Limitation of physical measurements

Tier 1 · Easy

Mark scheme for 3.1.2 Tier 1 · Easy
QuestionAnswersAdditional comments/GuidelinesMark
01.1
  • 0.61%0.61\%
Percentage uncertainty is (0.5/82.0)×100=0.6098%(0.5/82.0)\times100=0.6098\%, which is 0.61%0.61\% to two significant figures.2
02.1
  • ±0.3s\pm0.3\,\text{s}
The range is 14.814.2=0.6s14.8-14.2=0.6\,\text{s}. Half the range is 0.6/2=0.3s0.6/2=0.3\,\text{s}, so the absolute uncertainty is ±0.3s\pm0.3\,\text{s}.2

Tier 2 · Standard

Mark scheme for 3.1.2 Tier 2 · Standard
QuestionAnswersAdditional comments/GuidelinesMark
01.1
  • (8.8±0.2)cm2(8.8\pm0.2)\,\text{cm}^2
The area is A=4.20×2.10=8.82cm2A=4.20\times2.10=8.82\,\text{cm}^2. For a product, add percentage uncertainties: (0.05/4.20+0.03/2.10)×100=2.62%(0.05/4.20+0.03/2.10)\times100=2.62\%. The absolute uncertainty is 0.0262×8.82=0.231cm20.0262\times8.82=0.231\,\text{cm}^2. Quoting the uncertainty to one significant figure and the area to the same decimal place gives (8.8±0.2)cm2(8.8\pm0.2)\,\text{cm}^2.3
02.1
  • A systematic zero error makes every reading 0.15g0.15\,\text{g} too large; zero the balance or subtract 0.15g0.15\,\text{g} from each reading.
The offset is repeated with the same sign and size, so it is systematic rather than random. It shifts every measured mass upward by 0.15g0.15\,\text{g}. The error is removed by zeroing the balance before use or correcting each result by subtracting 0.15g0.15\,\text{g}.3
03.1
  • sensor B is more precise; sensor A is more accurate; B has a systematic error that averaging does not remove
Sensor B is more precise because its readings have no observed spread. Sensor A is more accurate because its readings are centred on the true value of 20.0C20.0\,^\circ\text{C}, whereas B is consistently 1.0C1.0\,^\circ\text{C} too high. Sensor B therefore has a systematic offset; repeats and averaging reduce random scatter but do not remove a fixed systematic error.3

Tier 3 · Hard

Mark scheme for 3.1.2 Tier 3 · Hard
QuestionAnswersAdditional comments/GuidelinesMark
01.1
  • (10.0±0.1)N kg1(10.0\pm0.1)\,\text{N kg}^{-1}
One period is T=36.4/20=1.82sT=36.4/20=1.82\,\text{s}; dividing both the value and absolute uncertainty by 2020 leaves its fractional uncertainty equal to 0.2/36.40.2/36.4. The value is g=4π2(0.842)/(1.82)2=10.03N kg1g=4\pi^2(0.842)/(1.82)^2=10.03\,\text{N kg}^{-1}. Because gLT2g\propto LT^{-2}, its percentage uncertainty is (0.002/0.842+2×0.2/36.4)×100=1.34%(0.002/0.842+2\times0.2/36.4)\times100=1.34\%. The absolute uncertainty is 0.0134×10.03=0.134N kg10.0134\times10.03=0.134\,\text{N kg}^{-1}, rounded to 0.1N kg10.1\,\text{N kg}^{-1}, so g=(10.0±0.1)N kg1g=(10.0\pm0.1)\,\text{N kg}^{-1}.5
02.1
  • (2.46±0.15)V A1(2.46\pm0.15)\,\text{V A}^{-1}
  • Percentage uncertainty =6.1%=6.1\%
The deviations from the best gradient are 2.582.46=0.12V A12.58-2.46=0.12\,\text{V A}^{-1} and 2.462.31=0.15V A12.46-2.31=0.15\,\text{V A}^{-1}. Use the larger deviation, so the absolute uncertainty is 0.15V A10.15\,\text{V A}^{-1}. The percentage uncertainty is (0.15/2.46)×100=6.0976%(0.15/2.46)\times100=6.0976\%, which is 6.1%6.1\% to two significant figures. Thus the gradient is (2.46±0.15)V A1(2.46\pm0.15)\,\text{V A}^{-1}.4
03.1
  • (0.25±0.02)s(-0.25\pm0.02)\,\text{s} (accept absolute uncertainty ±0.019\pm0.0190.02s0.02\,\text{s})
At the xx-intercept, 0=mx+c0=mx+c, so x=c/m=1.20/4.80=0.250sx=-c/m=-1.20/4.80=-0.250\,\text{s}. For the division, add fractional uncertainties: 0.06/1.20+0.12/4.80=0.0750.06/1.20+0.12/4.80=0.075, or 7.5%7.5\%. The absolute uncertainty is 0.075(0.250)=0.01875s0.075(0.250)=0.01875\,\text{s}, which rounds to 0.02s0.02\,\text{s}. Quoting the value to the same decimal place gives x=(0.25±0.02)sx=(-0.25\pm0.02)\,\text{s}.4
04.1
  • (0.260±0.002)m(0.260\pm0.002)\,\text{m} (accept an unrounded absolute uncertainty from 0.00170.0017 to 0.0020m0.0020\,\text{m})
Use the independent measured quantities in 1/f=1/u+1/v1/f=1/u+1/v. The focal length is f=[1/0.420+1/0.680]1=0.259636mf=[1/0.420+1/0.680]^{-1}=0.259636\,\text{m}. The reciprocal uncertainties are Δ(1/u)=Δu/u2=0.003/(0.420)2=0.0170m1\Delta(1/u)=\Delta u/u^2=0.003/(0.420)^2=0.0170\,\text{m}^{-1} and Δ(1/v)=Δv/v2=0.004/(0.680)2=0.00865m1\Delta(1/v)=\Delta v/v^2=0.004/(0.680)^2=0.00865\,\text{m}^{-1}. Hence Δ(1/f)=0.0170+0.00865=0.02566m1\Delta(1/f)=0.0170+0.00865=0.02566\,\text{m}^{-1}, which is 0.666%0.666\% of 1/f1/f. Therefore Δf=f2Δ(1/f)=(0.259636)2(0.02566)=0.00173m\Delta f=f^2\Delta(1/f)=(0.259636)^2(0.02566)=0.00173\,\text{m}. Quoting the uncertainty and value compatibly gives (0.260±0.002)m(0.260\pm0.002)\,\text{m}.5
05.1
  • K=11.7±1.8K=11.7\pm1.8 (accept unrounded uncertainty 1.771.77 or a consistently rounded equivalent); 13.813.8 is not consistent
The gradient deviations are 1.931.84=0.091.93-1.84=0.09 and 1.841.70=0.141.84-1.70=0.14, so use Δm=0.14\Delta m=0.14. The value is K=4π2/(1.84)2=11.6607K=4\pi^2/(1.84)^2=11.6607. Because Km2K\propto m^{-2}, its percentage uncertainty is 2(0.14/1.84)×100=15.217%2(0.14/1.84)\times100=15.217\%. Thus ΔK=0.15217(11.6607)=1.7745\Delta K=0.15217(11.6607)=1.7745, giving K=11.7±1.8K=11.7\pm1.8. The corresponding interval is approximately 9.99.9 to 13.413.4, which does not include 13.813.8, so the reference value is not consistent with this uncertainty range.5

3.1.3 · Estimation of physical quantities

Tier 1 · Easy

Mark scheme for 3.1.3 Tier 1 · Easy
QuestionAnswersAdditional comments/GuidelinesMark
01.1
  • 102kg10^2\,\text{kg}
The room volume is about 8×6×3=144m38\times6\times3=144\,\text{m}^3. Its air mass is therefore about 1×144=1.44×102kg1\times144=1.44\times10^2\,\text{kg}, whose nearest order of magnitude is 102kg10^2\,\text{kg}.1
02.1
  • 107s10^{-7}\,\text{s}
2.6×107s2.6\times10^{-7}\,\text{s} lies below the geometric boundary 10×107=3.162×107s\sqrt{10}\times10^{-7}=3.162\times10^{-7}\,\text{s}, so it is nearer 107s10^{-7}\,\text{s} than 106s10^{-6}\,\text{s}.1

Tier 2 · Standard

Mark scheme for 3.1.3 Tier 2 · Standard
QuestionAnswersAdditional comments/GuidelinesMark
01.1
  • 102510^{25} molecules
The water mass is about 250×1.0=250g250\times1.0=250\,\text{g}. The amount is 250/1814mol250/18\approx14\,\text{mol}, so the number of molecules is about 14×6.0×1023=8.4×102414\times6.0\times10^{23}=8.4\times10^{24}. This is nearer 102510^{25} than 102410^{24}, so the order of magnitude is 102510^{25} molecules.3
02.1
  • 10510^5 grains
One grain has mass 25mg=2.5×105kg25\,\text{mg}=2.5\times10^{-5}\,\text{kg}. The estimated number is 5/(2.5×105)=2×1055/(2.5\times10^{-5})=2\times10^5. This is nearer 10510^5 than 10610^6, so the order of magnitude is 10510^5 grains.3
03.1
  • 108kg10^8\,\text{kg}
The area is 25(103m)2=2.5×107m225(10^3\,\text{m})^2=2.5\times10^7\,\text{m}^2 and the depth is 1.2×102m1.2\times10^{-2}\,\text{m}. The water volume is (2.5×107)(1.2×102)=3.0×105m3(2.5\times10^7)(1.2\times10^{-2})=3.0\times10^5\,\text{m}^3. Its mass is (1.0×103)(3.0×105)=3.0×108kg(1.0\times10^3)(3.0\times10^5)=3.0\times10^8\,\text{kg}. The boundary is about 3.2×108kg3.2\times10^8\,\text{kg} (10×108kg\sqrt{10}\times10^8\,\text{kg}), so the nearest order of magnitude is 108kg10^8\,\text{kg}.4

Tier 3 · Hard

Mark scheme for 3.1.3 Tier 3 · Hard
QuestionAnswersAdditional comments/GuidelinesMark
01.1
  • 1010W10^{10}\,\text{W}
The number of households is approximately (6.8×107)/2.5=2.72×107(6.8\times10^7)/2.5=2.72\times10^7. The number of kettles operating is 0.04×2.72×107=1.09×1060.04\times2.72\times10^7=1.09\times10^6. Their total power is (1.09×106)(3×103)=3.26×109W(1.09\times10^6)(3\times10^3)=3.26\times10^9\,\text{W}. Since this is just above 3.2×109W3.2\times10^9\,\text{W}, the nearest order of magnitude is 1010W10^{10}\,\text{W}.5
02.1
  • 108J10^8\,\text{J}
There are 60×8=48060\times8=480 lamps, so their total power is 480×12=5760W480\times12=5760\,\text{W}. The operating time is 7×3600=25200s7\times3600=25200\,\text{s}. The energy is approximately 5760×25200=1.45152×108J5760\times25200=1.45152\times10^8\,\text{J}, whose nearest order of magnitude is 108J10^8\,\text{J}.5
03.1
  • 104410^{44} molecules
Earth's surface area is 4πR2=4π(6.4×106)2=5.15×1014m24\pi R^2=4\pi(6.4\times10^6)^2=5.15\times10^{14}\,\text{m}^2. Pressure times area gives the atmosphere's weight: W=pA=(1.0×105)(5.15×1014)=5.15×1019NW=pA=(1.0\times10^5)(5.15\times10^{14})=5.15\times10^{19}\,\text{N}. Its mass is m=W/g=5.25×1018kgm=W/g=5.25\times10^{18}\,\text{kg}, giving n=m/M=(5.25×1018)/(2.9×102)=1.81×1020moln=m/M=(5.25\times10^{18})/(2.9\times10^{-2})=1.81\times10^{20}\,\text{mol}. The number of molecules is nNA=(1.81×1020)(6.02×1023)=1.09×1044nN_A=(1.81\times10^{20})(6.02\times10^{23})=1.09\times10^{44}, whose nearest order of magnitude is 104410^{44} molecules.6
04.1
  • 102510^{25} electrons
The operating time is 2.0×3600×365=2.628×106s2.0\times3600\times365=2.628\times10^6\,\text{s}. The charge transferred is Q=It=1.4(2.628×106)=3.6792×106CQ=It=1.4(2.628\times10^6)=3.6792\times10^6\,\text{C}. The number of electrons is N=Q/e=(3.6792×106)/(1.60×1019)=2.2995×1025N=Q/e=(3.6792\times10^6)/(1.60\times10^{-19})=2.2995\times10^{25}. This is below the boundary 10×1025=3.162×1025\sqrt{10}\times10^{25}=3.162\times10^{25}, so its nearest order of magnitude is 102510^{25} electrons.5
05.1
  • 108N10^8\,\text{N}
The planet intercepts radiation over the disc area A=πR2=π(5.8×106)2=1.057×1014m2A=\pi R^2=\pi(5.8\times10^6)^2=1.057\times10^{14}\,\text{m}^2, not over its whole spherical surface. The intercepted power is P=IA=(7.1×102)(1.057×1014)=7.50×1016WP=IA=(7.1\times10^2)(1.057\times10^{14})=7.50\times10^{16}\,\text{W}. For complete absorption, F=P/c=(7.50×1016)/(3.00×108)=2.50×108NF=P/c=(7.50\times10^{16})/(3.00\times10^8)=2.50\times10^8\,\text{N}. This lies below 10×108N\sqrt{10}\times10^8\,\text{N} and is therefore nearer 108N10^8\,\text{N} than 109N10^9\,\text{N}.5