Absolute & Relative Errors

Every measurement made in physics carries some degree of uncertainty. No matter how precise our instruments are, there will always be a small difference between the measured value and the true value of a quantity. This difference is called a measurement error, and understanding how to quantify and express it is one of the most fundamental skills in experimental physics. There are two primary ways to express the size of a measurement error: as an absolute error and as a relative (or fractional) error. The absolute error tells you the magnitude of the difference between the measured and true values, expressed in the same units as the measurement itself. The relative error expresses this same difference as a proportion or percentage of the true value, making it dimensionless and far more useful for comparing the quality of different measurements. For example, an absolute error of 2 cm might seem large when measuring the diameter of a coin (true value ~2 cm, so the error is 100% of the measurement) but negligible when measuring the length of a football field (true value ~100 m). The relative error immediately reveals this difference in quality: 100% versus 0.002%. Mastering both concepts allows physicists to evaluate experimental precision, compare results from different experiments, and correctly propagate uncertainties through calculations.

Key takeaways
  • The True Value and Measured Value
  • Defining Absolute Error
  • Defining Relative Error
  • Why Relative Error is More Informative
  • Propagation of Errors in Calculations

The True Value and Measured Value

In any measurement, we define the true value x0x_0 as the actual, accepted value of the quantity being measured. The measured value xx is what our instrument records. In practice, the true value is often taken to be the mean of many repeated measurements. The discrepancy between these two values is the starting point for all error analysis.

Defining Absolute Error

The absolute error Δx\Delta x is simply the magnitude of the difference between the measured value and the true value: \Delta x = |x - x_0|. It has the same units as the measured quantity. When you take multiple measurements x1,x2,…,xnx_1, x_2, \ldots, x_n, the best estimate of the true value is the arithmetic mean xˉ=1n∑i=1nxi\bar{x} = \frac{1}{n}\sum_{i=1}^{n} x_i, and the absolute error for each reading is Δxi=∣xi−xˉ∣\Delta x_i = |x_i - \bar{x}|. The mean absolute error is then Δx‾=1n∑i=1n∣xi−xˉ∣\overline{\Delta x} = \frac{1}{n}\sum_{i=1}^{n}|x_i - \bar{x}|. This is also called the mean deviation. The final result is reported as x=xˉ±Δx‾x = \bar{x} \pm \overline{\Delta x}, meaning the true value almost certainly lies within this range.

Defining Relative Error

The relative error (also called fractional error) is defined as the ratio of the absolute error to the true (or mean) value: \varepsilon = \frac{\Delta x}{\bar{x}}. Since the units cancel, ε\varepsilon is dimensionless. It is often expressed as a percentage by multiplying by 100, giving the percentage error: ε%=Δxxˉ×100%\varepsilon_{\%} = \frac{\Delta x}{\bar{x}} \times 100\%. A small relative error means the measurement is highly precise relative to the size of the quantity being measured. This makes relative error the most useful tool for comparing the quality of measurements of different physical quantities.

Why Relative Error is More Informative

Consider two measurements: (A) a length of 5.0±0.15.0 \pm 0.1 m and (B) a length of 0.050±0.0010.050 \pm 0.001 m. The absolute errors are 0.1 m and 0.001 m respectively — measurement B has a smaller absolute error. However, the relative errors are: (A) 0.1/5.0=2%0.1/5.0 = 2\% and (B) 0.001/0.050=2%0.001/0.050 = 2\%. Both measurements have the same relative precision! Relative error strips away the scale of the measurement and reveals the true quality of the experimental technique.

Propagation of Errors in Calculations

When a result ZZ is calculated from measured quantities, errors combine according to specific rules. For addition or subtraction (Z=A±BZ = A \pm B), absolute errors add: ΔZ=ΔA+ΔB\Delta Z = \Delta A + \Delta B. For multiplication or division (Z=A×BZ = A \times B or Z=A/BZ = A/B), relative errors add: ΔZZ=ΔAA+ΔBB\frac{\Delta Z}{Z} = \frac{\Delta A}{A} + \frac{\Delta B}{B}. For a power law (Z=AnZ = A^n), the relative error is multiplied by the exponent: ΔZZ=∣n∣ΔAA\frac{\Delta Z}{Z} = |n| \frac{\Delta A}{A}. These rules follow from calculus (total differential) and are essential for any quantitative experimental work.

The Key Equation

ε%=Δx‾xˉ×100%\varepsilon_{\%} = \frac{\overline{\Delta x}}{\bar{x}} \times 100\%
  • \varepsilon_{\%} — Percentage error (dimensionless (percent)): The relative error expressed as a percentage; indicates how large the error is compared to the measured value.
  • \overline{\Delta x} — Mean absolute error (same as measured quantity): The average of the absolute deviations of each individual measurement from the mean value.
  • \bar{x} — Mean value (same as measured quantity): The arithmetic mean of all repeated measurements; serves as the best estimate of the true value.

Worked Example

Problem. A student measures the diameter of a steel ball five times and records the following values: 4.21 cm, 4.19 cm, 4.23 cm, 4.20 cm, and 4.22 cm. Calculate (a) the mean value, (b) the mean absolute error, (c) the relative error, and (d) the percentage error. Express the final result in the standard form xˉ±Δx‾\bar{x} \pm \overline{\Delta x}.

d=(4.21±0.01) cm,ε%≈0.3%d = (4.21 \pm 0.01) \text{ cm}, \quad \varepsilon_{\%} \approx 0.3\%

Answer. Mean = 4.21 cm; Mean absolute error = 0.01 cm; Relative error ≈ 0.003; Percentage error ≈ 0.3%; Final result: d = 4.21 ± 0.01 cm.

Figure
Diagram
Absolute vs Relative Error: Number Line VisualisationTrue value x₀Measured xΔx (absolute error)Comparison: Same Δx, Different Relative ErrorsΔx = 2 cmΔx = 2 cmMeasuring coin diameter: x₀ = 2 cmMeasuring field length: x₀ = 100 m = 10000 cmRelative error (coin): 2/2 = 100% ← very poor!Relative error (field): 2/10000 = 0.02% ← excellent!
Origins · 1 minCarl Friedrich Gauss and how this was discovered
CF
Carl Friedrich Gauss
1777–1855 · German

Gauss developed the method of least squares (1795, published 1809) and the theory of Gaussian (normal) error distribution, which provides the mathematical foundation for understanding random measurement errors. His work showed that random errors in repeated measurements follow a bell-shaped distribution, and that the arithmetic mean is the best estimate of the true value — concepts central to all modern error analysis. Gauss reportedly discovered the method of least squares at the age of 18, but did not publish it for over a decade. When the French mathematician Legendre published the same method in 1805, it sparked a priority dispute that Gauss won by showing letters proving his earlier discovery.

  • Random and Systematic Errors — Absolute and relative errors arise from two distinct sources — random fluctuations and systematic biases. Understanding the difference is essential for reducing measurement uncertainty.
  • Significant Figures and Precision — The number of significant figures used to express a measurement is directly related to its absolute error; proper use of significant figures ensures that reported precision matches actual measurement quality.
  • Propagation of Errors in Calculations — When derived quantities are calculated from measurements, absolute and relative errors must be combined using propagation rules — a direct application of the concepts introduced here.
  • Physical Quantities and SI Units — Absolute error is expressed in the units of the measured quantity, so a solid understanding of SI units is necessary to correctly interpret and report absolute errors.