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This lesson covers the small angle approximations for sin θ, cos θ, and tan θ when θ is small and measured in radians. These approximations simplify expressions and are used in limit calculations, mechanics, and numerical analysis. They are part of the AQA A-Level Mathematics specification 7357.
When θ is small and measured in radians:
sin θ ≈ θ
cos θ ≈ 1 − θ²/2
tan θ ≈ θ
These approximations become more accurate as θ gets closer to zero, and they are exact in the limit as θ → 0.
Crucially, θ must be in radians. The approximations do not work with degrees.
Consider the unit circle. For a small angle θ (in radians), the arc length subtended is θ (since s = rθ = 1 × θ), and the opposite side of the triangle (which equals sin θ) is approximately equal to the arc length for small angles. As the angle shrinks, the chord and the arc become indistinguishable.
More formally, from the Maclaurin series (Taylor series at 0):
sin θ = θ − θ³/3! + θ⁵/5! − ...
For small θ, the higher-order terms (θ³, θ⁵, ...) are negligibly small, so sin θ ≈ θ.
From the Maclaurin series:
cos θ = 1 − θ²/2! + θ⁴/4! − ...
For small θ, the terms from θ⁴ onwards are negligible, so cos θ ≈ 1 − θ²/2.
Alternatively, using cos θ = 1 − 2sin²(θ/2) and the approximation sin(θ/2) ≈ θ/2:
cos θ ≈ 1 − 2(θ/2)² = 1 − θ²/2
Since tan θ = sin θ / cos θ, and for small θ:
tan θ ≈ θ / (1 − θ²/2) ≈ θ × (1 + θ²/2 + ...) ≈ θ
The error term is of order θ³, just as for sin θ.
From the Maclaurin series:
tan θ = θ + θ³/3 + 2θ⁵/15 + ...
For small θ, tan θ ≈ θ.
Let us check the approximations for θ = 0.1 radians (about 5.7°):
| Function | Exact Value | Approximation | Error |
|---|---|---|---|
| sin(0.1) | 0.0998334... | 0.1 | 0.0001666... |
| cos(0.1) | 0.9950042... | 1 − 0.005 = 0.995 | 0.0000042... |
| tan(0.1) | 0.1003347... | 0.1 | 0.0003347... |
The approximations are very accurate for small angles. For θ = 0.01 radians, the errors would be even smaller (roughly 1000 times smaller).
For θ = 0.5 radians (about 28.6°):
| Function | Exact Value | Approximation | Error |
|---|---|---|---|
| sin(0.5) | 0.4794... | 0.5 | 0.0206... |
| cos(0.5) | 0.8776... | 1 − 0.125 = 0.875 | 0.0026... |
| tan(0.5) | 0.5463... | 0.5 | 0.0463... |
The errors are larger but the approximations are still reasonable. As a rule of thumb, the approximations are good for θ ≲ 0.2 radians and become progressively worse beyond that.
Example 1: Use small angle approximations to estimate (sin 3θ)/(2θ) when θ is small.
sin 3θ ≈ 3θ (since 3θ is also small when θ is small)
(sin 3θ)/(2θ) ≈ 3θ/(2θ) = 3/2
Example 2: Simplify (1 − cos θ)/θ² for small θ.
cos θ ≈ 1 − θ²/2
1 − cos θ ≈ θ²/2
(1 − cos θ)/θ² ≈ (θ²/2)/θ² = 1/2
Example 3: Simplify (tan 2θ − sin 2θ)/θ³ for small θ.
tan 2θ ≈ 2θ
sin 2θ ≈ 2θ
This gives (2θ − 2θ)/θ³ = 0/θ³ = 0, but this is not accurate enough — we need to keep more terms.
Using better approximations:
tan 2θ ≈ 2θ + (2θ)³/3 = 2θ + 8θ³/3
sin 2θ ≈ 2θ − (2θ)³/6 = 2θ − 8θ³/6 = 2θ − 4θ³/3
Therefore:
tan 2θ − sin 2θ ≈ (2θ + 8θ³/3) − (2θ − 4θ³/3) = 8θ³/3 + 4θ³/3 = 12θ³/3 = 4θ³
(tan 2θ − sin 2θ)/θ³ ≈ 4θ³/θ³ = 4
Example 4: Given that θ is small, find an approximate expression for (3θ + sin θ)/(2 − cos θ) as a linear expression in θ.
Numerator: 3θ + sin θ ≈ 3θ + θ = 4θ
Denominator: 2 − cos θ ≈ 2 − (1 − θ²/2) = 1 + θ²/2
For small θ, θ² is negligible compared to 1, so denominator ≈ 1.
(3θ + sin θ)/(2 − cos θ) ≈ 4θ/1 = 4θ
Example 5: Show that for small θ, (1 − cos 2θ)/(sin θ tan θ) ≈ 2.
1 − cos 2θ ≈ 1 − (1 − (2θ)²/2) = 1 − 1 + 2θ² = 2θ²
sin θ ≈ θ
tan θ ≈ θ
sin θ tan θ ≈ θ × θ = θ²
(1 − cos 2θ)/(sin θ tan θ) ≈ 2θ²/θ² = 2 ∎
The small angle approximations are directly connected to important limits:
lim(θ→0) sin θ / θ = 1
lim(θ→0) (1 − cos θ) / θ² = 1/2
lim(θ→0) tan θ / θ = 1
These limits are fundamental in proving the derivatives of sin x and cos x from first principles.
Example 6: Using the small angle approximation, explain why d/dx(sin x) = cos x.
From first principles:
d/dx(sin x) = lim(h→0) [sin(x + h) − sin x] / h
= lim(h→0) [sin x cos h + cos x sin h − sin x] / h
= lim(h→0) [sin x(cos h − 1) + cos x sin h] / h
= sin x × lim(h→0)(cos h − 1)/h + cos x × lim(h→0)(sin h)/h
Using small angle approximations:
cos h − 1 ≈ −h²/2, so (cos h − 1)/h ≈ −h/2 → 0
sin h ≈ h, so sin h / h ≈ 1
Therefore:
d/dx(sin x) = sin x × 0 + cos x × 1 = cos x
Problem 1: When θ is small, find approximate expressions for:
(a) (sin 5θ)/(3θ)
≈ 5θ/(3θ) = 5/3
(b) (1 − cos 4θ)/(8θ²)
cos 4θ ≈ 1 − (4θ)²/2 = 1 − 8θ²
1 − cos 4θ ≈ 8θ²
(1 − cos 4θ)/(8θ²) ≈ 8θ²/(8θ²) = 1
(c) (θ + tan θ)/(sin 2θ)
≈ (θ + θ)/(2θ) = 2θ/(2θ) = 1
Problem 2: The expression (2 − 2cos θ + sin²θ)/(4θ²) is approximately equal to k when θ is small. Find the value of k.
2 − 2cos θ ≈ 2 − 2(1 − θ²/2) = 2 − 2 + θ² = θ²
sin²θ ≈ θ²
(θ² + θ²)/(4θ²) = 2θ²/(4θ²) = 1/2
So k = 1/2.
Exam Tip: Small angle approximations are quick to apply but you must state clearly that you are using them (e.g., "Using the small angle approximation sin θ ≈ θ..."). In the exam, you may be asked to find the value of an expression correct to a certain order — make sure you include enough terms of the approximation. Always work in radians. If a question says "θ is small", this is your cue to use small angle approximations.
AQA 7357 specification, Paper 2 — Pure Mathematics, Section E (Trigonometry), Year 2 sub-strand E5 covers the standard small-angle approximations of sine, cosine and tangent: sinθ≈θ, cosθ≈1−21θ2, tanθ≈θ (where θ is in radians) (refer to the official specification document for exact wording). This is examined synoptically across 7357/2 (Pure Paper 2), often inside limits, differentiation-from-first-principles questions, and modelling contexts. The AQA formula booklet does not list these approximations — they must be memorised, along with the radian-only restriction. Examiners exploit the radian condition heavily: a candidate who slips into degrees mid-calculation cannot recover.
Question (8 marks):
(a) Using the small-angle approximations for sinx and tanx, evaluate
limx→0x3sin3x−tan3x
stating the order of accuracy required at each stage. (6)
(b) Hence explain why the approximation tanθ≈θ is insufficient when computing this limit, and state which extra term in the Taylor expansion of tanθ is required. (2)
Solution with mark scheme:
(a) Step 1 — recognise the order of accuracy required.
The denominator is x3, so any approximation truncated at lower order than x3 will lose information. We need expansions of sin3x and tan3x accurate to at least order x3.
M1 (AO3.1a) — identifying that the cubic denominator forces a cubic-order numerator expansion.
Step 2 — expand sin3x to cubic order.
Using sinθ≈θ−61θ3 (the standard approximation extended one further term, from the Maclaurin series), with θ=3x:
sin3x≈3x−6(3x)3=3x−627x3=3x−29x3
M1 — correct expansion to cubic order with θ=3x substituted before cubing.
Step 3 — expand tan3x to cubic order.
Using tanθ≈θ+31θ3 (Maclaurin extension), with θ=3x:
tan3x≈3x+3(3x)3=3x+327x3=3x+9x3
M1 — correct cubic-order expansion of tan3x. Common error: candidates use the bare tanθ≈θ from the formula sheet and obtain numerator 0, giving the indeterminate form 0/0 they cannot resolve.
Step 4 — subtract.
sin3x−tan3x≈(3x−29x3)−(3x+9x3)=−29x3−9x3=−227x3
A1 — the linear 3x terms cancel exactly, leaving a clean cubic-order numerator. The cancellation is the entire point of needing higher-order terms.
Step 5 — divide and take the limit.
x3sin3x−tan3x≈x3−27x3/2=−227
As x→0 the higher-order error terms (of order x5 and beyond) vanish, so:
limx→0x3sin3x−tan3x=−227
A1 — final exact answer.
B1 — explicit comment that the omitted terms are O(x5) and contribute 0 in the limit.
(b) Step 1 — diagnose the failure mode.
If only tanθ≈θ is used, then sin3x−tan3x≈−29x3−0=−29x3, which would give the (incorrect) limit −29. The cubic term +31θ3 in the Maclaurin expansion of tanθ is the missing ingredient — it is the same order as the −61θ3 term from sinθ, so dropping it changes the numerator by a factor that is not negligible.
B1 — identifying 31θ3 as the required extra term.
B1 — correct explanation that this term is the same order of magnitude as the cubic term from sinθ, so cannot be ignored.
Total: 8 marks (M3 A2 B3, split as shown).
Question (6 marks): A pendulum of length L swings under gravity. Its equation of motion for small displacement angle θ (in radians) is
θ¨=−Lgsinθ
(a) Using a small-angle approximation, show that for small θ this reduces to
θ¨≈−Lgθ
stating clearly the approximation used and the constraint on θ. (2)
(b) Given that this linearised equation has solution θ(t)=Acos(ωt+ϕ) for some constants, deduce ω and hence the period T. (3)
(c) Estimate the maximum amplitude (in radians) for which the linearised model is accurate to within 1%, using the next term of the expansion. (1)
Mark scheme decomposition by AO:
(a)
(b)
(c)
Total: 6 marks split AO1 = 3, AO2 = 2, AO3 = 1. This is the textbook synoptic mechanics-pure crossover that AQA favours in Year 2: small-angle approximation is the bridge between the (insoluble) nonlinear pendulum and the (tractable) simple harmonic motion model.
Small-angle approximations sit at a junction of several A-Level threads:
Section E — Differentiation of sinx from first principles. The proof that dxdsinx=cosx uses limh→0hsinh=1 (equivalent to sinh≈h) and limh→0hcosh−1=0 (equivalent to cosh≈1−21h2). Without small-angle results, the derivative cannot be derived; with them, it is two lines.
Section E — Maclaurin / Taylor series (Further Maths context). The small-angle approximations are the first non-zero terms of the Maclaurin expansions sinθ=θ−6θ3+120θ5−… and cosθ=1−2θ2+24θ4−…. AS-Level treats them as memorised facts; Further Maths derives them. Recognising the connection lifts a procedural skill into a structural one.
Mechanics (Paper 3) — pendulum and SHM. As shown in the specimen, small-angle linearisation converts the nonlinear pendulum equation into the SHM equation θ¨=−ω2θ with period T≈2πL/g. Every "estimate the period of a pendulum" question rests silently on sinθ≈θ.
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