- (A) If , , then prove that : .
- (A) If , , then prove that : .
Proved: from the given equations, and . Squaring both and adding gives (by the fundamental trigonometric identity), which is the required relation. Geometrically, this is the standard Cartesian equation of the ellipse whose parametric form is given, centred at with semi-axes a and b.
Marking Scheme
- 11 mark: rearranging the given equations to and .
- 21 mark: squaring both expressions correctly to get and .
- 31 mark: adding and applying to conclude the left side equals 1 (hence proved).
Hint
Make cos θ and sin θ the subjects: and ; square both, add, and use .
Quick Oral Answer
I rewrite the equations as and , square both and add; the right side becomes which equals , so is proved.
Analysis & Explanation
Eliminate the parameter θ between the two given equations using the Pythagorean identity to reach the required relation.
Concept
- Isolate cos θ and sin θ: and .
- Square both expressions and add; the right side becomes , which the identity collapses to .
- This proves .
Common mistakes
- Squaring before dividing by a and b (must isolate cos θ/sin θ first).
- Squaring only one of the two equations, or treating a and b as trigonometric quantities instead of constants moved to the denominator.
Real-world
- , are the parametric equations of an ellipse centred at with semi-axes a and b; the proved relation is exactly its standard Cartesian equation — the same algebra used to describe planetary orbits.
Common Mistakes
- 1Squaring the equations before dividing by a and b, leaving and tangled with the trig terms instead of cleanly getting and .
- 2Squaring only one of the two equations, or adding without squaring, so the identity cannot be applied.
- 3Writing as something other than 1 (e.g. leaving it unsimplified) and thus not completing the proof.
Interesting Facts
The relation proved, , is the standard equation of an ellipse centred at with semi-axes a and b — so this problem is secretly deriving the ellipse from its parametric form.
Parametric equations like , are how computers and animators trace out smooth curves, and how astronomers describe elliptical planetary orbits following Kepler's first law.
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Frequently Asked Questions
Why must I divide by a and b before squaring?
To isolate the pure trig ratios cos θ and sin θ. Only then does squaring give and , which the identity can simplify. Squaring first would leave and attached and block the identity.
Which identity is used to eliminate θ?
The fundamental Pythagorean identity . Once cos θ and sin θ are squared and added, the right-hand side becomes exactly this and equals 1.
What does the final equation represent?
It is the standard Cartesian equation of an ellipse with centre (h, k) and semi-axes a and b, so the problem effectively converts the parametric form of an ellipse into its Cartesian form.