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Ultimate Guide to Vector Equations of Curves and Spheres

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    Vu Hung
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Introduction

We have seen how vector equations can describe perfectly straight lines using r=a+λb\mathbf{r} = \mathbf{a} + \lambda\mathbf{b}. But the physical world is rarely straight. How do we describe the circular orbit of a satellite, or a complex 3D spiral, using vectors? In HSC Mathematics Extension 2, we extend our vector knowledge to describe Parametric Curves, Circles, and Spheres.

Executive Summary

This guide covers curved vector geometry:

  • Parametric Curves: Expressing curves as r(t)=(x(t)y(t))\mathbf{r}(t) = \begin{pmatrix} x(t) \\ y(t) \end{pmatrix}.
  • Circles in 2D: Deriving and using the vector equation rc=R|\mathbf{r} - \mathbf{c}| = R.
  • Spheres in 3D: Extending the circle equation to describe a 3D sphere.
  • Cartesian Conversion: Converting vector curve equations back into standard y=f(x)y=f(x) Cartesian algebra.

What is this about?

When defining a straight line, the parameter λ\lambda multiplied a constant direction vector. To define a curve, the components of the position vector themselves must change according to a parameter (often tt for time or θ\theta for angle).

Furthermore, the geometric definition of a circle is "the set of all points that are a fixed distance from a centre point". Because vectors are incredibly good at describing distances (using the magnitude/absolute value signs v|\mathbf{v}|), the vector equation of a circle perfectly translates this English definition into mathematics. This exact same logic extends flawlessly into 3-dimensional spheres.

Main Content

1. Vector Equations of Circles

Let c\mathbf{c} be the position vector of the centre of a circle, and RR be its radius. Let r\mathbf{r} be the position vector of any point on the circumference of the circle.

The vector pointing from the centre to the edge is rc\mathbf{r} - \mathbf{c}. Because every point on the edge is exactly distance RR away from the centre, the magnitude of this vector must be RR.

Therefore, the vector equation of a circle is: rc=R|\mathbf{r} - \mathbf{c}| = R

If the circle is centred at the origin (0,0)(0,0), then c=0\mathbf{c} = \mathbf{0}, and the equation simplifies to: r=R|\mathbf{r}| = R

Alternatively, using parametric equations with angle θ\theta, a circle at the origin can be written as: r(θ)=(RcosθRsinθ)\mathbf{r}(\theta) = \begin{pmatrix} R\cos\theta \\ R\sin\theta \end{pmatrix}

2. Vector Equations of Spheres

One of the most beautiful aspects of vector mathematics is how easily it scales to higher dimensions. The geometric definition of a sphere in 3D space is identical to a circle: "the set of all points in 3D space a fixed distance from a centre point".

Therefore, if r\mathbf{r} is a 3D vector (xyz)\begin{pmatrix} x\\y\\z \end{pmatrix} and c\mathbf{c} is a 3D centre (c1c2c3)\begin{pmatrix} c_1\\c_2\\c_3 \end{pmatrix}, the equation of the sphere is exactly the same! rc=R|\mathbf{r} - \mathbf{c}| = R

3. Parametric Curves and Cartesian Conversion

A curve can be defined generally as r(t)=x(t)i+y(t)j\mathbf{r}(t) = x(t)\mathbf{i} + y(t)\mathbf{j}. To find the Cartesian equation (an equation with only xx and yy, no tt), you must:

  1. Write the two parametric equations: x=x(t)x = x(t) and y=y(t)y = y(t).
  2. Use algebra (or trigonometric identities) to eliminate the parameter tt.

Example: Find the Cartesian equation for the curve r(t)=(2tt21)\mathbf{r}(t) = \begin{pmatrix} 2t \\ t^2 - 1 \end{pmatrix}.

  1. x=2t    t=x2x = 2t \implies t = \frac{x}{2}
  2. y=t21y = t^2 - 1 Substitute (1) into (2): y=(x2)21y = \left(\frac{x}{2}\right)^2 - 1 y=x241y = \frac{x^2}{4} - 1 (This is a parabola!)

Simple Worked Example

Question: A sphere has the vector equation rc=5|\mathbf{r} - \mathbf{c}| = 5, where c=(213)\mathbf{c} = \begin{pmatrix} 2 \\ -1 \\ 3 \end{pmatrix}. Find the Cartesian equation of this sphere.

Solution: Step 1: Set up the vector expression inside the magnitude. Let r=(xyz)\mathbf{r} = \begin{pmatrix} x \\ y \\ z \end{pmatrix}. rc=(xyz)(213)=(x2y+1z3)\mathbf{r} - \mathbf{c} = \begin{pmatrix} x \\ y \\ z \end{pmatrix} - \begin{pmatrix} 2 \\ -1 \\ 3 \end{pmatrix} = \begin{pmatrix} x - 2 \\ y + 1 \\ z - 3 \end{pmatrix}

Step 2: Apply the magnitude formula. The magnitude of a 3D vector (abc)\begin{pmatrix} a\\b\\c \end{pmatrix} is a2+b2+c2\sqrt{a^2 + b^2 + c^2}. rc=(x2)2+(y+1)2+(z3)2|\mathbf{r} - \mathbf{c}| = \sqrt{(x - 2)^2 + (y + 1)^2 + (z - 3)^2}

Step 3: Equate to the radius and square both sides. We are given that the magnitude equals 55. (x2)2+(y+1)2+(z3)2=5\sqrt{(x - 2)^2 + (y + 1)^2 + (z - 3)^2} = 5 Square both sides: (x2)2+(y+1)2+(z3)2=25(x - 2)^2 + (y + 1)^2 + (z - 3)^2 = 25

Final Answer: The Cartesian equation of the sphere is (x2)2+(y+1)2+(z3)2=25(x - 2)^2 + (y + 1)^2 + (z - 3)^2 = 25.

mini-FAQ page

Q: If rc=R|\mathbf{r} - \mathbf{c}| = R is the equation for both a circle and a sphere, how do I know which one it is? A: You look at the dimension of the vectors r\mathbf{r} and c\mathbf{c}. If they have two components (xy)\begin{pmatrix} x\\y \end{pmatrix}, it is a 2D circle. If they have three components (xyz)\begin{pmatrix} x\\y\\z \end{pmatrix}, it is a 3D sphere. The context of the question will always specify the dimension.

Q: How do I eliminate tt if the vector is r(θ)=(3cosθ3sinθ)\mathbf{r}(\theta) = \begin{pmatrix} 3\cos\theta \\ 3\sin\theta \end{pmatrix}? A: You use the Pythagorean identity! x=3cosθ    x3=cosθ    x29=cos2θx = 3\cos\theta \implies \frac{x}{3} = \cos\theta \implies \frac{x^2}{9} = \cos^2\theta y=3sinθ    y3=sinθ    y29=sin2θy = 3\sin\theta \implies \frac{y}{3} = \sin\theta \implies \frac{y^2}{9} = \sin^2\theta Add them together: x29+y29=cos2θ+sin2θ=1\frac{x^2}{9} + \frac{y^2}{9} = \cos^2\theta + \sin^2\theta = 1. x2+y2=9x^2 + y^2 = 9 (A circle of radius 3).

Common mistakes to avoid

  • Forgetting to square the radius: When converting rc=R|\mathbf{r} - \mathbf{c}| = R to Cartesian, the right-hand side of the Cartesian equation becomes R2R^2, not RR. In the example above, the radius was 5, but the Cartesian equation equals 25.
  • Messing up the signs: The vector equation uses rc\mathbf{r} - \mathbf{c}. If the centre is (2,1,3)(2, -1, 3), the vector is r(213)\mathbf{r} - \begin{pmatrix} 2 \\ -1 \\ 3 \end{pmatrix}. This creates a (y(1))(y - (-1)) which becomes (y+1)(y+1) in the Cartesian bracket. Watch your negative signs carefully!

Practice on Vu's Maths Hub

Converting between vector parameters and Cartesian curves is a common exam trick.

Further Readings

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