Parametric, polar and vector functions Knowledge-Based Study

Math · Calculus · Math · Calculus BC Topics

Math topic explanations on Parametric, polar and vector functions.

Study notes

  1. Parametric Equations

    A planar curve can often be represented parametrically by expressing both coordinates as functions of an independent parameter, typically denoted as tt:

    x=f(t),y=g(t)x = f(t), \quad y = g(t)

    Derivatives and Tangent Lines

    To analyze the slope of the tangent line to a parametric curve, apply the chain rule. If xx and yy are differentiable functions of tt and dxdt≠0\frac{dx}{dt} \neq 0, the first derivative is:

    dydx=dydtdxdt\frac{dy}{dx} = \frac{\frac{dy}{dt}}{\frac{dx}{dt}}

    The second derivative measures concavity and is computed by differentiating dydx\frac{dy}{dx} with respect to tt, then dividing by dxdt\frac{dx}{dt}:

    d2ydx2=ddx(dydx)=ddt(dydx)dxdt\frac{d^2y}{dx^2} = \frac{d}{dx}\left(\frac{dy}{dx}\right) = \frac{\frac{d}{dt}\left(\frac{dy}{dx}\right)}{\frac{dx}{dt}}

    Arc Length

    The arc length LL of a smooth curve traversed exactly once from t=at = a to t=bt = b is given by the definite integral:

    L=∫ab(dxdt)2+(dydt)2 dtL = \int_{a}^{b} \sqrt{\left(\frac{dx}{dt}\right)^2 + \left(\frac{dy}{dt}\right)^2}\, dt

    Vector-Valued Functions

    Motion in a two-dimensional plane is naturally described using a position vector r⃗(t)\vec{r}(t):

    r⃗(t)=⟨x(t),y(t)angle=x(t)i^+y(t)j^\vec{r}(t) = \langle x(t), y(t) angle = x(t)\hat{\mathbf{i}} + y(t)\hat{\mathbf{j}}

    Velocity, Speed, and Acceleration

    Differentiating the position vector with respect to time yields the velocity vector, speed scalar, and acceleration vector:

    • Velocity vector: v⃗(t)=r⃗′(t)=⟨x′(t),y′(t)angle\vec{v}(t) = \vec{r}'(t) = \langle x'(t), y'(t) angle
    • Speed: ∥v⃗(t)∥=(x′(t))2+(y′(t))2\|\vec{v}(t)\| = \sqrt{(x'(t))^2 + (y'(t))^2}
    • Acceleration vector: a⃗(t)=v⃗′(t)=r⃗′′(t)=⟨x′′(t),y′′(t)angle\vec{a}(t) = \vec{v}'(t) = \vec{r}''(t) = \langle x''(t), y''(t) angle

    Total Distance Traveled

    The total distance traveled by an object along its path from t=t1t = t_1 to t=t2t = t_2 equals the integral of its speed over the given interval:

    Total Distance=∫t1t2∥v⃗(t)∥ dt=∫t1t2(x′(t))2+(y′(t))2 dt\text{Total Distance} = \int_{t_1}^{t_2} \|\vec{v}(t)\|\, dt = \int_{t_1}^{t_2} \sqrt{(x'(t))^2 + (y'(t))^2}\, dt

    Notice that this formulation is identical to the arc length of the parametric path traced by the particle.

    Polar Coordinate Foundations

    In the polar coordinate system, points are represented as (r,θ)(r, \theta), where rr is the directed distance from the origin (pole) and θ\theta is the angle measured counterclockwise from the positive xx-axis (polar axis). The relationships connecting rectangular and polar coordinates are:

    x=rcos⁡θ,y=rsin⁡θ,r2=x2+y2,tan⁡θ=yxx = r\cos\theta, \quad y = r\sin\theta, \quad r^2 = x^2 + y^2, \quad \tan\theta = \frac{y}{x}

    Slopes of Polar Curves

    Given a polar equation r=f(θ)r = f(\theta), the curve can be treated as a set of parametric equations with parameter θ\theta:

    x(θ)=f(θ)cos⁡θ,y(θ)=f(θ)sin⁡θx(\theta) = f(\theta)\cos\theta, \quad y(\theta) = f(\theta)\sin\theta

    Applying the product rule yields:

    dxdθ=drdθcos⁡θ−rsin⁡θ\frac{dx}{d\theta} = \frac{dr}{d\theta}\cos\theta - r\sin\theta

    dydθ=drdθsin⁡θ+rcos⁡θ\frac{dy}{d\theta} = \frac{dr}{d\theta}\sin\theta + r\cos\theta

    The slope of the tangent line in rectangular coordinates is:

    dydx=dydθdxdθ=drdθsin⁡θ+rcos⁡θdrdθcos⁡θ−rsin⁡θ\frac{dy}{dx} = \frac{\frac{dy}{d\theta}}{\frac{dx}{d\theta}} = \frac{\frac{dr}{d\theta}\sin\theta + r\cos\theta}{\frac{dr}{d\theta}\cos\theta - r\sin\theta}

    A critical distinction exists between drdθ\frac{dr}{d\theta} and dydx\frac{dy}{dx}: drdθ\frac{dr}{d\theta} represents the rate of change of the distance from the origin with respect to θ\theta, whereas dydx\frac{dy}{dx} is the geometric slope of the tangent line in the xyxy-plane.

    Area Enclosed by Polar Curves

    The area of an infinitesimal polar sector of radius rr subtended by an angle dθd\theta is 12r2 dθ\frac{1}{2}r^2\, d\theta. Consequently, the area bounded by a continuous curve r=f(θ)r = f(\theta) and radial rays θ=α\theta = \alpha and θ=β\theta = \beta (where β−α≤2π\beta - \alpha \leq 2\pi) is given by:

    A=12∫αβ[f(θ)]2 dθ=12∫αβr2 dθA = \frac{1}{2}\int_{\alpha}^{\beta} [f(\theta)]^2\, d\theta = \frac{1}{2}\int_{\alpha}^{\beta} r^2\, d\theta

    Area Between Two Polar Curves

    When computing the area of a region bounded between an outer curve r2=f2(θ)r_2 = f_2(\theta) and an inner curve r1=f1(θ)r_1 = f_1(\theta) where r2≥r1≥0r_2 \geq r_1 \geq 0 over [α,β][\alpha, \beta], subtract the inner sector areas from the outer sector areas:

    A=12∫αβ([r2(θ)]2−[r1(θ)]2) dθA = \frac{1}{2}\int_{\alpha}^{\beta} \left( [r_2(\theta)]^2 - [r_1(\theta)]^2 \right)\, d\theta

    Polar Arc Length

    By substituting x=rcos⁡θx = r\cos\theta and y=rsin⁡θy = r\sin\theta into the parametric arc length formula and simplifying with trigonometric identities, the arc length of a polar curve from θ=α\theta = \alpha to θ=β\theta = \beta becomes:

    L=∫αβr2+(drdθ)2 dθL = \int_{\alpha}^{\beta} \sqrt{r^2 + \left(\frac{dr}{d\theta}\right)^2}\, d\theta