A vector-valued function packs a pair of parametric equations into one object: a vector whose tip traces the curve as t t t changes. The good news is that the calculus is no harder than what you already know. You differentiate and integrate one component at a time . This notation is the language of motion in the plane, which comes next in motion with vectors .
A vector in the plane has two components, written with angle brackets: ⟨ 3 , − 2 ⟩ \langle 3, -2 \rangle ⟨ 3 , − 2 ⟩ means “3 right, 2 down”. A vector-valued function assigns a vector to each t t t :
r ⃗ ( t ) = ⟨ x ( t ) , y ( t ) ⟩ \vec{r}(t) = \langle x(t),\ y(t) \rangle r ( t ) = ⟨ x ( t ) , y ( t )⟩
You’ll also see it written r ⃗ ( t ) = x ( t ) i + y ( t ) j \vec{r}(t) = x(t)\,\mathbf{i} + y(t)\,\mathbf{j} r ( t ) = x ( t ) i + y ( t ) j , or with a bold r ( t ) \mathbf{r}(t) r ( t ) . They all mean the same thing. AP questions usually use the angle-bracket form, so we’ll use ⟨ , ⟩ \langle\ ,\ \rangle ⟨ , ⟩ for components and r ⃗ ( t ) \vec{r}(t) r ( t ) for the function’s name.
Think of r ⃗ ( t ) \vec{r}(t) r ( t ) as an arrow from the origin to the point ( x ( t ) , y ( t ) ) (x(t), y(t)) ( x ( t ) , y ( t )) . As t t t changes, the arrow’s tip traces the same curve as the parametric equations x = x ( t ) x = x(t) x = x ( t ) , y = y ( t ) y = y(t) y = y ( t ) .
r ⃗ ′ ( t ) = ⟨ x ′ ( t ) , y ′ ( t ) ⟩ , r ⃗ ′ ′ ( t ) = ⟨ x ′ ′ ( t ) , y ′ ′ ( t ) ⟩ \vec{r}\,'(t) = \langle x'(t),\ y'(t) \rangle, \qquad \vec{r}\,''(t) = \langle x''(t),\ y''(t) \rangle r ′ ( t ) = ⟨ x ′ ( t ) , y ′ ( t )⟩ , r ′′ ( t ) = ⟨ x ′′ ( t ) , y ′′ ( t )⟩
All the usual rules (power, product, chain, and so on) apply to each component separately.
What r ⃗ ′ ( t ) \vec{r}\,'(t) r ′ ( t ) means. Drawn starting at the point ( x ( t ) , y ( t ) ) (x(t), y(t)) ( x ( t ) , y ( t )) , the vector r ⃗ ′ ( t ) \vec{r}\,'(t) r ′ ( t ) is tangent to the curve and points in the direction of increasing t t t . Its slope is y ′ ( t ) x ′ ( t ) \dfrac{y'(t)}{x'(t)} x ′ ( t ) y ′ ( t ) , which is the same d y d x \dfrac{dy}{dx} d x d y you found for parametric curves .
The ellipse traced by r(t) = <3 cos t, 2 sin t>, counterclockwise. The position vector r(pi/3) points from the origin to (3/2, root 3), and the derivative r'(pi/3) = <-3 root 3 / 2, 1> starts there, tangent to the ellipse.
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For r ⃗ ( t ) = ⟨ 3 cos t , 2 sin t ⟩ \vec{r}(t) = \langle 3\cos t, 2\sin t \rangle r ( t ) = ⟨ 3 cos t , 2 sin t ⟩ (Example 2): the position vector r ⃗ ( π 3 ) \vec{r}\left( \frac{\pi}{3} \right) r ( 3 π ) and the tangent vector r ⃗ ′ ( π 3 ) \vec{r}\,'\left( \frac{\pi}{3} \right) r ′ ( 3 π ) .
∫ r ⃗ ( t ) d t = ⟨ ∫ x ( t ) d t , ∫ y ( t ) d t ⟩ \int \vec{r}(t)\, dt = \left\langle \int x(t)\, dt,\ \int y(t)\, dt \right\rangle ∫ r ( t ) d t = ⟨ ∫ x ( t ) d t , ∫ y ( t ) d t ⟩
An indefinite integral gets a constant in each component. You can write them as a constant vector: + C ⃗ +\ \vec{C} + C , where C ⃗ = ⟨ C 1 , C 2 ⟩ \vec{C} = \langle C_1, C_2 \rangle C = ⟨ C 1 , C 2 ⟩ .
A definite integral gives a vector of numbers:
∫ a b r ⃗ ′ ( t ) d t = r ⃗ ( b ) − r ⃗ ( a ) \int_a^b \vec{r}\,'(t)\, dt = \vec{r}(b) - \vec{r}(a) ∫ a b r ′ ( t ) d t = r ( b ) − r ( a )
This is the Fundamental Theorem of Calculus, applied to each component. It’s the net change in r ⃗ \vec{r} r .
If you know r ⃗ ′ ( t ) \vec{r}\,'(t) r ′ ( t ) and one value such as r ⃗ ( 0 ) \vec{r}(0) r ( 0 ) , you can find r ⃗ ( t ) \vec{r}(t) r ( t ) : integrate each component, then use the initial condition to find each constant. Equivalently,
r ⃗ ( t ) = r ⃗ ( 0 ) + ∫ 0 t r ⃗ ′ ( u ) d u \vec{r}(t) = \vec{r}(0) + \int_0^t \vec{r}\,'(u)\, du r ( t ) = r ( 0 ) + ∫ 0 t r ′ ( u ) d u
Trig functions on this page use radians , as all AP calculus does.
Let r ⃗ ( t ) = ⟨ t 3 − 2 t , e 2 t ⟩ \vec{r}(t) = \langle t^3 - 2t,\ e^{2t} \rangle r ( t ) = ⟨ t 3 − 2 t , e 2 t ⟩ . Find r ⃗ ′ ( t ) \vec{r}\,'(t) r ′ ( t ) , r ⃗ ′ ′ ( t ) \vec{r}\,''(t) r ′′ ( t ) and r ⃗ ′ ( 0 ) \vec{r}\,'(0) r ′ ( 0 ) .
Solution. Differentiate each component:
r ⃗ ′ ( t ) = ⟨ 3 t 2 − 2 , 2 e 2 t ⟩ , r ⃗ ′ ′ ( t ) = ⟨ 6 t , 4 e 2 t ⟩ \vec{r}\,'(t) = \langle 3t^2 - 2,\ 2e^{2t} \rangle, \qquad \vec{r}\,''(t) = \langle 6t,\ 4e^{2t} \rangle r ′ ( t ) = ⟨ 3 t 2 − 2 , 2 e 2 t ⟩ , r ′′ ( t ) = ⟨ 6 t , 4 e 2 t ⟩
r ⃗ ′ ( 0 ) = ⟨ 0 − 2 , 2 e 0 ⟩ = ⟨ − 2 , 2 ⟩ \vec{r}\,'(0) = \langle 0 - 2,\ 2e^0 \rangle = \langle -2, 2 \rangle r ′ ( 0 ) = ⟨ 0 − 2 , 2 e 0 ⟩ = ⟨ − 2 , 2 ⟩
Let r ⃗ ( t ) = ⟨ 3 cos t , 2 sin t ⟩ \vec{r}(t) = \langle 3\cos t,\ 2\sin t \rangle r ( t ) = ⟨ 3 cos t , 2 sin t ⟩ . Find r ⃗ ( π 3 ) \vec{r}\left( \dfrac{\pi}{3} \right) r ( 3 π ) , r ⃗ ′ ( π 3 ) \vec{r}\,'\left( \dfrac{\pi}{3} \right) r ′ ( 3 π ) , and the slope of the tangent line at t = π 3 t = \dfrac{\pi}{3} t = 3 π .
Solution. Using cos π 3 = 1 2 \cos\dfrac{\pi}{3} = \dfrac{1}{2} cos 3 π = 2 1 and sin π 3 = 3 2 \sin\dfrac{\pi}{3} = \dfrac{\sqrt{3}}{2} sin 3 π = 2 3 :
r ⃗ ( π 3 ) = ⟨ 3 2 , 3 ⟩ \vec{r}\left( \frac{\pi}{3} \right) = \left\langle \frac{3}{2},\ \sqrt{3} \right\rangle r ( 3 π ) = ⟨ 2 3 , 3 ⟩
r ⃗ ′ ( t ) = ⟨ − 3 sin t , 2 cos t ⟩ , r ⃗ ′ ( π 3 ) = ⟨ − 3 3 2 , 1 ⟩ \vec{r}\,'(t) = \langle -3\sin t,\ 2\cos t \rangle, \qquad \vec{r}\,'\left( \frac{\pi}{3} \right) = \left\langle -\frac{3\sqrt{3}}{2},\ 1 \right\rangle r ′ ( t ) = ⟨ − 3 sin t , 2 cos t ⟩ , r ′ ( 3 π ) = ⟨ − 2 3 3 , 1 ⟩
The slope of the tangent line is
y ′ x ′ = 1 − 3 3 / 2 = − 2 3 3 = − 2 3 9 \frac{y'}{x'} = \frac{1}{-3\sqrt{3}/2} = -\frac{2}{3\sqrt{3}} = -\frac{2\sqrt{3}}{9} x ′ y ′ = − 3 3 /2 1 = − 3 3 2 = − 9 2 3
The figure above shows this: at ( 3 2 , 3 ) \left( \tfrac{3}{2}, \sqrt{3} \right) ( 2 3 , 3 ) the tangent vector points up and to the left, because the ellipse is traced counterclockwise.
Given r ⃗ ′ ( t ) = ⟨ 6 t 2 , 1 t + 1 ⟩ \vec{r}\,'(t) = \left\langle 6t^2,\ \dfrac{1}{t + 1} \right\rangle r ′ ( t ) = ⟨ 6 t 2 , t + 1 1 ⟩ for t > − 1 t \gt -1 t > − 1 and r ⃗ ( 0 ) = ⟨ 1 , − 3 ⟩ \vec{r}(0) = \langle 1, -3 \rangle r ( 0 ) = ⟨ 1 , − 3 ⟩ , find r ⃗ ( t ) \vec{r}(t) r ( t ) .
Solution. Integrate each component:
r ⃗ ( t ) = ⟨ 2 t 3 + C 1 , ln ( t + 1 ) + C 2 ⟩ \vec{r}(t) = \big\langle 2t^3 + C_1,\ \ln(t + 1) + C_2 \big\rangle r ( t ) = ⟨ 2 t 3 + C 1 , ln ( t + 1 ) + C 2 ⟩
(No absolute value is needed, since t + 1 > 0 t + 1 \gt 0 t + 1 > 0 .) Use r ⃗ ( 0 ) = ⟨ 1 , − 3 ⟩ \vec{r}(0) = \langle 1, -3 \rangle r ( 0 ) = ⟨ 1 , − 3 ⟩ :
0 + C 1 = 1 ⇒ C 1 = 1 , ln 1 + C 2 = − 3 ⇒ C 2 = − 3 0 + C_1 = 1 \ \Rightarrow\ C_1 = 1, \qquad \ln 1 + C_2 = -3 \ \Rightarrow\ C_2 = -3 0 + C 1 = 1 ⇒ C 1 = 1 , ln 1 + C 2 = − 3 ⇒ C 2 = − 3
r ⃗ ( t ) = ⟨ 2 t 3 + 1 , ln ( t + 1 ) − 3 ⟩ \vec{r}(t) = \big\langle 2t^3 + 1,\ \ln(t + 1) - 3 \big\rangle r ( t ) = ⟨ 2 t 3 + 1 , ln ( t + 1 ) − 3 ⟩
Check: r ⃗ ( 0 ) = ⟨ 1 , 0 − 3 ⟩ = ⟨ 1 , − 3 ⟩ \vec{r}(0) = \langle 1, 0 - 3 \rangle = \langle 1, -3 \rangle r ( 0 ) = ⟨ 1 , 0 − 3 ⟩ = ⟨ 1 , − 3 ⟩ .
Evaluate ∫ 0 π ⟨ sin t , 2 t ⟩ d t \displaystyle\int_0^{\pi} \langle \sin t,\ 2t \rangle\, dt ∫ 0 π ⟨ sin t , 2 t ⟩ d t . If r ⃗ ′ ( t ) = ⟨ sin t , 2 t ⟩ \vec{r}\,'(t) = \langle \sin t,\ 2t \rangle r ′ ( t ) = ⟨ sin t , 2 t ⟩ and r ⃗ ( 0 ) = ⟨ 1 , 0 ⟩ \vec{r}(0) = \langle 1, 0 \rangle r ( 0 ) = ⟨ 1 , 0 ⟩ , find r ⃗ ( π ) \vec{r}(\pi) r ( π ) .
Solution.
∫ 0 π ⟨ sin t , 2 t ⟩ d t = ⟨ [ − cos t ] 0 π , [ t 2 ] 0 π ⟩ = ⟨ 1 + 1 , π 2 ⟩ = ⟨ 2 , π 2 ⟩ \int_0^{\pi} \langle \sin t,\ 2t \rangle\, dt = \left\langle \Big[ -\cos t \Big]_0^{\pi},\ \Big[ t^2 \Big]_0^{\pi} \right\rangle = \langle 1 + 1,\ \pi^2 \rangle = \langle 2,\ \pi^2 \rangle ∫ 0 π ⟨ sin t , 2 t ⟩ d t = ⟨ [ − cos t ] 0 π , [ t 2 ] 0 π ⟩ = ⟨ 1 + 1 , π 2 ⟩ = ⟨ 2 , π 2 ⟩
This is the net change r ⃗ ( π ) − r ⃗ ( 0 ) \vec{r}(\pi) - \vec{r}(0) r ( π ) − r ( 0 ) , so
r ⃗ ( π ) = ⟨ 1 , 0 ⟩ + ⟨ 2 , π 2 ⟩ = ⟨ 3 , π 2 ⟩ \vec{r}(\pi) = \langle 1, 0 \rangle + \langle 2, \pi^2 \rangle = \langle 3,\ \pi^2 \rangle r ( π ) = ⟨ 1 , 0 ⟩ + ⟨ 2 , π 2 ⟩ = ⟨ 3 , π 2 ⟩
Only one constant of integration. Each component gets its own constant. Writing ⟨ 2 t 3 , ln ( t + 1 ) ⟩ + C \langle 2t^3, \ln(t + 1) \rangle + C ⟨ 2 t 3 , ln ( t + 1 )⟩ + C with a single number C C C added to both is wrong unless C C C is a vector ⟨ C 1 , C 2 ⟩ \langle C_1, C_2 \rangle ⟨ C 1 , C 2 ⟩ .
Treating the vector as a single number. You can’t “multiply out” or divide the components by each other. r ⃗ ′ ( t ) \vec{r}\,'(t) r ′ ( t ) is a vector; the slope y ′ x ′ \dfrac{y'}{x'} x ′ y ′ is a number. Make sure your answer has the form the question asks for.
Forgetting the initial position. ∫ 0 t r ⃗ ′ ( u ) d u \int_0^t \vec{r}\,'(u)\, du ∫ 0 t r ′ ( u ) d u is the change in r ⃗ \vec{r} r , not r ⃗ ( t ) \vec{r}(t) r ( t ) itself. Add r ⃗ ( 0 ) \vec{r}(0) r ( 0 ) .
Mixing up the components. Keep x x x first and y y y second all the way through. A swapped answer like ⟨ π 2 , 2 ⟩ \langle \pi^2, 2 \rangle ⟨ π 2 , 2 ⟩ in Example 4 is a different vector.
Drawing the tangent vector from the origin. The position vector starts at the origin. The derivative r ⃗ ′ ( t ) \vec{r}\,'(t) r ′ ( t ) is drawn starting at the point on the curve, where it shows the direction of motion.
1. (Warm-up) Let r ⃗ ( t ) = ⟨ t 2 , 5 t − 1 ⟩ \vec{r}(t) = \langle t^2,\ 5t - 1 \rangle r ( t ) = ⟨ t 2 , 5 t − 1 ⟩ . Find r ⃗ ′ ( t ) \vec{r}\,'(t) r ′ ( t ) and r ⃗ ′ ( 2 ) \vec{r}\,'(2) r ′ ( 2 ) .
Solution r ⃗ ′ ( t ) = ⟨ 2 t , 5 ⟩ , r ⃗ ′ ( 2 ) = ⟨ 4 , 5 ⟩ \vec{r}\,'(t) = \langle 2t,\ 5 \rangle, \qquad \vec{r}\,'(2) = \langle 4,\ 5 \rangle r ′ ( t ) = ⟨ 2 t , 5 ⟩ , r ′ ( 2 ) = ⟨ 4 , 5 ⟩
2. (Warm-up) Find ∫ ⟨ 2 t , 3 ⟩ d t \displaystyle\int \langle 2t,\ 3 \rangle\, dt ∫ ⟨ 2 t , 3 ⟩ d t .
Solution ∫ ⟨ 2 t , 3 ⟩ d t = ⟨ t 2 + C 1 , 3 t + C 2 ⟩ \int \langle 2t,\ 3 \rangle\, dt = \langle t^2 + C_1,\ 3t + C_2 \rangle ∫ ⟨ 2 t , 3 ⟩ d t = ⟨ t 2 + C 1 , 3 t + C 2 ⟩
3. (Warm-up) Let r ⃗ ( t ) = ⟨ e t , ln t ⟩ \vec{r}(t) = \langle e^t,\ \ln t \rangle r ( t ) = ⟨ e t , ln t ⟩ for t > 0 t \gt 0 t > 0 . Find r ⃗ ′ ′ ( t ) \vec{r}\,''(t) r ′′ ( t ) .
Solution r ⃗ ′ ( t ) = ⟨ e t , 1 t ⟩ , r ⃗ ′ ′ ( t ) = ⟨ e t , − 1 t 2 ⟩ \vec{r}\,'(t) = \left\langle e^t,\ \frac{1}{t} \right\rangle, \qquad \vec{r}\,''(t) = \left\langle e^t,\ -\frac{1}{t^2} \right\rangle r ′ ( t ) = ⟨ e t , t 1 ⟩ , r ′′ ( t ) = ⟨ e t , − t 2 1 ⟩
4. (Core) Let r ⃗ ( t ) = ⟨ t 2 − 1 , t 3 − t ⟩ \vec{r}(t) = \langle t^2 - 1,\ t^3 - t \rangle r ( t ) = ⟨ t 2 − 1 , t 3 − t ⟩ . Find r ⃗ ′ ( t ) \vec{r}\,'(t) r ′ ( t ) , and the equation of the tangent line to the curve at t = 2 t = 2 t = 2 .
Solution r ⃗ ′ ( t ) = ⟨ 2 t , 3 t 2 − 1 ⟩ \vec{r}\,'(t) = \langle 2t,\ 3t^2 - 1 \rangle r ′ ( t ) = ⟨ 2 t , 3 t 2 − 1 ⟩ , so r ⃗ ′ ( 2 ) = ⟨ 4 , 11 ⟩ \vec{r}\,'(2) = \langle 4, 11 \rangle r ′ ( 2 ) = ⟨ 4 , 11 ⟩ and the slope is 11 4 \dfrac{11}{4} 4 11 .
The point is r ⃗ ( 2 ) = ⟨ 3 , 6 ⟩ \vec{r}(2) = \langle 3, 6 \rangle r ( 2 ) = ⟨ 3 , 6 ⟩ . Tangent line:
y − 6 = 11 4 ( x − 3 ) y - 6 = \frac{11}{4}(x - 3) y − 6 = 4 11 ( x − 3 )
5. (Core) Given r ⃗ ′ ( t ) = ⟨ cos t , − 2 sin ( 2 t ) ⟩ \vec{r}\,'(t) = \langle \cos t,\ -2\sin(2t) \rangle r ′ ( t ) = ⟨ cos t , − 2 sin ( 2 t )⟩ and r ⃗ ( 0 ) = ⟨ 3 , 1 ⟩ \vec{r}(0) = \langle 3, 1 \rangle r ( 0 ) = ⟨ 3 , 1 ⟩ , find r ⃗ ( t ) \vec{r}(t) r ( t ) and r ⃗ ( π 2 ) \vec{r}\left( \dfrac{\pi}{2} \right) r ( 2 π ) .
Solution r ⃗ ( t ) = ⟨ sin t + C 1 , cos ( 2 t ) + C 2 ⟩ \vec{r}(t) = \langle \sin t + C_1,\ \cos(2t) + C_2 \rangle r ( t ) = ⟨ sin t + C 1 , cos ( 2 t ) + C 2 ⟩ At t = 0 t = 0 t = 0 : 0 + C 1 = 3 0 + C_1 = 3 0 + C 1 = 3 and 1 + C 2 = 1 1 + C_2 = 1 1 + C 2 = 1 , so C 1 = 3 C_1 = 3 C 1 = 3 and C 2 = 0 C_2 = 0 C 2 = 0 .
r ⃗ ( t ) = ⟨ 3 + sin t , cos ( 2 t ) ⟩ , r ⃗ ( π 2 ) = ⟨ 3 + 1 , cos π ⟩ = ⟨ 4 , − 1 ⟩ \vec{r}(t) = \langle 3 + \sin t,\ \cos(2t) \rangle, \qquad \vec{r}\left( \frac{\pi}{2} \right) = \langle 3 + 1,\ \cos\pi \rangle = \langle 4,\ -1 \rangle r ( t ) = ⟨ 3 + sin t , cos ( 2 t )⟩ , r ( 2 π ) = ⟨ 3 + 1 , cos π ⟩ = ⟨ 4 , − 1 ⟩
6. (Core) Evaluate ∫ 1 4 ⟨ t , 1 t ⟩ d t \displaystyle\int_1^4 \left\langle \sqrt{t},\ \frac{1}{t} \right\rangle dt ∫ 1 4 ⟨ t , t 1 ⟩ d t .
Solution ⟨ [ 2 3 t 3 / 2 ] 1 4 , [ ln t ] 1 4 ⟩ = ⟨ 2 3 ( 8 − 1 ) , ln 4 ⟩ = ⟨ 14 3 , ln 4 ⟩ \left\langle \left[ \frac{2}{3}t^{3/2} \right]_1^4,\ \Big[ \ln t \Big]_1^4 \right\rangle = \left\langle \frac{2}{3}(8 - 1),\ \ln 4 \right\rangle = \left\langle \frac{14}{3},\ \ln 4 \right\rangle ⟨ [ 3 2 t 3/2 ] 1 4 , [ ln t ] 1 4 ⟩ = ⟨ 3 2 ( 8 − 1 ) , ln 4 ⟩ = ⟨ 3 14 , ln 4 ⟩
7. (Core) A ball is thrown from a point 2 2 2 m above the ground. Its acceleration is r ⃗ ′ ′ ( t ) = ⟨ 0 , − 9.8 ⟩ \vec{r}\,''(t) = \langle 0, -9.8 \rangle r ′′ ( t ) = ⟨ 0 , − 9.8 ⟩ m/s², its initial velocity is r ⃗ ′ ( 0 ) = ⟨ 20 , 15 ⟩ \vec{r}\,'(0) = \langle 20, 15 \rangle r ′ ( 0 ) = ⟨ 20 , 15 ⟩ m/s, and r ⃗ ( 0 ) = ⟨ 0 , 2 ⟩ \vec{r}(0) = \langle 0, 2 \rangle r ( 0 ) = ⟨ 0 , 2 ⟩ (in metres, with x x x horizontal and y y y the height). Find r ⃗ ( t ) \vec{r}(t) r ( t ) , and the height of the ball when it is 30 30 30 m away horizontally.
Solution Integrate once and use r ⃗ ′ ( 0 ) \vec{r}\,'(0) r ′ ( 0 ) :
r ⃗ ′ ( t ) = ⟨ 0 + C 1 , − 9.8 t + C 2 ⟩ = ⟨ 20 , 15 − 9.8 t ⟩ \vec{r}\,'(t) = \langle 0 + C_1,\ -9.8t + C_2 \rangle = \langle 20,\ 15 - 9.8t \rangle r ′ ( t ) = ⟨ 0 + C 1 , − 9.8 t + C 2 ⟩ = ⟨ 20 , 15 − 9.8 t ⟩ Integrate again and use r ⃗ ( 0 ) \vec{r}(0) r ( 0 ) :
r ⃗ ( t ) = ⟨ 20 t , 2 + 15 t − 4.9 t 2 ⟩ \vec{r}(t) = \langle 20t,\ 2 + 15t - 4.9t^2 \rangle r ( t ) = ⟨ 20 t , 2 + 15 t − 4.9 t 2 ⟩ x = 30 x = 30 x = 30 when 20 t = 30 20t = 30 20 t = 30 , so t = 1.5 t = 1.5 t = 1.5 s. The height is
y ( 1.5 ) = 2 + 22.5 − 11.025 = 13.475 m y(1.5) = 2 + 22.5 - 11.025 = 13.475 \text{ m} y ( 1.5 ) = 2 + 22.5 − 11.025 = 13.475 m
8. (Challenge) Given r ⃗ ′ ( t ) = ⟨ 2 t e t 2 , 1 1 + t 2 ⟩ \vec{r}\,'(t) = \left\langle 2te^{t^2},\ \dfrac{1}{1 + t^2} \right\rangle r ′ ( t ) = ⟨ 2 t e t 2 , 1 + t 2 1 ⟩ and r ⃗ ( 0 ) = ⟨ − 1 , 2 ⟩ \vec{r}(0) = \langle -1, 2 \rangle r ( 0 ) = ⟨ − 1 , 2 ⟩ , find r ⃗ ( 1 ) \vec{r}(1) r ( 1 ) exactly.
Solution Use r ⃗ ( 1 ) = r ⃗ ( 0 ) + ∫ 0 1 r ⃗ ′ ( t ) d t \vec{r}(1) = \vec{r}(0) + \displaystyle\int_0^1 \vec{r}\,'(t)\, dt r ( 1 ) = r ( 0 ) + ∫ 0 1 r ′ ( t ) d t .
First component (substitute u = t 2 u = t^2 u = t 2 , d u = 2 t d t du = 2t\, dt d u = 2 t d t ):
∫ 0 1 2 t e t 2 d t = [ e t 2 ] 0 1 = e − 1 \int_0^1 2te^{t^2}\, dt = \Big[ e^{t^2} \Big]_0^1 = e - 1 ∫ 0 1 2 t e t 2 d t = [ e t 2 ] 0 1 = e − 1 Second component:
∫ 0 1 1 1 + t 2 d t = [ arctan t ] 0 1 = π 4 \int_0^1 \frac{1}{1 + t^2}\, dt = \Big[ \arctan t \Big]_0^1 = \frac{\pi}{4} ∫ 0 1 1 + t 2 1 d t = [ arctan t ] 0 1 = 4 π r ⃗ ( 1 ) = ⟨ − 1 + e − 1 , 2 + π 4 ⟩ = ⟨ e − 2 , 2 + π 4 ⟩ \vec{r}(1) = \left\langle -1 + e - 1,\ 2 + \frac{\pi}{4} \right\rangle = \left\langle e - 2,\ 2 + \frac{\pi}{4} \right\rangle r ( 1 ) = ⟨ − 1 + e − 1 , 2 + 4 π ⟩ = ⟨ e − 2 , 2 + 4 π ⟩
9. (Challenge) (Calculator active.) Given r ⃗ ′ ( t ) = ⟨ 1 + t 3 , cos ( t 2 ) ⟩ \vec{r}\,'(t) = \left\langle \sqrt{1 + t^3},\ \cos(t^2) \right\rangle r ′ ( t ) = ⟨ 1 + t 3 , cos ( t 2 ) ⟩ and r ⃗ ( 0 ) = ⟨ 2 , − 1 ⟩ \vec{r}(0) = \langle 2, -1 \rangle r ( 0 ) = ⟨ 2 , − 1 ⟩ , find r ⃗ ( 2 ) \vec{r}(2) r ( 2 ) . Explain why a calculator is needed.
Solution Neither 1 + t 3 \sqrt{1 + t^3} 1 + t 3 nor cos ( t 2 ) \cos(t^2) cos ( t 2 ) has an antiderivative you can write with ordinary functions, so evaluate the definite integrals numerically (radian mode):
r ⃗ ( 2 ) = ⟨ 2 + ∫ 0 2 1 + t 3 d t , − 1 + ∫ 0 2 cos ( t 2 ) d t ⟩ ≈ ⟨ 2 + 3.241 , − 1 + 0.461 ⟩ = ⟨ 5.241 , − 0.539 ⟩ \vec{r}(2) = \left\langle 2 + \int_0^2 \sqrt{1 + t^3}\, dt,\ -1 + \int_0^2 \cos(t^2)\, dt \right\rangle \approx \langle 2 + 3.241,\ -1 + 0.461 \rangle = \langle 5.241,\ -0.539 \rangle r ( 2 ) = ⟨ 2 + ∫ 0 2 1 + t 3 d t , − 1 + ∫ 0 2 cos ( t 2 ) d t ⟩ ≈ ⟨ 2 + 3.241 , − 1 + 0.461 ⟩ = ⟨ 5.241 , − 0.539 ⟩