The Calculus of VectorValued Functions
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To study the calculus of vectorvalued functions, we follow a similar path to the one we took in studying realvalued functions. First, we define the derivative, then we examine applications of the derivative, then we move on to defining integrals. However, we will find some interesting new ideas along the way as a result of the vector nature of these functions and the properties of space curves.
Derivatives of VectorValued Functions
Now that we have seen what a vectorvalued function is and how to take its limit, the next step is to learn how to differentiate a vectorvalued function. The definition of the derivative of a vectorvalued function is nearly identical to the definition of a realvalued function of one variable. However, because the range of a vectorvalued function consists of vectors, the same is true for the range of the derivative of a vectorvalued function.
Definition: Derivative of VectorValued Functions
The derivative of a vectorvalued function \(\vecs{r}(t)\) is
\[\vecs{r}′(t) = \lim \limits_{\Delta t \to 0} \dfrac{\vecs{r}(t+\Delta t)−\vecs{r}(t)}{ \Delta t} \label{eq1} \]
provided the limit exists. If \(\vecs{r}'(t)\) exists, then \(\vecs{r}(t)\) is differentiable at \(t\). If \(\vecs{r}′(t)\) exists for all \(t\) in an open interval \(\mathrm{(a,b)}\) then \(\vecs{r}(t)\) is differentiable over the interval \(\mathrm{(a,b)}\). For the function to be differentiable over the closed interval \(\mathrm{[a,b]}\), the following two limits must exist as well:
\[\vecs{r}′(a) = \lim \limits_{\Delta t \to 0^+} \dfrac{\vecs{r}(a+\Delta t)−\vecs{r}(a)}{ \Delta t} \]
and
\[\vecs{r}′(b) = \lim \limits_{\Delta t \to 0^} \dfrac{\vecs{r}(b+\Delta t)−\vecs{r}(b)}{ \Delta t}\]
Graphical Interpretation of the Derivative: Recall that the derivative of a realvalued function can be interpreted as the slope of a tangent line or the instantaneous rate of change of the function. The derivative of a vectorvalued function can be understood to be an instantaneous rate of change as well; for example, when the function represents the position of an object at a given point in time, the derivative represents its velocity at that same point in time.
To understand what this derivative represents geometrically, it helps to consider the diagram shown in Figure \(\PageIndex{1}\). For the purposes of this illustration, consider \(\vecs r(t)\) to the represent position of an object.
We see vectors \(\vecs r(t)\) and \(\vecs r(t + \Delta t)\), where \(\Delta t\) is a small change in time producing a second vector that is farther along in the direction of motion.
The difference of these two vectors gives us the displacement vector, \(\vecs r(t + \Delta t)  \vecs r(t)\), shown here in red.
As \(\Delta t \rightarrow 0\), \(\vecs r(t + \Delta t)\) will approach \(\vecs r(t)\), and the displacement vector \(\vecs r(t + \Delta t)  \vecs r(t)\) will become closer and closer to being tangent to the curve at the terminal point of \(\vecs r(t)\).
Although the length of the displacement vector is approaching \(0\), we are actually taking the limit not of the displacement vector itself, but of the average velocity over the time \(\Delta t\), found by dividing the displacement vector by the scalar \(\Delta t\).
\[\text{Average Velocity}\quad=\quad\frac{\vecs r(t + \Delta t)  \vecs r(t)}{\Delta t}\]
Since \(\Delta t\) is also approaching \(0\), dividing by it will tend to lengthen the average velocity vector (as long as \(\Delta t \lt 1\)).
The limit gives us the vector \(\vecs r′(t)\), the velocity of the motion along the curve, which is tangent to the curve at this point.
We now demonstrate taking the derivative of a vectorvalued function.
Example \(\PageIndex{1}\): Finding the Derivative of a VectorValued Function
Use the definition to calculate the derivative of the function
\[\vecs{r}(t)=(3t+4) \,\hat{\mathbf{i}}+(t^2−4t+3) \,\hat{\mathbf{j}} .\nonumber\]
Solution
Let’s use Equation \ref{eq1}:
\[\begin{align*} \vecs{r}′(t) & \mathrm{= \lim \limits_{\Delta t \to 0} \dfrac{\vecs{r}(t+Δt)− \vecs{r} (t)}{Δt}} \\[5pt] & \mathrm{= \lim \limits_{\Delta t \to 0} \dfrac{[(3(t+Δt)+4)\,\hat{\mathbf{i}}+((t+Δt)^2−4(t+Δt)+3)\,\hat{\mathbf{j}}]−[(3t+4) \,\hat{\mathbf{i}}+(t^2−4t+3) \,\hat{\mathbf{j}}]}{Δt}} \\[5pt] & \mathrm{= \lim \limits_{\Delta t \to 0} \dfrac{(3t+3Δt+4) 3Δt+4)\,\hat{\mathbf{i}}−(3t+4) \,\hat{\mathbf{i}}+(t^2+2tΔt+(Δt)^2−4t−4Δt+3) \,\hat{\mathbf{j}}−(t^2−4t+3)\,\hat{\mathbf{j}}}{Δt}} \\[5pt] & \mathrm{= \lim \limits_{\Delta t \to 0} \dfrac{(3Δt)3Δt)\,\hat{\mathbf{i}}+(2tΔt+(Δt)^2−4Δt)\,\hat{\mathbf{j}}}{Δt}} \\[5pt] & \mathrm{= \lim \limits_{\Delta t \to 0} (3 \,\hat{\mathbf{i}}+(2t+Δt−4)\,\hat{\mathbf{j}})} \\[5pt] & \mathrm{ =3 \,\hat{\mathbf{i}}+(2t−4) \,\hat{\mathbf{j}} } \end{align*} \]
Exercise \(\PageIndex{1}\)
Use the definition to calculate the derivative of the function \(\vecs{r}(t)=(2t^2+3) \,\hat{\mathbf{i}}+(5t−6) \,\hat{\mathbf{j}}\).
 Hint

Use Equation \ref{eq1}.
 Answer

\[\vecs{r}′(t)=4t \,\hat{\mathbf{i}}+5 \,\hat{\mathbf{j}} \nonumber\]
Notice that in the calculations in Example \(\PageIndex{1}\), we could also obtain the answer by first calculating the derivative of each component function, then putting these derivatives back into the vectorvalued function. This is always true for calculating the derivative of a vectorvalued function, whether it is in two or three dimensions. We state this in the following theorem. The proof of this theorem follows directly from the definitions of the limit of a vectorvalued function and the derivative of a vectorvalued function.
Theorem \(\PageIndex{1}\): Differentiation of VectorValued Functions
Let \(f\), \(g\), and \(h\) be differentiable functions of \(t\).
 If \(\vecs{r}(t)=f(t) \,\hat{\mathbf{i}}+g(t) \,\hat{\mathbf{j}}\) then \[\vecs{r}′(t)=f′(t) \,\hat{\mathbf{i}}+g′(t) \,\hat{\mathbf{j}}.\]
 If \(\vecs{r}(t)=f(t) \,\hat{\mathbf{i}}+g(t) \,\hat{\mathbf{j}} + h(t) \,\hat{\mathbf{k}}\) then \[\vecs{r}′(t)=f′(t) \,\hat{\mathbf{i}}+g′(t) \,\hat{\mathbf{j}} + h′(t) \,\hat{\mathbf{k}}.\]
Example \(\PageIndex{2}\): Calculating the Derivative of VectorValued Functions
Use Theorem \(\PageIndex{1}\) to calculate the derivative of each of the following functions.
 \(\vecs{r}(t)=(6t+8) \,\hat{\mathbf{i}}+(4t^2+2t−3) \,\hat{\mathbf{j}}\)
 \(\vecs{r}(t)=3 \cos t \,\hat{\mathbf{i}}+4 \sin t \,\hat{\mathbf{j}}\)
 \(\vecs{r}(t)=e^t \sin t \,\hat{\mathbf{i}}+e^t \cos t \,\hat{\mathbf{j}}−e^{2t} \,\hat{\mathbf{k}}\)
Solution
We use Theorem \(\PageIndex{1}\) and what we know about differentiating functions of one variable.
 The first component of \[\vecs r(t)=(6t+8) \,\hat{\mathbf{i}}+(4t^2+2t−3) \,\hat{\mathbf{j}} \nonumber\] is \(f(t)=6t+8\). The second component is \(g(t)=4t^2+2t−3\). We have \(f′(t)=6\) and \(g′(t)=8t+2\), so Theorem \(\PageIndex{1}\) gives \[\vecs r′(t)=6 \,\hat{\mathbf{i}}+(8t+2)\,\hat{\mathbf{j}} \nonumber\]
 The first component is \(f(t)=3 \cos t\) and the second component is \(g(t)=4 \sin t\). We have \(f′(t)=−3 \sin t\) and \(g′(t)=4 \cos t\), so we obtain \[\vecs r′(t)=−3 \sin t \,\hat{\mathbf{i}}+4 \cos t \,\hat{\mathbf{j}} \nonumber\]
 The first component of \(\vecs r(t)=e^t \sin t \,\hat{\mathbf{i}}+e^t \cos t \,\hat{\mathbf{j}}−e^{2t} \,\hat{\mathbf{k}}\) is \(f(t)=e^t \sin t\), the second component is \(g(t)=e^t \cos t\), and the third component is \(h(t)=−e^{2t}\). We have \(f′(t)=e^t(\sin t+\cos t)\), \(g′(t)=e^t (\cos t−\sin t)\), and \(h′(t)=−2e^{2t}\), so the theorem gives \[\vecs r′(t)=e^t(\sin t+\cos t)\,\hat{\mathbf{i}}+e^t(\cos t−\sin t)\,\hat{\mathbf{j}}−2e^{2t} \,\hat{\mathbf{k}} \nonumber\]
Exercise \(\PageIndex{2}\)
Calculate the derivative of the function
\[\vecs{r}(t)=(t \ln t)\,\hat{\mathbf{i}}+(5e^t) \,\hat{\mathbf{j}}+(\cos t−\sin t) \,\hat{\mathbf{k}}. \nonumber\]
 Hint

Identify the component functions and use Theorem \(\PageIndex{1}\).
 Answer

\[\vecs{r}′(t)=(1+ \ln t) \,\hat{\mathbf{i}}+5e^t \,\hat{\mathbf{j}}−(\sin t+\cos t)\,\hat{\mathbf{k}} \nonumber\]
Describing Motion with VectorValued Functions
As has been mentioned already in this section, vectorvalued functions are often used to describe motion in the plane or in space. Now that we understand the derivative of a vectorvalued function, let's make the relationships clear.
First, since the components of a vectorvalued function represent the coordinates of a point on the corresponding curve, it may help to write
\[\vecs r(t) = x(t) \,\,\hat{\mathbf{i}} + y(t) \,\,\hat{\mathbf{j}} + z(t) \, \,\hat{\mathbf{k}}\]
This approach has already been used in Section 12.1.
Now we can define how to calculate the velocity, speed, acceleration, and jerk of the object's motion.
Definition: Velocity, speed, Acceleration, and JERK
Let \(\vecs r(t)\) be a twicedifferentiable vectorvalued function of the parameter \(t\) that represents the position of an object as a function of time.
The velocity vector \(\vecs v(t)\) of the object is given by
\[\text{Velocity}\,=\vecs v(t)=\vecs r′(t). \label{Eq1}\]
The speed is defined to be
\[\mathrm{Speed}\,=‖\vecs v(t)‖=‖\vecs r′(t)‖=\dfrac{ds}{dt}. \label{Eq2}\]
The acceleration vector \(\vecs a(t)\) is defined to be
\[\text{Acceleration}\,=\vecs a(t)=\vecs v′(t)=\vecs r″(t). \label{Eq3}\]
If \(\vecs r(t)\) has a third derivative, we can also define the jerk vector \(\vecd{jerk}(t)\) to be
\[\text{Jerk}\,=\vecd{\text{jerk}}(t) = \vecs a'(t)=\vecs r'''(t). \label{Eq4}\]
Now let's see how this looks in the context of a particular position function.
Example \(\PageIndex{3}\): Finding velocity, speed, acceleration, and jerk
Consider the position function, \[\vecs r(t) = (1  t^2) \, \hat{\mathbf{i}} + t \, \hat{\mathbf{j}}, \, \text{where time is in seconds}\]
a. Determine the velocity, speed, acceleration, and jerk as functions of time for this position function.
b. Evaluate each of these functions, including the position function, at times \(t = 0\) sec and \(t = 2\) sec.
c. Sketch a graph of this position function and draw in each of the nonzero vectors from part b on the graph of \(\vecs r\), starting at the location of the object on the curve at the corresponding time.
Solution
a. Since \(\vecs r(t) = (1  t^2) \, \hat{\mathbf{i}} + t \, \hat{\mathbf{j}}\), we have
\[\begin{align*} \vecs v(t) &= \vecs r'(t) = 2t \, \hat{\mathbf{i}} + 1 \, \hat{\mathbf{j}},\\[5pt] \text{speed}(t) &= \ v(t) \ = \sqrt{(2t)^2 +(1)^2} = \sqrt{4t^2 + 1}, \\[5pt] \vecs a(t) &= \vecs v'(t) = 2 \, \hat{\mathbf{i}}, \\[5pt] \vecd{\text{jerk}}(t) &= \vecs 0 \end{align*}\]
b. Evaluating these functions at time \(t = 0\), we get:
\[\begin{align*} \vecs r(0) &= (1  0^2) \, \hat{\mathbf{i}} + 0 \, \hat{\mathbf{j}} = \hat{\mathbf{i}} \\
\vecs v(0) &= 2(0) \, \hat{\mathbf{i}} + 1 \, \hat{\mathbf{j}} = \hat{\mathbf{j}} \\
\text{speed}(0) &= \sqrt{4(0)^2 + 1} = \sqrt{1} = 1 \, \text{unit/sec} \\
\vecs a(0) &= 2 \, \hat{\mathbf{i}}, \\
\vecd{\text{jerk}}(0) &= \vecs 0 \end{align*}\]
And for time \(t = 2\), we have
\[\begin{align*} \vecs r(2) &= (1  2^2) \, \hat{\mathbf{i}} + 2 \, \hat{\mathbf{j}} = 3 \, \hat{\mathbf{i}} + 2 \, \hat{\mathbf{j}} \\
\vecs v(2) &= 2(2) \, \hat{\mathbf{i}} + 1 \, \hat{\mathbf{j}} = 4 \, \hat{\mathbf{i}} + \hat{\mathbf{j}} \\
\text{speed}(2) &= \sqrt{4(2)^2 + 1} = \sqrt{17} \, \text{units/sec} \\
\vecs a(0) &= 2 \, \hat{\mathbf{i}}, \\
\vecd{\text{jerk}}(0) &= \vecs 0 \end{align*}\]
c. The graph of this curve is shown below in Figure \(\PageIndex{2}\). We then drew in and labeled the vectors \(vecs v(0)\), \(vecs a(0)\), \(vecs v(2)\), and \(vecs a(2)\).
Smooth VectorValued Functions
Definition: smoothness
Let \(\vecs{r}(t)=f(t) \,\hat{\mathbf{i}}+g(t) \,\hat{\mathbf{j}} + h(t) \,\hat{\mathbf{k}}\) be the parameterization of a curve that is differentiable on an open interval \(I\).
Then \(\vecs r(t)\) is smooth on the open interval \(I\), if
\(\vecs r'(t) \neq \vecs 0\), for any value of \(t\) in the interval \(I\).
To put this another way, \(\vecs r(t)\) is smooth on the open interval \(I\) if:
 \(\vecs r(t)\) is defined and continuous on \(I\), and
 \(f', \, g'\) and \(h'\) are all continuous on \(I\), that is, \(\vecs r'(t)\) is defined and continuous on \(I\), and
 \(\vecs r'(t) \neq \vecs 0\) for all values of \(t\) in the interval \(I\).
The concept of smoothness is very closely connected to the application of vectorvalued functions to motion. If you have ever ridden rides at an amusement park, you can probably identify some where the ride felt smooth, and others where there are moments during the ride where it was not smooth. These moments often correspond to points in the motion where the relevant parameterization is not smooth by the definition above.
To identify open intervals in the domain of \(\vecs r\) on which \(\vecs r\) is smooth, we usually identify values of \(t\) for which \(\vecs r\) is not smooth.
In addition to using the definition above to identify these points, it is often apparent from the graph of the vectorvalued function \(\vecs r(t)\). A cusp, i.e., a sharp turning point, is a common occurrence at points where a curve is not smooth. In Figure \(\PageIndex{3}\) below, you can quickly identify points at which the parameterization fails to be smooth by locating cusps in the graph.
When we consider the motion described by \(\vecs r(t)\), there are at least two additional events that can occur at points where the parameterization fails to be smooth: a reversal of motion or a momentary pause in the motion. To summarize these events:
If a vectorvalued function \(\vecs r(t)\) is not smooth at time \(t\), we will observe that:
 There is a cusp at the associated point on the graph of \(\vecs r(t)\), or
 The motion reverses itself at the associated point, causing the motion to travel back along the same path in the opposite direction, or
 The motion actually stops and starts up again, with no visual cue, that is, where the curve appears smooth.
Let's consider a couple examples to see how this can look.
Example \(\PageIndex{4}\): Determining open intervals on which a vectorvalued function is smooth
Determine the open intervals on which each of the following vectorvalued functions is smooth:
 \(\vecs r(t) = \left( 2t^3  3t^2\right) \, \,\hat{\mathbf{i}} + \left( t^2  2t\right) \, \,\hat{\mathbf{j}} + 2\,\,\hat{\mathbf{k}}\)
 \(\vecs r(t) = t^3 \, \,\hat{\mathbf{i}} + \sqrt{t^2  1} \,\hat{\mathbf{j}}\)
 \(\vecs r(t) = t^4 \, \,\hat{\mathbf{i}} + \ln(t^2 + 1) \,\hat{\mathbf{j}}\)
 \(\vecs r(t) = \left( 6\cos t  \cos(6t)\right) \, \,\hat{\mathbf{i}} + \left( 6\sin t  \sin(6t) \right) \, \,\hat{\mathbf{j}}\), for \(0 \le t \le 2\pi\)
Solution
a. First we need to consider the domain of \(\vecs r\). In this case, \(\text{D}_{\vecs r} : (\infty, \infty)\).
Then we need to find \(\vecs r'(t)\). Since \(\vecs r(t) = \left( 2t^3  3t^2\right) \, \,\hat{\mathbf{i}} + \left( t^2  2t\right) \, \,\hat{\mathbf{j}} + 2\,\,\hat{\mathbf{k}}\),
\[\vecs r'(t) = \left( 6t^2  6t\right) \, \,\hat{\mathbf{i}} + \left( 2t  2\right) \, \,\hat{\mathbf{j}}\]
Next we need to consider the domain of \(\vecs r'\). Here, \(\text{D}_{\vecs r'} : (\infty, \infty)\).
Finally we need to determine if there are any values of \(t\) in \(\text{D}_{\vecs r}\) where \(\vecs r'(t) = \vecs 0\).
To do this, we set each component of \(\vecs r'(t)\) equal to \(0\) and solve for \(t\).
\[\begin{alignat} 6t^2  6t = 0 & \quad \text{and} \quad & 2t  2 = 0 \\ 6t(t 1) = 0 && 2(t  1) = 0 \\ t = 0 \quad \text{or} \quad t = 1 & & t = 1 \end{alignat}\]
Since \(t = 1\) makes both components of \(\vecs r'\) equal 0, we have \(\vecs r'(1) = \vecs 0\), so we know that \(\vecs r\) is not smooth at \(t = 1\).
Note however that \(\vecs r\) is smooth at \(t = 0\), because although one of the components of \(\vecs r'\) is \(0\), the other one is not.
Therefore we can conclude that \(\vecs r\) is smooth on the open intervals:
\[ (\infty, 1) \quad \text{and} \quad (1, \infty) \]
Note in the figure that there is a cusp in the curve when \(t = 1\).
b. The domain of \(\vecs r\) is \(\text{D}_{\vecs r} : (\infty, 1] \cup [1, \infty) \), since \(t^2  1\) is less than \(0\) between \(1\) and \(1\).
Now we calculate \(\vecs r'(t)\). Since \(\vecs r(t) = t^3 \, \,\hat{\mathbf{i}} + \sqrt{t^2  1} \,\hat{\mathbf{j}}\), we have
\[\vecs r'(t) = 3t^2 \, \,\hat{\mathbf{i}} + \frac{t}{\sqrt{t^21}} \, \,\hat{\mathbf{j}}\]
Then, since we cannot have zero in the denominator, \(t = 1\) and \(t = 1\) are not in the domain of \(\vecs r'\). Thus, \(\text{D}_{\vecs r'} : (\infty, 1) \cup (1, \infty) \).
Lastly we determine if there are any values of \(t\) in \(\text{D}_{\vecs r}\) where \(\vecs r'(t) = \vecs 0\).
Setting each component of \(\vecs r'(t)\) equal to \(0\) and solve for \(t\) we get:
\[\begin{alignat} 3t^2 = 0 & \quad \text{and} \quad & \frac{t}{\sqrt{t^21}} = 0 \\ t = 0 && t = 0 \end{alignat}\]
If \(t = 0\) were in the domain of \(\vecs r'\), then \(\vecs r\) would not be smooth there, but since it is not in the domain, we have nothing to remove, and we can conclude that \(\vecs r\) is smooth on the entire domain of its derivative \(\vecs r'\), that is,
\[\vecs r \, \text{is smooth on the open intervals:} \quad (\infty, 1) \quad \text{and} \quad (1, \infty).\]
Observe the two separate smooth pieces of this function in the graph below.
c.
Properties of the Derivative
We can extend to vectorvalued functions the properties of the derivative that we presented previously for realvalued functions of a single variable. In particular, the constant multiple rule, the sum and difference rules, the product rule, and the chain rule all extend to vectorvalued functions. However, in the case of the product rule, there are actually three extensions:
 for a realvalued function multiplied by a vectorvalued function,
 for the dot product of two vectorvalued functions, and
 for the cross product of two vectorvalued functions.
Theorem: Properties of the Derivative of VectorValued Functions
Let \(\vecs{r}\) and \(\vecs{u}\) be differentiable vectorvalued functions of \(t\), let \(f\) be a differentiable realvalued function of \(t\), and let \(c\) be a scalar.
\[\begin{array}{lrcll} \mathrm{i.} & \dfrac{d}{dt}[c\vecs r(t)] & = & c\vecs r′(t) & \text{Scalar multiple} \nonumber\\ \mathrm{ii.} & \dfrac{d}{dt}[\vecs r(t)±\vecs u(t)] & = & \vecs r′(t)±\vecs u′(t) & \text{Sum and difference} \nonumber\\ \mathrm{iii.} & \dfrac{d}{dt}[f(t)\vecs u(t)] & = & f′(t)\vecs u(t)+f(t)\vecs u′(t) & \text{Scalar product} \nonumber\\ \mathrm{iv.} & \dfrac{d}{dt}[\vecs r(t)⋅\vecs u(t)] & = & \vecs r′(t)⋅\vecs u(t)+\vecs r(t)⋅\vecs u′(t) & \text{Dot product} \nonumber\\ \mathrm{v.} & \dfrac{d}{dt}[\vecs r(t)×\vecs u(t)] & = & \vecs r′(t)×\vecs u(t)+\vecs r(t)×\vecs u′(t) & \text{Cross product} \nonumber\\ \mathrm{vi.} & \dfrac{d}{dt}[\vecs r(f(t))] & = & \vecs r′(f(t))⋅f′(t) & \text{Chain rule} \nonumber\\ \mathrm{vii.} & \text{If} \; \vecs r(t)·\vecs r(t) & = & c, \text{then} \; \vecs r(t)⋅\vecs r′(t) \; =0 \; . & \mathrm{} \nonumber \end{array} \nonumber \]
Proof
The proofs of the first two properties follow directly from the definition of the derivative of a vectorvalued function. The third property can be derived from the first two properties, along with the product rule. Let \(\vecs u(t)=g(t)\,\hat{\mathbf{i}}+h(t)\,\hat{\mathbf{j}}\). Then
\[\begin{align*} \dfrac{d}{dt}[f(t)\vecs u(t)] \; & =\dfrac{d}{dt}[f(t)(g(t) \,\hat{\mathbf{i}}+h(t) \,\hat{\mathbf{j}})] \\[5pt] & =\dfrac{d}{dt}[f(t)g(t) \,\hat{\mathbf{i}}+f(t)h(t) \,\hat{\mathbf{j}}] \\[5pt] & =\dfrac{d}{dt}[f(t)g(t)] \,\hat{\mathbf{i}}+\dfrac{d}{dt}[f(t)h(t)] \,\hat{\mathbf{j}} \\[5pt] & =(f′(t)g(t)+f(t)g′(t)) \,\hat{\mathbf{i}}+(f′(t)h(t)+f(t)h′(t)) \,\hat{\mathbf{j}} \\[5pt] & =f′(t)\vecs u(t)+f(t)\vecs u′(t). \end{align*} \]
To prove property iv. let \(\vecs r(t)=f_1(t) \,\hat{\mathbf{i}}+g_1(t) \,\hat{\mathbf{j}}\) and \(\vecs u(t)=f_2(t) \,\hat{\mathbf{i}}+g_2(t) \,\hat{\mathbf{j}}\). Then
\[\begin{align*} \dfrac{d}{dt}[\vecs r(t)⋅\vecs u(t)] & =\dfrac{d}{dt}[f_1(t)f_2(t)+g_1(t)g_2(t)] \\[5pt] & =f_1′(t)f_2(t)+f_1(t)f_2′(t)+g_1′(t)g_2(t)+g_1(t)g_2′(t)=f_1′(t)f_2(t)+g_1′(t)g_2(t)+f_1(t)f_2′(t)+g_1(t)g_2′(t) \\[5pt] & =(f_1′ \,\hat{\mathbf{i}}+g_1′ \,\hat{\mathbf{j}})⋅(f_2 \,\hat{\mathbf{i}}+g_2 \,\hat{\mathbf{j}})+(f_1 \,\hat{\mathbf{i}}+g_1 \,\hat{\mathbf{j}})⋅(f_2′ \,\hat{\mathbf{i}}+g_2′ \,\hat{\mathbf{j}}) \\[5pt] & =\vecs r′(t)⋅\vecs u(t)+\vecs r(t)⋅\vecs u′(t). \end{align*} \]
The proof of property v. is similar to that of property iv. Property vi. can be proved using the chain rule. Last, property vii. follows from property iv:
\[\begin{align*} \dfrac{d}{dt}[\vecs r(t)·\vecs r(t)] \; & =\dfrac{d}{dt}[c] \\ \vecs r′(t)·\vecs r(t)+\vecs r(t)·\vecs r′(t) \; & = 0 \\ 2\vecs r(t)·\vecs r′(t) \; & = 0 \\ \vecs r(t)·\vecs r′(t) \; & = 0 \end{align*} \]
Now for some examples using these properties.
Example \(\PageIndex{5}\): Using the Properties of Derivatives of VectorValued Functions
Given the vectorvalued functions
\[\vecs{r}(t)=(6t+8)\,\hat{\mathbf{i}}+(4t^2+2t−3)\,\hat{\mathbf{j}}+5t \,\hat{\mathbf{k}} \nonumber\]
and
\[\vecs{u}(t)=(t^2−3)\,\hat{\mathbf{i}}+(2t+4)\,\hat{\mathbf{j}}+(t^3−3t)\,\hat{\mathbf{k}}, \nonumber\]
calculate each of the following derivatives using the properties of the derivative of vectorvalued functions.
 \(\dfrac{d}{dt}[\vecs{r}(t)⋅ \vecs{u}(t)]\)
 \(\dfrac{d}{dt}[ \vecs{u} (t) \times \vecs{u}′(t)]\)
Solution
We have \(\vecs{r}′(t)=6 \,\hat{\mathbf{i}}+(8t+2) \,\hat{\mathbf{j}}+5 \,\hat{\mathbf{k}}\) and \(\vecs{u}′(t)=2t \,\hat{\mathbf{i}}+2 \,\hat{\mathbf{j}}+(3t^2−3) \,\hat{\mathbf{k}}\). Therefore, according to property iv:

\[\begin{align*} \dfrac{d}{dt}[\vecs r(t)⋅\vecs u(t)] \; = & \vecs r′(t)⋅\vecs u(t)+\vecs r(t)⋅\vecs u′(t) \\ = & (6 \,\hat{\mathbf{i}}+(8t+2) \,\hat{\mathbf{j}}+5 \,\hat{\mathbf{k}})⋅((t^2−3) \,\hat{\mathbf{i}}+(2t+4) \,\hat{\mathbf{j}}+(t^3−3t) \,\hat{\mathbf{k}}) \\[5pt] & +((6t+8) \,\hat{\mathbf{i}}+(4t^2+2t−3) \,\hat{\mathbf{j}}+5t \,\hat{\mathbf{k}})⋅(2t \,\hat{\mathbf{i}}+2 \,\hat{\mathbf{j}}+(3t^2−3)\,\hat{\mathbf{k}}) \\ = & 6(t^2−3)+(8t+2)(2t+4)+5(t^3−3t) \\[5pt] & +2t(6t+8)+2(4t^2+2t−3)+5t(3t^2−3) \\ = & 20t^3+42t^2+26t−16. \end{align*}\]
 First, we need to adapt property v for this problem:
\[\dfrac{d}{dt}[ \vecs{u}(t) \times \vecs{u}′(t)]=\vecs{u}′(t)\times \vecs{u}′(t)+ \vecs{u}(t) \times \vecs{u}′′(t). \nonumber\]
Recall that the cross product of any vector with itself is zero. Furthermore,\(\vecs u′′(t)\) represents the second derivative of \(\vecs u(t):\)
\[\vecs u′′(t)=\dfrac{d}{dt}[\vecs u′(t)]=\dfrac{d}{dt}[2t \,\hat{\mathbf{i}}+2 \,\hat{\mathbf{j}}+(3t^2−3) \,\hat{\mathbf{k}}]=2 \,\hat{\mathbf{i}}+6t \,\hat{\mathbf{k}}. \nonumber\]
Therefore,
\[\begin{align*} \dfrac{d}{dt}[\vecs u(t) \times \vecs u′(t)] \; & =0+((t^2−3)\,\hat{\mathbf{i}}+(2t+4)\,\hat{\mathbf{j}}+(t^3−3t)\,\hat{\mathbf{k}})\times (2 \,\hat{\mathbf{i}}+6t \,\hat{\mathbf{k}}) \\[5pt] & = \begin{array}{ccc} \,\hat{\mathbf{i}} & \,\hat{\mathbf{j}} & \,\hat{\mathbf{k}} \\ t^23 & 2t+4 & t^3 3t \\ 2 & 0 & 6t \end{array} \\[5pt] & =6t(2t+4) \,\hat{\mathbf{i}}−(6t(t^2−3)−2(t^3−3t)) \,\hat{\mathbf{j}}−2(2t+4) \,\hat{\mathbf{k}} \\[5pt] & =(12t^2+24t) \,\hat{\mathbf{i}}+(12t−4t^3) \,\hat{\mathbf{j}}−(4t+8)\,\hat{\mathbf{k}}. \end{align*}\]
Exercise \(\PageIndex{3}\)
Calculate \(\dfrac{d}{dt}[\vecs{r}(t)⋅ \vecs{r}′(t)]\) and \( \dfrac{d}{dt}[\vecs{u}(t) \times \vecs{r}(t)]\) for the vectorvalued functions:
 \(\vecs{r}(t)=\cos t \,\hat{\mathbf{i}}+ \sin t \,\hat{\mathbf{j}}−e^{2t} \,\hat{\mathbf{k}}\)
 \(\vecs{u}(t)=t \,\hat{\mathbf{i}}+ \sin t \,\hat{\mathbf{j}}+ \cos t \,\hat{\mathbf{k}}\),
 Hint

Follow the same steps as in Example \(\PageIndex{4}\).
 Answer

\(\dfrac{d}{dt}[\vecs{r}(t)⋅ \vecs{r}′(t)]=8e^{4t}\)
\( \dfrac{d}{dt}[ \vecs{u}(t) \times \vecs{r}(t)] =−(e^{2t}(\cos t+2 \sin t)+ \cos 2t) \,\hat{\mathbf{i}}+(e^{2t}(2t+1)− \sin 2t) \,\hat{\mathbf{j}}+(t \cos t+ \sin t− \cos 2t) \,\hat{\mathbf{k}}\)
Tangent Vectors and Unit Tangent Vectors
Recall that the derivative at a point can be interpreted as the slope of the tangent line to the graph at that point. In the case of a vectorvalued function, the derivative provides a tangent vector to the curve represented by the function. Consider the vectorvalued function
\[\vecs{r}(t)=\cos t \,\hat{\mathbf{i}} + \sin t \,\hat{\mathbf{j}} \label{eq10}\]
The derivative of this function is
\[\vecs{r}′(t)=−\sin t \,\hat{\mathbf{i}} + \cos t \,\hat{\mathbf{j}} \nonumber \]
If we substitute the value \(t=π/6\) into both functions we get
\[\vecs{r} \left(\dfrac{π}{6}\right)=\dfrac{\sqrt{3}}{2} \,\hat{\mathbf{i}}+\dfrac{1}{2}\,\hat{\mathbf{j}} \nonumber\]
and
\[ \vecs{r}′ \left(\dfrac{π}{6} \right)=−\dfrac{1}{2}\,\hat{\mathbf{i}}+\dfrac{\sqrt{3}}{2}\,\hat{\mathbf{j}}. \nonumber\]
The graph of this function appears in Figure \(\PageIndex{6}\), along with the vectors \(\vecs{r}\left(\dfrac{π}{6}\right)\) and \(\vecs{r}' \left(\dfrac{π}{6}\right)\).
Notice that the vector \(\vecs{r}′\left(\dfrac{π}{6}\right)\) is tangent to the circle at the point corresponding to \(t=\dfrac{π}{6}\). This is an example of a tangent vector to the plane curve defined by Equation \ref{eq10}.
Definition: principal unit tangent vector
Let \(C\) be a curve defined by a vectorvalued function \(\vecs{r}\), and assume that \(\vecs{r}′(t)\) exists when \(t=t_0\) A tangent vector \(\vecs{r}\) at \(t=t_0\) is any vector such that, when the tail of the vector is placed at point \(\vecs r(t_0)\) on the graph, vector \(\vecs{r}\) is tangent to curve \(C\). Vector \(\vecs{r}′(t_0)\) is an example of a tangent vector at point \(t=t_0\). Furthermore, assume that \(\vecs{r}′(t)≠0\). The principal unit tangent vector at \(t\) is defined to be
\[\vecs{T}(t)=\dfrac{ \vecs{r}′(t)}{‖\vecs{r}′(t)‖},\]
provided \(‖\vecs{r}′(t)‖≠0\).
The unit tangent vector is exactly what it sounds like: a unit vector that is tangent to the curve. To calculate a unit tangent vector, first find the derivative \(\vecs{r}′(t)\). Second, calculate the magnitude of the derivative. The third step is to divide the derivative by its magnitude.
Example \(\PageIndex{6}\): Finding a Unit Tangent Vector
Find the unit tangent vector for each of the following vectorvalued functions:
 \(\vecs{r}(t)=\cos t \,\hat{\mathbf{i}}+\sin t \,\hat{\mathbf{j}}\)
 \(\vecs{u}(t)=(3t^2+2t) \,\hat{\mathbf{i}}+(2−4t^3)\,\hat{\mathbf{j}}+(6t+5)\,\hat{\mathbf{k}}\)
Solution

\(\begin{array}{lrcl} \text{First step:} & \vecs r′(t) & = & − \sin t \,\hat{\mathbf{i}}+ \cos t \,\hat{\mathbf{j}} \\ \text{Second step:} & ‖\vecs r′(t)‖ & = & \sqrt{(− \sin t)^2+( \cos t)^2} = 1 \\ \text{Third step:} & \vecs T(t) & = & \dfrac{\vecs r′(t)}{‖\vecs r′(t)‖}=\dfrac{− \sin t \,\hat{\mathbf{i}}+ \cos t \,\hat{\mathbf{j}}}{1}=− \sin t \,\hat{\mathbf{i}}+ \cos t \,\hat{\mathbf{j}} \end{array}\)  \(\begin{array}{lrcl} \text{First step:} & \vecs r′(t) & = & (6t+2) \,\hat{\mathbf{i}}−12t^2 \,\hat{\mathbf{j}}+6 \,\hat{\mathbf{k}} \\ \text{Second step:} & ‖\vecs r′(t)‖ & = & \sqrt{(6t+2)^2+(−12t^2)^2+6^2} \\ \text{} & \text{} & = & \sqrt{144t^4+36t^2+24t+40} \\ \text{} & \text{} & = & 2 \sqrt{36t^4+9t^2+6t+10} \\ \text{Third step:} & \vecs T(t) & = & \dfrac{\vecs r′(t)}{‖\vecs r′(t)‖}=\dfrac{(6t+2) \,\hat{\mathbf{i}}−12t^2 \,\hat{\mathbf{j}}+6 \,\hat{\mathbf{k}}}{2 \sqrt{36t^4+9t^2+6t+10}} \\ \text{} & \text{} & = & \dfrac{3t+1}{\sqrt{36t^4+9t^2+6t+10}} \,\hat{\mathbf{i}}  \dfrac{6t^2}{\sqrt{36t^4+9t^2+6t+10}} \,\hat{\mathbf{j}} + \dfrac{3}{\sqrt{36t^4+9t^2+6t+10}} \,\hat{\mathbf{k}} \end{array}\)
Exercise \(\PageIndex{4}\)
Find the unit tangent vector for the vectorvalued function
\[\vecs r(t)=(t^2−3)\,\hat{\mathbf{i}}+(2t+1) \,\hat{\mathbf{j}}+(t−2) \,\hat{\mathbf{k}}. \nonumber\]
 Hint

Follow the same steps as in Example \(\PageIndex{5}\).
 Answer

\[\vecs T(t)=\dfrac{2t}{\sqrt{4t^2+5}}\,\hat{\mathbf{i}}+\dfrac{2}{\sqrt{4t^2+5}}\,\hat{\mathbf{j}}+\dfrac{1}{\sqrt{4t^2+5}}\,\hat{\mathbf{k}} \nonumber\]
Integrals of VectorValued Functions
We introduced antiderivatives of realvalued functions in Antiderivatives and definite integrals of realvalued functions in The Definite Integral. Each of these concepts can be extended to vectorvalued functions. Also, just as we can calculate the derivative of a vectorvalued function by differentiating the component functions separately, we can calculate the antiderivative in the same manner. Furthermore, the Fundamental Theorem of Calculus applies to vectorvalued functions as well.
The antiderivative of a vectorvalued function appears in applications. For example, if a vectorvalued function represents the velocity of an object at time t, then its antiderivative represents position. Or, if the function represents the acceleration of the object at a given time, then the antiderivative represents its velocity.
Definition: Definite and indefinite integrals of vectorvalued functions
Let f, g, and h be integrable realvalued functions over the closed interval \(\mathrm{[a,b].}\)
 The indefinite integral of a vectorvalued function \(\vecs{r}(t)=f(t) \,\hat{\mathbf{i}}+g(t) \,\hat{\mathbf{j}}\) is
\[\mathrm{\int [f(t) \,\hat{\mathbf{i}}+g(t) \,\hat{\mathbf{j}}]dt= \left[ \int f(t)dt \right] \,\hat{\mathbf{i}}+ \left[ \int g(t)dt \right] \,\hat{\mathbf{j}}.}\]
The definite integral of a vectorvalued function is\[\mathrm{\int_a^b [f(t) \,\hat{\mathbf{i}}+g(t) \,\hat{\mathbf{j}}]dt = \left[ \int_a^b f(t)dt \right] \,\hat{\mathbf{i}}+ \left[ \int_a^b g(t)dt \right] \,\hat{\mathbf{j}}.}\]
 The indefinite integral of a vectorvalued function \(\mathrm{r(t)=f(t) \,\hat{\mathbf{i}}+g(t) \,\hat{\mathbf{j}}+h(t) \,\hat{\mathbf{k}}}\) is
\[\mathrm{\int [f(t) \,\hat{\mathbf{i}}+g(t)\,\hat{\mathbf{j}} + h(t) \,\hat{\mathbf{k}}]dt= \left[ \int f(t)dt \right] \,\hat{\mathbf{i}}+ \left[ \int g(t)dt \right] \,\hat{\mathbf{j}} + \left[ \int h(t)dt \right] \,\hat{\mathbf{k}}.}\]
The definite integral of the vectorvalued function is\[\mathrm{\int_a^b [f(t) \,\hat{\mathbf{i}}+g(t) \,\hat{\mathbf{j}} + h(t) \,\hat{\mathbf{k}}]dt= \left[ \int_a^b f(t)dt \right] \,\hat{\mathbf{i}}+ \left[ \int_a^b g(t)dt \right] \,\hat{\mathbf{j}} + \left[ \int_a^b h(t)dt \right] \,\hat{\mathbf{k}}.}\]
Since the indefinite integral of a vectorvalued function involves indefinite integrals of the component functions, each of these component integrals contains an integration constant. They can all be different. For example, in the twodimensional case, we can have
\[\mathrm{\int f(t)dt=F(t)+C_1 \; and \; \int g(t)dt=G(t)+C_2,} \nonumber\]
where F and G are antiderivatives of f and g, respectively. Then
\[\begin{align*} \mathrm{\int [f(t) \,\hat{\mathbf{i}}+g(t) \,\hat{\mathbf{j}}]dt \;} & \mathrm{ = \left[ \int f(t)dt \right] \,\hat{\mathbf{i}}+ \left[ \int g(t)dt \right] \,\hat{\mathbf{j}}} \\[5pt] & \mathrm{= (F(t)+C_1) \,\hat{\mathbf{i}}+(G(t)+C_2) \,\hat{\mathbf{j}}} \\[5pt] & \mathrm{=F(t) \,\hat{\mathbf{i}}+G(t) \,\hat{\mathbf{j}}+C_1 \,\hat{\mathbf{i}}+C_2 \,\hat{\mathbf{j}}} \\[5pt] & \mathrm{= F(t) \,\hat{\mathbf{i}}+G(t) \,\hat{\mathbf{j}}+\vecs{C}} \end{align*}\]
where \(\vecs{C}=C_1 \,\hat{\mathbf{i}}+C_2 \,\hat{\mathbf{j}}\). Therefore, the integration constants becomes a constant vector.
Example \(\PageIndex{7}\): Integrating VectorValued Functions
Calculate each of the following integrals:
 \( \displaystyle \int [(3t^2+2t) \,\hat{\mathbf{i}}+(3t−6) \,\hat{\mathbf{j}}+(6t^3+5t^2−4) \,\hat{\mathbf{k}}]dt\)
 \( \displaystyle \int [⟨t,t^2,t^3⟩ \times ⟨t^3,t^2,t⟩] dt\)
 \( \displaystyle \int_{0}^{\frac{\pi}{3}} [\sin 2t \,\hat{\mathbf{i}}+ \tan t \,\hat{\mathbf{j}}+e^{−2t} \,\hat{\mathbf{k}}]dt\)
Solution
 We use the first part of the definition of the integral of a space curve:
\[\begin{align*} \mathrm{\int[(3t^2+2t)\,\hat{\mathbf{i}}+(3t−6) \,\hat{\mathbf{j}}+(6t^3+5t^2−4)\,\hat{\mathbf{k}}]dt} & \mathrm{=\left[\int 3t^2+2tdt \right]\,\hat{\mathbf{i}}+ \left[\int 3t−6dt \right] \,\hat{\mathbf{j}}+ \left[\int 6t^3+5t^2−4dt \right] \,\hat{\mathbf{k}}} \\[5pt] & \mathrm{=(t^3+t^2) \,\hat{\mathbf{i}}+(\dfrac{3}{2}t^2−6t) \,\hat{\mathbf{j}}+(\dfrac{3}{2}t^4+\dfrac{5}{3}t^3−4t)\,\hat{\mathbf{k}}+\vecs C.} \end{align*}\]
 First calculate \(\mathrm{⟨t,t^2,t^3⟩ \times ⟨t^3,t^2,t⟩:}\)
\[\begin{align*} \mathrm{⟨t,t^2,t^3⟩ \times ⟨t^3,t^2,t⟩} & = \begin{array}{ccc} \,\hat{\mathbf{i}} & \,\hat{\mathbf{j}} & \,\hat{\mathbf{k}} \\ \mathrm{t} & \mathrm{t^2} & \mathrm{t^3} \\ \mathrm{t^3} & \mathrm{t^2} & \mathrm{t} \end{array} \\[5pt] & \mathrm{=(t^2(t)−t^3(t^2)) \,\hat{\mathbf{i}}−(t^2−t^3(t^3))\,\hat{\mathbf{j}}+(t(t^2)−t^2(t^3))\,\hat{\mathbf{k}}} \\[5pt] & \mathrm{=(t^3−t^5)\,\hat{\mathbf{i}}+(t^6−t^2)\,\hat{\mathbf{j}}+(t^3−t^5)\,\hat{\mathbf{k}}.} \end{align*} \]
Next, substitute this back into the integral and integrate:\[\begin{align*} \mathrm{\int [⟨t,t^2,t^3⟩ \times ⟨t^3,t^2,t⟩]dt \;} & \mathrm{ = \int (t^3−t^5) \,\hat{\mathbf{i}}+(t^6−t^2) \,\hat{\mathbf{j}}+(t^3−t^5)\,\hat{\mathbf{k}}dt} \\[5pt] & \mathrm{=(\dfrac{t^4}{4}−\dfrac{t^6}{6})\,\hat{\mathbf{i}}+(\dfrac{t^7}{7}−\dfrac{t^3}{3})\,\hat{\mathbf{j}}+(\dfrac{t^4}{4}−\dfrac{t^6}{6})\,\hat{\mathbf{k}}+\vecs C.} \end{align*}\]
 Use the second part of the definition of the integral of a space curve:
\[\begin{align*} \mathrm{\int_0^{\dfrac{\pi}{3}} [\sin 2t \,\hat{\mathbf{i}}+ \tan t \,\hat{\mathbf{j}}+e^{−2t} \,\hat{\mathbf{k}}]dt} & \mathrm{=\left[\int_0^{\dfrac{π}{3}} \sin 2t dt \right] \,\hat{\mathbf{i}}+ \left[ \int_0^{\dfrac{π}{3}} \tan t dt \right] \,\hat{\mathbf{j}}+\left[\int_0^{\dfrac{π}{3}}e^{−2t}dt \right] \,\hat{\mathbf{k}}} \\[5pt] & \mathrm{= (−12 \cos 2t) \vert_{0}^{π/3} \,\hat{\mathbf{i}}−( \ln (\cos t))\vert_{0}^{π/3} \,\hat{\mathbf{j}}−(\dfrac{1}{2}e^{−2t})\vert_{0}^{π/3} \,\hat{\mathbf{k}}} \\[5pt] & \mathrm{=(−\dfrac{1}{2} \cos \dfrac{2π}{3}+\dfrac{1}{2} \cos 0) \,\hat{\mathbf{i}}−( \ln ( \cos \dfrac{π}{3})− \ln( \cos 0)) \,\hat{\mathbf{j}}−( \dfrac{1}{2}e^{−2π/3}−\dfrac{1}{2}e^{−2(0)}) \,\hat{\mathbf{k}}} \\[5pt] & \mathrm{=(\dfrac{1}{4}+\dfrac{1}{2}) \,\hat{\mathbf{i}}−(−\ln 2) \,\hat{\mathbf{j}}−(\dfrac{1}{2}e^{−2π/3}−\dfrac{1}{2}) \,\hat{\mathbf{k}}} \\[5pt] & \mathrm{=\dfrac{3}{4}\,\hat{\mathbf{i}}+(\ln 2) \,\hat{\mathbf{j}}+(\dfrac{1}{2}−\dfrac{1}{2}e^{−2π/3})\,\hat{\mathbf{k}}.} \end{align*}\]
Exercise \(\PageIndex{5}\)
Calculate the following integral:
\[\int_1^3 [(2t+4) \,\hat{\mathbf{i}}+(3t^2−4t) \,\hat{\mathbf{j}}]dt \nonumber\]
 Hint

Use the definition of the definite integral of a plane curve.
 Answer

\[\int_1^3 [(2t+4) \,\hat{\mathbf{i}}+(3t^2−4t) \,\hat{\mathbf{j}}]dt = 16 \,\hat{\mathbf{i}}+10 \,\hat{\mathbf{j}} \nonumber\]
Integration in the Context of Motion
Above, we defined velocity as the derivative of position and acceleration as the derivative of velocity. Integration allows us to go the other way! As you learned in first semester calculus, integration allows us to generate an object's velocity as a function of time given its acceleration and an initial velocity. We can also find the object's position function by integrating the velocity and using an initial position.
Let's consider an example.
Example \(\PageIndex{8}\): Finding an object's velocity from its acceleration
An object has an acceleration over time given by \(\vecs a(t) = \sin t \,\hat{\mathbf i}  2t \,\hat{\mathbf j}\), and it's initial velocity was \(\vecs v(0) = 2 \,\hat{\mathbf i} + \,\hat{\mathbf j}\).
a. Find the object's velocity as a function of time.
b. Assuming the object was located at the point (2, 3, 1) when time \(t = 0\), determine the object's position function and find its location at time \(t = 3\) sec.
Solution
a. First, we find the velocity as the antiderivative of the acceleration.
\[\begin{align*} \vecs v(t) = \int \vecs a(t) \, dt &= \int \left( \sin t \,\hat{\mathbf i}  2t \,\hat{\mathbf j}\right)\,dt \\
&= \cos t \,\hat{\mathbf i}  t^2\,\hat{\mathbf j} + \vecs C_1 \end{align*}\]
Now we use the initial velocity to determine \(\vecs C_1\).
\[\begin{align*} \vecs v(0) = \cos 0 \,\hat{\mathbf i}  (0)^2\,\hat{\mathbf j} + \vecs C_1 &= 2 \,\hat{\mathbf i} + \,\hat{\mathbf j} \\
\hat{\mathbf i} + \vecs C_1 &= 2 \,\hat{\mathbf i} + \,\hat{\mathbf j} \\ \\
\text{And so} \quad \vecs C_1 &= 3 \,\hat{\mathbf i} + \,\hat{\mathbf j} \end{align*}\]
Incorporating this constant vector into our velocity function from above, we obtain the velocity describing this object's motion over time:
\[\vecs v(t) = \left( 3 \cos t \right) \,\hat{\mathbf i} + \left(1  t^2\right) \,\hat{\mathbf j}\]
b. Since the object's position is at the point (2, 3, 1) when time \(t = 0\), we know \(\vecs r(0) = 2 \,\hat{\mathbf i} + 3 \,\hat{\mathbf j}  \,\hat{\mathbf k}\).
Now, to determine the object's position function, we integrate it's velocity.
\[\begin{align*} \vecs r(t) = \int \vecs v(t) \, dt &= \int \bigg[\left( 3 \cos t \right) \,\hat{\mathbf i} + \left(1  t^2\right) \,\hat{\mathbf j}\bigg]\,dt \\
&= \left( 3t \sin t \right) \,\hat{\mathbf i} + \left(t  \frac{t^3}{3}\right) \,\hat{\mathbf j} + \vecs C_2 \end{align*}\]
Now we use the initial position to determine \(\vecs C_2\).
\[\begin{align*} \vecs r(0) = \left( 3(0) \sin 0 \right) \,\hat{\mathbf i} + \left( 0  \frac{(0)^3}{3}\right) \,\hat{\mathbf j} + \vecs C_2 &= 2 \,\hat{\mathbf i} + 3 \,\hat{\mathbf j}  \,\hat{\mathbf k}\\ \\ \text{And so} \quad \vecs C_2 &= 2 \,\hat{\mathbf i} + 3 \,\hat{\mathbf j}  \,\hat{\mathbf k} \end{align*}\]
Incorporating this constant vector into our position function from above, we obtain:
\[\vecs r(t) = \left( 2 + 3t \sin t \right) \,\hat{\mathbf i} + \left(3 + t  \frac{t^3}{3}\right) \,\hat{\mathbf j}  \,\hat{\mathbf k} \]
To find the object's position at time \(t = 3\) seconds, we just evaluate this position function at \(t = 3\).
\[\begin{align*} \vecs r(3) &= \left( 2 + 3(3) \sin 3 \right) \,\hat{\mathbf i} + \left(3 + 3  \frac{(3)^3}{3}\right) \,\hat{\mathbf j}  \,\hat{\mathbf k} \\
&= \left( 11 \sin 3 \right) \,\hat{\mathbf i}  3 \,\hat{\mathbf j}  \,\hat{\mathbf k} \end{align*}\]
This position vector indicates that the object will be located at the point \( (11 \sin 3, 3, 1) \) at time \(t = 3\) seconds.
The Meaning of Definite Integrals of VectorValued Functions
Now let's turn our attention to the meaning of a definite integral of a vectorvalued function. The context in which this will make the most sense is where the function we integrate is a velocity function. That is,
\[\int_a^b \vecs v(t) \, dt\]
We know that the antiderivative of velocity is position and that this definite integral gives us the change in position over the time interval, \(a \le t\le b\). In other words,
\[\int_a^b \vecs v(t) \, dt = \vecs r(b)  \vecs r(a)\]
Thus, the definite integral of velocity over a time interval \(a \le t\le b\) gives us the displacement vector that indicates the change in position over this time interval.
In general, the definite integral
\(\displaystyle \int_a^b \vecs r(t) \, dt = \vecs q(b)  \vecs q(a)\), where \(\vecs q(t)\) is the antiderivative of \(\vecs r(t)\),
gives us a change in the antiderivative of our vectorvalued function over the given inteval \([a,b]\). This will always be a constant vector that would fit from tip to tip of the vectors given by the antiderivative function at \(t = a\) and \(t = b\), respectively (assuming the vectors were placed in standard position).
Summary
 To calculate the derivative of a vectorvalued function, calculate the derivatives of the component functions, then put them back into a new vectorvalued function.
 Many of the properties of differentiation of scalar fundtions also apply to vectorvalued functions.
 The derivative of a vectorvalued function \(r(t)\) is also a tangent vector to the curve. The unit tangent vector \(T(t)\) is calculated by dividing the derivative of a vectorvalued function by its magnitude.
 The antiderivative of a vectorvalued function is found by finding the antiderivatives of the component functions, then putting them back together in a vectorvalued function.
 The definite integral of a vectorvalued function is found by finding the definite integrals of the component functions, then putting them back together in a vectorvalued function.
Key Equations
 Derivative of a vectorvalued function\[\vecs r′(t) = \lim \limits_{\Delta t \to 0} \dfrac{\vecs r(t+\Delta t)−\vecs r(t)}{ \Delta t} \nonumber\]
 Principal unit tangent vector \[\vecs T(t)=\frac{\vecs r′(t)}{‖\vecs r′(t)‖}\]
 Indefinite integral of a vectorvalued function \[\int [f(t) \,\hat{\mathbf{i}}+g(t)\,\hat{\mathbf{j}} + h(t) \,\hat{\mathbf{k}}]dt= \left[ \int f(t)dt \right] \,\hat{\mathbf{i}}+ \left[ \int g(t)dt \right] \,\hat{\mathbf{j}} + \left[ \int h(t)dt \right] \,\hat{\mathbf{k}}\nonumber\]
 Definite integral of a vectorvalued function \[\int_a^b [f(t) \,\hat{\mathbf{i}}+g(t) \,\hat{\mathbf{j}} + h(t) \,\hat{\mathbf{k}}]dt= \left[\int_a^b f(t)dt \right] \,\hat{\mathbf{i}}+ \left[ \int _a^b g(t)dt \right] \,\hat{\mathbf{j}} + \left[ \int _a^b h(t)dt \right] \,\hat{\mathbf{k}}\nonumber\]
Glossary
 definite integral of a vectorvalued function
 the vector obtained by calculating the definite integral of each of the component functions of a given vectorvalued function, then using the results as the components of the resulting function
 derivative of a vectorvalued function
 the derivative of a vectorvalued function \(\vecs{r}(t)\) is \(\vecs{r}′(t) = \lim \limits_{\Delta t \to 0} \frac{\vecs r(t+\Delta t)−\vecs r(t)}{ \Delta t}\), provided the limit exists
 indefinite integral of a vectorvalued function
 a vectorvalued function with a derivative that is equal to a given vectorvalued function
 principal unit tangent vector
 a unit vector tangent to a curve C
 tangent vector
 to \(\vecs{r}(t)\) at \(t=t_0\) any vector \(\vecs v\) such that, when the tail of the vector is placed at point \(\vecs r(t_0)\) on the graph, vector \(\vecs{v}\) is tangent to curve C
Contributors
Gilbert Strang (MIT) and Edwin “Jed” Herman (Harvey Mudd) with many contributing authors. This content by OpenStax is licensed with a CCBYSANC 4.0 license. Download for free at http://cnx.org.
 Paul Seeburger (Monroe Community College) edited this section and added content on visualizing the derivative of a vectorvalued function and content on smooth vectorvalued functions.