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Find \(\mathbf{T}, \mathbf{N},\) and \(\kappa\) for the space curves. \(\mathbf{r}(t)=(3 \sin t) \mathbf{i}+(3 \cos t) \mathbf{j}+4 t \mathbf{k}\)

Short Answer

Expert verified
\( \mathbf{T}(t) = \left(\frac{3}{5} \cos t\right) \mathbf{i} - \left(\frac{3}{5} \sin t\right) \mathbf{j} + \frac{4}{5} \mathbf{k} \), \( \mathbf{N}(t) = -\sin t \mathbf{i} - \cos t \mathbf{j} \), \( \kappa = \frac{3}{25} \)

Step by step solution

01

Differentiate the Position Vector

To find the tangent vector \( \mathbf{T} \), we first need to differentiate the position vector \( \mathbf{r}(t) \).\[ \mathbf{r}'(t) = \frac{d}{dt} ((3 \sin t) \mathbf{i} + (3 \cos t) \mathbf{j} + 4t \mathbf{k}) = (3 \cos t) \mathbf{i} - (3 \sin t) \mathbf{j} + 4 \mathbf{k} \]
02

Find the Tangent Vector \( \mathbf{T} \)

The tangent vector \( \mathbf{T} \) is the unit vector in the direction of \( \mathbf{r}'(t) \). \[ \mathbf{T}(t) = \frac{\mathbf{r}'(t)}{\|\mathbf{r}'(t)\|} \] First, find the magnitude of \( \mathbf{r}'(t) \):\[ \|\mathbf{r}'(t)\| = \sqrt{(3 \cos t)^2 + (-3 \sin t)^2 + 4^2} = \sqrt{9 \cos^2 t + 9 \sin^2 t + 16} = \sqrt{25} = 5 \] Thus,\[ \mathbf{T}(t) = \frac{(3 \cos t) \mathbf{i} - (3 \sin t) \mathbf{j} + 4 \mathbf{k}}{5} = \left(\frac{3}{5} \cos t\right) \mathbf{i} - \left(\frac{3}{5} \sin t\right) \mathbf{j} + \frac{4}{5} \mathbf{k} \]
03

Differentiate the Tangent Vector

Differentiate the tangent vector \( \mathbf{T}(t) \) with respect to \( t \):\[ \mathbf{T}'(t) = \frac{d}{dt}\left(\frac{3}{5} \cos t \mathbf{i} - \frac{3}{5} \sin t \mathbf{j} + \frac{4}{5} \mathbf{k}\right) = \left(-\frac{3}{5} \sin t\right) \mathbf{i} - \left(\frac{3}{5} \cos t\right) \mathbf{j} \]
04

Find the Normal Vector \( \mathbf{N} \)

The normal vector \( \mathbf{N} \) is the unit vector in the direction of \( \mathbf{T}'(t) \). First, find the magnitude of \( \mathbf{T}'(t) \):\[ \|\mathbf{T}'(t)\| = \sqrt{\left(-\frac{3}{5} \sin t\right)^2 + \left(-\frac{3}{5} \cos t\right)^2} = \sqrt{\frac{9}{25} (\sin^2 t + \cos^2 t)} = \sqrt{\frac{9}{25}} = \frac{3}{5} \] Thus, the normal vector is:\[ \mathbf{N}(t) = \frac{\mathbf{T}'(t)}{\|\mathbf{T}'(t)\|} = \frac{\left(-\frac{3}{5} \sin t\right) \mathbf{i} - \left(\frac{3}{5} \cos t\right) \mathbf{j}}{\frac{3}{5}} = -\sin t \mathbf{i} - \cos t \mathbf{j} \]
05

Calculate the Curvature \( \kappa \)

The curvature \( \kappa \) is given by \( \kappa = \frac{\|\mathbf{T}'(t)\|}{\|\mathbf{r}'(t)\|} \). Thus,\[ \kappa = \frac{\frac{3}{5}}{5} = \frac{3}{25} \]

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Tangent Vector
A tangent vector is a vector that represents the direction of a curve at a particular point. Imagine you're walking along a winding path: the tangent vector is like an arrow pointing in the direction you're currently heading. It provides a snapshot of the curve's direction at any particular point along it.

In mathematical terms, if we have a space curve represented by a position vector function \( \mathbf{r}(t) \), the tangent vector \( \mathbf{T}(t) \) at any point is the derivative of \( \mathbf{r}(t) \) normalized. This means we first find \( \mathbf{r}'(t) \), the derivative of the position vector. For our example curve, \( \mathbf{r}'(t) = (3 \cos t) \mathbf{i} - (3 \sin t) \mathbf{j} + 4 \mathbf{k} \).

Next, we find the magnitude of \( \mathbf{r}'(t) \):
\[ \| \mathbf{r}'(t) \| = \sqrt{(3 \cos t)^2 + (-3 \sin t)^2 + 4^2} = 5 \]
This magnitude helps us convert \( \mathbf{r}'(t) \) into a unit vector, \( \mathbf{T}(t) \), which is calculated as:
\[ \mathbf{T}(t) = \frac{(3 \cos t) \mathbf{i} - (3 \sin t) \mathbf{j} + 4 \mathbf{k}}{5} \]
Thus, giving a precise, length-wise direction along the curve.
Normal Vector
The normal vector is another important concept when studying curves. While the tangent vector tells us in which direction the curve moves, the normal vector indicates the direction in which the curve is changing. It's like knowing which way the road curves as you drive around a bend.

To find the normal vector \( \mathbf{N}(t) \), we first need to differentiate the tangent vector \( \mathbf{T}(t) \). For our curve, that means computing:\(\[ \mathbf{T}'(t) = \frac{d}{dt}\left(\frac{3}{5} \cos t \mathbf{i} - \frac{3}{5} \sin t \mathbf{j} + \frac{4}{5} \mathbf{k}\right) = \left(-\frac{3}{5} \sin t\right) \mathbf{i} - \left(\frac{3}{5} \cos t\right) \mathbf{j} \] \)
Next, we determine the magnitude of \( \mathbf{T}'(t) \) to convert it into a unit vector:
\(\[ \|\mathbf{T}'(t)\| = \sqrt{\left(-\frac{3}{5} \sin t\right)^2 + \left(-\frac{3}{5} \cos t\right)^2} = \frac{3}{5} \] \)
This allows us to express \( \mathbf{N}(t) \) as:
\[\mathbf{N}(t) = \frac{\mathbf{T}'(t)}{\|\mathbf{T}'(t)\|} = -\sin t \mathbf{i} - \cos t \mathbf{j} \]
This unit vector highlights how the path is curving at any given point.
Curvature
Curvature is a measure of how rapidly a curve changes direction. High curvature means a sharp turn, like a hairpin bend on a racetrack.

Mathematically, curvature \( \kappa \) for a space curve is found using the relationship:
\[\kappa = \frac{\| \mathbf{T}'(t) \|}{\| \mathbf{r}'(t) \|}\]
For our specific curve, we already know that:
\( \|\mathbf{T}'(t)\| = \frac{3}{5} \)
and \( \|\mathbf{r}'(t)\| = 5 \).
Plugging these values into our formula gives:
\[\kappa = \frac{\frac{3}{5}}{5} = \frac{3}{25} \]
This number remains constant along the curve, indicating a uniform rate of bending in space.

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Most popular questions from this chapter

Solve the initial value problems in Exercises \(27-32\) for \(r\) as a vector function of \(t .\) $$ \begin{array}{ll}{\text { Differential equation: }} & {\frac{d \mathbf{r}}{d t}=\left(t^{3}+4 t\right) \mathbf{i}+t \mathbf{j}+2 t^{2} \mathbf{k}} \\\ {\text { Initial condition: }} & {\mathbf{r}(0)=\mathbf{i}+\mathbf{j}}\end{array} $$

Find \(\mathbf{T}, \mathbf{N},\) and \(\kappa\) for the space curves. \(\mathbf{r}(t)=\left(\cos ^{3} t\right) \mathbf{i}+\left(\sin ^{3} t\right) \mathbf{j}, \quad 0< t<\pi / 2\)

Find \(\mathbf{T}, \mathbf{N},\) and \(\kappa\) for the space curves. \(\mathbf{r}(t)=t \mathbf{i}+(a \cosh (t / a)) \mathbf{j}, \quad a>0\)

In Exercises 16 and \(17,\) two planets, planet \(A\) and planet \(B\) , are orbiting their sun in circular orbits with \(A\) being the inner planet and \(B\) being farther away from the sun. Suppose the positions of \(A\) and \(B\) at time \(t\) are $$ \mathbf{r}_{A}(t)=2 \cos (2 \pi t) \mathbf{i}+2 \sin (2 \pi t) \mathbf{j} $$ and $$ \mathbf{r}_{B}(t)=3 \cos (\pi t) \mathbf{i}+3 \sin (\pi t) \mathbf{j} $$ respectively, where the sun is assumed to be located at the origin and distance is measured in astronomical units. (Notice that planet \(A\) moves faster than planet \(B . )\) The people on planet \(A\) regard their planet, not the sun, as the center of their planetary system (their solar system). Using planet \(A\) as the origin, graph the path of planet \(B .\) This exercise illustrates the difficulty that people before Kepler's time, with an earth- centered (planet \(A\) ) view of our solar system, had in understanding the motions of the planets (i.e., planet \(B=\) Mars). See D. G. Saari's article in the American Mathematical Monthly, Vol. 97 (Feb. \(1990 ),\) pp. \(105-119\) .

Antiderivatives of vector functions a. Use Corollary 2 of the Mean Value Theorem for scalar functions to show that if two vector functions \(\mathbf{R}_{1}(t)\) and \(\mathbf{R}_{2}(t)\) have identical derivatives on an interval \(I\) , then the functions differ by a constant vector value throughout \(I .\) b. Use the result in part (a) to show that if \(\mathbf{R}(t)\) is any anti- derivative of \(\mathbf{r}(t)\) on \(I,\) then any other antiderivative of \(\mathbf{r}\) on \(I\) equals \(\mathbf{R}(t)+\mathbf{C}\) for some constant vector \(\mathbf{C}\) .

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