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Find the binormal vector \(\mathbf{B}(t)=\mathbf{T}(t) \times \mathbf{N}(t)\) at \(t=0\) and \(t=1 .\) Also, sketch the curve traced out by \(r(t)\) and the vectors \(\mathbf{T}, \mathbf{N}\) and \(\mathbf{B}\) at these points. $$\mathbf{r}(t)=\langle 4 \cos \pi t, 4 \sin \pi t, t\rangle$$

Short Answer

Expert verified
The binormal vector B at t=0 is B(0) = [0,0,1] and at t=1 is B(1) = [0,0,-1].

Step by step solution

01

Find derivative of r(t)

Calculate the derivative of the given vector function. Differentiate each component of the vector function r(t) with respect to t.
02

Calculate Unit Tangent Vector T(t)

The unit tangent vector T(t) can be computed by normalizing the derivative of r(t). This is done by dividing the derivative of r(t) by its magnitude.
03

Compute the derivative of the Unit Tangent Vector T(t)

Take derivative of T(t) with respect to t.
04

Calculate Unit Normal Vector N(t)

The unit normal vector N(t) can be found by normalizing the derivative of T(t). This is done by dividing the derivative of T(t) by its magnitude.
05

Compute the Binormal Vector B(t)

Use the formula B(t) = T(t) x N(t) for calculating the Binormal vector. Apply the cross product operation to the Unit Tangent and Unit Normal vectors T(t) and N(t) respectively.
06

Evaluate Binormal Vector B(t) at t=0 and t=1

Substitute t=0 and t=1 into B(t) to calculate the binormal vector at these points.
07

Sketch the curve and vectors

Make a 3D sketch of the curve described by r(t) and the vectors T(t), N(t) and B(t). Remember to indicate the orientation of the curve and vectors at points t=0 and t=1.

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Key Concepts

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

Unit Tangent Vector
Understanding the unit tangent vector is crucial when working with curves in three dimensions. Think of it as a vector that "touches" the curve at a certain point, indicating the direction in which the curve is moving. To calculate the unit tangent vector, denoted as \( \mathbf{T}(t) \), you first need to differentiate the given vector function \( \mathbf{r}(t) \).
After finding the derivative, you normalize it. This means dividing the derivative by its magnitude, thereby ensuring it has a length of one.
This process results in a unit tangent vector that points in the direction of the curve without affecting the scale.
  • Differentiate \( \mathbf{r}(t) \) to get the tangent direction.
  • Normalize the result to ensure its unit length.

For the curve \( \mathbf{r}(t) = \langle 4 \cos(\pi t), 4 \sin(\pi t), t \rangle \), this method helps us find how the curve behaves and moves as \( t \) changes.
Unit Normal Vector
The unit normal vector, denoted \( \mathbf{N}(t) \), plays an essential role in understanding the curvature of a 3D curve. It is always perpendicular to the unit tangent vector.
To determine \( \mathbf{N}(t) \), start by differentiating the unit tangent vector \( \mathbf{T}(t) \). Next, you'll normalize this new vector.
This step is similar to how you found the unit tangent vector: dividing the derivative of \( \mathbf{T}(t) \) by its magnitude.
  • Begin by finding \( \frac{d}{dt}\mathbf{T}(t) \).
  • Normalize the result to keep the vector unit length.
  • Ensure it remains orthogonal to \( \mathbf{T}(t) \).

This orthogonal nature helps in visualizing and calculating how the curve's direction is changing at any point \( t \).
Cross Product
The cross product is an operation essential to finding the binormal vector, \( \mathbf{B}(t) \). When applied to two vectors, say \( \mathbf{a} \) and \( \mathbf{b} \), it results in a third vector, perpendicular to both.
For binormal vector calculation, you use the cross product between the unit tangent vector \( \mathbf{T}(t) \) and the unit normal vector \( \mathbf{N}(t) \).
This product gives a vector \( \mathbf{B}(t) \) that is orthogonal to the plane formed by \( \mathbf{T}(t) \) and \( \mathbf{N}(t) \), adding a third dimension to the understanding of the curve.
  • Use the cross product formula: \( \mathbf{B}(t) = \mathbf{T}(t) \times \mathbf{N}(t) \).
  • The resulting \( \mathbf{B}(t) \) is orthogonal to both initial vectors.

Cross products like this are vital in many geometrical and physical applications, where understanding orientation is important.
3D Vector Sketching
Sketching 3D vectors can be a powerful tool for visualizing the dynamics of curves. It helps observers see how aspects like direction and orientation change along the curve.
For the curve given by \( \mathbf{r}(t) \), consider sketching the curve itself along with the unit tangent, normal, and binormal vectors at points of interest (like \( t = 0 \) and \( t = 1 \)).
Here are a few tips:
  • Start with the basic curve, marking its path in space.
  • At key points such as \( t = 0 \) and \( t = 1 \), draw the \( \mathbf{T}(t) \), \( \mathbf{N}(t) \), and \( \mathbf{B}(t) \) vectors stemming from the curve.
  • Ensure each vector's direction and relative position accurately represent the results of your calculations.

This exercise not only demonstrates mathematical relationships but also helps solidify the understanding of how different vectors interact and orient in a 3D space.

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Most popular questions from this chapter

Find a parametric representation of the surface. The portion of \(z=4-x^{2}-y^{2}\) above the \(x y\) -plane

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The following three formulas (called the Frenet-Serret formulas) are of great significance in the field of differential geometry: a. \(\left.\frac{d \mathbf{T}}{d s}=\kappa \mathbf{N} \text { [equation }(5.2)\right]\) b. \(\frac{d \mathbf{B}}{d s}=-\tau \mathbf{N}(\text { see exercise } 42)\) c. \(\frac{d \mathbf{N}}{d s}=-\kappa \mathbf{T}+\tau \mathbf{B}\) Use the fact that \(\mathbf{N}=\mathbf{B} \times \mathbf{T}\) and the product rule [Theorem \(2.3(\mathrm{v})]\) to establish \((\mathrm{c})\)

To show that the surface in example 6.1 is the entire sphere \(x^{2}+y^{2}+z^{2}=4,\) start by finding the trace of the sphere in the plane \(z=k\) for \(-2 \leq k \leq 2 .\) If \(z=2 \cos v=k,\) determine as fully as possible the value of \(2 \sin v\) and then determine the trace in the plane \(z=k\) for \(x=2 \cos u \sin v, y=2 \sin u \sin v\) and \(z=2 \cos v .\) If the traces are the same, then the surfaces are the same.

In this exercise, we prove Kepler's third law. Recall that the area of the ellipse \(\frac{x^{2}}{a^{2}}+\frac{y^{2}}{b^{2}}=1\) is \(\pi a b .\) From exercise \(39,\) the rate at which area is swept out is given by \(\frac{d A}{d t}=\frac{1}{2}\|\mathbf{r} \times \mathbf{v}\|\) Conclude that the period of the orbit is \(T=\frac{\pi \bar{a} b}{\frac{1}{2}\|\mathbf{r} \times \mathbf{v}\|}\) and so, \(T^{2}=\frac{4 \pi^{2} a^{2} b^{2}}{\|\mathbf{r} \times \mathbf{v}\|^{2}} .\) Use (5.17) to show that the minimum value of \(r\) is \(r_{\min }=\frac{e d}{1+e}\) and that the maximum value of \(r\) is \(r_{\max }=\frac{e d}{1-e} .\) Explain why \(2 a=r_{\min }+r_{\max }\) and use this to show that \(a=\frac{e d}{1-e^{2}} .\) Given that \(1-e^{2}=\frac{b^{2}}{a^{2}},\) show that \(\frac{b^{2}}{a}=e d .\) From \(e=\frac{b}{G M}\) and \(d=\frac{c^{2}}{b},\) show that \(e d=\frac{\|\mathbf{r} \times \mathbf{v}\|^{2}}{G M} .\) It then follows that \(\frac{b^{2}}{a}=\frac{\|\mathbf{r} \times \mathbf{v}\|^{2}}{G M} .\) Finally, show that \(T^{2}=k a^{3},\) where the constant \(k=\frac{4 \pi^{2}}{G M}\) does not depend on the specific orbit of the planet.

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