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Find the osculating circle at the given points. $$\mathbf{r}(t)=\left\langle t, t^{2}\right\rangle \text { at } t=0$$

Short Answer

Expert verified
The osculating circle at \(t=0\) for the curve \(\mathbf{r}(t)=\langle t, t^{2}\rangle\) has a radius \(\frac{1}{2}\) and a center at \( (0.5,0)\).

Step by step solution

01

Find the First and Second Derivatives

Start by finding the first and second derivatives of the given vector function \(\mathbf{r}(t)=\langle t, t^{2}\rangle\) with respect to \(t\). For the first derivative we find \(\mathbf{r}'(t)=\langle 1, 2t\rangle\). The second derivative is \(\mathbf{r}''(t)=\langle 0, 2\rangle\).
02

Calculate the Magnitudes

Next, we calculate the magnitudes of these two derivative vectors. The magnitude of \(\mathbf{r}'(t)\) is \(\|\mathbf{r}'\|=\sqrt{(1)^2+(2t)^2}\) and the magnitude of \(\mathbf{r}''(t)\) is \(\|\mathbf{r}''\|\)=|\(2\)|.
03

Compute the Curvature

The formula to compute curvature \(k\) is given by \(k= \frac{\|\mathbf{r}' \times \mathbf{r}''\|}{\|\mathbf{r}'\|^3}\). We use the formula to get \(k= \frac{\|\mathbf{r}' \times \mathbf{r}''\|}{\|\mathbf{r}'\|^3} = \frac{|2|}{|(1)^2+(2*0)^2|^{3/2}}=\frac{2}{1}=2\). Thus, the curvature at \(t=0\) is \(2\).
04

Find the Radius of the Osculating Circle

The radius \(R\) of the osculating circle is the reciprocal of the curvature, so \(R = \frac{1}{k} = \frac{1}{2}\).
05

Calculate the Center of the Osculating Circle

Using the formula for the center \(\mathbf{C}=\mathbf{r}+\frac{1}{k}\mathbf{N}\), where \(\mathbf{N}\) is the unit normal vector given by \(\mathbf{N}=\frac{\mathbf{r}' \times \mathbf{r}''}{\|\mathbf{r}' \times \mathbf{r}''\|}\), we can find the center. Since at \(t=0\), \(\mathbf{r}=\langle 0, 0\rangle\), \(\mathbf{r}'=\langle 1, 0\rangle\), and \(\mathbf{r}''=\langle 0, 2\rangle\), we have \(\mathbf{C}=\langle 0, 0\rangle + \frac{1}{2}\langle 1, 0\rangle = \langle 0.5, 0\rangle\). Thus, the center of the osculating circle is at \( (0.5,0)\).

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Key Concepts

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

Curvature Calculation
Understanding curvature is essential for students delving into higher-level calculus, especially in the study of the geometry of curves. Curvature, denoted as \( k \), is a measure of how sharply a curve bends at a particular point. To picture this, imagine the steering wheel of a car: the tighter you turn it, the sharper the car bends on its path. The same goes for a curve—the greater the curvature, the more pronounced the turn.

To calculate curvature for a vector function like \( \mathbf{r}(t)=\t)\), first, we compute the first and second derivatives of \( \mathbf{r}(t) \), capturing the slope and acceleration of the curve, respectively. The formula used is \( k = \frac{\|\mathbf{r}' \times \mathbf{r}''\|}{\|\mathbf{r}'\|^3} \), where \( \times \) denotes the cross product, and \( \| \cdot \| \) denotes the magnitude (or length) of a vector.

The cross product measures the vector orthogonal to \( \mathbf{r}'\) and \( \mathbf{r}''\), and its magnitude corresponds to the area of the parallelogram spanned by these vectors. Dividing by the cube of the magnitude of \( \mathbf{r}'\) ensures that curvature is dimensionless and only related to the shape, not the size of the curve.
Vector Functions Derivatives
Vector functions are functions that have vectors as outputs, and taking their derivatives involves finding the change in each component of the vector with respect to the input variable. In our case, the vector function \( \mathbf{r}(t) \) has two components: one depending linearly on \( t \) and the other quadratically on \( t \).

When we differentiate \( \mathbf{r}(t) \) with respect to \( t \), we find two new vectors: the velocity vector \( \mathbf{r}'(t) \) which shows the direction and speed of movement along the curve, and the acceleration vector \( \mathbf{r}''(t) \) indicating how the speed changes.

Linking Derivatives and Curvature

The link between these derivatives and curvature is intuitive: the velocity tells us how fast the curve's position is changing, while the acceleration shows how fast the velocity itself is changing. If you’re turning a car, the speed tells you how fast you're going, and the rate at which you rotate the wheel (akin to acceleration) tells you how sharply you're starting to turn—a parallel to how curvature measures a curve’s sharpness.
Radius of Curvature
The radius of curvature, \( R \), closely relates to the concept of curvature, and it describes the radius of the so-called osculating circle at a particular point on the curve—the circle that 'kisses' the curve just at that point and aligns perfectly with the curve's direction and bending. The term 'osculating' is derived from the Latin 'osculare', meaning 'to kiss', depicting the circle's gentle touch with the curve.

The formula for the radius is given by \( R = \frac{1}{k} \), signifying an inverse relationship between the radius and the curvature. A smaller radius corresponds to a sharper bend (high curvature), while a larger radius implies a gentle bend (low curvature).

To illustrate, imagine driving in a circle: The tighter the circle, the sharper you have to turn the wheel, and conversely, a wide curve requires less turning. In calculus, the radius of curvature provides a quantitative way to describe this turning and is particularly useful for engineers and scientists analyzing the motion of objects along curved paths.

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Most popular questions from this chapter

Example 3.3 is a model of a satellite orbiting the earth. In this case, the force \(\mathbf{F}\) is the gravitational attraction of the earth on the satellite. The magnitude of the force is \(\frac{m M G}{b^{2}}\), where \(m\) is the mass of the satellite, \(M\) is the mass of the earth and \(G\) is the universal gravitational constant. Using example 3.3 , this should be equal to \(m \omega^{2} b .\) For a geosynchronous orbit, the frequency \(\omega\) is such that the satellite completes one orbit in one day. (By orbiting at the same rate as the earth spins, the satellite can remain directly above the same point on the earth.) For a sidereal day of 23 hours, 56 minutes and 4 seconds, find \(\omega\) Using \(M G \approx 39.87187 \times 10^{13} \mathrm{N}-\mathrm{m}^{2} / \mathrm{kg},\) find \(b\) for a geosynchronous orbit (the units of \(b\) will be \(\mathrm{m}\) ).

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