Chapter 12: Problem 9
The speedometer on your car reads a steady 35 mph. Could you be accelerating? Explain.
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Chapter 12: Problem 9
The speedometer on your car reads a steady 35 mph. Could you be accelerating? Explain.
These are the key concepts you need to understand to accurately answer the question.
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Write a in the form \(\mathbf{a}=a_{\mathrm{T}} \mathbf{T}+a_{\mathrm{N}} \mathbf{N}\) without finding T and N. $$\mathbf{r}(t)=(1+3 t) \mathbf{i}+(t-2) \mathbf{j}-3 t \mathbf{k}$$
Solve the initial value problems for \(\mathbf{r}\) as a vector function of \(t.\) Differential equation:\(\frac{d \mathbf{r}}{d t}=\left(t^{3}+4 t\right) \mathbf{i}+t \mathbf{j}+2 t^{2} \mathbf{k}\)Initial condition: \(\quad \mathbf{r}(0)=\mathbf{i}+\mathbf{j}\)
a. Show that \(d \mathbf{B} / d s\) is orthogonal to \(\mathbf{T}\) and to \(\mathbf{B}\). b. Deduce from (a) that \(d \mathbf{B} / d s\) is parallel to \(\mathbf{N},\) so \(d \mathbf{B} / d s\) is a scalar multiple of N. Traditionally, we write $$\frac{d \mathbf{B}}{d s}=-\tau \mathbf{N}$$ The scalar \(\tau\) is called the torsion along the curve and may be positive, negative, or zero.
Find \(\mathbf{T}, \mathbf{N},\) and \(\kappa\) for the space curves. $$\mathbf{r}(t)=(3 \sin t) \mathbf{i}+(3 \cos t) \mathbf{j}+4 t \mathbf{k}$$
The eccentricity of Earth's orbit is \(e=0.0167,\) so the orbit is nearly circular, with radius approximately \(150 \times 10^{6} \mathrm{km}\). Find, in units of \(\mathrm{km}^{2} /\) sec, the rate \(d A /\) d \(t\) satisfying Kepler's second law.
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