-1
$\begingroup$

Given a position function of a particle: $$ \mathbf r=r\,\hat{\mathbf r}\left(\theta\right), $$ where $\hat{\mathbf r}(θ)$ is the polar unit vector, to find the velocity, we take the derivative which results in:

$$ \mathbf v = \frac{\mathrm d\mathbf r}{\mathrm dt} = \frac{\mathrm dr}{\mathrm dt} \hat{\mathbf r}(θ) + r\frac{\mathrm d\hat{\mathbf r}(θ)}{\mathrm dt}.$$

What does each term in the velocity equation mean?

$\endgroup$
4
  • $\begingroup$ r^(θ) is a unit vector that gives you the direction of the vector, and r gives the magnitude. I don't know of a reason to include the time derivative of the direction, so the second part of your velocity equation looks very suspect. $\endgroup$ Commented Aug 2, 2018 at 2:15
  • $\begingroup$ @DavidWhite No it does not look suspect to me at least. Without it there could be no velocity in the theta direction. I wonder if another (or perhaps better) name for $d\mathbf{\hat{r}}(\theta)/dt$ is just $\mathbf{\hat{\theta}} d\theta /dt$ or something similar? $\endgroup$
    – uhoh
    Commented Aug 2, 2018 at 2:58
  • $\begingroup$ Can you change the title to something more descriptive? $\endgroup$
    – user191954
    Commented Aug 2, 2018 at 6:09
  • $\begingroup$ Chair, your picture and brief write-up are a real HOOT! $\endgroup$ Commented Aug 2, 2018 at 18:17

1 Answer 1

1
$\begingroup$

You've made things a bit more complicated than they need to be by introducing the unspecified parameter $\theta$. So let's get rid of it and write $$\boldsymbol r(t) = r(t)\,\hat{\boldsymbol r}(t)$$ Taking the derivative with respect to time yields $$\frac{d\,\boldsymbol r(t)}{dt} = \frac{dr}{dt}\,\hat{\boldsymbol r}(t) + r(t)\frac{d\,\hat{\boldsymbol r}(t)}{dt}$$ The first term is the radial component of velocity and the second is the tangential component.

Given any two vectors, one can always express the second vector as comprising two components, one that is parallel to the first and another that is orthogonal to the first. This is exactly what is happening here: The first term ($\dot r\,\hat {\boldsymbol r}$) is necessarily parallel to the position vector while the second ($r \dot{\hat {\boldsymbol r}}$) is necessarily orthogonal to the position vector.

Now I'll reintroduce the intermediate parameter $\theta$. Suppose that $\boldsymbol r$ depends directly on $\theta$ only: $$\boldsymbol r(\theta) = r(\theta)\,\hat{\boldsymbol r}(\theta)$$ For example, $$\begin{aligned} r(\theta) &= \frac{a(1-e^2)}{1-e\cos\theta} \\ \hat{\boldsymbol r}(\theta) &= \cos\theta\,\hat{\boldsymbol x}+\sin\theta\,\hat{\boldsymbol y} \end{aligned}$$ Assuming $\theta$ varies with time, this describes an elliptical orbit about the origin. Differentiating with respect to time yields $$\frac{d\,\boldsymbol r(t)}{dt} = \frac{dr}{d\theta}\frac{d\theta}{dt}\,\hat{\boldsymbol r}(\theta) + r(\theta)\frac{d\,\hat{\boldsymbol r}(\theta)}{d\theta}\frac{d\theta}{dt}$$ As was the case where $r$ depended directly on $t$ only, the first term is necessarily parallel to the position vector while the second is necessarily orthogonal to the position vector.

$\endgroup$

Your Answer

By clicking “Post Your Answer”, you agree to our terms of service and acknowledge you have read our privacy policy.

Not the answer you're looking for? Browse other questions tagged or ask your own question.