Integral calculus: stellar stereography

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Discussion Overview

The discussion revolves around the application of integral calculus to stellar stereography, specifically focusing on the calculation of star density in a spherical cluster based on observed two-dimensional density. Participants explore various mathematical techniques, including integration by parts and trigonometric substitutions, to evaluate the integral involved in the problem.

Discussion Character

  • Mathematical reasoning, Technical explanation, Debate/contested

Main Points Raised

  • One participant presents the integral for perceived star density and seeks assistance with trigonometric substitution and limit changes.
  • Another participant reformulates the integral and suggests using integration by parts, providing specific substitutions for variables.
  • Subsequent posts detail the integration process, including the use of hyperbolic functions and identities, with varying approaches to changing limits and evaluating integrals.
  • There is a discussion about the correctness of expressions and terms, with some participants noting discrepancies in results, particularly regarding the presence of certain terms in the final expression.
  • Participants express confusion over notation, particularly the case of variables and limits, leading to further clarification attempts.

Areas of Agreement / Disagreement

Participants do not reach a consensus on the final form of the integral or the correctness of specific terms in their calculations. There are multiple competing views regarding the evaluation of the integral and the treatment of variables.

Contextual Notes

Limitations include unresolved mathematical steps, particularly in the integration process and the treatment of limits. The discussion reflects varying levels of understanding and approaches to the problem, with some participants expressing uncertainty about specific substitutions and identities.

Ciaran
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Hi there, I have a question I'm stuck on. It is:

Astronomers use a technique called stellar stereography to determine the density of stars in a star cluster
from the observed (two-dimensional) density that can be analysed from a photograph. Suppose that in
a spherical cluster of radius R the density of stars depends on ly on the distance r from the centre of
the cluster. If the perceived star density is given by y(s), where s is the observed planar distance from
the centre of the cluster, and x(r) is the actual density, it can be shown that

y(s) = integral from s to R of (2r x(r) dr)/ (r^2-s^2)^1/2 where x(r)=(1/2) ((R-r)^2)

I tried using the trig substitution r= s sec theta but haven't got far. I also am confused about how this substitution changes the limits. Can anyone please help?
 
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So, we are given:

$$y(s)=\int_s^R \frac{r(R-r)^2}{\sqrt{r^2-s^2}}\,dr$$

The first thing I see is that we have an improper integral, and so I would write:

$$y(s)=\lim_{s\to r}\left[\int_r^R \frac{w(R-w)^2}{\sqrt{w^2-s^2}}\,dw\right]$$

For the integral itself, I would try integration by parts, where:

$$u=(R-w)^2\,\therefore\,du=2(w-R)\,dw$$

$$dv=\frac{w}{\sqrt{w^2-s^2}}\,dw\,\therefore\,v=\sqrt{w^2-s^2}$$

Can you proceed?
 
So by integration by parts, we get

(R-w)^2 (w^2-s^2)^0.5- 2 \ int(w-R)*(w^2-s^2)^0.5 dw
 
Last edited:
Since it is a definite integral, we would get:

$$\left[(R-w)^2\sqrt{w^2-s^2}\right]_r^R-2\int_r^R(w-R)\sqrt{w^2-s^2}\,dw$$

And this reduces to:

$$(r-R)\sqrt{r^2-s^2}+2R\int_r^R\sqrt{w^2-s^2}\,dw-\int_r^R2w\sqrt{w^2-s^2}\,dw$$

For the first integral, I would suggest the substitution:

$$w=s\coth(u)$$

And for the second, I would try:

$$u=w^2-s^2$$
 
So for the first integral, it would be

integral from r to R of (s^2 (sqrt(coth^2u -1))(1-coth^2u) du?

And for the second I get

integral from r to R of 2 sqrt u du
 
Let's look first at the integral:

$$\int_r^R\sqrt{w^2-s^2}$$

If we let:

$$w=s\coth(u)$$

Then we find:

$$dw=-s\csch^2(u)\,du$$

And so the integral become:

$$s^2\int_{\arcoth\left(\frac{R}{s}\right)}^{\arcoth\left(\frac{r}{s}\right)}\csch^3(u)\,du$$

I would try playing with identities here to get a form you can integrate directly.

For the second integral, we would get:

$$\int_r^R2w\sqrt{w^2-s^2}\,dw$$

Let:

$$u=w^2-s^2$$

And so:

$$du=2w\,dw$$

And we have:

$$\int_{r^2-s^2}^{R^2-s^2}u^{\frac{1}{2}}\,du$$
 
How are you going about changing the limits? I also have never dealt with identities involving hyperbolic cubic functions
 
Ciaran said:
Hi there, I have a question I'm stuck on. It is:

$\vdots$

y(s) = integral from s to R of (2r x(r) dr)/ (r^2-s^2)^1/2 where x(r)=(1/2) ((R-r)^2)

I tried using the trig substitution r= s sec theta but haven't got far. I also am confused about how this substitution changes the limits. Can anyone please help?
I like your idea of substituting $r = s\sec\theta$. If you do that, you get $$\begin{aligned} y(s)=\int_s^R \frac{r(R-r)^2}{\sqrt{r^2-s^2}}\,dr &= \int_0^\Theta \frac{s\sec\theta(R - s\sec\theta)^2}{s\tan\theta}\cdot s\sec\theta\tan\theta\,d\theta \\ &= \int_0^\Theta \bigl( sR^2\sec^2\theta -2Rs^2\sec^3\theta + s^3\sec^4\theta\bigr)d\theta, \end{aligned}$$ where $\Theta = \arcsec\frac Rs$ (so that $\tan\Theta = \frac{\sqrt{R^2-s^2}}s$).

If you use the standard integrals $$\int\sec^2\theta\,d\theta = \tan\theta,$$ $$\int\sec^3\theta\,d\theta = \tfrac12\sec\theta\tan\theta + \tfrac12\ln \bigl|\,\sec\theta + \tan\theta\,\bigr|$$ and $$\int\sec^4\theta\,d\theta = \tfrac13\tan^3\theta + \tan\theta,$$ then you should be able to complete the calculation. I make the answer $$y(s) = \tfrac13\sqrt{R^2-s^2}\bigl(R^2 + 2s^2\bigr) - Rs^2\ln\biggl(\dfrac{R + \sqrt{R^2-s^2}}s\biggr).$$

[Mark is absolutely correct that the integral is improper and should really be evaluated as a limit. But in fact the integral converges, and by the time you have made the substitution $r = s\sec\theta$ the singularity has disappeared, because of the way that the $\tan\theta$ in the denominator of the integral cancels with the $\tan\theta$ coming from "$dr = s\sec\theta\tan\theta\,ds$".]
 
Last edited:
Hi there,

How come you changed the case of r to R in your expression for theta and the rest of the question but left it in the expression for tan of theta?
 
  • #10
Should it not be lowercase throughout as r= s sec theta implies theta= arcsec (r/s)?
 
  • #11
I get exactly the same except I don't get +2s^2; I get two s^2 terms but one is negative and they end up cancelling.
 
  • #12
Ciaran said:
Should it not be lowercase throughout as r= s sec theta implies theta= arcsec (r/s)?
It is lowercase when it is a variable, as in $r = s\sec\theta$, and it is upper case when it refers to the upper limit of the integral, $R = s\sec\Theta $.

Ciaran said:
I get exactly the same except I don't get +2s^2; I get two s^2 terms but one is negative and they end up cancelling.
I had $-\frac13s^2 + s^2 = \frac23s^2$. But I haven't been back to re-check it, so I may be wrong.
 

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