Date: Apr 27, 2009 8:22 AM
Author: David W. Cantrell
Subject: Re: A single term formula for calculating the circumference of ellipse
Shahram Zafary <shahram_zafary@yahoo.com> wrote:

> My formula for calculating the circumference of ellipse is attached as a

> small note. I will be grateful if you read and judge it.

>

> (See:

> http://mathforum.org/kb/servlet/JiveServlet/download/128-1921864-6683056-551607/circumference%20of%20an%20ellipse.pdf)

Congratulations on finding a nice approximation! (Concerning your note, I

should mention that your stated worst |rel. error| is overly pessimistic.

Instead of saying |rel. error| < 0.0017, you should have

said |rel. error| < 0.0013, but perhaps you simply made a typographical

mistake.)

A few comments:

In your formula, (pi/4) is raised to the power 4 a b/(a + b)^2. It is

interesting to note that that power can be written nicely in terms of the

geometric and arithmetic means of the semiaxes' lengths, namely, it is the

square of the ratio of those means: Letting gm = sqrt(a b) and

am = (a + b)/2 for brevity, your power can then be written as (gm/am)^2.

Your approximation formula for the perimeter of an ellipse could then be

written as

4 (a + b) (pi/4)^((gm/am)^2)

But the fact that the ratio of means is squared is not crucial to the

formula, and so it is natural to ask whether we could do "better" by

raising gm/am to some power p other than 2.

1) If our objective is to minimize worst |rel. error|, then, by numerical

methods, it can be determined that p = 2.016861... should be used. We then

obtain |rel. error| < 0.00078 . (Of course, a disadvantage of using

p = 2.016861... is that it's not as easily remembered as 2. But p could, if

desired, be rounded to 2.017 or approximated by the rational number 119/59;

in either case, worst |rel. error| would still be roughly 0.00078 .)

2) If our objective is to make the formula as accurate as possible for

nearly circular ellipses, then it can be shown that p = 1/(2 ln(4/pi)) =

2.0698... should be used and that, when eccentricity e is small, relative

error = (9 + 2/ln(pi/4))/16384 e^8 (1 + 2 e^2 +...). Of course, over all

eccentricities, worst |rel. error| is not so good, now being roughly 0.0028 . But this value of p gives us another feature which can often be useful:

We have an upper bound on the perimeter

4 (a + b) (pi/4)^((gm/am)^(1/(2 ln(4/pi)))) >= perimeter

with equality only when e = 0 or 1.

Best regards,

David W. Cantrell