Page:Scientific Papers of Josiah Willard Gibbs - Volume 2.djvu/139

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DETERMINATION OF ELLIPTIC ORBITS
123

This gives[1]

(20)

From the corrected values of we may calculate a new residual and from that determine another correction for each of the quantities

It will sometimes be worth while to use formulæ a little less simple for the sake of a more rapid approximation. Instead of equation (19) we may write, with a higher degree of accuracy,

(21)

where

(22)

It is evident that is generally many times greater than or the factor in the case of equal intervals, being exactly ten times as great as or This shows, in the first place, that the accurate determination of is of the most importance for the subsequent approximations. It also shows that we may attain nearly the same accuracy in writing

(23)

We may, however, often do a little better than this without using a more complicated equation. For may be estimated very roughly as equal to Whenever, therefore, and are about as large as as is often the case, it may be a little better to use the coefficient instead of in the last term.

For then, we have the equation

(24)

is easily computed from the formula

(25)

which may be derived from equations (18) and (22).

  1. These equations are obtained by taking the direct products of both members of the preceding equation with and respectively. See footnote on page 119.