Numerical Investigation of the Formulae for the Elimination of Geocentric And Ba

Cover Numerical Investigation of the Formulae for the Elimination of Geocentric And Ba
Numerical Investigation of the Formulae for the Elimination of Geocentric And Ba
Sarah De Camp Morgan
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111. IV. V. VI. X 40. 668778 +0. 6697OO +0. 669871 4-0. 668780 +0. 669562 +0, 669853 a Y* -0. 565036 -0. 564561 *0. 564782 -0. 365000 -0. 564584 -0. 564489 Z +0. 125224 +0. 125908 +0. 125589 +0. 125217 +O. 125793 +0. 125997 X^ +0. 446200 +0. 443864 +0. 445037 +0. 446198 -0. 443721 +0. 443432 Y' +0. 347541 +0. 347166 +0. 347367 +0. 347548 +0. 347165 +0. 347085 Zl +1. 393368 +1. 393785 +1. 393542 +1. 393387 +1. 393897 +1. 393841 The following comparison* are of particular interest.
VI -V VI -IV 1
...-1V X, + 291 + 1073 - 2 Y^ + 101 +517 +36 2 +204 +760 +7 X ' -289 - 276S + 2 . - T' - 85 - 463 - i 2' + 216 + 454 - 19 The differences between Orbit IV and Orbit vl show that Orbit IV is correct only to two places. In the comparison of Orbit 1 and Orbit IV where the parallax is entirely neglected the differences are so small and at the same tine are within the errors of computation that it is quits evident that the partial elimination has no decided effect upon the orbit.
The differences between Orbit V and Vl where parallax - 13 is completely eliminated show that Orbit VI is correct to three places.


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