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Gravitation; an elementary explanation of the principal perturbations in the solar system (1884)

Airy, George Biddell, Sir, 1801-1892 · London, Macmillan · leaf 116

An illustration from Gravitation; an elementary explanation of the principal perturbations in the solar system, 1884, leaf 116
from the old orbit) continues to recede from the old orbit till the diminution of velocity (26.) allows its path to be so much curved, that at e it begins to approach, and at L the new orbit intersects the old one; and after this, the path is inclined internally from the old orbit, till the… … independent of perturbation (the perijove being at any point D'), nevertheless, we may state that, in consequence of the disturbing force, the satellite will move in a curve F G H external to F E ; but when the disturbing force ceases at H, the satellite (which is moving in a path inclined…

Perturbation · Planets · Satellites · Lunar theory

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