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" The radial force, or that part of the disturbing force which acts in the direction of the line joining the centres of the sun and disturbed planet, has no effect on the areas, but is the cause of periodical changes of small extent in the distance of the... "
The Elements of Astronomy: Or, The World as it Is, and as it Appears - Page 272
by Anna Cabot Lowell - 1850 - 376 pages
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An Elementary Treatise on Astronomy. ..., Volume 2

Robert Woodhouse - Celestial mechanics - 1818 - 572 pages
...of the apogee depends, for nearly half its value, on the tangential force, and for the remainder on that part of the disturbing force which acts in the direction of its radius ; a conclusion widely different from that (see p. 147.) which the result from the first...
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On the Free Motion of Points, and on Universal Gravitation: Including the ...

William Whewell - Celestial mechanics - 1832 - 286 pages
...velocity as 1 — c : 1 . The motion of the apse of the orbit of a satellite, so far as it depends on the part of the disturbing force which acts in the direction of the radius PT, may be calculated by finding the mean value of this disturbing force (which we shall do...
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Astronomy

sir John Frederick W. Herschel (1st bart.) - 1833 - 500 pages
...be explained by Newton from his theory of gravitation. (554.) We come now to consider the effects of that part of the disturbing force which acts in the direction of the radius vector, and tends to alter the law of gravity, and therefore to derange, in a more direct and...
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Astronomy

Sir John Frederick William Herschel - Astronomy - 1833 - 444 pages
...be explained by Newton from his theory of gravitation. (554.) We come now to consider the effects of that part of the disturbing force which acts in the direction of the radius vector, and tends to alter the law of gravity, and therefore to derange, in a more direct and...
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On the Connexion of the Physical Sciences

Mary Somerville - Astronomy - 1835 - 532 pages
...inequality of this kind in the motions of Jupiter and Saturn, has a period of no less than 918 years. The radial force, or that part of the disturbing force...elliptical motion varies inversely as the square of the distance, and that a force following any other law, would cause the body to move in a curve of a very...
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On the Connection of the Physical Sciences

Mary Somerville - Physical sciences - 1846 - 496 pages
...inequality of this kind in the motions of Jupiter and Saturn, has a period of no less than 918 years. The radial force, or that part of the disturbing force...which acts in the direction of the line joining the centers of the sun and disturbed planet, has no effect on the areas, but is the cause of periodical...
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Unity of Purpose, Or Rational Analysis: Being a Treatise Designed to ...

Augustus Young - Circle-squaring - 1846 - 304 pages
...Murdock has given a method of computing the mean motion of the moon's apogee, by first considering only that part of the disturbing force which acts in the direction of the radius ; and then instead of supposing the earth to be at rest, by conceiving the earth and moon to...
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On the Connection of the Physical Sciences

Mary Somerville - Science - 1846 - 496 pages
...velocities in ellipses, the perturbations or changes in the motions of P are very numerous. Lastly, that part of the disturbing force which acts in the direction of a line pm, fig. 13, at right angles to the plane of the orbit Npn, may be called the perpendicular...
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Proceedings of the American Philosophical Society Held at ..., Volumes 4-5

American Philosophical Society - Electronic journals - 1847 - 422 pages
...left the earth, had at any instant reached. The whole shadow would, therefore, drag or fall behind the direction of the line joining the centres of the sun and earth. The angular amount of this dragging of the shadow would, however, be equal and opposite to the...
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On the Connexion of the Physical Sciences

Mary Somerville - Physical sciences - 1849 - 568 pages
...velocities in ellipses, the perturbations or changes in the motions of p are very numerous. Lastly, that part of the disturbing force which acts in the direction of a line pm, fig. 13, at right angles to the plane of the orbit Npn, may be called the perpendicular...
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