 | American Philosophical Society - 1874 - 758 pages
...relative masses of the principal planetary orbs. Stockwell has found* the following relations : I. Tfie mean motion of Jupiter's perihelion is exactly equal...the perihelion of Uranus, and the mean longitudes of these perihelia differ by exactly 180°. II. The mean motion of Jupiter's node on the invariable plane... | |
 | American Association for the Advancement of Science - 1869 - 432 pages
...researches, pertains to the relative motions and positions of the perihelia of the different planets. The mean motion of Jupiter's perihelion is exactly...to the mean motion of the perihelion of Uranus; and their mean longitudes differ by exactly 180°. The mean motion of Saturn's perihelion is very nearly... | |
 | American Philosophical Society - 1873 - 548 pages
...important of the correlated apsides are the same as are represented in my harmonic series, for he has pointed out the following curious relations : " I....mean longitudes of those perihelia differ by exactly 180°. II. The mean motion of Jupiter's node on the invariable plane is exactly equal to that of Saturn,... | |
 | American Philosophical Society - 1873 - 560 pages
...important of the correlated apsides are the same as are represented in my harmonic series, for he has pointed out the following curious relations : "I....mean longitudes of those perihelia differ by exactly 180°. II. The mean motion of Jupiter's node on the invariable plane is exactly equal to that of Saturn,... | |
 | Smithsonian Institution. Board of Regents - 1873 - 486 pages
...three planets Jupiter, Saturn, and Uranus. These relations are expressed by the two following theorems: I. The mean motion of Jupiter's perihelion is exactly...the perihelion of Uranus, and the mean longitudes of these perihelia differ by exactly 180°. II. The mean motion of Jupiter's node on the invariable plane... | |
 | Edward Isidore Sears - 1873 - 444 pages
...retrograde direction. These relations Mr. Stockwell embodies in two general propositions, as follows : " I. The mean motion of Jupiter's perihelion is exactly...the perihelion of Uranus, and the mean longitudes of these perihelia differ by exactly 180°. II. The mean motion of Jupiter's node on the invariable plane... | |
 | American Philosophical Society - 1876 - 742 pages
...principal planetary orbs. Stockwell has found* the following relations : I. The mean motion of Jupiter'* perihelion is exactly equal to the mean motion of...the perihelion of Uranus, and the mean longitudes of these perifieliit differ by er«cll>/ 18IP. II. The mean motion of Jupiter's node on the invariable... | |
 | 1894 - 446 pages
...planet is directly as the square root of that planet's distance from the sun. — Thomas Bassnett. 6. (i) The mean motion of Jupiter's perihelion is exactly...mean motion of the perihelion of Uranus, and the mean longitude of these perihelia differ by exactly 180°. (n) The mean motion of Jupiter's node on the... | |
 | 1896 - 410 pages
...what variations exist in the system. — Lagrange. James B. Babbitt ' s Theory of the Earth, p. 211. (i ) The mean motion of Jupiter's perihelion is exactly...the perihelion of Uranus, and the mean longitudes of these perihelia differ by exactly 180°. (2) The mean motion of Jupiter's nodes on the invariable plane... | |
 | 1901 - 432 pages
...and inversely as the square of the time of rotation of the central body. — MT Singleton. 17. (a) The mean motion of Jupiter's perihelion is exactly...mean motion of the perihelion of Uranus, and the mean longitude of these perhelia differ by exactly 180°. (V) The mean motion of Jupiter's node on the invariable... | |
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I. The mean motion of Jupiter's perihelion is exactly equal to the mean motion of the perihelion of Uranus, and the mean longitudes of these perihelia differ by exactly 180°. II. The mean motion of Jupiter's node on the invariable plane is exactly equal... 
