 | 1854 - 1112 sivua
...to this corresponds the period of revolution, eighty-eight days, by the third of Kepler's Laws : " The squares of the times of revolution are as the cubes of the mean distances from the Sun." Analysis has sho\rn that this proportion is only approximate, as it does not take into account the... | |
 | John Farrar - 1827 - 464 sivua
...conform to the laws discovered by Kepler in the case of the planets. In each system of satellites, the squares of the times of revolution are as the cubes of the mean distances. This law has enabled us to calculate the sidereal revolutions of the satellites of Uranus, by means... | |
 | John Farrar - 1827 - 456 sivua
...conform to the laws discovered by Kepler in the case of the planets. In each system of satellites, the squares of the times of revolution are as the cubes of the menu distances. This law has enabled us to calculate the sidereal revolutions of the satellites of... | |
 | Francis Lieber, Edward Wigglesworth, Thomas Gamaliel Bradford - 1831 - 620 sivua
...investigated their respective angles at the sun. This was called Kepler's problem. The third law teaches that, in the motion of the planets, the squares of the times...are as the cubes of the mean distances from the sun; one instance of the application of which law, in the want of other means, is in the determination of... | |
 | Francis Lieber, Edward Wigglesworth, Thomas Gamaliel Bradford, Henry Vethake - 1829 - 644 sivua
...describes equal areas in equal tjmes; and, lastly, that, in the revolutions of the planets and satellites, the squares of the times of revolution are as the cubes of the mean distances from the larger body. These three important truths are comprehended under the name of Kepler's laws. About the... | |
 | Francis Lieber, Edward Wigglesworth, Thomas Gamaliel Bradford, Henry Vethake - 1829 - 666 sivua
...describes equal areas in equal limes; and, lastly, that, in the revolutions of the planets and satellites, the squares of the times of revolution are as the cubes of the mean distances from the larger body. These three important truths are comprehended under the name of Kepler'1! laws. About... | |
 | Encyclopaedia Americana - 1831 - 608 sivua
...investigated then- respective angles at the sun. This was called Kepler's problem. The third law teaches that, in the motion of the planets, the squares of the times...are as the cubes of the mean distances from the sun ; one instance of the application of which law, in the want of other means, ie in the determination... | |
 | Francis Lieber, Edward Wigglesworth - 1831 - 618 sivua
...angles at the sun. This was called Kepler's problem. The third law teaches that, in the motioi.,of the planets, the squares of the times of revolution...are as the cubes of the mean distances from the sun; one instance of the application of which law, in the want of other means, is in the determination of... | |
 | Francis Lieber, Edward Wigglesworth, Thomas Gamaliel Bradford - 1831 - 616 sivua
...their respective angles at the sun. This was called Kepler's problem. The third law teaches tliat, in the motion of the planets, the squares of the times of revolution arc as the cubes of the mean distances from the sun ; one instance of the application of which law,... | |
 | 1832 - 498 sivua
...drawn from the sun to the planet or comet, sweep over equal areas, in equal portions of time, and that the squares of the times of revolution are as the cubes of the mean distances of the comet or planet from the sun. Planets and comets are opaque bodies, and shine only by the light... | |
| |
In the motion of the planets, the squares of the times of revolution are as the cubes of the mean distances from the sun. 
