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Moon, gravitational force

Book II investigates the dynamical conditions of fluid motion. Book III displays the law of gi avitatioii at work in the solar system. It is demonstrated from the revolutions of the six known planets, including Earth, and their satellites, though Newton could never quite perfect the difficult theory of the Moon s motion. It is also demonstrated from the motions of comets. The gravitational forces of the heavenly bodies are used to calculate their relative masses. The tidal ebb and flow and the precession of the equinoxes is explained m terms of the forces exerted by the Sun and Moon. These demonstrations are carried out with precise calculations. [Pg.846]

On the moon, a gold bar weighs less than it does on Earth. This is because the moon is much less massive than Earth hence, the gravitational force exerted by the moon on the bar is much less. On Jupiter, the gold bar would weigh more than it does on Earth because of the greater gravitational force exerted on the bar by this very massive planet. [Pg.15]

The moons of Saturn have a direct influence on Saturn s rings. A natural tendency of ring materials is to spread both toward and away from the planet, but the moons and a complex interplay of gravitational forces shape the rings and define their structure. Mimas. . . Tethys. . . Dione. . . Rhea. . . Enceladus. . . Iapetus. . . And Hyperion. . . ... [Pg.42]

The moons of Saturn have a direct influence on Saturn s rings. A natural tendency of ring materials is to spread both toward and away from the planet, but the moons and a complex tnterplay of gravitational forces shape the rings and define their structure. [Pg.42]

The view of the Moon remains the same (viewing the same face) because it rotates on its axis at the same rate that it travels around the Earth—once every 29.5 day. This is no mere coirKidence. The side of the Moon facing us is attracted more strongly by Earth s gravitational force than the opposite side. The force of gravity depends on the mass of the two interacting objects (here... [Pg.419]

Using Numbers If your weight is 120 pounds and your mass is 54 kilograms, how would those values change if you were on the moon The gravitational force on the moon is 1/6 the gravitational force on Earth. [Pg.9]

Fig. 1.4 Every two weeks, the Sun and Moon are aligned with Earth so that the gravitational forces of both heavenly bodies create very high tides called spring tides. When the Moon and Sun are at right angles to Earth, lower, or neap, tides result. Fig. 1.4 Every two weeks, the Sun and Moon are aligned with Earth so that the gravitational forces of both heavenly bodies create very high tides called spring tides. When the Moon and Sun are at right angles to Earth, lower, or neap, tides result.
Evaluate How would your mass and weight differ on the Moon The gravitational force of the Moon is one-sixth the gravitational force on Earth. [Pg.11]

The idea of scaling of the environment is changing once we increase accuracy. For example, we can say that the Earth gravity at accuracy better than one-ppm level is described by three forces attraction by Earth, Sun and Moon, while the acceleration of free fall, g, is a parameter of the interaction with Earth only. Alternatively, we can say that the complete gravitational force is always mg and it is varying in time because of the relative motion of Earth, Sun and Moon. That is not only a matter of definition. It depends on natural time scale of the experiment with respect to the periods of Earth motion and on whether we understand the planetary motion properly. [Pg.238]

The ocean tides are caused by the gravitational forces between the Earth, the Sun, and the Moon, along with the centrifugal force imposed by the Earth s rotation. As the Earth rotates, and as the three bodies move relative to one another, the gradual and recurring shifts in the balance of gravitational forces cause the water in the oceans to tend to move toward one coast or the other. [Pg.229]

According to Newton s law of gravitation the gravitational force exerted by a celestial body, e. g. the moon, on a mass particle of unit mass m=l, situated at the spatial point P, is expressed in the following way (see fig. 1) ... [Pg.12]


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See also in sourсe #XX -- [ Pg.16 ]

See also in sourсe #XX -- [ Pg.16 ]




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