Applying Newton's Universal Law
· At A, water is pulled towards the moon.
· At B, gravity is lower than at other places and so the water is higher. The Earth shields the moon's gravitational pull, and because the Earth rotates, the water is thrown out into space.
· These high tides stay relatively stationary with respect to the moon, but not with respect to the Earth's surface.
· The sun also plays a role. If the moon, Earth, and the sun line up, tides are higher than usual (spring tides).
· If the sun-Earth line is perpendicular to the Earth-moon line, tides are not as high (neap tides).
· Tides occur at different times of the day in a changing pattern because of the
o Earth's rotation.
o Lunar orbital period.
o Earth's orbital period.
· One new planet and one planetoid were discovered because of Newton's Universal Law of gravity.
o Small deviations (perturbations) were observed in the elliptical orbits of known planets.
o These perturbations could be explained by Newton's Universal Law of Gravity, if there was a planet beyond Uranus.
o Calculations predicted the location of the planet, and it was found (Neptune).
o Perturbations in Neptune's orbit led to the discovery of the planetoid Pluto (1930).
Earth Satellites
· If a satellite goes into a circular orbit, then there is a centripetal force causing the motion.
· The centripetal force is caused by gravitational force.
· Note that the above relationship tells us that the greater the orbit, the slower the speed.
· The above equation does not tell us that the greater the orbit, the smaller the kinetic energy of the satellite near launch. (In fact, the greater the orbit, the greater the kinetic energy needed at launch to get to orbit.
o E.G. Calculate the speed required by a satellite to maintain an orbit 100 km above the earth's surface. The radius of the Earth is 6.38 X 106 m.
· These other two forms can be equated to Fg to get equations for satellites in orbit.
· By equating the portion of the above equation which has period in it, to Newton's Universal Law of Gravity, and then rearranging, we find
· In the above equation, M is the mass of the planet the satellite orbits, and T is the period of the satellite's orbit.
· For a geosynchronous orbit, the radius of the orbit must be
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November 5, 2013