If you were directly between the two planets, their gravitational forces on you would oppose one another and at least partially cancel. Which planet would exert the stronger force on you would depend on their relative masses and on your distances from each of them. If one planet pulled on you more strongly than the other, you would find yourself falling toward that planet even though the other planet's gravity would oppose your descent and prolong the fall. However, there would also be a special location between the planets at which their gravitational forces would exactly cancel. If you were to begin motionless at that point in space, you wouldn't begin to fall at all. While the planets themselves would move and take the special location with them, there would be a brief moment when you would be able to hover in one place.
But there is something I've neglected: you aren't really at one location in space. Because your body has a finite size, the forces of gravity on different parts of your body would vary subtly according to their exact locations in space. Such variations in the strength of gravity are normally insignificant but would become important if you were extremely big (e.g. the size of the moon) or if the two planets you had in mind were extremely small but extraordinarily massive (e.g. black holes or neutron stars). In those cases, spatial variations in gravity would tend to pull unevenly on your body parts and might cause trouble. Such uneven forces are known as tidal forces and are indeed responsible for the earth's tides. While the tidal forces on a spaceship traveling between the earth and the moon would be difficult to detect, they would be easy to find if the spaceship were traveling between two small and nearby black holes. In that case, the tidal forces could become so severe that they could rip apart not only the spaceship and its occupants, but also their constituent molecules, atoms, and even subatomic particles.
To understand the two bulges, imagine three objects: the earth, a ball of water on the side of the earth nearest the moon, and a ball of water on the side of the earth farthest from the moon. Now picture those three objects orbiting the moon. In orbit, those three objects are falling freely toward the moon but are perpetually missing it because of their enormous sideways speeds. But the ball of water nearest the moon experiences a somewhat stronger moon-gravity than the other objects and it falls faster toward the moon. As a result, this ball of water pulls away from the earth—it bulges outward. Similarly, the ball of water farthest from the moon experiences a somewhat weaker moon-gravity than the other objects and it falls more slowly toward the moon. As a result, the earth and the other ball of water pull away from this outer ball so that this ball bulges outward, away from the earth.
It's interesting to note that the earth itself bulges slightly in response to these tidal forces. However, because the earth is more rigid than the water, its bulges are rather small compared to those of the water.
While the moon's gravity is the major cause of tides (the sun plays a secondary role), the moon's gravity isn't directly responsible for any true currents. Basically, water on the earth's surface swells up into two bulges: one on the side of the earth nearest the moon and one on the side farthest from the moon. As the earth turns, these bulges move across its surface and this movement is responsible for the tides.
If there were more than one moon, the tidal bulges would become misshapen. That is essentially what happens because of the sun. As the moon and sun adopt different arrangements around the earth, the strengths of the tides vary. The strongest tides (spring tides) occur when the moon and sun are on the same or opposite sides of the earth. The weakest tides (neap tides) occur when the moon and sun are at 90° from one another. Extra moons would probably just complicate this situation so that the strengths of the tides would vary erratically as the moons shifted their positions around the earth. Since the timing of the tides is still basically determined by the earth's rotation, there would still be approximately 2 highs and 2 lows a day.
There are two answers to this question because there are two possible interpretations of the word "waves." If you mean waves in the water beneath the bridge, then naturally the engineers must plan for the forces exerted on the bridge by the moving water that flows around its surfaces. But a more interesting wave issue is waves in the bridge itself. The bridge's surface can experience waves, just as a taut rope or a long beam can have waves running through it. For example, when a heavy object drops on the surface of the bridge, a ripple heads outward along the bridge surface and doesn't stop completely until it reaches the ends of the bridge. In fact, the wave will reflect from various portions of the bridge and its effects may not disappear for many seconds after the incident that started the waves.
Most of the time, these waves aren't important and can be ignored. But occasionally some special event will cause enormous waves to begin traveling through a bridge. The classic example was the Tacoma Narrows Bridge in Washington State that collapsed in 1940 when wind-driven waves in its surface ripped it apart. The entire collapse was captured on film and is a fascinating to watch. When a large group of soldiers crosses a footbridge, they are often instructed to break step so that their rhythmic cadence doesn't excite intense waves that might damage the bridge. In general, modern bridges are engineered to dampen these waves—wasting their energy through friction or friction-like effects so that they die away quickly. While it might be fun to watch waves traveling along the surface of a bridge from a safe vantage point, you probably wouldn't want to be on a bridge when it was experiencing strong ones.
Except during an eclipse, one half of the moon's surface is bathed in sunlight while the other half is in shadow. The phases of moon occur because we can only see half the moon at any moment and the fractions of lighted and shadowed moon that we see vary with about a four-week cycle—the lunar month. For example, when the moon is almost on the opposite side of the earth from the sun, we see only the lighted side of the moon and the moon appears full. When the moon is on the same side of the earth as the sun, we see only the shadowed side of the moon and it appears almost non-existent—a new moon. Each lunar month, our vantage point gradually evolves so that we see the new moon become a growing crescent moon, a half moon, a gibbous moon, and a full moon, a gibbous moon, a half moon, a shrinking crescent moon, and finally a new moon again. You can see this effect by illuminating a soccer ball with a bright flashlight and then walking around the soccer ball. You'll see the phases of the soccer ball.
The tide is caused primarily by the moon's gravity. Gravity is what keeps the moon and earth together as a pair—the moon and earth orbit one another because each is exerting an attractive force on the other. While they are effectively falling toward one another as the result of this gravitational attraction, their sideways motion keeps them from smashing together and they instead travel in elliptical paths around a common center of mass. But the moon's gravity is slightly stronger on the near side of the earth than it is on the far side of the earth. As a result, the water on the near side of the earth bulges outward toward the moon. The water on the far side of the earth also bulges outward because the earth itself is falling toward the moon slightly faster than that more distant water is. The distant water is being left behind as a bulge.
There are thus two separate tidal bulges in the earth's oceans: one on the side nearest the moon and one on the side farthest from the moon. But the earth rotates once a day, so these bulges move across the earth's surface. Since there are two bulges, a typical seashore passes through two bulges a day. At those times, the tide is high. During the times when the seashore is between bulges, the tide is low. Because the moon moves as the earth turns, high tides occur about 12 hours and 26 minutes apart, rather than every 12 hours. Since local water must flow to form the bulges as the earth rotates, there are cases where the tides are delayed as the water struggles to move through a channel. However, even in those cases, the high tides occur every 12 hours and 26 minutes. The sun's gravity also contributes to the tides, but its effects are smaller and serve mostly to vary the heights of high and low tide.
The moon orbits the earth about every 27.3 days, so its position relative to the sun changes from day to day. Because of the moon's movement around the earth, the moon rises and sets about 1 hour later every day. When the moon is on the sun side of the earth, it rises at sunrise and sets at sunset. Fourteen days later, when the moon is on the side opposite the sun, it rises at sunset and sets at sunrise.
A tsunami is simply a giant surface wave on water. Surface waves have several important characteristics, one of which is wavelength—that is, the distance between one crest and the next. The longer its wavelength, the faster a surface wave moves and also the deeper it extends below the surface of the water. In general a surface wave extends downward about one wavelength, so that if the crests are 100 meters apart, the wave is about 100 meters deep.
The wavelength of a tsunami is enormous—hundreds or even thousands of meters. As a result, a tsunami travels hundreds of kilometers per hour and extends downward deep into the ocean. Because it disturbs so much water, it carries a great deal of energy and it delivers this energy to the shore when it hits. Tsunamis are normally created by earthquakes or volcanic eruptions that sudden shift the supporting surfaces of a large amount of water. The water experiences a sudden impulse when the land or seabed shifts and a wave is emitted. You can launch a similar wave simply by shaking the end of a basin of water. But when a large region of land or seabed moves, the wave that's launched has a very long wavelength and tremendous energy. This tsunami heads off with enormous speed until it encounters the gradual shallowing of a seashore. There it becomes deformed because the lack of water in front of it causes its crest to become incomplete. Eventually the tsunami breaks in churning surf. The height of this breaking wave crest and the distance it travels onto shore before it stops depends on the total energy of the tsunami, but heights of 10 or 20 meters are not uncommon. Such waves can travel hundreds of meters up a beach or oceanfront if the slope is sufficiently gradual.
The wind pushes on wave crests. If the wind is relatively weak, it may add or subtract energy from the wave by doing work or negative work on it. But if the wind is too strong, it can blow the top off a crest. Choppy seas occur when the wind is so strong that it blows the surface water right out of wave crests and turns them white with foam.
They appear in rigid systems, such as beams or bridges. The Tacoma Narrows bridge failed because of a torsional (twisting) motion of its deck, driven by the wind. Before it failed, it was carrying torsional waves back and forth along its length. Torsional waves also appear in less spectacular engineering situations. When you lean on a loose tabletop, you actually send a torsional wave through it. However, it's so rigid that the wave is tiny and travels too quickly for you to see.
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