Fig. 6.2. The ideal global tide as seen from the South Pole. At the point in time captured in the figure, high tide crests are near South America and in the South Indian ocean basin, and low tide troughs are near the southern tip of Africa and New Zealand.
Image by Byron Inouye
Tides are predictable daily rises and falls in the surface water of the ocean and large lakes. On the coast, tides appear as the regular rise and fall of the sea surface. Tides are waves whose periods are so long that hours go by between their crests and troughs. The ideal wave of the tide wraps around the world with two crests and two troughs (Fig. 6.2). However, most of the time, and in most places, tides are much more complex.
Fig. 6.3. Tidal stages
Image by Byron Inouye
Tidal changes can be described by stages (Fig. 6.3). A high tide is the stage when the tidal crest arrives at a particular location on shore, raising the local sea level. A low tide is the stage when the trough arrives, lowering the local sea level. A flood tide is a rising or incoming tide between low tide and high tide. An ebb tide is a falling or outgoing tide between high tide and low tide. The vertical distance between high tide and low tide is the tidal range.
Tides are predictable because they are produced by a combination of forces that are predictable. These forces are determined by the movements and positions of objects in our solar system, particularly the earth and the moon in relation to the sun. To understand tides, therefore, it is important to understand the movements of the earth and the moon relative to the sun.
Model the movements of three objects in our solar system—the sun, the moon, and the earth—using your body.
