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Tide-generating
forces are a result of the gravitational attraction between
the Earth, sun, and moon. It was not until Sir Isaac Newton
(who lived from 1642-1727) discovered the law of gravity
that the effect of the sun and the moon on the tides was
fully understood. All surfaces of the Earth are pulled
toward the moon and sun. This force has little effect on
land masses, but it does have a very great and obvious
effect on the water of the Earth's oceans. Twice each month
the tidal range reaches a maximum and these large tides are
called the spring tides. Halfway through the monthly cycle
the range is much smaller, and these weak tides are called
neap tides.
As
the moon rotates around the Earth, it pulls the water on the
nearest side of the Earth outward into a bulge. A similar
bulge on the opposite side of the Earth is caused by the
water being thrown outward by the planet's spin. These two
bulges travel around the globe, producing two high tides
each day. During time of the new moon and full moon, when
the sun and moon are in a straight line, their gravitational
pulls combine and produce spring tides; at this time the high
tides are very high and the low tides are very low. When sun
and moon are at right angles from the Earth, during the
quarter phases of the moon, the gravitational pull on the
oceans is less producing a smaller difference between high
and low tide known as a neap tide.
Some locations have much bigger tides than others. Tidal
ranges are usually small in the middle of the ocean but can
be very large where tidal waters are funneled into a bay or
river estuary. Hawaii has hardly any tidal range at all
while the water in the Bay of Fundy, in Canada, has a range
of about 40 feet.
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