Predicting Weather By The Moon - Xavier University Libraries
Predicting Weather By The Moon - Xavier University Libraries
Predicting Weather By The Moon - Xavier University Libraries
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Tides<br />
rotation. As Earth’s rotation speed decreases the <strong>Moon</strong><br />
must move farther from Earth to conserve angular momentum.<br />
This process is slow. Every 350 years we have to add<br />
another second to the length of our year.<br />
Tides also occur in large lakes, within the solid crust<br />
of the Earth, and in the atmosphere. <strong>The</strong> latter really are<br />
‘high’ tides!<br />
ATMOSPHERIC TIDES<br />
<strong>The</strong> Sun is the major source of energy available to<br />
the Earth. At the Earth-Sun distance of 93,200,000 miles<br />
(150,000,000 km) about one two-billionth of the Sun’s outpouring<br />
of energy (mostly in the visible-light range of the<br />
spectrum) is intercepted by us. Most of this is absorbed by<br />
the atmosphere and the solid Earth, giving rise to heating<br />
of the gas of the atmosphere and the rock and water of the<br />
surface.<br />
<strong>The</strong> heat of the sun heat warms the atmosphere and<br />
the Earth. <strong>The</strong> atmosphere is a pile of gases 200 miles thick<br />
that, along with the body of water we call the sea, is held to<br />
the Earth by our own gravity. Without this gravity all the<br />
oceans would fly off into space. <strong>The</strong> atmosphere would go<br />
too.<br />
What does the atmosphere weigh? <strong>The</strong> total weight<br />
of Earth’s atmosphere is about 4.5 x 1018 kilograms, or<br />
nearly five thousand million million tons. Thus the weight<br />
of the atmosphere per unit area, or its pressure, is about a<br />
ton per square foot at sea level. A layer of water about 10<br />
meters, or 33 feet deep sitting on the Earth at every point,<br />
would exert the same pressure at the Earth’s surface as does<br />
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