Solve each problem. Solar Eclipse on Earth The sun has a diameter of about 865,000 mi with a maximum distance from Earth's surface of about 94,500,000 mi. The moon has a smaller diameter of 2159 mi. For a total solar eclipse to occur, the moon must pass between Earth and the sun. The moon must also be close enough to Earth for the moon's umbra (shadow) to reach the surface of Earth. (Data from Karttunen, H., P. Kröger, H. Oja, M. Putannen, and K. Donners, Editors, Fundamental Astronomy, Fourth Edition, Springer-Verlag.) a. Calculate the maximum distance, to the nearest thousand miles, that the moon can be from Earth and still have a total solar eclipse occur. (Hint: Use similar triangles.)
1. Measuring Angles
Complementary and Supplementary Angles
1. Measuring Angles
Complementary and Supplementary Angles
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Convert each degree measure to radians. If applicable, round to the nearest thousandth. See Example 1(c).
85.04°
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CONCEPT PREVIEW In each figure, find the measures of the numbered angles, given that lines m and n are parallel.
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Solve each problem. See Example 5. Height of a Carving of Lincoln Assume that Lincoln was 6 1/3 ft tall and his head was 3/4 ft long. Knowing that the carved head of Lincoln at Mt. Rushmore is 60 ft tall, find how tall his entire body would be if it were carved into the mountain.
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Give an expression that generates all angles coterminal with an angle of π/2 radians. Let n represent any integer.
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Convert each radian measure to degrees. Write answers to the nearest minute. See Example 2(c).
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