At sunset, there is a moment at which the bottom of the Sun appears to touch the horizon. From this point on, the Sun dips further below the horizon until the point at which it finally disappears from view. How much time (in minutes) passes between the moment the Sun touches the horizon to the moment it disappears?
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This is a superb illustration of the geometry of the problem.
Imagine a triangle whose sides are 149.6, 149.6, and 1.3926. Notice that the sides are scaled down and 1.3926 is the diameter of the sun. The angle opposite to 1.3926 is 0 . 5 3 3 4 ∘ . The sun traverses 3 6 0 ∘ in 24hours or 1440 minutes. So by proportion, 0 . 5 3 3 4 ∘ x = 3 6 0 ∘ 1 4 4 0 x = 2 . 1 3 3 6 m i n
Find the angle which diameter of sun subtend at earth. Find out what fraction of the total rotation of earth in a day it is then multiplying by 24 will give the answer in hours.
2 r / D = θ 2 π θ × 2 4 × 6 0 = A n s We are doing this to find out time in which earth rotates the angle which the sun subtends at any point on earth.
Slick. Would you have to modify this approach at all if the Sun were much closer to Earth?
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