The angle of elevation θ of the sun in the sky at any latitude L is calculated with the formula sinθ=cosDcosLcosω+sinDsinL. ω is the number of radians that the Earth has rotated through since noon when ω=0. D is the declination of the sun. Westville has latitude L=37.9°. Find the angle of elevation θ in degrees of the sun at 3 PM on February 29, 2012, where at that time D≈−0.1425
The angle of elevation θ of the sun in the sky at any latitude L is calculated with the formula sinθ=cosDcosLcosω+sinDsinL. ω is the number of radians that the Earth has rotated through since noon when ω=0. D is the declination of the sun. Westville has latitude L=37.9°. Find the angle of elevation θ in degrees of the sun at 3 PM on February 29, 2012, where at that time D≈−0.1425
Trigonometry (MindTap Course List)
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Author:Charles P. McKeague, Mark D. Turner
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Chapter6: Equations
Section6.1: Solving Trigonometric Equations
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The angle of elevation
θ
of the sun in the sky at any latitude L is calculated with the formula
sinθ=cosDcosLcosω+sinDsinL.
ω
is the number of radians that the Earth has rotated through since noon when
ω=0.
D is the declination of the sun. Westville has latitude
L=37.9°.
Find the angle of elevation
θ
in degrees of the sun at 3 PM on February 29, 2012, where at that time
D≈−0.1425
and
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