In Problems 79-84, use the following discussion. The formula D = 24 [ 1 − cos − 1 ( tan i tan θ ) π ] can be used to approximate the number of hours of daylight D when the declination of the Sun is i ∘ at a location θ ∘ north latitude for any date between the vernal equinox and autumnal equinox. The declination of the Sun is defined as the angle i between the equatorial plane and any ray of light from the Sun. The latitude of a location is the angle θ between the Equator and the location on the surface of Earth, with the vertex of the angle located at the center of Earth. See the figure. To use the formula, cos − 1 ( tan i tan θ ) must be expressed in radians. Approximate the number of hours of daylight in Anchorage, Alaska ( 61 ∘ 10 ' north latitude), for the following dates: (a) Summer solstice ( i = 23.5 ∘ ) (b) Vernal equinox ( i = 0 ∘ ) (c) July 4 ( i = 22 ∘ 48 ' )
In Problems 79-84, use the following discussion. The formula D = 24 [ 1 − cos − 1 ( tan i tan θ ) π ] can be used to approximate the number of hours of daylight D when the declination of the Sun is i ∘ at a location θ ∘ north latitude for any date between the vernal equinox and autumnal equinox. The declination of the Sun is defined as the angle i between the equatorial plane and any ray of light from the Sun. The latitude of a location is the angle θ between the Equator and the location on the surface of Earth, with the vertex of the angle located at the center of Earth. See the figure. To use the formula, cos − 1 ( tan i tan θ ) must be expressed in radians. Approximate the number of hours of daylight in Anchorage, Alaska ( 61 ∘ 10 ' north latitude), for the following dates: (a) Summer solstice ( i = 23.5 ∘ ) (b) Vernal equinox ( i = 0 ∘ ) (c) July 4 ( i = 22 ∘ 48 ' )
Solution Summary: The author calculates the number of hours of daylight D at the location north latitude.
In Problems 79-84, use the following discussion. The formula
can be used to approximate the number of hours of daylight D when the declination of the Sun is
at a location
north latitude for any date between the vernal equinox and autumnal equinox. The declination of the Sun is defined as the angle i between the equatorial plane and any ray of light from the Sun. The latitude of a location is the angle
between the Equator and the location on the surface of Earth, with the vertex of the angle located at the center of Earth. See the figure. To use the formula,
must be expressed in radians.
Approximate the number of hours of daylight in Anchorage, Alaska (
north latitude), for the following dates:
2. Suppose the graph below left is the function f(x). In the space below, describe what
transformations are occuring in the transformed function 3ƒ(-2x) + 1. The graph it on the
coordinate plane below right. (4 points)
1
1. Suppose we have the function f(x) = = and then we transform it by moving it four units to the
right and six units down, reflecting it horizontally, and stretching vertically by 5 units. What will
the formula of our new function g(x) be? (2 points)
g(x) =
Suppose an oil spill covers a circular area and the radius, r, increases according to the graph shown below where t
represents the number of minutes since the spill was first observed.
Radius (feet)
80
70
60
50
40
30
20
10
0
r
0 10 20 30 40 50 60 70 80 90
Time (minutes)
(a) How large is the circular area of the spill 30 minutes after it was first observed? Give your answer in terms of π.
square feet
(b) If the cost to clean the oil spill is proportional to the square of the diameter of the spill, express the cost, C, as a
function of the radius of the spill, r. Use a lower case k as the proportionality constant.
C(r) =
(c) Which of the following expressions could be used to represent the amount of time it took for the radius of the spill to
increase from 20 feet to 60 feet?
r(60) - r(20)
Or¹(80-30)
r(80) - r(30)
r-1(80) - r−1(30)
r-1(60) - r¹(20)
University Calculus: Early Transcendentals (4th Edition)
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