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lesya692 [45]
4 years ago
10

TV broadcast antennas are the tallest artificial structures on Earth. In 1987, a 69.0 kg physicist placed himself and 400 kg of

equipment at the top of one 610 m high antenna to perform gravity experiments. By how much (in mm) was the antenna compressed, if we consider it to be equivalent to a steel cylinder 0.175 m in radius?
Physics
1 answer:
Stolb23 [73]4 years ago
6 0

Answer:

see description

Explanation:

This is a problem where we have to assume we are in the linear region of the stress-strain curve for the antenna.

The physicist has a mass of 69 [Kg] and his equipment has a mass of 400 [Kg].

Now we just have to add those up, we end up with a mass of 469 [Kg].

The force exerted to the antenna (downwards) will be:

F = 469 [Kg] * 9.8 [m/s^2]=4956.2 [N]

To find the compression we have that the relationship between strain we take the equation:

\gamma = \frac{F*l_{o}}{A* \epsilon}

where \gamma is the young modulus, \epsilon is the strain on the material, F is the force exerted by the physicist+equipment, A is the cross-section area of the cylinder, and l_{o} is the initial longitude of the cylinder.

now the young modulus for steel is \gamma = 200*10^9 [Pa].

The cross section area for the cylinder is A = \pi *r^2 = \pi *(0.175)^2=0.0962[m^2]

The length of the antenna is l_{0}=610 [m]

we find \epsilon:

\epsilon = \frac{F*l_{o}}{A* \gamma}=\frac{4956.2*610}{0.0962*200*10^9} = 0.000157 [m] = 0.157 [mm]

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The intensity of sunlight reaching the earth is 1360 w/m2. Assuming all the sunligh is absorbed, what is the radiation pressure
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For an electromagnetic wave incident on a surface, the radiation pressure is given by (assuming all the radiation is absorbed)

p=\frac{I}{c}

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I is the intensity

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In this problem, I=1360 W/m^2; substituting this value, we find the radiation pressure:

p=\frac{1360 W/m^2}{3\cdot 10^8 m/s}=4.5\cdot 10^{-6} Pa

the force exerted on the Earth depends on the surface considered. Assuming that the sunlight hits half of the Earth's surface (the half illuminated by the Sun), we have to consider the area of a hemisphere, which is

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A=2\pi (6.37\cdot 10^6 m)^2=2.55\cdot 10^{14}m^2

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The gravitational force exerted by the Sun on the Earth is

F=G\frac{Mm}{r^2}

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G is the gravitational constant

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Substituting,

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And so, the radiation pressure force on Earth as a fraction of the sun's gravitational force on Earth is

\frac{1.15\cdot 10^9 N}{3.58\cdot 10^{22}N}=3.2\cdot 10^{-14}

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