Answer:
The time is ![t = 8.78 \ s](https://tex.z-dn.net/?f=t%20%3D%20%208.78%20%5C%20s)
Explanation:
From the question we are told that
The initial height of the eye is ![h _1 = 20 \ cm = 0.2 \ m](https://tex.z-dn.net/?f=h%20_1%20%3D%20%2020%20%5C%20%20cm%20%3D%20%200.2%20%5C%20%20m)
The height of the eye when you jumped up is ![h_2 = 150 \ cm = 1.5 \ m](https://tex.z-dn.net/?f=h_2%20%20%3D%20%20150%20%5C%20%20cm%20%20%3D%20%201.5%20%5C%20%20m)
An illustration of this question is shown on the first uploaded image
Generally the radius of the earth is ![R = 6.38*10^{6} \ m](https://tex.z-dn.net/?f=R%20%20%3D%20%206.38%2A10%5E%7B6%7D%20%5C%20%20m)
Now from the diagram first sun means first time you saw the sun and the second sun means second time you saw the sun then
H is the height increase when you quickly stood up which is mathematically evaluated as
![H = h_2 -h_1](https://tex.z-dn.net/?f=H%20%20%3D%20%20h_2%20-h_1)
![H = 1.5 - 0.2](https://tex.z-dn.net/?f=H%20%20%3D%201.5%20-%20%200.2)
![H = 1.3 \ m](https://tex.z-dn.net/?f=H%20%20%3D%201.3%20%5C%20m)
Also
i the angular displacement between the first and second position and from geometry it is also the angle at one of the sides of the right angle triangle
Applying Pythagoras theorem
![(R+H)^2 = K^2 + R^2](https://tex.z-dn.net/?f=%28R%2BH%29%5E2%20%20%3D%20%20K%5E2%20%20%2B%20R%5E2)
=> ![R^2 + H^2 + 2RH = K^2 + R^2](https://tex.z-dn.net/?f=R%5E2%20%2B%20H%5E2%20%2B%202RH%20%20%3D%20%20K%5E2%20%20%2B%20R%5E2)
Now given that H is very small compared to R the we ignore ![H^2](https://tex.z-dn.net/?f=H%5E2)
So
![R^2 + 2RH = K^2 + R^2](https://tex.z-dn.net/?f=R%5E2%20%2B%202RH%20%20%3D%20%20K%5E2%20%20%2B%20R%5E2)
=> ![K = \sqrt{2RH}](https://tex.z-dn.net/?f=K%20%20%3D%20%20%5Csqrt%7B2RH%7D)
=> ![K = \sqrt{2 * 6.38*10^6 * 1.3 }](https://tex.z-dn.net/?f=K%20%20%3D%20%20%5Csqrt%7B2%20%2A%20%206.38%2A10%5E6%20%2A%201.3%20%7D)
=> ![K = 4073 \ m](https://tex.z-dn.net/?f=K%20%20%3D%204073%20%5C%20%20m)
Now the
is mathematically evaluated using SOHCAHTOA as follows
![tan \theta = \frac{K}{R}](https://tex.z-dn.net/?f=tan%20%20%5Ctheta%20%20%3D%20%20%5Cfrac%7BK%7D%7BR%7D)
![\theta = tan^{-1}[ \frac{K}{R}]](https://tex.z-dn.net/?f=%5Ctheta%20%20%3D%20tan%5E%7B-1%7D%5B%20%5Cfrac%7BK%7D%7BR%7D%5D)
=> ![\theta = tan^{-1}[ \frac{ 4073}{6.38*10^{6}}]](https://tex.z-dn.net/?f=%5Ctheta%20%20%3D%20tan%5E%7B-1%7D%5B%20%5Cfrac%7B%204073%7D%7B6.38%2A10%5E%7B6%7D%7D%5D)
=> ![\theta = 0.0366^o](https://tex.z-dn.net/?f=%5Ctheta%20%3D%200.0366%5Eo)
Generally
![1 \revolution\ around \ the\ earth = 24 \ hours = 86400 \ seconds = 360 ^o](https://tex.z-dn.net/?f=1%20%5Crevolution%5C%20%20around%20%5C%20the%5C%20earth%20%3D%20%2024%20%5C%20hours%20%3D%20%2086400%20%5C%20seconds%20%3D%20%20360%20%5Eo)
So
![\frac{\theta}{360} = \frac{t}{86400}](https://tex.z-dn.net/?f=%5Cfrac%7B%5Ctheta%7D%7B360%7D%20%20%3D%20%20%5Cfrac%7Bt%7D%7B86400%7D)
=> ![\frac{0.0366}{360} = \frac{t}{86400}](https://tex.z-dn.net/?f=%5Cfrac%7B0.0366%7D%7B360%7D%20%3D%20%20%5Cfrac%7Bt%7D%7B86400%7D)
=> ![t = 8.78 \ s](https://tex.z-dn.net/?f=t%20%3D%20%208.78%20%5C%20s)