Explanation:
Given that,
Intensity = 1150 W/m²
(a). We need to calculate the magnetic field
Using formula of intensity
![I=\dfrac{E^2}{2\mu_{0}c}](https://tex.z-dn.net/?f=I%3D%5Cdfrac%7BE%5E2%7D%7B2%5Cmu_%7B0%7Dc%7D)
![E=\sqrt{2\times I\mu_{0}c}](https://tex.z-dn.net/?f=E%3D%5Csqrt%7B2%5Ctimes%20I%5Cmu_%7B0%7Dc%7D)
Put the value into the formula
![E=\sqrt{2\times1150\times4\pi\times10^{-7}\times3\times10^{8}}](https://tex.z-dn.net/?f=E%3D%5Csqrt%7B2%5Ctimes1150%5Ctimes4%5Cpi%5Ctimes10%5E%7B-7%7D%5Ctimes3%5Ctimes10%5E%7B8%7D%7D)
![E=931.17\ N/C](https://tex.z-dn.net/?f=E%3D931.17%5C%20N%2FC)
Using formula of magnetic field
![B = \dfrac{E}{c}](https://tex.z-dn.net/?f=B%20%3D%20%5Cdfrac%7BE%7D%7Bc%7D)
Put the value into the formula
![B=\dfrac{931.17}{3\times10^{8}}](https://tex.z-dn.net/?f=B%3D%5Cdfrac%7B931.17%7D%7B3%5Ctimes10%5E%7B8%7D%7D)
![B=0.0000031039\ T](https://tex.z-dn.net/?f=B%3D0.0000031039%5C%20T)
![B=3.10\times10^{-6}\ T](https://tex.z-dn.net/?f=B%3D3.10%5Ctimes10%5E%7B-6%7D%5C%20T)
(b). The relative strength of the gravitational and solar electromagnetic pressure forces of the sun on the earth
We need to calculate the gravitational force
Using gravitational force
![F=\dfrac{Gm_{s}M_{e}}{r^2}](https://tex.z-dn.net/?f=F%3D%5Cdfrac%7BGm_%7Bs%7DM_%7Be%7D%7D%7Br%5E2%7D)
Put the value into the formula
![F=\dfrac{6.67\times10^{-11}\times1.98\times10^{30}\times5.97\times10^{24}}{(1.496\times10^{11})^2}](https://tex.z-dn.net/?f=F%3D%5Cdfrac%7B6.67%5Ctimes10%5E%7B-11%7D%5Ctimes1.98%5Ctimes10%5E%7B30%7D%5Ctimes5.97%5Ctimes10%5E%7B24%7D%7D%7B%281.496%5Ctimes10%5E%7B11%7D%29%5E2%7D)
![F=3.522\times10^{22}\ N](https://tex.z-dn.net/?f=F%3D3.522%5Ctimes10%5E%7B22%7D%5C%20N)
We need to calculate the radiation force
Using formula of force
![F_{R}=\dfrac{I}{c}\pi\timesR_{E}^{2}](https://tex.z-dn.net/?f=F_%7BR%7D%3D%5Cdfrac%7BI%7D%7Bc%7D%5Cpi%5CtimesR_%7BE%7D%5E%7B2%7D)
Put the value into the formula
![F_{R}=\dfrac{1150}{3\times10^{8}}\times\pi\times(6.378\times10^{6})^2](https://tex.z-dn.net/?f=F_%7BR%7D%3D%5Cdfrac%7B1150%7D%7B3%5Ctimes10%5E%7B8%7D%7D%5Ctimes%5Cpi%5Ctimes%286.378%5Ctimes10%5E%7B6%7D%29%5E2)
![F_{R}=4.8\times10^{8}\ N](https://tex.z-dn.net/?f=F_%7BR%7D%3D4.8%5Ctimes10%5E%7B8%7D%5C%20N)
The gravitational and solar electromagnetic pressure forces of the sun on the earth
![\dfrac{F_{G}}{F_{R}}=\dfrac{3.522\times10^{22}}{4.8\times10^{8}}](https://tex.z-dn.net/?f=%5Cdfrac%7BF_%7BG%7D%7D%7BF_%7BR%7D%7D%3D%5Cdfrac%7B3.522%5Ctimes10%5E%7B22%7D%7D%7B4.8%5Ctimes10%5E%7B8%7D%7D)
![\dfrac{F_{G}}{F_{R}}=7.3375\times10^{13}](https://tex.z-dn.net/?f=%5Cdfrac%7BF_%7BG%7D%7D%7BF_%7BR%7D%7D%3D7.3375%5Ctimes10%5E%7B13%7D)
Hence, This is the required solution.