Answer:
[tex]F=3.53\times 10^{22}\ N[/tex]
Explanation:
Given that,
Mass of the Sun, [tex]m_1=1.99\times 10^{30}\ kg[/tex]
The distance of Sun from the Earth, [tex]r=150\times 10^9\ m[/tex]
We know that,
The mass of the Earth, [tex]m_2=6\times 10^{24}\ kg[/tex]
We need to find the gravitational force between the Sun and the Earth.
The formula between two masses is given by :
[tex]F=G\dfrac{m_1m_2}{r^2}\\\\F=6.67\times 10^{-11}\times \dfrac{1.99\times 10^{30}\times 6\times 10^{24}}{(150\times 10^9)^2}\\\\F=3.53\times 10^{22}\ N[/tex]
So, the gravitational force between the Sun and the Earth is [tex]3.53\times 10^{22}\ N[/tex]
