Respuesta :

Answer: [tex]3.524(10)^{22}N[/tex]

Explanation:

According to Newton's law of Gravitation, the force [tex]F[/tex] exerted between two bodies of masses [tex]m1[/tex] and [tex]m2[/tex]  and separated by a distance [tex]r[/tex]  is equal to the product of their masses and inversely proportional to the square of the distance:

[tex]F=G\frac{(m1)(m2)}{r^2}[/tex]   (1)

Where:

[tex]G[/tex] is the Gravitational Constant and its value is [tex]6.674(10)^{-11}\frac{m^{3}}{kgs^{2}}[/tex]

[tex]m1=1.99(10)^{30}kg[/tex] is the mass of the Sun

[tex]m2=5.972(10)^{24}kg[/tex] is the mass of the Earth

[tex]r=1.50(10)^{11}m[/tex]  is the distance between the Sun and the Earth

Substituting the values in (1):

[tex]F=6.674(10)^{-11}\frac{m^{3}}{kgs^{2}}\frac{(1.99(10)^{30}kg)(5.972(10)^{24}kg)}{(1.50(10)^{11}m)^2}[/tex]   (2)

Finally:

[tex]F=3.524(10)^{22}N[/tex]   This is the gravitational force of the Sun on the Earth.

ACCESS MORE