Respuesta :
Answer:
The gravitational force is [tex]\r F_{g} = \frac{mg}{R_e} \r rr[/tex]
Explanation:
The sketch describing this question is shown on the first uploaded image
from the sketch [tex]\r r[/tex] represent a unit vector pointing outward (This is shown the distance and the direction of the object
Now the gravitational force of a object on the surface earth with mass m is
Mathematically represented as
[tex]\u F = - \frac{Gmm_e}{R_e^2} =- mg \r r ----(1)[/tex]
Where [tex]m_e[/tex] is the mass o the earth and
[tex]R_e[/tex] is the radius of the earth
The minus sign shows that it is acting in the negative x-axis
Making the acceleration due to gravity a subject of the formula we have
[tex]g = \frac{Gm_e}{R_e^2} ----(2)[/tex]
Considering when the distance of the object to the center of the earth is r
Note: Any mass of the earth that is outside the distance covered by radius r as shown in the diagram does not affect the gravitational force
The mass of the enclosed earth can be mathematically represented as
[tex]M_{en} = \rho \frac{4}{3} \pi r^3 ----(3)[/tex]
Where [tex]\rho[/tex] is the mass density which is mathematically represented as
[tex]\rho = \frac{m_e}{(\frac{4}{3} )\pi R_e^3} ----(4)[/tex]
Now substituting these equation 3
[tex]M_{en} = \frac{,m_e}{(\frac{4}{3} )\pi R_e^3} (\frac{4}{3} ) \pi r^3 = \frac{m_er^3}{R_e^3} ---(5)[/tex]
Now substituting equation 5 into equation 1 to obtain the gravitational force as a function of distance r
[tex]\r F = -\frac{GmM_{en}}{r^2} \r r = \frac{Gmm_e r^3}{r^2R_e^3} \r r = \frac{Gmm_e}{R_e^3} r ----(6)[/tex]
From equation 2 we see that the [tex]g = \frac{Gm_e}{R_e^2}[/tex]
So substituting for g we have
[tex]\r F_{g} = \frac{mg}{R_e} \r rr[/tex]
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