Solveeit Logo

Question

Question: If \(R\) is the radius of the earth, then the value of acceleration due to gravity at a height \(h\)...

If RR is the radius of the earth, then the value of acceleration due to gravity at a height hh from the surface of the earth will become half its value on the surface of the earth if:

& A.h=2R \\\ & B.h=R \\\ & C.h=(\sqrt{2}+1)R \\\ & D.h=(\sqrt{2}-1)R \\\ \end{aligned}$$
Explanation

Solution

To find the relationship between RR and hh, we need to calculate the acceleration due to gravitation at RR and hh, using the general formula. Since a relationship between calculating the acceleration due to gravitation at RR and hh is given, we can equate them to find the required relation.

Formula used:
g=GmR2g=\dfrac{Gm}{R^{2}} and g=Gm(R+h)2g\prime =\dfrac{Gm}{(R+h)^{2}}

Complete step-by-step answer:
We know that according to Newton-Kepler law of gravitation, the force due to gravitation is given as F=Gm1m2r2F=G\dfrac{m_{1}m_{2}}{r^{2}}, where GG is the gravitational constant, m1,m2m_{1},m_{2} is the masses of the body, and rr is the distance between the two bodies.
We know that the acceleration due to gravitation on the surface of the earth is given as g=GmR2g=\dfrac{Gm}{R^{2}} and the acceleration due to gravitation at a height hh from the surface is given by g=Gm(R+h)2g\prime =\dfrac{Gm}{(R+h)^{2}} , where GG is the gravitational constant, mm is the mass of the body, RR is the radius of the earth and hh is the height from the surface of the earth .
Here, since the mass of the body is very small as compared to the mass of the earth, to calculate the force on the body, we can ignore the value of mass of the earth.
Since it is given that, the value of acceleration due to gravity at a height hh from the surface of the earth is half its value on the surface of the earth , i.e. g=g2g\prime=\dfrac{g}{2}
Then taking the ratio between gg and g.g\prime. we get,
gg=g2g=Gm(R+h)2GmR2\dfrac{g\prime}{g}=\dfrac{\dfrac{g}{2}}{g}=\dfrac{\dfrac{Gm}{(R+h)^{2}}}{\dfrac{Gm}{R^{2}}}
Assuming the mass of the body is same, and reducing, we get,
12=R2(R+h)2\dfrac{1}{2}=\dfrac{R^{2}}{(R+h)^{2}}
2=R+hR\Rightarrow \sqrt 2=\dfrac{R+h}{R}
2=1+hR\Rightarrow \sqrt 2=1+\dfrac{h}{R}
h=R(21)\Rightarrow h=R(\sqrt 2-1)

Note: The mass of the earth is larger than the mass of the object, it can be neglected. Also note that using the Newton-Kepler law of gravitation, the acceleration due to gravitation at a height hh from the surface is given by g=Gm(R+h)2g\prime =\dfrac{Gm}{(R+h)^{2}}.