Question #182072

An astronaut working on the Moon tries to determine the gravitational constant G by throwing a Moon rock of mass m with a velocity of v vertically into the sky. The astronaut knows that the moon has a density p of 3340 kg/m^3 and a radius R of 1740 km.


(a) Show with (1) that the potential energy of the rock at height h above the surface is given by:

E=(-4πG/3)mp.R^3/(R+H)


(b) Next, show that the gravitational constant can be determined by:

G=(3/8π)×(v^2/‌pR^2)×[1-{R/(R+H)}]^-1


(c)What is the resulting G if the rock is thrown with 30 km/h and reaches 21.5 m?


1
Expert's answer
2021-04-19T17:10:48-0400

a) the potential energy of a piece with mass m at a distance r from the spherically symmetric object of mass M is

E=GMmrE = -\dfrac{GMm}{r}

If the Moon has radius R and density ρ,\rho, then M=43πR3ρM =\dfrac43\pi R^3\rho .

E=GMmr=43πGR3ρmr=43πGR3ρmR+HE = -\dfrac{GMm}{r} = -\dfrac{\frac43 \pi G R^3\rho m}{r} = -\dfrac{\frac43 \pi G R^3\rho m}{R+H} .


b) If H is the maximum height, then the object stops there. Let us determine the total energy of the rock at the surface of the Moon and at the height h

Etot,1=mv2243πGR3ρmRE_{tot,1} = \dfrac{mv^2}{2} - \dfrac{\frac43 \pi G R^3\rho m}{R} ,

Etot,2=043πGR3ρmR+HE_{tot,2} = 0 - \dfrac{\frac43 \pi G R^3\rho m}{R+H} .

Therefore,


mv22=43πGR3ρmR43πGR3ρmR+H=43πGR3ρmR(1RR+H).\dfrac{mv^2}{2} = \dfrac{\frac43 \pi G R^3\rho m}{R} - \dfrac{\frac43 \pi G R^3\rho m}{R+H} = \dfrac{\frac43 \pi G R^3\rho m}{R} \cdot \Big(1 - \dfrac{R}{R+H}\Big).


G=mv2243πρmR2(1RR+H)1,G=3v28πρR2(1RR+H)1.G = \dfrac{mv^2}{2\cdot \frac43\pi \rho m R^2 } \cdot \Big(1 - \dfrac{R}{R+H}\Big)^{-1}, \\ G = \dfrac{3v^2}{8\pi \rho R^2 } \cdot \Big(1 - \dfrac{R}{R+H}\Big)^{-1}.

c) G=3v28πρR2(1RR+H)1=3(30000/3600)28π334017400002(117400001740000+21.5)1=6.6341011Nm2/kg2G = \dfrac{3v^2}{8\pi \rho R^2 } \cdot \Big(1 - \dfrac{R}{R+H}\Big)^{-1} = \dfrac{3\cdot(30000/3600)^2}{8\pi\cdot 3340\cdot 1740000^2}\cdot \Big(1 - \dfrac{1740000}{1740000+21.5} \Big)^{-1} = 6.634\cdot10^{-11}\,\mathrm{N\cdot m^2/kg^2}


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