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Juliette [100K]
3 years ago
6

Gravitational Acceleration inside a Planet

Physics
1 answer:
vazorg [7]3 years ago
3 0

Answer:

PART A

g(R) = \frac{G(rho)(4)\pi R}{3} ;

PART B

g(R) = g(Rp) × \frac{R}{Rp}.

Explanation:

Given density of planet = rho.

The planet's radius = Rp.

An object is located a distance R from the center of the planet,

where R< Rp.

The gravitational fore between two point masses m₁ and m₂ is,

F = \frac{Gm_{1}m_{2}}{r^{2} } ; G= universal gravitational constant

                                                                 r = distance between the masses.

for mass m₂ , F=  m₂ g;  where g = acceleration due to gravity;

so, g = \frac{F}{m_{2} } =  \frac{Gm_{1}}{r^{2} };

From figure, only inside part of the planet exerts force and which can be treated as a point mass.

so, g =  \frac{Gm_{R}}{R^{2} }

where m_{R} = mass of the planet with radius R.

⇒  m_{R} = rho × \frac{4}{3}×\pi×R³

 ⇒ g(R) = \frac{G(rho)(4)\pi R}{3} →  PART A

        PART B

  At the surface g(Rp) =  \frac{G(rho)(4)\pi Rp}{3}

⇒  g(R) = g(Rp) × \frac{R}{Rp}

         

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Answer:

Explanation:

Hi!

In order to obtain the Lagrangian of the system we must first write the Kinetic and Potential Energies. Lets orient our axes such that the axis of the cone coincide with the z axis. In cilindrical coordinates we have

v^{2} = \frac{dr}{dt}^{2}  +r^{2} \frac{d\theta }{dt} ^{2} +\frac{dz}{dt} ^{2} - (1)

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replacing (2) in (1) we obtain:

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Now the kinetic energy is given as:

T = \frac{1}{2}m(\frac{dr}{dt}^{2} (1+cot(45))+r^{2}\frac{d\theta }{dt} ^{2}) - (4)

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So the Langrangian is given by:

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