Step 1: Find the gravitational field inside the sphere.
The mass enclosed within a radius r (where r<R) for a constant density ρ is given by the volume of the inner sphere.
M(r)=34πρr3
The gravitational acceleration at radius r depends only on this enclosed mass.
g(r)=r2GM(r)
g(r)=34πGρr
Step 2: Set up the hydrostatic equilibrium equation.
The pressure gradient balances the inward gravitational force.
drdP=−ρg(r)
Substitute the expression for g(r).
drdP=−34πGρ2r
Step 3: Integrate to find the pressure profile P(r).
Integrate from radius r to the surface R, using the boundary condition that pressure at the surface is zero, P(R)=0.
∫P(r)0dP=−∫rR34πGρ2rdr
−P(r)=−32πGρ2(R2−r2)
P(r)=32πGρ2(R2−r2)
This can be written in terms of the central pressure Pc=P(0).
P(r)=Pc(1−R2r2)
Pc=32πGρ2R2
Step 4: Evaluate the pressure at the center.
Check the first option by evaluating the pressure at r=0.
P(0)=Pc=0
The pressure at the center is non-zero, so the first option is incorrect.
Step 5: Evaluate the ratio of pressures for the remaining options.
The ratio of pressures at any two distances a and b simplifies by canceling the constant factors.
P(b)P(a)=R2−b2R2−a2
Test the ratio for a=43R and b=32R.
P(32R)P(43R)=1−941−169
P(32R)P(43R)=95167
P(32R)P(43R)=8063
Test the ratio for a=53R and b=52R.
P(52R)P(53R)=1−2541−259
P(52R)P(53R)=25212516
P(52R)P(53R)=2116
Test the ratio for a=2R and b=3R.
P(3R)P(2R)=1−911−41
P(3R)P(2R)=9843
P(3R)P(2R)=3227=2720
Answer:
The correct options are:
- P(43R)/P(32R)=8063
- P(53R)/P(52R)=2116