Final answer:
The magnitude of the acceleration due to gravity, g(R), inside a spherical planet of uniform density can be expressed as (4/3)πGρR. It can also be expressed as gp times a function of R, where gp is the gravitational acceleration at the surface of the planet and f(R) is a function of R.
Step-by-step explanation:
To find the magnitude of the acceleration due to gravity, g(R), inside the planet, we can use the equation:
g(R) = (4/3)πGρR
where ρ is the density of the planet, R is the distance from the center of the planet, and G is the universal gravitational constant. This equation relates the acceleration due to gravity inside the planet to the density and radius of the planet.
g(R) can also be expressed as gp times a function of R:
g(R) = gp * f(R)
where gp is the gravitational acceleration at the surface of the planet and f(R) is a function of R.
The expression for f(R) can be obtained by rearranging the first equation:
f(R) = (4/3)πρ(R/Rp)
where Rp is the radius of the planet.