ApeXaviour
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Okay obviously a hypothetical situation, this planet has a radius R, uniform density, and it doesn't rotate.
Pressure in a liquid is given by
p=\rho g d where d is the depth.
So the liquid pressure a distance r from the centre of the planet is.
p=\rho g (R-r) (where r<R)
But g is also a function of r. A little bit of fiddling with Newton's gravitation law gives:
g(r)=GM\frac{r}{R^3}
So...
p=\rho GM\frac{r}{R^3}(R-r)
This would mean, at r=0 the core of the planet is under zero pressure...! Em, I don't believe this to be correct, so what am I missing? am I slipping up somewhere? Am I putting too much stock in the formula: p=\rho g d?
Pressure in a liquid is given by
p=\rho g d where d is the depth.
So the liquid pressure a distance r from the centre of the planet is.
p=\rho g (R-r) (where r<R)
But g is also a function of r. A little bit of fiddling with Newton's gravitation law gives:
g(r)=GM\frac{r}{R^3}
So...
p=\rho GM\frac{r}{R^3}(R-r)
This would mean, at r=0 the core of the planet is under zero pressure...! Em, I don't believe this to be correct, so what am I missing? am I slipping up somewhere? Am I putting too much stock in the formula: p=\rho g d?