Gravity due a hemispherical planet

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The discussion revolves around calculating gravity on a hemispherical planet, with the correct formula identified as g = πGρR. The user initially misapplied the distance in the gravitational formula, using R instead of r for the denominator. A correction was provided, emphasizing that not all volume elements (dV) are at a distance R from the origin, necessitating the use of r² instead. The user acknowledged the mistake and expressed gratitude for the clarification. The conversation highlights the importance of proper variable application in gravitational calculations.
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Homework Statement
find the acceleration due to gravity at the centre of a solid hemisphere.
Relevant Equations
##dg=\frac {GMdm}{r^2}##
Can someone help me? I am not sure where is my mistake

correct answer:
##g=\pi G\rho R##

my calculus
By symmetry, I only need to add the vertical component of gravity
##dg = \frac {GMdm}{d^2}\cdot cos\theta## (1) Where d=R
##\rho =\frac{dm}{dV} ##
##dm = \rho \cdot dV## (2)

(2) in (1)

##dg = \frac {G \rho cos\theta dV}{R^2}##

for spherical coordinate $$dV = r^2drsin\theta d\theta d\phi$$

so:
##dg=\frac {G\rho }{R^2} r^2dr sin\theta cos\theta d\theta d\phi##

##g=\frac {G\rho}{R^2} \int_0^R r^2 \, dr \int_0^\frac {\pi}{2} sin\theta cos\theta \, d\theta \int_0^{2\pi} \, d\phi##

##g = \frac {G\rho}{R^2} \cdot \frac{R^3}{3} \cdot \frac {1}{2} \cdot 2\pi##

##g = \frac {G\rho R\pi}{3}##

##g=\frac {\pi G\rho R}{3}##
 
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Yalanhar said:
Can someone help me? I am not sure where is my mistake

Here is your mistake.
Yalanhar said:
##dg = \frac {G \rho cos\theta dV}{R^2}##
Not all elements ##dV## are at distance ##R## from the origin. The denominator should be ##r^2##.
 
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kuruman said:
Here is your mistake.

Not all elements ##dV## are at distance ##R## from the origin. The denominator should be ##r^2##.
oh yes. I got it now. Thanks!
 
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