Gravitational attraction of a hemisphere at its pole

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Homework Help Overview

The discussion revolves around calculating the gravitational attraction of a solid hemisphere with a specified radius and density at its pole, where a unit point mass is placed. The problem is situated within the context of gravitational fields and involves the use of spherical coordinates for integration.

Discussion Character

  • Exploratory, Mathematical reasoning, Assumption checking

Approaches and Questions Raised

  • The original poster attempts to set up an integral using spherical coordinates and expresses uncertainty about the correctness of their integrand. They also seek clarification on how to establish the lower circular bound in their calculations. Other participants suggest leveraging symmetry and consider the gravitational field due to mass distribution, while questioning the interpretation of the problem's requirements.

Discussion Status

The discussion is ongoing, with participants exploring different methods and interpretations of the problem. Some guidance has been offered regarding the use of symmetry and the slicing method, but no consensus has been reached on the correct approach or limits for the integrals.

Contextual Notes

There are indications of potential confusion regarding the setup of the problem, particularly in relation to the coordinate system and the limits of integration. The original poster is focused on the gravitational attraction specifically at the pole of the hemisphere.

ozone
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Find the gravitational attraction of a solid hemisphere of radius a anddensity1 on a unit point mass placed at its pole.

My attempt:

Obviously I figured that spherical coordinates would work nicely for this problem.

I decided to invert the hemisphere thus placing the pole on the origin. Then I decided to split the upside down quarter disc into two integrals. The first integral was then for a cone shaped figure (r1 in the picture i made).

I set it up as follows

G \int_{\vartheta=0}^{2\pi} \int_{<br /> \varphi=0}^{\pi/3}\int_{\rho=0}^{a/sin(\phi)} sin(\phi)cos(\phi)d\phi d\rho d\theta

Plz let me know if i have made any mistakes with the above integrand (pi/3 is where a cone will intersect a circle of equal radius).

However I could not manage to think up the equation (in spherical coordinates) for the lower circular bound. I considered changing coordinate systems for the outer spherical part but setting up the equation for force of gravity might have been tricky. Any help will be greatly appreciated.
 

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well it would be given as the field due to the total mass within a gaussian surface through the point as if all that mass were concentrated at the center of mass.

Note: you can make your life easier by exploiting the symmetry even further - can you find the field at a perpendicular distance r from a disk radius R and thickness dz?
 
Simon Bridge said:
well it would be given as the field due to the total mass within a gaussian surface through the point as if all that mass were concentrated at the center of mass.

Note: you can make your life easier by exploiting the symmetry even further - can you find the field at a perpendicular distance r from a disk radius R and thickness dz?

Yes I could but were looking for the gravitational attraction on the surface of the pole since that is where the unit mass is placed, or am i misinterpreting you?
 
You sort-of have ... if you orient the hemesphere so it's axis is the z axis, and slice it into disks thickness dz, then the biggest disk (the base) will be distance R from the test mass.

I just have a feeling you've not got one of the limits right ... one of the advantages of the slice method is that you can conceptually check each stage. Still - run with what you are comfy with ;)
 

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