Write the observation point as with , reserving source coordinates for the integral. For the straight segment, and the separation is . Therefore its Newtonian gravitational potential is
Equivalently . At large it approaches , the Newtonian potential of a point mass with the segment's total mass.
Use source polar coordinates , on the semicircular disk, with and . Its surface area element is , and the separation from is . Thus
This Newtonian gravitational potential is half that of the full disk because the separation is independent of the polar angle. At large it approaches , with the correct total mass.
Use source spherical coordinates with radius , polar angle measured from the positive -axis, and azimuth . The lower half of the spherical shell has , , and . Its volume element is . At the observation point , , the separation is , so
The angular integral is elementary: put to obtain
We used since both are positive. Hence
Thus the axial potential of a uniform hemispherical shell, at every point of the positive -axis, is
There is no need to split into , , and : the observation point is outside the lower hemisphere in all three cases. As checks, as , and at large ,
The last factor is exactly the total mass of the lower half of the spherical shell.

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