Spherical aberration is a description of the fact that a spherical mirror has a focal length (call it ff) for light striking it far from the central axis that differs from the focal length (call it fc) for light striking it close to the central axis. By taking the "limiting" case of a hemisphere it becomes clear that
A) ff < fc for the outer rays not "far" from as well as for outer rays farther from the central axis.
B) ff < fc for the outer rays not "far" from the central axis, and ff > fc for outer rays farther from the central axis.
C) ff > fc for the outer rays not "far" from the central axis, and ff < fc for outer rays farther from the central axis.
D) ff > fc for the outer rays not "far" from as well as for outer rays farther from the central axis.
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