The displacement of sun with respect to earth is what
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r2 According to formula of Gravitational Force
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The sun's displacement from the earth is r2 d.
This 16-minute shift equates to a movement eastward or westward of around four degrees in the apparent position of the Sun, compared to its mean location, since the Earth spins at a mean speed of one degree every four minutes relative to the Sun.
The gap between the body's initial and final positions is known as displacement. The earth returns to its original location after one full revolution. As a result, the distance between the starting and ending positions is zero.
As a result, the earth's displacement is zero.
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