Integral Calculus provides the mathematical backbone for processes like adding up small, infinitely thin slices or sections of a geometric shape to find area or volume. In the case of deriving the formula for the volume of a sphere using Kepler’s method, integral calculus plays a pivotal role.
With the formula for the volume of an infinitesimal cone derived, \(dV = \frac{1}{3}r \, dA\), integral calculus aids in summing up these small volumes efficiently. We perform an integral to accumulate the volume of all infinitesimal cones, represented as:
- Initialize by setting up the integral \(V_{sphere} = \int dV = \int \frac{1}{3}r \, dA\).
- Recognize that the total surface area a across which we integrate these cones is the surface area of the sphere, \(4\pi r^2\).
- Executing the integral \(\int dA\) over this surface area parameterizes the final volume calculation: \(V_{sphere} = \frac{1}{3}r (4\pi r^2)\).
This results in revealing the classic formula for the volume of a sphere, \(V_{sphere} = \frac{4}{3}\pi r^3\). Integral Calculus elegantly pieces together the infinitesimal to reveal a comprehensive whole.