Density specifies how mass varies throughout the body and allows each infinitesimal element to be assigned a mass dm. Integrating the contributions from all such elements then produces whole-body quantities. If density is not uniform, regions with different mass content contribute unequally, so the resulting center of mass, inertia, torque, or gravitational field reflects the actual distribution.
The center of mass depends on how mass is distributed, not solely on the body's shape or dimensions. A region containing more mass has greater influence on the integrated position than a lighter region. Consequently, a nonuniform density can shift the center of mass away from the geometric center, affecting how the body is analyzed in mechanical and gravitational problems.
Moment of inertia depends on where the body's mass lies relative to the relevant axis. Mass positioned farther from that axis contributes differently from mass positioned closer to it, so two bodies with the same total mass can have different rotational behavior. Integrating these contributions across the shape captures effects that a point-mass model cannot represent.
A gravitational field produced by an extended body reflects contributions from many mass elements, and those contributions can differ in direction and magnitude across space. Integrating the elements combines their effects into the resulting field. This treatment is important when the body's finite size and shape make a single concentrated mass an inadequate representation of the interaction.
Begin by describing the body's shape and mass distribution with a density function, then divide it conceptually into infinitesimal elements carrying mass dm. Express the desired contribution from each element and integrate over the body's volume. The same workflow can yield the center of mass, moment of inertia, torque, or gravitational field, depending on the quantity being calculated.
An extended-mass model is appropriate when finite size, shape, or internal mass distribution can significantly affect the result. It supports analysis of real bodies in rigid-body motion, rotational dynamics, and gravitational interactions. A point-mass approximation may omit these effects, whereas integration preserves the spatial information needed to obtain more representative mechanical or gravitational quantities.
This approach connects a body's physical distribution to measurable mechanical descriptions, including its center of mass, moment of inertia, torque, and gravitational field. Those results help characterize both translational and rotational behavior and can be applied to orbital interactions. In this way, the method links mathematical integration with models of real objects rather than idealized concentrated masses.