List of moments of inertia

The moment of inertia, denoted by I, measures the extent to which an object resists rotational acceleration about a particular axis; it is the rotational analogue to mass (which determines an object's resistance to linear acceleration). The moments of inertia of a mass have units of dimension ML² ([mass] × [length]²). It should not be confused with the second moment of area, which has units of dimension L⁴ ([length]⁴) and is used in beam calculations. The mass moment of inertia is often also known as the rotational inertia or sometimes as the angular mass.

For simple objects with geometric symmetry, one can often determine the moment of inertia in an exact closed-form expression. Typically this occurs when the mass density is constant, but in some cases, the density can vary throughout the object as well. In general, it may not be straightforward to symbolically express the moment of inertia of shapes with more complicated mass distributions and lacking symmetry. In calculating moments of inertia, it is useful to remember that it is an additive function and exploit the parallel axis and the perpendicular axis theorems.

This article considers mainly symmetric mass distributions, with constant density throughout the object, and the axis of rotation is taken to be through the center of mass unless otherwise specified.

Moments of inertia

Following are scalar moments of inertia. In general, the moment of inertia is a tensor: see below.

Description	Figure	Moment(s) of inertia	Notes
Point mass M at a distance r from the axis of rotation.		${\displaystyle I=Mr^{2}}$	A point mass does not have a moment of inertia around its own axis, but using the parallel axis theorem a moment of inertia around a distant axis of rotation is achieved.
Two point masses, m1 and m2, with reduced mass μ and separated by a distance x, about an axis passing through the center of mass of the system and perpendicular to the line joining the two particles.		${\displaystyle I={\frac {m_{1}m_{2}}{m_{1}\!+\!m_{2}}}x^{2}=\mu x^{2}}$	Both bodies are treated as point masses: dots of different size indicate the difference in masses of bodies, not in their sizes.
Thin rod of length L and mass m, perpendicular to the axis of rotation, rotating about its center.		${\displaystyle I_{\mathrm {center} }={\frac {1}{12}}mL^{2}\,\!}$  [1]	This expression assumes that the rod is an infinitely thin (but rigid) wire. This is a special case of the thin rectangular plate with axis of rotation at the center of the plate, with w = L and h = 0.
Thin rod of length L and mass m, perpendicular to the axis of rotation, rotating about one end.		${\displaystyle I_{\mathrm {end} }={\frac {1}{3}}mL^{2}\,\!}$  [1]	This expression assumes that the rod is an infinitely thin (but rigid) wire. This is also a special case of the thin rectangular plate with axis of rotation at the end of the plate, with h = L and w = 0.
Thin circular loop of radius r and mass m.		${\displaystyle I_{z}=mr^{2}\!}$ ${\displaystyle I_{x}=I_{y}={\frac {1}{2}}mr^{2}\,\!}$	This is a special case of a torus for a = 0 (see below), as well as of a thick-walled cylindrical tube with open ends, with r1 = r2 and h = 0
Thin, solid disk of radius r and mass m.		${\displaystyle I_{z}={\frac {1}{2}}mr^{2}\,\!}$ ${\displaystyle I_{x}=I_{y}={\frac {1}{4}}mr^{2}\,\!}$	This is a special case of the solid cylinder, with h = 0. That ${\displaystyle I_{x}=I_{y}={\frac {I_{z}}{2}}\,}$ is a consequence of the perpendicular axis theorem.
A uniform annulus (disk with a concentric hole) of mass m, inner radius r1 and outer radius r2		${\displaystyle I_{z}={\frac {1}{2}}m(r_{1}^{2}+r_{2}^{2})}$ ${\displaystyle I_{x}=I_{y}={\frac {1}{4}}m(r_{1}^{2}+r_{2}^{2})}$
An annulus with a constant area density ${\displaystyle \rho _{A}}$		${\displaystyle I_{z}={\frac {1}{2}}\pi \rho _{A}(r_{2}^{4}-r_{1}^{4})}$ ${\displaystyle I_{x}=I_{y}={\frac {1}{4}}\pi \rho _{A}(r_{2}^{4}-r_{1}^{4})}$
Thin cylindrical shell with open ends, of radius r and mass m.		${\displaystyle I=mr^{2}\,\!}$  [1]	The expression ″thin″ indicates that the shell thickness is negligible. It is a special case of the thick-walled cylindrical tube of the same mass for r1 = r2.
Solid cylinder of radius r, height h and mass m.		${\displaystyle I_{z}={\frac {1}{2}}mr^{2}\,\!}$  [1] ${\displaystyle I_{x}=I_{y}={\frac {1}{12}}m\left(3r^{2}+h^{2}\right)}$	This is a special case of the thick-walled cylindrical tube, with r1 = 0.
Thick-walled cylindrical tube with open ends, of inner radius r1, outer radius r2, length h and mass m.		${\displaystyle I_{z}={\frac {1}{2}}m\left(r_{2}^{2}+r_{1}^{2}\right)=mr_{2}^{2}\left(1-t+{\frac {t^{2}}{2}}\right)}$   [1] [2] where ${\displaystyle t={\frac {r_{2}-r_{1}}{r_{2}}}}$ is a normalized thickness ratio; ${\displaystyle I_{x}=I_{y}={\frac {1}{12}}m\left(3\left(r_{2}^{2}+r_{1}^{2}\right)+h^{2}\right)}$[citation needed]	The given formula is for the ${\displaystyle xy}$ plane passing through the center of mass, which coincides with the geometric center of the cylinder. If the xy plane is at the base of the cylinder, i.e. offset by ${\displaystyle d={\frac {h}{2}},}$ then by the parallel axis theorem the following formula applies: ${\displaystyle I_{x}=I_{y}={\frac {1}{12}}m\left(3\left(r_{2}^{2}+r_{1}^{2}\right)+4h^{2}\right)}$
With a density of ρ and the same geometry		${\displaystyle I_{z}={\frac {\pi \rho h}{2}}\left(r_{2}^{4}-r_{1}^{4}\right)}$ ${\displaystyle I_{x}=I_{y}={\frac {\pi \rho h}{12}}\left(3(r_{2}^{4}-r_{1}^{4})+h^{2}(r_{2}^{2}-r_{1}^{2})\right)}$
Regular tetrahedron of side s and mass m with an axis of rotation passing through a tetrahedron's vertex and its center of mass		${\displaystyle I_{\mathrm {solid} }={\frac {1}{20}}ms^{2}\,\!}$ ${\displaystyle I_{\mathrm {hollow} }={\frac {1}{12}}ms^{2}\,\!}$ [3]
Regular octahedron of side s and mass m		${\displaystyle I_{x,\mathrm {hollow} }=I_{y,\mathrm {hollow} }=I_{z,\mathrm {hollow} }={\frac {1}{6}}ms^{2}\,\!}$ [3] ${\displaystyle I_{x,\mathrm {solid} }=I_{y,\mathrm {solid} }=I_{z,\mathrm {solid} }={\frac {1}{10}}ms^{2}\,\!}$ [3]
Regular dodecahedron of side s and mass m		${\displaystyle I_{x,\mathrm {hollow} }=I_{y,\mathrm {hollow} }=I_{z,\mathrm {hollow} }={\frac {39\phi +28}{90}}ms^{2}}$ ${\displaystyle I_{x,\mathrm {solid} }=I_{y,\mathrm {solid} }=I_{z,\mathrm {solid} }={\frac {39\phi +28}{150}}ms^{2}\,\!}$ (where ${\displaystyle \phi ={\frac {1+{\sqrt {5}}}{2}}}$) [3]
Regular icosahedron of side s and mass m		${\displaystyle I_{x,\mathrm {hollow} }=I_{y,\mathrm {hollow} }=I_{z,\mathrm {hollow} }={\frac {\phi ^{2}}{6}}ms^{2}}$ ${\displaystyle I_{x,\mathrm {solid} }=I_{y,\mathrm {solid} }=I_{z,\mathrm {solid} }={\frac {\phi ^{2}}{10}}ms^{2}\,\!}$ [3]
Hollow sphere of radius r and mass m.		${\displaystyle I={\frac {2}{3}}mr^{2}\,\!}$  [1]
Solid sphere (ball) of radius r and mass m.		${\displaystyle I={\frac {2}{5}}mr^{2}\,\!}$  [1]
Sphere (shell) of radius r2 and mass m, with centered spherical cavity of radius r1.		${\displaystyle I={\frac {2}{5}}m\cdot {\frac {r_{2}^{5}-r_{1}^{5}}{r_{2}^{3}-r_{1}^{3}}}\,\!}$  [1]	When the cavity radius r1 = 0, the object is a solid ball (above). When r1 becomes close to r2 the ratio ${\displaystyle {\frac {r_{2}^{5}-r_{1}^{5}}{r_{2}^{3}-r_{1}^{3}}}}$ approaches the value of ${\displaystyle {\frac {5}{3}}r_{2}^{2}}$, and in the limit the body becomes a thin hollow sphere with ${\displaystyle I={\frac {2}{5}}m\cdot {\frac {5}{3}}r_{2}^{2}={\frac {2}{3}}mr_{2}^{2}.}$
Right circular cone with radius r, height h and mass m		${\displaystyle I_{z}={\frac {3}{10}}mr^{2}\,\!}$  [4] About an axis passing through the tip: ${\displaystyle I_{x}=I_{y}=m\left({\frac {3}{20}}r^{2}+{\frac {3}{5}}h^{2}\right)\,\!}$  [4] About an axis passing through the base: ${\displaystyle I_{x}=I_{y}=m\left({\frac {3}{20}}r^{2}+{\frac {1}{10}}h^{2}\right)\,\!}$ About an axis passing through the center of mass: ${\displaystyle I_{x}=I_{y}=m\left({\frac {3}{20}}r^{2}+{\frac {3}{80}}h^{2}\right)\,\!}$ About a slanted axis passing through the apex (origin) and along the side generating line: ${\displaystyle I_{\text{slant}}={\frac {3}{20}}mr^{2}\left(1+5{\frac {h^{2}}{h^{2}+r^{2}}}\right)\,\!}$
Right circular hollow cone with radius r, height h and mass m		${\displaystyle I_{z}={\frac {1}{2}}mr^{2}\,\!}$  [4] ${\displaystyle I_{x}=I_{y}={\frac {1}{4}}m\left(r^{2}+2h^{2}\right)\,\!}$  [4]
Torus with minor radius a, major radius b and mass m.		About an axis passing through the center and perpendicular to the diameter: ${\displaystyle {\frac {1}{4}}m\left(4b^{2}+3a^{2}\right)}$  [5] About a diameter: ${\displaystyle {\frac {1}{8}}m\left(5a^{2}+4b^{2}\right)}$  [5]
Ellipsoid (solid) of semiaxes a, b, and c with mass m		${\displaystyle I_{x}={\frac {1}{5}}m\left(b^{2}+c^{2}\right)\,\!}$ ${\displaystyle I_{y}={\frac {1}{5}}m\left(a^{2}+c^{2}\right)\,\!}$ ${\displaystyle I_{z}={\frac {1}{5}}m\left(a^{2}+b^{2}\right)\,\!}$[6]
Thin rectangular plate of height h, width w and mass m (Axis of rotation at the end of the plate)		${\displaystyle I_{e}={\frac {1}{12}}m\left(4h^{2}+w^{2}\right)\,\!}$
Thin rectangular plate of height h, width w and mass m (Axis of rotation at the center)		${\displaystyle I_{c}={\frac {1}{12}}m\left(h^{2}+w^{2}\right)\,\!}$  [1]
Thin rectangular plate of mass m, length of side adjacent to side containing axis of rotation is r[a](Axis of rotation along a side of the plate)		${\displaystyle I={\frac {1}{3}}mr^{2}}$
Solid rectangular cuboid of height h, width w, and depth d, and mass m.[7]		${\displaystyle I_{h}={\frac {1}{12}}m\left(w^{2}+d^{2}\right)}$ ${\displaystyle I_{w}={\frac {1}{12}}m\left(d^{2}+h^{2}\right)}$ ${\displaystyle I_{d}={\frac {1}{12}}m\left(w^{2}+h^{2}\right)}$	For a cube with sides ${\displaystyle s}$, ${\displaystyle I={\frac {1}{6}}ms^{2}\,\!}$.
Solid cuboid of height D, width W, and length L, and mass m, rotating about the longest diagonal.		${\displaystyle I={\frac {1}{6}}m\left({\frac {W^{2}D^{2}+D^{2}L^{2}+W^{2}L^{2}}{W^{2}+D^{2}+L^{2}}}\right)}$	For a cube with sides ${\displaystyle s}$, ${\displaystyle I={\frac {1}{6}}ms^{2}\,\!}$.
Tilted solid cuboid of depth d, width w, and length l, and mass m, rotating about the vertical axis (axis y as seen in figure).		${\displaystyle I={\frac {m}{12}}\left(l^{2}\cos ^{2}\beta +d^{2}\sin ^{2}\beta +w^{2}\right)}$[8]	For a cube with sides ${\displaystyle s}$, ${\displaystyle I={\frac {1}{6}}ms^{2}\,\!}$.
Triangle with vertices at the origin and at P and Q, with mass m, rotating about an axis perpendicular to the plane and passing through the origin.		${\displaystyle I={\frac {1}{6}}m(\mathbf {P} \cdot \mathbf {P} +\mathbf {P} \cdot \mathbf {Q} +\mathbf {Q} \cdot \mathbf {Q} )}$
Plane polygon with vertices P1, P2, P3, ..., PN and mass m uniformly distributed on its interior, rotating about an axis perpendicular to the plane and passing through the origin.		${\displaystyle I=m{\frac {\sum \limits _{n=1}^{N}Q_{n}\left\|\mathbf {P} _{n+1}\times \mathbf {P} _{n}\right\|}{6\sum \limits _{n=1}^{N}\left\|\mathbf {P} _{n+1}\times \mathbf {P} _{n}\right\|}}}$ where ${\displaystyle Q_{n}=\left\|\mathbf {P} _{n}\right\|^{2}+\mathbf {P} _{n}\cdot \mathbf {P} _{n+1}+\left\|\mathbf {P} _{n+1}\right\|^{2}}$
Plane regular polygon with n-vertices and mass m uniformly distributed on its interior, rotating about an axis perpendicular to the plane and passing through its barycenter. R is the radius of the circumscribed circle.		${\displaystyle I={\frac {1}{2}}mR^{2}\left(1-{\frac {2}{3}}\sin ^{2}\left({\tfrac {\pi }{n}}\right)\right)}$  [9]
An isosceles triangle of mass M, vertex angle 2β and common-side length L (axis through tip, perpendicular to plane)		${\displaystyle I={\frac {1}{2}}mL^{2}\left(1-{\frac {2}{3}}\sin ^{2}\left(\beta \right)\right)}$  [9]
Infinite disk with mass distributed in a Bivariate Gaussian distribution on two axes around the axis of rotation with mass-density as a function of the position vector ${\displaystyle {\mathbf {x} }}$ $${\displaystyle \rho ({\mathbf {x} })=m{\frac {\exp \left(-{\frac {1}{2}}{\mathbf {x} }^{\mathrm {T} }{\boldsymbol {\Sigma }}^{-1}{\mathbf {x} }\right)}{\sqrt {(2\pi )^{2}|{\boldsymbol {\Sigma }}|}}}}$$		${\displaystyle I=m\cdot \operatorname {tr} ({\boldsymbol {\Sigma }})\,\!}$

List of 3D inertia tensors

This list of moment of inertia tensors is given for principal axes of each object.

To obtain the scalar moments of inertia I above, the tensor moment of inertia I is projected along some axis defined by a unit vector n according to the formula:

$${\displaystyle \mathbf {n} \cdot \mathbf {I} \cdot \mathbf {n} \equiv n_{i}I_{ij}n_{j}\,,}$$

where the dots indicate tensor contraction and the Einstein summation convention is used. In the above table, n would be the unit Cartesian basis e_x, e_y, e_z to obtain I_x, I_y, I_z respectively.

Description	Figure	Moment of inertia tensor
Solid sphere of radius r and mass m		${\displaystyle I={\begin{bmatrix}{\frac {2}{5}}mr^{2}&0&0\\0&{\frac {2}{5}}mr^{2}&0\\0&0&{\frac {2}{5}}mr^{2}\end{bmatrix}}}$
Hollow sphere of radius r and mass m		${\displaystyle I={\begin{bmatrix}{\frac {2}{3}}mr^{2}&0&0\\0&{\frac {2}{3}}mr^{2}&0\\0&0&{\frac {2}{3}}mr^{2}\end{bmatrix}}}$
Solid ellipsoid of semi-axes a, b, c and mass m		${\displaystyle I={\begin{bmatrix}{\frac {1}{5}}m(b^{2}+c^{2})&0&0\\0&{\frac {1}{5}}m(a^{2}+c^{2})&0\\0&0&{\frac {1}{5}}m(a^{2}+b^{2})\end{bmatrix}}}$
Right circular cone with radius r, height h and mass m, about the apex		${\displaystyle I={\begin{bmatrix}{\frac {3}{5}}mh^{2}+{\frac {3}{20}}mr^{2}&0&0\\0&{\frac {3}{5}}mh^{2}+{\frac {3}{20}}mr^{2}&0\\0&0&{\frac {3}{10}}mr^{2}\end{bmatrix}}}$
Solid cuboid of width w (x-direction), height h (y-direction), depth d (z-direction), and mass m	180x	${\displaystyle I={\begin{bmatrix}{\frac {1}{12}}m(h^{2}+d^{2})&0&0\\0&{\frac {1}{12}}m(w^{2}+d^{2})&0\\0&0&{\frac {1}{12}}m(w^{2}+h^{2})\end{bmatrix}}}$
Slender rod along y-axis of length l and mass m about end		${\displaystyle I={\begin{bmatrix}{\frac {1}{3}}ml^{2}&0&0\\0&0&0\\0&0&{\frac {1}{3}}ml^{2}\end{bmatrix}}}$
Slender rod along y-axis of length l and mass m about center		${\displaystyle I={\begin{bmatrix}{\frac {1}{12}}ml^{2}&0&0\\0&0&0\\0&0&{\frac {1}{12}}ml^{2}\end{bmatrix}}}$
Solid cylinder of radius r, height h and mass m		${\displaystyle I={\begin{bmatrix}{\frac {1}{12}}m(3r^{2}+h^{2})&0&0\\0&{\frac {1}{12}}m(3r^{2}+h^{2})&0\\0&0&{\frac {1}{2}}mr^{2}\end{bmatrix}}}$
Thick-walled cylindrical tube with open ends, of inner radius r1, outer radius r2, length h and mass m		${\displaystyle I={\begin{bmatrix}{\frac {1}{12}}m(3(r_{2}^{2}+r_{1}^{2})+h^{2})&0&0\\0&{\frac {1}{12}}m(3(r_{2}^{2}+r_{1}^{2})+h^{2})&0\\0&0&{\frac {1}{2}}m(r_{2}^{2}+r_{1}^{2})\end{bmatrix}}}$

See also

• List of second moments of area
• Parallel axis theorem
• Perpendicular axis theorem

Notes

1. Width perpendicular to the axis of rotation (side of plate); height (parallel to axis) is irrelevant.