What is Jacobian matrix?

Last updated: 2026-04-12

The Jacobian, or rather its modulus, is a measure of how a general mapping stretches space locally, near a particular point, even when this stretching effect varies from point to point. The Jacobian takes its name from the German mathematician Carl Jacobi (1804-1851).
Definition
Given two co-ordinates u(x,y)u(x,y) and v(x,y)v(x,y) which depend on variables xx and yy, we define the Jacobian
(u,v)(x,y)\begin{equation*}\frac{\partial(u,v)}{\partial(x,y)}\end{equation*}
to be the determinant
uxuyvxvy.\begin{equation*}\begin{vmatrix}\frac{\partial u}{\partial x} & \frac{\partial u}{\partial y} \\\frac{\partial v}{\partial x} & \frac{\partial v}{\partial y}\end{vmatrix}.\end{equation*}

Motivation and Examples

Illustration how area changes under mapping x=rcosθx = r\cos\theta and y=rsinθy = r\sin\theta
Let x=rcosθx = r\cos\theta and y=rsinθy = r\sin\theta where rr and θ\theta are polar co-ordinates. Then
(x,y)(r,θ)=det(xrxθyryθ)=det(cosθrsinθsinθrcosθ)=r(cos2θ+sin2θ)=r.\begin{align*}\frac{\partial(x,y)}{\partial(r,\theta)} &= \det\begin{pmatrix}\frac{\partial x}{\partial r} & \frac{\partial x}{\partial \theta} \\\frac{\partial y}{\partial r} & \frac{\partial y}{\partial \theta}\end{pmatrix} \\&= \det\begin{pmatrix}\cos\theta & -r\sin\theta \\\sin\theta & r\cos\theta\end{pmatrix} \\&= r(\cos^2\theta + \sin^2\theta) = r.\end{align*}

Mathematical justification for Jacobian

Theorem
Let f:RS\mathbf{f}: R \to S be a bijection between two regions of R2\mathbb{R}^2, which is differentiable and has differentiable inverse with
(u,v)(x,y),(x,y)(u,v),\begin{equation*}\frac{\partial(u,v)}{\partial(x,y)}, \quad \frac{\partial(x,y)}{\partial(u,v)},\end{equation*}
defined and non-zero everywhere. Further, write (u,v)=f(x,y)(u,v) = \mathbf{f}(x,y) and let ψ(x,y)=Ψ(u,v)\psi(x,y) = \Psi(u,v). Then
(u,v)SΨ(u,v)dudv=(x,y)Rψ(x,y)(u,v)(x,y)dxdy,\begin{equation*}\iint_{(u,v)\in S} \Psi(u,v)\,du\,dv = \iint_{(x,y)\in R} \psi(x,y)\left|\frac{\partial(u,v)}{\partial(x,y)}\right|\,dx\,dy,\end{equation*}(x,y)Rψ(x,y)dxdy=(u,v)SΨ(u,v)(x,y)(u,v)dudv.\begin{equation*}\iint_{(x,y)\in R} \psi(x,y)\,dx\,dy = \iint_{(u,v)\in S} \Psi(u,v)\left|\frac{\partial(x,y)}{\partial(u,v)}\right|\,du\,dv.\end{equation*}
\end{theorem}
\quad Proof. It is sufficient to prove the first integral identity.

Split the region into squares

Divide the region RR into NN square elements of equal area δxδy\delta x\delta y as previously with ψi\psi_i; the scalar field at the centre of the ithi^{th} element, i{1,N}i \in \{1,\ldots N\}.
Consider the mapping of the ithi^{th} element, which is bounded by the co-ordinate lines x=xix = x_i and x=xi+δxx = x_i + \delta x and y=yiy = y_i and y=yi+δyy = y_i + \delta y. The value of the scalar field at the mapped element centre is
Ψi=Ψ(f(xi+δx/2,yi+δy/2))=ψi=ψ(xi+δx/2,yi+δy/2).\begin{equation*}\Psi_i = \Psi(\mathbf{f}(x_i + \delta x/2, y_i + \delta y/2)) = \psi_i = \psi(x_i + \delta x/2, y_i + \delta y/2).\end{equation*}

Change the area of squares under the mapping

Also, given sufficiently small δx\delta x, δy\delta y the ithi^{th} element maps to an image region, denoted IMiIM_i, which is a deformed parallelogram spanned by the vectors
a=f(xi+δx,yi)f(xi,yi)fx(xi,yi)δx,b=f(xi,yi+δy)f(xi,yi)fy(xi,yi)δy,\begin{align*}\mathbf{a} &= \mathbf{f}(x_i + \delta x, y_i) - \mathbf{f}(x_i, y_i) \approx \frac{\partial\mathbf{f}}{\partial x}(x_i, y_i)\,\delta x, \\\mathbf{b} &= \mathbf{f}(x_i, y_i + \delta y) - \mathbf{f}(x_i, y_i) \approx \frac{\partial\mathbf{f}}{\partial y}(x_i, y_i)\,\delta y,\end{align*}
and, thus, of area
fxδxfyδy=fxfyδxδy.\begin{equation*}\left|\frac{\partial\mathbf{f}}{\partial x}\,\delta x \wedge \frac{\partial\mathbf{f}}{\partial y}\,\delta y\right| = \left|\frac{\partial\mathbf{f}}{\partial x} \wedge \frac{\partial\mathbf{f}}{\partial y}\right|\delta x\,\delta y.\end{equation*}
Now f=(u,v)\mathbf{f} = (u,v), so fx=(ux,vx)\mathbf{f}_x = (u_x, v_x), fy=(uy,vy)\mathbf{f}_y = (u_y, v_y) and thus
fxfyδxδy=(ux,vx)(uy,vy)δxδy=(uxvyuyvx)kδxδy=(u,v)(x,y)δxδy.\begin{equation*}\left|\frac{\partial\mathbf{f}}{\partial x} \wedge \frac{\partial\mathbf{f}}{\partial y}\right|\delta x\delta y = |(u_x, v_x) \wedge (u_y, v_y)|\delta x\delta y = |(u_x v_y - u_y v_x)\mathbf{k}|\delta x\delta y = \left|\frac{\partial(u,v)}{\partial(x,y)}\right|\delta x\delta y.\end{equation*}

Approximation of the integral

Thus, before taking limits, partitioning SS by the images IMiIM_i, we have an approximation for
(u,v)SΨ(u,v)dudv\begin{equation*}\iint_{(u,v)\in S} \Psi(u,v)du\,dv\end{equation*}
which is
i=1NΨiArea(IMi)=i=1NΨi(u,v)(x,y)δxδy=i=1Nψi(u,v)(x,y)δxδy.\begin{equation*}\sum_{i=1}^N \Psi_i\text{Area}(IM_i) = \sum_{i=1}^N \Psi_i\left|\frac{\partial(u,v)}{\partial(x,y)}\right|\delta x\delta y = \sum_{i=1}^N \psi_i\left|\frac{\partial(u,v)}{\partial(x,y)}\right|\delta x\delta y.\end{equation*}
Taking limits gives
(u,v)SΨ(u,v)dudv=(x,y)Rψ(x,y)(u,v)(x,y)dxdy.\begin{equation*}\iint_{(u,v)\in S} \Psi(u,v)du\,dv = \iint_{(x,y)\in R} \psi(x,y)\left|\frac{\partial(u,v)}{\partial(x,y)}\right|dx\,dy. \quad \Box\end{equation*}

References