As an example, we compute the tidal tensor for the vacuum field outside an isolated spherically symmetric massive object in two different ways.
Let us adopt the frame obtained from the polar spherical chart for our three-dimensional Euclidean space:
We will directly compute the tidal tensor, expressed in this frame, by elementary means, as follows. First, compare the gravitational forces on two nearby observers lying on the same radial line:
Because in discussing tensors we are dealing with multilinear algebra, we retain only first order terms, so . Similarly, we can compare the gravitational force on two nearby observers lying on the same sphere . Using some elementary trigonometry and the small angle approximation, we find that the force vectors differ by a vector tangent to the sphere which has magnitude
By using the small angle approximation, we have ignored all terms of order , so the tangential components are . Combining this information, we find that the tidal tensor is diagonal with frame components This is the Coulomb form characteristic of spherically symmetric central force fields in Newtonian physics.
Next, let us plug the gravitational potential into the Hessian. We can convert the expression above to one valid in polar spherical coordinates, or we can convert the potential to Cartesian coordinates before plugging in. Adopting the second course, we have , which gives
After a rotation of our frame, which is adapted to the polar spherical coordinates, this expression agrees with our previous result. (The easiest way to see this is probably to set y,z to zero so that the off-diagonal terms vanish and , and then invoke the spherical symmetry.)