Derivative of a Rotation Matrix with changing rotation axis Just to introduce the background of this question: As many of you know a Rotation Matrix can transform a point $^{B}\textrm{p}$ described in a rotated Coordinate Frame {B} into the point $^{A}\textrm{p}$ described in the Coordinate Frame {A} by:
$^{A}\textrm{p}$=$^{A}\textrm{R}_B \ ^{B}\textrm{p}$ 
The Rotation Matrix's $^{A}\textrm{R}_B$ columns are the unit vectors of {B}'s axis described in Frame {A}.
Also the Rotation about a given axis can be given by:
$^{A}\textrm{R}_B$=$e^{[\hat{w}]_x\theta}$ , whereas $[\hat{w}]_x$ is the skew-symmetric 3x3 matrix of the unit vector of $\hat{w}$ (deschribed in Frame A), around which the Frame is being rotated. $\theta$ is the rotation angle (and a scalar).
Now my question:
Almost every book and paper i found states that the time-derivative of the Rotation Matrix is the following:
$\frac{d}{dt}(^{A}\textrm{R}_B)$= $[w]_x \  ^{A}\textrm{R}_B \qquad (1)$ 
Does the solution require that the direction of $\hat{w}$ remains constant at all times?
Because if we use the chain rule on with a (1):
$\frac{d}{dt}e^{[\hat{w}]_x\theta}$ = $\frac{d}{dt}([\hat{w}(t)]_x\theta(t)) \cdot e^{[\hat{w}]_x\theta}$ = $\frac{d}{dt}([\hat{w}(t)]_x)\theta(t) e^{[\hat{w}(t)]_x\theta(t)} + [\hat{w}(t)]_x)\dot{\theta}(t) e^{[\hat{w}(t)]_x\theta(t)}$
which can be further simplified to:
$\frac{d}{dt}e^{[\hat{w}]_x\theta}$ = $(\frac{d}{dt}([\hat{w}(t)]_x)\theta(t)  + [w(t)]_x)^{A}\textrm{R}_B$ 
Whereas $[w(t)]_x=[\hat{w}(t)]_x\theta(t)$
Thus this is not equal to (1) and an addition term is generated.
So which of these equations is true now, when the rotation is not being done around a constant axis? Or did i do something wrong?
Greetings,
1lc
 A: As you noticed in your comment, the time (single-parameter) derivative of the matrix exponential doesn't have a nice form analogous to the scalar exponential.
Your Equation 1 is essentially the definition of the "angular velocity" vector $\omega$. An orthogonal time-varying matrix $R(t)$ always satisfies,
$$
R R^T = \mathbf{1} \ \ \ \ \forall t
$$$$
\implies\ \ \dot{R} R^T + R \dot{R}^T = \mathbf{0}\ \ \ \ \forall t
$$
We define the following also time-varying matrix,
$$
\Omega := \dot{R} R^T\ \ \ \ \forall t
$$
and note that, from the above, it is always skew-symmetric,
$$
\dot{R} R^T = -R \dot{R}^T\ \ \implies\ \ \Omega = -\Omega^T\ \ \ \ \forall t
$$
Thus $\Omega$ can be treated as the cross-product linear operator form of some time-varying vector $\omega(t)$. By simple rearrangement of the $\Omega$ definition, we have your Equation 1,
\begin{equation}
\dot{R} = [\omega]^{\times} R\ \ \ \ \forall t
\end{equation}
If $R$ rotates some $B$-coordinates to $A$-coordinates then we call $\omega$ the angular velocity expressed in $A$-coordinates.
In conclusion, your Equation 1 holds even for time-varying $\omega$, essentially by definition.
It is a linear time-varying matrix ODE, but don't take the "matrix" part lightly. The solution is non-trivial unless the direction of $\omega$ is constant. This is due to the lack of commutivity of the Lie group $\mathbb{SO}$. Hopefully that clears things up!
