You are asked to verify Kepler's Laws of Planetary Motion. For these exercises, assume that each planet moves in an orbit given by the vector-valued function $\mathbf{r}$. Let $\boldsymbol{r}=\|\mathbf{r}\|$, let $\boldsymbol{G}$ represent the universal gravitational constant, let $M$ represent the mass of the sun, and let $m$ represent the mass of the planet.
Prove that $\frac{d}{d t}\left[\frac{\mathbf{r}}{r}\right]=\frac{1}{r^{3}}\left\{\left[\mathbf{r} \times \mathbf{r}^{\prime}\right] \times \mathbf{r}\right\}$