Second Kepler's law explanation What is the explanation for the second Kepler's law? Why is the law valid?
Is it that the total energy of a planet equals to the kinetic energy plus the potential energy?
 A: The area of a sector is $A = \frac{1}{2}r^2 \theta$ and for small changes in time (where the distance of the planet to the sun is assumed constant), the rate that the area is swept out is $\frac{dA}{dt} = \frac{1}{2}r^2 \omega$
For orbits the angular momentum is constant, so $mr^2\omega$ is constant and that means that the rate that the area is swept out is constant too.
So we could compare the area swept out by the earth around the Sun for a day in January (for example), when it's closest and a day in July when it's furthest away and the areas would be the same.
A: Kepler's second law
according to Newton's second law
$$m\,\mathbf{\ddot{r}}=F(r)\,\frac{\mathbf r}{r}$$
where $~F(r)~$ is central force
from here
$$\mathbf r\times m\,\mathbf{\ddot{r}}=\frac{F(r)}{r}\left(\mathbf r\times \mathbf r\right)=\mathbf 0$$
with
$$\frac{d}{dt}\left(\mathbf r\times m\,\mathbf{\dot{r}}\right)=
\mathbf{\dot{r}}\times m\,\mathbf{\dot{r}}+\mathbf r\times m\,\mathbf{\ddot{r}}=
\mathbf 0$$
hence
$$ \mathbf r\times m\,\mathbf{\dot{r}}=\mathbf L=\textbf{const.}\tag 1$$
this is the conservation of the angular momentum
additional from equation (1) you obtain that $\mathbf r\cdot \mathbf L=\mathbf 0~$ this means that $~\mathbf r\perp\mathbf L~$ so the mass point m has a planner motion
from equation (1) $~\mathbf r\times \mathbf{\dot{r}}=\frac{\textbf{const.}}{m}$ with  polar coordinate you obtain
$$\mathbf r=r\,\begin{bmatrix}
  \cos(\varphi) \\
  \sin(\varphi) \\
  0 \\
\end{bmatrix}\\
\mathbf{\dot{r}}=\left[ \begin {array}{c} \cos \left( \varphi  \right) {\dot r}-r\sin
 \left( \varphi  \right) \dot\varphi \\ \sin \left( 
\varphi  \right) {\dot r}+r\cos \left( \varphi  \right) \dot\varphi 
\\ 0\end {array} \right]\quad \Rightarrow\\
|\mathbf r\times \mathbf{\dot{r}}|=r^2\,\dot\varphi
$$
or $$\frac{d A}{dt}=\frac 12 r^2\,\dot\varphi\\
\boxed{~A=\frac 12 r^2\,\varphi}$$
Kepler's second law

A: Kepler's second law (a line segment joining a planet and the Sun sweeps out equal areas during equal intervals of time) is a consequence of conservation of angular momentum. It applies not just to gravity, but also to motion under any central force i.e. a force that is always direct towards a fixed point.
Of course, Kepler himself derived his three laws empirically, by observing the motions of the known planets. It was Newton who proved that the Kepler's first and third laws are a consequence of the inverse-square nature of gravity, and that Kepler's second law applies more generally to any central force.
