Two planets of equal masses orbit a much more massive star. Planet \(m_1\) moves in a circular orbit of radius \(1 \times 10^8~\text{ km}\) with a period of \(2~\text{ years}\) and planet \(m_2\) moves in an elliptical orbit with closest distance \(r_1 = 1 \times 10^8~\text{km}\) and farthest distance \(r_2 = 1.8 \times 10^8~\text{km}\), as shown:
Compare the speed of planet \(m_2\) at \(\text{P}\)\((V_P)\) with that of at \(\text{A}\) \((V_A)\).