The master equation of orbits: v² = GM(2/r − 1/a) — speed at distance r depends only on the semi-major axis a (the orbit’s energy). Circle (a=r) gives v²=GM/r; parabola (a=∞) gives escape; hyperbola (a<0) is unbound. One line covers the whole family. The name is Leibniz’s old term for living force.
The demo shows the circle case (a=r) collapses to GM/r, and computes an ellipse’s speed: live demo
“Speed in orbit depends on where you are.” — it depends on r AND on a; two orbits crossing the same point at different a have different speeds. cited
Energy, written as a speed. physics
On i-13, the circle case (a=r) equals GM/r exactly; an ellipse gives a different v²: