A central force exerts no torque about the center because it acts along the radius. The spacecraft's angular momentum therefore stays constant during the ideal coast. Per unit mass its magnitude is h = r vₜ, where vₜ is the component of velocity perpendicular to the radius.
A component is a vector's part along a chosen direction. Resolve velocity into a radial component toward or away from the planet and a transverse component at right angles to the radius. At periapsis and apoapsis the radial component is zero. There, the entire velocity is transverse, so rₚvₚ = rₐvₐ.
This also explains equal swept areas. Over a short time Δt, the swept triangle has area approximately ½ r vₜ Δt = ½ h Δt. Constant h means equal area for equal time. Elsewhere on the ellipse, replacing vₜ with the total speed would be wrong because some motion is radial.
Thrust can change energy and angular momentum. Drag generally removes both from a prograde orbit. Conservation claims in these lessons apply to the unpowered two-body coast, not to a maneuver with an engine running.
Use components to distinguish orbits with equal energy
At a given point, choose one direction straight outward from the planet and another perpendicular to it in the orbital plane. Decompose the velocity into these radial and transverse parts. The radial part changes distance from the center. The transverse part changes direction around the center. The two components combine to produce the actual velocity, which need not point along either chosen direction.
For a concrete pair of states at radius 10,000 km, let craft A move entirely transversely at 5 km/s. Let craft B have outward radial speed 3 km/s and transverse speed 4 km/s. The right-triangle relation gives B the same total speed, 5 km/s. Both have kinetic energy 12.5 MJ/kg and potential energy about negative 39.860 MJ/kg, so their total specific energies match. Their paths nevertheless differ.
A's specific angular momentum is 10,000 times 5, or 50,000 square kilometers per second. B's is 10,000 times 4, or 40,000 in the same units. B's radial motion contributes nothing to this magnitude. Equal energy therefore does not imply equal angular momentum. The states have the same semi-major axis in the ideal bound model but different eccentricities. A complete orbit calculation must preserve both pieces of information.
Why is angular momentum conserved under gravity alone? Torque measures a force's tendency to turn momentum about a chosen center. A force directed exactly along the radius has no sideways lever arm about that center. Its torque there is zero. This preserves the angular momentum vector during the coast. Its direction also fixes the orbital plane. A thrust component outside that plane can change this vector, which is why plane changes require a maneuver.
The transverse speed itself is not generally constant. The product of radius and transverse speed is constant. As radius increases, transverse speed must fall to keep that product unchanged. The radial and transverse directions also rotate as the craft moves. Saying that gravity has no transverse component at each instant does not justify holding the numerical transverse speed fixed while changing the radius and the local coordinate directions.
At the apsides, radial speed vanishes, so total speed equals transverse speed. Multiplying 7,000 km by approximately 8.604 km/s and 13,000 km by approximately 4.633 km/s gives nearly the same angular momentum, with a small mismatch if you use rounded speeds. Taking the ratio before rounding gives the inverse radius ratio, thirteen sevenths. Between the apsides, multiplying radius by total speed would include radial motion and fail this check.
The swept-area argument now follows directly. Over a short interval, the radius is one side of a thin triangle and transverse displacement supplies its height. Its area is approximately half of radius times transverse speed times elapsed time. The first two factors form the conserved specific angular momentum. Equal elapsed times therefore produce equal areas. Energy explains how speed changes with radius; angular momentum explains how much of that motion is transverse.
When examining a simulation, check conserved quantities only during intervals where their assumptions hold. A successful burn should change the orbit's energy or angular momentum, so demanding the old values after the burn would be a faulty test. During a gravity-only coast, however, unexplained drift can indicate numerical or implementation error. Separate physical changes in the modeled system from errors introduced by the method used to calculate it.