For a conservative model, total energy limits the positions and speeds a body can have. Energy can therefore constrain a motion solver before you run a detailed trajectory.
Set mass and height. In this no-loss model, gravitational potential energy becomes kinetic energy at ground level.
Potential energy 98.07 J; predicted landing speed 9.90 m/s; kinetic energy 98.07 J.
For a one-dimensional conservative model, calculate remaining kinetic energy at a candidate location:
\[K(x)=E_{\mathrm{total}}-U(x), \qquad |v(x)|=\sqrt{\frac{2K(x)}{m}}.\]If remaining kinetic energy is below zero beyond a documented tolerance, that location is forbidden by the supplied total energy. If it is zero, it is a turning point. Return a tagged result such as allowed, turning point, or forbidden alongside the named total energy, potential, kinetic energy, mass, potential reference, and units. Do not pass a negative kinetic value to a square root and display an invented speed.
Energy does not choose the velocity sign. A particle at the same position and speed magnitude can travel left or right, and multidimensional motion needs direction or angular momentum data. A full solver uses force (F=-dU/dx) or a declared gradient to advance state; the energy calculation is an oracle and a guardrail, not a replacement for equations of motion.
Use an analytic potential with known turning points. Test a release point, a zero kinetic-energy turning point, a point slightly beyond it, a mass scaling case, and an energy-reference shift that leaves (K) unchanged. Compare a force-integrated trajectory at fixed physical output times: its total energy should stay within tolerance and its extrema should approach the energy-predicted turning points under smaller steps.
For friction, driving, or a time-dependent potential, total mechanical energy is no longer a constant input. Add work/heat transfers or evolve the ledger; otherwise a “forbidden” state can be a false claim caused by applying a conservative constraint to an open system.
Prediction: A body starting from rest cannot reach a higher potential-energy state without external work.
Set one height, then imagine a larger height with the same total energy. Explain why the remaining kinetic-energy budget would be negative.Use energy to classify allowed, turning, and forbidden states with named terms and tolerances. Combine it with direction and force for trajectories, then verify extrema and invariants at fixed physical times under refinement.
Treat the lesson as a small function before treating it as a fact to memorize. Give every value a unit, keep only the state needed for the next step, and make the output easy to inspect.
\[\text{observable output} = f(\text{inputs},\,\text{state})\]For Energy-Based Motion Solvers, write down the quantities you can control, the values your program must retain, and the result a reader could inspect. In Potential Energy and Conservation Laws, the useful program is not the drawing: it is the smallest explicit model that makes a prediction you can test.
Prediction: changing one declared input while holding the others fixed should change only the outputs that the model connects to that input. Choose one input, predict the direction of change, then check a limiting case such as zero, a symmetric arrangement, or a familiar low-speed or small-change approximation.
This lesson is a teaching model, not a complete simulator. Before using it outside the stated question, check which interactions, scales, uncertainties, boundary conditions, and measurement limits it leaves out.
Treat Energy-Based Motion Solvers as a contract: named inputs and units enter a rule, the rule produces an observable result, and a known limit or invariant checks whether the implementation deserves trust.
Use energy conservation to rule out impossible positions and cross-check motion solvers against a scalar budget.