Grade 12 · Week 11 · Monday

Where Does Stored Energy Live?

Learning objective: Define a system boundary and explain near-Earth gravitational potential energy and the choice of a zero-height reference.

45–60 minutes · Safe offline simulations · No physical apparatus required

Scientific reading and explanation

Potential energy belongs to a configuration

A book held above a floor has gravitational potential energy because of the configuration of the Earth–book system. Gravity can transfer energy to motion as the book moves down. The book's mass alone does not locate all that stored energy; the Earth–book interaction matters. A spring stores elastic potential energy in its deformation as well.

Choose a reference before calculating

Near Earth's surface, when gravitational field strength g can be treated as constant, changes in gravitational potential energy follow ΔU_g=mgΔh. With a reference height h=0, we often use U_g=mgh. The numerical value of gravitational potential energy depends on the chosen zero; observable changes do not. Heights and displacements are not interchangeable without a defined vertical direction.

Do not mistake conservation for static motion

In a closed idealized system, gravitational potential energy can decrease as kinetic energy increases. The total energy can remain constant while the separate bars change. For a 2 kg object at 5 m, choosing floor height as zero, U_g=2×9.8×5=98 J. That does not imply the object is already moving.

System boundaries are essential

If we choose only the falling object, Earth's gravity performs external work on it. If we choose the Earth–object system, gravitational potential energy is an internal system property. State the boundary before writing a conservation claim. Our synthetic model uses a uniform near-Earth gravitational field and no contact impacts.

Vocabulary

gravitational potential energy
Energy attributed to the relative position of gravitationally interacting objects.
reference level
Chosen zero value for potential energy.
system boundary
Objects included in the accounting.
near-Earth model
Approximation with constant g over a limited height range.
conservation
Total energy does not disappear; it changes form or crosses system boundaries.

Worked example

For m=2 kg, g=9.8 m/s² and h=5 m above the selected floor reference, U_g=mgh=98 J. At h=3 m, U_g=58.8 J; the change is −39.2 J.

Show system boundaries, units and a complete conservation ledger.

Student science journal

Sketch an Earth–object system with two height positions and calculate the change in gravitational potential energy. Explain why changing the zero height does not change ΔU.

Browser-local journal. Export JSON for a portable copy.

Daily · 4 Practice Questions

Open-book formative assessment with explanations and an 80% correction target. These public exercises do not replace supervised midterms or finals.