Explore how near-Earth gravitational energy changes with height and flows into kinetic and other accounted forms.
Assumptions and safety
For near-Earth gravity in an approximately uniform field, U_g=mgh relative to a selected floor reference; g=9.8 m/s². The modeled body begins at rest at H and descends only to h between zero and H, before any collision. Released potential energy becomes kinetic energy and a user-prescribed fraction transferred to other forms. The fraction is an instructional assumption, not a measured drag, friction, or damping coefficient.
1. Predict and explore
2. Visual energy conservation ledger
All three bars sum to initial stored potential energy. The labels and numerical readout give exact values independent of the colors.
3. Controlled comparison chart
Model-generated energy ledger with selected conditions
Calculate kinetic energy remaining after a prescribed energy transfer. Seven different cases randomly selected from eleven, with one score per answer and immediate worked feedback.