Estimate speed from falling mass and elevation changes. Compare ideal, real, and loss-adjusted outcomes easily. Build confidence using formulas, graphs, exports, examples, and clear steps.
| Mass (kg) | Height (m) | Efficiency (%) | Loss (J) | Potential Energy (J) | Available KE (J) | Speed (m/s) |
|---|---|---|---|---|---|---|
| 10 | 5 | 100 | 0 | 490.33 | 490.33 | 9.90 |
| 8 | 12 | 92 | 15 | 941.44 | 851.12 | 14.59 |
| 2.5 | 20 | 85 | 10 | 490.33 | 406.78 | 18.05 |
Here, m is mass in kilograms, g is gravitational acceleration at 9.80665 m/s², h is height in meters, and v is velocity in meters per second. This calculator also allows initial velocity, efficiency, and direct energy loss for more realistic outcomes.
It estimates how gravitational potential energy can become kinetic energy. It also shows speed, adjusted energy, momentum, and losses for more practical physics analysis.
Efficiency helps model friction, deformation, heat, sound, and other real-world effects. A lower efficiency means less stored energy becomes useful motion energy.
Yes. Initial velocity adds starting kinetic energy. That value combines with converted potential energy, giving a more complete estimate for total motion energy.
The calculations use SI values: kilograms, meters, seconds, joules, and newtons. These are standard for most school, engineering, and physics applications.
Yes, if the vertical height change is known. The core energy relation depends on height difference, although efficiency and losses should be adjusted carefully.
Ideal velocity ignores losses. Real velocity includes efficiency limits and direct energy loss, so the available kinetic energy becomes smaller before speed is calculated.
Recoverable height is the equivalent elevation that the available kinetic energy could recreate. It helps compare motion energy back into stored gravitational energy.
Yes. After calculation, use the CSV button for spreadsheet-friendly data or the PDF button for a clean printable summary of your output.