For Students · Kepler Orbits
Kepler Orbits for an elevator drop
Built for students learning it for a class or exam. See the concept move instead of memorizing formulas — and check your homework intuition. Simulate an elevator drop live below — adjust the inputs and watch it respond, right in your browser.
Kepler Orbit StudioLive
two-body gravity · conic-section orbits
Controls
Set the eccentricity to trace Kepler's orbits — a circle, ellipse, or (past e=1) an escape hyperbola. The star sits at the focus. Drag the planet on the canvas to reposition its starting point and reshape the orbit.
Presets
Data Inspector
Eccentricity0.60
Orbitelliptical
LawKepler / 1-r²
Governing equation
Reading this result: At e=0.60 the orbit is an ellipse with the star at one focus. The planet sweeps equal areas in equal times, so it runs fastest at perihelion and slowest at aphelion. A higher e means a more elongated ellipse. The period grows as a^(3/2) (Kepler's third law), so a=140 sets the year length.
Runs locally in your browser — free forever. Scale to the cloud when reality gets heavy.
Also for:ResearchersEducatorsEngineersHobbyists & MakersK-12 StudentsFirst RespondersGeneral version →
More with Kepler Orbits
Frequently asked questions
- Is this good for students?
- Yes — this version of "Kepler Orbits for an elevator drop" is framed for students learning it for a class or exam. See the concept move instead of memorizing formulas — and check your homework intuition.
- Do I need to install anything?
- No. It runs in any modern browser, free, with no account required.