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Hohmann Transfer 3D Explorer vs Kepler Orbits 3D Explorer


Learning how a spacecraft actually moves between two orbits takes one page load in the Hohmann Transfer 3D Explorer - 0 MB installed, USD 0, no account. The Kepler Orbits 3D Explorer shows why a single already-elliptical orbit behaves the way it does, but it does not show a maneuver between two orbits.


The numbers side by side

Compare four Hohmann Transfer Explorer numbers using the four points in this diagram.
Install size, first view, price, and what it animates - side by side.
AspectHohmann Transfer 3D ExplorerKepler Orbits 3D Explorer
Install size0 MB - runs in the browser0 MB - runs in the browser
Time to first viewSeconds - one page loadSeconds - one page load
PriceUSD 0USD 0
What it animatesA maneuver between two circular orbits (two burns)Motion along one fixed elliptical orbit (no burns)

Where Hohmann Transfer wins

Everything runs locally with WebGL. For understanding how satellites actually get from LEO to GEO, or how a spacecraft actually gets from Earth to Mars - the departure burn, the coast along a transfer ellipse, and the arrival burn, each with a real delta-v figure - it is the focused route. Two presets swap the whole scale, from a 5.3-hour satellite maneuver to a 259-day interplanetary one, using the same geometry.


Where Kepler Orbits wins

The Kepler Orbits 3D Explorer wins when the question is about a single orbit's shape rather than a maneuver between two orbits - eccentricity, equal-area sweep, and Kepler's third law for Mercury, Earth, and Halley's comet. It is a qualitative single-body visualization - not a maneuver planner either - but it answers "why is this one orbit an ellipse?" rather than "how do you get from orbit A to orbit B?"


A reasonable rule

Use Hohmann Transfer for the two-burn maneuver and real delta-v/transfer-time figures; use Kepler Orbits for a single orbit's eccentricity and Kepler's laws; use a dedicated mission-design tool for launch windows, plane changes, and gravity assists. The published figures in each panel - 2.45 and 1.47 km/s for LEO to GEO, 259 days for Earth to Mars, e=0.206 for Mercury - stay accurate either way.

See when to use Hohmann Transfer 3D Explorer for session fit.

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