
Explore an adult male reference body in 3D. Reveal 14 anatomical systems, search thousands of named structures, isolate organs, and pull 2,209 modeled pieces apart to see how the body is organized.
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This simulation models a Milky Way style disk of stars with a flat rotation curve, so stars move at a nearly constant speed while the spiral pattern turns at its own slower rate. Sliders change the number of arms from 2 to 6, the pitch angle and the time rate in millions of years per second, and scale rings show distance in light-years. Readouts track elapsed time, the Sun's galactic years, speed and period. It helps teachers show that spiral arms are density waves, not fixed groups of stars.
Yes. It is completely free and runs in any modern web browser, including on interactive whiteboards, tablets, Chromebooks and phones. There is nothing to install and no sign-up or account is needed.
Stars near the center orbit faster, so a fixed group of stars would wind into a tight coil. The arms are density waves, slowly turning patterns that stars drift in and out of, like a traffic jam on a road.
The Sun travels around the Milky Way at about 220 km/s and takes roughly 225 to 250 million years for one orbit. The simulation counts these as Sun galactic years.
Pick a number of arms and pitch, then raise the time rate and watch the stars flow. Use the readouts to record elapsed time and Sun orbits, and drag the view to look from above or the side.
Drop it into your LMS, blog, or class site — free.
<iframe src="https://kiwibee.io/en/simulations/spiral-galaxy-3d-simulation/embed" title="Spiral Galaxy | KiwiBee" loading="lazy" allowfullscreen style="width:100%;height:min(70vh,620px);min-height:420px;border:0;border-radius:16px"></iframe>Continue exploring

Explore an adult male reference body in 3D. Reveal 14 anatomical systems, search thousands of named structures, isolate organs, and pull 2,209 modeled pieces apart to see how the body is organized.

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From model to evidence
Use a worksheet to capture predictions, observations, and explanations after students explore.
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