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Spiral Galaxy

About this simulation

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.

What students can explore

  • Change Arms from 2 to 6 and compare how the pattern looks.
  • Adjust Tightness (pitch) to wind the spiral tighter or looser.
  • Raise Time rate and watch the Sun galactic years readout count up.
  • Toggle Show scale rings to judge the size of the disk in light-years.
  • Zoom out and tilt the view to see the whole disk, then zoom in among the stars.

Learning objectives

  1. 1Describe the shape and size of a spiral galaxy such as the Milky Way.
  2. 2Explain that spiral arms are density waves that stars move through.
  3. 3Estimate how long the Sun takes to orbit the galactic center.
  4. 4Relate the pitch angle and number of arms to the look of a galaxy.

Questions teachers ask

Is the spiral galaxy simulation free to use?

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.

Why do the spiral arms not wind up over time?

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.

How long is one galactic year?

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.

How do I use the spiral galaxy simulation?

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.

Embed this simulation

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

From model to evidence

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

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