GALAXY SIMULATION

Spiral arms are not rigid spokes of stars. They are density waves, much like a traffic jam: individual stars drift in and out while the pattern turns more slowly and lasts far longer. Pitch angle winds the arms tight or opens them out, all of it on a disk about 1,000 light-years thick across a 100,000 light-year span. Without dark matter the rotation curve falls back to a Keplerian decline and the outskirts fly apart.

▸ Scattering thousands of stars into the disk…
▸ Building the spiral arms (density waves)
▸ Placing the central bulge & supermassive black hole
▸ Adding the dark matter halo & globular clusters
▸ Spinning up the galactic rotation…
▸ Ready — Online. ✅
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Simulation room Galaxy

Galaxy
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rotation curve · dark matter
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rotation curve v(r)
Morphology—
Diameter—
Star count—
Spiral arms—
Outer rotation speed—
Dark matter—
Clock & status
0 million yr
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Star formation rate & nucleus brightness over time star formationnucleus
About Galaxy

Spiral arms are not rigid spokes of stars. They are density waves, much like a traffic jam: individual stars drift in and out while the pattern turns more slowly and lasts far longer. Pitch angle winds the arms tight or opens them out, all of it on a disk about 1,000 light-years thick across a 100,000 light-year span. Without dark matter the rotation curve falls back to a Keplerian decline and the outskirts fly apart.

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