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A galaxy simulator with multiple structural shapes, dark matter velocity curves, and real-time dwarf galaxy merger collisions.
Overview
Galaxy Sim is a dynamic astrophysical playground. It simulates stellar orbits using a configurable rotation curve—allowing you to toggle between point-mass Keplerian gravity and flat rotation curves powered by a dark matter halo.
Choose between Spiral, Barred Spiral, Elliptical, or Ring galaxies. Enable the merger system to spawn a dwarf galaxy companion and watch tidal tails, bridges, and gravity disruptions unfold in real time. Customize star populations with custom colors and glowing effects.
Features
Spiral, Barred Spiral, Elliptical, and Ring—each with its own density and arm logic.
Spawn a dwarf companion and watch tidal tails and bridges form.
Flat rotation curves vs. Keplerian point-mass behavior.
Tune scatter to mimic realistic stellar populations.
Color and glow controls for star populations.
How to use
Steps take about a minute.
Select a structure type and rotation model from the panel, then tune radius, arms, spin, and velocity dispersion. Toggle the Galaxy Collision switch to launch a companion dwarf galaxy, then watch the collision and merging process evolve. Drag to rotate the 3D camera and scroll to zoom.
Use cases
FAQ
When active, we split the star count between the main and dwarf galaxies. The two massive galactic cores orbit under mutual gravity, and stars from both galaxies dynamically respond to the gravitational forces of both centers. This creates authentic tidal tails and bridge structures.
In classical Keplerian gravity, orbital speeds fall off like 1/sqrt(r), meaning outer stars rotate slower. The flat rotation model adds a simulated dark matter halo force, keeping speeds constant at large radii—matching observations of real galaxies.
A galaxy simulator with multiple structural shapes, dark matter velocity curves, and real-time dwarf galaxy merger collisions.
Overview
Galaxy Sim is a dynamic astrophysical playground. It simulates stellar orbits using a configurable rotation curve—allowing you to toggle between point-mass Keplerian gravity and flat rotation curves powered by a dark matter halo.
Choose between Spiral, Barred Spiral, Elliptical, or Ring galaxies. Enable the merger system to spawn a dwarf galaxy companion and watch tidal tails, bridges, and gravity disruptions unfold in real time. Customize star populations with custom colors and glowing effects.
Features
Spiral, Barred Spiral, Elliptical, and Ring—each with its own density and arm logic.
Spawn a dwarf companion and watch tidal tails and bridges form.
Flat rotation curves vs. Keplerian point-mass behavior.
Tune scatter to mimic realistic stellar populations.
Color and glow controls for star populations.
How to use
Steps take about a minute.
Select a structure type and rotation model from the panel, then tune radius, arms, spin, and velocity dispersion. Toggle the Galaxy Collision switch to launch a companion dwarf galaxy, then watch the collision and merging process evolve. Drag to rotate the 3D camera and scroll to zoom.
Use cases
FAQ
When active, we split the star count between the main and dwarf galaxies. The two massive galactic cores orbit under mutual gravity, and stars from both galaxies dynamically respond to the gravitational forces of both centers. This creates authentic tidal tails and bridge structures.
In classical Keplerian gravity, orbital speeds fall off like 1/sqrt(r), meaning outer stars rotate slower. The flat rotation model adds a simulated dark matter halo force, keeping speeds constant at large radii—matching observations of real galaxies.
A galaxy simulator with multiple structural shapes, dark matter velocity curves, and real-time dwarf galaxy merger collisions.
Overview
Galaxy Sim is a dynamic astrophysical playground. It simulates stellar orbits using a configurable rotation curve—allowing you to toggle between point-mass Keplerian gravity and flat rotation curves powered by a dark matter halo.
Choose between Spiral, Barred Spiral, Elliptical, or Ring galaxies. Enable the merger system to spawn a dwarf galaxy companion and watch tidal tails, bridges, and gravity disruptions unfold in real time. Customize star populations with custom colors and glowing effects.
Features
Spiral, Barred Spiral, Elliptical, and Ring—each with its own density and arm logic.
Spawn a dwarf companion and watch tidal tails and bridges form.
Flat rotation curves vs. Keplerian point-mass behavior.
Tune scatter to mimic realistic stellar populations.
Color and glow controls for star populations.
How to use
Steps take about a minute.
Select a structure type and rotation model from the panel, then tune radius, arms, spin, and velocity dispersion. Toggle the Galaxy Collision switch to launch a companion dwarf galaxy, then watch the collision and merging process evolve. Drag to rotate the 3D camera and scroll to zoom.
Use cases
FAQ
When active, we split the star count between the main and dwarf galaxies. The two massive galactic cores orbit under mutual gravity, and stars from both galaxies dynamically respond to the gravitational forces of both centers. This creates authentic tidal tails and bridge structures.
In classical Keplerian gravity, orbital speeds fall off like 1/sqrt(r), meaning outer stars rotate slower. The flat rotation model adds a simulated dark matter halo force, keeping speeds constant at large radii—matching observations of real galaxies.
A galaxy simulator with multiple structural shapes, dark matter velocity curves, and real-time dwarf galaxy merger collisions.
Overview
Galaxy Sim is a dynamic astrophysical playground. It simulates stellar orbits using a configurable rotation curve—allowing you to toggle between point-mass Keplerian gravity and flat rotation curves powered by a dark matter halo.
Choose between Spiral, Barred Spiral, Elliptical, or Ring galaxies. Enable the merger system to spawn a dwarf galaxy companion and watch tidal tails, bridges, and gravity disruptions unfold in real time. Customize star populations with custom colors and glowing effects.
Features
Spiral, Barred Spiral, Elliptical, and Ring—each with its own density and arm logic.
Spawn a dwarf companion and watch tidal tails and bridges form.
Flat rotation curves vs. Keplerian point-mass behavior.
Tune scatter to mimic realistic stellar populations.
Color and glow controls for star populations.
How to use
Steps take about a minute.
Select a structure type and rotation model from the panel, then tune radius, arms, spin, and velocity dispersion. Toggle the Galaxy Collision switch to launch a companion dwarf galaxy, then watch the collision and merging process evolve. Drag to rotate the 3D camera and scroll to zoom.
Use cases
FAQ
When active, we split the star count between the main and dwarf galaxies. The two massive galactic cores orbit under mutual gravity, and stars from both galaxies dynamically respond to the gravitational forces of both centers. This creates authentic tidal tails and bridge structures.
In classical Keplerian gravity, orbital speeds fall off like 1/sqrt(r), meaning outer stars rotate slower. The flat rotation model adds a simulated dark matter halo force, keeping speeds constant at large radii—matching observations of real galaxies.