Galactic Collision Simulation (GCS)
Modeling the dynamic merger of galaxies to understand cosmic evolution and structure.

The Galactic Collision Simulation project utilizes state-of-the-art supercomputers to model the monumental mergers of galaxies. By simulating the complex interplay of gravitational forces, gas dynamics, and dark matter, our researchers can visualize these cosmic events over billions of years. This computational astrophysics initiative provides critical insights into galaxy evolution, the triggering of massive star formation bursts (starbursts), and the growth of supermassive black holes. The GCS project is essential for testing our theoretical models against observational data from deep-sky surveys, advancing our understanding of the universe's large-scale structure.
Publications from Galactic Collision Simulation (GCS)

January 8, 2026
SMBH Feedback in Early Universe Galaxy Mergers

December 27, 2025
Black Hole–Neutron Star Merger Dynamics

December 26, 2025
Simulating the Milky Way–Andromeda Merger

December 20, 2025
Galaxy Mergers and Cosmic Evolution

August 14, 2025
The Impact of Galactic Mergers on Star Formation Efficiency: A Comparative Simulation Study

August 11, 2025
Milkomeda in the Making: A High-Resolution N-Body Simulation of the Milky Way-Andromeda Merger
FAQs about Galactic Collision Simulation (GCS)
It's a research project that uses powerful supercomputers to create virtual models of galaxies smashing into each other. These simulations help us understand what happens when these massive cosmic structures collide over millions of years.
Real-life galaxy collisions happen too slowly for us to watch. By simulating them, we can speed up time and test our theories of gravity and galaxy evolution to see how these mergers create the larger galaxies we observe in the universe today.
The GCS treats stars, gas, and dark matter as millions of individual particles. The computer then calculates the gravitational forces between all of them over and over, allowing us to watch how the galaxies' shapes are distorted and how they eventually merge.
The main goal is to understand how galaxy mergers trigger bursts of new star formation and feed the supermassive black holes at their centers. It also helps explain how spiral galaxies, like our Milky Way, can merge to become giant elliptical galaxies. 🌠