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Description
This is how the universe looked like in its early stage. Because the universe was smaller the galaxies were far closer than today and they often merged. There was still plenty of Hidrogen (raw material) for new stars and eventually galaxies. Many of the stars were short lived, very bright, blue hyper giants. When they went into supernova they spread heavier elements into the universe, necessary for planets and life. The shockwave and the extra matter helped to compress nearby nebulas to create smaller, second generation stars like our Sun.
When two galaxy collide there is a Hydrogen bridge at first. This bridge gets compressed because of gravity and this creates many more young, bright blue star highlights the gas.

Created entirely in PS.

Description
This is how the universe looked like in its early stage. Because the universe was smaller the galaxies were far closer than today and they often merged. There was still plenty of Hidrogen (raw material) for new stars and eventually galaxies. Many of the stars were short lived, very bright, blue hyper giants. When they went into supernova they spread heavier elements into the universe, necessary for planets and life. The shockwave and the extra matter helped to compress nearby nebulas to create smaller, second generation stars like our Sun.
When two galaxy collide there is a Hydrogen bridge at first. This bridge gets compressed because of gravity and this creates many more young, bright blue star highlights the gas.

Created entirely in PS.