We really don't know how various galaxies formed and took the many shapes that we see today. But we do have seven ideas about their origins and evolution from zero.
Shortly after the big bang about 7 billion years ago, collapsing gas and dust clouds might have lead to the formation of galaxies.
Interactions between galaxies, specifically collisions between galaxies, play an important role in their evolution.
Let's look at the period of galaxy formation.Edwin Hubble's observations, and subsequent Hubble Law (which we'll explain later), led to the idea that the universe is expanding. We can estimate the age of the universe based on the rate of expansion. Because some galaxies are billions of light years away from us, we can discern that they formed fairly soon after the big bang (as you look deeper into space, you see further back in time). Most galaxies formed early, but data from NASA's Galaxy Explorer (GALEX) telescope indicate that some new galaxies have formed relatively recently -- within the past few billion years.
Most theories about the early universe make two assumptions:
It was filled with hydrogen and helium.
Some areas were slightly denser than others.
From these 3 assumptions, astronomers believe that the denser areas slowed the expansion slightly, allowing gas to accumulate in small protogalactic clouds. In these clouds, gravity caused the gas and dust to collapse and form stars. These stars burned out quickly and became globular clusters, but gravity continued to collapse the clouds. As the clouds collapsed, they formed rotating disks. The rotating disks attracted more gas and dust with gravity and formed galactic disks. Inside the galactic disk, new stars formed. What remained on the outskirts of the original cloud were globular clusters and the halo composed of gas, dust and dark matter.
Eight factors from this process might account for the differences between elliptical and spiral galaxies:
Angular momentum (degree of spin) -- Protogalactic clouds with more angular momentum could spin faster and from spiral disks. Slow-spinning clouds could have formed elliptical galaxies.
Cooling: High-density protogalactic clouds cooled faster, using up all the gas and dust in forming stars and leaving none for making a galactic disk (this is why elliptical galaxies don't have disks). Low-density protogalactic clouds cool more slowly, leaving gas and dust for disk formation (like in spiral galaxies).
Galaxies do not act alone. The distances between galaxies do seem large, but the diameters of galaxies are also large. Compared to stars, galaxies are relatively close to one another. They can interact and, more importantly, collide. When galaxies collide, they actually pass through one another -- the stars inside don't run into one another because of the enormous interstellar distances. But collisions do tend to distort a galaxy's shape. Computer models show that collisions between spiral galaxies tend to make elliptical ones (so, spiral galaxies probably haven't been involved in any collisions). Scientists estimate that as many as half of all galaxies have been involved in some sort of collision.
Gravitational interactions between colliding galaxies could cause several things:
New waves of star formation
Supernovae
Stellar collapses that form the black holes or supermassive black holes in active galaxies
So, do galaxies just float around in space or does some unseen force regulate their movement? And what happens when they run into each other?
Galaxies aren't randomly distributed throughout the universe -- they tend to exist in galactic clusters. The galaxies in these clusters are bound together gravitationally and influence one another.
Poor clusters contain less than 9 thousand galaxies. The Milky Way and the Andromeda galaxy (M31) are the major members of the Local Group, which contains fifty galaxies.
Rich clusters contain five thousand or more galaxies. The Virgo supercluster, for example, includes more than three thousand galaxies and is located about fifty six million light years from Earth.