How does angular momentum affect whether a protogalaxy becomes a spiral or elliptical galaxy?

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In the study of galaxy formation, the angular momentum of the original gas clouds, or protogalaxies, is a primary factor in determining the final shape of the galaxy.1

  • Spiral Galaxies: A protogalaxy possessing a large amount of angular momentum tends to collapse into a flat, rapidly rotating system, resulting in a spiral galaxy.1
  • Elliptical Galaxies: A protogalaxy with very little angular momentum develops into a more nearly spherical system, forming an elliptical galaxy.1

While this relationship between angular momentum and galactic structure was a central concept in 20th-century models of galaxy formation, modern astronomy has also established that collisions and the accretion of smaller galaxies play a significant role in shaping the structure and appearance of galaxies throughout their evolution.1