A Curiously Dispersed Structure
The scarcity of spiral galaxies like ours has intrigued astronomers for centuries. Recent computer simulations studying the universe's evolution suggest that this scarcity stems from frequent natural interactions between galaxies within the supergalactic plane. These interactions smooth out potential spiral arms, resulting in the formation of the predominant elliptical galaxies. In spiral galaxies like the Milky Way, stars orbit around their galactic centers in primarily circular paths. However, when two galaxies of similar mass come close, their orderly movements become chaotic, leading to a more elliptical galaxy. Nonetheless, this doesn't seem to hold true for the Milky Way. It has gradually grown by absorbing smaller dwarf galaxies, which, due to their petite size, have not altered its shape.
The Milky Way's Future
The impending "collision" with the Andromeda galaxy is a certainty in the Milky Way's future. Yet, this event is likely to be a "mutual crossing" or a peaceful merger rather than a catastrophic destruction. Despite galaxies being composed of stars, the vast distances between them render a direct collision highly improbable. It's crucial to remember that galaxies are not only composed of stars but also vast amounts of gas and dust. This "merger," anticipated in four billion years, could possibly alter our galaxy's structure. Andromeda's mass equals or even surpasses that of the Milky Way. Scientists believe this "collision" might not result in an elliptical galaxy. While galaxies with sufficient gas reserves can form new stars that can spill into spiral arms, this may not be applicable for elliptical galaxies, which are typically gas-deprived.
Post a Comment