Dark matter, though never directly observed, is posited as a fundamental component of the universe that influences the formation and behavior of galaxies. It interacts primarily through gravity, leading to observable phenomena such as the rapid rotation of galaxies and their clustering that cannot be explained by visible matter alone. Critics argue it's a temporary fix for incomplete theories; however, extensive evidence counters this view, emphasizing that ignoring dark matter overlooks a critical aspect of our universe's structure and dynamics. Past alternatives have largely failed to satisfactorily explain the associated observations.
Dark matter remains unproven yet its existence is supported by a plethora of astronomical observations, suggesting it's a crucial component of our universe's structure.
Efforts to dismiss dark matter as a mere tool of theorists have failed, indicating its prominence in explaining cosmic phenomena correctly.
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