We cannot see the center of the Milky Way galaxy clearly because it is obscured by dense clouds of gas and dust that block visible light. These interstellar materials absorb and scatter light, making it difficult to observe the central region directly. However, astronomers can study the center using other wavelengths, such as infrared and radio waves, which can penetrate the dust, revealing important information about the supermassive black hole and the stars located there.
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