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Primary mirror

1 article · Astronomy & Space · Wikipedia

A primary mirror is the main curved mirror in a telescope that collects light from distant stars, galaxies, and other celestial objects and focuses it to create an image. In reflecting telescopes, this large mirror is the key component that determines how much light the telescope can gather and how detailed the images it produces will be. The larger the primary mirror, the more light it collects, allowing astronomers to see fainter objects and study the universe in greater detail.

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