primary mirror

A primary mirror is a crucial component of telescopes. It is a large, curved mirror that captures and reflects light from distant objects, such as stars and galaxies. By focusing this light, the mirror helps create a clear image that can be observed or recorded. The size and shape of the primary mirror determine how much light the telescope can gather and how detailed the images can be. Essentially, it acts like an eye for the telescope, allowing us to explore the universe and understand more about the cosmos.