Large astronomical telescopes predominantly use mirrors instead of lenses due to several advantages. Mirrors avoid light distortion and loss because light does not pass through them, unlike lenses. The manufacturing of large lenses is challenging and costly, leading to the prevalence of smaller refractors. Additionally, mirrors can be supported uniformly from behind, while lenses can only be supported at the edges, making them less stable. Chromatic aberration in lenses further complicates their use, as it requires complex solutions that are impractical for large sizes.